Capturing WR140 at Periastron with the Chandra HETG

Details Capturing WR140 at Periastron with the Chandra HETG Capturing WR140 at Periastron with the Chandra HETG

Sep 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000cxo..prop..719p&link_type=abstract

Chandra Proposal ID #01208024

Astronomy and Astrophysics

Astronomy

Chandra Proposal Id #01208024

Scientific paper

This is a resubmission of our AO2 proposal number 02200508 which was rejected, despite high scores, because it was mistakenly thought that XMM would be making similar observations near periastron. In fact, according to its official WWW visibility tool, XMM is not able to observe any nearer than two months either side of periastron passage and possibly not at all. The compelling scientific justification was given in our original proposal and endorsed by the Peer Review. We are responding to the Review Panel's recommendation to apply for Director's Discretionary Time.

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