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WFRF:(Madrigal Aguado A.)
 

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LIBRIS Formathandbok  (Information om MARC21)
FältnamnIndikatorerMetadata
00006383naa a2200697 4500
001oai:lup.lub.lu.se:f8e2fe08-486b-4fa3-815f-9e92cc9e22f6
003SwePub
008240301s2024 | |||||||||||000 ||eng|
024a https://lup.lub.lu.se/record/f8e2fe08-486b-4fa3-815f-9e92cc9e22f62 URI
024a https://doi.org/10.1093/mnras/stae0722 DOI
040 a (SwePub)lu
041 a engb eng
042 9 SwePub
072 7a art2 swepub-publicationtype
072 7a ref2 swepub-contenttype
100a Kang, H.u University of Science and Technology of China,Purple Mountain Observatory, Chinese Academy of Sciences4 aut
2451 0a Simultaneous multicolour transit photometry of hot Jupiters HAT-P-19b, HAT-P-51b, HAT-P-55b, and HAT-P-65b
264 1c 2024
300 a 15 s.
520 a Accurate physical parameters of exoplanet systems are essential for further exploration of planetary internal structure, atmospheres, and formation history. We aim to use simultaneous multicolour transit photometry to improve the estimation of transit parameters, to search for transit timing variations (TTVs), and to establish which of our targets should be prioritized for follow-up transmission spectroscopy. We performed time series photometric observations of 12 transits for the hot Jupiters HAT-P-19b, HAT-P-51b, HAT-P-55b, and HAT-P-65b using the simultaneous four-colour camera MuSCAT2 on the Telescopio Carlos Sánchez. We collected 56 additional transit light curves from TESS photometry. To derive transit parameters, we modelled the MuSCAT2 light curves with Gaussian processes to account for correlated noise. To derive physical parameters, we performed EXOFASTv2 global fits to the available transit and radial velocity data sets, together with the Gaia DR3 parallax, isochrones, and spectral energy distributions. To assess the potential for atmospheric characterization, we compared the multicolour transit depths with a flat line and a clear atmosphere model. We consistently refined the transit and physical parameters. We improved the orbital period and ephemeris estimates, and found no evidence for TTVs or orbital decay. The MuSCAT2 broad-band transmission spectra of HAT-P-19b and HAT-P-65b are consistent with previously published low-resolution transmission spectra. We also found that, except for HAT-P-65b, the assumption of a planetary atmosphere can improve the fit to the MuSCAT2 data. In particular, we identified HAT-P-55b as a priority target among these four planets for further atmospheric studies using transmission spectroscopy.
650 7a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe
650 7a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng
653 a planetary systems
653 a planets and satellites: fundamental parameters
653 a planets and satellites: individual: (HAT-P-19b, HAT-P-51b, HAT-P-55b, HAT-P-65b)
653 a techniques: photometric
700a Chen, G.u Purple Mountain Observatory, Chinese Academy of Sciences,University of the Chinese Academy of Sciences4 aut
700a Pallé, E.u University of La Laguna (ULL),Instituto de Astrofísica de Canarias4 aut
700a Murgas, F.u University of La Laguna (ULL),Instituto de Astrofísica de Canarias4 aut
700a García, N. Abreuu University of La Laguna (ULL),Instituto de Astrofísica de Canarias4 aut
700a de Leon, J.u University of Tokyo4 aut
700a Enoc, G.u Instituto de Astrofísica de Canarias,University of La Laguna (ULL)4 aut
700a Esparza-Borges, E.u Instituto de Astrofísica de Canarias,University of La Laguna (ULL)4 aut
700a Fukuda, I.u University of Tokyo4 aut
700a Fukui, A.u Instituto de Astrofísica de Canarias,University of Tokyo4 aut
700a Galán, D.u University of La Laguna (ULL),Instituto de Astrofísica de Canarias4 aut
700a Hayashi, Y.u University of Tokyo4 aut
700a Isogai, K.u University of Tokyo,Kyoto University4 aut
700a Kagetani, T.u University of Tokyo4 aut
700a Kawauchi, K.u University of Tokyo,Ritsumeikan University, Biwako-Kusatsu4 aut
700a Korth, J.u Lund University,Lunds universitet,Astrofysik,Fysiska institutionen,Institutioner vid LTH,Lunds Tekniska Högskola,Astrophysics,Department of Physics,Departments at LTH,Faculty of Engineering, LTH4 aut0 (Swepub:lu)ju7237ko
700a Livingston, J. H.u National Institutes of Natural Sciences - AstroBiology Center,National Astronomical Observatory of Japan,Graduate University for Advanced Studies4 aut
700a Luque, R.4 aut
700a Ma, Y.u Purple Mountain Observatory, Chinese Academy of Sciences4 aut
700a Madrigal-Aguado, A.u Instituto de Astrofísica de Canarias4 aut
700a Meni, P.u Instituto de Astrofísica de Canarias,University of La Laguna (ULL)4 aut
700a Rodriguez, P. Montañesu Instituto de Astrofísica de Canarias4 aut
700a Mori, M.u University of Tokyo4 aut
700a Torres, S. Muñozu Instituto de Astrofísica de Canarias4 aut
700a Narita, N.u Instituto de Astrofísica de Canarias,University of Tokyo,National Institutes of Natural Sciences - AstroBiology Center4 aut
700a Orell-Miquel, J.u University of La Laguna (ULL),Instituto de Astrofísica de Canarias4 aut
700a Parviainen, H.u University of La Laguna (ULL),Instituto de Astrofísica de Canarias4 aut
700a Peláez-Torres, A.u University of La Laguna (ULL),Instituto de Astrofísica de Canarias4 aut
700a Stangret, M.u INAF - Osservatorio Astronomico di Padova4 aut
700a Tamura, M.u National Astronomical Observatory of Japan,National Institutes of Natural Sciences - AstroBiology Center,University of Tokyo4 aut
700a Watanabe, N.u University of Tokyo4 aut
710a University of Science and Technology of Chinab Purple Mountain Observatory, Chinese Academy of Sciences4 org
773t Monthly Notices of the Royal Astronomical Societyg 528:2, s. 1930-1944q 528:2<1930-1944x 0035-8711
856u http://dx.doi.org/10.1093/mnras/stae072x freey FULLTEXT
8564 8u https://lup.lub.lu.se/record/f8e2fe08-486b-4fa3-815f-9e92cc9e22f6
8564 8u https://doi.org/10.1093/mnras/stae072

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