WFPC2 Cycle 12 Close-Out Photometric Cross-Calibration

Details WFPC2 Cycle 12 Close-Out Photometric Cross-Calibration WFPC2 Cycle 12 Close-Out Photometric Cross-Calibration

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003hst..prop10078k&link_type=abstract

HST Proposal ID #10078

Physics

Hst Proposal Id #10078

Scientific paper

This proposal is aimed at providing photometric zeropoint cross-calibration between the commonly used WFPC2 photometric filter sets and those that will be used for ACS and WFC3. The proposal consists of observations of a set of standard stars, including the SDSS primary standard BD+17D4708 {F5} and two red standard stars, VB8 {an M7-dwarf} and 2M0036+18 {L3.5 dwarf}. For the red stars, medium and broad-band filters redward of F606W are calibrated, while for BD+17D4708 an extensive set of 22 medium and broad-band filters is used {from F185W to F1042M}. The intent is to observe these stars with as many filters as possible, to eventually allow cross-calibration of archival WFPC2 data with data from ACS, WFC3, SDSS and 2MASS.

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