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Monthly Notices of the Royal Astronomical Society|March 3, 2022
Quantifying acetaldehyde in astronomical ices and laboratory analogues: IR spectra, intensities, 13C shifts, and radiation chemistryReggie L Hudson, Robert F FerranteMonthly Notices of the Royal Astronomical Society|June 14, 2017
A unified framework for constructing, tuning and assessing photometric redshift density estimates in a selection bias settingP E Freeman, R Izbicki, A B LeeMonthly Notices of the Royal Astronomical Society|August 6, 2020
On the redshift distribution and physical properties of ACT-selected DSFGsT Su, T A Marriage, V Asboth, et al.Monthly Notices of the Royal Astronomical Society|July 7, 2020
A Novel multidimensional Boltzmann neutrino transport scheme for core-collapse supernovaeConrad Chan, Bernhard MüllerMonthly Notices of the Royal Astronomical Society|April 19, 2021
Search for L5 Earth Trojans with DECamLarissa Markwardt, D W Gerdes, R Malhotra, et al.Monthly Notices of the Royal Astronomical Society|January 1, 1989
Can interstellar H2S be formed via gas-phase reactions? Calculations concerning the rates of the ternary and radiative association reactions between HS+ and H2E Herbst, D J DeFrees, W KochMonthly Notices of the Royal Astronomical Society|February 5, 2019
Gas kinematics in FIRE simulated galaxies compared to spatially unresolved HI observationsKareem El-Badry, Jeremy Bradford, Eliot Quataert, et al.Monthly Notices of the Royal Astronomical Society|January 22, 2019
slug IV: a novel forward-modelling method to derive the demographics of star clustersMark R Krumholz, Angela Adamo, Michele Fumagalli, et al.Monthly Notices of the Royal Astronomical Society|January 1, 2019
SIDM on FIRE: hydrodynamical self-interacting dark matter simulations of low-mass dwarf galaxiesVictor H Robles, James S Bullock, Oliver D Elbert, et al.Monthly Notices of the Royal Astronomical Society|January 2, 2019
ETHOS - an effective theory of structure formation: predictions for the high-redshift Universe - abundance of galaxies and reionizationMark R Lovell, Jesús Zavala, Mark Vogelsberger, et al.Pageof 13