Zobrazeno 1 - 10
of 1 917
pro vyhledávání: '"A, MILISAVLJEVIC"'
Autor:
Sears, Huei, Chornock, Ryan, Blanchard, Peter, Margutti, Raffaella, Villar, V. Ashley, Pierel, Justin, Vallely, Patrick J., Alexander, Kate D., Berger, Edo, Eftekhari, Tarraneh, Jacobson-Galan, Wynn V., Laskar, Tanmoy, LeBaron, Natalie, Metzger, Brian D., Milisavljevic, Dan
GRB 221009A is one of the brightest transients ever observed with the highest peak gamma-ray flux for a gamma-ray burst (GRB). A type Ic-BL supernova (SN), SN 2022xiw, was definitively detected in late-time JWST spectroscopy (t = 195 days, observer-f
Externí odkaz:
http://arxiv.org/abs/2412.02663
Autor:
Nayana, A. J., Margutti, Raffaella, Wiston, Eli, Chornock, Ryan, Campana, Sergio, Laskar, Tanmoy, Murase, Kohta, Krips, Melanie, Migliori, Giulia, Tsuna, Daichi, Alexander, Kate D., Chandra, Poonam, Bietenholz, Michael, Berger, Edo, Chevalier, Roger A., De Colle, Fabio, Dessart, Luc, Diesing, Rebecca, Grefenstette, Brian W., Jacobson-Galan, Wynn V., Maeda, Keiichi, Marcote, Benito, Matthews, David, Milisavljevic, Dan, Ray, Alak K., Reguitti, Andrea, Polzin, Ava
We present the results from our extensive hard-to-soft X-ray (NuSTAR, Swift-XRT, XMM-Newton, Chandra) and meter-to-mm wave radio (GMRT, VLA, NOEMA) monitoring campaign of the very nearby (d $=6.9$ Mpc) Type II SN2023ixf spanning $\approx$ 4--165 d po
Externí odkaz:
http://arxiv.org/abs/2411.02647
Autor:
Orlando, S., Greco, E., Hirai, R., Matsuoka, T., Miceli, M., Nagataki, S., Ono, M., Chen, K. -J., Milisavljevic, D., Patnaude, D., Bocchino, F., Elias-Rosa, N.
We investigate SN 2014C using three-dimensional hydrodynamic modeling, focusing on its early interaction with dense circumstellar medium (CSM). Our objective is to uncover the pre-supernova (SN) CSM structure and constrain the progenitor star's mass-
Externí odkaz:
http://arxiv.org/abs/2410.17699
Autor:
Ibik, Adaeze L., Drout, Maria R., Margutti, Raffaela, Matthews, David, Villar, V. Ashley, Berger, Edo, Chornock, Ryan, Alexander, Kate D., Eftekhari, Tarraneh, Laskar, Tanmoy, Lunnan, Ragnhild, Foley, Ryan J., Jones, David, Milisavljevic, Dan, Rest, Armin, Scolnic, Daniel, Williams, Peter K. G.
Luminous interacting supernovae are a class of stellar explosions whose progenitors underwent vigorous mass loss in the years prior to core-collapse. While the mechanism by which this material is ejected is still debated, obtaining the full density p
Externí odkaz:
http://arxiv.org/abs/2410.15140
Autor:
Azfar, Farrukh, Tseng, Jeff, Molla, Marta Colomer, Scholberg, Kate, Habig, Alec, BenZvi, Segev, Kara, Melih, Kneller, James, Migenda, Jost, Milisavljevic, Dan, O'Connor, Evan
A Galactic core-collapse supernova (CCSN) is likely to be observed in neutrino detectors around the world minutes to hours before the electromagnetic radiation arrives. The SNEWS2.0 network of neutrino and dark matter detectors aims to use the relati
Externí odkaz:
http://arxiv.org/abs/2410.11984
Autor:
Shahbandeh, Melissa, Fox, Ori D., Temim, Tea, Dwek, Eli, Sarangi, Arkaprabha, Smith, Nathan, Dessart, Luc, Nickson, Bryony, Engesser, Michael, Filippenko, Alexei V., Brink, Thomas G., Zheng, Weikang, Szalai, Tamás, Johansson, Joel, Rest, Armin, Van Dyk, Schuyler D., Andrews, Jennifer, Ashall, Chris, Clayton, Geoffrey C., De Looze, Ilse, Derkacy, James M., Dulude, Michael, Foley, Ryan J., Gezari, Suvi, Gomez, Sebastian, Gonzaga, Shireen, Indukuri, Siva, Jencson, Jacob, Kasliwal, Mansi, Lane, Zachary G., Lau, Ryan, Law, David, Marston, Anthony, Milisavljevic, Dan, O'Steen, Richard, Pierel, Justin, Siebert, Matthew, Skrutskie, Michael, Strolger, Lou, Tinyanont, Samaporn, Wang, Qinan, Williams, Brian, Xiao, Lin, Yang, Yi, Zsíros, Szanna
Dust from core-collapse supernovae (CCSNe), specifically Type IIP SNe, has been suggested to be a significant source of the dust observed in high-redshift galaxies. CCSNe eject large amounts of newly formed heavy elements, which can condense into dus
Externí odkaz:
http://arxiv.org/abs/2410.09142
Autor:
De Looze, Ilse, Milisavljevic, Dan, Temim, Tea, Dickinson, Danielle, Fesen, Robert, Arendt, Richard G., Chastenet, Jeremy, Orlando, Salvatore, Vink, Jacco, Barlow, Michael J., Kirchschlager, Florian, Priestley, Felix D., Raymond, John C., Rho, Jeonghee, Sartorio, Nina S., Scheffler, Tassilo, Schmidt, Franziska, Blair, William P., Fox, Ori, Fryer, Christopher, Janka, Hans-Thomas, Koo, Bon-Chul, Laming, J. Martin, Matsuura, Mikako, Patnaude, Dan, Relano, Monica, Rest, Armin, Schmidt, Judy, Smith, Nathan, Sravan, Niharika
JWST observations of the young Galactic supernova remnant Cassiopeia A revealed an unexpected structure seen as a green emission feature in colored composite MIRI F1130W and F1280W images - hence dubbed the Green Monster - that stretches across the c
Externí odkaz:
http://arxiv.org/abs/2410.05402
Autor:
Gomez, Sebastian, Temim, Tea, Fox, Ori, Villar, V. Ashley, Shahbandeh, Melissa, Ashall, Chris, Jencson, Jacob E., Langeroodi, Danial, De Looze, Ilse, Milisavljevic, Dan, Pierel, Justin, Rest, Armin, Szalai, Tamás, Tinyanont, Samaporn
We present JWST/MIRI observations of the Type I superluminous supernova (SLSN) 2017gci taken over 2000 rest-frame days after the supernova (SN) exploded, which represent the latest phase images taken of any known SLSN. We find that archival \WISE det
Externí odkaz:
http://arxiv.org/abs/2408.15397
The SNEWS 2.0 Alert Software for the Coincident Detection of Neutrinos from Core-Collapse Supernovae
Autor:
Kara, M., Torres-Lara, S., Baxter-Depoian, A., BenZvi, S., Molla, M. Colomer, Habig, A., Kneller, J. P., Lai, M., Lang, R. F., Linvill, M., Milisavljevic, D., Migenda, J., Orr, C., Scholberg, K., Smolsky, J., Tseng, J., Tunnell, C. D., Vasel, J., Sheshukov, A.
The neutrino signal from the next galactic core-collapse supernova will provide an invaluable early warning of the explosion. By combining the burst trigger from several neutrino detectors, the location of the explosion can be triangulated minutes to
Externí odkaz:
http://arxiv.org/abs/2406.17743
Autor:
Rho, J., Park, S. -H., Arendt, R., Matsuura, M., Milisavljevic, D., Temim, T., De Looze, I., Blair, W. P., Rest, A., Fox, O., Ravi, A. P., Koo, B. -C., Barlow, M., Burrows, A., Chevalier, R., Clayton, G., Fesen, R., Fransson, C., Fryer, C., Gomez, H. L., Janka, H. -T., Kirchschlarger, F., Laming, J. M., Orlando, S., Patnaude, D., Pavlov, G., Plucinsky, P., Posselt, B., Priestley, F., Raymond, J., Sartorio, N., Schmidt, F., Slane, P., Smith, N., Sravan, N., Vink, J., Weil, K., Wheeler, J., Yoon, S. C.
We present JWST NIRCam (F356W and F444W filters) and MIRI (F770W) images and NIRSpec- IFU spectroscopy of the young supernova remnant Cassiopeia A (Cas A). We obtained the data as part of a JWST survey of Cas A. The NIRCam and MIRI images map the spa
Externí odkaz:
http://arxiv.org/abs/2406.03685