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Related papers: Correlated X-ray and optical variability in KV UMa

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This is the fifth paper in a series aimed at studying the chromospheres of active binary systems using several optical spectroscopic indicators to obtain or improve orbital solution and fundamental stellar parameters. We present here the…

Astrophysics · Physics 2009-11-13 M. C. Gálvez , D. Montes , M. J. Fernández-Figueroa , E. De Castro , M. Cornide

Using simultaneous optical (VLT/FORS2) and X-ray (XMM-Newton) data of NGC 5408, we present the first ever attempt to search for a reverberation signal in an ultraluminous X-ray source (NGC 5408 X-1). The idea is similar to AGN broad line…

High Energy Astrophysical Phenomena · Physics 2016-02-17 Dheeraj R. Pasham , Tod E. Strohmayer , S. Bradley Cenko , Margaret L. Trippe , Richard F. Mushotzky , Poshak Gandhi

We present results of five years of optical (UBVRI) observations of the very-high-energy gamma-ray blazar 1ES 1011+496 at the MDM Observatory. We calibrated UBVRI magnitudes of five comparison stars in the field of the object. Most of our…

High Energy Astrophysical Phenomena · Physics 2015-05-20 M. Boettcher , B. Hivick , J. Dashti , K. Fultz , S. Gupta , C. Gusbar , M. Joshi , A. Lamerato , T. Peery , D. Principe , A. Rajasingam , P. Roustazadeh , J. Shields

SAX J2103.5+4545 is the Be/X-ray binary with the shortest orbital period. It shows extended bright and faint X-ray states that last for a few hundred days. The main objective of this work is to investigate the relationship between the X-ray…

High Energy Astrophysical Phenomena · Physics 2015-05-14 P. Reig , A. Slowikowska , A Zezas , P. Blay

We report X-ray, optical, and near-infrared monitoring of the new X-ray transient MAXI J1820$+$070 discovered with MAXI on 2018 March 11. Its X-ray intensity reached $\sim 2$ Crab in 2--20 keV at the end of March, and then gradually…

We report on the optical spectroscopic monitoring of the X-ray transient MAXI J0709$-$159 (identified as the Be star LY CMa) performed for about 1.5 months after the X-ray detection with MAXI. The observed spectrum showed a double-peaked…

We explore the evolution of the X-ray luminosity function of quasars and the intrinsic correlation between the X-ray and 2500\AA $\,$ ultraviolet luminosities, utilizing techniques verified in previous works and a sample of over 4000…

Cosmology and Nongalactic Astrophysics · Physics 2022-08-02 J. Singal , S. Mutchnick , V. Petrosian

The blazar Mrk 421 is one of the closest, brightest and fastest varying source in the extragalactic X-ray/TeV sky. In the last years, many multi-wavelength campaigns have been carried out to study the correlation between the very high…

High Energy Astrophysical Phenomena · Physics 2015-08-27 Barbara Patricelli , Magdalena González , Nissim Fraija

ROTSE-IIId observations of the Be/X-ray transient system KS 1947+300 obtained between September 2004 and December 2005 make it possible to study the correlation between optical and X-ray activity. The optical outburst of 0.1 mag was…

Astrophysics · Physics 2009-11-11 U. Kiziloglu , A. Baykal , N. Kiziloglu

(Abridged) We present a detailed power density spectrum and cross-correlation analysis of the X-ray light curves of the BL Lac object PKS 2155-304, observed with BeppoSAX in 1997 and 1996, aimed at exploring the rapid variability properties…

V407 Vul (RXJ1914.4+2456) and HM Cnc (RXJ0806.3+1527) are X-ray emitting stars with X-ray light curves that are 100% modulated on periods of 569 and 321 seconds respectively. These periods are thought possibly to represent the orbital…

We present deep optical images of the historical X-ray Transient KY TrA in quiescence from which we confirm the identification of the counterpart reported by Murdin (1977) and derive an improved position of alpha=15:28:16.97 and…

Solar and Stellar Astrophysics · Physics 2015-10-28 C. Zurita , J. M. Corral-Santana , J. Casares

We present simultaneous X-ray (lambda_peak ~ 44A) and EUV (lambda_peak = 89A) light curves for the magnetic cataclysmic variable QQ Vulpeculae, obtained with the EUVE satellite. We find that the unique shape of the X-ray light curve is…

Astrophysics · Physics 2009-10-31 Kunegunda E. Belle , Steve B. Howell , Amy Mills

We report on a timing analysis of a new ~630ks XMM-Newton observation of the quasar, PG 1211+143. We find a well-defined X-ray power spectrum with a well-detected bend at ~7e-5 Hz, consistent with the established…

Astrophysics of Galaxies · Physics 2016-01-27 Andrew Lobban , Simon Vaughan , Ken Pounds , James Reeves

We present cross-correlation studies of gamma-ray (0.1-300 GeV), X-ray (0.2-10 keV) and optical (R-band) variability of a sample of 26 blazars during 2008-2016. The light curves are from Fermi-LAT, Swift-XRT, and the Yale-SMARTS blazar…

High Energy Astrophysical Phenomena · Physics 2020-04-08 Anwesh Majumder , Kaustav Mitra , Ritaban Chatterjee , C. M. Urry , C. D. Bailyn , Prantik Nandi

We present optical broadband (B and R) observations of the Seyfert 1 nucleus NGC 3516, obtained at Wise Observatory from 1997 March to 1998 September, contemporaneously with the X-ray 2-10 keV measurements of RXTE. The cross correlation…

Astrophysics · Physics 2009-10-31 Dan Maoz , Rick Edelson , Kirpal Nandra

We propose two dimensional x-ray coherent correlation spectroscopy (2DXCS) for the study of interactions between core-electron and valence transitions. This technique might find experimental applications in the future when very high…

Quantum Physics · Physics 2009-11-13 Igor V. Schweigert , Shaul Mukamel

Transient X-ray absorption techniques can measure ultrafast dynamics of the elemental edges in a material or multiple layer junction, giving them immense potential for deconvoluting concurrent processes. However, the interpretation of the…

Materials Science · Physics 2021-06-10 Hanzhe Liu , Isabel M. Klein , Jonathan M. Michelsen , Scott K. Cushing

We present the results of XMM-Newton observations of two AM CVn systems - V396 Hya and SDSS J1240-01. Both systems are detected in X-rays and in the UV: neither shows coherent variability in their light curves. We compare the rms…

Astrophysics · Physics 2009-11-11 Gavin Ramsay , Paul J. Groot , Tom Marsh , Gijs Nelemans , Danny Steeghs , Pasi Hakala
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