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astro-ph2009★ 44 cited

Swift-UVOT captures the earliest ultraviolet spectrum of a Gamma Ray Burst

N. P. M. Kuin, W. B. Landsman, M. J. Page +22

We present the earliest ever ultraviolet spectrum of a gamma-ray burst (GRB) as observed with the Swift-UVOT. The GRB 081203A spectrum was observed for 50 seconds with the UV grism…

astro-ph2008★ 7 cited

Search for Primordial Black Holes with SGARFACE

M. Schroedter, F. Krennrich, S. LeBohec +7

The Short GAmma Ray Front Air Cherenkov Experiment (SGARFACE) uses the Whipple 10 m telescope to search for bursts of rays. SGARFACE is sensitive to bursts with duration from a…

astro-ph2008★ 36 cited

Black Hole Spins of Radio Sources

Ruth A. Daly

A new approach to constraining or determining the spin of a massive black hole is proposed. A key parameter in the analysis is the dimensionless ratio, r, of the energy released to…

astro-ph2008★ 834 cited

Constraints on a phenomenologically parameterized neutron-star equation of state

Jocelyn S. Read, Benjamin D. Lackey, Benjamin J. Owen +1

We introduce a parameterized high-density equation of state (EOS) in order to systematize the study of constraints placed by astrophysical observations on the nature of neutron-sta…

astro-ph2008★ 52 cited

The Young, Massive, Star Cluster Sandage-96 After the Explosion of SN 2004dj in NGC 2403

J. Vinko, K. Sarneczky, Z. Balog +12

The bright Type II-plateau supernova (SN) 2004dj occurred within the young, massive stellar cluster Sandage-96 in a spiral arm of NGC 2403. New multi-wavelength observations obtain…

astro-ph2008★ 60 cited

Discovery of Very High-Energy Gamma-Ray Radiation from the BL Lac 1ES 0806+524

VERITAS Collaboration, V. Acciari, E. Aliu +90

The high-frequency-peaked BL-Lacertae object \objectname{1ES 0806+524}, at redshift z=0.138, was observed in the very-high-energy (VHE) gamma-ray regime by VERITAS between November…

astro-ph2008★ 310 cited

Jet breaks and Energetics of Swift GRB X-ray Afterglows

J. L. Racusin, E. W. Liang, D. N. Burrows +6

We present a systematic temporal and spectral study of all Swift-XRT observations of GRB afterglows discovered between 2005 January and 2007 December. After constructing and fittin…

astro-ph2008★ 1.8k cited

Methods and results of an automatic analysis of a complete sample of Swift-XRT observations of GRBs

P. A. Evans, A. P. Beardmore, K. L. Page +22

We present a homogeneous X-ray analysis of all 318 Gamma Ray Bursts detected by the X-ray Telescope on the Swift satellite up to 2008 July 23; this represents the largest sample of…

astro-ph2008★ 170 cited

Statistical Properties of Gamma-Ray Burst Polarization

Kenji Toma, Takanori Sakamoto, Bing Zhang +6

The emission mechanism and the origin and structure of magnetic fields in gamma-ray burst (GRB) jets are among the most important open questions concerning the nature of the centra…

astro-ph2008★ 50 cited

Late time observations of GRB080319B: jet break, host galaxy and accompanying supernova

Nial R. Tanvir, Evert Rol, Andrew Levan +15

The Swift discovered GRB080319B was by far the most distant source ever observed at naked eye brightness, reaching a peak apparent magnitude of 5.3 at a redshift of z=0.937. We pre…

astro-ph2008★ 5.4k cited

The Seventh Data Release of the Sloan Digital Sky Survey

K. Abazajian

This paper describes the Seventh Data Release of the Sloan Digital Sky Survey (SDSS), marking the completion of the original goals of the SDSS and the end of the phase known as SDS…

astro-ph2008★ 10 cited

Impact of star formation inhomogeneities on merger rates and interpretation of LIGO results

R. O'Shaughnessy, R. Kopparapu, K. Belczynski

Within the next decade, ground based gravitational wave detectors are in principle capable of determining the compact object merger rate per unit volume of the local universe to be…

astro-ph2008★ 61 cited

Modelling the spectral response of the Swift-XRT CCD camera: Experience learnt from in-flight calibration

O. Godet, A. P. Beardmore, A. F. Abbey +11

(Abbreviated) We show that the XRT spectral response calibration was complicated by various energy offsets in photon counting (PC) and windowed timing (WT) modes related to the way…

astro-ph2008★ 25 cited

The AGN nature of three INTEGRAL sources: IGR J18249-3243, IGR J19443+2117 and IGR J22292+6647

R. Landi, J. B. Stephen, N. Masetti +6

The third INTEGRAL/IBIS survey has revealed several new hard X-ray sources, which are still unclassified. To identify these sources, we need to find their counterparts at other wav…

astro-ph2008★ 175 cited

A Golden Standard Type Ia Supernova SN 2005cf: Observations from the Ultraviolet to the Near-Infrared Wavebands

Xiaofeng Wang, Weidong Li, Alexei V. Filippenko +31

We present extensive photometry at ultraviolet (UV), optical, and near-infrared (NIR) wavelengths, as well as dense sampling of optical spectra, for the normal type Ia supernova (S…

astro-ph2008★ 96 cited

An Energetic AGN Outburst Powered by a Rapidly Spinning Supermassive Black Hole or an Accreting Ultramassive Black Hole

B. R. McNamara, F. Kazemzadeh, D. A. Rafferty +4

Powering the 10^62 erg nuclear outburst in the MS0735.6+7421 cluster central galaxy by accretion implies that its supermassive black hole (SMBH) grew by ~6x10^8 solar masses over t…

astro-ph2008★ 25 cited

Testing the Possible Intrinsic Origin of the Excess of Very Strong MgII Absorbers Along GRB Lines-of-Sight

A. Cucchiara, T. Jones, J. C. Charlton +3

The startling discovery of Prochter et al. (2006) that the frequency of very strong (W_r(2796)>1 A) MgII absorbers along gamma-ray burst (GRB) lines of sight ([dN/dz]_{GRB} = 0.90)…

astro-ph2008★ 32 cited

LISA detection of massive black hole binaries: imprint of seed populations and of exterme recoils

A. Sesana, M. Volonteri, F. Haardt

All the physical processes involved in the formation, merging, and accretion history of massive black holes along the hierarchical build--up of cosmic structures are likely to leav…

astro-ph2008★ 1 cited

Swift monitoring of Supergiant Fast X-ray Transients: the out-of-outburst behaviour and the flares from IGRJ17544-2916 and XTEJ1739-302

L. Sidoli, P. Romano, G. Cusumano +10

Supergiant Fast X-ray Transients (SFXTs) are a sub-class of High Mass X-ray Binaries (HMXBs) associated with OB supergiant companions and displaying transient X-ray activity. This…

astro-ph2008★ 56 cited

High-Resolution X-ray Spectroscopy of SNR 1987A: Chandra LETG and HETG Observations in 2007

Svetozar A. Zhekov, Richard McCray, Daniel Dewey +4

We present an extended analysis of the deep Chandra LETG and HETG observations of the supernova remnant 1987A (SNR 1987A) carried out in 2007. The global fits to the grating spectr…

astro-ph2008★ 34 cited

Nonthermal X-Rays from Supernova Remnant G330.2+1.0 and the Characteristics of its Central Compact Object

Sangwook Park, Oleg Kargaltsev, George G. Pavlov +5

We present results from our X-ray data analysis of the SNR G330.2+1.0 and its CCO, CXOU J160103.1--513353 (J1601). Using our XMM-Newton and Chandra observations, we find that the X…

astro-ph2008★ 132 cited

The 2dF-SDSS LRG and QSO Survey: The spectroscopic QSO catalogue

Scott M. Croom, Gordon T. Richards, Tom Shanks +27

We present the final spectroscopic QSO catalogue from the 2dF-SDSS LRG and QSO (2SLAQ) Survey. This is a deep, 18<g<21.85 (extinction corrected), sample aimed at probing in detail…

astro-ph2008★ 11 cited

Results from Seven Years of AMANDA-II

Tyce DeYoung

AMANDA is a first-generation high energy neutrino telescope, which has taken data at the South Pole in its final configuration since 2000. Results from seven years of operation are…

astro-ph2008★ 31 cited

Ejection of hypervelocity binary stars by a black hole of intermediate mass orbiting Sgr A*

A. Sesana, P. Madau, F. Haardt

The discovery of hypervelocity binary stars (HVBs) in the Galactic halo would provide definite evidence of the existence of a massive black hole companion to Sgr A*. Here we use an…