DN
Desika Narayanan
astro-ph.GAastro-ph.COastro-ph.IMastro-phastro-ph.HEastro-ph.SRcs.LGcs.CVastro-ph.EPcs.AI
On Valency
published · living versionsW_unu28bt7·v1 · currentpublished
Why a Multi-Cycle Treasury Program is Essential to Maximize JWST's Scientific Contributions to Galaxy Formation
with Genesis Community, Alice Shapley, Steven L. Finkelstein, Rachel S. Somerville +416
1 version
Preprints & journals
214 papers in the corpus · 2003–2026The Impact of an AGN on PAH Spectral Features in Galaxy Evolution Simulations: Continuum Dilution and Excitation of PAHs2610.24778v1 · Grant P. Donnelly, Desika Narayanan, Paul Torrey et al.2026 · 0 citationsarXiv
Simulations of Dust Content and Attenuation in Galaxies2610.19379v1 · Dhruv T. Zimmerman, Jed McKinney, Desika Narayanan et al.2026 · 0 citationsarXiv
SQuIGGLE: Radio AGN Found Predominantly in Young, Gas-rich Post-starburst Galaxies at z ~ 0.72610.19146v1 · Vincenzo R. D'Onofrio, Justin S. Spilker, Krista L. Smith et al.2026 · 0 citationsarXiv
The DAWN JWST Archive: A spectroscopically-informed population study of the physical properties of galaxies at z>22610.15901v1 · Rashmi Gottumukkala, Gabriel Brammer, Sune Toft et al.2026 · 0 citationsarXiv
Unveiling the Origins of the Molecular Gas Reservoirs in Recently Quenched Massive Galaxies2610.06680v1 · E. Savitch, D. Narayanan, D. J. Setton et al.2026 · 0 citationsarXiv
The abundance and emission of PAHs from the local to early Universe2609.35533v1 · Massimiliano Parente, Desika Narayanan, Paul Torrey et al.2026 · 0 citationsarXiv
SQuIGGE: Spatially resolved NIRSpec Pa reveals that the most CO-luminous, post-starburst galaxies exhibit falling---but still active---star formation behind optically thick dust2609.31307v1 · David J. Setton, Jenny E. Greene, Rachel Bezanson et al.2026 · 0 citationsarXiv
ALMA Chemical Evolution (ACE) survey: an overview -- extending dust and gas inference to low metallicities at cosmic noon2609.21604v1 · Irene Shivaei, Gergo Popping, Leindert A. Boogaard et al.2026 · 0 citationsarXiv
ALMA Chemical Evolution (ACE) survey: The gas fundamental metallicity relation at cosmic noon2609.20921v2 · I. Langan, I. Shivaei, G. Popping et al.2026 · 0 citationsarXiv
ALMA Chemical Evolution (ACE) survey: dust-to-gas ratios in sub-solar metallicity galaxies at cosmic noon2609.20926v1 · N. N. Geesink, G. Popping, L. A. Boogaard et al.2026 · 0 citationsarXiv
ALMA Chemical Evolution (ACE) Survey: Molecular gas properties of low-mass, low-metallicity galaxies at cosmic noon2609.21072v1 · Gergo Popping, Ivanna Langan, Nikki N. Geesink et al.2026 · 0 citationsarXiv
Dust and PAHs in late-stage galaxy evolution: Imprints of TP-AGB dust injection, grain growth and AGN feedback in high-z quiescent galaxies with JWST and ALMA2608.27571v2 · D. Donevski, A. Nanni, K. E. Whitaker et al.2026 · 0 citationsarXiv
JWST Whirlpool Galaxy Treasury: Mid-Infrared Emission in M51 and its Relation to Gas Column and Star Formation2608.16802v1 · Mansi Padave, Karin M. Sandstrom, Daniel A. Dale et al.2026 · 0 citationsarXiv
The HII Regions' Molecular Law of Star Formation2608.00918v1 · Daniela Calzetti, Drew Lapeer, Robert C. Kennicutt et al.2026 · 0 citationsarXiv
JWST spectroscopy of galaxies at : Damped Ly absorbers reveal efficient star formation and hidden redshift biases2606.30787v1 · Kasper E. Heintz, Clara L. Pollock, Joris Witstok et al.2026 · 0 citationsarXiv
Reimagining SED Fitting with Cosmological Galaxy Simulations and Machine Learning2606.19447v1 · Dhruv T. Zimmerman, Desika Narayanan2026 · 0 citationsarXiv
Dust in the Average Galaxy: Attenuation, Emission, and Opacity from 2606.17270v2 · Caitlin M. Casey, Hollis B. Akins, Andrew J. Battisti et al.2026 · 1 citationarXiv
The AURORA Survey: Multiple Balmer and Paschen Emission Lines for Individual Star-forming Galaxies at z=1.5-4.4. II. Implications for Nebular Dust Corrections, Nebular SFRs, and Differential Reddening2605.30427v1 · Naveen A. Reddy, Alice E. Shapley, Ryan L. Sanders et al.2026 · 0 citationsarXiv
Dust and Grain Size Evolution in Galaxy Simulations: What Matters and What Does Not2604.06314v2 · Massimiliano Parente, Desika Narayanan, Paul Torrey2026 · 2 citationsarXiv
The Drivers of Cosmic Dust Temperature Evolution2603.04505v2 · Massimiliano Parente, Francesco Salvestrini, Gian Luigi Granato et al.2026 · 1 citationarXiv
Tracing the AGN-Merger Connection: insights from cosmological simulations and JWST mock observations2603.03439v1 · Hannah Jhee, Ena Choi, Rachel S. Somerville et al.2026 · 0 citationsarXiv
Molecular Gas Excitation in z ~ 0.7 Gas-Rich Post-starburst Galaxies from SQuIGGLE2602.17766v2 · Vincenzo R. D'Onofrio, Justin S. Spilker, Rachel Bezanson et al.2026 · 0 citationsarXiv
How To Use Thermal Dust Continuum Emission To Measure The Physical Properties Of Dusty Astrophysical Objects2601.10989v1 · Yancy L. Shirley (1, Jeffrey G. Mangum, Desika Narayanan et al.2026 · 0 citationsarXiv
A census of star-formation and gas mass tracers in two lensed dusty star-forming galaxies2601.04133v1 · David Vizgan, Joaquin D. Vieira, Justin S. Spilker et al.2026 · 0 citationsarXiv
Linking Warm Dark Matter to Merger Tree Histories via Deep Learning Networks2511.05367v1 · Ilem Leisher, Paul Torrey, Alex M. Garcia et al.2025 · 0 citationsarXiv
The ALPINE-CRISTAL-JWST Survey: The Fast Metal Enrichment of Massive Galaxies at z~52510.16106v2 · Andreas L. Faisst, Lun-Jun Liu, Yohan Dubois et al.2025 · 4 citationsarXiv
Discovery of red galaxy candidates at z ~ 12: Early dust growth or significant nebular emission with high-temperature stars?2510.13240v1 · Ikki Mitsuhashi, Katherine A. Suess, Joel Leja et al.2025 · 0 citationsarXiv
Evidence for inefficient dust production in a massive, metal-rich galaxy at uncovered by JWST and ALMA2510.07936v2 · Kasper E. Heintz, Darach Watson, Francesco Valentino et al.2025 · 1 citationarXiv
The Growth of Dust in Galaxies in the First Billion Years with Applications to Blue Monsters2509.18266v2 · Desika Narayanan, Paul Torrey, Daniel Stark et al.2025 · 7 citationsarXiv
The Metallicity Dependence of PAH Emission in Galaxies II: Insights from JWST/NIRCam Imaging of the Smallest Dust Grains in M1012509.18347v2 · Cory M. Whitcomb, J.-D. T. Smith, Elizabeth Tarantino et al.2025 · 3 citationsarXiv
ALMA reveals diverse dust-to-gas mass ratios and quenching modes in old quiescent galaxies2509.10079v1 · Giuliano Lorenzon, Darko Donevski, Allison W. S. Man et al.2025 · 2 citationsarXiv
Bright [CII]158m Streamers as a Beacon for Giant Galaxy Formation in SPT2349$-$56 at 2509.08035v1 · Nikolaus Sulzenauer, Axel Weiß, Ryley Hill et al.2025 · 2 citationsarXiv
SQuIGGE: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, post-starburst galaxies2509.00148v1 · David J. Setton, Justin S. Spilker, Rachel Bezanson et al.2025 · 0 citationsarXiv
The AURORA Survey: High-Redshift Empirical Metallicity Calibrations from Electron Temperature Measurements at z=2-102508.10099v2 · Ryan L. Sanders, Alice E. Shapley, Michael W. Topping et al.2025 · 14 citationsarXiv
Quenching Through Tidal Gas Removal: Molecular Gas and Star Formation in Tidal Tails of z ~ 0.7 Post-Starburst Galaxies2507.21249v1 · Vincenzo R. D'Onofrio, Justin S. Spilker, Rachel Bezanson et al.2025 · 4 citationsarXiv
JWST+ALMA reveal the build up of stellar mass in the cores of dusty star-forming galaxies at Cosmic Noon2507.19472v3 · Sarah Bodansky, Katherine E. Whitaker, Ayesha Abdullah et al.2025 · 2 citationsarXiv
Unusually High Gas-to-Dust Ratios Observed in High-Redshift Quiescent Galaxies2507.16914v2 · Justin S. Spilker, Katherine E. Whitaker, Desika Narayanan et al.2025 · 4 citationsarXiv
The AURORA Survey: Robust Helium Abundances at High Redshift Reveal A Subpopulation of Helium-Enhanced Galaxies in the Early Universe2507.17057v1 · Danielle A. Berg, Ryan L. Sanders, Alice E. Shapley et al.2025 · 6 citationsarXiv
The AURORA Survey: Tracing Galactic Outflows at with JWST/NIRSpec NUV Absorption Lines2506.17381v2 · Emily Kehoe, Alice E. Shapley, Ryan L. Sanders et al.2025 · 1 citationarXiv
The JWST/AURORA Survey: Multiple Balmer and Paschen Emission Lines for Individual Star-forming Galaxies at z=1.5-4.4. I. A Diversity of Nebular Attenuation Curves and Evidence for Non-Unity Dust Covering Fractions2506.17396v2 · Naveen A. Reddy, Alice E. Shapley, Ryan L. Sanders et al.2025 · 11 citationsApJ, 999, 15 (2026)
Cold gas in a post-starburst pair at z ~ 1.4: major mergers as a pathway to quenching in the HeavyMetal survey2506.14361v1 · Katherine A. Suess, Aliza G. Beverage, Mariska Kriek et al.2025 · 0 citationsarXiv
Predicting the resolved CO emission of star-forming galaxies2506.13899v2 · Ravishankar Anirudh, Melanie Kaasinen, Gergo Popping et al.2025 · 1 citationA&A, 699, A19 (2025)
The ALMA-CRISTAL survey: Gas, dust, and stars in star-forming galaxies when the Universe was ~1 Gyr old I. Survey overview and case studies2505.06340v1 · R. Herrera-Camus, J. Gonz'alez-L'opez, N. Forster Schreiber et al.2025 · 28 citationsA&A 699, A80 (2025)
ALMA Band 3 Selection of Ultra-high Redshift Dropouts: The final challenge to {\Lambda}CDM2503.24312v1 · C. Lovell, M. Lee, A. Vijayan et al.2025 · 0 citationsarXiv
The AURORA Survey: The Evolution of Multi-phase Electron Densities at High Redshift2502.08712v1 · Michael W. Topping, Ryan L. Sanders, Alice E. Shapley et al.2025 · 43 citationsarXiv
SQuIGGE: Observational Evidence of Low Ongoing Star Formation Rates in Gas-Rich Post-Starburst Galaxies2501.16459v1 · Pengpei Zhu, Katherine A. Suess, Mariska Kriek et al.2025 · 7 citationsApJ 981 60 (2025)
RUBIES: JWST/NIRSpec resolves evolutionary phases of dusty star-forming galaxies at 2410.08387v1 · Olivia R. Cooper, Gabriel Brammer, Kasper E. Heintz et al.2024 · 0 citationsarXiv
The AURORA Survey: An Extraordinarily Mature, Star-forming Galaxy at 2410.00110v3 · Alice E. Shapley, Ryan L. Sanders, Michael W. Topping et al.2024 · 0 citationsarXiv
The Ultraviolet Slopes of Early Universe Galaxies: The Impact of Bursty Star Formation, Dust, and Nebular Continuum Emission2408.13312v1 · Desika Narayanan, Daniel P. Stark, Steven L. Finkelstein et al.2024 · 27 citationsarXiv
The AURORA Survey: The Nebular Attenuation Curve of a Galaxy at z=4.41 from Ultraviolet to Near-Infrared Wavelengths2408.05273v2 · Ryan L. Sanders, Alice E. Shapley, Michael W. Topping et al.2024 · 22 citationsarXiv
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