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Dealing with the RFI Environment at Arecibo Observatory
British Library Conference Proceedings | 1998| -
THE DIPOLE ANISOTROPY OF THE FIRST ALL-SKY X-RAY CLUSTER SAMPLE
British Library Online Contents | 2004| -
The Dipole Anisotropy of the First All-Sky X-ray Cluster Sample
British Library Conference Proceedings | 2005| -
XMM-Newton Observations of CIZA J1324.7-5736 - A Massive, Newly Discovered Galaxy Cluster in the Great Attractor Region
British Library Conference Proceedings | 2005| -
The X-ray Properties of Moderate-redshift Galaxy Groups Selected by Association with Gravitational Lenses
Free accessArXiv | 2007| -
The X-Ray Properties of Moderate-Redshift Galaxy Groups Selected by Association with Gravitational Lenses
Online Contents | 2008|Contributors: Kocevski, D. D. -
The mass distribution of a moderate redshift galaxy group and brightest group galaxy from gravitational lensing and kinematics
Oxford University Press | 2010| -
The mass distribution of a moderate redshift galaxy group and brightest group galaxy from gravitational lensing and kinematics
British Library Online Contents | 2010| -
Observational constraints on the physics behind the evolution of AGN since z ~ 1
Free accessArXiv | 2011| -
Observational constraints on the physics behind the evolution of active galactic nuclei since z- 1
British Library Online Contents | 2011| -
X-ray selected AGN Hosts are Similar to Inactive Galaxies out to z=3: Results from CANDELS/CDF-S
Free accessArXiv | 2011| -
CANDELS Observations of the Structural Properties and Evolution of Galaxies in a Cluster at z=1.62
Free accessArXiv | 2011| -
Observational constraints on the physics behind the evolution of active galactic nuclei since z∼ 1
Online Contents | 2011|Contributors: Kocevski, D. D. -
Extreme Emission Line Galaxies in CANDELS: Broad-Band Selected, Star-Bursting Dwarf Galaxies at z>1
Free accessArXiv | 2011| -
EXTREME EMISSION-LINE GALAXIES IN CANDELS: BROADBAND-SELECTED, STARBURSTING DWARF GALAXIES AT z > 1 111
Online Contents | 2011|Contributors: Kocevski, D D
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