Optical identifications of two SWIFT sources

Details Optical identifications of two SWIFT sources Optical identifications of two SWIFT sources

Nov 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006atel..948....1m&link_type=abstract

The Astronomer's Telegram, #948

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3

Optical, X-Ray, Gamma Ray, Agn

Scientific paper

We report optical spectroscopic identification of two SWIFT sources SWIFTJ1745.4+2906 and 1RXSJ193347.6+325422. Optical data were obtained with the Russian-Turkish 1.5-m telescope (RTT-150, Bakirlitepe, TUBITAK National Observatory, Turkey), using the TFOSC spectrograph. Both sources were localized by SWIFT/XRT and are associated with nuclei of relatively bright (V~=16m) galaxies. The optical spectra of the galaxy nuclei show redshifted and broadened H_alpha (blended with NII), H_beta and other Balmer lines and narrow emission lines [OIII] 4959,5007 and others.

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