Author: "Zeidler, Peter" - Searchworks@Jio Institute Digital Library Search Results

Your search keyword '"Zeidler, Peter"' showing total 161 results

Start Over Author "Zeidler, Peter"

161 results on '"Zeidler, Peter"'

1. The NIRSpec Micro-Shutter Array: Operability and Operations After Two Years of JWST Science

Author: Bechtold, Katie, Böker, Torsten, Franz, David E., Plate, Maurice te, Rawle, Timothy D., Wu, Rai, and Zeidler, Peter
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: The Near Infrared Spectrograph (NIRSpec) on the James Webb Space Telescope affords the astronomical community an unprecedented space-based Multi-Object Spectroscopy (MOS) capability through the use of a programmable array of micro-electro-mechanical shutters. Launched in December 2021 and commissioned along with a suite of other observatory instruments throughout the first half of 2022, NIRSpec has been carrying out scientific observations since the completion of commissioning. These observations would not be possible without a rigorous program of engineering operations to actively monitor and maintain NIRSpec's hardware health and safety and enhance instrument efficiency and performance. Although MOS is only one of the observing modes available to users, the complexity and uniqueness of the Micro-Shutter Assembly (MSA) that enables it has presented a variety of engineering challenges, including the appearance of electrical shorts that produce contaminating glow in exposures. Despite these challenges, the NIRSpec Multi-Object Spectrograph continues to perform robustly with no discernible degradation or significant reduction in capability. This paper provides an overview of the NIRSpec micro-shutter subsystem's state of health and operability and presents some of the developments that have taken place in its operation since the completion of instrument commissioning., Comment: SPIE Astronomical Telescopes + Instrumentation: Ground-based and Airborne Instrumentation for Astronomy X (Yokohama 2024), paper number 13092-38
Published: 2024
Full Text: View/download PDF

2. Young Stellar Objects in NGC 346: A JWST NIRCam/MIRI Imaging Survey

Author: Habel, Nolan, Nally, Conor, Lenkic, Laura, Meixner, Margaret, De Marchi, Guido, Kavanagh, Patrick J., Fahrion, Katja, Nayak, Omnarayani, Hirschauer, Alec S., Jones, Olivia C., Biazzo, Katia, Brandl, Bernhard R., Jaspers, Jeroen, Pontoppidan, Klaus M., Robberto, Massimo, Rogers, Ciaran, Sabbi, Elena, Sargent, B. A., Soderblom, David R., and Zeidler, Peter
Subjects: Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Astrophysics of Galaxies
Abstract: We present a JWST imaging survey with NIRCam and MIRI of NGC 346, the brightest star-forming region in the Small Magellanic Cloud (SMC). By combining aperture and point spread function (PSF) photometry of eleven wavelength bands across these two instruments, we have detected more than 200,000 unique sources. Using near-infrared (IR) color analysis, we observe various evolved and young populations, including 196 young stellar objects (YSOs) and pre-main sequence stars suitable for forthcoming spectroscopic studies. We expand upon this work, creating mid-IR color-magnitude diagrams and determining color cuts to identify 833 reddened sources which are YSO candidates. We observe that these candidate sources are spatially associated with regions of dusty, filamentary nebulosity. Furthermore, we fit model YSO spectral energy distributions (SEDs) to a selection of sources with detections across all of our MIRI bands. We classify with a high degree of confidence 23 YSOs in this sample and estimate their radii, bolometric temperatures, luminosities, and masses. We detect YSOs approaching 1 solar mass, the lowest-mass extragalactic YSOs confirmed to date.
Published: 2024

3. Exploring the Mpc Environment of the Quasar ULAS J1342+0928 at z = 7.54

Author: Rojas-Ruiz, Sofía, Mazzucchelli, Chiara, Finkelstein, Steven L., Bañados, Eduardo, Farina, Emanuele P., Venemans, Bram P., Decarli, Roberto, Willott, Christopher J., Wang, Feige, Walter, Fabian, Congiu, Enrico, Brammer, Gabriel B., and Zeidler, Peter
Subjects: Astrophysics - Astrophysics of Galaxies
Abstract: Theoretical models predict that z~6 quasars are hosted in the most massive halos of the underlying dark matter distribution and thus would be immersed in protoclusters of galaxies. However, observations report inconclusive results. We investigate the 1.1 pMpc2 environment of the z = 7.54 luminous quasar ULAS J1342+0928. We search for Lyman-break galaxy candidates (LBG) using deep imaging from the Hubble Space Telescope (HST) in the ACS/F814W, WFC3/F105W/F125W bands, and Spitzer/IRAC at 3.6 $\mu$m and 4.5 $\mu$m. We report a zphot = $7.69^{+0.33}_{-0.23}$ LBG with magF125W = 26.41 at 223 projected-pkpc from the quasar. We find no HST counterpart to one [CII]-emitter previously found with ALMA at 27 projected-pkpc and $z[CII]=7.5341\pm0.0009$ (Venemans et al. 2020). We estimate the completeness of our LBG candidates using results from CANDELS/GOODS deep blank field searches sharing a similar filter setup. We find that >50% of the z~7.5 LBGs with magF125W >25.5 are missed due to the absence of a filter redward of the Lyman-break in F105W, hindering the UV color accuracy of the candidates. We conduct a QSO-LBG clustering analysis revealing a low LBG excess of $0.46^{+1.52}_{-0.08}$ in this quasar field, consistent with an average or low-density field. Consequently, this result does not present strong evidence of an LBG overdensity around ULAS J1342+0928. Furthermore, we identify two LBG candidates with a zphot matching a confirmed z=6.84 absorber along the line-of-sight to the quasar. All these galaxy candidates are excellent targets for follow-up observations with JWST and/or ALMA to confirm their redshift and physical properties., Comment: Accepted to ApJ, 16 pages, 8 figures
Published: 2024

4. The VLT MUSE NFM view of outflows and externally photoevaporating discs near the Orion Bar

Author: Haworth, Thomas J., Reiter, Megan, O'Dell, C. Robert, Zeidler, Peter, Berne, Olivier, Manara, Carlo F., Ballabio, Giulia, Kim, Jinyoung S., Bally, John, Goicoechea, Javier R., Aru, Mari-Liis, Gupta, Aashish, and Miotello, Anna
Subjects: Astrophysics - Astrophysics of Galaxies, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics
Abstract: We present VLT/MUSE Narrow Field Mode (NFM) observations of a pair of disc-bearing young stellar objects towards the Orion Bar: 203-504 and 203-506. Both of these discs are subject to external photoevaporation, where winds are launched from their outer regions due to environmental irradiation. Intriguingly, despite having projected separation from one another of only 1.65{\arcsec} (660au at 400pc), 203-504 has a classic teardrop shaped ``proplyd'' morphology pointing towards $\theta^2$Ori A (indicating irradiation by the EUV of that star, rather than $\theta^1$ Ori C) but 203-506 has no ionisation front, indicating it is not irradiated by stellar EUV at all. However, 203-506 does show [CI] 8727{\AA} and [OI] 6300{\AA} in emission, indicating irradiation by stellar FUV. This explicitly demonstrates the importance of FUV irradiation in driving mass loss from discs. We conclude that shielding of 203-506 from EUV is most likely due to its position on the observers side of an ionized layer lying in the foreground of the Huygens Region. We demonstrate that the outflow HH 519, previously thought to be emanating from 203-504 is actually an irradiated cloud edge and identify a new compact outflow from that object approximately along our line of sight with a velocity $\sim130$\,km\,s$^{-1}$., Comment: 14 pages, 8 figures. Accepted for publication in MNRAS
Published: 2023

5. The James Webb Space Telescope Mission

Author: Gardner, Jonathan P., Mather, John C., Abbott, Randy, Abell, James S., Abernathy, Mark, Abney, Faith E., Abraham, John G., Abraham, Roberto, Abul-Huda, Yasin M., Acton, Scott, Adams, Cynthia K., Adams, Evan, Adler, David S., Adriaensen, Maarten, Aguilar, Jonathan Albert, Ahmed, Mansoor, Ahmed, Nasif S., Ahmed, Tanjira, Albat, Rüdeger, Albert, Loïc, Alberts, Stacey, Aldridge, David, Allen, Mary Marsha, Allen, Shaune S., Altenburg, Martin, Altunc, Serhat, Alvarez, Jose Lorenzo, Álvarez-Márquez, Javier, de Oliveira, Catarina Alves, Ambrose, Leslie L., Anandakrishnan, Satya M., Andersen, Gregory C., Anderson, Harry James, Anderson, Jay, Anderson, Kristen, Anderson, Sara M., Aprea, Julio, Archer, Benita J., Arenberg, Jonathan W., Argyriou, Ioannis, Arribas, Santiago, Artigau, Étienne, Arvai, Amanda Rose, Atcheson, Paul, Atkinson, Charles B., Averbukh, Jesse, Aymergen, Cagatay, Bacinski, John J., Baggett, Wayne E., Bagnasco, Giorgio, Baker, Lynn L., Balzano, Vicki Ann, Banks, Kimberly A., Baran, David A., Barker, Elizabeth A., Barrett, Larry K., Barringer, Bruce O., Barto, Allison, Bast, William, Baudoz, Pierre, Baum, Stefi, Beatty, Thomas G., Beaulieu, Mathilde, Bechtold, Kathryn, Beck, Tracy, Beddard, Megan M., Beichman, Charles, Bellagama, Larry, Bely, Pierre, Berger, Timothy W., Bergeron, Louis E., Darveau-Bernier, Antoine, Bertch, Maria D., Beskow, Charlotte, Betz, Laura E., Biagetti, Carl P., Birkmann, Stephan, Bjorklund, Kurt F., Blackwood, James D., Blazek, Ronald Paul, Blossfeld, Stephen, Bluth, Marcel, Boccaletti, Anthony, Boegner Jr., Martin E., Bohlin, Ralph C., Boia, John Joseph, Böker, Torsten, Bonaventura, N., Bond, Nicholas A., Bosley, Kari Ann, Boucarut, Rene A., Bouchet, Patrice, Bouwman, Jeroen, Bower, Gary, Bowers, Ariel S., Bowers, Charles W., Boyce, Leslye A., Boyer, Christine T., Boyer, Martha L., Boyer, Michael, Boyer, Robert, Bradley, Larry D., Brady, Gregory R., Brandl, Bernhard R., Brannen, Judith L., Breda, David, Bremmer, Harold G., Brennan, David, Bresnahan, Pamela A., Bright, Stacey N., Broiles, Brian J., Bromenschenkel, Asa, Brooks, Brian H., Brooks, Keira J., Brown, Bob, Brown, Bruce, Brown, Thomas M., Bruce, Barry W., Bryson, Jonathan G., Bujanda, Edwin D., Bullock, Blake M., Bunker, A. J., Bureo, Rafael, Burt, Irving J., Bush, James Aaron, Bushouse, Howard A., Bussman, Marie C., Cabaud, Olivier, Cale, Steven, Calhoon, Charles D., Calvani, Humberto, Canipe, Alicia M., Caputo, Francis M., Cara, Mihai, Carey, Larkin, Case, Michael Eli, Cesari, Thaddeus, Cetorelli, Lee D., Chance, Don R., Chandler, Lynn, Chaney, Dave, Chapman, George N., Charlot, S., Chayer, Pierre, Cheezum, Jeffrey I., Chen, Bin, Chen, Christine H., Cherinka, Brian, Chichester, Sarah C., Chilton, Zachary S., Chittiraibalan, Dharini, Clampin, Mark, Clark, Charles R., Clark, Kerry W., Clark, Stephanie M., Claybrooks, Edward E., Cleveland, Keith A., Cohen, Andrew L., Cohen, Lester M., Colón, Knicole D., Coleman, Benee L., Colina, Luis, Comber, Brian J., Comeau, Thomas M., Comer, Thomas, Reis, Alain Conde, Connolly, Dennis C., Conroy, Kyle E., Contos, Adam R., Contreras, James, Cook, Neil J., Cooper, James L., Cooper, Rachel Aviva, Correia, Michael F., Correnti, Matteo, Cossou, Christophe, Costanza, Brian F., Coulais, Alain, Cox, Colin R., Coyle, Ray T., Cracraft, Misty M., Noriega-Crespo, Alberto, Crew, Keith A., Curtis, Gary J., Cusveller, Bianca, Maciel, Cleyciane Da Costa, Dailey, Christopher T., Daugeron, Frédéric, Davidson, Greg S., Davies, James E., Davis, Katherine Anne, Davis, Michael S., Day, Ratna, de Chambure, Daniel, de Jong, Pauline, De Marchi, Guido, Dean, Bruce H., Decker, John E., Delisa, Amy S., Dell, Lawrence C., Dellagatta, Gail, Dembinska, Franciszka, Demosthenes, Sandor, Dencheva, Nadezhda M., Deneu, Philippe, DePriest, William W., Deschenes, Jeremy, Dethienne, Nathalie, Detre, Örs Hunor, Diaz, Rosa Izela, Dicken, Daniel, DiFelice, Audrey S., Dillman, Matthew, Disharoon, Maureen O., van Dishoeck, Ewine F., Dixon, William V., Doggett, Jesse B., Dominguez, Keisha L., Donaldson, Thomas S., Doria-Warner, Cristina M., Santos, Tony Dos, Doty, Heather, Douglas Jr., Robert E., Doyon, René, Dressler, Alan, Driggers, Jennifer, Driggers, Phillip A., Dunn, Jamie L., DuPrie, Kimberly C., Dupuis, Jean, Durning, John, Dutta, Sanghamitra B., Earl, Nicholas M., Eccleston, Paul, Ecobichon, Pascal, Egami, Eiichi, Ehrenwinkler, Ralf, Eisenhamer, Jonathan D., Eisenhower, Michael, Eisenstein, Daniel J., Hamel, Zaky El, Elie, Michelle L., Elliott, James, Elliott, Kyle Wesley, Engesser, Michael, Espinoza, Néstor, Etienne, Odessa, Etxaluze, Mireya, Evans, Leah, Fabreguettes, Luce, Falcolini, Massimo, Falini, Patrick R., Fatig, Curtis, Feeney, Matthew, Feinberg, Lee D., Fels, Raymond, Ferdous, Nazma, Ferguson, Henry C., Ferrarese, Laura, Ferreira, Marie-Héléne, Ferruit, Pierre, Ferry, Malcolm, Filippazzo, Joseph Charles, Firre, Daniel, Fix, Mees, Flagey, Nicolas, Flanagan, Kathryn A., Fleming, Scott W., Florian, Michael, Flynn, James R., Foiadelli, Luca, Fontaine, Mark R., Fontanella, Erin Marie, Forshay, Peter Randolph, Fortner, Elizabeth A., Fox, Ori D., Framarini, Alexandro P., Francisco, John I., Franck, Randy, Franx, Marijn, Franz, David E., Friedman, Scott D., Friend, Katheryn E., Frost, James R., Fu, Henry, Fullerton, Alexander W., Gaillard, Lionel, Galkin, Sergey, Gallagher, Ben, Galyer, Anthony D., Marín, Macarena García, Gardner, Lisa E., Garland, Dennis, Garrett, Bruce Albert, Gasman, Danny, Gáspár, András, Gastaud, René, Gaudreau, Daniel, Gauthier, Peter Timothy, Geers, Vincent, Geithner, Paul H., Gennaro, Mario, Gerber, John, Gereau, John C., Giampaoli, Robert, Giardino, Giovanna, Gibbons, Paul C., Gilbert, Karolina, Gilman, Larry, Girard, Julien H., Giuliano, Mark E., Gkountis, Konstantinos, Glasse, Alistair, Glassmire, Kirk Zachary, Glauser, Adrian Michael, Glazer, Stuart D., Goldberg, Joshua, Golimowski, David A., Gonzaga, Shireen P., Gordon, Karl D., Gordon, Shawn J., Goudfrooij, Paul, Gough, Michael J., Graham, Adrian J., Grau, Christopher M., Green, Joel David, Greene, Gretchen R., Greene, Thomas P., Greenfield, Perry E., Greenhouse, Matthew A., Greve, Thomas R., Greville, Edgar M., Grimaldi, Stefano, Groe, Frank E., Groebner, Andrew, Grumm, David M., Grundy, Timothy, Güdel, Manuel, Guillard, Pierre, Guldalian, John, Gunn, Christopher A., Gurule, Anthony, Gutman, Irvin Meyer, Guy, Paul D., Guyot, Benjamin, Hack, Warren J., Haderlein, Peter, Hagan, James B., Hagedorn, Andria, Hainline, Kevin, Haley, Craig, Hami, Maryam, Hamilton, Forrest Clifford, Hammann, Jeffrey, Hammel, Heidi B., Hanley, Christopher J., Hansen, Carl August, Hardy, Bruce, Harnisch, Bernd, Harr, Michael Hunter, Harris, Pamela, Hart, Jessica Ann, Hartig, George F., Hasan, Hashima, Hashim, Kathleen Marie, Hashimoto, Ryan, Haskins, Sujee J., Hawkins, Robert Edward, Hayden, Brian, Hayden, William L., Healy, Mike, Hecht, Karen, Heeg, Vince J., Hejal, Reem, Helm, Kristopher A., Hengemihle, Nicholas J., Henning, Thomas, Henry, Alaina, Henry, Ronald L., Henshaw, Katherine, Hernandez, Scarlin, Herrington, Donald C., Heske, Astrid, Hesman, Brigette Emily, Hickey, David L., Hilbert, Bryan N., Hines, Dean C., Hinz, Michael R., Hirsch, Michael, Hitcho, Robert S., Hodapp, Klaus, Hodge, Philip E., Hoffman, Melissa, Holfeltz, Sherie T., Holler, Bryan Jason, Hoppa, Jennifer Rose, Horner, Scott, Howard, Joseph M., Howard, Richard J., Huber, Jean M., Hunkeler, Joseph S., Hunter, Alexander, Hunter, David Gavin, Hurd, Spencer W., Hurst, Brendan J., Hutchings, John B., Hylan, Jason E., Ignat, Luminita Ilinca, Illingworth, Garth, Irish, Sandra M., Isaacs III, John C., Jackson Jr., Wallace C., Jaffe, Daniel T., Jahic, Jasmin, Jahromi, Amir, Jakobsen, Peter, James, Bryan, James, John C., James, LeAndrea Rae, Jamieson, William Brian, Jandra, Raymond D., Jayawardhana, Ray, Jedrzejewski, Robert, Jeffers, Basil S., Jensen, Peter, Joanne, Egges, Johns, Alan T., Johnson, Carl A., Johnson, Eric L., Johnson, Patricia, Johnson, Phillip Stephen, Johnson, Thomas K., Johnson, Timothy W., Johnstone, Doug, Jollet, Delphine, Jones, Danny P., Jones, Gregory S., Jones, Olivia C., Jones, Ronald A., Jones, Vicki, Jordan, Ian J., Jordan, Margaret E., Jue, Reginald, Jurkowski, Mark H., Justis, Grant, Justtanont, Kay, Kaleida, Catherine C., Kalirai, Jason S., Kalmanson, Phillip Cabrales, Kaltenegger, Lisa, Kammerer, Jens, Kan, Samuel K., Kanarek, Graham Childs, Kao, Shaw-Hong, Karakla, Diane M., Karl, Hermann, Kassin, Susan A., Kauffman, David D., Kavanagh, Patrick, Kelley, Leigh L., Kelly, Douglas M., Kendrew, Sarah, Kennedy, Herbert V., Kenny, Deborah A., Keski-Kuha, Ritva A., Keyes, Charles D., Khan, Ali, Kidwell, Richard C., Kimble, Randy A., King, James S., King, Richard C., Kinzel, Wayne M., Kirk, Jeffrey R., Kirkpatrick, Marc E., Klaassen, Pamela, Klingemann, Lana, Klintworth, Paul U., Knapp, Bryan Adam, Knight, Scott, Knollenberg, Perry J., Knutsen, Daniel Mark, Koehler, Robert, Koekemoer, Anton M., Kofler, Earl T., Kontson, Vicki L., Kovacs, Aiden Rose, Kozhurina-Platais, Vera, Krause, Oliver, Kriss, Gerard A., Krist, John, Kristoffersen, Monica R., Krogel, Claudia, Krueger, Anthony P., Kulp, Bernard A., Kumari, Nimisha, Kwan, Sandy W., Kyprianou, Mark, Labador, Aurora Gadiano, Labiano, Álvaro, Lafrenière, David, Lagage, Pierre-Olivier, Laidler, Victoria G., Laine, Benoit, Laird, Simon, Lajoie, Charles-Philippe, Lallo, Matthew D., Lam, May Yen, LaMassa, Stephanie Marie, Lambros, Scott D., Lampenfield, Richard Joseph, Lander, Matthew Ed, Langston, James Hutton, Larson, Kirsten, Larson, Melora, LaVerghetta, Robert Joseph, Law, David R., Lawrence, Jon F., Lee, David W., Lee, Janice, Lee, Yat-Ning Paul, Leisenring, Jarron, Leveille, Michael Dunlap, Levenson, Nancy A., Levi, Joshua S., Levine, Marie B., Lewis, Dan, Lewis, Jake, Lewis, Nikole, Libralato, Mattia, Lidon, Norbert, Liebrecht, Paula Louisa, Lightsey, Paul, Lilly, Simon, Lim, Frederick C., Lim, Pey Lian, Ling, Sai-Kwong, Link, Lisa J., Link, Miranda Nicole, Lipinski, Jamie L., Liu, XiaoLi, Lo, Amy S., Lobmeyer, Lynette, Logue, Ryan M., Long, Chris A., Long, Douglas R., Long, Ilana D., Long, Knox S., López-Caniego, Marcos, Lotz, Jennifer M., Love-Pruitt, Jennifer M., Lubskiy, Michael, Luers, Edward B., Luetgens, Robert A., Luevano, Annetta J., Lui, Sarah Marie G. Flores, Lund III, James M., Lundquist, Ray A., Lunine, Jonathan, Lützgendorf, Nora, Lynch, Richard J., MacDonald, Alex J., MacDonald, Kenneth, Macias, Matthew J., Macklis, Keith I., Maghami, Peiman, Maharaja, Rishabh Y., Maiolino, Roberto, Makrygiannis, Konstantinos G., Malla, Sunita Giri, Malumuth, Eliot M., Manjavacas, Elena, Marini, Andrea, Marrione, Amanda, Marston, Anthony, Martel, André R, Martin, Didier, Martin, Peter G., Martinez, Kristin L., Maschmann, Marc, Masci, Gregory L., Masetti, Margaret E., Maszkiewicz, Michael, Matthews, Gary, Matuskey, Jacob E., McBrayer, Glen A., McCarthy, Donald W., McCaughrean, Mark J., McClare, Leslie A., McClare, Michael D., McCloskey, John C., McClurg, Taylore D., McCoy, Martin, McElwain, Michael W., McGregor, Roy D., McGuffey, Douglas B., McKay, Andrew G., McKenzie, William K., McLean, Brian, McMaster, Matthew, McNeil, Warren, De Meester, Wim, Mehalick, Kimberly L., Meixner, Margaret, Meléndez, Marcio, Menzel, Michael P., Menzel, Michael T., Merz, Matthew, Mesterharm, David D., Meyer, Michael R., Meyett, Michele L., Meza, Luis E., Midwinter, Calvin, Milam, Stefanie N., Miller, Jay Todd, Miller, William C., Miskey, Cherie L., Misselt, Karl, Mitchell, Eileen P., Mohan, Martin, Montoya, Emily E., Moran, Michael J., Morishita, Takahiro, Moro-Martín, Amaya, Morrison, Debra L., Morrison, Jane, Morse, Ernie C., Moschos, Michael, Moseley, S. H., Mosier, Gary E., Mosner, Peter, Mountain, Matt, Muckenthaler, Jason S., Mueller, Donald G., Mueller, Migo, Muhiem, Daniella, Mühlmann, Prisca, Mullally, Susan Elizabeth, Mullen, Stephanie M., Munger, Alan J, Murphy, Jess, Murray, Katherine T., Muzerolle, James C., Mycroft, Matthew, Myers, Andrew, Myers, Carey R., Myers, Fred Richard R., Myers, Richard, Myrick, Kaila, Nagle IV, Adrian F., Nayak, Omnarayani, Naylor, Bret, Neff, Susan G., Nelan, Edmund P., Nella, John, Nguyen, Duy Tuong, Nguyen, Michael N., Nickson, Bryony, Nidhiry, John Joseph, Niedner, Malcolm B., Nieto-Santisteban, Maria, Nikolov, Nikolay K., Nishisaka, Mary Ann, Nota, Antonella, O'Mara, Robyn C., Oboryshko, Michael, O'Brien, Marcus B., Ochs, William R., Offenberg, Joel D., Ogle, Patrick Michael, Ohl, Raymond G., Olmsted, Joseph Hamden, Osborne, Shannon Barbara, O'Shaughnessy, Brian Patrick, Östlin, Göran, O'Sullivan, Brian, Otor, O. Justin, Ottens, Richard, Ouellette, Nathalie N. -Q., Outlaw, Daria J., Owens, Beverly A., Pacifici, Camilla, Page, James Christophe, Paranilam, James G., Park, Sang, Parrish, Keith A., Paschal, Laura, Patapis, Polychronis, Patel, Jignasha, Patrick, Keith, Pattishall Jr., Robert A., Paul, Douglas William, Paul, Shirley J., Pauly, Tyler Andrew, Pavlovsky, Cheryl M., Peña-Guerrero, Maria, Pedder, Andrew H., Peek, Matthew Weldon, Pelham, Patricia A., Penanen, Konstantin, Perriello, Beth A., Perrin, Marshall D., Perrine, Richard F., Perrygo, Chuck, Peslier, Muriel, Petach, Michael, Peterson, Karla A., Pfarr, Tom, Pierson, James M., Pietraszkiewicz, Martin, Pilchen, Guy, Pipher, Judy L., Pirzkal, Norbert, Pitman, Joseph T., Player, Danielle M., Plesha, Rachel, Plitzke, Anja, Pohner, John A., Poletis, Karyn Konstantin, Pollizzi, Joseph A., Polster, Ethan, Pontius, James T., Pontoppidan, Klaus, Porges, Susana C., Potter, Gregg D., Prescott, Stephen, Proffitt, Charles R., Pueyo, Laurent, Neira, Irma Aracely Quispe, Radich, Armando, Rager, Reiko T., Rameau, Julien, Ramey, Deborah D., Alarcon, Rafael Ramos, Rampini, Riccardo, Rapp, Robert, Rashford, Robert A., Rauscher, Bernard J., Ravindranath, Swara, Rawle, Timothy, Rawlings, Tynika N., Ray, Tom, Regan, Michael W., Rehm, Brian, Rehm, Kenneth D., Reid, Neill, Reis, Carl A., Renk, Florian, Reoch, Tom B., Ressler, Michael, Rest, Armin W., Reynolds, Paul J., Richon, Joel G., Richon, Karen V., Ridgaway, Michael, Riedel, Adric Richard, Rieke, George H., Rieke, Marcia, Rifelli, Richard E., Rigby, Jane R., Riggs, Catherine S., Ringel, Nancy J., Ritchie, Christine E., Rix, Hans-Walter, Robberto, Massimo, Robinson, Michael S., Robinson, Orion, Rock, Frank W., Rodriguez, David R., del Pino, Bruno Rodríguez, Roellig, Thomas, Rohrbach, Scott O., Roman, Anthony J., Romelfanger, Frederick J., Romo Jr., Felipe P., Rosales, Jose J., Rose, Perry, Roteliuk, Anthony F., Roth, Marc N., Rothwell, Braden Quinn, Rouzaud, Sylvain, Rowe, Jason, Rowlands, Neil, Roy, Arpita, Royer, Pierre, Rui, Chunlei, Rumler, Peter, Rumpl, William, Russ, Melissa L., Ryan, Michael B., Ryan, Richard M., Saad, Karl, Sabata, Modhumita, Sabatino, Rick, Sabbi, Elena, Sabelhaus, Phillip A., Sabia, Stephen, Sahu, Kailash C., Saif, Babak N., Salvignol, Jean-Christophe, Samara-Ratna, Piyal, Samuelson, Bridget S., Sanders, Felicia A., Sappington, Bradley, Sargent, B. A., Sauer, Arne, Savadkin, Bruce J., Sawicki, Marcin, Schappell, Tina M., Scheffer, Caroline, Scheithauer, Silvia, Scherer, Ron, Schiff, Conrad, Schlawin, Everett, Schmeitzky, Olivier, Schmitz, Tyler S., Schmude, Donald J., Schneider, Analyn, Schreiber, Jürgen, Schroeven-Deceuninck, Hilde, Schultz, John J., Schwab, Ryan, Schwartz, Curtis H., Scoccimarro, Dario, Scott, John F., Scott, Michelle B., Seaton, Bonita L., Seely, Bruce S., Seery, Bernard, Seidleck, Mark, Sembach, Kenneth, Shanahan, Clare Elizabeth, Shaughnessy, Bryan, Shaw, Richard A., Shay, Christopher Michael, Sheehan, Even, Sheth, Kartik, Shih, Hsin-Yi, Shivaei, Irene, Siegel, Noah, Sienkiewicz, Matthew G., Simmons, Debra D., Simon, Bernard P., Sirianni, Marco, Sivaramakrishnan, Anand, Slade, Jeffrey E., Sloan, G. C., Slocum, Christine E., Slowinski, Steven E., Smith, Corbett T., Smith, Eric P., Smith, Erin C., Smith, Koby, Smith, Robert, Smith, Stephanie J., Smolik, John L., Soderblom, David R., Sohn, Sangmo Tony, Sokol, Jeff, Sonneborn, George, Sontag, Christopher D., Sooy, Peter R., Soummer, Remi, Southwood, Dana M., Spain, Kay, Sparmo, Joseph, Speer, David T., Spencer, Richard, Sprofera, Joseph D., Stallcup, Scott S., Stanley, Marcia K., Stansberry, John A., Stark, Christopher C., Starr, Carl W., Stassi, Diane Y., Steck, Jane A., Steeley, Christine D., Stephens, Matthew A., Stephenson, Ralph J., Stewart, Alphonso C., Stiavelli, Massimo, Stockman Jr., Hervey, Strada, Paolo, Straughn, Amber N., Streetman, Scott, Strickland, David Kendal, Strobele, Jingping F., Stuhlinger, Martin, Stys, Jeffrey Edward, Such, Miguel, Sukhatme, Kalyani, Sullivan, Joseph F., Sullivan, Pamela C., Sumner, Sandra M., Sun, Fengwu, Sunnquist, Benjamin Dale, Swade, Daryl Allen, Swam, Michael S., Swenton, Diane F., Swoish, Robby A., Litten, Oi In Tam, Tamas, Laszlo, Tao, Andrew, Taylor, David K., Taylor, Joanna M., Plate, Maurice te, Van Tea, Mason, Teague, Kelly K., Telfer, Randal C., Temim, Tea, Texter, Scott C., Thatte, Deepashri G., Thompson, Christopher Lee, Thompson, Linda M., Thomson, Shaun R., Thronson, Harley, Tierney, C. M., Tikkanen, Tuomo, Tinnin, Lee, Tippet, William Thomas, Todd, Connor William, Tran, Hien D., Trauger, John, Trejo, Edwin Gregorio, Truong, Justin Hoang Vinh, Tsukamoto, Christine L., Tufail, Yasir, Tumlinson, Jason, Tustain, Samuel, Tyra, Harrison, Ubeda, Leonardo, Underwood, Kelli, Uzzo, Michael A., Vaclavik, Steven, Valenduc, Frida, Valenti, Jeff A., Van Campen, Julie, van de Wetering, Inge, Van Der Marel, Roeland P., van Haarlem, Remy, Vandenbussche, Bart, Vanterpool, Dona D., Vernoy, Michael R., Costas, Maria Begoña Vila, Volk, Kevin, Voorzaat, Piet, Voyton, Mark F., Vydra, Ekaterina, Waddy, Darryl J., Waelkens, Christoffel, Wahlgren, Glenn Michael, Walker Jr., Frederick E., Wander, Michel, Warfield, Christine K., Warner, Gerald, Wasiak, Francis C., Wasiak, Matthew F., Wehner, James, Weiler, Kevin R., Weilert, Mark, Weiss, Stanley B., Wells, Martyn, Welty, Alan D., Wheate, Lauren, Wheeler, Thomas P., White, Christy L., Whitehouse, Paul, Whiteleather, Jennifer Margaret, Whitman, William Russell, Williams, Christina C., Willmer, Christopher N. A., Willott, Chris J., Willoughby, Scott P., Wilson, Andrew, Wilson, Debra, Wilson, Donna V., Windhorst, Rogier, Wislowski, Emily Christine, Wolfe, David J., Wolfe, Michael A., Wolff, Schuyler, Wondel, Amancio, Woo, Cindy, Woods, Robert T., Worden, Elaine, Workman, William, Wright, Gillian S., Wu, Carl, Wu, Chi-Rai, Wun, Dakin D., Wymer, Kristen B., Yadetie, Thomas, Yan, Isabelle C., Yang, Keith C., Yates, Kayla L., Yeager, Christopher R., Yerger, Ethan John, Young, Erick T., Young, Gary, Yu, Gene, Yu, Susan, Zak, Dean S., Zeidler, Peter, Zepp, Robert, Zhou, Julia, Zincke, Christian A., Zonak, Stephanie, and Zondag, Elisabeth
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: Twenty-six years ago a small committee report, building on earlier studies, expounded a compelling and poetic vision for the future of astronomy, calling for an infrared-optimized space telescope with an aperture of at least $4m$. With the support of their governments in the US, Europe, and Canada, 20,000 people realized that vision as the $6.5m$ James Webb Space Telescope. A generation of astronomers will celebrate their accomplishments for the life of the mission, potentially as long as 20 years, and beyond. This report and the scientific discoveries that follow are extended thank-you notes to the 20,000 team members. The telescope is working perfectly, with much better image quality than expected. In this and accompanying papers, we give a brief history, describe the observatory, outline its objectives and current observing program, and discuss the inventions and people who made it possible. We cite detailed reports on the design and the measured performance on orbit., Comment: Accepted by PASP for the special issue on The James Webb Space Telescope Overview, 29 pages, 4 figures
Published: 2023
Full Text: View/download PDF

6. Discovery of dusty sub-solar mass young stellar objects in NGC 346 with JWST/NIRCam

Author: Jones, Olivia C., Nally, Conor, Habel, Nolan, Lenkić, Laura, Fahrion, Katja, Hirschauer, Alec S., Chu, Laurie E. U., Meixner, Margaret, De Marchi, Guido, Nayak, Omnarayani, Robberto, Massimo, Sabbi, Elena, Zeidler, Peter, de Oliveira, Catarina Alves, Beck, Tracy, Biazzo, Katia, Brandl, Bernhard, Giardino, Giovanna, Jerabkova, Teresa, Keyes, Charles, Muzerolle, James, Panagia, Nino, Pontoppidan, Klaus M., Rogers, Ciaran, Sargent, B. A., and Soderblom, David R.
Subjects: Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Astrophysics of Galaxies
Abstract: JWST observations of NGC 346, a star-forming region in the metal-poor Small Magellanic Cloud, reveal a substantial population of sub-solar mass young stellar objects (YSOs) with IR excess. We detected $\sim$500 YSOs and pre main sequence (PMS) stars from more than 45,000 unique sources utilizing all four NIRCam wide filters with deep, high-resolution imaging, where ongoing low-mass star formation is concentrated along dust filaments. From these observations, we construct detailed near-IR colour-magnitude diagrams with which preliminary categorizations of YSO classes are made. For the youngest, most deeply-embedded objects, JWST/NIRCam reaches over 10 magnitudes below Spitzer observations at comparable wavelengths, and two magnitudes fainter than HST for more-evolved PMS sources, corresponding to $\sim$0.1 M$_\odot$. For the first time in an extragalactic environment, we detect embedded low-mass star-formation. Furthermore, evidence of IR excess and accretion suggests that dust required for rocky planet formation is present at metallicities as low as 0.2 $Z_\odot$., Comment: 16 pages, 2 figures, Accepted Nature Astronomy
Published: 2023

7. The internal line-of-sight kinematics of NGC 346: the rotation of the core region

Author: Zeidler, Peter, Sabbi, Elena, and Nota, Antonella
Subjects: Astrophysics - Astrophysics of Galaxies
Abstract: We present the stellar radial velocity analysis of the central 1x1' of the young massive Small Magellanic Cloud star cluster NGC 346. Using VLT/MUSE integral field spectroscopy in combination with Hubble Space Telescope photometry we extract 103 spectra of cluster member stars suited to measure accurate line-of-sight kinematics. The cluster member stars show two distinct velocity groups at v1 = -3.3 (+0.3/-0.2) km/s and v2 = 2.6 (+0.1/-0.1) km/s, relative to the systemic velocity of 165.5+/-0.2 km/s, and hint for a third group at v3 = 9.4 (+0.1/-0.1 km/s. We show that there is neither a correlation between the velocity groups and the spatial location of the stars, nor their locus on optical color-magnitude diagrams, which makes the stellar velocity a key parameter to separate individual stellar components in such a young star cluster. Velocity group 2 shows clear rotation with Omega2 = -0.4 +/- 0.1 1/Myr, corresponding to -4.9+/-0.7 km/s at radial distance of 10 pc from the center, a possible remnant of the formation process of NGC 346 through the hierarchical collapse of the giant molecular cloud. The ionizing gas has lost any natal kinematic imprint and shows clear expansion, driven by far ultra violet fluxes and stellar winds of the numerous OB stars in the cluster center. The size of this expanding bubble and its expansion velocity of 7.9 km/s is in excellent agreement with the estimate that the latest star formation episode occurred about two million years ago., Comment: 16 pages, 10 Figures, accepted for publication of ApJ
Published: 2022
Full Text: View/download PDF

8. The In-Flight Noise Performance of the JWST/NIRSpec Detector System

Author: Birkmann, Stephan M., Giardino, Giovanna, Sirianni, Marco, Ferruit, Pierre, Rauscher, Bernhard, de Oliveira, Catarina Alves, Böker, Torsten, Kumari, Nimisha, Lützgendorf, Nora, Manjavacas, Elena, Proffitt, Charles, Rawle, Timothy D., Plate, Maurice te, and Zeidler, Peter
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: The Near-Infrared Spectrograph (NIRSpec) is one the four focal plane instruments on the James Webb Space Telescope (JWST) which was launched on December 25, 2021. We present the in-flight status and performance of NIRSpec's detector system as derived from the instrument commissioning data. The instrument features two 2048 x 2048 HAWAII-2RG sensor chip assemblies (SCAs) that are operated at a temperature of about 42.8 K and are read out via a pair of SIDECAR ASICs. NIRSpec supports "Improved Reference Sampling and Subtraction" (IRS2) readout mode that was designed to meet NIRSpec's stringent noise requirements and to reduce 1/f and correlated noise. In addition, NIRSpec features subarrays optimized for bright object time series observations, e.g. for the observation of exoplanet transit around bright host stars. We focus on the dark signal as well as the read and total noise performance of the detectors., Comment: 12 pages, 7 figures, SPIE Astronomical Telescopes + Instrumentation 2022
Published: 2022

9. Astrometric and Wavelength Calibration of the NIRSpec Instrument during Commissioning using a model-based approach

Author: Lützgendorf, Nora, Giardino, Giovanna, de Oliveira, Catarina Alves, Zeidler, Peter, Ferruit, Pierre, Jakobsen, Peter, Kumari, Nimisha, Rawle, Timothy, Birkmann, Stephan M., Böker, Torsten, Proffitt, Charles, Sirianni, Marco, Plate, Maurice Te, and Sohn, Sangmo Tony
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: The NIRSpec instrument for the James Webb Space Telescope (JWST) is a highly versatile near-infrared spectrograph that can be operated in various observing modes, slit apertures, and spectral resolutions. Obtaining dedicated calibration data for all possible combinations of aperture and disperser is an intractable task. We have therefore developed a procedure to derive a highly realistic model of the instrument's optical geometry across the entire field of view, using calibration data acquired through only a subset of NIRSpec apertures, which nevertheless allows the light paths within the spectrograph to be accurately computed for all apertures and all observing modes. This parametric instrument model thus provides the basis for the extraction of wavelength-calibrated spectra from any NIRSpec exposure, regardless of observing mode or aperture used. Optimizing the NIRSpec instrument model and deriving its final wavelength and astrometric calibration was one of the most crucial elements of the NIRSpec commissioning phase. Here, we describe the process of re-fitting the NIRSpec instrument model with in-orbit commissioning data, and present its final performance in terms of wavelength accuracy and astrometric calibration., Comment: 15 pages, to appear in Proceedings of SPIE conference "Space Telescopes and Instrumentation 2022: Optical, Infrared, and Millimeter Wave"
Published: 2022

10. In-flight performance and calibration of the Grating Wheel Assembly sensors (NIRSpec/JWST)

Author: de Oliveira, Catarina Alves, Luetzgendorf, Nora, Zeidler, Peter, Giardino, Giovanna, Ferruit, Pierre, Kumari, Nimisha, Rawle, Timothy, Birkmann, Stephan M., Boeker, Torsten, Proffitt, Charles, Sirianni, Marco, and Plate, Maurice Te
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: The Near-Infrared Spectrograph (NIRSpec) on board of the James Webb Space Telescope will be the first multi-object spectrograph in space offering ~250,000 configurable micro-shutters, apart from being equipped with an integral field unit and fixed slits. At its heart, the NIRSpec grating wheel assembly is a cryogenic mechanism equipped with six dispersion gratings, a prism, and a mirror. The finite angular positioning repeatability of the wheel causes small but measurable displacements of the light beam on the focal plane, precluding a static solution to predict the light-path. To address that, two magneto-resistive position sensors are used to measure the tip and tilt displacement of the selected GWA element each time the wheel is rotated. The calibration of these sensors is a crucial component of the model-based approach used for NIRSpec for calibration, spectral extraction, and target placement in the micro-shutters. In this paper, we present the results of the evolution of the GWA sensors performance and calibration from ground to space environments., Comment: To appear in Proceedings of SPIE conference "Space Telescopes and Instrumentation 2022: Optical, Infrared, and Millimeter Wave"
Published: 2022

11. In-flight performance of the NIRSpec Micro Shutter Array

Author: Rawle, Timothy D., Giardino, Giovanna, Franz, David E., Rapp, Robert, Plate, Maurice te, Zincke, Christian A., Abul-Huda, Yasin M., de Oliveira, Catarina Alves, Bechtold, Katie, Beck, Tracy, Birkmann, Stephan M., Böker, Torsten, Ehrenwinkler, Ralf, Ferruit, Pierre, Garland, Dennis, Jakobsen, Peter, Karakla, Diane, Karl, Hermann, Keyes, Charles D., Koehler, Robert, Kumari, Nimisha, Lützgendorf, Nora, Manjavacas, Elena, Marston, Anthony, Moseley, S. Harvey, Mosner, Peter, Muzerolle, James, Ogle, Patrick, Proffitt, Charles, Sabbi, Elena, Sirianni, Marco, Wahlgren, Glenn, Wislowski, Emily, Wright, Raymond H., Wu, Chi Rai, and Zeidler, Peter
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: The NIRSpec instrument on the James Webb Space Telescope (JWST) brings the first multi-object spectrograph (MOS) into space, enabled by a programmable Micro Shutter Array (MSA) of ~250,000 individual apertures. During the 6-month Commissioning period, the MSA performed admirably, completing ~800 reconfigurations with an average success rate of ~96% for commanding shutters open in science-like patterns. We show that 82.5% of the unvignetted shutter population is usable for science, with electrical short masking now the primary cause of inoperable apertures. In response, we propose a plan to recheck existing shorts during nominal operations, which is expected to reduce the number of affected shutters. We also present a full assessment of the Failed Open and Failed Closed shutter populations, which both show a marginal increase in line with predictions from ground testing. We suggest an amendment to the Failed Closed shutter flagging scheme to improve flexibility for MSA configuration planning. Overall, the NIRSpec MSA performed very well during Commissioning, and the MOS mode was declared ready for science operations on schedule., Comment: 15 pages, 6 figures, to appear in Proceedings of SPIE conference "Space Telescopes and Instrumentation 2022: Optical, Infrared, and Millimeter Wave"
Published: 2022

12. In-orbit Commissioning of the Near-Infrared Spectrograph on the James Webb Space Telescope

Author: Böker, Torsten, Abul-Huda, Yasin, Altenburg, Martin, de Oliveira, Catarina Alves, Bechtold, Katie, Beck, Tracy, Birkmann, Stephan M., Bonaventura, Nina, Ehrenwinkler, Ralf, Ferruit, Pierre, Franz, David E., Giardino, Giovanna, Jakobsen, Peter, Jensen, Peter, Jollet, Delphine, Karakla, Diane, Karl, Hermann, Keyes, Charles, Kumari, Nimisha, Lander, Matthew, López-Caniego, Marcos, Lützgendorf, Nora, Manjavacas, Elena, Marston, Anthony, Maschmann, Marc, Mosner, Peter, Muzerolle, James, Ogle, Patrick, Guerrero, Maria Pena, Plesha, Rachel, Proffitt, Charles, Rapp, Robert, Rawle, Timothy, Del Pino, Bruno Rodríguez, Sabbi, Elena, Sauer, Arne, Sirianni, Marco, Smith, Corbett, Plate, Maurice te, Wahlgren, Glenn, Wislowski, Emily, Wu, Rai, Zeidler, Peter, and Zincke, Christian A.
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: The Near-Infrared Spectrograph (NIRSpec) is one of the four focal plane instruments on the James Webb Space Telescope which was launched on Dec. 25, 2021. We present an overview of the as-run NIRSpec commissioning campaign, with particular emphasis on the sequence of activities that led to the verification of all hardware components of NIRSpec. We also discuss the mechanical, thermal, and operational performance of NIRSpec, as well as the readiness of all NIRSpec observing modes for use in the upcoming JWST science program., Comment: 10 pages, to appear in Proceedings of SPIE conference "Space Telescopes and Instrumentation 2022: Optical, Infrared, and Millimeter Wave"
Published: 2022

13. The Science Performance of JWST as Characterized in Commissioning

Author: Rigby, Jane, Perrin, Marshall, McElwain, Michael, Kimble, Randy, Friedman, Scott, Lallo, Matt, Doyon, René, Feinberg, Lee, Ferruit, Pierre, Glasse, Alistair, Rieke, Marcia, Rieke, George, Wright, Gillian, Willott, Chris, Colon, Knicole, Milam, Stefanie, Neff, Susan, Stark, Christopher, Valenti, Jeff, Abell, Jim, Abney, Faith, Abul-Huda, Yasin, Acton, D. Scott, Adams, Evan, Adler, David, Aguilar, Jonathan, Ahmed, Nasif, Albert, Loïc, Alberts, Stacey, Aldridge, David, Allen, Marsha, Altenburg, Martin, Marquez, Javier Alvarez, de Oliveira, Catarina Alves, Andersen, Greg, Anderson, Harry, Anderson, Sara, Argyriou, Ioannis, Armstrong, Amber, Arribas, Santiago, Artigau, Etienne, Arvai, Amanda, Atkinson, Charles, Bacon, Gregory, Bair, Thomas, Banks, Kimberly, Barrientes, Jaclyn, Barringer, Bruce, Bartosik, Peter, Bast, William, Baudoz, Pierre, Beatty, Thomas, Bechtold, Katie, Beck, Tracy, Bergeron, Eddie, Bergkoetter, Matthew, Bhatawdekar, Rachana, Birkmann, Stephan, Blazek, Ronald, Blome, Claire, Boccaletti, Anthony, Boeker, Torsten, Boia, John, Bonaventura, Nina, Bond, Nicholas, Bosley, Kari, Boucarut, Ray, Bourque, Matthew, Bouwman, Jeroen, Bower, Gary, Bowers, Charles, Boyer, Martha, Bradley, Larry, Brady, Greg, Braun, Hannah, Breda, David, Bresnahan, Pamela, Bright, Stacey, Britt, Christopher, Bromenschenkel, Asa, Brooks, Brian, Brooks, Keira, Brown, Bob, Brown, Matthew, Brown, Patricia, Bunker, Andy, Burger, Matthew, Bushouse, Howard, Cale, Steven, Cameron, Alex, Cameron, Peter, Canipe, Alicia, Caplinger, James, Caputo, Francis, Cara, Mihai, Carey, Larkin, Carniani, Stefano, Carrasquilla, Maria, Carruthers, Margaret, Case, Michael, Catherine, Riggs, Chance, Don, Chapman, George, Charlot, Stéphane, Charlow, Brian, Chayer, Pierre, Chen, Bin, Cherinka, Brian, Chichester, Sarah, Chilton, Zack, Chonis, Taylor, Clampin, Mark, Clark, Charles, Clark, Kerry, Coe, Dan, Coleman, Benee, Comber, Brian, Comeau, Tom, Connolly, Dennis, Cooper, James, Cooper, Rachel, Coppock, Eric, Correnti, Matteo, Cossou, Christophe, Coulais, Alain, Coyle, Laura, Cracraft, Misty, Curti, Mirko, Cuturic, Steven, Davis, Katherine, Davis, Michael, Dean, Bruce, DeLisa, Amy, deMeester, Wim, Dencheva, Nadia, Dencheva, Nadezhda, DePasquale, Joseph, Deschenes, Jeremy, Detre, Örs Hunor, Diaz, Rosa, Dicken, Dan, DiFelice, Audrey, Dillman, Matthew, Dixon, William, Doggett, Jesse, Donaldson, Tom, Douglas, Rob, DuPrie, Kimberly, Dupuis, Jean, Durning, John, Easmin, Nilufar, Eck, Weston, Edeani, Chinwe, Egami, Eiichi, Ehrenwinkler, Ralf, Eisenhamer, Jonathan, Eisenhower, Michael, Elie, Michelle, Elliott, James, Elliott, Kyle, Ellis, Tracy, Engesser, Michael, Espinoza, Nestor, Etienne, Odessa, Etxaluze, Mireya, Falini, Patrick, Feeney, Matthew, Ferry, Malcolm, Filippazzo, Joseph, Fincham, Brian, Fix, Mees, Flagey, Nicolas, Florian, Michael, Flynn, Jim, Fontanella, Erin, Ford, Terrance, Forshay, Peter, Fox, Ori, Franz, David, Fu, Henry, Fullerton, Alexander, Galkin, Sergey, Galyer, Anthony, Marin, Macarena Garcia, Gardner, Jonathan, Gardner, Lisa, Garland, Dennis, Garrett, Bruce, Gasman, Danny, Gaspar, Andras, Gaudreau, Daniel, Gauthier, Peter, Geers, Vincent, Geithner, Paul, Gennaro, Mario, Giardino, Giovanna, Girard, Julien, Giuliano, Mark, Glassmire, Kirk, Glauser, Adrian, Glazer, Stuart, Godfrey, John, Golimowski, David, Gollnitz, David, Gong, Fan, Gonzaga, Shireen, Gordon, Michael, Gordon, Karl, Goudfrooij, Paul, Greene, Thomas, Greenhouse, Matthew, Grimaldi, Stefano, Groebner, Andrew, Grundy, Timothy, Guillard, Pierre, Gutman, Irvin, Ha, Kong Q., Haderlein, Peter, Hagedorn, Andria, Hainline, Kevin, Haley, Craig, Hami, Maryam, Hamilton, Forrest, Hammel, Heidi, Hansen, Carl, Harkins, Tom, Harr, Michael, Hart, Jessica, Hart, Quyen, Hartig, George, Hashimoto, Ryan, Haskins, Sujee, Hathaway, William, Havey, Keith, Hayden, Brian, Hecht, Karen, Heller-Boyer, Chris, Henriques, Caroline, Henry, Alaina, Hermann, Karl, Hernandez, Scarlin, Hesman, Brigette, Hicks, Brian, Hilbert, Bryan, Hines, Dean, Hoffman, Melissa, Holfeltz, Sherie, Holler, Bryan J., Hoppa, Jennifer, Hott, Kyle, Howard, Joseph, Howard, Rick, Hunter, Alexander, Hunter, David, Hurst, Brendan, Husemann, Bernd, Hustak, Leah, Ignat, Luminita Ilinca, Illingworth, Garth, Irish, Sandra, Jackson, Wallace, Jahromi, Amir, Jakobsen, Peter, James, LeAndrea, James, Bryan, Januszewski, William, Jenkins, Ann, Jirdeh, Hussein, Johnson, Phillip, Johnson, Timothy, Jones, Vicki, Jones, Ron, Jones, Danny, Jones, Olivia, Jordan, Ian, Jordan, Margaret, Jurczyk, Sarah, Jurling, Alden, Kaleida, Catherine, Kalmanson, Phillip, Kammerer, Jens, Kang, Huijo, Kao, Shaw-Hong, Karakla, Diane, Kavanagh, Patrick, Kelly, Doug, Kendrew, Sarah, Kennedy, Herbert, Kenny, Deborah, Keski-kuha, Ritva, Keyes, Charles, Kidwell, Richard, Kinzel, Wayne, Kirk, Jeff, Kirkpatrick, Mark, Kirshenblat, Danielle, Klaassen, Pamela, Knapp, Bryan, Knight, J. Scott, Knollenberg, Perry, Koehler, Robert, Koekemoer, Anton, Kovacs, Aiden, Kulp, Trey, Kumari, Nimisha, Kyprianou, Mark, La Massa, Stephanie, Labador, Aurora, Ortega, Alvaro Labiano, Lagage, Pierre-Olivier, Lajoie, Charles-Phillipe, Lallo, Matthew, Lam, May, Lamb, Tracy, Lambros, Scott, Lampenfield, Richard, Langston, James, Larson, Kirsten, Law, David, Lawrence, Jon, Lee, David, Leisenring, Jarron, Lepo, Kelly, Leveille, Michael, Levenson, Nancy, Levine, Marie, Levy, Zena, Lewis, Dan, Lewis, Hannah, Libralato, Mattia, Lightsey, Paul, Link, Miranda, Liu, Lily, Lo, Amy, Lockwood, Alexandra, Logue, Ryan, Long, Chris, Long, Douglas, Loomis, Charles, Lopez-Caniego, Marcos, Alvarez, Jose Lorenzo, Love-Pruitt, Jennifer, Lucy, Adrian, Luetzgendorf, Nora, Maghami, Peiman, Maiolino, Roberto, Major, Melissa, Malla, Sunita, Malumuth, Eliot, Manjavacas, Elena, Mannfolk, Crystal, Marrione, Amanda, Marston, Anthony, Martel, André, Maschmann, Marc, Masci, Gregory, Masciarelli, Michaela, Maszkiewicz, Michael, Mather, John, McKenzie, Kenny, McLean, Brian, McMaster, Matthew, Melbourne, Katie, Meléndez, Marcio, Menzel, Michael, Merz, Kaiya, Meyett, Michele, Meza, Luis, Miskey, Cherie, Misselt, Karl, Moller, Christopher, Morrison, Jane, Morse, Ernie, Moseley, Harvey, Mosier, Gary, Mountain, Matt, Mueckay, Julio, Mueller, Michael, Mullally, Susan, Murphy, Jess, Murray, Katherine, Murray, Claire, Mustelier, David, Muzerolle, James, Mycroft, Matthew, Myers, Richard, Myrick, Kaila, Nanavati, Shashvat, Nance, Elizabeth, Nayak, Omnarayani, Naylor, Bret, Nelan, Edmund, Nickson, Bryony, Nielson, Alethea, Nieto-Santisteban, Maria, Nikolov, Nikolay, Noriega-Crespo, Alberto, O'Shaughnessy, Brian, O'Sullivan, Brian, Ochs, William, Ogle, Patrick, Oleszczuk, Brenda, Olmsted, Joseph, Osborne, Shannon, Ottens, Richard, Owens, Beverly, Pacifici, Camilla, Pagan, Alyssa, Page, James, Park, Sang, Parrish, Keith, Patapis, Polychronis, Paul, Lee, Pauly, Tyler, Pavlovsky, Cheryl, Pedder, Andrew, Peek, Matthew, Pena-Guerrero, Maria, Pennanen, Konstantin, Perez, Yesenia, Perna, Michele, Perriello, Beth, Phillips, Kevin, Pietraszkiewicz, Martin, Pinaud, Jean-Paul, Pirzkal, Norbert, Pitman, Joseph, Piwowar, Aidan, Platais, Vera, Player, Danielle, Plesha, Rachel, Pollizi, Joe, Polster, Ethan, Pontoppidan, Klaus, Porterfield, Blair, Proffitt, Charles, Pueyo, Laurent, Pulliam, Christine, Quirt, Brian, Neira, Irma Quispe, Alarcon, Rafael Ramos, Ramsay, Leah, Rapp, Greg, Rapp, Robert, Rauscher, Bernard, Ravindranath, Swara, Rawle, Timothy, Regan, Michael, Reichard, Timothy A., Reis, Carl, Ressler, Michael E., Rest, Armin, Reynolds, Paul, Rhue, Timothy, Richon, Karen, Rickman, Emily, Ridgaway, Michael, Ritchie, Christine, Rix, Hans-Walter, Robberto, Massimo, Robinson, Gregory, Robinson, Michael, Robinson, Orion, Rock, Frank, Rodriguez, David, Del Pino, Bruno Rodriguez, Roellig, Thomas, Rohrbach, Scott, Roman, Anthony, Romelfanger, Fred, Rose, Perry, Roteliuk, Anthony, Roth, Marc, Rothwell, Braden, Rowlands, Neil, Roy, Arpita, Royer, Pierre, Royle, Patricia, Rui, Chunlei, Rumler, Peter, Runnels, Joel, Russ, Melissa, Rustamkulov, Zafar, Ryden, Grant, Ryer, Holly, Sabata, Modhumita, Sabatke, Derek, Sabbi, Elena, Samuelson, Bridget, Sapp, Benjamin, Sappington, Bradley, Sargent, B., Sauer, Arne, Scheithauer, Silvia, Schlawin, Everett, Schlitz, Joseph, Schmitz, Tyler, Schneider, Analyn, Schreiber, Jürgen, Schulze, Vonessa, Schwab, Ryan, Scott, John, Sembach, Kenneth, Shanahan, Clare, Shaughnessy, Bryan, Shaw, Richard, Shawger, Nanci, Shay, Christopher, Sheehan, Evan, Shen, Sharon, Sherman, Allan, Shiao, Bernard, Shih, Hsin-Yi, Shivaei, Irene, Sienkiewicz, Matthew, Sing, David, Sirianni, Marco, Sivaramakrishnan, Anand, Skipper, Joy, Sloan, Gregory, Slocum, Christine, Slowinski, Steven, Smith, Erin, Smith, Eric, Smith, Denise, Smith, Corbett, Snyder, Gregory, Soh, Warren, Sohn, Tony, Soto, Christian, Spencer, Richard, Stallcup, Scott, Stansberry, John, Starr, Carl, Starr, Elysia, Stewart, Alphonso, Stiavelli, Massimo, Straughn, Amber, Strickland, David, Stys, Jeff, Summers, Francis, Sun, Fengwu, Sunnquist, Ben, Swade, Daryl, Swam, Michael, Swaters, Robert, Swoish, Robby, Taylor, Joanna M., Taylor, Rolanda, Plate, Maurice Te, Tea, Mason, Teague, Kelly, Telfer, Randal, Temim, Tea, Thatte, Deepashri, Thompson, Christopher, Thompson, Linda, Thomson, Shaun, Tikkanen, Tuomo, Tippet, William, Todd, Connor, Toolan, Sharon, Tran, Hien, Trejo, Edwin, Truong, Justin, Tsukamoto, Chris, Tustain, Samuel, Tyra, Harrison, Ubeda, Leonardo, Underwood, Kelli, Uzzo, Michael, Van Campen, Julie, Vandal, Thomas, Vandenbussche, Bart, Vila, Begoña, Volk, Kevin, Wahlgren, Glenn, Waldman, Mark, Walker, Chanda, Wander, Michel, Warfield, Christine, Warner, Gerald, Wasiak, Matthew, Watkins, Mitchell, Weaver, Andrew, Weilert, Mark, Weiser, Nick, Weiss, Ben, Weissman, Sarah, Welty, Alan, West, Garrett, Wheate, Lauren, Wheatley, Elizabeth, Wheeler, Thomas, White, Rick, Whiteaker, Kevin, Whitehouse, Paul, Whiteleather, Jennifer, Whitman, William, Williams, Christina, Willmer, Christopher, Willoughby, Scott, Wilson, Andrew, Wirth, Gregory, Wislowski, Emily, Wolf, Erin, Wolfe, David, Wolff, Schuyler, Workman, Bill, Wright, Ray, Wu, Carl, Wu, Rai, Wymer, Kristen, Yates, Kayla, Yeager, Christopher, Yeates, Jared, Yerger, Ethan, Yoon, Jinmi, Young, Alice, Yu, Susan, Zak, Dean, Zeidler, Peter, Zhou, Julia, Zielinski, Thomas, Zincke, Cristian, and Zonak, Stephanie
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: This paper characterizes the actual science performance of the James Webb Space Telescope (JWST), as determined from the six month commissioning period. We summarize the performance of the spacecraft, telescope, science instruments, and ground system, with an emphasis on differences from pre-launch expectations. Commissioning has made clear that JWST is fully capable of achieving the discoveries for which it was built. Moreover, almost across the board, the science performance of JWST is better than expected; in most cases, JWST will go deeper faster than expected. The telescope and instrument suite have demonstrated the sensitivity, stability, image quality, and spectral range that are necessary to transform our understanding of the cosmos through observations spanning from near-earth asteroids to the most distant galaxies., Comment: 5th version as accepted to PASP; 31 pages, 18 figures; https://iopscience.iop.org/article/10.1088/1538-3873/acb293
Published: 2022
Full Text: View/download PDF

14. The impact of pre-supernova feedback and its dependence on environment

Author: Mcleod, Anna F., Ali, Ahmad A., Chevance, Mélanie, Della Bruna, Lorenza, Schruba, Andreas, Stevance, Heloise F., Adamo, Angela, Kruijssen, J. M. Diederik, Longmore, Steven N., Weisz, Daniel R., and Zeidler, Peter
Subjects: Astrophysics - Astrophysics of Galaxies
Abstract: Integral field units enable resolved studies of a large number of star-forming regions across entire nearby galaxies, providing insight on the conversion of gas into stars and the feedback from the emerging stellar populations over unprecedented dynamic ranges in terms of spatial scale, star-forming region properties, and environments. We use the VLT/MUSE legacy data set covering the central $35$ arcmin$^{2}$ (${\sim}12$ kpc$^{2}$) of the nearby galaxy NGC 300 to quantify the effect of stellar feedback as a function of the local galactic environment. We extract spectra from emission line regions identified within dendrograms, combine emission line ratios and line widths to distinguish between HII regions, planetary nebulae, and supernova remnants, and compute their ionised gas properties, gas-phase oxygen abundances, and feedback-related pressure terms. For the HII regions, we find that the direct radiation pressure ($P_\mathrm{dir}$) and the pressure of the ionised gas ($P_{HII}$) weakly increase towards larger galactocentric radii, i.e. along the galaxy's (negative) abundance and (positive) extinction gradients. While the increase of $P_{HII}$ with galactocentric radius is likely due to higher photon fluxes from lower-metallicity stellar populations, we find that the increase of $P_\mathrm{dir}$ is likely driven by the combination of higher photon fluxes and enhanced dust content at larger galactocentric radii. In light of the above, we investigate the effect of increased pre-supernova feedback at larger galactocentric distances (lower metallicities and increased dust mass surface density) on the ISM, finding that supernovae at lower metallicities expand into lower-density environments, thereby enhancing the impact of supernova feedback., Comment: Accepted for publication in MNRAS
Published: 2021
Full Text: View/download PDF

15. JWST/NIRCam detections of dusty subsolar-mass young stellar objects in the Small Magellanic Cloud

Author: Jones, Olivia C., Nally, Conor, Habel, Nolan, Lenkić, Laura, Fahrion, Katja, Hirschauer, Alec S., Chu, Laurie E. U., Meixner, Margaret, De Marchi, Guido, Nayak, Omnarayani, Robberto, Massimo, Sabbi, Elena, Zeidler, Peter, Alves de Oliveira, Catarina, Beck, Tracy, Biazzo, Katia, Brandl, Bernhard, Giardino, Giovanna, Jerabkova, Teresa, Keyes, Charles, Muzerolle, James, Panagia, Nino, Pontoppidan, Klaus, Rogers, Ciaran, Sargent, B. A., and Soderblom, David
Published: 2023
Full Text: View/download PDF

16. The young massive star cluster Westerlund 2 observed with MUSE. III. A cluster in motion -- the complex internal dynamics

Author: Zeidler, Peter, Sabbi, Elena, Nota, Antonella, and McLeod, Anna F.
Subjects: Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Astrophysics of Galaxies
Abstract: Analyzing the dynamical state of nearby young massive star clusters is essential understanding star cluster formation and evolution during their earliest stages. In this work we analyze the stellar and gas kinematics of the young massive star cluster Westerlund 2 (Wd2) using data from the integral field unit MUSE and complement them with proper motions from the Gaia DR2. The mean gas radial velocity of $15.9\,{\rm km}\,{\rm s}^{-1}$ agrees with the assumption that Wd2 is the result of a cloud-cloud collision. The gas motions show the expansion of the HII region, driven by the radiation from the many OB stars in the cluster center. The velocity profile of the cluster member stars reveal an increasing velocity dispersion with decreasing stellar mass and that the low-mass stars show five distinct velocity groups. Based on their spatial correlation with the cluster's two clumps, we concluded that this is the imprint of the initial cloud collapse that formed Wd2. A thorough analysis of the dynamical state of Wd2, which determines a dynamical mass range of $M_{\rm dyn,Wd2} = (7.5 \pm 1.9)\cdot10^4 - (4.4 \pm 1.1)\cdot10^5\,{\rm M}_\odot$ and exceeds the photometric mass by at least a factor of two leads to the conclusion that Wd2 is not massive enough to remain gravitationally bound. Additionally we also identify 22 runaway candidates with peculiar velocities between 30 and $546\,{\rm km}\,{\rm s}^{-1}$., Comment: 23 pages, 14 figures, 4 tables, accepted to AJ
Published: 2021
Full Text: View/download PDF

17. Stellar Parameter Determination from Photometry using Invertible Neural Networks

Author: Ksoll, Victor F., Ardizzone, Lynton, Klessen, Ralf, Koethe, Ullrich, Sabbi, Elena, Robberto, Massimo, Gouliermis, Dimitrios, Rother, Carsten, Zeidler, Peter, and Gennaro, Mario
Subjects: Astrophysics - Solar and Stellar Astrophysics
Abstract: Photometric surveys with the Hubble Space Telescope (HST) allow us to study stellar populations with high resolution and deep coverage, with estimates of the physical parameters of the constituent stars being typically obtained by comparing the survey data with adequate stellar evolutionary models. This is a highly non-trivial task due to effects such as differential extinction, photometric errors, low filter coverage, or uncertainties in the stellar evolution calculations. These introduce degeneracies that are difficult to detect and break. To improve this situation, we introduce a novel deep learning approach, called conditional invertible neural network (cINN), to solve the inverse problem of predicting physical parameters from photometry on an individual star basis and to obtain the full posterior distributions. We build a carefully curated synthetic training data set derived from the PARSEC stellar evolution models to predict stellar age, initial/current mass, luminosity, effective temperature and surface gravity. We perform tests on synthetic data from the MIST and Dartmouth models, and benchmark our approach on HST data of two well-studied stellar clusters, Westerlund 2 and NGC 6397. For the synthetic data we find overall excellent performance, and note that age is the most difficult parameter to constrain. For the benchmark clusters we retrieve reasonable results and confirm previous findings for Westerlund 2 on cluster age ($1.04_{-0.90}^{+8.48}\,\mathrm{Myr} $), mass segregation, and the stellar initial mass function. For NGC 6397 we recover plausible estimates for masses, luminosities and temperatures, however, discrepancies between stellar evolution models and observations prevent an acceptable recovery of age for old stars., Comment: Accepted for Publication by MNRAS on 19. September, 41 pages, 48 figures, 2 tables
Published: 2020
Full Text: View/download PDF

18. Star clusters near and far; tracing star formation across cosmic time

Author: Adamo, Angela, Zeidler, Peter, Kruijssen, J. M. Diederik, Chevance, Mélanie, Gieles, Mark, Calzetti, Daniela, Charbonnel, Corinne, Zinnecker, Hans, and Krause, Martin G. H.
Subjects: Astrophysics - Astrophysics of Galaxies
Abstract: Star clusters are fundamental units of stellar feedback and unique tracers of their host galactic properties. In this review, we will first focus on their constituents, i.e.\ detailed insight into their stellar populations and their surrounding ionised, warm, neutral, and molecular gas. We, then, move beyond the Local Group to review star cluster populations at various evolutionary stages, and in diverse galactic environmental conditions accessible in the local Universe. At high redshift, where conditions for cluster formation and evolution are more extreme, we are only able to observe the integrated light of a handful of objects that we believe will become globular clusters. We therefore discuss how numerical and analytical methods, informed by the observed properties of cluster populations in the local Universe, are used to develop sophisticated simulations potentially capable of disentangling the genetic map of galaxy formation and assembly that is carried by globular cluster populations., Comment: Final published version. 61 pages, 10 figures. To appear in Space Science Reviews (submitted January 31, 2020; accepted May 8, 2020), topical collection Star formation
Published: 2020
Full Text: View/download PDF

19. Original use of MUSE's laser tomography adaptive optics to directly image young accreting exoplanets

Author: Girard, Julien H., de Boer, Jozua, Haffert, Sebastiaan, Zeidler, Peter, Bohn, Alexander, van Holstein, Rob G., Snellen, Ignas, Brinchmann, Jarle, Keller, Christoph, Bacon, Roland, and Bae, Jaehan
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics
Abstract: We present recent results obtained with the VLT/MUSE Integral Field Spectrograph fed by the 4LGSF and its laser tomography adaptive optics module GALACSI. While this so-called narrow-field mode of MUSE was not designed to perform directly imaging of exoplanets and outflows, we show that it can be a game changer to detect and characterize young exoplanets with a prominent emission lines (i.e H{\alpha}, tracer of accretion), at moderate contrasts. These performances are achieved thanks to the combo of a near-diffraction limited PSF and a medium resolution spectrograph and a cross-correlation approach in post-processing . We discuss this in the context of ground and space, infrared and visible wavelengths, preparing for missions like JWST and WFIRST in great synergy and as pathfinder for future ELT/GSMT (Extremely Large and/or Giant Segmented Mirror Telescopes) instruments., Comment: AO4ELT6 Conference Proceedings (2019), 12 pages, 6 figures (http://ao4elt6.copl.ulaval.ca/proceedings.html)
Published: 2020

20. Stellar Feedback and Resolved Stellar IFU Spectroscopy in the nearby Spiral Galaxy NGC 300

Author: McLeod, Anna F., Kruijssen, J. M. Diederik, Weisz, Daniel R., Zeidler, Peter, Schruba, Andreas, Dalcanton, Julianne J., Longmore, Steven N., Chevance, Mélanie, Faesi, Christopher M., and Byler, Nell
Subjects: Astrophysics - Astrophysics of Galaxies
Abstract: We present MUSE Integral Field Unit (IFU) observations of five individual HII regions in two giant (>100 pc in radius) star-forming complexes in the low-metallicity ($Z$~0.33 $Z_{\odot}$) nearby (D ~ 2 Mpc) dwarf spiral galaxy NGC 300. We combine the IFU data with high spatial resolution HST photometry to demonstrate the extraction of stellar spectra and the classification of individual stars from ground-based data at the distance of 2 Mpc. For the two star-forming complexes, in which no O-type stars had previously been identified, we find a total of 13 newly identified O-type stars in the mass range 15-50 M$_{\odot}$, as well as 4 Wolf-Rayet stars. We use the derived massive stellar content to analyze the impact of stellar feedback on the HII regions. As already found for HII regions in the Magellanic Clouds, the dynamics of the analyzed NGC 300 HII regions are dominated by a combination of the pressure of the ionized gas and stellar winds. By comparing the derived ionized gas mass loading factors to the total gas mass loading factor across the NGC 300 disk, we find that the latter is an order of magnitude higher, either indicating very early evolutionary stages for these HII regions, or being a direct result of the multi-phase nature of feedback-driven bubbles. Moreover, we analyze the relation between the star formation rate and the pressure of the ionized gas as derived from small (<100 pc) scales, as both quantities are systematically overestimated when derived on galactic scales. With the wealth of ongoing and upcoming IFU instruments and programs, this study serves as a pathfinder for the systematic investigation of resolved stellar feedback in nearby galaxies, and it delivers the necessary analysis tools to enable massive stellar content and feedback studies sampling an unprecedented range of HII region properties across entire galaxies in the nearby Universe., Comment: Accepted for publication in ApJ
Published: 2019
Full Text: View/download PDF

21. The young massive star cluster Westerlund 2 observed with MUSE. II. MUSEpack -- a Python package to analyze the kinematics of young star clusters

Author: Zeidler, Peter, Nota, Antonella, Sabbi, Elena, Luljak, Peter, McLeod, Anna F., Grebel, Eva K., Pasquali, Anna, and Tosi, Monica
Subjects: Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Astrophysics of Galaxies, Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: We mapped the Galactic young massive star cluster Westerlund 2 (Wd2) with the integral field spectrograph MUSE (spatial resolution: 0.2arcsec/px, spectral resolution: $\Delta \lambda$ = 1.25A, wavelength range 4600-9350A) mounted on the VLT, as part of an on-going study to measure the stellar and gas kinematics of the cluster region. In this paper we present the fully reduced dataset and introduce our new Python package "MUSEpack", which we developed to measure stellar radial velocities with an absolute precision of 1-2km/s without the necessity of a spectral template library. This novel method uses the two-dimensional spectra and an atomic transition line library to create templates around strong absorption lines for each individual star. The code runs fully automatically on multi-core machines, which makes it possible to efficiently determine stellar radial velocities of a large number of stars with the necessary precision to measure the velocity dispersion of young star clusters. MUSEpack also provides an enhanced method for removing telluric lines in crowded fields without sky exposures and a Python wrapper for ESO's data reduction pipeline. We observed Wd2 with a total of 11 short and 5 long exposures to cover the bright nebular emission and OB stars, as well as the fainter pre-main sequence stars down to ~1M$_\odot$. The survey covers an area of ~11arcmin$^2$ (15.8pc$^2$). In total, we extracted 1,725 stellar spectra with a mean S/N>5 per pixel. A typical radial velocity (RV) uncertainty of 4.78km/s, 2.92km/s, and 1.1km/s is reached for stars with a mean S/N>10, S/N>20, S/N>50 per pixel, respectively. Depending on the number of spectral lines used to measure the RVs, it is possible to reach RV accuracies of 0.9km/s, 1.3km/s, and 2.2km/s with $\geq5$, 3-4, and 1-2 spectral lines, respectively. The combined statistical uncertainty on the radial velocity measurements is 1.10km/s., Comment: accepted to AJ; 19 pages, 10 figures, 4 tables; MUSEpack is available from https://github.com/pzeidler89/MUSEpack; The documentation can be found on: https://musepack.readthedocs.io/en/latest/index.html
Published: 2019
Full Text: View/download PDF

22. Astro2020 Science White Paper: Spatially Resolved UV Nebular Diagnostics in Star-Forming Galaxies

Author: James, Bethan, Berg, Danielle, Bordoloi, Rongmon, Byler, Nell, Chisholm, John, Erb, Dawn, Hathi, Nimish, Hayes, Matthew, Henry, Alaina, Jaskot, Anne, Kewley, Lisa, Oey, Sally, Peeples, Molly, Ravindranath, Swara, Rigby, Jane, Scarlata, Claudia, Stark, Daniel, Tumlinson, Jason, and Zeidler, Peter
Subjects: Astrophysics - Astrophysics of Galaxies
Abstract: Diagnosing the physical and chemical conditions within star-forming galaxies (SFGs) is of paramount importance to understanding key components of galaxy formation and evolution: star-formation, gas enrichment, outflows, and accretion. Well established optical emission-line diagnostics used to discern such properties (i.e., metal content, density, strength/shape of ionizing radiation) will be observationally inaccessible for the earliest galaxies, emphasizing the need for robust, reliable interstellar medium (ISM) diagnostics at ultraviolet (UV) wavelengths. Calibrating these UV diagnostics requires a comprehensive comparison of the UV and optical emission lines in nearby SFGs. Optical integral field unit (IFU) surveys have revealed the inhomogeneous nature of the ISM in SFGs, which leads to non-systematic biases in the interpretation of unresolved sources. Spatial variations are especially important to consider at UV wavelengths, where the strongest emission features originate from only the highest excitation regions of the nebula and are challenging to distinguish from competing high-ionization sources (e.g., shocks, AGN, etc.). Since surveys collecting large-scale optical integral field unit (IFU) spectroscopy are already underway, this white paper calls for an IFU or multi-object far-UV (FUV) spectroscopic instrument with high sensitivity, high spatial resolution, and large field of view (FoV). Given the impact of large-scale optical IFU surveys over the past decade, this white paper emphasizes the scientific need for a comparable foundation of spatially-resolved far-UV spectroscopy survey of nearby galaxies that will lay the foundation of diagnostics critical to the interpretation of the distant universe., Comment: Astro2020 White Paper
Published: 2019

23. The young massive star cluster Westerlund 2 observed with MUSE. I. First results on the cluster internal motion from stellar radial velocities

Author: Zeidler, Peter, Sabbi, Elena, Nota, Antonella, Pasquali, Anna, Grebel, Eva K., McLeod, Anna Faye, Kamann, Sebastian, Tosi, Monica, Cignoni, Michele, and Ramsey, Suzanne
Subjects: Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Astrophysics of Galaxies
Abstract: Westerlund 2 (Wd2) is the central ionizing star cluster of the \ion{H}{2} region RCW~49 and the second most massive young star cluster (${\rm M} = (3.6 \pm 0.3)\times 10^4\,{\rm M}_\odot$) in the Milky Way. Its young age ($\sim2\,$Myr) and close proximity to the Sun ($\sim 4\,$kpc) makes it a perfect target to study stars emerging from their parental gas cloud, the large number of OB-stars and their feedback onto the gas, and the gas dynamics. We combine high-resolution multi-band photometry obtained in the optical and near-infrared with the \textit{Hubble} Space Telescope (HST), and VLT/MUSE integral field spectroscopy to study the gas, the stars, and their interactions, simultaneously. In this paper we focus on a small, $64\times64\,{\rm arcsec}^2$ region North of the main cluster center, which we call the Northern Bubble (NB), a circular cavity carved into the gas of the cluster region. Using MUSE data, we determined the spectral types of 17 stars in the NB from G9III to O7.5. With the estimation of these spectral types we add 2 O and 5 B-type stars to the previously published census of 37 OB-stars in Wd2. To measure radial velocities we extracted 72 stellar spectra throughout Wd2, including the 17 of the NB, and show that the cluster member stars follow a bimodal velocity distribution centered around $(8.10 \pm 1.53)\,{\rm km}\,{\rm s}^{-1}$ and $(25.41 \pm 1.57)\,{\rm km}\,{\rm s}^{-1}$ with a dispersion of $(4.52 \pm 1.78)\,{\rm km}\,{\rm s}^{-1}$ and $(3.46 \pm 1.29)\,{\rm km}\,{\rm s}^{-1}$, respectively. These are in agreement with CO($J=1$-2) studies of RCW~49 leaving cloud-cloud collision as a viable option for the formation scenario of Wd2. The bimodal distribution is also detected in the Gaia DR2 proper motions., Comment: 20 pages, 11 figures, 3 tables
Published: 2018
Full Text: View/download PDF

24. A High-Resolution Multiband Survey of Westerlund 2 With the Hubble Space Telescope. III. The present-day stellar mass function

Author: Zeidler, Peter, Nota, Antonella, Grebel, Eva K., Sabbi, Elena, Pasquali, Anna, Tosi, Monica, and Christian, Carol
Subjects: Astrophysics - Astrophysics of Galaxies, Astrophysics - Solar and Stellar Astrophysics
Abstract: We present a detailed analysis of the spatial distribution of the stellar population and the present-day mass function (PDMF) of the Westerlund 2 (Wd2) region using the data from our high resolution multi-band survey with the Hubble Space Telescope. We used state-of-the-art artificial star tests to determine spatially resolved completeness maps for each of the broad-band filters. We reach a level of completeness of 50 % down to F555W=24.8 mag (0.7 $M_\odot$) and F814W=23.3 mag (0.2 $M_\odot$) in the optical and F125W=20.2 mag and F160W=19.4 mag (both 0.12 $M_\odot$) in the infrared throughout the field of view. We had previously reported that the core of Wd2 consists of two clumps: namely the main cluster (MC) and the northern clump (NC). From the spatial distribution of the completeness corrected population, we find that their stellar surface densities are 1114 stars pc$^{-2}$ and 555 stars pc$^{-2}$, respectively, down to F814W=21.8 mag. We find that the present-day mass function (PDMF) of Wd2 has a slope of $\Gamma=-1.46 \pm 0.06$, which translates to a total stellar cluster mass of $(3.6 \pm 0.3) \cdot 10^4 M_\odot$. The spatial analysis of the PDMF reveals that the cluster population is mass-segregated, most likely primordial. In addition, we report the detection of a stellar population of spatially uniformly distributed low-mass (<0.15 $M_\odot$) stars, extending into the gas ridges of the surrounding gas and dust cloud, as well as a confined region of reddened stars, likely caused by a foreground CO cloud. We find hints that a cloud-cloud collision might be the origin of the formation of Wd2., Comment: 21 pages, 9 figures, 5 tables, accepted to AJ
Published: 2017
Full Text: View/download PDF

25. Exploring the Mpc Environment of the Quasar ULAS J1342+0928 at z = 7.54

Author: Rojas-Ruiz, Sofía, primary, Mazzucchelli, Chiara, additional, Finkelstein, Steven L., additional, Bañados, Eduardo, additional, Farina, Emanuele Paolo, additional, Venemans, Bram P., additional, Decarli, Roberto, additional, Willott, Chris J., additional, Wang, Feige, additional, Walter, Fabian, additional, Congiu, Enrico, additional, Brammer, Gabriel, additional, and Zeidler, Peter, additional
Published: 2024
Full Text: View/download PDF

26. A High-Resolution Multiband Survey of Westerlund 2 With the Hubble Space Telescope. II. Mass accretion in the Pre-Main Sequence Population

Author: Zeidler, Peter, Grebel, Eva K., Nota, Antonella, Sabbi, Elena, Pasquali, Anna, Tosi, Monica, Bonanos, Alceste Z., and Christian, Carol
Subjects: Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Astrophysics of Galaxies
Abstract: We present a detailed analysis of the pre-main-sequence (PMS) population of the young star cluster Westerlund~2 (Wd2), the central ionizing cluster of the HII region RCW 49, using data from a high resolution multi-band survey with the Hubble Space Telescope. The data were acquired with the Advanced Camera for Surveys in the F555W, F814W, and F658N filters and with the Wide Field Camera 3 in the F125W, F160W, and F128N filters. We find a mean age of the region of 1.04+-0.72 Myr. The combination of dereddened F555W and F814W photometry in combination with F658N photometry allows us to study and identify stars with H_alpha excess emission. With a careful selection of 240 bona-fide PMS H_alpha excess emitters we were able to determine their H_alpha luminosity, which has a mean value L(H_alpha)=1.67 x 10^{-31} erg s^{-1}. Using the PARSEC 1.2S isochrones to obtain the stellar parameters of the PMS stars we determined a mean mass accretion rate \dot M_acc=4.43 x 10^{-8} M_sun yr^{-1} per star. A careful analysis of the spatial dependence of the mass-accretion rate suggests that this rate is ~25% lower in center of the two density peaks of Wd2 in close proximity to the luminous OB stars, compared to the Wd2 average. This rate is higher with increasing distance from the OB stars, indicating that the PMS accretion disks are being rapidly destroyed by the far-ultra-violet radiation emitted by the OB population., Comment: 21 pages, 17 figures, 4 tables
Published: 2016
Full Text: View/download PDF

27. EWOCS-I: The catalog of X-ray sources in Westerlund 1 from the Extended Westerlund 1 and 2 Open Clusters Survey

Author: Universidad de Alicante. Departamento de Física Aplicada, Guarcello, Mario Giuseppe, Flaccomio, E., Albacete-Colombo, J. F., Almendros-Abad, Víctor, Anastasopoulou, Konstantina, Andersen, M., Argiroffi, C., Bayo, A., Bartlett, Elizabeth S., Bastian, N., De Becker, Michaël, Best, William, Bonito, R., Borghese, Alice, Calzetti, D., Castellanos, Raul, Cecchi-Pestellini, C., Clark, J. Simon, Clarke, C.J., Coti Zelati, Francesco, Damiani, F., Drake, J.J., Gennaro, Mario, Ginsburg, A., Grebel, E.K., Hora, Joseph L., Israel, Gian Luca, Lawrence, Grace, Locci, D., Mapelli, M., Martinez-Galarza, J.R., Micela, G., Miceli, M., Moraux, E., Muzic, K., Najarro de la Parra, Francisco, Negueruela, Ignacio, Nota, A., Pallanca, C., Prisinzano, L., Ritchie, Benedict, Robberto, M., Rom, Tamara, Sabbi, Elena, Scholz, A., Sciortino, Salvatore, Trigilio, Corrado, Umana, G., Winter, A., Wright, N.J., Zeidler, Peter, Universidad de Alicante. Departamento de Física Aplicada, Guarcello, Mario Giuseppe, Flaccomio, E., Albacete-Colombo, J. F., Almendros-Abad, Víctor, Anastasopoulou, Konstantina, Andersen, M., Argiroffi, C., Bayo, A., Bartlett, Elizabeth S., Bastian, N., De Becker, Michaël, Best, William, Bonito, R., Borghese, Alice, Calzetti, D., Castellanos, Raul, Cecchi-Pestellini, C., Clark, J. Simon, Clarke, C.J., Coti Zelati, Francesco, Damiani, F., Drake, J.J., Gennaro, Mario, Ginsburg, A., Grebel, E.K., Hora, Joseph L., Israel, Gian Luca, Lawrence, Grace, Locci, D., Mapelli, M., Martinez-Galarza, J.R., Micela, G., Miceli, M., Moraux, E., Muzic, K., Najarro de la Parra, Francisco, Negueruela, Ignacio, Nota, A., Pallanca, C., Prisinzano, L., Ritchie, Benedict, Robberto, M., Rom, Tamara, Sabbi, Elena, Scholz, A., Sciortino, Salvatore, Trigilio, Corrado, Umana, G., Winter, A., Wright, N.J., and Zeidler, Peter
Abstract: Context. With a mass exceeding several 104 M⊙ and a rich and dense population of massive stars, supermassive young star clusters represent the most massive star-forming environment that is dominated by the feedback from massive stars and gravitational interactions among stars. Aims. In this paper we present the Extended Westerlund 1 and 2 Open Clusters Survey (EWOCS) project, which aims to investigate the influence of the starburst environment on the formation of stars and planets, and on the evolution of both low and high mass stars. The primary targets of this project are Westerlund 1 and 2, the closest supermassive star clusters to the Sun. Methods. The project is based primarily on recent observations conducted with the Chandra and JWST observatories. Specifically, the Chandra survey of Westerlund 1 consists of 36 new ACIS-I observations, nearly co-pointed, for a total exposure time of 1 Msec. Additionally, we included 8 archival Chandra/ACIS-S observations. This paper presents the resulting catalog of X-ray sources within and around Westerlund 1. Sources were detected by combining various existing methods, and photon extraction and source validation were carried out using the ACIS-Extract software. Results. The EWOCS X-ray catalog comprises 5963 validated sources out of the 9420 initially provided to ACIS-Extract, reaching a photon flux threshold of approximately 2 × 10−8 photons cm−2 s−1. The X-ray sources exhibit a highly concentrated spatial distribution, with 1075 sources located within the central 1 arcmin. We have successfully detected X-ray emissions from 126 out of the 166 known massive stars of the cluster, and we have collected over 71 000 photons from the magnetar CXO J164710.20-455217.
Published: 2024

28. Hubble Tarantula Treasury Project. IV. The extinction law

Author: De Marchi, Guido, Panagia, Nino, Sabbi, Elena, Lennon, Daniel, Anderson, Jay, van der Marel, Roeland, Cignoni, Michele, Grebel, Eva K., Larsen, Soeren, Zaritsky, Dennis, Zeidler, Peter, Gouliermis, Dimitrios, and Aloisi, Alessandra
Subjects: Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Astrophysics of Galaxies
Abstract: We report on the study of interstellar extinction across the Tarantula nebula (30 Doradus), in the Large Magellanic Cloud, using observations from the Hubble Tarantula Treasury Project in the 0.3 - 1.6 micron range. The considerable and patchy extinction inside the nebula causes about 3500 red clump stars to be scattered along the reddening vector in the colour-magnitude diagrams, thereby allowing an accurate determination of the reddening slope in all bands. The measured slope of the reddening vector is remarkably steeper in all bands than in the the Galactic diffuse interstellar medium. At optical wavelengths, the larger ratio of total-to-selective extinction, namely Rv = 4.5 +/- 0.2, implies the presence of a grey component in the extinction law, due to a larger fraction of large grains. The extra large grains are most likely ices from supernova ejecta and will significantly alter the extinction properties of the region until they sublimate in 50 - 100 Myr. We discuss the implications of this extinction law for the Tarantula nebula and in general for regions of massive star formation in galaxies. Our results suggest that fluxes of strongly star forming regions are likely to be underestimated by a factor of about 2 in the optical., Comment: 15 pages, 10 figures, accepted for publication in MNRAS; Updated references, corrected typos in Table 3
Published: 2015
Full Text: View/download PDF

29. The VISTA Carina Nebula Survey II. Spatial distribution of the infrared-excess-selected young stellar population

Author: Zeidler, Peter, Preibisch, Thomas, Ratzka, Thorsten, Roccatagliata, Veronica, and Petr-Gotzens, Monika G.
Subjects: Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Astrophysics of Galaxies
Abstract: We performed a deep wide-field (6.76 deg^2) near-infrared survey with the VISTA telescope that covers the entire extent of the Carina nebula complex (CNC). The point-source catalog created from these data contains around four million individual objects down to masses of 0.1 M_sun. We present a statistical study of the large-scale spatial distribution and an investigation of the clustering properties of infrared-excesses objects, which are used to trace disk-bearing young stellar objects (YSOs). We find that a (J - H) versus (Ks - [4.5]) color-color diagram is well suited to tracing the population of YSO-candidates (cYSOs) by their infrared excess. We identify 8781 sources with strong infrared excess, which we consider as cYSOs. This sample is used to investigate the spatial distribution of the cYSOs with a nearest-neighbor analysis. The surface density distribution of cYSOs agrees well with the shape of the clouds as seen in our Herschel far-infrared survey. The strong decline in the surface density of excess sources outside the area of the clouds supports the hypothesis that our excess-selected sample consists predominantly of cYSOs with a low level of background contamination. This analysis allows us to identify 14 groups of cYSOs outside the central area. Our results suggest that the total population of cYSOs in the CNC comprises about 164000 objects, with a substantial fraction (~35%) located in the northern, still not well studied parts. Our cluster analysis suggests that roughly half of the cYSOs constitute a non-clustered, dispersed population., Comment: 15 pages, 8 figures, 3 tables accepted in A&A
Published: 2015
Full Text: View/download PDF

30. A High-Resolution Multiband Survey of Westerlund 2 With the Hubble Space Telescope I: Is the Massive Star Cluster Double?

Author: Zeidler, Peter, Sabbi, Elena, Nota, Antonella, Grebel, Eva K., Tosi, Monica, Bonanos, Alceste Z., Pasquali, Anna, Christian, Carol, de Mink, Selma E., and Ubeda, Leonardo
Subjects: Astrophysics - Solar and Stellar Astrophysics
Abstract: We present first results from a high resolution multi-band survey of the Westerlund 2 region with the Hubble Space Telescope. Specifically, we imaged Westerlund 2 with the Advanced Camera for Surveys through the $F555W$, $F814W$, and $F658N$ filters and with the Wide Field Camera 3 in the $F125W$, $F160W$, and $F128N$ filters. We derive the first high resolution pixel-to-pixel map of the color excess $E(B-V)_g$ of the gas associated with the cluster, combining the H$\alpha$ ($F658N$) and Pa$\beta$ ($F128N$) line observations. We demonstrate that, as expected, the region is affected by significant differential reddening with a median of $E(B-V)_g=1.87$~mag. After separating the populations of cluster members and foreground contaminants using a $(F814W-F160W)$ vs. $F814W$ color-magnitude diagram, we identify a pronounced pre-main-sequence population in Westerlund 2 showing a distinct turn-on. After dereddening each star of Westerlund 2 individually in the color-magnitude diagram we find via over-plotting PARSEC isochrones that the distance is in good agreement with the literature value of $\sim4.16 \pm 0.33$~kpc. With zero-age-main-sequence fitting to two-color-diagrams, we derive a value of total to selective extinction of $R_V=3.95 \pm 0.135$. A spatial density map of the stellar content reveals that the cluster might be composed of two clumps. We estimate the same age of 0.5-2.0 Myr for both clumps. While the two clumps appear to be coeval, the northern clump shows a $\sim 20 \%$ lower stellar surface density., Comment: 24 pages, 27 figures, 7 tables; Accepted for publication to The Astronomical Journal
Published: 2015
Full Text: View/download PDF

31. The VLT MUSE NFM view of outflows and externally photoevaporating discs near the orion bar★

Author: Haworth, Thomas J, primary, Reiter, Megan, additional, O’Dell, C Robert, additional, Zeidler, Peter, additional, Berne, Olivier, additional, Manara, Carlo F, additional, Ballabio, Giulia, additional, Kim, Jinyoung S, additional, Bally, John, additional, Goicoechea, Javier R, additional, Aru, Mari-Liis, additional, Gupta, Aashish, additional, and Miotello, Anna, additional
Published: 2023
Full Text: View/download PDF

32. The James Webb Space Telescope Mission

Author: Gardner, Jonathan P., primary, Mather, John C., additional, Abbott, Randy, additional, Abell, James S., additional, Abernathy, Mark, additional, Abney, Faith E., additional, Abraham, John G., additional, Abraham, Roberto, additional, Abul-Huda, Yasin M., additional, Acton, Scott, additional, Adams, Cynthia K., additional, Adams, Evan, additional, Adler, David S., additional, Adriaensen, Maarten, additional, Aguilar, Jonathan Albert, additional, Ahmed, Mansoor, additional, Ahmed, Nasif S., additional, Ahmed, Tanjira, additional, Albat, Rüdeger, additional, Albert, Loïc, additional, Alberts, Stacey, additional, Aldridge, David, additional, Allen, Mary Marsha, additional, Allen, Shaune S., additional, Altenburg, Martin, additional, Altunc, Serhat, additional, Alvarez, Jose Lorenzo, additional, Álvarez-Márquez, Javier, additional, de Oliveira, Catarina Alves, additional, Ambrose, Leslie L., additional, Anandakrishnan, Satya M., additional, Andersen, Gregory C., additional, Anderson, Harry James, additional, Anderson, Jay, additional, Anderson, Kristen, additional, Anderson, Sara M., additional, Aprea, Julio, additional, Archer, Benita J., additional, Arenberg, Jonathan W., additional, Argyriou, Ioannis, additional, Arribas, Santiago, additional, Artigau, Étienne, additional, Arvai, Amanda Rose, additional, Atcheson, Paul, additional, Atkinson, Charles B., additional, Averbukh, Jesse, additional, Aymergen, Cagatay, additional, Bacinski, John J., additional, Baggett, Wayne E., additional, Bagnasco, Giorgio, additional, Baker, Lynn L., additional, Balzano, Vicki Ann, additional, Banks, Kimberly A., additional, Baran, David A., additional, Barker, Elizabeth A., additional, Barrett, Larry K., additional, Barringer, Bruce O., additional, Barto, Allison, additional, Bast, William, additional, Baudoz, Pierre, additional, Baum, Stefi, additional, Beatty, Thomas G., additional, Beaulieu, Mathilde, additional, Bechtold, Kathryn, additional, Beck, Tracy, additional, Beddard, Megan M., additional, Beichman, Charles, additional, Bellagama, Larry, additional, Bely, Pierre, additional, Berger, Timothy W., additional, Bergeron, Louis E., additional, Bernier, Antoine-Darveau, additional, Bertch, Maria D., additional, Beskow, Charlotte, additional, Betz, Laura E., additional, Biagetti, Carl P., additional, Birkmann, Stephan, additional, Bjorklund, Kurt F., additional, Blackwood, James D., additional, Blazek, Ronald Paul, additional, Blossfeld, Stephen, additional, Bluth, Marcel, additional, Boccaletti, Anthony, additional, Boegner Jr, Martin E., additional, Bohlin, Ralph C., additional, Boia, John Joseph, additional, Böker, Torsten, additional, Bonaventura, N., additional, Bond, Nicholas A., additional, Bosley, Kari Ann, additional, Boucarut, Rene A., additional, Bouchet, Patrice, additional, Bouwman, Jeroen, additional, Bower, Gary, additional, Bowers, Ariel S., additional, Bowers, Charles W., additional, Boyce, Leslye A., additional, Boyer, Christine T., additional, Boyer, Martha L., additional, Boyer, Michael, additional, Boyer, Robert, additional, Bradley, Larry D., additional, Brady, Gregory R., additional, Brandl, Bernhard R., additional, Brannen, Judith L., additional, Breda, David, additional, Bremmer, Harold G., additional, Brennan, David, additional, Bresnahan, Pamela A., additional, Bright, Stacey N., additional, Broiles, Brian J., additional, Bromenschenkel, Asa, additional, Brooks, Brian H., additional, Brooks, Keira J., additional, Brown, Bob, additional, Brown, Bruce, additional, Brown, Thomas M., additional, Bruce, Barry W., additional, Bryson, Jonathan G., additional, Bujanda, Edwin D., additional, Bullock, Blake M., additional, Bunker, A. J., additional, Bureo, Rafael, additional, Burt, Irving J., additional, Bush, James Aaron, additional, Bushouse, Howard A., additional, Bussman, Marie C., additional, Cabaud, Olivier, additional, Cale, Steven, additional, Calhoon, Charles D., additional, Calvani, Humberto, additional, Canipe, Alicia M., additional, Caputo, Francis M., additional, Cara, Mihai, additional, Carey, Larkin, additional, Case, Michael Eli, additional, Cesari, Thaddeus, additional, Cetorelli, Lee D., additional, Chance, Don R., additional, Chandler, Lynn, additional, Chaney, Dave, additional, Chapman, George N., additional, Charlot, S., additional, Chayer, Pierre, additional, Cheezum, Jeffrey I., additional, Chen, Bin, additional, Chen, Christine H., additional, Cherinka, Brian, additional, Chichester, Sarah C., additional, Chilton, Zachary S., additional, Chittiraibalan, Dharini, additional, Clampin, Mark, additional, Clark, Charles R., additional, Clark, Kerry W., additional, Clark, Stephanie M., additional, Claybrooks, Edward E., additional, Cleveland, Keith A., additional, Cohen, Andrew L., additional, Cohen, Lester M., additional, Colón, Knicole D., additional, Coleman, Benee L., additional, Colina, Luis, additional, Comber, Brian J., additional, Comeau, Thomas M., additional, Comer, Thomas, additional, Reis, Alain Conde, additional, Connolly, Dennis C., additional, Conroy, Kyle E., additional, Contos, Adam R., additional, Contreras, James, additional, Cook, Neil J., additional, Cooper, James L., additional, Cooper, Rachel Aviva, additional, Correia, Michael F., additional, Correnti, Matteo, additional, Cossou, Christophe, additional, Costanza, Brian F., additional, Coulais, Alain, additional, Cox, Colin R., additional, Coyle, Ray T., additional, Cracraft, Misty M., additional, Crew, Keith A., additional, Curtis, Gary J., additional, Cusveller, Bianca, additional, Maciel, Cleyciane Da Costa, additional, Dailey, Christopher T., additional, Daugeron, Frédéric, additional, Davidson, Greg S., additional, Davies, James E., additional, Davis, Katherine Anne, additional, Davis, Michael S., additional, Day, Ratna, additional, de Chambure, Daniel, additional, de Jong, Pauline, additional, De Marchi, Guido, additional, Dean, Bruce H., additional, Decker, John E., additional, Delisa, Amy S., additional, Dell, Lawrence C., additional, Dellagatta, Gail, additional, Dembinska, Franciszka, additional, Demosthenes, Sandor, additional, Dencheva, Nadezhda M., additional, Deneu, Philippe, additional, DePriest, William W., additional, Deschenes, Jeremy, additional, Dethienne, Nathalie, additional, Detre, Örs Hunor, additional, Diaz, Rosa Izela, additional, Dicken, Daniel, additional, DiFelice, Audrey S., additional, Dillman, Matthew, additional, Disharoon, Maureen O., additional, Dixon, William V., additional, Doggett, Jesse B., additional, Dominguez, Keisha L., additional, Donaldson, Thomas S., additional, Doria-Warner, Cristina M., additional, Santos, Tony Dos, additional, Doty, Heather, additional, Douglas, Jr, Robert E., additional, Doyon, René, additional, Dressler, Alan, additional, Driggers, Jennifer, additional, Driggers, Phillip A., additional, Dunn, Jamie L., additional, DuPrie, Kimberly C., additional, Dupuis, Jean, additional, Durning, John, additional, Dutta, Sanghamitra B., additional, Earl, Nicholas M., additional, Eccleston, Paul, additional, Ecobichon, Pascal, additional, Egami, Eiichi, additional, Ehrenwinkler, Ralf, additional, Eisenhamer, Jonathan D., additional, Eisenhower, Michael, additional, Eisenstein, Daniel J., additional, El Hamel, Zaky, additional, Elie, Michelle L., additional, Elliott, James, additional, Elliott, Kyle Wesley, additional, Engesser, Michael, additional, Espinoza, Néstor, additional, Etienne, Odessa, additional, Etxaluze, Mireya, additional, Evans, Leah, additional, Fabreguettes, Luce, additional, Falcolini, Massimo, additional, Falini, Patrick R., additional, Fatig, Curtis, additional, Feeney, Matthew, additional, Feinberg, Lee D., additional, Fels, Raymond, additional, Ferdous, Nazma, additional, Ferguson, Henry C., additional, Ferrarese, Laura, additional, Ferreira, Marie-Héléne, additional, Ferruit, Pierre, additional, Ferry, Malcolm, additional, Filippazzo, Joseph Charles, additional, Firre, Daniel, additional, Fix, Mees, additional, Flagey, Nicolas, additional, Flanagan, Kathryn A., additional, Fleming, Scott W., additional, Florian, Michael, additional, Flynn, James R., additional, Foiadelli, Luca, additional, Fontaine, Mark R., additional, Fontanella, Erin Marie, additional, Forshay, Peter Randolph, additional, Fortner, Elizabeth A., additional, Fox, Ori D., additional, Framarini, Alexandro P., additional, Francisco, John I., additional, Franck, Randy, additional, Franx, Marijn, additional, Franz, David E., additional, Friedman, Scott D., additional, Friend, Katheryn E., additional, Frost, James R., additional, Fu, Henry, additional, Fullerton, Alexander W., additional, Gaillard, Lionel, additional, Galkin, Sergey, additional, Gallagher, Ben, additional, Galyer, Anthony D., additional, García Marín, Macarena, additional, Gardner, Lisa E., additional, Garland, Dennis, additional, Garrett, Bruce Albert, additional, Gasman, Danny, additional, Gáspár, András, additional, Gastaud, René, additional, Gaudreau, Daniel, additional, Gauthier, Peter Timothy, additional, Geers, Vincent, additional, Geithner, Paul H., additional, Gennaro, Mario, additional, Gerber, John, additional, Gereau, John C., additional, Giampaoli, Robert, additional, Giardino, Giovanna, additional, Gibbons, Paul C., additional, Gilbert, Karoline, additional, Gilman, Larry, additional, Girard, Julien H., additional, Giuliano, Mark E., additional, Gkountis, Konstantinos, additional, Glasse, Alistair, additional, Glassmire, Kirk Zachary, additional, Glauser, Adrian Michael, additional, Glazer, Stuart D., additional, Goldberg, Joshua, additional, Golimowski, David A., additional, Gonzaga, Shireen P., additional, Gordon, Karl D., additional, Gordon, Shawn J., additional, Goudfrooij, Paul, additional, Gough, Michael J., additional, Graham, Adrian J., additional, Grau, Christopher M., additional, Green, Joel David, additional, Greene, Gretchen R., additional, Greene, Thomas P., additional, Greenfield, Perry E., additional, Greenhouse, Matthew A., additional, Greve, Thomas R., additional, Greville, Edgar M., additional, Grimaldi, Stefano, additional, Groe, Frank E., additional, Groebner, Andrew, additional, Grumm, David M., additional, Grundy, Timothy, additional, Güdel, Manuel, additional, Guillard, Pierre, additional, Guldalian, John, additional, Gunn, Christopher A., additional, Gurule, Anthony, additional, Gutman, Irvin Meyer, additional, Guy, Paul D., additional, Guyot, Benjamin, additional, Hack, Warren J., additional, Haderlein, Peter, additional, Hagan, James B., additional, Hagedorn, Andria, additional, Hainline, Kevin, additional, Haley, Craig, additional, Hami, Maryam, additional, Hamilton, Forrest Clifford, additional, Hammann, Jeffrey, additional, Hammel, Heidi B., additional, Hanley, Christopher J., additional, Hansen, Carl August, additional, Hardy, Bruce, additional, Harnisch, Bernd, additional, Harr, Michael Hunter, additional, Harris, Pamela, additional, Hart, Jessica Ann, additional, Hartig, George F., additional, Hasan, Hashima, additional, Hashim, Kathleen Marie, additional, Hashimoto, Ryan, additional, Haskins, Sujee J., additional, Hawkins, Robert Edward, additional, Hayden, Brian, additional, Hayden, William L., additional, Healy, Mike, additional, Hecht, Karen, additional, Heeg, Vince J., additional, Hejal, Reem, additional, Helm, Kristopher A., additional, Hengemihle, Nicholas J., additional, Henning, Thomas, additional, Henry, Alaina, additional, Henry, Ronald L., additional, Henshaw, Katherine, additional, Hernandez, Scarlin, additional, Herrington, Donald C., additional, Heske, Astrid, additional, Hesman, Brigette Emily, additional, Hickey, David L., additional, Hilbert, Bryan N., additional, Hines, Dean C., additional, Hinz, Michael R., additional, Hirsch, Michael, additional, Hitcho, Robert S., additional, Hodapp, Klaus, additional, Hodge, Philip E., additional, Hoffman, Melissa, additional, Holfeltz, Sherie T., additional, Holler, Bryan Jason, additional, Hoppa, Jennifer Rose, additional, Horner, Scott, additional, Howard, Joseph M., additional, Howard, Richard J., additional, Huber, Jean M., additional, Hunkeler, Joseph S., additional, Hunter, Alexander, additional, Hunter, David Gavin, additional, Hurd, Spencer W., additional, Hurst, Brendan J., additional, Hutchings, John B., additional, Hylan, Jason E., additional, Ignat, Luminita Ilinca, additional, Illingworth, Garth, additional, Irish, Sandra M., additional, Isaacs III, John C., additional, Jackson Jr, Wallace C., additional, Jaffe, Daniel T., additional, Jahic, Jasmin, additional, Jahromi, Amir, additional, Jakobsen, Peter, additional, James, Bryan, additional, James, John C., additional, James, LeAndrea Rae, additional, Jamieson, William Brian, additional, Jandra, Raymond D., additional, Jayawardhana, Ray, additional, Jedrzejewski, Robert, additional, Jeffers, Basil S., additional, Jensen, Peter, additional, Joanne, Egges, additional, Johns, Alan T., additional, Johnson, Carl A., additional, Johnson, Eric L., additional, Johnson, Patricia, additional, Johnson, Phillip Stephen, additional, Johnson, Thomas K., additional, Johnson, Timothy W., additional, Johnstone, Doug, additional, Jollet, Delphine, additional, Jones, Danny P., additional, Jones, Gregory S., additional, Jones, Olivia C., additional, Jones, Ronald A., additional, Jones, Vicki, additional, Jordan, Ian J., additional, Jordan, Margaret E., additional, Jue, Reginald, additional, Jurkowski, Mark H., additional, Justis, Grant, additional, Justtanont, Kay, additional, Kaleida, Catherine C., additional, Kalirai, Jason S., additional, Kalmanson, Phillip Cabrales, additional, Kaltenegger, Lisa, additional, Kammerer, Jens, additional, Kan, Samuel K., additional, Kanarek, Graham Childs, additional, Kao, Shaw-Hong, additional, Karakla, Diane M., additional, Karl, Hermann, additional, Kassin, Susan A., additional, Kauffman, David D., additional, Kavanagh, Patrick, additional, Kelley, Leigh L., additional, Kelly, Douglas M., additional, Kendrew, Sarah, additional, Kennedy, Herbert V., additional, Kenny, Deborah A., additional, Keski-Kuha, Ritva A., additional, Keyes, Charles D., additional, Khan, Ali, additional, Kidwell, Richard C., additional, Kimble, Randy A., additional, King, James S., additional, King, Richard C., additional, Kinzel, Wayne M., additional, Kirk, Jeffrey R., additional, Kirkpatrick, Marc E., additional, Klaassen, Pamela, additional, Klingemann, Lana, additional, Klintworth, Paul U., additional, Knapp, Bryan Adam, additional, Knight, Scott, additional, Knollenberg, Perry J., additional, Knutsen, Daniel Mark, additional, Koehler, Robert, additional, Koekemoer, Anton M., additional, Kofler, Earl T., additional, Kontson, Vicki L., additional, Kovacs, Aiden Rose, additional, Kozhurina-Platais, Vera, additional, Krause, Oliver, additional, Kriss, Gerard A., additional, Krist, John, additional, Kristoffersen, Monica R., additional, Krogel, Claudia, additional, Krueger, Anthony P., additional, Kulp, Bernard A., additional, Kumari, Nimisha, additional, Kwan, Sandy W., additional, Kyprianou, Mark, additional, Labador, Aurora Gadiano, additional, Labiano, Álvaro, additional, Lafrenière, David, additional, Lagage, Pierre-Olivier, additional, Laidler, Victoria G., additional, Laine, Benoit, additional, Laird, Simon, additional, Lajoie, Charles-Philippe, additional, Lallo, Matthew D., additional, Lam, May Yen, additional, LaMassa, Stephanie Marie, additional, Lambros, Scott D., additional, Lampenfield, Richard Joseph, additional, Lander, Matthew Ed, additional, Langston, James Hutton, additional, Larson, Kirsten, additional, Larson, Melora, additional, LaVerghetta, Robert Joseph, additional, Law, David R., additional, Lawrence, Jon F., additional, Lee, David W., additional, Lee, Janice, additional, Lee, Yat-Ning Paul, additional, Leisenring, Jarron, additional, Leveille, Michael Dunlap, additional, Levenson, Nancy A., additional, Levi, Joshua S., additional, Levine, Marie B., additional, Lewis, Dan, additional, Lewis, Jake, additional, Lewis, Nikole, additional, Libralato, Mattia, additional, Lidon, Norbert, additional, Liebrecht, Paula Louisa, additional, Lightsey, Paul, additional, Lilly, Simon, additional, Lim, Frederick C., additional, Lim, Pey Lian, additional, Ling, Sai-Kwong, additional, Link, Lisa J., additional, Link, Miranda Nicole, additional, Lipinski, Jamie L., additional, Liu, XiaoLi, additional, Lo, Amy S., additional, Lobmeyer, Lynette, additional, Logue, Ryan M., additional, Long, Chris A., additional, Long, Douglas R., additional, Long, Ilana D., additional, Long, Knox S., additional, López-Caniego, Marcos, additional, Lotz, Jennifer M., additional, Love-Pruitt, Jennifer M., additional, Lubskiy, Michael, additional, Luers, Edward B., additional, Luetgens, Robert A., additional, Luevano, Annetta J., additional, G. Flores Lui, Sarah Marie, additional, Lund III, James M., additional, Lundquist, Ray A., additional, Lunine, Jonathan, additional, Lützgendorf, Nora, additional, Lynch, Richard J., additional, MacDonald, Alex J., additional, MacDonald, Kenneth, additional, Macias, Matthew J., additional, Macklis, Keith I., additional, Maghami, Peiman, additional, Maharaja, Rishabh Y., additional, Maiolino, Roberto, additional, Makrygiannis, Konstantinos G., additional, Malla, Sunita Giri, additional, Malumuth, Eliot M., additional, Manjavacas, Elena, additional, Marini, Andrea, additional, Marrione, Amanda, additional, Marston, Anthony, additional, Martel, André R, additional, Martin, Didier, additional, Martin, Peter G., additional, Martinez, Kristin L., additional, Maschmann, Marc, additional, Masci, Gregory L., additional, Masetti, Margaret E., additional, Maszkiewicz, Michael, additional, Matthews, Gary, additional, Matuskey, Jacob E., additional, McBrayer, Glen A., additional, McCarthy, Donald W., additional, McCaughrean, Mark J., additional, McClare, Leslie A., additional, McClare, Michael D., additional, McCloskey, John C., additional, McClurg, Taylore D., additional, McCoy, Martin, additional, McElwain, Michael W., additional, McGregor, Roy D., additional, McGuffey, Douglas B., additional, McKay, Andrew G., additional, McKenzie, William K., additional, McLean, Brian, additional, McMaster, Matthew, additional, McNeil, Warren, additional, De Meester, Wim, additional, Mehalick, Kimberly L., additional, Meixner, Margaret, additional, Meléndez, Marcio, additional, Menzel, Michael P., additional, Menzel, Michael T., additional, Merz, Matthew, additional, Mesterharm, David D., additional, Meyer, Michael R., additional, Meyett, Michele L., additional, Meza, Luis E., additional, Midwinter, Calvin, additional, Milam, Stefanie N., additional, Miller, Jay Todd, additional, Miller, William C., additional, Miskey, Cherie L., additional, Misselt, Karl, additional, Mitchell, Eileen P., additional, Mohan, Martin, additional, Montoya, Emily E., additional, Moran, Michael J., additional, Morishita, Takahiro, additional, Moro-Martín, Amaya, additional, Morrison, Debra L., additional, Morrison, Jane, additional, Morse, Ernie C., additional, Moschos, Michael, additional, Moseley, S. H., additional, Mosier, Gary E., additional, Mosner, Peter, additional, Mountain, Matt, additional, Muckenthaler, Jason S., additional, Mueller, Donald G., additional, Mueller, Migo, additional, Muhiem, Daniella, additional, Mühlmann, Prisca, additional, Mullally, Susan Elizabeth, additional, Mullen, Stephanie M., additional, Munger, Alan J, additional, Murphy, Jess, additional, Murray, Katherine T., additional, Muzerolle, James C., additional, Mycroft, Matthew, additional, Myers, Andrew, additional, Myers, Carey R., additional, R. Myers, Fred Richard, additional, Myers, Richard, additional, Myrick, Kaila, additional, Nagle, IV, Adrian F., additional, Nayak, Omnarayani, additional, Naylor, Bret, additional, Neff, Susan G., additional, Nelan, Edmund P., additional, Nella, John, additional, Nguyen, Duy Tuong, additional, Nguyen, Michael N., additional, Nickson, Bryony, additional, Nidhiry, John Joseph, additional, Niedner, Malcolm B., additional, Nieto-Santisteban, Maria, additional, Nikolov, Nikolay K., additional, Nishisaka, Mary Ann, additional, Noriega-Crespo, Alberto, additional, Nota, Antonella, additional, O’Mara, Robyn C., additional, Oboryshko, Michael, additional, O’Brien, Marcus B., additional, Ochs, William R., additional, Offenberg, Joel D., additional, Ogle, Patrick Michael, additional, Ohl, Raymond G., additional, Olmsted, Joseph Hamden, additional, Osborne, Shannon Barbara, additional, O’Shaughnessy, Brian Patrick, additional, Östlin, Göran, additional, O’Sullivan, Brian, additional, Otor, O. Justin, additional, Ottens, Richard, additional, Ouellette, Nathalie N.-Q., additional, Outlaw, Daria J., additional, Owens, Beverly A., additional, Pacifici, Camilla, additional, Page, James Christophe, additional, Paranilam, James G., additional, Park, Sang, additional, Parrish, Keith A., additional, Paschal, Laura, additional, Patapis, Polychronis, additional, Patel, Jignasha, additional, Patrick, Keith, additional, Pattishall Jr, Robert A., additional, Paul, Douglas William, additional, Paul, Shirley J., additional, Pauly, Tyler Andrew, additional, Pavlovsky, Cheryl M., additional, Peña-Guerrero, Maria, additional, Pedder, Andrew H., additional, Peek, Matthew Weldon, additional, Pelham, Patricia A., additional, Penanen, Konstantin, additional, Perriello, Beth A., additional, Perrin, Marshall D., additional, Perrine, Richard F., additional, Perrygo, Chuck, additional, Peslier, Muriel, additional, Petach, Michael, additional, Peterson, Karla A., additional, Pfarr, Tom, additional, Pierson, James M., additional, Pietraszkiewicz, Martin, additional, Pilchen, Guy, additional, Pipher, Judy L., additional, Pirzkal, Norbert, additional, Pitman, Joseph T., additional, Player, Danielle M., additional, Plesha, Rachel, additional, Plitzke, Anja, additional, Pohner, John A., additional, Poletis, Karyn Konstantin, additional, Pollizzi, Joseph A., additional, Polster, Ethan, additional, Pontius, James T., additional, Pontoppidan, Klaus, additional, Porges, Susana C., additional, Potter, Gregg D., additional, Prescott, Stephen, additional, Proffitt, Charles R., additional, Pueyo, Laurent, additional, Quispe Neira, Irma Aracely, additional, Radich, Armando, additional, Rager, Reiko T., additional, Rameau, Julien, additional, Ramey, Deborah D., additional, Alarcon, Rafael Ramos, additional, Rampini, Riccardo, additional, Rapp, Robert, additional, Rashford, Robert A., additional, Rauscher, Bernard J., additional, Ravindranath, Swara, additional, Rawle, Timothy, additional, Rawlings, Tynika N., additional, Ray, Tom, additional, Regan, Michael W., additional, Rehm, Brian, additional, Rehm, Kenneth D., additional, Reid, Neill, additional, Reis, Carl A., additional, Renk, Florian, additional, Reoch, Tom B., additional, Ressler, Michael, additional, Rest, Armin W., additional, Reynolds, Paul J., additional, Richon, Joel G., additional, Richon, Karen V., additional, Ridgaway, Michael, additional, Riedel, Adric Richard, additional, Rieke, George H., additional, Rieke, Marcia J., additional, Rifelli, Richard E., additional, Rigby, Jane R., additional, Riggs, Catherine S., additional, Ringel, Nancy J., additional, Ritchie, Christine E., additional, Rix, Hans-Walter, additional, Robberto, Massimo, additional, Robinson, Gregory L., additional, Robinson, Michael S., additional, Robinson, Orion, additional, Rock, Frank W., additional, Rodriguez, David R., additional, del Pino, Bruno Rodríguez, additional, Roellig, Thomas, additional, Rohrbach, Scott O., additional, Roman, Anthony J., additional, Romelfanger, Frederick J., additional, Romo Jr, Felipe P., additional, Rosales, Jose J., additional, Rose, Perry, additional, Roteliuk, Anthony F., additional, Roth, Marc N., additional, Rothwell, Braden Quinn, additional, Rouzaud, Sylvain, additional, Rowe, Jason, additional, Rowlands, Neil, additional, Roy, Arpita, additional, Royer, Pierre, additional, Rui, Chunlei, additional, Rumler, Peter, additional, Rumpl, William, additional, Russ, Melissa L., additional, Ryan, Michael B., additional, Ryan, Richard M., additional, Saad, Karl, additional, Sabata, Modhumita, additional, Sabatino, Rick, additional, Sabbi, Elena, additional, Sabelhaus, Phillip A., additional, Sabia, Stephen, additional, Sahu, Kailash C., additional, Saif, Babak N., additional, Salvignol, Jean-Christophe, additional, Samara-Ratna, Piyal, additional, Samuelson, Bridget S., additional, Sanders, Felicia A., additional, Sappington, Bradley, additional, Sargent, B. A., additional, Sauer, Arne, additional, Savadkin, Bruce J., additional, Sawicki, Marcin, additional, Schappell, Tina M., additional, Scheffer, Caroline, additional, Scheithauer, Silvia, additional, Scherer, Ron, additional, Schiff, Conrad, additional, Schlawin, Everett, additional, Schmeitzky, Olivier, additional, Schmitz, Tyler S., additional, Schmude, Donald J., additional, Schneider, Analyn, additional, Schreiber, Jürgen, additional, Schroeven-Deceuninck, Hilde, additional, Schultz, John J., additional, Schwab, Ryan, additional, Schwartz, Curtis H., additional, Scoccimarro, Dario, additional, Scott, John F., additional, Scott, Michelle B., additional, Seaton, Bonita L., additional, Seely, Bruce S., additional, Seery, Bernard, additional, Seidleck, Mark, additional, Sembach, Kenneth, additional, Shanahan, Clare Elizabeth, additional, Shaughnessy, Bryan, additional, Shaw, Richard A., additional, Shay, Christopher Michael, additional, Sheehan, Even, additional, Sheth, Kartik, additional, Shih, Hsin-Yi, additional, Shivaei, Irene, additional, Siegel, Noah, additional, Sienkiewicz, Matthew G., additional, Simmons, Debra D., additional, Simon, Bernard P., additional, Sirianni, Marco, additional, Sivaramakrishnan, Anand, additional, Slade, Jeffrey E., additional, Sloan, G. C., additional, Slocum, Christine E., additional, Slowinski, Steven E., additional, Smith, Corbett T., additional, Smith, Eric P., additional, Smith, Erin C., additional, Smith, Koby, additional, Smith, Robert, additional, Smith, Stephanie J., additional, Smolik, John L., additional, Soderblom, David R., additional, Sohn, Sangmo Tony, additional, Sokol, Jeff, additional, Sonneborn, George, additional, Sontag, Christopher D., additional, Sooy, Peter R., additional, Soummer, Remi, additional, Southwood, Dana M., additional, Spain, Kay, additional, Sparmo, Joseph, additional, Speer, David T., additional, Spencer, Richard, additional, Sprofera, Joseph D., additional, Stallcup, Scott S., additional, Stanley, Marcia K., additional, Stansberry, John A., additional, Stark, Christopher C., additional, Starr, Carl W., additional, Stassi, Diane Y., additional, Steck, Jane A., additional, Steeley, Christine D., additional, Stephens, Matthew A., additional, Stephenson, Ralph J., additional, Stewart, Alphonso C., additional, Stiavelli, Massimo, additional, Jr, Hervey Stockman, additional, Strada, Paolo, additional, Straughn, Amber N., additional, Streetman, Scott, additional, Strickland, David Kendal, additional, Strobele, Jingping F., additional, Stuhlinger, Martin, additional, Stys, Jeffrey Edward, additional, Such, Miguel, additional, Sukhatme, Kalyani, additional, Sullivan, Joseph F., additional, Sullivan, Pamela C., additional, Sumner, Sandra M., additional, Sun, Fengwu, additional, Sunnquist, Benjamin Dale, additional, Swade, Daryl Allen, additional, Swam, Michael S., additional, Swenton, Diane F., additional, Swoish, Robby A., additional, Tam Litten, Oi In, additional, Tamas, Laszlo, additional, Tao, Andrew, additional, Taylor, David K., additional, Taylor, Joanna M., additional, Plate, Maurice te, additional, Van Tea, Mason, additional, Teague, Kelly K., additional, Telfer, Randal C., additional, Temim, Tea, additional, Texter, Scott C., additional, Thatte, Deepashri G., additional, Thompson, Christopher Lee, additional, Thompson, Linda M., additional, Thomson, Shaun R., additional, Thronson, Harley, additional, Tierney, C. M., additional, Tikkanen, Tuomo, additional, Tinnin, Lee, additional, Tippet, William Thomas, additional, Todd, Connor William, additional, Tran, Hien D., additional, Trauger, John, additional, Trejo, Edwin Gregorio, additional, Vinh Truong, Justin Hoang, additional, Tsukamoto, Christine L., additional, Tufail, Yasir, additional, Tumlinson, Jason, additional, Tustain, Samuel, additional, Tyra, Harrison, additional, Ubeda, Leonardo, additional, Underwood, Kelli, additional, Uzzo, Michael A., additional, Vaclavik, Steven, additional, Valenduc, Frida, additional, Valenti, Jeff A., additional, Van Campen, Julie, additional, van de Wetering, Inge, additional, Van Der Marel, Roeland P., additional, van Haarlem, Remy, additional, Vandenbussche, Bart, additional, van Dishoeck, Ewine F., additional, Vanterpool, Dona D., additional, Vernoy, Michael R., additional, Vila Costas, Maria Begoña, additional, Volk, Kevin, additional, Voorzaat, Piet, additional, Voyton, Mark F., additional, Vydra, Ekaterina, additional, Waddy, Darryl J., additional, Waelkens, Christoffel, additional, Wahlgren, Glenn Michael, additional, Walker Jr, Frederick E., additional, Wander, Michel, additional, Warfield, Christine K., additional, Warner, Gerald, additional, Wasiak, Francis C., additional, Wasiak, Matthew F., additional, Wehner, James, additional, Weiler, Kevin R., additional, Weilert, Mark, additional, Weiss, Stanley B., additional, Wells, Martyn, additional, Welty, Alan D., additional, Wheate, Lauren, additional, Wheeler, Thomas P., additional, White, Christy L., additional, Whitehouse, Paul, additional, Whiteleather, Jennifer Margaret, additional, Whitman, William Russell, additional, Williams, Christina C., additional, Willmer, Christopher N. A., additional, Willott, Chris J., additional, Willoughby, Scott P., additional, Wilson, Andrew, additional, Wilson, Debra, additional, Wilson, Donna V., additional, Windhorst, Rogier, additional, Wislowski, Emily Christine, additional, Wolfe, David J., additional, Wolfe, Michael A., additional, Wolff, Schuyler, additional, Wondel, Amancio, additional, Woo, Cindy, additional, Woods, Robert T., additional, Worden, Elaine, additional, Workman, William, additional, Wright, Gillian S., additional, Wu, Carl, additional, Wu, Chi-Rai, additional, Wun, Dakin D., additional, Wymer, Kristen B., additional, Yadetie, Thomas, additional, Yan, Isabelle C., additional, Yang, Keith C., additional, Yates, Kayla L., additional, Yeager, Christopher R., additional, Yerger, Ethan John, additional, Young, Erick T., additional, Young, Gary, additional, Yu, Gene, additional, Yu, Susan, additional, Zak, Dean S., additional, Zeidler, Peter, additional, Zepp, Robert, additional, Zhou, Julia, additional, Zincke, Christian A., additional, Zonak, Stephanie, additional, and Zondag, Elisabeth, additional
Published: 2023
Full Text: View/download PDF

33. The Science Performance of JWST as Characterized in Commissioning

Author: Rigby, Jane, primary, Perrin, Marshall, additional, McElwain, Michael, additional, Kimble, Randy, additional, Friedman, Scott, additional, Lallo, Matt, additional, Doyon, René, additional, Feinberg, Lee, additional, Ferruit, Pierre, additional, Glasse, Alistair, additional, Rieke, Marcia, additional, Rieke, George, additional, Wright, Gillian, additional, Willott, Chris, additional, Colon, Knicole, additional, Milam, Stefanie, additional, Neff, Susan, additional, Stark, Christopher, additional, Valenti, Jeff, additional, Abell, Jim, additional, Abney, Faith, additional, Abul-Huda, Yasin, additional, Scott Acton, D., additional, Adams, Evan, additional, Adler, David, additional, Aguilar, Jonathan, additional, Ahmed, Nasif, additional, Albert, Loïc, additional, Alberts, Stacey, additional, Aldridge, David, additional, Allen, Marsha, additional, Altenburg, Martin, additional, Álvarez-Márquez, Javier, additional, Alves de Oliveira, Catarina, additional, Andersen, Greg, additional, Anderson, Harry, additional, Anderson, Sara, additional, Argyriou, Ioannis, additional, Armstrong, Amber, additional, Arribas, Santiago, additional, Artigau, Etienne, additional, Arvai, Amanda, additional, Atkinson, Charles, additional, Bacon, Gregory, additional, Bair, Thomas, additional, Banks, Kimberly, additional, Barrientes, Jaclyn, additional, Barringer, Bruce, additional, Bartosik, Peter, additional, Bast, William, additional, Baudoz, Pierre, additional, Beatty, Thomas, additional, Bechtold, Katie, additional, Beck, Tracy, additional, Bergeron, Eddie, additional, Bergkoetter, Matthew, additional, Bhatawdekar, Rachana, additional, Birkmann, Stephan, additional, Blazek, Ronald, additional, Blome, Claire, additional, Boccaletti, Anthony, additional, Böker, Torsten, additional, Boia, John, additional, Bonaventura, Nina, additional, Bond, Nicholas, additional, Bosley, Kari, additional, Boucarut, Ray, additional, Bourque, Matthew, additional, Bouwman, Jeroen, additional, Bower, Gary, additional, Bowers, Charles, additional, Boyer, Martha, additional, Bradley, Larry, additional, Brady, Greg, additional, Braun, Hannah, additional, Breda, David, additional, Bresnahan, Pamela, additional, Bright, Stacey, additional, Britt, Christopher, additional, Bromenschenkel, Asa, additional, Brooks, Brian, additional, Brooks, Keira, additional, Brown, Bob, additional, Brown, Matthew, additional, Brown, Patricia, additional, Bunker, Andy, additional, Burger, Matthew, additional, Bushouse, Howard, additional, Cale, Steven, additional, Cameron, Alex, additional, Cameron, Peter, additional, Canipe, Alicia, additional, Caplinger, James, additional, Caputo, Francis, additional, Cara, Mihai, additional, Carey, Larkin, additional, Carniani, Stefano, additional, Carrasquilla, Maria, additional, Carruthers, Margaret, additional, Case, Michael, additional, Catherine, Riggs, additional, Chance, Don, additional, Chapman, George, additional, Charlot, Stéphane, additional, Charlow, Brian, additional, Chayer, Pierre, additional, Chen, Bin, additional, Cherinka, Brian, additional, Chichester, Sarah, additional, Chilton, Zack, additional, Chonis, Taylor, additional, Clampin, Mark, additional, Clark, Charles, additional, Clark, Kerry, additional, Coe, Dan, additional, Coleman, Benee, additional, Comber, Brian, additional, Comeau, Tom, additional, Connolly, Dennis, additional, Cooper, James, additional, Cooper, Rachel, additional, Coppock, Eric, additional, Correnti, Matteo, additional, Cossou, Christophe, additional, Coulais, Alain, additional, Coyle, Laura, additional, Cracraft, Misty, additional, Curti, Mirko, additional, Cuturic, Steven, additional, Davis, Katherine, additional, Davis, Michael, additional, Dean, Bruce, additional, DeLisa, Amy, additional, deMeester, Wim, additional, Dencheva, Nadia, additional, Dencheva, Nadezhda, additional, DePasquale, Joseph, additional, Deschenes, Jeremy, additional, Hunor Detre, Örs, additional, Diaz, Rosa, additional, Dicken, Dan, additional, DiFelice, Audrey, additional, Dillman, Matthew, additional, Dixon, William, additional, Doggett, Jesse, additional, Donaldson, Tom, additional, Douglas, Rob, additional, DuPrie, Kimberly, additional, Dupuis, Jean, additional, Durning, John, additional, Easmin, Nilufar, additional, Eck, Weston, additional, Edeani, Chinwe, additional, Egami, Eiichi, additional, Ehrenwinkler, Ralf, additional, Eisenhamer, Jonathan, additional, Eisenhower, Michael, additional, Elie, Michelle, additional, Elliott, James, additional, Elliott, Kyle, additional, Ellis, Tracy, additional, Engesser, Michael, additional, Espinoza, Nestor, additional, Etienne, Odessa, additional, Etxaluze, Mireya, additional, Falini, Patrick, additional, Feeney, Matthew, additional, Ferry, Malcolm, additional, Filippazzo, Joseph, additional, Fincham, Brian, additional, Fix, Mees, additional, Flagey, Nicolas, additional, Florian, Michael, additional, Flynn, Jim, additional, Fontanella, Erin, additional, Ford, Terrance, additional, Forshay, Peter, additional, Fox, Ori, additional, Franz, David, additional, Fu, Henry, additional, Fullerton, Alexander, additional, Galkin, Sergey, additional, Galyer, Anthony, additional, García Marín, Macarena, additional, Gardner, Jonathan P., additional, Gardner, Lisa, additional, Garland, Dennis, additional, Garrett, Bruce, additional, Gasman, Danny, additional, Gaspar, Andras, additional, Gaudreau, Daniel, additional, Gauthier, Peter, additional, Geers, Vincent, additional, Geithner, Paul, additional, Gennaro, Mario, additional, Giardino, Giovanna, additional, Girard, Julien, additional, Giuliano, Mark, additional, Glassmire, Kirk, additional, Glauser, Adrian, additional, Glazer, Stuart, additional, Godfrey, John, additional, Golimowski, David, additional, Gollnitz, David, additional, Gong, Fan, additional, Gonzaga, Shireen, additional, Gordon, Michael, additional, Gordon, Karl, additional, Goudfrooij, Paul, additional, Greene, Thomas, additional, Greenhouse, Matthew, additional, Grimaldi, Stefano, additional, Groebner, Andrew, additional, Grundy, Timothy, additional, Guillard, Pierre, additional, Gutman, Irvin, additional, Ha, Kong Q., additional, Haderlein, Peter, additional, Hagedorn, Andria, additional, Hainline, Kevin, additional, Haley, Craig, additional, Hami, Maryam, additional, Hamilton, Forrest, additional, Hammel, Heidi, additional, Hansen, Carl, additional, Harkins, Tom, additional, Harr, Michael, additional, Hart, Jessica, additional, Hart, Quyen, additional, Hartig, George, additional, Hashimoto, Ryan, additional, Haskins, Sujee, additional, Hathaway, William, additional, Havey, Keith, additional, Hayden, Brian, additional, Hecht, Karen, additional, Heller-Boyer, Chris, additional, Henriques, Caroline, additional, Henry, Alaina, additional, Hermann, Karl, additional, Hernandez, Scarlin, additional, Hesman, Brigette, additional, Hicks, Brian, additional, Hilbert, Bryan, additional, Hines, Dean, additional, Hoffman, Melissa, additional, Holfeltz, Sherie, additional, Holler, Bryan J., additional, Hoppa, Jennifer, additional, Hott, Kyle, additional, Howard, Joseph M., additional, Howard, Rick, additional, Hunter, Alexander, additional, Hunter, David, additional, Hurst, Brendan, additional, Husemann, Bernd, additional, Hustak, Leah, additional, Ilinca Ignat, Luminita, additional, Illingworth, Garth, additional, Irish, Sandra, additional, Jackson, Wallace, additional, Jahromi, Amir, additional, Jakobsen, Peter, additional, James, LeAndrea, additional, James, Bryan, additional, Januszewski, William, additional, Jenkins, Ann, additional, Jirdeh, Hussein, additional, Johnson, Phillip, additional, Johnson, Timothy, additional, Jones, Vicki, additional, Jones, Ron, additional, Jones, Danny, additional, Jones, Olivia, additional, Jordan, Ian, additional, Jordan, Margaret, additional, Jurczyk, Sarah, additional, Jurling, Alden, additional, Kaleida, Catherine, additional, Kalmanson, Phillip, additional, Kammerer, Jens, additional, Kang, Huijo, additional, Kao, Shaw-Hong, additional, Karakla, Diane, additional, Kavanagh, Patrick, additional, Kelly, Doug, additional, Kendrew, Sarah, additional, Kennedy, Herbert, additional, Kenny, Deborah, additional, Keski-kuha, Ritva, additional, Keyes, Charles, additional, Kidwell, Richard, additional, Kinzel, Wayne, additional, Kirk, Jeff, additional, Kirkpatrick, Mark, additional, Kirshenblat, Danielle, additional, Klaassen, Pamela, additional, Knapp, Bryan, additional, Scott Knight, J., additional, Knollenberg, Perry, additional, Koehler, Robert, additional, Koekemoer, Anton, additional, Kovacs, Aiden, additional, Kulp, Trey, additional, Kumari, Nimisha, additional, Kyprianou, Mark, additional, La Massa, Stephanie, additional, Labador, Aurora, additional, Labiano, Alvaro, additional, Lagage, Pierre-Olivier, additional, Lajoie, Charles-Philippe, additional, Lallo, Matthew, additional, Lam, May, additional, Lamb, Tracy, additional, Lambros, Scott, additional, Lampenfield, Richard, additional, Langston, James, additional, Larson, Kirsten, additional, Law, David, additional, Lawrence, Jon, additional, Lee, David, additional, Leisenring, Jarron, additional, Lepo, Kelly, additional, Leveille, Michael, additional, Levenson, Nancy, additional, Levine, Marie, additional, Levy, Zena, additional, Lewis, Dan, additional, Lewis, Hannah, additional, Libralato, Mattia, additional, Lightsey, Paul, additional, Link, Miranda, additional, Liu, Lily, additional, Lo, Amy, additional, Lockwood, Alexandra, additional, Logue, Ryan, additional, Long, Chris, additional, Long, Douglas, additional, Loomis, Charles, additional, Lopez-Caniego, Marcos, additional, Lorenzo Alvarez, Jose, additional, Love-Pruitt, Jennifer, additional, Lucy, Adrian, additional, Luetzgendorf, Nora, additional, Maghami, Peiman, additional, Maiolino, Roberto, additional, Major, Melissa, additional, Malla, Sunita, additional, Malumuth, Eliot, additional, Manjavacas, Elena, additional, Mannfolk, Crystal, additional, Marrione, Amanda, additional, Marston, Anthony, additional, Martel, André, additional, Maschmann, Marc, additional, Masci, Gregory, additional, Masciarelli, Michaela, additional, Maszkiewicz, Michael, additional, Mather, John, additional, McKenzie, Kenny, additional, McLean, Brian, additional, McMaster, Matthew, additional, Melbourne, Katie, additional, Meléndez, Marcio, additional, Menzel, Michael, additional, Merz, Kaiya, additional, Meyett, Michele, additional, Meza, Luis, additional, Miskey, Cherie, additional, Misselt, Karl, additional, Moller, Christopher, additional, Morrison, Jane, additional, Morse, Ernie, additional, Moseley, Harvey, additional, Mosier, Gary, additional, Mountain, Matt, additional, Mueckay, Julio, additional, Mueller, Michael, additional, Mullally, Susan, additional, Murphy, Jess, additional, Murray, Katherine, additional, Murray, Claire, additional, Mustelier, David, additional, Muzerolle, James, additional, Mycroft, Matthew, additional, Myers, Richard, additional, Myrick, Kaila, additional, Nanavati, Shashvat, additional, Nance, Elizabeth, additional, Nayak, Omnarayani, additional, Naylor, Bret, additional, Nelan, Edmund, additional, Nickson, Bryony, additional, Nielson, Alethea, additional, Nieto-Santisteban, Maria, additional, Nikolov, Nikolay, additional, Noriega-Crespo, Alberto, additional, O’Shaughnessy, Brian, additional, O’Sullivan, Brian, additional, Ochs, William, additional, Ogle, Patrick, additional, Oleszczuk, Brenda, additional, Olmsted, Joseph, additional, Osborne, Shannon, additional, Ottens, Richard, additional, Owens, Beverly, additional, Pacifici, Camilla, additional, Pagan, Alyssa, additional, Page, James, additional, Park, Sang, additional, Parrish, Keith, additional, Patapis, Polychronis, additional, Paul, Lee, additional, Pauly, Tyler, additional, Pavlovsky, Cheryl, additional, Pedder, Andrew, additional, Peek, Matthew, additional, Pena-Guerrero, Maria, additional, Penanen, Konstantin, additional, Perez, Yesenia, additional, Perna, Michele, additional, Perriello, Beth, additional, Phillips, Kevin, additional, Pietraszkiewicz, Martin, additional, Pinaud, Jean-Paul, additional, Pirzkal, Norbert, additional, Pitman, Joseph, additional, Piwowar, Aidan, additional, Platais, Vera, additional, Player, Danielle, additional, Plesha, Rachel, additional, Pollizi, Joe, additional, Polster, Ethan, additional, Pontoppidan, Klaus, additional, Porterfield, Blair, additional, Proffitt, Charles, additional, Pueyo, Laurent, additional, Pulliam, Christine, additional, Quirt, Brian, additional, Quispe Neira, Irma, additional, Ramos Alarcon, Rafael, additional, Ramsay, Leah, additional, Rapp, Greg, additional, Rapp, Robert, additional, Rauscher, Bernard, additional, Ravindranath, Swara, additional, Rawle, Timothy, additional, Regan, Michael, additional, Reichard, Timothy A., additional, Reis, Carl, additional, Ressler, Michael E., additional, Rest, Armin, additional, Reynolds, Paul, additional, Rhue, Timothy, additional, Richon, Karen, additional, Rickman, Emily, additional, Ridgaway, Michael, additional, Ritchie, Christine, additional, Rix, Hans-Walter, additional, Robberto, Massimo, additional, Robinson, Gregory, additional, Robinson, Michael, additional, Robinson, Orion, additional, Rock, Frank, additional, Rodriguez, David, additional, Rodriguez Del Pino, Bruno, additional, Roellig, Thomas, additional, Rohrbach, Scott, additional, Roman, Anthony, additional, Romelfanger, Fred, additional, Rose, Perry, additional, Roteliuk, Anthony, additional, Roth, Marc, additional, Rothwell, Braden, additional, Rowlands, Neil, additional, Roy, Arpita, additional, Royer, Pierre, additional, Royle, Patricia, additional, Rui, Chunlei, additional, Rumler, Peter, additional, Runnels, Joel, additional, Russ, Melissa, additional, Rustamkulov, Zafar, additional, Ryden, Grant, additional, Ryer, Holly, additional, Sabata, Modhumita, additional, Sabatke, Derek, additional, Sabbi, Elena, additional, Samuelson, Bridget, additional, Sapp, Benjamin, additional, Sappington, Bradley, additional, Sargent, B., additional, Sauer, Arne, additional, Scheithauer, Silvia, additional, Schlawin, Everett, additional, Schlitz, Joseph, additional, Schmitz, Tyler, additional, Schneider, Analyn, additional, Schreiber, Jürgen, additional, Schulze, Vonessa, additional, Schwab, Ryan, additional, Scott, John, additional, Sembach, Kenneth, additional, Shanahan, Clare, additional, Shaughnessy, Bryan, additional, Shaw, Richard, additional, Shawger, Nanci, additional, Shay, Christopher, additional, Sheehan, Evan, additional, Shen, Sharon, additional, Sherman, Allan, additional, Shiao, Bernard, additional, Shih, Hsin-Yi, additional, Shivaei, Irene, additional, Sienkiewicz, Matthew, additional, Sing, David, additional, Sirianni, Marco, additional, Sivaramakrishnan, Anand, additional, Skipper, Joy, additional, Sloan, G. C., additional, Slocum, Christine, additional, Slowinski, Steven, additional, Smith, Erin, additional, Smith, Eric, additional, Smith, Denise, additional, Smith, Corbett, additional, Snyder, Gregory, additional, Soh, Warren, additional, Tony Sohn, Sangmo, additional, Soto, Christian, additional, Spencer, Richard, additional, Stallcup, Scott, additional, Stansberry, John, additional, Starr, Carl, additional, Starr, Elysia, additional, Stewart, Alphonso, additional, Stiavelli, Massimo, additional, Straughn, Amber, additional, Strickland, David, additional, Stys, Jeff, additional, Summers, Francis, additional, Sun, Fengwu, additional, Sunnquist, Ben, additional, Swade, Daryl, additional, Swam, Michael, additional, Swaters, Robert, additional, Swoish, Robby, additional, Taylor, Joanna M., additional, Taylor, Rolanda, additional, Te Plate, Maurice, additional, Tea, Mason, additional, Teague, Kelly, additional, Telfer, Randal, additional, Temim, Tea, additional, Thatte, Deepashri, additional, Thompson, Christopher, additional, Thompson, Linda, additional, Thomson, Shaun, additional, Tikkanen, Tuomo, additional, Tippet, William, additional, Todd, Connor, additional, Toolan, Sharon, additional, Tran, Hien, additional, Trejo, Edwin, additional, Truong, Justin, additional, Tsukamoto, Chris, additional, Tustain, Samuel, additional, Tyra, Harrison, additional, Ubeda, Leonardo, additional, Underwood, Kelli, additional, Uzzo, Michael, additional, Van Campen, Julie, additional, Vandal, Thomas, additional, Vandenbussche, Bart, additional, Vila, Begoña, additional, Volk, Kevin, additional, Wahlgren, Glenn, additional, Waldman, Mark, additional, Walker, Chanda, additional, Wander, Michel, additional, Warfield, Christine, additional, Warner, Gerald, additional, Wasiak, Matthew, additional, Watkins, Mitchell, additional, Weaver, Andrew, additional, Weilert, Mark, additional, Weiser, Nick, additional, Weiss, Ben, additional, Weissman, Sarah, additional, Welty, Alan, additional, West, Garrett, additional, Wheate, Lauren, additional, Wheatley, Elizabeth, additional, Wheeler, Thomas, additional, White, Rick, additional, Whiteaker, Kevin, additional, Whitehouse, Paul, additional, Whiteleather, Jennifer, additional, Whitman, William, additional, Williams, Christina, additional, Willmer, Christopher, additional, Willoughby, Scott, additional, Wilson, Andrew, additional, Wirth, Gregory, additional, Wislowski, Emily, additional, Wolf, Erin, additional, Wolfe, David, additional, Wolff, Schuyler, additional, Workman, Bill, additional, Wright, Ray, additional, Wu, Carl, additional, Wu, Rai, additional, Wymer, Kristen, additional, Yates, Kayla, additional, Yeager, Christopher, additional, Yeates, Jared, additional, Yerger, Ethan, additional, Yoon, Jinmi, additional, Young, Alice, additional, Yu, Susan, additional, Zak, Dean, additional, Zeidler, Peter, additional, Zhou, Julia, additional, Zielinski, Thomas, additional, Zincke, Cristian, additional, and Zonak, Stephanie, additional
Published: 2023
Full Text: View/download PDF

34. The VLT MUSE NFM view of outflows and externally photoevaporating discs near the orion bar★.

Author: Haworth, Thomas J, Reiter, Megan, O'Dell, C Robert, Zeidler, Peter, Berne, Olivier, Manara, Carlo F, Ballabio, Giulia, Kim, Jinyoung S, Bally, John, Goicoechea, Javier R, Aru, Mari-Liis, Gupta, Aashish, and Miotello, Anna
Subjects: STAR formation, NATURAL satellites, IRRADIATION, ORIGIN of planets
Abstract: We present Very Large Telescope/Multi-Unit Spectroscopic Explorer Narrow Field Mode observations of a pair of disc-bearing young stellar objects towards the Orion Bar: 203–504 and 203–506. Both of these discs are subject to external photoevaporation, where winds are launched from their outer regions due to environmental irradiation. Intriguingly, despite having projected separation from one another of only 1.65 arcsec(660 au at 400 pc), 203–504 has a classic teardrop shaped 'proplyd' morphology pointing towards θ2 Ori A (indicating irradiation by the EUV of that star, rather than |$\rm \theta ^1$| Ori C) but 203–506 has no ionization front, indicating it is not irradiated by stellar EUV at all. However, 203–506 does show [C i ] 8727 Å and [O i ] 6300 Å in emission, indicating irradiation by stellar FUV. This explicitly demonstrates the importance of FUV irradiation in driving mass loss from discs. We conclude that shielding of 203–506 from EUV is most likely due to its position on the observers side of an ionized layer lying in the foreground of the Huygens Region. We demonstrate that the outflow HH 519, previously thought to be emanating from 203–504 is actually an irradiated cloud edge and identify a new compact outflow from that object approximately along our line of sight with a velocity ∼130 km s−1. [ABSTRACT FROM AUTHOR]
Published: 2023
Full Text: View/download PDF

35. The Internal Line-of-Sight Kinematics of NGC 346: The Rotation of the Core Region

Author: Zeidler, Peter, primary, Sabbi, Elena, additional, and Nota, Antonella, additional
Published: 2022
Full Text: View/download PDF

36. Optical throughput and sensitivity of JWST NIRSpec

Author: Giardino, Giovanna, primary, Bhatawdekar, Rachana, additional, Birkmann, Stephan M., additional, Ferruit, Pierre, additional, Rawle, Tim, additional, Alves de Oliveira, Catarina, additional, Böker, Torsten, additional, Jakobsen, Peter, additional, Kumari, Nimisha, additional, Lopez-Caniego, Marcos, additional, Lützgendorf, Nora, additional, Manjavacas, Elena, additional, Proffitt, Charles, additional, Sirianni, Marco, additional, Te Plate, Maurice, additional, and Zeidler, Peter, additional
Published: 2022
Full Text: View/download PDF

37. In-flight performance and calibration of the grating wheel assembly sensors (NIRSpec/JWST)

Author: Alves de Oliveira, Catarina, primary, Lützgendorf, Nora, additional, Zeidler, Peter, additional, Giardino, Giovanna, additional, Ferruit, Pierre, additional, Kumari, Nimisha, additional, Rawle, Timothy D., additional, Birkmann, Stephan M., additional, Boeker, Torsten, additional, Proffitt, Charles, additional, Sirianni, Marco, additional, and te Plate, Maurice, additional
Published: 2022
Full Text: View/download PDF

38. In-orbit commissioning of the near-infrared spectrograph on the James Webb Space Telescope

Author: Böker, Torsten, primary, Abul-Huda, Yasin, additional, Altenburg, Martin, additional, Alves de Oliveira, Catarina, additional, Bechtold, Katie, additional, Beck, Tracy, additional, Birkmann, Stephan M., additional, Bonaventura, Nina, additional, Ehrenwinkler, Ralf, additional, Ferruit, Pierre, additional, Franz, David E., additional, Giardino, Giovanna, additional, Jakobsen, Peter, additional, Jensen, Peter, additional, Jollet, Delphine, additional, Karakla, Diane, additional, Karl, Hermann, additional, Keyes, Charles D., additional, Kumari, Nimisha, additional, Lander, Matthew, additional, Lopez-Caniego, Marcos, additional, Luetzgendorf, Nora, additional, Manjavacas, Elena, additional, Marston, Anthony, additional, Maschmann, Marc, additional, Mosner, Peter, additional, Muzerolle, James, additional, Ogle, Patrick, additional, Pena Guerrero, Maria, additional, Plesha, Rachel, additional, Proffitt, Charles, additional, Rapp, Robert, additional, Rawle, Timothy, additional, Rodriguez del Pino, Bruno, additional, Sabbi, Elena, additional, Sauer, Arne, additional, Sirianni, Marco, additional, Smith, Corbett, additional, te Plate, Maurice, additional, Wahlgren, Glenn, additional, Wislowski, Emily, additional, Wu, Rai, additional, Zeidler, Peter, additional, and Zincke, Christian A., additional
Published: 2022
Full Text: View/download PDF

39. Astrometric and wavelength calibration of the NIRSpec instrument during commissioning using a model-based approach

Author: Lützgendorf, Nora, primary, Giardino, Giovanna, additional, Alves de Oliveira, Catarina, additional, Zeidler, Peter, additional, Ferruit, Pierre, additional, Jakobsen, Peter, additional, Kumari, Nimisha, additional, Rawle, Tim, additional, Birkmann, Stephan M., additional, Böker, Torsten, additional, Proffitt, Charles, additional, Sirianni, Marco, additional, Te Plate, Maurice, additional, and Sohn, Sangmo Tony, additional
Published: 2022
Full Text: View/download PDF

40. In-flight performance of the NIRSpec micro shutter array

Author: Rawle, Timothy D., primary, Giardino, Giovanna, additional, Franz, David E., additional, Rapp, Robert, additional, te Plate, Maurice, additional, Zincke, Christian A., additional, Abul-Huda, Yasin M., additional, Alves de Oliveira, Catarina, additional, Bechtold, Katie, additional, Beck, Tracy, additional, Birkmann, Stephan M., additional, Böker, Torsten, additional, Ehrenwinkler, Ralf, additional, Ferruit, Pierre, additional, Garland, Dennis, additional, Jakobsen, Peter, additional, Karakla, Diane, additional, Karl, Hermann, additional, Keyes, Charles D., additional, Koehler, Robert, additional, Nimisha, Kumari, additional, Lützgendorf, Nora, additional, Manjavacas, Elena, additional, Marston, Anthony, additional, Moseley, S. Harvey, additional, Mosner, Peter, additional, Muzerolle, James, additional, Ogle, Patrick, additional, Proffitt, Charles, additional, Sabbi, Elena, additional, Sirianni, Marco, additional, Wahlgren, Glenn, additional, Wislowski, Emily, additional, Wright, Raymond H., additional, Wu, Chi Rai, additional, and Zeidler, Peter, additional
Published: 2022
Full Text: View/download PDF

41. The in-flight noise performance of the JWST/NIRSpec detector system

Author: Birkmann, Stephan M., primary, Giardino, Giovanna, additional, Sirianni, Marco, additional, Ferruit, Pierre, additional, Rauscher, Bernhard J., additional, Alves de Oliveira, Catarina, additional, Böker, Torsten, additional, Kumari, Nimisha, additional, Lützgendorf, Nora, additional, Manjavacas, Elena, additional, Proffitt, Charles, additional, Rawle, Tim, additional, te Plate, Maurice, additional, and Zeidler, Peter, additional
Published: 2022
Full Text: View/download PDF

42. Emotional labour and its outcomes: a study of a Philippine call centre

Author: P. Ruppel, Cynthia, L. Sims, Randi, and Zeidler, Peter
Published: 2013
Full Text: View/download PDF

43. Optical throughput and sensitivity of JWST NIRSpec

Author: Giardino, Giovanna, Bhatawdekar, Rachana, Birkmann, Stephan M., Ferruit, Pierre, Rawle, Timothy, Alves de Oliveira, Catarina, Boker, Torsten, Jakobsen, Peter, Kumari, Nimisha, Lopez-Caniego, Marcos, Lutzgendorf, Nora, Manjavacas, Elena, Proffitt, Charles, Sirianni, Marco, Te Plate, Maurice, Zeidler, Peter, Giardino, Giovanna, Bhatawdekar, Rachana, Birkmann, Stephan M., Ferruit, Pierre, Rawle, Timothy, Alves de Oliveira, Catarina, Boker, Torsten, Jakobsen, Peter, Kumari, Nimisha, Lopez-Caniego, Marcos, Lutzgendorf, Nora, Manjavacas, Elena, Proffitt, Charles, Sirianni, Marco, Te Plate, Maurice, and Zeidler, Peter
Abstract: To achieve its ambitious scientific goals, the Near-Infrared Spectrograph, NIRSpec, on board the Webb Space Telescope, needs to meet very demanding throughput requirements, here quantified in terms of photon-conversion efficiency (PCE). During the calibration activities performed for the instrument commissioning, we have obtained the first in-flight measurements of its PCE and also updated the modeling of the light losses occurring in the NIRSpec slit devices.The measured PCE of NIRSpec fixed-slit and multi-object spectroscopy modes overall meets or exceeds the pre-launch model predictions. The results are more contrasted for the integral-field spectroscopy mode, where the differences with the model can reach -20%, above 4 mu m, and exceed +30%, below 2 mu m. Additionally, thanks to the high quality of the JWST point-spread function, our slit-losses, at the shorter wavelength, are significantly decreased with respect to the pre-flight modeling.These results, combined with the confirmed low noise performance of the detectors, make of NIRSpec an exceptionally sensitive spectrograph.
Published: 2022

44. Work Strain, Job Satisfaction, and Intention to Quit: The Moderating Effect of Long-Term Orientation

Author: Sims, Randi L., Ruppel, Cynthia P., and Zeidler, Peter
Published: 2016
Full Text: View/download PDF

45. The impact of pre-supernova feedback and its dependence on environment

Author: McLeod, Anna F, primary, Ali, Ahmad A, additional, Chevance, Mélanie, additional, Della Bruna, Lorenza, additional, Schruba, Andreas, additional, Stevance, Heloise F, additional, Adamo, Angela, additional, Kruijssen, J M Diederik, additional, Longmore, Steven N, additional, Weisz, Daniel R, additional, and Zeidler, Peter, additional
Published: 2021
Full Text: View/download PDF

46. Star clusters near and far

Author: Adamo, Angela, Zeidler, Peter, Kruijssen, J. M. Diederik, Chevance, Mélanie, Gieles, Mark, Calzetti, Daniela, Charbonnel, Corinne, Zinnecker, Hans, Krause, Martin G. H., Stockholm University, Swedish Research Council, Swedish National Space Agency, German Research Foundation, European Commission, European Research Council, and Swiss National Science Foundation
Abstract: Star clusters are fundamental units of stellar feedback and unique tracers of their host galactic properties. In this review, we will first focus on their constituents, i.e. detailed insight into their stellar populations and their surrounding ionised, warm, neutral, and molecular gas. We, then, move beyond the Local Group to review star cluster populations at various evolutionary stages, and in diverse galactic environmental conditions accessible in the local Universe. At high redshift, where conditions for cluster formation and evolution are more extreme, we are only able to observe the integrated light of a handful of objects that we believe will become globular clusters. We therefore discuss how numerical and analytical methods, informed by the observed properties of cluster populations in the local Universe, are used to develop sophisticated simulations potentially capable of disentangling the genetic map of galaxy formation and assembly that is carried by globular cluster populations. Open access funding provided by Stockholm University. We thank the anonymous referee for a constructive and careful revision of this work. We thank the staff at ISSI for their generous hospitality, and the editors to invite us to contribute to this topic collection. We are grateful to Hui Li and Joel Pfeffer for sharing their data and Nate Bastian for providing comments on the manuscript. A.A. thanks Matteo Messa, Katie Hollyhead and the LEGUS and HiPEEC teams for support with the analyses showed in this review. A.A. acknowledges the support of the Swedish Research Council, Vetenskapsrådet, and the Swedish National Space Agency (SNSA). P.Z. acknowledges support by the Forschungsstipendium (grant number ZE 1159/1-1) of the German Research Foundation (DFG). J.M.D.K. and M.C. gratefully acknowledge funding from the German Research Foundation (DFG) in the form of an Emmy Noether Research Group (grant number KR4801/1-1) and a DFG Sachbeihilfe Grant (grant number KR4801/2-1). J.M.D.K. gratefully acknowledges funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme via the ERC Starting Grant MUSTANG (grant agreement number 714907), and from Sonderforschungsbereich SFB 881 “The Milky Way System” (subproject B2) of the DFG. C.C.acknowledges funding from the Swiss National Foundation (SNF grants 200021_169125 and 200020_192039).
Published: 2020

47. Tracing star formation across cosmic time

Author: Adamo, Angela, Zeidler, Peter, Diederik Kruijssen, J. M., Chevance, Mélanie, Gieles, Mark, Calzetti, Daniela, Charbonnel, Corinne, Zinnecker, Hans, Krause, Martin G. H., Stockholm University, Swedish Research Council, Swedish National Space Agency, German Research Foundation, European Commission, European Research Council, and Swiss National Science Foundation
Subjects: Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics::Galaxy Astrophysics
Abstract: Star clusters are fundamental units of stellar feedback and unique tracers of their host galactic properties. In this review, we will first focus on their constituents, i.e. detailed insight into their stellar populations and their surrounding ionised, warm, neutral, and molecular gas. We, then, move beyond the Local Group to review star cluster populations at various evolutionary stages, and in diverse galactic environmental conditions accessible in the local Universe. At high redshift, where conditions for cluster formation and evolution are more extreme, we are only able to observe the integrated light of a handful of objects that we believe will become globular clusters. We therefore discuss how numerical and analytical methods, informed by the observed properties of cluster populations in the local Universe, are used to develop sophisticated simulations potentially capable of disentangling the genetic map of galaxy formation and assembly that is carried by globular cluster populations., Open access funding provided by Stockholm University. We thank the anonymous referee for a constructive and careful revision of this work. We thank the staff at ISSI for their generous hospitality, and the editors to invite us to contribute to this topic collection. We are grateful to Hui Li and Joel Pfeffer for sharing their data and Nate Bastian for providing comments on the manuscript. A.A. thanks Matteo Messa, Katie Hollyhead and the LEGUS and HiPEEC teams for support with the analyses showed in this review. A.A. acknowledges the support of the Swedish Research Council, Vetenskapsrådet, and the Swedish National Space Agency (SNSA). P.Z. acknowledges support by the Forschungsstipendium (grant number ZE 1159/1-1) of the German Research Foundation (DFG). J.M.D.K. and M.C. gratefully acknowledge funding from the German Research Foundation (DFG) in the form of an Emmy Noether Research Group (grant number KR4801/1-1) and a DFG Sachbeihilfe Grant (grant number KR4801/2-1). J.M.D.K. gratefully acknowledges funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme via the ERC Starting Grant MUSTANG (grant agreement number 714907), and from Sonderforschungsbereich SFB 881 “The Milky Way System” (subproject B2) of the DFG. C.C.acknowledges funding from the Swiss National Foundation (SNF grants 200021_169125 and 200020_192039).
Published: 2020

48. Star clusters near and far

Author: Stockholm University, Swedish Research Council, Swedish National Space Agency, German Research Foundation, European Commission, European Research Council, Swiss National Science Foundation, Adamo, Angela, Zeidler, Peter, Diederik Kruijssen, J. M., Chevance, Mélanie, Gieles, Mark, Calzetti, Daniela, Charbonnel, Corinne, Zinnecker, Hans, Krause, Martin G. H., Stockholm University, Swedish Research Council, Swedish National Space Agency, German Research Foundation, European Commission, European Research Council, Swiss National Science Foundation, Adamo, Angela, Zeidler, Peter, Diederik Kruijssen, J. M., Chevance, Mélanie, Gieles, Mark, Calzetti, Daniela, Charbonnel, Corinne, Zinnecker, Hans, and Krause, Martin G. H.
Abstract: Star clusters are fundamental units of stellar feedback and unique tracers of their host galactic properties. In this review, we will first focus on their constituents, i.e. detailed insight into their stellar populations and their surrounding ionised, warm, neutral, and molecular gas. We, then, move beyond the Local Group to review star cluster populations at various evolutionary stages, and in diverse galactic environmental conditions accessible in the local Universe. At high redshift, where conditions for cluster formation and evolution are more extreme, we are only able to observe the integrated light of a handful of objects that we believe will become globular clusters. We therefore discuss how numerical and analytical methods, informed by the observed properties of cluster populations in the local Universe, are used to develop sophisticated simulations potentially capable of disentangling the genetic map of galaxy formation and assembly that is carried by globular cluster populations.
Published: 2020

49. The Young Massive Star Cluster Westerlund 2 Observed with MUSE. III. A Cluster in Motion—The Complex Internal Dynamics

Author: Zeidler, Peter, primary, Sabbi, Elena, additional, Nota, Antonella, additional, and McLeod, Anna F., additional
Published: 2021
Full Text: View/download PDF

50. The importance of organisational justice on schedule satisfaction: a study of Latin American call centre employees

Author: Sims, Randi L., primary, Yurova, Yuliya, additional, and Zeidler, Peter, additional
Published: 2021
Full Text: View/download PDF

Catalog

Books, media, physical & digital resources

See catalog results

Searchworks

Select search scope, currently: Articles Catalog books, media & more in Jio Institute collections Articles journal articles & other e-resources

Search

Search Constraints

Refine your results

Search Limiters

Topic

Publication Year Range

Language

Publication Type

Journal

Region

Database

Publisher

161 results on '"Zeidler, Peter"'

Search Results

Catalog

Select search scope, currently: Articles

Catalog

books, media & more in Jio Institute collections

Articles

journal articles & other e-resources