The Low-redshift Lyman Continuum Survey. I. New, Diverse Local Lyman Continuum Emitters

Autor: Sophia R. Flury, Anne E. Jaskot, Harry C. Ferguson, Gábor Worseck, Kirill Makan, John Chisholm, Alberto Saldana-Lopez, Daniel Schaerer, Stephan McCandliss, Bingjie Wang, N. M. Ford, Timothy Heckman, Zhiyuan Ji, Mauro Giavalisco, Ricardo Amorin, Hakim Atek, Jeremy Blaizot, Sanchayeeta Borthakur, Cody Carr, Marco Castellano, Stefano Cristiani, Stephane De Barros, Mark Dickinson, Steven L. Finkelstein, Brian Fleming, Fabio Fontanot, Thibault Garel, Andrea Grazian, Matthew Hayes, Alaina Henry, Valentin Mauerhofer, Genoveva Micheva, M. S. Oey, Goran Ostlin, Casey Papovich, Laura Pentericci, Swara Ravindranath, Joakim Rosdahl, Michael Rutkowski, Paola Santini, Claudia Scarlata, Harry Teplitz, Trinh Thuan, Maxime Trebitsch, Eros Vanzella, Anne Verhamme, Xinfeng Xu

Publikováno v: The Astrophysical Journal Supplement Series
The Astrophysical Journal Supplement Series, 2022, 260 (1), pp.1. ⟨10.3847/1538-4365/ac5331⟩
The Astrophysical Journal Supplement Series, 260:1. IOP PUBLISHING LTD

The origins of Lyman continuum (LyC) photons responsible for the reionization of the universe are as of yet unknown and highly contested. Detecting LyC photons from the epoch of reionization is not possible due to absorption by the intergalactic medi

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ed33be95fb3d3e9a40d691d1e68dd9dd
https://hal.science/hal-03817541

Five Key Exoplanet Questions Answered via the Analysis of 25 Hot-Jupiter Atmospheres in Eclipse

Autor: Q. Changeat, B. Edwards, A. F. Al-Refaie, A. Tsiaras, J. W. Skinner, J. Y. K. Cho, K. H. Yip, L. Anisman, M. Ikoma, M. F. Bieger, O. Venot, S. Shibata, I. P. Waldmann, G. Tinetti

Publikováno v: The Astrophysical Journal Supplement Series
The Astrophysical Journal Supplement Series, IOPscience 2022, 260, ⟨10.3847/1538-4365/ac5cc2⟩

Population studies of exoplanets are key to unlocking their statistical properties. So far the inferred properties have been mostly limited to planetary, orbital and stellar parameters extracted from, e.g., Kepler, radial velocity, and GAIA data. Mor

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bbf6fba1d342851660905c2774252d23
https://doi.org/10.3847/1538-4365/ac5cc2