XMM-Newton Proposal 02065401

Details XMM-Newton Proposal 02065401 XMM-Newton Proposal 02065401

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003xmm..prop..339a&link_type=abstract

XMM-Newton Proposal ID #02065401

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Pdfj011423-453430, Xmm-Newton Proposal 02065401

Scientific paper

Strongly dust obscured galaxies are believed to hold the key to understanding galaxy evolution. This has only been revealed over the past few years, with studies in different wavelength windows (NIR, sub-mm and X-rays) discovering an important population of dusty galaxies. Characterizing these sources, often identified through their extreme optical-NIR colours, has been so far hampered by their faintness and large distances. Here we propose to perform the first detailed X-ray study of an Extremely Red Object, by observing the nearest and most well studied ERO to date. Unlike any other galaxy in the local Universe, this source offers a unique opportunity for a detailed X-ray study of an ERO, necessary to begin understanding the more distant dusty galaxy population.

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