Zobrazeno 1 - 10
of 67
pro vyhledávání: '"K. Barbary"'
Autor:
P.-F. Léget, E. Gangler, F. Mondon, G. Aldering, P. Antilogus, C. Aragon, S. Bailey, C. Baltay, K. Barbary, S. Bongard, K. Boone, C. Buton, N. Chotard, Y. Copin, S. Dixon, P. Fagrelius, U. Feindt, D. Fouchez, B. Hayden, W. Hillebrandt, A. Kim, M. Kowalski, D. Kuesters, S. Lombardo, Q. Lin, J. Nordin, R. Pain, E. Pecontal, R. Pereira, S. Perlmutter, K. A. Ponder, M. V. Pruzhinskaya, 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
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2020, 636, pp.A46. ⟨10.1051/0004-6361/201834954⟩
Astronomy and astrophysics 636, A46-(2020). doi:10.1051/0004-6361/201834954
Astron.Astrophys.
Astron.Astrophys., 2020, 636, pp.A46. ⟨10.1051/0004-6361/201834954⟩
Astronomy & Astrophysics
Astronomy and Astrophysics-A&A, 2020, 636, pp.A46. ⟨10.1051/0004-6361/201834954⟩
Astronomy and astrophysics 636, A46-(2020). doi:10.1051/0004-6361/201834954
Astron.Astrophys.
Astron.Astrophys., 2020, 636, pp.A46. ⟨10.1051/0004-6361/201834954⟩
Astronomy & Astrophysics
Type Ia Supernovae (SNe Ia) are widely used to measure the expansion of the Universe. Improving distance measurements of SNe Ia is one technique to better constrain the acceleration of expansion and determine its physical nature. This document develo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::12f6fc1508e769bea3578dfc64343698
https://hal.science/hal-02371622
https://hal.science/hal-02371622
Autor:
Nao Suzuki, Mark Brodwin, Steven Williams, Susana E. Deustua, R. R. Gupta, Brian Hayden, K. Barbary, David Rubin, A. L. Spadafora, Zachary Raha, S. Dixon, Eric V. Linder, Kyle Boone, Rahman Amanullah, Pilar Ruiz-Lapuente, S. A. Stanford, C. Lidman, Marek Kowalski, A. S. Fruchter, Ariel Goobar, D. Stern, Anthony H. Gonzalez, M. J. Jee, Clare Saunders, Jakob Nordin, Kyle Luther, Reynald Pain, X. Huang, A. G. Kim, Greg Aldering, Caroline Sofiatti, Isobel Hook, Saul Perlmutter, M. Rigault, Peter Eisenhardt
Publikováno v:
Astrophys.J.
Astrophys.J., 2018, 866 (1), pp.65. ⟨10.3847/1538-4357/aad565⟩
Astrophysical Journal, vol 866, iss 1
Rubin, D; Hayden, B; Huang, X; Aldering, G; Amanullah, R; Barbary, K; et al.(2018). The Discovery of a Gravitationally Lensed Supernova Ia at Redshift 2.22. Astrophysical Journal, 866(1). doi: 10.3847/1538-4357/aad565. Lawrence Berkeley National Laboratory: Retrieved from: http://www.escholarship.org/uc/item/00x6m3wh
The Astrophysical Journal, vol 866, iss 1
Astrophys.J., 2018, 866 (1), pp.65. ⟨10.3847/1538-4357/aad565⟩
Astrophysical Journal, vol 866, iss 1
Rubin, D; Hayden, B; Huang, X; Aldering, G; Amanullah, R; Barbary, K; et al.(2018). The Discovery of a Gravitationally Lensed Supernova Ia at Redshift 2.22. Astrophysical Journal, 866(1). doi: 10.3847/1538-4357/aad565. Lawrence Berkeley National Laboratory: Retrieved from: http://www.escholarship.org/uc/item/00x6m3wh
The Astrophysical Journal, vol 866, iss 1
We present the discovery and measurements of a gravitationally lensed supernova (SN) behind the galaxy cluster MOO J1014+0038. Based on multi-band Hubble Space Telescope and Very Large Telescope (VLT) photometry of the supernova, and VLT spectroscopy
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b80d1959e64426760fc73eb1ddebc837
https://doi.org/10.3847/1538-4357/aad565
https://doi.org/10.3847/1538-4357/aad565
Autor:
Emmanuel Pecontal, S. Lombardo, C. Saunders, R. Pereira, Cecilia Aragon, C. Baltay, V. Brinnel, Marek Kowalski, Caroline Sofiatti, Mickael Rigault, Greg Aldering, Stephen Bailey, Wolfgang Hillebrandt, U. Feindt, David Rubin, P. Antilogus, D. Kuesters, S. Bongard, K. Barbary, A. G. Kim, Jakob Nordin, R. C. Thomas, N. Chotard, Reynald Pain, David Rabinowitz, Dominique Fouchez, C. Buton, Kyle Boone, E. Gangler, Nao Suzuki, Saul Perlmutter, Parker Fagrelius, Dale Andrew Howell, Q. Lin, Y. Copin, Brian Hayden, S. Taubenberger, P.-F. Leget, G. Smadja, S. Dixon, K. Runge, Charling Tao, M. Childress
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2020, 644, pp.A176. ⟨10.1051/0004-6361/201730404⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 644, pp.A176. ⟨10.1051/0004-6361/201730404⟩
Astronomy and astrophysics 644, A176 (1-20) (2020). doi:10.1051/0004-6361/201730404
Astronomy and Astrophysics-A&A, 2020, 644, pp.A176. ⟨10.1051/0004-6361/201730404⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 644, pp.A176. ⟨10.1051/0004-6361/201730404⟩
Astronomy and astrophysics 644, A176 (1-20) (2020). doi:10.1051/0004-6361/201730404
Astronomy and astrophysics 644, A176 (1-20) (2020). doi:10.1051/0004-6361/201730404
As part of an on-going effort to identify, understand and correct for astrophysics biases in the standardization of Type Ia supernovae (SNIa) for cosmology, we h
As part of an on-going effort to identify, understand and correct for astrophysics biases in the standardization of Type Ia supernovae (SNIa) for cosmology, we h
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bb67615848709b2198903cd6d701ea89
https://hal.archives-ouvertes.fr/hal-01827966
https://hal.archives-ouvertes.fr/hal-01827966
Autor:
Mickael Rigault, S. Bongard, K. Barbary, Greg Aldering, C. Baltay, Q. Lin, L.-P. Says, David Rabinowitz, S. Lombardo, C. Saunders, Stephen Bailey, Charling Tao, M. Childress, A. G. Kim, P.-F. Leget, N. Chotard, Caroline Sofiatti, D. Kuesters, Dominique Fouchez, C. Buton, Kyle Boone, Nao Suzuki, Philippe Luc Yves Gris, E. Gangler, Marek Kowalski, K. Runge, Dale Andrew Howell, Emmanuel Pecontal, A. Ciulli, Parker Fagrelius, Wolfgang Hillebrandt, U. Feindt, S. Dixon, R. Pereira, P. Antilogus, Saul Perlmutter, Maria Pruzhinskaya, Reynald Pain, Cecilia Aragon, Y. Copin, G. Smadja, Brian Hayden, S. Taubenberger, Jakob Nordin, R. C. Thomas, David Rubin
Publikováno v:
Astron.Astrophys.
Astron.Astrophys., 2018, 615, pp.A162. ⟨10.1051/0004-6361/201832932⟩
Astronomy & Astrophysics
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2018, 615, pp.A162. ⟨10.1051/0004-6361/201832932⟩
Astronomy and astrophysics 615, A162 (2018). doi:10.1051/0004-6361/201832932
Astron.Astrophys., 2018, 615, pp.A162. ⟨10.1051/0004-6361/201832932⟩
Astronomy & Astrophysics
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2018, 615, pp.A162. ⟨10.1051/0004-6361/201832932⟩
Astronomy and astrophysics 615, A162 (2018). doi:10.1051/0004-6361/201832932
Astronomy and astrophysics 615, A162 (2018). doi:10.1051/0004-6361/201832932
Context. 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)
Context. 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)
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::715603eeeb0a234711b78b9b507b0ce9
https://hal.archives-ouvertes.fr/hal-01781928
https://hal.archives-ouvertes.fr/hal-01781928
Autor:
V. Brinnel, Reynald Pain, D. Kuesters, P. Antilogus, David Rabinowitz, R. Pereira, G. Smadja, S. Dixon, C. Baltay, K. Barbary, P. F. Leget, Dominique Fouchez, Kyle Boone, S. Bongard, Cecilia Aragon, Charling Tao, M. Childress, Parker Fagrelius, Saul Perlmutter, K. Runge, Caroline Sofiatti, E. Gangler, Marek Kowalski, N. Chotard, C. Buton, Q. Lin, M. Rigault, Alex G. Kim, David Rubin, Greg Aldering, Jakob Nordin, S. Lombardo, C. Saunders, R. C. Thomas, U. Feindt, Stephen Bailey, Wolfgang Hillebrandt, Nao Suzuki, Y. Copin, Brian Hayden, S. Taubenberger, E. Pecontal
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2018, 614, pp.A71. ⟨10.1051/0004-6361/201732137⟩
NASA Astrophysics Data System
Astron.Astrophys.
Astron.Astrophys., 2018, 614, pp.A71. ⟨10.1051/0004-6361/201732137⟩
Astronomy and Astrophysics-A&A, 2018, 614, pp.A71. ⟨10.1051/0004-6361/201732137⟩
NASA Astrophysics Data System
Astron.Astrophys.
Astron.Astrophys., 2018, 614, pp.A71. ⟨10.1051/0004-6361/201732137⟩
Context. Observations of Type Ia supernovae (SNe Ia) can be used to derive accurate cosmological distances through empirical standardization techniques. Despite this success neither the progenitors of SNe Ia nor the explosion process are fully unders
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::81138b37af6fe55c998beac1b854b3ff
https://hal.science/hal-01703686
https://hal.science/hal-01703686
Autor:
C. Buton, S. Lombardo, Charling Tao, Alex G. Kim, Stephen Bailey, K. Barbary, E. Gangler, Marek Kowalski, Stefan Taubenberger, David Rubin, J. Chen, S. Dixon, G. Smadja, D. Küsters, Greg Aldering, Klaus Reif, N. Chotard, M. Rigault, A. Hoffmann, David Rabinowitz, C. Baltay, K. Runge, Dominique Fouchez, Y. Copin, Kyle Boone, Brian Hayden, L. Mckay, Jakob Nordin, R. C. Thomas, S. Bongard, Saul Perlmutter, U. Feindt, E. Pecontal, Parker Fagrelius, P. Antilogus, R. Pereira, Wolfgang Hillebrandt, Clare Saunders, P. F. Leget, Reynald Pain, Nao Suzuki, D. Baugh
Publikováno v:
Lombardo, S; Küsters, D; Kowalski, M; Aldering, G; Antilogus, P; Bailey, S; et al.(2017). SCALA: In situ calibration for integral field spectrographs. Astronomy and Astrophysics, 607. doi: 10.1051/0004-6361/201731076. Lawrence Berkeley National Laboratory: Retrieved from: http://www.escholarship.org/uc/item/5q18t7vw
Astronomy and astrophysics 607, A113 (2017). doi:10.1051/0004-6361/201731076
Astron.Astrophys.
Astron.Astrophys., 2017, 607, pp.A113. ⟨10.1051/0004-6361/201731076⟩
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2017, 607, pp.A113. ⟨10.1051/0004-6361/201731076⟩
Astronomy and Astrophysics-A&A, 2017, 607, pp.A113. ⟨10.1051/0004-6361/201731076⟩
Astronomy and astrophysics 607, A113 (2017). doi:10.1051/0004-6361/201731076
Astron.Astrophys.
Astron.Astrophys., 2017, 607, pp.A113. ⟨10.1051/0004-6361/201731076⟩
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2017, 607, pp.A113. ⟨10.1051/0004-6361/201731076⟩
Astronomy and Astrophysics-A&A, 2017, 607, pp.A113. ⟨10.1051/0004-6361/201731076⟩
Astronomy and astrophysics 607, A113 (2017). doi:10.1051/0004-6361/201731076
The scientific yield of current and future optical surveys is increasingly limited by systematic uncertainties in the flux calibration. This is the case for type Ia sup
The scientific yield of current and future optical surveys is increasingly limited by systematic uncertainties in the flux calibration. This is the case for type Ia sup
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c489fefa2929d7c2e4a09d07885575f9
http://www.escholarship.org/uc/item/5q18t7vw
http://www.escholarship.org/uc/item/5q18t7vw
Autor:
Tomonori Totani, D. Andrew Howell, Hisanori Furusawa, Gerson Goldhaber, Yutaka Ihara, Hiroyuki Utsunomiya, Joshua Meyers, Kyle S. Dawson, Takeshi Oda, Naohiro Takanashi, Nobunari Kashikawa, Junji Hayano, Takashi Hattori, A. L. Spadafora, Naoki Yasuda, David Rubin, Christopher Lidman, Greg Aldering, Isobel Hook, Reynald Pain, K. Barbary, Saul Perlmutter, R. A. Knop, Kohki Konishi, Kouichi Tokita, Mamoru Doi, Tomoki Morokuma, Lifan Wang, Nao Suzuki, Vitaliy Fadeyev, H. K. Fakhouri, Ariel Goobar, Rahman Amanullah
Publikováno v:
Publications of the Astronomical Society of Japan. 62:19-37
We present spectra of high-redshift supernovae (SNe) that were taken with the Subaru low resolution optical spectrograph, FOCAS. These SNe were found in SN surveys with Suprime-Cam on Subaru, the CFH12k camera on the Canada-France-Hawaii Telescope (C
Autor:
Evan R. Sparks, Michael J. Franklin, Frank Austin Nothaft, David A. Patterson, K. Barbary, Saul Perlmutter, Oliver Zahn, Zhao Zhang
Publikováno v:
IEEE BigData
Scientific analyses commonly compose multiple single-process programs into a dataflow. An end-to-end dataflow of single-process programs is known as a many-task application. Typically, tools from the HPC software stack are used to parallelize these a
Autor:
Dominique Fouchez, C. Buton, Kyle Boone, M. Strovink, E. Gangler, J. Ren, H. K. Fakhouri, Marek Kowalski, Cecilia Aragon, Nao Suzuki, Parker Fagrelius, P. Antilogus, G. Smadja, Caroline Sofiatti, A. G. Kim, K. Barbary, David Rubin, N. Chotard, Y. Copin, Charling Tao, M. Rigault, Greg Aldering, Brian Hayden, M. Childress, Jakob Nordin, R. Pereira, Saul Perlmutter, R. C. Thomas, K. Runge, David Rabinowitz, Benjamin A. Weaver, J. Chen, U. Feindt, C. Baltay, P.-F. Leget, R. Pain, D. Baugh, M. Fleury, Richard Scalzo, Emmanuel Pecontal, S. Bongard, S. Lombardo, C. Saunders, Stephen Bailey
Publikováno v:
Fakhouri, HK; Boone, K; Aldering, G; Antilogus, P; Aragon, C; Bailey, S; et al.(2015). IMPROVING COSMOLOGICAL DISTANCE MEASUREMENTS USING TWIN TYPE IA SUPERNOVAE. Astrophysical Journal, 815(1). doi: 10.1088/0004-637X/815/1/58. Lawrence Berkeley National Laboratory: Retrieved from: http://www.escholarship.org/uc/item/9wd067wg
The Astrophysical Journal
The Astrophysical Journal, American Astronomical Society, 2015, 815, pp.58. ⟨10.1088/0004-637X/815/1/58⟩
The Astrophysical Journal, vol 815, iss 1
The Astrophysical Journal, 2015, 815, pp.58. ⟨10.1088/0004-637X/815/1/58⟩
Astrophysical Journal, vol 815, iss 1
The astrophysical journal / 1 815(1), 58-(2015). doi:10.1088/0004-637X/815/1/58
The Astrophysical Journal
The Astrophysical Journal, American Astronomical Society, 2015, 815, pp.58. ⟨10.1088/0004-637X/815/1/58⟩
The Astrophysical Journal, vol 815, iss 1
The Astrophysical Journal, 2015, 815, pp.58. ⟨10.1088/0004-637X/815/1/58⟩
Astrophysical Journal, vol 815, iss 1
The astrophysical journal / 1 815(1), 58-(2015). doi:10.1088/0004-637X/815/1/58
The astrophysical journal 815(1), 58 - (2015). doi:10.1088/0004-637X/815/1/58
We introduce a method for identifying "twin" Type Ia supernovae (SNe Ia) and using them to improve distance measurements. This novel approach to SN Ia standardization
We introduce a method for identifying "twin" Type Ia supernovae (SNe Ia) and using them to improve distance measurements. This novel approach to SN Ia standardization
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::748b8bb21c82ff17b345e382021c1758
Autor:
K. Barbary, Patrick McDonald, Michael Levi, Michael Sholl, Michael Lampton, Patrick N. Jelinsky, Claire Poppett, Alex G. Kim, David J. Schlegel, Jerry Edelstein, Nick Mostek, Natalie A. Roe, Arjun Dey, Chris Bebek
Publikováno v:
SPIE Proceedings.
[The BigBOSS experiment is a redshift survey designed to map the large scale structure of the universe and probe the nature of dark energy. Using massively-multiplexed _ber spectroscopy over 14,000 deg2 of sky, the survey will deliver more than 20 mi