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Related papers: A new redback pulsar candidate 4FGL J2054.2+6904

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We report our detailed data analysis for 39 $\gamma$-ray sources selected from the 992 unassociated sources in the \textit{Fermi} Large Area Telescope (LAT) third source catalog. The selection criteria, which were set for finding candidate…

High Energy Astrophysical Phenomena · Physics 2021-06-03 Xuejie Dai , Zhongxiang Wang , V. Jithesh , Yi Xing

We present X-ray, ultraviolet, and optical observations of 1RXS J154439.4-112820, the most probable counterpart of the unassociated Fermi LAT source 3FGL J1544.6-1125. The optical data reveal rapid variability, which is a feature of…

High Energy Astrophysical Phenomena · Physics 2015-06-24 Slavko Bogdanov , Jules P. Halpern

The Large Area Telescope (LAT) onboard the Fermi satellite opened a new era for pulsar astronomy, detecting gamma-ray pulsations from more than 60 pulsars, ~40% of which are not seen at radio wavelengths. One of the most interesting sources…

High Energy Astrophysical Phenomena · Physics 2015-05-27 A. De Luca , M. Marelli , R. P. Mignani , P. A. Caraveo , W. Hummel , S. Collins , A. Shearer , P. M. Saz Parkinson , A. Belfiore , G. F. Bignami

PSR J1744-3922 is a binary pulsar exhibiting highly variable pulsed radio emission. We report on a statistical multi-frequency study of the pulsed radio flux variability which suggests that this phenomenon is extrinsic to the pulsar and…

We present optical observations of the redback millisecond pulsar PSR J1048+2339, which is a 4.66 ms radio pulsar in a compact binary with an orbital period of six hours. We obtained high-quality light curves of PSR J1048+2339 with the…

High Energy Astrophysical Phenomena · Physics 2019-01-16 Yee Xuan Yap , K. L. Li , A. K. H. Kong , J. Takata , J. Lee , C. Y. Hui

A large number of new "black widow" and "redback" energetic millisecond pulsars with irradiated stellar companions have been discovered through radio and optical searches of unidentified \textit{Fermi} sources. Synchrotron emission, from…

High Energy Astrophysical Phenomena · Physics 2016-02-23 Zorawar Wadiasingh , Alice K. Harding , Christo Venter , Markus Boettcher

We present the first optical spectroscopy of five confirmed (or strong candidate) redback millisecond pulsar binaries, obtaining complete radial velocity curves for each companion star. The properties of these millisecond pulsar binaries…

We have used deep V and R images acquired at the ESO Very Large Telescope to identify the optical companion to the binary pulsar PSR J0610-2100, one of the black-widow millisecond pulsars recently detected by the Fermi Gamma-ray Telescope…

Solar and Stellar Astrophysics · Physics 2015-06-05 C. Pallanca , R. P. Mignani , E. Dalessandro , F. R. Ferraro , B. Lanzoni , A. Possenti , M. Burgay , E. Sabbi

We present multiwavelength observations of the persistent Fermi-LAT unidentified gamma-ray source 1FGL J1417.7-4407, showing it is likely to be associated with a newly discovered X-ray binary containing a massive neutron star (nearly 2…

In the 4FGL-DR4 point-source catalog of the Large Area Telescope (LAT) onboard NASA's Fermi Gamma-ray Observatory (Fermi-LAT), around a third of the sources are still unidentified (unIDs). In this work, we perform a detailed study of one of…

Since the launch of the Fermi satellite, the number of known gamma-ray pulsars has increased tenfold. Most gamma-ray detected pulsars are young and energetic, and many are associated with TeV sources. PSR J1357-6429 is a high spin-down…

Time-domain analysis of an archival XMM-Newton observation unveiled a very unusual variability pattern in the soft X-ray emission of PSR J1311-3430, a black widow millisecond pulsar in a tight binary (P_B=93.8 min) with a very low-mass…

High Energy Astrophysical Phenomena · Physics 2022-11-16 Andrea De Luca , Martino Marelli , Sandro Mereghetti , Ruben Salvaterra , Roberto Mignani , Andrea Belfiore

PSR J0205+6449 is a young ({\approx} 5400 years), Crab-like pulsar detected in radio and at X and {\gamma}-ray energies and has the third largest spin-down flux among known rotation powered pulsars. It also powers a bright synchrotron…

High Energy Astrophysical Phenomena · Physics 2015-06-16 P. Moran , R. P. Mignani , S. Collins , A. de Luca , N. Rea , A. Shearer

The latest source catalog of the Fermi-LAT telescope contains more than 7000 $\gamma$-ray sources at GeV energies, with the two dominant source classes thought to be blazars and rotation-powered pulsars. Our target is the identification of…

High Energy Astrophysical Phenomena · Physics 2024-02-09 Martin G. F. Mayer , Werner Becker

We report the results of a high-energy multi-instrumental campaign with INTEGRAL, RXTE, and Swift of the recently discovered INTEGRAL source IGR J19294+1816. The Swift/XRT data allow us to refine the position of the source to RA= 19h 29m…

High Energy Astrophysical Phenomena · Physics 2015-05-14 J. Rodriguez , J. A. Tomsick , A. Bodaghee , J. -A. Zurita Heras , S. Chaty , A. Paizis , S. Corbel

Because of the disappearance of its accretion disk since the time period around 2012 November--December, XSS J12270-4859 has recently been identified as, in addition to PSR J1023+0038, another transitional millisecond pulsar binary. We have…

High Energy Astrophysical Phenomena · Physics 2015-08-06 Yi Xing , Zhongxiang Wang

PSR J2215+5135 (J2215) is a `redback' spider pulsar, where the intrabinary shock (IBS) wraps around the pulsar rather than the stellar-mass companion. Spider orbital light curves are modulated, dominated by their binary companion thermal…

High Energy Astrophysical Phenomena · Physics 2024-09-05 Andrew G. Sullivan , Roger W. Romani

We report the discovery of eight gamma-ray pulsars in blind frequency searches using the LAT, onboard the Fermi Gamma-ray Space Telescope. Five of the eight pulsars are young (tau_c<100 kyr), energetic (Edot>10^36 erg/s), and located within…

Sixteen pulsars have been discovered so far in blind searches of photons collected with the Large Area Telescope on the Fermi Gamma-ray Space Telescope. We here report the discovery of radio pulsations from two of them. PSR J1741-2054, with…

We have presented the first joint {\it XMM-Newton} and {\it NuSTAR} analysis of the millisecond pulsar (MSP) binary PSR J1653$-$0158. The 75-minute orbital period inferred from optical and gamma-ray observations together with the 1.97-ms…

High Energy Astrophysical Phenomena · Physics 2022-06-14 Jane SiNan Long , Albert K. H. kong , Kinwah Wu , Jumpei Takata , Qin Han , David C. Y. Hui , Kwan Lok Li