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20022009
most citedCosmological Constraints from the SDSS Luminous Red Galaxies

1.4k citations

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41 papers · 1 filter

astro-ph2008115 cited

Detectability of Gravitational Waves from Phase Transitions

Tina Kahniashvili, Arthur Kosowsky, Grigol Gogoberidze +1

Gravitational waves potentially represent our only direct probe of the universe when it was less than one second old. In particular, first-order phase transitions in the early univ…

astro-ph200874 cited

Clustering properties of a sterile neutrino dark matter candidate

D. Boyanovsky

The clustering properties of sterile neutrinos are studied within an extension of the minimal standard model, where these are produced via the decay of a gauge singlet scalar. The…

astro-ph200833 cited

The dark matter transfer function: free streaming, particle statistics and memory of gravitational clustering

D. Boyanovsky, H. J. de Vega, N. Sanchez

The transfer function of dark matter (DM) perturbations during matter domination is obtained by solving the collisionless Boltzmann-Vlasov equation. We find an \emph{exact}…

astro-ph200876 cited

Faraday Rotation Limits on a Primordial Magnetic Field from WMAP Five-Year Data

Tina Kahniashvili, Yurii Maravin, Arthur Kosowsky

A primordial magnetic field in the early universe will cause Faraday rotation of the linear polarization of the cosmic microwave background generated via Compton scattering at the…

astro-ph2008311 cited

From Shock Breakout to Peak and Beyond: Extensive Panchromatic Observations of the Type Ib Supernova 2008D associated with Swift X-ray Transient 080109

Maryam Modjaz, W. Li, N. Butler +38

We present extensive early photometric (ultraviolet through near-infrared) and spectroscopic (optical and near-infrared) data on supernova (SN) 2008D as well as X-ray data analysis…

astro-ph200878 cited

The DEEP2 Galaxy Redshift Survey: Environments of Poststarburst Galaxies at z~0.1 and z~0.8

Renbin Yan, Jeffrey A. Newman, S. M. Faber +6

Postststarburst (K+A) galaxies are candidates for galaxies in transition from a star-forming phase to a passively-evolving phase. We have spectroscopically identified large samples…