Zobrazeno 1 - 10
of 262
pro vyhledávání: '"Turner O"'
Autor:
Cegla, H. M., Roguet-Kern, N., Lendl, M., Akinsanmi, B., McCormac, J., Oshagh, M., Wheatley, P. J., Chen, G., Allart, R., Mortier, A., Bourrier, V., Buchschacher, N., Lovis, C., Sosnowska, D., Sulis, S., Turner, O., Casasayas-Barris, N., Palle, E., Yan, F., Burleigh, M. R., Casewell, S. L., Goad, M. R., Hawthorn, F., Wyttenbach, A.
Publikováno v:
A&A 674, A174 (2023)
We analyse spectroscopic and photometric transits of the hot Jupiters WASP-52b and HAT-P30b obtained with ESPRESSO, Eulercam and NGTS for both targets, and additional TESS data for HAT-P-30. Our goal is to update the system parameters and refine our
Externí odkaz:
http://arxiv.org/abs/2304.11022
Autor:
Leleu, A., Alibert, Y., Hara, N. C., Hooton, M. J., Wilson, T. G., Robutel, P., Delisle, J. -B., Laskar, J., Hoyer, S., Lovis, C., Bryant, E. M., Ducrot, E., Cabrera, J., Delrez, L., Acton, J. S., Adibekyan, V., Allart, R., Prieto, C. Allende, Alonso, R., Alves, D., Anderson, D. R., Angerhausen, D., Escudé, G. Anglada, Asquier, J., Barrado, D., Barros, S. C. C., Baumjohann, W., Bayliss, D., Beck, M., Beck, T., Bekkelien, A., Benz, W., Billot, N., Bonfanti, A., Bonfils, X., Bouchy, F., Bourrier, V., Boué, G., Brandeker, A., Broeg, C., Buder, M., Burdanov, A., Burleigh, M. R., Bárczy, T., Cameron, A. C., Chamberlain, S., Charnoz, S., Cooke, B. F., Van Damme, C. Corral, Correia, A. C. M., Cristiani, S., Damasso, M., Davies, M. B., Deleuil, M., Demangeon, O. D. S., Demory, B. -O., Di Marcantonio, P., Di Persio, G., Dumusque, X., Ehrenreich, D., Erikson, A., Figueira, P., Fortier, A., Fossati, L., Fridlund, M., Futyan, D., Gandolfi, D., Muñoz, A. García, Garcia, L. J., Gill, S., Gillen, E., Gillon, M., Goad, M. R., Hernández, J. I. González, Guedel, M., Günther, M. N., Haldemann, J., Henderson, B., Heng, K., Hogan, A. E., Isaak, K., Jehin, E., Jenkins, J. S., Jordán, A., Kiss, L., Kristiansen, M. H., Lam, K., Lavie, B., Etangs, A. Lecavelier des, Lendl, M., Lillo-Box, J., Curto, G. Lo, Magrin, D., Martins, C. J. A. P., Maxted, P. F. L., McCormac, J., Mehner, A., Micela, G., Molaro, P., Moyano, M., Murray, C. A., Nascimbeni, V., Nunes, N. J., Olofsson, G., Osborn, H. P., Oshagh, M., Ottensamer, R., Pagano, I., Pallé, E., Pedersen, P. P., Pepe, F. A., Persson, C. M., Peter, G., Piotto, G., Polenta, G., Pollacco, D., Poretti, E., Pozuelos, F. J., Queloz, D., Ragazzoni, R., Rando, N., Ratti, F., Rauer, H., Raynard, L., Rebolo, R., Reimers, C., Ribas, I., Santos, N. C., Scandariato, G., Schneider, J., Sebastian, D., Sestovic, M., Simon, A. E., Smith, A. M. S., Sousa, S. G., Sozzetti, A., Steller, M., Mascareño, A. Suárez, Szabó, Gy. M., Ségransan, D., Thomas, N., Thompson, S., Tilbrook, R. H., Triaud, A., Turner, O., Udry, S., Van Grootel, V., Venus, H., Verrecchia, F., Vines, J. I., Walton, N. A., West, R. G., Wheatley, P. J., Wolter, D., Osorio, M. R. Zapatero
Determining the architecture of multi-planetary systems is one of the cornerstones of understanding planet formation and evolution. Resonant systems are especially important as the fragility of their orbital configuration ensures that no significant
Externí odkaz:
http://arxiv.org/abs/2101.09260
Autor:
Smith, A. M. S., Acton, J. S., Anderson, D. R., Armstrong, D. J., Bayliss, D., Belardi, C., Bouchy, F., Brahm, R., Briegal, J. T., Bryant, E. M., Burleigh, M. R., Cabrera, J., Chaushev, A., Cooke, B. F., Costes, J. C., Csizmadia, Sz., Eigmüller, Ph., Erikson, A., Gill, S., Gillen, E., Goad, M. R., Günther, M. N., Henderson, B. A., Hogan, A., Jordán, A., Lendl, M., McCormac, J., Moyano, M., Nielsen, L. D., Rauer, H., Raynard, L., Tilbrook, R. H., Turner, O., Udry, S., Vines, J. I., Watson, C. A., West, R. G., Wheatley, P. J.
Publikováno v:
A&A 646, A183 (2021)
Context: The sub-Jovian or Neptunian desert is a previously-identified region of parameter space where there is a relative dearth of intermediate-mass planets at short orbital periods. Aims: We present the discovery of a new transiting planetary syst
Externí odkaz:
http://arxiv.org/abs/2101.01470
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:
Nielsen, L. D., Brahm, R., Bouchy, F., Espinoza, N., Turner, O., Rappaport, S., Pearce, L., Ricker, G., Vanderspek, R., Latham, D. W., Seager, S., Winn, J. N., Jenkins, J. M., Acton, J. S., Bakos, G., Barclay, T., Barkaoui, K., Bhatti, W., Briceño, C., Bryant, E. M., Burleigh, M. R., Ciardi, D. R., Collins, K. A., Collins, K. I., Cooke, B. F., Csubry, Z., Santos, L. A. dos, Eigmüller, Ph., Fausnaugh, M. M., Gan, T., Gillon, M., Goad, M. R., Guerrero, N., Hagelberg, J., Hart, R., Henning, T., Huang, C. X., Jehin, E., Jenkins, J. S., Jordàn, A., Kielkopf, J. F., Kossakowski, D., Lavie, B., Law, N., Lendl, M., de Leon, J. P., Lovis, C., Mann, A. W., Marmier, M., McCormac, J., Mori, M., Moyano, M., Narita, N., Osip, D., Otegi, J. F., Pepe, F., Pozuelos, F. J., Raynard, L., Relles, H. M., Sarkis, P., Segransan, D., Seidel, J. V., Shporer, A., Stalport, M., Stockdale, C., Suc, V., Tamura, M., Tan, T. G., Tilbrook, R. H., Ting, E. B., Trifonov, T., Udry, S., Vanderburg, A., Wheatley, P. J., Wingham, G., Zhan, Z., Ziegler, C.
Publikováno v:
A&A 639, A76 (2020)
We report the confirmation and mass determination of three hot Jupiters discovered by the Transiting Exoplanet Survey Satellite (TESS) mission: HIP 65Ab (TOI-129, TIC-201248411) is an ultra-short-period Jupiter orbiting a bright (V=11.1 mag) K4-dwarf
Externí odkaz:
http://arxiv.org/abs/2003.05932
Autor:
Chen, Chian-Chou, Harrison, C. M., Smail, I., Swinbank, A. M., Turner, O. J., Wardlow, J. L., Brandt, W. N., Rivera, G. Calistro, Chapman, S. C., Cooke, E. A., Dannerbauer, H., Dunlop, J. S., Farrah, D., Michałowski, M. J., Schinnerer, E., Simpson, J. M., Thomson, A. P., van der Werf, P. P.
Publikováno v:
A&A 635, A119 (2020)
Using data from ALMA and near-infrared (NIR) integral field spectrographs including both SINFONI and KMOS on the VLT, we investigate the two-dimensional distributions of H$\alpha$ and rest-frame far-infrared (FIR) continuum in six submillimeter galax
Externí odkaz:
http://arxiv.org/abs/2002.03545
Autor:
Scholtz, J., Harrison, C. M., Rosario, D. J., Alexander, D. M., Chen, C-C., Kakkad, D., Mainieri, V., Tiley, A. L., Turner, O., Cirasuolo, M., Sharples, R. M., Stach, S.
As part of our KMOS AGN Survey at High-redshift (KASHz), we present spatially-resolved VLT/KMOS and VLT/SINFONI spectroscopic data and ALMA 870$\mu$m continuum imaging of eight $z$=1.4--2.6 moderate AGN ($L_{\rm 2-10 \rm kev}$ = $10^{42} - 10^{45}$ e
Externí odkaz:
http://arxiv.org/abs/2001.02242
Autor:
Hellier, C., Anderson, D. R., Barkaoui, K., Benkhaldoun, Z., Bouchy, F., Burdanov, A., Cameron, A. Collier, Delrez, L., Gillon, M., Jehin, E., Nielsen, L. D., Maxted, P. F. L., Pepe, F., Pollacco, D., Pozuelos, F. J., Queloz, D., Segransan, D., Smalley, B., Triaud, A. H. M. J., Turner, O. D., Udry, S., West, R. G.
We report on four new transiting hot Jupiters discovered by the WASP-South survey. WASP-178b transits a V = 9.9, A1V star with Teff = 9350 +/- 150 K, the second-hottest transit host known. It has a highly bloated radius of 1.81 +/- 0.09 Rjup, in line
Externí odkaz:
http://arxiv.org/abs/1907.11667
Autor:
Gill, S., Maxted, P. F. L., Evans, J. A., Evans, D. F., Southworth, J., Smalley, B., Gary, B. L., Anderson, D. R., Bouchy, F., Cameron, A. C., Dominik, M., Faedi, F., Gillon, M., Chew, Y. Gomez Maqueo, Hebb, L., Hellier, C., Jørgensen, U. G., Longa-Peña, P., Martin, D. V., McCormac, J., Pepe, F. V., Pollaco, D., Queloz, D., Ségransan, D., Snodgrass, C., Turner, O. D., Triaud, A. H. M., Udry, S., Snodgrass, R. G. West, West, R. G.
Publikováno v:
A&A 626, A119 (2019)
Some M-dwarfs around F-/G-type stars have been measured to be hotter and larger than predicted by stellar evolution models. Inconsistencies between observations and models need addressing with more mass, radius and luminosity measurements of low-mass
Externí odkaz:
http://arxiv.org/abs/1904.12695
Autor:
Nielsen, L. D., Bouchy, F., Turner, O. D., Anderson, D. R., Barkaoui, K., Benkhaldoun, Z., Burdanov, A., Cameron, A. Collier, Delrez, L., Gillon, M., Ducrot, E., Hellier, C., Jehin, E., Lendl, M., Maxted, P. F. L., Pepe, F., Pollacco, D., Pozuelos, F. J., Queloz, D., Segransan, D., Smalley, B., Triaud, A. H. M. J., Udry, S., West, R. G.
We present the discovery of four new giant planets from \WASP, three hot Jupiters and one bloated sub-Saturn mass planet; WASP-169b, WASP-171b, WASP-175b and WASP-182b. Besides the discovery photometry from \wasp\ we use radial velocity measurements
Externí odkaz:
http://arxiv.org/abs/1904.10388