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J/A+A/433/1163      Spectral catalog of BeppoSAX blazars     (Donato+, 2005)

Six years of BeppoSAX observations of blazars: A spectral catalog. Donato D., Sambruna R.M., Gliozzi M. <Astron. Astrophys., 433, 1163-1169 (2005)> =2005A&A...433.1163D
ADC_Keywords: X-ray sources ; Active gal. nuclei ; BL Lac objects ; QSOs Keywords: galaxies: active - galaxies: fundamental parameters - galaxies: nuclei - X-rays: galaxies - catalogs Abstract: We present a spectral catalog for blazars based on the BeppoSAX archive. The sample includes 44 High-energy peaked BL Lacs (HBLs), 14 Low-energy peaked BL Lacs (LBLs), and 28 Flat Spectrum Radio Quasars (FSRQs). A total of 168 LECS, MECS, and PDS spectra were analyzed, corresponding to observations taken in the period 1996-2002. The 0.1-50keV continuum of LBLs and FSRQs is generally fitted by a single power law with Galactic column density. Description: Spectral parameters for 168 BeppoSAX observations of 86 blazars are presented. For each blazars observation data, count rates, flux, spectral parameters (intrinsic absorption, photon index, energy break, and reduced chi-squared) derived from the analysis are given. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 57 86 The sample table2.dat 95 168 Observation Log table3.dat 99 107 Sources with power law as best-fit model table4.dat 158 61 Spectra best-fitted by a curved model table5.dat 71 61 Single power law fits for Spectra in Table 4
See also: J/A+A/375/739 : Hard X-ray properties of blazars (Donato+, 2001) Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1 A1 --- Type [HLF] Object type (G1) 3- 19 A17 --- Name Object name 21- 22 I2 h RAh Right ascension (J2000) 24- 25 I2 min RAm Right ascension (J2000) 27- 30 F4.1 s RAs Right ascension (J2000) 32 A1 --- DE- Declination sign (J2000) 33- 34 I2 deg DEd Declination sign (J2000) 36- 37 I2 arcmin DEm Declination sign (J2000) 39- 42 F4.1 arcsec DEs Declination sign (J2000) 44- 48 F5.3 --- z ?=- Redshift 50- 54 F5.2 10+20cm-2 NH Galactic absorption (1) 56- 57 I2 --- Nobs ? Number of observations in the archive
Note (1): Galactic absorption based on Dickey & Lockman (1990ARA&A..28..215D)
Byte-by-byte Description of file: table2.dat
Bytes Format Units Label Explanations
1 A1 --- Type [HLF] Type of objects (G1) 3- 19 A17 --- Name Source Name 21- 30 A10 "DD/MM/YYYY" Date Observation Date 32- 40 A9 --- Seq Sequence Number of the observation 42- 46 F5.1 ks ExpL Exposure time for LECS 48- 53 F6.2 c/s CRL ?=- Counts rate for LECS in band 0.1-2keV (1) 55- 59 F5.2 c/s e_CRL ?=- Error on counts rate for LECS 61- 65 F5.1 ks ExpM Exposure time for MECS 67- 72 F6.2 c/s CRM ?=- Counts rate for MECS in band 2-10keV (1) 74- 78 F5.2 c/s e_CRM ?=- Error on counts rate for MECS 80- 83 F4.1 ks ExpP Exposure time for PDS 85- 89 F5.1 c/s CRP ?=- Counts rate for PDS in band 13-50keV (1) 91- 93 F3.1 c/s e_CRP ?=- Error on counts rate for PDS 95 I1 --- Code [1/6] Model used for the best fit (2)
Note (1): Less than 3σ detections are omitted Note (2): Code for model used for the best fit as follows: 1 = Power law with absorption fixed at Galactic value 2 = Power law with free absorption 3 = Broken power law with absorption fixed at Galactic value 4 = Continuously curved parabola with absorption fixed at Galactic value 5 = Broken power law with free absorption 6 = Continuously curved parabola with free absorption
Byte-by-byte Description of file: table3.dat
Bytes Format Units Label Explanations
1 A1 --- Type [HLF] Object type (G1) 3- 19 A17 --- Name Source Name 21- 30 A10 "DD/MM/YYYY" Date Observation Date 32- 35 F4.2 --- Gamma ? Photon spectral index (intrinsic absorption fixed to the Galactic value) (G2) 37- 40 F4.2 --- E_Gamma ? Upper Error on Gamma 42- 45 F4.2 --- e_Gamma ? Lower Error on Gamma 47- 50 F4.2 --- Chi2 ? Reduced Chi Squared 52- 54 I3 --- DOF ? Degrees of Freedom 56- 59 F4.1 10+20cm-2 NH ? Intrinsic absorption 61- 64 F4.1 10+20cm-2 E_NH ? Upper Error on NH 66- 69 F4.1 10+20cm-2 e_NH ? Lower Error on NH 71- 74 F4.2 --- Gammaf ? Photon spectral index (intrinsic absorption free to vary) 76- 79 F4.2 --- E_Gammaf ? Upper Error on Gammaf 81- 84 F4.2 --- e_Gammaf ? Lower Error on Gammaf 86- 89 F4.2 --- Chi2f ? Reduced Chi Squared 91- 93 I3 --- DOFf ? Degrees of Freedom 95- 99 F5.1 10-15W/m2 F3-9keV X-ray unabsorbed flux in 3-9keV energy range
Byte-by-byte Description of file: table4.dat
Bytes Format Units Label Explanations
1 A1 --- Type [HLF] Object type (G1) 3- 19 A17 --- Name Source Name 21- 30 A10 "DD/MM/YYYY" Date Observation Date 32- 35 F4.2 --- Chi2 ? Reduced Chi Squared (broken power law or the continuously curved parabola model with intrinsic absorption fixed to the Galactic value) 37- 39 I3 --- DOF ? Degrees of Freedom 41- 44 F4.2 --- Gamma1 ? First Photon spectral index (G2) 46- 49 F4.2 --- E_Gamma1 ? Upper Error on Gamma1 51- 54 F4.2 --- e_Gamma1 ? Lower Error on Gamma1 56- 59 F4.2 keV EBreak ? Energy break 61- 65 F5.2 keV E_EBreak ? Upper Error on EBreak 67- 70 F4.2 keV e_EBreak ? Lower Error on EBreak 72- 75 F4.2 --- Gamma2 ? Second Photon spectral index (G2) 77- 80 F4.2 --- E_Gamma2 ? Upper Error on Gamma2 82- 85 F4.2 --- e_Gamma2 ? Lower Error on Gamma2 87- 90 F4.2 --- Chi2f ? Reduced Chi Squared (broken power law or the continuously curved parabola model with intrinsic absorption free to vary) 92- 94 I3 --- DOFf ? Degrees of Freedom 96- 99 F4.1 10+20cm-2 NH ? Intrinsic absorption 101-103 F3.1 10+20cm-2 E_NH ? Upper Error on NH 105-107 F3.1 10+20cm-2 e_NH ? Lower Error on NH 109-112 F4.2 --- Gamma1f ? First Photon spectral index (G2) 114-117 F4.2 --- E_Gamma1f ? Upper Error on Gamma1f 119-122 F4.2 --- e_Gamma1f ? Lower Error on Gamma1f 124-127 F4.2 keV EBreakf ? Energy break 129-132 F4.2 keV E_EBreakf ? Upper Error on EBreakf 134-137 F4.2 keV e_EBreakf ? Lower Error on EBreakf 139-142 F4.2 --- Gamma2f ? Second Photon spectral index (G2) 144-147 F4.2 --- E_Gamma2f ? Upper Error on Gamma2f 149-152 F4.2 --- e_Gamma2f ? Lower Error on Gamma2f 154-158 F5.1 10-15W/m2 F4-8keV X-ray unabsorbed flux in the energy range 4-8keV
Byte-by-byte Description of file: table5.dat
Bytes Format Units Label Explanations
1 A1 --- Type [HLF] Object type (G1) 3- 19 A17 --- Name Source Name 21- 30 A10 "DD/MM/YYYY" Date Observation Date 32- 35 F4.2 --- Chi1p Reduced Chi Squared (single power law model) 37- 39 I3 --- DOF1p Degrees of Freedom 41- 45 F5.1 10+20cm-2 NH1p ? Intrinsic absorption 47- 51 F5.1 10+20cm-2 E_NH1p ? Upper Error on NH 53- 56 F4.1 10+20cm-2 e_NH1p ? Lower Error on NH 58- 61 F4.2 --- Gamma1p Photon spectral index (G2) 63- 66 F4.2 --- E_Gamma1p Upper Error on Gamma 68- 71 F4.2 --- e_Gamma1p Lower Error on Gamma
Global notes: Note (G1): Type of objects as follows: H = High-energy peaked BL Lacs L = Low-energy peaked BL Lacs F = Flat Spectrum Radio Quasars Note (G2): Photon index Gamma defined as F(nu)∝nu-(Gamma-1)
Acknowledgements: Davide Donato, davide(at)physics.gmu.edu
(End) Patricia Vannier [CDS] 20-Apr-2005
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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