A supernova at Z = 0.28 and the rate of distant supernovae

Details A supernova at Z = 0.28 and the rate of distant supernovae A supernova at Z = 0.28 and the rate of distant supernovae

Feb 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...211l...9h&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 211, no. 1, Feb. 1989, p. L9-L11.

Astronomy and Astrophysics

Astrophysics

18

Blue Stars, Galactic Clusters, Spiral Galaxies, Supernovae, Astronomical Photometry, Astronomical Spectroscopy, Faint Objects, Light Curve, Red Shift, Stellar Luminosity

Scientific paper

From the results of repeated deep optical imaging, an event was identified in a faint galaxy (V = 21.7) which is a member of a cluster at a redshift of z = 28. The results of the photometric and spectroscopic records of this event are consistent with the hypothesis that the event is a Type II supernova in a late type spiral galaxy. Its color is blue, and its mean apparent magnitude (V = 23.4) is close to the expected maximum brightness of a Type II supernova at z = 0.28.

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