Zobrazeno 1 - 10
of 81
pro vyhledávání: '"Penprase, Bryan"'
Autor:
Cañas, Caleb I., Kanodia, Shubham, Libby-Roberts, Jessica, Lin, Andrea S. J., Schutte, Maria, Powers, Luke, Jones, Sinclaire, Monson, Andrew, Wang, Songhu, Stefánsson, Guðmundur, Cochran, William D., Robertson, Paul, Mahadevan, Suvrath, Kowalski, Adam F., Wisniewski, John, Parker, Brock A., Larsen, Alexander, Chapman, Franklin A. L., Kobulnicky, Henry A., Gupta, Arvind F., Everett, Mark E., Penprase, Bryan Edward, Zeimann, Gregory, Beard, Corey, Bender, Chad F., Colón, Knicole D., Diddams, Scott A., Fredrick, Connor, Halverson, Samuel, Ninan, Joe P., Ramsey, Lawrence W., Roy, Arpita, Schwab, Christian
Publikováno v:
AJ, 166, 30 (2023)
We confirm the planetary nature of two gas giants discovered by TESS to transit M dwarfs with stellar companions at wide separations. TOI-3984 A ($J=11.93$) is an M4 dwarf hosting a short-period ($4.353326 \pm 0.000005$ days) gas giant ($M_p=0.14\pm0
Externí odkaz:
http://arxiv.org/abs/2302.07714
Autor:
Wee, Jerrick, Blagorodnova, Nadejda, Penprase, Bryan Edward, Facey, Jett Pierce, Morioka, Taiga, Corbett, Hank, Barlow, Brad N., Kupfer, Thomas, Law, Nicholas M., Ratzloff, Jeffrey K., Howard, Ward S., Chavez, Ramses Gonzalez, Glazier, Amy, Soto, Alan Vasquez, Horiuchi, Takashi
We present optical and infrared photometry of the classical nova V906 Car, also known as Nova Car 2018 and ASASSN-18fv, discovered by ASASS-SN survey on 16.32 March 2018 UT (MJD 58193.0). The nova reached its maximum on MJD 58222.56 at $V_{\rm{max}}
Externí odkaz:
http://arxiv.org/abs/2006.14336
Autor:
Bolin, Bryce T., Lisse, Carey M., Kasliwal, Mansi M., Quimby, Robert, Tan, Hanjie, Copperwheat, Chris, Lin, Zhong-Yi, Morbidelli, Alessandro, Abe, Lyu, Bendjoya, Philippe, Bauer, James, Burdge, Kevin B., Coughlin, Michael, Fremling, Christoffer, Itoh, Ryosuke, Koss, Michael, Masci, Frank J., Maeno, Syota, Mamajek, Eric E., Marocco, Federico, Murata, Katsuhiro, Rivet, Jean-Pierre, Sitko, Michael L., Stern, Daniel, Vernet, David, Walters, Richard, Yan, Lin, Andreoni, Igor, Bhalerao, Varun, Bodewits, Dennis, De, Kishalay, Deshmukh, Kunal P., Bellm, Eric C., Blagorodnova, Nadejda, Buzasi, Derek, Cenko, S. Bradley, Chang, Chan-Kao, Chojnowski, Drew, Dekany, Richard, Duev, Dmitry A., Graham, Matthew, Juric, Mario, Kramer, Emily A., Kulkarni, Shrinivas R., Kupfer, Thomas, Mahabal, Ashish, Neill, James D., Ngeow, Chow-Choong, Penprase, Bryan, Riddle, Reed, Rodriguez, Hector, Rosnet, Philippe, Smith, Roger M., Sollerman, Jesper, Soumagnac, Maayane T.
We present visible and near-infrared photometric and spectroscopic observations of interstellar object 2I/Borisov taken from 2019 September 10 to 2019 November 29 using the GROWTH, the APO ARC 3.5 m and the NASA/IRTF 3.0 m combined with post and pre-
Externí odkaz:
http://arxiv.org/abs/1910.14004
Autor:
Bellm, Eric C., Kulkarni, Shrinivas R., Graham, Matthew J., Dekany, Richard, Smith, Roger M., Riddle, Reed, Masci, Frank J., Helou, George, Prince, Thomas A., Adams, Scott M., Barbarino, C., Barlow, Tom, Bauer, James, Beck, Ron, Belicki, Justin, Biswas, Rahul, Blagorodnova, Nadejda, Bodewits, Dennis, Bolin, Bryce, Brinnel, Valery, Brooke, Tim, Bue, Brian, Bulla, Mattia, Burruss, Rick, Cenko, S. Bradley, Chang, Chan-Kao, Connolly, Andrew, Coughlin, Michael, Cromer, John, Cunningham, Virginia, De, Kishalay, Delacroix, Alex, Desai, Vandana, Duev, Dmitry A., Eadie, Gwendolyn, Farnham, Tony L., Feeney, Michael, Feindt, Ulrich, Flynn, David, Franckowiak, Anna, Frederick, S., Fremling, C., Gal-Yam, Avishay, Gezari, Suvi, Giomi, Matteo, Goldstein, Daniel A., Golkhou, V. Zach, Goobar, Ariel, Groom, Steven, Hacopians, Eugean, Hale, David, Henning, John, Ho, Anna Y. Q., Hover, David, Howell, Justin, Hung, Tiara, Huppenkothen, Daniela, Imel, David, Ip, Wing-Huen, Ivezić, Željko, Jackson, Edward, Jones, Lynne, Juric, Mario, Kasliwal, Mansi M., Kaspi, S., Kaye, Stephen, Kelley, Michael S. P., Kowalski, Marek, Kramer, Emily, Kupfer, Thomas, Landry, Walter, Laher, Russ R., Lee, Chien-De, Lin, Hsing Wen, Lin, Zhong-Yi, Lunnan, Ragnhild, Mahabal, Ashish, Mao, Peter, Miller, Adam A., Monkewitz, Serge, Murphy, Patrick, Ngeow, Chow-Choong, Nordin, Jakob, Nugent, Peter, Ofek, Eran, Patterson, Maria T., Penprase, Bryan, Porter, Michael, Rauch, Ludwig, Rebbapragada, Umaa, Reiley, Dan, Rigault, Mickael, Rodriguez, Hector, van Roestel, Jan, Rusholme, Ben, van Santen, Jakob, Schulze, S., Shupe, David L., Singer, Leo P., Soumagnac, Maayane T., Stein, Robert, Surace, Jason, Sollerman, Jesper, Szkody, Paula, Taddia, F., Terek, Scott, Van Sistine, Angela, van Velzen, Sjoert, Vestrand, W. Thomas, Walters, Richard, Ward, Charlotte, Ye, Quan-Zhi, Yu, Po-Chieh, Yan, Lin, Zolkower, Jeffry
Publikováno v:
Publications of the Astronomical Society of the Pacific, Volume 131, Issue 995, pp. 018002 (2019)
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 second readout time, yielding more than an order of ma
Externí odkaz:
http://arxiv.org/abs/1902.01932
Autor:
Graham, Matthew J., Kulkarni, S. R., Bellm, Eric C., Adams, Scott M., Barbarino, Cristina, Blagorodnova, Nadejda, Bodewits, Dennis, Bolin, Bryce, Brady, Patrick R., Cenko, S. Bradley, Chang, Chan-Kao, Coughlin, Michael W., De, Kishalay, Eadie, Gwendolyn, Farnham, Tony L., Feindt, Ulrich, Franckowiak, Anna, Fremling, Christoffer, Gal-yam, Avishay, Gezari, Suvi, Ghosh, Shaon, Goldstein, Daniel A., Golkhou, V. Zach, Goobar, Ariel, Ho, Anna Y. Q., Huppenkothen, Daniela, Ivezic, Zeljko, Jones, R. Lynne, Juric, Mario, Kaplan, David L., Kasliwal, Mansi M., Kelley, Michael S. P., Kupfer, Thomas, Lee, Chien-De, Lin, Hsing Wen, Lunnan, Ragnhild, Mahabal, Ashish A., Miller, Adam A., Ngeow, Chow-Choong, Nugent, Peter, Ofek, Eran O., Prince, Thomas A., Rauch, Ludwig, van Roestel, Jan, Schulze, Steve, Singer, Leo P., Sollerman, Jesper, Taddia, Francesco, Yan, Lin, Ye, Quan-Zhi, Yu, Po-Chieh, Andreoni, Igor, Barlow, Tom, Bauer, James, Beck, Ron, Belicki, Justin, Biswas, Rahul, Brinnel, Valery, Brooke, Tim, Bue, Brian, Bulla, Mattia, Burdge, Kevin, Burruss, Rick, Connolly, Andrew, Cromer, John, Cunningham, Virginia, Dekany, Richard, Delacroix, Alex, Desai, Vandana, Duev, Dmitry A., Hacopians, Eugean, Hale, David, Helou, George, Henning, John, Hover, David, Hillenbrand, Lynne A., Howell, Justin, Hung, Tiara, Imel, David, Ip, Wing-Huen, Jackson, Edward, Kaspi, Shai, Kaye, Stephen, Kowalski, Marek, Kramer, Emily, Kuhn, Michael, Landry, Walter, Laher, Russ R., Mao, Peter, Masci, Frank J., Monkewitz, Serge, Murphy, Patrick, Nordin, Jakob, Patterson, Maria T., Penprase, Bryan, Porter, Michael, Rebbapragada, Umaa, Reiley, Dan, Riddle, Reed, Rigault, Mickael, Rodriguez, Hector, Rusholme, Ben, van Santen, Jakob, Shupe, David L., Smith, Roger M., Soumagnac, Maayane T., Stein, Robert, Surace, Jason, Szkody, Paula, Terek, Scott, van Sistine, Angela, van Velzen, Sjoert, Vestrand, W. Thomas, Walters, Richard, Ward, Charlotte, Zhang, Chaoran, Zolkower, Jeffry
The Zwicky Transient Facility (ZTF), a public-private enterprise, is a new time domain survey employing a dedicated camera on the Palomar 48-inch Schmidt telescope with a 47 deg$^2$ field of view and 8 second readout time. It is well positioned in th
Externí odkaz:
http://arxiv.org/abs/1902.01945
Autor:
Perley, Daniel A., Mazzali, Paolo A., Yan, Lin, Cenko, S. Bradley, Gezari, Suvi, Taggart, Kirsty, Blagorodnova, Nadia, Fremling, Christoffer, Mockler, Brenna, Singh, Avinash, Tominaga, Nozomu, Tanaka, Masaomi, Watson, Alan M., Ahumada, Tomás, Anupama, G. C., Ashall, Chris, Becerra, Rosa L., Bersier, David, Bhalerao, Varun, Bloom, Joshua S., Butler, Nathaniel R., Copperwheat, Chris, Coughlin, Michael W., De, Kishalay, Drake, Andrew J., Duev, Dmitry A., Frederick, Sara, González, J. Jesús, Goobar, Ariel, Heida, Marianne, Ho, Anna Y. Q., Horst, John, Hung, Tiara, Itoh, Ryosuke, Jencson, Jacob E., Kasliwal, Mansi M., Kawai, Nobuyuki, Kulkarni, Shrinivas R., Kumar, Brajesh, Kumar, Harsh, Kutyrev, Alexander S., Khanam, Tanazza, Lee, William H., Maeda, Keiichi, Mahabal, Ashish, Murata, Katsuhiro L., Neill, James D., Ngeow, Chow-Choong, Penprase, Bryan, Pian, Elena, Quimby, Robert, Ramirez-Ruiz, Enrico, Richer, Michael, Román-Zúñiga, Carlos G., Srivastava, Shubham, Socia, Quentin, Sollerman, Jesper, Tachibana, Yutaro, Taddia, Francesco, Tinyanont, Samaporn, Troja, Eleonora, Ward, Charlotte, Wee, Jerrick
Wide-field optical surveys have begun to uncover large samples of fast (t_rise < 5d), luminous (M_peak < -18), blue transients. While commonly attributed to the breakout of a supernova shock into a dense wind, the great distances to the transients of
Externí odkaz:
http://arxiv.org/abs/1808.00969
On 2017 March 11, the DLT40 Transient Discovery Survey discovered SN 2017cbv in NGC5643, a Type 2 Seyfert Galaxy in the Lupus Constellation. SN 2017cbv went on to become a bright Type Ia supernova, with a $V_{max}$ of 11.51 $\pm$ 0.05 mag. We present
Externí odkaz:
http://arxiv.org/abs/1806.08794