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J/A+AS/131/197      F, G and K stars BVRI photometry (Metanomski+ 1998)

F, G and K stars in the ROSAT all-sky survey. I. Photometry. Metanomski A.D.F., Pasquini L., Krautter J., Cutispoto G., Fleming T.A. <Astron. Astrophys. Suppl. Ser. 131, 197 (1998)> =1998A&AS..131..197M (SIMBAD/NED BibCode)
ADC_Keywords: Radio sources ; Stars, late-type ; Photometry, UBVRI Mission_Name: ROSAT Keywords: stars: late-type - X-ray: stars - surveys Abstract: We present accurate BV(RI)c photometry for a sample of F, G and K stars detected in selected areas of the ROSAT all-sky survey (RASS). We have used the photometry, in addition to low-resolution spectroscopy, to estimate spectral classifications, distances and X-ray luminosities. The log(LX/LV) in the sample lies below -2. Although the sample contains also nearby, inactive stars, it is dominated by active objects. The median X-ray luminosity in our sample is <LX≥29.88 and the mean value of the hardness ratios <HR1≥0.13±0.35. We compare the derived X-ray luminosity function with similar functions obtained from the serendipitous samples of the Einstein Observatory medium sensitivity survey (EMSS, Cat. IX/15) and EXOSAT (Cat. J/A+AS/115/41). Our sample is completely consistent with the EMSS sample of solar type stars, indicating that both our sources and the EMSS sources are representative of the high galactic latitude X-ray stellar population. We do not find extremely active stars (log(LX)≥32), as are found in the EMSS sample, and we argue that these objects are rare. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table3.dat 195 107 Summary of X-ray and observational data as well as results for the studied sample notes.dat 80 86 Individual notes
See also: IX/10 : ROSAT All-Sky Bright Source Catalogue (1RXS) (Voges+ 1996) IX/15 : Einstein EMSS Survey (Gioia+ 1990, Stocke+ 1991) J/ApJS/99/701 : EMSS (Fleming+ 1995) J/A+AS/115/41 : UBV(RI) photometry of cool stars (Cutispoto+, 1996) Byte-by-byte Description of file: table3.dat
Bytes Format Units Label Explanations
1- 15 A15 --- RXJ ROSAT name 16 A1 --- n_RXJ [*] *: see note detailed in file notes.dat 17- 18 I2 h RAXh X-ray source right ascension (J2000.0) 20- 21 I2 min RAXm X-ray source right ascension (J2000.0) 23- 26 F4.1 s RAXs X-ray source right ascension (J2000.0) 28 A1 --- DEX- X-ray source declination sign 29- 30 I2 deg DEXd X-ray source declination (J2000.0) 32- 33 I2 arcmin DEXm X-ray source declination (J2000.0) 35- 36 I2 arcsec DEXs X-ray source declination (J2000.0) 38- 44 F7.5 ct/s Counts Count-rate for the X-ray source 46- 52 F7.2 s Texp Total exposition time 54- 58 F5.2 --- HR1 ? Hardness Ratio 1 (1) 60- 61 I2 h RAh Counterpart right ascension (J2000.0) 63- 64 I2 min RAm Counterpart right ascension (J2000.0) 66- 69 F4.1 s RAs Counterpart right ascension (J2000.0) 71 A1 --- DE- Counterpart declination sign 72- 73 I2 deg DEd Counterpart declination (J2000.0) 75- 76 I2 arcmin DEm Counterpart declination (J2000.0) 78- 79 I2 arcsec DEs Counterpart declination (J2000.0) 81- 84 F4.1 arcsec DX-C Distance between X-ray and counterpart positions 86- 94 A9 --- SpType Spectral type 96- 98 A3 --- n_SpType Note on Spectral type for binaries (2) 100-102 I3 pc Dist Distance of the star form the Sun 104-106 I3 pc E_Dist ? Error in Distance (upper limit) 108-109 I2 pc e_Dist ? Error in Distance (lower limit) 111-115 F5.2 10-15W/m2 fX X-ray flux 117-120 F4.2 10-15W/m2 E_fX Error in fX (upper limit) 122-125 F4.2 10-15W/m2 e_fX Error in fX (lower limit) 127-133 F7.3 10+22W LX X-ray luminosity 135-140 F6.2 10+22W E_LX Error in LX (upper limit) 142-147 F6.2 10+22W e_LX Error in Lx (lower limit) 149-162 A14 --- Name Counterpart name 164-171 A8 --- SpTypeO Counterpart spectral type 173-177 F5.2 mag Vmag Counterpart V magnitude 179-183 F5.2 mag B-V Counterpart B-V colour index 185-189 F5.2 mag V-R ? Counterpart V-R colour index 191-194 F4.2 mag V-I ? Counterpart V-I colour index
Note (1): HR1 = (CR[ch52-201]-CR[ch11-41])/CR[ch11-240] where CD[cha-b] being the count-rate in the channels "a" to "b"Note (2): 1: the binarity/multiplicity obtained by the photometry was confirmed Note (2): 1: the binarity/multiplicity obtained by the photometry was confirmed by the high-resolution spectra 2: the binarity was determined for the high-resolution spectra 3: the binarity is a visual one 4: the binarity information was only obtained through the literature
Byte-by-byte Description of file: notes.dat
Bytes Format Units Label Explanations
1- 15 A15 --- RXJ Source name 17- 18 I2 --- Ntot Total number of lines for the RXJ object 20- 21 I2 --- Nline Running line number in range [1,Ntot] 23- 80 A58 --- Note Text of the note
History: Prepared via OCR at CDS An error was detected in the original publication and corrected. For RXJ 1413.7-0050, the position of the Counterpart (HD 124425) is 14 13 40.6 -00 50 40 instead of 14 13 40.6 -00 05 40
(End) Patricia Bauer [CDS] 31-Jul-1998
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

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