7 results on '"Brandon Patel"'
Search Results
2. Exclusion of a luminous red giant as a companion star to the progenitor of supernova SN 2011fe
- Author
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Peter Nugent, Kate Maguire, Nathaniel R. Butler, Weidong Li, Robert M. Quimby, Nicholas M. Law, Jeffrey M. Silverman, Joshua S. Bloom, Mohan Ganeshalingam, Alexei V. Filippenko, Joseph W. Richards, Philipp Podsiadlowski, Lars Bildsten, Eran O. Ofek, Adam A. Miller, Ken J. Shen, S. Bradley Cenko, Mark Sullivan, Hsin-Yi Shih, Shrinivas R. Kulkarni, Joanne Bibby, Saurabh Jha, D. Andrew Howell, Dovi Poznanski, Brandon Patel, A. Stockton, Michael M. Shara, C. McCully, and Mansi M. Kasliwal
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Physics ,Multidisciplinary ,Red giant ,Carbon detonation ,Astrophysics::High Energy Astrophysical Phenomena ,White dwarf ,Astronomy ,Astrophysics ,Astrophysics::Cosmology and Extragalactic Astrophysics ,Type II supernova ,01 natural sciences ,Black dwarf ,Supernova ,0103 physical sciences ,Astrophysics::Solar and Stellar Astrophysics ,Astrophysics::Earth and Planetary Astrophysics ,010306 general physics ,010303 astronomy & astrophysics ,Stellar evolution ,Blue dwarf ,Astrophysics::Galaxy Astrophysics - Abstract
Type Ia supernovae are thought to result from a thermonuclear explosion of an accreting white dwarf in a binary system1, 2, but little is known of the precise nature of the companion star and the physical properties of the progenitor system. There are two classes of models1, 3: double-degenerate (involving two white dwarfs in a close binary system2, 4) and single-degenerate models5, 6. In the latter, the primary white dwarf accretes material from a secondary companion until conditions are such that carbon ignites, at a mass of 1.38 times the mass of the Sun. The type Ia supernova SN 2011fe was recently detected in a nearby galaxy7. Here we report an analysis of archival images of the location of SN 2011fe. The luminosity of the progenitor system (especially the companion star) is 10–100 times fainter than previous limits on other type Ia supernova progenitor systems8, 9, 10, allowing us to rule out luminous red giants and almost all helium stars as the mass-donating companion to the exploding white dwarf.
- Published
- 2016
3. 'Refsdal' Meets Popper: Comparing Predictions of the Re-appearance of the Multiply Imaged Supernova Behind MACSJ1149.5+2223
- Author
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G. B. Caminha, Jose M. Diego, Tom Broadhurst, Masafumi Ishigaki, Claudio Grillo, Brandon Patel, Alexei V. Filippenko, Kasper B. Schmidt, Austin Hoag, Sherry H. Suyu, Italo Balestra, Adi Zitrin, L. G. Strolger, Aleksi Halkola, Traci L. Johnson, W. Karman, Saurabh Jha, Ryota Kawamata, Tommaso Treu, Patrick L. Kelly, Marusa Bradac, R. J. Foley, Keren Sharon, Gabriel B. Brammer, Steven A. Rodney, Piero Rosati, Amata Mercurio, Masamune Oguri, Astronomy, ITA, USA, DEU, Ministry of Education, Culture, Sports, Science and Technology (Japan), Alfred P. Sloan Foundation, Villum Fonden, National Science Foundation (US), David and Lucile Packard Foundation, National Aeronautics and Space Administration (US), and Ministerio de Economía y Competitividad (España)
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Cosmology and Nongalactic Astrophysics (astro-ph.CO) ,gravitational lensing ,FOS: Physical sciences ,Magnification ,Scale (descriptive set theory) ,Astrophysics ,Astrophysics::Cosmology and Extragalactic Astrophysics ,strong ,01 natural sciences ,Cosmology ,NO ,0103 physical sciences ,010306 general physics ,010303 astronomy & astrophysics ,Astrophysics::Galaxy Astrophysics ,Physics ,Line-of-sight ,gravitational lensing: strong ,Astronomy and Astrophysics ,Extragalactic astronomy ,Supernova ,Gravitational lens ,Space and Planetary Science ,Event (particle physics) ,Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
arXiv:1510.05750v2.-- et al., Supernova "Refsdal", multiply imaged by cluster MACS1149.5+2223, represents a rare opportunity to make a true blind test of model predictions in extragalactic astronomy, on a timescale that is short compared to a human lifetime. In order to take advantage of this event, we produced seven gravitational lens models with five independent methods, based on Hubble Space Telescope (HST) Hubble Frontier Field images, along with extensive spectroscopic follow-up observations by HST, the Very Large and the Keck Telescopes. We compare the model predictions and show that they agree reasonably well with the measured time delays and magnification ratios between the known images, even though these quantities were not used as input. This agreement is encouraging, considering that the models only provide statistical uncertainties, and do not include additional sources of uncertainties such as structure along the line of sight, cosmology, and the mass sheet degeneracy. We then present the model predictions for the other appearances of supernova >Refsdal.> A future image will reach its peak in the first half of 2016, while another image appeared between 1994 and 2004. The past image would have been too faint to be detected in existing archival images. The future image should be approximately one-third as bright as the brightest known image (i.e., mag at peak and mag six months before peak), and thus detectable in single-orbit HST images. We will find out soon whether our predictions are correct., This work is supported by NASA through grants HST-GO-13459 and HST-GO-14041 from the Space Telescope Science Institute (STScI), which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555. T.T. is supported by the Packard Foundation in the form of a Packard Research Fellowship. J.M.D. is grateful for support from the consolider project CSD2010-00064 and AYA2012-39475-C02-01 funded by the Ministerio de Economia y Competitividad. A.V.F.'s research is supported by the Christopher R. Redlich Fund, the TABASGO Foundation, and NSF grant AST-1211916. C.G. acknowledges support by the VILLUM FONDEN Young Investigator Programme through grant no. 10123. Support for A.Z. was provided by NASA through Hubble Fellowship grant #HST-HF2-51334.001-A awarded by STScI. The work of M.O. was supported in part by World Premier International Research Center Initiative (WPI Initiative), MEXT, Japan, and Grant-in-Aid for Scientific Research from the JSPS (26800093). Financial support for this work was provided to S.A.R. by NASA through grants HST-HF-51312 and HST-GO-13386 from STScI. A.H. is supported by NASA Head-quarters under the NASA Earth and Space Science Fellowship Program, grant ASTRO14F-0007. R.J.F. gratefully acknowledges support from NSF grant AST-1518052, NASA grants HST-GO-14041 and HST-GO-13386, and the Alfred P. Sloan Foundation. This work was supported in part by a NASA Keck PI Data Award (PID 47/2014B N125D, PI Jha).
- Published
- 2016
4. Illuminating a dark lens : a Type Ia Supernova magnified by the Frontier Fields galaxy cluster Abell 2744
- Author
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Liliya L. R. Williams, Tom Broadhurst, Jose M. Diego, Curtis McCully, Alberto Molino, Mathilde Jauzac, Tommaso Treu, Adi Zitrin, Traci L. Johnson, Daniel Scolnic, Brandon Patel, Julian Merten, Massimo Meneghetti, Xin Wang, Johan Richard, Marusa Bradac, Jens Hjorth, Elinor Medezinski, Steven A. Rodney, Or Graur, Daniel Lam, Saurabh Jha, Gabriel Brammer, Keren Sharon, Louis-Gregory Strolger, Adam G. Riess, Patrick L. Kelly, Dan Coe, Austin Hoag, Ryan J. Foley, Johns Hopkins University (JHU), Rutgers University System (Rutgers), Department of Physics [Chicago], University of Chicago, University of Illinois at Urbana-Champaign [Urbana], University of Illinois System, Universidad de Granada = University of Granada (UGR), Space Telescope Science Institute (STSci), Institute for Computational Cosmology (ICC), Durham University, University of California [Davis] (UC Davis), University of California (UC), Ikerbasque - Basque Foundation for Science, Universidad de Cantabria [Santander], New York University [New York] (NYU), NYU System (NYU), Dark Cosmology Centre (DARK), Niels Bohr Institute [Copenhagen] (NBI), Faculty of Science [Copenhagen], University of Copenhagen = Københavns Universitet (UCPH)-University of Copenhagen = Københavns Universitet (UCPH)-Faculty of Science [Copenhagen], University of Copenhagen = Københavns Universitet (UCPH)-University of Copenhagen = Københavns Universitet (UCPH), University of Michigan [Ann Arbor], University of Michigan System, Lawrence Berkeley National Laboratory [Berkeley] (LBNL), The University of Hong Kong (HKU), Las Cumbres Observatory (LCO), INAF - Osservatorio Astronomico di Bologna (OABO), Istituto Nazionale di Astrofisica (INAF), Department of Physics [Oxford], University of Oxford, Centre de Recherche Astrophysique de Lyon (CRAL), École normale supérieure de Lyon (ENS de Lyon)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Department of Physics and Astronomy [UCLA, Los Angeles], University of California [Los Angeles] (UCLA), University of California (UC)-University of California (UC), Department of Physics [Santa Barbara] (PHYSICS-UCSB), University of California [Santa Barbara] (UC Santa Barbara), University of Minneapolis, California Institute of Technology (CALTECH), California Institute of Technology, Ministerio de Economía y Competitividad (España), National Science Foundation (US), Rutgers University, Fundação para o Desenvolvimento da Unesp, National Aeronautics and Space Administration (US), European Commission, David and Lucile Packard Foundation, University of Minnesota, Danish National Research Foundation, University of Granada [Granada], University of California, Fisika Teorikoa (IKERBASQUE), University of Copenhagen = Københavns Universitet (KU)-University of Copenhagen = Københavns Universitet (KU)-Faculty of Science [Copenhagen], University of Copenhagen = Københavns Universitet (KU)-University of Copenhagen = Københavns Universitet (KU), University of Oxford [Oxford], École normale supérieure - Lyon (ENS Lyon)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS), University of California-University of California, and University of California [Santa Barbara] (UCSB)
- Subjects
Galaxies: clusters: individual (Abell 2744) ,Cosmology and Nongalactic Astrophysics (astro-ph.CO) ,Gravitational lensing: strong ,Supernovae: general ,individual (HFF14Tom) [Supernovae] ,general [Supernovae] ,FOS: Physical sciences ,Magnification ,Astrophysics ,clusters: general [Galaxies] ,strong [Gravitational lensing] ,01 natural sciences ,law.invention ,[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO] ,Gravitational lensing: weak ,law ,0103 physical sciences ,Cluster (physics) ,010303 astronomy & astrophysics ,Galaxy cluster ,Physics ,010308 nuclear & particles physics ,clusters: individual (Abell 2744) [Galaxies] ,Astronomy and Astrophysics ,Galaxy ,Redshift ,Lens (optics) ,individual (HFF14Tom). [Supernovae] ,Supernovae: individual (HFF14Tom) ,Supernova ,Abell 2744 ,Space and Planetary Science ,Galaxies: clusters: general ,weak [Gravitational lensing] ,Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
Facility: HST (WFC3).-- Rodney, Steven A. et al., SN HFF14Tom is a Type Ia SN discovered at Z = 1.3457 ± 0.0001 behind the galaxy cluster Abell 2744 (Z = 0.308). In a cosmology-independent analysis, we find that HFF14Tom is 0.77 ± 0.15 mag brighter than unlensed Type Ia SNe at similar redshift, implying a lensing magnification of μ = 2.03 ± 0.29. This observed magnification provides a rare opportunity for a direct empirical test of galaxy cluster lens models. Here we test 17 lens models, 13 of which were generated before the SN magnification was known, qualifying as pure >blind tests. > The models are collectively fairly accurate: 8 of the models deliver median magnifications that are consistent with the measured μ to within 1λ. However, there is a subtle systematic bias: the significant disagreements all involve models overpredicting the magnification. We evaluate possible causes for this mild bias, and find no single physical or methodological explanation to account for it. We do find that model accuracy can be improved to some extent with stringent quality cuts on multiply imaged systems, such as requiring that a large fraction have spectroscopic redshifts. In addition to testing model accuracies as we have done here, Type Ia SN magnifications could also be used as inputs for future lens models of Abell 2744 and other clusters, providing valuable constraints in regions where traditional strong- and weak-lensing information is unavailable., Financial support for this work was provided to S.A.R. by NASA through grants HST-HF-51312 and HST-GO-13386 from STScI, which is operated by Associated Universities for Research in Astronomy, Inc. (AURA), under NASA contract NAS 5-26555. A.M. acknowledge the financial support of the Brazilian funding agency FAPESP (Post-doc fellowship—process number 2014/11806-9). Support for this research at Rutgers University was provided in part by NSF CAREER award AST-0847157 to SWJ. The Dark Cosmology Centre is supported by the Danish National Research Foundation. J.M.D. acknowledges support of the consolider project CSD2010-00064 and AYA2012–39475-C02-01 funded by the Ministerio de Economia y Competitividad. J.M. contributed to this research from the Jet Propulsion Laboratory, California Institute of Technology, under a contract with NASA and acknowledges support from NASA Grants HST-GO-13343.05-A and HST-GO-13386.13-A. The research leading to these results has received funding from the People Programme (Marie Curie Actions) of the European Union's Seventh Framework Programme (FP7/20072013) under REA grant agreement number 627288. A.Z. acknowledges financial support from NASA through grant HST-HF-51334.01-A awarded by STScI and operated by AURA. T.T. acknowledges support by the Packard Foundation in the form of Packard Research Fellowship. GLASS is funded by NASA through HST grant GO-13459. L.L.R.W. acknowledges the support of the Minnesota Supercomputing Institute.
- Published
- 2015
5. Multiple images of a highly magnified supernova formed by an early-type cluster galaxy lens
- Author
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Alessandro Sonnenfeld, Anja von der Linden, Michele Trenti, B. E. Tucker, Marc Postman, Brandon Patel, Adam G. Riess, Benjamin J. Weiner, Or Graur, Steven A. Rodney, Alexei V. Filippenko, Raphael Gavazzi, Matthew A. Malkan, Patrick L. Kelly, Daniel Scolnic, Marusa Bradac, Jens Hjorth, Curtis McCully, Gabriel B. Brammer, Julian Merten, Adriano Fontana, Ryan J. Foley, Melissa L. Graham, Adi Zitrin, T. A. Jones, Alan Dressler, Tommaso Treu, Kasper B. Schmidt, S. Bradley Cenko, Saurabh Jha, and Louis-Gregory Strolger
- Subjects
Cosmology and Nongalactic Astrophysics (astro-ph.CO) ,General Science & Technology ,Astrophysics::High Energy Astrophysical Phenomena ,astro-ph.GA ,FOS: Physical sciences ,Astrophysics ,Astrophysics::Cosmology and Extragalactic Astrophysics ,01 natural sciences ,Metric expansion of space ,symbols.namesake ,Gravitational potential ,0103 physical sciences ,010303 astronomy & astrophysics ,Astrophysics::Galaxy Astrophysics ,Physics ,Multidisciplinary ,010308 nuclear & particles physics ,Astrophysics - Astrophysics of Galaxies ,Redshift ,Galaxy ,Einstein Cross ,Supernova ,Gravitational lens ,Astrophysics of Galaxies (astro-ph.GA) ,Elliptical galaxy ,symbols ,astro-ph.CO ,Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
In 1964, Refsdal hypothesized that a supernova whose light traversed multiple paths around a strong gravitational lens could be used to measure the rate of cosmic expansion. We report the discovery of such a system. In Hubble Space Telescope imaging, we have found four images of a single supernova forming an Einstein cross configuration around a redshift z=0.54 elliptical galaxy in the MACS J1149.6+2223 cluster. The cluster's gravitational potential also creates multiple images of the z=1.49 spiral supernova host galaxy, and a future appearance of the supernova elsewhere in the cluster field is expected. The magnifications and staggered arrivals of the supernova images probe the cosmic expansion rate, as well as the distribution of matter in the galaxy and cluster lenses., Published in the 6 March 2015 issue of Science; 17 pages, 7 figures, and 3 tables including Supplementary Materials
- Published
- 2015
6. Astrophysics. Multiple images of a highly magnified supernova formed by an early-type cluster galaxy lens
- Author
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Patrick L, Kelly, Steven A, Rodney, Tommaso, Treu, Ryan J, Foley, Gabriel, Brammer, Kasper B, Schmidt, Adi, Zitrin, Alessandro, Sonnenfeld, Louis-Gregory, Strolger, Or, Graur, Alexei V, Filippenko, Saurabh W, Jha, Adam G, Riess, Marusa, Bradac, Benjamin J, Weiner, Daniel, Scolnic, Matthew A, Malkan, Anja, von der Linden, Michele, Trenti, Jens, Hjorth, Raphael, Gavazzi, Adriano, Fontana, Julian C, Merten, Curtis, McCully, Tucker, Jones, Marc, Postman, Alan, Dressler, Brandon, Patel, S Bradley, Cenko, Melissa L, Graham, and Bradley E, Tucker
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General Science & Technology ,Astrophysics::High Energy Astrophysical Phenomena ,Astrophysics::Cosmology and Extragalactic Astrophysics ,Astrophysics::Galaxy Astrophysics - Abstract
In 1964, Refsdal hypothesized that a supernova whose light traversed multiple paths around a strong gravitational lens could be used to measure the rate of cosmic expansion. We report the discovery of such a system. In Hubble Space Telescope imaging, we have found four images of a single supernova forming an Einstein cross configuration around a redshift z = 0.54 elliptical galaxy in the MACS J1149.6+2223 cluster. The cluster's gravitational potential also creates multiple images of the z = 1.49 spiral supernova host galaxy, and a future appearance of the supernova elsewhere in the cluster field is expected. The magnifications and staggered arrivals of the supernova images probe the cosmic expansion rate, as well as the distribution of matter in the galaxy and cluster lenses.
- Published
- 2015
7. ILLUMINATING A DARK LENS: A TYPE Ia SUPERNOVA MAGNIFIED BY THE FRONTIER FIELDS GALAXY CLUSTER ABELL 2744.
- Author
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Steven A. Rodney, Brandon Patel, Daniel Scolnic, Ryan J. Foley, Alberto Molino, Gabriel Brammer, Mathilde Jauzac, Maruša Bradač, Tom Broadhurst, Dan Coe, Jose M. Diego, Or Graur, Jens Hjorth, Austin Hoag, Saurabh W. Jha, Traci L. Johnson, Patrick Kelly, Daniel Lam, Curtis McCully, and Elinor Medezinski
- Subjects
- *
GALAXY clusters , *TYPE I supernovae , *CATACLYSMIC variable stars , *METAPHYSICAL cosmology , *LARGE quasar groups - Abstract
SN HFF14Tom is a Type Ia SN discovered at behind the galaxy cluster Abell 2744 (z = 0.308). In a cosmology-independent analysis, we find that HFF14Tom is 0.77 ± 0.15 mag brighter than unlensed Type Ia SNe at similar redshift, implying a lensing magnification of This observed magnification provides a rare opportunity for a direct empirical test of galaxy cluster lens models. Here we test 17 lens models, 13 of which were generated before the SN magnification was known, qualifying as pure “blind tests.” The models are collectively fairly accurate: 8 of the models deliver median magnifications that are consistent with the measured μ to within 1σ. However, there is a subtle systematic bias: the significant disagreements all involve models overpredicting the magnification. We evaluate possible causes for this mild bias, and find no single physical or methodological explanation to account for it. We do find that model accuracy can be improved to some extent with stringent quality cuts on multiply imaged systems, such as requiring that a large fraction have spectroscopic redshifts. In addition to testing model accuracies as we have done here, Type Ia SN magnifications could also be used as inputs for future lens models of Abell 2744 and other clusters, providing valuable constraints in regions where traditional strong- and weak-lensing information is unavailable. [ABSTRACT FROM AUTHOR]
- Published
- 2015
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