Search Results - "SHARP, Elmer H"

Progress Toward Transition Edge Sensor Arrays With On-Chip Thermal Stabilization by Borrelli, Rachel B., Chervenak, James A., Sharp, Elmer H., Wassell, Edward J., Wollack, Edward J.

“…Electrothermal feedback in a transition edge sensor (TES) suppresses thermal fluctuations in the TES and well-thermally coupled regions in proximity. We have…”
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STAR AND DUST FORMATION ACTIVITIES IN AzTEC-3, A STARBURST GALAXY AT z = 5.3 by DWEK, Eli, STAGUHN, Johannes G, MOSELEY, Samuel H, SCHINNERER, Eva, SHARP, Elmer H, ARENDT, Richard G, CAPAK, Peter L, KOVACS, Attila, BENFORD, Dominic J, FIXSEN, Dale, KARIM, Alexander, LECLERCQ, Samuel, MAHER, Stephen F

“…Analyses of high-redshift ultraluminous infrared (IR) galaxies traditionally use the observed optical to submillimeter spectral energy distribution (SED) and…”
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THE GISMO TWO-MILLIMETER DEEP FIELD IN GOODS-N by Staguhn, Johannes G., Kovács, Attila, Arendt, Richard G., Benford, Dominic J., Decarli, Roberto, Dwek, Eli, Fixsen, Dale J., Hilton, Gene C., Irwin, Kent D., Jhabvala, Christine A., Karim, Alexander, Leclercq, Samuel, Maher, Stephen F., Miller, Timothy M., Moseley, S. Harvey, Sharp, Elmer H., Walter, Fabian, Wollack, Edward J.

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THE GISMO TWO-MILLIMETER DEEP FIELD IN GOODS-N by Staguhn, Johannes G, Kovacs, Attila, Arendt, Richard G, Benford, Dominic J, DeCarli, Roberto, Dwek, Eli, Fixsen, Dale J, Hilton, Gene C, Irwin, Kent D, Jhabvala, Christine A

“…We present deep continuum observations using the GISMO camera at a wavelength of 2 mm centered on the Hubble Deep Field in the GOODS-N field. These are the…”
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High-sensitivity transition-edge-sensed bolometers: improved speed and characterization with AC and DC bias by Foote, Logan, Audley, Michael D, Charles, Bradford, de Lange, Gert, Echternach, Pierre, Fixsen, Dale J, Hui, Howard, Kenyon, Matthew, Nguyen, Hien, O'Brient, Roger, Sharp, Elmer H, Staguhn, Johannes G, van der Kuur, Jan, Zmuidzinas, Jonas

“…J. Appl. Phys. 7 September 2023; 134 (9): 094503 We report on efforts to improve the speed of low-G far-infrared transition-edged-sensed bolometers. We use a…”
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The GISMO 2-millimeter Deep Field in GOODS-N by Staguhn, Johannes G, Kovacs, Attila, Arendt, Richard G, Benford, Dominic J, Decarli, Roberto, Dwek, Eli, Fixsen, Dale J, Hilton, Gene C, Irwin, Kent D, Jhabvala, Christine A, Karim, Alexander, Leclercq, Samuel, Maher, Stephen F, Miller, Timothy M, Moseley, S. Harvey, Sharp, Elmer H, Walter, Fabian, Wollack, Edward J

“…We present deep continuum observations using the GISMO camera at a wavelength of 2 mm centered on the Hubble Deep Field (HDF) in the GOODS-N field. These are…”
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Star and dust formation activities in AzTEC-3: A starburst galaxy at z = 5.3 by Dwek, Eli, Staguhn, Johannes G, Arendt, Richard G, Capak, Peter L, Kovacs, Attila, Benford, Dominic, Fixsen, Dale, Karim, Alexander, Leclercq, Samuel, Maher, Stephen F, Moseley, Samuel H, Schinnerer, Eva, Sharp, Elmer H

“…Analyses of high-redshift ultraluminous infrared (IR) galaxies traditionally use the observed optical to submillimeter spectral energy distribution (SED) and…”
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