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Based on the X-ray observations from XMM-Newton and Swift, and optical observations from Transiting Exoplanet Survey Satellite (TESS) and AAVSO, we present temporal and spectral properties of probable intermediate polar SWIFT J0503.7-2819.…

High Energy Astrophysical Phenomena · Physics 2022-10-05 Nikita Rawat , J. C. Pandey , Arti Joshi , Simone Scaringi , Umesh Yadava

We report the identification of the cataclysmic variable 1RXSJ062518.2+733433 as an intermediate polar. The orbital period of the system is determined to be 283.0+-2 min from the radial velocity variation of Halpha, measured in an extensive…

Astrophysics · Physics 2009-11-07 S. Araujo-Betancor , B. T. Gaensicke , H. -J. Hagen , P. Rodriguez-Gil , D. Engels

We present 20 epochs of optical spectroscopy obtained with the GTC-10.4m telescope across the bright discovery outburst of the black hole candidate Swift J1727.8-162. The spectra cover the main accretion states and are characterised by the…

High Energy Astrophysical Phenomena · Physics 2024-02-02 D. Mata Sánchez , T. Muñoz-Darias , M. Armas Padilla , J. Casares , M. A. P. Torres

We present a multi-frequency study of eclipse properties of a transitional redback millisecond pulsar J1227$-$4853 discovered in 2014 with the GMRT. Emission from this pulsar is eclipsed at 607 MHz for about 37% of its orbit around the…

High Energy Astrophysical Phenomena · Physics 2020-07-21 Sanjay Kudale , Jayanta Roy , Bhaswati Bhattacharyya , Ben Stappers , Jayaram Chengalur

We report the results of a twenty-eight-month photometric campaign studying V1432 Aql, the only known eclipsing, asynchronous polar. Our data show that both the residual eclipse flux and eclipse O-C timings vary strongly as a function of…

We report on an {unusually} bright observation of PSR J1720$-$0533 using the Five-hundred-meter Aperture Spherical radio Telescope (FAST). The pulsar is in a black widow system that {was discovered by the Commensal Radio Astronomy FAST…

High Energy Astrophysical Phenomena · Physics 2021-11-24 S. Q. Wang , J. B. Wang , N. Wang , J. M. Yao , G. Hobbs , S. Dai , F. F. Kou , C. C. Miao , D. Li , Y. Feng , S. J. Dang , D. H. Wang , P. Wang , J. P. Yuan , C. M. Zhang , L. Zhang , S. B. Zhang , W. W. Zhu

Polarimetry of IGR J1401-4306, a long period (12.7 hours), eclipsing intermediate polar and remnant of Nova Scorpii 1437 A.D., reveals periodic variations of optical circular polarization, confirming the system as the longest period…

High Energy Astrophysical Phenomena · Physics 2017-12-06 Stephen B. Potter , David A. H. Buckley

We report the discovery of the first radio pulsar associated with NGC 6712, an eclipsing black widow (BW) pulsar, J1853$-$0842A, found by high-sensitivity searches using the Five-hundred-meter Aperture Spherical radio Telescope. This 2.15…

High Energy Astrophysical Phenomena · Physics 2021-11-17 Zhen Yan , Zhi-chen Pan , Scott M. Ransom , Duncan R. Lorimer , Lei Qian , Pei Wang , Zhi-qiang Shen , Di Li , Peng Jiang , Jin-Tao Luo , Jie Liu , Zhi-peng Huang

We report the discovery and analysis of PTF1 J085713+331843, a new eclipsing post common-envelope detached white-dwarf red-dwarf binary with a 2.5h orbital period discovered by the Palomar Transient Factory. ULTRACAM multicolour photometry…

Solar and Stellar Astrophysics · Physics 2017-04-19 J. van Roestel , P. J. Groot , D. Levitan , T. A. Prince , S. Bloemen , T. R. Marsh , V. S. Dhillon , D. Shupe , R. Laher

We report the discovery and characterization of PSR J1810-0623, a fully recycled millisecond pulsar with a spin period of 4.55 ms, discovered with the Five-hundred-meter Aperture Spherical radio Telescope (FAST) and followed up with FAST…

High Energy Astrophysical Phenomena · Physics 2026-03-17 Jie Zhang , Zerui Wang , Lei Zhang , Yulan Liu , Alessandro Ridolfi , Meng Guo , Di Li , Ryan S. Lynch , Cong Wang , Pei Wang , Mengmeng Ni , Jiale Hu , Mengquan Liu , Zhie Liu , Bo Han , Chenchen Miao

We report the discovery of ZTF J2243+5242, an eclipsing double white dwarf binary with an orbital period of just $8.8$ minutes, the second known eclipsing binary with an orbital period less than ten minutes. The system likely consists of…

This study presents a detailed timing analyses of two cataclysmic variables (CVs), [PK2008] HalphaJ115927 and IGR J14091-610, utilizing the optical data from the Transiting Exoplanet Survey Satellite (TESS). Periods of 7.20$\pm$0.02 h,…

Solar and Stellar Astrophysics · Physics 2025-04-23 Arti Joshi

We report optical and X-ray observations of the high-field polar RXJ1007.5-2017 performed between 1990 and 2012. It has an orbital period of 208.60 min determined from the ellipsoidal modulation of the secondary star in an extended low…

High Energy Astrophysical Phenomena · Physics 2015-06-11 H. -C. Thomas , K. Beuermann , K. Reinsch , A. D. Schwope , V. Burwitz

We present optical photometry and spectroscopy of the new eclipsing Cataclysmic Variable MASTER OTJ192328.22+612413.5, discovered by the MASTER team. We find the orbital period to be P=0.16764612(5) day /4.023507(1) hour. The depth of the…

Solar and Stellar Astrophysics · Physics 2016-07-13 M. R. Kennedy , P. Callanan , P. M. Garnavich , P. Szkody , S. Bounane , B. M. Rose , P. Bendjoya , L. Abe , J. P. Rivet , O. Suarez

We present a study of PSR J1723-2837, an eclipsing, 1.86 ms millisecond binary radio pulsar discovered in the Parkes Multibeam survey. Radio timing indicates that the pulsar has a circular orbit with a 15 hr orbital period, a low-mass…

PSR J1928+1815 is a 10.55 ms millisecond pulsar in a 3.6 hr orbit with a massive ($1.0$-$1.6\,M_{\odot}$) companion that produces extended radio eclipses. The companion, proposed to be a stripped helium star, is undetected in optical and…

Solar and Stellar Astrophysics · Physics 2026-04-07 Pranav Nagarajan , Kareem El-Badry , Jim Fuller , Yunlang Guo , Thomas M. Tauris

We report the discovery of ZTF J0127+5258, a compact mass-transferring binary with an orbital period of 13.7 minutes. The system contains a white dwarf accretor, which likely originated as a post-common envelope carbon-oxygen (CO) white…

A new magnetic cataclysmic variable is identified as the counterpart of the X-ray source RX J0719.2+6557. The emission lines show radial velocity variations with a period of 98.2 min. This coincides with the period of deep eclipses (up to 4…

We report the discovery of a new totally-eclipsing binary (RA=06:40:29.11; Dec=+38:56:52.2; J=2000.0; Rmax=17.2 mag) with an sdO primary and a strongly irradiated red dwarf companion. It has an orbital period of Porb=0.187284394(11) d and…

We present time-resolved spectroscopy and photometry of SDSS J100658.40+233724.4, which we have discovered to be an eclipsing cataclysmic variable with an orbital period of 0.18591324 days (267.71507 min). The observed velocity amplitude of…

Solar and Stellar Astrophysics · Physics 2015-05-14 John Southworth , R. D. G. Hickman , T. R. Marsh , A. Rebassa-Mansergas , B. T. Gansicke , C. M. Copperwheat , P. Rodriguez-Gil