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J/ApJ/570/100       BeppoSAX HELLAS survey. V.               (La Franca+, 2002)

The BeppoSAX High-Energy Large-Area Survey. V. The nature of the hard X-ray source population and its evolution. La Franca F., Fiore F., Vignali C., Antonelli A., Comastri A., Giommi P., Matt G., Molendi S., Perola G.C., Pompilio F. <Astrophys. J. 570, 100 (2002)> =2002ApJ...570..100L
ADC_Keywords: X-ray sources ; Active gal. nuclei ; QSOs ; Redshifts ; Spectroscopy Mission_Name: BeppoSAX Keywords: cosmology: observations - galaxies: active - galaxies: distances and redshifts - galaxies: evolution - quasars: general Abstract: We present optical spectroscopic identifications of hard X-ray (5-10keV) selected sources belonging to the High-Energy Large-Area Survey sample obtained with BeppoSAX down to a 5-10keV flux limit of F(5-10kev)∼3x10-14erg/cm2/s. The sample consists of 118 sources. There are 25 sources that have been identified through correlations with catalogs of known sources. A spectroscopic identification for 49 more has been searched for with the telescope. The results of 13 fields were empty down to R=21. There were 37 sources identified as type 1 active galactic nuclei (AGNs) and nine as type 2 AGNs. The remaining sources are five narrow emission-line galaxies, six clusters, two BL Lac objects, one radio galaxy, and one star. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table3.dat 81 61 Identified hard X-ray sources in the HELLAS catalog table4.dat 26 13 Empty fields in the HELLAS catalog table5.dat 62 99 Emission line measurements
See also: J/A+A/362/799 : The BeppoSAX 2-10 keV Survey (Giommi+, 2000) J/MNRAS/327/771 : BeppoSAX HELLAS survey. II. (Fiore+, 2001) J/A+A/370/900 : BeppoSAX HELLAS survey. IV (Vignali+, 2001) J/MNRAS/342/575 : BeppoSAX HELLAS survey. VI. (Ciliegi+, 2003) J/A+A/409/79 : HELLAS2XMM survey. IV. (Fiore+, 2003) http://argos.mporzio.astro.it/hellas/ : The High Energy Large Area Survey (HELLAS) Home Page Table 2: Observing Log -------------------------------------------------------------------------------- Date Telescope -------------------------------------------------------------------------------- 1998 Dec 28: 3 nights ESO/3.6 m EFOSC2 1999 Jun 8: 3 nights ESO/3.6 m EFOSC2 2000 Jan 3: 3 nights ESO/3.6 m EFOSC2 2000 Jul 29: 3 nights ESO/3.6 m EFOSC2 Byte-by-byte Description of file: table3.dat
Bytes Format Units Label Explanations
1- 2 I2 h RAh BeppoSax right ascension (J2000.0) 4- 5 I2 min RAm BeppoSax right ascension (J2000.0) 7- 10 F4.1 s RAs BeppoSax right ascension (J2000.0) 12 A1 --- DE- BeppoSax Declination sign (J2000) 13- 14 I2 deg DEd BeppoSax declination (J2000.0) 16- 17 I2 arcmin DEm BeppoSax declination (J2000.0) 19- 20 I2 arcsec DEs BeppoSax declination (J2000.0) 23- 24 I2 h RAoh Optical right ascension (J2000.0) 26- 27 I2 min RAom Optical right ascension (J2000.0) 29- 32 F4.1 s RAos Optical right ascension (J2000.0) 34 A1 --- DEo- Optical Declination sign (J2000) 35- 36 I2 deg DEod Optical declination (J2000.0) 38- 39 I2 arcmin DEom Optical declination (J2000.0) 41- 42 I2 arcsec DEos Optical declination (J2000.0) 44- 46 I3 arcsec DXO Difference between X-ray and optical positions 48- 49 I2 arcsec Offx Offaxis 51- 54 F4.1 10-16W/m2/s FX Flux at 5-10keV 56- 59 F4.1 mag Rmag ? R magnitude 61- 72 A12 --- Type Spectroscopic identification 73 A1 --- n_Type [de] Note on Type (1) 75- 79 F5.3 --- z Redshift 80 A1 --- n_z [abc] Note on Redshift (2) 81 A1 --- Note [*] *: cross-correlation with existing catalogs
Note (1): Note on Type: d: Also possible AGN 1: Hβ has a rest frame FWHM∼1000km/s e: Quite a noisy spectrum. Hβ has a rest frame FWHM∼1500km/s Note (2): Note on Redshfit: a: From Colafrancesco et al., 2000A&AS..144..187C b: From Gorosabel et al., 1998A&A...339..719G, misidentified in Fiore et al., 2000NewA....5..143F. c: Wrong coordinates and magnitudes in Fiore et al., 1999MNRAS.306L..55F
Byte-by-byte Description of file: table4.dat
Bytes Format Units Label Explanations
1- 2 I2 h RAh BeppoSax right ascension (J2000.0) 4- 5 I2 min RAm BeppoSax right ascension (J2000.0) 7- 10 F4.1 s RAs BeppoSax right ascension (J2000.0) 12 A1 --- DE- BeppoSax Declination sign (J2000) 13- 14 I2 deg DEd BeppoSax declination (J2000.0) 16- 17 I2 arcmin DEm BeppoSax declination (J2000.0) 19- 20 I2 arcsec DEs BeppoSax declination (J2000.0) 23- 26 F4.2 10-16W/m2/s FX Flux at 5-10keV
Byte-by-byte Description of file: table5.dat
Bytes Format Units Label Explanations
1 A1 --- --- [H] 2- 14 A13 --- Name HELLAS name (Hhhmmss+ddmmss) 16- 20 F5.3 --- z Redshift 22- 25 A4 --- Type EW, FWHM or FWZI measure (1) 27- 31 F5.1 0.1nm MgII ? MgII measurement (2) 32 A1 --- n_MgII [a] a: CIV line instead of MgII line 33- 37 F5.1 0.1nm OII ? OII measurement (2) 39- 43 F5.1 0.1nm Hbeta ? Hbeta measurement (2) 45- 49 F5.1 0.1nm OIII ? OIII measurement (2) 51- 55 F5.1 0.1nm Ha+NII ? Hα+NII measurement (2) 57- 60 F4.1 0.1nm SII ? SII measurement (2)
Note (1): Type of measure: EW: Equivalent width FWHM: Full width half maximum FWZI: Full width at zero intensity Note (2): Observed frame. Negative values correspond to absorption lines
History: From electronic version of the journal References: Fiore et al., Paper I 1999MNRAS.306L..55F Fiore et al., Paper II 2001MNRAS.327..771F, Cat. J/MNRAS/327/771 Comastri et al., Paper III 2001MNRAS.327..781C Vignali et al., Paper IV 2001A&A...370..900V, Cat. J/A+A/370/900
(End) James Marcout, Patricia Bauer [CDS] 21-Jun-2002
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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