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1. Making the diamond vortex phase masks for the METIS instrument

Author: Forsberg, Pontus, Karvinen, Petri, Ronayette, Samuel, Kuittinen, Markku, Absil, Olivier, König, Lorenzo, Delacroix, Christian, Orban de Xivry, Gilles, Barrière, Jean-Christophe, Pantin, Eric, and Karlsson, Mikael
Published: 2024
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2. The DESI Experiment Part I: Science,Targeting, and Survey Design

Author: DESI Collaboration, Aghamousa, Amir, Aguilar, Jessica, Ahlen, Steve, Alam, Shadab, Allen, Lori E., Prieto, Carlos Allende, Annis, James, Bailey, Stephen, Balland, Christophe, Ballester, Otger, Baltay, Charles, Beaufore, Lucas, Bebek, Chris, Beers, Timothy C., Bell, Eric F., Bernal, José Luis, Besuner, Robert, Beutler, Florian, Blake, Chris, Bleuler, Hannes, Blomqvist, Michael, Blum, Robert, Bolton, Adam S., Briceno, Cesar, Brooks, David, Brownstein, Joel R., Buckley-Geer, Elizabeth, Burden, Angela, Burtin, Etienne, Busca, Nicolas G., Cahn, Robert N., Cai, Yan-Chuan, Cardiel-Sas, Laia, Carlberg, Raymond G., Carton, Pierre-Henri, Casas, Ricard, Castander, Francisco J., Cervantes-Cota, Jorge L., Claybaugh, Todd M., Close, Madeline, Coker, Carl T., Cole, Shaun, Comparat, Johan, Cooper, Andrew P., Cousinou, M. -C., Crocce, Martin, Cuby, Jean-Gabriel, Cunningham, Daniel P., Davis, Tamara M., Dawson, Kyle S., de la Macorra, Axel, De Vicente, Juan, Delubac, Timothée, Derwent, Mark, Dey, Arjun, Dhungana, Govinda, Ding, Zhejie, Doel, Peter, Duan, Yutong T., Ealet, Anne, Edelstein, Jerry, Eftekharzadeh, Sarah, Eisenstein, Daniel J., Elliott, Ann, Escoffier, Stéphanie, Evatt, Matthew, Fagrelius, Parker, Fan, Xiaohui, Fanning, Kevin, Farahi, Arya, Farihi, Jay, Favole, Ginevra, Feng, Yu, Fernandez, Enrique, Findlay, Joseph R., Finkbeiner, Douglas P., Fitzpatrick, Michael J., Flaugher, Brenna, Flender, Samuel, Font-Ribera, Andreu, Forero-Romero, Jaime E., Fosalba, Pablo, Frenk, Carlos S., Fumagalli, Michele, Gaensicke, Boris T., Gallo, Giuseppe, Garcia-Bellido, Juan, Gaztanaga, Enrique, Fusillo, Nicola Pietro Gentile, Gerard, Terry, Gershkovich, Irena, Giannantonio, Tommaso, Gillet, Denis, Gonzalez-de-Rivera, Guillermo, Gonzalez-Perez, Violeta, Gott, Shelby, Graur, Or, Gutierrez, Gaston, Guy, Julien, Habib, Salman, Heetderks, Henry, Heetderks, Ian, Heitmann, Katrin, Hellwing, Wojciech A., Herrera, David A., Ho, Shirley, Holland, Stephen, Honscheid, Klaus, Huff, Eric, Hutchinson, Timothy A., Huterer, Dragan, Hwang, Ho Seong, Laguna, Joseph Maria Illa, Ishikawa, Yuzo, Jacobs, Dianna, Jeffrey, Niall, Jelinsky, Patrick, Jennings, Elise, Jiang, Linhua, Jimenez, Jorge, Johnson, Jennifer, Joyce, Richard, Jullo, Eric, Juneau, Stéphanie, Kama, Sami, Karcher, Armin, Karkar, Sonia, Kehoe, Robert, Kennamer, Noble, Kent, Stephen, Kilbinger, Martin, Kim, Alex G., Kirkby, David, Kisner, Theodore, Kitanidis, Ellie, Kneib, Jean-Paul, Koposov, Sergey, Kovacs, Eve, Koyama, Kazuya, Kremin, Anthony, Kron, Richard, Kronig, Luzius, Kueter-Young, Andrea, Lacey, Cedric G., Lafever, Robin, Lahav, Ofer, Lambert, Andrew, Lampton, Michael, Landriau, Martin, Lang, Dustin, Lauer, Tod R., Goff, Jean-Marc Le, Guillou, Laurent Le, Van Suu, Auguste Le, Lee, Jae Hyeon, Lee, Su-Jeong, Leitner, Daniela, Lesser, Michael, Levi, Michael E., L'Huillier, Benjamin, Li, Baojiu, Liang, Ming, Lin, Huan, Linder, Eric, Loebman, Sarah R., Lukić, Zarija, Ma, Jun, MacCrann, Niall, Magneville, Christophe, Makarem, Laleh, Manera, Marc, Manser, Christopher J., Marshall, Robert, Martini, Paul, Massey, Richard, Matheson, Thomas, McCauley, Jeremy, McDonald, Patrick, McGreer, Ian D., Meisner, Aaron, Metcalfe, Nigel, Miller, Timothy N., Miquel, Ramon, Moustakas, John, Myers, Adam, Naik, Milind, Newman, Jeffrey A., Nichol, Robert C., Nicola, Andrina, da Costa, Luiz Nicolati, Nie, Jundan, Niz, Gustavo, Norberg, Peder, Nord, Brian, Norman, Dara, Nugent, Peter, O'Brien, Thomas, Oh, Minji, Olsen, Knut A. G., Padilla, Cristobal, Padmanabhan, Hamsa, Padmanabhan, Nikhil, Palanque-Delabrouille, Nathalie, Palmese, Antonella, Pappalardo, Daniel, Pâris, Isabelle, Park, Changbom, Patej, Anna, Peacock, John A., Peiris, Hiranya V., Peng, Xiyan, Percival, Will J., Perruchot, Sandrine, Pieri, Matthew M., Pogge, Richard, Pollack, Jennifer E., Poppett, Claire, Prada, Francisco, Prakash, Abhishek, Probst, Ronald G., Rabinowitz, David, Raichoor, Anand, Ree, Chang Hee, Refregier, Alexandre, Regal, Xavier, Reid, Beth, Reil, Kevin, Rezaie, Mehdi, Rockosi, Constance M., Roe, Natalie, Ronayette, Samuel, Roodman, Aaron, Ross, Ashley J., Ross, Nicholas P., Rossi, Graziano, Rozo, Eduardo, Ruhlmann-Kleider, Vanina, Rykoff, Eli S., Sabiu, Cristiano, Samushia, Lado, Sanchez, Eusebio, Sanchez, Javier, Schlegel, David J., Schneider, Michael, Schubnell, Michael, Secroun, Aurélia, Seljak, Uros, Seo, Hee-Jong, Serrano, Santiago, Shafieloo, Arman, Shan, Huanyuan, Sharples, Ray, Sholl, Michael J., Shourt, William V., Silber, Joseph H., Silva, David R., Sirk, Martin M., Slosar, Anze, Smith, Alex, Smoot, George F., Som, Debopam, Song, Yong-Seon, Sprayberry, David, Staten, Ryan, Stefanik, Andy, Tarle, Gregory, Tie, Suk Sien, Tinker, Jeremy L., Tojeiro, Rita, Valdes, Francisco, Valenzuela, Octavio, Valluri, Monica, Vargas-Magana, Mariana, Verde, Licia, Walker, Alistair R., Wang, Jiali, Wang, Yuting, Weaver, Benjamin A., Weaverdyck, Curtis, Wechsler, Risa H., Weinberg, David H., White, Martin, Yang, Qian, Yeche, Christophe, Zhang, Tianmeng, Zhao, Gong-Bo, Zheng, Yi, Zhou, Xu, Zhou, Zhimin, Zhu, Yaling, Zou, Hu, and Zu, Ying
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: DESI (Dark Energy Spectroscopic Instrument) is a Stage IV ground-based dark energy experiment that will study baryon acoustic oscillations (BAO) and the growth of structure through redshift-space distortions with a wide-area galaxy and quasar redshift survey. To trace the underlying dark matter distribution, spectroscopic targets will be selected in four classes from imaging data. We will measure luminous red galaxies up to $z=1.0$. To probe the Universe out to even higher redshift, DESI will target bright [O II] emission line galaxies up to $z=1.7$. Quasars will be targeted both as direct tracers of the underlying dark matter distribution and, at higher redshifts ($ 2.1 < z < 3.5$), for the Ly-$\alpha$ forest absorption features in their spectra, which will be used to trace the distribution of neutral hydrogen. When moonlight prevents efficient observations of the faint targets of the baseline survey, DESI will conduct a magnitude-limited Bright Galaxy Survey comprising approximately 10 million galaxies with a median $z\approx 0.2$. In total, more than 30 million galaxy and quasar redshifts will be obtained to measure the BAO feature and determine the matter power spectrum, including redshift space distortions.
Published: 2016

3. The DESI Experiment Part II: Instrument Design

Author: DESI Collaboration, Aghamousa, Amir, Aguilar, Jessica, Ahlen, Steve, Alam, Shadab, Allen, Lori E., Prieto, Carlos Allende, Annis, James, Bailey, Stephen, Balland, Christophe, Ballester, Otger, Baltay, Charles, Beaufore, Lucas, Bebek, Chris, Beers, Timothy C., Bell, Eric F., Bernal, José Luis, Besuner, Robert, Beutler, Florian, Blake, Chris, Bleuler, Hannes, Blomqvist, Michael, Blum, Robert, Bolton, Adam S., Briceno, Cesar, Brooks, David, Brownstein, Joel R., Buckley-Geer, Elizabeth, Burden, Angela, Burtin, Etienne, Busca, Nicolas G., Cahn, Robert N., Cai, Yan-Chuan, Cardiel-Sas, Laia, Carlberg, Raymond G., Carton, Pierre-Henri, Casas, Ricard, Castander, Francisco J., Cervantes-Cota, Jorge L., Claybaugh, Todd M., Close, Madeline, Coker, Carl T., Cole, Shaun, Comparat, Johan, Cooper, Andrew P., Cousinou, M. -C., Crocce, Martin, Cuby, Jean-Gabriel, Cunningham, Daniel P., Davis, Tamara M., Dawson, Kyle S., de la Macorra, Axel, De Vicente, Juan, Delubac, Timothée, Derwent, Mark, Dey, Arjun, Dhungana, Govinda, Ding, Zhejie, Doel, Peter, Duan, Yutong T., Ealet, Anne, Edelstein, Jerry, Eftekharzadeh, Sarah, Eisenstein, Daniel J., Elliott, Ann, Escoffier, Stéphanie, Evatt, Matthew, Fagrelius, Parker, Fan, Xiaohui, Fanning, Kevin, Farahi, Arya, Farihi, Jay, Favole, Ginevra, Feng, Yu, Fernandez, Enrique, Findlay, Joseph R., Finkbeiner, Douglas P., Fitzpatrick, Michael J., Flaugher, Brenna, Flender, Samuel, Font-Ribera, Andreu, Forero-Romero, Jaime E., Fosalba, Pablo, Frenk, Carlos S., Fumagalli, Michele, Gaensicke, Boris T., Gallo, Giuseppe, Garcia-Bellido, Juan, Gaztanaga, Enrique, Fusillo, Nicola Pietro Gentile, Gerard, Terry, Gershkovich, Irena, Giannantonio, Tommaso, Gillet, Denis, Gonzalez-de-Rivera, Guillermo, Gonzalez-Perez, Violeta, Gott, Shelby, Graur, Or, Gutierrez, Gaston, Guy, Julien, Habib, Salman, Heetderks, Henry, Heetderks, Ian, Heitmann, Katrin, Hellwing, Wojciech A., Herrera, David A., Ho, Shirley, Holland, Stephen, Honscheid, Klaus, Huff, Eric, Hutchinson, Timothy A., Huterer, Dragan, Hwang, Ho Seong, Laguna, Joseph Maria Illa, Ishikawa, Yuzo, Jacobs, Dianna, Jeffrey, Niall, Jelinsky, Patrick, Jennings, Elise, Jiang, Linhua, Jimenez, Jorge, Johnson, Jennifer, Joyce, Richard, Jullo, Eric, Juneau, Stéphanie, Kama, Sami, Karcher, Armin, Karkar, Sonia, Kehoe, Robert, Kennamer, Noble, Kent, Stephen, Kilbinger, Martin, Kim, Alex G., Kirkby, David, Kisner, Theodore, Kitanidis, Ellie, Kneib, Jean-Paul, Koposov, Sergey, Kovacs, Eve, Koyama, Kazuya, Kremin, Anthony, Kron, Richard, Kronig, Luzius, Kueter-Young, Andrea, Lacey, Cedric G., Lafever, Robin, Lahav, Ofer, Lambert, Andrew, Lampton, Michael, Landriau, Martin, Lang, Dustin, Lauer, Tod R., Goff, Jean-Marc Le, Guillou, Laurent Le, Van Suu, Auguste Le, Lee, Jae Hyeon, Lee, Su-Jeong, Leitner, Daniela, Lesser, Michael, Levi, Michael E., L'Huillier, Benjamin, Li, Baojiu, Liang, Ming, Lin, Huan, Linder, Eric, Loebman, Sarah R., Lukić, Zarija, Ma, Jun, MacCrann, Niall, Magneville, Christophe, Makarem, Laleh, Manera, Marc, Manser, Christopher J., Marshall, Robert, Martini, Paul, Massey, Richard, Matheson, Thomas, McCauley, Jeremy, McDonald, Patrick, McGreer, Ian D., Meisner, Aaron, Metcalfe, Nigel, Miller, Timothy N., Miquel, Ramon, Moustakas, John, Myers, Adam, Naik, Milind, Newman, Jeffrey A., Nichol, Robert C., Nicola, Andrina, da Costa, Luiz Nicolati, Nie, Jundan, Niz, Gustavo, Norberg, Peder, Nord, Brian, Norman, Dara, Nugent, Peter, O'Brien, Thomas, Oh, Minji, Olsen, Knut A. G., Padilla, Cristobal, Padmanabhan, Hamsa, Padmanabhan, Nikhil, Palanque-Delabrouille, Nathalie, Palmese, Antonella, Pappalardo, Daniel, Pâris, Isabelle, Park, Changbom, Patej, Anna, Peacock, John A., Peiris, Hiranya V., Peng, Xiyan, Percival, Will J., Perruchot, Sandrine, Pieri, Matthew M., Pogge, Richard, Pollack, Jennifer E., Poppett, Claire, Prada, Francisco, Prakash, Abhishek, Probst, Ronald G., Rabinowitz, David, Raichoor, Anand, Ree, Chang Hee, Refregier, Alexandre, Regal, Xavier, Reid, Beth, Reil, Kevin, Rezaie, Mehdi, Rockosi, Constance M., Roe, Natalie, Ronayette, Samuel, Roodman, Aaron, Ross, Ashley J., Ross, Nicholas P., Rossi, Graziano, Rozo, Eduardo, Ruhlmann-Kleider, Vanina, Rykoff, Eli S., Sabiu, Cristiano, Samushia, Lado, Sanchez, Eusebio, Sanchez, Javier, Schlegel, David J., Schneider, Michael, Schubnell, Michael, Secroun, Aurélia, Seljak, Uros, Seo, Hee-Jong, Serrano, Santiago, Shafieloo, Arman, Shan, Huanyuan, Sharples, Ray, Sholl, Michael J., Shourt, William V., Silber, Joseph H., Silva, David R., Sirk, Martin M., Slosar, Anze, Smith, Alex, Smoot, George F., Som, Debopam, Song, Yong-Seon, Sprayberry, David, Staten, Ryan, Stefanik, Andy, Tarle, Gregory, Tie, Suk Sien, Tinker, Jeremy L., Tojeiro, Rita, Valdes, Francisco, Valenzuela, Octavio, Valluri, Monica, Vargas-Magana, Mariana, Verde, Licia, Walker, Alistair R., Wang, Jiali, Wang, Yuting, Weaver, Benjamin A., Weaverdyck, Curtis, Wechsler, Risa H., Weinberg, David H., White, Martin, Yang, Qian, Yeche, Christophe, Zhang, Tianmeng, Zhao, Gong-Bo, Zheng, Yi, Zhou, Xu, Zhou, Zhimin, Zhu, Yaling, Zou, Hu, and Zu, Ying
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: DESI (Dark Energy Spectropic Instrument) is a Stage IV ground-based dark energy experiment that will study baryon acoustic oscillations and the growth of structure through redshift-space distortions with a wide-area galaxy and quasar redshift survey. The DESI instrument is a robotically-actuated, fiber-fed spectrograph capable of taking up to 5,000 simultaneous spectra over a wavelength range from 360 nm to 980 nm. The fibers feed ten three-arm spectrographs with resolution $R= \lambda/\Delta\lambda$ between 2000 and 5500, depending on wavelength. The DESI instrument will be used to conduct a five-year survey designed to cover 14,000 deg$^2$. This powerful instrument will be installed at prime focus on the 4-m Mayall telescope in Kitt Peak, Arizona, along with a new optical corrector, which will provide a three-degree diameter field of view. The DESI collaboration will also deliver a spectroscopic pipeline and data management system to reduce and archive all data for eventual public use.
Published: 2016

4. Super-resolution method using sparse regularization for point-spread function recovery

Author: Mboula, Fred Maurice Ngolè, Starck, Jean-Luc, Ronayette, Samuel, Okumura, Koryo, and Amiaux, Jérôme
Subjects: Computer Science - Computer Vision and Pattern Recognition, Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: In large-scale spatial surveys, such as the forthcoming ESA Euclid mission, images may be undersampled due to the optical sensors sizes. Therefore, one may consider using a super-resolution (SR) method to recover aliased frequencies, prior to further analysis. This is particularly relevant for point-source images, which provide direct measurements of the instrument point-spread function (PSF). We introduce SPRITE, SParse Recovery of InsTrumental rEsponse, which is an SR algorithm using a sparse analysis prior. We show that such a prior provides significant improvements over existing methods, especially on low SNR PSFs.
Published: 2014
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5. The ELT/METIS Annular Groove Phase Masks

Author: Delacroix, Christian, König, Lorenzo, Absil, Olivier, Orban De Xivry, Gilles, Forsberg, Pontus, Karlsson, Mikael, Ronayette, Samuel, Pantin, Eric, Barrière, Jean-Christophe, Delacroix, Christian, König, Lorenzo, Absil, Olivier, Orban De Xivry, Gilles, Forsberg, Pontus, Karlsson, Mikael, Ronayette, Samuel, Pantin, Eric, and Barrière, Jean-Christophe
Published: 2024
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6. SPICES: Spectro-Polarimetric Imaging and Characterization of Exoplanetary Systems

Author: Boccaletti, Anthony, Schneider, Jean, Traub, Wes, Lagage, Pierre-Olivier, Stam, Daphne, Gratton, Raffaele, Trauger, John, Cahoy, Kerri, Snik, Frans, Baudoz, Pierre, Galicher, Raphael, Reess, Jean-Michel, Mawet, Dimitri, Augereau, Jean-Charles, Patience, Jennifer, Kuchner, Marc, Wyatt, Mark, Pantin, Eric, Maire, Anne-Lise, Verinaud, Christophe, Ronayette, Samuel, Dubreuil, Didier, Min, Michiel, Rodenhuis, Michiel, Mesa, Dino, Belikov, Ruslan, Guyon, Olivier, Tamura, Motohide, Murakami, Naoshi, Beerer, Ingrid Mary, and team, the SPICES
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: SPICES (Spectro-Polarimetric Imaging and Characterization of Exoplanetary Systems) is a five-year M-class mission proposed to ESA Cosmic Vision. Its purpose is to image and characterize long-period extrasolar planets and circumstellar disks in the visible (450 - 900 nm) at a spectral resolution of about 40 using both spectroscopy and polarimetry. By 2020/22, present and near-term instruments will have found several tens of planets that SPICES will be able to observe and study in detail. Equipped with a 1.5 m telescope, SPICES can preferentially access exoplanets located at several AUs (0.5-10 AU) from nearby stars ($<$25 pc) with masses ranging from a few Jupiter masses to Super Earths ($\sim$2 Earth radii, $\sim$10 M$_{\oplus}$) as well as circumstellar disks as faint as a few times the zodiacal light in the Solar System.
Published: 2012
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7. The ELT/METIS annular groove phase masks

Author: Navarro, Ramón, Jedamzik, Ralf, Delacroix, Christian, König, Lorenzo, Absil, Olivier, Orban De Xivry, Gilles, Forsberg, Pontus, Karlsson, Mikael, Ronayette, Samuel, Pantin, Eric, and Barrière, Jean-Christophe
Published: 2024
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8. The DDRAGO wide-field imager for the COLIBRÍ telescope

Author: Bryant, Julia J., Motohara, Kentaro, Vernet, Joël R. D., Langarica, Rosalía, Watson, Alan M., Álvarez Núñez, Luis Carlos, Angeles, Fernando, Atteia, Jean-Luc, Basa, Stéphane, Cuevas, Salvador, Dolon, François, Farah, Alejandro, Dornic, Damien, Floriot, Johan, Fuentes-Fernández, Jorge, Langlois, Arthur, Lee, William H., Lombardo, Simona, Pereyra, Margarita, Ruíz Díaz-Soto, Jaime, Ronayette, Samuel, Tinoco, Silvio, and Valentín, Hervé
Published: 2024
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9. The Mid-Infrared Instrument for the James Webb Space Telescope , IV: The Low-Resolution Spectrometer

Author: Kendrew, Sarah, Scheithauer, Silvia, Bouchet, Patrice, Amiaux, Jerome, Azzollini, Ruymán, Bouwman, Jeroen, Chen, C. H., Dubreuil, D., Fischer, Sebastian, Glasse, Alistair, Greene, T. P., Lagage, P.-O., Lahuis, Fred, Ronayette, Samuel, Wright, David, and Wright, G. S.
Published: 2015
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10. The Mid-Infrared Instrument for the James Webb Space Telescope , III: MIRIM, The MIRI Imager

Author: Bouchet, Patrice, García-Marín, Macarena, Lagage, P.-O., Amiaux, Jérome, Auguéres, J.-L., Bauwens, Eva, Blommaert, J. A. D. L., Chen, C. H., Detre, Ö. H., Dicken, Dan, Dubreuil, D., Galdemard, Ph., Gastaud, R., Glasse, A., Gordon, K. D., Gougnaud, F., Guillard, Phillippe, Justtanont, K., Krause, Oliver, Leboeuf, Didier, Longval, Yuying, Martin, Laurant, Mazy, Emmanuel, Moreau, Vincent, Olofsson, Göran, Ray, T. P., Rees, J.-M., Renotte, Etienne, Ressler, M. E., Ronayette, Samuel, Salasca, Sophie, Scheithauer, Silvia, Sykes, Jon, Thelen, M. P., Wells, Martyn, Wright, David, and Wright, G. S.
Published: 2015
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11. Quantix and Intrapix: test benches dedicated to quantum efficiency measurement and intra-pixel response of detectors from VIS to LWIR

Author: Pichon, Thibault, primary, Bounab, Ayoub, additional, Cervera, Cyril, additional, Delisle, Cyrille, additional, Derelle, Sophie, additional, Dubreuil, Didier, additional, Horeau, Benoit, additional, Huard, Eduard, additional, Ketchazo, Christian, additional, Moreau, Vincent, additional, Mulet, Patrick, additional, Lortholary, Michel, additional, Orduna, Thierry, additional, Provost, Léna, additional, Ronayette, Samuel, additional, Tellier, Olivier, additional, and Boulade, Olivier, additional
Published: 2022
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12. Characterization of the MIRIm double prism assembly at short wavelengths: implications for transit observations of exoplanets

Author: Bouchet, Patrice, primary, Gastaud, René, additional, Lagage, Pierre-Olivier, additional, Kendrew, Sarah, additional, Bombardi, Oriane, additional, Coulais, Alain, additional, Ronayette, Samuel, additional, Sloan, Gregory C., additional, Moreau, Vincent, additional, Orduna, Thierry, additional, Grégoire, Emmanuel, additional, Dyrek, Achrène, additional, Bouwman, Jeroen, additional, Glasse, Alistair C., additional, and Wright, Gillian S., additional
Published: 2022
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13. COLIBRI, a wide-field 1.3 m robotic telescope dedicated to the transient sky

Author: Basa, Stéphane, primary, Lee, William H., additional, Dolon, François, additional, Watson, Alan M., additional, Floriot, Johan, additional, Atteia, Jean-Luc, additional, Butler, Nathaniel, additional, Dornic, Damien, additional, Lombardo, Simona, additional, Ronayette, Samuel, additional, Ageron, Michel, additional, Agneray, François, additional, Ángeles, Fernando, additional, Bautista, Ludovik, additional, Benamar-Aissa, Hafid, additional, Blanpain, Cyrille, additional, Boulade, Olivier, additional, Boy, Jérémie, additional, Buat, Veronique, additional, Cadena, Edgar, additional, Cuevas, Salvador, additional, Farah, Alejandro, additional, Figueroa, Liliana, additional, Fuentes, Jorge, additional, Gaïti, Carole, additional, Gallais, Pascal, additional, Kajfasz, Eric, additional, Langarica, Rosalía, additional, Langlois, Arthur, additional, Larrieu, Marie, additional, Le Van Suu, Auguste, additional, Lecubin, Julien, additional, López Ángeles, Eduardo, additional, Lugo-Ibarra, Erica E., additional, Malgoyre, Adrien, additional, Mathon, Romain, additional, Moreau, Chrystel, additional, Nouvel-De-La-Fleche, Alix, additional, Ochoa, José L., additional, Pedrayes-López, María H., additional, Ramon, Pascale, additional, Ruíz-Díaz-Soto, Jaime, additional, Tinoco, Silvio, additional, and Valentin, Hervé, additional
Published: 2022
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14. An N-band test bench for the METIS coronagraphic masks

Author: Ronayette, Samuel, primary, Mouzali, Salima, additional, Barrière, Jean Christophe, additional, Pantin, Éric, additional, Orduna, Thierry, additional, Gallais, Pascal, additional, Lortholary, Michel, additional, Dumaye, Luc, additional, Absil, Olivier, additional, Delacroix, Christian, additional, Ives, Derek J., additional, and Karlsson, Mikael, additional
Published: 2020
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15. Testing the 10 spectrograph units for DESI: approach and results

Author: Perruchot, Sandrine, primary, Blanc, Pierre-Éric, additional, Guy, Julien, additional, Le Guillou, Laurent, additional, Ronayette, Samuel, additional, Régal, Xavier, additional, Castagnoli, Gérard, additional, Le Van Suu, Auguste, additional, Sepulveda, Eduardo, additional, Jullo, Eric, additional, Cuby, Jean-Gabriel, additional, Karkar, Sonia, additional, Ghislain, Patrick, additional, Repain, Philippe, additional, Carton, P.-H., additional, Magneville, C., additional, Ealet, Anne, additional, Escoffier, Stéphanie, additional, Secroun, Aurélia, additional, Honscheid, Klaus, additional, Elliott, Ann, additional, Jelinsky, Patrick N., additional, David, Brooks, additional, Peter, Doel, additional, Yutong, Duan, additional, Jerry, Edelstein, additional, Juan Cruz, Estrada, additional, Enrique, Gastañaga, additional, Armin, Karcher, additional, Martin, Landriau, additional, Michael, Levi, additional, Paul, Martini, additional, Nathalie, Palanque-Delabrouille, additional, Francisco, Prada, additional, Gragory, Tarle, additional, and Kai, Zhang, additional
Published: 2020
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16. An N-band test bench for the METIS coronagraphic masks

Author: Ronayette, Samuel, Mouzali, Salima, Barrière, Jean-Christophe, Pantin, Éric, Orduna, Thierry, Gallais, Pascal, Lortholary, Michel, Dumaye, Luc, Absil, Olivier, Delacroix, Christian, Ives, Derek, Karlsson, Mikael, Ronayette, Samuel, Mouzali, Salima, Barrière, Jean-Christophe, Pantin, Éric, Orduna, Thierry, Gallais, Pascal, Lortholary, Michel, Dumaye, Luc, Absil, Olivier, Delacroix, Christian, Ives, Derek, and Karlsson, Mikael
Abstract: METIS is one of the first three instruments for the ELT, Europe's next-generation ground-based telescope. It will offer imaging, coronagraphy and spectroscopy in the L, M and N bands for general-purpose science in astrophysics. Among its main science drivers are circumstellar disks and extrasolar planets observations, which requires demanding high contrast imaging techniques. In that framework, METIS will be equipped with state-of-the-art phase mask coronagraphs: Apodizing Phase Plate (APP) and Annular Grooves Phase Mask (AGPM). Manufacturing the AGPM coronagraphs is a complex process that requires performance assessment with specific testing before implementation into the instrument. At Department of Astrophysics (CEA Saclay, France), responsible for the testing of the N-band AGPMs, a previously available test bench with a telescope simulator and cryogenic facility has been upgraded to comply with the AGPM tests requirements. This paper presents these requirements and describes the test bench design adopted. Then, based on preliminary results, we discuss the original solutions that permitted to reach our goals.
Published: 2020
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17. COLIBRI, a wide-field 1.3 m robotic telescope dedicated to the transient sky

Author: Marshall, Heather K., Spyromilio, Jason, Usuda, Tomonori, Basa, Stéphane, Lee, William H., Dolon, François, Watson, Alan M., Floriot, Johan, Atteia, Jean-Luc, Butler, Nathaniel R., Dornic, Damien, Lombardo, Simona, Ronayette, Samuel, Ageron, Michel, Agneray, François, Ángeles, Fernando, Bautista, Ludovik, Benamar-Aissa, Hafid, Blanpain, Cyril, Boulade, Olivier, Boy, Jérémie, Buat, Veronique, Cadena, Edgar, Cuevas, Salvador, Farah, Alejandro, Figueroa, Liliana, Fuentes, Jorge, Gaïti, Carole, Gallais, Pascal, Kajfasz, Eric, Langarica, Rosalía, Langlois, Arthur, Larrieu, Marie, Le Van Suu, Auguste, Lecubin, Julien, López Ángeles, Eduardo, Lugo, Erica, Malgoyre, Adrien, Mathon, Romain, Moreau, Chrystel, Nouvel-De-La-Flèche, Alix, Ochoa, José Luis, Pedrayes-López, Maria, Ramon, Pascale, Ruíz-Díaz-Soto, Jaime, Tinoco, Silvio, and Valentin, Hervé
Published: 2022
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18. Primary and secondary mirror manufacturing for COLIBRI ground follow-up telescope of the SVOM mission

Author: Floriot, Johan, primary, Marcos, Michel, primary, Fuentes-Fernández, Jorge, primary, Watson, Alan, primary, Cuevas Cardona, Salvador, primary, Lee, William H., primary, Basa, Stéphane, primary, Corre, David, primary, Ferrari, Marc, primary, Dohlen, Kjetil, primary, Ángeles Uribe, Fernando, primary, Farah Simon, Alejandro, primary, Langarica Lebre, Rosaliá, primary, Pallier, Etienne, primary, Platzer, Jacqueline, primary, Klotz, Alain, primary, Atteia, Jean-Luc, primary, Valentin, Hervé, primary, Mathon, Romain, primary, Boy, Jérémie, primary, Ambert, Philippe, primary, Le Borgne, Jean-François, primary, Dornic, Damien, primary, Meessen, Christophe, primary, Ageron, Michel, primary, Boulade, Olivier, primary, Cordier, Bertrand, primary, Dubreuil, Didier, primary, Ronayette, Samuel, primary, Gallais, Pascal, primary, Le Van Suu, Auguste, primary, Blanc, Pierre-Éric, primary, Dolon, François, primary, Hugot, E., primary, Jiménez-Bailón, Elena, primary, Ochoa, José Luis, primary, Quirós, Fernando, primary, Cadena, Edgar, primary, and Figueroa, Liliana, primary
Published: 2018
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19. End-to-end simulations for COLIBRI, ground follow-up telescope for the SVOM mission.

Author: Corre, David, primary, Basa, Stéphane, primary, Klotz, Alain, primary, Watson, Alan Morgan, primary, Ageron, Michel, primary, Ambert, Philippe, primary, Ángeles, Fernando, primary, Atteia, Jean-Luc, primary, Blanc, Pierre-Éric, primary, Boulade, Olivier, primary, Boy, Jérémie, primary, Cadena, Edgar, primary, Cordier, Bertrand, primary, Cuevas Cardona, Salvador, primary, Dolon, François, primary, Dornic, Damien, primary, Dubreuil, Didier, primary, Farah, Alejandro, primary, Figueroa, Liliana, primary, Floriot, Johan, primary, Fuentes-Fernández, Jorge, primary, Gallais, Pascal, primary, Jiménez-Bailón, Elena, primary, Langarica Lebre, Rosaliá, primary, Le Borgne, Jean-François, primary, Lee, William Henry, primary, Le Van Suu, Auguste, primary, Marcos, Michel, primary, Mathon, Romain, primary, Meessen, Christophe, primary, Ochoa, José Luis, primary, Pallier, Etienne, primary, Platzer, Jacqueline, primary, Quirós, Fernando, primary, Ronayette, Samuel, primary, Valentin, Hervé, primary, Vergani, Susanna, primary, and Turpin, Damien, primary
Published: 2018
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20. Integration and testing of the DESI multi-object spectrograph: performance tests and results for the first unit out of ten

Author: Perruchot, Sandrine, primary, Guy, Julien, primary, Le Guillou, Laurent, primary, Blanc, Pierre-Éric, primary, Ronayette, Samuel, primary, Régal, Xavier, primary, Castagnoli, Gérard, primary, Le Van Suu, Auguste, primary, Jullo, Eric, primary, Cuby, Jean-Gabriel, primary, Ghislain, Patrick, primary, Repain, Philippe, primary, Ealet, Anne, primary, Escoffier, Stéphanie, primary, Honscheid, Klaus, primary, Elliot, Ann, primary, Jelinsky, Patrick N., primary, Karkar, Sonia, primary, Sepulveda, Eduardo, primary, Carton, Pierre-Henri, primary, Magneville, Christophe, primary, Cousinou, Marie-Claude, primary, Brooks, David, primary, Tarlè, Gregory, primary, and Secroun, A., primary
Published: 2018
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21. The DESI Experiment Part I: Science,Targeting, and Survey Design

Author: Aghamousa, Amir, Aguilar, Jessica, Ahlen, Steve, Alam, Shadab, Allen, Lori E., Prieto, Carlos Allende, Annis, James, Bailey, Stephen, Balland, Christophe, Ballester, Otger, Baltay, Charles, Beaufore, Lucas, Bebek, Chris, Beers, Timothy C., Bell, Eric F., Bernal, José Luis, Besuner, Robert, Beutler, Florian, Blake, Chris, Bleuler, Hannes, Blomqvist, Michael, Blum, Robert, Bolton, Adam S., Briceno, Cesar, Brooks, David, Brownstein, Joel R., Buckley-Geer, Elizabeth, Burden, Angela, Burtin, Etienne, Busca, Nicolás G., Cahn, Robert N., Cai, Yan-Chuan, Cardiel-Sas, Laia, Carlberg, Raymond G., Carton, Pierre-Henri, Casas, Ricard, Castander, Francisco J., Cervantes-Cota, Jorge L., Claybaugh, Todd M., Close, Madeline, Coker, Carl T., Cole, Shaun, Comparat, Johan, Cooper, Andrew P., Cousinou, M. -C., Crocce, Martin, Cuby, Jean-Gabriel, Cunningham, Daniel P., Davis, Tamara M., Dawson, Kyle S., de La Macorra, Axel, de Vicente, Juan, Delubac, Timothée, Derwent, Mark, Dey, Arjun, Dhungana, Govinda, Ding, Zhejie, Doel, Peter, Duan, Yutong T., Ealet, Anne, Edelstein, Jerry, Eftekharzadeh, Sarah, Eisenstein, Daniel J., Elliott, Ann, Escoffier, Stephanie, Evatt, Matthew, Fagrelius, Parker, Fan, Xiaohui, Fanning, Kevin, Farahi, Arya, Farihi, Jay, Favole, Ginevra, Feng, Yu, Fernandez, Enrique, Findlay, Joseph R., Finkbeiner, Douglas P., Fitzpatrick, Michael J., Flaugher, Brenna, Flender, Samuel, Font-Ribera, Andreu, Forero-Romero, Jaime E., Fosalba, Pablo, Frenk, Carlos S., Fumagalli, Michele, Gaensicke, Boris T., Gallo, Giuseppe, Garcia-Bellido, Juan, Gaztanaga, Enrique, Fusillo, Nicola Pietro Gentile, Gerard, Terry, Gershkovich, Irena, Giannantonio, Tommaso, Gillet, Denis, Gonzalez-De-Rivera, Guillermo, Gonzalez-Perez, Violeta, Gott, Shelby, Graur, Or, Gutierrez, Gaston, Guy, Julien, Habib, Salman, Heetderks, Henry, Heetderks, Ian, Heitmann, Katrin, Hellwing, Wojciech A., Herrera, David A., Ho, Shirley, Holland, Stephen, Honscheid, Klaus, Huff, Eric, Hutchinson, Timothy A., Huterer, Dragan, Hwang, Ho Seong, Laguna, Joseph Maria Illa, Ishikawa, Yuzo, Jacobs, Dianna, Jeffrey, Niall, Jelinsky, Patrick, Jennings, Elise, Jiang, Linhua, Jimenez, Jorge, Johnson, Jennifer, Joyce, Richard, Jullo, Eric, Juneau, Stéphanie, Kama, Sami, Karcher, Armin, Karkar, Sonia, Kehoe, Robert, Kennamer, Noble, Kent, Stephen, Kilbinger, Martin, Kim, Alex G., Kirkby, David, Kisner, Theodore, Kitanidis, Ellie, Kneib, Jean-Paul, Koposov, Sergey, Kovacs, Eve, Koyama, Kazuya, Kremin, Anthony, Kron, Richard, Kronig, Luzius, Kueter-Young, Andrea, Lacey, Cedric G., Lafever, Robin, Lahav, Ofer, Lambert, Andrew, Lampton, Michael, Landriau, Martin, Lang, Dustin, Lauer, Tod R., Goff, Jean-Marc Le, Guillou, Laurent Le, van Suu, Auguste Le, Lee, Jae Hyeon, Lee, Su-Jeong, Leitner, Daniela, Lesser, Michael, Levi, Michael E., L'Huillier, Benjamin, Li, Baojiu, Liang, Ming, Lin, Huan, Linder, Eric, Loebman, Sarah R., Lukić, Zarija, Ma, Jun, Maccrann, Niall, Magneville, Christophe, Makarem, Laleh, Manera, Marc, Manser, Christopher J., Marshall, Robert, Martini, Paul, Massey, Richard, Matheson, Thomas, Mccauley, Jeremy, Mcdonald, Patrick, Mcgreer, Ian D., Meisner, Aaron, Metcalfe, Nigel, Miller, Timothy N., Miquel, Ramon, Moustakas, John, Myers, Adam, Naik, Milind, Newman, Jeffrey A., Nichol, Robert C., Nicola, Andrina, da Costa, Luiz Nicolati, Nie, Jundan, Niz, Gustavo, Norberg, Peder, Nord, Brian, Norman, Dara, Nugent, Peter, O'Brien, Thomas, Oh, Minji, Olsen, Knut A. G., Padilla, Cristobal, Padmanabhan, Hamsa, Padmanabhan, Nikhil, Palanque-Delabrouille, Nathalie, Palmese, Antonella, Pappalardo, Daniel, Paris, Isabelle, Park, Changbom, Patej, Anna, Peacock, John A., Peiris, Hiranya V., Peng, Xiyan, Percival, Will J., Perruchot, Sandrine, Pieri, Matthew M., Pogge, Richard, Pollack, Jennifer E., Poppett, Claire, Prada, Francisco, Prakash, Abhishek, Probst, Ronald G., Rabinowitz, David, Raichoor, Anand, Ree, Chang Hee, Refregier, Alexandre, Régal, Xavier, Reid, Beth, Reil, Kevin, Rezaie, Mehdi, Rockosi, Constance M., Roe, Natalie, Ronayette, Samuel, Roodman, Aaron, Ross, Ashley J., Ross, Nicholas P., Rossi, Graziano, Rozo, Eduardo, Ruhlmann-Kleider, Vanina, Rykoff, Eli S., Sabiu, Cristiano, Samushia, Lado, Sanchez, Eusebio, Sanchez, Javier, Schlegel, David J., Schneider, Michael, Schubnell, Michael, Secroun, Aurélia, Seljak, Uros, Seo, Hee-Jong, Serrano, Santiago, Shafieloo, Arman, Shan, Huanyuan, Sharples, Ray, Sholl, Michael J., Shourt, William V., Silber, Joseph H., Silva, David R., Sirk, Martin M., Slosar, Anze, Smith, Alex, Smoot, George F., Som, Debopam, Song, Yong-Seon, Sprayberry, David, Staten, Ryan, Stefanik, Andy, Tarlè, Gregory, Tie, Suk Sien, Tinker, Jeremy L., Tojeiro, Rita, Valdes, Francisco, Valenzuela, Octavio, Valluri, Monica, Vargas-Magaña, Mariana, Verde, Licia, Walker, Alistair R., Wang, Jiali, Wang, Yuting, Weaver, Benjamin A., Weaverdyck, Curtis, Wechsler, Risa H., Weinberg, David H., White, Martin, Yang, Qian, Yeche, Christophe, Zhang, Tianmeng, Zhao, Gong-Bo, Zheng, Yi, Zhou, Xu, Zhou, Zhimin, Zhu, Yaling, Zou, Hu, Zu, Ying, Korea Astronomy and Space Science Institute (KASI), Okayama University, University of California [Berkeley], University of California, National Optical Astronomy Observatory (NOAO), Instituto de Astrofisica de Canarias (IAC), Fermi National Accelerator Laboratory (Fermilab), Lawrence Berkeley National Laboratory [Berkeley] (LBNL), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Institut de Física d’Altes Energies [Barcelone] (IFAE), Universitat Autònoma de Barcelona (UAB), Yale University [New Haven], Ohio State University [Columbus] (OSU), The University of Notre Dame [Sydney], Department of Astronomy, University of Michigan, University of Michigan [Ann Arbor], University of Michigan System-University of Michigan System, Institut de Ciencies del Cosmos (ICCUB), Universitat de Barcelona (UB), Space Sciences Laboratory [Berkeley] (SSL), University of California-University of California, University of Portsmouth, University of British Columbia (UBC), Ecole Polytechnique Fédérale de Lausanne (EPFL), Laboratoire d'Astrophysique de Marseille (LAM), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES), Cerro Tololo Inter-American Observatory, Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, APC - Cosmologie, AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Institute for Astronomy [Edinburgh] (IfA), University of Edinburgh, Department of Astronomy & Astrophysics [University of Toronto], University of Toronto, Institut de Ciencies de l'Espai [Barcelona] (ICE-CSIC), Consejo Superior de Investigaciones Científicas [Madrid] (CSIC), Carreterra Mexico-Toluca, Department of Physics [Durham University], Durham University, Department of Astronomy, The Ohio State University, Departamento de FisicaTeorica e IFT-UAM/CSIC, Universidad Autonoma de Madrid (UAM), Institute for Computational Cosmology (ICC), Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Universidad Nacional Autónoma de México (UNAM), Department of Applied Physics, Departamento de Fisica Aplicada [Granada], Universidad de Granada (UGR)-Universidad de Granada (UGR), University College of London [London] (UCL), University of Wyoming (UW), Harvard-Smithsonian Center for Astrophysics (CfA), Harvard University [Cambridge]-Smithsonian Institution, Arizona State University [Tempe] (ASU), Department of Information Engineering, Zhejiang University of Technology, Zhejiang University of Technology, Institute for Astronomy [Honolulu], University of Hawai‘i [Mānoa] (UHM), Università degli Studi di Milano-Bicocca [Milano] (UNIMIB), Departamento de Fisica Teorica, Institute of Cosmology & Gravitation [Portsmouth], Carnegie Mellon University [Pittsburgh] (CMU), NASA Goddard Space Flight Center (GSFC), Korea Institute for Advanced Study (KIAS), Department of Physics and Astronomy [Irvine], University of California [Irvine] (UCI), Department of Physics, University of California, University of California [Los Angeles] (UCLA), Institute of Astronomy [Cambridge], University of Cambridge [UK] (CAM), Institute of Cosmology & Gravitation, Dennis Sciama Building, University of Portsmouth, Observatoire de Haute-Provence (OHP), Institut Pythéas (OSU PYTHEAS), Institut de Recherche pour le Développement (IRD)-Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Institut de Recherche pour le Développement (IRD)-Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE), Center for Cosmology & AstroParticle Physics, California Institute of Technology (CALTECH), Department of Physics and Astronomy [Pittsburgh], University of Pittsburgh (PITT), Pennsylvania Commonwealth System of Higher Education (PCSHE)-Pennsylvania Commonwealth System of Higher Education (PCSHE), Institute for Astronomy [Zürich], Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology [Zürich] (ETH Zürich), School of Physics and Astronomy [Nottingham], University of Nottingham, UK (UON), Department of Physics [Durham], University of New Hampshire (UNH), University of Waterloo [Waterloo], Universität Zürich [Zürich] = University of Zurich (UZH), Department of Astronomy and Space Science [Sejong University], Sejong University, Department of Physics [Oxford], University of Oxford [Oxford], Institute of Plasma Physics, Chinese Academy of Sciences (ASIPP), Department of Physics [Ann Arbor], University of St Andrews [Scotland], University of Science and Technology of China [Hefei] (USTC), Department of Computer Science and Engineering [Minneapolis], University of Minnesota [Twin Cities] (UMN), University of Minnesota System-University of Minnesota System, Karlsruhe Institute of Technology (KIT), National University of Defense Technology [China], DESI Collaboration, University of California [Berkeley] (UC Berkeley), University of California (UC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), University of California (UC)-University of California (UC), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Universidad Autónoma de Madrid (UAM), Universidad Nacional Autónoma de México = National Autonomous University of Mexico (UNAM), Universidad de Granada = University of Granada (UGR)-Universidad de Granada = University of Granada (UGR), Harvard University-Smithsonian Institution, Università degli Studi di Milano-Bicocca = University of Milano-Bicocca (UNIMIB), University of California [Irvine] (UC Irvine), University of Oxford, and Escoffier, Stephanie
Subjects: [PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], Astrophysics::Cosmology and Extragalactic Astrophysics, [PHYS.ASTR.IM] Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], Astrophysics::Galaxy Astrophysics
Abstract: DESI (Dark Energy Spectroscopic Instrument) is a Stage IV ground-based dark energy experiment that will study baryon acoustic oscillations (BAO) and the growth of structure through redshift-space distortions with a wide-area galaxy and quasar redshift survey. To trace the underlying dark matter distribution, spectroscopic targets will be selected in four classes from imaging data. We will measure luminous red galaxies up to $z=1.0$. To probe the Universe out to even higher redshift, DESI will target bright [O II] emission line galaxies up to $z=1.7$. Quasars will be targeted both as direct tracers of the underlying dark matter distribution and, at higher redshifts ($ 2.1 < z < 3.5$), for the Ly-$\alpha$ forest absorption features in their spectra, which will be used to trace the distribution of neutral hydrogen. When moonlight prevents efficient observations of the faint targets of the baseline survey, DESI will conduct a magnitude-limited Bright Galaxy Survey comprising approximately 10 million galaxies with a median $z\approx 0.2$. In total, more than 30 million galaxy and quasar redshifts will be obtained to measure the BAO feature and determine the matter power spectrum, including redshift space distortions.
Published: 2016

22. The mid-infrared instrument for the James Webb Space Telescope: performance and operation of the Low-Resolution Spectrometer

Author: Kendrew, Sarah, additional, Scheithauer, Silvia, additional, Bouchet, Patrice, additional, Amiaux, Jerome, additional, Azzollini, Ruymán, additional, Bouwman, Jeroen, additional, Chen, Christine, additional, Dubreuil, Didier, additional, Fischer, Sebastian, additional, Fox, Ori D., additional, Glasse, Alistair, additional, Gordon, Karl, additional, Greene, Tom, additional, Hines, Dean C., additional, Lagage, Pierre-Olivier, additional, Lahuis, Fred, additional, Ronayette, Samuel, additional, Wright, David, additional, and Wright, Gillian S., additional
Published: 2016
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23. The Mid-Infrared Instrument for theJames Webb Space Telescope, IV: The Low-Resolution Spectrometer

Author: Kendrew, Sarah, primary, Scheithauer, Silvia, additional, Bouchet, Patrice, additional, Amiaux, Jerome, additional, Azzollini, Ruymán, additional, Bouwman, Jeroen, additional, Chen, C. H., additional, Dubreuil, D., additional, Fischer, Sebastian, additional, Glasse, Alistair, additional, Greene, T. P., additional, Lagage, P.-O., additional, Lahuis, Fred, additional, Ronayette, Samuel, additional, Wright, David, additional, and Wright, G. S., additional
Published: 2015
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24. The Mid-Infrared Instrument for theJames Webb Space Telescope, III: MIRIM, The MIRI Imager

Author: Bouchet, Patrice, primary, García-Marín, Macarena, additional, Lagage, P.-O., additional, Amiaux, Jérome, additional, Auguéres, J.-L., additional, Bauwens, Eva, additional, Blommaert, J. A. D. L., additional, Chen, C. H., additional, Detre, Ö. H., additional, Dicken, Dan, additional, Dubreuil, D., additional, Galdemard, Ph., additional, Gastaud, R., additional, Glasse, A., additional, Gordon, K. D., additional, Gougnaud, F., additional, Guillard, Phillippe, additional, Justtanont, K., additional, Krause, Oliver, additional, Leboeuf, Didier, additional, Longval, Yuying, additional, Martin, Laurant, additional, Mazy, Emmanuel, additional, Moreau, Vincent, additional, Olofsson, Göran, additional, Ray, T. P., additional, Rees, J.-M., additional, Renotte, Etienne, additional, Ressler, M. E., additional, Ronayette, Samuel, additional, Salasca, Sophie, additional, Scheithauer, Silvia, additional, Sykes, Jon, additional, Thelen, M. P., additional, Wells, Martyn, additional, Wright, David, additional, and Wright, G. S., additional
Published: 2015
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25. TALC: a new deployable concept for a 20m far-infrared space telescope

Author: Durand, Gilles, additional, Sauvage, Marc, additional, Bonnet, Aymeric, additional, Rodriguez, Louis, additional, Ronayette, Samuel, additional, Chanial, Pierre, additional, Scola, Loris, additional, Révéret, Vincent, additional, Aussel, Hervé, additional, Carty, Michael, additional, Durand, Matthis, additional, Durand, Lancelot, additional, Tremblin, Pascal, additional, Pantin, Eric, additional, Berthe, Michel, additional, Martignac, Jérôme, additional, Motte, Frédérique, additional, Talvard, Michel, additional, Minier, Vincent, additional, and Bultel, Pascal, additional
Published: 2014
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26. The science case and data processing strategy for the Thinned Aperture Light Collector (TALC): a project for a 20m far-infrared space telescope

Author: Sauvage, Marc, additional, Chanial, Pierre, additional, Durand, Gilles A., additional, Rodriguez, Louis R., additional, Starck, Jean-Luc, additional, Ronayette, Samuel, additional, Aussel, Hervé, additional, Minier, Vincent, additional, Motte, Frédérique, additional, Pantin, Eric J., additional, Sureau, Florent, additional, and Terrisse, Robin, additional
Published: 2014
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27. Antarctic observations at long wavelengths with the IRAIT-ITM Telescope at Dome C

Author: Durand, Gilles A., additional, Tremblin, Pascal, additional, Minier, Vincent, additional, Reinert, Yann, additional, Leroy dos Santos, Christophe, additional, Rodriguez, Louis, additional, Joffrin, Xavier, additional, Busso, Maurizio, additional, Tosti, Gino, additional, Nucciarelli, Giuliano, additional, Dolci, Mauro, additional, Straniero, Oscar, additional, Valentini, Angelo, additional, Abia, Carlos, additional, Christille, Jean Marc, additional, Doumayrou, Eric, additional, Lortholary, Michel, additional, Charron, Patrice, additional, Lotrus, Paul, additional, Walter, Christian, additional, Ronayette, Samuel, additional, Challita, Zalpha, additional, Fromont, Laurent, additional, Condamin, Mathieu, additional, Kwon, Min Kyong, additional, and Tavagnacco, Daniele, additional
Published: 2014
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28. SPICES: spectro-polarimetric imaging and characterization of exoplanetary systems

Author: Massachusetts Institute of Technology. Department of Aeronautics and Astronautics, Cahoy, Kerri, Boccaletti, Anthony, Schneider, Jean, Traub, Wes, Lagage, Pierre-Olivier, Stam, Daphne, Gratton, Raffaele, Trauger, John, Snik, Frans, Baudoz, Pierre, Galicher, Raphael, Reess, Jean-Michel, Mawet, Dimitri, Augereau, Jean-Charles, Patience, Jenny, Kuchner, Marc J., Wyatt, Mark, Pantin, Eric, Maire, Anne-Lise, Vérinaud, Christophe, Ronayette, Samuel, Dubreuil, Didier, Min, Michiel, Rodenhuis, Michiel, Mesa, Dino, Belikov, Russ, Guyon, Olivier, Tamura, Motohide, Murakami, Naoshi, Beerer, Ingrid Mary, Massachusetts Institute of Technology. Department of Aeronautics and Astronautics, Cahoy, Kerri, Boccaletti, Anthony, Schneider, Jean, Traub, Wes, Lagage, Pierre-Olivier, Stam, Daphne, Gratton, Raffaele, Trauger, John, Snik, Frans, Baudoz, Pierre, Galicher, Raphael, Reess, Jean-Michel, Mawet, Dimitri, Augereau, Jean-Charles, Patience, Jenny, Kuchner, Marc J., Wyatt, Mark, Pantin, Eric, Maire, Anne-Lise, Vérinaud, Christophe, Ronayette, Samuel, Dubreuil, Didier, Min, Michiel, Rodenhuis, Michiel, Mesa, Dino, Belikov, Russ, Guyon, Olivier, Tamura, Motohide, Murakami, Naoshi, and Beerer, Ingrid Mary
Abstract: SPICES (Spectro-Polarimetric Imaging and Characterization of Exoplanetary Systems) is a five-year M-class mission proposed to ESA Cosmic Vision. Its purpose is to image and characterize long-period extrasolar planets and circumstellar disks in the visible (450–900 nm) at a spectral resolution of about 40 using both spectroscopy and polarimetry. By 2020/2022, present and near-term instruments will have found several tens of planets that SPICES will be able to observe and study in detail. Equipped with a 1.5 m telescope, SPICES can preferentially access exoplanets located at several AUs (0.5–10 AU) from nearby stars (<25 pc) with masses ranging from a few Jupiter masses to Super Earths (∼2 Earth radii, ∼10 M[subscript ⊕]) as well as circumstellar disks as faint as a few times the zodiacal light in the Solar System.
Published: 2013

29. First results from Herschel-SPIRE performance tests

Author: Mather, John C., Lim, Tanya, Swinyard, Bruce, Aramburu, Asier, Bock, James, Ferlet, Marc, Griffin, Douglas, Griffin, Matthew, Hargrave, Peter C., King, Kenneth, Leeks, Sarah, Naylor, David, Ronayette, Samuel, Sawyer, Eric, Schulz, Bernhard, Sidher, Sunil, Spencer, Locke, Smith, David, Woodcraft, Adam, Mather, John C., Lim, Tanya, Swinyard, Bruce, Aramburu, Asier, Bock, James, Ferlet, Marc, Griffin, Douglas, Griffin, Matthew, Hargrave, Peter C., King, Kenneth, Leeks, Sarah, Naylor, David, Ronayette, Samuel, Sawyer, Eric, Schulz, Bernhard, Sidher, Sunil, Spencer, Locke, Smith, David, and Woodcraft, Adam
Abstract: The Spectral and Photometric Imaging REceiver (SPIRE) is one of the three scientific instruments on the European Space Agency's Herschel mission. At the start of 2004 the Cryogenic Qualification Model (CQM) of SPIRE was tested with the aim of verifying the instrument system design and evaluating key performance parameters. We present a description of the test facility, an overview of the instrument tests carried out on the CQM, and the first results from the analysis of the test data. Instrument optical efficiency and detector noise levels are close to the values expected from unit-level tests, and the SPIRE instrument system works well, with no degradation in performance from stray light, electromagnetic interference or microphonically induced noise. Some anomalies and imperfections in the instrument performance, test set-up, and test procedures have been identified and will be addressed in the next test campaign.
Published: 2004

30. METIS opto-mechanical design and packaging study

Author: Kroes, Gabby, primary, ter Horst, Rik, additional, Kragt, Jan, additional, Roelfsema, Ronald, additional, Navarro, Ramón, additional, Venema, Lars, additional, Lenzen, Rainer, additional, Rohloff, Ralf R., additional, Durand, Gilles, additional, Pantin, Eric, additional, Ronayette, Samuel, additional, Todd, Stephen, additional, Bennett, Richard, additional, Glasse, Alistair, additional, Blommaert, Joris, additional, Brandl, Bernhard, additional, Teuwen, Maurice, additional, Janssen, Huub, additional, and Huisman, Robert, additional
Published: 2010
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31. See-coast: polarimetric and spectral characterization of exoplanets with a small space telescope

Author: Galicher, Raphaël, primary, Baudoz, Pierre, additional, Boccaletti, Anthony, additional, Maire, Anne-Lise, additional, Ronayette, Samuel, additional, and Schneider, Jean, additional
Published: 2010
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32. Manufacturing and verification of ZnS and Ge prisms for the JWST MIRI imager

Author: Rossi, Laurence, primary, Jamoye, Jean-François, additional, Renotte, Etienne, additional, Mazy, Emmanuel, additional, Plesseria, Jean-Yves, additional, Ninane, Nathalie, additional, Wielandts, Marc, additional, Fischer, Sebastian, additional, Straubmeier, Christian, additional, Augueres, Jean-Louis, additional, Dubreuil, Didier, additional, Amiaux, Jérôme, additional, Poupar, Sébastien, additional, and Ronayette, Samuel, additional
Published: 2008
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33. Cryogenic pupil alignment test architecture for the James Webb Space Telescope integrated science instrument module

Author: Bos, Brent J., primary, Kubalak, David A., additional, Antonille, Scott R., additional, Ohl, Raymond G., additional, Hagopian, John G., additional, Davila, Pamela S., additional, Sullivan, Joseph, additional, Sánchez, Michael, additional, Sabatke, Derek, additional, Woodruff, Robert A., additional, te Plate, Maurice, additional, Evans, Clinton, additional, Isbrucker, Victor, additional, Somerstein, Stephen, additional, Wells, Martyn, additional, and Ronayette, Samuel, additional
Published: 2008
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34. First tests of the coronagraphic device of MIRI/JWST

Author: Cavarroc, Céline, primary, Amiaux, Jérôme, additional, Baudoz, Pierre, additional, Boccaletti, Anthony, additional, Bouchet, Patrice, additional, Dubreuil, Didier, additional, Lagage, Pierre-Olivier, additional, Moreau, Vincent, additional, Pantin, Eric J., additional, Reess, Jean-Michel, additional, Ronayette, Samuel, additional, and Wright, Gillian S., additional
Published: 2008
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35. COLIBRI, a wide-field 1.3 m robotic telescope dedicated to the transient sky.

Author: Basa, Stéphane, Lee, William H., Dolon, François, Watson, Alan M., Floriot, Johan, Atteia, Jean-Luc, Butler, Nathaniel R., Dornic, Damien, Lombardo, Simona, Ronayette, Samuel, Ageron, Michel, Agneray, François, Ángeles, Fernando, Bautista, Ludovik, Benamar-Aissa, Hafid, Blanpain, Cyril, Boulade, Olivier, Boy, Jérémie, Buat, Veronique, and Cadena, Edgar
Published: 2022
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36. First results from Herschel-SPIRE performance tests.

Author: Lim, Tanya L., Swinyard, Bruce M., Aramburu, Asier A., Bock, James J., Ferlet, Marc, Griffin, Douglas, Griffin, Matthew J., Hargrave, Peter, King, Kenneth, Leeks, Sarah, Naylor, David A., Ronayette, Samuel D., Sawyer, Eric, Schulz, Bernhard, Sidher, Sunil, Spencer, Locke D., Smith, David, and Woodcraft, Adam L.
Published: 2004
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37. A Fourier transform spectrometer for ground testing of the Herschel/SPIRE instrument.

Author: Spencer, Locke D., Naylor, David A., Swinyard, Bruce M., Aramburu, Asier A., Fulton, Trevor R., Lim, Tanya L., Ronayette, Samuel D., and Schofield, Ian S.
Published: 2004
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38. The science case and data processing strategy for the Thinned Aperture Light Collector (TALC): a project for a 20m far-infrared space telescope

Author: Oschmann, Jacobus M., Clampin, Mark, Fazio, Giovanni G., MacEwen, Howard A., Sauvage, Marc, Chanial, Pierre, Durand, Gilles A., Rodriguez, Louis R., Starck, Jean-Luc, Ronayette, Samuel, Aussel, Hervé, Minier, Vincent, Motte, Frédérique, Pantin, Eric J., Sureau, Florent, and Terrisse, Robin
Published: 2014
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39. TALC: a new deployable concept for a 20m far-infrared space telescope

Author: Oschmann, Jacobus M., Clampin, Mark, Fazio, Giovanni G., MacEwen, Howard A., Durand, Gilles, Sauvage, Marc, Bonnet, Aymeric, Rodriguez, Louis, Ronayette, Samuel, Chanial, Pierre, Scola, Loris, Révéret, Vincent, Aussel, Hervé, Carty, Michael, Durand, Matthis, Durand, Lancelot, Tremblin, Pascal, Pantin, Eric, Berthe, Michel, Martignac, Jérôme, Motte, Frédérique, Talvard, Michel, Minier, Vincent, and Bultel, Pascal
Published: 2014
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40. Antarctic observations at long wavelengths with the IRAIT-ITM Telescope at Dome C

Author: Stepp, Larry M., Gilmozzi, Roberto, Hall, Helen J., Durand, Gilles A., Tremblin, Pascal, Minier, Vincent, Reinert, Yann, Leroy dos Santos, Christophe, Rodriguez, Louis, Joffrin, Xavier, Busso, Maurizio, Tosti, Gino, Nucciarelli, Giuliano, Dolci, Mauro, Straniero, Oscar, Valentini, Angelo, Abia, Carlos, Christille, Jean Marc, Doumayrou, Eric, Lortholary, Michel, Charron, Patrice, Lotrus, Paul, Walter, Christian, Ronayette, Samuel, Challita, Zalpha, Fromont, Laurent, Condamin, Mathieu, Kwon, Min Kyong, and Tavagnacco, Daniele
Published: 2014
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41. The DESI Experiment Part I: Science,Targeting, and Survey Design

Author: Desi, Collaboration, Aghamousa, Amir, Aguilar, Jessica, Ahlen, Steve, Alam, Shadab, Allen, Lori E., Allende Prieto, Carlos, Annis, James, Bailey, Stephen, Balland, Christophe, Ballester, Otger, Baltay, Charles, Beaufore, Lucas, Bebek, Chris, Beers, Timothy C., Bell, Eric F., Bernal, José Luis, Besuner, Robert, Beutler, Florian, Blake, Chris, Bleuler, Hannes, Blomqvist, Michael, Blum, Robert, Bolton, Adam S., Briceno, Cesar, Brooks, David, Brownstein, Joel R., Buckley-Geer, Elizabeth, Burden, Angela, Burtin, Etienne, Busca, Nicolas G., Cahn, Robert N., Cai, Yan-Chuan, Cardiel-Sas, Laia, Carlberg, Raymond G., Carton, Pierre-Henri, Casas, Ricard, Castander, Francisco J., Cervantes-Cota, Jorge L., Claybaugh, Todd M., Close, Madeline, Coker, Carl T., Cole, Shaun, Comparat, Johan, Cooper, Andrew P., Cousinou, M. -C, Crocce, Martin, Cuby, Jean-Gabriel, Cunningham, Daniel P., Davis, Tamara M., Dawson, Kyle S., La Macorra, Axel, Vicente, Juan, Delubac, Timothée, Derwent, Mark, Dey, Arjun, Dhungana, Govinda, Ding, Zhejie, Doel, Peter, Duan, Yutong T., Ealet, Anne, Edelstein, Jerry, Eftekharzadeh, Sarah, Eisenstein, Daniel J., Elliott, Ann, Escoffier, Stéphanie, Evatt, Matthew, Fagrelius, Parker, Fan, Xiaohui, Fanning, Kevin, Farahi, Arya, Farihi, Jay, Favole, Ginevra, Feng, Yu, Fernandez, Enrique, Findlay, Joseph R., Finkbeiner, Douglas P., Fitzpatrick, Michael J., Flaugher, Brenna, Flender, Samuel, Font-Ribera, Andreu, Forero-Romero, Jaime E., Fosalba, Pablo, Frenk, Carlos S., Fumagalli, Michele, Gaensicke, Boris T., Gallo, Giuseppe, Garcia-Bellido, Juan, Gaztanaga, Enrique, Pietro Gentile Fusillo, Nicola, Gerard, Terry, Gershkovich, Irena, Giannantonio, Tommaso, Gillet, Denis, Gonzalez-De-Rivera, Guillermo, Gonzalez-Perez, Violeta, Gott, Shelby, Graur, Or, Gutierrez, Gaston, Guy, Julien, Habib, Salman, Heetderks, Henry, Heetderks, Ian, Heitmann, Katrin, Hellwing, Wojciech A., Herrera, David A., Ho, Shirley, Holland, Stephen, Honscheid, Klaus, Huff, Eric, Hutchinson, Timothy A., Huterer, Dragan, Hwang, Ho Seong, Illa Laguna, Joseph Maria, Ishikawa, Yuzo, Jacobs, Dianna, Jeffrey, Niall, Jelinsky, Patrick, Jennings, Elise, Jiang, Linhua, Jimenez, Jorge, Johnson, Jennifer, Joyce, Richard, Jullo, Eric, Juneau, Stéphanie, Kama, Sami, Karcher, Armin, Karkar, Sonia, Kehoe, Robert, Kennamer, Noble, Kent, Stephen, Kilbinger, Martin, Kim, Alex G., Kirkby, David, Kisner, Theodore, Kitanidis, Ellie, Kneib, Jean-Paul, Koposov, Sergey, Kovacs, Eve, Koyama, Kazuya, Kremin, Anthony, Kron, Richard, Kronig, Luzius, Kueter-Young, Andrea, Lacey, Cedric G., Lafever, Robin, Lahav, Ofer, Lambert, Andrew, Lampton, Michael, Landriau, Martin, Lang, Dustin, Lauer, Tod R., Le Goff, Jean-Marc, Le Guillou, Laurent, Le Suu, Auguste, Lee, Jae Hyeon, Lee, Su-Jeong, Leitner, Daniela, Lesser, Michael, Levi, Michael E., L Huillier, Benjamin, Li, Baojiu, Liang, Ming, Lin, Huan, Linder, Eric, Loebman, Sarah R., Lukić, Zarija, Ma, Jun, Maccrann, Niall, Magneville, Christophe, Makarem, Laleh, Manera, Marc, Manser, Christopher J., Marshall, Robert, Martini, Paul, Massey, Richard, Matheson, Thomas, Mccauley, Jeremy, Mcdonald, Patrick, Mcgreer, Ian D., Meisner, Aaron, Metcalfe, Nigel, Miller, Timothy N., Miquel, Ramon, Moustakas, John, Myers, Adam, Naik, Milind, Newman, Jeffrey A., Nichol, Robert C., Nicola, Andrina, Nicolati Da Costa, Luiz, Nie, Jundan, Niz, Gustavo, Norberg, Peder, Nord, Brian, Norman, Dara, Nugent, Peter, O Brien, Thomas, Oh, Minji, Olsen, Knut A. G., Padilla, Cristobal, Padmanabhan, Hamsa, Padmanabhan, Nikhil, Palanque-Delabrouille, Nathalie, Palmese, Antonella, Pappalardo, Daniel, Pâris, Isabelle, Park, Changbom, Patej, Anna, Peacock, John A., Peiris, Hiranya V., Peng, Xiyan, Percival, Will J., Perruchot, Sandrine, Pieri, Matthew M., Pogge, Richard, Pollack, Jennifer E., Poppett, Claire, Prada, Francisco, Prakash, Abhishek, Probst, Ronald G., Rabinowitz, David, Raichoor, Anand, Ree, Chang Hee, Refregier, Alexandre, Regal, Xavier, Reid, Beth, Reil, Kevin, Rezaie, Mehdi, Rockosi, Constance M., Roe, Natalie, Ronayette, Samuel, Roodman, Aaron, Ross, Ashley J., Ross, Nicholas P., Rossi, Graziano, Rozo, Eduardo, Ruhlmann-Kleider, Vanina, Rykoff, Eli S., Sabiu, Cristiano, Samushia, Lado, Sanchez, Eusebio, Sanchez, Javier, Schlegel, David J., Schneider, Michael, Schubnell, Michael, Secroun, Aurélia, Seljak, Uros, Seo, Hee-Jong, Serrano, Santiago, Shafieloo, Arman, Shan, Huanyuan, Sharples, Ray, Sholl, Michael J., Shourt, William V., Silber, Joseph H., Silva, David R., Sirk, Martin M., Slosar, Anze, Smith, Alex, Smoot, George F., Som, Debopam, Song, Yong-Seon, Sprayberry, David, Staten, Ryan, Stefanik, Andy, Tarle, Gregory, Sien Tie, Suk, Tinker, Jeremy L., Tojeiro, Rita, Valdes, Francisco, Valenzuela, Octavio, Valluri, Monica, Vargas-Magana, Mariana, Verde, Licia, Walker, Alistair R., Wang, Jiali, Wang, Yuting, Weaver, Benjamin A., Weaverdyck, Curtis, Wechsler, Risa H., Weinberg, David H., White, Martin, Yang, Qian, Yeche, Christophe, Zhang, Tianmeng, Zhao, Gong-Bo, Zheng, Yi, Zhou, Xu, Zhou, Zhimin, Zhu, Yaling, Zou, Hu, and Ying Zu
Subjects: Cosmology and Nongalactic Astrophysics (astro-ph.CO), astro-ph.CO, FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics, Instrumentation and Methods for Astrophysics (astro-ph.IM), Astrophysics::Galaxy Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics, astro-ph.IM
Abstract: DESI (Dark Energy Spectroscopic Instrument) is a Stage IV ground-based dark energy experiment that will study baryon acoustic oscillations (BAO) and the growth of structure through redshift-space distortions with a wide-area galaxy and quasar redshift survey. To trace the underlying dark matter distribution, spectroscopic targets will be selected in four classes from imaging data. We will measure luminous red galaxies up to $z=1.0$. To probe the Universe out to even higher redshift, DESI will target bright [O II] emission line galaxies up to $z=1.7$. Quasars will be targeted both as direct tracers of the underlying dark matter distribution and, at higher redshifts ($ 2.1 < z < 3.5$), for the Ly-$��$ forest absorption features in their spectra, which will be used to trace the distribution of neutral hydrogen. When moonlight prevents efficient observations of the faint targets of the baseline survey, DESI will conduct a magnitude-limited Bright Galaxy Survey comprising approximately 10 million galaxies with a median $z\approx 0.2$. In total, more than 30 million galaxy and quasar redshifts will be obtained to measure the BAO feature and determine the matter power spectrum, including redshift space distortions.

42. The DESI Experiment Part II: Instrument Design

Author: Desi, Collaboration, Aghamousa, Amir, Aguilar, Jessica, Ahlen, Steve, Alam, Shadab, Allen, Lori E., Allende Prieto, Carlos, Annis, James, Bailey, Stephen, Balland, Christophe, Ballester, Otger, Baltay, Charles, Beaufore, Lucas, Bebek, Chris, Beers, Timothy C., Bell, Eric F., Bernal, José Luis, Besuner, Robert, Beutler, Florian, Blake, Chris, Bleuler, Hannes, Blomqvist, Michael, Blum, Robert, Bolton, Adam S., Briceno, Cesar, Brooks, David, Brownstein, Joel R., Buckley-Geer, Elizabeth, Burden, Angela, Burtin, Etienne, Busca, Nicolas G., Cahn, Robert N., Cai, Yan-Chuan, Cardiel-Sas, Laia, Carlberg, Raymond G., Carton, Pierre-Henri, Casas, Ricard, Castander, Francisco J., Cervantes-Cota, Jorge L., Claybaugh, Todd M., Close, Madeline, Coker, Carl T., Cole, Shaun, Comparat, Johan, Cooper, Andrew P., Cousinou, M. -C, Crocce, Martin, Cuby, Jean-Gabriel, Cunningham, Daniel P., Davis, Tamara M., Dawson, Kyle S., La Macorra, Axel, Vicente, Juan, Delubac, Timothée, Derwent, Mark, Dey, Arjun, Dhungana, Govinda, Ding, Zhejie, Doel, Peter, Duan, Yutong T., Ealet, Anne, Edelstein, Jerry, Eftekharzadeh, Sarah, Eisenstein, Daniel J., Elliott, Ann, Escoffier, Stéphanie, Evatt, Matthew, Fagrelius, Parker, Fan, Xiaohui, Fanning, Kevin, Farahi, Arya, Farihi, Jay, Favole, Ginevra, Feng, Yu, Fernandez, Enrique, Findlay, Joseph R., Finkbeiner, Douglas P., Fitzpatrick, Michael J., Flaugher, Brenna, Flender, Samuel, Font-Ribera, Andreu, Forero-Romero, Jaime E., Fosalba, Pablo, Frenk, Carlos S., Fumagalli, Michele, Gaensicke, Boris T., Gallo, Giuseppe, Garcia-Bellido, Juan, Gaztanaga, Enrique, Pietro Gentile Fusillo, Nicola, Gerard, Terry, Gershkovich, Irena, Giannantonio, Tommaso, Gillet, Denis, Gonzalez-De-Rivera, Guillermo, Gonzalez-Perez, Violeta, Gott, Shelby, Graur, Or, Gutierrez, Gaston, Guy, Julien, Habib, Salman, Heetderks, Henry, Heetderks, Ian, Heitmann, Katrin, Hellwing, Wojciech A., Herrera, David A., Ho, Shirley, Holland, Stephen, Honscheid, Klaus, Huff, Eric, Hutchinson, Timothy A., Huterer, Dragan, Hwang, Ho Seong, Illa Laguna, Joseph Maria, Ishikawa, Yuzo, Jacobs, Dianna, Jeffrey, Niall, Jelinsky, Patrick, Jennings, Elise, Jiang, Linhua, Jimenez, Jorge, Johnson, Jennifer, Joyce, Richard, Jullo, Eric, Juneau, Stéphanie, Kama, Sami, Karcher, Armin, Karkar, Sonia, Kehoe, Robert, Kennamer, Noble, Kent, Stephen, Kilbinger, Martin, Kim, Alex G., Kirkby, David, Kisner, Theodore, Kitanidis, Ellie, Kneib, Jean-Paul, Koposov, Sergey, Kovacs, Eve, Koyama, Kazuya, Kremin, Anthony, Kron, Richard, Kronig, Luzius, Kueter-Young, Andrea, Lacey, Cedric G., Lafever, Robin, Lahav, Ofer, Lambert, Andrew, Lampton, Michael, Landriau, Martin, Lang, Dustin, Lauer, Tod R., Le Goff, Jean-Marc, Le Guillou, Laurent, Le Suu, Auguste, Lee, Jae Hyeon, Lee, Su-Jeong, Leitner, Daniela, Lesser, Michael, Levi, Michael E., L Huillier, Benjamin, Li, Baojiu, Liang, Ming, Lin, Huan, Linder, Eric, Loebman, Sarah R., Lukić, Zarija, Ma, Jun, Maccrann, Niall, Magneville, Christophe, Makarem, Laleh, Manera, Marc, Manser, Christopher J., Marshall, Robert, Martini, Paul, Massey, Richard, Matheson, Thomas, Mccauley, Jeremy, Mcdonald, Patrick, Mcgreer, Ian D., Meisner, Aaron, Metcalfe, Nigel, Miller, Timothy N., Miquel, Ramon, Moustakas, John, Myers, Adam, Naik, Milind, Newman, Jeffrey A., Nichol, Robert C., Nicola, Andrina, Nicolati Da Costa, Luiz, Nie, Jundan, Niz, Gustavo, Peder Norberg, Nord, Brian, Norman, Dara, Nugent, Peter, O Brien, Thomas, Oh, Minji, Olsen, Knut A. G., Padilla, Cristobal, Padmanabhan, Hamsa, Padmanabhan, Nikhil, Palanque-Delabrouille, Nathalie, Palmese, Antonella, Pappalardo, Daniel, Pâris, Isabelle, Park, Changbom, Patej, Anna, Peacock, John A., Peiris, Hiranya V., Peng, Xiyan, Percival, Will J., Perruchot, Sandrine, Pieri, Matthew M., Pogge, Richard, Pollack, Jennifer E., Poppett, Claire, Prada, Francisco, Prakash, Abhishek, Probst, Ronald G., Rabinowitz, David, Raichoor, Anand, Ree, Chang Hee, Refregier, Alexandre, Regal, Xavier, Reid, Beth, Reil, Kevin, Rezaie, Mehdi, Rockosi, Constance M., Roe, Natalie, Ronayette, Samuel, Roodman, Aaron, Ross, Ashley J., Ross, Nicholas P., Rossi, Graziano, Rozo, Eduardo, Ruhlmann-Kleider, Vanina, Rykoff, Eli S., Sabiu, Cristiano, Samushia, Lado, Sanchez, Eusebio, Sanchez, Javier, Schlegel, David J., Schneider, Michael, Schubnell, Michael, Secroun, Aurélia, Seljak, Uros, Seo, Hee-Jong, Serrano, Santiago, Shafieloo, Arman, Shan, Huanyuan, Sharples, Ray, Sholl, Michael J., Shourt, William V., Silber, Joseph H., Silva, David R., Sirk, Martin M., Slosar, Anze, Smith, Alex, Smoot, George F., Som, Debopam, Song, Yong-Seon, Sprayberry, David, Staten, Ryan, Stefanik, Andy, Tarle, Gregory, Sien Tie, Suk, Tinker, Jeremy L., Tojeiro, Rita, Valdes, Francisco, Valenzuela, Octavio, Valluri, Monica, Vargas-Magana, Mariana, Verde, Licia, Walker, Alistair R., Wang, Jiali, Wang, Yuting, Weaver, Benjamin A., Weaverdyck, Curtis, Wechsler, Risa H., Weinberg, David H., White, Martin, Yang, Qian, Yeche, Christophe, Zhang, Tianmeng, Zhao, Gong-Bo, Zheng, Yi, Zhou, Xu, Zhou, Zhimin, Zhu, Yaling, Zou, Hu, Zu, Ying, Korea Astronomy and Space Science Institute (KASI), University of California [Berkeley] (UC Berkeley), University of California (UC), Boston University [Boston] (BU), Carnegie Mellon University [Pittsburgh] (CMU), University of Edinburgh, National Optical Astronomy Observatory (NOAO), Instituto de Astrofisica de Canarias (IAC), Fermi National Accelerator Laboratory (Fermilab), Lawrence Berkeley National Laboratory [Berkeley] (LBNL), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Institut de Física d’Altes Energies [Barcelone] (IFAE), Universitat Autònoma de Barcelona (UAB), Yale University [New Haven], Ohio State University [Columbus] (OSU), The University of Notre Dame [Sydney], Department of Astronomy, University of Michigan, University of Michigan [Ann Arbor], University of Michigan System-University of Michigan System, Institut de Ciencies del Cosmos (ICCUB), Universitat de Barcelona (UB), Space Sciences Laboratory [Berkeley] (SSL), University of California (UC)-University of California (UC), University of Portsmouth, Centre for Astrophysics & Supercomputing, Swinburne University of Technology (Hawthorn campus), Ecole Polytechnique Fédérale de Lausanne (EPFL), Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), The University of Utah, Cerro Tololo Inter-American Observatory, University College of London [London] (UCL), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, APC - Cosmologie, AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Institute for Astronomy [Edinburgh] (IfA), Department of Astronomy & Astrophysics [University of Toronto], University of Toronto, Institut de Ciencies de l'Espai [Barcelona] (ICE-CSIC), Consejo Superior de Investigaciones Científicas [Madrid] (CSIC), Carreterra Mexico-Toluca, Department of Physics [Durham University], Durham University, Department of Astronomy, The Ohio State University, Institute for Computational Cosmology (ICC), Instituto de Fisica Teorica C-XVI (IFT-UAM/CSIC), Universidad Autónoma de Madrid (UAM), Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Universidad Nacional Autónoma de México = National Autonomous University of Mexico (UNAM), Department of Applied Physics, Departamento de Fisica Aplicada [Granada], Universidad de Granada = University of Granada (UGR)-Universidad de Granada = University of Granada (UGR), University of Wyoming (UW), Harvard-Smithsonian Center for Astrophysics (CfA), Harvard University-Smithsonian Institution, Arizona State University [Tempe] (ASU), Department of Physics, University of California, University of California [Los Angeles] (UCLA), Institute for Astronomy [Honolulu], University of Hawai‘i [Mānoa] (UHM), Department of Physics [Durham], University of New Hampshire (UNH), Departamento de Fisica Teorica, Korea Institute for Advanced Study (KIAS), Centre d'Immunologie et des Maladies Infectieuses (CIMI), Institut National de la Santé et de la Recherche Médicale (INSERM)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Department of Physics and Astronomy [Irvine], University of California [Irvine] (UC Irvine), Institute of Astronomy [Cambridge], University of Cambridge [UK] (CAM), Institute of Cosmology & Gravitation, Dennis Sciama Building, University of Portsmouth, Observatoire de Haute-Provence (OHP), Institut Pythéas (OSU PYTHEAS), Institut de Recherche pour le Développement (IRD)-Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Institut de Recherche pour le Développement (IRD)-Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE), Center for Cosmology & AstroParticle Physics, Department of Physics and Astronomy [Pittsburgh], University of Pittsburgh (PITT), Pennsylvania Commonwealth System of Higher Education (PCSHE)-Pennsylvania Commonwealth System of Higher Education (PCSHE), Institute for Astronomy [Zürich], Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology [Zürich] (ETH Zürich), School of Physics and Astronomy [Nottingham], University of Nottingham, UK (UON), School of Physics, University of Waterloo [Waterloo], Department of Astronomy and Space Science [Sejong University], Sejong University, Brookhaven National Laboratory [Upton, NY] (BNL), UT-Battelle, LLC-Stony Brook University [SUNY] (SBU), State University of New York (SUNY)-State University of New York (SUNY)-U.S. Department of Energy [Washington] (DOE), Department of Physics [Ann Arbor], University of St Andrews [Scotland], University of Science and Technology of China [Hefei] (USTC), Department of Computer Science and Engineering [Minneapolis], University of Minnesota [Twin Cities] (UMN), University of Minnesota System-University of Minnesota System, Karlsruhe Institute of Technology (KIT), Key Laboratory for Liquid-Solid Structural Evolution and Processing of Materials, Shandong University, National University of Defense Technology [China], Avidea Technologies, Inc, DESI Collaboration, Okayama University, University of California [Berkeley], University of California, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), University of California-University of California, Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Universidad Autonoma de Madrid (UAM), Universidad Nacional Autónoma de México (UNAM), Universidad de Granada (UGR)-Universidad de Granada (UGR), Harvard University [Cambridge]-Smithsonian Institution, Centre d'Immunologie et de Maladies Infectieuses (CIMI), University of California [Irvine] (UCI), U.S. Department of Energy [Washington] (DOE)-UT-Battelle, LLC-Stony Brook University [SUNY] (SBU), State University of New York (SUNY)-State University of New York (SUNY), and Escoffier, Stephanie
Subjects: [SDU.ASTR.IM] Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], Cosmology and Nongalactic Astrophysics (astro-ph.CO), astro-ph.CO, Astrophysics::Instrumentation and Methods for Astrophysics, FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics, Instrumentation and Methods for Astrophysics (astro-ph.IM), astro-ph.IM, Astrophysics - Cosmology and Nongalactic Astrophysics, [SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]
Abstract: DESI (Dark Energy Spectropic Instrument) is a Stage IV ground-based dark energy experiment that will study baryon acoustic oscillations and the growth of structure through redshift-space distortions with a wide-area galaxy and quasar redshift survey. The DESI instrument is a robotically-actuated, fiber-fed spectrograph capable of taking up to 5,000 simultaneous spectra over a wavelength range from 360 nm to 980 nm. The fibers feed ten three-arm spectrographs with resolution $R= \lambda/\Delta\lambda$ between 2000 and 5500, depending on wavelength. The DESI instrument will be used to conduct a five-year survey designed to cover 14,000 deg$^2$. This powerful instrument will be installed at prime focus on the 4-m Mayall telescope in Kitt Peak, Arizona, along with a new optical corrector, which will provide a three-degree diameter field of view. The DESI collaboration will also deliver a spectroscopic pipeline and data management system to reduce and archive all data for eventual public use.

43. The mid-infrared instrument for the James Webb Space Telescope: performance and operation of the Low-Resolution Spectrometer

Author: MacEwen, Howard A., Fazio, Giovanni G., Lystrup, Makenzie, Batalha, Natalie, Siegler, Nicholas, Tong, Edward C., Kendrew, Sarah, Scheithauer, Silvia, Bouchet, Patrice, Amiaux, Jerome, Azzollini, Ruymán, Bouwman, Jeroen, Chen, Christine, Dubreuil, Didier, Fischer, Sebastian, Fox, Ori D., Glasse, Alistair, Gordon, Karl, Greene, Tom, Hines, Dean C., Lagage, Pierre-Olivier, Lahuis, Fred, Ronayette, Samuel, Wright, David, and Wright, Gillian S.
Published: 2016
Full Text: View/download PDF

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43 results on '"Ronayette, Samuel"'

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