Early Optical Spectroscopy of SN 2011dh in M51

Details Early Optical Spectroscopy of SN 2011dh in M51 Early Optical Spectroscopy of SN 2011dh in M51

Jun 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011atel.3428....1s&link_type=abstract

The Astronomer's Telegram, #3428

Astronomy and Astrophysics

Astronomy

Optical, Supernovae, Transient

Scientific paper

We obtained optical spectroscopy of SN 2011dh (PTF11eon) in M51 (ATEL
#3398; CBET #2736) with the Palomar Hale 5m on UT 2011 June 5.18 using
the Double Spectrograph. The red and blue cameras were set to provide a
resolving power of R~4700 with a wavelength range covering roughly
6170-6850 A and R~3000 spanning 3500-5050 A, respectively.

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