Zobrazeno 1 - 10
of 412
pro vyhledávání: '"Williams, Robert E A"'
Publikováno v:
In Energy & Buildings 1 May 2024 310
Autor:
Chatterjee, Sharmistha, Ricciardi, Loredana, Deitz, Julia I., Williams, Robert E. A., McComb, David W., Strangi, Giuseppe
Publikováno v:
Nanoscale Advances, 2019, DOI: 10.1039/C9NA00301K
In this contribution experimental evidence of plasmonic edge modes and breathing acoustic modes in gold nanostars (AuNS) is reported. AuNS are synthesized in a surfactant-free, one-step wet-chemistry method. Optical extinction measurements of AuNS co
Externí odkaz:
http://arxiv.org/abs/1905.11444
Autor:
Jencson, Jacob E., Adams, Scott M., Bond, Howard E., van Dyk, Schuyler D., Kasliwal, Mansi M., Bally, John, Blagorodnova, Nadejda, De, Kishalay, Fremling, Christoffer, Yao, Yuhan, Fruchter, Andrew, Rubin, David, Barbarino, Cristina, Sollerman, Jesper, Miller, Adam A., Hicks, Erin K. S., Malkan, Matthew A., Andreoni, Igor, Bellm, Eric C., Buchheim, Robert, Dekany, Richard, Feeney, Michael, Frederick, Sara, Gal-Yam, Avishay, Gehrz, Robert D., Giomi, Matteo, Graham, Matthew J., Green, Wayne, Hale, David, Hankins, Matthew J., Hanson, Mark, Helou, George, Ho, Anna Y. Q., Hung, T., Jurić, Mario, Kendurkar, Malhar R., Kulkarni, S. R., Lau, Ryan M., Masci, Frank J., Neill, James D., Quin, Kevin, Riddle, Reed L., Rusholme, Ben, Sims, Forrest, Smith, Nathan, Smith, Roger M., Soumagnac, Maayane T., Tachibana, Yutaro, Tinyanont, Samaporn, Walters, Richard, Watson, Stanley, Williams, Robert E.
Publikováno v:
The Astrophysical Journal Letters, 880 (2019) L20
We present the discovery of an optical transient (OT) in Messier 51, designated M51 OT2019-1 (also ZTF19aadyppr, AT 2019abn, ATLAS19bzl), by the Zwicky Transient Facility (ZTF). The OT rose over 15 days to an observed luminosity of $M_r=-13$ (${\nu}L
Externí odkaz:
http://arxiv.org/abs/1904.07857
Autor:
Jencson, Jacob E., Kasliwal, Mansi M., Adams, Scott M., Bond, Howard E., De, Kishalay, Johansson, Joel, Karambelkar, Viraj, Lau, Ryan M., Tinyanont, Samaporn, Ryder, Stuart D., Cody, Ann Marie, Masci, Frank J., Bally, John, Blagorodnova, Nadia, Castellón, Sergio, Fremling, Christoffer, Gehrz, Robert D., Helou, George, Kilpatrick, Charles D., Milne, Peter A., Morrell, Nidia, Perley, Daniel A., Phillips, M. M., Smith, Nathan, van Dyk, Schuyler D., Williams, Robert E.
Publikováno v:
The Astrophysical Journal 886 (2019) 40
We present a systematic study of the most luminous ($M_{\mathrm{IR}}$ [Vega magnitudes] brighter than $-14$) infrared (IR) transients discovered by the SPitzer InfraRed Intensive Transients Survey (SPIRITS) between 2014 and 2018 in nearby galaxies ($
Externí odkaz:
http://arxiv.org/abs/1901.00871
Autor:
Sion, Edward M., Wilson, R. E., Godon, Patrick, Starrfield, Sumner, Williams, Robert E., Darnley, Matt J.
An HST COS Far UV spectrum (1170 A to 1800 A) was obtained for the short orbital period recurrent novae (T Pyxidis subclass), CI Aquilae. CI Aql is the only classical CV known to have two eclipses of sensible depth per orbit cycle and also have pre-
Externí odkaz:
http://arxiv.org/abs/1812.09993
Autor:
Shara, Michael M., Zurek, David, Schaefer, Bradley E., Bond, Howard E., Godon, Patrick, Mac Low, Mordecai-Mark, Pagnotta, Ashley, Prialnik, Dina, Sion, Edward M., Toraskar, Jayashree, Williams, Robert E.
T Pyxidis is the only recurrent nova surrounded by knots of material ejected in previous outbursts. Following the eruption that began on 2011 April 14.29, we obtained seven epochs (from 4 to 383 days after eruption) of Hubble Space Telescope narrowba
Externí odkaz:
http://arxiv.org/abs/1503.08840
We modelled the late-time {\it Hubble Space Telescope} imaging of RS Ophiuchi with models from Ribeiro et al. (2009), which at the time due to the unknown availability of simultaneous ground-based spectroscopy left some open questions as to the evolu
Externí odkaz:
http://arxiv.org/abs/1410.0148
Autor:
Mason, Elena, Orio, Marina, Mukai, Koji, Bianchini, Antonio, de Martino, Domitilla, di Mille, Francesco, Williams, Robert E., Abbot, Timothy, de Propris, Roberto
We present new X-ray and optical spectra of the old nova CP Pup (nova Pup 1942) obtained with Chandra and the CTIO 4m telescope. The X-ray spectrum reveals a multi-temperature optically thin plasma reaching a maximum temperature of 36$^{+19}_{-16}$ k
Externí odkaz:
http://arxiv.org/abs/1308.5175
Autor:
Mason, Elena, Bianchini, Antonio, Orio, Marina, Williams, Robert E., Mukai, Koji, de Marino, Domitilla, Abbot, Timothy . M. C., di Mille, Francesco
Fast cadence time resolved spectra taken at the CTIO-4m telescope with the RC-spectrograph during 2 consecutive nights revealed a long term modulation of the binary radial velocity. Chandra hard X-ray spectra taken with the HETGS instrument showed fe
Externí odkaz:
http://arxiv.org/abs/1303.2777
Publikováno v:
In Annals of Nuclear Energy June 2019 128:209-215