output
19922026
most citedLSST: from Science Drivers to Reference Design and Anticipated Data Products

3.5k citations

Showing 2013Show all

129 papers · 1 filter

astro-ph.HE2013★ 86 cited

A Three-Year Multi-Wavelength Study of the Very High Energy Gamma-ray Blazar 1ES 0229+200

E. Aliu, S. Archambault, T. Arlen +83

The high-frequency-peaked BL Lacertae object 1ES 0229+200 is a relatively distant (z = 0.1396), hard-spectrum (Gamma ~ 2.5), very-high-energy-emitting (E > 100 GeV) gamma-ray blaza…

astro-ph.IM2013★ 28 cited

Calibrating Data from the Hinode/X-Ray Telescope and Associated Uncertainties

Adam R. Kobelski, Steven H. Saar, Mark A. Weber +2

The X-Ray Telescope (XRT) onboard the Hinode satellite, launched 23 September 2006 by the Japanese Aerospace Exploration Agency (JAXA) is a joint mission between Japan, the United…

astro-ph.SR2013★ 30 cited

SDSS J074511.56+194926.5: Discovery of a Metal-Rich and Tidally Distorted Extremely Low Mass White Dwarf

A. Gianninas, J. J. Hermes, Warren R. Brown +5

We present the discovery of an unusual, tidally-distorted extremely low mass white dwarf (WD) with nearly solar metallicity. Radial velocity measurements confirm that this is a com…

astro-ph.HE2013★ 15 cited

Variable Doppler shifts of the thermal wind absorption lines in low-mass X-ray binaries

O. K. Madej, P. G. Jonker, M. Diaz Trigo +1

In this paper we address the general applicability of the method pioneered by \citet{Zhang2012} in which the motion of the compact object can be tracked using wind X-ray absorption…

astro-ph.IM2013★ 180 cited

Micro-Arcsecond Radio Astrometry

M. J. Reid, M. Honma

Astrometry provides the foundation for astrophysics. Accurate positions are required for the association of sources detected at different times or wavelengths, and distances are es…

astro-ph.GA2013★ 7 cited

The variable ionized absorber in the Seyfert 2 Mrk 348

E. Marchese, V. Braito, J. N Reeves +6

We present the results of the analysis of the X-ray spectrum of the Seyfert 2 Mrk 348, observed by Suzaku and XMM-Newton. The overall spectrum of Mrk 348 can be described by a prim…