Priyamvada Natarajan
Joseph S. and Sophia S. Fruton Professor of Astronomy and Professor of PhysicsCards
About
Research
Publications
2026
A GLIMPSE of Intermediate Mass Black Holes in the Epoch of Reionization: Witnessing the Descendants of Direct Collapse?
Fei Q, Fujimoto S, Naidu R, Chisholm J, Atek H, Brammer G, Asada Y, Berg D, Bromm V, Furtak L, Greene J, Hsiao T, Jeon J, Kokorev V, Matthee J, Natarajan P, Pan R, Richard J, Saldana-Lopez A, Schaerer D, Volonteri M, Zitrin A. A GLIMPSE of Intermediate Mass Black Holes in the Epoch of Reionization: Witnessing the Descendants of Direct Collapse? The Astrophysical Journal 2026, 1003: 244. DOI: 10.3847/1538-4357/ae6248.Peer-Reviewed Original Researchactive galactic nucleisupermassive black holesblack holebroad-line active galactic nucleiintermediate mass black holesmass black holesmassive gas cloudsseed black holesBH mass functionnarrow-line componentepoch of reionizationhigh-z galaxiesstellar mass ratiolow-mass endMBH–MBH massgalactic nucleiearly universeBH formationnarrow-lineSchechter functionemission linesmass regimemock observationsdirect collapseLittle Red Dot − Host Galaxy = Black Hole Star: A Gas-Enshrouded Heart at the Center of Every Little Red Dot
Sun W, Naidu R, Matthee J, de Graaff A, Chisholm J, Greene J, Oesch P, Torralba A, Hviding R, Brammer G, Simcoe R, Bose S, Bouwens R, Dayal P, Eilers A, Fei Q, Furtak L, Gottumukkala R, Goulding A, Heintz K, Hirschmann M, Kokorev V, Leja J, Liu Z, Natarajan P, Santarelli A, Setton D, Smith A, Tacchella S, Volonteri M, Walter F, Weibel A, Williams C. Little Red Dot − Host Galaxy = Black Hole Star: A Gas-Enshrouded Heart at the Center of Every Little Red Dot. The Open Journal Of Astrophysics 2026, 9 DOI: 10.33232/001c.162505.Peer-Reviewed Original ResearchBridging Scales in Black Hole Accretion and Feedback: Subgrid Prescription from First Principles
Cho H, Prather C, Narayan R, Su K, Ricarte A, Natarajan P, Porras-Valverde A. Bridging Scales in Black Hole Accretion and Feedback: Subgrid Prescription from First Principles. The Astrophysical Journal Letters 2026, 1002: l43. DOI: 10.3847/2041-8213/ae61ae.Peer-Reviewed Original ResearchGRMHD simulationsblack holesubgrid prescriptionhot accretion modesupermassive black holesblack hole accretionhot accretion flowmagnetic field strengthBH spinquiescent accretionEddington ratioaccretion flowgalaxy scaleshost galaxiesspin evolutionaccretion modegalaxy evolutioncosmological simulationsevent horizonspin propertiesanalytical fitlong-term accretionfirst-principlesgalaxiessemianalytical modelA Kiloparsec-scale Stellar Cavity in the Center of A402-BCG May Be Caused by Dynamic Interactions with an Ultramassive Black Hole
McDonald M, Khullar G, Lagattuta D, Mahler G, Dattathri S, Diego J, Edge A, Floyd B, Gladders M, Hughes S, Jauzac M, Khonji N, Leroy G, Massey R, Montes M, Natarajan P, Reefe M, Sharon K, van den Bosch F, Werner S, Zitrin A. A Kiloparsec-scale Stellar Cavity in the Center of A402-BCG May Be Caused by Dynamic Interactions with an Ultramassive Black Hole. The Astrophysical Journal Letters 2026, 1002: l19. DOI: 10.3847/2041-8213/ae5bbe.Peer-Reviewed Original Researchactive galactic nucleistellar density fieldHubble Space Telescopeultramassive black holeblack holestellar distributiondual active galactic nucleiHubble Space Telescope databinary black hole systemdensity fieldsupermassive black holesblack hole systemsthree-body scatteringgalactic nucleikiloparsec separationsMUSE spectroscopybinary massSpace Telescopecentral galaxieshole systemsbinary hardeningdipole instabilitymissing starsflattened coreJWSTNew Cold Dark Matter Crisis Revealed by Multiscale Cluster Lensing
Natarajan P, Chiang B, Dutra I. New Cold Dark Matter Crisis Revealed by Multiscale Cluster Lensing. The Astrophysical Journal Letters 2026, 1001: l12. DOI: 10.3847/2041-8213/ae53ea.Peer-Reviewed Original Researchcollisionless cold DMself-interacting DMradial distribution of subhalosdistribution of subhalosradial distributiontruncation radiusmass functiondensity profilegalaxy–galaxy strong lensesinner density slopetidal truncation radiusinner density profilesubhalo mass functioncluster member galaxiesinternal density profileproperties of substructurescold DMsubhalo propertiesgalaxy clustersmassive clustersCluster Lensinggravitational lensingdensity slopestrong lensingmember galaxiesStrong LensIng and Cluster Evolution (SLICE) with JWST: Early Results, Lens Models, and High-redshift Detections
Cerny C, Mahler G, Sharon K, Jauzac M, Khullar G, Beauchesne B, Diego J, Lagattuta D, Limousin M, Patel N, Richard J, Cornil-Baïotto C, Gladders M, Werner S, Doppel J, Floyd B, Gonzalez A, Massey R, Montes M, Bayliss M, Bleem L, Canning R, Edge A, McDonald M, Natarajan P, Stark A, Gassis R. Strong LensIng and Cluster Evolution (SLICE) with JWST: Early Results, Lens Models, and High-redshift Detections. The Astrophysical Journal 2026, 1001: 60. DOI: 10.3847/1538-4357/ae41b0.Peer-Reviewed Original Researchstrong lensingsource galaxiescluster evolutionHubble Space Telescope imagesLaboratoire d’Astrophysique de Marseillehighest redshift detectionground-based spectroscopystrong-lensing modelslens modellensed background galaxiesinterior mass distributiondusty galaxieshigher redshiftsTelescope imagesredshift rangelensing galaxybackground galaxieslensed imagesgalaxiesJWSTJWST imagesmass rangemass profilesuperb resolutionmass distributionBridging Scales: Modeling Suppressed Bondi Accretion on Black Holes and Its Impact on Galaxy Growth
Porras-Valverde A, Natarajan P, Ricarte A, Su K, Cho H, Narayan R, Prather B. Bridging Scales: Modeling Suppressed Bondi Accretion on Black Holes and Its Impact on Galaxy Growth. The Astrophysical Journal 2026, 1000: 173. DOI: 10.3847/1538-4357/ae47fd.Peer-Reviewed Original Researchactive galactic nucleiblack hole masshole massgas accretionblack holemagnetic suppressionmagnetic fielddistribution of black hole massesluminous active galactic nucleimagnetically arrested disk stateJames Webb Space Telescopeaccretion rate regimelow-redshift constraintsblack hole growthhot gas accretiongalaxy-formation modelsgalactic nucleiGRMHD simulationsgalaxy growthstellar massBondi accretioncircumgalactic mediumSpace Telescopeaccretion physicsgalaxy assemblyMESA-QUEST: Tracing the Formation of Direct Collapse Black Hole Seeds via Quasi-stars
Santarelli A, Campbell C, Farag E, Bellinger E, Natarajan P, Caplan M. MESA-QUEST: Tracing the Formation of Direct Collapse Black Hole Seeds via Quasi-stars. The Astrophysical Journal 2026, 998: 150. DOI: 10.3847/1538-4357/ae371e.Peer-Reviewed Original Researchsupermassive black holesblack holequasi-staraccreting black holesblack hole seedsmass-loss prescriptionrelativistic radiation hydrodynamicsradiation-driven windsenvelope accretionstellar windBondi accretionaccretion physicsBH seedsMESA codegas cloudsradiation hydrodynamicsmagnetic fieldaccretionmass ratioholesconvection modelChandraJWSTgalaxiesconvection regimeBridging Scales: How Much Do Supermassive Black Holes Grow in the Suppressed Bondi Regime?
Su K, Ricarte A, Natarajan P, Porras-Valverde A, Cho H, Narayan R, Faucher-Giguère C, Hopkins P, Prather B. Bridging Scales: How Much Do Supermassive Black Holes Grow in the Suppressed Bondi Regime? The Astrophysical Journal Letters 2026, 998: l18. DOI: 10.3847/2041-8213/ae3724.Peer-Reviewed Original Researchsupermassive black holesblack holeblack hole-galaxy scaling relationscoevolution of supermassive black holeslow-luminosity active galactic nucleisupermassive black hole masssupermassive black hole populationeffective accretion ratesspin-dependent manneractive galactic nucleiblack hole accretionquenching star formationrelativistic windgalactic nucleihost galaxiesstar formationcircumgalactic mediumaccretion modecosmic timeevent horizonaccretion ratemagnetic stressesself-consistentlymassive seedsscaling relationsThe NANOGrav 15 yr Dataset: Targeted Searches for Supermassive Black Hole Binaries
Agarwal N, Agazie G, Anumarlapudi A, Archibald A, Arzoumanian Z, Baier J, Baker P, Bécsy B, Blecha L, Brazier A, Brook P, Burke-Spolaor S, Burnette R, Case R, Casey-Clyde J, Chang Y, Charisi M, Chatterjee S, Cohen T, Coppi P, Cordes J, Cornish N, Crawford F, Cromartie H, Crowter K, DeCesar M, Demorest P, Deng H, Dey L, Dolch T, D’Orazio D, Eisenberg E, Ferrara E, Doskoch G, Fiore W, Fonseca E, Freedman G, Gardiner E, Garver-Daniels N, Gentile P, Gersbach K, Glaser J, Graham M, Good D, Gültekin K, Harris C, Hazboun J, Hutchison F, Jennings R, Johnson A, Jones M, Kaplan D, Kelley L, Kerr M, Key J, Laal N, Lam M, Lamb W, Larsen B, Lazio T, Lewandowska N, Liu T, Lorimer D, Luo J, Lynch R, Ma C, Madison D, Matt C, McEwen A, McKee J, McLaughlin M, McMann N, Meyers B, Meyers P, Mingarelli C, Mitridate A, Natarajan P, Ng C, Nice D, Nichols S, Ocker S, Olum K, Pennucci T, Perera B, Petrov P, Pol N, Radovan H, Ransom S, Ray P, Romano J, Runnoe J, Saffer A, Sardesai S, Schmiedekamp A, Schmiedekamp C, Schmitz K, Semenzato F, Shapiro-Albert B, Shivakumar R, Siemens X, Simon J, Fiscella S, Stairs I, Stinebring D, Stovall K, Susobhanan A, Swiggum J, Taylor J, Taylor S, Thompson M, Turner J, Vallisneri M, van Haasteren R, Vigeland S, Wahl H, Willson L, Wilson K, Witt C, Wright D, Young O, Zheng Q, Collaboration T. The NANOGrav 15 yr Dataset: Targeted Searches for Supermassive Black Hole Binaries. The Astrophysical Journal Letters 2026, 998: l11. DOI: 10.3847/2041-8213/ae3719.Peer-Reviewed Original Researchcontinuous gravitational wavessupermassive black hole binariesblack hole binariespulsar timing array searchesactive galactic nucleiconsistent with noisegalactic nucleigravitational wavesupper limitparameter spaceNANOGravCW detectionbinariestrial factorsCW signalCW frequencymultimessengerelectromagnetic interpretationredshifttarget searchBayesian comparisoncoherencewaveBayes factorsnucleus