相关论文: The Hubble Space Telescope Cluster Supernova Surve…

The Hubble Space Telescope Cluster Supernova Survey: II. The Type Ia Supernova Rate in High-Redshift Galaxy Clusters

We report a measurement of the Type Ia supernova (SN Ia) rate in galaxy clusters at 0.9 < z < 1.45 from the Hubble Space Telescope (HST) Cluster Supernova Survey. This is the first cluster SN Ia rate measurement with detected z > 0.9 SNe.…

宇宙学与河外天体物理 · 物理学 2019-08-14 K. Barbary , G. Aldering , R. Amanullah , M. Brodwin , N. Connolly , K. S. Dawson , M. Doi , P. Eisenhardt , L. Faccioli , V. Fadeyev , H. K. Fakhouri , A. S. Fruchter , D. G. Gilbank , M. D. Gladders , G. Goldhaber , A. Goobar , T. Hattori , E. Hsiao , X. Huang , Y. Ihara , N. Kashikawa , B. Koester , K. Konishi , M. Kowalski , C. Lidman , L. Lubin , J. Meyers , T. Morokuma , T. Oda , N. Panagia , S. Perlmutter , M. Postman , P. Ripoche , P. Rosati , D. Rubin , D. J. Schlegel , A. L. Spadafora , S. A. Stanford , M. Strovink , N. Suzuki , N. Takanashi , K. Tokita , N. Yasuda

Type-Ia Supernova Rates to Redshift 2.4 from CLASH: the Cluster Lensing And Supernova survey with Hubble

We present the supernova (SN) sample and Type-Ia SN (SN Ia) rates from the Cluster Lensing And Supernova survey with Hubble (CLASH). Using the Advanced Camera for Surveys and the Wide Field Camera 3 on the Hubble Space Telescope (HST), we…

宇宙学与河外天体物理 · 物理学 2015-06-17 O. Graur , S. A. Rodney , D. Maoz , A. G. Riess , S. W. Jha , M. Postman , T. Dahlen , T. W. -S. Holoien , C. McCully , B. Patel , L. -G. Strolger , N. Benitez , D. Coe , S. Jouvel , E. Medezinski , A. Molino , M. Nonino , L. Bradley , A. Koekemoer , I. Balestra , S. B. Cenko , K. I. Clubb , M. E. Dickinson , A. V. Filippenko , T. F. Frederiksen , P. Garnavich , J. Hjorth , D. O. Jones , B. Leibundgut , T. Matheson , B. Mobasher , P. Rosati , J. M. Silverman , V. U , K. Jedruszczuk , C. Li , K. Lin , M. Mirmelstein , J. Neustadt , A. Ovadia , E. H. Rogers

The Rate of Type Ia Supernovae at z~0.2 from SDSS-I Overlapping Fields

In the course of the Sloan Digital Sky Survey (SDSS-I), a large fraction of the surveyed area was observed more than once due to field tiling overlap, usually at different epochs. We utilize some of these data to perform a supernova (SN)…

天体物理学 · 物理学 2009-11-13 Assaf Horesh , Dovi Poznanski , Eran O. Ofek , Dan Maoz

An Intensive HST Survey for z>1 Supernovae by Targeting Galaxy Clusters

We present a new survey strategy to discover and study high redshift Type Ia supernovae (SNe Ia) using the Hubble Space Telescope (HST). By targeting massive galaxy clusters at 0.9<z<1.5, we obtain a twofold improvement in the efficiency of…

宇宙学与河外天体物理 · 物理学 2010-03-23 K. S. Dawson , G. Aldering , R. Amanullah , K. Barbary , L. F. Barrientos , M. Brodwin , N. Connolly , A. Dey , M. Doi , M. Donahue , P. Eisenhardt , E. Ellingson , L. Faccioli , V. Fadeyev , H. K. Fakhouri , A. S. Fruchter , D. G. Gilbank , M. D. Gladders , G. Goldhaber , A. H. Gonzalez , A. Goobar , A. Gude , T. Hattori , H. Hoekstra , X. Huang , Y. Ihara , B. T. Jannuzi , D. Johnston , K. Kashikawa , B. Koester , K. Konishi , M. Kowalski , C. Lidman , E. V. Linder , L. Lubin , J. Meyers , T. Morokuma , F. Munshi , C. Mullis , T. Oda , N. Panagia , S. Perlmutter , M. Postman , T. Pritchard , J. Rhodes , P. Rosati , D. Rubin , D. J. Schlegel , A. Spadafora , S. A. Stanford , V. Stanishev , D. Stern , M. Strovink , N. Suzuki , N. Takanashi , K. Tokita , M. Wagner , L. Wang , N. Yasuda , H. K. C. Yee

The Type Ia Supernova Rate in Redshift 0.5--0.9 Galaxy Clusters

Supernova (SN) rates are potentially powerful diagnostics of metal enrichment and SN physics, particularly in galaxy clusters with their deep, metal-retaining potentials and relatively simple star-formation histories. We have carried out a…

宇宙学与河外天体物理 · 物理学 2015-05-19 Keren Sharon , Avishay Gal-Yam , Dan Maoz , Alexei V. Filippenko , Ryan J. Foley , Jeffrey M. Silverman , Harald Ebeling , Cheng-Jiun Ma , Eran O. Ofek , Jean-Paul Kneib , Megan Donahue , Richard S. Ellis , Wendy L. Freedman , Robert P. Kirshner , John S. Mulchaey , Vicki L. Sarajedini , G. Mark Voit

The HST See Change Program: I. Survey Design, Pipeline, and Supernova Discoveries

The See Change survey was designed to make $z>1$ cosmological measurements by efficiently discovering high-redshift Type Ia supernovae (SNe Ia) and improving cluster mass measurements through weak lensing. This survey observed twelve galaxy…

宇宙学与河外天体物理 · 物理学 2021-05-19 Brian Hayden , David Rubin , Kyle Boone , Greg Aldering , Jakob Nordin , Mark Brodwin , Susana Deustua , Sam Dixon , Parker Fagrelius , Andy Fruchter , Peter Eisenhardt , Anthony Gonzalez , Ravi Gupta , Isobel Hook , Chris Lidman , Kyle Luther , Adam Muzzin , Zachary Raha , Pilar Ruiz-Lapuente , Clare Saunders , Caroline Sofiatti , Adam Stanford , Nao Suzuki , Tracy Webb , Steven C. Williams , Gillian Wilson , Mike Yen , Rahman Amanullah , Kyle Barbary , Hans Bohringer , Greta Chappell , Carlos Cunha , Miles Currie , Rene Fassbender , Michael Gladders , Ariel Goobar , Hendrik Hildenrandt , Henk Hoekstra , Xiaosheng Huang , Dragan Huterer , M. James Jee , Alex Kim , Marek Kowalski , Eric Linder , Joshua E. Meyers , Reynald Pain , Saul Perlmutter , Johan Richard , Piero Rosati , Eduardo Rozo , Eli Rykoff , Joana Santos , Anthony Spadafora , Daniel Stern , Risa Wechsler , The Supernova Cosmology Project

Type Ia Supernova Distances at z > 1.5 from the Hubble Space Telescope Multi-Cycle Treasury Programs: The Early Expansion Rate

We present an analysis of 15 Type Ia supernovae (SNe Ia) at redshift z > 1 (9 at 1.5 < z < 2.3) recently discovered in the CANDELS and CLASH Multi-Cycle Treasury programs using WFC3 on the Hubble Space Telescope. We combine these SNe Ia…

宇宙学与河外天体物理 · 物理学 2018-02-14 Adam G. Riess , Steven A. Rodney , Daniel M. Scolnic , Daniel L. Shafer , Louis-Gregory Strolger , Henry C. Ferguson , Marc Postman , Or Graur , Dan Maoz , Saurabh W. Jha , Bahram Mobasher , Stefano Casertano , Brian Hayden , Alberto Molino , Jens Hjorth , Peter M. Garnavich , David O. Jones , Robert P. Kirshner , Anton M. Koekemoer , Norman A. Grogin , Gabriel Brammer , Shoubaneh Hemmati , Mark Dickinson , Peter M. Challis , Schuyler Wolff , Kelsey I. Clubb , Alexei V. Filippenko , Hooshang Nayyeri , U Vivian , David C. Koo , Sandra M. Faber , Dale Kocevski , Larry Bradley , Dan Coe

The Hubble Space Telescope Cluster Supernova Survey: V. Improving the Dark Energy Constraints Above z>1 and Building an Early-Type-Hosted Supernova Sample

We present ACS, NICMOS, and Keck AO-assisted photometry of 20 Type Ia supernovae SNe Ia from the HST Cluster Supernova Survey. The SNe Ia were discovered over the redshift interval 0.623 < z < 1.415. Fourteen of these SNe Ia pass our strict…

宇宙学与河外天体物理 · 物理学 2012-08-21 N. Suzuki , D. Rubin , C. Lidman , G. Aldering , R. Amanullah , K. Barbary , L. F. Barrientos , J. Botyanszki , M. Brodwin , N. Connolly , K. S. Dawson , A. Dey , M. Doi , M. Donahue , S. Deustua , P. Eisenhardt , E. Ellingson , L. Faccioli , V. Fadeyev , H. K. Fakhouri , A. S. Fruchter , D. G. Gilbank , M. D. Gladders , G. Goldhaber , A. H. Gonzalez , A. Goobar , A. Gude , T. Hattori , H. Hoekstra , E. Hsiao , X. Huang , Y. Ihara , M. J. Jee , D. Johnston , N. Kashikawa , B. Koester , K. Konishi , M. Kowalski , E. V. Linder , L. Lubin , J. Melbourne , J. Meyers , T. Morokuma , F. Munshi , C. Mullis , T. Oda , N. Panagia , S. Perlmutter , M. Postman , T. Pritchard , J. Rhodes , P. Ripoche , P. Rosati , D. J. Schlegel , A. Spadafora , S. A. Stanford , V. Stanishev , D. Stern , M. Strovink , N. Takanashi , K. Tokita , M. Wagner , L. Wang , N. Yasuda , H. K. C. Yee

A Measurement of the Rate of type-Ia Supernovae at Redshift $z\approx$ 0.1 from the First Season of the SDSS-II Supernova Survey

We present a measurement of the rate of type Ia supernovae (SNe Ia) from the first of three seasons of data from the SDSS-II Supernova Survey. For this measurement, we include 17 SNe Ia at redshift $z\le0.12$. Assuming a flat cosmology with…

天体物理学 · 物理学 2010-11-05 Benjamin Dilday , R. Kessler , J. A. Frieman , J. Holtzman , J. Marriner , G. Miknaitis , R. C. Nichol , R. Romani , M. Sako , B. Bassett , A. Becker , D. Cinabro , F. DeJongh , D. L. Depoy , M. Doi , P. M. Garnavich , C. J. Hogan , S. Jha , K. Konishi , H. Lampeitl , J. L. Marshall , D. McGinnis , J. L. Prieto , A. G. Riess , M. W. Richmond , D. P. Schneider , M. Smith , N. Takanashi , K. Tokita , K. van der Heyden , N. Yasuda , C. Zheng , J. Barentine , H. Brewington , C. Choi , A. Crotts , J. Dembicky , M. Harvanek , M. Im , W. Ketzeback , S. J. Kleinman , J. Krzesiński , D. C. Long , E. Malanushenko , V. Malanushenko , R. J. McMillan , A. Nitta , K. Pan , G. Saurage , S. A. Snedden , S. Watters , J. C. Wheeler , D. York

Supernovae in Deep Hubble Space Telescope Galaxy Cluster Fields: Cluster Rates and Field Counts

We have searched for high-redshift supernova (SN) candidates in multiple deep Hubble Space Telescope (HST) archival images of nine galaxy-cluster fields. We detect six apparent SNe, with I814 between 21.6 and 28.4 mag. There is roughly 1 SN…

天体物理学 · 物理学 2009-11-07 Avishay Gal-Yam , Dan Maoz , Keren Sharon

The Hubble Space Telescope Cluster Supernova Survey: III. Correlated Properties of Type Ia Supernovae and Their Hosts at 0.9 < z < 1.46

Using the sample of Type Ia supernovae (SNe Ia) discovered by the Hubble Space Telescope (HST) Cluster Supernova Survey and augmented with HST-observed SNe Ia in the GOODS fields, we search for correlations between the properties of SNe and…

宇宙学与河外天体物理 · 物理学 2019-08-14 J. Meyers , G. Aldering , K. Barbary , L. F. Barrientos , M. Brodwin , K. S. Dawson , S. Deustua , M. Doi , P. Eisenhardt , L. Faccioli , H. K. Fakhouri , A. S. Fruchter , D. G. Gilbank , M. D. Gladders , G. Goldhaber , A. H. Gonzalez , T. Hattori , E. Hsiao , Y. Ihara , N. Kashikawa , B. Koester , K. Konishi , C. Lidman , L. Lubin , T. Morokuma , T. Oda , S. Perlmutter , M. Postman , P. Ripoche , P. Rosati , D. Rubin , E. Rykoff , A. Spadafora , S. A. Stanford , N. Suzuki , N. Takanashi , K. Tokita , N. Yasuda

The rate of Type-Ia supernovae in galaxy clusters and the delay-time distribution out to redshift 1.75

The observed delay-time distribution (DTD) of Type-Ia supernovae (SNe Ia) is a valuable probe of SN Ia progenitors and physics, and of the role of SNe Ia in cosmic metal enrichment. The SN Ia rate in galaxy clusters as a function of cluster…

星系天体物理 · 物理学 2018-07-11 Matan Friedmann , Dan Maoz

Measurements of the Rate of Type Ia Supernovae at Redshift z < ~0.3 from the SDSS-II Supernova Survey

We present a measurement of the volumetric Type Ia supernova (SN Ia) rate based on data from the Sloan Digital Sky Survey II (SDSS-II) Supernova Survey. The adopted sample of supernovae (SNe) includes 516 SNe Ia at redshift z \lesssim 0.3,…

宇宙学与河外天体物理 · 物理学 2010-05-07 Benjamin Dilday , Mathew Smith , Bruce Bassett , Andrew Becker , Ralf Bender , Francisco Castander , David Cinabro , Alexei V. Filippenko , Joshua A. Frieman , Lluis Galbany , Peter M. Garnavich , Ariel Goobar , Ulrich Hopp , Yutaka Ihara , Saurabh W. Jha , Richard Kessler , Hubert Lampeitl , John Marriner , Ramon Miquel , Mercedes Molla , Robert C. Nichol , Jakob Nordin , Adam G. Riess , Masao Sako , Donald P. Schneider , Jesper Sollerman , J. Craig Wheeler , Linda Ostman , Dmitry Bizyaev , Howard Brewington , Elena Malanushenko , Viktor Malanushenko , Dan Oravetz , Kaike Pan , Audrey Simmons , Stephanie Snedden

The Type Ia Supernova Rate at z$\sim 0.4 $

We present the first measurement of the rate of Type Ia supernovae at high redshift. The result is derived using a large subset of data from the Supernova Cosmology Project. Three supernovae were discovered in a surveyed area of 1.7 square…

天体物理学 · 物理学 2011-03-10 R. Pain , I. M. Hook , S. Deustua , S. Gabi , G. Goldhaber , A. Goobar , D. Groom , A. G. Kim , M. Y. Kim , J. C. Lee , C. R. Pennypacker , S. Perlmutter , I. A. Small , R. S. Ellis , R. G. McMahon , K. Glazebrook , B. J. Boyle , P. S. Bunclark , D. Carter , M. J. Irwin

Supernovae in Low-Redshift Galaxy Clusters: the Type-Ia Supernova Rate

Supernova (SN) rates are a potentially powerful diagnostic of star formation history (SFH), metal enrichment, and SN physics, particularly in galaxy clusters with their deep, metal-retaining potentials, and simple SFH. However, a…

天体物理学 · 物理学 2011-02-11 Keren Sharon , Avishay Gal-Yam , Dan Maoz , Alexei V. Filippenko , Puragra GuhaThakurta , .

A New Determination of the High Redshift Type Ia Supernova Rates with the Hubble Space Telescope Advanced Camera for Surveys

We present a new measurement of the volumetric rate of Type Ia supernova up to a redshift of 1.7, using the Hubble Space Telescope (HST) GOODS data combined with an additional HST dataset covering the North GOODS field collected in 2004. We…

天体物理学 · 物理学 2009-11-13 N. Kuznetsova , K. Barbary , B. Connolly , A. G. Kim , R. Pain , N. A. Roe , G. Aldering , R. Amanullah , K. Dawson , M. Doi , V. Fadeyev , A. S. Fruchter , R. Gibbons , G. Goldhaber , A. Goobar , A. Gude , R. A. Knop , M. Kowalski , C. Lidman , T. Morokuma , J. Meyers , S. Perlmutter , D. Rubin , D. J. Schlegel , A. L. Spadafora , V. Stanishev , M. Strovink , N. Suzuki , L. Wang , N. Yasuda

Correcting for peculiar velocities of Type Ia Supernovae in clusters of galaxies

Type Ia Supernovae (SNe Ia) are widely used to measure the expansion of the Universe. To perform such measurements the luminosity and cosmological redshift ($z$) of the SNe Ia have to be determined. The uncertainty on $z$ includes an…

宇宙学与河外天体物理 · 物理学 2018-08-01 P. -F. Léget , M. V. Pruzhinskaya , A. Ciulli , E. Gangler , G. Aldering , P. Antilogus , C. Aragon , S. Bailey , C. Baltay , K. Barbary , S. Bongard , K. Boone , C. Buton , M. Childress , N. Chotard , Y. Copin , S. Dixon , P. Fagrelius , U. Feindt , D. Fouchez , P. Gris , B. Hayden , W. Hillebrandt , D. A. Howell , A. Kim , M. Kowalski , D. Kuesters , S. Lombardo , Q. Lin , J. Nordin , R. Pain , E. Pecontal , R. Pereira , S. Perlmutter , D. Rabinowitz , M. Rigault , K. Runge , D. Rubin , C. Saunders , L. -P. Says , G. Smadja , C. Sofiatti , N. Suzuki , S. Taubenberger , C. Tao , R. C. Thomas

Confirmation of Hostless Type Ia Supernovae Using Hubble Space Telescope Imaging

We present deep Hubble Space Telescope imaging at the locations of four, potentially hostless, long-faded Type Ia supernovae (SNe Ia) in low-redshift, rich galaxy clusters that were identified in the Multi-Epoch Nearby Cluster Survey.…

星系天体物理 · 物理学 2015-07-15 Melissa L. Graham , David J. Sand , Dennis Zaritsky , Chris J. Pritchet

New Hubble Space Telescope Discoveries of Type Ia Supernovae at z > 1: Narrowing Constraints on the Early Behavior of Dark Energy

We have discovered 21 new Type Ia supernovae (SNe Ia) with the Hubble Space Telescope (HST) and have used them to trace the history of cosmic expansion over the last 10 billion years. These objects, which include 13 spectroscopically…

天体物理学 · 物理学 2008-11-26 Adam G. Riess , Louis-Gregory Strolger , Stefano Casertano , Henry C. Ferguson , Bahram Mobasher , Ben Gold , Peter J. Challis , Alexei V. Filippenko , Saurabh Jha , Weidong Li , John Tonry , Ryan Foley , Robert P. Kirshner , Mark Dickinson , Emily MacDonald , Daniel Eisenstein , Mario Livio , Josh Younger , Chun Xu , Tomas Dahlen , Daniel Stern

Two Type Ia Supernovae at Redshift ~2 : Improved Classification and Redshift Determination with Medium-band Infrared Imaging

We present two supernovae (SNe) discovered with the Hubble Space Telescope (HST) in the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey (CANDELS), an HST multi-cycle treasury program. We classify both objects as Type Ia SNe…

宇宙学与河外天体物理 · 物理学 2016-02-17 Steven A. Rodney , Adam G. Riess , Daniel M. Scolnic , David O. Jones , Shoubaneh Hemmati , Alberto Molino , Curtis McCully , Bahram Mobasher , Louis-Gregory Strolger , Or Graur , Brian Hayden , Stefano Casertano