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IGR J04571+4527 and Swift J0525.6+2416 are two hard X-ray sources detected in the Swift/BAT and INTEGRAL/IBIS surveys. They were proposed to be magnetic cataclysmic variables of the Intermediate Polar (IP) type, based on optical…

High Energy Astrophysical Phenomena · Physics 2015-09-16 F. Bernardini , D. de Martino , K. Mukai , G. Israel , M. Falanga , G. Ramsay , N. Masetti

We conducted time-resolved optical spectroscopy and/or time-series photometry of 15 cataclysmic binaries that were discovered in hard X-ray surveys by the Swift Burst Alert Telescope (BAT) and the International Gamma-Ray Astrophysics…

High Energy Astrophysical Phenomena · Physics 2018-06-06 J. P. Halpern , J. R. Thorstensen , P. Cho , G. Collver , M. Motsoaledi , H. Breytenbach , D. A. H. Buckley , P. A. Woudt

We aim at characterizing a sample of 9 new hard X-ray selected Cataclysmic Variable (CVs), to unambiguously identify them as magnetic systems of the Intermediate Polar (IP) type. We performed timing and spectral analysis by using X-ray, and…

High Energy Astrophysical Phenomena · Physics 2015-06-04 F. Bernardini , D. de Martino , M. Falanga , K. Mukai , G. Matt , J. -M. Bonnet-Bidaud , N. Masetti , M. Mouchet

Swift J2218.4+1925, a hard X-ray source detected by Swift BAT, has been proposed as a candidate magnetic cataclysmic variable of the polar type from optical spectroscopy. Using XMM-Newton we perform detailed timing and spectral analysis…

High Energy Astrophysical Phenomena · Physics 2015-06-22 Federico Bernardini , Domitilla de Martino , Koji Mukai , Maurizio Falanga

We report on the Swift/XRT Deep Galactic Plane Survey discovery and multi-wavelength follow-up observations of a new intermediate polar Cataclysmic Variable, Swift J183920.1-045350. A 449.7 s spin period is found in Xmm-Newton and NuSTAR…

We conducted time-resolved optical spectroscopy and/or photometry of ten cataclysmic binaries that were discovered in hard X-ray surveys, with the goal of measuring their orbital periods and searching for evidence that they are magnetic.…

High Energy Astrophysical Phenomena · Physics 2022-01-19 J. P. Halpern , J. R. Thorstensen

The INTEGRAL and Swift hard X-ray surveys have identified a large number of new sources, among which many are proposed as Cataclysmic Variables (CVs). Here we present the first detailed study of three X-ray selected CVs, Swift J1907.3-2050,…

Optical and X-ray observations suggested that the 9.38 h binary, SWIFT J0746.3- 1608 could be a Cataclysmic Variable of the magnetic or nova-like type, or a low mass X-ray binary. Its optical, UV, and X-ray light curves are strongly…

High Energy Astrophysical Phenomena · Physics 2019-01-09 F. Bernardini , D. de Martino , K. Mukai , M. Falanga

We present the first X-ray observations with the XMM-Newton and INTEGRAL satellites of the recently discovered cataclysmic variable 1RXSJ173021.5-055933, together with simultaneous UV and coordinated optical photometry aiming at…

A significant number of cataclysmic variables were detected as hard X-ray sources in the INTEGRAL survey, most of them of the magnetic intermediate polar type. We present a detailed X-ray broad-band study of two new sources, IGR J00234+6141…

Solar and Stellar Astrophysics · Physics 2010-07-21 G. Anzolin , D. de Martino , M. Falanga , K. Mukai , J. -M. Bonnet-Bidaud , M. Mouchet , Y. Terada , M. Ishida

We present the results of our optical identifications of four hard X-ray sources from the Swift all-sky survey. We obtained optical spectra for each of the program objects with the 6-m BTA telescope (Special Astrophysical Observatory,…

High Energy Astrophysical Phenomena · Physics 2015-06-04 A. Lutovinov , R. Burenin , M. Revnivtsev , S. Sazonov , O. Sholukhova , A. Valeev

We present multi-wavelength temporal and spectral characteristics of a magnetic cataclysmic variable (MCV) Swift J0503.7-2819, using far ultraviolet (FUV) and X-ray data from AstroSat, supplemented with optical data from the Southern…

From a set of thirteen cataclysmic binaries that were discovered in the Swift Burst Alert Telescope (BAT) survey, we conducted time-resolved optical spectroscopy and/or time-series photometry of eleven, with the goal of measuring their…

High Energy Astrophysical Phenomena · Physics 2015-11-11 J. P. Halpern , J. R. Thorstensen

Here, we present the results of our multi-wavelength campaign aimed at classifying \textit{Swift} J170800$-$402551.8 as part of the \textit{Swift} Deep Galactic Plane Survey (DGPS). We utilized Target of Opportunity (ToO) observations with…

We analyze the first X-ray observations with XMM-Newton of RXS J070407.9+262501 and 1RXS 180340.0+401214, in order to characterize their broad-band temporal and spectral properties, also in the UV/optical domain, and to confirm them as…

Among hard X-ray Galactic sources detected in the Swift and INTEGRAL surveys, those discovered as accreting white dwarf binaries have suprisingly boosted in number in the recent years. The majority are identified as magnetic Cataclysmic…

High Energy Astrophysical Phenomena · Physics 2020-01-24 D. de Martino , F. Bernardini , K. Mukai , M. Falanga , N. Masetti

Several persistent, low luminosity (L_X 10^{34} erg s^{-1}), long spin period (P>100 s) High Mass X-ray Binaries have been reported with blackbody components with temperatures >1 keV. These hot thermal excesses have correspondingly small…

High Energy Astrophysical Phenomena · Physics 2016-03-02 E. S. Bartlett , M. J. Coe , W. C. G. Ho

In the last years the hard X-ray astronomy has made a significant step forward, thanks to the monitoring of the IBIS/ISGRI telescope on board the INTEGRAL satellite and of the Burst Alert Telescope (BAT) on board of the Swift observatory.…

High Energy Astrophysical Phenomena · Physics 2015-06-16 A. Segreto , G. Cusumano , V. La Parola , A. D'Aì , N. Masetti , P. D'Avanzo

IGR J14257-6117 is an unclassified source in the hard X-ray catalogues. Optical follow-ups suggest it could be a Cataclysmic Variable of the magnetic type. We present the first high S/N X-ray observation performed by \XMM\ at 0.3--10 keV,…

High Energy Astrophysical Phenomena · Physics 2018-05-16 F. Bernardini , D. de Martino , K. Mukai , M. Falanga

We report on XMM-Newton and optical results for 6 cataclysmic variables that were selected from Sloan Digital Sky Survey spectra because they showed strong HeII emission lines, indicative of being candidates for containing white dwarfs with…

Solar and Stellar Astrophysics · Physics 2009-11-13 Eric J. Hilton , Paula Szkody , Anjum Mukadam , Arne Henden , William Dillon , Gary D. Schmidt
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