Desika Narayanan

University of Copenhagen — Denmark

Physics and Astronomy · Physical Sciences

59h-index12.7kcitations357works5.22yr avg
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Research Topics

Galaxies: Formation, Evolution, Phenomena(238), Astrophysics and Star Formation Studies(180), Astronomy and Astrophysical Research(160), Stellar, planetary, and galactic studies(118), Gamma-ray bursts and supernovae(36)

Publications358 total

A Census of Star-formation and Gas Mass Tracers in Two Lensed <i>z</i>  ∼ 4 Dusty Star-forming Galaxies
The Astrophysical Journal·2026Open Access
The AURORA Survey: Multiple Balmer and Paschen Emission Lines for Individual Star-forming Galaxies at <i>z</i>  = 1.5–4.4. I. A Diversity of Nebular Attenuation Curves and Evidence for Non-unity Dust Covering Fractions
The Astrophysical Journal·2026Open Access
Molecular Gas Excitation in z ~ 0.7 Gas-Rich Post-starburst Galaxies from SQuIGGLE
arXiv (Cornell University)·2026Open Access
Molecular Gas Excitation in z ~ 0.7 Gas-Rich Post-starburst Galaxies from SQuIGGLE
arXiv (Cornell University)·2026Open Access
Bright [C <scp>II</scp> ]158 <i>μ</i> m Streamers as a Beacon for Giant Galaxy Formation in SPT2349-56 at <i>z</i> = 4.3
The Astrophysical Journal·2026Open Access
Bright [C <scp>II</scp> ]158 <i>μ</i> m Streamers as a Beacon for Giant Galaxy Formation in SPT2349-56 at <i>z</i> = 4.3
The Astrophysical Journal·2026Open Access
How To Use Thermal Dust Continuum Emission To Measure The Physical Properties Of Dusty Astrophysical Objects
arXiv (Cornell University)·2026Open Access
How To Use Thermal Dust Continuum Emission To Measure The Physical Properties Of Dusty Astrophysical Objects
ArXiv.org·2026Open Access
A census of star-formation and gas mass tracers in two lensed $z \sim 4$ dusty star-forming galaxies
ArXiv.org·2026Open Access
A census of star-formation and gas mass tracers in two lensed $z \sim 4$ dusty star-forming galaxies
arXiv (Cornell University)·2026Open Access
The AURORA Survey: Robust Helium Abundances at High Redshift Reveal a Subpopulation of Helium-enhanced Galaxies in the Early Universe
The Astrophysical Journal·2025Open Access
ALMA Reveals Diverse Dust-to-gas Mass Ratios and Quenching Modes in Old Quiescent Galaxies
The Astrophysical Journal Letters·2025Open Access
SQuIGGLE: Buried Star Formation Cannot Explain the Rapidly Fading CO(2-1) Luminosity in Massive, z ~ 0.7 Post-starburst Galaxies
Universität Zürich, ZORA·2025Open Access
SQuIGG <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mover> <mml:mrow> <mml:mi>L</mml:mi> </mml:mrow> <mml:mrow> <mml:mo>→</mml:mo> </mml:mrow> </mml:mover> </mml:math> E: Buried Star Formation Cannot Explain the Rapidly Fading CO(2–1) Luminosity in Massive, <i>z</i> ∼ 0.7 Post-starburst Galaxies
The Astronomical Journal·2025Open Access
The AURORA Survey: Tracing Galactic Outflows at <i>z</i> ≳ 2.5 with JWST/NIRSpec Near-ultraviolet Absorption Lines
The Astrophysical Journal·2025Open Access
Unusually High Gas-to-dust Ratios Observed in High-redshift Quiescent Galaxies
The Astrophysical Journal Letters·2025· 1 citedOpen Access
Unusually High Gas-to-dust Ratios Observed in High-redshift Quiescent Galaxies
Universität Zürich, ZORA·2025Open Access
Cold Gas in a Post-starburst Pair in the <i>z</i> ∼ 1.4 HeavyMetal Survey: Major Mergers as a Pathway to Retain Gas in Quenched Galaxies
The Astrophysical Journal·2025· 1 citedOpen Access
The ALPINE-CRISTAL-JWST Survey: The Fast Metal Enrichment of Massive Galaxies at z~5
arXiv (Cornell University)·2025Open Access
Discovery of red galaxy candidates at z ~ 12: Early dust growth or significant nebular emission with high-temperature stars?
arXiv (Cornell University)·2025Open Access
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Frequent Co-authors

Christopher C. Hayward(18), Romeel Davé(13), Lars Hernquist(13), Philip F. Hopkins(10), M. Béthermin(9), Thomas J. Cox(8), Justin Spilker(7), E. Ibar(6), Pascal A. Oesch(6), J. D. Vieira(6), C. De Breuck(6), T. R. Greve(6), Dušan Kereš(5), J. E. Geach(5), Mark R. Krumholz(5), Andreas L. Faisst(5), Sune Toft(5), Daniel P. Marrone(5), Manuel Aravena(5), Yashar Hezaveh(5)