English
Related papers

Related papers: Fermi Variability Study of the Candidate Pulsar Bi…

200 papers

We present the results of precision gamma-ray timing measurements of the binary millisecond pulsar PSR J2339$-$0533, an irradiating system of "redback" type, using data from the Fermi Large Area Telescope. We describe an optimized analysis…

High Energy Astrophysical Phenomena · Physics 2015-06-30 Holger J. Pletsch , Colin J. Clark

The Fermi $\gamma$-ray source 1FGL J1417.7--4407 (J1417) is a compact X-ray binary with a neutron star primary and a red giant companion in a $\sim$5.4 day orbit. This initial conclusion, based on optical and X-ray data, was confirmed when…

Using the 100-m Effelsberg radio telescope operating at 1.36 GHz, we have performed a targeted radio pulsar survey of 289 unassociated gamma-ray sources discovered by the Large Area Telescope (LAT) aboard the Fermi satellite and published…

We report on a search for steep spectrum radio sources within the 95% confidence error ellipses of the Fermi unassociated sources from the Large Array Telescope (LAT). Using existing catalogs and the newly released GMRT all-sky survey at…

High Energy Astrophysical Phenomena · Physics 2016-07-27 D. A. Frail , K. P. Mooley , P. Jagannathan , H. T. Intema

The Fermi Gamma-ray Space Telescope has revolutionized our knowledge of the gamma-ray pulsar population, leading to the discovery of almost 100 gamma-ray pulsars and dozens of gamma-ray millisecond pulsars (MSPs). Although the outer-gap…

High Energy Astrophysical Phenomena · Physics 2015-06-03 A. K. H. Kong , R. H. H. Huang , K. S. Cheng , J. Takata , Y. Yatsu , C. C. Cheung , D. Donato , L. C. C. Lin , J. Kataoka , Y. Takahashi , K. Maeda , C. Y. Hui , P. H. T. Tam

We present an optical, X-ray, and $\gamma$-ray study of 1SXPS J042749.2-670434, an eclipsing X-ray binary which has an associated $\gamma$-ray counterpart, 4FGL J0427.8-6704. This association has led to the source being classified as a…

High Energy Astrophysical Phenomena · Physics 2020-04-22 M. R. Kennedy , R. P. Breton , C. J. Clark , V. S. Dhillon , M. Kerr , D. A. H. Buckley , S. B. Potter , D. Mata Sánchez , J. G. Stringer , T. R. Marsh

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 search for the counterpart to the Fermi-LAT source 3FGL J0838.8-2829, we performed a multi-wavelength campaign, in the X-ray band with Swift and XMM-Newton, performed infrared, optical (with OAGH, ESO-NTT and IAC80) and radio (ATCA)…

We report on the identification of the gamma-ray source 0FGL J20001.0+4352 listed in the Fermi bright source catalogue. This object, which has an observed 1-100 GeV flux of (7.8 +/- 1.2) x 10^{-9} ph cm^{-2} s^{-1} and is located close to…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-13 L. Bassani , R. Landi , N. Masetti , P. Parisi , A. Bazzano , P. Ubertini

Fermi J1544-0639/ASASSN-17gs/AT2017egv was identified as a gamma-ray/optical transient on May 15, 2017. Subsequent multiwavelength observations suggest that this source may belong to the new class of radio-weak BL Lacs. We studied the X-ray…

High Energy Astrophysical Phenomena · Physics 2019-02-06 F. Ursini , L. Bassani , F. Panessa , E. Pian , G. Bruni , A. Bazzano , N. Masetti , K. Sokolovsky , P. Ubertini

We consider the 1.5 years Fermi Large Area Telescope light curves (E > 100 MeV) of the flat spectrum radio quasars 3C 454.3 and PKS 1510-089, which show high activity in this period of time. We characterise the duty cycle of the source by…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-18 F. Tavecchio , G. Ghisellini , G. Bonnoli , G. Ghirlanda

This paper presents the gamma-ray spectral and timing results from the long-term regular observations of Mrk 421 with the Large Area Telescope (LAT) onboard Fermi during 2008 August - 2023 August. We discerned six periods the relatively…

High Energy Astrophysical Phenomena · Physics 2025-03-05 B. Kapanadze , A. Gurchumelia , M. Aller

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

We have discovered a new X-ray emitting compact binary that is the likely counterpart to the unassociated Fermi-LAT GeV $\gamma$-ray source 4FGL J1120.0-2204, the second brightest Fermi source that still remains formally unidentified. Using…

High Energy Astrophysical Phenomena · Physics 2022-03-02 Samuel J. Swihart , Jay Strader , Elias Aydi , Laura Chomiuk , Kristen C. Dage , Adam Kawash , Kirill V. Sokolovsky , Elizabeth C. Ferrara

SAX J0635.2+0533 is a binary pulsar with a very short pulsation period ($P$ = 33.8 ms) and a high long-term spin down ($\dot P$ $>$ 3.8$\times10^{-13}$ s s$^{-1}$), which suggests a rotation-powered (instead of an accretion-powered) nature…

High Energy Astrophysical Phenomena · Physics 2017-06-28 N. La Palombara , S. Mereghetti

In our recent investigation, we utilized a century's worth of archival optical data to search for a decade-long periodicity from the blazar PG 1553+113, finding a hint of a 22-yr period. Building on this foundation, the current study…

High Energy Astrophysical Phenomena · Physics 2025-06-03 Sagar Adhikari , Pablo Peñil , Alberto Domínguez , Marco Ajello , Sara Buson , Alba Rico

The detection of periodicities in light curves of active galacticnuclei (AGN) could have profound consequences for our understanding of the nature and radiation physics of these objects. At high energies (HE; E>100 MeV) 5 blazars (PG…

High Energy Astrophysical Phenomena · Physics 2020-02-26 F. Ait Benkhali , W. Hofmann , F. M. Rieger , N. Chakraborty

We report the discovery of the millisecond pulsar PSR J2043+1711 in a search of a Fermi Large Area Telescope (LAT) source with no known associations, with the Nancay Radio Telescope. The new pulsar, confirmed with the Green Bank Telescope,…

J1415+1320 is a well-studied blazar that exhibits strong flux density variability at a wide range of radio frequencies (2.4 $-$ 230~GHz). In this letter, we present a variability study of this source at 327~MHz using the data obtained with…

Astrophysics of Galaxies · Physics 2022-02-28 Sravani Vaddi , P. K. Manoharan , Anish Roshi

The long-term optical, X-ray and $\gamma$-ray data of blazar 3C 279 have been compiled from $Swift$-XRT, $RXTE$ PCA, $Fermi$-LAT, SMARTS and literature. The source exhibits strong variability on long time scales. Since 1980s to now, the…

High Energy Astrophysical Phenomena · Physics 2021-11-03 Bing-Kai Zhang , Min Jin , Xiao-Yun Zhao , Li Zhang , Ben-Zhong Dai