Search Results - "MAHER, Stephen F"

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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Bump at the end of the bridge by Jean-Louis Briaud, Maher, Stephen F, James, Ray W

“…Interface bumps between bridge abutments and embankments increase risk and add over $100 million to maintenance expenses every year. Several common causes for…”
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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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