J/ApJS/117/319 Northern RASS X-ray sources catalog (Appenzeller+ 1998) ================================================================================ Identification of a complete sample of northern ROSAT All-Sky Survey X-ray sources. III. The catalog. Appenzeller I., Thiering I., Zickgraf F.-J., Krautter J., Voges W., Chavarria C., Kneer R., Mujica R., Pakull M., Rosso C., Ruzicka F., Serrano A., Ziegler B.=1998ApJS..117..319A ================================================================================ ADC_Keywords: Radio sources ; Photometry Mission_Name: ROSAT Keywords: galaxies: active - galaxies: clusters: general - surveys - X-rays: galaxies - X-rays: general - X-rays: stars Abstract: We present a catalog of optical identifications of a representative sample of northern ({delta})>-9{deg}) ROSAT All-Sky Survey (RASS) sources. A full identification has been carried out for a count-rate- and area-limited complete RASS subsample comprising 674 sources. All sources are within six study areas outside the galactic plane (|b|>19.6{deg}), one area being near the north Galactic pole and one near the north ecliptic pole. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 151 674 Count-rate- and area-limited X-ray complete subsample table2.dat 151 70 Additional sources outside the count-rate- and Area-limited subsample notes.dat 80 452 Individual notes -------------------------------------------------------------------------------- See also: IX/10 : ROSAT All-Sky Bright Source Catalogue (1RXS) (Voges+ 1996) VIII/14 : 87GB Catalog of radio sources (Gregory et al., 1991) Byte-by-byte Description of file: table1.dat table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 A4 --- Seq Internal designation for the X-ray sources in the six study areas (1) 6- 16 A11 --- RXJ RXJ designation 18- 19 I2 h RAh X-source right ascension (2000) 21- 22 I2 min RAm X-source right ascension (2000) 24- 27 F4.1 s RAs X-source right ascension (2000) 29 A1 --- DE- X-source declination sign (2000) 30- 31 I2 deg DEd X-source declination (2000) 33- 34 I2 arcmin DEm X-source declination (2000) 36- 37 I2 arcsec DEs X-source declination (2000) 39- 44 F6.3 ct/s CRate Net X-ray source count rate (2) 46- 50 F5.3 ct/s e_CRate rms uncertainty on CountRate 52- 57 F6.2 --- HR1 Hardness ratio HR1 (3) 59- 63 F5.2 --- e_HR1 rms uncertainty on HR1 65- 69 F5.2 --- HR2 Hardness ratio HR2 (3) 71- 75 F5.2 -- e_HR2 rms uncertainty on HR2 77- 81 F5.1 10-13mW/m2 FX X-ray flux 83- 85 I3 arcsec DRA ? RA(X)-RA(O) (4) 87- 89 I3 arcsec DDE ? DE(X)-DE(O) (4) 91 I1 --- Q [1-4] Identification quality index (5) 93- 99 A7 --- Class Classification of the optical counterpart (6) 101-107 A7 --- SpType Spectral type for stellar sources 109-113 F5.3 --- z ? Redshift for extragalactic sources 115-119 F5.2 mag Vmag ? V magnitude 121-125 F5.2 mag B-V ? B-V colour index 127-131 F5.2 --- XV ? XV index (log(f_X_/f_V_) (7) 133-136 I4 mJy F4.85GHz ? Radio flux at 4.85GHz (6cm) for sources within 0{deg} ) 138-149 A12 ---- Name designation of the (main) optical counterpart, if known (8) 151 A1 --- Rem [R] remark detailed in file notes.dat -------------------------------------------------------------------------------- Note (1): The letters A through F refer to study areas I, II, III, IV, V and VI. Note (2): Net X-ray source count rate as derived after superposition of all ROSAT scan stripes and correction for vignetting and dead time. Note (3): HR1=(B-A)/(B+A) and HR2=(D-C)/(D+C) A: integrated counts in the energy range 0.11-0.41keV B: integrated counts in the energy range 0.52-2.01keV. C: integrated counts in the energy range 0.52-0.90keV. D: integrated counts in the energy range 0.91-2.01keV. Note (4): No values for extended objects (such as clusters), double stars and other cases where no accurate position could be determined. Note (5): 1: reliable identifications based on our own observations 2: reliable informations with a known object based on literature data 3: likely but uncertain identifications 4: case in which no plausible optical counterpart could be found Note (6): For multiple (maximum 3) counterparts, the entries are listed in order of likelihood or assumed relative contribution to the total X-ray flux and are separated by a colon. st: normal star (i.e., an unresolved objects showing a stellar absorption spectrum, including late-type stars showing chromospheric emission lines, such as dMe stars). ES: (hot) emission-line star (unresolved objects showing a blue continuum, with or without absorption lines, and unshifted emission lines. Most objects classified ES show typical CV spectra). WD: white dwarf (star showing absorption lines with FWHM>1500km/s). WDA: white dwarf with Balmer lines only. S1: Seyfert 1 galaxy (galaxy with an unresolved nucleus showing a Seyfert-type spectrum with broad (>2000km/s) permitted lines and with M_B_>-23.5). S15..S19: Seyfert galaxy of type 1.5-1.9 NL1: Narrow-line Seyfert 1 galaxy (spectrum showing line ratios typical of Seyfert 1 but with lower FWHM of permitted lines). S2: Seyfert 2 galaxy LI: LINER QSO: quasi-stellar object (unresolved or resolved object with M_B_<-23.5 showing a Seyfert 1 spectrum). BLL: BL Lac object G: (single) galaxy Gin: interacting galaxy pair Gr: radio galaxy GSB: starburst galaxy C: cluster or group of galaxies Note (7): Decadic logarithm of the ratio of the X-ray flux and the visual flux Note (8): For stars, the entry numbers in the most common star catalogs are listed. For other objects, the corresponding designations and abbreviations listed in the NED and SIMBAD databases are given. In a few cases of very long designations, the names have been shortened or truncated. Since in all these cases coordinate information is given in the table, this should not result in ambiguities. The full designations can be obtained from the NED. Although in the Remarks (Sect. 3, below) NRAO VLA Sky Survey (NVSS) (Condon et al., 1998, Cat. ) data are quoted for some sources, no NVSS designations are used since the final version of the NVSS catalog is still listed as "in preparation." -------------------------------------------------------------------------------- Byte-by-byte Description of file: notes.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 A4 --- Seq Sequential number 6- 80 A75 --- Note Text of the note -------------------------------------------------------------------------------- History: From ApJS electronic version References: Zickgraf et al., Paper I. 1998AN....319...42Z Zickgraf et al., Paper II. 1997A&AS..123..103Z Zickgraf et al., Paper V. 1997A&A...323L..21Z Zickgraf et al., Paper VI. 1998A&A...339..457Z ================================================================================ (End) James Marcout, Patricia Bauer [CDS] 24-Sep-1998