X-ray galaxies selected from HyperLEDA database
arXiv:2210.10707 · doi:10.30970/jps.26.4901
Abstract
We cross-matched the 4XMM-DR10 catalog with the HyperLEDA database and obtained the new sample of galaxies that contain X-ray sources. Excluding duplicate observations and false matches, we present a total of 7759 galaxies with X-ray sources. In the current work, we present general properties of the sample: namely the distribution in equatorial coordinates, radial velocity distribution, morphological type, and X-ray fluxes. The sample includes morphological classification for 5241 galaxies with X-ray emission, almost half of which, 42\%, are elliptical (E, E-S0). Most galaxies in the sample have nuclear X-ray emission (6313 or 81\%), and the remaining 1443 (19\%) present X-ray emission from the host galaxy. This sample can be used for future deep studies of multi wavelengths properties of the galaxies with X-ray emission.
arXiv comment11 pages and 5 figures
References in corpus (17)
- HyperLEDA. III. The catalogue of extragalactic distances
- What Drives the Growth of Black Holes?
- Deep Extragalactic X-ray Surveys
- The XMM-Newton serendipitous survey IX. The fourth XMM-Newton serendipitous source catalogue
- The XXL Survey: I. Scientific motivations - XMM-Newton observing plan - Follow-up observations and simulation programme
- A Spectroscopic Survey of X-ray Selected AGN in the Northern XMM-XXL Field
- A census of ultraluminous X-ray sources in the local Universe
- Observations of Magnetic Fields and Relativistic Beaming in Four Quasar Jets
- The XXL survey XXXV. The role of cluster mass in AGN activity
- SPIDERS: An Overview of The Largest Catalogue of Spectroscopically Confirmed X-ray Galaxy Clusters
- Evidence for a population of beamed radio intermediate quasars
- Populations of super-soft X-ray sources in galaxies of different morphological types
- XXL Survey XXI. The environment and clustering of X-ray AGN in the XXL-South field
- Isolated AGNs NGC 5347, ESO 438-009, MCG-02-04-090, and J11366-6002: Swift and NuSTAR joined view
- X-ray Emission and Orientation of Selected PF Galaxy Clusters
- Determination of the Galaxy Cluster Orientation Using X-ray Images by FOCAS Method
- Predicted multiply-imaged X-ray AGNs in the XXL survey