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We report results of RXTE observations of PSR B1951+32 using the PCA instrument for 19k seconds during 1996 March 24th. We applied the contemporaneous radio ephemeris and various statistical tests to search for evidence of pulsation. These…

Astrophysics · Physics 2016-08-30 Hsiang-Kuang Chang , Cheng Ho

We report on the first X-ray observation of the 0.28 s isolated radio pulsar PSR J1154--6250 obtained with the XMM-Newton observatory in February 2018. A point-like source is firmly detected at a position consistent with that of PSR…

In 2003, the magnetar XTE J1810-197 started an outburst that lasted until early 2007. In the following 11 years, the source stayed in a quiescent/low activity phase. XTE J1810-197 is one of the closest magnetars, hence its X-ray properties…

High Energy Astrophysical Phenomena · Physics 2018-12-19 Fabio Pintore , Sandro Mereghetti , Paolo Esposito , Roberto Turolla , Andrea Tiengo , Nanda Rea , Federico Bernardini , Gian Luca Israel

Context. In 1998 the first accreting millisecond pulsar, SAX J1808.4-3658, was discovered and to date 18 systems showing coherent, high frequency (> 100 Hz) pulsations in low mass X-ray binaries are known. Since their discovery, this class…

High Energy Astrophysical Phenomena · Physics 2017-07-18 A. Marino , T. Di Salvo , A. F. Gambino , R. Iaria , L. Burderi , M. Matranga , A. Sanna , A. Riggio

We report the first detection of pulsed X-ray emission from the young, energetic radio and Gamma-ray pulsar PSR B1706-44. We find a periodic signal at a frequency of f = 9.7588088 +/- 0.0000026 Hz (at epoch 51585.34104 MJD), consistent with…

Astrophysics · Physics 2009-11-07 E. V. Gotthelf , J. P. Halpern , R. Dodson

I review the properties of three X-ray accreting millisecond pulsars observed with INTEGRAL. Out of seven recently discovered accretion-powered pulsars (one discovered by INTEGRAL), three were observed with the INTEGRAL satellite up to 300…

Astrophysics · Physics 2007-11-07 Maurizio Falanga

We report the discovery of millisecond oscillations in the X-ray emission from the X-ray transient SAX J1750.8-2900. Millisecond quasiperiodic oscillations (kHz QPOs) were present in the persistent emission with frequencies ranging from 543…

Astrophysics · Physics 2009-11-07 P. Kaaret , J. J. M. in 't Zand , J. Heise , J. A. Tomsick

The TRAPUM collaboration has used the MeerKAT telescope to conduct a search for pulsed radio emission from the young Small Magellanic Cloud pulsar J0058-7218 located in the supernova remnant IKT 16, following its discovery in X-rays with…

In this work, the temporal and spectral properties of the poorly studied X-ray pulsar Swift J1808.4$-$1754 were investigated in the 0.8-79 keV energy range based on the data from the NuSTAR and Swift observatories collected during the 2014…

High Energy Astrophysical Phenomena · Physics 2022-06-08 Alexander Salganik , Sergey S. Tsygankov , Alexander A. Lutovinov , Anlaug A. Djupvik , Dmitri I. Karasev , Sergey V. Molkov

We report on the timing analysis of the 2015 outburst of the intermittent accreting millisecond X-ray pulsar SAX J1748.9-2021 observed on March 4 by the X-ray satellite XMM-Newton. By phase-connecting the time of arrivals of the observed…

High Energy Astrophysical Phenomena · Physics 2016-04-20 A. Sanna , L. Burderi , A. Riggio , F. Pintore , T. Di Salvo , A. F. Gambino , R. Iaria , M. Matranga , F. Scarano

We present the search methods and initial results for transient radio signals in the High Time Resolution Universe (HTRU) Survey. The HTRU survey's single-pulse search, the software designed to perform the search, and a determination of the…

Using observations made with the XMM-Newton Observatory, we report the probable X-ray detection of the high-magnetic-field radio pulsar PSR J1734-3333. This pulsar has an inferred surface dipole magnetic field of B = 5.2e13 G, just below…

High Energy Astrophysical Phenomena · Physics 2010-12-16 S. A. Olausen , V. M. Kaspi , A. G. Lyne , M. Kramer

We observed four southern AXPs in 1999 near 1400 MHz with the Parkes 64-m radio telescope to search for periodic radio emission. No Fourier candidates were discovered in the initial analysis, but the recent radio activity observed for the…

Astrophysics · Physics 2008-11-26 F. Crawford , J. W. T. Hessels , V. M. Kaspi

Vela X-1 is a well-studied accreting X-ray pulsar, with a distinctive pulse profile that has been found to be very similar in different observations spread out over decades. On the other hand, significant variations down to the timescale of…

A new pulsar, 1SAX J1452.8-5949, was discovered during a BeppoSAX galactic plane survey on 1999 July 20 at R.A.=14h 52m 49s, Dec=-59 49' 18'' (J2000) with a 90% confidence uncertainty radius of 50''. Coherent pulsations were detected with a…

We describe a systematic search for X-ray counterparts of radio pulsars. The search was accomplished by cross-correlating the radio timing positions of all radio pulsars from the ATNF pulsar database (version 1.54) with archival XMM-Newton…

High Energy Astrophysical Phenomena · Physics 2016-08-05 Tobias Prinz , Werner Becker

We present the first broadband spectral and timing study of the Be/X-ray pulsar XTE J0111.2$-$7317 (SXP31.0) during the first major outburst since its discovery in 1998. This giant type II outburst, observed between April and September…

We present the results of the observations of the giant bursts from the X-ray pu lsar A0535+26 made by HEXE onboard Mir-Kvant in April 1989, November 1993 and February 1994. The pulse periods were measured, pulse profiles in different…

SAX J1748.9-2021 is a transient accretion powered millisecond X-ray pulsar located in the Globular cluster NGC 6440. We report on the spectral and timing analysis of SAX J1748.9-2021 performed on AstroSat data taken during its faint and…

High Energy Astrophysical Phenomena · Physics 2020-01-22 Rahul Sharma , Aru Beri , Andrea Sanna , Anjan Dutta

A new pulsating X-ray source, AX J183220-0840, with a 1549.1-s period was discovered at R.A.= 18h32m20s and Dec.=-8d40'30'' (J2000, uncertainty=0.6degree) during an ASCA observation on the Galactic plane. The source was observed two times,…

Astrophysics · Physics 2009-10-31 M. Sugizaki , K. Kinugasa , K. Matsuzaki , Y. Terada , S. Yamauchi , J. Yokogawa