Zobrazeno 1 - 10
of 602
pro vyhledávání: '"Bersier, D."'
Autor:
Zhu, Jiazheng, Jiang, Ning, Dong, Subo, Filippenko, Alexei V., Rudy, Richard J., Pastorello, A., Ashall, Christopher, Bose, Subhash, Post, R. S., Bersier, D., Benetti, Stefano, Brink, Thomas G., Chen, Ping, Dou, Liming, Elias-Rosa, N., Lundqvist, Peter, Mattila, Seppo, Russell, Ray W., Sitko, Michael L., Somero, Auni, Stritzinger, M. D., Wang, Tinggui, Brown, Peter J., Cappellaro, E., Fraser, Morgan, Kankare, Erkki, Moran, S., Prentice, Simon, Pursimo, Tapio, Reynolds, T. M., Zheng, WeiKang
When discovered, SN~2017egm was the closest (redshift $z=0.03$) hydrogen-poor superluminous supernova (SLSN-I) and a rare case that exploded in a massive and metal-rich galaxy. Thus, it has since been extensively observed and studied. We report spect
Externí odkaz:
http://arxiv.org/abs/2303.03424
Autor:
Holoien, T. W.-S., Brown, J. S., Stanek, K. Z., Kochanek, C. S., Shappee, B. J., Prieto, J. L., Dong, Subo, Brimacombe, J., Bishop, D. W., Basu, U., Beacom, J. F., Bersier, D., Chen, Ping, Danilet, A. B., Falco, E., Godoy-Rivera, D., Goss, N., Pojmanski, G., Simonian, G. V., Skowron, D. M., Thompson, Todd A., Woźniak, P. R., Ávila, C. G., Bock, G., Carballo, J.-L. G., Conseil, E., Contreras, C., Cruz, I., Andújar, J. M. F., Guo, Zhen, Hsiao, E. Y., Kiyota, S., Koff, R. A., Krannich, G., Madore, B. F., Marples, P., Masi, G., Morrell, N., Monard, L. A. G., Munoz-Mateos, J. C., Nicholls, B., Nicolas, J., Wagner, R. M., Wiethoff, W. S.
This manuscript presents information for all supernovae discovered by the All-Sky Automated Survey for SuperNovae (ASAS-SN) during 2015, its second full year of operations. The same information is presented for bright (m(V)
Externí odkaz:
http://hdl.handle.net/10150/623927
http://arizona.openrepository.com/arizona/handle/10150/623927
http://arizona.openrepository.com/arizona/handle/10150/623927
Autor:
Shappee, B. J., Piro, A. L., Holoien, T. W.-S., Prieto, J. L., Contreras, C., Itagaki, K., Burns, C. R., Kochanek, C. S., Stanek, K. Z., Alper, E., Basu, U., Beacom, J. F., Bersier, D., Brimacombe, J., Conseil, E., Danilet, A. B., Dong, Subo, Falco, E., Grupe, D., Hsiao, E. Y., Kiyota, S., Morrell, N., Nicolas, J., Phillips, M. M., Pojmanski, G., Simonian, G., Stritzinger, M., Szczygieł, D. M., Taddia, F., Thompson, T. A., Thorstensen, J., Wagner, M. R., Woźniak, P. R.
On 2014 December 9.61, the All-sky Automated Survey for SuperNovae (ASAS-SN or "Assassin") discovered ASASSN-141p just similar to 2 days after first light using a global array of 14 cm diameter telescopes. ASASSN-141p went on to become a bright super
Externí odkaz:
http://hdl.handle.net/10150/621393
http://arizona.openrepository.com/arizona/handle/10150/621393
http://arizona.openrepository.com/arizona/handle/10150/621393
Autor:
Neumann, K. D., Holoien, T. W. -S., Kochanek, C. S., Stanek, K. Z., Vallely, P. J., Shappee, B. J., Prieto, J. L., Pessi, T., Jayasinghe, T., Brimacombe, J., Bersier, D., Aydi, E., Basinger, C., Beacom, J. F., Bose, S., Brown, J. S., Chen, P., Clocchiatti, A., Desai, D. D., Dong, Subo, Falco, E., Holmbo, S., Morrell, N., Shields, J. V., Sokolovsky, K. V., Strader, J., Stritzinger, M. D., Swihart, S., Thompson, T. A., Way, Z., Aslan, L., Bishop, D. W., Bock, G., Bradshaw, J., Cacella, P., Castro-Morales, N., Conseil, E., Cornect, R., Cruz, I., Farfan, R. G., Fernandez, J. M., Gabuya, A., Gonzalez-Carballo, J. -L., Kendurkar, M. R., Kiyota, S., Koff, R. A., Krannich, G., Marples, P., Masi, G., Monard, L. A. G., Muñoz, J. A., Nicholls, B., Post, R. S., Pujic, Z., Stone, G., Tomasella, L., Trappett, D. L., Wiethoff, W. S.
Publikováno v:
MNRAS, 520, 4356 (2023)
We catalog the 443 bright supernovae discovered by the All-Sky Automated Survey for Supernovae (ASAS-SN) in $2018-2020$ along with the 519 supernovae recovered by ASAS-SN and 516 additional $m_{peak}\leq18$ mag supernovae missed by ASAS-SN. Our stati
Externí odkaz:
http://arxiv.org/abs/2210.06492
Autor:
Chen, Ping, Dong, Subo, Ashall, Chris, Benetti, S., Bersier, D., Bose, S., Brimacombe, Joseph, Brink, Thomas G., Buckley, David A. H., Cappellaro, Enrico, Christie, Grant W., Elias-Rosa, N., Filippenko, Alexei V., Gromadzki, Mariusz, Holoien, Thomas W. -S., Hu, Shaoming, Kochanek, C. S., Koff, Robert, Kollmeier, Juna A., Lundqvist, P., Mattila, S., Milne, Peter A., Munoz, J. A., Mutel, Robert, Natusch, Tim, Nicolas, Joel, Pastorello, A., Prentice, Simon, Prieto, J. L., Roth, Tyler, Shappee, B. J., Stone, Geoffrey, Stanek, K. Z., Stritzinger, M. D., Thompson, Todd A., Tomasella, Lina, Villanueva, Steven
Using data from the Complete Nearby ($z_{host}<0.02$) sample of Type Ia Supernovae (CNIa0.02), we discover a linear relation between two parameters derived from the $B-V$ color curves of Type Ia supernovae: the "color stretch" $s_{BV}$ and the rising
Externí odkaz:
http://arxiv.org/abs/2112.13364
Autor:
Chen, Ping, Dong, Subo, Kochanek, C. S., Stanek, K. Z., Post, R. S., Stritzinger, M. D., Prieto, J. L., Filippenko, Alexei V., Kollmeier, Juna A., Elias-Rosa, N., Katz, Boaz, Tomasella, Lina, Bose, S., Ashall, Chris, Benetti, S., Bersier, D., Brimacombe, Joseph, Brink, Thomas G., Brown, P., Buckley, David A. H., Cappellaro, Enrico, Christie, Grant W., Fraser, Morgan, Gromadzki, Mariusz, Holoien, Thomas W. -S., Hu, Shaoming, Kankare, Erkki, Koff, Robert, Lundqvist, P., Mattila, S., Milne, P. A., Morrell, Nidia, Munoz, J. A., Mutel, Robert, Natusch, Tim, Nicolas, Joel, Pastorello, A., Prentice, Simon, Roth, Tyler, Shappee, B. J., Stone, Geoffrey, Thompson, Todd A., Villanueva, Steven, Zheng, WeiKang
Publikováno v:
ApJS, 259, 53 (2022)
The CNIa0.02 project aims to collect a complete, nearby sample of Type Ia supernovae (SNe Ia) light curves, and the SNe are volume-limited with host-galaxy redshifts z_host < 0.02. The main scientific goal is to infer the distributions of key propert
Externí odkaz:
http://arxiv.org/abs/2011.02461
Autor:
Gutiérrez, C. P., Pastorello, A., Jerkstrand, A., Galbany, L., Sullivan, M., Anderson, J. P., Taubenberger, S., Kuncarayakti, H., González-Gaitán, S., Wiseman, P., Inserra, C., Fraser, M., Maguire, K., Smartt, S., Müller-Bravo, T. E., Arcavi, I., Benetti, S., Bersier, D., Bose, S., Bostroem, K. A., Burke, J., Chen, P., Chen, T. -W., Della Valle, M., Dong, Subo, Gal-Yam, A., Gromadzki, M., Hiramatsu, D., Holoien, T. W. -S., Hosseinzadeh, G., Howell, D. A., Kankare, E., Kochanek, C. S., McCully, C., Nicholl, M., Pignata, G., Prieto, J. L., Shappee, B., Taggart, K., Tomasella, L., Valenti, S., Young, D. R.
We present the photometric and spectroscopic evolution of the Type II supernova (SN II) SN 2017ivv (also known as ASASSN-17qp). Located in an extremely faint galaxy (M$_r=-10.3$ mag), SN 2017ivv shows an unprecedented evolution during the two years o
Externí odkaz:
http://arxiv.org/abs/2008.09628
Autor:
Terreran, G., Margutti, R., Bersier, D., Brimacombe, J., Caprioli, D., Challis, P., Chornock, R., Coppejans, D. L., Dong, Subo, Guidorzi, C., Hurley, K., Kirshner, R., Migliori, G., Milisavljevic, D., Palmer, D. M., Prieto, J. L., Tomasella, L., Marchant, P., Pastorello, A., Shappee, B. J., Stanek, K. Z., Stritzinger, M. D., Benetti, S., Demarchi, L., Elias-rosa, N., Gall, C., Harmanen, J., Mattila, S.
We present comprehensive observations and analysis of the energetic H-stripped SN 2016coi (a.k.a. ASASSN-16fp), spanning the $\gamma$-ray through optical and radio wavelengths, acquired within the first hours to $\sim$420 days post explosion. Our cam
Externí odkaz:
http://arxiv.org/abs/1905.02226
Autor:
Chen, Ping, Dong, Subo, Stritzinger, M. D., Holmbo, Simon, Strader, Jay, Kochanek, C. S., Peng, Eric W., Benetti, S., Bersier, D., Brownsberger, Sasha, Buckley, David A. H., Gromadzki, Mariusz, Moran, Shane, Pastorello, A., Aydi, Elias, Bose, Subhash, Connor, Thomas, Elias-Rosa, N., French, K. Decker, Holoien, Thomas W. -S., Mattila, Seppo, Shappee, B. J., Stark, Antony A., Swihart, Samuel J.
Publikováno v:
ApJL 889 L6 (2020)
We report observations of the hydrogen-deficient supernova (SN) 2019bkc/ATLAS19dqr. With B- and r-band decline between peak and 10 days post peak of Delta m_10(B)=5.24+/-0.07 mag and Delta m_10(r)=3.85+/-0.10$ mag, respectively, SN 2019bkc is the mos
Externí odkaz:
http://arxiv.org/abs/1905.02205
Autor:
Prentice, S. J., Ashall, C., James, P. A., Short, L., Mazzali, P. A., Bersier, D., Crowther, P. A., Barbarino, C., Chen, T. -W., Copperwheat, C. M., Darnley, M. J., Denneau, L., Elias-Rosa, N., Fraser, M., Galbany, L., Gal-Yam, A., Harmanen, J., Howell, D. A., Hosseinzadeh, G., Inserra, C., Kankare, E., Karamehmetoglu, E., Lamb, G. P., Limongi, M., Maguire, K., McCully, C., E., F. Olivares, Piascik, A. S., Pignata, G., Reichart, D. E., Reynolds, A. Rest T., Rodríguez, Ó., Saario, J. L. O., Schulze, S., Smartt, S. J., Smith, K. W., Sollerman, J., Stalder, B., Sullivan, M., Taddia, F., Valenti, S., Vergani, S. D., Williams, S. C., Young, D. R.
We present observations and analysis of 18 stripped-envelope supernovae observed during 2013 -- 2018. This sample consists of 5 H/He-rich SNe, 6 H-poor/He-rich SNe, 3 narrow lined SNe Ic and 4 broad lined SNe Ic. The peak luminosity and characteristi
Externí odkaz:
http://arxiv.org/abs/1812.03716