TY - GEN
T1 - Coronagraphic Exploration Camera (CorECam)
AU - Clampin, Mark
AU - Lyon, Richard
AU - Petro, Larry
AU - Seager, Sara
AU - Marley, Mark
AU - Melnick, Gary
AU - Weinberger, Alycia
AU - Woodruff, Robert
AU - Horner, Scott
AU - Ford, Holland
AU - Illingworth, Garth
AU - Kasting, Jim
AU - Lin, Doug
AU - Kuchner, Marc
AU - Shao, Mike
AU - Sparks, William
AU - Rauscher, Bernard
AU - Tolls, Volker
AU - Carter, Ruth
PY - 2006
Y1 - 2006
N2 - The CorECam Instrument Concept Study (ICS) addressed the requirements and science program for the Terrestrial Planet Finder Coronagraph's (TPF-C) primary camera. CorECam provides a simple interface to TPF-C's Starlight Suppression System (SSS) which would be provided by the TPF-C Program, and comprises camera modules providing visible, and near-infrared (NIR) camera focal plane imaging. In its primary operating mode, CorECam will conduct the core science program of TPF-C, detecting terrestrial planets at visible wavelengths. CorECam additionally provides the imaging capabilities to characterize terrestrial planets, and conduct an extended science program focused on investigating the nature of the exosolar systems in which terrestrial planets are detected. In order to evaluate the performance of CorECam we developed a comprehensive, end-to-end model using OSCAR which has provided a number of key conclusions on the robustness of the TPF-C baseline design, and allows investigation of alternative techniques for wavefront sensing and control. CorECam recommends photon counting detectors be baselined for imaging with TPF-C since they provide mitigations against the background radiation environment, improved sensitivity and facilitate alternative WFSC approaches.
AB - The CorECam Instrument Concept Study (ICS) addressed the requirements and science program for the Terrestrial Planet Finder Coronagraph's (TPF-C) primary camera. CorECam provides a simple interface to TPF-C's Starlight Suppression System (SSS) which would be provided by the TPF-C Program, and comprises camera modules providing visible, and near-infrared (NIR) camera focal plane imaging. In its primary operating mode, CorECam will conduct the core science program of TPF-C, detecting terrestrial planets at visible wavelengths. CorECam additionally provides the imaging capabilities to characterize terrestrial planets, and conduct an extended science program focused on investigating the nature of the exosolar systems in which terrestrial planets are detected. In order to evaluate the performance of CorECam we developed a comprehensive, end-to-end model using OSCAR which has provided a number of key conclusions on the robustness of the TPF-C baseline design, and allows investigation of alternative techniques for wavefront sensing and control. CorECam recommends photon counting detectors be baselined for imaging with TPF-C since they provide mitigations against the background radiation environment, improved sensitivity and facilitate alternative WFSC approaches.
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U2 - 10.1117/12.672816
DO - 10.1117/12.672816
M3 - Conference contribution
AN - SCOPUS:33749017646
SN - 0819463302
SN - 9780819463302
T3 - Proceedings of SPIE - The International Society for Optical Engineering
BT - Space Telescopes and Instrumentation I
T2 - Space Telescopes and Instrumentation I: Optical, Infrared, and Millimeter
Y2 - 24 May 2006 through 31 May 2006
ER -