Zobrazeno 1 - 10
of 23
pro vyhledávání: '"Günther MN"'
Autor:
Bryant, EM, Bayliss, D, Nielsen, LD, Veras, D, Acton, JS, Anderson, DR, Armstrong, DJ, Bouchy, F, Briegal, JT, Burleigh, MR, Cabrera, J, Casewell, SL, Chaushev, A, Cooke, BF, Csizmadia, S, Eigmüller, P, Erikson, A, Gill, S, Gillen, E, Goad, MR, Grieves, N, Günther, MN, Henderson, B, Hogan, A, Jenkins, JS, Lendl, M, McCormac, J, Moyano, M, Queloz, D, Rauer, H, Raynard, L, Smith, AMS, Tilbrook, RH, Udry, S, Vines, JI, Watson, CA, West, RG, Wheatley, PJ
We report the discovery of the transiting exoplanet NGTS-12b by the Next Generation Transit Survey (NGTS). The host star, NGTS-12, is a V=12.38 mag star with an effective temperature of T$_{\rm eff}$=$5690\pm130$ K. NGTS-12b orbits with a period of $
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::bc00ee288a9b407be8aa5f7c6ea285a1
Autor:
Sebastian, D, Pedersen, PP, Murray, CA, Ducrot, E, Garcia, LJ, Burdanov, A, Pozuelos, FJ, Delrez, L, Wells, R, Dransfield, G, Gillon, M, Demory, BO, Queloz, D, Triaud, AHMJ, De Witt, J, Jehin, E, Gómez Maqueo Chew, Y, Günther, MN, Niraula, P, Rackham, BV, Schanche, N, Sohy, S, Thompson, S
SPECULOOS (Search for habitable Planets EClipsing ULtra-cOOl Stars) aims to perform a transit search on the nearest ($
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::867926116f435f4845d54c88f2ab6d4a
Autor:
Grieves, N, Nielsen, LD, Vines, JI, Bryant, EM, Gill, S, Bouchy, F, Lendl, M, Bayliss, D, Eigmueller, P, Segransan, D, Acton, JS, Anderson, DR, Burleigh, MR, Casewell, SL, Chaushev, A, Cooke, BF, Gillen, E, Goad, MR, Günther, MN, Henderson, BA, Hogan, A, Jenkins, JS, Alves, DR, Jordán, A, McCormac, J, Moyano, M, Queloz, D, Raynard, L, Seidel, JV, Smith, AMS, Tilbrook, RH, Udry, S, West, RG, Wheatley, PJ
We report the discovery of the massive hot Jupiter NGTS-13b by the Next Generation Transit Survey (NGTS). The V = 12.7 host star is likely in the subgiant evolutionary phase with log g$_{*}$ = 4.04 $\pm$ 0.05, T$_{eff}$ = 5819 $\pm$ 73 K, M$_{*}$ = 1
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1e952bd6ebb0f5185dc953a655449038
Autor:
Jenkins, JS, Díaz, MR, Kurtovic, NT, Espinoza, N, Vines, JI, Rojas, PAP, Brahm, R, Torres, P, Cortés-Zuleta, P, Soto, MG, Lopez, ED, King, GW, Wheatley, PJ, Winn, JN, Ciardi, DR, Ricker, G, Vanderspek, R, Latham, DW, Seager, S, Jenkins, JM, Beichman, CA, Bieryla, A, Burke, CJ, Christiansen, JL, Henze, CE, Klaus, TC, McCauliff, S, Mori, M, Narita, N, Nishiumi, T, Tamura, M, De Leon, JP, Quinn, SN, Villaseñor, JN, Vezie, M, Lissauer, JJ, Collins, KA, Collins, KI, Isopi, G, Mallia, F, Ercolino, A, Petrovich, C, Jordán, A, Acton, JS, Armstrong, DJ, Bayliss, D, Bouchy, F, Belardi, C, Bryant, EM, Burleigh, MR, Cabrera, J, Casewell, SL, Chaushev, A, Cooke, BF, Eigmüller, P, Erikson, A, Foxell, E, Gänsicke, BT, Gill, S, Gillen, E, Günther, MN, Goad, MR, Hooton, MJ, Jackman, JAG, Louden, T, McCormac, J, Moyano, M, Nielsen, LD, Pollacco, D, Queloz, D, Rauer, H, Raynard, L, Smith, AMS, Tilbrook, RH, Titz-Weider, R, Turner, O, Udry, S, Walker, Watson, CA, West, RG, Palle, E, Ziegler, C, Law, N, Mann, AW
About one out of 200 Sun-like stars has a planet with an orbital period shorter than one day: an ultra-short-period planet (Sanchis-ojeda et al. 2014; Winn et al. 2018). All of the previously known ultra-short-period planets are either hot Jupiters,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::2d8e03a0751428daa54fe9ab2146ed07
Autor:
Ducrot, E, Gillon, M, Delrez, L, Agol, E, Rimmer, P, Turbet, M, Günther, MN, Demory, BO, Triaud, AHMJ, Bolmont, E, Burgasser, A, Carey, SJ, Ingalls, JG, Jehin, E, Leconte, J, Lederer, SM, Queloz, D, Raymond, SN, Selsis, F, Van Grootel, V, De Wit, J
With more than 1000 hours of observation from Feb 2016 to Oct 2019, the Spitzer Exploration Program Red Worlds (ID: 13067, 13175 and 14223) exclusively targeted TRAPPIST-1, a nearby (12pc) ultracool dwarf star orbited by seven transiting Earth-sized
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e4d0d18be43c9e79717a7c578888f587
Autor:
Wheatley, PJ, West, RG, Goad, MR, Jenkins, JS, Pollacco, DL, Queloz, D, Rauer, H, Udry, S, Watson, CA, Chazelas, B, Eigmüller, P, Lambert, G, Genolet, L, McCormac, J, Walker, S, Armstrong, DJ, Bayliss, D, Bento, J, Bouchy, F, Burleigh, MR, Cabrera, J, Casewell, SL, Chaushev, A, Chote, P, Csizmadia, S, Erikson, A, Faedi, F, Foxell, E, Gänsicke, BT, Gillen, E, Grange, A, Günther, MN, Hodgkin, ST, Jackman, J, Jordán, A, Louden, T, Metrailler, L, Moyano, M, Nielsen, LD, Osborn, HP, Poppenhaeger, K, Raddi, R, Raynard, L, Smith, AMS, Soto, M, Titz-Weider, R
© 2017 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society. We describe the Next Generation Transit Survey (NGTS), which is a ground-based project searching for transiting exoplanets orbiting bright stars.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c4166309cca9f105377381d857a279a0
Autor:
Eigmüller, P, Chaushev, A, Gillen, E, Smith, A, Nielsen, LD, Turner, O, Csizmadia, S, Smalley, B, Bayliss, D, Belardi, C, Bouchy, F, Burleigh, MR, Cabrera, J, Casewell, SL, Chazelas, B, Cooke, BF, Erikson, A, Gänsicke, BT, Günther, MN, Goad, MR, Grange, A, Jackman, JAG, Jenkins, JS, McCormac, J, Moyano, M, Pollacco, D, Poppenhaeger, K, Queloz, D, Raynard, L, Rauer, H, Udry, S, Walker, Watson, CA, West, RG, Wheatley, PJ
Context: Planetary population analysis gives us insight into formation and evolution processes. For short-period planets, the subJovian desert has been discussed in recent years with regard to the planet population in the mass/period and radius/perio
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3f99ced2a93bd597a390d4263d03d9cf
Autor:
Murray, CA, Delrez, L, Pedersen, PP, Queloz, D, Gillon, M, Burdanov, A, Ducrot, E, Garcia, LJ, Lienhard, F, Demory, BO, Jehin, E, McCormac, J, Sebastian, D, Sohy, S, Thompson, SJ, Triaud, AHMJ, Grootel, Günther, MN, Huang, CX
SPECULOOS-South, an observatory composed of four independent 1m robotic telescopes, located at ESO Paranal, Chile, started scientific operation in January 2019. This Southern Hemisphere facility operates as part of SPECULOOS, an international network
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::6b907347fba7c9ae44875a6ffc2ca629
Autor:
Tilbrook, RH, Burleigh, MR, Costes, JC, Gill, S, Nielsen, LD, Vines, JI, Queloz, D, Hodgkin, ST, Worters, HL, Goad, MR, Acton, JS, Henderson, BA, Armstrong, DJ, Anderson, DR, Bayliss, D, Bouchy, F, Briegal, JT, Bryant, EM, Casewell, SL, Chaushev, A, Cooke, BF, Eigmüller, P, Gillen, E, Günther, MN, Hogan, A, Jenkins, JS, Lendl, M, McCormac, J, Moyano, M, Raynard, L, Smith, AMS, Udry, S, Watson, CA, West, RG, Wheatley, PJ, Breytenbach, H, Sefako, RR, Thomas, JK, Alves, DR
We report the discovery of four new hot Jupiters with the Next Generation Transit Survey (NGTS). NGTS-15b, NGTS-16b, NGTS-17b, and NGTS-18b are short-period ($P
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::dfe20c4c57b22ddccae47994ca92c9ad
Autor:
Costes, JC, Watson, CA, De Mooij, E, Saar, SH, Dumusque, X, Cameron, C, Phillips, DF, Günther, MN, Jenkins, JS, Mortier, A, Thompson, APG
Long-term stellar activity variations can affect the detectability of long-period and Earth-analogue extrasolar planets. We have, for 54 stars, analysed the long-term trend of five activity indicators: log$R'_\mathrm{{HK}}$, the cross-correlation fun
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::18813dcbc2212a827478f5714d12f99f