N
Nino Panagia
Researcher at Space Telescope Science Institute
Publications - 483
Citations - 52007
Nino Panagia is an academic researcher from Space Telescope Science Institute. The author has contributed to research in topics: Supernova & Galaxy. The author has an hindex of 89, co-authored 478 publications receiving 48961 citations. Previous affiliations of Nino Panagia include Cornell University & University of Catania.
Papers
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Journal ArticleDOI
Measurements of Omega and Lambda from 42 High-Redshift Supernovae
Saul Perlmutter,Saul Perlmutter,Greg Aldering,Gerson Goldhaber,Gerson Goldhaber,R. A. Knop,Peter Nugent,P. G. Castro,P. G. Castro,Susana E. Deustua,Sebastien Fabbro,Sebastien Fabbro,A. Goobar,A. Goobar,Donald E. Groom,I. M. Hook,I. M. Hook,A. G. Kim,A. G. Kim,A. G. Kim,M. Y. Kim,Julia C. Lee,Julia C. Lee,Nelson J. Nunes,Nelson J. Nunes,Reynald Pain,Reynald Pain,C. R. Pennypacker,C. R. Pennypacker,Robert Quimby,Christopher Lidman,Richard S. Ellis,Mike Irwin,Richard G. McMahon,Pilar Ruiz-Lapuente,Nicholas A. Walton,Bradley E. Schaefer,B. J. Boyle,Alexei V. Filippenko,Thomas Matheson,A. S. Fruchter,Nino Panagia,Nino Panagia,Heidi Jo Newberg,Warrick J. Couch +44 more
TL;DR: In this paper, the mass density, Omega_M, and cosmological-constant energy density of the universe were measured using the analysis of 42 Type Ia supernovae discovered by the Supernova Cosmology project.
Journal ArticleDOI
Discovery of a supernova explosion at half the age of the Universe
Saul Perlmutter,Saul Perlmutter,Greg Aldering,M. Della Valle,S. Deustua,S. Deustua,Richard S. Ellis,Sebastien Fabbro,Andrew S. Fruchter,Gerson Goldhaber,Gerson Goldhaber,Donald E. Groom,I. M. Hook,A. G. Kim,A. G. Kim,M. Y. Kim,R. A. Knop,Christopher Lidman,Richard G. McMahon,Peter Nugent,Reynald Pain,Nino Panagia,C. R. Pennypacker,C. R. Pennypacker,Pilar Ruiz-Lapuente,Bradley E. Schaefer,N. A. Walton +26 more
TL;DR: The most distant spectroscopically confirmed supernova was reported in this paper, and it was found to be similar to nearby type Ia supernovae, which suggests that we may live in a low-mass-density universe.
Journal ArticleDOI
The Hubble Space Telescope Cluster Supernova Survey. V. Improving the Dark-energy Constraints above z > 1 and Building an Early-type-hosted Supernova Sample
Nao Suzuki,Nao Suzuki,David Rubin,David Rubin,C. Lidman,Greg Aldering,Rahman Amanullah,K. Barbary,K. Barbary,L. F. Barrientos,János Botyánszki,Mark Brodwin,Natalia Connolly,Kyle S. Dawson,Arjun Dey,Mamoru Doi,Megan Donahue,Susana E. Deustua,Peter Eisenhardt,Erica Ellingson,L. Faccioli,L. Faccioli,Vitaliy Fadeyev,H. K. Fakhouri,H. K. Fakhouri,A. S. Fruchter,David Gilbank,Michael D. Gladders,Gerson Goldhaber,Gerson Goldhaber,Anthony H. Gonzalez,Ariel Goobar,Alexander Gude,Alexander Gude,Takashi Hattori,Henk Hoekstra,Eric Hsiao,Eric Hsiao,X. Huang,X. Huang,Yutaka Ihara,Myungkook J. Jee,David Johnston,David Johnston,Nobunari Kashikawa,Benjamin P. Koester,Kohki Konishi,M. Kowalski,Eric V. Linder,Eric V. Linder,Lori M. Lubin,Jason Melbourne,J. Meyers,J. Meyers,Tomoki Morokuma,Tomoki Morokuma,F. Munshi,F. Munshi,Christopher R. Mullis,Takeshi Oda,Nino Panagia,Saul Perlmutter,Saul Perlmutter,Marc Postman,T. A. Pritchard,T. A. Pritchard,Jason Rhodes,P. Ripoche,P. Ripoche,Piero Rosati,David J. Schlegel,A. L. Spadafora,S. A. Stanford,S. A. Stanford,Vallery Stanishev,Vallery Stanishev,Daniel Stern,M. Strovink,M. Strovink,Naohiro Takanashi,Kouichi Tokita,M. Wagner,Lifan Wang,Naoki Yasuda,H. K. C. Yee +84 more
TL;DR: In this article, Advanced Camera for Surveys, NICMOS and Keck adaptive-optics-assisted photometry of 20 Type Ia supernovae (SNe Ia) from the Hubble Space Telescope (HST) Cluster Supernova Survey was presented.
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
SPECTRA AND HUBBLE SPACE TELESCOPE LIGHT CURVES OF SIX TYPE Ia SUPERNOVAE AT 0.511 <z< 1.12 AND THE UNION2 COMPILATION ∗
Rahman Amanullah,Chris Lidman,David Rubin,David Rubin,Greg Aldering,Pierre Astier,Kyle Barbary,Kyle Barbary,M. S. Burns,A. Conley,Kyle S. Dawson,S. E. Deustua,Mamoru Doi,Sebastien Fabbro,L. Faccioli,L. Faccioli,H. K. Fakhouri,H. K. Fakhouri,Gastón Folatelli,A. S. Fruchter,Hisanori Furusawa,G. Garavini,G. Goldhaber,G. Goldhaber,Ariel Goobar,Donald E. Groom,I. M. Hook,I. M. Hook,D. A. Howell,D. A. Howell,Nobunari Kashikawa,A. G. Kim,R. A. Knop,M. Kowalski,Eric V. Linder,J. Meyers,J. Meyers,Tomoki Morokuma,S. Nobili,J. Nordin,Peter Nugent,Linda Ostman,Reynald Pain,Nino Panagia,Nino Panagia,Saul Perlmutter,Saul Perlmutter,J. Raux,Pilar Ruiz-Lapuente,A. L. Spadafora,M. Strovink,M. Strovink,Nao Suzuki,Lifan Wang,W. M. Wood-Vasey,Naoki Yasuda +55 more
TL;DR: Kowalski et al. as mentioned in this paper reported on work to increase the number of well-measured Type Ia supernovae (SNe Ia) at high redshifts.