Zobrazeno 1 - 9
of 9
pro vyhledávání: '"Taggart, Kirsty"'
Autor:
Das, Kaustav K., Kasliwal, Mansi M., Sollerman, Jesper, Fremling, Christoffer, Irani, I., Leung, Shing-Chi, Yang, Sheng, Wu, Samantha, Fuller, Jim, Anand, Shreya, Andreoni, Igor, Barbarino, C., Brink, Thomas G., De, Kishalay, Dugas, Alison, Groom, Steven L., Helou, George, Hinds, K-Ryan, Ho, Anna Y. Q., Karambelkar, Viraj, Kulkarni, S. R., Perley, Daniel A., Purdum, Josiah, Regnault, Nicolas, Schulze, Steve, Sharma, Yashvi, Sit, Tawny, Srinivasaragavan, Gokul P., Stein, Robert, Taggart, Kirsty, Tartaglia, Leonardo, Tzanidakis, Anastasios, Wold, Avery, Yan, Lin, Yao, Yuhan, Zolkower, Jeffry
Eruptive mass loss of massive stars prior to supernova (SN) explosion is key to understanding their evolution and end fate. An observational signature of pre-SN mass loss is the detection of an early, short-lived peak prior to the radioactive-powered
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0097336c0da3bb99f7d2123eff29dd85
http://arxiv.org/abs/2306.04698
http://arxiv.org/abs/2306.04698
Autor:
Schulze, Steve, Fransson, Claes, Kozyreva, Alexandra, Chen, Ting-Wan, Yaron, Ofer, Jerkstrand, Anders, Gal-Yam, Avishay, Sollerman, Jesper, Yan, Lin, Kangas, Tuomas, Leloudas, Giorgos, Omand, Conor M. B., Smartt, Stephen J., Yang, Yi, Nicholl, Matt, Sarin, Nikhil, Yao, Yuhan, Brink, Thomas G., Sharon, Amir, Rossi, Andrea, Chen, Ping, Chen, Zhihao, Cikota, Aleksandar, De, Kishalay, Drake, Andrew J., Filippenko, Alexei V., Fremling, Christoffer, Freour, Laurane, Fynbo, Johan P. U., Ho, Anna Y. Q., Inserra, Cosimo, Irani, Ido, Kuncarayakti, Hanindyo, Lunnan, Ragnhild, Mazzali, Paolo, Ofek, Eran O., Palazzi, Eliana, Perley, Daniel A., Pursiainen, Miika, Rothberg, Barry, Shingles, Luke J., Smith, Ken, Taggart, Kirsty, Tartaglia, Leonardo, Zheng, WeiKang, Anderson, Joseph P., Cassara, Letizia, Christensen, Eric, Djorgovski, S. George, Galbany, Lluis, Gkini, Anamaria, Graham, Matthew J., Gromadzki, Mariusz, Groom, Steven L., Hiramatsu, Daichi, Howell, D. Andrew, Kasliwal, Mansi M., McCully, Curtis, Müller-Bravo, Tomas E., Paiano, Simona, Paraskeva, Emmanouela, Pessi, Priscila J., Polishook, David, Rau, Arne, Rigault, Mickael, Rusholme, Ben
Abridged - Stars with ZAMS masses between 140 and $260 M_\odot$ are thought to explode as pair-instability supernovae (PISNe). During their thermonuclear runaway, PISNe can produce up to several tens of solar masses of radioactive nickel, resulting i
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c525e8c986ed8153c13df5198e1cdd39
http://arxiv.org/abs/2305.05796
http://arxiv.org/abs/2305.05796
Autor:
Wang, Qinan, Goel, Anika, Dessart, Luc, Fox, Ori D., Shahbandeh, Melissa, Rest, Sofia, Rest, Armin, Groh, Jose H., Allan, Andrew, Fransson, Claes, Smith, Nathan, Hosseinzadeh, Griffin, Filippenko, Alexei V., Andrews, Jennifer, Bostroem, K. Azalee, Brink, Thomas G., Brown, Peter, Burke, Jamison, Chevalier, Roger, Clayton, Geoffrey C., Dai, Mi, Davis, Kyle W., Foley, Ryan J., Gomez, Sebastian, Harris, Chelsea, Hiramatsu, Daichi, Howell, D. Andrew, Jennings, Connor, Jha, Saurabh W., Kasliwal, Mansi M., Kelly, Patrick L., Kool, Erik C., Liu, Evelyn, Ma, Emily, McCully, Curtis, Miller, Adam M., Murakami, Yukei, Pellegrino, Craig, Gonzalez, Estefania Padilla, Perera, Derek, Pierel, Justin, Rojas-Bravo, César, Siebert, Matthew R., Sollerman, Jesper, Szalai, Tamás, Tinyanont, Samaporn, Van Dyk, Schuyler D., Zheng, WeiKang, Chambers, Kenneth C., Coulter, David A., de Boer, Thomas, Earl, Nicholas, Farias, Diego, Gall, Christa, McGill, Peter, Ransome, Conor L., Taggart, Kirsty, Villar, V. Ashley
A growing number of supernovae (SNe) are now known to exhibit evidence for significant interaction with a dense, pre-existing, circumstellar medium (CSM). SNe Ibn comprise one such class that can be characterised by both rapidly evolving light curves
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::56954555170a5856560e346113d945ee
http://arxiv.org/abs/2305.05015
http://arxiv.org/abs/2305.05015
Autor:
Wang, Qinan, Rest, Armin, Dimitriadis, Georgios, Ridden-harper, Ryan, Siebert, Matthew R., Magee, Mark, Angus, Charlotte R., Auchettl, Katie, Davis, Kyle W., Foley, Ryan J., Fox, Ori D., Gomez, Sebastian, Jencson, Jacob E., Jones, David O., Kilpatrick, Charles D., Pierel, Justin D. R., Piro, Anthony L., Polin, Abigail, Politsch, Collin A., Rojas-bravo, César, Shahbandeh, Melissa, Villar, V. Ashley, Zenati, Yossef, Ashall, C., Chambers, Kenneth C., Coulter, David A., De Boer, Thomas, Dilullo, Nico, Gall, Christa, Gao, Hua, Hsiao, Eric Y., Huber, Mark E., Izzo, Luca, Khetan, Nandita, Lebaron, Natalie, Magnier, Eugene A., Mandel, Kaisey S., Mcgill, Peter, Miao, Hao-yu, Pan, Yen-chen, Stevens, Catherine P., Swift, Jonathan J., Taggart, Kirsty, Yang, Grace
We present high-cadence ultraviolet through near-infrared observations of the Type Ia supernova (SN Ia) 2023bee in NGC~2708 ($D = 32 \pm 3$ Mpc), finding excess flux in the first days after explosion relative to the expected power-law rise from an ex
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6812dc44e7ff17c83575af6025ff0ad7
http://arxiv.org/abs/2305.03779
http://arxiv.org/abs/2305.03779
Autor:
Singh, Mridweeka, Sahu, Devendra. K., Dastidar, Raya, Barna, Barnabas, Misra, Kuntal, Gangopadhyay, Anjasha, Howell, D. Andrew, Jha, Saurabh W., Im, Hyobin, Taggart, Kirsty, Andrews, Jennifer, Hiramatsu, Daichi, Teja, Rishabh Singh, Pellegrino, Craig, Foley, Ryan J., Joshi, Arti, Anupama, G. C., Bostroem, K. Azalee, Burke, Jamison, Camacho-Neves, Yssavo, Dutta, Anirban, Kwok, Lindsey A., McCully, Curtis, Pan, Yen-Chen, Siebert, Matt, Srivastav, Shubham, Szalai, Tamas, Swift, Jonathan J., Yang, Grace, Zhou, Henry, DiLullo, Nico, Scheer, Jackson
We present the optical photometric and spectroscopic analysis of two type Iax SNe 2018cni and 2020kyg. SN 2018cni is a bright type Iax SN (M$_{V,peak}$ = $-$17.81$\pm$0.21 mag) whereas SN 2020kyg (M$_{V,peak}$ = $-$14.52$\pm$0.21 mag) is a faint one.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::34ebd937d6ec2df0d223477274d2fab2
Autor:
Siebert, Matthew R., Foley, Ryan J., Zenati, Yossef, Dimitriadis, Georgios, Yang, Grace, Davis, Kyle W., Taggart, Kirsty, Rojas-Bravo, César
We present nebular spectroscopy of SN 2020hvf, a Type Ia supernova (SN Ia) with an early bump in its light curve. SN 2020hvf shares many spectroscopic and photometric similarities to the carbon-rich high-luminosity "03fg-like" SNe Ia. At $>$240 days
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ebeb15817dca57944a90e4ca9c63f277
Autor:
Tinyanont, Samaporn, Woosley, Stan E., Taggart, Kirsty, Foley, Ryan J., Yan, Lin, Lunnan, Ragnhild, Davis, Kyle W., Kilpatrick, Charles D., Siebert, Matthew R., Schulze, Steve, Ashall, Chris, Chen, Ting-Wan, De, Kishalay, Dimitriadis, Georgios, Dong, Dillon Z., Fremling, Christoffer, Gagliano, Alexander, Jha, Saurabh W., Jones, David O., Kasliwal, Mansi M., Miao, Hao-Yu, Pan, Yen-Chen, Perley, Daniel A., Ravi, Vikram, Rojas-Bravo, César, Sfaradi, Itai, Sollerman, Jesper, Alarcon, Vanessa, Angulo, Rodrigo, Clever, Karoli E., Crawford, Payton, Couch, Cirilla, Dandu, Srujan, Dhara, Atirath, Johnson, Jessica, Lai, Zhisen, Smith, Carli
We present observations of a peculiar hydrogen- and helium-poor stripped-envelope (SE) supernova (SN) 2020wnt, primarily in the optical and near-infrared (near-IR). Its peak absolute bolometric magnitude of -20.9 mag and a rise time of 69~days are re
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9f2b841db0105b6aeae5a7b5b59e1858
http://arxiv.org/abs/2212.00177
http://arxiv.org/abs/2212.00177
Autor:
Jacobson-Galán, Wynn, Venkatraman, Padma, Margutti, Raffaella, Khatami, David, Terreran, Giacomo, Foley, Ryan J., Angulo, Rodrigo, Angus, Charlotte R., Auchettl, Katie, Blanchard, Peter K., Bobrick, Alexey, Bright, Joe S., Couch, Cirilla D., Coulter, David A., Clever, Karoli, Davis, Kyle W., de Boer, Thomas, DeMarchi, Lindsay, Dodd, Sierra A., Jones, David O., Johnson, Jessica, Kilpatrick, Charles D., Khetan, Nandita, Lai, Zhisen, Langeroodi, Danial, Lin, Chien-Cheng, Magnier, Eugene A., Milisavljevic, Dan, Perets, Hagai B., Pierel, Justin D. R., Raymond, John, Rest, Sofia, Rest, Armin, Ridden-Harper, Ryan, Shen, Ken J., Siebert, Matthew R., Smith, Carli, Taggart, Kirsty, Tinyanont, Samaporn, Valdes, Frank, Villar, Victoria A., Wang, Qinan, Yadavalli, S. Karthik, Zenati, Yossef, Zenteno, Alfredo
We present panchromatic observations and modeling of calcium-strong supernovae (SNe) 2021gno in the star-forming host galaxy NGC 4165 (D = 30.5 Mpc) and 2021inl in the outskirts of elliptical galaxy NGC 4923 (D = 80 Mpc), both monitored through the Y
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::82b504f1b249ceb7cbfcb9a78bd6e523
http://arxiv.org/abs/2203.03785
http://arxiv.org/abs/2203.03785
Autor:
Kasliwal, Mansi M., Anand, Shreya, Ahumada, Tomas, Stein, Robert, Carracedo, Ana Sagues, Andreoni, Igor, Coughlin, Michael W., Singer, Leo P., Kool, Erik C., De, Kishalay, Kumar, Harsh, AlMualla, Mouza, Yao, Yuhan, Bulla, Mattia, Dobie, Dougal, Reusch, Simeon, Perley, Daniel A., Cenko, S. Bradley, Bhalerao, Varun, Kaplan, David L., Sollerman, Jesper, Goobar, Ariel, Copperwheat, Christopher M., Bellm, Eric C., Anupama, G. C., Corsi, Alessandra, Nissanke, Samaya, Agudo, Ivan, Bagdasaryan, Ashot, Barway, Sudhanshu, Belicki, Justin, Bloom, Joshua S., Bolin, Bryce, Buckley, David A. H., Burdge, Kevin B., Burruss, Rick, Caballero-Garc��a, Maria D., Cannella, Chris, Castro-Tirado, Alberto J., Cook, David O., Cooke, Jeff, Cunningham, Virginia, Dahiwale, Aishwarya, Deshmukh, Kunal, Dichiara, Simone, Duev, Dmitry A., Dutta, Anirban, Feeney, Michael, Franckowiak, Anna, Frederick, Sara, Fremling, Christoffer, Gal-Yam, Avishay, Gatkine, Pradip, Ghosh, Shaon, Goldstein, Daniel A., Golkhou, V. Zach, Graham, Matthew J., Graham, Melissa L., Hankins, Matthew J., Helou, George, Hu, Youdong, Ip, Wing-Huen, Jaodand, Amruta, Karambelkar, Viraj, Kong, Albert K. H., Kowalski, Marek, Khandagale, Maitreya, Kulkarni, S. R., Kumar, Brajesh, Laher, Russ R., Li, K. L., Mahabal, Ashish, Masci, Frank J., Miller, Adam A., Mogotsi, Moses, Mohite, Siddharth, Mooley, Kunal, Mroz, Przemek, Newman, Jeffrey A., Ngeow, Chow-Choong, Oates, Samantha R., Patil, Atharva Sunil, Pandey, Shashi B., Pavana, M., Pian, Elena, Riddle, Reed, Sanchez-Ram��rez, Ruben, Sharma, Yashvi, Singh, Avinash, Smith, Roger, Soumagnac, Maayane T., Taggart, Kirsty, Tan, Hanjie, Tzanidakis, Anastasios, Troja, Eleonora, Valeev, Azamat F., Walters, Richard, Waratkar, Gaurav, Webb, Sara, Yu, Po-Chieh, Zhang, Bin-Bin, Zhou, Rongpu, Zolkower, Jeffry
We present a systematic search for optical counterparts to 13 gravitational wave (GW) triggers involving at least one neutron star during LIGO/Virgo's third observing run. We searched binary neutron star (BNS) and neutron star black hole (NSBH) merge
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::baa60dccd5d674d96bfbcd000df1441a
http://arxiv.org/abs/2006.11306
http://arxiv.org/abs/2006.11306