Physical properties, transmission and emission spectra of the WASP-19 planetary system from multi-colour photometry

Eamonn Kerins, L {Mancini}, S {Ciceri}, G {Chen}, J {Tregloan-Reed}, J J {Fortney}, J {Southworth}, T G {Tan}, M {Burgdorf}, S {Calchi Novati}, M {Dominik}, X-S {Fang}, F {Finet}, T {Gerner}, S {Hardis}, T C {Hinse}, U G {J{\o}rgensen}, C {Liebig}, N {Nikolov}, D {Ricci}S {Schäfer}, F {Schönebeck}, J {Skottfelt}, O {Wertz}, K A {Alsubai}, V {Bozza}, P {Browne}, P {Dodds}, S-H {Gu}, K {Harps{\o}e}, T {Henning}, M {Hundertmark}, J {Jessen-Hansen}, N {Kains}, E {Kerins}, H {Kjeldsen}, M N {Lund}, M {Lundkvist}, N {Madhusudhan}, M {Mathiasen}, M T {Penny}, S {Prof}, S {Rahvar}, K {Sahu}, G {Scarpetta}, C {Snodgrass}, J {Surdej}

    Research output: Contribution to journalArticlepeer-review

    Original languageEnglish
    Pages (from-to)2-18
    Number of pages17
    JournalMonthly Notices of the Royal Astronomical Society
    Volume436
    DOIs
    Publication statusPublished - Nov 2013

    Keywords

    • techniques: photometric
    • stars: fundamental parameters
    • stars: individual: WASP-19
    • planetary systems
    • starspots

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