Observing transiting planets with JWST (Corrigendum)
Prime targets and their synthetic spectral observations
1 Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany
e-mail: molliere@mpia.de
2 Irfu, CEA, Université Paris-Saclay, 91191 Gif-sur-Yvette, France
3 AIM, Université Paris Diderot, 91191 Gif-sur-Yvette, France
4 SRON Netherlands Institute for Space Research, Sorbonnelaan 2, 3584 CA Utrecht, The Netherlands
5 Astronomical institute Anton Pannekoek, University of Amsterdam, Science Park 904, 1098 XH Amsterdam, The Netherlands
Key words: methods: numerical / planets and satellites: atmospheres / radiative transfer / errata, addenda
In Sect. 6.2 it was incorrectly stated that NIRISS provides little diagnostic power to distinguish between the various cases of strongly irradiated planets without heat re-distribution. In fact, from radiometric considerations alone, NIRISS is as good or better than NIRSpec in these cases, as is apparent in Fig. 7.
© ESO, 2017