Sökning: WFRF:(Andersen Henning) > Physical properties...
Fältnamn | Indikatorer | Metadata |
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000 | 03613naa a2200757 4500 | |
001 | oai:DiVA.org:su-172055 | |
003 | SwePub | |
008 | 190823s2019 | |||||||||||000 ||eng| | |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-1720552 URI |
024 | 7 | a https://doi.org/10.1093/mnras/stz6612 DOI |
040 | a (SwePub)su | |
041 | a engb eng | |
042 | 9 SwePub | |
072 | 7 | a ref2 swepub-contenttype |
072 | 7 | a art2 swepub-publicationtype |
100 | 1 | a Mancini, L.4 aut |
245 | 1 0 | a Physical properties and transmission spectrum of the WASP-74 planetary system from multiband photometry |
264 | c 2019-03-14 | |
264 | 1 | b Oxford University Press (OUP),c 2019 |
338 | a print2 rdacarrier | |
520 | a We present broad-band photometry of 11 planetary transits of the hot Jupiter WASP-74 b, using three medium-class telescopes and employing the telescope-defocusing technique. Most of the transits were monitored through I filters and one was simultaneously observed in five optical (U, g', r', i', z') and three near-infrared (J, H, K) passbands, for a total of 18 light curves. We also obtained new high-resolution spectra of the host star. We used these new data to review the orbital and physical properties of the WASP-74 planetary system. We were able to better constrain the main system characteristics, measuring smaller radius and mass for both the hot Jupiter and its host star than previously reported in the literature. Joining our optical data with those taken with the HST in the near infrared, we built up an observational transmission spectrum of the planet, which suggests the presence of strong optical absorbers, as TiO and VO gases, in its atmosphere. | |
650 | 7 | a NATURVETENSKAPx Fysik0 (SwePub)1032 hsv//swe |
650 | 7 | a NATURAL SCIENCESx Physical Sciences0 (SwePub)1032 hsv//eng |
653 | a techniques: photometric | |
653 | a stars: fundamental parameters | |
653 | a stars: individual: WASP-74 | |
653 | a planetary systems | |
700 | 1 | a Southworth, J.4 aut |
700 | 1 | a Mollière, P.4 aut |
700 | 1 | a Tregloan-Reed, J.4 aut |
700 | 1 | a Juvan, I. G.4 aut |
700 | 1 | a Chen, G.4 aut |
700 | 1 | a Sarkis, P.4 aut |
700 | 1 | a Bruni, I.4 aut |
700 | 1 | a Ciceri, Simonau Stockholms universitet,Institutionen för astronomi4 aut0 (Swepub:su)scice |
700 | 1 | a Andersen, M. I.4 aut |
700 | 1 | a Bozza, V.4 aut |
700 | 1 | a Bramich, D. M.4 aut |
700 | 1 | a Burgdorf, M.4 aut |
700 | 1 | a D'Ago, G.4 aut |
700 | 1 | a Dominik, M.4 aut |
700 | 1 | a Evans, D. F.4 aut |
700 | 1 | a Figuera Jaimes, R.4 aut |
700 | 1 | a Fossati, L.4 aut |
700 | 1 | a Henning, Th.4 aut |
700 | 1 | a Hinse, T. C.4 aut |
700 | 1 | a Hundertmark, M.4 aut |
700 | 1 | a Jørgensen, U. G.4 aut |
700 | 1 | a Kerins, E.4 aut |
700 | 1 | a Korhonen, H.4 aut |
700 | 1 | a Küffmeier, M.4 aut |
700 | 1 | a Longa, P.4 aut |
700 | 1 | a Peixinho, N.4 aut |
700 | 1 | a Popovas, A.4 aut |
700 | 1 | a Rabus, M.4 aut |
700 | 1 | a Rahvar, S.4 aut |
700 | 1 | a Skottfelt, J.4 aut |
700 | 1 | a Snodgrass, C.4 aut |
700 | 1 | a Tronsgaard, R.4 aut |
700 | 1 | a Wang, Y.4 aut |
700 | 1 | a Wertz, O.4 aut |
710 | 2 | a Stockholms universitetb Institutionen för astronomi4 org |
773 | 0 | t Monthly notices of the Royal Astronomical Societyd : Oxford University Press (OUP)g 485:4, s. 5168-5179q 485:4<5168-5179x 0035-8711x 1365-2966 |
856 | 4 | u https://arxiv.org/pdf/1903.02800 |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-172055 |
856 | 4 8 | u https://doi.org/10.1093/mnras/stz661 |
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