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J/ApJ/649/L9     INTEGRAL IBIS census of the sky beyond 100keV  (Bazzano+, 2006)

INTEGRAL IBIS census of the sky beyond 100 keV. Bazzano A., Stephen J.B., Fiocchi M., Bird A.J., Bassani L., Dean A.J., Malizia A., Ubertini P., Lebrun F., Walter R., Winkler C. <Astrophys. J., 649, L9-L12 (2006)> =2006ApJ...649L...9B
ADC_Keywords: Surveys ; Gamma rays Mission_Name: INTEGRAL Keywords: galaxies: active - gamma rays: observations - surveys Abstract: We report on the first census of INTEGRAL IBIS detections (≳4σ significance) above 100keV based on the Core Program and public open-time observations up to 2005 April. There are 49 sources detected in the 100-150keV band, of which 14 are also seen in the 150-300keV range. The low-energy sample is dominated by X-ray binary systems of both low and high mass but also includes 10 active galaxies. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 103 49 IBIS detections in (100-150)keV and (150-300)keV energy bands refs.dat 185 23 References types.dat 48 40 Source types (from Bird et al. 2007, J/ApJS/170/175)
See also: J/ApJS/170/175 : Third IBIS/ISGRI soft gamma-ray survey catalog (Bird+, 2007) Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 14 A14 --- Name Source name (1) 16- 26 A11 --- Type Bird et al. (2006, Cat. J/ApJ/636/765) classification of source 28- 34 F7.2 --- S(20-40)I IBIS 20-40keV flux in mCrabs (1) 36- 39 F4.2 --- e_S(20-40)I Uncertainty in S(20-40)I 41- 46 F6.1 --- S(40-100)I IBIS 40-100keV flux in mCrabs (1) 48- 50 F3.1 --- e_S(40-100)I Uncertainty in S(40-100)I 52- 57 F6.1 --- S(100-150)I IBIS 100-150keV flux in mCrabs (1) 59- 61 F3.1 --- e_S(100-150)I Uncertainty in S(100-150)I 63- 66 I4 --- S(150-300)I ? IBIS 150-300keV flux in mCrabs (1) 68 I1 --- e_S(150-300)I ? Uncertainty in IBIS S(150-300)I 70- 75 F6.1 --- S(100-150)B ? Beppo-Sax 100-150keV flux in mCrabs (1) 77- 79 F3.1 --- E_S(100-150)B ? Upper limit uncertainty in S(100-150)B 81- 83 F3.1 --- e_S(100-150)B ? Lower limit uncertainty in S(100-150)B 85 A1 --- Mo [a-c] Model flag on the Beppo-Sax data (2) 87- 92 F6.1 --- S(150-200)B ? Beppo-Sax 150-200keV flux in mCrabs (1) 94- 96 F3.1 --- E_S(150-200)B ? Upper limit uncertainty in S(150-200)B 98-100 F3.1 --- e_S(150-200)B ? Lower limit uncertainty in S(150-200)B 102-103 I2 --- r_Name ? Reference, in refs.dat file
Note (1): Only sources detected with signal to noise >4 are reported. 1mCrab=3.2E-12erg/cm2/s (3.2fW/m2) in the 100-150keV range and 1mCrab=4.8E-12erg/cm2/s (4.8fW/m2) in the 150-300keV range. Note (2): Model flag as follows: a = simple power law b = cut-off power law c = broken power law
Byte-by-byte Description of file: refs.dat
Bytes Format Units Label Explanations
1- 2 I2 --- Ref Reference code 4- 22 A19 --- BibCode BibCode 24- 43 A20 --- Aut Author's name 45-185 A141 --- Com Comments
Byte-by-byte Description of file: types.dat
Bytes Format Units Label Explanations
1- 9 A9 --- Type Source type 11- 48 A38 --- Def Definition
History: From electronic version of the journal
(End) Greg Schwarz [AAS], Patricia Vannier [CDS] 18-Jul-2008
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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