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PSR J1119-6127 is a radio pulsar that behaved magnetar like bursts, and we performed a comprehensive investigation of this pulsar using the archival high-energy observations obtained after its outburst in 2016 July. After the 2016 outburst,…

High Energy Astrophysical Phenomena · Physics 2018-10-17 Lupin Chun-Che Lin , Hui-Hui Wang , Kwan-Lok Li , Jumpei Takata , Chin-Ping Hu , C. -Y. Ng , C. Y. Hui , A. K. H. Kong , Pak-Hin T. Tam , Paul K. H. Yeung

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…

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

We present the results of an XMM-Newton observation of the radio-quiet X-ray pulsar 1E 1207-5209 located at the center of the shell-like supernova remnant G296.5+10.0. The X-ray spectrum is characterized by the presence of two…

Astrophysics · Physics 2009-11-07 S. Mereghetti , A. De Luca , P. A. Caraveo , W. Becker , R. Mignani , G. F. Bignami

We have searched 92 unidentified sources from the FIRST and NVSS radio catalogs for pulsations at 610 MHz. The selected sources are bright, have no identifications, are unresolved and have significant linear polarization. Our search was…

Astrophysics · Physics 2007-05-23 F. Crawford , V. M. Kaspi , J. F. Bell

We report on observations of the unusual neutron-star binary system FIRST J102347.6+003841 carried out using the XMM-Newton satellite. This system consists of a radio millisecond pulsar in an 0.198-day orbit with a ~0.2 solar-mass…

We report on X-ray monitoring of two isolated pulsars within the same RXTE field of view. PSR J1811-1925 in the young supernova remnant G11.2-0.3 has a nearly sinusoidal pulse profile with a hard pulsed spectrum (photon index \~1.2). The…

RX J1856.5-3754 is one of the brightest, nearby isolated neutron stars, and considerable observational resources have been devoted to its study. In previous work, we found that our latest models of a magnetic, hydrogen atmosphere matches…

Astrophysics · Physics 2009-11-13 Wynn C. G. Ho

During a search for coherent signals in the X-ray archival data of XMM-Newton, we discovered a modulation at 1.2 s in 3XMM J004301.4+413017 (3X J0043), a source lying in the direction of an external arm of M 31. This short period indicates…

Swift J1749.4-2807 is a transient neutron star low-mass X-ray binary that contains an accreting millisecond X-ray pulsar spinning at 518 Hz. It is the first of its kind that displays X-ray eclipses, which holds significant promise to…

High Energy Astrophysical Phenomena · Physics 2015-06-04 N. Degenaar , A. Patruno , R. Wijnands

The study of high-magnetic-field pulsars is important for examining the relationships between radio pulsars, magnetars, and X-ray-isolated neutron stars (XINSs). Here we report on X-ray observations of three such high-magnetic-field radio…

High Energy Astrophysical Phenomena · Physics 2013-09-18 S. A. Olausen , W. W. Zhu , J. K. Vogel , V. M. Kaspi , A. G. Lyne , C. M. Espinoza , B. W. Stappers , R. N. Manchester , M. A. McLaughlin

We report on the discovery of coherent pulsations at a period of 2.9 ms from the X-ray transient MAXI J0911-655 in the globular cluster NGC 2808. We observed X-ray pulsations at a frequency of $\sim339.97$ Hz in three different observations…

High Energy Astrophysical Phenomena · Physics 2017-02-01 A. Sanna , A. Papitto , L. Burderi , E. Bozzo , A. Riggio , T. Di Salvo , C. Ferrigno , N. Rea , R. Iaria

MAXI J181-195 is a newly discovered accreting millisecond X-ray pulsar that went outburst in June 2022. Through timing analysis with NICER and NuSTAR observations, we find a transient modulation at ~2.5 Hz during the decay period of MAXI…

High Energy Astrophysical Phenomena · Physics 2023-08-09 P. P. Li , L. Tao , L. Zhang , Q. C. Bu , J. L. Qu , L. Ji , P. J. Wang , Y. P. Chen , S. Zhang , R. C. Ma , Z. X. Yang , W. T. Ye , S. J. Zhao , Q. C. Zhao , Y. Huang , X. Ma , E. L. Qiao , S. M. Jia , S. N. Zhang

This study reports pulse variation analysis results for the forth discovered accretion-powered millisecond pulsar XTE J1807-294 during its 2003 outburst observed by {\it Rossi X-ray Timing Explorer}. The pulsation is significantly detected…

Astrophysics · Physics 2009-11-13 Y. Chou , Y. Chung , C. P. Hu , T. C. Yang

We have used the Green Bank Telescope to measure HI absorption against the anomalous X-ray pulsar XTE J1810-197. Assuming a flat rotation curve, we find that XTE J1810-197 is located at a distance of 3.4(+0.5,-0.7) kpc. For a rotation curve…

We report the discovery by the RXTE PCA of a second transient accreting millisecond pulsar, XTE J1751-305, during regular monitoring observations of the galactic bulge region. The pulsar has a spin frequency of 435 Hz, making it one of the…

We report the detection of 376.05 Hz (2.66 ms) coherent X-ray pulsations in NICER observations of a transient outburst of the low-mass X-ray binary IGR J17494-3030 in 2020 October/November. The system is an accreting millisecond X-ray…

MAXI J1816-195 is a newly discovered accreting millisecond pulsar with prolific thermonuclear bursts, detected during its outburst in 2022 June by Insight-HXMT and NICER. During the outburst, Insight-HXMT detected 73 bursts in its peak and…

High Energy Astrophysical Phenomena · Physics 2025-02-24 Yu-Peng Chen , Shu Zhang , Long Ji , Shuang-Nan Zhang , Peng-Ju Wang , Ling-Da Kong , Zhi Chang , Jing-Qiang Peng , Qing-Cang Shui , Jian Li , Lian Tao , Ming-Yu Ge , Jin-Lu Qu

The search for radio emission from the gamma pulsar J0357+3205 in the meter wavelength range was carried out. Periodic emission was found in one of the 1,700 observation sessions. The average pulsar profile is single-component with a…

High Energy Astrophysical Phenomena · Physics 2022-04-18 S. A. Tyul'bashev , M. A. Kitaeva

We report the discovery of a 38.5 ms X-ray pulsar in observations of the soft gamma-ray source IGR J18490-0000 with the Rossi X-ray Timing Explorer (RXTE). PSR J1849-0001 is spinning down rapidly with period derivative 1.42E-14 s/s,…

High Energy Astrophysical Phenomena · Physics 2015-05-20 E. V. Gotthelf , J. P. Halpern , R. Terrier , F. Mattana