Zobrazeno 1 - 10
of 5 420
pro vyhledávání: '"Quimby A"'
Autor:
Bolin, B. T., Masci, F. J., Coughlin, M. W., Duev, D. A., Ivezić, Ž., Jones, R. L., Yoachim, P., Ahumada, T., Bhalerao, V., Choudhary, H., Contreras, C., Cheng, Y. -C., Copperwheat, C. M., Deshmukh, K., Fremling, C., Granvik, M., Hardegree-Ullman, K. K., Ho, A. Y. Q., Jedicke, R., Kasliwal, M., Kumar, H., Lin, Z. -Y., Mahabal, A., Monson, A., Neill, J. D., Nesvorný, D., Perley, D. A., Purdum, J. N., Quimby, R., Serabyn, E., Sharma, K., Swain, V.
Near-sun sky twilight observations allow for the detection of asteroid interior to the orbit of Venus (Aylos), the Earth (Atiras), and comets. We present the results of observations with the Palomar 48-inch telescope (P48)/Zwicky Transient Facility (
Externí odkaz:
http://arxiv.org/abs/2409.15263
Autor:
Pierel, J. D. R., Engesser, M., Coulter, D. A., Decoursey, C., Siebert, M. R., Rest, A., Egami, E., Chen, W., Fox, O. D., Jones, D. O., Joshi, B. A., Moriya, T. J., Zenati, Y., Bunker, A. J., Cargile, P. A., Curti, M., Eisenstein, D. J., Gezari, S., Gomez, S., Guolo, M., Johnson, B. D., Karmen, M., Maiolino, R., Quimby, Robert M., Robertson, B., Shahbandeh, M., Strolger, L. G., Sun, F., Wang, Q., Wevers, T.
We present the JWST discovery of SN 2023adsy, a transient object located in a host galaxy JADES-GS$+53.13485$$-$$27.82088$ with a host spectroscopic redshift of $2.903\pm0.007$. The transient was identified in deep James Webb Space Telescope (JWST)/N
Externí odkaz:
http://arxiv.org/abs/2406.05089
Autor:
Siebert, M. R., Decoursey, C., Coulter, D. A., Engesser, M., Pierel, J. D. R., Rest, A., Egami, E., Shahbandeh, M., Chen, W., Fox, O. D., Zenati, Y., Moriya, T. J., Bunker, A. J., Cargile, P. A., Curti, M., Eisenstein, D. J., Gezari, S., Gomez, S., Guolo, M., Johnson, B. D., Joshi, B. A., Karmen, M., Maiolino, R., Quimby, R. M., Robertson, B., Strolger, L. G., Sun, F., Wang, Q., Wevers, T.
We present JWST NIRCam and NIRSpec observations of a Type Ic supernova (SN Ic) and its host galaxy (JADES-GS+53.13533-27.81457) at $z = 2.83$. This SN (named SN 2023adta) was identified in deep James Webb Space Telescope (JWST)/NIRCam imaging from th
Externí odkaz:
http://arxiv.org/abs/2406.05076
Autor:
DeCoursey, Christa, Egami, Eiichi, Pierel, Justin D. R., Sun, Fengwu, Rest, Armin, Coulter, David A., Engesser, Michael, Siebert, Matthew R., Hainline, Kevin N., Johnson, Benjamin D., Bunker, Andrew J., Cargile, Phillip A., Charlot, Stephane, Chen, Wenlei, Curti, Mirko, DeFour-Remy, Shea, Eisenstein, Daniel J., Fox, Ori D., Gezari, Suvi, Gomez, Sebastian, Jencson, Jacob, Joshi, Bhavin A., Khairnar, Sanvi, Lyu, Jianwei, Maiolino, Roberto, Moriya, Takashi J., Quimby, Robert M., Rieke, George H., Rieke, Marcia J., Robertson, Brant, Shahbandeh, Melissa, Strolger, Louis-Gregory, Tacchella, Sandro, Wang, Qinan, Williams, Christina C., Willmer, Christopher N. A., Willott, Chris, Zenati, Yossef
The JWST Advanced Deep Extragalactic Survey (JADES) is a multi-cycle JWST program that has taken among the deepest near-/mid-infrared images to date (down to $\sim$30 ABmag) over $\sim$25 arcmin$^2$ in the GOODS-S field in two sets of observations wi
Externí odkaz:
http://arxiv.org/abs/2406.05060
Autor:
Jha, Saurabh W., Casetti-Dinescu, Dana I., Bernstein, Gary M., Hayes, Matthew J., Oskinova, Lidia M., Pace, Andrew B., Quimby, Robert M., Reiter, Megan, Rest, Armin, Riess, Adam G., Sand, David J., Weisz, Daniel R.
The Astro2020 Decadal Survey recognizes time-domain astronomy as a key science area over the next decade and beyond. With over 30 years of HST data and the potential for 20 years of JWST operations, these flagship observatories offer an unparalleled
Externí odkaz:
http://arxiv.org/abs/2405.12297
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:
Dhungana, Govinda, Kehoe, Robert, Staten, Ryan, Vinko, Jozsef, Wheeler, J. Craig, Akerlof, Carl W., Doss, David, Farrente, Farley V., Gibson, Coyne A., Lasker, James, Marion, G. H., Pandey, Shashi Bhushan, Quimby, Robert, Rykoff, Eli, Smith, Donald A., Yuan, Fang, Zheng, WeiKang
We present cosmological analysis of 12 nearby ($z<0.06$) Type IIP supernovae (SNe IIP) observed with the ROTSE-IIIb telescope. To achieve precise photometry, we present a new image differencing technique that is implemented for the first time on the
Externí odkaz:
http://arxiv.org/abs/2308.00916
Autor:
L. S. Moussaoui, M. Quimby, H. Avancini, A. Salawdi, F. Skaik, R. Bani Odeh, O. Desrichard, N. Claxton
Publikováno v:
Archives of Public Health, Vol 82, Iss 1, Pp 1-17 (2024)
Abstract Background Informing humanitarian action directly from community members is recognized as critical. However, collecting community insights is also a challenge in practice. This paper reports data collected among community members and Red Cre
Externí odkaz:
https://doaj.org/article/d2dc5cf337624a63991888f392d2944d
Autor:
Gomez, Sebastian, Alexander, Kate, Berger, Edo, Blanchard, Peter K., Broekgaarden, Floor, Eftekhari, Tarraneh, Fox, Ori, Gill, Kiranjyot, Hiramatsu, Daichi, Joshi, Bhavin, Karmen, Mitchell, Moriya, Takashi, Nicholl, Matt, Quimby, Robert, Regos, Eniko, Rest, Armin, Rose, Benjamin, Shahbandeh, Melissa, Villar, V. Ashley
Type-I Superluminous Supernovae (SLSNe) are an exotic class of core-collapse SN (CCSN) that can be up to 100 times brighter and more slowly-evolving than normal CCSNe. SLSNe represent the end-stages of the most massive stripped stars, and are thought
Externí odkaz:
http://arxiv.org/abs/2306.17233
Autor:
Moriya, Takashi, Fox, Ori D., Quimby, Robert, Schulze, Steve, Villar, Ashley, Rest, Armin, Grogin, Norman, Gomez, Sebastian, Rubin, David, Siebert, Matt, Kassin, Susan, Regos, Eniko, Strolger, Lou, Koekemoer, Anton, Finkelstein, Steven, Gezari, Suvi, Mattila, Seppo, Temim, Tea, Shahbandeh, Melissa, Williams, Bob, Chen, Ting-Wan, Hook, Isobel, Pierel, Justin, Ouchi, Masami, Harikane, Yuichi
Pair-instability supernovae (PISNe) are explosions of very massive stars that may have played a critical role in the chemical evolution and reionization of the early Universe. In order to quantify their roles, it is required to know the PISN event ra
Externí odkaz:
http://arxiv.org/abs/2306.17212