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REVIEW 3 major objections 4 minor 114 references

What drives the growth of black holes: a decade of progress

T0 review · 3 major / 4 minor · reviewed 2026-08-06 · deepseek-v4-flash

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Pith's one-line read The central claim of this review is that the past decade established active galactic nuclei as transient, recurrent events within galaxy lifecycles, and that the field's progress was driven by five identifiable forces: new facilities…

desk verdict A thorough, authoritative update of AH12 that will serve as a standard reference; the driver-of-progress taxonomy is a transparently subjective add-on, not a demonstrated result, but the science review itself is solid. read the letter →

arxiv 2506.19166 v2 pith:SRRQDT44 submitted 2025-06-23 astro-ph.GA astro-ph.HE

D.M. Alexander (CEA-Durham) , R.C. Hickox (Dartmouth College) , J. Aird (Edinburgh) , F. Combes (Obs de Paris) , T. Costa (Newcastle) , M. Habouzit (Geneva) , C.M. Harrison (Newcastle) , R.I. Leng (Edinburgh)
show 3 more authors
L.K. Morabito (CEA-Durham) S.L. Uckelman (Durham) P. Vickers (Durham)
This is my paper
classification astro-ph.GAastro-ph.HE
keywords blackholesaccretionactivegalacticnucleiquasarsfeedbackgalaxiescitationnetworkanalysisscientificprogress
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 review argues that the last decade produced a qualitative shift in how astronomers think about supermassive black hole growth: an active galactic nucleus is not a freak event but a recurrent, relatively short phase in the ordinary life of galaxies. It reports a new consensus that the obscuring material around accreting black holes is a dynamic, clumpy disk plus a polar wind, rather than a static doughnut. The review also attempts to explain the progress itself, using the authors' own 2012 review as a decade-old snapshot and a citation network of 60,924 papers to map the field. It concludes that progress in this area has been driven mainly by new facilities, larger datasets, new analysis techniques, community engagement, and conceptual shifts.

What carries the argument

The carrying objects are (1) the AGN-as-event framework, quantified by the probability distribution of specific black hole accretion rates $p(\lambda_{\rm sBHAR})$ (the AGN luminosity per unit host stellar mass), which explains why instantaneous AGN luminosity correlates weakly with star formation while average accretion tracks galaxy growth; (2) the dynamic obscurer model, in which a clumpy molecular disk and a polar dusty wind replace the static torus; and (3) a citation-network analysis built from 60,924 papers and 1,378,057 links, clustered with the Leiden algorithm, which lets the authors identify sub-fields and locate their own review relative to the field. Driving all three is the 'know it when you see it' method: specialists compare the present field against the 2012 snapshot and attribute progress to the five categories of Table 1.

What would settle it

Give an independent panel of AGN specialists the same 2012-vs-now comparison and ask them to attribute each landmark advance to one of the five driver categories; if inter-rater agreement is no better than chance, the driver taxonomy is not a stable empirical claim. Alternatively, apply the same citation-network method starting from a different decade baseline and ask whether the five categories still reproduce; systematic disagreement would falsify the taxonomy.

Watch

Extended reading notes

Core claim

On the paper's own terms, the central claim is that the growth of supermassive black holes is best understood as a sequence of AGN 'events' inside galaxy lifecycles: galaxies repeatedly pass through short (<100 Myr) phases of strong accretion, separated by longer inactive periods, and the same galaxy can host many such events. A second claim is that the classic 'dusty torus' picture of AGN obscuration has been replaced by a more physical picture in which a clumpy, geometrically thin molecular disk supplies the fuel and a polar dusty cone, shaped by an AGN-driven wind, contributes much of the line-of-sight obscuration. A third claim is that the field's progress over the last decade is attributable to five identifiable drivers, and the citation network shows where this review and its predecessor sit within black-hole research.

Load-bearing premise

The driver analysis rests on the assumption that scientific progress can be reliably recognised by specialists and fairly attributed to the five categories of Table 1, using the authors' own 2012 review as a baseline; if that judgement is subjective, the claimed identification of progress drivers is anecdotal rather than measured.

Editorial extensions

If this is right

  • If AGN are recurrent short events, then single-epoch surveys systematically miss most SMBH growth, and interpreting AGN demographics requires duty cycles, not just triggering rates.
  • If the obscurer is a clumpy disk plus polar wind, then the simple Type 1/Type 2 unification dichotomy must be replaced by a distribution of covering factors tied to accretion state and wind activity.
  • If citation clusters track sub-fields, then the 13-cluster map of black-hole research can be used to forecast which areas are positioned to grow, such as time-domain AGN and high-redshift JWST samples.
  • If the five drivers are real, then deliberately investing in community events and cross-disciplinary workshops, alongside facilities and data, should measurably accelerate progress.

Reading between the lines

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

  • An extension the authors leave implicit: the AGN-as-event picture implies that the local SMBH mass function is built by repeated short bursts rather than continuous growth, so models that enforce a fixed Eddington ratio will misestimate the scatter in the $M_{\rm BH}$–$M_{\star}$ relation.
  • A testable extension is to compare the $p(\lambda_{\rm sBHAR})$ distribution measured from deep X-ray surveys against the stochastic accretion variability in modern magnetohydrodynamic simulations; the simulations' duty cycles are a direct prediction of the event picture.
  • The citation-network method could be turned from retrospective into prospective: track whether newly commissioned facilities and upcoming time-domain surveys produce the predicted acceleration in AGN discovery rates, and whether the community-engagement driver shows up as citation bursts at specific workshops.
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Editorial analysis

A structured set of objections, weighed in public.

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

Referee Report

3 major / 4 minor

Summary. The paper is a review of the past decade of research on the growth of supermassive black holes, framed as an update to Alexander & Hickox (2012, AH12). It surveys the main scientific topics (gas accretion from kpc to sub-pc scales, the AGN-host-galaxy connection, high-redshift quasars, and AGN feedback), and it adds a bibliometric component: a citation-network analysis of the broader black-hole literature intended to place the review in context and to identify what has driven scientific progress over the last decade. The authors explicitly state that, in the absence of a widely accepted quantitative measure, they adopt a "know it when you see it" approach to recognizing progress, and they postulate five categories of drivers (facilities, data, techniques, community, and conceptual shifts; Table 1). The scientific synthesis is the main body of the paper, while the driver analysis is presented as a secondary objective and is summarized in the abstract as a causal statement about what has "enabled" progress.

Significance. If read as an expert synthesis, the review is valuable and broadly consonant with current consensus: AGN as recurrent events in galaxy lifecycles, a clumpy disk plus polar-wind obscuring medium, and major advances from new facilities (ALMA, JWST, eROSITA, LOFAR, EHT) and large multiwavelength datasets. The paper is transparent about its qualitative method, and it makes a useful attempt to structure the field through the AH12 baseline and citation-network analysis. However, the paper's distinctive contribution, the identification of the drivers of progress, rests on the authors' own subjective classification and is not tested by the quantitative analysis. The claims about drivers should therefore be regarded as expert hypotheses rather than measured conclusions; in its current form the causal language in the abstract and Section 7 is stronger than the evidence presented. The strengths of the paper are its comprehensiveness, its explicit philosophical framing, and the reproducible citation-network construction; these make it a useful community resource even if the driver attribution is provisional.

major comments (3)
  1. [§2.3, Table 1, Abstract] The abstract states that the progress described in the paper "has been enabled by" new facilities, larger datasets, new techniques, and community engagement, but this causal attribution is not quantitatively supported. Section 2.3 explicitly adopts a "know it when you see it" approach and Table 1 labels the five categories as "postulated"; the citation-network analysis in Sections 2.1 and 7 identifies clusters of papers but does not map advances onto the five driver categories, nor does it test whether community engagement or conceptual shifts preceded the cited progress. The paper should either provide an explicit operational mapping between the citation-network statistics and the driver categories, or reframe the abstract and Section 7 conclusions as expert hypotheses rather than established causal claims.
  2. [§7.2 (and §2.3, category 4)] Community engagement is proposed as a driver of progress, with the citation network offered as a proxy, but citation networks measure bibliographic proximity and co-citation patterns, not community interactions such as workshops, discussions, or funding structures. The example of the 2017 Lorentz Center workshop leading to influential articles is asserted without evidence of a causal or even temporal link beyond co-occurrence. To make this category credible, the paper should state what specific observable would confirm or refute the claim that community engagement drove a particular advance, or explicitly acknowledge that this category is currently supported only by anecdote.
  3. [§1, §2, and §2.3] The use of the authors' own AH12 review as the baseline snapshot, combined with the 2022 workshop sessions being arranged to mirror the 2010 meeting, introduces a selection channel: the same group that wrote the baseline review, organized the workshop, and wrote the current review also decides which advances count as "progress" and which driver category applies. This is a reasonable design for an expert review, but the paper should discuss this self-referential structure explicitly and identify what external evidence could disconfirm the driver classification. Without such a discussion, the driver analysis risks being circular, as the reader cannot independently assess whether the baseline choice biases the selection of progress examples.
minor comments (4)
  1. [Figure 20] Figure 20 contains the visible placeholder text "MAKE THIS POINT IN TEXT", which is clearly an editing artifact and must be removed or implemented before publication.
  2. [Introduction] There are several typographical errors, including "occuring" in the first sentence and "Laser Inteferometer Space Antenna" in the introductory section; these should be corrected.
  3. [Equation (1)] Equation (1) uses cgs units for the stellar density but does not state the units explicitly; the text should note that ρ* is in g cm^-3.
  4. [Footnote 13] The "philosophical aside" in footnote 13 interrupts the scientific narrative; consider moving this reflection to the main text or to a more appropriate location, or deleting it if space is limited.

Circularity Check

0 steps flagged · score 2.0 of 10

No significant circularity: the review's scientific content is grounded in the independent literature, and the driver analysis is explicitly interpretive rather than a derivation.

full rationale

This is a review article, not a quantitative derivation, so the main circularity patterns (fitted parameters renamed as predictions, uniqueness theorems imported from the authors, ansatz smuggled via citation) do not apply. The central scientific claims about AGN as transient events and about the clumpy disk plus polar wind obscuring picture are supported by citations to a broad external literature. The only self-referential element is the use of the authors' own AH12 review as the baseline 'snapshot' and the reuse of the same workshop session structure. The paper explicitly acknowledges that progress is identified by a 'know it when you see it' approach in Section 2.3, and that the five driver categories in Table 1 are 'postulated' rather than measured. This makes the driver attribution an interpretive classification exercise, not a derivation that reduces to its inputs by construction. The citation-network analysis in Sections 2.1 and 7 locates AH12 in the literature and identifies clusters, but the paper does not claim that this analysis proves the causal driver attribution. A potential bias from using the authors' own prior review as the baseline is real, but it is disclosed and it does not force the scientific conclusions. No equation or fitted parameter is presented as an independent prediction. The figure-caption artifact 'MAKE THIS POINT IN TEXT' is an editorial leftover, not circularity. Overall, the paper is self-aware about its subjective progress taxonomy, and its substantive claims about black-hole growth are independently sourced, so the circularity score is low.

Assumptions & free parameters 0 free parameters · 4 assumptions · 0 invented entities

The central scientific content is a synthesis of published results; the load-bearing assumptions are the standard AGN paradigm plus the paper's explicit qualitative framework for measuring progress.

assumptions (4)
  • domain assumption AGN luminosity traces SMBH accretion power with radiative efficiency near 0.1, via L = eta dM/dt c^2.
    Used throughout Sections 3 to 5 to convert observables into accretion rates and growth estimates; standard in the field.
  • ad hoc to paper The 'know it when you see it' method reliably identifies scientific progress.
    Explicitly adopted in Section 2.3 as the practical measurement framework for the driver analysis; no independent validation is provided.
  • domain assumption Clusters from Leiden modularity maximization on citation links correspond to scientific subfields.
    Invoked in Section 2.1 to define clusters and locate AH12; depends on the citation graph being representative of research topics.
  • domain assumption The Web of Science keyword-selected set of 60,924 papers is representative of black-hole research.
    Section 2.1 and Appendix B; selection depends on indexing and keyword terms, and no sensitivity analysis is provided.

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Cite this review

Pith. "Pith review of What drives the growth of black holes: a decade of progress." pith.science (2026). https://pith.science/paper/SRRQDT44

@misc{pith2026250619166,
  author       = {Pith},
  title        = {Pith review of: What drives the growth of black holes: a decade of progress},
  year         = {2026},
  howpublished = {\url{https://pith.science/paper/SRRQDT44}},
  note         = {Machine review of arXiv:2506.19166}
}
read the original abstract

The last decade has witnessed significant progress in our understanding of the growth of super-massive black holes (SMBHs). It is now clear that an Active Galactic Nucleus (AGN: the observed manifestation of a growing SMBH) is an "event" within the broader lifecycle of a galaxy, which can significantly influence the shape and evolution of the galaxy itself. Our view of the obscuring medium that affects the observed properties of an AGN has also undergone a revolution, and we now have a more physical understanding of the connection between the fuelling of (and feedback from) the SMBH and the broader host-galaxy and larger-scale environment. We have a greater understanding of the physics of SMBH accretion, can identify AGNs out to z = 8-10 witnessing the very earliest phases of SMBH growth, and have a more complete census of AGN activity than ever before. This great progress has been enabled by new innovative facilities, an ever-increasing quantity of multi-wavelength data, the exploitation and development of new techniques, and greater community-wide engagement. In this article we review our understanding of AGNs and the growth of SMBHs, providing an update of the earlier Alexander and Hickox (2012) review. Using citation-network analyses we also show where this review fits within the broader black-hole research literature and, adopting the previous article as a snapshot of the field over a decade ago, identify the drivers that have enabled the greatest scientific progress.

Figures

Figures reproduced from arXiv: 2506.19166 by the authors.

Figure 1
Figure 1. (a) Simple schematic representation of an AGN within the broader host-galaxy and halo environment over (logarithmic) milli-parsec to mega-parcsec [PITH_FULL_IMAGE:figures/full_fig_p002_1.png] view at source ↗
Figure 2
Figure 2. Broad-band SED of an unobscured AGN (black curve) across the [PITH_FULL_IMAGE:figures/full_fig_p003_2.png] view at source ↗
Figure 3
Figure 3. Citation network diagram (CND) for (a) papers related to black [PITH_FULL_IMAGE:figures/full_fig_p004_3.png] view at source ↗
Figures from the paper (35 more)
Figure 5
Figure 5. Figure 5: Left: Main stellar orbits in the bar rotating frame. The bar is along the [PITH_FULL_IMAGE:figures/full_fig_p007_5.png]
Figure 4
Figure 4. Figure 4: Rotational velocity and angular momentum versus radius around a [PITH_FULL_IMAGE:figures/full_fig_p007_4.png]
Figure 6
Figure 6. Figure 6: Left: in the absence of a central SMBH, a leading spiral is expected [PITH_FULL_IMAGE:figures/full_fig_p008_6.png]
Figure 7
Figure 7. Figure 7: Top: Schematic representation of the main morphological features [PITH_FULL_IMAGE:figures/full_fig_p009_7.png]
Figure 8
Figure 8. Figure 8: Left: Molecular gas distribution in NGC 613: inside the ILR ring, [PITH_FULL_IMAGE:figures/full_fig_p010_8.png]
Figure 9
Figure 9. Figure 9: Zoom-in on the nuclear spiral observed with ALMA inside the ILR [PITH_FULL_IMAGE:figures/full_fig_p011_9.png]
Figure 10
Figure 10. Figure 10: Schematic view of the circum-nuclear environment of the SMBH, [PITH_FULL_IMAGE:figures/full_fig_p011_10.png]
Figure 11
Figure 11. Figure 11: The hard X-ray spectrum is characteristic of a low￾luminosity regime. This is shown in Kang et al. (2024) and Hagen et al. (2024), with observational evidence of changes in accretion disk SED with Eddington ratio, in particular see [PITH_FULL_IMAGE:figures/full_fig_p…
Figure 12
Figure 12. Figure 12: X-ray spectra of ESO 323–G77 showing significant time-variable [PITH_FULL_IMAGE:figures/full_fig_p013_12.png]
Figure 13
Figure 13. Figure 13: An outburst in the changing-look AGN Mrk 1018 shown at three [PITH_FULL_IMAGE:figures/full_fig_p014_13.png]
Figure 14
Figure 14. Figure 14: Hydrodynamical simulations of gas accretion onto an SMBH, illustrated at 3 epochs separated by just 30 years. The strong variability illustrates the [PITH_FULL_IMAGE:figures/full_fig_p016_14.png]
Figure 15
Figure 15. Figure 15: Left panel: SMBH mass as a function of the total stellar mass of their host galaxies in the local Universe, demonstrating the overall connection between the growth of galaxies and their central SMBHs. The sources are categorized into several groups: SMBHs with dynamic…
Figure 16
Figure 16. Figure 16: Coverage of the rest-frame 2-10 keV luminosity–redshift plane obtained through X-ray selection of AGN with di [PITH_FULL_IMAGE:figures/full_fig_p021_16.png]
Figure 17
Figure 17. Figure 17: Measurements of the space density of X-ray selected AGN of di [PITH_FULL_IMAGE:figures/full_fig_p022_17.png]
Figure 18
Figure 18. Figure 18: Diagram illustrating the picture established over the last decade that explains the relation between AGN and galaxy SFRs over the bulk of cosmic time [PITH_FULL_IMAGE:figures/full_fig_p026_18.png]
Figure 19
Figure 19. Figure 19: Schematic showing how the incidence of AGN, quantified by the probability distribution of specific SMBH accretion rates, [PITH_FULL_IMAGE:figures/full_fig_p028_19.png]
Figure 20
Figure 20. Figure 20: Illustration of how the AGN luminosity function (space density of [PITH_FULL_IMAGE:figures/full_fig_p029_20.png]
Figure 22
Figure 22. Figure 22: Illustration of different phases of a central SMBH (cf [PITH_FULL_IMAGE:figures/full_fig_p031_22.png]
Figure 23
Figure 23. Figure 23: Top: Cumulative fraction of radio-selected AGN with specific Black Hole Kinetic Power (λsBHKP ∝ Pkin/M∗) exceeds a given value, providing a tracer of the relative power carried by the jet. We have divided the radio￾selected AGN into those with high radiative power (λs…
Figure 24
Figure 24. Figure 24: Illustration of the determination of the HOD from spatial clustering measurements. (a) Schematic of an autocorrelation measurement for radio AGN; the [PITH_FULL_IMAGE:figures/full_fig_p035_24.png]
Figure 25
Figure 25. Figure 25: Bolometric luminosity (top) and black-hole mass (bottom) versus spectroscopic redshift for quasars from SDSS DR14 (grey dots) and dedicated [PITH_FULL_IMAGE:figures/full_fig_p039_25.png]
Figure 26
Figure 26. Figure 26: (left): rest-frame UV spectral composite of [PITH_FULL_IMAGE:figures/full_fig_p041_26.png]
Figure 27
Figure 27. Figure 27: Eddington-ratio–black-hole mass plane for quasars at [PITH_FULL_IMAGE:figures/full_fig_p042_27.png]
Figure 28
Figure 28. Figure 28: Quasar evolutionary model schematic showing the gas-inflow trigger options (merger or secular), the key quasar phases with di [PITH_FULL_IMAGE:figures/full_fig_p045_28.png]
Figure 29
Figure 29. Figure 29: Record-breaking quasar redshifts as a function of their year of discovery, starting from the first “distant” quasar at [PITH_FULL_IMAGE:figures/full_fig_p047_29.png]
Figure 30
Figure 30. Figure 30: AGN bolometric luminosity function at z ∼ 5. The shaded green region shows the combination of the luminosity functions, including Poisson uncertainties, from the Horizon-AGN, Illustris (Tng 50, Tng 100, Tng 300), Eagle, Simba, and Astrid large-scale cosmological simul…
Figure 31
Figure 31. Figure 31: Black-hole mass versus redshift for several [PITH_FULL_IMAGE:figures/full_fig_p052_31.png]
Figure 32
Figure 32. Figure 32: Despite the use of different hydrodynamic solvers, different models for star formation, stellar feedback, interstellar medium, virtually all cosmological models of galaxy evolution must invoke feedback from AGN in order to produce a realistic population of massive gal…
Figure 33
Figure 33. Figure 33: Energy-driven outflow powered by a spherical wind with velocity [PITH_FULL_IMAGE:figures/full_fig_p057_33.png]
Figure 34
Figure 34. Figure 34: In an energy-driven outflow, ambient gas is driven out via adiabatic expansion of a hot, energy-conserving bubble. These outflows impact galaxies [PITH_FULL_IMAGE:figures/full_fig_p058_34.png]
Figure 35
Figure 35. Figure 35: Simulation of relativistic low-power jet interacting with inhomoge [PITH_FULL_IMAGE:figures/full_fig_p059_35.png]
Figure 36
Figure 36. Figure 36: In cosmological simulations, massive galaxies quench when AGN-driven outflows clear out the CGM. Shown here is the fraction of total halo mass in the [PITH_FULL_IMAGE:figures/full_fig_p060_36.png]
Figure 37
Figure 37. Figure 37: Top: Outflow velocity as a function of normalized radius (dust sub [PITH_FULL_IMAGE:figures/full_fig_p062_37.png]
Figure 38
Figure 38. Figure 38: (a) Annual number of publications per year for the 13 research clusters identified in §2.1 over 2003–2023 using the same colour coding as that adopted [PITH_FULL_IMAGE:figures/full_fig_p064_38.png]
Figure 39
Figure 39. Figure 39: The temporal evolution of the citation network diagram presented [PITH_FULL_IMAGE:figures/full_fig_p065_39.png]

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Works this paper leans on

114 extracted references · 29 canonical work pages

  1. [1]

    Choi, E., Ostriker, J.P., Naab, T., Johansson, P.H., 2012

    doi: 10.3847/1538-4357/aad184, arXiv:1805.01467. Choi, E., Ostriker, J.P., Naab, T., Johansson, P.H., 2012. Radiative and Momentum-based Mechanical Active Galactic Nucleus Feedback in a Three-dimensional Galaxy Evolution Code. ApJ 754, 125. doi: 10.1088/ 0004-637X/754/2/125, arXiv:1205.2082. Choi, E., Ostriker, J.P., Naab, T., Oser, L., Moster, B.P., 2015...

    arXiv 2012

  2. [2]

    doi: 10.3847/1538-4365/ac6c05, arXiv:2207.12432. Koss, M.J., Treister, E., Kakkad, D., Casey-Clyde, J.A., Kawamuro, T., Williams, J., Foord, A., Trakhtenbrot, B., Bauer, F.E., Privon, G.C., Ricci, C., Mushotzky, R., Barcos-Munoz, L., Blecha, L., Connor, T., Harrison, F., Liu, T., Magno, M., Mingarelli, C.M.F., Muller-Sanchez, F., Oh, K., Shimizu, T.T., Sm...

    arXiv

  3. [3]

    doi: 10.1111/j.1365-2966.2011.19675.x, arXiv:1106.4284

    MNRAS 419, 95–115. doi: 10.1111/j.1365-2966.2011.19675.x, arXiv:1106.4284. M¨uller, A., 2004. Black hole astrophysics: magnetohydrodynamics on the Kerr geometry. Ph.D. thesis. University of Heidelberg, Germany. M¨uller-S´anchez, F., Comerford, J.M., Nevin, R., Barrows, R.S., Cooper, M.C., Greene, J.E., 2015. The Origin of Double-peaked Narrow Lines in Ac-...

    arXiv 2011

  4. [7]

    arXiv e-prints , arXiv:2306.07320doi: 10.48550/arXiv.2306.07320, arXiv:2306.07320. Labbe, I., Greene, J.E., Matthee, J., Treiber, H., Kokorev, V ., Miller, T.B., Kra- marenko, I., Setton, D.J., Ma, Y ., Goulding, A.D., Bezanson, R., Naidu, R.P., Williams, C.C., Atek, H., Brammer, G., Cutler, S.E., Chemerynska, I., Cloonan, A.P., Dayal, P., de Graaff, A., ...

    arXiv doi:10.48550/arxiv.2306.07320

  5. [9]

    Primordial environment of supermassive black holes. II. Deep Y- and J-band images around the z 6.3 quasar SDSS J1030+0524. A&A 606, A23. doi:10.1051/0004-6361/201730683, arXiv:1706.02317. Banerji, M., Alaghband-Zadeh, S., Hewett, P.C., McMahon, R.G., 2015. Heav- ily reddened type 1 quasars at z > 2 - I. Evidence for significant obscured black hole growth ...

    arXiv

  6. [17]

    doi: 10.3847/1538-4365/ab99c5, arXiv:1910.10395. Ramos Almeida, C., Levenson, N.A., Alonso-Herrero, A., Asensio Ramos, A., Rodr´ıguez Espinosa, J.M., P ´erez Garc´ıa, A.M., Packham, C., Mason, R., Radomski, J.T., D´ıaz-Santos, T., 2011. Testing the Unification Model for Active Galactic Nuclei in the Infrared: Are the Obscuring Tori of Type 1 and 2 Seyfert...

    arXiv 1910

  7. [19]

    ApJ 963, 53

    An Excess of Active Galactic Nuclei Triggered by Galaxy Merg- ers in MaNGA Galaxies of Stellar Mass ∼1011 M ⊙. ApJ 963, 53. doi:10.3847/1538-4357/ad1a15, arXiv:2404.14490. Comerford, J.M., Schluns, K., Greene, J.E., Cool, R.J., 2013. Dual Supermas- sive Black Hole Candidates in the AGN and Galaxy Evolution Survey. ApJ 777, 64. doi: 10.1088/0004-637X/777/1...

    arXiv

  8. [21]

    Ni, Q., Brandt, W.N., Luo, B., Garmire, G.P., Hall, P.B., Plotkin, R.M., Shemmer, O., Timlin, J.D., Vito, F., Wu, J., Yi, W., 2022a

    doi: 10.3847/1538-4365/ac0dc6, arXiv:2106.10572. Ni, Q., Brandt, W.N., Luo, B., Garmire, G.P., Hall, P.B., Plotkin, R.M., Shemmer, O., Timlin, J.D., Vito, F., Wu, J., Yi, W., 2022a. Sensitive Chandra coverage of a representative sample of weak-line quasars: re- vealing the full range of X-ray properties. MNRAS 511, 5251–5264. doi:10.1093/mnras/stac394, ar...

    arXiv

Show all 114 references
  1. [22]

    arXiv e-prints , arXiv:2401.11242doi:10.48550/arXiv.2401

    UNCOVERing the contribution of black holes to reionization in the JWST era. arXiv e-prints , arXiv:2401.11242doi:10.48550/arXiv.2401. 11242, arXiv:2401.11242. De Cicco, D., Paolillo, M., Covone, G., Falocco, S., Longo, G., Grado, A., Limatola, L., Botticella, M.T., Pignata, G....

    doi arXiv

  2. [26]

    MNRAS 453, 2779–2798

    Clustering of intermediate redshift quasars using the final SDSS III- BOSS sample. MNRAS 453, 2779–2798. doi: 10.1093/mnras/stv1763, arXiv:1507.08380. Ehlert, S., Allen, S.W., Brandt, W.N., Canning, R.E.A., Luo, B., Mantz, A., Morris, R.G., von der Linden, A., Xue, Y .Q., 2015...

    arXiv

  3. [27]

    doi: 10.1088/0004-637X/804/1/27, arXiv:1408.1092. Assef, R.J., Kochanek, C.S., Ashby, M.L.N., Brodwin, M., Brown, M.J.I., Cool, R., Forman, W., Gonzalez, A.H., Hickox, R.C., Jannuzi, B.T., Jones, C., Le Floc’h, E., Moustakas, J., Murray, S.S., Stern, D., 2011. The Mid-IR- and ...

    arXiv

  4. [28]

    II – Post-merger quench- ing peaks within 500 Myr of coalescence

    Galaxy evolution in the post-merger regime. II – Post-merger quench- ing peaks within 500 Myr of coalescence. The Open Journal of Astrophysics 7, 121. doi: 10.33232/001c.127779, arXiv:2410.06357. Ellison, S.L., Mendel, J.T., Patton, D.R., Scudder, J.M., 2013. Galaxy pairs in t...

    arXiv

  5. [29]

    ApJ 848, 78

    Mapping the Lyα Emission around a z∼ 6.6 QSO with MUSE: Ex- tended Emission and a Companion at a Close Separation. ApJ 848, 78. doi:10.3847/1538-4357/aa8df4, arXiv:1709.06096. Fassbender, R., ˇSuhada, R., Nastasi, A., 2012. AGN Triggering in the In- fall Regions of Distant X-R...

    2012 arXiv

  6. [30]

    A&A 601, A143

    AGN wind scaling relations and the co-evolution of black holes and galaxies. A&A 601, A143. doi: 10.1051/0004-6361/201629478, arXiv:1702.04507. Fischer, J., Sturm, E., Gonz ´alez-Alfonso, E., Graci ´a-Carpio, J., Hailey- Dunsheath, S., Poglitsch, A., Contursi, A., Lutz, D., Ge...

    arXiv

  7. [32]

    Jiang, Y .F., Stone, J.M., Davis, S.W., 2019

    doi: 10.3847/1538-4365/abd1dc, arXiv:2012.06806. Jiang, Y .F., Stone, J.M., Davis, S.W., 2019. Super-Eddington Accretion Disks around Supermassive Black Holes. ApJ 880, 67. doi: 10.3847/ 1538-4357/ab29ff, arXiv:1709.02845. Jin, C., Ward, M., Done, C., Gelbord, J., 2012. A comb...

    2012 arXiv

  8. [37]

    ApJ 966, 204

    ReveaLLAGN 0: First Look at JWST MIRI Data of Sombrero and NGC 1052. ApJ 966, 204. doi: 10.3847/1538-4357/ad3065, arXiv:2307.01252. Gordon, Y .A., Pimbblet, K.A., Owers, M.S., Bland-Hawthorn, J., Brough, S., Brown, M.J.I., Cluver, M.E., Croom, S.M., Holwerda, B.W., Loveday, J....

    arXiv

  9. [42]

    MNRAS 514, 4912–4931

    The black hole population in low-mass galaxies in large-scale cos- mological simulations. MNRAS 514, 4912–4931. doi: 10.1093/mnras/ 93 stac1659, arXiv:2201.09888. Hainline, K.N., Maiolino, R., Juodzbalis, I., Scholtz, J., Ubler, H., D’Eugenio, F., Helton, J.M., Sun, Y ., Sun, ...

    arXiv

  10. [45]

    A&A 686, A43

    The LOFAR - eFEDS survey: The incidence of radio and X-ray AGN and the disk-jet connection. A&A 686, A43. doi: 10.1051/0004-6361/ 202349069, arXiv:2402.16943. Ikeda, S., Awaki, H., Terashima, Y ., 2009. Study on X-Ray Spectra of Obscured Active Galactic Nuclei Based on Monte C...

    2009 arXiv

  11. [47]

    Almaini, O., Wild, V ., Maltby, D., Taylor, E., Rowlands, K., de Lisle, T., Alat- alo, K., Harrold, J., Hewitt, G., Patil, P., Skarbinski, M., 2025

    doi: 10.1088/0004-637X/758/1/47, arXiv:1209.2420. Almaini, O., Wild, V ., Maltby, D., Taylor, E., Rowlands, K., de Lisle, T., Alat- alo, K., Harrold, J., Hewitt, G., Patil, P., Skarbinski, M., 2025. No evidence for excess AGN activity in recently quenched massive galaxies at c...

    2025 arXiv

  12. [48]

    MNRAS 530, 2688–2730

    The wide-field, multiplexed, spectroscopic facility WEA VE: Survey design, overview, and simulated implementation. MNRAS 530, 2688–2730. doi:10.1093/mnras/stad557, arXiv:2212.03981. Jogee, S., 2006. The Fueling and Evolution of AGN: Internal and External Triggers, in: Alloin, ...

    2006 arXiv

  13. [49]

    ApJ 925, 203

    The Black Hole-Galaxy Connection: Interplay between Feedback, Obscuration, and Host Galaxy Substructure. ApJ 925, 203. doi: 10.3847/ 1538-4357/ac425f, arXiv:2112.08380. Juodˇzbalis, I., Ji, X., Maiolino, R., D’Eugenio, F., Scholtz, J., Risaliti, G., Fabian, A.C., Mazzolari, G....

  14. [52]

    ApJ 965, L21

    A Candidate Supermassive Black Hole in a Gravitationally Lensed Galaxy at Z ≈ 10. ApJ 965, L21. doi: 10.3847/2041-8213/ad391f, arXiv:2403.14745. Krishnan, C., Almaini, O., Hatch, N.A., Wilkinson, A., Maltby, D.T., Con- selice, C.J., Kocevski, D., Suh, H., Wild, V ., 2020. The ...

    arXiv

  15. [53]

    More massive black holes reside in more massive dark matter halos

    The spatial clustering of ROSAT All-Sky Survey Active Galactic Nuclei IV . More massive black holes reside in more massive dark matter halos. ApJ in press (arXiv:1509.01261) arXiv:1509.01261. Kubota, A., Done, C., 2018. A physical model of the broad-band con- tinuum of AGN and...

    2018 arXiv

  16. [54]

    UNCOVER: Candidate Red Active Galactic Nuclei at 3 < z <

  17. [56]

    Nature 616, 266–269

    A population of red candidate massive galaxies 600 Myr after the Big Bang. Nature 616, 266–269. doi: 10.1038/s41586-023-05786-2 , arXiv:2207.12446. Lacy, M., Ridgway, S.E., Sajina, A., Petric, A.O., Gates, E.L., Urrutia, T., Storrie-Lombardi, L.J., 2015. The Spitzer Mid-infrar...

    arXiv

  18. [58]

    Changing Look

    Accretion properties of X-ray AGN: evidence for radiation-regulated obscuration with redshift-dependent host galaxy contribution. MNRAS 532, 3459–3479. doi: 10.1093/mnras/stae1649, arXiv:2403.07109. LaMassa, S.M., Cales, S., Moran, E.C., Myers, A.D., Richards, G.T., Era- cleou...

    arXiv

  19. [59]

    arXiv e-prints , arXiv:2303.08918doi: 10.48550/arXiv.2303

    A CEERS Discovery of an Accreting Supermassive Black Hole 570 Myr after the Big Bang: Identifying a Progenitor of Massive z > 6 Quasars. arXiv e-prints , arXiv:2303.08918doi: 10.48550/arXiv.2303. 08918, arXiv:2303.08918. Lasota, J.P., 2016. Black Hole Accretion Discs, in: Bamb...

    doi arXiv

  20. [61]

    ApJ 691, 687–695

    The Chandra Deep Protocluster Survey: Evidence for an Enhance- ment of AGN Activity in the SSA22 Protocluster at z = 3.09. ApJ 691, 687–695. doi: 10.1088/0004-637X/691/1/687, arXiv:0809.5058. Lehmer, B.D., Lucy, A.B., Alexander, D.M., Best, P.N., Geach, J.E., Harri- son, C.M.,...

    arXiv

  21. [62]

    The z = 0.54 LoBAL Quasar SDSS J085053.12+445122.5. I. Spectral Synthesis Analysis Reveals a Massive Outflow. ApJ 866, 7. doi: 10.3847/ 1538-4357/aadee6, arXiv:1808.02441. Leipski, C., Meisenheimer, K., Walter, F., Klaas, U., Dannerbauer, H., De Rosa, G., Fan, X., Haas, M., Kr...

    arXiv

  22. [63]

    ApJ 966, 229

    Active Galactic Nuclei Selection and Demographics: A New Age with JWST /MIRI. ApJ 966, 229. doi: 10.3847/1538-4357/ad3643, arXiv:2310.12330. Lyu, J., Rieke, G., 2022. Infrared Spectral Energy Distribution and Variability of Active Galactic Nuclei: Clues to the Structure of Cir...

    2022 arXiv

  23. [64]

    Astronomy and Computing 48, 100835

    Learning from the present for the future: The J ¨ulich LOFAR Long- term Archive. Astronomy and Computing 48, 100835. doi: 10.1016/j. ascom.2024.100835, arXiv:2406.03547. Marchesi, S., Lanzuisi, G., Civano, F., Iwasawa, K., Suh, H., Comastri, A., Zamorani, G., Allevato, V ., Gr...

    2024

  24. [65]

    Frontiers in Astronomy and Space Sciences 5, 6

    A main sequence for quasars. Frontiers in Astronomy and Space Sciences 5, 6. doi: 10.3389/fspas.2018.00006, arXiv:1802.05575. Masini, A., Civano, F., Comastri, A., Fornasini, F., Ballantyne, D.R., Lans- bury, G.B., Treister, E., Alexander, D.M., Boorman, P.G., Brandt, W.N., Fa...

    2018

  25. [67]

    MNRAS 478, 2576–2591

    Intermediate-mass black holes in dwarf galaxies out to redshift∼2.4 in the Chandra COSMOS-Legacy Survey. MNRAS 478, 2576–2591. doi: 10. 1093/mnras/sty1163, arXiv:1802.01567. Mezcua, M., Dom ´ınguez S´anchez, H., 2020. Hidden AGNs in Dwarf Galax- ies Revealed by MaNGA: Light Ec...

    2020 arXiv

  26. [74]

    Overzier, R.A., 2016

    doi: 10.3847/1538-4357/aab35b, arXiv:1802.08912. Overzier, R.A., 2016. The realm of the galaxy protoclusters. A re- view. A&A Rev. 24, 14. doi: 10.1007/s00159-016-0100-3 , arXiv:1610.05201. Pacifici, C., Iyer, K.G., Mobasher, B., da Cunha, E., Acquaviva, V ., Burgarella, D., C...

    2016 arXiv

  27. [75]

    ApJ 944,

    The Art of Measuring Physical Parameters in Galaxies: A Critical Assessment of Spectral Energy Distribution Fitting Techniques. ApJ 944,

  28. [76]

    Pacucci, F., Narayan, R., 2024

    doi: 10.3847/1538-4357/acacff, arXiv:2212.01915. Pacucci, F., Narayan, R., 2024. Mildly Super-Eddington Accretion onto Slowly Spinning Black Holes Explains the X-Ray Weakness of the Little Red Dots. ApJ 976, 96. doi: 10.3847/1538-4357/ad84f7, arXiv:2407.15915. Padovani, P., Al...

    2024 arXiv

  29. [78]

    Little Red Dots

    Identifying galaxy mergers in observations and simulations with deep learning. A&A 626, A49. doi: 10.1051/0004-6361/201935355, arXiv:1902.10626. Peca, A., Cappelluti, N., LaMassa, S., Urry, C.M., Moscetti, M., Marchesi, S., Sanders, D., Auge, C., Ghosh, A., Ananna, T.T., Torre...

    1902 arXiv

  30. [79]

    Nature 588, 227–231

    Detection of large-scale X-ray bubbles in the Milky Way halo. Nature 588, 227–231. doi:10.1038/s41586-020-2979-0 , arXiv:2012.05840. Proga, D., 2005. How Much X-Ray and UV Radiation Processes Are Coupled in Accretion Disks? The Active Galactic Nucleus Case. ApJ 630, L9–L12. do...

    2012 arXiv

  31. [82]

    doi: 10.1088/0004-637X/736/2/82, arXiv:1105.2368. Alonso-Tetilla, A.V ., Shankar, F., Fontanot, F., Menci, N., Valentini, M., Buch- ner, J., Laloux, B., Lapi, A., Puglisi, A., Alexander, D.M., Allevato, V ., An- donie, C., Bonoli, S., Hirschmann, M., L ´opez, I.E., Raimundo, S...

    arXiv

  32. [83]

    (Eds.), UV , X-Ray, and Gamma-Ray Space Instru- mentation for Astronomy XXIII, p

    Overview of the advanced x-ray imaging satellite (AXIS), in: Sieg- mund, O.H., Hoadley, K. (Eds.), UV , X-Ray, and Gamma-Ray Space Instru- mentation for Astronomy XXIII, p. 126781E. doi: 10.1117/12.2677468, arXiv:2311.00780. Ricarte, A., Narayan, R., Curd, B., 2023. Recipes fo...

    arXiv

  33. [84]

    Ricci, C., Bauer, F.E., Treister, E., Schawinski, K., Privon, G.C., Blecha, L., Arevalo, P., Armus, L., Harrison, F., Ho, L.C., Iwasawa, K., Sanders, D.B., Stern, D., 2017a

    doi: 10.3847/1538-4357/ac8e67, arXiv:2209.00014. Ricci, C., Bauer, F.E., Treister, E., Schawinski, K., Privon, G.C., Blecha, L., Arevalo, P., Armus, L., Harrison, F., Ho, L.C., Iwasawa, K., Sanders, D.B., Stern, D., 2017a. Growing supermassive black holes in the late stages of...

    arXiv

  34. [85]

    MNRAS 483, 2712–2720

    The abundances and properties of Dual AGN and their host galaxies in the EAGLE simulations. MNRAS 483, 2712–2720. doi: 10.1093/mnras/ sty3251, arXiv:1805.01479. Rose, M., Tadhunter, C., Ramos Almeida, C., Rodr ´ıguez Zaur´ın, J., Santoro, F., Spence, R., 2018. Quantifying the ...

    arXiv

  35. [86]

    The most massive galaxies are always switched on

    The LoTSS view of radio AGN in the local Universe. The most massive galaxies are always switched on. A&A 622, A17. doi: 10.1051/ 0004-6361/201833883, arXiv:1811.05528. Sadowski, A., 2016. Thin accretion discs are stabilized by a strong mag- netic field. MNRAS 459, 4397–4407. d...

    2016 arXiv

  36. [88]

    Are we surprised to find SMBHs with JWST at z > 9? arXiv e-prints , arXiv:2305.12504doi: 10.48550/arXiv.2305.12504, arXiv:2305.12504. Scholtz, J., Alexander, D.M., Harrison, C.M., Rosario, D.J., McAlpine, S., Mullaney, J.R., Stanley, F., Simpson, J., Theuns, T., Bower, R.G., H...

    doi arXiv

  37. [89]

    arXiv e-prints , arXiv:2311.18731doi: 10.48550/arXiv.2311

    JADES: A large population of obscured, narrow line AGN at high redshift. arXiv e-prints , arXiv:2311.18731doi: 10.48550/arXiv.2311. 18731, arXiv:2311.18731. Schramm, M., Silverman, J.D., 2013. The black hole-bulge mass relation of active galactic nuclei in the extended chandra...

    2013 doi arXiv

  38. [90]

    little red dots

    doi: 10.1088/0004-637X/746/1/90, arXiv:1107.4368. Aird, J., Coil, A.L., Moustakas, J., Diamond-Stanic, A.M., Blanton, M.R., Cool, R.J., Eisenstein, D.J., Wong, K.C., Zhu, G., 2013. PRIMUS: An Observationally Motivated Model to Connect the Evolution of the Ac- tive Galactic Nuc...

    2013 arXiv

  39. [91]

    A&A 575, A74

    The Herschel view of the dominant mode of galaxy growth from z= 4 to the present day. A&A 575, A74. doi:10.1051/0004-6361/201425017, arXiv:1409.5433. Schulze, A., Silverman, J.D., Daddi, E., Rujopakarn, W., Liu, D., Schramm, M., Mainieri, V ., Imanishi, M., Hirschmann, M., Jah...

    arXiv

  40. [92]

    V-Shaped

    The origin of the α-enhancement of massive galaxies. MNRAS 461, L102–L106. doi: 10.1093/mnrasl/slw111, arXiv:1603.05653. Sesana, A., Haiman, Z., Kocsis, B., Kelley, L.Z., 2018. Testing the Bi- nary Hypothesis: Pulsar Timing Constraints on Supermassive Black Hole Binary Candida...

    2018 arXiv

  41. [93]

    MNRAS 429, 2199–2211

    Galaxy Zoo: bulgeless galaxies with growing black holes. MNRAS 429, 2199–2211. doi: 10.1093/mnras/sts491, arXiv:1207.4190. Simpson, C., Mortlock, D., Warren, S., Cantalupo, S., Hewett, P., McLure, R., McMahon, R., Venemans, B., 2014. No excess of bright galaxies around the red...

    arXiv

  42. [96]

    Lehmer, B.D., Alexander, D.M., Geach, J.E., Smail, I., Basu-Zych, A., Bauer, F.E., Chapman, S.C., Matsuda, Y ., Scharf, C.A., V olonteri, M., Yamada, T.,

    doi: 10.3847/1538-4357/abee80, arXiv:2103.07482. Lehmer, B.D., Alexander, D.M., Geach, J.E., Smail, I., Basu-Zych, A., Bauer, F.E., Chapman, S.C., Matsuda, Y ., Scharf, C.A., V olonteri, M., Yamada, T.,

    arXiv

  43. [97]

    arXiv e-prints , arXiv:2112.15275doi: 10.48550/arXiv.2112.15275, arXiv:2112.15275

    Learned Coarse Models for E fficient Turbulence Simulation. arXiv e-prints , arXiv:2112.15275doi: 10.48550/arXiv.2112.15275, arXiv:2112.15275. Stanley, F., Alexander, D.M., Harrison, C.M., Rosario, D.J., Wang, L., Aird, J.A., Bourne, N., Dunne, L., Dye, S., Eales, S., Knudsen,...

    doi arXiv

  44. [99]

    arXiv e-prints , arXiv:2409.06772doi:10

    Broad-Line AGN at 3.5< z< 6: The Black Hole Mass Function and a Connection with Little Red Dots. arXiv e-prints , arXiv:2409.06772doi:10. 48550/arXiv.2409.06772, arXiv:2409.06772. Taylor, A.J., Kokorev, V ., Kocevski, D.D., Akins, H.B., Cullen, F., Dickin- son, M., Finkelstein...

    doi arXiv

  45. [100]

    ApJ 836, 8

    ALMA Observations Show Major Mergers Among the Host Galax- ies of Fast-growing, High-redshift Supermassive Black Holes. ApJ 836, 8. doi:10.3847/1538-4357/836/1/8, arXiv:1612.00010. Trefoloni, B., Ji, X., Maiolino, R., D’Eugenio, F., ¨Ubler, H., Scholtz, J., Mar- coni, A., Marc...

    arXiv

  46. [102]

    doi: 10.1088/0004-637X/802/2/102, arXiv:1501.04118. Lacy, M., Storrie-Lombardi, L.J., Sajina, A., Appleton, P.N., Armus, L., 99 Chapman, S.C., Choi, P.I., Fadda, D., Fang, F., Frayer, D.T., Hein- richsen, I., Helou, G., Im, M., Marleau, F.R., Masci, F., Shupe, D.L., Soifer, B....

    arXiv

  47. [103]

    arXiv e-prints , arXiv:2312.03589doi: 10.48550/arXiv.2312

    GA-NIFS: JWST discovers an offset AGN 740 million years after the Big Bang. arXiv e-prints , arXiv:2312.03589doi: 10.48550/arXiv.2312. 03589, arXiv:2312.03589. Ueda, Y ., Akiyama, M., Hasinger, G., Miyaji, T., Watson, M.G., 2014. Toward the Standard Population Synthesis Model ...

    doi arXiv

  48. [104]

    ApJ 698, 1232–1243

    On the Size and Comoving Mass Density Evolution of Early-Type Galaxies. ApJ 698, 1232–1243. doi: 10.1088/0004-637X/698/2/1232, arXiv:0903.4857. van Velzen, S., Holoien, T.W.S., Onori, F., Hung, T., Arcavi, I., 2020. Optical- Ultraviolet Tidal Disruption Events. Space Sci. Rev....

    2020 arXiv

  49. [105]

    Visbal, E., Haiman, Z., Bryan, G.L., 2014

    doi: 10.1093/mnras/stw3037, arXiv:1611.06236. Visbal, E., Haiman, Z., Bryan, G.L., 2014. Direct collapse black hole formation from synchronized pairs of atomic cooling haloes. MNRAS 445, 1056–

    2014 arXiv

  50. [108]

    Nature 566, 85–88

    Formation of massive black holes in rapidly growing pre-galactic gas clouds. Nature 566, 85–88. doi: 10.1038/s41586-019-0873-4 , arXiv:1901.07563. Wolf, J., Nandra, K., Salvato, M., Liu, T., Buchner, J., Brusa, M., Hoang, D.N., Moss, V ., Arcodia, R., Br¨uggen, M., Comparat, J...

    1901 arXiv

  51. [109]

    Assef, R.J., Eisenhardt, P.R.M., Stern, D., Tsai, C.W., Wu, J., Wylezalek, D., Blain, A.W., Bridge, C.R., Donoso, E., Gonzales, A., Gri ffith, R.L., Jarrett, T.H., 2015

    doi: 10.3847/0004-637X/822/2/109, arXiv:1603.02710. Assef, R.J., Eisenhardt, P.R.M., Stern, D., Tsai, C.W., Wu, J., Wylezalek, D., Blain, A.W., Bridge, C.R., Donoso, E., Gonzales, A., Gri ffith, R.L., Jarrett, T.H., 2015. Half of the Most Luminous Quasars May Be Obscured: Inve...

    2015 arXiv

  52. [110]

    doi: 10.3847/1538-4357/aa9ff3, arXiv:1703.06888. Wu, J., Tsai, C.W., Sayers, J., Benford, D., Bridge, C., Blain, A., Eisenhardt, P.R.M., Stern, D., Petty, S., Assef, R., Bussmann, S., Comerford, J.M., Cutri, R., Evans, Neal J., I., Gri ffith, R., Jarrett, T., Lake, S., Lonsdal...

    arXiv

  53. [111]

    Jacomy, M., Venturini, T., Heymann, S., Bastian, M., 2014

    doi: 10.1093/pasj/psz096, arXiv:1904.07345. Jacomy, M., Venturini, T., Heymann, S., Bastian, M., 2014. Forceatlas2, a continuous graph layout algorithm for handy network visualization designed for the gephi software. PloS one 9, e98679. doi:10.1371/journal.pone. 0098679. Janss...

    1904 arXiv

  54. [112]

    Wylezalek, D., Morganti, R., 2018

    doi: 10.1088/0004-637X/756/1/96, arXiv:1208.5518. Wylezalek, D., Morganti, R., 2018. Questions and challenges of what powers galactic outflows in active galactic nuclei. Nature Astronomy 2, 181–182. doi:10.1038/s41550-018-0409-0 , arXiv:1802.10307. Wylezalek, D., Zakamska, N.L...

    2018 arXiv

  55. [113]

    Davis, S.W., Tchekhovskoy, A., 2020

    doi: 10.3847/1538-4357/aae820, arXiv:1810.04888. Davis, S.W., Tchekhovskoy, A., 2020. Magnetohydrodynamics Simulations of Active Galactic Nucleus Disks and Jets. ARA&A 58, 407–439. doi: 10. 1146/annurev-astro-081817-051905 , arXiv:2101.08839. Dayal, P., 2024. Exploring a primo...

    2020 arXiv

  56. [114]

    MNRAS 459, 3144–3160

    Discovery of extreme [O III] λ5007 Å outflows in high-redshift red quasars. MNRAS 459, 3144–3160. doi: 10.1093/mnras/stw718, arXiv:1512.02642. Zakamska, N.L., Sun, A.L., Strauss, M.A., Alexandro ff, R.M., Brandt, W.N., Chiaberge, M., Greene, J.E., Hamann, F., Liu, G., Perrotta...

    arXiv

  57. [115]

    ApJ 640, 574–578

    An Overdensity of Galaxies near the Most Distant Radio-loud Quasar. ApJ 640, 574–578. doi: 10.1086/500167, arXiv:astro-ph/0511734. Zinger, E., Pillepich, A., Nelson, D., Weinberger, R., Pakmor, R., Springel, V ., Hernquist, L., Marinacci, F., V ogelsberger, M., 2020. Ejective ...

    arXiv

  58. [141]

    Mezcua, M., 2017

    doi: 10.3847/1538-4357/ac4f67, arXiv:2201.09720. Mezcua, M., 2017. Observational evidence for intermediate-mass black holes. International Journal of Modern Physics D 26, 1730021. doi: 10.1142/ S021827181730021X, arXiv:1705.09667. Mezcua, M., Civano, F., Fabbiano, G., Miyaji, ...

    2017 arXiv

  59. [158]

    Scannapieco, E., Oh, S.P., 2004

    doi: 10.1088/0004-637X/805/2/158, arXiv:1503.06800. Scannapieco, E., Oh, S.P., 2004. Quasar Feedback: The Missing Link in Structure Formation. ApJ 608, 62–79. doi: 10.1086/386542, arXiv:astro-ph/0401087. Schawinski, K., Koss, M., Berney, S., Sartori, L.F., 2015. Active galacti...

    2004 arXiv

  60. [162]

    Chevallard, J., Charlot, S., 2016

    doi: 10.3847/1538-4357/ac401b, arXiv:2108.01672. Chevallard, J., Charlot, S., 2016. Modelling and interpreting spectral energy distributions of galaxies with BEAGLE. MNRAS 462, 1415–1443. doi:10. 1093/mnras/stw1756, arXiv:1603.03037. Chiaberge, M., Marconi, A., 2011. On the or...

    2016 arXiv

  61. [231]

    Rakshit, S., Stalin, C.S., Kotilainen, J., 2020

    doi: 10.1086/507672, arXiv:astro-ph/0605323. Rakshit, S., Stalin, C.S., Kotilainen, J., 2020. Spectral Properties of Quasars from Sloan Digital Sky Survey Data Release 14: The Catalog. ApJS 249,

    2020 arXiv

  62. [391]

    Little Red Dots

    doi: 10.1088/0004-637X/720/1/368, arXiv:1007.1453. Xue, Y .Q., Luo, B., Brandt, W.N., Alexander, D.M., Bauer, F.E., Lehmer, B.D., Yang, G., 2016. The 2 Ms Chandra Deep Field-North Survey and the 250 ks Extended Chandra Deep Field-South Survey: Improved Point- source Catalogs. ...

    2016 arXiv

  63. [515]

    Deane, R.P., Paragi, Z., Jarvis, M.J., Coriat, M., Bernardi, G., Fender, R.P., Frey, S., Heywood, I., Kl ¨ockner, H.R., Grainge, K., Rumsey, C., 2014

    doi: 10.1126/science.149.3683.510. Deane, R.P., Paragi, Z., Jarvis, M.J., Coriat, M., Bernardi, G., Fender, R.P., Frey, S., Heywood, I., Kl ¨ockner, H.R., Grainge, K., Rumsey, C., 2014. A close-pair binary in a distant triple supermassive black hole system. Nature 511, 57–60. ...

    2014 arXiv

  64. [753]

    Tremmel, M., Karcher, M., Governato, F., V olonteri, M., Quinn, T.R., Pontzen, A., Anderson, L., Bellovary, J., 2017

    doi: 10.1086/341002, arXiv:astro-ph/0203468. Tremmel, M., Karcher, M., Governato, F., V olonteri, M., Quinn, T.R., Pontzen, A., Anderson, L., Bellovary, J., 2017. The Romulus cosmological simula- tions: a physical approach to the formation, dynamics and accretion mod- els of S...

    2017 arXiv

  65. [830]

    doi: 10.1093/mnras/staf062, arXiv:2402.15240. Smith, D.J.B., Best, P.N., Duncan, K.J., Hatch, N.A., Jarvis, M.J., R ¨ottgering, H.J.A., Simpson, C.J., Stott, J.P., Cochrane, R.K., Coppin, K.E., Danner- bauer, H., Davis, T.A., Geach, J.E., Hale, C.L., Hardcastle, M.J., Hatfield...

    arXiv

  66. [919]

    Hickox, R.C., Mullaney, J.R., Alexander, D.M., Chen, C.T.J., Civano, F.M., Goulding, A.D., Hainline, K.N., 2014

    doi: 10.1088/0004-637X/696/1/891, arXiv:0901.4121. Hickox, R.C., Mullaney, J.R., Alexander, D.M., Chen, C.T.J., Civano, F.M., Goulding, A.D., Hainline, K.N., 2014. Black Hole Variability and the Star Formation-Active Galactic Nucleus Connection: Do All Star-forming Galaxies Ho...

    2014 arXiv

  67. [977]

    Genzel, R., Eisenhauer, F., Gillessen, S., 2024

    doi: 10.1093/mnras/stae2144, arXiv:2405.08870. Genzel, R., Eisenhauer, F., Gillessen, S., 2024. Experimental studies of black holes: status and future prospects. A&A Rev. 32, 3. doi: 10.1007/ s00159-024-00154-z , arXiv:2404.03522. Georgakakis, A., Aird, J., Schulze, A., Dwelly...

    2024 arXiv

  68. [1063]

    Vito, F., Brandt, W.N., Comastri, A., Gilli, R., Ivison, R.J., Lanzuisi, G., Lehmer, B.D., Lopez, I.E., Tozzi, P., Vignali, C., 2024

    doi: 10.1093/mnras/stu1794, arXiv:1406.7020. Vito, F., Brandt, W.N., Comastri, A., Gilli, R., Ivison, R.J., Lanzuisi, G., Lehmer, B.D., Lopez, I.E., Tozzi, P., Vignali, C., 2024. Fast supermassive black hole growth in the SPT2349–56 protocluster at z = 4.3. A&A 689, A130. doi:...

    2024 arXiv

  69. [1195]

    97 Kelly, B.C., Shen, Y ., 2013

    doi: 10.1086/115207. 97 Kelly, B.C., Shen, Y ., 2013. The Demographics of Broad-line Quasars in the Mass-Luminosity Plane. II. Black Hole Mass and Eddington Ra- tio Functions. ApJ 764, 45. doi: 10.1088/0004-637X/764/1/45, arXiv:1209.0477. Kennicutt, Jr., R.C., 1998. Star Forma...

    2013 arXiv

  70. [1229]

    Haehnelt, M.G., Natarajan, P., Rees, M.J., 1998

    doi: 10.1093/mnras/stz2105, arXiv:1810.11535. Haehnelt, M.G., Natarajan, P., Rees, M.J., 1998. High-redshift galaxies, their active nuclei and central black holes. MNRAS 300, 817–827. doi:10.1046/ j.1365-8711.1998.01951.x, arXiv:astro-ph/9712259. Hagen, S., Done, C., Silverman...

    1998 arXiv

  71. [1420]

    doi: 10.1093/mnras/stad1468, arXiv:2305.05053. Dolag, K., Remus, R.S., Valenzuela, L.M., Kimmig, L.C., Seidel, B., Fortune, S., Stoiber, J., Ivleva, A., Ho ffmann, T., Bi ffi, V ., Marini, I., Popesso, P., Vladutescu-Zopp, S., 2025. Encyclopedia Magneticum: Scaling Relations f...

    arXiv

  72. [1828]

    doi: 10.1093/mnras/sty2900, arXiv:1810.03686. Hamann, F., Zakamska, N.L., Ross, N., Paris, I., Alexandro ff, R.M., Villforth, C., Richards, G.T., Herbst, H., Brandt, W.N., Cook, B., Denney, K.D., Greene, J.E., Schneider, D.P., Strauss, M.A., 2017. Extremely red quasars in BOSS...

    arXiv

  73. [1995]

    Nature 375, 469–471

    Evidence for a large undetected population of dust-reddened quasars. Nature 375, 469–471. doi: 10.1038/375469a0. Weinberger, R., Ehlert, K., Pfrommer, C., Pakmor, R., Springel, V ., 2017a. Simulating the interaction of jets with the intracluster medium. MNRAS 470, 4530–4546. d...

    arXiv

  74. [2001]

    Georgakakis, A., Ruiz, A., LaMassa, S.M., 2020

    doi: 10.1093/mnras/stx1602, arXiv:1705.01133. Georgakakis, A., Ruiz, A., LaMassa, S.M., 2020. Forward modelling the multiwavelength properties of active galactic nuclei: application to X-ray and WISE mid-infrared samples. MNRAS 499, 710–729. doi: 10.1093/ mnras/staa2528, arXiv...

    2020 arXiv

  75. [2004]

    ApJ 607, 800–809

    A Systematic Study of Radio-induced X-Ray Cavities in Clus- ters, Groups, and Galaxies. ApJ 607, 800–809. doi: 10.1086/383519, arXiv:astro-ph/0402348. Bischetti, M., Fiore, F., Feruglio, C., D’Odorico, V ., Arav, N., Costa, T., Zubo- vas, K., Becker, G., Bosman, S.E.I., Cupani...

    arXiv

  76. [2005]

    Space Sci

    The Burst Alert Telescope (BAT) on the SWIFT Midex Mis- sion. Space Sci. Rev. 120, 143–164. doi: 10.1007/s11214-005-5096-3 , arXiv:astro-ph/0507410. Baskin, A., Laor, A., 2005. What controls the CIV line profile in active galactic nuclei? MNRAS 356, 1029–1044. doi: 10.1111/j.1...

    2005 arXiv

  77. [2006]

    Black Hole Star

    First Measurement of the Clustering Evolution of Photometri- cally Classified Quasars. ApJ 638, 622–634. doi: 10.1086/499093, arXiv:arXiv:astro-ph/0510371. Naidu, R.P., Matthee, J., Katz, H., de Graaff, A., Oesch, P., Smith, A., Greene, J.E., Brammer, G., Weibel, A., Hviding, ...

    arXiv

  78. [2007]

    ApJ 660, L11–L14

    AEGIS: The Color-Magnitude Relation for X-Ray-selected Ac- tive Galactic Nuclei. ApJ 660, L11–L14. doi: 10.1086/517918, arXiv:astro-ph/0607270. Nandra, K., Laird, E.S., Aird, J.A., Salvato, M., Georgakakis, A., Barro, G., Perez-Gonzalez, P.G., Barmby, P., Chary, R.R., Coil, A....

    arXiv

  79. [2008]

    ApJS 179, 360–422

    Thermonuclear (Type I) X-Ray Bursts Observed by the Rossi X-Ray Timing Explorer. ApJS 179, 360–422. doi: 10.1086/592044, arXiv:astro-ph/0608259. G´amez Rosas, V ., Isbell, J.W., Ja ffe, W., Petrov, R.G., Leftley, J.H., Hof- mann, K.H., Millour, F., Burtscher, L., Meisenheimer,...

    arXiv

  80. [2009]

    ApJ 692, 758–777

    A Catalog of Broad Absorption Line Quasars in Sloan Digital Sky Survey Data Release 5. ApJ 692, 758–777. doi: 10.1088/0004-637X/ 692/1/758, arXiv:0810.2747. Gilli, R., Comastri, A., Hasinger, G., 2007. The synthesis of the cosmic X- ray background in the Chandra and XMM-Newton...

    2007 arXiv

  81. [2010]

    A&A 518, L26

    Star formation in AGN hosts in GOODS-N. A&A 518, L26. doi:10.1051/0004-6361/201014606, arXiv:1005.2562. She, R., Ho, L.C., Feng, H., 2017. Chandra Survey of Nearby Galaxies: A Sig- nificant Population of Candidate Central Black Holes in Late-type Galaxies. ApJ 842, 131. doi: 1...

    2017 arXiv

  82. [2012]

    Mid-infrared Selection of Active Galactic Nuclei with the Wide-Field Infrared Survey Explorer. I. Characterizing WISE-selected Active Galactic Nuclei in COSMOS. ApJ 753, 30. doi: 10.1088/0004-637X/753/1/30, arXiv:1205.0811. Stern, D., Eisenhardt, P., Gorjian, V ., Kochanek, C....

    arXiv

  83. [2013]

    ApJ 776, L41

    A Direct Measurement of the Linear Bias of Mid-infrared-selected Quasars at z≈ 1 Using Cosmic Microwave Background Lensing. ApJ 776, L41. doi: 10.1088/2041-8205/776/2/L41, arXiv:1307.1706. Gebhardt, K., Bender, R., Bower, G., Dressler, A., Faber, S.M., Filippenko, A.V ., Green...

    arXiv

  84. [2015]

    MNRAS 451, 517–526

    Discovery of millimetre-wave excess emission in radio-quiet active galactic nuclei. MNRAS 451, 517–526. doi: 10.1093/mnras/stv988, arXiv:1504.01226. Bellm, E.C., Kulkarni, S.R., Graham, M.J., Dekany, R., Smith, R.M., Rid- dle, R., Masci, F.J., Helou, G., Prince, T.A., Adams, S...

    arXiv

  85. [2016]

    ApJ 823, L12

    ALMA Resolves the Torus of NGC 1068: Continuum and Molecu- lar Line Emission. ApJ 823, L12. doi: 10.3847/2041-8205/823/1/L12, arXiv:1604.00205. Garc´ıa-Burillo, S., Combes, F., Usero, A., Aalto, S., Krips, M., Viti, S., Alonso- Herrero, A., Hunt, L.K., Schinnerer, E., Baker, A...

    arXiv

  86. [2017]

    MNRAS 464, 2840–2853

    Gravitational torque-driven black hole growth and feedback in cos- mological simulations. MNRAS 464, 2840–2853. doi: 10.1093/mnras/ stw2565, arXiv:1603.08007. Angl´es-Alc´azar, D., Quataert, E., Hopkins, P.F., Somerville, R.S., Hayward, C.C., Faucher-Gigu`ere, C.A., Bryan, G.L...

    arXiv

  87. [2018]

    ApJS 234, 23

    The WISE AGN Catalog. ApJS 234, 23. doi: 10.3847/1538-4365/ aaa00a, arXiv:1706.09901. Audibert, A., Combes, F., Garc ´ıa-Burillo, S., Hunt, L., Eckart, A., Aalto, S., Casasola, V ., Boone, F., Krips, M., Viti, S., Muller, S., Dasyra, K., van der Werf, P., Mart´ın, S., 2019. AL...

    arXiv

  88. [2019]

    Nature Astronomy 3, 387–396

    The origin of radio emission from radio-quiet active galactic nu- clei. Nature Astronomy 3, 387–396. doi: 10.1038/s41550-019-0765-4 , arXiv:1902.05917. Pardo, K., Goulding, A.D., Greene, J.E., Somerville, R.S., Gallo, E., Hickox, R.C., Miller, B.P., Reines, A.E., Silverman, J....

    1902 arXiv

  89. [2020]

    (Eds.), Space Telescopes and Instrumentation 2020: Optical, Infrared, and Millimeter Wave, p

    SPHEREx: NASA’s near-infrared spectrophotometric all-sky survey, in: Lystrup, M., Perrin, M.D. (Eds.), Space Telescopes and Instrumentation 2020: Optical, Infrared, and Millimeter Wave, p. 114430I. doi: 10.1117/ 12.2567224, arXiv:2404.11017. Croom, S.M., Boyle, B.J., Shanks, T...

    2020 arXiv

  90. [2021]

    MNRAS 505, 5753–5783

    Properties of the multiphase outflows in local (ultra)luminous infrared galaxies. MNRAS 505, 5753–5783. doi: 10.1093/mnras/stab1666, arXiv:2006.13232. Fornasini, F.M., Civano, F., Fabbiano, G., Elvis, M., Marchesi, S., Miyaji, T., Zezas, A., 2018. Low-luminosity AGN and X-Ray ...

    2006 arXiv

  91. [2022]

    ApJ 934, L34

    XMM and NuSTAR Observations of an Optically Quiescent Quasar. ApJ 934, L34. doi: 10.3847/2041-8213/ac83a0, arXiv:2208.01627. Greenwell, C., Gandhi, P., Stern, D., Lansbury, G., Mainieri, V ., Boorman, P., Toba, Y ., 2024a. A population of Optically Quiescent Quasars from WISE ...

    arXiv

  92. [2023]

    Subaru High-z Exploration of Low-luminosity Quasars (SHELLQs). XVIII. The Dark Matter Halo Mass of Quasars at z 6. ApJ 954, 210. doi:10. 3847/1538-4357/ace43a, arXiv:2307.02531. Arita, J., Kashikawa, N., Onoue, M., Yoshioka, T., Takeda, Y ., Hoshi, H., Shimizu, S., 2025. The n...

    arXiv

  93. [2024]

    ApJ 965, 12

    Testing EMRI Models for Quasi-periodic Eruptions with 3.5 yr of Monitoring eRO-QPE1. ApJ 965, 12. doi: 10.3847/1538-4357/ad2941, arXiv:2402.08722. Chakraborty, P., Chatterjee, S., Dutta, A., Myers, A.D., 2018. Mean Occupation Function of High-redshift Quasars from the Planck C...

    2018 arXiv

  94. [2025]

    MNRAS 537, 1369–1384

    I Zw 1 and H0557-385: the dusty tori of two high Eddington AGNs observed in the MATISSE LM bands. MNRAS 537, 1369–1384. doi:10.1093/mnras/staf110, arXiv:2501.10352. Driver, S.P., Norberg, P., Baldry, I.K., Bamford, S.P., Hopkins, A.M., Liske, J., Loveday, J., Peacock, J.A., Hi...

  95. [2421]

    Coil, A.L., Aird, J., Reddy, N., Shapley, A.E., Kriek, M., Siana, B., Mobasher, B., Freeman, W.R., Price, S.H., Shivaei, I., 2015

    doi: 10.1093/mnras/stad1528, arXiv:2303.12858. Coil, A.L., Aird, J., Reddy, N., Shapley, A.E., Kriek, M., Siana, B., Mobasher, B., Freeman, W.R., Price, S.H., Shivaei, I., 2015. The MOSDEF Survey: Optical Active Galactic Nucleus Diagnostics at z˜2.3. ApJ 801, 35. doi:10. 1088/...

    2015 arXiv

  96. [2455]

    van de V oort, F., Schaye, J., Booth, C.M., Dalla Vecchia, C., 2011

    doi: 10.1093/mnras/stu1613, arXiv:1409.2873. van de V oort, F., Schaye, J., Booth, C.M., Dalla Vecchia, C., 2011. The drop in the cosmic star formation rate below redshift 2 is caused by a change in the mode of gas accretion and by active galactic nucleus feedback. MNRAS 415, ...

    2011 arXiv

  97. [2730]

    Zakamska, N.L., Greene, J.E., 2014

    doi: 10.1093/mnras/stad2474, arXiv:2306.06303. Zakamska, N.L., Greene, J.E., 2014. Quasar feedback and the origin of radio emission in radio-quiet quasars. MNRAS 442, 784–804. doi: 10.1093/ mnras/stu842, arXiv:1402.6736. Zakamska, N.L., Hamann, F., P ˆaris, I., Brandt, W.N., G...

    2014 arXiv

  98. [3042]

    Habouzit, M., V olonteri, M., Somerville, R.S., Dubois, Y ., Peirani, S., Pichon, C., Devriendt, J., 2019

    doi: 10.1093/mnras/stab3147, arXiv:2111.01802. Habouzit, M., V olonteri, M., Somerville, R.S., Dubois, Y ., Peirani, S., Pichon, C., Devriendt, J., 2019. The diverse galaxy counts in the environment of high-redshift massive black holes in Horizon-AGN. MNRAS 489, 1206–

    2019 arXiv

  99. [3071]

    doi: 10.1093/mnras/sty1274, arXiv:1711.02094. Bogd´an, ´A., Goulding, A.D., Natarajan, P., Kov´acs, O.E., Tremblay, G.R., Cha- dayammuri, U., V olonteri, M., Kraft, R.P., Forman, W.R., Jones, C., Chu- razov, E., Zhuravleva, I., 2024. Evidence for heavy-seed origin of early sup...

    arXiv

  100. [3389]

    Banerji, M., McMahon, R.G., Hewett, P.C., Alaghband-Zadeh, S., Gonzalez- Solares, E., Venemans, B.P., Hawthorn, M.J., 2012

    doi: 10.1093/mnras/stu2649, arXiv:1501.00815. Banerji, M., McMahon, R.G., Hewett, P.C., Alaghband-Zadeh, S., Gonzalez- Solares, E., Venemans, B.P., Hawthorn, M.J., 2012. Heavily reddened quasars at z∼ 2 in the UKIDSS Large Area Survey: a transitional phase in AGN evolution. MN...

    2012 arXiv

  101. [3391]

    Stachenfeld, K., Fielding, D.B., Kochkov, D., Cranmer, M., Pfa ff, T., Godwin, J., Cui, C., Ho, S., Battaglia, P., Sanchez-Gonzalez, A.,

    doi: 10.1093/mnras/stac2765, arXiv:2207.09484. Stachenfeld, K., Fielding, D.B., Kochkov, D., Cranmer, M., Pfa ff, T., Godwin, J., Cui, C., Ho, S., Battaglia, P., Sanchez-Gonzalez, A.,

    arXiv

  102. [3622]

    doi: 10.1093/mnras/stu2648, arXiv:1408.5141. Noeske, K.G., Weiner, B.J., Faber, S.M., Papovich, C., Koo, D.C., Somerville, R.S., Bundy, K., Conselice, C.J., Newman, J.A., Schiminovich, D., Le Floc’h, E., Coil, A.L., Rieke, G.H., Lotz, J.M., Primack, J.R., Barmby, P., Cooper, M...

    arXiv

  103. [3650]

    Talbot, R.Y ., Sijacki, D., Bourne, M.A., 2022

    doi: 10.1093/mnras/stab804, arXiv:2011.10580. Talbot, R.Y ., Sijacki, D., Bourne, M.A., 2022. Blandford-Znajek jets in galaxy formation simulations: exploring the diversity of outflows produced by spin- driven AGN jets in Seyfert galaxies. MNRAS 514, 4535–4559. doi: 10. 1093/m...

    2011 arXiv

  104. [4132]

    Graham, M.J., Djorgovski, S.G., Stern, D., Drake, A.J., Mahabal, A.A., Donalek, C., Glikman, E., Larson, S., Christensen, E., 2015

    doi: 10.1093/mnras/stx1456, arXiv:1706.03079. Graham, M.J., Djorgovski, S.G., Stern, D., Drake, A.J., Mahabal, A.A., Donalek, C., Glikman, E., Larson, S., Christensen, E., 2015. A system- atic search for close supermassive black hole binaries in the Catalina Real- time Transie...

    2015 arXiv

  105. [4169]

    Rantala, A., Naab, T., 2025

    doi: 10.1093/mnras/stab302, arXiv:2101.12635. Rantala, A., Naab, T., 2025. A rapid channel for the collisional formation and gravitational wave driven mergers of supermassive black hole seeds at high redshift. arXiv e-prints , arXiv:2503.21879doi: 10.48550/arXiv.2503. 21879, a...

    2025 arXiv

  106. [5566]

    AGN Main Sequence

    doi: 10.1093/mnras/sty1776, arXiv:1803.08305. Mullaney, J.R., Alexander, D.M., Fine, S., Goulding, A.D., Harrison, C.M., Hickox, R.C., 2013. Narrow-line region gas kinematics of 24 264 optically selected AGN: the radio connection. MNRAS 433, 622–638. doi:10.1093/ mnras/stt751,...

    2013 arXiv

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