@article{https://doi.org/10.48550/arxiv.2011.06329,
doi = {10.48550/ARXIV.2011.06329},
url = {https://arxiv.org/abs/2011.06329},
author = {Chen,
G. and Palle,
E. and Parviainen,
H. and Wang,
H. and van Boekel,
R. and Murgas,
F. and Yan,
F. and Bejar,
V. J. S. and Casasayas-Barris,
N. and Crouzet,
N. and Esparza-Borges,
E. and Fukui,
A. and Garai,
Z. and Kawauchi,
K. and Kurita,
S. and Kusakabe,
N. and de Leon,
J. P. and Livingston,
J. and Luque,
R. and Madrigal-Aguado,
A. and Mori,
M. and Narita,
N. and Nishiumi,
T. and Oshagh,
M. and Sanchez-Benavente,
M. and Tamura,
M. and Terada,
Y. and Watanabe,
N.},
keywords = {Earth and Planetary Astrophysics (astro-ph.EP),
Solar and Stellar Astrophysics (astro-ph.SR),
FOS: Physical sciences,
FOS: Physical sciences},
title = {An enhanced slope in the transmission spectrum of the hot Jupiter WASP-104b},
publisher = {arXiv},
year = {2020},
copyright = {arXiv.org perpetual,
non-exclusive license} }