Zobrazeno 1 - 10
of 398
pro vyhledávání: '"Van Dyk, Schuyler D"'
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:
Van Dyk, Schuyler D., Szalai, Tamas, Cutri, Roc M., Kirkpatrick, J. Davy, Grillmair, Carl J., Fajardo-Acosta, Sergio B., Masiero, Joseph R., Mainzer, Amy K., Gelino, Christopher R., Vinko, Jozsef, Joo, Andras Peter, Pal, Andras, Konyves-Toth, Reka, Kriskovics, Levente, Szakats, Robert, Vida, Krisztian, Zheng, WeiKang, Brink, Thomas G., Filippenko, Alexei V.
The reactivated Near-Earth Object Wide-field Infrared Survey Explorer (NEOWISE-R) serendipitously caught the Type II supernova SN 2023ixf in Messier 101 on the rise, starting day 3.6 through day 10.9, and on the late-time decline from days 211 throug
Externí odkaz:
http://arxiv.org/abs/2406.18005
Autor:
Baer-Way, Raphael, DeGraw, Asia, Zheng, Weikang, Van Dyk, Schuyler D., Filippenko, Alexei V., Fox, Ori D., Brink, Thomas G., Kelly, Patrick L., Smith, Nathan, Vasylyev, Sergiy S., de Jaeger, Thomas, Zhang, Keto, Stegman, Samantha, Ross, Timothy, Yunus, Sameen
Over recent decades, robotic (or highly automated) searches for supernovae (SNe) have discovered several thousand events, many of them in quite nearby galaxies (distances < 30 Mpc). Most of these SNe, including some of the best-studied events to date
Externí odkaz:
http://arxiv.org/abs/2401.12185
Autor:
Zsíros, Szanna, Szalai, Tamás, De Looze, Ilse, Sarangi, Arkaprabha, Shahbandeh, Melissa, Fox, Ori D., Temim, Tea, Milisavljevic, Dan, Van Dyk, Schuyler D., Smith, Nathan, Filippenko, Alexei V., Brink, Thomas G., Zheng, WeiKang, Dessart, Luc, Jencson, Jacob, Johansson, Joel, Pierel, Justin, Rest, Armin, Tinyanont, Samaporn, Niculescu-Duvaz, Maria, Barlow, M. J., Wesson, Roger, Andrews, Jennifer, Clayton, Geoff, De, Kishalay, Dwek, Eli, Engesser, Michael, Foley, Ryan J., Gezari, Suvi, Gomez, Sebastian, Gonzaga, Shireen, Kasliwal, Mansi, Lau, Ryan, Marston, Anthony, O'Steen, Richard, Siebert, Matthew, Skrutskie, Michael, Strolger, Lou, Wang, Qinan, Williams, Brian, Williams, Robert, Xiao, Lin
We present mid-infrared (mid-IR) imaging of the Type IIL supernova (SN) 1980K with the James Webb Space Telescope (JWST) more than 40 yr post-explosion. SN 1980K, located in the nearby ($D\approx7$ Mpc) "SN factory" galaxy NGC 6946, was serendipitous
Externí odkaz:
http://arxiv.org/abs/2310.03448
Autor:
Dong, Yize, Valenti, Stefano, Ashall, Chris, Williamson, Marc, Sand, David J., Van Dyk, Schuyler D., Filippenko, Alexei V., Jha, Saurabh W., Lundquist, Michael, Modjaz, Maryam, Andrews, Jennifer E., Jencson, Jacob E., Hosseinzadeh, Griffin, Pearson, Jeniveve, Kwok, Lindsey A., Boland, Teresa, Hsiao, Eric Y., Smith, Nathan, Elias-Rosa, Nancy, Srivastav, Shubham, Smartt, Stephen, Fulton, Michael, Zheng, WeiKang, Brink, Thomas G., Shahbandeh, Melissa, Bostroem, K. Azalee, Hoang, Emily, Janzen, Daryl, Mehta, Darshana, Meza, Nicolas, Shrestha, Manisha, Wyatt, Samuel, Auchettl, Katie, Burns, Christopher R., Farah, Joseph, Galbany, L., Gonzalez, Estefania Padilla, Haislip, Joshua, Hinkle, Jason T., Howell, D. Andrew, De Jaeger, Thomas, Kouprianov, Vladimir, Kumar, Sahana, Lu, Jing, McCully, Curtis, Moran, Shane, Morrell, Nidia, Newsome, Megan, Pellegrino, Craig, Polin, Abigail, Reichart, Daniel E., Shappee, B. J., Stritzinger, Maximilian D., Terreran, Giacomo, Tucker, M. A.
Publikováno v:
ApJ 974 316 (2024)
We present optical and near-infrared observations of SN~2022crv, a stripped envelope supernova in NGC~3054, discovered within 12 hrs of explosion by the Distance Less Than 40 Mpc Survey. We suggest SN~2022crv is a transitional object on the continuum
Externí odkaz:
http://arxiv.org/abs/2309.09433
Autor:
Van Dyk, Schuyler D., Srinivasan, Sundar, Andrews, Jennifer E., Soraisam, Monika, Szalai, Tamas, Howell, Steve B., Isaacson, Howard, Matheson, Thomas, Petigura, Erik, Scicluna, Peter, Stephens, Andrew W., Van Zandt, Judah, Zheng, WeiKang, Chun, Sang-Hyun, Filippenko, Alexei V.
We follow our first paper with an analysis of the ensemble of the extensive pre-explosion ground- and space-based infrared observations of the red supergiant (RSG) progenitor candidate for the nearby core-collapse supernova SN 2023ixf in Messier 101,
Externí odkaz:
http://arxiv.org/abs/2308.14844
Autor:
Soraisam, Monika D., Szalai, Tamás, Van Dyk, Schuyler D., Andrews, Jennifer E., Srinivasan, Sundar, Chun, Sang-Hyun, Matheson, Thomas, Scicluna, Peter, Vasquez-Torres, Diego A.
Observational evidence points to a red supergiant (RSG) progenitor for SN 2023ixf. The progenitor candidate has been detected in archival images at wavelengths (>0.6 micron) where RSGs typically emit profusely. This object is distinctly variable in t
Externí odkaz:
http://arxiv.org/abs/2306.10783
Autor:
Shivvers, Isaac, Zheng, WeiKang, Van Dyk, Schuyler D., Mauerhan, Jon, Filippenko, Alexei V., Smith, Nathan, Foley, Ryan J., Mazzali, Paolo, Kamble, Atish, Kilpatrick, Charles D., Margutti, Raffaella, Yuk, Heechan, Graham, Melissa L., Kelly, Patrick L., Andrews, Jennifer, Matheson, Thomas, Wood-Vasey, W. Michael, Ponder, Kara A., Brown, Peter J., Chevalier, Roger, Milisavljevic, Dan, Drout, Maria, Parrent, Jerod, Soderberg, Alicia, Ashall, Chris, Piascik, Andrzej, Prentice, Simon
We present the results of an extensive observational campaign on the nearby Type Ibn SN 2015G, including data from radio through ultravioletwavelengths. SN2015Gwas asymmetric, showing late-time nebular lines redshifted by similar to 1000 km s(-1). It
Externí odkaz:
http://hdl.handle.net/10150/625796
http://arizona.openrepository.com/arizona/handle/10150/625796
http://arizona.openrepository.com/arizona/handle/10150/625796
Autor:
Tinyanont, Samaporn, Kasliwal, Mansi M., Fox, Ori D., Lau, Ryan, Smith, Nathan, Williams, Robert, Jencson, Jacob, Perley, Daniel, Dykhoff, Devin, Gehrz, Robert, Johansson, Joel, Van Dyk, Schuyler D., Masci, Frank, Cody, Ann Marie, Prince, Thomas
We present a systematic study of mid-infrared emission from 141 nearby supernovae (SNe). observed with Spitzer/IRAC as part of the ongoing SPIRITS survey. We detect 8 Type Ia and 36 core-collapse SNe. All Type. Ia/Ibc SNe. become undetectable within
Externí odkaz:
http://hdl.handle.net/10150/622682
http://arizona.openrepository.com/arizona/handle/10150/622682
http://arizona.openrepository.com/arizona/handle/10150/622682
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:
http://arxiv.org/abs/2305.05015