Zobrazeno 1 - 10
of 57
pro vyhledávání: '"Krzesiński, Jurek"'
Autor:
Uzundag, Murat, Krzesinski, Jurek, Pelisoli, Ingrid, Nemeth, Peter, Silvotti, Roberto, Dawson, Maja Vuckovic Harry, Geier, Stephan
Hot subdwarf B (sdB) stars are evolved, subluminous, helium-burning stars, most likely formed when red-giant stars lose their hydrogen envelope via interactions with close companions. They play an important role in our understanding of binary evoluti
Externí odkaz:
http://arxiv.org/abs/2401.17707
Akademický článek
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Autor:
Berry, Michael, Ivezić, Željko, Sesar, Branimir, Jurić, Mario, Schlafly, Edward F., Bellovary, Jillian, Finkbeiner, Douglas, Vrbanec, Dijana, Beers, Timothy C., Brooks, Keira J., Schneider, Donald P., Gibson, Robert R., Kimball, Amy, Jones, Lynne, Yoachim, Peter, Krughoff, Simon, Connolly, Andrew J., Loebman, Sarah, Bond, Nicholas A., Schlegel, David, Dalcanton, Julianne, Yanny, Brian, Majewski, Steven R., Knapp, Gillian R., Gunn, James E., Smith, J. Allyn, Fukugita, Masataka, Kent, Steve, Barentine, John, Krzesinski, Jurek, Long, Dan
We use SDSS photometry of 73 million stars to simultaneously obtain best-fit main-sequence stellar energy distribution (SED) and amount of dust extinction along the line of sight towards each star. Using a subsample of 23 million stars with 2MASS pho
Externí odkaz:
http://arxiv.org/abs/1111.4985
Autor:
Doi, Mamoru, Tanaka, Masayuki, Fukugita, Masataka, Gunn, James E., Yasuda, Naoki, Ivezic, Zeljko, Brinkmann, Jon, de Haars, Ernst, Kleinman, Scott J., Krzesinski, Jurek, Leger, R. French
The monochromatic illumination system is constructed to carry out in situ measurements of the response function of the mosaicked CCD imager used in the Sloan Digital Sky Survey (SDSS). The system is outlined and the results of the measurements, mostl
Externí odkaz:
http://arxiv.org/abs/1002.3701
Autor:
Ivezic, Zeljko, Sesar, Branimir, Juric, Mario, Bond, Nicholas, Dalcanton, Julianne, Rockosi, Constance M., Yanny, Brian, Newberg, Heidi J., Beers, Timothy C., Prieto, Carlos Allende, Wilhelm, Ron, Lee, Young Sun, Sivarani, Thirupathi, Norris, John E., Bailer-Jones, Coryn A. L., Fiorentin, Paola Re, Schlegel, David, Uomoto, Alan, Lupton, Robert H., Knapp, Gillian R., Gunn, James E., Covey, Kevin R., Smith, J. Allyn, Miknaitis, Gajus, Doi, Mamoru, Tanaka, Masayuki, Fukugita, Masataka, Kent, Steve, Finkbeiner, Douglas, Munn, Jeffrey A., Pier, Jeffrey R., Quinn, Tom, Hawley, Suzanne, Anderson, Scott, Kiuchi, Furea, Chen, Alex, Bushong, James, Sohi, Harkirat, Haggard, Daryl, Kimball, Amy, Barentine, John, Brewington, Howard, Harvanek, Mike, Kleinman, Scott, Krzesinski, Jurek, Long, Dan, Nitta, Atsuko, Snedden, Stephanie, Lee, Brian, Harris, Hugh, Brinkmann, Jonathan, Schneider, Donald P., York, Donald G.
Publikováno v:
Astrophys.J.684:287-325,2008
Using effective temperature and metallicity derived from SDSS spectra for ~60,000 F and G type main sequence stars (0.2
Externí odkaz:
http://arxiv.org/abs/0804.3850
Autor:
Zheng, Chen, Romani, Roger W., Sako, Masao, Marriner, John, Bassett, Bruce, Becker, Andrew, Choi, Changsu, Cinabro, David, DeJongh, Fritz, Depoy, Darren L., Dilday, Ben, Doi, Mamoru, Frieman, Joshua A., Garnavich, Peter M., Hogan, Craig J., Holtzman, Jon, Im, Myungshin, Jha, Saurabh, Kessler, Richard, Konishi, Kohki, Lampeitl, Hubert, Marshall, Jennifer L., McGinnis, David, Miknaitis, Gajus, Nichol, Robert C., Prieto, Jose Luis, Riess, Adam G., Richmond, Michael W., Schneider, Donald P., Smith, Mathew, Takanashi, Naohiro, Tokita, Kouichi, van der Heyden, Kurt, Yasuda, Naoki, Assef, Roberto J., Barentine, John, Bender, Ralf, Blandford, Roger D., Bremer, Malcolm, Brewington, Howard, Collins, Chris A., Crotts, Arlin, Dembicky, Jack, Eastman, Jason, Edge, Alastair, Elson, Ed, Eyler, Michael E., Filippenko, Alexei V., Foley, Ryan J., Frank, Stephan, Goobar, Ariel, Harvanek, Michael, Hopp, Ulrich, Ihara, Yutaka, Kahn, Steven, Ketzeback, William, Kleinman, Scott J., Kollatschny, Wolfram, Krzesiński, Jurek, Leloudas, Giorgos, Long, Daniel C., Lucey, John, Malanushenko, Elena, Malanushenko, Viktor, McMillan, Russet J., Morgan, Christopher W., Morokuma, Tomoki, Nitta, Atsuko, Ostman, Linda, Pan, Kaike, Romer, A. Kathy, Saurage, Gabrelle, Schlesinger, Katie, Snedden, Stephanie A., Sollerman, Jesper, Stritzinger, Maximilian, Watson, Linda C., Watters, Shannon, Wheeler, J. Craig, York, Donald
Publikováno v:
Astron.J.135:1766-1784,2008
This paper presents spectroscopy of supernovae discovered in the first season of the Sloan Digital Sky Survey-II Supernova Survey. This program searches for and measures multi-band light curves of supernovae in the redshift range z = 0.05 - 0.4, comp
Externí odkaz:
http://arxiv.org/abs/0802.3220
Autor:
Schneider, Donald P., Hall, Patrick B., Richards, Gordon T., Strauss, Michael A., Berk, Daniel E. Vanden, Anderson, Scott F., Brandt, W. N., Fan, Xiaohui, Jester, Sebastian, Gray, Jim, Gunn, James E., SubbaRao, Mark U., Thakar, Anirudda R., Stoughton, Chris, Szalay, Alexander S., Yanny, Brian, York, Donald G., Bahcall, Neta A., Barentine, J., Blanton, Michael R., Brewington, Howard, Brinkmann, J., Brunner, Robert J., Castander, Francisco J., Csabai, Istvan, Frieman, Joshua A., Fukugita, Masataka, Harvanek, Michael, Hogg, David W., Ivezic, Zeljko, Kent, Stephen M., Kleinman, S. J., Knapp, G. R., Kron, Richard G., Krzesinski, Jurek, Long, Daniel C., Lupton, Robert H., Nitta, Atsuko, Pier, Jeffrey R., Saxe, David H., Shen, Yue, Snedden, Stephanie A., Weinberg, David H., Wu, Jian
Publikováno v:
Astron.J.134:102-117,2007
We present the fourth edition of the Sloan Digital Sky Survey (SDSS) Quasar Catalog. The catalog contains 77,429 objects; this is an increase of over 30,000 entries since the previous edition. The catalog consists of the objects in the SDSS Fifth Dat
Externí odkaz:
http://arxiv.org/abs/0704.0806
Autor:
Eisenstein, Daniel J., Liebert, James, Koester, Detlev, Kleinmann, S. J., Nitta, Atsuko, Smith, Paul S., Barentine, J. C., Brewington, Howard J., Brinkmann, J., Harvanek, Michael, Krzesinski, Jurek, Neilsen Jr., Eric H., Long, Dan, Schneider, Donald P., Snedden, Stephanie A.
Publikováno v:
Astron.J.132:676-691,2006
We present ugriz photometry and optical spectroscopy for 28 DB and DO white dwarfs with temperatures between 28,000K and 45,000K. About 10 of these are particularly well-observed; the remainder are candidates. These are the hottest DB stars yet found
Externí odkaz:
http://arxiv.org/abs/astro-ph/0606702
Autor:
Eisenstein, Daniel J., Liebert, James, Harris, Hugh C., Kleinmann, S. J., Nitta, Atsuko, Silvestri, Nicole, Anderson, Scott A., Barentine, J. C., Brewington, Howard J., Brinkmann, J., Harvanek, Michael, Krzesinski, Jurek, Neilsen Jr., Eric H., Long, Dan, Schneider, Donald P., Snedden, Stephanie A.
Publikováno v:
Astrophys.J.Suppl.167:40-58,2006
We present a catalog of 9316 spectroscopically confirmed white dwarfs from the Sloan Digital Sky Survey Data Release 4. We have selected the stars through photometric cuts and spectroscopic modeling, backed up by a set of visual inspections. Roughly
Externí odkaz:
http://arxiv.org/abs/astro-ph/0606700
Autor:
Zucker, Daniel B., Kniazev, Alexei Y., Martinez-Delgado, David, Bell, Eric F., Rix, Hans-Walter, Grebel, Eva K., Holtzman, Jon A., Walterbos, Rene A. M., Rockosi, Constance M., York, Donald G., Barentine, J. C., Brewington, Howard, Brinkmann, J., Harvanek, Michael, Kleinman, S. J., Krzesinski, Jurek, Long, Dan, Neilsen, Jr., Eric H., Nitta, Atsuko, Snedden, Stephanie A.
Publikováno v:
Astrophys.J.659:L21-L24,2007
We report the discovery of Andromeda X, a new dwarf spheroidal satellite of M31, based on stellar photometry from the Sloan Digital Sky Survey (SDSS). Using follow-up imaging data we have estimated its distance and other physical properties. We find
Externí odkaz:
http://arxiv.org/abs/astro-ph/0601599