C
Catherine T. Marx
Researcher at Goddard Space Flight Center
Publications - 36
Citations - 3930
Catherine T. Marx is an academic researcher from Goddard Space Flight Center. The author has contributed to research in topics: Telescope & Grism. The author has an hindex of 9, co-authored 34 publications receiving 3691 citations.
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Journal ArticleDOI
The Infrared Array Camera (IRAC) for the Spitzer Space Telescope
Giovanni G. Fazio,Joseph L. Hora,Lori E. Allen,M. L. N. Ashby,Pauline Barmby,Lynne K. Deutsch,Lynne K. Deutsch,J.-S. Huang,S. C. Kleiner,Massimo Marengo,S. T. Megeath,Gary J. Melnick,Michael A. Pahre,Brian M. Patten,J. Polizotti,Howard A. Smith,R. S. Taylor,Zhong Wang,S. P. Willner,William F. Hoffmann,Judy Pipher,William J. Forrest,C. W. McMurty,Craig R. McCreight,Mark E. McKelvey,Robert E. McMurray,David G. Koch,Samuel H. Moseley,R. G. Arendt,John Eric Mentzell,Catherine T. Marx,P. Losch,P. Mayman,W. Eichhorn,Danny J. Krebs,Murzy D. Jhabvala,Daniel Y. Gezari,D. J. Fixsen,J. Flores,K. Shakoorzadeh,R. Jungo,Claef Hakun,Lois G. Workman,Gabriel Karpati,R. Kichak,R. Whitley,S. Mann,Eric V. Tollestrup,Peter Eisenhardt,Daniel Stern,Varoujan Gorjian,Bidushi Bhattacharya,Sean Carey,Brant O. Nelson,William J. Glaccum,Mark Lacy,Patrick J. Lowrance,Seppo Laine,William T. Reach,J. A. Stauffer,Jason Surace,Gillian Wilson,Edward L. Wright,Alan W. Hoffman,George Domingo,Martin Cohen +65 more
TL;DR: The Infrared Array Camera (IRAC) is one of three focal plane instruments on the Spitzer Space Telescope as mentioned in this paper, which is a four-channel camera that obtains simultaneous broadband images at 3.6, 4.5, 5.8, and 8.0 m.
Proceedings ArticleDOI
In-flight performance and calibration of the Infrared Array Camera (IRAC) for the Spitzer Space Telescope
Joseph L. Hora,Giovanni G. Fazio,Lori E. Allen,Matthew L. N. Ashby,Pauline Barmby,Lynne K. Deutsch,Jiasheng S. Huang,Massimo Marengo,S. T. Megeath,Gary J. Melnick,Michael A. Pahre,Brian M. Patten,Howard A. Smith,Zhong Wang,Steven P. Willner,William F. Hoffmann,Judith L. Pipher,William J. Forrest,Craig W. McMurtry,Craig R. McCreight,Mark E. McKelvey,Robert E. McMurray,Samuel H. Moseley,Richard G. Arendt,John Eric Mentzell,Catherine T. Marx,D. J. Fixsen,Eric V. Tollestrup,Peter Eisenhardt,Daniel Stern,Varoujan Gorjian,Bidushi Bhattacharya,Sean Carey,William J. Glaccum,Mark Lacy,Patrick Lowrance,Seppo Laine,Brant O. Nelson,William T. Reach,John R. Stauffer,Jason Surace,Gillian Wilson,Edward L. Wright +42 more
TL;DR: In this paper, the authors summarize the in-flight scientific, technical, and operational performance of IRAC in two nearly adjacent fields of view on the Spitzer Space Telescope (SST) and show that IRAC is a four-channel camera that obtains simultaneous broad-band images at 3.6, 4.5, 5.8, and 8.0 μm.
Proceedings ArticleDOI
GISMO: a 2-millimeter bolometer camera for the IRAM 30 m telescope
Johannes G. Staguhn,Dominic J. Benford,Christine A. Allen,S. Harvey Moseley,Elmer Sharp,Troy Ames,Walter Brunswig,David T. Chuss,Eli Dwek,Stephen F. Maher,Catherine T. Marx,Timothy M. Miller,S. Navarro,Edward J. Wollack +13 more
TL;DR: In this paper, a bolometer camera (the Goddard-Iram Superconducting 2-Millimeter Observer, GISMO) was built for the IRAM 30 m telescope to provide the capability to rapidly observe galactic and extragalactic dust emission.
Journal ArticleDOI
GISMO, a 2 mm Bolometer Camera Optimized for the Study of High Redshift Galaxies
Johannes Staguhn,Johannes Staguhn,Christine A. Allen,Dominic J. Benford,Elmer Sharp,Troy Ames,R. G. Arendt,David T. Chuss,Eli Dwek,Attila Kovács,Stephen F. Maher,Catherine T. Marx,Timothy M. Miller,S. Harvey Moseley,S. Navarro,A. Sievers,George M. Voellmer,Edward J. Wollack +17 more
TL;DR: GISMO (the Goddard-IRAM Superconducting 2-Millimeter Observer) is a 2 mm, 128 element superconducting Transition Edge Sensor (TES) based bolometer camera for the IRAM 30 m telescope in Spain this article.
Proceedings ArticleDOI
Angle-of-incidence effects in the spectral performance of the infrared array camera of the Spitzer Space Telescope
TL;DR: In this article, a ray-tracing analysis of the IRAC optical system indicates a distribution of angles that is position-dependent at each optical element and the focal-plane arrays, which is necessary to attain the highest possible photometric accuracy when using IRAC for astronomical observations.