SN 1992A
1992A: The supernova is not detected on the V band images. The magnitude
lower limit is >27.0, but more sophisticated analysis may
push that higher.
Sn 1992A light curve (postscript)
- Summary of data
- WFPC2 images F439W (B), F555W (V) Aug. 2, 1994 V=25.8 B > 25.7
- WFPC2 image F555W(V) Sep. 3, 1996 not detected lower limit V > 27.0
- FOC imaging
- Jan. 24, 1992
- April 5, 1992
- Nov. 8, 1992
- FOS spectra
- HRS March 16, 1992
- Papers
- R.P. Kirshner, D.J. Jeffery, B. Leibundgut, P.M. Challis, G.
Sonneborn, M.M. Phillips, N.B. Suntzeff, R.C. Smith, P.F. Winkler, C.
Winge, M. Hamuy, D.A. Hunter, K.C. Roth, J.C. Blades, D. Branch, R.A.
Chevalier, C. Fransson, N. Panagia, R.V. Wagoner, J.Craig
Wheeler, R.P. Harkness: ``SN1992A: Ultraviolet and Optical Studies
based on HST, IUE and CTIAO Observations", 1993 {\it Astrophys. J.},
{\bf 415}, 589.\\
- P. Ruiz-Lapuente, R. P. Kirshner, M. M. Phillips, P. M.
Challis, B. P. Schmidt, A. V. Filippenko, and J. C. Wheeler,
``Late-Time Spectra and Type Ia Supernovae Models: New Clues from the
Hubble Space Telescope,'',1994 {\it ApJ},{\bf 439},60 \\
- P. Nugent, E. Baron, P.H. Hauschildt, and D. Branch,
``Spectrum
Synthesis of the Type Ia SNe 1992A and 1981B", {\it Astrophysical
Journal}, {\bf
441}, L33 (1995).\\
- "A study of SN 1992H in NGC 5377," A. Clocchiatti, S. Benetti,
J. C. Wheeler, W. Wren, J. Boisseau, E. Capellaro, M. Turatto,
F. Patat, D. A. Swartz, R. P. Harkness, M. S. Brotherton,
B. Wills, P. Hemenway, M. Cornell, M. Frueh, and M. B. Kaiser,
1995, Ap. J. in press.\\
- ``The Very Late-Time Light Curve of Supernova 1992A'', P.
Garnavich, N. Suntzeff, M. Hamuy, M. Phillips, .....SINS,1995, in
preparation.\\
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