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Catalog Service:
HST monitoring of flaring stars in the Galactic bulge

Short name: J/ApJ/754/4
IVOA Identifier: ivo://CDS.VizieR/J/ApJ/754/4
DOI (Digital Object Identifier): 10.26093/cds/vizier.17540004
Publisher: CDS[+][Pub. ID]
More Info: https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/754/4
VO Compliance: Level 2: This is a VO-compliant resource.
Status: active
Registered: 2014 Mar 24 11:32:25Z
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Description


We utilize the Sagittarius Window Eclipsing Extrasolar Planet Search Hubble Space Telescope/Advanced Camera for Surveys data set for a Deep Rapid Archival Flare Transient Search (DRAFTS) to constrain the flare rate toward the older stellar population in the Galactic bulge. During seven days of monitoring 229293 stars brighter than V=29.5, we find evidence for flaring activity in 105 stars between V=20 and V=28. We divided the sample into non-variable stars and variable stars whose light curves contain large-scale variability. The flare rate on variable stars is ~700 times that of non-variable stars, with a significant correlation between the amount of underlying stellar variability and peak flare amplitude. The flare energy loss rates are generally higher than those of nearby well-studied single dMe flare stars.

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