Zobrazeno 1 - 10
of 112
pro vyhledávání: '"Kleinman, Scot J."'
Autor:
Uzundag, Murat, De Gerónimo, Francisco C., Córsico, Alejandro H., Silvotti, Roberto, Bradley, Paul A., Montgomery, Michael H., Catelan, Márcio, Toloza, Odette, Bell, Keaton J., Kepler, S. O., Althaus, Leandro G., Kleinman, Scot J., Kilic, Mukremin, Mullally, Susan E., Gänsicke, Boris T., Bąkowska, Karolina, Barber, Sam, Nitta, Atsuko
G\,29$-$38 (TIC~422526868) is one of the brightest ($V=13.1$) and closest ($d = 17.51$\,pc) pulsating white dwarfs with a hydrogen-rich atmosphere (DAV/ZZ Ceti class). It was observed by the {\sl TESS} spacecraft in sectors 42 and 56. The atmosphere
Externí odkaz:
http://arxiv.org/abs/2309.04809
Autor:
Kepler, S. O., Pelisoli, Ingrid, Koester, Detlev, Ourique, Gustavo, Romero, Alejandra Daniela, Reindl, Nicole, Kleinman, Scot J., Eisenstein, Daniel J., Valois, A. Dean M., Amaral, Larissa A.
We report the discovery of 6576 new spectroscopically confirmed white dwarf and subdwarf stars in the Sloan Digital Sky Survey Data Release 12. We obtain Teff, log g and mass for hydrogen atmosphere white dwarf stars (DAs) and helium atmosphere white
Externí odkaz:
http://arxiv.org/abs/1510.08409
Autor:
Kepler, S. O., Pelisoli, Ingrid, Koester, Detlev, Ourique, Gustavo, Kleinman, Scot J., Romero, Alejandra Daniela, Nitta, Atsuko, Eisenstein, Daniel J., Costa, José Eduardo da Silveira, Külebi, Baybars, Jordan, Stefan, Dufour, Patrick, Giommi, Paolo, Rebassa-Mansergas, Alberto
We report the discovery of 9 089 new spectroscopically confirmed white dwarfs and subdwarfs in the Sloan Digital Sky Survey Data Release 10. We obtain Teff, log g and mass for hydrogen atmosphere white dwarf stars (DAs) and helium atmosphere white dw
Externí odkaz:
http://arxiv.org/abs/1411.4149
Akademický článek
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Autor:
Kepler, S. O., Pelisoli, Ingrid, Jordan, Stefan, Kleinman, Scot J., Kulebi, Baybars, Koester, Detlev, Peçanha, Viviane, Castanheira, Bárbara G., Nitta, Atsuko, Costa, José Eduardo da Silveira, Winget, Don Earl, Kanaan, Antonio, Fraga, Luciano
To obtain a better statistics on the occurrence of magnetism among white dwarfs, we searched the spectra of the hydrogen atmosphere white dwarf stars (DAs) in the Data Release 7 of the Sloan Digital Sky Survey (SDSS) for Zeeman splittings and estimat
Externí odkaz:
http://arxiv.org/abs/1211.5709
Autor:
Uzundag, Murat, De Gerónimo, Francisco C, Córsico, Alejandro H, Silvotti, Roberto, Bradley, Paul A, Montgomery, Michael H, Catelan, Márcio, Toloza, Odette, Bell, Keaton J, Kepler, S O, Althaus, Leandro G, Kleinman, Scot J, Kilic, Mukremin, Mullally, Susan E, Gänsicke, Boris T, Bąkowska, Karolina, Barber, Sam, Nitta, Atsuko
Publikováno v:
Monthly Notices of the Royal Astronomical Society; Dec2023, Vol. 526 Issue 2, p2846-2862, 17p
Autor:
Raymond, Sean N., Fraser, Oliver J., Garg, Arti, Hawley, Suzanne L., Jedicke, Robert, Miknaitis, Gajus, Quinn, Thomas, Rockosi, Constance M., Stubbs, Christopher W., Anderson, Scott F., Hogan, Craig J., Ivezic, Zeljko, Lupton, Robert H., West, Andrew A., Brewington, Howard, Brinkmann, J., Harvanek, Michael, Kleinman, Scot J., Krzesinski, Jurek, Long, Dan, Neilsen, Eric H., Newman, Peter R., Nitta, Atsuko, Snedden, Stephanie A.
Publikováno v:
Astron.J.127:2978-2987,2004
We present a detailed observational strategy for finding Near Earth Objects (NEOs) with the Sloan Digital Sky Survey (SDSS) telescope. We investigate strategies in normal, unbinned mode as well as binning the CCDs 2x2 or 3x3, which affects the sky co
Externí odkaz:
http://arxiv.org/abs/astro-ph/0401438
Autor:
Goto, Tomotsugu, Okamura, Sadanori, Sekiguchi, Maki, Bernardi, Mariangela, Brinkmann, Jon., Gomez, Percy L., Harvanek, Michael, Kleinman, Scot. J., Krzesinski, Jurek, Long, Dan, Loveday, Jon, Miller, Christopher J., Neilsen, Eric H., Newman, Peter R., Nitta, Atsuko, Sheth, Ravi K., Snedden, Stephanie A., Yamauchi, Chisato
Publikováno v:
Publ.Astron.Soc.Jap.55:757,2003
In previous work on galaxy clusters, several authors reported a discovery of an unusual population of galaxies, which have spiral morphologies, but do not show any star formation activity. These galaxies are called ``passive spirals'', and have been
Externí odkaz:
http://arxiv.org/abs/astro-ph/0301303
Akademický článek
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Autor:
Adler, David S., Seaman, Robert L., Benn, Chris R., Kim, Hwihyun, Peck, Alison B., Diaz, Ruben J., Adamson, Andrew J., Kleinman, Scot J.
Publikováno v:
Proceedings of SPIE; August 2022, Vol. 12186 Issue: 1 p121861C-121861C-5, 1096755p