The Optical Counterpart to XTE J1817-330.

Details The Optical Counterpart to XTE J1817-330. The Optical Counterpart to XTE J1817-330.

Feb 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006atel..733....1t&link_type=abstract

The Astronomer's Telegram, #733

Astronomy and Astrophysics

Astronomy

11

Request For Observations, Binaries, Black Holes, Transients

Scientific paper

We report the counterpart to the X-ray transient and black hole candidate XTE J1817-330 (ATEL #714). Our observations consist of a series of 5s and 10s g'-band images obtained with the 6.5m Magellan Clay telescope during 2006 Feb 10 09:23-09:42 UT using the multi-object imaging spectrograph LDSS-3. The frames were acquired with an image quality of 1.2 arcsec and a projected pixel scale of 0.188 arcsec/pixel.

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