A
A. Conley
Researcher at Lawrence Berkeley National Laboratory
Publications - 6
Citations - 1930
A. Conley is an academic researcher from Lawrence Berkeley National Laboratory. The author has contributed to research in topics: Supernova & Redshift. The author has an hindex of 4, co-authored 6 publications receiving 1856 citations. Previous affiliations of A. Conley include University of California, Berkeley & Association of Universities for Research in Astronomy.
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Journal ArticleDOI
New Constraints on ΩM, ΩΛ, and w from an Independent Set of 11 High-Redshift Supernovae Observed with the Hubble Space Telescope*
R. A. Knop,R. A. Knop,Greg Aldering,Greg Aldering,Rahman Amanullah,Pierre Astier,G. Blanc,G. Blanc,M. S. Burns,A. Conley,A. Conley,Susana E. Deustua,Susana E. Deustua,Mamoru Doi,Richard S. Ellis,Sebastien Fabbro,Sebastien Fabbro,Gastón Folatelli,A. S. Fruchter,G. Garavini,S. Garmond,S. Garmond,K. Garton,R. Gibbons,Gerson Goldhaber,Gerson Goldhaber,Ariel Goobar,Donald E. Groom,Donald E. Groom,D. Hardin,I. M. Hook,Dale Andrew Howell,A. G. Kim,A. G. Kim,Brian C. Lee,Christopher Lidman,Javier Méndez,S. Nobili,Peter Nugent,Peter Nugent,Reynald Pain,Nino Panagia,C. R. Pennypacker,Saul Perlmutter,Robert Quimby,J. Raux,N. Regnault,N. Regnault,Pilar Ruiz-Lapuente,G. Sainton,Bradley E. Schaefer,K. Schahmaneche,E. Smith,A. L. Spadafora,Vallery Stanishev,Mark Sullivan,Mark Sullivan,Nicholas A. Walton,Lifan Wang,W. M. Wood-Vasey,W. M. Wood-Vasey,Naoki Yasuda +61 more
TL;DR: In this paper, a set of high-redshift supernovae were used to confirm previous supernova evidence for an accelerating universe, and the supernova results were combined with independent flat-universe measurements of the mass density from CMB and galaxy redshift distortion data, they provided a measurement of $w=-1.05^{+0.15}-0.09$ if w is assumed to be constant in time.
Journal ArticleDOI
Spectroscopic observations and analysis of the peculiar SN 1999aa
G. Garavini,Gastón Folatelli,Ariel Goobar,S. Nobili,Greg Aldering,Greg Aldering,Alexis Amadon,Rahman Amanullah,Pierre Astier,Christophe Balland,Christophe Balland,G. Blanc,G. Blanc,M. S. Burns,A. Conley,A. Conley,A. Conley,Tomas Dahlen,Susana E. Deustua,Susana E. Deustua,Richard S. Ellis,Sebastien Fabbro,Xiaohui Fan,Brenda Frye,E. L. Gates,R. Gibbons,Gerson Goldhaber,Gerson Goldhaber,Bertrand Goldman,Donald E. Groom,J. Haissinski,D. Hardin,I. M. Hook,Dale Andrew Howell,Daniel Kasen,Steve Kent,Alex G. Kim,R. A. Knop,Brian C. Lee,Christopher Lidman,Javier Méndez,G. J. Miller,G. J. Miller,M. Moniez,A. Mourao,Heidi Jo Newberg,Peter Nugent,Reynald Pain,O. Perdereau,Saul Perlmutter,V. Prasad,Robert Quimby,J. Raux,N. Regnault,Jeffrey A. Rich,Gordon T. Richards,Pilar Ruiz-Lapuente,G. Sainton,Bradley E. Schaefer,K. Schahmaneche,E. Smith,A. L. Spadafora,Vallery Stanishev,Nicholas A. Walton,L. Wang,W. M. Wood-Vasey,W. M. Wood-Vasey +66 more
TL;DR: In this paper, an extensive time series of spectroscopic data of the peculiar SN 1999aa in NGC 2595 is presented, including 25 optical spectra between -11 and +58 days with respect to B-band maximum light, providing an unusually complete time history.
Journal ArticleDOI
Quantitative comparison between Type Ia supernova spectra at low and high redshifts: A case study
G. Garavini,G. Garavini,Gastón Folatelli,S. Nobili,Greg Aldering,Rahman Amanullah,P. Antilogus,Pierre Astier,G. Blanc,T. J. Bronder,M. S. Burns,A. Conley,A. Conley,S. E. Deustua,Masao Doi,Sebastien Fabbro,V. Fadeyev,R. Gibbons,G. Goldhaber,G. Goldhaber,Ariel Goobar,Donald E. Groom,I. M. Hook,D. A. Howell,Nobunari Kashikawa,A. G. Kim,Marek Kowalski,N. Kuznetsova,Brian C. Lee,Chris Lidman,Javier Méndez,Tomoki Morokuma,Kentaro Motohara,Peter Nugent,Reynald Pain,Saul Perlmutter,Saul Perlmutter,Robert Quimby,J. Raux,Nicolas Regnault,Pilar Ruiz-Lapuente,G. Sainton,K. Schahmaneche,E. Smith,A. L. Spadafora,Vallery Stanishev,R. C. Thomas,Nicholas A. Walton,Lifan Wang,W. M. Wood-Vasey,W. M. Wood-Vasey,Naoki Yasuda +51 more
TL;DR: In this article, the strength of the absorption features in Type Ia supernova (SN Ia) spectra was measured and used to make a quantitative comparison between the spectra of SNe Ia at low and high redshifts.
Journal ArticleDOI
Restframe I-band Hubble diagram for type Ia supernovae up to redshift z~0.5
S. Nobili,S. Nobili,Rahman Amanullah,G. Garavini,G. Garavini,Ariel Goobar,Chris Lidman,Vallery Stanishev,Greg Aldering,P. Antilogus,Pierre Astier,M. S. Burns,A. Conley,A. Conley,S. E. Deustua,Richard S. Ellis,Sebastien Fabbro,V. Fadeyev,Gastón Folatelli,R. Gibbons,G. Goldhaber,G. Goldhaber,Donald E. Groom,I. M. Hook,Dale Andrew Howell,A. G. Kim,R. A. Knop,Peter Nugent,Reynald Pain,Saul Perlmutter,Saul Perlmutter,Robert Quimby,J. Raux,N. Regnault,N. Regnault,Pilar Ruiz-Lapuente,G. Sainton,K. Schahmaneche,E. Smith,A. L. Spadafora,R. C. Thomas,Lifan Wang +41 more
TL;DR: In this article, the authors presented a technique for fitting restframe I-band light curves on a data set of 42 type la supernovae (SNe Ia) and constructed a Hubble diagram with 26 SNe from the subset at 0.01 < z < 0.1.
Restframe I-band Hubble diagram for type Ia supernovae up to redshift z ~; 0.5 - eScholarship
S. Nobili,Rahman Amanullah,G. Garavini,A. Goobar,Christopher Lidman,Vallery Stanishev,G. Aldering,P. Antilogus,P. Astier,Burns,A. Conley,Susana E. Deustua,R. Ellis,S. Fabbro,Vitaliy Fadeyev,G. Folatelli,R. Gibbons,G. Goldhaber,Donald E. Groom,I. M. Hook,Dale Andrew Howell,A.G. Kim,R. A. Knop,P. E. Nugent,R. Pain,S. Perlmutter,Robert Quimby,J. Raux,N. Regnault,P. Ruiz-Lapuente,G. Sainton,K. Schahmaneche,Eric P. Smith,A. L. Spadafora,R. C. Thomas,Ling-Jun Wang +35 more
TL;DR: In this paper, the authors presented a technique for fitting restframe I-band light curves on a data set of 42 type Ia supernovae (SNe Ia), and constructed a Hubble diagram with 26 SNe from the subset at 0.01 < z < 0.1.