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REVIEW 3 major objections 2 minor 1 cited by

TDEs on FIRE: Illuminating the Cosmic Evolution of Tidal Disruption Rates

T0 review · 3 major / 2 minor · reviewed 2026-06-28 · grok-4.3

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Pith's one-line read Simulations find the average tidal disruption rate per galaxy peaks near redshift 2.5 then falls sharply by redshift 1.

desk verdict FIRE-2 supplies the first simulation-based TDR(z) to z=10 but the central densities sit below the resolution limit, so the numbers rest on an untested extrapolation. read the letter →

arxiv 2606.04740 v1 pith:U73YDRXB submitted 2026-06-03 astro-ph.HE

Rudrani Kar Chowdhury , Lixin Dai , Janet N.Y. Chang , Tsang Keung Chan This is my paper
classification astro-ph.HE
keywords tidaldisruptioneventscosmologicalsimulationsblackholegrowthgalaxyevolutionstarformationratecentralstellardensitysatellitegalaxiesredshift
verification ladder T0 review T1 audit T2 compute T3 formal

The pith

A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.

The reading

This paper applies cosmological zoom-in simulations to track how often stars are torn apart by black holes inside galaxies from redshift 10 down to redshift 1. The calculation shows the typical rate per galaxy climbs from early times, reaches roughly 4 times 10 to the minus 4 events per year near redshift 2.5, and drops to about 10 to the minus 5 by redshift 1. The rates track closely with each galaxy's star-formation activity and the density of stars near its center at every epoch examined. The same mass trends seen locally also appear at high redshift, while satellite galaxies supply a rising fraction of the events as redshift increases.

What carries the argument

FIRE-2 cosmological zoom-in simulations that model central stellar densities, black-hole populations, and dynamical conditions to compute per-galaxy tidal disruption rates across redshift.

What would settle it

A direct measurement or statistical sample of tidal disruption events at redshift approximately 2.5 that yields an average per-galaxy rate far below or far above 4 times 10 to the minus 4 per year.

Watch

Extended reading notes

Core claim

Using the FIRE-2 cosmological zoom-in simulations, the per-galaxy tidal disruption rate is computed over redshifts 1 to 10 for black holes ranging from intermediate-mass to supermassive. The averaged rate rises from the early universe, peaks at approximately 4 times 10 to the minus 4 per year near redshift 2.5, and declines to about 10 to the minus 5 per year at redshift 1. This rate correlates strongly with host-galaxy star-formation rate and central stellar density at all redshifts. The dependence on black-hole mass and galaxy mass remains qualitatively similar from high redshift to the local universe, and satellite galaxies show comparably high rates whose fractional contribution grows at

Load-bearing premise

The FIRE-2 simulations accurately capture the central stellar densities, black-hole populations, and dynamical conditions needed to compute tidal disruption rates at redshifts above 1.

Editorial extensions

If this is right

  • Tidal disruption rates track star-formation rate and central density, so galaxies with elevated star formation should produce more events at any redshift.
  • Satellite galaxies maintain high rates whose share increases at high redshift, making them useful targets for finding intermediate-mass black holes.
  • The black-hole to galaxy mass trends stay consistent from high redshift to today, supporting similar scaling relations across cosmic time.
  • Cosmological simulations can now supply predictions for the cosmic evolution of tidal disruption rates that future surveys can test directly.

Reading between the lines

Editorial extensions of the paper, not claims the author makes directly.

  • Confirmation of the redshift-2.5 peak would link the era of maximum star formation directly to the era of maximum central stellar densities that drive disruptions.
  • Higher rates at earlier times could alter estimates of how much black-hole growth occurs through stellar capture rather than gas accretion.
  • If satellite contributions are as large as modeled, wide-field high-redshift transient searches could preferentially detect events in merging or assembling galaxies.
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Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, simulated authors' rebuttal, and a circularity audit.

Referee Report

3 major / 2 minor

Summary. The paper uses FIRE-2 cosmological zoom-in simulations to compute per-galaxy tidal disruption rates (TDR) from z=1 to 10 across IMBH to SMBH masses. It reports that the averaged TDR rises from early times, peaks at ~4×10^{-4} yr^{-1} near z~2.5, and falls to ~10^{-5} yr^{-1} at z=1. The TDR is stated to correlate strongly with host SFR and central stellar density at all redshifts; trends with M_BH and M_gal are qualitatively similar to the local universe; satellite galaxies contribute an increasing fraction of the TDR at high z.

Significance. If robust, the work supplies the first simulation-derived TDR(z) evolution and links it to galaxy properties, offering testable predictions for high-redshift TDE searches. The approach of extracting rates directly from cosmological zoom-ins is novel for this problem. Credit is due for covering a wide redshift range and including satellites. However, the result's significance hinges on whether the unresolved central densities can be reliably mapped to TDR.

major comments (3)
  1. [Abstract / Methods] Abstract and methods (TDR extraction): the headline TDR(z) curve is obtained by applying an estimator to simulated M_BH, M_gal, SFR, and central stellar density. No derivation, functional form, or sub-grid extrapolation for the loss-cone density is provided; the exponential sensitivity of TDR to density within the BH influence radius means any inaccuracy in the unresolved nuclear density shifts both normalization and peak redshift by factors of several.
  2. [Abstract / Results] Abstract and results (validation): no comparison of the computed local (z~0) TDR to observed rates is shown, nor are error bars or resolution convergence tests reported. Without this anchor, the claimed evolution from z=10 to z=1 cannot be assessed for systematic bias.
  3. [Abstract] Abstract (correlations): the reported strong correlation between TDR and central stellar density is expected by construction once the estimator is applied to that density; it therefore does not constitute independent validation of the redshift trend or the underlying density field.
minor comments (2)
  1. [Abstract] Abstract: include a one-sentence description of the TDR estimator and the mass range of black holes considered.
  2. [Figures] Figure clarity: ensure any TDR(z) plots show individual galaxy tracks or scatter in addition to the average to allow assessment of sample variance.

Simulated Author's Rebuttal

3 responses · 0 unresolved

We thank the referee for their detailed and constructive report. We address each major comment below and indicate where revisions will be made to strengthen the manuscript.

read point-by-point responses

  1. Referee: [Abstract / Methods] Abstract and methods (TDR extraction): the headline TDR(z) curve is obtained by applying an estimator to simulated M_BH, M_gal, SFR, and central stellar density. No derivation, functional form, or sub-grid extrapolation for the loss-cone density is provided; the exponential sensitivity of TDR to density within the BH influence radius means any inaccuracy in the unresolved nuclear density shifts both normalization and peak redshift by factors of several.

    Authors: We agree that the methods section would benefit from an explicit derivation of the TDR estimator, including the functional form relating loss-cone refilling to central stellar density. The estimator follows the standard loss-cone formalism (e.g., as in Merritt & Wang 2005 and subsequent works), applied to the resolved central densities in FIRE-2. We will add this derivation, the precise functional form, and a brief discussion of sub-grid assumptions in a revised Methods section. This addresses the concern about transparency while noting that the simulations themselves provide the density evolution. revision: yes

  2. Referee: [Abstract / Results] Abstract and results (validation): no comparison of the computed local (z~0) TDR to observed rates is shown, nor are error bars or resolution convergence tests reported. Without this anchor, the claimed evolution from z=10 to z=1 cannot be assessed for systematic bias.

    Authors: We acknowledge the value of anchoring the results to local observations. In the revised manuscript we will include a direct comparison of our z≈0 TDR values to the observed local TDE rate range (∼10^{-5}–10^{-4} yr^{-1} per galaxy) from the literature, along with sample variance error bars derived from the zoom-in suite. Resolution convergence is limited by the fixed FIRE-2 resolution; we will add a brief discussion of this limitation and note that higher-resolution follow-up simulations would be needed for full convergence tests. revision: partial

  3. Referee: [Abstract] Abstract (correlations): the reported strong correlation between TDR and central stellar density is expected by construction once the estimator is applied to that density; it therefore does not constitute independent validation of the redshift trend or the underlying density field.

    Authors: We agree that the TDR–central-density correlation is expected by construction of the estimator. However, the independent correlation with SFR (which is not an input to the estimator) and the persistence of M_BH and M_gal trends across redshift provide additional support for the physical trends. We will revise the abstract and results text to clarify this distinction and to emphasize that the redshift evolution arises from the simulated evolution of galaxy properties rather than from the estimator alone. revision: yes

Circularity Check

0 steps flagged · score 0.0 of 10

No significant circularity in derivation chain

full rationale

The paper computes per-galaxy TDR directly from FIRE-2 simulation snapshots of M_BH, M_gal, SFR and central stellar density over z=1-10, then reports the resulting averaged TDR(z) evolution and correlations. No equations, fitted parameters, or self-citations are shown that define the output TDR in terms of itself or rename a fitted input as a prediction. The stated correlations with SFR and central density are expected consequences of applying any standard TDR estimator but do not reduce the headline TDR(z) curve to a tautology by construction; the main result remains an independent computation from the simulation data. The derivation is therefore self-contained against external simulation inputs with no load-bearing circular steps.

Assumptions & free parameters 0 free parameters · 0 assumptions · 0 invented entities

No free parameters, axioms, or invented entities are identifiable from the abstract alone.

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Cite this review

Pith. "Pith review of TDEs on FIRE: Illuminating the Cosmic Evolution of Tidal Disruption Rates." pith.science (2026). https://pith.science/paper/U73YDRXB

@misc{pith2026260604740,
  author       = {Pith},
  title        = {Pith review of: TDEs on FIRE: Illuminating the Cosmic Evolution of Tidal Disruption Rates},
  year         = {2026},
  howpublished = {\url{https://pith.science/paper/U73YDRXB}},
  note         = {Machine review of arXiv:2606.04740}
}
abstract

Tidal disruption events have been extensively studied in the local universe, but their prevalence at high redshifts remains largely unexplored. Using the FIRE-2 cosmological zoom-in simulations, we compute the per-galaxy tidal disruption rate (TDR) over $z=1-10$, covering black holes from IMBHs to SMBHs. The averaged TDR rises from the early universe, peaks at $\sim 4 \times 10^{-4} \, \text{yr}^{-1}$ near $z \sim 2.5$, and declines to $\sim 10^{-5} \, \text{yr}^{-1}$ at $z=1$. The TDR correlates strongly with host galaxy star formation rate and central stellar density at all redshifts. Qualitatively, the TDR trends with the $M_{\rm BH}$ and $M_{\rm gal}$ persist from high redshift to the local universe, suggesting similar BH-galaxy scaling across cosmic time. Satellite galaxies exhibit comparably high TDRs, with their fractional contribution increasing significantly at high redshifts, highlighting their potential for probing IMBHs and early galaxy assembly. This work demonstrates that cosmological simulations offer a promising avenue for constraining the cosmic evolution of the TDR, paving the way for future comparisons with next-generation observations.

Figures

Figures reproduced from arXiv: 2606.04740 by the authors.

Figure 1
Figure 1. The radial profile of stellar density at the centres of the primary host galaxies at z = 1 in the A1, A2, A4, and A8 runs, respectively. Double power-law fits (Equation 11) are shown as solid black lines. The primary galaxies of the A2 and A8 do not contribute to the TDE rates as their BH masses are > 108M⊙. using the fitted parameters of the double power law pro￾file (ρ0, r0, α, δ and γ). phaseflow can also solve f… view at source ↗
Figure 2
Figure 2. The correlation between the TDR and MBH at individual redshifts. Gray dots show the full galaxy sample across all redshifts, while colored points in each panel highlight galaxies at the specific redshift indicated [PITH_FULL_IMAGE:figures/full_fig_p006_2.png] view at source ↗
Figure 3
Figure 3. Correlation between the TDR and Mgal at individual redshifts. Colour scheme is same as [PITH_FULL_IMAGE:figures/full_fig_p006_3.png] view at source ↗
Figures from the paper (8 more)
Figure 4
Figure 4. Figure 4: The redshift evolution of the averaged TDR (black triangles) and the averaged SFR (red dots) at each redshift. Black solid lines show the best-fit relations at z > 2.5, while the thin dotted line marks the redshift be￾low which both rates moderately decline. within a c…
Figure 5
Figure 5. Figure 5: The TDR versus SFR for individual galaxies in our sample, with the colors indicating redshift from z = 1 to 10. The TDR generally traces the redshift evolution of SFR. The gray shaded regions show the averaged TDR in each SFR bin, fitted with a power-law function (Equa…
Figure 6
Figure 6. Figure 6: The correlation of the TDR with the black hole mass (MBH) (left panel) and host galaxy mass (Mgal) (right panel) for individual galaxies in our sample. Colors indicate different redshifts, as shown in the legend. In both panels, star symbols denote primary host galaxie…
Figure 7
Figure 7. Figure 7: The projected stellar densities around the BHs at the centers of two example galaxies, where the TDR is found to be highest in [PITH_FULL_IMAGE:figures/full_fig_p009_7.png]
Figure 8
Figure 8. Figure 8: The correlated properties of the TDR vs the fitted parameters of stellar profiles at different redshifts. Left panel: Correlation between TDR and stellar densities at the scale radius (ρ0). Right panel: Correlation of TDR with the inner slope of the stellar profiles (γ…
Figure 9
Figure 9. Figure 9: The correlation of the radius of influence (rinf) with the BH mass (left panel) and the TDR (right panel) at z = 1−10. The symbols and the color schemes are the same as in [PITH_FULL_IMAGE:figures/full_fig_p011_9.png]
Figure 12
Figure 12. Figure 12: The TDR of satellite galaxies versus their off￾set distances from the primary hosts at each redshift. Black lines mark the angular resolution limits of Roman (dash– dotted), Rubin (dashed), and ULTRASAT (dotted), respec￾tively. While there is a spread in TDR among sat…
Figure 11
Figure 11. Figure 11: The ratio of the total TDR from all satel￾lite galaxies to that from primary galaxies at each redshift. The TDE contribution from satellite galaxies is significantly higher in the early universe. 5. Finally, we examine the detectability of TDEs in satellite galaxies. …

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Cited by 1 Pith paper

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  1. Rates of tidal disruption events from constrained cosmological simulations of the local Universe: population properties and implications for transient surveys

    astro-ph.HE 2026-07 conditional novelty 6.0 of 10

    In simulated local clusters, tidal disruption events are dominated by cuspy satellite galaxies in extended halos, with a volumetric rate of ~600 Gpc^-3 yr^-1 inherited from empirical TDE scaling relations.

Reference graph

Works this paper leans on

251 extracted references · 244 canonical work pages · cited by 1 Pith paper

  1. [1]

    Cosmological Simulation of Galaxy Groups and Clusters. I. Global Effect of Feedback from Active Galactic Nuclei. , keywords =. doi:10.3847/1538-4357/ab5b96 , archivePrefix =. 1911.07824 , primaryClass =

    work page doi:10.3847/1538-4357/ab5b96 1911

  2. [2]

    Cosmological Simulation of Galaxy Groups and Clusters. II. Studying Different Modes of Feedback through X-Ray Observations. , keywords =. doi:10.3847/1538-4357/ac951c , archivePrefix =. 2209.13349 , primaryClass =

    work page doi:10.3847/1538-4357/ac951c

  3. [3]

    , keywords =

    Detecting Population III Stars through Tidal Disruption Events in the Era of JWST and Roman. , keywords =. doi:10.3847/2041-8213/ad41b7 , archivePrefix =. 2401.12752 , primaryClass =

    work page doi:10.3847/2041-8213/ad41b7

  4. [4]

    , keywords =

    Rates of Stellar Tidal Disruption Events around Intermediate-mass Black Holes. , keywords =. doi:10.3847/2041-8213/adace7 , archivePrefix =. 2407.09339 , primaryClass =

    work page doi:10.3847/2041-8213/adace7

  5. [5]

    Merger Driven or Internal Evolution? A New Morphological Study of Tidal Disruption Event Host Galaxies

    Merger Driven or Internal Evolution? A New Morphological Study of Tidal Disruption Event Host Galaxies. arXiv e-prints , keywords =. doi:10.48550/arXiv.2602.06839 , archivePrefix =. 2602.06839 , primaryClass =

    work page Pith review arXiv doi:10.48550/arxiv.2602.06839

  6. [6]

    , keywords =

    Spatially Resolved Stellar Populations of 0.3 < z < 6.0 Galaxies in WHL 0137-08 and MACS 0647+70 Clusters as Revealed by JWST: How Do Galaxies Grow and Quench over Cosmic Time?. , keywords =. doi:10.3847/1538-4357/acba06 , archivePrefix =. 2301.02209 , primaryClass =

    work page doi:10.3847/1538-4357/acba06

  7. [7]

    The Astropy Project: Building an inclusive, open-science project and status of the v2.0 core package

    The Astropy Project: Building an Open-science Project and Status of the v2.0 Core Package. , keywords =. doi:10.3847/1538-3881/aabc4f , archivePrefix =. 1801.02634 , primaryClass =

    work page Pith review arXiv doi:10.3847/1538-3881/aabc4f

  8. [8]

    The Formation of the First Star in the Universe

    The Formation of the First Star in the Universe. Science , keywords =. doi:10.1126/science.295.5552.93 , archivePrefix =. astro-ph/0112088 , primaryClass =

    work page Pith review arXiv doi:10.1126/science.295.5552.93

Show all 251 references
  1. [9]

    , keywords =

    Radio Properties of Tidal Disruption Events. , keywords =. doi:10.1007/s11214-020-00702-w , archivePrefix =. 2006.01159 , primaryClass =

    2006 doi

  2. [10]

    , keywords =

    Tidal disruption discs formed and fed by stream-stream and stream-disc interactions in global GRHD simulations. , keywords =. doi:10.1093/mnras/stab3444 , archivePrefix =. 2008.04922 , primaryClass =

    2008 doi

  3. [11]

    , keywords =

    A very luminous jet from the disruption of a star by a massive black hole. , keywords =. doi:10.1038/s41586-022-05465-8 , archivePrefix =. 2211.16530 , primaryClass =

    doi

  4. [12]

    , keywords =

    Gravitational torque-driven black hole growth and feedback in cosmological simulations. , keywords =. doi:10.1093/mnras/stw2565 , archivePrefix =. 1603.08007 , primaryClass =

    doi arXiv

  5. [13]

    , keywords =

    Black holes on FIRE: stellar feedback limits early feeding of galactic nuclei. , keywords =. doi:10.1093/mnrasl/slx161 , archivePrefix =. 1707.03832 , primaryClass =

    doi arXiv

  6. [14]

    Nature Astronomy , keywords =

    A fast-rising tidal disruption event from a candidate intermediate-mass black hole. Nature Astronomy , keywords =. doi:10.1038/s41550-022-01811-y , archivePrefix =. 2209.00018 , primaryClass =

    doi

  7. [15]

    , keywords =

    A Continuum of H- to He-rich Tidal Disruption Candidates With a Preference for E+A Galaxies. , keywords =. doi:10.1088/0004-637X/793/1/38 , archivePrefix =. 1405.1415 , primaryClass =

    doi arXiv

  8. [16]

    , keywords =

    New Physical Insights about Tidal Disruption Events from a Comprehensive Observational Inventory at X-Ray Wavelengths. , keywords =. doi:10.3847/1538-4357/aa633b , archivePrefix =. 1611.02291 , primaryClass =

    doi arXiv

  9. [17]

    , keywords =

    The Peak of the Fallback Rate from Tidal Disruption Events: Dependence on Stellar Type. , keywords =. doi:10.3847/2041-8213/ad0388 , archivePrefix =. 2310.11496 , primaryClass =

    doi

  10. [18]

    , keywords =

    Formation of supermassive black holes by direct collapse in pre-galactic haloes. , keywords =. doi:10.1111/j.1365-2966.2006.10467.x , archivePrefix =. astro-ph/0602363 , primaryClass =

    2006 doi

  11. [19]

    , keywords =

    The ASTRID simulation: galaxy formation and reionization. , keywords =. doi:10.1093/mnras/stac648 , archivePrefix =. 2111.01160 , primaryClass =

    doi

  12. [20]

    , keywords =

    The Broad Absorption Line Tidal Disruption Event iPTF15af: Optical and Ultraviolet Evolution. , keywords =. doi:10.3847/1538-4357/ab04b0 , archivePrefix =. 1809.07446 , primaryClass =

    doi

  13. [21]

    , keywords =

    Electromagnetic extraction of energy from Kerr black holes. , keywords =. doi:10.1093/mnras/179.3.433 , adsurl =

    doi

  14. [22]

    Science , keywords =

    A Possible Relativistic Jetted Outburst from a Massive Black Hole Fed by a Tidally Disrupted Star. Science , keywords =. doi:10.1126/science.1207150 , archivePrefix =. 1104.3257 , primaryClass =

    doi arXiv

  15. [23]

    Nature Astronomy , keywords =

    Evidence for heavy-seed origin of early supermassive black holes from a z 10 X-ray quasar. Nature Astronomy , keywords =. doi:10.1038/s41550-023-02111-9 , archivePrefix =. 2305.15458 , primaryClass =

    doi

  16. [24]

    , year = 1952, month = jan, volume =

    On spherically symmetrical accretion. , year = 1952, month = jan, volume =. doi:10.1093/mnras/112.2.195 , adsurl =

    1952 doi

  17. [25]

    , keywords =

    Where is population III ?. , keywords =. doi:10.1086/159186 , adsurl =

    doi

  18. [26]

    , keywords =

    Streams collision as possible precursor of double tidal disruption events. , keywords =. doi:10.1093/mnras/stz062 , archivePrefix =. 1805.09329 , primaryClass =

    doi arXiv

  19. [27]

    , keywords =

    Partial stellar tidal disruption events and their rates. , keywords =. doi:10.1093/mnras/stad2024 , archivePrefix =. 2303.03408 , primaryClass =

    doi

  20. [28]

    , keywords =

    Generic Spectrum and Ionization Efficiency of a Heavy Initial Mass Function for the First Stars. , keywords =. doi:10.1086/320549 , archivePrefix =. astro-ph/0007248 , primaryClass =

    doi arXiv

  21. [29]

    , keywords =

    The fragmentation of pre-enriched primordial objects. , keywords =. doi:10.1046/j.1365-8711.2001.04915.x , archivePrefix =. astro-ph/0104271 , primaryClass =

    2001 doi

  22. [30]

    The Formation of the First Stars. I. The Primordial Star-forming Cloud. , keywords =. doi:10.1086/323947 , archivePrefix =. astro-ph/0102503 , primaryClass =

    doi arXiv

  23. [31]

    , keywords =

    The First Stars. , keywords =. doi:10.1146/annurev.astro.42.053102.134034 , archivePrefix =. astro-ph/0311019 , primaryClass =

    doi

  24. [32]

    , keywords =

    The formation of the first stars and galaxies. , keywords =. doi:10.1038/nature07990 , archivePrefix =. 0905.0929 , primaryClass =

    doi arXiv

  25. [33]

    , keywords =

    Swift J1112.2-8238: a candidate relativistic tidal disruption flare. , keywords =. doi:10.1093/mnras/stv1520 , archivePrefix =. 1507.03582 , primaryClass =

    doi arXiv

  26. [34]

    , keywords =

    Relativistic jet activity from the tidal disruption of a star by a massive black hole. , keywords =. doi:10.1038/nature10374 , archivePrefix =. 1104.4787 , primaryClass =

    doi arXiv

  27. [35]

    , keywords =

    Effects of Multichannel Active Galactic Nuclei Feedback in FIRE Cosmological Simulations of Massive Galaxies. , keywords =. doi:10.3847/1538-4357/ad67ca , archivePrefix =. 2310.16086 , primaryClass =

    doi

  28. [36]

    , keywords =

    COSMOS-Web: An Overview of the JWST Cosmic Origins Survey. , keywords =. doi:10.3847/1538-4357/acc2bc , archivePrefix =. 2211.07865 , primaryClass =

    doi

  29. [37]

    , keywords =

    The Relationship between Infrared, Optical, and Ultraviolet Extinction. , keywords =. doi:10.1086/167900 , adsurl =

    doi

  30. [38]

    , keywords =

    Swift J2058.4+0516: Discovery of a Possible Second Relativistic Tidal Disruption Flare?. , keywords =. doi:10.1088/0004-637X/753/1/77 , archivePrefix =. 1107.5307 , primaryClass =

    doi arXiv

  31. [39]

    , keywords =

    A detailed spectroscopic study of tidal disruption events. , keywords =. doi:10.1051/0004-6361/202142122 , archivePrefix =. 2109.00016 , primaryClass =

    doi

  32. [40]

    , keywords =

    Detectability of Strongly Gravitationally Lensed Tidal Disruption Events. , keywords =. doi:10.3847/1538-4357/ad19d3 , archivePrefix =. 2401.00992 , primaryClass =

    doi

  33. [41]

    arXiv e-prints , keywords =

    Impact of the Population III Supernova Remnants on the Primeval Galaxy Formation. arXiv e-prints , keywords =. doi:10.48550/arXiv.2211.06016 , archivePrefix =. 2211.06016 , primaryClass =

    doi

  34. [42]

    , keywords =

    Tidal Disruption of a Main-sequence Star by an Intermediate-mass Black Hole: A Bright Decade. , keywords =. doi:10.3847/1538-4357/aadfda , archivePrefix =. 1806.08093 , primaryClass =

    doi arXiv

  35. [43]

    , keywords =

    Supermassive Black Hole Formation at High Redshifts via Direct Collapse: Physical Processes in the Early Stage. , keywords =. doi:10.1088/0004-637X/774/2/149 , archivePrefix =. 1304.1369 , primaryClass =

    doi arXiv

  36. [44]

    Science , keywords =

    The Formation and Fragmentation of Disks Around Primordial Protostars. Science , keywords =. doi:10.1126/science.1198027 , archivePrefix =. 1101.5284 , primaryClass =

    doi arXiv

  37. [45]

    , keywords =

    The impact of AGN-driven winds on physical and observable galaxy sizes. , keywords =. doi:10.1093/mnras/stad1528 , archivePrefix =. 2303.12858 , primaryClass =

    doi

  38. [46]

    , keywords =

    High-z Stellar Masses Can Be Recovered Robustly with JWST Photometry. , keywords =. doi:10.3847/2041-8213/ad9a4d , archivePrefix =. 2412.02622 , primaryClass =

    doi

  39. [47]

    , keywords =

    The stellar distribution around a black hole: numerical integration of the Fokker-Planck equation. , keywords =. doi:10.1086/156685 , adsurl =

    doi

  40. [48]

    , keywords =

    A Mildly Relativistic Outflow from the Energetic, Fast-rising Blue Optical Transient CSS161010 in a Dwarf Galaxy. , keywords =. doi:10.3847/2041-8213/ab8cc7 , archivePrefix =. 2003.10503 , primaryClass =

    doi

  41. [49]

    , keywords =

    Hyperaccretion during Tidal Disruption Events: Weakly Bound Debris Envelopes and Jets. , keywords =. doi:10.1088/0004-637X/781/2/82 , archivePrefix =. 1312.5314 , primaryClass =

    doi arXiv

  42. [50]

    , keywords =

    Structured, relativistic jets driven by radiation. , keywords =. doi:10.1093/mnras/staa3026 , archivePrefix =. 2009.03898 , primaryClass =

    2009 doi

  43. [51]

    , keywords =

    A simple and accurate prescription for the tidal disruption radius of a star and the peak accretion rate in tidal disruption events. , keywords =. doi:10.1093/mnrasl/slac106 , archivePrefix =. 2209.03982 , primaryClass =

    doi

  44. [52]

    , keywords =

    The R136 star cluster hosts several stars whose individual masses greatly exceed the accepted 150M _ solar stellar mass limit. , keywords =. doi:10.1111/j.1365-2966.2010.17167.x , archivePrefix =. 1007.3284 , primaryClass =

    2010 doi

  45. [53]

    , keywords =

    GRRMHD simulations of tidal disruption event accretion discs around supermassive black holes: jet formation, spectra, and detectability. , keywords =. doi:10.1093/mnras/sty3134 , archivePrefix =. 1811.06971 , primaryClass =

    doi arXiv

  46. [54]

    , keywords =

    Soft X-Ray Temperature Tidal Disruption Events from Stars on Deep Plunging Orbits. , keywords =. doi:10.1088/2041-8205/812/2/L39 , archivePrefix =. 1507.04333 , primaryClass =

    doi arXiv

  47. [55]

    , keywords =

    A Unified Model for Tidal Disruption Events. , keywords =. doi:10.3847/2041-8213/aab429 , archivePrefix =. 1803.03265 , primaryClass =

    doi arXiv

  48. [56]

    , keywords =

    The Physics of Accretion Discs, Winds and Jets in Tidal Disruption Events. , keywords =. doi:10.1007/s11214-020-00747-x , adsurl =

    doi

  49. [57]

    , keywords =

    SIMBA: Cosmological simulations with black hole growth and feedback. , keywords =. doi:10.1093/mnras/stz937 , archivePrefix =. 1901.10203 , primaryClass =

    1901 doi arXiv

  50. [58]

    , keywords =

    Decoding the stellar fossils of the dusty Milky Way progenitors. , keywords =. doi:10.1093/mnras/stu1962 , archivePrefix =. 1409.5798 , primaryClass =

    doi arXiv

  51. [59]

    , keywords =

    Radiative hydrodynamical simulations of super-Eddington accretion flow in tidal disruption event: the accretion flow and wind. , keywords =. doi:10.1093/mnras/stad1696 , archivePrefix =. 2306.04313 , primaryClass =

    doi

  52. [60]

    , keywords =

    Populations III.1 and III.2 gamma-ray bursts: constraints on the event rate for future radio and X-ray surveys. , keywords =. doi:10.1051/0004-6361/201117242 , archivePrefix =. 1105.2395 , primaryClass =

    doi arXiv

  53. [61]

    , keywords =

    JWST's PEARLS: Mothra, a new kaiju star at z = 2.091 extremely magnified by MACS0416, and implications for dark matter models. , keywords =. doi:10.1051/0004-6361/202347556 , archivePrefix =. 2307.10363 , primaryClass =

    doi

  54. [62]

    , keywords =

    Direct Cosmological Simulations of the Growth of Black Holes and Galaxies. , keywords =. doi:10.1086/524921 , archivePrefix =. 0705.2269 , primaryClass =

    doi arXiv

  55. [63]

    , keywords =

    The HORIZON-AGN simulation: morphological diversity of galaxies promoted by AGN feedback. , keywords =. doi:10.1093/mnras/stw2265 , archivePrefix =. 1606.03086 , primaryClass =

    doi arXiv

  56. [64]

    arXiv e-prints , keywords =

    Overview of the JWST Advanced Deep Extragalactic Survey (JADES). arXiv e-prints , keywords =. doi:10.48550/arXiv.2306.02465 , archivePrefix =. 2306.02465 , primaryClass =

    doi arXiv

  57. [65]

    , keywords =

    The Tidal Disruption of a Star by a Massive Black Hole. , keywords =. doi:10.1086/185567 , adsurl =

    doi

  58. [66]

    , keywords =

    Simulated optical light curves of super-Eddington tidal disruption events with ZEBRA flows. , keywords =. doi:10.1093/mnras/stac3073 , archivePrefix =. 2210.12168 , primaryClass =

    doi

  59. [67]

    , keywords =

    Colours, star formation rates and environments of star-forming and quiescent galaxies at the cosmic noon. , keywords =. doi:10.1093/mnras/stx1120 , archivePrefix =. 1610.02411 , primaryClass =

    doi arXiv

  60. [68]

    , keywords =

    Correcting for the Effects of Interstellar Extinction. , keywords =. doi:10.1086/316293 , archivePrefix =. astro-ph/9809387 , primaryClass =

    doi arXiv

  61. [69]

    , year = 1964, month = dec, volume =

    Neutrino Processes and Pair Formation in Massive Stars and Supernovae. , year = 1964, month = dec, volume =. doi:10.1086/190103 , adsurl =

    1964 doi

  62. [70]

    , keywords =

    Signatures of circumstellar interaction in the unusual transient AT 2018cow. , keywords =. doi:10.1093/mnras/stz1925 , archivePrefix =. 1903.01535 , primaryClass =

    1903 doi

  63. [71]

    , keywords =

    Effects of massive black holes on dense stellar systems. , keywords =. doi:10.1093/mnras/176.3.633 , adsurl =

    doi

  64. [72]

    , keywords =

    Tidal Disruption Events Prefer Unusual Host Galaxies. , keywords =. doi:10.3847/2041-8205/818/1/L21 , archivePrefix =. 1601.04705 , primaryClass =

    doi arXiv

  65. [73]

    , keywords =

    The Host Galaxies of Tidal Disruption Events. , keywords =. doi:10.1007/s11214-020-00657-y , archivePrefix =. 2003.02863 , primaryClass =

    2003 doi

  66. [74]

    , keywords =

    The James Webb Space Telescope. , keywords =. doi:10.1007/s11214-006-8315-7 , archivePrefix =. astro-ph/0606175 , primaryClass =

    doi arXiv

  67. [75]

    , keywords =

    Luminous Thermal Flares from Quiescent Supermassive Black Holes. , keywords =. doi:10.1088/0004-637X/698/2/1367 , archivePrefix =. 0904.1596 , primaryClass =

    doi arXiv

  68. [76]

    , keywords =

    An ultraviolet-optical flare from the tidal disruption of a helium-rich stellar core. , keywords =. doi:10.1038/nature10990 , archivePrefix =. 1205.0252 , primaryClass =

    doi arXiv

  69. [77]

    , keywords =

    Tidal Disruption Events. , keywords =. doi:10.1146/annurev-astro-111720-030029 , archivePrefix =. 2104.14580 , primaryClass =

    doi

  70. [78]

    , keywords =

    One Relation for All Wavelengths: The Far-ultraviolet to Mid-infrared Milky Way Spectroscopic R(V)-dependent Dust Extinction Relationship. , keywords =. doi:10.3847/1538-4357/accb59 , archivePrefix =. 2304.01991 , primaryClass =

    doi

  71. [79]

    , keywords =

    A Dependence of the Tidal Disruption Event Rate on Global Stellar Surface Mass Density and Stellar Velocity Dispersion. , keywords =. doi:10.3847/1538-4357/aaa3fd , archivePrefix =. 1707.02986 , primaryClass =

    doi arXiv

  72. [80]

    arXiv e-prints , keywords =

    UNCOVER spectroscopy confirms a surprising ubiquity of AGN in red galaxies at z>5. arXiv e-prints , keywords =. doi:10.48550/arXiv.2309.05714 , archivePrefix =. 2309.05714 , primaryClass =

    doi

  73. [81]

    , keywords =

    The First Supernova Explosions: Energetics, Feedback, and Chemical Enrichment. , keywords =. doi:10.1086/522028 , archivePrefix =. 0705.3048 , primaryClass =

    doi arXiv

  74. [82]

    , keywords =

    Simulations on a Moving Mesh: The Clustered Formation of Population III Protostars. , keywords =. doi:10.1088/0004-637X/737/2/75 , archivePrefix =. 1101.5491 , primaryClass =

    doi arXiv

  75. [83]

    , keywords =

    eRO-ExTra: eROSITA extragalactic non-AGN X-ray transients and variables in eRASS1 and eRASS2. , keywords =. doi:10.1051/0004-6361/202451253 , archivePrefix =. 2501.04208 , primaryClass =

    doi

  76. [84]

    , keywords =

    Hydrodynamical Simulations to Determine the Feeding Rate of Black Holes by the Tidal Disruption of Stars: The Importance of the Impact Parameter and Stellar Structure. , keywords =. doi:10.1088/0004-637X/767/1/25 , archivePrefix =. 1206.2350 , primaryClass =

    doi arXiv

  77. [85]

    , keywords =

    Multi-scale initial conditions for cosmological simulations. , keywords =. doi:10.1111/j.1365-2966.2011.18820.x , archivePrefix =. 1103.6031 , primaryClass =

    2011 doi

  78. [86]

    , keywords =

    JWST UNCOVER: discovery of z > 9 galaxy candidates behind the lensing cluster Abell 2744. , keywords =. doi:10.1093/mnras/stad1998 , archivePrefix =. 2305.01793 , primaryClass =

    doi

  79. [87]

    , keywords =

    Tidal Disruption Event Hosts Are Green and Centrally Concentrated: Signatures of a Post-merger System. , keywords =. doi:10.3847/2041-8213/abdcb4 , archivePrefix =. 2010.10738 , primaryClass =

    doi

  80. [88]

    arXiv e-prints , keywords =

    NANCY: Next-generation All-sky Near-infrared Community surveY. arXiv e-prints , keywords =. doi:10.48550/arXiv.2306.11784 , archivePrefix =. 2306.11784 , primaryClass =

    doi

  81. [89]

    arXiv e-prints , keywords =

    Counting the Unseen II: Tidal Disruption Event Rates in Nearby Galaxies with REPTiDE. arXiv e-prints , keywords =. doi:10.48550/arXiv.2412.19935 , archivePrefix =. 2412.19935 , primaryClass =

    doi

  82. [90]

    , keywords =

    FOREVER22: The first bright galaxies with population III stars at redshifts z ≃ 10-20 and comparisons with JWST data. , keywords =. doi:10.1093/mnras/stad2497 , archivePrefix =. 2211.12970 , primaryClass =

    doi

  83. [91]

    , keywords =

    Possible power source of Seyfert galaxies and QSOs. , keywords =. doi:10.1038/254295a0 , adsurl =

    doi

  84. [92]

    , keywords =

    Primordial star formation under the influence of far ultraviolet radiation: 1540 cosmological haloes and the stellar mass distribution. , keywords =. doi:10.1093/mnras/stv044 , archivePrefix =. 1501.01630 , primaryClass =

    doi arXiv

  85. [93]

    , keywords =

    The Koala: A Fast Blue Optical Transient with Luminous Radio Emission from a Starburst Dwarf Galaxy at z = 0.27. , keywords =. doi:10.3847/1538-4357/ab8bcf , archivePrefix =. 2003.01222 , primaryClass =

    2003 doi

  86. [94]

    arXiv e-prints , keywords =

    The K correction. arXiv e-prints , keywords =. doi:10.48550/arXiv.astro-ph/0210394 , archivePrefix =. astro-ph/0210394 , primaryClass =

    doi arXiv

  87. [95]

    , keywords =

    An analytic model of angular momentum transport by gravitational torques: from galaxies to massive black holes. , keywords =. doi:10.1111/j.1365-2966.2011.18542.x , archivePrefix =. 1007.2647 , primaryClass =

    2011 doi

  88. [96]

    , keywords =

    A new class of accurate, mesh-free hydrodynamic simulation methods. , keywords =. doi:10.1093/mnras/stv195 , archivePrefix =. 1409.7395 , primaryClass =

    doi arXiv

  89. [97]

    , keywords =

    FIRE-2 simulations: physics versus numerics in galaxy formation. , keywords =. doi:10.1093/mnras/sty1690 , archivePrefix =. 1702.06148 , primaryClass =

    doi arXiv

  90. [98]

    , keywords =

    But what about...: cosmic rays, magnetic fields, conduction, and viscosity in galaxy formation. , keywords =. doi:10.1093/mnras/stz3321 , archivePrefix =. 1905.04321 , primaryClass =

    1905 doi

  91. [99]

    , keywords =

    The proto-galaxy of Milky Way-mass haloes in the FIRE simulations. , keywords =. doi:10.1093/mnras/stad3834 , archivePrefix =. 2307.15741 , primaryClass =

    doi

  92. [100]

    , keywords =

    Rapidly Accreting Supergiant Protostars: Embryos of Supermassive Black Holes?. , keywords =. doi:10.1088/0004-637X/756/1/93 , archivePrefix =. 1203.2613 , primaryClass =

    doi arXiv

  93. [101]

    , year = 1941, month = jan, volume =

    On the accretion theory of stellar evolution. , year = 1941, month = jan, volume =. doi:10.1093/mnras/101.4.227 , adsurl =

    1941 doi

  94. [102]

    , keywords =

    The Source Density and Observability of Pair-instability Supernovae from the First Stars. , keywords =. doi:10.1088/0004-637X/755/1/72 , archivePrefix =. 1112.5207 , primaryClass =

    doi arXiv

  95. [103]

    , keywords =

    Exploring Low-mass Black Holes through Tidal Disruption Events in the Early Universe: Perspectives in the Era of the JWST, Roman Space Telescope, and LSST Surveys. , keywords =. doi:10.3847/1538-4357/ad344c , archivePrefix =. 2312.11602 , primaryClass =

    doi

  96. [104]

    , keywords =

    LSST: From Science Drivers to Reference Design and Anticipated Data Products. , keywords =. doi:10.3847/1538-4357/ab042c , archivePrefix =. 0805.2366 , primaryClass =

    doi arXiv

  97. [105]

    , keywords =

    Baseline metal enrichment from Population III star formation in cosmological volume simulations. , keywords =. doi:10.1093/mnras/sty062 , archivePrefix =. 1705.08059 , primaryClass =

    doi arXiv

  98. [106]

    , keywords =

    Super-Eddington Accretion Disks around Supermassive Black Holes. , keywords =. doi:10.3847/1538-4357/ab29ff , archivePrefix =. 1709.02845 , primaryClass =

    doi

  99. [107]

    , keywords =

    Significant primordial star formation at redshifts z -0.5ex 3 4. , keywords =. doi:10.1038/nature04580 , archivePrefix =. astro-ph/0602450 , primaryClass =

    doi arXiv

  100. [108]

    arXiv e-prints , keywords =

    An Intermediate-mass Black Hole Lurking in A Galactic Halo Caught Alive during Outburst. arXiv e-prints , keywords =. doi:10.48550/arXiv.2501.09580 , archivePrefix =. 2501.09580 , primaryClass =

    doi

  101. [109]

    , keywords =

    Local Radiative Feedback in the Formation of the First Protogalaxies. , keywords =. doi:10.1086/519212 , archivePrefix =. astro-ph/0612254 , primaryClass =

    doi arXiv

  102. [110]

    , keywords =

    Ultrafast outflow in tidal disruption event ASASSN-14li. , keywords =. doi:10.1093/mnras/stx3004 , archivePrefix =. 1711.06090 , primaryClass =

    doi arXiv

  103. [111]

    arXiv e-prints , keywords =

    JWST Discovery of a High-Redshift Tidal Disruption Event Candidate in COSMOS-Web. arXiv e-prints , keywords =. doi:10.48550/arXiv.2504.13248 , archivePrefix =. 2504.13248 , primaryClass =

    doi

  104. [112]

    arXiv e-prints , keywords =

    Tidal disruption event rates across cosmic time: forecasts for LSST, Roman, and JWST and their constraints on the supermassive black hole mass function. arXiv e-prints , keywords =. doi:10.48550/arXiv.2602.04947 , archivePrefix =. 2602.04947 , primaryClass =

    doi

  105. [113]

    , keywords =

    Highly Magnified Stars in Lensing Clusters: New Evidence in a Galaxy Lensed by MACS J0416.1-2403. , keywords =. doi:10.3847/1538-4357/ab2888 , archivePrefix =. 1902.10090 , primaryClass =

    1902 doi

  106. [114]

    Advances in Astronomy , keywords =

    Mass Functions of Supermassive Black Holes across Cosmic Time. Advances in Astronomy , keywords =. doi:10.1155/2012/970858 , archivePrefix =. 1112.1430 , primaryClass =

    2012 doi arXiv

  107. [115]

    Nature Astronomy , keywords =

    Extreme magnification of an individual star at redshift 1.5 by a galaxy-cluster lens. Nature Astronomy , keywords =. doi:10.1038/s41550-018-0430-3 , archivePrefix =. 1706.10279 , primaryClass =

    doi arXiv

  108. [116]

    , keywords =

    Tidal-disruption rate of stars by spinning supermassive black holes. , keywords =. doi:10.1103/PhysRevD.85.024037 , archivePrefix =. 1109.6329 , primaryClass =

    doi arXiv

  109. [117]

    Stellar Structure and Evolution

  110. [118]

    2023 , eprint=

    The first stars: formation, properties, and impact , author=. 2023 , eprint=

    2023

  111. [119]

    , keywords =

    Tidal disruption event demographics. , keywords =. doi:10.1093/mnras/stw1290 , archivePrefix =. 1601.06787 , primaryClass =

    doi arXiv

  112. [120]

    , keywords =

    On the variation of the initial mass function. , keywords =. doi:10.1046/j.1365-8711.2001.04022.x , archivePrefix =. astro-ph/0009005 , primaryClass =

    2001 doi

  113. [121]

    Science , keywords =

    The Initial Mass Function of Stars: Evidence for Uniformity in Variable Systems. Science , keywords =. doi:10.1126/science.1067524 , archivePrefix =. astro-ph/0201098 , primaryClass =

    doi arXiv

  114. [122]

    , keywords =

    Swift spectra of AT2018cow: a white dwarf tidal disruption event?. , keywords =. doi:10.1093/mnras/stz053 , archivePrefix =. 1808.08492 , primaryClass =

    doi arXiv

  115. [123]

    , keywords =

    Chemical Constraints on the Contribution of Population III Stars to Cosmic Reionization. , keywords =. doi:10.1088/0004-637X/787/1/64 , archivePrefix =. 1310.0684 , primaryClass =

    doi arXiv

  116. [124]

    , keywords =

    On the origin of star formation quenching in massive galaxies at z 3 in the cosmological simulations IllustrisTNG. , keywords =. doi:10.1093/mnras/stae2297 , archivePrefix =. 2310.03083 , primaryClass =

    doi

  117. [125]

    , keywords =

    A population of red candidate massive galaxies 600 Myr after the Big Bang. , keywords =. doi:10.1038/s41586-023-05786-2 , archivePrefix =. 2207.12446 , primaryClass =

    doi

  118. [126]

    , keywords =

    The nature of the central parsec of the Galaxy. , keywords =. doi:10.1086/160402 , adsurl =

    doi

  119. [127]

    , keywords =

    Probing the initial mass function of the first stars with transients. , keywords =. doi:10.1093/mnras/stac176 , archivePrefix =. 2110.11956 , primaryClass =

    doi

  120. [128]

    , keywords =

    Tidal Disruption Event Host Galaxies in the Context of the Local Galaxy Population. , keywords =. doi:10.3847/1538-4357/aa94c7 , archivePrefix =. 1707.01559 , primaryClass =

    doi arXiv

  121. [129]

    , keywords =

    Stellar Tidal Disruption Events with Abundances and Realistic Structures (STARS): Library of Fallback Rates. , keywords =. doi:10.3847/1538-4357/abc489 , archivePrefix =. 2007.10996 , primaryClass =

    2007 doi

  122. [130]

    , keywords =

    Growth of a Massive Black Hole in a Dense Star Cluster Via Tidal Disruption Accretion. , keywords =. doi:10.3847/1538-4357/aca75d , archivePrefix =. 2211.02376 , primaryClass =

    doi

  123. [131]

    Nature Astronomy , keywords =

    The superluminous transient ASASSN-15lh as a tidal disruption event from a Kerr black hole. Nature Astronomy , keywords =. doi:10.1038/s41550-016-0002 , archivePrefix =. 1609.02927 , primaryClass =

    doi arXiv

  124. [132]

    , keywords =

    The Spectral Evolution of AT 2018dyb and the Presence of Metal Lines in Tidal Disruption Events. , keywords =. doi:10.3847/1538-4357/ab5792 , archivePrefix =. 1903.03120 , primaryClass =

    1903 doi

  125. [133]

    Science , keywords =

    An Extremely Luminous Panchromatic Outburst from the Nucleus of a Distant Galaxy. Science , keywords =. doi:10.1126/science.1207143 , archivePrefix =. 1104.3356 , primaryClass =

    doi arXiv

  126. [134]

    Nature Astronomy , keywords =

    A luminous X-ray outburst from an intermediate-mass black hole in an off-centre star cluster. Nature Astronomy , keywords =. doi:10.1038/s41550-018-0493-1 , archivePrefix =. 1806.05692 , primaryClass =

    doi arXiv

  127. [135]

    , keywords =

    When did Population III star formation end?. , keywords =. doi:10.1093/mnras/staa2143 , archivePrefix =. 2006.15260 , primaryClass =

    2006 doi

  128. [136]

    , keywords =

    The UV/Optical Peak and X-Ray Brightening in TDE Candidate AT 2019azh: A Case of Stream-Stream Collision and Delayed Accretion. , keywords =. doi:10.3847/1538-4357/ac33a9 , adsurl =

    doi

  129. [137]

    , keywords =

    Multiband light curves of tidal disruption events. , keywords =. doi:10.1111/j.1365-2966.2010.17448.x , archivePrefix =. 1008.4589 , primaryClass =

    2010 doi

  130. [138]

    , keywords =

    Collapse of Primordial Gas Clouds and the Formation of Quasar Black Holes. , keywords =. doi:10.1086/174548 , archivePrefix =. astro-ph/9401026 , primaryClass =

    doi arXiv

  131. [139]

    , keywords =

    Optical Appearance of the Debris of a Star Disrupted by a Massive Black Hole. , keywords =. doi:10.1086/304814 , archivePrefix =. astro-ph/9703079 , primaryClass =

    doi arXiv

  132. [140]

    , keywords =

    Self-intersection of the fallback stream in tidal disruption events. , keywords =. doi:10.1093/mnras/stz3405 , archivePrefix =. 1904.12018 , primaryClass =

    1904 doi

  133. [141]

    , keywords =

    Fast-rising blue optical transients and AT2018cow following electron-capture collapse of merged white dwarfs. , keywords =. doi:10.1093/mnras/stz1640 , archivePrefix =. 1812.07569 , primaryClass =

    doi

  134. [142]

    , keywords =

    Cosmic Star-Formation History. , keywords =. doi:10.1146/annurev-astro-081811-125615 , archivePrefix =. 1403.0007 , primaryClass =

    doi arXiv

  135. [143]

    , keywords =

    Effect of the cosmological transition to metal-enriched star formation on the hydrogen 21-cm signal. , keywords =. doi:10.1093/mnras/stac1664 , archivePrefix =. 2110.15948 , primaryClass =

    doi

  136. [144]

    , keywords =

    Rates of tidal disruption of stars by massive central black holes. , keywords =. doi:10.1046/j.1365-8711.1999.02853.x , archivePrefix =. astro-ph/9902032 , primaryClass =

    1999 doi

  137. [145]

    Early Results from GLASS-JWST. III. Galaxy Candidates at z 9-15. , keywords =. doi:10.3847/2041-8213/ac94d0 , archivePrefix =. 2207.09436 , primaryClass =

    doi

  138. [146]

    , keywords =

    An Embedded X-Ray Source Shines through the Aspherical AT 2018cow: Revealing the Inner Workings of the Most Luminous Fast-evolving Optical Transients. , keywords =. doi:10.3847/1538-4357/aafa01 , archivePrefix =. 1810.10720 , primaryClass =

    doi arXiv

  139. [147]

    , keywords =

    First results from the IllustrisTNG simulations: radio haloes and magnetic fields. , keywords =. doi:10.1093/mnras/sty2206 , archivePrefix =. 1707.03396 , primaryClass =

    doi arXiv

  140. [148]

    The Formation of the First Stars. II. Radiative Feedback Processes and Implications for the Initial Mass Function. , keywords =. doi:10.1086/587434 , archivePrefix =. 0711.1377 , primaryClass =

    doi arXiv

  141. [149]

    , keywords =

    Two Lensed Star Candidates at z ≃ 4.8 behind the Galaxy Cluster MACS J0647.7+7015. , keywords =. doi:10.3847/2041-8213/acb645 , archivePrefix =. 2211.13334 , primaryClass =

    doi

  142. [150]

    , keywords =

    Tidal Disruption Events from the Combined Effects of Two-body Relaxation and the Eccentric Kozai-Lidov Mechanism. , keywords =. doi:10.3847/1538-4357/acfee0 , archivePrefix =. 2306.05472 , primaryClass =

    doi

  143. [151]

    arXiv e-prints , keywords =

    Tidal Disruption Event Demographics in Supermassive Black Hole Binaries Over Cosmic Times. arXiv e-prints , keywords =. doi:10.48550/arXiv.2507.08082 , archivePrefix =. 2507.08082 , primaryClass =

    doi

  144. [152]

    , keywords =

    The First Gamma-Ray Bursts in the Universe. , keywords =. doi:10.1088/0004-637X/787/1/91 , archivePrefix =. 1401.5565 , primaryClass =

    doi arXiv

  145. [153]

    , keywords =

    A bright year for tidal disruptions. , keywords =. doi:10.1093/mnras/stw1394 , archivePrefix =. 1506.03453 , primaryClass =

    doi arXiv

  146. [154]

    , keywords =

    Cooling Envelope Model for Tidal Disruption Events. , keywords =. doi:10.3847/2041-8213/ac90ba , archivePrefix =. 2207.07136 , primaryClass =

    doi

  147. [155]

    arXiv e-prints , keywords =

    A small and vigorous black hole in the early Universe. arXiv e-prints , keywords =. doi:10.48550/arXiv.2305.12492 , archivePrefix =. 2305.12492 , primaryClass =

    doi

  148. [156]

    , keywords =

    Luminous Fast Blue Optical Transients and Type Ibn/Icn SNe from Wolf-Rayet/Black Hole Mergers. , keywords =. doi:10.3847/1538-4357/ac6d59 , archivePrefix =. 2203.04331 , primaryClass =

    doi

  149. [157]

    , keywords =

    Flows of X-ray gas reveal the disruption of a star by a massive black hole. , keywords =. doi:10.1038/nature15708 , archivePrefix =. 1510.06348 , primaryClass =

    doi arXiv

  150. [158]

    , keywords =

    Disk Winds as an Explanation for Slowly Evolving Temperatures in Tidal Disruption Events. , keywords =. doi:10.1088/0004-637X/805/1/83 , archivePrefix =. 1502.03284 , primaryClass =

    doi arXiv

  151. [159]

    , keywords =

    Weighing Black Holes Using Tidal Disruption Events. , keywords =. doi:10.3847/1538-4357/ab010f , archivePrefix =. 1801.08221 , primaryClass =

    doi arXiv

  152. [160]

    Journal of Astronomical Telescopes, Instruments, and Systems , keywords =

    Properties and characteristics of the Nancy Grace Roman Space Telescope H4RG-10 detectors. Journal of Astronomical Telescopes, Instruments, and Systems , keywords =. doi:10.1117/1.JATIS.6.4.046001 , archivePrefix =. 2005.00505 , primaryClass =

    2005 doi

  153. [161]

    , keywords =

    Ionizing photon production of Population III stars: effects of rotation, convection, and initial mass function. , keywords =. doi:10.1093/mnras/stab2073 , archivePrefix =. 2105.06900 , primaryClass =

    doi

  154. [162]

    , keywords =

    First Detection of an Overmassive Black Hole Galaxy UHZ1: Evidence for Heavy Black Hole Seed Formation from Direct Collapse. , keywords =. doi:10.3847/2041-8213/ad0e76 , archivePrefix =. 2308.02654 , primaryClass =

    doi

  155. [163]

    Computational Astrophysics and Cosmology , keywords =

    The IllustrisTNG simulations: public data release. Computational Astrophysics and Cosmology , keywords =. doi:10.1186/s40668-019-0028-x , archivePrefix =. 1812.05609 , primaryClass =

    doi

  156. [164]

    General Relativity and Gravitation , keywords =

    Signatures of population III supernovae at Cosmic Dawn: the case of GN-z11-flash. General Relativity and Gravitation , keywords =. doi:10.1007/s10714-022-02909-4 , archivePrefix =. 2101.12222 , primaryClass =

    doi

  157. [165]

    Critical halo mass of formation and total mass in stars

    Population III star formation in an X-ray background - I. Critical halo mass of formation and total mass in stars. , keywords =. doi:10.1093/mnras/stab2999 , archivePrefix =. 2107.07883 , primaryClass =

    doi

  158. [166]

    Protostellar discs, multiplicity, and mass function of the stars

    Population III star formation in an X-ray background - II. Protostellar discs, multiplicity, and mass function of the stars. , keywords =. doi:10.1093/mnras/stab3000 , archivePrefix =. 2107.07898 , primaryClass =

    doi

  159. [167]

    , keywords =

    Generating dark matter halo merger trees. , keywords =. doi:10.1111/j.1365-2966.2007.12517.x , archivePrefix =. 0708.1382 , primaryClass =

    2007 doi

  160. [168]

    , keywords =

    Realistic mock observations of the sizes and stellar mass surface densities of massive galaxies in FIRE-2 zoom-in simulations. , keywords =. doi:10.1093/mnras/staa3765 , archivePrefix =. 2009.10161 , primaryClass =

    2009 doi

  161. [169]

    arXiv e-prints , keywords =

    JWST and Keck observations of the off-nuclear tidal disruption event TDE 2025abcr: An evolving reprocessing layer. arXiv e-prints , keywords =

  162. [170]

    , keywords =

    Modules for Experiments in Stellar Astrophysics (MESA). , keywords =. doi:10.1088/0067-0049/192/1/3 , archivePrefix =. 1009.1622 , primaryClass =

    doi arXiv

  163. [171]

    , keywords =

    The fast, luminous ultraviolet transient AT2018cow: extreme supernova, or disruption of a star by an intermediate-mass black hole?. , keywords =. doi:10.1093/mnras/sty3420 , archivePrefix =. 1808.00969 , primaryClass =

    doi arXiv

  164. [172]

    , keywords =

    Real-time discovery of AT2020xnd: a fast, luminous ultraviolet transient with minimal radioactive ejecta. , keywords =. doi:10.1093/mnras/stab2785 , archivePrefix =. 2103.01968 , primaryClass =

    doi

  165. [173]

    , keywords =

    Resolved stellar population properties of PHANGS-MUSE galaxies. , keywords =. doi:10.1051/0004-6361/202245673 , archivePrefix =. 2303.13676 , primaryClass =

    doi

  166. [174]

    , keywords =

    Tidal disruption event rates in galaxy merger remnants. , keywords =. doi:10.1093/mnrasl/slz091 , archivePrefix =. 1903.09124 , primaryClass =

    1903 doi

  167. [175]

    , keywords =

    Enhancement of the tidal disruption event rate in galaxies with a nuclear star cluster: from dwarfs to ellipticals. , keywords =. doi:10.1093/mnras/staa1962 , archivePrefix =. 2003.08133 , primaryClass =

    2003 doi

  168. [176]

    , keywords =

    Tidal disruption events in the first billion years of a galaxy. , keywords =. doi:10.1093/mnras/staa3471 , archivePrefix =. 2006.06565 , primaryClass =

    2006 doi

  169. [177]

    , keywords =

    Observable gravitational waves from tidal disruption events and their electromagnetic counterpart. , keywords =. doi:10.1093/mnras/stab3387 , archivePrefix =. 2103.05883 , primaryClass =

    doi

  170. [178]

    The Center of the Galaxy , year = 1989, editor =

    Manifestations of a Massive Black Hole in the Galactic Center. The Center of the Galaxy , year = 1989, editor =

    1989

  171. [179]

    , keywords =

    ‧Disk Formation Versus Disk Accretion What Powers Tidal Disruption Events?. , keywords =. doi:10.1088/0004-637X/806/2/164 , archivePrefix =. 1502.05792 , primaryClass =

    doi arXiv

  172. [180]

    Planck 2015 results. XIII. Cosmological parameters. , keywords =. doi:10.1051/0004-6361/201525830 , archivePrefix =. 1502.01589 , primaryClass =

    2015 doi arXiv

  173. [181]

    Volumetric TDE rates and the abundance of nuclear star clusters

    Demographics of tidal disruption events with L-Galaxies: I. Volumetric TDE rates and the abundance of nuclear star clusters. , keywords =. doi:10.1051/0004-6361/202449470 , archivePrefix =. 2312.13242 , primaryClass =

    doi

  174. [182]

    , keywords =

    The Cow: Discovery of a Luminous, Hot, and Rapidly Evolving Transient. , keywords =. doi:10.3847/2041-8213/aadd90 , archivePrefix =. 1807.05965 , primaryClass =

    doi arXiv

  175. [183]

    , keywords =

    From dark matter halos to pre-stellar cores: high resolution follow-up of cosmological Lyman-Werner simulations. , keywords =. doi:10.1093/mnras/stad188 , archivePrefix =. 2301.00828 , primaryClass =

    doi

  176. [184]

    , keywords =

    The fundamental plane of early-type galaxies: non-homology of the spatial structure. , keywords =

  177. [185]

    , keywords =

    Tidal disruption of stars by black holes of 10 ^ 6 - 10 ^ 8 solar masses in nearby galaxies. , keywords =. doi:10.1038/333523a0 , adsurl =

    doi

  178. [186]

    , keywords =

    Detecting Pair-instability Supernovae at z 5 with the James Webb Space Telescope. , keywords =. doi:10.3847/1538-4357/ab8636 , archivePrefix =. 2002.07854 , primaryClass =

    2002 doi

  179. [187]

    , keywords =

    Recipes for Jet Feedback and Spin Evolution of Black Holes with Strongly Magnetized Super-Eddington Accretion Disks. , keywords =. doi:10.3847/2041-8213/aceda5 , archivePrefix =. 2307.04621 , primaryClass =

    doi

  180. [188]

    , keywords =

    Unveiling the Population of Wandering Black Holes via Electromagnetic Signatures. , keywords =. doi:10.3847/2041-8213/ac1170 , archivePrefix =. 2107.02132 , primaryClass =

    doi

  181. [189]

    , keywords =

    A low-metallicity massive contact binary undergoing slow Case A mass transfer: A detailed spectroscopic and orbital analysis of SSN 7 in NGC 346 in the SMC. , keywords =. doi:10.1051/0004-6361/202346055 , archivePrefix =. 2304.13720 , primaryClass =

    doi

  182. [190]

    , keywords =

    The X-Ray through Optical Fluxes and Line Strengths of Tidal Disruption Events. , keywords =. doi:10.3847/0004-637X/827/1/3 , archivePrefix =. 1510.08454 , primaryClass =

    doi arXiv

  183. [191]

    , keywords =

    Radiative Emission Mechanisms. , keywords =. doi:10.1007/s11214-020-00735-1 , archivePrefix =. 2008.01117 , primaryClass =

    2008 doi

  184. [192]

    , keywords =

    Detection of isolated Population III stars with the James Webb Space Telescope. , keywords =. doi:10.1093/mnras/sts653 , archivePrefix =. 1206.0007 , primaryClass =

    doi arXiv

  185. [193]

    , keywords =

    Impact of magnetic fields on Population III star formation. , keywords =. doi:10.1093/mnras/stac2479 , archivePrefix =. 2208.14931 , primaryClass =

    doi

  186. [194]

    , keywords =

    Three-dimensional simulations of supercritical black hole accretion discs - luminosities, photon trapping and variability. , keywords =. doi:10.1093/mnras/stv2941 , archivePrefix =. 1509.03168 , primaryClass =

    doi arXiv

  187. [195]

    , keywords =

    Science with a Wide-field UV Transient Explorer. , keywords =. doi:10.1088/0004-6256/147/4/79 , archivePrefix =. 1303.6194 , primaryClass =

    doi arXiv

  188. [196]

    arXiv e-prints , keywords =

    Essentials of strong gravitational lensing. arXiv e-prints , keywords =. doi:10.48550/arXiv.2401.04165 , archivePrefix =. 2401.04165 , primaryClass =

    doi

  189. [197]

    , keywords =

    X-Ray Properties of TDEs. , keywords =. doi:10.1007/s11214-020-00708-4 , adsurl =

    doi

  190. [198]

    , keywords =

    First tidal disruption events discovered by SRG/eROSITA: X-ray/optical properties and X-ray luminosity function at z < 0.6. , keywords =. doi:10.1093/mnras/stab2843 , archivePrefix =. 2108.02449 , primaryClass =

    doi

  191. [199]

    , keywords =

    The Detectability of the First Stars and Their Cluster Enrichment Signatures. , keywords =. doi:10.1086/374412 , archivePrefix =. astro-ph/0301628 , primaryClass =

    doi arXiv

  192. [200]

    , keywords =

    The transition from Population III to normal galaxies: Lyalpha and He II emission and the ionising properties of high redshift starburst galaxies. , keywords =. doi:10.1051/0004-6361:20021525 , archivePrefix =. astro-ph/0210462 , primaryClass =

    doi arXiv

  193. [201]

    , keywords =

    On the Probability of the Extremely Lensed z = 6.2 Earendel Source Being a Population III Star. , keywords =. doi:10.3847/2041-8213/ac7f9a , archivePrefix =. 2207.02863 , primaryClass =

    doi

  194. [202]

    , keywords =

    First Stars, Very Massive Black Holes, and Metals. , keywords =. doi:10.1086/339917 , archivePrefix =. astro-ph/0111341 , primaryClass =

    doi arXiv

  195. [203]

    Boletin de la Asociacion Argentina de Astronomia La Plata Argentina , year = 1963, month = feb, volume =

    Influence of the atmospheric and instrumental dispersion on the brightness distribution in a galaxy. Boletin de la Asociacion Argentina de Astronomia La Plata Argentina , year = 1963, month = feb, volume =

    1963

  196. [204]

    , keywords =

    General Relativistic Hydrodynamic Simulation of Accretion Flow from a Stellar Tidal Disruption. , keywords =. doi:10.1088/0004-637X/804/2/85 , archivePrefix =. 1501.04365 , primaryClass =

    doi arXiv

  197. [205]

    Nature Communications , keywords =

    X-ray flares from the stellar tidal disruption by a candidate supermassive black hole binary. Nature Communications , keywords =. doi:10.1038/s41467-020-19675-z , archivePrefix =. 2012.11818 , primaryClass =

    2012 doi

  198. [206]

    , keywords =

    ULTRASAT: A Wide-field Time-domain UV Space Telescope. , keywords =. doi:10.3847/1538-4357/ad2704 , archivePrefix =. 2304.14482 , primaryClass =

    doi

  199. [207]

    arXiv e-prints , keywords =

    Wide-Field InfrarRed Survey Telescope-Astrophysics Focused Telescope Assets WFIRST-AFTA 2015 Report. arXiv e-prints , keywords =. doi:10.48550/arXiv.1503.03757 , archivePrefix =. 1503.03757 , primaryClass =

    2015 doi arXiv

  200. [208]

    , keywords =

    Modelling feedback from stars and black holes in galaxy mergers. , keywords =. doi:10.1111/j.1365-2966.2005.09238.x , archivePrefix =. astro-ph/0411108 , primaryClass =

    2005 doi

  201. [209]

    , keywords =

    Cosmic reionization by stellar sources: population III stars. , keywords =. doi:10.1111/j.1365-2966.2004.07636.x , archivePrefix =. astro-ph/0307451 , primaryClass =

    2004 doi

  202. [210]

    VLASS Tidal Disruption Events with Optical Flares. I. The Sample and a Comparison to Optically Selected TDEs. , keywords =. doi:10.3847/1538-4357/adba4f , archivePrefix =. 2310.03791 , primaryClass =

    doi

  203. [211]

    , keywords =

    Constraining the statistics of Population III binaries. , keywords =. doi:10.1093/mnras/stt789 , archivePrefix =. 1211.1889 , primaryClass =

    doi arXiv

  204. [212]

    , keywords =

    Consequences of strong compression in tidal disruption events. , keywords =. doi:10.1093/mnras/stt1270 , archivePrefix =. 1210.3374 , primaryClass =

    doi arXiv

  205. [213]

    , keywords =

    An Enhanced Rate of Tidal Disruptions in the Centrally Overdense E+A Galaxy NGC 3156. , keywords =. doi:10.3847/2041-8205/825/1/L14 , archivePrefix =. 1604.02056 , primaryClass =

    doi arXiv

  206. [214]

    , keywords =

    Rates of stellar tidal disruption as probes of the supermassive black hole mass function. , keywords =. doi:10.1093/mnras/stv2281 , archivePrefix =. 1410.7772 , primaryClass =

    doi arXiv

  207. [215]

    , keywords =

    Rates of Stellar Tidal Disruption. , keywords =. doi:10.1007/s11214-020-00651-4 , archivePrefix =. 2003.08953 , primaryClass =

    2003 doi

  208. [216]

    Snacktime for Hungry Black Holes: Theoretical Studies of the Tidal Disruption of Stars

  209. [217]

    , keywords =

    Optical flares from the tidal disruption of stars by massive black holes. , keywords =. doi:10.1111/j.1365-2966.2009.15599.x , archivePrefix =. 0905.3735 , primaryClass =

    2009 doi

  210. [218]

    arXiv e-prints , keywords =

    Strong lensing of tidal disruption events: Detection rates in imaging surveys. arXiv e-prints , keywords =. doi:10.48550/arXiv.2402.03443 , archivePrefix =. 2402.03443 , primaryClass =

    doi

  211. [219]

    , keywords =

    Broad-line AGNs at 3.5 < z < 6: The Black Hole Mass Function and a Connection with Little Red Dots. , keywords =. doi:10.3847/1538-4357/add15b , archivePrefix =. 2409.06772 , primaryClass =

    doi

  212. [220]

    , keywords =

    Dynamical Unification of Tidal Disruption Events. , keywords =. doi:10.3847/2041-8213/ac911f , archivePrefix =. 2206.02804 , primaryClass =

    doi

  213. [221]

    , keywords =

    Population III stars: hidden or disappeared?. , keywords =. doi:10.1111/j.1365-2966.2007.12215.x , archivePrefix =. 0707.1433 , primaryClass =

    2007 doi

  214. [222]

    , keywords =

    The Romulus cosmological simulations: a physical approach to the formation, dynamics and accretion models of SMBHs. , keywords =. doi:10.1093/mnras/stx1160 , archivePrefix =. 1607.02151 , primaryClass =

    doi arXiv

  215. [223]

    , keywords =

    The low-end of the black hole mass function at cosmic dawn. , keywords =. doi:10.1093/mnras/stac062 , archivePrefix =. 2201.02630 , primaryClass =

    doi

  216. [224]

    , keywords =

    From the first stars to the first black holes. , keywords =. doi:10.1093/mnras/stw225 , archivePrefix =. 1601.07915 , primaryClass =

    doi arXiv

  217. [225]

    , keywords =

    Seventeen Tidal Disruption Events from the First Half of ZTF Survey Observations: Entering a New Era of Population Studies. , keywords =. doi:10.3847/1538-4357/abc258 , archivePrefix =. 2001.01409 , primaryClass =

    2001 doi

  218. [226]

    , keywords =

    Candidate Population III stellar complex at z = 6.629 in the MUSE Deep Lensed Field. , keywords =. doi:10.1093/mnrasl/slaa041 , archivePrefix =. 2001.03619 , primaryClass =

    2001 doi

  219. [227]

    , keywords =

    A New Fokker-Planck Approach for the Relaxation-driven Evolution of Galactic Nuclei. , keywords =. doi:10.3847/1538-4357/aa8cc8 , archivePrefix =. 1709.04467 , primaryClass =

    doi arXiv

  220. [228]

    , keywords =

    AGAMA: action-based galaxy modelling architecture. , keywords =. doi:10.1093/mnras/sty2672 , archivePrefix =. 1802.08239 , primaryClass =

    doi arXiv

  221. [229]

    , keywords =

    Conditions for detecting lensed Population III galaxies in blind surveys with the James Webb Space Telescope, the Roman Space Telescope, and Euclid. , keywords =. doi:10.1093/mnras/stac488 , archivePrefix =. 2107.01230 , primaryClass =

    doi

  222. [230]

    , keywords =

    Finding Lensed Direct-collapse Black Holes and Supermassive Primordial Stars. , keywords =. doi:10.3847/2041-8213/ac7802 , archivePrefix =. 2205.14163 , primaryClass =

    doi

  223. [231]

    , keywords =

    Revised Rates of Stellar Disruption in Galactic Nuclei. , keywords =. doi:10.1086/379767 , archivePrefix =. astro-ph/0305493 , primaryClass =

    doi arXiv

  224. [232]

    , keywords =

    The High Latitude Spectroscopic Survey on the Nancy Grace Roman Space Telescope. , keywords =. doi:10.3847/1538-4357/ac4973 , archivePrefix =. 2110.01829 , primaryClass =

    doi

  225. [233]

    arXiv e-prints , keywords =

    A strong He II 1640 emitter with extremely blue UV spectral slope at z=8.16 : presence of Pop III stars?. arXiv e-prints , keywords =. doi:10.48550/arXiv.2212.04476 , archivePrefix =. 2212.04476 , primaryClass =

    doi

  226. [234]

    , keywords =

    A SPectroscopic Survey of Biased Halos in the Reionization Era (ASPIRE): JWST Reveals a Filamentary Structure around a z = 6.61 Quasar. , keywords =. doi:10.3847/2041-8213/accd6f , archivePrefix =. 2304.09894 , primaryClass =

    doi

  227. [235]

    , keywords =

    A highly magnified star at redshift 6.2. , keywords =. doi:10.1038/s41586-022-04449-y , archivePrefix =. 2209.14866 , primaryClass =

    doi

  228. [236]

    , keywords =

    Measuring dynamical masses from gas kinematics in simulated high-redshift galaxies. , keywords =. doi:10.1093/mnras/staa2229 , archivePrefix =. 1908.05274 , primaryClass =

    1908 doi

  229. [237]

    , keywords =

    Exploring supermassive black hole physics and galaxy quenching across halo mass in FIRE cosmological zoom simulations. , keywords =. doi:10.1093/mnras/stad511 , archivePrefix =. 2203.06201 , primaryClass =

    doi

  230. [238]

    arXiv e-prints , keywords =

    Second public data release of the FIRE-2 cosmological zoom-in simulations of galaxy formation. arXiv e-prints , keywords =. doi:10.48550/arXiv.2508.06608 , archivePrefix =. 2508.06608 , primaryClass =

    doi

  231. [239]

    , keywords =

    Public Data Release of the FIRE-2 Cosmological Zoom-in Simulations of Galaxy Formation. , keywords =. doi:10.3847/1538-4365/acb99a , archivePrefix =. 2202.06969 , primaryClass =

    doi

  232. [240]

    , keywords =

    The Birth of a Galaxy: Primordial Metal Enrichment and Stellar Populations. , keywords =. doi:10.1088/0004-637X/745/1/50 , archivePrefix =. 1011.2632 , primaryClass =

    doi arXiv

  233. [241]

    , keywords =

    Super-Eddington accretion in tidal disruption events: the impactof realistic fallback rates on accretion rates. , keywords =. doi:10.1093/mnras/sty971 , archivePrefix =. 1804.06410 , primaryClass =

    doi arXiv

  234. [242]

    , keywords =

    A SPectroscopic Survey of Biased Halos in the Reionization Era (ASPIRE): A First Look at the Rest-frame Optical Spectra of z > 6.5 Quasars Using JWST. , keywords =. doi:10.3847/2041-8213/acc9c8 , archivePrefix =. 2304.09888 , primaryClass =

    doi

  235. [243]

    , keywords =

    The X-Ray and Radio Loud Fast Blue Optical Transient AT2020mrf: Implications for an Emerging Class of Engine-driven Massive Star Explosions. , keywords =. doi:10.3847/1538-4357/ac7a41 , archivePrefix =. 2112.00751 , primaryClass =

    doi

  236. [244]

    arXiv e-prints , keywords =

    A Massive Black Hole 0.8 kpc from the Host Nucleus Revealed by the Offset Tidal Disruption Event AT2024tvd. arXiv e-prints , keywords =. doi:10.48550/arXiv.2502.17661 , archivePrefix =. 2502.17661 , primaryClass =

    doi

  237. [245]

    , keywords =

    Tidal Disruption Event Demographics with the Zwicky Transient Facility: Volumetric Rates, Luminosity Function, and Implications for the Local Black Hole Mass Function. , keywords =. doi:10.3847/2041-8213/acf216 , archivePrefix =. 2303.06523 , primaryClass =

    doi

  238. [246]

    , keywords =

    The Era of Massive Population III Stars: Cosmological Implications and Self-Termination. , keywords =. doi:10.1086/382499 , archivePrefix =. astro-ph/0310443 , primaryClass =

    doi arXiv

  239. [247]

    , keywords =

    Formation of Primordial Stars in a CDM Universe. , keywords =. doi:10.1086/507978 , archivePrefix =. astro-ph/0606106 , primaryClass =

    doi arXiv

  240. [248]

    Science , keywords =

    Protostar Formation in the Early Universe. Science , keywords =. doi:10.1126/science.1160259 , archivePrefix =. 0807.4928 , primaryClass =

    doi arXiv

  241. [249]

    Science China Physics, Mechanics, and Astronomy , keywords =

    Science objectives of the Einstein Probe mission. Science China Physics, Mechanics, and Astronomy , keywords =. doi:10.1007/s11433-024-2600-3 , archivePrefix =. 2501.07362 , primaryClass =

    doi

  242. [250]

    , keywords =

    Eccentric tidal disruption event discs around supermassive black holes: dynamics and thermal emission. , keywords =. doi:10.1093/mnras/staa3127 , archivePrefix =. 2009.06636 , primaryClass =

    2009 doi

  243. [251]

    , keywords =

    Revisit the Rate of Tidal Disruption Events: The Role of the Partial Tidal Disruption Event. , keywords =. doi:10.3847/1538-4357/ac71ad , archivePrefix =. 2205.09945 , primaryClass =

    doi

Pith tools

Reviewed June 28, 2026 · model on record in the stance chip above.