Zobrazeno 1 - 10
of 100
pro vyhledávání: '"Kurtz, Dw"'
Autor:
Miglio, A, Chiappini, C, Mosser, B, Davies, GR, Freeman, K, Girardi, L, Jofré, P, Kawata, D, Rendle, BM, Valentini, M, Casagrande, L, Chaplin, WJ, Gilmore, G, Hawkins, K, Holl, B, Appourchaux, T, Belkacem, K, Bossini, D, Brogaard, K, Goupil, MJ, Montalbán, J, Noels, A, Anders, F, Rodrigues, T, Piotto, G, Pollacco, D, Rauer, H, Prieto, CA, Avelino, PP, Babusiaux, C, Barban, C, Barbuy, B, Basu, S, Baudin, F, Benomar, O, Bienaymé, O, Binney, J, Bland-Hawthorn, J, Bressan, A, Cacciari, C, Campante, TL, Cassisi, S, Christensen-Dalsgaard, J, Combes, F, Creevey, O, Cunha, MS, Jong, RS, Laverny, P, Degl'Innocenti, S, Deheuvels, S, Depagne, Ridder, J, Matteo, PD, Mauro, MPD, Dupret, MA, Eggenberger, P, Elsworth, Y, Famaey, B, Feltzing, S, García, RA, Gerhard, O, Gibson, BK, Gizon, L, Haywood, M, Handberg, R, Heiter, U, Hekker, S, Huber, D, Ibata, R, Katz, D, Kawaler, SD, Kjeldsen, H, Kurtz, DW, Lagarde, N, Lebreton, Y, Lund, MN, Majewski, Marigo, P
Deciphering the assembly history of the Milky Way is a formidable task, which becomes possible only if one can produce high-resolution chrono-chemo-kinematical maps of the Galaxy. Data from large-scale astrometric and spectroscopic surveys will soon
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cac8ef8d9ad3e18fc7d1d9a6eabd4f3c
https://www.repository.cam.ac.uk/handle/1810/269656
https://www.repository.cam.ac.uk/handle/1810/269656
Publikováno v:
EPJ Web of Conferences, Vol 101, p 06013 (2015)
The δ Sct star KIC 7106205 showed amplitude modulation in a single p mode, whilst all other p and g modes remained stable in amplitude and phase over 1470 d of the Kepler dataset. The data were divided into 30 time bins of equal length and a series
Autor:
Çelik, L, Ekmekçi, F, Nemec, J, Kolenberg, Katrien, Benkö, JM, Szabó, R, Kurtz, DW, Kinemuchi, K, Senavci, HC
One of the most challenging difficulties that precedes the frequency analysis of Kepler data for a Blazhko star is stitching together the data from different seasons (quarters). We discuss the preliminary steps in the stitching, detrending and rescal
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______1131::da56a8e2feaa09ba49fbf7f30ccfdab4
https://lirias.kuleuven.be/handle/123456789/493607
https://lirias.kuleuven.be/handle/123456789/493607
Autor:
Catanzaro, Giovanni, Ripepi, V, Bernabei, S, Marconi, M, Balona, L, Kurtz, Dw, Smalley, B, Borucki, Wj, Bruntt, H, Christensen Dalsgaard, J, Grigahcene, A, Kjeldsen, H, Koch, Dg, Monteiro, Mjpfg, Suarez, Jc, Szabo, R, Uytterhoeven, K.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______4731::370843963d3d6794b2b93f5fe421f518
http://hdl.handle.net/20.500.11769/251637
http://hdl.handle.net/20.500.11769/251637
Autor:
Breger, M, Balona, L, Lenz, P, Hollek, Jk, Kurtz, Dw, Catanzaro, Giovanni, Marconi, M, Pamyatnykh, Aa, Smalley, B, Suarez, Jc, Szabo, R, Uytterhoeven, K, Ripepi, V, Christensen Dalsgaard, J, Kjeldsen, H, Fanelli, Mn, Ibrahim, Ka, Uddin, K.
In the faint star KIC 9700322 observed by the Kepler satellite, 76 frequencies with amplitudes from 14 to 29000 ppm were detected. The two dominant frequencies at 9.79 and 12.57 c/d (113.3 and 145.5 \mu Hz), interpreted to be radial modes, are accomp
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::19ad39b620194e0f7acec71605be4b9a
http://arxiv.org/abs/1012.4373
http://arxiv.org/abs/1012.4373
Autor:
Grigahcene, A, Uytterhoeven, K, Antoci, V, Balona, L, Catanzaro, Giovanni, Daszynska Daszkiewicz, J, Guzik, Ja, Handler, G, Houdek, G, Kurtz, Dw, Marconi, M, Monteiro, Mjpfg, Moya, A, Ripepi, V, Suarez, Jc, Borucki, Wj, Brown, Tm, Christensen Dalsgaard, J, Gilliland, Rl, Jenkins, Jm, Kjeldsen, H, Koch, D, Bernabei, S, Bradley, P, Breger, M, Di Criscienzo, M, Dupret, Ma, Garcia, Ra, Hernandez, Ag, Jackiewicz, J, Kaiser, A, Lehmann, H, Martin Ruiz, S, Mathias, P, Molenda Zakowicz, J, Nemec, Jm, Nuspl, J, Paparo, M, Roth, M, Szabo, R, Suran, Md, Ventura, R.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______4731::440c7da90642fe3ce1ee5f7ebd132be5
http://hdl.handle.net/20.500.11769/239968
http://hdl.handle.net/20.500.11769/239968
Autor:
Kolenberg, Katrien, Bryson, S, Szabo, R, Kurtz, DW, Smolec, R, Nemec, JM, Guggenberger, E, Moskalik, P, Benko, JM, Chadid, M, Jeon, Y-B, Kiss, LL, Kopacki, G, Nuspl, J, Still, M, Christensen-Dalsgaard, J, Kjeldsen, H, Borucki, WJ, Caldwell, DA, Jenkins, JM, Koch, D
Publikováno v:
Kolenberg, K, Bryson, S, Szabó, R, Kurtz, D W, Smolec, R, Nemec, J M, Guggenberger, E, Moskalik, P, Benkö, J M, Chadid, M, Jeon, Y-B, Kiss, L L, Kopacki, G, Nuspl, J, Still, M, Christensen-Dalsgaard, J, Kjeldsen, H, Borucki, W J, Caldwell, D A, Jenkins, J M & Koch, D 2011, ' Kepler photometry of the prototypical Blazhko star RR Lyr: an old friend seen in a new light ', Royal Astronomical Society. Monthly Notices, vol. 411, no. 2, pp. 878-890 . https://doi.org/10.1111/j.1365-2966.2010.17728.x
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2011, 411,2, pp.878-890. ⟨10.1111/j.1365-2966.2010.17728.x⟩
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2011, 411,2, pp.878-890. ⟨10.1111/j.1365-2966.2010.17728.x⟩
We present our analysis of the long cadence Kepler data for the well-studied Blazhko star RR Lyr, gathered during the first two quarters of the satellite's observations and covering a total of 127d. Besides being of great importance for our understan
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e7187253938bb14823ce9b070aac71c3
Autor:
Grigahcene, A, Antoci, V, Balona, L, Catanzaro, Giovanni, Daszynska Daszkiewicz, J, Guzik, Ja, Handler, G, Houdek, G, Kurtz, Dw, Marconi, M, Monteiro, Mjpfg, Moya, A, Ripepi, V, Suarez, Jc, Uytterhoeven, K, Borucki, Wj, Brown, Tm, Christensen Dalsgaard, J, Gilliland, Rl, Jenkins, Jm, Kjeldsen, H, Koch, D, Bernabei, S, Bradley, P, Breger, M, Di Criscienzo, M, Dupret, Ma, Garcia, Ra, Hernandez, Ag, Jackiewicz, J, Kaiser, A, Lehmann, H, Martin Ruiz, S, Mathias, P, Molenda Zakowicz, J, Nemec, Jm, Nuspl, J, Paparo, M, Roth, M, Szabo, R, Suran, Md, Ventura, R.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______4731::d5ceda529c077a530f3158b7c01bdc2e
http://hdl.handle.net/20.500.11769/243719
http://hdl.handle.net/20.500.11769/243719
Autor:
García, RA, Nemec, JM, Balona, LA, Kinemuchi, K, Murphy, SJ, Jeon, Y-B, Kurtz, DW, Pigulski, A, Ballot, J
Publikováno v:
EPJ Web of Conferences, Vol 101, p 06049 (2015)
High-resolution spectroscopic observations have been made for 32 of the 34 candidate SX Phe stars identified in the Kepler field by Balona & Nemec (2012). All available long- and short-cadence Q0-Q17 Kepler photometry has been analyzed for the 34 c