English
Related papers

Related papers: Polarimetric and spectroscopic optical observation…

200 papers

We present the first X-ray polarimetric study of the dipping accreting neutron star 4U 1624$-$49 with the Imaging X-ray Polarimetry Explorer (IXPE). We report a detection of polarization in the non-dip time intervals with a confidence level…

High Energy Astrophysical Phenomena · Physics 2024-01-29 M. Lynne Saade , Philip Kaaret , Andrea Gnarini , Juri Poutanen , Francesco Ursini , Stefano Bianchi , Anna Bobrikova , Fabio La Monaca , Alessandro Di Marco , Fiamma Capitanio , Alexandra Veledina , Ivan Agudo , Lucio A. Antonelli , Matteo Bachetti , Luca Baldini , Wayne H. Baumgartner , Ronaldo Bellazzini , Stephen D. Bongiorno , Raffaella Bonino , Alessandro Brez , Niccolo Bucciantini , Simone Castellano , Elisabetta Cavazzuti , Chien-Ting Chen , Stefano Ciprini , Enrico Costa , Alessandra De Rosa , Ettore Del Monte , Laura Di Gesù , Niccolo Di Lalla , Immacolata Donnarumma , Victor Doroshenko , Michal Dovciak , Steven R. Ehlert , Teruaki Emote , Yuri Evangelista , Sergio Fabiani , Riccardo Ferrazzoli , Javier A. Garcia , Shuichi Gunji , Kiyoshi Hayashida , Jeremy Heyl , Wataru Iwakiri , Svetlana G. Jorstad , Vladimir Karas , Fabian Kislat , Takao Kitaguchi , Jeffery J. Kolodziejczak , Henric Krawczynski , Luca Latronico , Ioannis Liodakis , Simone Maldera , Alberto Manfreda , Frederic Marin , Andrea Marinucci , Alan P. Marscher , Herman L. Marshall , Francesco Massaro , Giorgio Matt , Ikuyuki Mitsuishi , Tsunefumi Mizudo , Fabio Muleri , 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 , Pierre-Oliver Petrucci , Maura Pilia , Andrea Possenti , Simonetta Puccetti , Brian D. Ramsey , John Rankin , Ajay Ratheesh , Oliver J. Roberts , Roger W. Romani , Carmelo Sgro , Patrick Slane , Paolo Soffitta , Gloria Spandre , Douglas Z. Zwartz , Toru Tamagawa , Fabrizio Tavecchio , Roberto Taverna , Yuzuru Tawara , Allyn F. Tenant , Nicholas E. Thomas , Francesco Tombesi , Alessio Trois , Sergey S. Tsygankov , Roberto Turolla , Jacco Vink , Martin C. Weisskopf , Kinwah Wu , Fei Xie , Silvia Zane

We observed the anomalous X-ray pulsar 4U 0142+61 using the Proportional Counter Array (PCA) aboard the Rossi X-ray Timing Explorer (RXTE) in March 1996. The pulse frequency was measured as f = 0.11510039(3) Hz with an upper limit of df/dt…

4U 1820-30 is a ultracompact X-ray binary located in the globular cluster NGC 6624, consisting of a neutron star accreting material from a helium white dwarf companion characterized by the shortest known orbital period for this type of star…

High Energy Astrophysical Phenomena · Physics 2025-04-04 A. Anitra , A. Gnarini , T. Di Salvo , R. Iaria , A. Sanna , L. Burderi , A. Marino , M. Del Santo , G. Matt , F. Ursini , S. Bianchi , F. Capitanio , S. Fabiani , A. Tarana , A. Di Marco

We report on optical imaging of the X-ray binary SAX J1808.4-3658 with the 8-m Gemini South Telescope. The binary, containing an accretion-powered millisecond pulsar, appears to have a large periodic modulation in its quiescent optical…

Astrophysics · Physics 2011-02-11 Zhongxiang Wang , Cees Bassa , Andrew Cumming , Victoria M. Kaspi

The X-ray burster 4U1850-087, located in the Galactic globular cluster NGC6712, is an ultracompact binary (orbital period~21 min),likely harbouring a degenerate companion.The source has been observed at soft gamma-rays several times with…

Astrophysics · Physics 2009-11-11 L. Sidoli , A. Paizis , A. Bazzano , S. Mereghetti

Ultra-compact X-ray binaries consist of a neutron star or black hole that accretes material from a white dwarf-donor star. The ultra-compact nature is expressed in very short orbital periods of less than 1 hour. In the case of 4U 0614+091…

High Energy Astrophysical Phenomena · Physics 2015-05-19 O. K. Madej , P. G. Jonker , A. C. Fabian , C. Pinto , F. Verbunt , J. de Plaa

We observed the ultra-compact binary candidate 4U 0614+091 for a total of 200 ksec with the high-energy transmission gratings onboard the \chandra X-ray Observatory. The source is found at various intensity levels with spectral variations…

High Energy Astrophysical Phenomena · Physics 2015-05-18 Norbert S. Schulz , Michael P. Nowak , Deepto Chakrabarty , Claude R. Canizares

We present the first optical polarimetric study of the two transitional pulsars PSR J1023+0038 and XSS J12270-4859. This work is focused on the search for intrinsical linear polarisation (LP) in the optical emission from the two systems. We…

Solar and Stellar Astrophysics · Physics 2016-06-22 M. C. Baglio , P. D'Avanzo , S. Campana , F. Coti Zelati , S. Covino , D. M. Russell

We report the results of quasi-simultaneous optical and NIR photometry of the low-mass X-ray binary, 4U 1957+115. Our observations cover B, V, R, I, J, H and K-bands and additional time-series NIR photometry. We measure a spectral energy…

High Energy Astrophysical Phenomena · Physics 2015-06-22 Pasi Hakala , Panu Muhli , Phil Charles

We report results from long-term (approximately 1240 days) X-ray (0.3-8.0 keV) monitoring of the ultraluminous X-ray source NGC 5408 X-1 with the Swift/X-Ray Telescope. Here we expand on earlier work by Strohmayer (2009) who used only a…

High Energy Astrophysical Phenomena · Physics 2013-08-09 Dheeraj R. Pasham , Tod E. Strohmayer

We report here results from detailed timing and spectral studies of the high mass X-ray binary pulsar 4U~1538--52 over several binary periods using observations made with the Rossi X-ray Timing Explorer (RXTE) and BeppoSAX satellites. Pulse…

Astrophysics · Physics 2007-05-23 U. Mukherjee , H. Raichur , B. Paul , S. Naik , N. Bhatt

In this study, we examine 51 archival NICER observations and 6 archival NuSTAR observations of the neutron star (NS) ultra-compact X-ray binary (UCXB) 4U 0614+091, which span over 5 years. The source displays persistent reflection features,…

High Energy Astrophysical Phenomena · Physics 2024-09-17 David L. Moutard , Renee M. Ludlam , Edward M. Cackett , Javier A. García , Jon M. Miller , Dan R. Wilkins

We report the detection of a long X-ray burst triggered on MJD 60171.65 from the ultra-compact binary 4U 1850$-$087 by the Monitor of All-sky X-ray Image and Neutron Star Interior Composition Explorer (NICER). We analyse the NICER data…

High Energy Astrophysical Phenomena · Physics 2024-07-31 Yongqi Lu , Zhaosheng Li , Wenhui Yu , Yuanyue Pan , Maurizio Falanga

We report on X-ray and radio observations of the ultra-compact X-ray binary 4U 1543-624 taken in August 2017 during an enhanced accretion episode. We obtained NICER monitoring of the source over a $\sim10$ day period during which…

On 2025 January 10, a thermonuclear (Type I) X-ray burst from the neutron star low-mass X-ray binary \textit{4U~0614+091} was detected with the ECLAIRs instrument on board the \textit{SVOM} mission. We present here a time-resolved…

We report on a pair of X-ray Multi-Mirror Mission (XMM-Newton) observations of the Supergiant X-ray binary 4U 1909+07, which were performed on 2021 October 3 and 2021 October 8, respectively. We measure the neutron star rotation period in…

We observed the neutron star (NS) ultra-compact X-ray binary 4U0614+091 quasi-simultaneously in the radio band (VLA), mid-IR/IR (Spitzer/MIPS and IRAC), near-IR/optical (SMARTS), optical-UV (Swift/UVOT), soft and hard X-rays (Swift/XRT and…

High Energy Astrophysical Phenomena · Physics 2014-11-20 S. Migliari , J. A. Tomsick , J. C. A. Miller-Jones , S. Heinz , R. I. Hynes , R. P. Fender , E. Gallo , P. G. Jonker , T. J. Maccarone

We present a comprehensive spectro-polarimetric and timing analysis of twelve black hole X-ray binaries, namely Cyg X-1, 4U 1630-47, Cyg X-3, LMC X-1, 4U 1957+115, LMC X-3, Swift J1727.8-1613, GX 339-4, Swift J151857.0-572147, IGR…

High Energy Astrophysical Phenomena · Physics 2025-11-07 Seshadri Majumder , Ankur Kushwaha , Swapnil Singh , Kiran M. Jayasurya , Santabrata Das , Anuj Nandi

We present timing and broad-band spectral studies of the high mass X-ray binary pulsar 4U 1909+07 using data from Suzaku observation during 2010 November 2-3. The pulse period of the pulsar is estimated to be 604.11+/-0.14 s. Pulsations are…

High Energy Astrophysical Phenomena · Physics 2016-02-16 Gaurava K. Jaisawal , Sachindra Naik , Biswajit Paul

We analyse \emph{INTEGRAL} (between 2005 October and 2007 November) and \emph{RXTE} (between 2007 June and 2011 March) observations of the accretion powered pulsar 4U 1907+09. From \emph{INTEGRAL} IBIS-ISGRI and \emph{RXTE}-PCA…

High Energy Astrophysical Phenomena · Physics 2015-05-28 S. Sahiner , S. C. Inam , A. Baykal