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20 April 2024
 
  » arxiv » astro-ph/0511078

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XMM-Newton and Deep Optical Observations of the OTELO fields: the Groth-Westphal Strip
M. Sanchez-Portal ; A. M. Perez-Garcia ; J. Cepa-Nogue ; E. Alfaro ; H. Castaneda ; J. Gallego ; J. Gonzalez-Gonzalez ; J. I. Gonzalez-Serrano ;
Date 2 Nov 2005
AbstractOTELO (OSIRIS Tunable Emission Line Object Survey) will be carried out with the OSIRIS instrument at the 10 m GTC telescope at La Palma, and is aimed to be the deepest and richest survey of emission line objects to date. The deep narrow-band optical data from OSIRIS will be complemented by means of additional observations that include: (i) an exploratory broad-band survey that is already being carried out in the optical domain, (ii) FIR and sub-mm observations to be carried with the Herschel space telescope and the GTM, and (iii) deep X-Ray observations from XMM-Newton and Chandra.Here we present a preliminary analysis of public EPIC data of one of the OTELO targets,the Groth-Westphal strip, gathered from the XMM-Newton Science Archive (XSA). EPIC images are combined with optical BVRI data from our broadband survey carried out with the 4.2m WHT at La Palma. Distance-independent diagnostics (involving X/O ratio, hardness ratios, B/T ratio) are tested.
Source arXiv, astro-ph/0511078
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