J/ApJS/173/673          M dwarf UV flares in GALEX         (Welsh+, 2007)

The detection of M dwarf UV flare events in the GALEX data archives. Welsh B.Y., Wheatley J.M., Seibert M., Browne S.E., West A.A., Siegmund O.H.W., Barlow T.A., Forster K., Friedman P.G., Martin D.C., Morrissey P., Small T., Wyder T., Schiminovich D., Neff S., Rich R.M. <Astrophys. J. Suppl. Ser., 173, 673-681 (2007)> =2007ApJS..173..673W 2007ApJS..173..673W
ADC_Keywords: Stars, variable ; Magnitudes ; Ultraviolet Keywords: stars: variables: other - ultraviolet: stars Abstract: We present the preliminary results from implementing a new software tool that enables inspection of time-tagged photon data for the astronomical sources contained within individual GALEX ultraviolet (UV) images of the sky. We have inspected the photon data contained within 1802 GALEX images to reveal rapid, short-term (≲500s) UV source variability in the form of stellar "flares." The mean associated change in near-UV (NUV) magnitude due to this flaring activity is 2.7±0.3mag. A list of 49 new UV variable star candidates is presented (associated with 52 separate flare events), together with their associated Sloan Digital Sky Survey (SDSS) photometric magnitudes. From these data we can associate the main source of these UV flare events with magnetic activity on M dwarf stars. Photometric parallaxes have been determined for 32 of these sources, placing them at distances ranging from approximately 25 to 1000pc. The average UV flare energy for these flare events is 2.5x1030ergs, which is of a similar energy to that of U-band, X-ray, and EUV flares observed on many local M dwarf stars. We have found that stars of classes M0 to M5 flare with energies spanning a far larger range and with an energy approximately 5 times greater than those of later (M6 to M8) spectral type. Description: Our initial search for variability within the time-tagged source photon lists was performed with data generated from 1802 individual sky-field images contained in the GALEX data release IR1.1+GR1. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 132 52 List of short-term UV variable objects table2.dat 50 33 M dwarf distances, NUV luminosities and flare energies -------------------------------------------------------------------------------- See also: J/AJ/130/825 : GALEX ultraviolet variability catalog (Welsh+, 2005) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 F6.2 deg RAdeg Right Ascension in degrees (J2000) 8- 13 F6.2 deg DEdeg Declination in degrees (J2000) 15- 33 A19 --- SDSS SDSS-DR4 ID (JHHMMSS.ss+DDMMSS.s) (1) 35- 56 A22 --- Field GALEX Field (MAST Identifier) 58- 60 I3 --- Nobs Number of observations 62- 66 F5.2 mag NUVm NUV (175-275nm) magnitude maximum 68- 71 F4.2 mag NUVv NUV (175-275nm) magnitude variation 73- 77 F5.2 mag gmag ?=- SDSS g band magnitude 78 A1 --- f_gmag [b] magnitude uncertain due to CCD saturation 80- 84 F5.2 mag rmag ?=- SDSS r band magnitude 85 A1 --- f_rmag [b] magnitude uncertain due to CCD saturation 87- 91 F5.2 mag imag ?=- SDSS i band magnitude 92 A1 --- f_imag [b] magnitude uncertain due to CCD saturation 94- 98 F5.2 mag zmag ?=- SDSS z band magnitude 99 A1 --- f_zmag [b] magnitude uncertain due to CCD saturation 101-131 A31 --- Notes Probable spectral Type (or Simbad identifier) 132 A1 --- f_Notes [c] Spectral type based on USNOB data 134-152 A19 --- SDSS-DR6 Exact name from SDSS-DR6 (column added at CDS) -------------------------------------------------------------------------------- Note (1): Format is sometimes rounded: JHHMMSS.ss+DDMMSS; CR = SDSS image cosmic-ray contaminated. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 19 A19 --- SDSS SDSS-DR4 Identifier 21- 25 A5 --- SpType Spectral Type 27- 29 I3 pc Dist Heliocentric distance 31- 35 F5.2 [solLum] Lbol Log of bolometric luminosity 37- 43 E7.2 10-7J ENUV Total NUV flare energy 44 A1 --- n_ENUV [a] Note when two flares observed 46- 49 F4.1 [-] Lfl/Lbol log of NUV flare luminosity referenced to the stellar bolometric luminosity 50 A1 --- n_Lfl/Lbol [a] 'a' when two flares observed -------------------------------------------------------------------------------- History: * 28-May-2009: from electronic version of the journal * 07-Jul-2009: added column "SDSS-DR6" in table1, in order to give the accurate SDSS name
(End) Emmanuelle Perret [CDS] 28-May-2009
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line