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

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dc.creatorSanchez-Portal, M.
dc.creatorPerez-Garcia, A. M.
dc.creatorCepa-Nogue, J.
dc.creatorAlfaro, E.
dc.creatorCastaneda, H.
dc.creatorGallego, J.
dc.creatorGonzalez-Gonzalez, J.
dc.creatorGonzalez-Serrano, J. I.
dc.date2005-11-02
dc.date.accessioned2026-07-07T06:44:50Z
dc.date.available2026-07-07T06:44:50Z
dc.descriptionOTELO (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.
dc.description2 pages, 2 figures, uses graphicx package. To appear in proceedings of "The X-Ray Universe 2005", San Lorenzo del Escorial, Spain, September 26-30, 2005
dc.identifierhttps://arxiv.org/abs/astro-ph/0511078
dc.identifierhttp://arxiv.org/abs/astro-ph/0511078
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/102884
dc.subjectAstrophysics
dc.titleXMM-Newton and Deep Optical Observations of the OTELO fields: the Groth-Westphal Strip
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