VizieR Online Data Catalog: PHAT X. UV-IR photometry of M31 stars (Williams+, 2014)
Abstract
The data for the Panchromatic Hubble Andromeda Treasury (PHAT) survey were obtained from 2010 July 12 to 2013 October 12 using the Advanced Camera for Surveys (ACS) Wide Field Channel (WFC), the Wide Field Camera 3 (WFC3) IR (infrared) channel, and the WFC3 UVIS (ultraviolet-optical) channel. The observing strategy is described in detail in Dalcanton et al. (2012ApJS..200...18D). A list of the target names, observing dates, coordinates, orientations, instruments, exposure times, and filters is given in Table 1. Using the ACS and WFC3 cameras aboard HST, we have photometered 414 contiguous WFC3/IR footprints covering 0.5deg2 of the M31 star-forming disk.
(4 data files).- Publication:
-
VizieR Online Data Catalog
- Pub Date:
- January 2015
- DOI:
- 10.26093/cds/vizier.22150009
- Bibcode:
- 2015yCat..22150009W
- Keywords:
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- Galaxies: nearby;
- Photometry: HST;
- Surveys;
- Ultraviolet;
- Infrared sources