Zobrazeno 1 - 5
of 5
pro vyhledávání: '"Swayne, M. I."'
Autor:
Swayne, M. I., Maxted, P. F. L., Triaud, A. H. M. J., Sousa, S. G., Deline, A., Ehrenreich, D., Hoyer, S., Olofsson, G., Boisse, I., Duck, A., Gill, S., Martin, D., McCormac, J., Persson, C. M., Santerne, A., Sebastian, D., Standing, M. R., Acuña, L., Alibert, Y., Alonso, R., Anglada, G., Bárczy, T., Navascues, D. Barrado, Barros, S. C. C., Baumjohann, W., Baycroft, T. A., Beck, M., Beck, T., Benz, W., Billot, N., Bonfils, X., Borsato, L., Bourrier, V., Brandeker, A., Broeg, C., Carmona, A., Charnoz, S., Cameron, A. Collier, Cortés-Zuleta, P., Csizmadia, Sz., Cubillos, P. E., Davies, M. B., Deleuil, M., Delfosse, X., Delrez, L., Demangeon, O. D. S., Demory, B. -O., Dransfield, G., Erikson, A., Fortier, A., Forveille, T., Fossati, L., Fridlund, M., Gandolfi, D., Gillon, M., Güdel, M., Günther, M. N., Hara, N., Hébrard, G., Heidari, N., Hellier, C., Helling, Ch., Isaak, K. G., Kerschbaum, F., Kiefer, F., Kiss, L. L., Kunovac, V., Lalitha, S., Lam, K. W. F., Laskar, J., Etangs, A. Lecavelier des, Lendl, M., Magrin, D., Marafatto, L., Martioli, E., Miller, N. J., Mordasini, C., Moutou, C., Nascimbeni, V., Ottensamer, R., Pagano, I., Pallé, E., Peter, G., Piazza, D., Piotto, G., Pollacco, D., Queloz, D., Ragazzoni, R., Rando, N., Rauer, H., Ribas, I., Santos, N. C., Scandariato, G., Ségransan, D., Simon, A. E., Smith, A. M. S., Southworth, R., Stalport, M., Szabó, Gy. M., Thomas, N., Udry, S., Ulmer, B., Van Grootel, V., Venturini, J., Walton, N. A., Willett, E., Wilson, T. G.
Observations of low-mass stars have frequently shown a disagreement between observed stellar radii and radii predicted by theoretical stellar structure models. This ``radius inflation'' problem could have an impact on both stellar and exoplanetary sc
Externí odkaz:
http://arxiv.org/abs/2312.11339
Autor:
Sebastian, D., Swayne, M. I., Maxted, P. F. L., Triaud, A. H. M. J., Sousa, S. G., Olofsson, G., Beck, M., Billot, N., Hoyer, S., Gill, S., Heidari, N., Martin, D. V., Persson, C. M., Standing, M. R., Alibert, Y., Alonso, R., Anglada, G., Asquier, J., Bárczy, T., Barrado, D., Barros, S. C. C., Battley, M. P., Baumjohann, W., Beck, T., Benz, W., Bergomi, M., Boisse, I., Bonfils, X., Brandeker, A., Broeg, C., Cabrera, J., Charnoz, S., Cameron, A. Collier, Csizmadia, Sz., Davies, M. B., Deleuil, M., Delrez, L., Demangeon, O. D. S., Demory, B. -O., Dransfield, G., Ehrenreich, D., Erikson, A., Fortier, A., Fossati, L., Fridlund, M., Gandolfi, D., Gillon, M., Güdel, M., Hasiba, J., Hébrard, G., Heng, K., Isaak, K. G., Kiss, L. L., Kopp, E., Kunovac, V., Laskar, J., Etangs, A. Lecavelier des, Lendl, M., Lovis, C., Magrin, D., McCormac, J., Miller, N. J., Nascimbeni, V., Ottensamer, R., Pagano, I., Pallé, E., Pepe, F. A., Peter, G., Piotto, G., Pollacco, D., Queloz, D., Ragazzoni, R., Rando, N., Rauer, H., Ribas, I., Lalitha, S., Santerne, A., Santos, N. C., Scandariato, G., Ségransan, D., Simon, A. E., Smith, A. M. S., Steller, M., Szabó, Gy. M., Thomas, N., Udry, S., Van Grootel, V., Walton, N. A.
Eclipsing binaries are important benchmark objects to test and calibrate stellar structure and evolution models. This is especially true for binaries with a fully convective M-dwarf component for which direct measurements of these stars' masses and r
Externí odkaz:
http://arxiv.org/abs/2209.03128
Autor:
Maxted, P. F. L., Ehrenreich, D., Wilson, T. G., Alibert, Y., Cameron, A. Collier, Hoyer, S., Sousa, S. G., Olofsson, G., Bekkelien, A., Deline, A., Delrez, L., Bonfanti, A., Borsato, L., Alonso, R., Escudé, G. Anglada, Barrado, D., Barros, S. C. C., Baumjohann, W., Beck, M., Beck, T., Benz, W., Billot, N., Biondi, F., Bonfils, X., Brandeker, A., Broeg, C., Bárczy, T., Cabrera, J., Charnoz, S., Van Damme, C. Corral, Csizmadia, Sz., Davies, M. B., Deleuil, M., Demangeon, O. D. S., Demory, B. -O., Erikson, A., Florén, H. G., Fortier, A., Fossati, L., Fridlund, M., Futyan, D., Gandolfi, D., Gillon, M., Guedel, M., Guterman, P., Heng, K., Isaak, K. G., Kiss, L., Laskar, J., Etangs, A. Lecavelier des, Lendl, M., Lovis, C., Magrin, D., Nascimbeni, V., Ottensamer, R., Pagano, I., Pallé, E., Peter, G., Piotto, G., Pollacco, D., Pozuelos, F. J., Queloz, D., Ragazzoni, R., Rando, N., Rauer, H., Reimers, C., Ribas, I., Salmon, S., Santos, N. C., Scandariato, G., Simon, A. E., Smith, A. M. S., Steller, M., Swayne, M. I., Szabó, Gy. M., Ségransan, D., Thomas, N., Udry, S., Van Grootel, V., Walton, N. A.
CHEOPS(CHaracterising ExOPlanet Satellite) is an ESA S-class mission that observes bright stars at high cadence from low-Earth orbit. The main aim of the mission is to characterize exoplanets that transit nearby stars using ultrahigh precision photom
Externí odkaz:
http://arxiv.org/abs/2111.08828
Autor:
Swayne, M. I., Maxted, P. F. L., Triaud, A. H. M. J., Sousa, S. G., Broeg, C., Florén, H. -G., Guterman, P., Simon, A. E., Boisse, I., Bonfanti, A., Martin, D., Santerne, A., Salmon, S., Standing, M. R., Van Grootel, V., Wilson, T. G., Alibert, Y., Alonso, R., Escudé, G. Anglada, Asquier, J., Bárczy, T., Barrado, D., Barros, S. C. C., Battley, M., Baumjohann, W., Beck, M., Beck, T., Bekkelien, A., Benz, W., Billot, N., Bonfils, X., Brandeker, A., Busch, M. -D., Cabrera, J., Charnoz, S., Cameron, A. Collier, Csizmadia, Sz., Davies, M. B., Deleuil, M., Deline, A., Delrez, L., Demangeon, O. D. S., Demory, B. -O., Dransfield, G., Ehrenreich, D., Erikson, A., Fortier, A., Fossati, L., Fridlund, M., Futyan, D., Gandolfi, D., Gillon, M., Guedel, M., Hébrard, G., Heidari, N., Hellier, C., Heng, K., Hobson, M., Hoyer, S., Isaak, K. G., Kiss, L., Hodžić, V. Kunovac, Lalitha, S., Laskar, J., Etangs, A. Lecavelier des, Lendl, M., Lovis, C., Magrin, D., Marafatto, L., McCormac, J., Miller, N., Nascimbeni, V., Olofsson, G., Ottensamer, R., Pagano, I., Pallé, E., Peter, G., Piotto, G., Pollacco, D., Queloz, D., Ragazzoni, R., Rando, N., Rauer, H., Ribas, I., Santos, N. C., Scandariato, G., Ségransan, D., Smith, A. M. S., Steinberger, M., Steller, M., Szabó, Gy. M., Thomas, N., Udry, S., Walter, I., Walton, N. A., Willett, E.
Publikováno v:
MNRAS 506 (2021) 306-322
The accuracy of theoretical mass, radius and effective temperature values for M-dwarf stars is an active topic of debate. Differences between observed and theoretical values have raised the possibility that current theoretical stellar structure and e
Externí odkaz:
http://arxiv.org/abs/2106.07276
Autor:
Maxted, P F L, Miller, N J, Hoyer, S, Adibekyan, V, Sousa, S G, Billot, N, Fortier, A, Simon, A E, Cameron, A Collier, Swayne, M I, Gutermann, P, Triaud, A H M J, Southworth, J, Alibert, Y, Alonso, R, Anglada, G, Bárczy, T, Navascues, D Barrado y, Barros, S C C, Baumjohann, W, Beck, M, Beck, T, Benz, W, Bonfils, X, Brandeker, A, Broeg, C, Buder, M, Cabrera, J, Charnoz, S, van Damme, C Corral, Csizmadia, Sz, Davies, M B, Deleuil, M, Delrez, L, Demangeon, O, Demory, B.-O., Ehrenreich, D, Erikson, A, Fossati, L, Fridlund, M, Gandolfi, D, Gillon, M, Güdel, M, Heng, K, Leon, J E Hernández, Isaak, K G, Kiss, L L, Laskar, J, Etangs, A Lecavelier des, Lendl, M, Lovis, C, Magrin, D, Munari, M, Nascimbeni, V, Olofsson, G, Ottensamer, R, Pagano, I, Pallé, E, Peter, G, Piotto, G, Pollacco, D, Queloz, D, Ragazzoni, R, Rando, N, Rauer, H, Ribas, I, Santos, N C, Scandariato, G, Ségransan, D, Smith, A M S, Steinberger, M, Steller, M, Szabó, Gy M, Thomas, N, Udry, S, Van Grootel, V, Walton, N
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2022, 513, pp.6042-6057. ⟨10.1093/mnras/stac1270⟩
Maxted, P F L; Miller, N J; Hoyer, S; Adibekyan, V; Sousa, S G; Billot, N; Fortier, A; Simon, A E; Cameron, A Collier; Swayne, M I; Gutermann, P; Triaud, A H M J; Southworth, J; Alibert, Y; Alonso, R; Anglada, G; Bárczy, T; Navascues, D Barrado y; Barros, S C C; Baumjohann, W; ... (2022). Fundamental effective temperature measurements for eclipsing binary stars – III. SPIRou near-infrared spectroscopy and CHEOPS photometry of the benchmark G0V star EBLM J0113+31. Monthly notices of the Royal Astronomical Society, 513(4), pp. 6042-6057. Wiley 10.1093/mnras/stac1270
Monthly Notices of the Royal Astronomical Society, 513(4), 6042-6057
Monthly Notices of the Royal Astronomical Society, 513 (4)
Monthly Notices of the Royal Astronomical Society, 2022, 513, pp.6042-6057. ⟨10.1093/mnras/stac1270⟩
Maxted, P F L; Miller, N J; Hoyer, S; Adibekyan, V; Sousa, S G; Billot, N; Fortier, A; Simon, A E; Cameron, A Collier; Swayne, M I; Gutermann, P; Triaud, A H M J; Southworth, J; Alibert, Y; Alonso, R; Anglada, G; Bárczy, T; Navascues, D Barrado y; Barros, S C C; Baumjohann, W; ... (2022). Fundamental effective temperature measurements for eclipsing binary stars – III. SPIRou near-infrared spectroscopy and CHEOPS photometry of the benchmark G0V star EBLM J0113+31. Monthly notices of the Royal Astronomical Society, 513(4), pp. 6042-6057. Wiley 10.1093/mnras/stac1270
Monthly Notices of the Royal Astronomical Society, 513(4), 6042-6057
Monthly Notices of the Royal Astronomical Society, 513 (4)
EBLM J0113+31 is a moderately bright (V = 10.1), metal-poor ([Fe/H] approximate to-0.3) GOV star with a much fainter M dwarf companion on a wide, eccentric orbit (= 14.3 d). We have used near-infrared spectroscopy obtained with the SPIRou spectrograp
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6a8465189de9cdfa9ab371e18a4b91cf
https://elib.dlr.de/187323/
https://elib.dlr.de/187323/