C. Brambora
Goddard Space Flight Center
18 Papers
138 Citations
C. Brambora is an academic researcher from Goddard Space Flight Center. The author has contributed to research in topics: James Webb Space Telescope & Spectrograph. The author has an hindex of 7, co-authored 16 publications.
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Papers
SMAP L-Band Microwave Radiometer: Instrument Design and First Year on Orbit
Jeffrey R. Piepmeier,Paolo Focardi,Kevin Horgan,Joseph Knuble,Negar Ehsan,Jared Lucey,C. Brambora,Paula R. Brown,Pamela Hoffman,Richard French,Rebecca Mikhaylov,Eug-Yun Kwack,Eric M. Slimko,Douglas Dawson,Derek Hudson,Jinzheng Peng,Priscilla N. Mohammed,Giovanni De Amici,Adam P. Freedman,James Medeiros,Fred Sacks,Robert H. Estep,Michael W. Spencer,Curtis W. Chen,K. Wheeler,W. Edelstein,Peggy O'Neill,Eni G. Njoku +27 more
TL;DR: The SMAP radiometer electronics are thermally controlled to achieve good radiometric stability, and analyses of on-orbit results indicate that the electrical and thermal characteristics of the electronics and internal calibration sources are very stable and promote excellent gain stability.
The OSIRIS-REx Visible and InfraRed Spectrometer (OVIRS): Spectral Maps of the Asteroid Bennu
D. C. Reuter,Amy Simon,Jason Hair,Allen Lunsford,Sridhar S. Manthripragada,Vincent T. Bly,Brent J. Bos,C. Brambora,E. Caldwell,G. Casto,Z. Dolch,Paul Finneran,D. E. Jennings,Murzy D. Jhabvala,E. Matson,M. McLelland,Wayne D. Roher,T. Sullivan,E. Weigle,Yiting Wen,Donna Wilson,Dante S. Lauretta +21 more
TL;DR: The OSIRIS-REx VISible and Infrared Spectrometer (OVIRS) as mentioned in this paper is a point spectrometer covering the spectral range of 0.4 to 4.3 microns (25,000-2300 cm-1).
Detector arrays for the James Webb Space Telescope near-infrared spectrograph
Bernard J. Rauscher,David Alexander,C. Brambora,Rebecca J. Derro,Chuck Engler,Ori Fox,Ori Fox,Matthew B. Garrison,Greg Henegar,Robert J. Hill,Thomas Johnson,Don J. Lindler,Sridhar S. Manthripragada,Cheryl J. Marshall,Brent Mott,Thomas M. Parr,Wayne D. Roher,Kamdin B. Shakoorzadeh,Kamdin B. Shakoorzadeh,Miles Smith,Augustyn Waczynski,Yiting Wen,Donna Wilson,Wei Xia-Serafino,Craig A. Cabelli,Edward Cheng,James D. Garnett,Markus Loose,Majid Zandian,Joseph Zino,Tim Ellis,Bryan Howe,Mirium Jurado,Ginn Lee,John Nieznanski,Peter Wallis,James York,Michael W. Regan,Georgio Bagnasco,Torsten Böker,Guido De Marchi,Pierre Ferruit,Peter Jakobsen,Paolo Strada +43 more
TL;DR: The James Webb Space Telescope's (JWST) Near Infrared Spectrograph (NIRSpec) incorporates two 5 micron cutoff (lambda(sub co) = 5 microns) 2048x2048 pixel Teledyne HgCdTe HAWAII-2RG sensor chip assemblies as discussed by the authors.
Lunar Ice Cube Mission: Determining Lunar Water Dynamics with a First Generation Deep Space CubeSat
Pamela Clark,Benjamin Malphrus,Kevin Brown,Dennis C. Reuter,Robert J. MacDowall,D. Folta,Avi Mandell,Terry Hurford,C. Brambora,D. Patel,S. Banks,W. Farrell,Noah E. Petro,M. Tsay,V. Hruby,Carl Brandon,Peter Chapin +16 more
- 01 Mar 2016
TL;DR: Pamela Clark, Ben Malphrus, Kevin Brown, Dennis Reuter, Robert MacDowall, David Folta, Avi Mandell, Terry Hurford, Cliff Brambora, Deepak Patel, Stuart Banks, William Farrell, Noah Petro, Michael Tsay, V. E.
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Detectors for the James Webb Space Telescope near infrared spectrograph (NIRSpec)
Bernard J. Rauscher,Torsten Böker,Craig A. Cabelli,Guido De Marchi,Pierre Ferruit,James D. Garnett,Robert J. Hill,Markus Loose,Michael W. Regan,Augustyn Waczynski,Yiting Wen,Selmer Wong,M. Zandian,David Alexander,C. Brambora,Rebecca J. Derro,Carol Dunn,Tim Ellis,Matthew B. Garrison,Bryan Howe,Peter Jakobsen,Thomas E. Johnson,Miriam Jurado,Ginn Lee,Sridhar S. Manthripragada,James M. Marsh,Cheryl J. Marshall,Robert J. Martineau,Brent Mott,John Nieznanski,Wayne D. Roher,Kamdin B. Shakoorzadeh,Miles Smith,Paolo Strada,Peter Wallis,Wei Xia-Serafino,James York +36 more
TL;DR: In this paper, the authors summarize recent progress on the NIRSpec detector subsystem including tests demonstrating that JWST's Rockwell HAWAII-2RG sensor chip assemblies have achieved Technology Readiness Level 6 (TRL-6).
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