pith. sign in

arxiv: 2606.26998 · v1 · pith:AISEBKRNnew · submitted 2026-06-25 · 🌌 astro-ph.HE

Exploring Tidal Disruption Events with SKA and VLBI: Unveiling the Mystery of Black Hole Feeding and Outflows

Xinwen Shu , Guobin Mou , Tao An , S. Komossa , Miguel Perez-Torres , Weihua Lei , Luming Sun , Ning Jiang
show 3 more authors
Tinggui Wang Chichuan Jin Jun Yang
This is my paper

Pith reviewed 2026-06-26 03:58 UTC · model grok-4.3

classification 🌌 astro-ph.HE
keywords tidal disruption eventsSKAVLBIblack hole jetsradio outflowsproper motionpolarimetrynuclear localization
0
0 comments X

The pith

SKA Mid phased for VLBI will measure proper motions in tidal disruption events to distinguish relativistic jets from subrelativistic winds at a rate of about five detections per year.

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

The paper argues that SKA Mid, when used in VLBI mode with global networks, supplies milliarcsecond imaging, tens of microarcsecond astrometry, and microJy sensitivity needed to track radio-emitting outflows from tidal disruption events. These capabilities would separate off-axis jets from slower winds, map magnetic field structures through polarimetry, and pin down the exact location of the disrupted star relative to the black hole. With optical and X-ray surveys expected to deliver hundreds of TDE alerts annually and late-time radio flares appearing common, the setup would yield routine samples for studying black hole accretion and jet launching on human timescales.

Core claim

SKA Mid phased for VLBI delivers milliarcsecond imaging, tens of microarcsecond astrometry, and microJy sensitivity that enable proper motion measurements to discriminate off-axis relativistic jets from subrelativistic winds, resolved morphologies and magnetic field diagnostics via polarimetry, and precise nuclear localization to distinguish supermassive from intermediate-mass black holes or to reveal recoiling or binary systems, with a forecast of about five proper motion detections of jetted TDEs per year.

What carries the argument

SKA Mid phased for VLBI, using wide frequency coverage from 0.35 to 15.4 GHz, 1-hour continuum sensitivities of 3 to 10 microJy per beam, multibeam tied-array VLBI, and a transient buffer for rapid triggers.

If this is right

  • Proper motion measurements will discriminate off-axis relativistic jets from subrelativistic winds in TDEs.
  • Resolved morphologies and magnetic field diagnostics will become available via polarimetry.
  • Precise nuclear localization will distinguish supermassive black holes from intermediate-mass black holes and reveal recoiling or binary systems.
  • Routine core shift constraints at the microarcsecond level will constrain jet structure.
  • TDEs will serve as laboratories for jet launching, particle acceleration including neutrinos, black hole accretion history, and circumnuclear medium properties.

Where Pith is reading between the lines

These are editorial extensions of the paper, not claims the author makes directly.

  • The same VLBI astrometry could be applied to test whether TDE rates correlate with galaxy merger histories in large samples.
  • Coordinated radio and neutrino observations might reveal whether TDE jets accelerate high-energy particles at detectable levels.
  • If binary black hole systems are localized, the technique could provide targets for future gravitational wave searches.
  • Extending the frequency coverage to lower bands might map larger-scale outflow interactions with the host galaxy interstellar medium.

Load-bearing premise

Late-time radio flares are common in TDEs and that LSST, Einstein Probe, and SVOM will increase TDE alerts to hundreds per year, together with the jet and outflow models used for the detection forecasts.

What would settle it

A two-year campaign on a sample of 50 TDE radio flares yielding zero proper motion detections at the forecasted sensitivity would falsify the claim of about five detections per year.

Figures

Figures reproduced from arXiv: 2606.26998 by Chichuan Jin, Guobin Mou, Jun Yang, Luming Sun, Miguel Perez-Torres, Ning Jiang, S. Komossa, Tao An, Tinggui Wang, Weihua Lei, Xinwen Shu.

Figure 1
Figure 1. Figure 1: The left panels show the near-infrared outburst of the TDE Arp 299-B AT1 (B and C) and the color-composite optical image of its host galaxy (A). The evolution of the radio morphology as imaged with VLBI at 8.4 GHz (Mattila et al., 2018) is shown in panel D. It can be seen that an initially unresolved radio source develops into a resolved jet structure a few years after the explosion, which is viewed with a… view at source ↗
Figure 2
Figure 2. Figure 2: Natural-weighted images of VLBA observations of AT2018cqh at three frequencies (upper panel), which reveal a compact radio emission, unresolved at a scale of < ∼ 0.13 pc (Yang et al., 2025). Lower panel shows the radio light curves at 0.89 GHz, 1.3-1.6 GHz and 3 GHz (left), and the radio SEDs over three epochs (right). The green, orange, and blue lines represent the best fits to each SED, which are the mod… view at source ↗
Figure 3
Figure 3. Figure 3: The left panels show the snapshots of gas density and energy density of relativistic electrons during the outflow-CNM/cloud interaction (in Gaussian-cgs units), as well as the synthetic radio spectra (𝑑𝐿 = 100 Mpc). The spectral panel displays both the BS+FS component and the FS component alone, from which the impact and the rapid variability feature of the BS can be observed. The shaded regions represent … view at source ↗
read the original abstract

Tidal disruption events (TDEs) probe the birth and evolution of black hole accretion flows and jets on human timescales. Radio emission traces shocks and outflows from thermal TDEs and powerful relativistic jets in the rare jetted class. SKA Mid, phased for VLBI and used together with global networks, will deliver milliarcsecond imaging, tens of microarcsecond astrometry, and microJy sensitivity, enabling: (i) proper motion measurements that discriminate off axis relativistic jets from subrelativistic winds; (ii) resolved morphologies and magnetic field diagnostics via polarimetry; and (iii) precise nuclear localization to distinguish SMBH vs. IMBH and to reveal recoiling or binary systems. SKA's wide frequency coverage (0.35 to 15.4 GHz) and 1h continuum sensitivities of 3 to 10 microJy per beam, together with multibeam tiedarray VLBI and a transient buffer for rapid triggers, are transformational. LSST, Einstein Probe, and SVOM will increase TDE alerts to hundreds per year, and late time radio flares appear common, ensuring rich SKA VLBI samples. We provide observing strategies, detection forecasts, and predictions, e.g., about 5 proper motion detections of jetted (or off axis) TDEs per year and routine core shift constraints at the microarcsecond level. This program will establish TDEs as laboratories for exploring jet launching, particle acceleration (including neutrinos), black hole accretion history and demographics, and properties of circumnuclear medium.

Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, simulated authors' rebuttal, and a circularity audit. Tearing a paper down is the easy half of reading it; the pith above is the substance, this is the friction.

Referee Report

2 major / 0 minor

Summary. The manuscript argues that SKA Mid, when phased for VLBI with global networks, will deliver milliarcsecond imaging, tens of microarcsecond astrometry, and microJy sensitivity, enabling proper-motion measurements to distinguish off-axis relativistic jets from subrelativistic winds in TDEs, resolved morphologies via polarimetry, and precise nuclear localization. It forecasts ~5 proper motion detections of jetted TDEs per year, driven by hundreds of annual TDE alerts from LSST, Einstein Probe, and SVOM together with the assumed commonality of late-time radio flares, and outlines observing strategies and additional predictions such as routine core-shift constraints.

Significance. If the numerical forecasts hold after detailed validation, the work would usefully map SKA-VLBI capabilities onto TDE science questions including jet launching, particle acceleration, and circumnuclear medium properties. The emphasis on proper-motion discrimination and multi-messenger triggering is a concrete strength, though the paper's impact is limited by its dependence on external rate and model assumptions rather than new derivations.

major comments (2)
  1. [Abstract] Abstract: the headline forecast of ~5 proper motion detections per year is presented without any description of the underlying calculation, error propagation, or sensitivity to input parameters such as the fraction of TDEs exhibiting late-time radio flares or the assumed Lorentz-factor distribution of jets.
  2. [Abstract] Abstract: the detection forecasts rely on external literature values for TDE rates, flare incidence, and jet/outflow properties rather than reducing to quantities defined or tested within the manuscript, so that changes in those inputs by factors of a few would alter the annual yield substantially.

Simulated Author's Rebuttal

2 responses · 0 unresolved

We thank the referee for the detailed and constructive report. The comments correctly identify that the abstract presents the headline forecast without sufficient context on its derivation. We address both points below and will revise the manuscript accordingly.

read point-by-point responses

  1. Referee: [Abstract] Abstract: the headline forecast of ~5 proper motion detections per year is presented without any description of the underlying calculation, error propagation, or sensitivity to input parameters such as the fraction of TDEs exhibiting late-time radio flares or the assumed Lorentz-factor distribution of jets.

    Authors: We agree that the abstract would be strengthened by brief context on the forecast. In the revised version we will add one sentence summarizing the main inputs (TDE alert rates from LSST/Einstein Probe/SVOM, assumed late-time flare incidence drawn from existing radio follow-up campaigns, and a fiducial jet Lorentz-factor range) and explicitly refer readers to the dedicated forecast section for the full calculation, error propagation, and parameter-sensitivity analysis. revision: yes

  2. Referee: [Abstract] Abstract: the detection forecasts rely on external literature values for TDE rates, flare incidence, and jet/outflow properties rather than reducing to quantities defined or tested within the manuscript, so that changes in those inputs by factors of a few would alter the annual yield substantially.

    Authors: The forecasts necessarily incorporate published TDE rates and outflow statistics because these quantities are not re-derived in the present work. To make the dependence transparent, we will insert a short sensitivity subsection (or paragraph in the forecast section) that shows how the ~5 detections yr⁻¹ figure scales when the flare incidence or Lorentz-factor distribution is varied by factors of 2–3. This addition will quantify the robustness without altering the core science case. revision: yes

Circularity Check

0 steps flagged

No significant circularity; forecasts rest on external inputs

full rationale

The paper's central numerical forecasts (e.g., ~5 proper-motion detections per year) are presented as conditional predictions that explicitly depend on external literature values for TDE alert rates from LSST/Einstein Probe/SVOM, the assumed commonality of late-time radio flares, and specific jet/outflow models. No derivation step reduces by construction to a quantity defined inside the paper, no self-citation is invoked as a uniqueness theorem or load-bearing premise, and no fitted parameter is relabeled as a prediction. The chain is therefore self-contained against external benchmarks rather than tautological.

Axiom & Free-Parameter Ledger

0 free parameters · 0 axioms · 0 invented entities

Only the abstract is available, so the ledger is necessarily incomplete. The numerical forecasts implicitly rest on assumed TDE occurrence rates, jet opening angles, and radio luminosity functions drawn from earlier papers; no new free parameters or invented entities are introduced in the provided text.

pith-pipeline@v0.9.1-grok · 5852 in / 1139 out tokens · 47324 ms · 2026-06-26T03:58:44.559003+00:00 · methodology

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Reference graph

Works this paper leans on

76 extracted references · 70 canonical work pages · 25 internal anchors

  1. [1]

    Science Bulletin , keywords =

    A fast powerful X-ray transient from possible tidal disruption of a white dwarf. Science Bulletin , keywords =. doi:10.1016/j.scib.2025.12.050 , archivePrefix =. 2509.25877 , primaryClass =

    work page doi:10.1016/j.scib.2025.12.050 2025

  2. [2]

    A new class of flares from accreting supermassive black holes

    A new class of flares from accreting supermassive black holes. Nature Astronomy , keywords =. doi:10.1038/s41550-018-0661-3 , archivePrefix =. 1901.03731 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1038/s41550-018-0661-3 1901

  3. [3]

    T., Holoien, T

    The Curious Case of ASASSN-20hx: A Slowly Evolving, UV- and X-Ray-Luminous, Ambiguous Nuclear Transient. , keywords =. doi:10.3847/1538-4357/ac5f54 , archivePrefix =. 2108.03245 , primaryClass =

    work page doi:10.3847/1538-4357/ac5f54

  4. [4]

    , keywords =

    To TDE or not to TDE: the luminous transient ASASSN-18jd with TDE-like and AGN-like qualities. , keywords =. doi:10.1093/mnras/staa859 , archivePrefix =. 1910.01142 , primaryClass =

    work page doi:10.1093/mnras/staa859 1910

  5. [5]

    , keywords =

    Dust-obscured radio-emitting tidal disruption event coincident with a high-energy neutrino event. , keywords =. doi:10.1103/j8g9-f6hh , archivePrefix =. 2601.05601 , primaryClass =

    work page doi:10.1103/j8g9-f6hh

  6. [6]

    Swift J1112.2-8238: A Candidate Relativistic Tidal Disruption Flare

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

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1093/mnras/stv1520

  7. [7]

    Swift J2058.4+0516: Discovery of a Possible Second Relativistic Tidal Disruption Flare?

    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 =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1088/0004-637x/753/1/77

  8. [8]

    , keywords =

    Generalized equipartition method from an arbitrary viewing angle. , keywords =. doi:10.1093/mnras/stad1269 , archivePrefix =. 2211.10051 , primaryClass =

    work page doi:10.1093/mnras/stad1269

  9. [9]

    , keywords =

    Late-time Radio Flares in Tidal Disruption Events. , keywords =. doi:10.3847/1538-4357/ad58ba , archivePrefix =. 2404.15966 , primaryClass =

    work page doi:10.3847/1538-4357/ad58ba

  10. [10]

    , keywords =

    Misaligned precessing jets are choked by the accretion disc wind. , keywords =. doi:10.1093/mnras/stae1770 , archivePrefix =. 2310.15336 , primaryClass =

    work page doi:10.1093/mnras/stae1770

  11. [11]

    , keywords =

    A Unified Theory of Jetted Tidal Disruption Events: From Promptly Escaping Relativistic to Delayed Transrelativistic Jets. , keywords =. doi:10.3847/2041-8213/ad0037 , archivePrefix =. 2308.05161 , primaryClass =

    work page doi:10.3847/2041-8213/ad0037 2041

  12. [12]

    , keywords =

    Ubiquitous Late Radio Emission from Tidal Disruption Events. , keywords =. doi:10.3847/1538-4357/ad5541 , archivePrefix =. 2308.13595 , primaryClass =

    work page doi:10.3847/1538-4357/ad5541

  13. [13]

    , keywords =

    A Mildly Relativistic Outflow Launched Two Years after Disruption in Tidal Disruption Event AT2018hyz. , keywords =. doi:10.3847/1538-4357/ac88d0 , archivePrefix =. 2206.14297 , primaryClass =

    work page doi:10.3847/1538-4357/ac88d0

  14. [14]

    Discovery of the Onset of Rapid Accretion by a Dormant Massive Black Hole

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

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1038/nature10374

  15. [15]

    , keywords =

    EP241021a: A Months-duration X-Ray Transient with Luminous Optical and Radio Emission. , keywords =. doi:10.3847/2041-8213/adf4cd , archivePrefix =. 2505.07665 , primaryClass =

    work page doi:10.3847/2041-8213/adf4cd 2041

  16. [16]

    , keywords =

    Detection of a Drag Force in G2's Orbit: Measuring the Density of the Accretion Flow onto Sgr A* at 1000 Schwarzschild Radii. , keywords =. doi:10.3847/1538-4357/aaf4f8 , adsurl =

    work page doi:10.3847/1538-4357/aaf4f8

  17. [17]

    Nature Astronomy , keywords =

    Delayed radio flares from a tidal disruption event. Nature Astronomy , keywords =. doi:10.1038/s41550-021-01300-8 , archivePrefix =. 2102.11290 , primaryClass =

    work page doi:10.1038/s41550-021-01300-8

  18. [18]

    Swift J1644+57 gone MAD: the case for dynamically-important magnetic flux threading the black hole in a jetted tidal disruption event

    Swift J1644+57 gone MAD: the case for dynamically important magnetic flux threading the black hole in a jetted tidal disruption event. , keywords =. doi:10.1093/mnras/stt2085 , archivePrefix =. 1301.1982 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1093/mnras/stt2085 1982

  19. [19]

    Tidal disruption of stars by supermassive black holes: Status of observations

    Tidal disruption of stars by supermassive black holes: Status of observations. Journal of High Energy Astrophysics , keywords =. doi:10.1016/j.jheap.2015.04.006 , archivePrefix =. 1505.01093 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1016/j.jheap.2015.04.006 2015

  20. [20]

    , keywords =

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

    work page doi:10.1038/333523a0

  21. [21]

    , keywords =

    The Analogous Structure of Accretion Flows in Supermassive and Stellar Mass Black Holes: New Insights from Faded Changing-look Quasars. , keywords =. doi:10.3847/1538-4357/ab3c1a , archivePrefix =. 1903.02553 , primaryClass =

    work page doi:10.3847/1538-4357/ab3c1a 1903

  22. [22]

    The Man Behind the Curtain: X-rays Drive the UV through NIR Variability in the 2013 AGN Outburst in NGC 2617

    The Man behind the Curtain: X-Rays Drive the UV through NIR Variability in the 2013 Active Galactic Nucleus Outburst in NGC 2617. , keywords =. doi:10.1088/0004-637X/788/1/48 , archivePrefix =. 1310.2241 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1088/0004-637x/788/1/48 2013

  23. [23]

    Chandra X-ray Spectroscopic Imaging of Sgr A* and the Central Parsec of the Galaxy

    Chandra X-Ray Spectroscopic Imaging of Sagittarius A* and the Central Parsec of the Galaxy. , keywords =. doi:10.1086/375145 , archivePrefix =. astro-ph/0102151 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1086/375145

  24. [24]

    Caltech-NRAO Stripe 82 Survey (CNSS). III. The First Radio-discovered Tidal Disruption Event, CNSS J0019+00. , keywords =. doi:10.3847/1538-4357/abb94b , archivePrefix =. 1910.11912 , primaryClass =

    work page doi:10.3847/1538-4357/abb94b 1910

  25. [25]

    A dust-enshrouded tidal disruption event with a resolved radio jet in a galaxy merger

    A dust-enshrouded tidal disruption event with a resolved radio jet in a galaxy merger. Science , keywords =. doi:10.1126/science.aao4669 , archivePrefix =. 1806.05717 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1126/science.aao4669

  26. [26]

    Radio Monitoring of the Tidal Disruption Event Swift J164449.3+573451. III. Late-time Jet Energetics and a Deviation from Equipartition. , keywords =. doi:10.3847/1538-4357/aaa8e0 , archivePrefix =. 1710.07289 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.3847/1538-4357/aaa8e0

  27. [27]

    Hyperaccretion during tidal disruption events: weakly bound debris envelopes and jets

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

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1088/0004-637x/781/2/82

  28. [28]

    Discovery of an outflow from radio observations of the tidal disruption event ASASSN-14li

    Discovery of an Outflow from Radio Observations of the Tidal Disruption Event ASASSN-14li. , keywords =. doi:10.3847/2041-8205/819/2/L25 , archivePrefix =. 1510.01226 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.3847/2041-8205/819/2/l25 2041

  29. [29]

    , keywords =

    AT2022cmc: A Tidal Disruption Event with a Two-component Jet in a Bondi-profile Circumnuclear Medium. , keywords =. doi:10.3847/1538-4357/ad20f3 , adsurl =

    work page doi:10.3847/1538-4357/ad20f3

  30. [30]

    , keywords =

    Simulations of the Collision between a Debris Stream and an Outer Dusty Torus: A Possible Channel for Forming a Fast-rise and Long-delay Radio Outburst in Tidal Disruption Events. , keywords =. doi:10.3847/1538-4357/ad8ba5 , archivePrefix =. 2410.20127 , primaryClass =

    work page doi:10.3847/1538-4357/ad8ba5

  31. [31]

    Discovery of a time lag between the soft X-ray and radio emission of the tidal disruption flare ASASSN-14li: Evidence for linear disk-jet coupling

    Discovery of a Time Lag between the Soft X-Ray and Radio Emission of the Tidal Disruption Flare ASASSN-14li: Evidence for Linear Disk-Jet Coupling. , keywords =. doi:10.3847/1538-4357/aab361 , archivePrefix =. 1709.02882 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.3847/1538-4357/aab361

  32. [32]

    2019 , eprint=

    Anticipated Performance of the Square Kilometre Array -- Phase 1 (SKA1) , author=. 2019 , eprint=

    2019

  33. [33]

    2015 , publisher=

    Advancing Astrophysics with the Square Kilometre Array (AASKA14) , author=. 2015 , publisher=

    2015

  34. [34]

    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 =

    work page doi:10.48550/arxiv.2501.09580

  35. [35]

    , keywords =

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

    work page doi:10.1007/s11214-020-00702-w 2006

  36. [36]

    2026 ,publisher =

    Tao An and author2 and author3 and author4 and author5 ,title =. 2026 ,publisher =

    2026

  37. [37]

    2026 ,publisher =

    Quirino D'Amato and author2 and author3 and author4 and author5 ,title =. 2026 ,publisher =

    2026

  38. [38]

    A VLBA survey of the core shift effect in AGN jets. I. Evidence of dominating synchrotron opacity. , keywords =. doi:10.1051/0004-6361/201016072 , archivePrefix =. 1103.6032 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1051/0004-6361/201016072

  39. [39]

    , keywords =

    A Massive Black Hole 0.8 kpc from the Host Nucleus Revealed by the Offset Tidal Disruption Event AT2024tvd. , keywords =. doi:10.3847/2041-8213/add7de , archivePrefix =. 2502.17661 , primaryClass =

    work page doi:10.3847/2041-8213/add7de 2041

  40. [40]

    On the Missing Energy Puzzle of Tidal Disruption Events

    On the Missing Energy Puzzle of Tidal Disruption Events. , keywords =. doi:10.3847/1538-4357/aad54a , archivePrefix =. 1802.02151 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.3847/1538-4357/aad54a

  41. [41]

    , keywords =

    Swift J1644+57 as an off-axis Jet. , keywords =. doi:10.1093/mnras/stad1950 , archivePrefix =. 2305.06370 , primaryClass =

    work page doi:10.1093/mnras/stad1950

  42. [42]

    Radius constraints and minimal equipartition energy of relativistically moving synchrotron sources

    Radius Constraints and Minimal Equipartition Energy of Relativistically Moving Synchrotron Sources. , keywords =. doi:10.1088/0004-637X/772/1/78 , archivePrefix =. 1301.6759 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1088/0004-637x/772/1/78

  43. [43]

    , keywords =

    1ES 1927+654: An AGN Caught Changing Look on a Timescale of Months. , keywords =. doi:10.3847/1538-4357/ab39e4 , archivePrefix =. 1903.11084 , primaryClass =

    work page doi:10.3847/1538-4357/ab39e4 1927

  44. [44]

    , keywords =

    The Destruction and Recreation of the X-Ray Corona in a Changing-look Active Galactic Nucleus. , keywords =. doi:10.3847/2041-8213/ab91a1 , archivePrefix =. 2007.07275 , primaryClass =

    work page doi:10.3847/2041-8213/ab91a1 2041

  45. [45]

    , keywords =

    Could TDE outflows produce the PeV neutrino events?. , keywords =. doi:10.1093/mnras/stac1621 , archivePrefix =. 2112.01748 , primaryClass =

    work page doi:10.1093/mnras/stac1621

  46. [46]

    , keywords =

    Establishing accretion flares from supermassive black holes as a source of high-energy neutrinos. , keywords =. doi:10.1093/mnras/stae610 , archivePrefix =. 2111.09391 , primaryClass =

    work page doi:10.1093/mnras/stae610

  47. [47]

    A milliparsec supermassive black hole binary candidate in the galaxy SDSS J120136.02+300305.5

    A Milliparsec Supermassive Black Hole Binary Candidate in the Galaxy SDSS J120136.02+300305.5. , keywords =. doi:10.1088/0004-637X/786/2/103 , archivePrefix =. 1404.4933 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1088/0004-637x/786/2/103

  48. [48]

    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 =

    work page doi:10.1038/s41467-020-19675-z 2012

  49. [49]

    arXiv e-prints , keywords =

    Numerical Studies on the Radio Afterglows in TDE (I): Forward Shock. arXiv e-prints , keywords =

  50. [50]

    arXiv e-prints , year = 2025, month = oct, eid =

    Numerical Studies on the Radio Afterglows in TDE: Bow Shock. arXiv e-prints , year = 2025, month = oct, eid =

    2025

  51. [51]

    Nature Astronomy , keywords =

    A tidal disruption event coincident with a high-energy neutrino. Nature Astronomy , keywords =. doi:10.1038/s41550-020-01295-8 , archivePrefix =. 2005.05340 , primaryClass =

    work page doi:10.1038/s41550-020-01295-8 2005

  52. [52]

    , keywords =

    The On-axis Jetted Tidal Disruption Event AT2022cmc: X-Ray Observations and Broadband Spectral Modeling. , keywords =. doi:10.3847/1538-4357/ad2b6b , archivePrefix =. 2308.09834 , primaryClass =

    work page doi:10.3847/1538-4357/ad2b6b

  53. [53]

    Relativistic Dynamics and Extreme Mass Ratio Inspirals

    Relativistic dynamics and extreme mass ratio inspirals. Living Reviews in Relativity , keywords =. doi:10.1007/s41114-018-0013-8 , archivePrefix =. 1205.5240 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1007/s41114-018-0013-8

  54. [54]

    , keywords =

    The PARSEC view of star formation in galaxy centres: from protoclusters to star clusters in an early-type spiral. , keywords =. doi:10.1093/mnras/stae1822 , archivePrefix =. 2407.20860 , primaryClass =

    work page doi:10.1093/mnras/stae1822

  55. [55]

    Tidal Disruption Flares from Recoiling Supermassive Black Holes

    Tidal Disruption Flares from Recoiling Supermassive Black Holes. , keywords =. doi:10.1086/591420 , archivePrefix =. 0807.0223 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1086/591420

  56. [56]

    Interruption of Tidal Disruption Flares By Supermassive Black Hole Binaries

    Interruption of Tidal-Disruption Flares by Supermassive Black Hole Binaries. , keywords =. doi:10.1088/0004-637X/706/1/L133 , archivePrefix =. 0910.4152 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1088/0004-637x/706/1/l133

  57. [57]

    , keywords =

    Multiwavelength Follow-up of the Hyperluminous Intermediate-mass Black Hole Candidate 3XMM J215022.4-055108. , keywords =. doi:10.3847/2041-8213/ab745b , archivePrefix =. 2002.04618 , primaryClass =

    work page doi:10.3847/2041-8213/ab745b 2041

  58. [58]

    The Deep and Transient Universe in the SVOM Era: New Challenges and Opportunities - Scientific prospects of the SVOM mission

    The Deep and Transient Universe in the SVOM Era: New Challenges and Opportunities - Scientific prospects of the SVOM mission. arXiv e-prints , keywords =. doi:10.48550/arXiv.1610.06892 , archivePrefix =. 1610.06892 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.48550/arxiv.1610.06892

  59. [59]

    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 =

    work page doi:10.1007/s11433-024-2600-3

  60. [60]

    No apparent superluminal motion in the first-known jetted tidal disruption event Swift J1644+5734

    No apparent superluminal motion in the first-known jetted tidal disruption event Swift J1644+5734. , keywords =. doi:10.1093/mnrasl/slw107 , archivePrefix =. 1605.06461 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1093/mnrasl/slw107

  61. [61]

    Serbian Astronomical Journal , keywords =

    The Extremes of Continuum and Emission-Line Variability of AGN: Changing-Look Events and Binary SMBHS. Serbian Astronomical Journal , keywords =. doi:10.2298/SAJ2409001K , adsurl =

    work page doi:10.2298/saj2409001k

  62. [62]

    , 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 =

    work page doi:10.1038/s41586-022-05465-8

  63. [63]

    , keywords =

    Late-time Radio Brightening and Emergence of a Radio Jet in the Changing-look AGN 1ES 1927+654. , keywords =. doi:10.3847/2041-8213/ad8651 , archivePrefix =. 2406.18061 , primaryClass =

    work page doi:10.3847/2041-8213/ad8651 1927

  64. [64]

    , keywords =

    Radio emission from outflow-cloud interaction and its constraint on tidal disruption event outflow. , keywords =. doi:10.1093/mnras/stab3742 , archivePrefix =. 2108.11296 , primaryClass =

    work page doi:10.1093/mnras/stab3742

  65. [65]

    Tidal Disruption Events Prefer Unusual Host Galaxies

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

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.3847/2041-8205/818/1/l21 2041

  66. [66]

    A tidal disruption event in the nearby ultra-luminous infrared galaxy F01004-2237

    A tidal disruption event in the nearby ultra-luminous infrared galaxy F01004-2237. Nature Astronomy , keywords =. doi:10.1038/s41550-017-0061 , archivePrefix =. 1702.02573 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1038/s41550-017-0061

  67. [67]

    , keywords =

    Forward Modeling Populations of Flares from Tidal Disruptions of Stars by Supermassive Black Holes. , keywords =. doi:10.3847/1538-4357/abdf50 , archivePrefix =. 2008.11231 , primaryClass =

    work page doi:10.3847/1538-4357/abdf50 2008

  68. [68]

    Mid-infrared Outbursts in Nearby Galaxies (MIRONG). I. Sample Selection and Characterization. , keywords =. doi:10.3847/1538-4365/abd1dc , archivePrefix =. 2012.06806 , primaryClass =

    work page doi:10.3847/1538-4365/abd1dc 2012

  69. [69]

    , keywords =

    The Nascent Milliquasar VT J154843.06+220812.6: Tidal Disruption Event or Extreme Accretion State Change?. , keywords =. doi:10.3847/1538-4357/ac5e29 , archivePrefix =. 2108.12431 , primaryClass =

    work page doi:10.3847/1538-4357/ac5e29

  70. [70]

    , 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 =

    work page doi:10.3847/2041-8213/acf216 2041

  71. [71]

    , keywords =

    Outflow─Cloud Interaction as the Possible Origin of the Peculiar Radio Emission in the Tidal Disruption Event AT2018cqh. , keywords =. doi:10.3847/2041-8213/ae0caa , archivePrefix =. 2509.21299 , primaryClass =

    work page doi:10.3847/2041-8213/ae0caa 2041

  72. [72]

    , keywords =

    A New Population of Mid-infrared-selected Tidal Disruption Events: Implications for Tidal Disruption Event Rates and Host Galaxy Properties. , keywords =. doi:10.3847/1538-4357/ad18bb , archivePrefix =. 2401.01403 , primaryClass =

    work page doi:10.3847/1538-4357/ad18bb

  73. [73]

    , keywords =

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

    work page doi:10.1146/annurev-astro-111720-030029

  74. [74]

    , keywords =

    High-resolution VLBI Observations of and Modeling the Radio Emission from the Tidal Disruption Event AT2019dsg. , keywords =. doi:10.3847/1538-4357/ac4cb2 , archivePrefix =. 2106.15799 , primaryClass =

    work page doi:10.3847/1538-4357/ac4cb2

  75. [75]

    Constraining High-Energy Cosmic Neutrino Sources: Implications and Prospects

    Constraining high-energy cosmic neutrino sources: Implications and prospects. , keywords =. doi:10.1103/PhysRevD.94.103006 , archivePrefix =. 1607.01601 , primaryClass =

    work page internal anchor Pith review Pith/arXiv arXiv doi:10.1103/physrevd.94.103006

  76. [76]

    , keywords =

    Candidate Tidal Disruption Event AT2019fdr Coincident with a High-Energy Neutrino. , keywords =. doi:10.1103/PhysRevLett.128.221101 , archivePrefix =. 2111.09390 , primaryClass =

    work page doi:10.1103/physrevlett.128.221101