Showing 2010 · astro-ph.HEShow all

81 papers · 2 filters

astro-ph.HE2010★ 61 cited

The Optical Afterglow and z=0.92 Early-type Host Galaxy of the Short GRB 100117A

Wen-fai Fong, Edo Berger, Ryan Chornock +6

We present the discovery of the optical afterglow and early-type host galaxy of the short-duration GRB 100117A. The faint afterglow is detected 8.3 hr after the burst with r_AB = 2…

astro-ph.HE2010★ 102 cited

Spectral Energy Distribution of Markarian 501: Quiescent State vs. Extreme Outburst

The VERITAS Collaboration, V. A. Acciari, T. Arlen +225

The very high energy (VHE; E > 100 GeV) blazar Markarian 501 has a well-studied history of extreme spectral variability and is an excellent laboratory for studying the physical pro…

astro-ph.HE2010★ 172 cited

Time-Integrated Searches for Point-like Sources of Neutrinos with the 40-String IceCube Detector

The IceCube Collaboration, R. Abbasi

We present the results of time-integrated searches for astrophysical neutrino sources in both the northern and southern skies. Data were collected using the partially-completed Ice…

astro-ph.HE2010★ 19 cited

Ultraviolet and X-ray Variability of the Seyfert 1.5 Galaxy Markarian 817

Lisa M. Winter, Charles Danforth, Ranjan Vasudevan +9

We present an investigation of the ultraviolet and X-ray spectra of the Seyfert 1.5 galaxy Markarian 817. The ultraviolet analysis includes two recent observations taken with the C…

astro-ph.HE2010★ 23 cited

Confirmation of the Supergiant Fast X-ray Transient nature of AX J1841.0-0536 from Swift outburst observations

P. Romano, V. Mangano, G. Cusumano +8

Swift observed an outburst from the supergiant fast X-ray transients (SFXT) AX J1841.0-0536 on 2010 June 5, and followed it with XRT for 11 days. The X-ray light curve shows an ini…

astro-ph.HE2010★ 267 cited

Detection of a Thermal Spectral Component in the Prompt Emission of GRB 100724B

Sylvain Guiriec, Valerie Connaughton, Michael S. Briggs +29

Observations of GRB 100724B with the Fermi Gamma-Ray Burst Monitor (GBM) find that the spectrum is dominated by the typical Band functional form, which is usually taken to represen…

astro-ph.HE2010★ 126 cited

The Super-Soft X-ray Phase of Nova RS Ophiuchi 2006

J. P. Osborne, K. L. Page, A. P. Beardmore +13

Swift X-ray observations of the ~60 day super-soft phase of the recurrent nova RS Ophiuchi 2006 show the progress of nuclear burning on the white dwarf in exquisite detail. First s…

astro-ph.HE2010★ 239 cited

Insights Into the High-Energy Gamma-ray Emission of Markarian 501 from Extensive Multifrequency Observations in the Fermi Era

LAT collaboration, A. A. Abdo et al., the MAGIC collaboration +6

We report on the gamma-ray activity of the blazar Mrk 501 during the first 480 days of Fermi operation. We find that the average LAT gamma-ray spectrum of Mrk 501 can be well descr…

astro-ph.HE2010★ 105 cited

Search for a Lorentz-violating sidereal signal with atmospheric neutrinos in IceCube

IceCube Collaboration, R. Abbasi, Y. Abdou +258

A search for sidereal modulation in the flux of atmospheric muon neutrinos in IceCube was performed. Such a signal could be an indication of Lorentz-violating physics. Neutrino osc…

astro-ph.HE2010★ 66 cited

Photometric redshifts for GRB afterglows from GROND and Swift/UVOT

T. Krühler, P. Schady, J. Greiner +18

We present a framework to obtain photometric redshifts (photo-zs) for gamma-ray burst afterglows. Using multi-band photometry from GROND and Swift/UVOT, photo-zs are derived for fi…

astro-ph.HE2010★ 87 cited

Multi-wavelength Observations of the Flaring Gamma-ray Blazar 3C 66A in 2008 October

LAT collaboration, A. A. Abdo et al., the VERITAS collaboration +4

The BL Lacertae object 3C 66A was detected in a flaring state by the Fermi Large Area Telescope (LAT) and VERITAS in 2008 October. In addition to these gamma-ray observations, F-GA…

astro-ph.HE2010★ 43 cited

Chandra Observations of the High-Magnetic-Field Radio Pulsar J1718-3718

W. W. Zhu, V. M. Kaspi, M. A. McLaughlin +5

High-magnetic-field pulsars represent an important class of objects for studying the relationship between magnetars and radio pulsars. Here we report on four Chandra observations o…

astro-ph.HE2010★ 114 cited

Search for Gravitational Wave Bursts from Six Magnetars

J. Abadie, B. P. Abbott, R. Abbott +765

Soft gamma repeaters (SGRs) and anomalous X-ray pulsars (AXPs) are thought to be magnetars: neutron stars powered by extreme magnetic fields. These rare objects are characterized b…

astro-ph.HE2010★ 57 cited

On the Implications of Late Internal Dissipation for Shallow-Decay Afterglow Emission and Associated High-Energy Gamma-Ray Signals

Kohta Murase, Kenji Toma, Ryo Yamazaki +1

The origin of the shallow-decay emission during early X-ray afterglows has been an open issue since the launch of the Swift satellite. One of the appealing models is the late inter…

astro-ph.HE2010★ 27 cited

A Statistical Comparison of the Optical/UV and X-ray Afterglows of Gamma-Ray Bursts using the Swift Ultra-violet Optical and X-ray Telescopes

S. R. Oates, M. J. Page, P. Schady +11

We present the systematic analysis of the UVOT and XRT light curves for a sample of 26 Swift Gamma-Ray Bursts (GRBs). By comparing the optical/UV and X-ray light curves, we found t…

astro-ph.HE2010★ 30 cited

The quasar PG 0844+349 in an X-ray weak state

L. C. Gallo, D. Grupe, N. Schartel +4

In March 2009 the well-studied quasar, PG 0844+349, was discovered with Swift to be in an X-ray weak state. A follow-up XMM-Newton observation several weeks later generated a good…

astro-ph.HE2010★ 82 cited

The first gamma-ray outburst of a Narrow-Line Seyfert 1 Galaxy: the case of PMN J0948+0022 in July 2010

L. Foschini, G. Ghisellini, Y. Y. Kovalev +24

We report on a multiwavelength campaign on the radio-loud Narrow-Line Seyfert 1 (NLS1) Galaxy PMN J0948+0022 (z=0.5846) performed in 2010 July-September and triggered by a high-ene…

astro-ph.HE2010★ 197 cited

Measurement of the atmospheric neutrino energy spectrum from 100 GeV to 400 TeV with IceCube

IceCube Collaboration, R. Abbasi, Y. Abdou +258

A measurement of the atmospheric muon neutrino energy spectrum from 100 GeV to 400 TeV was performed using a data sample of about 18,000 up-going atmospheric muon neutrino events i…

astro-ph.HE2010★ 45 cited

Prompt X-ray and Optical Excess Emission due to Hadronic Cascades in Gamma-Ray Bursts

Katsuaki Asano, Susumu Inoue, Peter Meszaros

A fraction of gamma-ray bursts exhibit distinct spectral features in their prompt emission below few 10s of keV that exceed simple extrapolations of the low-energy power-law portio…

astro-ph.HE2010★ 18 cited

Searching for compact objects in SNRs G27.8+0.6 and G28.8+1.5

Zdenka Misanovic, Oleg Kargaltsev, George G. Pavlov

We analyzed XMM-Newton observations of two center-filled supernova remnants, G27.8+0.6 and G28.8+1.5, to search for pulsars/pulsar wind nebulae (PWNe) and other types of neutron st…

astro-ph.HE2010★ 68 cited

On Relativistic Disk Spectroscopy in Compact Objects with X-ray CCD Cameras

J. M. Miller, A. D'Ai, M. W. Bautz +11

X-ray charge-coupled devices (CCDs) are the workhorse detectors of modern X-ray astronomy. Typically covering the 0.3-10.0 keV energy range, CCDs are able to detect photoelectric a…

astro-ph.HE2010★ 34 cited

Two years of monitoring Supergiant Fast X-ray Transients with Swift

P. Romano, V. La Parola, S. Vercellone +10

We present two years of intense Swift monitoring of three SFXTs, IGR J16479-4514, XTE J1739-302, and IGR J17544-2619 (since October 2007). Out-of-outburst intensity-based X-ray (0.…

astro-ph.HE2010★ 1 cited

Relativistic jets in Narrow-Line Seyfert 1

L. Foschini, E. Angelakis, G. Bonnoli +20

Narrow-Line Seyfert 1 (NLS1) class of active galactic nuclei (AGNs) is generally radio-quiet, but a small percent of them are radio-loud. The recent discovery by Fermi/LAT of high-…

astro-ph.HE2010★ 104 cited

A Tidal Disruption Flare in Abell 1689 from an Archival X-ray Survey of Galaxy Clusters

Peter Maksym, Melville P. Ulmer, Michael Eracleous

Theory suggests that a star making a close passage by a supermassive black hole at the center of a galaxy can under most circumstances be expected to emit a giant flare of radiatio…