output
19972026
most citedThe Eleventh and Twelfth Data Releases of the Sloan Digital Sky Survey: Final Data from SDSS-III

2.5k citations

Showing 2001Show all

10 papers · 1 filter

astro-ph2001★ 60 cited

Modelling of surface magnetic field in neutron stars: application to radio pulsars

Janusz A. Gil, George I. Melikidze, Dipanjan Mitra

We propose a vacuum gap (VG) model which can be applied uniformly for normal and high magnetic field pulsars. The model requires strong and non-dipolar surface magnetic field near…

astro-ph2001★ 309 cited

Gravitational Radiation From Cosmological Turbulence

Arthur Kosowsky, Andrew Mack, Tinatin Kahniashvili

An injection of energy into the early Universe on a given characteristic length scale will result in turbulent motions of the primordial plasma. We calculate the stochastic backgro…

astro-ph2001★ 10 cited

Abundance and evolution of galaxy clusters in cosmological models with massive neutrino

N. A. Arhipova, T. Kahniashvili, V. N. Lukash

The time evolution of the number density of galaxy clusters and their mass and temperature functions are used to constrain cosmological parameters in the spatially flat dark matter…

astro-ph2001★ 196 cited

Optical and radio variability of the BL Lac object AO 0235+16: a possible 5-6 year periodicity

C. M. Raiteri, M. Villata, H. D. Aller +33

New optical and radio data on the BL Lacertae object AO 0235+16 have been collected in the last four years by a wide international collaboration, which confirm the intense activity…

astro-ph2001★ 65 cited

Intermediate resolution H-beta spectroscopy and photometric monitoring of 3C 390.3 I. Further evidence of a nuclear accretion disk

A. I. Shapovalova, A. N. Burenkov, L. Carrasco +13

We have monitored the AGN 3C390.3 between 1995 and 2000.Two large amplitude outbursts, of different duration, in continuum and H beta light were observed ie.: in October 1994 a bri…

astro-ph2001

Evolution of galaxy clusters in MDM cosmologies

N. A. Arkhipova, T. Kahniashvili, V. N. Lukash

The time evolution of galaxy cluster abundance is used to constrain cosmological parameters in dark matter models containing a fraction of hot particles (massive neutrino). We test…

astro-ph2001★ 68 cited

Day-Scale Variability of 3C 279 and Searches for Correlations in Gamma-Ray, X-Ray, and Optical Bands

R. C. Hartman, M. Villata, T. J. Balonek +36

Light curves of 3C 279 are presented in optical (R-band), X-rays (RXTE/PCA), and gamma rays (CGRO/EGRET) for 1999 Jan-Feb and 2000 Jan-Mar. During both of those epochs the gamma-ra…

astro-ph2001★ 210 cited

Microwave Background Signatures of a Primordial Stochastic Magnetic Field

Andrew Mack, Tina Kahniashvili, Arthur Kosowsky

A stochastic magnetic field in the early Universe will produce anisotropies in the temperature and polarization of the cosmic microwave background. We derive analytic expressions f…

astro-ph2001★ 142 cited

Multi-Epoch Multiwavelength Spectra and Models for Blazar 3C~279

R. C. Hartman, M. Boettcher

Of the blazars detected by EGRET in GeV gamma rays, 3C 279 is not only the best-observed by EGRET, but also one of the best-monitored at lower frequencies. We have assembled eleven…

astro-ph2001★ 14 cited

On the age of PSR B1509-58

V. V. Gvaramadze

It is generally accepted that the PSR B1509-58 is associated with the supernova remnant (SNR) MSH 15-52 (G 320.4-01.2). The spin-down age of the pulsar is \simeq 1700 years, while…