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We present a Chandra X-ray observation of G12.82-0.02, a shell-like radio supernova remnant coincident with the TeV gamma-ray source HESS J1813-178. We resolve the X-ray emission from the co-located ASCA source into a point source…

Pulsar wind nebula DA~495 (G65.7+1.2) has been extensively observed from radio to TeV $\gamma$-ray bands. We present LHAASO observations of DA~495, revealing an energy-dependent morphology, where an extended source with…

High Energy Astrophysical Phenomena · Physics 2026-01-19 The LHAASO Collaboration

We report an observation of X-ray emission from the exciting region of Cepheus A with the Chandra/ACIS instrument. What had been an unresolved X-ray source comprising the putative power sources is now resolved into at least 3 point-like…

Astrophysics of Galaxies · Physics 2014-11-20 S. H. Pravdo , Y. Tsuboi , A. Uzawa , Y. Ezoe

On 4 July 2001, X-rays from Mars were detected for the first time. The observation was performed with the ACIS-I detector onboard Chandra and yielded data of high spatial and temporal resolution, together with spectral information. Mars is…

Astrophysics · Physics 2009-11-07 Konrad Dennerl

We report on high-resolution spatial and timing observations of the millisecond pulsar PSR J0218+4232 performed with the Chandra X-ray Observatory (CXO) and the Rossi X-ray Timing Explorer (RXTE). With these observations we were able to…

Astrophysics · Physics 2009-11-10 L. Kuiper , W. Hermsen , B. Stappers

We present results from deep (70 ks) Chandra ACIS observations and Hubble Space Telescope ACS F475W observations of two highly optically polarized quasars belonging to the MOJAVE blazar sample, viz., PKS B0106+013 and 1641+399 (3C345).…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-03 Preeti Kharb , Matthew Lister , Herman Marshall , Brandon Hogan

We report the first detection of radio emission from any anomalous X-ray pulsar (AXP). Data from the Very Large Array (VLA) MAGPIS survey with angular resolution 6" reveals a point-source of flux density 4.5 +/- 0.5 mJy at 1.4 GHz at the…

Astrophysics · Physics 2009-11-13 J. P. Halpern , E. V. Gotthelf , R. H. Becker , D. J. Helfand , R. L. White

We discover an unidentified strong emission feature in the X-ray spectrum of EXO 1745$-$248 obtained by RXTE at 40 hr after the peak of a superburst. The structure was centered at 6.6 keV and significantly broadened with a large equivalent…

High Energy Astrophysical Phenomena · Physics 2021-09-08 Wataru B. Iwakiri , Motoko Serino , Tatehiro Mihara , Liyi Gu , Hiroya Yamaguchi , Megumi Shidatsu , Kazuo Makishima

We report on the discovery of a new pulsating X-ray source during Rossi X-ray Timing Explorer observations of a low galactic latitude field centered at RA (J2000) = 19 hr 05 m 43 s and Dec (J2000) = +08 deg 58 arcmin 48 arcsec. Significant…

Astrophysics · Physics 2009-10-30 D. Marsden , D. E. Gruber , W. A. Heindl , M. R. Pelling , R. E. Rothschild

We have conducted a radio study at 3.6, 6 and 20 cm using ATCA and VLA and reprocessed XMM-Newton and Chandra data of the pulsar wind nebula (PWN) in the supernova remnant (SNR) G0.9+0.1. The new observations revealed that the morphology…

Astrophysics · Physics 2009-11-13 Gloria Dubner , Elsa Giacani , Anne Decourchelle

We report the discovery of pulsed X-ray emission from the compact object CXOU J112439.1-591620 within the supernova remnant (SNR) G292.0+1.8 using the High Resolution Camera on the Chandra X-ray Observatory. The X-ray period (P=0.13530915…

We report the discovery with the EPIC CCD cameras onboard XMM-Newton of a 54 mHz quasiperiodic oscillation (QPO) in the > 2 keV X-ray flux from an ultraluminous X-ray source (ULX) in the starburst galaxy M82. This is the first detection of…

Astrophysics · Physics 2009-11-07 Tod E. Strohmayer , Richard F. Mushotzky

The anomalous X-ray pulsars (AXPs) represent a growing class of neutron stars discovered at X-ray energies. While the nature of their multi-wavelength emission mechanism is still under debate, evidence has been recently accumulating in…

Astrophysics · Physics 2009-11-10 Samar Safi-Harb , Jennifer West

We have searched the entire ROSAT archive for useful observations to study X-ray emission from Galactic planetary nebulae (PNs). The search yields a sample of 63 PNs, which we call the ROSAT PN sample. About 20-25% of this sample show X-ray…

Astrophysics · Physics 2009-10-31 Martin A. Guerrero , You-Hua Chu , Robert A. Gruendl

We report the discovery of 70.5 ms pulsations from the X-ray source AX J1838.0-0655 using the Rossi X-ray Timing Explorer (RXTE). PSR J1838-0655 is a rotation-powered pulsar with spin-down luminosity Edot = 5.5e36 ergs/s, characteristic age…

Astrophysics · Physics 2009-11-13 E. V. Gotthelf , J. P. Halpern

In this short paper, we study the photometric precision of stellar light curves obtained by the CoRoT satellite in its planet finding channel, with a particular emphasis on the timescales characteristic of planetary transits. Together with…

XMM-Newton and Chandra observations of the transient 7.8 s pulsar XTE J1829-098 are used to characterize its pulse shape and spectrum, and to facilitate a search for an optical or infrared counterpart. In outburst, the absorbed, hard X-ray…

Astrophysics · Physics 2009-11-13 J. P. Halpern , E. V. Gotthelf

We report on spectral and timing observations of the nearest millisecond pulsar J0437-4715 with Chandra. The pulsar spectrum, detected up to 7 keV, cannot be described by a simple one-component model. We suggest that it consists of two…

Astrophysics · Physics 2009-11-07 V. E. Zavlin , G. G. Pavlov , D. Sanwal , R. N. Manchester , J. Truemper , J. P. Halpern , W. Becker

We report X-ray imaging, timing, and spectral studies of XTE J1810-197, a 5.54s pulsar discovered by Ibrahim et al. (2003) in recent RXTE observations. In a set of short exposures with the Chandra HRC camera we detect a strongly modulated…

Astrophysics · Physics 2009-11-10 E. V. Gotthelf , J. P. Halpern , M. Buxton , C. Bailyn

We present the results from an investigation of the energy dependence of Quasi-Periodic Oscillations (QPOs) exhibited by accreting X-ray pulsars using data from archival \textit{XMM-Newton}, \textit{NuSTAR}, \textit{RXTE}, and…

High Energy Astrophysical Phenomena · Physics 2024-05-01 Hemanth Manikantan , Biswajit Paul , Rahul Sharma , Pragati Pradhan , Vikram Rana
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