Wf/pc SV Observation Set #3/PHOTOMETRIC and Quantum Efficiency Sta

Details Wf/pc SV Observation Set #3/PHOTOMETRIC and Quantum Efficiency Sta Wf/pc SV Observation Set #3/PHOTOMETRIC and Quantum Efficiency Sta

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990hst..prop.1323w&link_type=abstract

HST Proposal ID #1323

Physics

Hst Proposal Id #1323

Scientific paper

The observations made in WF/PC SV Observation Set #1 of the calibration fields in globular clusters produce a stable photometric system that is related to ground-based work. However, these observations are not sufficient to monitor short term variations in the chips. To verify the short term stability as required by the CEIS requires additional work. A subset of the filters will be used to verify this stability. The procedure is to return to the calibration field in Omega Centauri (NGC 5139) or the one in NGC 6752 according to a planned schedule. Most proposal sequences are spaced relative to the first UV flood, at the start of SV. The repeat of the observations are CONDITIONAL on a second flood being scheduled. Dark calibration exposures are taken with each filter sequence. Note these dark exposures do not require dark time

Affiliated with

Also associated with

No associations

Rating

Wf/pc SV Observation Set #3/PHOTOMETRIC and Quantum Efficiency Sta 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 Wf/pc SV Observation Set #3/PHOTOMETRIC and Quantum Efficiency Sta, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Wf/pc SV Observation Set #3/PHOTOMETRIC and Quantum Efficiency Sta will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1093941