Magellan optical spectroscopy of Swift J1357.2-0933

Details Magellan optical spectroscopy of Swift J1357.2-0933 Magellan optical spectroscopy of Swift J1357.2-0933

Feb 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011atel.3143....1t&link_type=abstract

The Astronomer's Telegram, #3143

Astronomy and Astrophysics

Astronomy

1

Optical, Binary, Nova, Star, Transient, Variables

Scientific paper

A 10-min spectrum of the optical counterpart to the new X-ray transient Swift J1357.2-0933 (Krimm et al. ATel #3138) was acquired with the MagE echellette spectrograph on the Magellan-Clay telescope at Las Campanas Observatory on 2011 Feb 02 09:23 UT. A 1 arcsec slit provided a spectral resolution of R~4100 in the range 3200-9200 Angstroms. Apart from the blue continuum, no Balmer lines (in either emission or absorption) are detected, nor was there evidence for HeII 4686 A or Bowen blend emission.

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