Potential progenitor detection for the transient in NGC 5775 in archival HST data

Details Potential progenitor detection for the transient in NGC 5775 in archival HST data Potential progenitor detection for the transient in NGC 5775 in archival HST data

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012atel.4009....1b&link_type=abstract

The Astronomer's Telegram, #4009

Astronomy and Astrophysics

Astronomy

Optical, Transient

Scientific paper

We observed the location of the Catalina Sky Survey transient PSN J14535395+0334049, which spectroscopically resembles SN2008S (Howerton et al. ATEL #4004), with the MMT & Magellan Infrared Spectrograph (MMIRS) on 2012 March 29.33 UT. Observations were obtained in J-band in ~0.5" seeing. Using 17 sources in common between our MMIRS image and an archival HST ACS/F625W image of NGC 5775 (program 10416; PI: Rossa), we locate the position of the transient to a relative astrometric accuracy of about 60 mas in RA and Dec.

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