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Related papers: The Chandra High Resolution Spectra of Mkn 421

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We observed the "micro-quasar" GRS 1758-258 four times with Chandra. Two HRC-I observations were made in 2000 September-October spanning an intermediate-to-hard spectral transition (identified with RXTE). Another HRC-I and an ACIS/HETG…

Astrophysics · Physics 2009-11-07 W. A. Heindl , D. M. Smith

Since its commissioning in fall 1996, the stereoscopic system of Imaging Atmospheric Cherenkov Telescope (IACTs) of HEGRA with an energy threshold of 500 GeV, an angular resolution of 0.1 degree and an energy resolution of 20% per…

Astrophysics · Physics 2007-05-23 F. A. Aharonian

The X-ray luminous RS CVn binary system HR 1099 has been observed on several occasions in the early phases of \textit{Chandra} and \textit{XMM-Newton}. A very hot (up to 40 MK) dominant coronal plasma has been identified from the…

Astrophysics · Physics 2007-05-23 M. Audard , M. Guedel , R. L. J. van der Meer

The HEGRA 5 m^2 air Cherenkov telescope (CT1) was used to search for gamma-ray emission above 1.5 TeV from a series of low redshift AGN (Mkn 421, Mkn 501, MS 0116+319, PKS 2209+236, NGC 315 and W Comae). Here we present results from a total…

We report on the X-ray observation of the radio selected supernova SN1979C carried out with ASCA in 1997 December and serendipitously available from a Chandra Guaranteed Time Observation in 1999 November. The supernova, of type SN II-Linear…

Astrophysics · Physics 2009-11-06 A. Ray , R. Petre , E. M. Schlegel

We present some early results on AGN from the Chandra X-ray Observatory, highlighting high resolution spectroscopy using the High Energy Transmission Grating Spectrometer (HETGS). The quasar PKS 0637-752 was found to have a very bright…

Astrophysics · Physics 2009-10-31 H. L. Marshall

The highest spectral resolution data for the Fe-K lines in type I AGN, as observed with the Chandra High Energy Grating (HEG), reveal a variety of line shapes. However, the energies of the most prominent peak are all clustered tightly…

Astrophysics · Physics 2007-05-23 T. Yaqoob , U. Padmanabhan

As part of the Chandra GTO program we are monitoring and surveying M31 using the HRC and ACIS cameras. These observations have resolved the nuclear X-ray source into five separate sources, one of which is very soft and may (or may not!) be…

Astrophysics · Physics 2007-05-23 M. R. Garcia , S. S. Murray , F. A. Primini , W. R. Forman , C. Jones , J. E. McClintock

We observed the "micro-quasar" GRS 1758-258 four times with Chandra. Two HRC-I observations were made in 2000 September-October spanning an intermediate-to-hard spectral transition (identified with RXTE). Another HRC-I and an ACIS/HETGS…

Astrophysics · Physics 2007-05-23 W. A. Heindl , D. M. Smith

We present a multi-wavelength analysis of MCG+11-11-032, a nearby AGN with the unique classification of both a binary and a dual AGN candidate. With new Chandra observations we aim to resolve any dual AGN system via imaging data, and search…

Mkn 421 was observed during a high flux state for nine nights in April and May 2004 with the fully operational High Energy Stereoscopic System (H.E.S.S.) in Namibia. The observations were carried out at zenith angles of…

Astrophysics · Physics 2012-08-27 H. E. S. S. Collaboration , : , F. Aharonian

We observed MS 1054-0321, the highest redshift cluster of galaxies in the Einstein Medium Sensitivity Survey (EMSS), with the Chandra ACIS-S detector. We find the X-ray temperature of the cluster to be 10.4^{+1.7}_{-1.5} keV, slightly lower…

We present three observations (four exposures) of Mkn 421 performed by XMM--Newton in the Autumn of 2002, concentrating on the EPIC--PN camera data. The X-ray spectra were soft and steepening toward high energies. The source was highly…

Astrophysics · Physics 2009-11-10 M. Ravasio , G. Tagliaferri , G. Ghisellini , F. Tavecchio

The bright blazar Mkn 421 has been observed four times for uninterrupted durations of ~ 9 - 13 hr during the performance verification and calibration phases of the XMM-Newton mission. The source was strongly variable in all epochs, with…

Astrophysics · Physics 2009-11-07 S. Sembay , R. Edelson , A. Markowitz , R. G. Griffiths , M. J. L. Turner

We report the results of the {\it Chandra} ACIS-S observations of the elliptical galaxy NGC 821, which harbors a supermassive nuclear black hole (of $3.5 \times 10^7 M_{\odot}$), but does not show sign of AGN activity. A small,…

Astrophysics · Physics 2015-06-24 G. Fabbiano , A. Baldi , S. Pellegrini , A. Siemiginowska , M. Elvis , A. Zezas , J. McDowell

We have been monitoring M31 with HRC and ACIS onboard \chandra regularly in the past two years. By combining eight \chandra ACIS-I observations taken between 1999 to 2001, we have identified 204 X-ray sources within the central $\sim…

Astrophysics · Physics 2007-05-23 A. K. H. Kong , M. R. Garcia , F. A. Primini , R. Di Stefano , S. S. Murray

We report the results of the Chandra ACIS-S observations of the elliptical galaxy NGC 821, which harbors a supermassive nuclear black hole (of 3.5x10^7 solar masses), but does not show sign of AGN activity. A small, 8.5" long (~1 kpc at the…

Astrophysics · Physics 2007-05-23 A. Baldi , G. Fabbiano , S. Pellegrini , A. Siemiginowska , M. Elvis , A. Zezas , J. C. McDowell

We present a high resolution X-ray spectrum of the iron K bandpass in MCG-6-30-15 based on a 522 ksec observation with Chandra's High Energy Transmission Grating Spectrometer. The Chandra spectrum is consistent with the presence of a…

Astrophysics · Physics 2009-09-17 A. J. Young , J. C. Lee , A. C. Fabian , C. S. Reynolds , R. R. Gibson , C. R. Canizares

We report the first high-resolution X-ray spectra of two high-redshift quasars, S5 0836+710 and PKS 2149-306, obtained with the Chandra High Energy Transmission Grating Spectrometer (HETGS). The primary goal of this observation is to use…

Astrophysics · Physics 2009-11-06 T. Fang , H. L. Marshall , G. L. Bryan , C. R. Canizares

We report results from Chandra observations of the X-ray jet of 3C~273 during the calibration phase in 2000 January. The zeroeth-order images and spectra from two 40-ks exposures with the HETG and LETG+ACIS-S show a complex X-ray structure.…

Astrophysics · Physics 2009-11-06 Rita M. Sambruna , C. Megan Urry , F. Tavecchio , L. Maraschi , R. Scarpa , G. Chartas , T. Muxlow
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