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Results from the All-Sky Monitor (ASM) on the Rossi X-ray Timing Explorer are reviewed. A number of recurrent transient sources have been detected, while only a few previously unreported sources have been discovered. The ASM light curves…

Astrophysics · Physics 2009-10-30 Alan M. Levine

We present light curves of a sample of "transient" sources observed with the All-Sky Monitor (ASM) of the Rossi X-ray Timing Explorer (RXTE). The light curves extend over 3.5 years. They are presented in three groups: six neutron-star…

Astrophysics · Physics 2007-05-23 Hale Bradt , Alan M. Levine , Ronald A. Remillard , Donald A. Smith

The lack of unambiguous detections of atomic features in the X-ray spectra of ultraluminous X-ray sources (ULXs) has proven a hindrance in diagnosing the nature of the accretion flow. The possible association of spectral residuals at soft…

High Energy Astrophysical Phenomena · Physics 2015-10-28 Matthew J. Middleton , Dominic J. Walton , Andrew Fabian , Timothy P. Roberts , Lucy Heil , Ciro Pinto , Gemma Anderson , Andrew Sutton

We have obtained spectral and timing data on GX 3+1 and Ser X-1. Both sources were observed simultaneously with BeppoSAX and RXTE. The RXTE data is used to provide power spectra and colour-colour diagrams in order to constrain the state…

Astrophysics · Physics 2009-10-31 T. Oosterbroek , D. Barret , M. Guainazzi , E. C. Ford

Cyg X-3 is an unusual X-ray binary which shows remarkable correlative behavior between the hard X-ray, soft X-ray, and the radio. We present an analysis of these long term light curves in the context of spectral changes of the system. This…

We present Rossi X-ray Timing Explorer, monitoring observations of the Seyfert 2 galaxy Markarian 3 spanning a 200 day period during which time the source flux varied by a factor $\sim 2$ in the 4-20 keV bandpass. In broad agreement with…

We present a systematic analysis of the X-ray spectra of NGC 1313 X-1 and NGC 1313 X-2, using six years of XMM-Newton observations (17 observations). We fitted the continuum with a Comptonization model plus a multicolor blackbody disc, that…

High Energy Astrophysical Phenomena · Physics 2015-05-20 Fabio Pintore , Luca Zampieri

The RXTE All Sky Monitor provides a public database that includes more than one year of X-ray monitoring observations (2-12 keV) of X-ray binaries and a few active galactic nuclei. The instrument operates with a 40% duty cycle, and the…

Astrophysics · Physics 2009-09-25 Ronald A. Remillard , Alan M. Levine

We studied a time history of X-ray spectral states of a black-hole candidate, 4U 1630-47, utilizing data from a number of monitoring observations with the Rossi X-Ray Timing Explorer over 1996--2004. These observations covered five…

Astrophysics · Physics 2015-06-24 Yukiko Abe , Yasushi Fukazawa , Aya Kubota , Daisuke Kasama , Kazuo Makishima

We study the coherence of the near-infrared and X-ray background fluctuations and the X-ray spectral properties of the sources producing it. We use data from multiple Spitzer and Chandra surveys, including the UDS/SXDF surveys, the Hubble…

Astrophysics of Galaxies · Physics 2019-10-02 Yanxia Li , Nico Cappelluti , Günther Hasinger , Richard G. Arendt , Alexander Kashlinsky , Fabio Pacucci

AGILE data on Cygnus X-3 are reviewed focussing on the correlation between the production of gamma-ray transient emission and spectral state changes of the source. AGILE clearly establishes a relation between enhanced gamma-ray emission and…

High Energy Astrophysical Phenomena · Physics 2019-08-15 G. Piano , A. Bulgarelli , M. Tavani , V. Vittorini , M. McCollough , G. Pooley , S. Trushkin

Suzaku observation of an ultraluminous X-ray source, NGC 2403 Source 3, performed on 2006 March 16--17, is reported. The Suzaku XIS spectrum of Source 3 was described with a multi-color black-body-like emission from an optically thick…

We report on the average and orbital phase-resolved polarization of Cyg X-3 in the hard state during the 2023 Imaging X-ray Polarimetry Explorer (IXPE) observational campaign. We find the polarization degree of $ 21.2 \pm 0.4 \% $ and…

High Energy Astrophysical Phenomena · Physics 2025-12-16 Romana Mikušincová , Alexandra Veledina , Fabio Muleri , Raul Ciancarella , Andrzej Zdziarski , David A. Green , Michael McCollough , Henric Krawczynski , James F. Steiner , Michal Dovčiak , Varpu Ahlberg , Stefano Bianchi , Alessandro Di Marco , Javier A. García , Adam Ingram , Philip Kaaret , Timothy Kallman , Hu Kun , Fabio La Monaca , Alexander Lange , Vladislav Loktev , Guglielmo Mastroserio , Giorgio Matt , Razieh Emami , Pierre-Olivier Petrucci , Jakub Podgorný , Juri Poutanen , Ajay Ratheesh , Nicole Rodriguez , Jiří Svoboda , Francesco Tombesi , Francesco Ursini , Iván Agudo , Lucio A. Antonelli , Matteo Bachetti , Luca Baldini , Wayne H. Baumgartner , Ronaldo Bellazzini , Stephen D. Bongiorno , Raffaella Bonino , Alessandro Brez , Niccolò Bucciantini , Fiamma Capitanio , Simone Castellano , Elisabetta Cavazzuti , Chien-Ting Chen , Stefano Ciprini , Enrico Costa , Alessandra De Rosa , Ettore Del Monte , Laura Di Gesu , Niccolò Di Lalla , Immacolata Donnarumma , Victor Doroshenko , Steven R. Ehlert , Teruaki Enoto , Yuri Evangelista , Sergio Fabiani , Riccardo Ferrazzoli , Shuichi Gunji , Kiyoshi Hayashida , Jeremy Heyl , Wataru Iwakiri , Svetlana G. Jorstad , Vladimir Karas , Fabian Kislat , Takao Kitaguchi , Jeffery J. Kolodziejczak , Luca Latronico , Ioannis Liodakis , Simone Maldera , Alberto Manfreda , Frédéric Marin , Andrea Marinucci , Alan P. Marscher , Herman L. Marshall , Francesco Massaro , Ikuyuki Mitsuishi , Tsunefumi Mizuno , Michela Negro , Chi-Yung Ng , Stephen L. O'Dell , Nicola Omodei , Chiara Oppedisano , Alessandro Papitto , George G. Pavlov , Abel L. Peirson , Matteo Perri , Melissa Pesce-Rollins , Maura Pilia , Andrea Possenti , Simonetta Puccetti , Brian D. Ramsey , John Rankin , Oliver J. Roberts , Roger W. Romani , Carmelo Sgrò , Patrick Slane , Paolo Soffitta , Gloria Spandre , Douglas A. Swartz , Toru Tamagawa , Fabrizio Tavecchio , Roberto Taverna , Yuzuru Tawara , Allyn F. Tennant , Nicholas E. Thomas , Alessio Trois , Sergey S. Tsygankov , Roberto Turolla , Jacco Vink , Martin C. Weisskopf , Kinwah Wu , Fei Xie , Silvia Zane

X-ray binaries are known to exhibit different spectral states which are often associated with different black hole accretion modes. The exact geometry and properties of these accretion modes is still uncertain. Recent IXPE measurements of…

High Energy Astrophysical Phenomena · Physics 2024-04-05 Monika Moscibrodzka

RXTE ASM count rates from the X-ray pulsar Her X-1 began falling consistently during the late months of 2003. The source is undergoing another state transition similar to the anomalous low state of 1999. This new event has triggered…

Astrophysics · Physics 2009-11-10 M. Still , P. Boyd

Extragalactic black hole X-ray binaries LMC X-1 and LMC X-3 are the persistent sources, usually found in soft spectral state. We present the results from spectral and timing study of these sources using MAXI, NICER, NuSTAR and AstroSat…

High Energy Astrophysical Phenomena · Physics 2022-04-27 Bhuvana G. R. , Radhika D. , Anuj Nandi

We study the soft X-ray variability of Cygnus X-3. By combining data from the All-Sky Monitor and Proportional Counter Array instruments on the RXTE satellite with EXOSAT Medium Energy (ME) detector observations, we are able to analyse the…

High Energy Astrophysical Phenomena · Physics 2009-11-13 Magnus Axelsson , Stefan Larsson , Linnea Hjalmarsdotter

Highlights from the RXTE All Sky Monitor (ASM) during 1996 and 1997 are reviewed with particular attention to X-ray transients. The ASM has detected 117 sources. These include 12 recurrent transients and 10 new X-ray sources, some of which…

Astrophysics · Physics 2009-09-25 R. A. Remillard

We present broadband X-ray spectral analysis of the black hole X-ray binary MAXI J1348--630, performed using five AstroSat observations. The source was in the soft spectral state for the first three and in the hard state for the last two…

High Energy Astrophysical Phenomena · Physics 2023-01-18 Gitika Mall , Jithesh Vadakkumthani , Ranjeev Misra

We present an investigation of the X-ray properties of 13 LINERs based on ROSAT all-sky survey and pointed PSPC and HRI observations. Several sources are studied for the first time in X-rays. The X-ray spectra are best described by a…

Astrophysics · Physics 2007-05-23 Stefanie Komossa , Hans Boehringer , John P. Huchra