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1841. http://hea.iki.rssi.ru/integral06/papers/I05_Hanlon01-25Jan07_18:09:56.pdf
... й %Ф ? ? P? й ? ї ф Ё в? Ў jї ? SWIFT 15 q? Number of GRBs 20 30 35 40 4800 5000 5200 counts per bin counts per bin 5400 5600 5800 6000 6200 10000 11000 12000 6000 7000 counts per bin counts per bin 8000 9000 4000 -10 5000 INTEGRAL b? 0 -1.5 -1 0 -0.5 Log GRB Peak Flux (ph/cm2/s) зЄ є З З ?Н є н н к В f В У і к tШ Ш к В ? л У ? н З їк ? wл ? ? Ь aМ і & o }z j o qp | ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/I05_Hanlon01-25Jan07_18:09:56.pdf -- 386.4 Кб -- 25.01.2007
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1842. http://hea.iki.rssi.ru/integral06/papers/B34_Schanne03-23Jan07_09:40:00_bandw.pdf
TYPE Ia SUPERNOVA RATE IN THE GALACTIC CENTER REGION StИphane Schanne (1) (2) (1,*) , Michel CassИ (1,2) , Patrick Sizun(1), Bertrand Cordier(1), Jacques Paul( 1) CEA-Saclay, DAPNIA ... Paris, France (*) corresponding author: schanne{at}hep.saclay.cea.fr ABSTRACT According to recent analyses of the type-Ia supernova rate as a function of redshift, delayed and prompt typeIa supernovae (SN Ia) should explode respectively in the Galactic bulge and in the ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/B34_Schanne03-23Jan07_09:40:00_bandw.pdf -- 234.9 Кб -- 24.01.2007
[ Текст ] Ссылки http://hea.iki.rssi.ru/integral06/papers/B34_Schanne03-23Jan07_09:40:00_color.pdf -- 234.9 Кб -- 24.01.2007
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[ Текст ] Ссылки http://hea.iki.rssi.ru/integral06/papers/B34_Schanne03-23Jan07_09:40:00_color.pdf -- 234.9 Кб -- 24.01.2007
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1843. http://hea.iki.rssi.ru/integral06/papers/G39_Filippova01-23Jan07_14:14:00.pdf
... List of X-ray pulsars detected with INTEGRAL and their best-fit spectral parameters Name A 0114+650 SMC X-1 RX J0146.9+6121 V0332+53 4U 0352+309 LMC X-4 A 0535+26 Vela X-1(eclipse) Vela X-1(outside eclipse) CEN X-3(quiescent state ) CEN X-3(outbursts) 4U 1145-619 1E 1145.1-614 GX 301-2 (high state ) GX 301-2 (low state ) 2RXP130159.6-635806 4U 1538-52 4U 1626-67 IGR/AX J16320-4752 IGR J16358-4726 IGR J16465-4507 OAO 1657-415 EXO 1722-363 GX 1+4 ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/G39_Filippova01-23Jan07_14:14:00.pdf -- 273.5 Кб -- 23.01.2007
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1844. http://hea.iki.rssi.ru/integral06/papers/C02_Revnivtsev01-22Jan07_17:13:38.pdf
... t? x ge f gW ` s vS hс hWЭ pf ?Н E? W T w v` Л Pw я ?e } gW e v hd f v gw ` 1e e ` tb gW z ?e ve 5b W s te c} ` pw v w xe s 3 $s v` s c g f gd Yf ?s w a d e g W v b d 5 Y} b 1e de !b ?w ?w W e s j Ce лe Ys v d c v zr ge f s $ ?s gw z gW пw ae ` n # W zr ?w e W g |w e c} P? 9В cВ cs cb s vЕ pS ? ... Dwarf novae i di di ai i p di vЧ Ч ? ... vВ GRXE spectrum of unit stellar mass Е ? ... Polars Active stars (RS CVns) Energy, keV Luminosity, 1027 erg/sec/ Intermediate polars ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/C02_Revnivtsev01-22Jan07_17:13:38.pdf -- 739.4 Кб -- 22.01.2007
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1845. http://hea.iki.rssi.ru/integral06/papers/D01_Bassani01-22Jan07_16:19:17.pdf
INTEGRAL/IBIS 20-100 KEV EXTRAGALACTIC SURVEY: AN UPDATE L. Bassani, A. Malizia and J.B. Stephen On behalf of the INTEGRAL AGNs survey team IASF-Bologna/INAF, via P. Gobetti 101, 40129 Bologna, Italy ABSTRACT Analysis of INTEGRAL Core Program and public Open Time observations has recently provided a sample of 60 extragalactic sources selected in the 20-100 keV band above a flux of 1.5 10-11 erg cm-2 s-1 . ... Figure 2. ... Column density versus 20-100 keV luminosity for AGNs in the present sample 4. ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/D01_Bassani01-22Jan07_16:19:17.pdf -- 235.4 Кб -- 22.01.2007
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1846. http://hea.iki.rssi.ru/integral06/papers/G06_Tsygankov01-22Jan07_11:45:59.pdf
PULSE PROFILES AND CYCLOTRON LINE ENERGY DEPENDENCE ON X-RAY PULSARS LUMINOSITY S. Tsygankov, A. Lutovinov, E. Churazov, and R. Sunyaev Space Research Institute, Profsoyuznaya str. ... CYCLOTRON LINE ENERGY 2.1. ... We concentrate on the luminosity and energy dependence of the pulse profile and the variations of the cyclotron line energy. In V0332+53 the line energy changes nearly linearly with the source luminosity, while in 4U0115+63 its behavior is more complicated. ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/G06_Tsygankov01-22Jan07_11:45:59.pdf -- 864.1 Кб -- 22.01.2007
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1847. http://hea.iki.rssi.ru/integral06/papers/I09_Kazanas01-19Jan07_22:27:55.pdf
THE SUPERCRITICAL PILE GRB MODEL : AFTERGLOWS AND GRB , XRR, XRF UNIFICATION Demosthenes Kazanas1 , Apostolos Mastichiadis2 , and Markos Georganopoulos Astrophysics Science Division, ... MD 21250 2 1 1,3 3 ABSTRACT We present the general notions and observational consequences of the Supercritical Pile GRB model ; the fundamental feature of this model is a detailed process for the conversion of the energy stored in relativistic ... The dissipation of the RBW kinetic energy. ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/I09_Kazanas01-19Jan07_22:27:55.pdf -- 153.3 Кб -- 19.01.2007
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1848. http://hea.iki.rssi.ru/integral06/papers/D02_Beckmann01-19Jan07_20:50:38.pdf
THE HARD X-RAY LUMINOSITY FUNCTION OF INTEGRAL DETECTED AGN V. Beckmann1 , C. R. Shrader1 , N. Gehrels1 , S. Soldi2 , and N. Produit 1 2 NASA Goddard Space Flight Center, Astrophysics Science Division, Code 661, Greenbelt, MD 20771, USA 2 Є INTEGRAL Science Data Centre, Chemin d' Ecogia 16, 1290 Versoix, Switzerland ABSTRACT We have compiled a complete extragalactic sample based on 25, 000 deg2 to a limiting flux of 3 в 10-11 ergs cm-2 ... NUMBER-FLUX DISTRIBUTION OF INTEGRAL AGN 3.1. ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/D02_Beckmann01-19Jan07_20:50:38.pdf -- 156.2 Кб -- 19.01.2007
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1849. http://hea.iki.rssi.ru/integral06/papers/B33_Schanne02-12Jan07_15:38:00_color.pdf
EVIDENCE FOR 1809 keV GAMMA-RAY EMISSION FROM 26Al DECAYS IN THE VELA REGION WITH INTEGRAL/ SPI StИphane Schanne(1,*), Patrick Sizun(1), David Maurin(1), Bertrand Cordier(1), Andreas von Kienlin(2), Clarisse Hamadache (1) (2 ... -Institut fЭr extraterrestrische Physik, D-85740 Garching, Germany (*) corresponding author: schanne{at}hep.saclay.cea.fr ABSTRACT The Vela ... SPI Single Events spectrum 26Al Fig. ... 34 5 6 Fig 2. SPI background in the 26Al signal region. ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/B33_Schanne02-12Jan07_15:38:00_color.pdf -- 402.9 Кб -- 19.01.2007
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1850. http://hea.iki.rssi.ru/integral06/papers/B33_Schanne02-12Jan07_15:38:00_bandw.pdf
EVIDENCE FOR 1809 keV GAMMA-RAY EMISSION FROM 26Al DECAYS IN THE VELA REGION WITH INTEGRAL/ SPI StИphane Schanne(1,*), Patrick Sizun(1), David Maurin(1), Bertrand Cordier(1), Andreas von Kienlin(2), Clarisse Hamadache (1) (2 ... -Institut fЭr extraterrestrische Physik, D-85740 Garching, Germany (*) corresponding author: schanne{at}hep.saclay.cea.fr ABSTRACT The Vela ... SPI background in the 26Al signal region. ... 1995, A&A 298, L25, 1.809 MeV gammarays from the VELA region. ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/B33_Schanne02-12Jan07_15:38:00_bandw.pdf -- 407.8 Кб -- 19.01.2007
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1851. http://hea.iki.rssi.ru/integral06/papers/D30_Malizia01-19Jan07_18:12:36.pdf
SWIFT / XRT FOLLOW-UP OBSERVATIONS OF INTEGRAL AGNS R. Landi, A. Malizia, L. Bassani , N. Masetti, J.B. Stephen, F.Gianotti, F. Schiavone 1 , A. Bazzano, P. Ubertini 2 , A. J. Bird, A. J. Dean3 , and R. Walter4 IASF-INAF, Bologna, Italy 2 IASF- INAF, Roma, Italy 3 University of Southampton, Southampton, UK INTEGRAL Science Data Centre, Versoix, Switzerland 1 4 ABSTRACT In five years of operation, data from ... In this work we present X-ray data (0.2ґ10 keV) for a set of 8 identified with AGN. ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/D30_Malizia01-19Jan07_18:12:36.pdf -- 545.4 Кб -- 19.01.2007
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1852. http://hea.iki.rssi.ru/integral06/papers/F05_Takahashi01-14Jan07_20:06:21_bandw.pdf
... Background-subtracted wide-band (0.7ґ300 keV) energy spectra of GRO J1655-40, obtained with the XIS, HXD-PIN (green) and HXD-GSO (blue). ... Energy Spectra and High Energy Cutoff Figure 3 shows wide-band energy spectra of GRO J1655-40 from 0.7 keV to 300 keV, obtained with the XIS and HXD, by averaging all the data. ... The XIS spectra As a first-cut spectral study, we tried an absorbed single power-law model on the XIS data of GRO J1655-40, as suggested by the Crab ratio in figure 4. ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/F05_Takahashi01-14Jan07_20:06:21_bandw.pdf -- 360.9 Кб -- 18.01.2007
[ Текст ] Ссылки http://hea.iki.rssi.ru/integral06/papers/F05_Takahashi01-14Jan07_20:06:21_color.pdf -- 360.9 Кб -- 18.01.2007
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[ Текст ] Ссылки http://hea.iki.rssi.ru/integral06/papers/F05_Takahashi01-14Jan07_20:06:21_color.pdf -- 360.9 Кб -- 18.01.2007
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1853. http://hea.iki.rssi.ru/integral06/papers/G46_Schanne01-05Jan07_17:47:00_bandw.pdf
... Using data from ISGRI, SPI and JEM-X, we firmly confirm the existence of cyclotron resonant scattering features (CRSF) at ~27 keV and ~54 keV, implying a neutronstar magnetic field of 3в1012 Gauss, and the presence of an iron emission line at ~6.5 keV. ... SEARCH FOR SOURCES IN VELA REGION the full IBIS/I s in the Vela of the region most suited SGRI data region, by (Fig. 1) in for new set, we search for point constructing a mosaic the 18-60 keV energy source detection. The Fig. ... FC Fig. ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/G46_Schanne01-05Jan07_17:47:00_bandw.pdf -- 482.8 Кб -- 10.01.2007
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1854. http://hea.iki.rssi.ru/integral06/papers/G46_Schanne01-05Jan07_17:47:00_color.pdf
... Using data from ISGRI, SPI and JEM-X, we firmly confirm the existence of cyclotron resonant scattering features (CRSF) at ~27 keV and ~54 keV, implying a neutronstar magnetic field of 3в1012 Gauss, and the presence of an iron emission line at ~6.5 keV. ... SEARCH FOR SOURCES IN VELA REGION the full IBIS/I s in the Vela of the region most suited SGRI data region, by (Fig. 1) in for new set, we search for point constructing a mosaic the 18-60 keV energy source detection. The Fig. ... FC Fig. ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/G46_Schanne01-05Jan07_17:47:00_color.pdf -- 396.8 Кб -- 10.01.2007
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1855. http://hea.iki.rssi.ru/integral06/papers/F32_Caballero-Garcia01-03Jan07_13:18:18.pdf
... Key words: Gamma rays: observations; Black hole physics; Accretion, accretion disks. lower mass accretion rate, corresponding to several percent of the Eddington luminosity, a BHB usually enters the low-hard (LH) state and at very low accretion rates it reaches the quiescent state, which may be just an extreme of the LH state. ... OBSERVATIONS The data were obtained with INTEGRAL and cover the outburst using the instruments SPI, IBIS/ISGRI, JEM-X and OMC. ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/F32_Caballero-Garcia01-03Jan07_13:18:18.pdf -- 787.0 Кб -- 03.01.2007
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1856. http://hea.iki.rssi.ru/conf/hea2007/bbclone/images/ext_ext.txt
width:14 height:14 author:BBClone Team
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Ссылки http://hea.iki.rssi.ru/conf/hea2007/bbclone/images/ext_ext.txt -- 1.0 Кб -- 28.12.2006
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1857. http://hea.iki.rssi.ru/conf/hea2007/bbclone/images/ext2/ext.txt
width:16 height:11 author:Christoph Brill
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Ссылки http://hea.iki.rssi.ru/conf/hea2007/bbclone/images/ext2/ext.txt -- 1.0 Кб -- 28.12.2006
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1858. http://hea.iki.rssi.ru/conf/hea2007/bbclone/doc/options.txt
... The default value is pointing to the parent directory. ... Link to parent directory $BBC_MAINSITE = ""; => Show no link $BBC_SHOW_CONFIG BBClone defaults to revealing the stats' settings. ... BBC_LANGUAGE = "en"; $BBC_MAXTIME This variable defines the length of an unique visit in seconds. ... BBC_NO_HITS = ""; => Show hits in time stats $BBC_NO_HITS = 1; => Show unique visits in time stats $BBC_IGNORE_IP This option can be used to exclude particular IP addresses or address ranges from counting. ...
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Ссылки http://hea.iki.rssi.ru/conf/hea2007/bbclone/doc/options.txt -- 13.2 Кб -- 27.12.2006
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1859. http://hea.iki.rssi.ru/integral06/papers/I36_Marcinkowski02-25Dec06_16:20:29.pdf
... Ujazdowskie 4, PL-00-478 Warszawa, Poland 5 SAp CEA, Saclay, 91191 Gif sur Yvette, France 6 UMR 7164 11 Place M. Berthelot, 75231 Paris, France 7 MPE, Giessenbachstrasse, 85748 Garching, Germany 8 DA DPM&A, CIT, Pasadena, CA 91125, USA 2 7,8 4 ABSTRACT We present the first catalogue of the gamma-ray bursts (GRB) taking place outside of the INTEGRAL1 /IBIS field of view. ... IBIS/INTEGRAL data. Table 1 shows 28 localized offaxis GRBs detected by INTEGRAL between November 2002 and December 2004. ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/I36_Marcinkowski02-25Dec06_16:20:29.pdf -- 22.3 Кб -- 25.12.2006
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1860. http://hea.iki.rssi.ru/integral06/papers/G32_Fiocchi01-22Dec06_16:28:45.pdf
... Via Fosso del Cavaliere 100, Roma, I-00133, Italy ABSTRACT Recent INTEGRAL observations and archival BeppoSAX data have been analyzed to deeply investigate the hard X-ray behavior of the neutron star, atoll type, low mass X-ray Binary 4U 1636ґ53 . ... In fact, the source was detected in both the canonical high and low state and moreover in one occasion INTEGRAL spectrum shows, for first time in this source, a hard tail dominating the emission above 30 keV. ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/G32_Fiocchi01-22Dec06_16:28:45.pdf -- 325.0 Кб -- 22.12.2006
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