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We report on radio timing and multiwavelength observations of the 4.66 ms redback pulsar J1048+2339, which was discovered in an Arecibo search targeting the Fermi-LAT source 3FGLJ1048.6+2338. Two years of timing allowed us to derive precise…

High Energy Astrophysical Phenomena · Physics 2016-06-01 J. S. Deneva , P. S. Ray , F. Camilo , J. P. Halpern , K. Wood , H. T. Cromartie , E. Ferrara , M. Kerr , S. M. Ransom , M. T. Wolff , K. C. Chambers , E. A. Magnier

PSR J1829+2456 is a radio pulsar in a relativistic binary system with another neutron star. It has a rotational period of 41 ms and a mildly eccentric ($e = 0.14$) 28-hr orbit. We have continued its observations with the Arecibo radio…

We present time-resolved optical spectroscopy of the `redback' binary millisecond pulsar system PSR J1023+0038 during both its radio pulsar (2009) and accretion disc states (2014 and 2016). We provide observational evidence for the…

Solar and Stellar Astrophysics · Physics 2019-06-19 T. Shahbaz , M. Linares , P. Rodriguez-Gil , J. Casares

We report the discovery of a 2.11 ms binary millisecond pulsar during a targeted search of the redback optical candidate coincident with the $\gamma$-ray source 3FGL J0212.5+5320 using the Robert C. Byrd Green Bank Telescope (GBT) with the…

High Energy Astrophysical Phenomena · Physics 2023-08-02 Karen I. Perez , Slavko Bogdanov , Jules P. Halpern , Vishal Gajjar

In a search of the unidentified Fermi gamma-ray source 3FGL J1417.5-4402 with the Parkes radio telescope, we discovered PSR J1417-4402, a 2.66 ms pulsar having the same 5.4 day orbital period as the optical and X-ray binary identified by…

Solar and Stellar Astrophysics · Physics 2016-03-23 F. Camilo , J. E. Reynolds , S. M. Ransom , J. P. Halpern , S. Bogdanov , M. Kerr , P. S. Ray , J. M. Cordes , J. Sarkissian , E. D. Barr , E. C. Ferrara

We analyze photometry and spectra of the "redback" millisecond pulsar binary J2339$-$0533. These observations include new measurements from Keck and GROND, as well as archival measurements from the OISTER, WIYN, SOAR, and HET telescopes.…

High Energy Astrophysical Phenomena · Physics 2020-11-04 D. Kandel , Roger W. Romani , Alexei V. Filippenko , Thomas G. Brink , WeiKang Zheng

We present a Chandra X-ray Observatory ACIS-S variability, spectroscopy, and imaging study of the peculiar binary containing the millisecond pulsar J1023+0038. The X-ray emission from the system exhibits highly significant (12.5 sigma)…

The maximum mass of a neutron star has important implications across multiple research fields, including astrophysics, nuclear physics and gravitational wave astronomy. Compact binary millisecond pulsars (with orbital periods shorter than…

High Energy Astrophysical Phenomena · Physics 2019-10-23 Manuel Linares

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

Aims: The binary pulsar PSR J1811-1736 has been identified, since its discovery, as a member of a double neutron star system. Observations of such binary pulsars allow the measurement of general relativistic effects, which in turn lead to…

Astrophysics · Physics 2009-11-11 A. Corongiu , M. Kramer , B. W. Stappers , A. G. Lyne , A. Jessner , A. Possenti , N. D'Amico , O. Loehmer

The binary millisecond radio pulsar PSR J1023+0038 has been recently the subject of multiwavelength monitoring campaigns which revealed that an accretion disc has formed around the neutron star (since 2013 June). We present here the results…

PSR J1811-1736 (P=104 ms) is an old (~1.89 Gyrs) binary pulsar (P_orb=18.8 d) in a highly eccentric orbit (e=0.828) with an unidentified companion. Interestingly enough, the pulsar timing solution yields an estimated companion mass 0.93…

Solar and Stellar Astrophysics · Physics 2015-06-12 R. P. Mignani , A. Corongiu , C. Pallanca , F. R. Ferraro

We have investigated the intrabinary shock emission from the redback millisecond pulsar PSR J2129-0429 with XMM-Newton and Fermi. Orbital modulation in X-ray and UV can be clearly seen. Its X-ray modulation has a double-peak structure with…

High Energy Astrophysical Phenomena · Physics 2015-06-23 C. Y. Hui , C. P. Hu , S. M. Park , J. Takata , K. L. Li , P. H. T. Tam , L. C. C. Lin , A. K. H. Kong , K. S. Cheng , Chunglee Kim

We present the first results from a joint XMM-Newton and NuSTAR observation of the gamma-ray emitting millisecond pulsar compact binary PSR J2129-0429. X-ray emission up to about 40 keV is detected and the joint spectrum can be modeled with…

High Energy Astrophysical Phenomena · Physics 2018-07-11 A. K. H. Kong , J. Takata , C. Y. Hui , J. Zhao , K. L. Li , P. H. T. Tam

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

We report on the first NuSTAR observation of the gamma-ray emitting millisecond pulsar binary PSR J1723-2837. X-ray radiation up to 79 keV is clearly detected and the simultaneous NuSTAR and Swift spectrum is well described by an absorbed…

High Energy Astrophysical Phenomena · Physics 2017-05-03 A. K. H. Kong , C. Y. Hui , J. Takata , K. L. Li , P. H. T. Tam

We report on a series of spectroscopic observations of PSR J1311-3430, an extreme black-widow gamma-ray pulsar with a helium-star companion. In a previous study we estimated the neutron star mass as M_NS= 2.68+/-0.14M_Sun (statistical…

High Energy Astrophysical Phenomena · Physics 2015-05-27 Roger W. Romani , Alexei V. Filippenko , S. Bradley Cenko

PSR J1306--40 is a millisecond pulsar binary with a non-degenerate companion in an unusually long $\sim$1.097 day orbit. We present new optical photometry and spectroscopy of this system, and model these data to constrain fundamental…

High Energy Astrophysical Phenomena · Physics 2019-05-01 Samuel J. Swihart , Jay Strader , Laura Chomiuk , Laura Shishkovsky

Pulsar timing of double neutron star (DNS) systems is one of the best methodologies to study the neutron star masses distribution. Here we report the discovery of a double neutron star system PSR J0641+0448 in the Five-hundred-meter…

High Energy Astrophysical Phenomena · Physics 2026-03-12 Z. L. Yang , J. L. Han , P. F. Wang , C. Wang , N. N. Cai , W. C. Jing , W. Q. Su , T. Wang , J. Xu , Yi Yan , D. J. Zhou

We report here the Einstein@Home discovery of PSR J1913+1102, a 27.3-ms pulsar found in data from the ongoing Arecibo PALFA pulsar survey. The pulsar is in a 4.95-hr double neutron star (DNS) system with an eccentricity of 0.089. From radio…

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