Zobrazeno 1 - 10
of 51
pro vyhledávání: '"Kasliwal MM"'
Autor:
Kasliwal, MM, Anand, S, Ahumada, T, Stein, R, Carracedo, AS, Andreoni, I, Coughlin, MW, Singer, LP, Kool, EC, De, K, Kumar, H, Almualla, M, Yao, Y, Bulla, M, Dobie, D, Reusch, S, Perley, DA, Cenko, SB, Bhalerao, V, Kaplan, DL, Sollerman, J, Goobar, A, Copperwheat, CM, Bellm, EC, Anupama, GC, Corsi, A, Nissanke, S, Agudo, I, Bagdasaryan, A, Barway, S, Belicki, J, Bloom, JS, Bolin, B, Buckley, DAH, Burdge, KB, Burruss, R, Caballero-García, MD, Cannella, C, Castro-Tirado, AJ, Cook, DO, Cooke, J, Cunningham, V, Dahiwale, A, Deshmukh, K, Dichiara, S, Duev, DA, Dutta, A, Feeney, M, Franckowiak, A, Frederick, S, Fremling, C, Gal-Yam, A, Gatkine, P, Ghosh, S, Goldstein, DA, Golkhou, VZ, Graham, MJ, Graham, ML, Hankins, MJ, Helou, G, Hu, Y, Ip, WH, Jaodand, A, Karambelkar, V, Kong, AKH, Kowalski, M, Khandagale, M, Kulkarni, SR, Kumar, B, Laher, RR, Li, KL, Mahabal, A, Masci, FJ, Miller, AA, Mogotsi, M, Mohite, S, Mooley, K, Mroz, P, Newman, JA, Ngeow, CC, Oates, SR, Patil, AS, Pandey, SB, Pavana, M, Pian, E, Riddle, R, Sánchez-Ramírez, R, Sharma, Y, Singh, A, Smith, R, Soumagnac, MT, Taggart, K, Tan, H, Tzanidakis, A, Troja, E, Valeev, AF, Walters, R, Waratkar, G, Webb, S, Yu, PC
Publikováno v:
The Astrophysical Journal, vol 905, iss 2
Astrophysical Journal, vol 905, iss 2
Astrophysical Journal, vol 905, iss 2
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 (O3). We searched binary neutron star (BNS) and neutron star black hole (NSBH)
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::8fb53061658e3a4f99889c5620ab98f4
https://escholarship.org/uc/item/849251pq
https://escholarship.org/uc/item/849251pq
Autor:
Irani, I, Schulze, S, Gal-Yam, A, Lunnan, R, Brink, TG, Zheng, W, Filippenko, AV, Yang, Y, De Jaeger, T, Nugent, PE, Kasliwal, MM, Fremling, C, Neill, JD, Rebbapragada, U, Masci, FJ, Sollerman, J, Yaron, O
Publikováno v:
Astrophysical Journal, vol 887, iss 2
Type II supernovae (SNe) stem from the core collapse of massive (>8 M o) stars. Due to their short lifespan, we expect a very low rate of such events in elliptical hosts, where the star formation rate is low, and which are mostly comprised of an old
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______325::4ceb0f91e2344589d5bd427f344b7762
https://escholarship.org/uc/item/7zz7x0b5
https://escholarship.org/uc/item/7zz7x0b5
Autor:
Hsiao, EY, Phillips, MM, Marion, GH, Kirshner, RP, Morrell, N, Sand, DJ, Burns, CR, Contreras, C, Hoeflich, P, Stritzinger, MD, Valenti, S, Anderson, JP, Ashall, C, Baltay, C, Baron, E, Banerjee, DPK, Davis, S, Diamond, TR, Folatelli, G, Freedman, Wendy L, Förster, F, Galbany, L, Gall, C, González-Gaitán, S, Goobar, A, Hamuy, M, Holmbo, S, Kasliwal, MM, Krisciunas, K, Kumar, S, Lidman, C, Lu, J, Nugent, PE, Perlmutter, S, Persson, SE, Piro, AL, Rabinowitz, D, Roth, M, Ryder, SD, Schmidt, BP, Shahbandeh, M, Suntzeff, NB, Taddia, F, Uddin, S, Wang, L
Publikováno v:
Publications of the Astronomical Society of the Pacific, vol 131, iss 995
Shifting the focus of Type Ia supernova (SN Ia) cosmology to the near infrared (NIR) is a promising way to significantly reduce the systematic errors, as the strategy minimizes our reliance on the empirical width-luminosity relation and uncertain dus
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______325::5b692e393819f099f3dfa2773beafb53
https://escholarship.org/uc/item/6zx853d1
https://escholarship.org/uc/item/6zx853d1
Autor:
Bellm, EC, Kulkarni, SR, Graham, MJ, Dekany, R, Smith, RM, Riddle, R, Masci, FJ, Helou, G, Prince, TA, Adams, SM, Barbarino, C, Barlow, T, Bauer, J, Beck, R, Belicki, J, Biswas, R, Blagorodnova, N, Bodewits, D, Bolin, B, Brinnel, V, Brooke, T, Bue, B, Bulla, M, Burruss, R, Cenko, SB, Chang, CK, Connolly, A, Coughlin, M, Cromer, J, Cunningham, V, De, K, Delacroix, A, Desai, V, Duev, DA, Eadie, G, Farnham, TL, Feeney, M, Feindt, U, Flynn, D, Franckowiak, A, Frederick, S, Fremling, C, Gal-Yam, A, Gezari, S, Giomi, M, Goldstein, DA, Golkhou, VZ, Goobar, A, Groom, S, Hacopians, E, Hale, D, Henning, J, Ho, AYQ, Hover, D, Howell, J, Hung, T, Huppenkothen, D, Imel, D, Ip, WH, Ivezić, Ž, Jackson, E, Jones, L, Juric, M, Kasliwal, MM, Kaspi, S, Kaye, S, Kelley, MSP, Kowalski, M, Kramer, E, Kupfer, T, Landry, W, Laher, RR, Lee, CD, Lin, HW, Lin, ZY, Lunnan, R, Mahabal, A, Mao, P, Miller, AA, Monkewitz, S, Murphy, P, Ngeow, CC, Nordin, J, Nugent, P, Ofek, E, Patterson, MT, Penprase, B, Porter, M, Rauch, L, Rebbapragada, U, Reiley, D, Rigault, M, Rodriguez, H, van Roestel, J, Rusholme, B, van Santen, J, Schulze, S, Shupe, DL, Singer, LP
Publikováno v:
Publications of the Astronomical Society of the Pacific, vol 131, iss 995
The Zwicky Transient Facility (ZTF) is a new optical time-domain survey that uses the Palomar 48 inch Schmidt telescope. A custom-built wide-field camera provides a 47 deg 2 field of view and 8 s readout time, yielding more than an order of magnitude
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______325::49e520f077d626d6552d6ebc0a48d3bd
https://escholarship.org/uc/item/28z8s056
https://escholarship.org/uc/item/28z8s056
Autor:
Kasliwal, MM, Nakar, E, Singer, LP, Kaplan, DL, Cook, DO, Van Sistine, A, Lau, RM, Fremling, C, Gottlieb, O, Jencson, JE, Adams, SM, Feindt, U, Hotokezaka, K, Ghosh, S, Perley, DA, Yu, P-C, Piran, T, Allison, JR, Anupama, GC, Balasubramanian, A, Bannister, KW, Bally, J, Barnes, J, Barway, S, Bellm, E, Bhalerao, V, Bhattacharya, D, Blagorodnova, N, Bloom, JS, Brady, PR, Cannella, C, Chatterjee, D, Cenko, SB, Cobb, BE, Copperwheat, C, Corsi, A, De, K, Dobie, D, Emery, SWK, Evans, PA, Fox, OD, Frail, DA, Frohmaier, C, Goobar, A, Hallinan, G, Harrison, F, Helou, G, Hinderer, T, Ho, AYQ, Horesh, A, Ip, W-H, Itoh, R, Kasen, D, Kim, H, Kuin, NPM, Kupfer, T, Lynch, C, Madsen, K, Mazzali, PA, Miller, AA, Mooley, K, Murphy, T, Ngeow, C-C, Nichols, D, Nissanke, S, Nugent, P, Ofek, EO, Qi, H, Quimby, RM, Rosswog, S, Rusu, F, Sadler, EM, Schmidt, P, Sollerman, J, Steele, I, Williamson, AR, Xu, Y, Yan, L, Yatsu, Y, Zhang, C, Zhao, W
Publikováno v:
Science (New York, N.Y.), vol 358, iss 6370
Merging neutron stars offer an excellent laboratory for simultaneously studying strong-field gravity and matter in extreme environments. We establish the physical association of an electromagnetic counterpart (EM170817) with gravitational waves (GW17
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::395faec0f36dc1f700f00da306259989
https://escholarship.org/uc/item/183320km
https://escholarship.org/uc/item/183320km
Autor:
Miller, AA, Kasliwal, MM, Cao, Y, Adams, SM, Goobar, A, Knežević, S, Laher, RR, Lunnan, R, Masci, FJ, Nugent, PE, Perley, DA, Petrushevska, T, Quimby, RM, Rebbapragada, UD, Sollerman, J, Taddia, F, Kulkarni, SR
Publikováno v:
The Astrophysical Journal, vol 848, iss 1
Modern wide-field, optical time-domain surveys must solve a basic optimization problem: maximize the number of transient discoveries or minimize the follow-up needed for the new discoveries. Here, we describe the Color Me Intrigued experiment, the fi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______325::32501021828e4e990bfe9e1f531574cd
https://escholarship.org/uc/item/0zx3z1bh
https://escholarship.org/uc/item/0zx3z1bh
Autor:
Kasliwal, MM, Cenko, SB, Singer, LP, Corsi, A, Cao, Y, Barlow, T, Bhalerao, V, Bellm, E, Cook, D, Duggan, GE, Ferretti, R, Frail, DA, Horesh, A, Kendrick, R, Kulkarni, SR, Lunnan, R, Palliyaguru, N, Laher, R, Masci, F, Manulis, I, Miller, AA, Nugent, PE, Perley, D, Prince, TA, Quimby, RM, Rana, J, Rebbapragada, U, Sesar, B, Singhal, A, Surace, J, Sistine, AV
Publikováno v:
The Astrophysical Journal Letters, vol 824, iss 2
Kasliwal, MM; Cenko, SB; Singer, LP; Corsi, A; Cao, Y; Barlow, T; et al.(2016). IPTF SEARCH for AN OPTICAL COUNTERPART to GRAVITATIONAL-WAVE TRANSIENT GW150914. Astrophysical Journal Letters, 824(2). doi: 10.3847/2041-8205/824/2/L24. Lawrence Berkeley National Laboratory: Retrieved from: http://www.escholarship.org/uc/item/5tp05351
Astrophysical Journal Letters, vol 824, iss 2
Kasliwal, MM; Cenko, SB; Singer, LP; Corsi, A; Cao, Y; Barlow, T; et al.(2016). IPTF SEARCH for AN OPTICAL COUNTERPART to GRAVITATIONAL-WAVE TRANSIENT GW150914. Astrophysical Journal Letters, 824(2). doi: 10.3847/2041-8205/824/2/L24. Lawrence Berkeley National Laboratory: Retrieved from: http://www.escholarship.org/uc/item/5tp05351
Astrophysical Journal Letters, vol 824, iss 2
© 2016. The American Astronomical Society. All rights reserved.. The intermediate Palomar Transient Factory (iPTF) autonomously responded to and promptly tiled the error region of the first gravitational-wave event GW150914 to search for an optical
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::26a862d90875da66bb1298b449a9bbd0
https://escholarship.org/uc/item/5tp05351
https://escholarship.org/uc/item/5tp05351
Autor:
Ofek, EO, Cenko, SB, Shaviv, NJ, Duggan, G, Strotjohann, N-L, Rubin, A, Kulkarni, SR, Gal-Yam, A, Sullivan, M, Cao, Y, Nugent, PE, Kasliwal, MM, Sollerman, J, Fransson, C, Filippenko, AV, Perley, DA, Yaron, O, Laher, R
Publikováno v:
The Astrophysical Journal, vol 824, iss 1
The progenitors of some supernovae (SNe) exhibit outbursts with super-Eddington luminosities prior to their final explosions. This behavior is common among SNe IIn, but the driving mechanisms of these precursors are not yet well-understood. SNHunt 27
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______325::ca7308d93289aaaf3043e531d681aad2
https://escholarship.org/uc/item/642308s4
https://escholarship.org/uc/item/642308s4
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