Zobrazeno 1 - 10
of 57
pro vyhledávání: '"Boldt, Luis"'
Autor:
Burns, Christopher. R., Parent, Emilie, Phillips, M. M., Stritzinger, Maximillian, Krisciunas, Kevin, Suntzeff, Nicholas B., Hsiao, Eric Y., Contreras, Carlos, Anais, Jorge, Boldt, Luis, Busta, Luis, Campillay, Abdo, Castellon, Sergio, Folatelli, Gaston, Freedman, Wendy L., Gonzalez, Consuelo, Hamuy, Mario, Heoflich, Peter, Krzeminski, Wojtek, Madore, Barry F., Morrell, Nidia, Persson, S. E., Roth, Miguel, Salgado, Francisco, Seron, Jacqueline, Torres, Simon
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:
http://arxiv.org/abs/1809.06381
Autor:
Krisciunas, Kevin, Contreras, Carlos, Burns, Christopher R., Phillips, M. M., Stritzinger, Maximilian D., Morrell, Nidia, Hamuy, Mario, Anais, Jorge, Boldt, Luis, Busta, Luis, Campillay, Abdo, Castellon, Sergio, Folatelli, Gaston, Freedman, Wendy L., Gonzalez, Consuelo, Hsiao, Eric. Y., Krzeminski, Wojtek, Persson, Sven Eric, Roth, Miguel, Salgado, Francisco, Seron, Jacqueline, Suntzeff, Nicholas B., Torres, Simon, Filippenko, Alexei V., Li, Weidong, Madore, Barry F., DePoy, D. L., Marshall, Jennifer L., Rheault, Jean-Philippe, Villanueva, Steven
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:
http://arxiv.org/abs/1709.05146
Autor:
Burns, Christopher R., Stritzinger, Maximilian, Phillips, M. M., Hsiao, E. Y., Contreras, Carlos, Persson, S. E., Folatelli, Gaston, Boldt, Luis, Campillay, Abdo, Catellón, Sergio, Freedman, Wendy L., Madore, Barry F., Morrell, Nidia, Salgado, Francisco, Suntzeff, Nicholas B.
We present an updated analysis of the intrinsic colors of SNe Ia using the latest data release of the Carnegie Supernova Project. We introduce a new light-curve parameter very similar to stretch that is better suited for fast-declining events, and fi
Externí odkaz:
http://arxiv.org/abs/1405.3934
Autor:
Boldt, Luis, Stritzinger, Maximilian, Burns, Chris, Hsiao, Eric, Phillips, Mark, Goobar, Ariel, Marion, Howie, Stanishev, Vallery
In this paper we use near-infrared (NIR) spectral observations of Type Ia supernovae (SNe Ia) to study the uncertainties inherent to NIR K corrections. To do so, 75 previously published NIR spectra of 33 SNe Ia are employed to determine K-correction
Externí odkaz:
http://arxiv.org/abs/1402.5095
Autor:
Folatelli, Gastón, Morrell, Nidia, Phillips, Mark M., Hsiao, Eric, Campillay, Abdo, Contreras, Carlos, Castellón, Sergio, Hamuy, Mario, Krzeminski, Wojtek, Roth, Miguel, Stritzinger, Maximilian, Burns, Christopher R., Freedman, Wendy L., Madore, Barry F., Murphy, David, Persson, S. E., Prieto, José L., Suntzeff, Nicholas B., Krisciunas, Kevin, Anderson, Joseph P., Förster, Francisco, Maza, José, Pignata, Giuliano, Rojas, P. Andrea, Boldt, Luis, Salgado, Francisco, Wyatt, Pamela, E., Felipe Olivares, Gal-Yam, Avishay, Sako, Masao
Publikováno v:
2013 ApJ 773 53
This is the first release of optical spectroscopic data of low-redshift Type Ia supernovae (SNe Ia) by the Carnegie Supernova Project including 604 previously unpublished spectra of 93 SNe Ia. The observations cover a range of phases from 12 days bef
Externí odkaz:
http://arxiv.org/abs/1305.6997
Autor:
Stritzinger, Maximilian, Taddia, Francesco, Fransson, Claes, Fox, Ori D., Morrell, Nidia, Phillips, M. M., Sollerman, Jesper, Anderson, J. P., Boldt, Luis, Brown, Peter J., Campillay, Abdo, Castellon, Sergio, Contreras, Carlos, Folatelli, Gaston, Habergham, S. M., Hamuy, Mario, Hjorth, Jens, James, Phil A., Krzeminski, Wojtek, Mattila, Seppo, Persson, Sven E., Roth, Miguel
We present an observational study of the Type IIn supernovae (SNe IIn) 2005ip and 2006jd. Broad-band UV, optical and near-IR photometry, and visual-wavelength spectroscopy of SN 2005ip complement and extend upon published observations to 6.5 years pa
Externí odkaz:
http://arxiv.org/abs/1206.5575
Autor:
Folatelli, Gastón, Phillips, M. M., Morrell, Nidia, Tanaka, Masaomi, Maeda, Keiichi, Nomoto, Ken'ichi, Stritzinger, Maximilian, Burns, Christopher R., Hamuy, Mario, Mazzali, Paolo, Boldt, Luis, Campillay, Abdo, Contreras, Carlos, Gonzalez, Sergio, Roth, Miguel, Salgado, Francisco, Freedman, W. L., Madore, Barry F., Persson, S. E., Suntzeff, Nicholas B.
(Abridged) The presence of unburned material in the ejecta of normal Type Ia supernovae (SNeIa) is investigated using early-time spectroscopy obtained by the CSP. The tell-tale signature of pristine material from a C+O white dwarf progenitor star is
Externí odkaz:
http://arxiv.org/abs/1110.3789
Autor:
Pignata, Giuliano, Stritzinger, Maximilian, Soderberg, Alicia, Mazzali, Paolo, Phillips, M. M., Morrell, Nidia, Anderson, J. P., Boldt, Luis, Campillay, Abdo, Contreras, Carlos, Folatelli, Gastón, Förster, Francisco, González, Sergio, Hamuy, Mario, Krzeminski, Wojtek, Maza, José, Roth, Miguel, Levesque, Francisco Salgado Emily M., Rest, Armin, Crain, J. Adam, Foster, Andrew C., Haislip, Joshua B., Ivarsen, Kevin M., LaCluyze, Aaron P., Nysewander, Melissa C., Reichart, Daniel E.
Ultraviolet, optical, and near-infrared photometry and optical spectroscopy of the broad-lined Type Ic supernova (SN) 2009bb are presented, following the flux evolution from -10 to +285 days past B-band maximum. Thanks to the very early discovery, it
Externí odkaz:
http://arxiv.org/abs/1011.6126
Autor:
Burns, Christopher R., Stritzinger, Maximilian, Phillips, M. M., Kattner, ShiAnne, Persson, S. E., Madore, Barry F., Freedman, Wendy L., Boldt, Luis, Campillay, Abdo, Contreras, Carlos, Folatelli, Gaston, Gonzalez, Sergio, Krzeminski, Wojtek, Morrell, Nidia, Salgado, Francisco, Suntzeff, Nicholas B.
In providing an independent measure of the expansion history of the Universe, the Carnegie Supernova Project (CSP) has observed 71 high-z Type Ia supernovae (SNe Ia) in the near-infrared bands Y and J. These can be used to construct rest-frame i-band
Externí odkaz:
http://arxiv.org/abs/1010.4040
Autor:
Stritzinger, Maximilian, Burns, Chris, Phillips, Mark, Folatelli, Gaston, Krisciunas, Kevin, Persson, Eric, Boldt, Luis, Campillay, Abdo, Contreras, Carlos, Krzeminski, Wojtek, Salgado, Francisco, Freedman, Wendy, Hamuy, Mario, Madore, Barry, Roth, Miguel, Suntzeff, Nicholas
The giant elliptical galaxy NGC 1316 (Fornax A) is a well-studied member of the Fornax Cluster and a prolific producer of Type Ia supernovae, having hosted four observed events since 1980. Here we present detailed optical and near-infrared light curv
Externí odkaz:
http://arxiv.org/abs/1009.4390