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pro vyhledávání: '"Michael A. K. Gross"'
Autor:
Michael A. K. Gross, Charles R. Taylor
Publikováno v:
SPIE Proceedings.
The Stratospheric Observatory for Infrared Astronomy (SOFIA) tracking camera simulator is a component of the Telescope Assembly Simulator (TASim). TASim is a software simulation of the telescope optics, mounting, and control software. Currently in it
Autor:
Douglas Hoffman, Peter T. Zell, Allan W. Meyer, Jürgen Wolf, William D. Vacca, Erin C. Smith, Maureen L. Savage, Elizabeth Moore, Eric B. Burgh, B-G Andersson, Hans Zinnecker, Stefan Teufel, Jeffrey Van Cleve, William T. Reach, Scott R. Miller, Alfred Krabbe, Jeff Homan, Ting C. Tseng, Geoffrey Ediss, Stephen C. Jensen, Thomas L. Roellig, John Rasmussen, Randolf Klein, Charles Kaminski, Rick Brewster, Andrew L. Helton, John E. Vaillancourt, Enrico Pfueller, Manuel Wiedemann, Ehsan Talebi, Oliver Zeile, Adwin Boogert, Sybil Adams, Julie Schonfeld, Jeanette Le, Eddie Zavala, S. Shenoy, William B. Latter, J. T. Radomski, Yannick Lammen, Andreas Reinacher, Jim De Buizer, Donald J. Nickison, Daniel Kozarsky, J. W. Miles, Randy Grashuis, Walter E. Miller, Ravi Sankrit, Nancy McKown, Brent R. Cobleigh, Maura Fujieh, Riccardo Melchiorri, Pasquale Temi, Göran Sandell, Michael A. K. Gross, Kortney Opshaug, Erick T. Young, Pamela M. Marcum, Edward Harmon, Eric E. Becklin, Edward W. Dunham, Ralph Y. Shuping, Michael Hutwohl, Ulrich Lampater, Joseph D. Adams, Holger Jakob, Christian Engfer, Steven Culp
Publikováno v:
Web of Science
The Stratospheric Observatory for Infrared Astronomy (SOFIA) has recently concluded a set of engineering flights for Observatory performance evaluation. These in-flight opportunities are viewed as a first comprehensive assessment of the Observatory's
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7ee27abcd3b6288571e87abc7a5bc3c2
Autor:
Michael A. K. Gross, Joel R. Primack
Publikováno v:
Current Aspects of Neutrino Physics ISBN: 9783642074240
Cosmological dark matter (DM) in the form of neutrinos with masses of up to a few electron volts is known as hot dark matter (HDM). In 1979–83, this appeared to be perhaps the most plausible dark-matter candidate. Such HDM models of cosmological st
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1fac20e97747ab67141c427f0f203e82
https://doi.org/10.1007/978-3-662-04597-8_12
https://doi.org/10.1007/978-3-662-04597-8_12
Autor:
Michael A. K. Gross, Avishai Dekel, Rachel S. Somerville, Joel R. Primack, Risa H. Wechsler, George R. Blumenthal
We review our analysis of the clustering properties of ``Lyman-break'' galaxies (LBGs) at redshift z~3, previously discussed in Wechsler et al (1998). We examine the likelihood of spikes found by Steidel et al (1998) in the redshift distribution of L
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0d609409cc4a82e3878339beadd8bcc6
We address the high peaks found by Steidel et al (1997) in the redshift distribution of ``Lyman-break'' objects (LBOs) at redshift z~3. The highest spike represents a relative overdensity of 2.6 in the distribution of LBOs in pixels of comoving size
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ae386139bbaf9358eb79608565a29b34
http://arxiv.org/abs/astro-ph/9712141
http://arxiv.org/abs/astro-ph/9712141
Reconstruction of the linear power spectrum from observational data provides a way to compare cosmological models to a large amount of data, as Peacock & Dodds (1994, 1996) have shown. By applying the appropriate corrections to the observational powe
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cee2dfd7aa522e7d2b1a9ffc052317a7