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Star Cluster Formation and Survival in the First Galaxies, Garcia, Ricotti, Sugimura, and Park (to appear soon)
"JWST UNCOVER: A triply imaged faint quasar candidate at z_{phot} = 7.7 " Furtak et al.
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"Growth of A Massive Black Hole In A Dense Star Cluster Via Tidal Disruption Accretion", Lee, S. et al., 2022, arXiv:2211.02376
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"Diverse Properties of Molecular Gas in the Host Galaxies of Fast Radio Bursts", B., Hatsukade, et al. 2022, arXiv:2211.02279
"Stellar feedback-regulated black hole growth: driving factors from nuclear to halo scales", Byrne, L. et al. 2022, arXiv:2210.09320
"A shot in the Dark (Ages): a faint galaxy at z=9.76 confirmed with JWST", G. Roberts-Borsani et al. 2022, arXiv:2210.15639
"The extent of metal enrichment from galactic winds during the Cosmic Dawn", N. Yamaguchi et al. 2022, arXiv:2209.09345
Non-ideal magnetohydrodynamic simulations of the first star formation, Sadanari et al. (to appear soon)
The Challenges of Identifying Population III Stars in the Early Universe, Katz et al. 2022, https://arxiv.org/abs/2207.04751
Unveiling the contribution of Pop III stars in primeval galaxies at redshift ≥ 6, Riaz et al. 2022, https://arxiv.org/abs/2208.01673
First Peek with JWST/NIRCam Wide-field Slitless Spectroscopy: Serendipitous Discovery of a Strong [O III]/Hα Emitter at z=6.11, Sun et al. 2022, https://iopscience.iop.org/article/10.3847/2041-8213/ac8938
Magnetic Effects Promote Supermassive Star Formation in Metal-enriched Atomic-cooling Halos, Hirano et al. (2022), arXiv:2209.03574
Single Fluid vs. Multifluid: Comparison between single fluid and multifluid dust models for disc planet interactions, K. Chan. & S. Paardekooper (2022), arXiv:2209.09830
A Lower Bound of Star Formation Activity in Ultra-high Redshift Galaxies Detected with JWST: Implications for Stellar Populations and Radiation Sources, Inayoshi et al. (2022), arXiv:2208.06872
Templates for Fitting Photometry of Ultra-High-Redshift Galaxies, Steinhardt et al. (2022), arXiv:2208.07879
Self-regulation of black hole accretion via jets in early protogalaxies, Su, Bryan, Haiman, et al., arXiv:2207.11270
"Hyper-Eddington Black Hole Growth in Star-Forming Molecular Clouds and Galactic Nuclei: Can It Happen?", Shi et al. 2022, arXiv:2208.05025
"Stress testing ΛCDM with high-redshift galaxy candidates", Michael Boylan-Kolchin , arXiv:2208.01611
"Observational Signatures of Massive Black Hole Progenitor Pathways: is Leo I a Smoking Gun?", John A. Regan et al., arXiv:2208.02546
"Exponentially amplified magnetic field eliminates disk fragmentation around the Population III protostar", Shingo Hirano and Masahiro Machida, arXiv:2208.01216
"Unusual gas structure in an otherwise normal spiral galaxy hosting GRB 171205A / SN 2017iuk", M. Arabsalmani et al., arXiv:2206.07060
"Understanding the high-mass binary black hole population from stable mass transfer and super-Eddington accretion in BPASS", Briel, M. M., et al. 2022, arXiv:2206.13842
Naidu e al. 2022 "Two Remarkably Luminous Galaxy Candidates at z ≈ 11 − 13 Revealed by JWST"
https://arxiv.org/pdf/2207.09434.pdf
Castellano et al. 2022 "Early results from GLASS-JWST. III: Galaxy candidates at z∼9-15"
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Schaerer et al. 2022 "First look with JWST spectroscopy: z ∼ 8 galaxies resemble local analogues"
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"The imprint of gas on gravitational waves from LISA intermediate-mass black hole binaries", Garg M. et al., arXiv: 2206.05292
"Primordial magnetic fields in Population III star formation: a magnetised resolution study", Prole et al., arXiv:2206.1191
"A Green Pea starburst arising from a galaxy-galaxy merger", S., Purkayastha et al., arXiv: 2206.07726
"A Challenge to the Standard Cosmological Model", Secrest et al., arXiv:2206.05624
"Gaia DR3 in 6D: The search for fast hypervelocity stars and constraints on the Galactic Centre environment", Marchetti et al., arXiv:2206.06962
``Accretion on to a binary from a polar circumbinary disc'', J. L. Smallwood., S. H. Lubow., & R. G. Martin, 2022, arXiv:2205.09183
"Dust coagulation during the early stages of star formation: molecular cloud collapse and first hydrostatic core evolution" Matthew R. Bate, arXiv:2205.07681
"The low-end of the black hole mass function at cosmic dawn" Trinca Alessandro, Schneider Raffaella et al., arXiv:2201.02630
"How long do high-redshift massive black hole seeds remain outliers in black hole vs. host galaxy relations?", Matthew T. Scoggins, Zoltán Haiman, John H. Wise, 2022; https://arxiv.org/abs/2205.09611
"Mechanical feedback effects on primordial black hole accretion", Bosch-Ramon N. Bellomo .2020;https://www.aanda.org/articles/aa/pdf/2020/06/aa37537-20.pdf
"3D hydrodynamical simulations of the impact of mechanical feedback on accretion in supersonic stellar-mass black holes", Bosch-Ramon. 2022; 2201.09601
"Euclid: Discovering pair-instability supernovae with the Deep Survey", Moriya et al. 2022, https://arxiv.org/abs/2204.08727
"Euclid detectability of pair instability supernovae in binary population synthesis models consistent with merging binary black holes", Tanikawa et al. 2022, https://arxiv.org/abs/2204.09402
High Equivalent Width of Hα+[N II] Emission in z ∼ 8 Lyman-break Galaxies from IRAC 5.8μm Observations: Evidence for Efficient Lyman-continuum Photon production in the Epoch of Re-ionization, https://arxiv.org/abs/2204.02986
Introducing the THESAN project: radiation-magneto-hydrodynamic simulations of the epoch of reionization, https://arxiv.org/abs/2110.00584
"Formation of black holes in the pair-instability mass gap: Hydrodynamical simulation of a massive star collision", Ballone, A., et al. 2022, arXiv:2204.03493
"Formation of black holes in the pair-instability mass gap: evolution of a post-collision star", Costa, G., et al. 2022, arXiv:2204.03492
"Slow Star Formation in the Milky Way: Theory Meets Observations", Evans, N., J., et al. 2022, arXiv:2204.02314
"Radiation-MagnetoHydrodynamics simulations of cosmic ray feedback in disc galaxies", Farcy et al. 2022, arXiv:2202.01245
"A highly magnified star at redshift 6.2", Welch et al. 2022, Nature [link to Nature]
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``Trapping of HII regions in Population III star formation'' O. Jaura et al., arXiv:2202.09803
"Misaligned Spinning Binary Black Hole Mergers in Hot Magnetized Plasma"
Cattorini, F. et al. 2022, https://arxiv.org/abs/2202.08282
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Kretschmer et al. 2021 https://arxiv.org/abs/2103.06882
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"A Search for H-Dropout Lyman Break Galaxies at z~13"
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''Second generation star formation in globular clusters of different masses``, A. Yaghoobi et al. 2021, arXiv:2112.06992
The candidate tidal disruption event AT2019fdr coincident with high a high-energy neutrino, Reusch et al. 2021, https://arxiv.org/abs/2111.09390
Could TDE outflows produce the PeV neutrino events? Wu et al. 2021, https://arxiv.org/abs/2112.01748
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"Not the Birth Cluster: the Stellar Clustering that Shapes Planetary Systems is Generated by Galactic-Dynamical Perturbations", Kruijssen et al., arXiv:2109.061282
"Hot Jupiters, cold kinematics: High phase space densities of host stars reflect an age bias", Mustill et al., arXiv:2103.15823
"The formation of massive stellar clusters in converging galactic flows with photoionisation", Dobbs, Bending, Pettitt, & Bate, arXiv:2110.09201
"Probing the initial mass function of the first stars with transients ", Lazar & Bromm , arXiv: 2110.11956
"Massive Star Cluster Formation and Destruction in Luminous Infrared Galaxies in GOALS II: An ACS/WFC3 Survey of Nearby LIRGs", Linden et al. arXiv: 2110.03638
"Star Formation Regulation and Self-Pollution by Stellar Wind Feedback", Lancaster et al. arXiv: 2110.05508
``On the low ortho-to-para H2 ratio in star-forming filaments'', Lupi et al. (2021) arXiv:2109.02655
"The CHIME FRB population do not track the star formation history of the universe", Rachel C. Zhang et al. (2021), arXiv:2109.07558
"Fast radio bursts as probes of feedback from active galactic nuclei", Adam J. Batten et al. (2021), arXiv:2109.13472
"Probing Early Super-massive Black Hole Growth and Quasar Evolution with Near-infrared Spectroscopy of 37 Reionization-era Quasars at 6.3 < z <= 7.64", Yang et al. (2021), arXiv:2109.13942
"Hunting intermediate-mass black holes with LISA binary radial velocity measurements", Strokov et al. (2021), arXiv:2109.08154
"The nature of high [OIII]-[CII] galaxies in the epoch of reionization: low carbon abundance and a top-heavy IMF? ", Katz, H., et al. 2021, arXiv:2108.01074
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Hoyle-Lyttleton accretion on to black hole accretion disks with super-Eddington luminosity for dusty gas, Ogata, et al. arXiv:2106.12866
"Dust Settling and Clumping in MRI Turbulent Outer Protoplanetary Disks", Xu & Bai (2021), arXiv:2108.10486
"Spatial Statistics in Star Forming Regions: Is Star Formation Driven By Column Density Alone?" Retter et al. (2021) arXiv:2108.02466
Dust in the Wind with Resonant Drag Instabilities: I. The Dynamics of Dust-Driven Outflows in GMCs and HII regions; arXiv:2107.04608
The Mass Budgets and Spatial Scales of Exoplanet Systems and Protopalnetary Disks arXiv:2107.12520
''Differential rotation in a 3D simulation of oxygen shell burning'', McNeill et al. (2021), arXiv:2107.00173
"R-process elements from magnetorotational hypernovae", Yong et al. (2021), arXiv:2107:03010
"Conditions for Detecting Lensed Population III Galaxies in Blind Surveys with the James Webb Space Telescope, the Roman Space Telescope and Euclid." Vikaeus et al. (2021), arXiv:2107.01230
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Magnetohydrodynamic Winds Driven by the Line Force from the Standard Thin Disk around Supermassive Black Holes. I. The Case of Weak Magnetic Field : arXiv:2104.08058
"Hunting isolated neutron stars with proper motions from wide-area optical surveys", Toyouchi, D., et al. 2020, arXiv:2106.04846
Transport of Protostellar Cosmic Rays in Turbulent Dense Cores: arXiv2105.00028
Stellar feedback and triggered star formation in the prototypical bubble RCW 120
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"No Sub-Saturn Mass Planet Desert in the CORALIE/HARPS Radial Velocity Sample", Bennett et al., 2021, arXiv:2104.05713
"Probing supermassive stars and massive black hole seeds through gravitational wave inspirals", Raveh et al.,2021, arXiv:2104.02083
"A two-step gravitational cascade for the fragmentation of self-gravitating discs", Brucy & Hennebelle, 2021, arXiv:2103.05508
"Resonant-line radiative transfer within power-law density profiles", Lao & Smith, 2020, arXiv:2005.09692
"Lyman-alpha radiation pressure: an analytical exploration", Tomaselli & Ferrara . 2021, arXiv:2103.14655
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"Testing the Turbulent Origin of the Stellar Initial Mass Function", Nam et al. 2021, arXiv:2102.08564
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"Effects of turbulence in the Circumnuclear Disk", Dinh et al. 2021, arXiv:2102.09569
"Stellar Evolution in the Disks of Active Galactic Nuclei Produces Rapidly Rotating Massive Stars", Jermyn et al. 2021, arXiv:2102.13114
"Observational properties of a general relativistic instability supernova from a primordial supermassive star", Moriya et al. 2021, arXiv:2103.01336
"Steady State by Recycling prevents Premature Collapse of Protoplanetary Atmospheres" , Moldenhauer et al. (2021), arXiv:2102.00939
"Equilibrium eccentricity of accreting binaries", Zrake et al. arXiv:2010.09707
"Formation of intermediate-mass planets via magnetically-controlled disk fragmentation", Deng, Mayer, & Helled, arXiv:2101.01331
Outflow from super-Eddington flow: where it originates from and how much impact it gives?, arxiv.org/abs/2101.11028
VVV CL001: The Most Likely Metal-Poor Surviving Globular Cluster in the Inner Galaxy
Predicting the Observability of Population III Stars with ELT-HARMONI via the Helium 1640Å emission line, Kearn Grisdale et al., 2021, arXiv:2101.01725
The properties of clusters, and the orientation of magnetic fields relative to filaments, in magnetohydrodynamic simulations of colliding clouds, Dobbs & Wurster, 2021, arXiv:2101.07637
Regulating Star Formation in Nearby Dusty Galaxies: Low Photoelectric Efficiencies in the Most Compact Systems, McKinney et al., 2021, arXiv:2101.01182
"A relation between the radial velocity dispersion of young clusters and their age: Evidence for hardening as the formation scenario of massive close binaries", Ramirez-Tannus, M. C. et al. 2021
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Kim et al. arXiv: 2011.07772
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Maeda, Inoue & Fukui, arXiv: 2011.11650
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Koushik Chatterjee et al. arXiv: 2011.08904
"Stellar clustering shapes the architectures of planetary systems"
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"The critical dark matter halo mass for Population III star formation: dependence on Lyman-Werner radiation, baryon-dark matter streaming velocity, and redshift", Kulkarni et al., 2020, arXiv:2010.04169
"Detectable environmental effects in GW190521-like black-hole binaries with LISA", Toubiana et al. 2020, arXiv:2010.06056
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"GW190521 from the Merger of Ultra-Dwarf Galaxies", arXiv:2009.10688
"GW190521 as a Highly Eccentric Black Hole Merger", arXiv:2009.05461
"Candidate Electromagnetic Counterpart to the Binary Black Hole Merger Gravitational-Wave Event S190521g*", arXiv:2006.14122
"Current observations are insufficient to confidently associate thebinary black hole merger GW190521 with AGN J124942.3+344929", arXiv:2009.12346
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Implementation of stellar heating feedback in simulations of star cluster formation: effects on the initial mass function
https://arxiv.org/abs/2007.01875
Massive Star Formation in Metal-Enriched Haloes at High Redshift
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Magnetic field amplification in accretion discs around the first stars: implications for the primordial IMF
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"HST Survey of the Orion Nebula Cluster in the H2O 1.4 μm Absorption Band. II. The Substellar IMF Down to Planetary Masses", Gennaro & Robberto 2020, 2020ApJ...896...80G
"ASASSN-15lh: a TDE about a maximally rotating 10^9 Msun black hole" Mummery, A. and Balbus, S. A. 2020, arXiv:2006.00803
"Highly Fe-enriched metal-poor galaxies with ~1.0 (Fe/H)sun and 0.02 (O/H)sun: possible traces of super massive (> 300 Msun) stars in early galaxies" Kojima, T. et al. 2020, arXiv:2006.03831
"On the maximum stellar rotation to form a black hole without an accompanying luminous transient" Ariadna Murguia-Berthier et al. 2020, arXiv:2005.10212
Photoionising feedback in spiral arm molecular clouds, T. J. R. Bending, C. L. Dobbs and M. R. Bate 2020, arXiv:2005.06234
A census of baryons in the Universe from localized fast radio bursts, Macquart et al. (2020), arXiv:2005.13161
Searching for Black Holes in the Outer Solar System with LSST, Siraj & Loeb (2020), arXiv:2005.12280
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"Figuring Out Gas & Galaxies In Enzo (FOGGIE). IV. The Stochasticity of Ram Pressure Stripping in Galactic Halos", Simons et al. (2020), arXiv:2004.14394
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