J/A+A/596/A49  Synthetic GALEX photometry for IUE sources (Beitia-Antero+, 2016)

A database of synthetic photometry in the GALEX ultraviolet bands for the stellar sources observed with the International Ultraviolet Explorer. Beitia-Antero L., Gomez de Castro A.I. <Astron. Astrophys. 596, A49 (2016)> =2016A&A...596A..49B 2016A&A...596A..49B (SIMBAD/NED BibCode)
ADC_Keywords: Milky Way ; Photometry, ultraviolet Keywords: astronomical databases - catalogues - surveys - ultraviolet: stars Abstract: The Galaxy Evolution Explorer (GALEX) has produced the largest photometric catalogue of ultraviolet (UV) sources. As such, it has defined the new standard bands for UV photometry: the near UV band (NUV) and the far UV band (FUV). However, due to brightness limits, the GALEX mission has avoided the Galactic plane which is crucial for astrophysical research and future space missions. The International Ultraviolet Explorer (IUE) satellite obtained 63,755 spectra in the low dispersion mode (λ/δλ∼300) during its 18-year lifetime. We have derived the photometry in the GALEX bands for the stellar sources in the IUE Archive to extend the GALEX database with observations including the Galactic plane. Good quality spectra have been selected for the IUE classes of stellar sources. The GALEX FUV and NUV magnitudes have been computed using the GALEX transmission curves, as well as the conversion equations between flux and magnitudes provided by the mission (galexgi.gsfc.nasa.gov). Consistency between GALEX and IUE synthetic photometries has been tested using White Dwarfs (WD) contained in both samples. The non-linear response performance of GALEX inferred from this data agrees with the results from GALEX calibration. The photometric database is made available to the community through the services of the Centre de Donnees Stellaires at Strasbourg (CDS). The catalogue contains FUV magnitudes for 1628 sources, ranging from FUV=1.81 to FUV=18.65mag. In the NUV band, the catalogue includes observations for 999 stars ranging from NUV=3.34 to NUV=17.74mag. UV photometry for 1490 sources not included in the GALEX AIS GR5 catalogue is provided; most of them are hot (O-A spectral type) stars. The sources in the catalogue are distributed over the full sky, including the Galactic plane. Description: Synthetic photometry in the GALEX bands for stellar sources observed with the IUE in low dispersion mode is provided. Only high signal-to-noise ratio photometric observations have been used (see bibliographic reference). There are two catalogues: maincat contains synthetic magnitudes for non-variable stars; fuvvar contains synthetic FUV magnitudes for variable stars. Non-variable means that no variation in the UV flux has been detected by IUE. For each entry, coordinates, FUV and NUV magnitudes and magnitude errors are provided. SUMMARY OF CONTENTS: maincat includes FUV and/or NUV synthetic magnitudes for 1722 stars. FUV magnitude is provided for 1628 sources, ranging from FUV=1.81 to FUV=18.65mag. NUV magnitude is provided for 999 stars, ranging from NUV=3.34 to NUV=17.74mag. Also the number of observations used for the calculation is indicated. fuvvar includes FUV synthetic magnitude and error as well as observation date and time for each one of the 88 variable sources in FUV. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file maincat.dat 90 1722 Catalogue of 1722 non-variable stars fuvvar.dat 79 895 FUV magnitudes of 895 observations corresponding to 88 variable stars -------------------------------------------------------------------------------- See also: II/312 : GALEX-DR5 (GR5) sources from AIS and MIS (Bianchi+ 2011) J/MNRAS/427/2180 : GALEX survey subdwarf atmospheric parameters (Nemeth+, 2012) Byte-by-byte Description of file: maincat.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 19 A19 ---- Name IUE object identification 21- 22 I2 h RAh Right ascension (J2000) 24- 25 I2 min RAm Right ascension (J2000) 27- 31 F5.2 s RAs Right ascension (J2000) 33 A1 --- DE- Declination sign (J2000) 34- 35 I2 deg DEd Declination (J2000) 37- 38 I2 arcmin DEm Declination (J2000) 40- 44 F5.2 arcsec DEs Declination (J2000) 46- 48 I3 --- nSWP Number of SWP observations used 50- 55 F6.3 mag FUV ?=- FUV synthetic magnitude 57- 61 F5.3 mag E_FUV ?=- Error on FUV (upper value) 63- 67 F5.3 mag e_FUV ?=- Error on FUV (lower value) 69- 71 I3 --- nLW Number of LW observations used 73- 78 F6.3 mag NUV ?=- NUV synthetic magnitude 80- 84 F5.3 mag E_NUV ?=- Error on NUV (upper value) 86- 90 F5.3 mag e_NUV ?=- Error on NUV (lower value) -------------------------------------------------------------------------------- Byte-by-byte Description of file: fuvvar.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 15 A15 --- Name IUE object identification 17- 18 I2 h RAh Right ascension (J2000) 20- 21 I2 min RAm Right ascension (J2000) 23- 27 F5.2 s RAs Right ascension (J2000) 29 A1 --- DE- Declination sign (J2000) 30- 31 I2 deg DEd Declination (J2000) 33- 34 I2 arcmin DEm Declination (J2000) 36- 40 F5.2 arcsec DEs Declination (J2000) 42- 51 A10 "YYYY-MM-DD" Obs.date Observation date 53- 60 A8 "h:m:s" Obs.time Observation time 62- 67 F6.3 mag FUV FUV synthetic magnitude 69- 73 F5.3 mag E_FUV FUV error on FUV (upper value) 75- 79 F5.3 mag e_FUV FUV error on FUV (lower value) -------------------------------------------------------------------------------- Acknowledgements: Leire Beitia-Antero, lbeitia(at)ucm.es Ana Ines Gomez de Castro, aig(at)ucm.es
(End) Leire Beitia-Antero [UCM, Spain], Patricia Vannier [CDS] 13-Oct-2016
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