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FIXING THE U-BAND PHOTOMETRY OF TYPE Ia SUPERNOVAE

Journal Article · · Astronomical Journal (New York, N.Y. Online)
; ;  [1]; ;  [2]; ; ; ; ;  [3];  [4]
  1. Department of Physics and Astronomy, Texas A and M University, 4242 TAMU, College Station, TX 77843-4242 (United States)
  2. Cerro Tololo Inter-American Observatory, Casilla 603, La Serena (Chile)
  3. Las Campanas Observatory, Casilla 601, La Serena (Chile)
  4. Departamento de Astronomia, Universidad de Chile, Casilla 36-D, Santiago (Chile)
We present previously unpublished photometry of supernovae 2003gs and 2003hv. Using spectroscopically derived corrections to the U-band photometry, we reconcile U-band light curves made from imagery with the Cerro Tololo 0.9 m, 1.3 m, and Las Campanas 1 m telescopes. Previously, such light curves showed a 0.4 mag spread at one month after maximum light. This gives us hope that a set of corrected ultraviolet light curves of nearby objects can contribute to the full utilization of rest-frame U-band data of supernovae at redshift {approx}0.3-0.8. As pointed out recently by Kessler et al. in the context of the Sloan Digital Sky Survey supernova search, if we take the published U-band photometry of nearby Type Ia supernovae at face value, there is a 0.12 mag U-band anomaly in the distance moduli of higher redshift objects. This anomaly led the Sloan survey to eliminate from their analyses all photometry obtained in the rest-frame U-band. The Supernova Legacy Survey eliminated observer frame U-band photometry, which is to say nearby objects observed in the U-band, but they used photometry of high-redshift objects no matter in which band the photons were emitted.
OSTI ID:
22089736
Journal Information:
Astronomical Journal (New York, N.Y. Online), Journal Name: Astronomical Journal (New York, N.Y. Online) Journal Issue: 1 Vol. 145; ISSN 1538-3881
Country of Publication:
United States
Language:
English

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