Confirmation of counterpart to SWIFT J1626.6-5156

Details Confirmation of counterpart to SWIFT J1626.6-5156 Confirmation of counterpart to SWIFT J1626.6-5156

Feb 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006atel..739....1n&link_type=abstract

The Astronomer's Telegram, #739

Astronomy and Astrophysics

Astronomy

4

Optical, Binaries, Pulsars, Transients

Scientific paper

The candidate counterpart to SWIFT J1626.6-5156 (ATel #678, #679, #688) proposed by Rea et al. (ATel #713) was observed on the night of 2006 Feb 15 with the NTT (La Silla, Chile). The instrument used was EMMI with grism #6. This configuration covers the 570-870 nm range with a dispersion of 0.7A/pixel. The candidate (2MASS16263652-5156305 = USNO-B1.0 0380-0649488) displays H-alpha strongly in emission, with an EW=-38° and broad wings.

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