Zobrazeno 1 - 10
of 217
pro vyhledávání: '"Rupen, Michael P."'
Autor:
Sokolovsky, Kirill V., Aydi, Elias, Malanchev, Konstantin, Burke, Colin J., Mukai, Koji, Sokoloski, J. L., Metzger, Brian D., Atapin, Kirill E., Belinski, Aleksandre A., Chen, Yu-Ching, Chomiuk, Laura, Dubovsky, Pavol A., Faucher-Giguere, Claude-Andre, Hounsell, Rebekah A., Ikonnikova, Natalia P., Lander, Vsevolod Yu., Li, Junyao, Linford, Justin D., Mioduszewski, Amy J., Molina, Isabella, Munari, Ulisse, Potanin, Sergey A., Quimby, Robert M., Rupen, Michael P., Scaringi, Simone, Shatsky, Nicolai I., Shen, Yue, Steinberg, Elad, Stone, Zachary, Tatarnikov, Andrey M., Vurm, Indrek, Williams, Montana N., Azcona, Antonio Agudo, Boyd, David, Bean, Stewart, Braunwarth, Horst, Blackwell, John, Bolzoni, Simone, Casas, Ricard, Fernandez, David Cejudo, Dubois, Franky, Foster, James, Farfan, Rafael, Galdies, Charles, Hodge, John, Gallego, Jose Prieto, Lane, David J., Larsson, Magnus, Lindner, Peter, Logie, Ludwig, Mantero, Andrea, Aimar, Mario Morales, Menzies, Kenneth, Nakonechny, Keith, Philpot, Jerry, Filho, Antonio Padilla, Ramey, Brian, Rau, Steve, Reina, Esteban, Romanov, Filipp D., Ruocco, Nello, Shears, Jeremy, Serreau, Marc, Schmidt, Richard, Solomonov, Yuri, Tracy, Bob, Tulloch, Gord, Tomlin, Ray, Tordai, Tamas, Vanaverbeke, Siegfried, Wenzel, Klaus
Lightcurves of many classical novae deviate from the canonical "fast rise - smooth decline" pattern and display complex variability behavior. We present the first TESS-space-photometry-based investigation of this phenomenon. We use TESS Sector 41 ful
Externí odkaz:
http://arxiv.org/abs/2311.04903
Autor:
Finzell, Thomas, Chomiuk, Laura, Metzger, Brian D., Walter, Frederick M., Linford, Justin D., Mukai, Koji, Nelson, Thomas, Weston, Jennifer H. S., Zheng, Yong, Sokoloski, Jennifer L., Mioduszewski, Amy, Rupen, Michael P., Dong, Subo, Starrfield, Sumner, Cheung, C. C., Woodward, Charles E., Taylor, Gregory B., Bohlsen, Terry, Buil, Christian, Prieto, Jose, Wagner, R. Mark, Bensby, Thomas, Bond, I. A., Sumi, T., Bennett, D. P., Abe, F., Koshimoto, N., Suzuki, D., Tristram, P. J., Christie, Grant W., Natusch, Tim, McCormick, Jennie, Yee, Jennifer, Gould, Andy
It has recently been discovered that some, if not all, classical novae emit GeV gamma-rays during outburst, but the mechanisms involved in the production ofgamma-rays are still not well understood. We present here a comprehensive multiwavelength data
Externí odkaz:
http://hdl.handle.net/10150/626558
http://arizona.openrepository.com/arizona/handle/10150/626558
http://arizona.openrepository.com/arizona/handle/10150/626558
Autor:
Hughes, Andrew K., Sivakoff, Gregory R., Macpherson, Christopher E., Miller-Jones, James C. A., Tetarenko, Alexandra J., Altamirano, Diego, Anderson, Gemma E., Belloni, Tomaso M., Heinz, Sebastian, Jonker, Peter G., Körding, Elmar G., Maitra, Dipankar, Markoff, Sera B., Migliari, Simone, Mooley, Kunal P., Rupen, Michael P., Russell, David M., Russell, Thomas D., Sarazin, Craig L., Soria, Roberto, Tudose, Valeriu
We present a high time resolution, multi-frequency linear polarization analysis of Very Large Array (VLA) radio observations during some of the brightest radio flaring (~1 Jy) activity of the 2015 outburst of V404 Cygni. The VLA simultaneously captur
Externí odkaz:
http://arxiv.org/abs/2301.13281
Autor:
Sokolovsky, Kirill V., Li, Kwan-Lok, de Oliveira, Raimundo Lopes, Ness, Jan-Uwe, Mukai, Koji, Chomiuk, Laura, Aydi, Elias, Steinberg, Elad, Vurm, Indrek, Metzger, Brian D., Babul, Aliya-Nur, Kawash, Adam, Linford, Justin D., Nelson, Thomas, Page, Kim L., Rupen, Michael P., Sokoloski, Jennifer L., Strader, Jay, Kilkenny, David
Peaking at 3.7 mag on 2020 July 11, YZ Ret was the second-brightest nova of the decade. The nova's moderate proximity (2.7 kpc from Gaia) provided an opportunity to explore its multi-wavelength properties in great detail. Here we report on YZ Ret as
Externí odkaz:
http://arxiv.org/abs/2108.03241
Autor:
Chomiuk, Laura, Linford, Justin D., Aydi, Elias, Bannister, Keith W., Krauss, Miriam I., Mioduszewski, Amy J., Mukai, Koji, Nelson, Thomas J., Rupen, Michael P., Ryder, Stuart D., Sokoloski, Jennifer L., Sokolovsky, Kirill V., Strader, Jay, Filipovic, Miroslav D., Finzell, Tom, Kawash, Adam, Kool, Erik C., Metzger, Brian D., Nyamai, Miriam M., Ribeiro, Valerio A. R. M., Roy, Nirupam, Urquhart, Ryan, Weston, Jennifer
We present radio observations (1--40 GHz) for 36 classical novae, representing data from over five decades compiled from the literature, telescope archives, and our own programs. Our targets display a striking diversity in their optical parameters (e
Externí odkaz:
http://arxiv.org/abs/2107.06251
Autor:
Nelson, Thomas, Mukai, Koji, Chomiuk, Laura, Sokoloski, Jennifer L., Linford, Justin D., Finzell, Thomas, Mioduszewski, Amy J., Rupen, Michael P., Weston, Jennifer, de Oliveira, Raimundo Lopes
X-ray observations of shocked gas in novae can provide a useful probe of the dynamics of the ejecta. Here we report on X-ray observations of the nova V959 Mon, which was also detected in GeV gamma-rays with the Fermi satellite. We find that the X-ray
Externí odkaz:
http://arxiv.org/abs/2007.15702
Autor:
Sokolovsky, Kirill V., Mukai, Koji, Chomiuk, Laura, de Oliveira, Raimundo Lopes, Aydi, Elias, Li, Kwan-Lok, Steinberg, Elad, Vurm, Indrek, Metzger, Brian D., Kawash, Adam, Linford, Justin D., Mioduszewski, Amy J., Nelson, Thomas, Ness, Jan-Uwe, Page, Kim L., Rupen, Michael P., Sokoloski, Jennifer L., Strader, Jay
Shocks in gamma-ray emitting classical novae are expected to produce bright thermal and non-thermal X-rays. We test this prediction with simultaneous NuSTAR and Fermi/LAT observations of nova V906 Car, which exhibited the brightest GeV gamma-ray emis
Externí odkaz:
http://arxiv.org/abs/2007.07885
Autor:
Spekkens, Kristine, Chiang, Cynthia, Kothes, Roland, Rosolowsky, Erik, Rupen, Michael, Safi-Harb, Samar, Sievers, Jonathan, Sivakoff, Greg, Stairs, Ingrid, van der Marel, Nienke, Abraham, Bob, Alexandroff, Rachel, Bartel, Norbert, Baum, Stefi, Bietenholz, Michael, Boley, Aaron, Bond, Dick, Brown, Joanne, Brown, Toby, Davis, Gary, English, Jayanne, Fahlman, Greg, Ferrarese, Laura, Di Francesco, James, Gaensler, Bryan, Gaudet, Severin, Graber, Vanessa, Halpern, Mark, Hill, Alex, Hlavacek-Larrondo, Julie, Irwin, Judith, Johnstone, Doug, Joncas, Gilles, Kaspi, Vicky, Kavelaars, JJ, Liu, Adrian, Matthews, Brenda, Mirocha, Jordan, Monsalve, Raul, Ng, Cherry, O'Dea, Chris, Pen, Ue-Li, Plume, Rene, Robishaw, Tim, Sadavoy, Sarah, Sanghai, Viraj, Scholz, Paul, Simard, Luc, Shaw, Richard, Singh, Saurabh, Sigurdson, Kris, Smith, Kendrick, Stevens, David, Stil, Jeroen, Tulin, Sean, van Eck, Cameron, Wall, Jasper, West, Jennifer, Woods, Tyrone, Wulf, Dallas
This white paper submitted for the 2020 Canadian Long-Range Planning process (LRP2020) presents the prospects for Canada and the Square Kilometre Array (SKA) from 2020-2030, focussing on the first phase of the project (SKA1) scheduled to begin constr
Externí odkaz:
http://arxiv.org/abs/1911.03250
Autor:
Di Francesco, James, Chalmers, Dean, Denman, Nolan, Fissel, Laura, Friesen, Rachel, Gaensler, Bryan, Hlavacek-Larrondo, Julie, Kirk, Helen, Matthews, Brenda, O'Dea, Christopher, Robishaw, Tim, Rosolowsky, Erik, Rupen, Michael, Sadavoy, Sarah, Safi-Harb, Samar, Sivakoff, Greg, Tahani, Mehrnoosh, van der Marel, Nienke, White, Jacob, Wilson, Christine
The next generation Very Large Array (ngVLA) is a transformational radio observatory being designed by the U.S. National Radio Astronomy Observatory (NRAO). It will provide order of magnitude improvements in sensitivity, resolution, and uv coverage o
Externí odkaz:
http://arxiv.org/abs/1911.01517
Autor:
Eadie, Gwendolyn, Bahramian, Arash, Barmby, Pauline, Craiu, Radu, Bingham, Derek, Hložek, Renée, Kavelaars, JJ, Stenning, David, Benincasa, Samantha, Thomas, Guillaume, Thanjavur, Karun, Bovy, Jo, Cami, Jan, Carlberg, Ray, Lawler, Sam, Liu, Adrian, Ngo, Henry, Rahman, Mubdi, Rupen, Michael
(Abridged from Executive Summary) This white paper focuses on the interdisciplinary fields of astrostatistics and astroinformatics, in which modern statistical and computational methods are applied to and developed for astronomical data. Astrostatist
Externí odkaz:
http://arxiv.org/abs/1910.08857