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22 results on '"Moseley, S. Harvey"'

1. 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
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2. The Origins Survey Spectrometer (OSS): a far-IR discovery machine for the Origins Space Telescope

Author

Bradford, Charles M., primary, Cameron, Bruce, primary, Moore, Bradley D., primary, Armus, Lee, primary, Pope, Alexandra, primary, Amatucci, Edward, primary, Bradley, Damon, primary, Corsetti, James, primary, Leisawitz, David, primary, Moseley, S. Harvey, primary, Staguhn, Johannes, primary, Tuttle, James, primary, Brown, Ari, primary, Pontoppidan, Klaus, primary, and Meixner, Margaret, primary

Published
2018
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4. The Primordial Inflation Polarization Explorer (PIPER)

Author

Lazear, Justin, additional, Ade, Peter A. R., additional, Benford, Dominic, additional, Bennett, Charles L., additional, Chuss, David T., additional, Dotson, Jessie L., additional, Eimer, Joseph R., additional, Fixsen, Dale J., additional, Halpern, Mark, additional, Hilton, Gene, additional, Hinderks, James, additional, Hinshaw, Gary F., additional, Irwin, Kent, additional, Jhabvala, Christine, additional, Johnson, Bradley, additional, Kogut, Alan, additional, Lowe, Luke, additional, McMahon, Jeff J., additional, Miller, Timothy M., additional, Mirel, Paul, additional, Moseley, S. Harvey, additional, Rodriguez, Samelys, additional, Sharp, Elmer, additional, Staguhn, Johannes G., additional, Switzer, Eric R., additional, Tucker, Carole E., additional, Weston, Amy, additional, and Wollack, Edward J., additional

Published
2014
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5. The Primordial Inflation Polarization Explorer (PIPER)

Author

Kogut, Alan, primary, Ade, Peter A. R., additional, Benford, Dominic, additional, Bennett, Charles L., additional, Chuss, David T., additional, Dotson, Jessie L., additional, Eimer, Joseph R., additional, Fixsen, Dale J., additional, Halpern, Mark, additional, Hilton, Gene, additional, Hinderks, James, additional, Hinshaw, Gary F., additional, Irwin, Kent, additional, Jhabvala, Christine, additional, Johnson, Brad, additional, Lazear, Justin, additional, Lowe, Luke, additional, Miller, Timothy, additional, Mirel, Paul, additional, Moseley, S. Harvey, additional, Rodriguez, Samelys, additional, Sharp, Elmer, additional, Staguhn, Johannes G., additional, Tucker, Carole E., additional, Weston, Amy, additional, and Wollack, Edward J., additional

Published
2012
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6. The Primordial Inflation Explorer (PIXIE)

Author

Kogut, Alan, primary, Chuss, David T., additional, Dotson, Jessie, additional, Fixsen, Dale J., additional, Halpern, Mark, additional, Hinshaw, Gary F., additional, Meyer, Stephan, additional, Moseley, S. Harvey, additional, Seiffert, Michael D., additional, Spergel, David N., additional, and Wollack, Edward J., additional

Published
2011
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7. The Primordial Inflation Polarization Explorer (PIPER)

Author

Chuss, David T., primary, Ade, Peter A. R., additional, Benford, Dominic J., additional, Bennett, Charles L., additional, Dotson, Jessie L., additional, Eimer, Joseph R., additional, Fixsen, Dale J., additional, Halpern, Mark, additional, Hilton, Gene, additional, Hinderks, James, additional, Hinshaw, Gary, additional, Irwin, Kent, additional, Jackson, Michael L., additional, Jah, Muzariatu A., additional, Jethava, Nikhil, additional, Jhabvala, Christine, additional, Kogut, Alan J., additional, Lowe, Luke, additional, McCullagh, Nuala, additional, Miller, Timothy, additional, Mirel, Paul, additional, Moseley, S. Harvey, additional, Rodriguez, Samelys, additional, Rostem, Karwan, additional, Sharp, Elmer, additional, Staguhn, Johannes G., additional, Tucker, Carole E., additional, Voellmer, George M., additional, Wollack, Edward J., additional, and Zeng, Lingzhen, additional

Published
2010
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9. 5,120 superconducting bolometers for the PIPER balloon-borne CMB polarization experiment

Author

Benford, Dominic J., primary, Chuss, David T., additional, Hilton, Gene C., additional, Irwin, Kent D., additional, Jethava, Nikhil S., additional, Jhabvala, Christine A., additional, Kogut, Alan J., additional, Miller, Timothy M., additional, Mirel, Paul, additional, Moseley, S. Harvey, additional, Rostem, Karwan, additional, Sharp, Elmer H., additional, Staguhn, Johannes G., additional, Stiehl, Gregory M., additional, Voellmer, George M., additional, and Wollack, Edward J., additional

Published
2010
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11. HAWCPol: a first-generation far-infrared polarimeter for SOFIA

Author

Dowell, C. Darren, primary, Cook, Brant T., additional, Harper, D. Al, additional, Lin, Lung-Sheng, additional, Looney, Leslie W., additional, Novak, Giles, additional, Stephens, Ian, additional, Berthoud, Marc, additional, Chuss, David T., additional, Crutcher, Richard M., additional, Dotson, Jessie L., additional, Hildebrand, Roger H., additional, Houde, Martin, additional, Jones, Terry J., additional, Krejny, Megan, additional, Lazarian, Alexandre, additional, Moseley, S. Harvey, additional, Tassis, Kostas, additional, Vaillancourt, John E., additional, and Werner, Michael W., additional

Published
2010
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12. The Primordial Inflation Explorer (PIXIE) Mission

Author

Kogut, Alan J., primary, Chuss, David T., additional, Dotson, Jessie L., additional, Fixsen, Dale J., additional, Halpern, Mark, additional, Hinshaw, Gary F., additional, Meyer, Stephan M., additional, Moseley, S. Harvey, additional, Seiffert, Michael D., additional, Spergel, David N., additional, and Wollack, Edward J., additional

Published
2010
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14. Instrument performance of GISMO, a 2 millimeter TES bolometer camera used at the IRAM 30 m Telescope

Author

Staguhn, Johannes G., primary, Benford, Dominic J., additional, Allen, Christine A., additional, Maher, Stephen F., additional, Sharp, Elmer H., additional, Ames, Troy J., additional, Arendt, Richard G., additional, Chuss, David T., additional, Dwek, Eli, additional, Fixsen, Dale J., additional, Miller, Tim M., additional, Moseley, S. Harvey, additional, Navarro, Santiago, additional, Sievers, Albrecht, additional, and Wollack, Edward J., additional

Published
2008
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18. Far infrared through millimeter backshort-under-grid arrays

Author

Allen, Christine A., primary, Abrahams, John, additional, Benford, Dominic J., additional, Chervenak, James A., additional, Chuss, David T., additional, Staguhn, Johannes G., additional, Miller, Timothy M., additional, Moseley, S. Harvey, additional, and Wollack, Edward J., additional

Published
2006
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19. First astronomical images with a multiplexed superconducting bolometer array

Author

Benford, Dominic J., primary, Staguhn, Johannes G., additional, Ames, Troy J., additional, Allen, Christine A., additional, Chervenak, James A., additional, Kennedy, Catherine R., additional, Lefranc, Sebastien, additional, Maher, Stephen F., additional, Moseley, S. Harvey, additional, Pajot, François, additional, Rioux, Cyrille, additional, Shafer, Richard A., additional, and Voellmer, George M., additional

Published
2006
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21. The primordial inflation polarization explorer (PIPER): current status and performance of the first flight

Author

Pawlyk, Samuel, Ade, Peter A. R., Benford, Dominic, Bennett, Charles L., Chuss, David T., Datta, Rahul, Dotson, Jessie L., Eimer, Joseph R., Fixsen, Dale J., Gandilo, Natalie N., Essinger-Hileman, Thomas M., Halpern, Mark, Hilton, Gene, Hinshaw, Gary F., Irwin, Kent, Jhabvala, Christine, Kimball, Mark, Kogut, Alan, Lowe, Luke, McMahon, Jeff J., Miller, Timothy M., Mirel, Paul, Moseley, S. Harvey, Rodriguez, Samelys, Sharp III, Elmer, Shirron, Peter, Staguhn, Johannes G., Sullivan, Dan F., Switzer, Eric R., Taraschi, Peter, Tucker, Carole E., Walts, Alexander, Wollack, Edward J., Pawlyk, Samuel, Ade, Peter A. R., Benford, Dominic, Bennett, Charles L., Chuss, David T., Datta, Rahul, Dotson, Jessie L., Eimer, Joseph R., Fixsen, Dale J., Gandilo, Natalie N., Essinger-Hileman, Thomas M., Halpern, Mark, Hilton, Gene, Hinshaw, Gary F., Irwin, Kent, Jhabvala, Christine, Kimball, Mark, Kogut, Alan, Lowe, Luke, McMahon, Jeff J., Miller, Timothy M., Mirel, Paul, Moseley, S. Harvey, Rodriguez, Samelys, Sharp III, Elmer, Shirron, Peter, Staguhn, Johannes G., Sullivan, Dan F., Switzer, Eric R., Taraschi, Peter, Tucker, Carole E., Walts, Alexander, and Wollack, Edward J.

Abstract

The Primordial Inflation Polarization ExploreR (PIPER) is a balloon-borne instrument optimized to measure the polarization of the CMB at large angular scales. It will map 85% of the sky over a series of conventional balloon flights from the Northern and Southern hemispheres, measuring the B-mode polarization power spectrum over a range of multipoles from 2-300 covering both the reionization bump and the recombination peak, with sensitivity to measure the tensor-to-scalar ratio down to r = 0.007. PIPER will observe in four frequency bands centered at 200, 270, 350, and 600 GHz to characterize dust foregrounds. The instrument has background-limited sensitivity provided by fully cryogenic (1.7 K) optics focusing the sky signal onto kilo-pixel arrays of time-domain multiplexed Transition-Edge Sensor (TES) bolometers held at 100 mK. Polarization sensitivity and systematic control are provided by front-end Variable-delay Polarization Modulators (VPMs). PIPER had its engineering ight in October 2017 from Fort Sumner, New Mexico. This papers outlines the major components in the PIPER system discussing the conceptual design as well as specific choices made for PIPER. We also report on the results of the engineering flight, looking at the functionality of the payload systems, particularly VPM, as well as pointing out areas of improvement....

22. The Primordial Inflation Polarization Explorer (PIPER)

Author

Holland, Wayne S., Zmuidzinas, Jonas, Chuss, David T., Ade, Peter A. R., Benford, Dominic J., Bennett, Charles L., Dotson, Jessie L., Eimer, Joseph R., Fixsen, Dale J., Halpern, Mark, Hilton, Gene, Hinderks, James, Hinshaw, Gary, Irwin, Kent, Jackson, Michael L., Jah, Muzariatu A., Jethava, Nikhil, Jhabvala, Christine, Kogut, Alan J., Lowe, Luke, McCullagh, Nuala, Miller, Timothy, Mirel, Paul, Moseley, S. Harvey, Rodriguez, Samelys, Rostem, Karwan, Sharp, Elmer, Staguhn, Johannes G., Tucker, Carole Elizabeth, Voellmer, George M., Wollack, Edward J., Zeng, Lingzhen, Holland, Wayne S., Zmuidzinas, Jonas, Chuss, David T., Ade, Peter A. R., Benford, Dominic J., Bennett, Charles L., Dotson, Jessie L., Eimer, Joseph R., Fixsen, Dale J., Halpern, Mark, Hilton, Gene, Hinderks, James, Hinshaw, Gary, Irwin, Kent, Jackson, Michael L., Jah, Muzariatu A., Jethava, Nikhil, Jhabvala, Christine, Kogut, Alan J., Lowe, Luke, McCullagh, Nuala, Miller, Timothy, Mirel, Paul, Moseley, S. Harvey, Rodriguez, Samelys, Rostem, Karwan, Sharp, Elmer, Staguhn, Johannes G., Tucker, Carole Elizabeth, Voellmer, George M., Wollack, Edward J., and Zeng, Lingzhen

Abstract

The Primordial Inflation Polarization Explorer (PIPER) is a balloon-borne instrument designed to search for the faint signature of inflation in the polarized component of the cosmic microwave background (CMB). Each flight will be configured for a single frequency, but in order to aid in the removal of the polarized foreground signal due to Galactic dust, the filters will be changed between flights. In this way, the CMB polarization at a total of four different frequencies (200, 270, 350, and 600 GHz) will be measured on large angular scales. PIPER consists of a pair of cryogenic telescopes, one for measuring each of Stokes Q and U in the instrument frame. Each telescope receives both linear orthogonal polarizations in two 32 × 40 element planar arrays that utilize Transition-Edge Sensors (TES). The first element in each telescope is a variable-delay polarization modulator (VPM) that fully modulates the linear Stokes parameter to which the telescope is sensitive. There are several advantages to this architecture. First, by modulating at the front of the optics, instrumental polarization is unmodulated and is therefore cleanly separated from source polarization. Second, by implementing this system with the appropriate symmetry, systematic effects can be further mitigated. In the PIPER design, many of the systematics are manifest in the unmeasured linear Stokes parameter for each telescope and thus can be separated from the desired signal. Finally, the modulation cycle never mixes the Q and U linear Stokes parameters, and thus residuals in the modulation do not twist the observed polarization vector. This is advantageous because measuring the angle of linear polarization is critical for separating the inflationary signal from other polarized components.

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