Zobrazeno 1 - 10
of 637
pro vyhledávání: '"Taddia P"'
Autor:
Anderson, J. P., Contreras, C., Stritzinger, M. D., Hamuy, M., Phillips, M. M., Suntzeff, N. B., Morrell, N., Gonzalez-Gaitan, S., Gutierrez, C. P., Burns, C. R., Hsiao, E. Y., Anais, J., Ashall, C., Baltay, C., Baron, E., Bersten, M., Busta, L., Castellon, S., de Jaeger, T., DePoy, D., Filippenko, A. V., Folatelli, G., Forster, F., Galbany, L., Gall, C., Goobar, A., Gonzalez, C., Hadjiyska, E., Hoeflich, P., Krisciunas, K., Krzeminski, W., Li, W., Madore, B., Marshall, J., Martinez, L., Nugent, P., Pessi, P. J., Piro, A. L., Rheault, J-P., Ryder, S., Seron, J., Shappee, B. J., Taddia, F., Torres, S., Thomas-Osip, J., Uddin, S.
Type II supernovae (SNeII) mark the endpoint in the lives of hydrogen-rich massive stars. Their large explosion energies and luminosities allow us to measure distances, metallicities, and star formation rates into the distant Universe. To fully explo
Externí odkaz:
http://arxiv.org/abs/2410.06738
Autor:
Morrell, N., Phillips, M. M., Folatelli, G., Stritzinger, M. D., Hamuy, M., Suntzeff, N. B., Hsiao, E. Y., Taddia, F., Burns, C. R., Hoeflich, P., Ashall, C., Contreras, C., Galbany, L., Lu, J., Piro, A. L., Anais, J., Baron, E., Burrow, A., Busta, L., Campillay, A., Castellón, S., Corco, C., Diamond, T., Freedman, W. L., González, C., Krisciunas, K., Kumar, S., Persson, S. E., Serón, J., Shahbandeh, M., Torres, S., Uddin, S. A., Anderson, J. P., Baltay, C., Gall, C., Goobar, A., Hadjiyska, E., Holmbo, S., Kasliwal, M., Lidman, C., Marion, G. H., Mazzali, P., Nugent, P., Perlmutter, S., Pignata, G., Rabinowitz, D., Roth, M., Ryder, S. D., Shappee, B. J., Vinkó, J., Wheeler, J. C., de Jaeger, T., Lira, P., Ruiz, M. T., Rich, J. A., Prieto, J. L., Di Mille, F., Osip, D., Blanc, G., Palunas, P.
We present the second and final release of optical spectroscopy of Type Ia Supernovae (SNe Ia) obtained during the first and second phases of the Carnegie Supernova Project (CSP-I and CSP-II). The newly released data consist of 148 spectra of 30 SNe
Externí odkaz:
http://arxiv.org/abs/2404.19208
Autor:
Stritzinger, Maximilian D., Baron, Eddie, Taddia, Francesco, Burns, Chris R., Galbany, Morgan Fraserm Lluis, Holmbo, Simon, Hoeflich, Peter, Morrell, Nidia, Hsiao, E. Y., Johansson, Joel P., Karamehmetoglu, Emir, Kuncarayakti, Hanindyo, Lyman, Joe, Moriya, Takashi J., Phan, Kim, Phillips, Mark M., Anderson, Joseph P., Ashall, Chris, Brown, Peter J., Castellon, Sergio, Della Valle, Massimo, Gonzalez-Gaitan, Santiago, Gromadzki, Mariusz, Handberg, Rasmus, Lu, Jing, Nicholl, Matt, Shahbandeh, Melissa
Publikováno v:
A&A 686, A79 (2024)
We present a comprehensive data set of supernova (SN) 2016adj located within the central dust lane of Centaurus A. SN 2016adj is significantly reddened and after correcting the peak apparent $B$-band magnitude ($m_B = 17.48\pm0.05$) for Milky Way red
Externí odkaz:
http://arxiv.org/abs/2309.05031
Autor:
Uddin, Syed A., Burns, Christopher R., Phillips, Mark M., Suntzeff, Nicholas B., Freedman, Wendy L., Brown, Peter J., Morrell, Nidia, Hamuy, Mario, Krisciunas, Kevin, Wang, Lifan, Hsiao, Eric Y., Goobar, Ariel, Perlmutter, Saul, Lu, Jing, Stritzinger, Maximilian, Anderson, Joseph P., Ashall, Chris, Hoeflich, Peter, Shappee, Benjamin J., Persson, S. E., Piro, Anthony L., Baron, Eddie, Contreras, Carlos, Galbany, Lluís, Kumar, Sahana, Shahbandeh, Melissa, Davis, Scott, Anais, Jorge, Busta, Luis, Campillay, Abdo, Castellón, Sergio, Corco, Carlos, Diamond, Tiara, Gall, Christa, Gonzalez, Consuelo, Holmbo, Simon, Roth, Miguel, Serón, Jacqueline, Taddia, Francesco, Torres, Simón, Baltay, Charles, Folatelli, Gastón, Hadjiyska, Ellie, Kasliwal, Mansi, Nugent, Peter E., Rabinowitz, David, Ryder, Stuart D.
We present an analysis of Type Ia Supernovae (SNe~Ia) from both the Carnegie Supernova Project~I (CSP-I) and II (CSP-II), and extend the Hubble diagram from the optical to the near-infrared wavelengths ($uBgVriYJH$). We calculate the Hubble constant,
Externí odkaz:
http://arxiv.org/abs/2308.01875
Autor:
Holmbo, S., Stritzinger, M. D., Karamehmetoglu, E., Burns, C. R., Morrell, N., Ashall, C., Hsiao, E. Y., Galbany, L., Folatelli, G., Phillips, M. M., Baron, E., Gutierrez, C. P., Leloudas, G., Muller-Bravo, T. E., Hoeflich, P., Taddia, F., Suntzeff, N. B.
An analysis leveraging 170 optical spectra of 35 stripped-envelope (SE) core-collapse supernovae observed by the Carnegie Supernova Project-I and published in a companion paper is presented. Mean template spectra are constructed for the SNe IIb, Ib a
Externí odkaz:
http://arxiv.org/abs/2302.11304
Autor:
Stritzinger, Maximilian, Taddia, Francesco, Lawrence, Stephen S., Patat, Ferdinando, Fraser, Morgan, Galbany, Lluís, Holmbo, Simon, Hyder, Ali, Karamehmetoglu, Emir
We present a multi-band sequence of $Hubble~Space~Telescope$ images documenting the emergence and evolution of multiple light echoes (LEs) linked to the stripped-envelope supernova (SN) 2016adj located in the central dust-lane of Centaurus A. Followi
Externí odkaz:
http://arxiv.org/abs/2210.14778
Autor:
Karamehmetoglu, E., Sollerman, J., Taddia, F., Barbarino, C., Feindt, U., Fremling, C., Gal-Yam, A., Kasliwal, M. M., Petrushevska, T., Schulze, S., Stritzinger, M. D., Zapartas, E.
Publikováno v:
A&A 678, A87 (2023)
If high-mass stars (>20-25 Msun) are the progenitors of stripped-envelope (SE) supernovae (SNe), their massive ejecta should lead to broad, long-duration lightcurves (LCs). Instead, literature samples of SE~SNe have reported relatively narrow LCs wit
Externí odkaz:
http://arxiv.org/abs/2210.09402
Autor:
Chen, Z. H., Yan, Lin, Kangas, T., Lunnan, R., Schulze, S., Sollerman, J., Perley, D. A., Chen, T. -W., Taggart, K., Hinds, K. R., Gal-Yam, A., Wang, X. F., Andreoni, I., Bellm, E., Bloom, J. S., Burdge, K., Burgos, A., Cook, D., Dahiwale, A., De, K., Dekany, R., Dugas, A., Frederik, S., Fremling, C., Graham, M., Hankins, M., Ho, A., Jencson, J., Karambelkar, V., Kasliwal, M., Kulkarni, S., Laher, R., Rusholme, B., Sharma, Y., Taddia, F., Tartaglia, L., Thomas, B. P., Tzanidakis, A., Van Roestel, J., Walter, R., Yang, Y., Yao, Y. H., Yaron, O.
During the Zwicky Transient Facility (ZTF) Phase-I operation, 78 hydrogen-poor superluminous supernovae (SLSNe-I) were discovered in less than three years, making up the largest sample from a single survey. This paper (Paper I) presents the data, inc
Externí odkaz:
http://arxiv.org/abs/2202.02059
Autor:
Shahbandeh, M., Hsiao, E. Y., Ashall, C., Teffs, J., Hoeflich, P., Morrell, N., Phillips, M. M., Anderson, J. P., Baron, E., Burns, C. R., Contreras, C., Davis, S., Diamond, T. R., Folatelli, G., Galbany, L., Gall, C., Hachinger, S., Holmbo, S., Karamehmetoglu, E., Kasliwal, M. M., Kirshner, R. P., Krisciunas, K., Kumar, S., Lu, J., Marion, G. H., Mazzali, P. A., Piro, A. L., Sand, D. J., Stritzinger, M. D., Suntzeff, N. B., Taddia, F., Uddin, S. A.
We present 75 near-infrared (NIR; 0.8$-$2.5 $\mu$m) spectra of 34 stripped-envelope core-collapse supernovae (SESNe) obtained by the Carnegie Supernova Project-II (CSP-II), encompassing optical spectroscopic Types IIb, Ib, Ic, and Ic-BL. The spectra
Externí odkaz:
http://arxiv.org/abs/2110.12083
Publikováno v:
Frontiers in Earth Science, Vol 12 (2024)
The influence of climatic factors on landslides triggers and displacement rates is a crucial research topic, especially due to the growing need to understand the evolution of climate change in historical periods of intense precipitation and anomalous
Externí odkaz:
https://doaj.org/article/b2c361360be142acbc3f8fed2b8d1d06
