output
19922026
most citedThe Seventh Data Release of the Sloan Digital Sky Survey

5.4k citations

Showing 2007 · astro-phShow all

26 papers · 2 filters

astro-ph2007★ 31 cited

The Subaru/XMM-Newton Deep Survey (SXDS) - V. Optically Faint Variable Object Survey

Tomoki Morokuma, Mamoru Doi, Naoki Yasuda +19

We present our survey for optically faint variable objects using multi-epoch (8-10 epochs over 2-4 years) -band imaging data obtained with Subaru Suprime-Cam over 0.918 deg…

astro-ph2007★ 607 cited

Constraining the Age-Activity Relation for Cool Stars: The SDSS DR5 Low-Mass Star Spectroscopic Sample

Andrew A. West, Suzanne L. Hawley, John J. Bochanski +5

We present a spectroscopic analysis of over 38,000 low-mass stars from the Sloan Digital Sky Survey (SDSS) Data Release 5 (DR5). Analysis of this unprecedentedly large sample confi…

astro-ph2007★ 220 cited

Thawing quintessence with a nearly flat potential

Robert J. Scherrer, A. A. Sen

The thawing quintessence model with a nearly flat potential provides a natural mechanism to produce an equation of state parameter, w, close to -1 today. We examine the behavior of…

astro-ph2007

The Monitor project: tracking the evolution of low mass and pre-main sequence stars

Suzanne Aigrain, Jonathan Irwin, Leslie Hebb +4

The Monitor project is a large-scale program of photometric and spectroscopic monitoring of young open clusters using telescopes at ESO and other observatories. Its primary goal is…

astro-ph2007★ 27 cited

Detection of strong activity in the eclipsing binary brown dwarf 2MASSJ05352184-0546085 - A possible explanation for the temperature reversal

A. Reiners, A. Seifahrt, K. G. Stassun +2

We show high resolution spectra of the eclipsing brown dwarf binary 2MASSJ05352184-0546085 taken at the two opposite radial velocity maxima. Comparisons of the TiO bands to model a…

astro-ph2007★ 71 cited

A New Determination of the High Redshift Type Ia Supernova Rates with the Hubble Space Telescope Advanced Camera for Surveys

N. Kuznetsova, K. Barbary, B. Connolly +27

We present a new measurement of the volumetric rate of Type Ia supernova up to a redshift of 1.7, using the Hubble Space Telescope (HST) GOODS data combined with an additional HST…

astro-ph2007★ 19 cited

Dirac Fields in Loop Quantum Gravity and Big Bang Nucleosynthesis

Martin Bojowald, Rupam Das, Robert J. Scherrer

Big Bang nucleosynthesis requires a fine balance between equations of state for photons and relativistic fermions. Several corrections to equation of state parameters arise from cl…

astro-ph2007★ 41 cited

The B and Be Star Population of NGC 3766

M. Virginia McSwain, Wenjin Huang, Douglas R. Gies +2

We present multiple epochs of H-alpha spectroscopy for 47 members of the open cluster NGC 3766 to investigate the long term variability of its Be stars. Sixteen of the stars in thi…

astro-ph2007★ 43 cited

A Photometric Survey for Variables and Transits in the Field of Praesepe with KELT

Joshua Pepper, K. Z. Stanek, Richard W. Pogge +5

The Kilodegree Extremely Little Telescope (KELT) project is a small aperture, wide-angle search for planetary transits of solar-type stars. In this paper, we present the results of…

astro-ph2007★ 39 cited

Discovery of Par 1802 as a Low-Mass, Pre-Main-Sequence Eclipsing Binary in the Orion Star-Forming Region

P. A. Cargile, K. G. Stassun, R. D. Mathieu

We report the discovery of a pre-main-sequence, low-mass, double-lined, spectroscopic, eclipsing binary in the Orion star-forming region. We present our observations including radi…

astro-ph2007★ 68 cited

Evidence for Accretion in the High-resolution X-ray Spectrum of the T Tauri Star System Hen 3-600

David P. Huenemoerder, Joel H. Kastner, Paola Testa +2

We present high-resolution X-ray spectra of the multiple T Tauri star system Hen 3-600, obtained with the High Energy Transmission Grating Spectrograph on the Chandra X-ray Observa…

astro-ph2007★ 126 cited

Gravitational Wave Recoil and the Retention of Intermediate Mass Black Holes

Kelly Holley-Bockelmann, Kayhan Gultekin, Deirdre Shoemaker +1

During the inspiral and merger of a binary black hole, gravitational radiation is emitted anisotropically due to asymmetries in the merger configuration. This anisotropic radiation…

astro-ph2007★ 52 cited

The Effect of Binarity on Stellar Rotation - Beyond the Reach of Tides

S. Meibom, R. D. Mathieu, K. G. Stassun

We present a comparison between the rotation period distributions of solar-type single stars and primary stars in close binaries (0.1 AU ~< a ~< 5 AU) in the young (150 Myr) open c…

astro-ph2007★ 50 cited

The Monitor project: JW 380 -- a 0.26, 0.15 Msol pre main sequence eclipsing binary in the Orion Nebula Cluster

Jonathan Irwin, Suzanne Aigrain, Simon Hodgkin +14

We report the discovery of a low-mass (0.26 +/- 0.02, 0.15 +/- 0.01 Msol) pre-main-sequence eclipsing binary with a 5.3 day orbital period. JW 380 was detected as part of a high-ca…

astro-ph2007★ 62 cited

The light curve of the companion to PSR B1957+20

Mark Reynolds, Paul Callanan, Andrew Fruchter +3

We present a new analysis of the light curve for the secondary star in the eclipsing binary millisecond pulsar system PSR B1957+20. Combining previous data and new data points at m…

astro-ph2007★ 83 cited

Periodic accretion from a circumbinary disk in the young binary UZ Tau E

Eric L. N. Jensen, Saurav Dhital, Keivan G. Stassun +6

Close pre-main-sequence binary stars are expected to clear central holes in their protoplanetary disks, but the extent to which material can flow from the circumbinary disk across…

astro-ph2007★ 111 cited

A Surprising Reversal of Temperatures in the Brown-Dwarf Eclipsing Binary 2MASS J05352184-0546085

Keivan G. Stassun, Robert D. Mathieu, Jeff A. Valenti

The newly discovered brown-dwarf eclipsing binary 2MASS J05352184-0546085 provides a unique laboratory for testing the predictions of theoretical models of brown-dwarf formation an…

astro-ph2007★ 57 cited

The Return of a Static Universe and the End of Cosmology

Lawrence M. Krauss, Robert J. Scherrer

We demonstrate that as we extrapolate the current CDM universe forward in time, all evidence of the Hubble expansion will disappear, so that observers in our "island universe" w…

astro-ph2007★ 64 cited

Quantitative comparison between Type Ia supernova spectra at low and high redshifts: A case study

G. Garavini, G. Folatelli, S. Nobili +44

We develop a method to measure the strength of the absorption features in Type Ia supernova (SN Ia) spectra and use it to make a quantitative comparison between the spectra of Type…

astro-ph2007★ 68 cited

The Weak Energy Condition and the Expansion History of the Universe

A. A. Sen, Robert J. Scherrer

We examine flat models containing a dark matter component and an arbitrary dark energy component, subject only to the constraint that the dark energy satisfies the weak energy cond…

astro-ph2007★ 71 cited

Stellar Kinematics in the Complicated Inner Spheroid of M31: Discovery of Substructure Along the Southeastern Minor Axis and its Relationship to the Giant Southern Stream

Karoline M. Gilbert, Mark Fardal, Jasonjot S. Kalirai +9

We present the discovery of a kinematically-cold stellar population along the SE minor axis of the Andromeda galaxy (M31) that is likely the forward continuation of M31's giant sou…

astro-ph2007★ 1 cited

Cosmic Deconstructionism

Lawrence M. Krauss, Glenn D. Starkman

Dark Matter that is composed of WIMP remnants of incomplete particle-antiparticle annihilation in the early universe experiences ongoing annihilation in gravitationally bound large…

astro-ph2007★ 8 cited

Radiation can never again dominate Matter in a Vacuum Dominated Universe

Lawrence M. Krauss, Robert J. Scherrer

We demonstrate that in a vacuum-energy-dominated expansion phase, surprisingly neither the decay of matter nor matter-antimatter annihilation into relativistic particles can ever c…

astro-ph2007★ 30 cited

A Simultaneous Optical and X-ray Variability Study of the Orion Nebula Cluster. II. A Common Origin in Magnetic Activity

K. G. Stassun, M. van den Berg, E. Feigelson

We present a statistical analysis of simultaneous optical and X-ray light curves, spanning 600 ks, for 814 pre-main-sequence (PMS) stars in the Orion Nebula Cluster. The aim of thi…