VizieR Online Data Catalog: Variable Stars in the Galactic Center (Dong+, 2017)
Abstract
We use the 'DOLPHOT' to detect sources and extract photometry from the HST WFC3/IR observations at the F127M and F135M bands of the Galactic Centre from 2010 to 2014. The F153M observations, which are used to identify variable stars, include 290 dithered exposures from six HST programs.
The detailed description of the HST dataset are given in Table 1 of the paper. We identified 33070 sources. Their F127M and F153M magnitudes, as well as their uncertainties, are given in Table 3. For each star, we used the least chi square method to identify whether it is variable or not. The output from the least chi square method are chi2y and chi2d, which are calculated from all the 290 dithered exposures and the exposures in March and April, 2014, respectively, to examine whether the star varies among years and/or days. In order to reduce the potential variation among dithered exposures, which could be potentially introduced by instrument effects, we also bin the dithered exposures and use the least chi square method to calculate chi2y,b and chi2{d,b}. We classify stars with chi2y>3 and chi2y,b>2 are variables among years and stars with chi2d>3 and chi2d,b>2 are variables among days. The detailed description about the data analysis is given in the paper. In Table 4, we gives the magnitudes of sources in individual dithered exposures, as well as the photometric uncertainties and the quality control parameters provided by 'DOLPHOT', such as signal-to-noise ratio, sharpness^2, crowd and flag. We also cross-correlated our variables with previous variable studies taken by ground-based telescopes in Table 8 and spectroscopic observations in Table 9. (4 data files).- Publication:
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VizieR Online Data Catalog
- Pub Date:
- June 2017
- Bibcode:
- 2017yCat..74703427D
- Keywords:
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- Milky Way;
- Stars: variable;
- Photometry: infrared