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pro vyhledávání: '"Koviak, Kathleen"'
Autor:
Greklek-McKeon, Michael, Vissapragada, Shreyas, Knutson, Heather A., Fukui, Akihiko, Saidel, Morgan, Barrientos, Jonathan Gomez, Levine, W. Garrett, Behmard, Aida, Batygin, Konstantin, Chachan, Yayaati, Vasisht, Gautam, Hu, Renyu, Cloutier, Ryan, Latham, David, López-Morales, Mercedes, Vanderburg, Andrew, Heffner, Carolyn, Nied, Paul, Milburn, Jennifer, Wilson, Isaac, Roderick, Diana, Koviak, Kathleen, Barlow, Tom, Stone, John F., Kiman, Rocio, Korth, Judith, de Leon, Jerome P., Fukuda, Izuru, Hayashi, Yuya, Ikoma, Masahiro, Ikuta, Kai, Isogai, Keisuke, Kawai, Yugo, Kawauchi, Kiyoe, Kusakabe, Nobuhiko, Livingston, John H., Mori, Mayuko, Narita, Norio, Tamura, Motohide, Watanabe, Noriharu, Fernández-Rodríguez, Gareb
TOI-1266 is a benchmark system of two temperate ($<$ 450 K) sub-Neptune-sized planets orbiting a nearby M dwarf exhibiting a rare inverted architecture with a larger interior planet. In this study, we characterize transit timing variations (TTVs) in
Externí odkaz:
http://arxiv.org/abs/2409.16374
Autor:
Cartier, Régis, Hamuy, Mario, Pignata, Giuliano, Förster, Francisco, Zelaya, Paula, Folatelli, Gaston, Phillips, Mark M., Morrell, Nidia, Krisciunas, Kevin, Suntzeff, Nicholas B., Clocchiatti, Alejandro, Coppi, Paolo, Contreras, Carlos, Roth, Miguel, Koviak, Kathleen, Maza, José, González, Luis, González, Sergio, Huerta, Leonor
Publikováno v:
ApJ 789 89, 2014
We present well-sampled $UBVRIJHK$ photometry of SN 2002fk starting 12 days before maximum light through 122 days after peak brightness, along with a series of 15 optical spectra from -4 to +95 days since maximum. Our observations show the presence o
Externí odkaz:
http://arxiv.org/abs/1312.3342
Autor:
Hamuy, Mario, Deng, Jinsong, Mazzali, Paolo A., Morrell, Nidia I., Phillips, Mark M., Roth, Miguel, Gonzalez, Sergio, Thomas-Osip, Joanna, Krzeminski, Wojtek, Contreras, Carlos, Maza, Jose, Gonzalez, Luis, Huerta, Leonor, Folatelli, Gaston, Chornock, Ryan, Filippenko, Alexei V., Persson, S. E., Freedman, W. L., Koviak, Kathleen, Suntzeff, Nicholas B., Krisciunas, Kevin
Optical and near-infrared photometry and optical spectroscopy are reported for SN 2003bg, starting a few days after explosion and extending for a period of more than 300 days. Our early-time spectra reveal the presence of broad, high-velocity Balmer
Externí odkaz:
http://arxiv.org/abs/0908.1783
Autor:
Krisciunas, Kevin, Hamuy, Mario, Suntzeff, Nicholas B., Espinoza, Juan, Gonzalez, David, Gonzalez, Luis, Gonzalez, Sergio, Koviak, Kathleen, Krzeminski, Wojtek, Morrell, Nidia, Phillips, Mark M., Roth, Miguel, Thomas-Osip, Joanna
We present infrared photometry of SN 1999em, plus optical photometry, infrared photometry, and optical spectroscopy of SN 2003hn. Both objects were Type II-P supernovae. The V-[RIJHK] color curves of these supernovae evolved in a very similar fashion
Externí odkaz:
http://arxiv.org/abs/0809.2591
Akademický článek
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Akademický článek
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