Zobrazeno 1 - 10
of 37
pro vyhledávání: '"Verilhac, D."'
Autor:
Almenara, J. M., Hébrard, G., Díaz, R. F., Laskar, J., Correia, A. C. M., Anderson, D. R., Boisse, I., Bonfils, X., Brown, D. J. A., Casanova, V., Cameron, A. Collier, Fernández, M., Jenkins, J. M., Kiefer, F., Étangs, A. Lecavelier des, Lissauer, J. J, Maciejewski, G., McCormac, J., Osborn, H., Pollacco, D., Ricker, G., Sánchez, J., Seager, S., Udry, S., Verilhac, D., Winn, J.
Publikováno v:
A&A 663, A134 (2022)
WASP-148 is a recently announced extra-solar system harbouring at least two giant planets. The inner planet transits its host star. The planets travel on eccentric orbits and are near the 4:1 mean-motion resonance, which implies significant mutual gr
Externí odkaz:
http://arxiv.org/abs/2204.06656
Autor:
St-Louis, N., Piaulet, C., Richardson, N. D., Shenar, T., Moffat, A. F. J., Eversberg, T., Hill, G. M., Gauza, B., Knapen, J. H., Kubat, J., Kubatova, B., Sablowski, D. P., Simon-Diaz, S., Bolduan, F., Dias, F. M., Dubreuil, P., Fuchs, D., Garrel, T., Grutzeck, G., Hunger, T., Kusters, D., Langenbrink, M., Leadbeater, R., Li, D., Lopez, A., Mauclaire, B., Moldenhawer, T., Potter, M., Santos, E. M. dos, Schanne, L., Schmidt, J., Sieske, H., Strachan, J., Stinner, E., Stinner, P., Stober, B., Strandbaek, K., Syder, T., Verilhac, D., Waldschlager, U., Weiss, D., Wendt, A.
We present the results of a four-month, spectroscopic campaign of the Wolf-Rayet dust-making binary, WR137. We detect only small-amplitude, random variability in the CIII5696 emission line and its integrated quantities (radial velocity, equivalent wi
Externí odkaz:
http://arxiv.org/abs/2007.09239
Autor:
Hebrard, G., Diaz, R. F., Correia, A. C. M., Cameron, A. Collier, Laskar, J., Pollacco, D., Almenara, J. -M., Anderson, D. R., Barros, S. C. C., Boisse, I., Bonomo, A. S., Bouchy, F., Boue, G., Boumis, P., Brown, D. J. A., Dalal, S., Deleuil, M., Demangeon, O., Doyle, A. P., Haswell, C. A., Hellier, C., Osborn, H., Kiefer, F., Kolb, U. C., Lam, K., Etangs, A. Lecavelier des, Lopez, T., Martin-Lagarde, M., Maxted, P., McCormac, J., Nielsen, L. D., Palle, E., Prieto-Arranz, J., Queloz, D., Santerne, A., Smalley, B., Turner, O., Udry, S., Verilhac, D., West, R., Wheatley, P. J., Wilson, P. A.
Publikováno v:
A&A 640, A32 (2020)
We present the discovery and characterization of WASP-148, a new extrasolar system that includes at least two giant planets. The host star is a slowly rotating inactive late-G dwarf with a V=12 magnitude. The planet WASP-148b is a hot Jupiter of 0.72
Externí odkaz:
http://arxiv.org/abs/2004.14645
Autor:
Meza, E., Sicardy, B., Assafin, M., Ortiz, J. L., Bertrand, T., Lellouch, E., Desmars, J., Forget, F., Bérard, D., Doressoundiram, A., Lecacheux, J., Oliveira, J. Marques, Roques, F., Widemann, T., Colas, F., Vachier, F., Renner, S., Leiva, R., Braga-Ribas, F., Benedetti-Rossi, G., Camargo, J. I. B., Dias-Oliveira, A., Morgado, B., Gomes-Júnior, A. R., Vieira-Martins, R., Behrend, R., Tirado, A. Castro, Duffard, R., Morales, N., Santos-Sanz, P., Jelínek, M., Cunniffe, R., Querel, R., Harnisch, M., Jansen, R., Pennell, A., Todd, S., Ivanov, V. D., Opitom, C., Gillon, M., Jehin, E., Manfroid, J., Pollock, J., Reichart, D. E., Haislip, J. B., Ivarsen, K. M., LaCluyze, A. P., Maury, A., Gil-Hutton, R., Dhillon, V., Littlefair, S., Marsh, T., Veillet, C., Bath, K. -L., Beisker, W., Bode, H. -J., Kretlow, M., Herald, D., Gault, D., Kerr, S., Pavlov, H., Faragó, O., Klös, O., Frappa, E., Lavayssière, M., Cole, A. A., Giles, A. B., Greenhill, J. G., Hill, K. M., Buie, M. W., Olkin, C. B., Young, E. F., Young, L. A., Wasserman, L. H., Devogèle, M., French, R. G., Bianco, F. B., Marchis, F., Brosch, N., Kaspi, S., Polishook, D., Manulis, I., Larbi, M. Ait Moulay, Benkhaldoun, Z., Daassou, A., Azhari, Y. El, Moulane, Y., Broughton, J., Milner, J., Dobosz, T., Bolt, G., Lade, B., Gilmore, A., Kilmartin, P., Allen, W. H., Graham, P. B., Loader, B., McKay, G., Talbot, J., Parker, S., Abe, L., Bendjoya, Ph., Rivet, J. -P., Vernet, D., Di Fabrizio, L., Lorenzi, V., Magazzù, A., Molinari, E., Gazeas, K., Tzouganatos, L., Carbognani, A., Bonnoli, G., Marchini, A., Leto, G., Sanchez, R. Zanmar, Mancini, L., Kattentidt, B., Dohrmann, M., Guhl, K., Rothe, W., Walzel, K., Wortmann, G., Eberle, A., Hampf, D., Ohlert, J., Krannich, G., Murawsky, G., Gährken, B., Gloistein, D., Alonso, S., Román, A., Communal, J. -E., Jabet, F., de Visscher, S., Sérot, J., Janik, T., Moravec, Z., Machado, P., Selva, A., Perelló, C., Rovira, J., Conti, M., Papini, R., Salvaggio, F., Noschese, A., Tsamis, V., Tigani, K., Barroy, P., Irzyk, M., Neel, D., Godard, J. P., Lanoiselée, D., Sogorb, P., Vérilhac, D., Bretton, M., Signoret, F., Ciabattari, F., Naves, R., Boutet, M., De Queiroz, J., Lindner, P., Lindner, K., Enskonatus, P., Dangl, G., Tordai, T., Eichler, H., Hattenbach, J., Peterson, C., Molnar, L. A., Howell, R. R.
Publikováno v:
A&A 625, A42 (2019)
Context. Pluto's tenuous nitrogen (N2) atmosphere undergoes strong seasonal effects due to high obliquity and orbital eccentricity, and has been recently (July 2015) observed by the New Horizons spacecraft. Goals are (i) construct a well calibrated r
Externí odkaz:
http://arxiv.org/abs/1903.02315
Autor:
Gillet, D., Mauclaire, B., Garrel, T., Lemoult, T., Mathias, Ph., de France, T., Devaux, J-S., Boussier, H., Verilhac, D., Brabant, G., Desbordes, J., Garde, O., Collaboration, the GRRR
Publikováno v:
A&A 607, A51 (2017)
The so-called H$\alpha$ third emission occurs around pulsation phase $\varphi$=0.30. It has been observed for the first time in 2011 in some RR Lyrae stars. The emission intensity is very weak, and its profile is a tiny persistent hump in the red sid
Externí odkaz:
http://arxiv.org/abs/1709.03556
Autor:
Aldoretta, E. J., St-Louis, N., Richardson, N. D., Moffat, A. F. J., Eversberg, T., Hill, G. M., Shenar, T., Artigau, É., Gauza, B., Knapen, J. H., Kubát, J., Kubátová, B., Maltais-Tariant, R., Muñoz, M., Pablo, H., Ramiaramanantsoa, T., Richard-Laferrière, A., Sablowski, D. P., Simón-Díaz, S., St-Jean, L., Bolduan, F., Dias, F. M., Dubreuil, P., Fuchs, D., Garrel, T., Grutzeck, G., Hunger, T., Küsters, D., Langenbrink, M., Leadbeater, R., Li, D., Lopez, A., Mauclaire, B., Moldenhawer, T., Potter, M., Santos, E. M. dos, Schanne, L., Schmidt, J., Sieske, H., Strachan, J., Stinner, E., Stinner, P., Stober, B., Strandbaek, K., Syder, T., Verilhac, D., Waldschläger, U., Weiss, D., Wendt, A.
During the summer of 2013, a 4-month spectroscopic campaign took place to observe the variabilities in three Wolf-Rayet stars. The spectroscopic data have been analyzed for WR 134 (WN6b), to better understand its behaviour and long-term periodicity,
Externí odkaz:
http://arxiv.org/abs/1605.04868
Autor:
Santerne, A., Hébrard, G., Lillo-Box, J., Armstrong, D. J., Barros, S. C. C., Demangeon, O., Barrado, D., Debackere, A., Deleuil, M., Mena, E. Delgado, Montalto, M., Pollacco, D., Osborn, H. P., Sousa, S. G., Abe, L., Adibekyan, V., Almenara, J. -M., André, P., Arlic, G., Barthe, G., Bendjoya, P., Behrend, R., Boisse, I., Bouchy, F., Boussier, H., Bretton, M., Brown, D. J. A., Carry, B., Cailleau, A., Conseil, E., Courcol, B., Dauchet, B., Dalouzy, J. -C., Deldem, M., Dubreuil, P., Fehrenbach, J. -M., Ferratfiat, S., Girelli, R., Gregorio, J., Jaecques, S., Kugel, F., Kirk, J., Labrevoir, O., Lachurié, J. -C., Lam, K. W. F., Guen, P. Le, Martinez, P., Maurin, L., McCormac, J., Pioppa, J-B., Quadri, U., Rajpurohit, A., Rey, J., Rivet, J. -P., Roy, R., Santos, N. C., Signoret, F., Strabla, L., Suarez, O., Toublanc, D., Tsantaki, M., Wilson, P. A., Bachschmidt, M., Colas, F., Gerteis, O., Louis, P., Mario, J. -C., Marlot, C., Montier, J., Perroud, V., Pic, V., Romeuf, D., Ubaud, S., Verilhac, D.
Publikováno v:
2016, ApJ, 825, 55
In the present paper we report the discovery of a new hot Jupiter, EPIC211089792 b, first detected by the Super-WASP observatory and then by the K2 space mission during its campaign 4. The planet has a period of 3.25d, a mass of 0.73 +/- 0.04 Mjup, a
Externí odkaz:
http://arxiv.org/abs/1601.07680
Autor:
Santerne, A., Hébrard, G., Deleuil, M., Havel, M., Correia, A. C. M., Almenara, J. -M., Alonso, R., Arnold, L., Barros, S. C. C., Behrend, R., Bernasconi, L., Boisse, I., Bonomo, A. S., Bouchy, F., Bruno, G., Damiani, C., Díaz, R. F., Gravallon, D., Guillot, T., Labrevoir, O., Montagnier, G., Moutou, C., Rinner, C., Santos, N. C., Abe, L., Audejean, M., Bendjoya, P., Gillier, C., Gregorio, J., Martinez, P., Michelet, J., Montaigut, R., Poncy, R., Rivet, J. -P., Rousseau, G., Roy, R., Suarez, O., Vanhuysse, M., Verilhac, D.
Publikováno v:
A&A 571, A37 (2014)
In this paper we report a new transiting warm giant planet: KOI-1257 b. It was first detected in photometry as a planet-candidate by the ${\it Kepler}$ space telescope and then validated thanks to a radial velocity follow-up with the SOPHIE spectrogr
Externí odkaz:
http://arxiv.org/abs/1406.6172
Autor:
Almenara, J. M., Hébrard, G., Díaz, R. F., Laskar, J., Correia, A. C. M., Anderson, D. R., Boisse, I., Bonfils, X., Brown, D. J. A., Casanova, V., Cameron, A. Collier, Fernández, M., Jenkins, J. M., Kiefer, F., des Étangs, A. Lecavelier, Lissauer, J. J., Maciejewski, G., McCormac, J., Osborn, H., Pollacco, D., Ricker, G., Sánchez, J., Seager, S., Udry, S., Verilhac, D., Winn, J.
Funding for the TESS mission is provided by the NASA Explorer Program. Resources supporting this work were provided by the NASA High-End Computing (HEC) Program through the NASA Advanced Supercomputing (NAS) Division at Ames Research Center for the p
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::82c7c9c3bf2736d9dce2465ec599c238
http://wrap.warwick.ac.uk/168457/1/WRAP-Photodynamical-analysis-resonant-planetary-system-WASP-148-22.pdf
http://wrap.warwick.ac.uk/168457/1/WRAP-Photodynamical-analysis-resonant-planetary-system-WASP-148-22.pdf
Autor:
Hébrard, G., Díaz, R. F., Correia, A. C. M., Collier Cameron, A., Laskar, J., Pollacco, D., Almenara, J.-M., Anderson, D. R., Barros, S. C. C., Boisse, I., Bonomo, A. S., Bouchy, F., Boué, G., Boumis, P., Brown, D. J. A., Dalal, S., Deleuil, M., Demangeon, O. D. S., Doyle, A. P., Haswell, C.A., Hellier, C., Osborn, H., Kiefer, F., Kolb, U.C., Lam, K., Lecavelier des Étangs, A., Lopez, T., Martin-Lagarde, M., Maxted, P., McCormac, J., Nielsen, L. D., Pallé, E., Prieto-Arranz, J., Queloz, D., Santerne, A., Smalley, B., Turner, O., Udry, S., Verilhac, D., West, R., Wheatley, P. J., Wilson, P. A.
We present the discovery and characterization of WASP-148, a new extrasolar system that includes at least two giant planets. The host star is a slowly rotating inactive late-G dwarf with a V = 12 magnitude. The planet WASP-148b is a hot Jupiter of 0.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=core_ac_uk__::b5f728dd5d606c97749121b6552df9b6
http://oro.open.ac.uk/72019/1/72019.pdf
http://oro.open.ac.uk/72019/1/72019.pdf