LogN–LogS Studies of EGRET Sources
نویسنده
چکیده
A comprehensive investigation of logN–logS distributions of gamma-ray sources discovered by EGRET has been performed for subsequent use in population studies. Existing models explaining the spatial arrangement of unidentified sources do not compare against an observed logN–logS distribution. However, viable population models not only have to reproduce the logN–logS distribution for different source classes globally, they have to correspond to apparent differences among their spatial, spectral and variability characteristics. Furthermore, it needs to be understood in which way results from selections among the unidentified sources like ”persistent” (Grenier, 2000) or ”steady” sources (Gehrels et al., 2000) are related to the overall picture regarding their logN–logS characteristics.
منابع مشابه
Cosmological Implications of Number Counts of Clusters of Galaxies: logN–logS in X-Ray and Submm Bands
We compute the number counts of clusters of galaxies, the logN–logS relation, in several X-ray and submm bands on the basis of the Press-Schechter theory. We pay particular attention to a set of theoretical models which well reproduce the ROSAT 0.52 keV band logN–logS, and explore possibilities to further constrain the models from future observations with ASCA and/or at submm bands. The latter ...
متن کاملProperties of the Chandra Sources in M81
The Chandra X-ray Observatory obtained a 50-ks observation of the central region of M81 using the ACIS-S in imaging mode. The global properties of the 97 x-ray sources detected in the inner 8.3× 8.3 field of M81 are examined. Roughly half the sources are concentrated within the central bulge. The remainder are distributed throughout the disk with the brightest disk sources lying preferentially ...
متن کاملPulsars and Their Nebulae as EGRET Sources
At the end of the EGRET mission, only 6-8 Galactic sources had been identified as young pulsars. Since then, several energetic pulsars have been discovered in EGRET error boxes along the Galactic plane, as well as several pulsar wind nebulae from which pulsations have not yet been discovered. Some of these nebulae are associated with moderately variable EGRET sources, suggesting that the γ-ray ...
متن کاملPWN in EGRET Error Boxes
A remarkable number of pulsar wind nebulae (PWN) are coincident with EGRET γ-ray sources. X-ray and radio imaging studies of unidentified EGRET sources have resulted in the discovery of at least 6 new pulsar wind nebulae (PWN). Stationary PWN (SPWN) appear to be associated with steady EGRET sources with hard spectra, typical for γ-ray pulsars. Their toroidal morphologies can help determine the ...
متن کاملX-ray Spectral Properties of the Bat Agn Sample
The 9-month SWIFT Burst Alert Telescope (BAT) catalog provides the first unbiased (NH < 10 cm) look at local (< z >= 0.03) AGN. In this paper, we present the collected X-ray properties (0.3 – 12 keV) for the 153 AGN detected. In addition, we examine the X-ray properties for a complete sample of non-beamed sources, above the Galactic plane (b≥ 15). Of these, 45% are best fit by simple power law ...
متن کامل