J/ApJ/754/4 HST monitoring of flaring stars in the Galactic bulge (Osten+, 2012)

DRAFTS: a Deep, Rapid Archival Flare Transient Search in the Galactic bulge. Osten R.A., Kowalski A., Sahu K., Hawley S.L. <Astrophys. J., 754, 4 (2012)> =2012ApJ...754....4O 2012ApJ...754....4O
ADC_Keywords: Stars, flare ; Photometry, HST ; Stars, variable Keywords: binaries: close; stars: activity; stars: flare; stars: late-type Abstract: 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. Description: The data used in this paper originally came from the Sagittarius Window Eclipsing Extrasolar Planet Search (SWEEPS) project, described in Sahu et al. (2006Natur.443..534S 2006Natur.443..534S). The SWEEPS field (202"x202") was imaged continuously for seven days in 2004 February. The observations consist of 254 exposures in V (F606W) and 265 in I (F814W), each with an exposure time of 339s. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table3.dat 57 105 Properties of DRAFTS flaring stars -------------------------------------------------------------------------------- See also: B/hst : HST Archived Exposures Catalog (STScI, 2007) J/ApJS/207/15 : M dwarf flare spectra (Kowalski+, 2013) J/AJ/141/50 : White-light flares on Kepler cool stars (Walkowicz+, 2011) J/AJ/140/1402 : M dwarf flares from SDSS spectra (Hilton+, 2010) J/other/A+ARV/17.251 : Stars observed with Doppler imaging (Strassmeier, 2009) J/ApJ/685/463 : ChaMPlane X-ray sources in the Galactic bulge (Koenig+, 2008) J/ApJS/173/673 : M dwarf UV flares in GALEX (Welsh+, 2007) Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 I2 h RAh [17] Hour of right ascension (J2000) 4- 5 I2 min RAm [58/59] Minute of right ascension (J2000) 7- 11 F5.2 s RAs Second of right ascension (J2000) 13 A1 --- DE- [-] Sign of declination (J2000) 14- 15 I2 deg DEd [29] Degree of declination (J2000) 17- 18 I2 arcmin DEm [10/13] Arcminute of declination (J2000) 20- 24 F5.2 arcsec DEs Arcsecond of declination (J2000) 26- 30 F5.2 mag Vmag [20/28] HST/ACS F606W magnitude 32- 36 F5.2 mag Imag [18/26] HST/ACS F814W magnitude 38- 46 A9 --- Var Variability type ("flat" or "var/irreg", "var/reg") 48- 52 F5.2 d Per [0.06/11.8]? Period of any underlying regular variability 54- 57 F4.2 mag DAmp [0.02/2.51] Range of the amplitude (1) -------------------------------------------------------------------------------- Note (1): Range is defined as the difference in amplitude between the values in the 95th and 5th percentile in the original light curve; see Section 4.2 for details. -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Emmanuelle Perret [CDS] 25-Feb-2014
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