Computer Science – Performance
Scientific paper
Dec 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aas...203.4602s&link_type=abstract
American Astronomical Society Meeting 203, #46.02; Bulletin of the American Astronomical Society, Vol. 35, p.1280
Computer Science
Performance
1
Scientific paper
HST provides a unique resource for high contrast imaging with its panchromatic complement of coronagraphically augmented imagers: NICMOS (near-IR), STIS (broad band optical), and ACS (UV/Optical). With the advent of the NICMOS Cooling System (NCS), coronagraphy with NICMOS camera 2 (76 mas/pixel) was re-enabled at higher quantum efficiency (compared to Cycle 7) through the HST Cycle 11 SMOV program and fully recalibrated in Cycle 12. In preparation for HST cycle 13, we discuss the performance levels of NCS-era NICMOS coronagraphy in terms of background (scattered and diffracted) background light rejection from coronagraphically occulted stars, coronagraphic optical artifacts, instrumental sensitivity and detectability of point sources and low surface brightness circumstellar dust. We comment on the efficacy of astrometric and photometric measures in very high contrast coronagraphic fields. We compare the attributes of the three HST coronagraphic imagers as they have been applied to studies of circumstellar debris disks, in particular to HD 141569A and HR 4796A for which ground-based observations have also been attempted, and in consideration of future HST imaging programs. We discuss direct imaging of low mass, (L & T) dwarf companions and hot giant planets in``close'' (> 0.3 arcsec) proximity to their host stars and explore this in light of the companion detection performance capabilities demonstrated with the Keck AO system. We present the status of the calibration of a new NICMOS observing mode -- coronagraphic polarimetry -- which is now under study. This work was supported by NASA grants NAG5-3042 and 10843 to the NICMOS Instrument Definition and Guaranteed Time Observing Teams.
Hines Dean
Schneider Gerardo
Silverstone Murray
No associations
LandOfFree
HST/NICMOS Coronagraphy: Prospects for Cycle 13 and Beyond - A Choice of Coronagraphic Imagers does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with HST/NICMOS Coronagraphy: Prospects for Cycle 13 and Beyond - A Choice of Coronagraphic Imagers, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and HST/NICMOS Coronagraphy: Prospects for Cycle 13 and Beyond - A Choice of Coronagraphic Imagers will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1419798