N
N. Suzuki
Publications - 13
Citations - 213
N. Suzuki is an academic researcher. The author has contributed to research in topics: Supernova & Redshift. The author has an hindex of 3, co-authored 10 publications receiving 208 citations.
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Journal ArticleDOI
A New Determination of the High Redshift Type Ia Supernova Rates with the Hubble Space Telescope Advanced Camera for Surveys
N. Kuznetsova,Kyle Barbary,B.M. Connolly,A. G. Kim,R. Pain,Natalie A. Roe,Greg Aldering,Rahman Amanullah,Kyle Dawson,Masao Doi,Vitaliy Fadeyev,A. S. Fruchter,R. Gibbons,G. Goldhaber,A. Goobar,Alexander Gude,R. A. Knop,M. Kowalski,C. Lidman,Tomoki Morokuma,J. Meyers,Saul Perlmutter,David Rubin,David J. Schlegel,A. L. Spadafora,Vallery Stanishev,M. Strovink,N. Suzuki,Ling-Jun Wang,Naoki Yasuda +29 more
TL;DR: In this paper, a new measurement of the volumetric rate of Type Ia supernova up to a redshift of 1.7 was presented, using the Hubble Space Telescope (HST) GOODS data combined with an additional HST dataset covering the North GOODS field collected in 2004.
Journal ArticleDOI
A Concordance Model of the Lyman-alpha Forest at z = 1.95
Tridivesh Jena,Michael L. Norman,D. Tytler,David Kirkman,N. Suzuki,A. Chapman,Carl Melis,Geoffrey C. So,Brian W. O'Shea,Wen-Ching Lin,Dan Lubin,Pascal Paschos,Dieter Reimers,E. Janknecht,Cora Fechner +14 more
TL;DR: In this article, the authors present 40 fully hydrodynamical numerical simulations of the intergalactic gas that gives rise to the Ly-alpha forest and compare the output from the simulations to data from HIRES and UVES spectra and give a new measurement of the flux power from these spectra at z = 1.95.
SPECTRA AND HUBBLE SPACE TELESCOPE LIGHT CURVES OF SIX TYPE Ia SUPERNOVAE AT 0.511
Rahman Amanullah,Chris Lidman,David Rubin,Greg Aldering,Pierre Astier,Kyle Barbary,M. S. Burns,Alex Conley,Ks S. Dawson,S. E. Deustua,Mamoru Doi,S. Fabbro,L. Faccioli,Hk K. Fakhouri,G. Folatelli,As S. Fruchter,Hisanori Furusawa,G. Garavini,G. Goldhaber,Ariel Goobar,De E. Groom,I. M. Hook,D. A. Howell,Nobunari Kashikawa,A. G. Kim,Ra A. Knop,M. Kowalski,Eric V. Linder,J. Meyers,Tomoki Morokuma,S. Nobili,J. Nordin,Pe E. Nugent,L. Ostman,R. Pain,Nino Panagia,Saul Perlmutter,J. Raux,P. Ruiz-Lapuente,A. L. Spadafora,M. Strovink,N. Suzuki,Longlu Wang,Wm M. Wood-Vasey,Naoki Yasuda,Sc Project +45 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.
Journal ArticleDOI
Uniform Recalibration of Common Spectrophotometry Standard Stars onto the CALSPEC System Using the SuperNova Integral Field Spectrograph
David T. Rubin,Greg Aldering,P. Antilogus,Cecilia Aragon,Sheila G. Bailey,C. Baltay,S. Bongard,K. Boone,C. Buton,Y. Copin,S. Dixon,Dominique Fouchez,E. Gangler,R. R. Gupta,Brian Hayden,Wolfgang Hillebrandt,A. G. Kim,Marek Kowalski,D. Kuesters,P.-F. Leget,F. Mondon,J. Nordin,Reynald Pain,E. Pecontal,R. Pereira,S. Perlmutter,K. A. Ponder,David Rabinowitz,Mickael Rigault,K. Runge,Clare Saunders,G. Smadja,N. Suzuki,Charling Tao,S. Taubenberger,R. C. Thomas,M. Vincenzi,The Nearby Supernova Factory +37 more
TL;DR: In this article , the authors calibrate spectrophotometric optical spectra of 32 stars commonly used as standard stars, referenced to 14 stars already on the Hubble Space Telescope-based CALSPEC flux system.
Discovery of an Unusual Optical Transient with the Hubble Space Telescope
Kyle Barbary,Kyle S. Dawson,Kouichi Tokita,Greg Aldering,Rahman Amanullah,Natalia Connolly,Mamoru Doi,L. Faccioli,Vitaliy Fadeyev,A. S. Fruchter,G. Goldhaber,A. Goobar,Alexander Gude,X. Huang,Yutaka Ihara,Kohki Konishi,M. Kowalski,C. Lidman,J. Meyers,Tomoki Morokuma,Peter Nugent,Saul Perlmutter,David Rubin,David J. Schlegel,A. L. Spadafora,N. Suzuki,H. Swift,Naohiro Takanashi,R. C. Thomas,Naoki Yasuda,Supernova Cosmology +30 more
TL;DR: In this article, the authors present observations of SCP 06F6, an unusual optical transient discovered during the Hubble Space Telescope Cluster Supernova Survey, which brightened over a period of ~100 days, reached a peak magnitude of ~21.0 in both i_775 and z_850, and then declined over a similar timescale.