Friday, December 17, 2004


Mateos et al. analyze X-ray spectra of 1137 serendipitous XMM sources. They find absorption in only ~40% of the number of sources predicted by XRB synthesis models.

Lee & Ravel investigate the feasibility of measuring ISM grain composition due to EXAFS in the Fe K absorption edge observed using XRS on Astro-E2.

Konacki et al. confirm a 3-day period transiting giant planet in OGLE-TR-10.

Keywords: papers, AGN, EXAFS, planets

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