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Related papers: Radio pulse search from Aql X-1

200 papers

Using the Parkes radio telescope, we have searched for pulsed radio emission from the recently discovered X-ray pulsars AX J1811.5-1926 and PSR J0537-6910 in the supernova remnants G11.2-0.3 and N157B, respectively. We detected no…

Astrophysics · Physics 2007-05-23 F. Crawford , V. M. Kaspi , R. N. Manchester , F. Camilo , A. G. Lyne , N. D'Amico

We report on simultaneous X-ray and radio observations of the mode-switching pulsar PSR B0943+10 obtained with the XMM-Newton satellite and the LOFAR, LWA and Arecibo radio telescopes in November 2014. We confirm the synchronous X-ray/radio…

We report on optical and NIR observations obtained during and after the 2004 December discovery outburst of the X-ray transient and accretion-powered millisecond pulsar IGR J00291+5934. Our observations monitored the evolution of the…

We report on the discovery of X-ray pulsations from the Be/X-ray system LS 992/RX J0812.4-3114 during an RXTE observation. From a timing analysis of the source we obtained a barycentric pulse period of 31.8851 \pm 0.0004 s. The pulse…

Astrophysics · Physics 2009-10-31 Pablo Reig , Paul Roche

We report on the discovery of polarized X-ray emission from an accreting millisecond pulsar. During a 10-day-long coverage of the February 2024 outburst of SRGA J144459.2-604207, the Imaging X-ray Polarimetry Explorer (IXPE) detected an…

We report on a series of Swift/XRT observations, performed between February and 22 March 2012, during the quiescent state of the neutron-star X-ray binary SAX J1750.8-2900. In these observations, the source was either just detected or…

High Energy Astrophysical Phenomena · Physics 2015-06-15 Rudy Wijnands , Nathalie Degenaar

The rapidly oscillating Ap (roAp) star 10 Aql shows one of the lowest photometric pulsation amplitudes and is characterized by an unusual spectroscopic pulsational behavior compared to other roAp stars. More than 1000 spectra were taken…

Astrophysics · Physics 2009-11-13 M. Sachkov , O. Kochukhov , T. Ryabchikova , D. Huber , F. Leone , S. Bagnulo , W. W. Weiss

We studied spectra for 34 accretion-powered X-ray and one millisecond pulsars that were within the field of view of the INTEGRAL observatory over two years (December 2002 - January 2005) of its in-orbit operation and that were detected by…

Astrophysics · Physics 2007-05-23 E. V. Filippova , S. S. Tsygankov , A. A. Lutovinov , R. A. Sunyaev

PSR J1023+0038 is the first millisecond pulsar discovered to pulsate in the visible band; such a detection took place when the pulsar was surrounded by an accretion disk and also showed X-ray pulsations. We report on the first high time…

We report on NuSTAR observations of transient pulsations in the neutron star X-ray binary SMC X-1. The transition from non-pulsing to pulsing states was not accompanied by a large change in flux. Instead, both pulsing and non-pulsing states…

We report on an XMM-Newton observation of the accreting millisecond pulsar, IGR J17511-3057. Pulsations at 244.8339512(1) Hz are observed with an RMS pulsed fraction of 14.4(3)%. A precise solution for the P_orb=12487.51(2)s binary system…

High Energy Astrophysical Phenomena · Physics 2015-05-19 A. Papitto , A. Riggio , T. Di Salvo , L. Burderi , A. D'Aì , R. Iaria , E. Bozzo , M. T. Menna

IGR J17591--2342, a transient accretion-powered millisecond X-ray pulsar, was discovered during its 2018 outburst. Here, we present a timing and spectral analysis of the source using {\it AstroSat} data of the same outburst. From the timing…

High Energy Astrophysical Phenomena · Physics 2024-12-17 Akshay Singh , Andrea Sanna , Sudip Bhattacharyya , Sudiip Chakraborty , Sarita Jangle , Tlak Katoch , H. M. Antia , Nitinkumar Bijewar

We report on optical and X-ray observations of the accretion powered ms pulsar IGR J00291+5934 in quiescence. Time resolved I-band photometry has been obtained with the 4.2 m William Herschel Telescope, while a 3 ks Chandra observation…

Astrophysics · Physics 2008-02-19 P. G. Jonker , M. A. P. Torres , D. Steeghs

We report on the serendipitous X-ray detection, using the Chandra X-ray Observatory, of the radio pulsar J1718-3718. This pulsar has one of the highest inferred surface dipole magnetic fields in the radio pulsar population (B = 7.4e13 G),…

Astrophysics · Physics 2009-11-10 V. M. Kaspi , M. A. McLaughlin

We report X-ray imaging, timing, and spectral studies of XTE J1810-197, a 5.54s pulsar discovered by Ibrahim et al. (2003) in recent RXTE observations. In a set of short exposures with the Chandra HRC camera we detect a strongly modulated…

Astrophysics · Physics 2009-11-10 E. V. Gotthelf , J. P. Halpern , M. Buxton , C. Bailyn

Aql X--1 is one of the most prolific low mass X-ray binary transients (LMXBTs) showing outbursts almost annually. We present the results of our spectral analyses of RXTE/PCA observations of the 2000 and the 2011 outbursts. We investigate…

High Energy Astrophysical Phenomena · Physics 2017-10-09 Can Güngör , Kazım Yavuz Ekşi , Ersin Göğüş , Tolga Güver

We report on timing, flux density, and polarimetric observations of the transient magnetar and 5.54 s radio pulsar XTE J1810-197 using the GBT, Nancay, and Parkes radio telescopes beginning in early 2006, until its sudden disappearance as a…

Solar and Stellar Astrophysics · Physics 2016-04-13 F. Camilo , S. M. Ransom , J. P. Halpern , J. A. J. Alford , I. Cognard , J. E. Reynolds , S. Johnston , J. Sarkissian , W. van Straten

We present RXTE monitoring of the eclipsing X-ray binary Hercules X-1 conducted over the short-high state of July 1998. This was one of the last major short-high states before the source entered an anomalous low-state of activity. A…

The Fermi Large Area Telescope has detected over 260 gamma-ray pulsars. About one quarter of these are labeled as radio-quiet. In the population of nonrecycled gamma-ray pulsars, the fraction of radio-quiet pulsars is higher, about one…

High Energy Astrophysical Phenomena · Physics 2021-10-13 J. -M. Grießmeier , D. A. Smith , G. Theureau , T. J. Johnson , M. Kerr , L. Bondonneau , I. Cognard , M. Serylak

New radio (MeerKAT and Parkes) and X-ray (XMM-Newton, Swift, Chandra, and NuSTAR) observations of PSR J1622-4950 indicate that the magnetar, in a quiescent state since at least early 2015, reactivated between 2017 March 19 and April 5. The…

High Energy Astrophysical Phenomena · Physics 2018-04-06 F. Camilo , P. Scholz , M. Serylak , S. Buchner , M. Merryfield , V. M. Kaspi , R. F. Archibald , M. Bailes , A. Jameson , W. van Straten , J. Sarkissian , J. E. Reynolds , S. Johnston , G. Hobbs , T. D. Abbott , R. M. Adam , G. B. Adams , T. Alberts , R. Andreas , K. M. B. Asad , D. E. Baker , T. Baloyi , E. F. Bauermeister , T. Baxana , T. G. H. Bennett , G. Bernardi , D. Booisen , R. S. Booth , D. H. Botha , L. Boyana , L. R. S. Brederode , J. P. Burger , T. Cheetham , J. Conradie , J. P. Conradie , D. B. Davidson , G. de Bruin , B. de Swardt , C. de Villiers , D. I. L. de Villiers , M. S. de Villiers , W. de Villiers , C. de Waal , M. A. Dikgale , G. du Toit , L. J. du Toit , S. W. P. Esterhuyse , B. Fanaroff , S. Fataar , A. R. Foley , G. Foster , D. Fourie , R. Gamatham , T. Gatsi , R. Geschke , S. Goedhart , T. L. Grobler , S. C. Gumede , M. J. Hlakola , A. Hokwana , D. H. Hoorn , D. Horn , J. Horrell , B. Hugo , A. Isaacson , O. Jacobs , J. P. Jansen van Rensburg , J. L. Jonas , B. Jordaan , A. Joubert , F. Joubert , G. I. G. Jozsa , R. Julie , C. C. Julius , F. Kapp , A. Karastergiou , F. Karels , M. Kariseb , R. Karuppusamy , V. Kasper , E. C. Knox-Davies , D. Koch , P. P. A. Kotze , A. Krebs , N. Kriek , H. Kriel , T. Kusel , S. Lamoor , R. Lehmensiek , D. Liebenberg , I. Liebenberg , R. T. Lord , B. Lunsky , N. Mabombo , T. Macdonald , P. Macfarlane , K. Madisa , L. Mafhungo , L. G. Magnus , C. Magozore , O. Mahgoub , J. P. L. Main , S. Makhathini , J. A. Malan , P. Malgas , J. R. Manley , M. Manzini , L. Marais , N. Marais , S. J. Marais , M. Maree , A. Martens , S. D. Matshawule , N. Matthysen , T. Mauch , L. D. Mc Nally , B. Merry , R. P. Millenaar , C. Mjikelo , N. Mkhabela , N. Mnyandu , I. T. Moeng , O. J. Mokone , T. E. Monama , K. Montshiwa , V. Moss , M. Mphego , W. New , B. Ngcebetsha , K. Ngoasheng , H. Niehaus , P. Ntuli , A. Nzama , F. Obies , M. Obrocka , M. T. Ockards , C. Olyn , N. Oozeer , A. J. Otto , Y. Padayachee , S. Passmoor , A. A. Patel , S. Paula , A. Peens-Hough , B. Pholoholo , P. Prozesky , S. Rakoma , A. J. T. Ramaila , I. Rammala , Z. R. Ramudzuli , M. Rasivhaga , S. Ratcliffe , H. C. Reader , R. Renil , L. Richter , A. Robyntjies , D. Rosekrans , A. Rust , S. Salie , N. Sambu , C. T. G. Schollar , L. Schwardt , S. Seranyane , G. Sethosa , C. Sharpe , R. Siebrits , S. K. Sirothia , M. J. Slabber , O. Smirnov , S. Smith , L. Sofeya , N. Songqumase , R. Spann , B. Stappers , D. Steyn , T. J. Steyn , R. Strong , A. Struthers , C. Stuart , P. Sunnylall , P. S. Swart , B. Taljaard , C. Tasse , G. Taylor , I. P. Theron , V. Thondikulam , K. Thorat , A. Tiplady , O. Toruvanda , J. van Aardt , T. van Balla , L. van den Heever , A. van der Byl , C. van der Merwe , P. van der Merwe , P. C. van Niekerk , R. van Rooyen , J. P. van Staden , V. van Tonder , R. van Wyk , I. Wait , A. L. Walker , B. Wallace , M. Welz , L. P. Williams , B. Xaia , N. Young , S. Zitha
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