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We report on the first continuous, 80 day optical monitoring of the transitional millisecond pulsar PSR J1023+0038 carried out in mid-2017 with Kepler in the K2 configuration, when an X-ray subluminous accretion disk was present in the…

We report the results of XMM-Newton and BeppoSAX observations of the radio and X-ray emitting star LS I +61 303, likely associated with the gamma-ray source 2CG 135+01 and recently detected also at TeV energies. The data include a long…

We present ground-based and Swift photometric and spectroscopic observations of the tidal disruption event (TDE) ASASSN-15oi, discovered at the center of 2MASX J20390918-3045201 ($d\simeq216$ Mpc) by the All-Sky Automated Survey for…

From late September 2017 to February 2018, the Be X-ray binary (BeXB) Swift J0243.6+6124 underwent an unprecedently bright giant outburst. The reported X-ray luminosities were so high that the system was classified as an Ultraluminous X-ray…

We present an optical (gri) study during quiescence of the accreting millisecond X-ray pulsar IGR J00291+5934 performed with the 10.4m Gran Telescopio Canarias (GTC) in August 2014. Despite the source being in quiescence at the time of our…

High Energy Astrophysical Phenomena · Physics 2017-04-12 M. C. Baglio , S. Campana , P. D'Avanzo , A. Papitto , L. Burderi , T. Di Salvo , T. Muñoz Darias , N. Rea , D. F. Torres

We present the identifications of a flux-limited sample of highly variable X-ray sources on long time-scales from the second catalogue of the XMM$-$Newton SLew survey (XMMSL2). The carefully constructed sample, comprising 265 sources (2.5…

High Energy Astrophysical Phenomena · Physics 2022-04-12 Dongyue Li , R. L. C. Starling , R. D. Saxton , Hai-Wu Pan , Weimin Yuan

We present the results of analyzing the XMM-Newton data obtained in 2001 November 7 - 8. A flare is observed simultaneously in X-ray and UV together with a quiescence. We find that during the flare event X-ray flux varies with UV with no…

Astrophysics · Physics 2008-11-26 Chul-Sung Choi , Tadayasu Dotani

Context: In April 2013, the nearby (z=0.031) TeV blazar, Mkn 421, showed one of the largest flares in X-rays since the past decade. Aim: To study all multiwavelength data available during MJD 56392 to 56403, with special emphasis on X-ray…

Astrophysics of Galaxies · Physics 2015-08-12 Atreyee Sinha , Amit Shukla , Ranjeev Misra , Varsha R. Chitnis , A. R. Rao , B. S. Acharya

Observational astronomy of tidal disruption events (TDEs) began with the detection of X-ray flares from quiescent galaxies during the ROSAT all-sky survey of 1990-1991. The flares complied with theoretical expectations, having high peak…

High Energy Astrophysical Phenomena · Physics 2021-03-30 R. Saxton , S. Komossa , K. Auchettl , P. G Jonker

The narrow-line Seyfert 1 galaxy Mrk 335 was one of the X-ray brightest AGN, but it has systematically faded since 2007. Here, we report the discovery with Swift of a sequence of bright and rapid X-ray flare events that reveal the emergence…

High Energy Astrophysical Phenomena · Physics 2020-11-18 S. Komossa , D. Grupe , L. C. Gallo , P. Poulos , D. Blue , E. Kara , G. Kriss , A. L. Longinotti , M. L. Parker , D. Wilkins

At the end of March 2004, the blazar S5 0716+714 underwent an optical outburst that prompted for quasi-simultaneous target-of-opportunity observations with the INTEGRAL and XMM-Newton satellites. In this paper, we report the results of the…

We present the first results from a detailed analysis of a new, long ($\sim100$ ks) XMM-Newton observation of the narrow-line Seyfert 1 galaxy PG 1404$+$226 which showed a large-amplitude, rapid X-ray variability by a factor of $\sim7$ in…

High Energy Astrophysical Phenomena · Physics 2018-08-29 Labani Mallick , Gulab C. Dewangan

We report an observational estimate of the rate of stellar tidal disruption flares (TDFs), based on our (successful) search for these events in archival Sloan Digital Sky Survey (SDSS) multi-epoch imaging data. Our pipeline took advantage…

Cosmology and Nongalactic Astrophysics · Physics 2013-01-30 Sjoert van Velzen , Glennys R. Farrar

The BL Lacertae OJ 287 is a supermassive black holes binary (SMBHB) system with complex physics of its irregular flares. During 2016 October -- 2017 April period, a surprising outburst in the X-ray, UV and optical bands was detected, while…

High Energy Astrophysical Phenomena · Physics 2021-11-09 Shifeng Huang , Shaoming Hu , Hongxing Yin , Xu Chen , Sofya Alexeeva , Dongyang Gao , Yunguo Jiang

Characterizing the distribution of flare properties and occurrence rates is important for understanding habitability of M dwarf exoplanets. The GALEX space telescope observed the GJ 65 system, composed of the active, flaring M stars BL Cet…

Solar and Stellar Astrophysics · Physics 2022-03-30 Scott W. Fleming , Chase Million , Rachel A. Osten , Dmitrii Y. Kolotkov , C. E. Brasseur

It has long been suggested that supermassive black holes in non-active galaxies might be tracked down by occasional tidal disruptions of stars on nearly radial orbits. A tidal disruption event would reveal itself by a luminous flare of…

Astrophysics · Physics 2009-11-07 Stefanie Komossa

Tidal disruption events are possible sources of temporary nuclear activity in galactic nuclei and can be considered as good indicators of the existence of super massive black holes in the centers of galaxies. A new X-ray source has been…

Cosmology and Nongalactic Astrophysics · Physics 2009-11-13 N. Cappelluti , M. Ajello , P. Rebusco , S. Komossa , A. Bongiorno , C. Clemens , M. Salvato , P. Esquej , T. Aldcroft , J. Greiner , H. Quintana

XTE J1701-407 is a new transient X-ray source discovered on June 8th, 2008. More than one month later it showed a rare type of thermonuclear explosion: a long type I X-ray burst. We report herein the results of our study of the spectral and…

During a 50 ks monitoring observation of the Galactic bulge performed in September 1999 by the Wide Field Cameras on board the BeppoSAX satellite, an X-ray burst was detected from a sky position ~3 degrees off the Galactic centre. No…

Recent observations of the Small Magellanic Cloud (SMC) with Einstein Probe (EP) revealed a new transient X-ray source, most likely identified as Be/X-ray binary. To characterise the X-ray properties of EP J005146.9-730930 and in particular…

High Energy Astrophysical Phenomena · Physics 2025-07-24 F. Haberl , Y. Xu , C. Maitra , G. Vasilopoulos , W. Zhang , W. Yuan , C. Jin , H. N. Yang , L. Ducci , D. M. Kaltenbrunner , P. Maggi , A. Rau