XMM-Newton View of the Hubble Deep Field-North and Groth-Westphal Strip Regions

Simple item page
dc.creatorMiyaji, T.
dc.creatorGriffiths, R. E.
dc.creatorLumb, D.
dc.creatorSarajedini, V.
dc.creatorSiddiqui, H.
dc.date2002-11-14
dc.date2003-05-06
dc.date.accessioned2026-07-07T10:31:27Z
dc.date.available2026-07-07T10:31:27Z
dc.descriptionWe report the progress on our analysis of two deep XMM observations in the areas of Hubble Deep Field-North and the Groth-Westphal Strip field. We present the source detection method, Monte-Carlo simulation on source detection, and our preliminary Log N -- Log S relations. Comparing these two fields and other fields in literature, we find up to 30% variations in number counts near our flux limits, which is most likely to be due to cosmic variance. This serves as a pilot study for a more systematic investigation. The nature of the X-ray sources in the Groth-Westphal field is also discussed in terms of hardness ratios, morphology and spectroscopic properties.
dc.descriptionReplaced Fig. 3 which had an incorrect data point. Astron. Nachr. issue dedicated to the proceedings of the workshop "X-ray Surveys in the light of New Observatories", Sep. 2002, Santander, Spain
dc.identifierhttps://arxiv.org/abs/astro-ph/0211343
dc.identifierhttp://arxiv.org/abs/astro-ph/0211343
dc.identifierAstron.Nachr.324:24,2003
dc.identifierdoi:10.1002/asna.200310007
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/178415
dc.subjectAstrophysics
dc.titleXMM-Newton View of the Hubble Deep Field-North and Groth-Westphal Strip Regions
dc.typetext

Files

Collections

arXiv