Emilio Romano-Díaz

Physics and Astronomy · Physical Sciences

20h-index1.2kcitations55works1.82yr avg
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Research Topics

Galaxies: Formation, Evolution, Phenomena(41), Astronomy and Astrophysical Research(32), Stellar, planetary, and galactic studies(17), Cosmology and Gravitation Theories(12), Astrophysics and Star Formation Studies(12)

Publications55 total

Probing the warm dark matter mass with [C II] intensity mapping
Springer Link (Chiba Institute of Technology)·2026
Probing the warm dark matter mass with [C II] intensity mapping
Astronomy and Astrophysics·2026Open Access
Modeling Cosmological Evolution of Jetted Seyfert Galaxies for <i>z</i>  ≲ 10
The Astrophysical Journal·2025Open Access
Constraining the [C II] luminosity function from the power spectrum of line-intensity maps at redshift 3.6
Astronomy and Astrophysics·2025Open Access
The [C II] line emission as an interstellar medium probe in the MARIGOLD galaxies
Astronomy and Astrophysics·2025· 3 citedOpen Access
Jetted Seyfert Galaxies at <i>z</i> = 0: Simulating Feedback Effects on Galactic Morphology and Beyond
The Astrophysical Journal·2025· 3 citedOpen Access
Jetted Seyfert Galaxies at z = 0: Simulating Feedback Effects on\n Galactic Morphology and Beyond
arXiv (Cornell University)·2024Open Access
The [C II] line emission as an interstellar medium probe in the MARIGOLD galaxies
arXiv (Cornell University)·2024Open Access
[CII] line intensity mapping the epoch of reionization with the Prime-Cam on FYST II. CO foreground masking based on an external catalog
arXiv (Cornell University)·2024Open Access
HYACINTH: HYdrogen And Carbon chemistry in the INTerstellar medium in Hydro simulations
Springer Link (Chiba Institute of Technology)·2024· 1 citedOpen Access
Connecting stellar and galactic scales: Energetic feedback from stellar wind bubbles to supernova remnants
Astronomy and Astrophysics·2024· 6 citedOpen Access
HYACINTH: HYdrogen And Carbon chemistry in the INTerstellar medium in Hydro simulations
Astronomy and Astrophysics·2024· 7 citedOpen Access
Dissecting cosmological filaments at high redshifts: emergence of spaghetti-type flow inside DM haloes
Monthly Notices of the Royal Astronomical Society·2023· 3 citedOpen Access
Dissecting Cosmological Filaments at High Redshifts: Emergence of Spaghetti-type Flow Inside DM Haloes
arXiv (Cornell University)·2023Open Access
The Ly α, C <scp>iv</scp>, and He <scp>ii</scp>nebulae around J1000+0234: a galaxy pair at the centre of a galaxy overdensity at<i>z</i> = 4.5
Monthly Notices of the Royal Astronomical Society·2023· 7 citedOpen Access
Bringing Stellar Evolution and Feedback Together: Summary of Proposals from the Lorentz Center Workshop
Publications of the Astronomical Society of the Pacific·2023· 10 citedOpen Access
Bringing Stellar Evolution &amp; Feedback Together: Summary of proposals from the Lorentz Center Workshop, 2022
arXiv (Cornell University)·2023Open Access
Modeling Evolution of Galactic Bars at Cosmic Dawn
The Astrophysical Journal·2022· 24 citedOpen Access
Mechanical feedback from stellar winds with an application to galaxy formation at high redshift
Monthly Notices of the Royal Astronomical Society·2022· 13 citedOpen Access
Emergence of galactic morphologies at cosmic dawn: input from numerical modelling
Monthly Notices of the Royal Astronomical Society·2022· 8 citedOpen Access
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Frequent Co-authors

Isaac Shlosman(18), C. Porciani(13), B. Magnelli(7), Prachi Khatri(7), F. Bertoldi(6), Yehuda Hoffman(5), Clayton Heller(5), Eric F. Jiménez-Andrade(5), L. Grassitelli(5), Matteo Tomassetti(5), Aaron D. Ludlow(5), Da Bi(5), Cristiano Porciani(5), Enrico Garaldi(4), Kevin C. Harrington(4), V. Smolčić(4), Mikolaj Borzyszkowski(3), T. Bădescu(3), Sune Toft(3), A. Karim(3)