PySpecKit: Python Spectroscopic Toolkit A Ginsburg, J Mirocha Astrophysics Source Code Library, ascl: 1109.001, 2011 | 236 | 2011 |
What does the first highly redshifted 21-cm detection tell us about early galaxies? J Mirocha, SR Furlanetto Monthly Notices of the Royal Astronomical Society 483 (2), 1980-1992, 2019 | 179 | 2019 |
The global 21-cm signal in the context of the high-z galaxy luminosity function J Mirocha, SR Furlanetto, G Sun Monthly Notices of the Royal Astronomical Society 464 (2), 1365-1379, 2017 | 128 | 2017 |
HERA phase I limits on the cosmic 21 cm signal: constraints on astrophysics and cosmology during the epoch of reionization Z Abdurashidova, JE Aguirre, P Alexander, ZS Ali, Y Balfour, R Barkana, ... The Astrophysical Journal 924 (2), 51, 2022 | 112 | 2022 |
Decoding the X-ray properties of pre-reionization era sources J Mirocha Monthly Notices of the Royal Astronomical Society 443 (2), 1211-1223, 2014 | 93 | 2014 |
A minimalist feedback-regulated model for galaxy formation during the epoch of reionization SR Furlanetto, J Mirocha, RH Mebane, G Sun Monthly Notices of the Royal Astronomical Society 472 (2), 1576-1592, 2017 | 85 | 2017 |
Interpreting the Global 21-cm Signal from High Redshifts. II. Parameter Estimation for Models of Galaxy Formation J Mirocha, GJA Harker, JO Burns The Astrophysical Journal 813 (1), 11, 2015 | 74 | 2015 |
The effects of population III radiation backgrounds on the cosmological 21-cm signal RH Mebane, J Mirocha, SR Furlanetto Monthly Notices of the Royal Astronomical Society 493 (1), 1217-1226, 2020 | 72 | 2020 |
Improved Constraints on the 21 cm EoR Power Spectrum and the X-Ray Heating of the IGM with HERA Phase I Observations T Adams, JE Aguirre, P Alexander, ZS Ali, R Baartman, Y Balfour, ... The Astrophysical Journal 945 (2), 124, 2023 | 67 | 2023 |
Unique signatures of Population III stars in the global 21-cm signal J Mirocha, RH Mebane, SR Furlanetto, K Singal, D Trinh Monthly Notices of the Royal Astronomical Society 478 (4), 5591-5606, 2018 | 64 | 2018 |
A space-based observational strategy for characterizing the first stars and galaxies using the redshifted 21 cm global spectrum JO Burns, R Bradley, K Tauscher, S Furlanetto, J Mirocha, R Monsalve, ... The Astrophysical Journal 844 (1), 33, 2017 | 63 | 2017 |
The Persistence of Population III Star Formation RH Mebane, J Mirocha, SR Furlanetto Monthly Notices of the Royal Astronomical Society 479 (4), 4544-4559, 2018 | 62 | 2018 |
High-mass X-ray binaries in nearby metal-poor galaxies: on the contribution to nebular He ii emission P Senchyna, DP Stark, J Mirocha, AE Reines, S Charlot, T Jones, ... Monthly Notices of the Royal Astronomical Society 494 (1), 941-957, 2020 | 61 | 2020 |
Balancing the efficiency and stochasticity of star formation with dust extinction in z ≳ 10 galaxies observed by JWST J Mirocha, SR Furlanetto Monthly Notices of the Royal Astronomical Society 519 (1), 843-853, 2023 | 56 | 2023 |
Interpreting the Global 21 cm Signal from High Redshifts. I. Model-independent constraints J Mirocha, GJA Harker, JO Burns The Astrophysical Journal 777 (2), 118, 2013 | 54 | 2013 |
Optimized Multi-frequency Spectra for Applications in Radiative Feedback and Cosmological Reionization J Mirocha, S Skory, JO Burns, JH Wise The Astrophysical Journal 756 (1), 94, 2012 | 43 | 2012 |
astroquery v0. 3.1 A Ginsburg, M Parikh, J Woillez Zenodo, doi 10, 2016 | 39* | 2016 |
Bursty star formation during the Cosmic Dawn driven by delayed stellar feedback SR Furlanetto, J Mirocha Monthly Notices of the Royal Astronomical Society 511 (3), 3895-3909, 2022 | 36 | 2022 |
Parametrizations of the 21-cm global signal and parameter estimation from single-dipole experiments GJA Harker, J Mirocha, JO Burns, JR Pritchard Monthly Notices of the Royal Astronomical Society 455 (4), 3829-3840, 2016 | 35 | 2016 |
Global 21 cm Signal Extraction from Foreground and Instrumental Effects. II. Efficient and Self-consistent Technique for Constraining Nonlinear Signal Models D Rapetti, K Tauscher, J Mirocha, JO Burns The Astrophysical Journal 897 (2), 174, 2020 | 30 | 2020 |