D
D. Carter
Researcher at University of Cambridge
Publications - 3
Citations - 29
D. Carter is an academic researcher from University of Cambridge. The author has contributed to research in topics: Redshift & Galaxy. The author has an hindex of 2, co-authored 3 publications receiving 28 citations. Previous affiliations of D. Carter include University of New South Wales & Lawrence Berkeley National Laboratory.
Papers
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Book ChapterDOI
Scheduled Discoveries of 7+ High-Redshift Supernovae:First Cosmology Results and Bounds on q 0
Saul Perlmutter,Susana E. Deustua,S. Gabi,G. Goldhaber,Donald E. Groom,I. M. Hook,A. G. Kim,M. Y. Kim,Julia C. Lee,R. Pain,C. R. Pennypacker,I. A. Small,Ariel Goobar,Richard S. Ellis,Richard G. McMahon,B. J. Boyle,P. S. Bunclark,D. Carter,Karl Glazebrook,M. Irwin,Heidi Jo Newberg,Alexei V. Filippenko,Thomas Matheson,Michael A. Dopita,Jeremy Mould,Warrick J. Couch +25 more
TL;DR: Kim et al. as mentioned in this paper used a batch search strategy to find high-redshift Type Ia supernovae and observed their spectra and light curves using the peak of their light curves.
Journal ArticleDOI
Cosmological time dilation using type Ia supernovae as clocks
G. Goldhaber,G. Goldhaber,B. J. Boyle,B. J. Boyle,P. S. Bunclark,P. S. Bunclark,D. Carter,D. Carter,Warrick J. Couch,Warrick J. Couch,S. Deustua,Michael A. Dopita,Michael A. Dopita,Richard S. Ellis,Richard S. Ellis,A. V. Filippenko,A. V. Filippenko,S. Gabi,Karl Glazebrook,Karl Glazebrook,Ariel Goobar,Ariel Goobar,D. Groom,I. Hook,Mike Irwin,Mike Irwin,A. Kim,Julia C. Lee,Thomas Matheson,Thomas Matheson,R. McMahon,R. McMahon,H. Newberg,R. Pain,R. Pain,C. Pennypacker,S. Perlmutter,S. Perlmutter,I. Small,I. Small +39 more
TL;DR: In this article, the first results from a systematic search for high redshift Type Ia supernovae were reported, with redshift z = 0.35 − 0.46.
Journal ArticleDOI
The distant supernova search and implications for the cosmological deceleration
A. Goobar,A. Goobar,B. J. Boyle,B. J. Boyle,P. S. Bunclark,P. S. Bunclark,D. Carter,D. Carter,Richard S. Ellis,Richard S. Ellis,S. Gabi,S. Gabi,G. Goldhaber,G. Goldhaber,Mike Irwin,Mike Irwin,A. G. Kim,A. G. Kim,M. Y. Kim,M. Y. Kim,Richard G. McMahon,Richard G. McMahon,Richard A. Muller,Richard A. Muller,R. Pain,R. Pain,C. R. Pennypacker,C. R. Pennypacker,Saul Perlmutter,Saul Perlmutter,I. A. Small,I. A. Small +31 more
TL;DR: In this article, a supernova at z = 0.458 (SN1992bi) was discovered and its photometry closely matched the lightcurve calculated for its redshift from the template of well-observed nearby Type la supernovae giving a best fit value for the deceleration parameter: q o = 0 1 ± 0.3 (± 0.55) with Λ = 0, where the first uncertainty is due to the photometry of the distant supernova and the second reflects the estimated intrinsic width of the Type la absolute magnitude distribution based on nearby