Zobrazeno 1 - 10
of 85
pro vyhledávání: '"Miguel Roth"'
Autor:
Syed A. Uddin, Christopher R. Burns, M M. Phillips, Nicholas B. Suntzeff, Wendy L. Freedman, Peter J. Brown, Nidia Morrell, Mario Hamuy, Kevin Krisciunas, Lifan Wang, Eric Y. Hsiao, Ariel Goobar, Saul Perlmutter, Jing Lu, Maximilian Stritzinger, Joseph P. Anderson, Chris Ashall, Peter Hoeflich, Benjamin J. Shappee, S. E. Persson, Anthony L. Piro, E Baron, Carlos Contreras, Lluís Galbany, Sahana Kumar, Melissa Shahbandeh, Scott Davis, Jorge Anais, Luis Busta, Abdo Campillay, Sergio Castellón, Carlos Corco, Tiara Diamond, Christa Gall, Consuelo Gonzalez, Simon Holmbo, Miguel Roth, Jacqueline Serón, Francesco Taddia, Simón Torres, Charles Baltay, Gastón Folatelli, Ellie Hadjiyska, Mansi Kasliwal, Peter E. Nugent, David Rabinowitz, Stuart D. Ryder
Publikováno v:
The Astrophysical Journal, Vol 970, Iss 1, p 72 (2024)
We present an analysis of Type Ia supernovae (SNe Ia) from the Carnegie Supernova Project I and II and extend the Hubble diagram from optical to near-infrared wavelengths ( uBgVriYJH ). We calculate the Hubble constant, H _0 , using various distance
Externí odkaz:
https://doaj.org/article/28e475ec0cc9466b88a955ded83817d5
Autor:
Régis Cartier, Mario Hamuy, Carlos Contreras, Joseph P Anderson, Mark M Phillips, Nidia Morrell, Maximilian D Stritzinger, Emilio D Hueichapan, Alejandro Clocchiatti, Miguel Roth, Joanna Thomas-Osip, Luis E González
Publikováno v:
Cartier, R, Hamuy, M, Contreras, C, Anderson, J P, Phillips, M M, Morrell, N, Stritzinger, M D, Hueichapan, E D, Clocchiatti, A, Roth, M, Thomas-Osip, J & González, L E 2022, ' A puzzle solved after two decades : SN 2002gh among the brightest of superluminous supernovae ', Monthly Notices of the Royal Astronomical Society, vol. 514, no. 2, pp. 2627-2649 . https://doi.org/10.1093/mnras/stac1371
We present optical photometry and spectroscopy of the superluminous SN 2002gh from maximum light to $+204$ days, obtained as part of the Carnegie Type II Supernova (CATS) project. SN 2002gh is among the most luminous discovered supernovae ever, yet i
IRAS 12272-6240 is a complex star forming region with a compact massive dense clump and several associated masers, located at a well-determined distance of $d=9.3$ kpc from the Sun. For this study, we obtained sub-arcsec broad- and narrow-band near-I
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2f31b95775486a99b6fbc509660f437a
Autor:
Barry F. Madore, Kevin Krisciunas, Peter Heoflich, Wojtek Krzeminski, Christopher R. Burns, Wendy L. Freedman, Carlos Contreras, Nicholas B. Suntzeff, L. Busta, S. Castellon, Gastón Folatelli, Nidia Morrell, Mario Hamuy, Simón Torres, E. Parent, J. Serón, Mark M. Phillips, J. Anais, Eric Hsiao, Maximilian Stritzinger, C. Gonzalez, Abdo Campillay, Luis Boldt, S. E. Persson, Miguel Roth, Francisco Salgado
Publikováno v:
Burns, C R, Parent, E, Phillips, M M, Stritzinger, M, Krisciunas, K, Suntzeff, N B, Hsiao, E Y, Contreras, C, Anais, J, Boldt, L, Busta, L, Campillay, A, Castellón, S, Folatelli, G, Freedman, W L, González, C, Hamuy, M, Heoflich, P, Krzeminski, W, Madore, B F, Morrell, N, Roth, M, Salgado, F, Serón, J & Torres, S 2018, ' The Carnegie Supernova Project : Absolute Calibration and the Hubble Constant ', Astrophysical Journal, vol. 869, no. 1, 56 . https://doi.org/10.3847/1538-4357/aae51c
Burns, C R, Parent, E, Phillips, M M, Stritzinger, M, Krisciunas, K, Suntzeff, N B, Hsiao, E Y, Contreras, C, Anais, J, Boldt, L, Busta, L, Campillay, A, Castellon, S, Folatelli, G, Freedman, W L, Gonzalez, C, Hamuy, M, Heoflich, P, Krzeminski, W, Madore, B F, Morrell, N, Persson, S E, Roth, M, Salgado, F, Seron, J & Torres, S 2018, ' The Carnegie Supernova Project : Absolute Calibration and the Hubble Constant ', Astrophysical Journal, vol. 869, no. 1, 56 . https://doi.org/10.3847/1538-4357/aae51c
Burns, C R, Parent, E, Phillips, M M, Stritzinger, M, Krisciunas, K, Suntzeff, N B, Hsiao, E Y, Contreras, C, Anais, J, Boldt, L, Busta, L, Campillay, A, Castellón, S, Folatelli, G, Freedman, W L, González, C, Hamuy, M, Heoflich, P, Krzeminski, W, Madore, B F, Morrell, N, Persson, S E, Roth, M, Salgado, F, Serón, J & Torres, S 2018, ' The Carnegie Supernova Project : Absolute Calibration and the Hubble Constant ', Astrophysical Journal, vol. 869, no. 1, 56 . https://doi.org/10.3847/1538-4357/aae51c
Burns, C R, Parent, E, Phillips, M M, Stritzinger, M, Krisciunas, K, Suntzeff, N B, Hsiao, E Y, Contreras, C, Anais, J, Boldt, L, Busta, L, Campillay, A, Castellon, S, Folatelli, G, Freedman, W L, Gonzalez, C, Hamuy, M, Heoflich, P, Krzeminski, W, Madore, B F, Morrell, N, Persson, S E, Roth, M, Salgado, F, Seron, J & Torres, S 2018, ' The Carnegie Supernova Project : Absolute Calibration and the Hubble Constant ', Astrophysical Journal, vol. 869, no. 1, 56 . https://doi.org/10.3847/1538-4357/aae51c
Burns, C R, Parent, E, Phillips, M M, Stritzinger, M, Krisciunas, K, Suntzeff, N B, Hsiao, E Y, Contreras, C, Anais, J, Boldt, L, Busta, L, Campillay, A, Castellón, S, Folatelli, G, Freedman, W L, González, C, Hamuy, M, Heoflich, P, Krzeminski, W, Madore, B F, Morrell, N, Persson, S E, Roth, M, Salgado, F, Serón, J & Torres, S 2018, ' The Carnegie Supernova Project : Absolute Calibration and the Hubble Constant ', Astrophysical Journal, vol. 869, no. 1, 56 . https://doi.org/10.3847/1538-4357/aae51c
We present an analysis of the final data release of the Carnegie Supernova Project I, focusing on the absolute calibration of the luminosity-decline-rate relation for Type Ia supernovae (SNeIa) using new intrinsic color relations with respect to the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0d41921536f50dee74171ad57d9f1763
https://pure.au.dk/portal/da/publications/the-carnegie-supernova-project(e84902e0-3c27-4b7b-9a0c-f2f1b8b7d5a2).html
https://pure.au.dk/portal/da/publications/the-carnegie-supernova-project(e84902e0-3c27-4b7b-9a0c-f2f1b8b7d5a2).html
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 459:1946-1958
The far-infrared IRAS 15507-5359 source is known to be a medium-mass star-forming region associated with a compact H II region and a near-infrared embedded cluster. We present a survey of infrared-calibrated images ranging from 1.2 to 500 μm obtaine
Autor:
Nicholas B. Suntzeff, Kevin Krisciunas, Mansi M. Kasliwal, Christa Gall, L. Busta, J. Anais, Anthony L. Piro, Mario Hamuy, E. Hadjiyska, B. J. Shappee, Syed Uddin, C. Corco, Lluís Galbany, J. P. Anderson, A. Goobar, Carlos Contreras, David Rabinowitz, M. M. Phillips, Stuart D. Ryder, Gastón Folatelli, C. Lidman, Maximilian Stritzinger, T. Diamond, C. Ashall, Abdo Campillay, C. Gonzalez, S. Holmbo, Emma S. Walker, Peter Hoeflich, Nidia Morrell, F. Taddia, Simón Torres, Peter Nugent, Saul Perlmutter, C. Baltay, Wendy L. Freedman, Brian P. Schmidt, S. Castellon, Eric Hsiao, Christopher R. Burns, Miguel Roth, J. Serón, S. E. Persson, E. Baron
Publikováno v:
Phillips, M M, Contreras, C, Hsiao, E Y, Morrell, N, Burns, C R, Stritzinger, M, Ashall, C, Freedman, W L, Hoeflich, P, Persson, S E, Piro, A L, Suntzeff, N B, Uddin, S A, Anais, J, Baron, E, Busta, L, Campillay, A, Castellon, S, Corco, C, Diamond, T, Gall, C, Gonzalez, C, Holmbo, S, Krisciunas, K, Roth, M, Seron, J, Taddia, F, Torres, S, Anderson, J P, Baltay, C, Folatelli, G, Galbany, L, Goobar, A, Hadjiyska, E, Hamuy, M, Kasliwal, M, Lidman, C, Nugent, P E, Perlmutter, S, Rabinowitz, D, Ryder, S D, Schmidt, B P, Shappee, B J & Walker, E S 2019, ' Carnegie Supernova Project-II : Extending the Near-infrared Hubble Diagram for Type Ia Supernovae to z similar to 0.1 ', Publications of the Astronomical Society of the Pacific, vol. 131, no. 995, 014001 . https://doi.org/10.1088/1538-3873/aae8bd
Phillips, MM; Contreras, Carlos; Hsiao, EY; Morrell, Nidia; Burns, Christopher R; Stritzinger, Maximilian; et al.(2019). Carnegie Supernova Project-II: Extending the Near-infrared Hubble Diagram for Type Ia Supernovae to z ∼ 0.1. Publications of the Astronomical Society of the Pacific, 131(995), 014001-014001. doi: 10.1088/1538-3873/aae8bd. Lawrence Berkeley National Laboratory: Retrieved from: http://www.escholarship.org/uc/item/2kh1d38b
Phillips, MM; Contreras, Carlos; Hsiao, EY; Morrell, Nidia; Burns, Christopher R; Stritzinger, Maximilian; et al.(2019). Carnegie Supernova Project-II: Extending the Near-infrared Hubble Diagram for Type Ia Supernovae to z ∼ 0.1. Publications of the Astronomical Society of the Pacific, 131(995), 014001-014001. doi: 10.1088/1538-3873/aae8bd. Lawrence Berkeley National Laboratory: Retrieved from: http://www.escholarship.org/uc/item/2kh1d38b
The Carnegie Supernova Project-II (CSP-II) was an NSF-funded, four-year program to obtain optical and near-infrared observations of a "Cosmology" sample of $\sim100$ Type Ia supernovae located in the smooth Hubble flow ($0.03 \lesssim z \lesssim 0.10
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::023bcb6073dbce073636e7c3878f2eb6
http://arxiv.org/abs/1810.09252
http://arxiv.org/abs/1810.09252
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 446:4088-4097
Autor:
Miguel Roth, Christopher R. Burns, J. Anais, Carlos Contreras, Jennifer L. Marshall, C. Gonzalez, L. Busta, Alexei V. Filippenko, Barry F. Madore, Luis Boldt, Francisco Salgado, Weidong Li, Jean Philippe Rheault, Darren L. DePoy, Maximilian Stritzinger, J. Serón, Steven Villanueva, Wojtek Krzeminski, Mario Hamuy, S. Castellon, Kevin Krisciunas, Mark M. Phillips, S. E. Persson, Wendy L. Freedman, Simón Torres, Abdo Campillay, Gastón Folatelli, Nidia Morrell, Nicholas B. Suntzeff, Eric Hsiao
Publikováno v:
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Krisciunas, K, Contreras, C, Burns, C R, Phillips, M M, Stritzinger, M D, Morrell, N, Hamuy, M, Anais, J, Boldt, L, Busta, L, Campillay, A, Castellon, S, Folatelli, G, Freedman, W L, Gonzalez, C, Hsiao, E Y, Krzeminski, W, Persson, S E, Roth, M, Salgado, F, Seron, J, Suntzeff, N B, Torres, S, Filippenko, A V, Li, W, Madore, B F, Depoy, D L, Marshall, J L, Rheault, J-P & Villanueva, S 2017, ' The Carnegie Supernova Project. I. Third Photometry Data Release of Low-redshift Type Ia Supernovae and Other White Dwarf Explosions ', Astronomical Journal, vol. 154, no. 5, 211 . https://doi.org/10.3847/1538-3881/aa8df0
SEDICI (UNLP)
Universidad Nacional de La Plata
instacron:UNLP
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Krisciunas, K, Contreras, C, Burns, C R, Phillips, M M, Stritzinger, M D, Morrell, N, Hamuy, M, Anais, J, Boldt, L, Busta, L, Campillay, A, Castellon, S, Folatelli, G, Freedman, W L, Gonzalez, C, Hsiao, E Y, Krzeminski, W, Persson, S E, Roth, M, Salgado, F, Seron, J, Suntzeff, N B, Torres, S, Filippenko, A V, Li, W, Madore, B F, Depoy, D L, Marshall, J L, Rheault, J-P & Villanueva, S 2017, ' The Carnegie Supernova Project. I. Third Photometry Data Release of Low-redshift Type Ia Supernovae and Other White Dwarf Explosions ', Astronomical Journal, vol. 154, no. 5, 211 . https://doi.org/10.3847/1538-3881/aa8df0
SEDICI (UNLP)
Universidad Nacional de La Plata
instacron:UNLP
We present final natural-system optical (ugriBV) and near-infrared (YJH) photometry of 134 supernovae (SNe) with probable white dwarf progenitors that were observed in 2004-2009 as part of the first stage of the Carnegie Supernova Project (CSP-I). Th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b76dcdb28efb568e3e11792a13be469c
http://iopscience.iop.org/article/10.3847/1538-3881/aa8df0/meta
http://iopscience.iop.org/article/10.3847/1538-3881/aa8df0/meta
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 416:2163-2173
New deep broad- and narrow-band (JHK and Br γ at 2.17 µm and H2 at 2.12µm) nearinfrared (near-IR) images of the mid-IR source G287.47−0.54 (Tr14-N4) taken with the Baade Magellan telescope are presented and analysed along with archive 3.6–8µm
Autor:
Mansi M. Kasliwal, George H Marion, Lluís Galbany, Stefano Valenti, Mario Hamuy, Syed Uddin, P. Hoeflich, Mark M. Phillips, Sanjay Kumar, Scott C. Davis, Nicholas B. Suntzeff, C. Lidman, Robert P. Kirshner, Peter Nugent, David Rabinowitz, David J. Sand, Saul Perlmutter, Francesco Taddia, Nidia Morrell, Kevin Krisciunas, F. Forster, Santiago González-Gaitán, Chris Ashall, Jessica R. Lu, Anthony L. Piro, Christopher R. Burns, Christa Gall, Maximilian Stritzinger, Stuart D. Ryder, Ariel Goobar, Joseph P. Anderson, Wendy L. Freedman, Brian P. Schmidt, Debabrata Banerjee, S. Holmbo, C. Baltay, E. Baron, T. R. Diamond, Melissa Shahbandeh, Eric Hsiao, S. E. Persson, Gastón Folatelli, Carlos Contreras, Lian-Tao Wang, Miguel Roth
Publikováno v:
Hsiao, EY; Phillips, MM; Marion, GH; Kirshner, RP; Morrell, N; Sand, DJ; et al.(2019). Carnegie Supernova Project-II: The Near-infrared Spectroscopy Program. PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC, 131(995), 014002-014002. doi: 10.1088/1538-3873/aae961. Lawrence Berkeley National Laboratory: Retrieved from: http://www.escholarship.org/uc/item/6zx853d1
Hsiao, E Y, Phillips, M M, Marion, G H, Kirshner, R P, Morrell, N, Sand, D J, Burns, C R, Contreras, C, Hoeflich, P, Stritzinger, M D, Valenti, S, Anderson, J P, Ashall, C, Baltay, C, Baron, E, Banetjee, D P K, Davis, S, Diamond, T R, Folatelli, G, Freedman, W L, Forster, F, Galbany, L, Gall, C, Gonzalez-Gaitan, S, Goobar, A, Hamuy, M, Holmbo, S, Kasliwal, M M, Krisciunas, K, Kumar, S, Lidman, C, Lu, J, Nugent, P E, Perlmutter, S, Persson, S E, Piro, A L, Rabinowitz, D, Roth, M, Ryder, S D, Schmidt, B P, Shahbandeh, M, Suntzeff, N B, Taddia, F, Uddin, S & Wang, L 2019, ' Carnegie Supernova Project-II : The Near-infrared Spectroscopy Program ', Publications of the Astronomical Society of the Pacific, vol. 131, no. 995, 014002 . https://doi.org/10.1088/1538-3873/aae961
SEDICI (UNLP)
Universidad Nacional de La Plata
instacron:UNLP
Hsiao, E Y, Phiilips, M M, Marion, G H, Kirshner, R P, Morrell, N, Sand, D J, Burns, C R, Contreras, C, Hoeflich, P, Stritzinger, M D, Valenti, S, Anderson, J P, Ashall, C, Baltay, C, Baron, E, Banerjee, D P K, Davis, S, Diamond, T R, Folatelli, G, Freedman, W L, Forster, F, Galbany, L, Gall, C, Gonzalez-Gaitan, S, Goobar, A, Hamuy, M, Holmbo, S, Kasliwal, M M, Krisciunas, K, Kumar, S, Lidman, C, Lu, J, Nugent, P E, Perlmutter, S, Persson, S E, Piro, A L, Rabinowitz, D, Roth, M, Ryder, S D, Schmidt, B P, Shahbandeh, M, Suntzeff, N B, Taddia, F, Uddin, S & Wang, L 2019, ' Carnegie Supernova Project-II : The Near-infrared Spectroscopy Program ', Publications of the Astronomical Society of the Pacific, vol. 131, no. 995, 014002 . https://doi.org/10.1088/1538-3873/aae961
Publications of the Astronomical Society of the Pacific, vol 131, iss 995
Hsiao, E Y, Phillips, M M, Marion, G H, Kirshner, R P, Morrell, N, Sand, D J, Burns, C R, Contreras, C, Hoeflich, P, Stritzinger, M D, Valenti, S, Anderson, J P, Ashall, C, Baltay, C, Baron, E, Banetjee, D P K, Davis, S, Diamond, T R, Folatelli, G, Freedman, W L, Forster, F, Galbany, L, Gall, C, Gonzalez-Gaitan, S, Goobar, A, Hamuy, M, Holmbo, S, Kasliwal, M M, Krisciunas, K, Kumar, S, Lidman, C, Lu, J, Nugent, P E, Perlmutter, S, Persson, S E, Piro, A L, Rabinowitz, D, Roth, M, Ryder, S D, Schmidt, B P, Shahbandeh, M, Suntzeff, N B, Taddia, F, Uddin, S & Wang, L 2019, ' Carnegie Supernova Project-II : The Near-infrared Spectroscopy Program ', Publications of the Astronomical Society of the Pacific, vol. 131, no. 995, 014002 . https://doi.org/10.1088/1538-3873/aae961
SEDICI (UNLP)
Universidad Nacional de La Plata
instacron:UNLP
Hsiao, E Y, Phiilips, M M, Marion, G H, Kirshner, R P, Morrell, N, Sand, D J, Burns, C R, Contreras, C, Hoeflich, P, Stritzinger, M D, Valenti, S, Anderson, J P, Ashall, C, Baltay, C, Baron, E, Banerjee, D P K, Davis, S, Diamond, T R, Folatelli, G, Freedman, W L, Forster, F, Galbany, L, Gall, C, Gonzalez-Gaitan, S, Goobar, A, Hamuy, M, Holmbo, S, Kasliwal, M M, Krisciunas, K, Kumar, S, Lidman, C, Lu, J, Nugent, P E, Perlmutter, S, Persson, S E, Piro, A L, Rabinowitz, D, Roth, M, Ryder, S D, Schmidt, B P, Shahbandeh, M, Suntzeff, N B, Taddia, F, Uddin, S & Wang, L 2019, ' Carnegie Supernova Project-II : The Near-infrared Spectroscopy Program ', Publications of the Astronomical Society of the Pacific, vol. 131, no. 995, 014002 . https://doi.org/10.1088/1538-3873/aae961
Publications of the Astronomical Society of the Pacific, vol 131, iss 995
Shifting the focus of Type Ia supernova (SN Ia) cosmology to the near-infrared (NIR) is a promising way to significantly reduce the systematic errors, as the strategy minimizes our reliance on the empirical width-luminosity relation and uncertain dus