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25 April 2024
 
  » arxiv » astro-ph/0001384

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Tests of the Accelerating Universe with Near-Infrared Observations of a High-Redshift Type Ia Supernova
Adam G. Riess ; Alexei V. Filippenko ; Michael C. Liu ; Peter Challis ; Alejandro Clocchiatti ; Alan Diercks ; Peter M. Garnavich ; Craig J. Hogan ; Saurabh Jha ; Robert P. Kirshner ; B. Leibundgut ; M. M. Phillips ; David Reiss ; Brian P. Schmidt ; Robert A. Schommer ; R. Chris Smith ; J. Spyromilio ; Christopher Stubbs ; Nicholas B. Suntzeff ; John Tonry ; Patrick Woudt ; Robert J. Brunner ; Arjun Dey ; Roy Gal ; James Graham ; James Larkin ; Steve C. Odewah n ; Ben Oppenheimer ;
Date 21 Dec 1999
Journal Astrophys.J. 536 (2000) 62
Subject astro-ph
AbstractWe have measured the rest-frame B,V, and I-band light curves of a high-redshift type Ia supernova (SN Ia), SN 1999Q (z=0.46), using HST and ground-based near-infrared detectors. A goal of this study is the measurement of the color excess, E_{B-I}, which is a sensitive indicator of interstellar or intergalactic dust which could affect recent cosmological measurements from high-redshift SNe Ia. Our observations disfavor a 30% opacity of SN Ia visual light by dust as an alternative to an accelerating Universe. This statement applies to both Galactic-type dust (rejected at the 3.4 sigma confidence level) and greyer dust (grain size > 0.1 microns; rejected at the 2.3 to 2.6 sigma confidence level) as proposed by Aguirre (1999). The rest-frame $I$-band light cur ve shows the secondary maximum a month after B maximum typical of nearby SNe Ia of normal luminosi ty, providing no indication of evolution as a function of redshift out to z~0.5. A n expanded set of similar observations could improve the constraints on any contribution of extragalactic dust to the dimming of high-redshift SNe Ia.
Source arXiv, astro-ph/0001384
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