Berkeley SSL/LBL / UW Infra-Red Supernova Search

[Picture of M51 W/out SN]
SN 1994I: A massive, exploding star in the Whirlpool galaxy (M51) recorded in the Infra-Red (2.1 micron K' band), taken at the Wyoming IR Observatory (WIRO) 4/16/94. The galaxy is about 9 Mpc (~27 Million Light-Years) distant.

Our paper is available for perusal by collaborators.

The IR supernova (SN) Search is a monthly patrol of nearby starburst Galaxies for the purpose of discovering SNe hidden to optical astronomers, so that they may be observed by the Gamma-Ray Observatory (GRO) and others.

Update: Click here for the most current IR SN Search Details. These include results of the first test of the ORCA (Optimum Resolution Camera Adapter), 4/17-4/21.

Click here for IR SN Search Details 

Current Status

Camera Upgrade A COMPLETE SUCCESS!!
Click Here for Details and Images

THE IR SEARCH SN INFORMATION LINK

Information about nearby SNe is posted here regularly. Last update: 1/30/94

WATCH THIS SPACE:

SN updates, IR SN photometry data, and general SN news will happen sometime soon.

Last Update: 6/15/96 
The IR Supernova Search at UC Berkeley/LBL is:
Robert Tripp (P.I.) & Bruce Grossan(Postdoc/Observer/Programmer/Hardware)
Carl Pennypacker, Saul Perlmutter, Gerson Goldhaber
Lawrence Berkeley Lab 50-232
1 Cyclotron Road
Berkeley, CA 94720
bruce@singu.lbl.gov

[PHONE] 510.486.5489
 

At UW: Earl Spillar
Norbert Pirzkal (sp?)
Harley Thronsen
Paul Johnson
...And Many Thanks to the WIRO and UW Physics and Astro dept. staff and Students. 


Mail comments to bruce[at]singu[dot]lbl[dot]gov

(anti-spam address format)

Last Update 30 Oct98