XMM-Newton and Deep Optical Observations of the OTELO Fields: the Groth-Westphal Strip

Bibcode
2006ESASP.604..841S
Sánchez-Portal, M.; Pérez-García, A. M.; Cepa, J.; Alfaro, E.; Castañeda, H.; Gallego, J.; González-González, J. J.; González-Serrano, J. I.
Referencia bibliográfica

Proceedings of the The X-ray Universe 2005 (ESA SP-604). 26-30 September 2005, El Escorial, Madrid, Spain. Editor: A. Wilson, p.841

Fecha de publicación:
1
2006
Número de autores
8
Número de autores del IAC
0
Número de citas
1
Número de citas referidas
0
Descripción
OTELO (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.
Tipo
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