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Related papers: IGR J18293-1213 is an eclipsing Cataclysmic Variab…

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On 2011 August 11, INTEGRAL discovered the hard X-ray source IGR J17361-4441 near the centre of the globular cluster NGC 6388. Follow up observations with Chandra showed the position of the transient was inconsistent with the cluster…

The International Gamma-Ray Astrophysics Laboratory (INTEGRAL) satellite has detected in excess of 1000 sources in the ~20-100 keV band during its surveys of the sky over the past 17 years. We obtained 5 ks observations of 15 unclassified…

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

We report the results of a high-energy multi-instrumental campaign with INTEGRAL, RXTE, and Swift of the recently discovered INTEGRAL source IGR J19294+1816. The Swift/XRT data allow us to refine the position of the source to RA= 19h 29m…

High Energy Astrophysical Phenomena · Physics 2015-05-14 J. Rodriguez , J. A. Tomsick , A. Bodaghee , J. -A. Zurita Heras , S. Chaty , A. Paizis , S. Corbel

IGR J16320-4751 is a highly obscured HMXB source containing a very slow neutron star ($P_{spin}\sim1300$ sec) orbiting its supergiant companion star with a period of $\sim$9 days. It shows high column density ($N_{H}\sim2-5\times10^{23}$…

High Energy Astrophysical Phenomena · Physics 2022-10-07 Varun , Nirmal Iyer , Biswajit Paul

We present further results from our ongoing optical spectrophotometric campaign at the Astronomical Observatory of Bologna in Loiano (Italy) on unidentified hard X-ray sources detected by INTEGRAL. We observed spectroscopically the putative…

In this paper we report on a long multi-wavelength observational campaign of the supergiant fast X-ray transient prototype IGR J17544-2619. A 150 ks-long observation was carried out simultaneously with XMM-Newton and NuSTAR, catching the…

High Energy Astrophysical Phenomena · Physics 2016-12-07 E. Bozzo , V. Bhalerao , P. Pradhan , J. Tomsick , P. Romano , C. Ferrigno , S. Chaty , L. Oskinova , A. Manousakis , R. Walter , M. Falanga , S. Campana , L. Stella , M. Ramolla , R. Chini

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

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

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

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 number of new X-ray sources (IGR J17091-3624, IGR/XTE J17391-3021, IGR J17464-3213 (= XTE J17464-3213 = H 1743-322), IGR J17597-2201, SAX/IGR J18027-2017) have been observed with the INTEGRAL observatory during ultra deep exposure of the…

Astrophysics · Physics 2009-11-10 A. Lutovinov , M. Revnivtsev , S. Molkov , R. Sunyaev

IGR J18219-1347 is a hard X-ray source discovered by INTEGRAL in 2010. We have analyzed the X-ray emission of this source exploiting the BAT survey data up to March 2012 and the XRT data that include also an observing campaign performed in…

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

IGR J18179-1621 is an obscured accreting X-ray pulsar discovered by INTEGRAL on 2012 February 29. We report on our 20 ksec Chandra-High Energy Transmission Gratings Spectrometer observation of the source performed on 2012 March 17, on two…

High Energy Astrophysical Phenomena · Physics 2015-06-05 M. A. Nowak , A. Paizis , J. Rodriguez , S. Chaty , M. Del Santo , V. Grinberg , J. Wilms , P. Ubertini , R. Chini

Hard X-ray imaging of the Galactic plane by the INTEGRAL satellite is uncovering large numbers of 20-100 keV "IGR" sources. We present results from Chandra, INTEGRAL, optical, and IR observations of 4 IGR sources: 3 sources in the Norma…

We analyze 18 sources that were found to show interesting properties of periodicity, very soft spectra and/or large long-term variability in X-rays in our project of classification of sources from the 2XMMi-DR3 catalog but were poorly…

High Energy Astrophysical Phenomena · Physics 2015-06-17 Dacheng Lin , Natalie A. Webb , Didier Barret

We report on a 12 hr XMM-Newton observation of the supergiant High-Mass X-ray Binary IGR J16207-5129. This is only the second soft X-ray (0.4-15 keV, in this case) study of the source since it was discovered by the INTEGRAL satellite. The…

The growing number of multi-epoch optical and infrared sky surveys are uncovering unprecedented numbers of new variable stars, of an increasing number of types. The short interval between observations in adjacent near infrared filters in…

Solar and Stellar Astrophysics · Physics 2022-06-29 C. Morris , T. J. Maccarone , P. W. Lucas , J. Strader , C. T. Britt , N. Miller , S. J. Swihart , W. J. Cooper , J. E. Drew , Z. Guo

Here we report on X-ray observations of ten 17-60 keV sources discovered by the INTEGRAL satellite. The primary new information is sub-arcsecond positions obtained by the Chandra X-ray Observatory. In six cases (IGR J17040-4305, IGR…

We present analysis of archival X-ray data obtained with the XMM-Newton and Suzaku for a new Intermediate Polar identified as a counterpart of an INTEGRAL discovered gamma-ray source, IGR J17195-4100. We report a new period of 1053.7\pm12.2…

High Energy Astrophysical Phenomena · Physics 2015-06-11 V. Girish , K. P. Singh