Showing 2001 · astro-phShow all

29 papers · 2 filters

astro-ph2001★ 1 cited

High-Energy Gamma Rays from Neutron Stars in Supernova Remnants: From EGRET to GLAST

D. J. Thompson, S. W. Digel, P. L. Nolan +1

At least three pulsars in supernova remnants were detected at E > 100 MeV by EGRET on the Compton Gamma Ray Observatory. Efforts to search for additional pulsars in the EGRET data…

astro-ph2001

New Statistical Methods for Analysis of Large Surveys: Distributions and Correlations

Vahe' Petrosian

The aim of this paper is to describe new statistical methods for determination of the correlations among and distributions of physical parameters from a multivariate data with gene…

astro-ph2001★ 147 cited

Looptop Hard X-Ray Emission in Solar Flares: Images and Statistics

Vahe' Petrosian, Timothy Q. Donaghy, James M. McTiernan

The discovery of hard X-ray sources near the top of a flaring loop by the HXT instrument on board the YOHKOH satellite represents a significant progress towards the understanding o…

astro-ph2001★ 3 cited

Experimental CMB Status and Prospects: A Report from Snowmass 2001

S. Staggs, S. Church

In recent years the promise of experimental study of the cosmic microwave background (CMB) has been demonstrated. Herein a brief summary of the field is followed by an indication o…

astro-ph2001★ 2 cited

CMB and Inflation: the report from Snowmass 2001

S. Church, A. Jaffe, L. Knox

Astrophysical observations provide the best evidence of physics beyond the particle physicists' standard model. Over the past decade, the case has solidified for inflation, dark en…

astro-ph2001★ 40 cited

The Munich Near-Infrared Cluster Survey (MUNICS) - Number density evolution of massive field galaxies to z ~ 1.2 as derived from the K-band selected survey

N. Drory, R. Bender, J. Snigula +5

We derive the number density evolution of massive field galaxies in the redshift range 0.4 < z < 1.2 using the K-band selected field galaxy sample from the Munich Near-IR Cluster S…