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Related papers: New BeppoSAX-WFC results on superbursts

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In an ongoing effort to search for X-ray transients on diverse time scales in the data archive of the BeppoSAX Wide Field Cameras we have identified four GRBs that are long (between 540 and at least 2550 s) and faint (with 3 events having…

An X-ray flaring source was found near the galaxy NGC 4697. Two flares were seen, separated by four years. The flux increased by a factor of 90 on a timescale of about one minute. Both flares were very brief. There is no optical counterpart…

We report the first-time detection of a type-I X-ray burst from a position that is consistent with that of 1RXS J171824.2-402934. The detection was made on Sep 23, 1996, with the Wide Field Cameras on board the BeppoSAX satellite. The burst…

Astrophysics · Physics 2007-05-23 R. G. Kaptein , J. J. M. in 't Zand , E. Kuulkers , F. Verbunt , J. Heise , R. Cornelisse

We report on 4 BeppoSAX Target Of Opportunity observations of MXB 1730-335, the Rapid Burster (RB), made during the 1998 February-March outburst. In the first observation, approximately 20 days after the outburst peak, the X-ray light curve…

During the operational life of the Italian/Dutch X-ray satellite (1996-2002), BeppoSAX, its two Wide Field Cameras performed observations that covered the full sky at different epochs. Although the majority of analysis performed on BeppoSAX…

High Energy Astrophysical Phenomena · Physics 2015-05-28 F. Capitanio , A. J. Bird , M. Fiocchi , S. Scaringi , P. Ubertini

We present deep 2.2 micron imaging of twelve gamma-ray burst host galaxies. Template spectral energy distributions are fit to the multiband photometry between visible and near-infrared wavelengths to derive a better constraint on the…

Astrophysics · Physics 2016-08-30 R. Chary , E. E. Becklin , L. Armus

The positions of over 1000 gamma-ray bursts detected with the BATSE experiment on board of the Compton Gamma Ray Observatory are uniformly and randomly distributed in the sky, with no significant concentration to the galactic plane or to…

Astrophysics · Physics 2016-08-30 Bohdan Paczynski

Starting in 1999, the Rossi X-ray Timing Explorer (RXTE) has monitored the central bulge region of the Galaxy with the Proportional Counter Array (PCA), resolving about 50 binary X-ray sources, including 18 sources discovered by RXTE and…

Astrophysics · Physics 2007-05-23 J. Swank , C. Markwardt

Dusty galaxies with luminosities in excess of 10^11 solar luminosities have been detected out to redshifts of about unity by the Infrared Space Observatory (ISO), and to higher redshifts using millimetre(mm)- and submm-wave cameras on…

Astrophysics · Physics 2007-05-23 Andrew W. Blain

We present the main results of a study of spectral and energetics properties of twelve gamma-ray bursts (GRBs) with redshift estimates. All GRBs in our sample were detected by BeppoSAX in a broad energy range (2-700 keV). From the redshift…

The transient X-ray source GS 1826-238 was monitored during five different observing periods between August 1996 and October 1998 with the BeppoSAX Wide Field Camera instrument in the framework of a deep observation of the Galactic Center…

Astrophysics · Physics 2009-10-31 P. Ubertini , A. Bazzano , M. Cocchi , L. Natalucci , J. Heise , J. M. Muller , J. J. M. in 't Zand

We report the discovery with BeppoSAX-WFC of two new X-ray sources that were only seen during bursts: SAX J1753.5-2349 and SAX J1806.5-2215. For both sources, no steady emission was detected above an upper limit of 5 mCrab (2 to 8 keV) for…

Astrophysics · Physics 2009-10-30 J. J. M. in 't Zand , J. Heise , J. M. Muller , A. Bazzano , M. Cocchi , L. Natalucci , P. Ubertini

Time resolved X-ray spectroscopy of thermonuclear bursts observed from low mass X-ray binaries offer a unique tool to measure neutron star masses and radii. In this paper, we continue our systematic analysis of all the X-ray bursts observed…

High Energy Astrophysical Phenomena · Physics 2012-02-22 Tolga Guver , Feryal Ozel , Dimitrios Psaltis

Luminous X-ray outbursts with variability amplitudes as high as ~1000 have been detected from a small number of galactic nuclei. These events are likely associated with transient fueling of nuclear supermassive black holes. In this paper,…

Astrophysics · Physics 2009-11-13 B. Luo , W. N. Brandt , A. T. Steffen , F. E. Bauer

We report the analysis of the first superburst from a transiently accreting neutron star system with the All-Sky Monitor (ASM) on the Rossi X-ray Timing Explorer. The superburst occurred 55 days after the onset of an accretion outburst in…

Astrophysics · Physics 2009-11-13 L. Keek , J. J. M. in 't Zand , E. Kuulkers , A. Cumming , E. F. Brown , M. Suzuki

Two type I X-ray bursts were detected from a position consistent with the transient X-ray source in NGC 6652 with the Wide Field Camera of the BeppoSAX satellite, strongly suggesting that this transient is a neutron star. Our detection…

We report results of the first search specifically targeting short-timescale X-ray flares from low-mass X-ray binaries in an early-type galaxy. A new method for flare detection is presented. In NGC 4697, the nearest, optically luminous,…

Astrophysics · Physics 2009-11-10 Gregory R. Sivakoff , Craig L. Sarazin , Andres Jordan

We present the complete on-line catalogue of gamma-ray bursts observed by the two Wide Field Cameras on board \sax in the period 1996-2002. Our aim is to provide the community with the largest published data set of GRB's prompt emission…

Astrophysics · Physics 2009-11-13 L. Vetere , P. Soffitta , E. Massaro , P. Giommi , E. Costa

INTEGRAL detected on August 31, 2004, an unusual thermonuclear X-ray burst from the low-mass X-ray binary GX 3+1. Its duration was 30 min, which is between the normal burst durations for this source (<~10 s) and the superburst observed in…

We present an overview of our Supergiant Fast X-ray Transients (SFXT) project, that started in 2007, by highlighting the unique observational contribution Swift is giving to this exciting new field. By means of outburst detection with…

High Energy Astrophysical Phenomena · Physics 2011-04-01 P. Romano , S. Vercellone , V. La Parola , G. Cusumano , V. Mangano , P. Esposito , J. A. Kennea , D. N. Burrows , H. A. Krimm , C. Pagani , N. Gehrels