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

AutorSánchez-Portal, Miguel; Pérez-García, Ana M.; Cepa, Jordi; Alfaro, Emilio J. ; Castañeda, Héctor; Gallego, Jesús; González-González, J. J.; González-Serrano, José Ignacio
Palabras claveX-rays: surveys
X-rays: background
Galaxies: morphology
Fecha de publicación2-nov-2005
EditorEuropean Space Agency. Publications Division
Proceedings of the ‘The X-ray Universe 2005’. Topic G: Extragalactic Surveys & Population Studies: the Cosmic X-ray Background. Poster papers, pp. 841-842
SerieESA SP-604
ResumenOTELO (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.
Descripción2 pages, 2 figures, uses graphicx package.-- Published in Proceedings of "The X-Ray Universe 2005", San Lorenzo del Escorial (Madrid), Spain, September 26-30, 2005.
Aparece en las colecciones: (IAA) Comunicaciones congresos
(IFCA) Comunicaciones congresos
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