Zobrazeno 1 - 10
of 16
pro vyhledávání: '"Haywood RD"'
Autor:
Lacedelli, G, Wilson, TG, Malavolta, L, Hooton, MJ, Collier Cameron, A, Alibert, Y, Mortier, A, Bonfanti, A, Haywood, RD, Hoyer, S, Piotto, G, Bekkelien, A, Vanderburg, AM, Benz, W, Dumusque, X, Deline, A, Lopez-Morales, M, Borsato, L, Rice, K, Fossati, L, Latham, DW, Brandeker, A, Poretti, E, Sousa, SG, Sozzetti, A, Salmon, S, Burke, CJ, Van Grootel, V, Fausnaugh, MM, Adibekyan, V, Huang, CX, Osborn, HP, Mustill, AJ, Palle, E, Bourrier, V, Nascimbeni, V, Alonso, R, Anglada, G, Barczy, T, Barrado Y Navascues, D, Barros, SCC, Baumjohann, W, Beck, M, Beck, T, Billot, N, Bonfils, X, Broeg, C, Buchhave, LA, Cabrera, J, Charnoz, S, Cosentino, R, Csizmadia, S, Davies, MB, Deleuil, M, Delrez, L, Demangeon, O, Demory, BO, Ehrenreich, D, Erikson, A, Esparza-Borges, E, Floren, HG, Fortier, A, Fridlund, M, Futyan, D, Gandolfi, D, Ghedina, A, Gillon, M, Güdel, M, Guterman, P, Harutyunyan, A, Heng, K, Isaak, KG, Jenkins, JM, Kiss, L, Laskar, J, Lecavelier Des Etangs, A, Lendl, M, Lovis, C, Magrin, D, Marafatto, L, Martinez Fiorenzano, AF, Maxted, PFL, Mayor, M, Micela, G, Molinari, E, Murgas, F, Narita, N, Olofsson, G, Ottensamer, R, Pagano, I, Pasetti, A, Pedani, M, Pepe, FA, Peter, G, Phillips, DF, Pollacco, D, Queloz, D, Ragazzoni, R, Rando, N, Ratti, F
We present a precise characterization of the TOI-561 planetary system obtained by combining previously published data with TESS and CHEOPS photometry, and a new set of $62$ HARPS-N radial velocities (RVs). Our joint analysis confirms the presence of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::71b42fabcaf5754135d8e8c72573eeb5
https://www.repository.cam.ac.uk/handle/1810/333408
https://www.repository.cam.ac.uk/handle/1810/333408
Autor:
Mayo, AW, Rajpaul, VM, Buchhave, LA, Dressing, CD, Mortier, A, Zeng, L, Fortenbach, CD, Aigrain, S, Bonomo, AS, Cameron, AC, Charbonneau, D, Coffinet, A, Cosentino, R, Damasso, M, Dumusque, X, Fiorenzano, AFM, Haywood, RD, Latham, DW, López-Morales, M, Malavolta, L, Micela, G, Molinari, E, Pearce, L, Pepe, F, Phillips, D, Piotto, G, Poretti, E, Rice, K, Sozzetti, A, Udry, S
Publikováno v:
Astronomical Journal, vol 159, iss 1
The semimajor axis and planet insolation flux of Kepler-538b were incorrectly calculated in the published article. This error did not impact any other parameters or any other results in the paper. Table 2 has been included in full here with the corre
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______325::699b89683dfa4322eb6e4d3208396a27
https://escholarship.org/uc/item/56d2x089
https://escholarship.org/uc/item/56d2x089
Autor:
Thompson, APG, Watson, CA, Haywood, RD, Costes, JC, De Mooij, E, Collier Cameron, A, Dumusque, X, Phillips, DF, Saar, SH, Mortier, A, Milbourne, TW, Aigrain, S, Cegla, HM, Charbonneau, D, Cosentino, R, Ghedina, A, Latham, DW, López-Morales, M, Micela, G, Molinari, E, Poretti, E, Sozzetti, A, Thompson, S, Walsworth, R
Stellar activity is the major roadblock on the path to finding true Earth-analogue planets with the Doppler technique. Thus, identifying new indicators that better trace magnetic activity (i.e. faculae and spots) is crucial to aid in disentangling th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::5d7895ef1c2ee1b1ed9b1d026e8fdf90
Autor:
Langellier, N, Milbourne, TW, Phillips, DF, Haywood, RD, Saar, SH, Mortier, A, Malavolta, L, Thompson, S, Cameron, AC, Dumusque, X, Cegla, HM, Latham, DW, Maldonado, J, Watson, CA, Buchschacher, N, Cecconi, M, Charbonneau, D, Cosentino, R, Ghedina, A, Gonzalez, M, Li, CH, Lodi, M, López-Morales, M, Micela, G, Molinari, E, Pepe, F, Poretti, E, Rice, K, Sasselov, D, Sozzetti, A, Udry, S, Walsworth, RL
Radial velocity (RV) searches for Earth-mass exoplanets in the habitable zone around Sun-like stars are limited by the effects of stellar variability on the host star. In particular, suppression of convective blueshift and brightness inhomogeneities
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c85c4cf6a8846b01ee202cace59ab29b
Autor:
Mortier, A, Zapatero Osorio, MR, Malavolta, L, Alibert, Y, Rice, K, Lillo-Box, J, Vanderburg, A, Oshagh, M, Buchhave, L, Adibekyan, V, Delgado Mena, E, Lopez-Morales, M, Charbonneau, D, Sousa, SG, Lovis, C, Affer, L, Allende Prieto, C, Barros, SCC, Benatti, S, Bonomo, AS, Boschin, W, Bouchy, F, Cabral, A, Collier Cameron, A, Cosentino, R, Cristiani, S, Demangeon, ODS, Di Marcantonio, P, D'Odorico, V, Dumusque, X, Ehrenreich, D, Figueira, P, Fiorenzano, A, Ghedina, A, González Hernández, JI, Haldemann, J, Harutyunyan, A, Haywood, RD, Latham, DW, Lavie, B, Lo Curto, G, Maldonado, J, Manescau, A, Martins, CJAP, Mayor, M, Mégevand, D, Mehner, A, Micela, G, Molaro, P, Molinari, E, Nunes, NJ, Pepe, FA, Palle, E, Phillips, D, Piotto, G, Pinamonti, M, Poretti, E, Riva, M, Rebolo, R, Santos, NC, Sasselov, D, Sozzetti, A, Suárez Mascareño, A, Udry, S, West, RG, Watson, CA, Wilson, TG
This paper reports on the detailed characterisation of the K2-111 planetary system with K2, WASP, and ASAS-SN photometry as well as high-resolution spectroscopic data from HARPS-N and ESPRESSO. The host, K2-111, is confirmed to be a mildly evolved ($
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::bbf676f39ea083d90fa2b102cbdb0c47
Autor:
Malavolta, L, Borsato, L, Granata, V, Piotto, G, Lopez, E, Vanderburg, A, Figueira, P, Mortier, A, Nascimbeni, V, Affer, L, Bonomo, AS, Bouchy, F, Buchhave, LA, Charbonneau, D, Cameron, AC, Cosentino, R, Dressing, CD, Dumusque, X, Fiorenzano, AFM, Harutyunyan, A, Haywood, RD, Johnson, JA, Latham, DW, Lopez-Morales, M, Lovis, C, Mayor, M, Micela, G, Molinari, E, Motalebi, F, Pepe, F, Phillips, DF, Pollacco, D, Queloz, D, Rice, K, Sasselov, D, Ségransan, D, Sozzetti, A, Udry, S, Watson, C
We report a detailed characterization of the Kepler-19 system. This star was previously known to host a transiting planet with a period of 9.29 days, a radius of 2.2 R⊕ and an upper limit on the mass of 20 M⊕. The presence of a second, non-transi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d7f05695cabd70c19cd2e23d0923cfb1
Akademický článek
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Autor:
Kunimoto, Michelle, Vanderburg, Andrew, Huang, Chelsea X., Davis, M. Ryleigh, Affer, Laura, Cameron, Andrew Collier, Charbonneau, David, Cosentino, Rosario, Damasso, Mario, Dumusque, Xavier, Fiorenzano, A. F. Martnez, Ghedina, Adriano, Haywood, R. D., Lienhard, Florian, López-Morales, Mercedes, Mayor, Michel, Pepe, Francesco, Pinamonti, Matteo, Poretti, Ennio, Maldonado, Jesús, Rice, Ken, Sozzetti, Alessandro, Wilson, Thomas G., Udry, Stéphane, Baptista, Jay, Barkaoui, Khalid, Becker, Juliette, Benni, Paul, Bieryla, Allyson, Bosch-Cabot, Pau, Ciardi, David R., Collins, Karen A., Collins, Kevin I., Evans, Elise, Dupuy, Trent J., Goliguzova, Maria V., Guerra, Pere, Kraus, Adam, Lissauer, Jack J., Huber, Daniel, Murgas, Felipe, Palle, Enric, Quinn, Samuel N., Safonov, Boris S., Schwarz, Richard P., Shporer, Avi, Stassun, Keivan G., Jenkins, Jon M., Latham, David W., Ricker, George R., Seager, Sara, Vanderspek, Roland, Winn, Joshua, Essack, Zahra, Lewis, Hannah M., Rose, Mark E.
We report the confirmation of three exoplanets transiting TOI-4010 (TIC-352682207), a metal-rich K dwarf observed by TESS in Sectors 24, 25, 52, and 58. We confirm these planets with HARPS-N radial velocity observations and measure their masses with
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b435e24f5ea52038ab46e58786ae93ce
Autor:
Victoria DiTomasso, Chantanelle Nava, Mercedes López-Morales, Allyson Bieryla, Ryan Cloutier, Luca Malavolta, Annelies Mortier, Lars A. Buchhave, Keivan G. Stassun, Alessandro Sozzetti, Aldo Stefano Bonomo, David Charbonneau, Andrew Collier Cameron, Rosario Cosentino, Mario Damasso, Xavier Dumusque, A. F. Martínez Fiorenzano, Adriano Ghedina, Avet Harutyunyan, R. D. Haywood, David Latham, Emilio Molinari, Francesco A. Pepe, Matteo Pinamonti, Ennio Poretti, Ken Rice, Dimitar Sasselov, Manu Stalport, Stéphane Udry, Christopher Watson, Thomas G. Wilson
Publikováno v:
DiTomasso, V, Nava, C, López-Morales, M, Bieryla, A, Cloutier, R, Malavolta, L, Mortier, A, Buchhave, L A, Stassun, K G, Sozzetti, A, Bonomo, A S, Charbonneau, D, Collier Cameron, A, Cosentino, R, Damasso, M, Dumusque, X, Martínez Fiorenzano, A F, Ghedina, A, Harutyunyan, A, Haywood, R D, Latham, D, Molinari, E, Pepe, F A, Pinamonti, M, Poretti, E, Rice, K, Sasselov, D, Stalport, M, Udry, S, Watson, C & Wilson, T G 2023, ' Independent validation of the Temperate Super-Earth HD 79211 b using HARPS-N ', Astronomical Journal, vol. 165, no. 2, 38 . https://doi.org/10.3847/1538-3881/ac9ccd
DiTomasso, V, Nava, C, López-Morales, M, Bieryla, A, Cloutier, R, Malavolta, L, Mortier, A, Buchhave, L A, Stassun, K G, Sozzetti, A, Bonomo, A S, Charbonneau, D, Collier Cameron, A, Cosentino, R, Damasso, M, Dumusque, X, Martínez Fiorenzano, A F, Ghedina, A, Harutyunyan, A, Haywood, R D, Latham, D, Molinari, E, Pepe, F A, Pinamonti, M, Poretti, E, Rice, K, Sasselov, D, Stalport, M, Udry, S, Watson, C & Wilson, T G 2023, ' Independent Validation of the Temperate Super-Earth HD 79211 b using HARPS-N ', Astronomical Journal, vol. 165, no. 2, 38 . https://doi.org/10.3847/1538-3881/ac9ccd
DiTomasso, V, Nava, C, López-Morales, M, Bieryla, A, Cloutier, R, Malavolta, L, Mortier, A, Buchhave, L A, Stassun, K G, Sozzetti, A, Bonomo, A S, Charbonneau, D, Cameron, A C, Cosentino, R, Damasso, M, Dumusque, X, Fiorenzano, A F M, Ghedina, A, Harutyunyan, A, Haywood, R D, Latham, D, Molinari, E, Pepe, F A, Pinamonti, M, Poretti, E, Rice, K, Sasselov, D, Stalport, M, Udry, S, Watson, C & Wilson, T G 2023, ' Independent validation of the temperate Super-Earth HD79211 b using HARPS-N ', Astronomical Journal, vol. 165, no. 2, 38, pp. 1-22 . https://doi.org/10.3847/1538-3881/ac9ccd
DiTomasso, V, Nava, C, López-Morales, M, Bieryla, A, Cloutier, R, Malavolta, L, Mortier, A, Buchhave, L A, Stassun, K G, Sozzetti, A, Bonomo, A S, Charbonneau, D, Collier Cameron, A, Cosentino, R, Damasso, M, Dumusque, X, Martínez Fiorenzano, A F, Ghedina, A, Harutyunyan, A, Haywood, R D, Latham, D, Molinari, E, Pepe, F A, Pinamonti, M, Poretti, E, Rice, K, Sasselov, D, Stalport, M, Udry, S, Watson, C & Wilson, T G 2023, ' Independent Validation of the Temperate Super-Earth HD 79211 b using HARPS-N ', Astronomical Journal, vol. 165, no. 2, 38 . https://doi.org/10.3847/1538-3881/ac9ccd
DiTomasso, V, Nava, C, López-Morales, M, Bieryla, A, Cloutier, R, Malavolta, L, Mortier, A, Buchhave, L A, Stassun, K G, Sozzetti, A, Bonomo, A S, Charbonneau, D, Cameron, A C, Cosentino, R, Damasso, M, Dumusque, X, Fiorenzano, A F M, Ghedina, A, Harutyunyan, A, Haywood, R D, Latham, D, Molinari, E, Pepe, F A, Pinamonti, M, Poretti, E, Rice, K, Sasselov, D, Stalport, M, Udry, S, Watson, C & Wilson, T G 2023, ' Independent validation of the temperate Super-Earth HD79211 b using HARPS-N ', Astronomical Journal, vol. 165, no. 2, 38, pp. 1-22 . https://doi.org/10.3847/1538-3881/ac9ccd
We present high-precision radial velocities (RVs) from the HARPS-N spectrograph for HD79210 and HD79211, two M0V members of a gravitationally-bound binary system. We detect a planet candidate with a period of $24.421^{+0.016}_{-0.017}$ days around HD
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f63f9fe1ab3a26da23373cb2b172b01f
https://hdl.handle.net/11577/3468253
https://hdl.handle.net/11577/3468253
Autor:
R. D. Haywood, T. W. Milbourne, S. H. Saar, A. Mortier, D. Phillips, D. Charbonneau, A. Collier Cameron, H. M. Cegla, N. Meunier, M. L. Palumbo III
We estimate disc-averaged RV variations of the Sun over the last magnetic cycle, from the single Fe I line observed by SDO/HMI, using a physical model for rotationally modulated magnetic activity that was previously validated against HARPS-N solar ob
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::681db9209cdc3be093754c0d4dbd69de
http://wrap.warwick.ac.uk/168052/7/WRAP-Unsigned-magnetic-flux-proxy-radial-velocity-variations-sun-like-stars-22.pdf
http://wrap.warwick.ac.uk/168052/7/WRAP-Unsigned-magnetic-flux-proxy-radial-velocity-variations-sun-like-stars-22.pdf