X-ray sources close to 3C 295 galaxy cluster (D'Elia+, 2008)

Details X-ray sources close to 3C 295 galaxy cluster (D'Elia+, 2008) X-ray sources close to 3C 295 galaxy cluster (D'Elia+, 2008)

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008ycat..34840303d&link_type=abstract

VizieR On-line Data Catalog: J/A+A/484/303. Originally published in: 2008A&A...484..303D

Physics

Clusters: Galaxy, X-Ray Sources

Scientific paper

To acquire the optical spectra of the 3C 295 sources, we proposed a Multi Object Spectroscopy (MOS) programme using DOLORES@TNG (AOT 9). Two acquisition images each of exposure time 900 s and with a limiting magnitude of R~24, had already been obtained using DOLORES on March 19, 2002. We acquired the spectral data on 22 and 23 March, 2004.
(1 data file).

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