Zobrazeno 1 - 10
of 56
pro vyhledávání: '"Caton, Daniel"'
Autor:
Tampo, Yusuke, Kato, Taichi, Isogai, Keisuke, Kimura, Mariko, Kojiguchi, Naoto, Nogami, Daisaku, Ito, Junpei, Shibata, Masaaki, Yamanaka, Masayuki, Taguchi, Kenta, Maehara, Hiroyuki, Itoh, Hiroshi, Matsumoto, Katsura, Nakagawa, Momoka, Nishida, Yukitaka, Dvorak, Shawn, Murata, Katsuhiro L., Hosokawa, Ryohei, Imai, Yuri, Ito, Naohiro, Niwano, Masafumi, Sato, Shota, Noto, Ryotaro, Yamaguchi, Ryodai, Schramm, Malte, Oasa, Yumiko, Kanai, Takahiro, Sasaki, Yu, Tordai, Tamás, Vanmunster, Tonny, Kiyota, Seiichiro, Katysheva, Nataly, Shugarov, Sergey Yu., Zubareva, Alexandra M., Antipin, Sergei, Ikonnikova, Natalia, Belinski, Alexandr, Dubovsky, Pavol A., Medulka, Tomáš, Takahashi, Jun, Takayama, Masaki, Ohshima, Tomohito, Saito, Tomoki, Tozuka, Miyako, Sako, Shigeyuki, Tanaka, Masaomi, Tominaga, Nozomu, Horiuchi, Takashi, Hanayama, Hidekazu, Reichart, Daniel E., Kouprianov, Vladimir V., Davidson Jr, James W., Caton, Daniel B., Romanov, Filipp D., Lane, David J., Hambsch, Franz-josef, Narita, Norio, Fukui, Akihiko, Ikoma, Masahiro, Tamura, Motohide, Kawabata, Koji S., Nakaoka, Tatsuya, Imazawa, Ryo
We present a detailed study of the MASTER OT J030227.28+191754.5 outburst in 2021-2022, reaching an amplitude of 10.2 mag and a duration of 60 d. The detections of (1) the double-peaked optical emission lines, and (2) the early and ordinary superhump
Externí odkaz:
http://arxiv.org/abs/2408.13783
Autor:
Kuźmicz, Agnieszka, Goyal, Arti, Zola, Stanisław, Jamrozy, Marek, Dróżdż, Marek, Ogłoza, Waldemar, Siwak, Michał, Reichart, Daniel E., Kouprianov, Vladimir V., Caton, Daniel B.
We characterize the optical variability properties of eight lobe-dominated radio quasars (QSOs): B2 0709$+$37, FBQS J095206.3$+$235245, PG 1004$+$130, [HB89] 1156$+$631, [HB89] 1425$+$267, [HB89] 1503$+$691, [HB89] 1721$+$343, 4C $+$74.26, systematic
Externí odkaz:
http://arxiv.org/abs/2210.04058
Autor:
Laine, Seppo, Dey, Lankeswar, Valtonen, Mauri, Gopakumar, A., Zola, Stanislaw, Komossa, S., Kidger, Mark, Pihajoki, Pauli, Gómez, Jose L., Caton, Daniel, Ciprini, Stefano, Drozdz, Marek, Gazeas, Kosmas, Godunova, Vira, Haque, Shirin, Hildebrandt, Felix, Hudec, Rene, Jermak, Helen, Kong, Albert K. H., Lehto, Harry, Liakos, Alexios, Matsumoto, Katsura, Mugrauer, Markus, Pursimo, Tapio, Reichart, Daniel E., Simon, Andrii, Siwak, Michal, Sonbas, Eda
Binary black hole (BH) central engine description for the unique blazar OJ 287 predicted that the next secondary BH impact-induced bremsstrahlung flare should peak on 2019 July 31. This prediction was based on detailed general relativistic modeling o
Externí odkaz:
http://arxiv.org/abs/2004.13392
Autor:
Tucker, Michael A., Fleming, Scott W., Pelisoli, Ingrid, Romero, Alejandra, Bell, Keaton J., Kepler, S. O., Caton, Daniel B., Debes, John, Montgomery, Michael H., Thompson, Susan E., Koester, Detlev, Million, Chase, Shiao, Bernie
We present results from a search for short time-scale white dwarf variability using \texttt{gPhoton}, a time-tagged database of \textit{GALEX} photon events and associated software package. We conducted a survey of $320$ white dwarf stars in the McCo
Externí odkaz:
http://arxiv.org/abs/1712.07146
Autor:
Caton, Daniel, Gentry, Davis R., Samec, Ronald G., Chamberlain, Heather, Robb, Russell, Faulkner, Danny R., Hill, Robert
Publikováno v:
Publications of the Astronomical Society of the Pacific, 2019 May 01. 131(999), 1-14.
Externí odkaz:
https://www.jstor.org/stable/26660751
Autor:
Reed, Phillip A., McCluskey, Jr., George E., Kondo, Yoji, Sahade, Jorge, Guinan, Edward F., Giménez, Alvaro, Caton, Daniel B., Reichart, Daniel E., Ivarsen, Kevin M., Nysewander, Melissa C.
The eclipsing and strongly interacting binary star system R Arae (HD149730) is in a very active and very short-lived stage of its evolution. R Ara consists of a B9V primary and an unknown secondary. We have collected the International Ultraviolet Exp
Externí odkaz:
http://arxiv.org/abs/0909.4047
Spectroscopic measurements of Mira variable stars, as a function of phase, probe the stellar atmospheres and underlying pulsation mechanisms. For example, measuring variations in TiO, VO, and ZrO with phase can be used to help determine whether these
Externí odkaz:
http://arxiv.org/abs/astro-ph/0007380
Autor:
Caton, Daniel B., Samec, Ronald G., Robb, Russell, Faulkner, Danny R., Van Hamme, Walter, Clark, Jimmy D., Shebs, Travis
Publikováno v:
Publications of the Astronomical Society of the Pacific, 2017 Jun 01. 129(976), 1-15.
Externí odkaz:
https://www.jstor.org/stable/26660126
Publikováno v:
Publications of the Astronomical Society of the Pacific, 2016 May 01. 128(963), 1-21.
Externí odkaz:
https://www.jstor.org/stable/26659952
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