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Paper Citation Record · LEDGER

Directly Imaging the Cooling Flow in the Phoenix Cluster

As of 11 August 2026, this Paper Citation Record lists 71 of 71 outbound references and 0 inbound Pith citation observations for arXiv:2502.08619.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
2502.08619 v1

Coverage vector

measured 71 of 71 reference resolution

Typed states for the displayed outbound observations.

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measured 71 of 71 standing notices

One-hop event checks from named stored sources.

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measured 0 of 0 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: cited_works

Reference resolution

71 of 71 outbound references displayed

  • verified exact27
  • verified fuzzy1
  • unresolved37
  • parse uncertain0
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External citation measurements

No source-named external measurement is stored.

Outbound references

Observation 601c4fc1-aab7-4878-a774-b7aa4ccdfe10 · outbound

This paper cites an unresolved cited work.

Directly Imaging the Cooling Flow in the Phoenix Cluster Unresolved cited work

Reference 1

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Observation 2eaa3232-96a3-402a-a436-1ee9ad417bf0 · outbound

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Directly Imaging the Cooling Flow in the Phoenix Cluster Unresolved cited work

Reference 2

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Observation 17ad89dc-f9c6-47c0-b55c-253888deee25 · outbound

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Directly Imaging the Cooling Flow in the Phoenix Cluster Unresolved cited work

Reference 3

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Observation 7f82baf3-13a1-4104-aaf5-e95a8d077ab1 · outbound

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Directly Imaging the Cooling Flow in the Phoenix Cluster Unresolved cited work

Reference 4

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Observation c8282687-cfce-459a-b3f7-fa0b411d7933 · outbound

This paper cites Star Formation Rates in Cooling Flow Clusters: A UV Pilot Study with Archival XMM-Newton Optical Monitor Data.

Directly Imaging the Cooling Flow in the Phoenix Cluster Star Formation Rates in Cooling Flow Clusters: A UV Pilot Study with Archival XMM-Newton Optical Monitor Data

Reference 5

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Observation 35d0312a-9a51-44a1-8025-e6a9b755148d · outbound

This paper cites Revisiting the Cooling Flow Problem in Galaxies, Groups, and Clusters of Galaxies.

Directly Imaging the Cooling Flow in the Phoenix Cluster Revisiting the Cooling Flow Problem in Galaxies, Groups, and Clusters of Galaxies

Reference 6

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Observation f2f61f1f-a596-4efb-a680-0ef533f16d3c · outbound

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Directly Imaging the Cooling Flow in the Phoenix Cluster Unresolved cited work

Reference 7

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Observation 286380a6-a83d-45a8-be32-cef2c8d80360 · outbound

This paper cites A High Resolution Study of the Hydra A Cluster with Chandra: Comparison of the Core Mass Distribution with Theoretical Predictions and Evidence for Feedback in the Cooling Flow.

Directly Imaging the Cooling Flow in the Phoenix Cluster A High Resolution Study of the Hydra A Cluster with Chandra: Comparison of the Core Mass Distribution with Theoretical Predictions and Evidence for Feedback in the Cooling Flow

Reference 8

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Observation 80970b5d-5a4c-47c2-af87-e7533479d79f · outbound

This paper cites High Resolution X-ray Spectroscopic Constraints on Cooling-Flow Models for Clusters of Galaxies.

Directly Imaging the Cooling Flow in the Phoenix Cluster High Resolution X-ray Spectroscopic Constraints on Cooling-Flow Models for Clusters of Galaxies

Reference 9

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Observation f73588c0-9bc0-4b6a-933d-76b50463ce01 · outbound

This paper cites Heating Hot Atmospheres with Active Galactic Nuclei.

Directly Imaging the Cooling Flow in the Phoenix Cluster Heating Hot Atmospheres with Active Galactic Nuclei

Reference 10

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Observation d1ae64df-00f9-450c-a733-f679762f3933 · outbound

This paper cites Observational Evidence of AGN Feedback.

Directly Imaging the Cooling Flow in the Phoenix Cluster Observational Evidence of AGN Feedback

Reference 11

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Observation 7505b562-cafc-4c9b-8414-7985a1d2f98d · outbound

This paper cites X-ray cavities in a sample of 83 SPT-selected clusters of galaxies: Tracing the evolution of AGN feedback in clusters of galaxies out to z=1.2.

Directly Imaging the Cooling Flow in the Phoenix Cluster X-ray cavities in a sample of 83 SPT-selected clusters of galaxies: Tracing the evolution of AGN feedback in clusters of galaxies out to z=1.2

Reference 12

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Observation 024588fd-3f06-48f6-a501-9ede81afbbfc · outbound

This paper cites The Dance of Heating and Cooling in Galaxy Clusters: 3D Simulations of Self-Regulated AGN Outflows.

Directly Imaging the Cooling Flow in the Phoenix Cluster The Dance of Heating and Cooling in Galaxy Clusters: 3D Simulations of Self-Regulated AGN Outflows

Reference 13

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Observation 7e57c2ba-1b48-4e71-bb1d-dc590132a7c3 · outbound

This paper cites Cool core cycles: Cold gas and AGN jet feedback in cluster cores.

Directly Imaging the Cooling Flow in the Phoenix Cluster Cool core cycles: Cold gas and AGN jet feedback in cluster cores

Reference 14

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Observation eef3dc57-4433-49ee-a796-940655a19c5f · outbound

This paper cites AGN Heating in Simulated Cool-Core Clusters.

Directly Imaging the Cooling Flow in the Phoenix Cluster AGN Heating in Simulated Cool-Core Clusters

Reference 15

Resolution
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Observation 90d3b141-6771-457f-b6e0-edd3b6d6d1ac · outbound

This paper cites The Impact of Radio AGN Bubble Composition on the Dynamics and Thermal Balance of the Intracluster Medium.

Directly Imaging the Cooling Flow in the Phoenix Cluster The Impact of Radio AGN Bubble Composition on the Dynamics and Thermal Balance of the Intracluster Medium

Reference 16

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Observation d329545e-27d9-4f27-81f2-05c145f1bf8a · outbound

This paper cites A Massive, Cooling-Flow-Induced Starburst in the Core of a Highly Luminous Galaxy Cluster.

Directly Imaging the Cooling Flow in the Phoenix Cluster A Massive, Cooling-Flow-Induced Starburst in the Core of a Highly Luminous Galaxy Cluster

Reference 17

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Observation 21055553-0139-4eae-a069-af40f3d4d4c0 · outbound

This paper cites A Mechanism for Stimulating AGN Feedback by Lifting Gas in Massive Galaxies.

Directly Imaging the Cooling Flow in the Phoenix Cluster A Mechanism for Stimulating AGN Feedback by Lifting Gas in Massive Galaxies

Reference 18

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Observation ced2a1c1-d253-4265-8f72-4afe185e700f · outbound

This paper cites Formation of cold filaments in cooling flow clusters.

Directly Imaging the Cooling Flow in the Phoenix Cluster Formation of cold filaments in cooling flow clusters

Reference 19

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Observation 65b88c28-767e-4df4-aebe-3192b7939a20 · outbound

This paper cites Anatomy of a Cooling Flow: The Feedback Response to Pure Cooling in the Core of the Phoenix Cluster.

Directly Imaging the Cooling Flow in the Phoenix Cluster Anatomy of a Cooling Flow: The Feedback Response to Pure Cooling in the Core of the Phoenix Cluster

Reference 20

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Observation e460d1b7-794b-4344-ba70-982e8bef1a70 · outbound

This paper cites ALMA observations of massive molecular gas filaments encasing radio bubbles in the Phoenix cluster.

Directly Imaging the Cooling Flow in the Phoenix Cluster ALMA observations of massive molecular gas filaments encasing radio bubbles in the Phoenix cluster

Reference 21

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Observation 96461930-c037-4635-89ab-97db5a42a6b2 · outbound

This paper cites Shaken Snow Globes: Kinematic Tracers of the Multiphase Condensation Cascade in Massive Galaxies, Groups, and Clusters.

Directly Imaging the Cooling Flow in the Phoenix Cluster Shaken Snow Globes: Kinematic Tracers of the Multiphase Condensation Cascade in Massive Galaxies, Groups, and Clusters

Reference 22

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Observation fc361a7b-a8ad-4f8c-928e-3acda3ac1299 · outbound

This paper cites Deep Chandra, HST-COS, and Megacam Observations of the Phoenix Cluster: Extreme Star Formation and AGN Feedback on Hundred Kiloparsec Scales.

Directly Imaging the Cooling Flow in the Phoenix Cluster Deep Chandra, HST-COS, and Megacam Observations of the Phoenix Cluster: Extreme Star Formation and AGN Feedback on Hundred Kiloparsec Scales

Reference 23

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Observation da55fd6d-4abc-4db2-976c-af64adcb14ae · outbound

This paper cites AGN feedback in the Phoenix cluster.

Directly Imaging the Cooling Flow in the Phoenix Cluster AGN feedback in the Phoenix cluster

Reference 24

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local_arxiv, observed 2026-08-08T04:32:45.313541Z

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Observation 0f32af15-c219-4912-9252-a169172aef18 · outbound

This paper cites FUSE Observations of Cooling Flow Gas in the Galaxy Clusters A1795 and A2597.

Directly Imaging the Cooling Flow in the Phoenix Cluster FUSE Observations of Cooling Flow Gas in the Galaxy Clusters A1795 and A2597

Reference 25

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local_arxiv, observed 2026-08-08T04:32:45.294433Z

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Observation c852efe5-9c2b-4a93-98ad-88e4ac58dac4 · outbound

This paper cites OVI Observations of Galaxy Clusters: Evidence for Modest Cooling Flows.

Directly Imaging the Cooling Flow in the Phoenix Cluster OVI Observations of Galaxy Clusters: Evidence for Modest Cooling Flows

Reference 26

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Observation cc9c2013-1a38-4b4b-a67d-e40c715c574a · outbound

This paper cites Hidden Cooling Flows in Clusters of Galaxies.

Directly Imaging the Cooling Flow in the Phoenix Cluster Hidden Cooling Flows in Clusters of Galaxies

Reference 27

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local_arxiv, observed 2026-08-08T04:32:45.255333Z

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Observation b993cb48-f8b0-4389-bdd3-1f98b3518b33 · outbound

This paper cites Hundred Thousand Degree Gas in the Virgo Cluster of Galaxies.

Directly Imaging the Cooling Flow in the Phoenix Cluster Hundred Thousand Degree Gas in the Virgo Cluster of Galaxies

Reference 28

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local_arxiv, observed 2026-08-08T04:32:45.235563Z

Source-reported events for the cited work

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Observation fdea2b89-320b-4e5e-841f-1a291575c76e · outbound

This paper cites Searching for FUV line emission from $10^7$ K gas in massive elliptical galaxies and galaxy clusters as a tracer of turbulent velocities.

Directly Imaging the Cooling Flow in the Phoenix Cluster Searching for FUV line emission from $10^7$ K gas in massive elliptical galaxies and galaxy clusters as a tracer of turbulent velocities

Reference 29

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Observation 144743c3-d894-4896-a4c2-752b3b302e7e · outbound

This paper cites Detection of optical coronal emission from 10^6 K gas in the core of the Centaurus cluster.

Directly Imaging the Cooling Flow in the Phoenix Cluster Detection of optical coronal emission from 10^6 K gas in the core of the Centaurus cluster

Reference 30

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local_arxiv, observed 2026-08-08T04:32:45.195979Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

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Observation 1cce9c70-dc6c-4cea-85e5-1fd718d2c574 · outbound

This paper cites Implications of Coronal Line Emission in NGC 4696.

Directly Imaging the Cooling Flow in the Phoenix Cluster Implications of Coronal Line Emission in NGC 4696

Reference 31

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local_arxiv, observed 2026-08-08T04:32:45.176000Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-08-08T04:32:44.390702Z digest=sha256:7359c4e2fe9e1a575803aeb48de1bb3e7cba2f84535026d8e49260114cff53c1

Observation 08adf810-e660-4aa4-9532-4f35effb87db · outbound

This paper cites The State of the Warm and Cold Gas in the Extreme Starburst at the Core of the Phoenix Galaxy Cluster (SPT-CLJ2344-4243).

Directly Imaging the Cooling Flow in the Phoenix Cluster The State of the Warm and Cold Gas in the Extreme Starburst at the Core of the Phoenix Galaxy Cluster (SPT-CLJ2344-4243)

Reference 32

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local_arxiv, observed 2026-08-08T04:32:45.157077Z

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No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

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Observation 47583c1c-be68-4ce4-a383-da175ca54993 · outbound

This paper cites Mass transport by buoyant bubbles in galaxy clusters.

Directly Imaging the Cooling Flow in the Phoenix Cluster Mass transport by buoyant bubbles in galaxy clusters

Reference 33

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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

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Observation a32fa30b-7a8f-40dc-b50b-961644cb6ccc · outbound

This paper cites Cause and Effect of Feedback: Multiphase Gas in Cluster Cores Heated by AGN Jets.

Directly Imaging the Cooling Flow in the Phoenix Cluster Cause and Effect of Feedback: Multiphase Gas in Cluster Cores Heated by AGN Jets

Reference 34

Resolution
unresolved
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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 1dc1843e-a1c0-49b9-a1a0-abc748238880 · outbound

This paper cites Dissecting the turbulent weather driven by mechanical AGN feedback.

Directly Imaging the Cooling Flow in the Phoenix Cluster Dissecting the turbulent weather driven by mechanical AGN feedback

Reference 35

Resolution
metadata mismatch
local_arxiv, observed 2026-08-08T04:32:45.101171Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

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Observation 80dd3662-f002-4411-bcc4-b664ed5e3d4b · outbound

This paper cites an unresolved cited work.

Directly Imaging the Cooling Flow in the Phoenix Cluster Unresolved cited work

Reference 36

Resolution
unresolved
raw_fallback, observed 2026-08-08T04:32:45.737384Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-08-08T04:32:44.414999Z digest=sha256:5599eb90dec74db35672b0dd5c3cfc0bd13e6711ba5431dbca2ef770ed3e003d

Observation c31b0d76-ab74-4b70-87af-c247c83d7c50 · outbound

This paper cites The 2023 release of Cloudy.

Directly Imaging the Cooling Flow in the Phoenix Cluster The 2023 release of Cloudy

Reference 37

Resolution
unresolved
no resolver link, observed 2026-08-08T04:32:44.419725Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-08T04:32:44.419725Z digest=sha256:e9f28499f499348d5497ecac0c368611704e8fad20d34bf98eb0ec2bb0031295

Observation cf717f3e-90af-4be2-86c1-3f57d0783902 · outbound

This paper cites The WISSH quasars project XI. The mean Spectral Energy Distribution and Bolometric Corrections of the most luminous quasars.

Directly Imaging the Cooling Flow in the Phoenix Cluster The WISSH quasars project XI. The mean Spectral Energy Distribution and Bolometric Corrections of the most luminous quasars

Reference 38

Resolution
unresolved
no resolver link, observed 2026-08-08T04:32:44.424343Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-08T04:32:44.424343Z digest=sha256:b39ceb0cd2114705f34f7edc9b4322755ef3783ce7b28ff5becef667fd303af6

Observation bf8af708-1daa-47ef-ad4f-eadec8eca3ae · outbound

This paper cites H3+ in Diffuse Interstellar Clouds: a Tracer for the Cosmic-Ray Ionization Rate.

Directly Imaging the Cooling Flow in the Phoenix Cluster H3+ in Diffuse Interstellar Clouds: a Tracer for the Cosmic-Ray Ionization Rate

Reference 39

Resolution
metadata mismatch
local_arxiv, observed 2026-08-08T04:32:45.053395Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-08-08T04:32:44.428967Z digest=sha256:d38213a722dcb5228e98d4e3254ec8e285c1e5c6713189d7cb7c53cc0e84bd5f

Observation af949d99-817f-42c5-a633-1b570d37c8e8 · outbound

This paper cites Shaping the X-ray spectrum of galaxy clusters with AGN feedback and turbulence.

Directly Imaging the Cooling Flow in the Phoenix Cluster Shaping the X-ray spectrum of galaxy clusters with AGN feedback and turbulence

Reference 40

Resolution
verified exact
local_arxiv, observed 2026-08-08T04:32:45.032311Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-08-08T04:32:44.433561Z digest=sha256:b9bcc50cd606d1bea172139125535ac0451aa81bf27ccaeb5674f34adb91961f

Observation b67c1609-a21f-4477-9e69-0723b5fec253 · outbound

This paper cites A Unified Representation of Gas-Phase Element Depletions in the Interstellar Medium.

Directly Imaging the Cooling Flow in the Phoenix Cluster A Unified Representation of Gas-Phase Element Depletions in the Interstellar Medium

Reference 41

Resolution
unresolved
no resolver link, observed 2026-08-08T04:32:44.438255Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-08T04:32:44.438255Z digest=sha256:d5634439b9ad31a9a5c0a3668dc08d1a796773751b1e7ef0ef2772fecdcf4a8f

Observation 3e3cd039-7c18-4e0c-94a8-c5d7f0f2a4af · outbound

This paper cites Raining on black holes and massive galaxies: the top-down multiphase condensation model.

Directly Imaging the Cooling Flow in the Phoenix Cluster Raining on black holes and massive galaxies: the top-down multiphase condensation model

Reference 42

Resolution
unresolved
no resolver link, observed 2026-08-08T04:32:44.443169Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-08T04:32:44.443169Z digest=sha256:78d87ebc0fea92b8ccae139b744add343ae16f26bacec77ad7e8b89c2199dd90

Observation 65c79934-c07c-48c9-bc4d-ff09ad053fe1 · outbound

This paper cites Cool-Core Cycles and Phoenix.

Directly Imaging the Cooling Flow in the Phoenix Cluster Cool-Core Cycles and Phoenix

Reference 43

Resolution
verified exact
local_arxiv, observed 2026-08-08T04:32:44.982153Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-08-08T04:32:44.447736Z digest=sha256:403460cfc6e399f3fef56d6f420a90e3fe48367d3d83d1ed13ea2865c4d27c20

Observation 5e5611f6-0d3d-4165-94ab-43d1a4b8910f · outbound

This paper cites The relationship between the optical Halpha filaments and the X-ray emission in the core of the Perseus cluster.

Directly Imaging the Cooling Flow in the Phoenix Cluster The relationship between the optical Halpha filaments and the X-ray emission in the core of the Perseus cluster

Reference 44

Resolution
verified exact
local_arxiv, observed 2026-08-08T04:32:44.962052Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-08-08T04:32:44.452274Z digest=sha256:4b55d7cdd638389eb4683c01ba0e886969a45021bd7a37a210c3e92e008a2898

Observation 0c6562e8-b986-41e2-978f-ee9e152a2975 · outbound

This paper cites Revealing the velocity structure of the filamentary nebula in NGC 1275 in its entirety.

Directly Imaging the Cooling Flow in the Phoenix Cluster Revealing the velocity structure of the filamentary nebula in NGC 1275 in its entirety

Reference 45

Resolution
unresolved
no resolver link, observed 2026-08-08T04:32:44.456699Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-08T04:32:44.456699Z digest=sha256:bf7c6269d9e47b2b850111a8fae420fd83c3e211cc8d09e7a529b2b3e8b76409

Observation ddc774b5-15f5-487b-9dc0-13775175a430 · outbound

This paper cites Mechanical Feedback from Active Galactic Nuclei in Galaxies, Groups, and Clusters.

Directly Imaging the Cooling Flow in the Phoenix Cluster Mechanical Feedback from Active Galactic Nuclei in Galaxies, Groups, and Clusters

Reference 46

Resolution
unresolved
no resolver link, observed 2026-08-08T04:32:44.461500Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-08T04:32:44.461500Z digest=sha256:9fa544ae7ce42e4a6c901b237659bd912f413cbe4b4c1bbe44c9b635065626c2

Observation 962d8142-5016-4f43-a56d-4e1f2e30ac4f · outbound

This paper cites Hidden Cooling Flows in Clusters of Galaxies II: A Wider Sample.

Directly Imaging the Cooling Flow in the Phoenix Cluster Hidden Cooling Flows in Clusters of Galaxies II: A Wider Sample

Reference 47

Resolution
verified exact
local_arxiv, observed 2026-08-08T04:32:44.913872Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-08-08T04:32:44.466013Z digest=sha256:74584745a42c398841a57be027c2e7ba5f23cb601410b65cec9ef764b0da3349

Observation 23e1eed2-93b1-4d0b-a513-22b3c223f676 · outbound

This paper cites Spatial variations in aromatic hydrocarbon emission in a dust-rich galaxy.

Directly Imaging the Cooling Flow in the Phoenix Cluster Spatial variations in aromatic hydrocarbon emission in a dust-rich galaxy

Reference 48

Resolution
verified exact
local_arxiv, observed 2026-08-08T04:32:44.893747Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-08-08T04:32:44.470684Z digest=sha256:ba995cc5cb16c97b3684458896771b2d2f219eb23e5dd0645d29c22b755208f8

Observation 5e1560bd-40a5-4f21-ab38-5163327cd12d · outbound

This paper cites , author Edelman, A.

Directly Imaging the Cooling Flow in the Phoenix Cluster , author Edelman, A

Reference 49

Resolution
unresolved
no resolver link, observed 2026-08-08T04:32:44.475406Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-08T04:32:44.475406Z digest=sha256:a889e065ead35563441cd1d0a7e7cbe07c81ddb6c14623d03eeab1d27ec8e357

Observation 73c55e93-cd9f-47ba-a075-d84e65d27a03 · outbound

This paper cites The Mid-Infrared Spectrum of Star-Forming Galaxies: Global Properties of PAH Emission.

Directly Imaging the Cooling Flow in the Phoenix Cluster The Mid-Infrared Spectrum of Star-Forming Galaxies: Global Properties of PAH Emission

Reference 50

Resolution
unresolved
no resolver link, observed 2026-08-08T04:32:44.480103Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-08T04:32:44.480103Z digest=sha256:f73da09a18e37e8d75e1d42eda32d66dc10ba7a947732d7a47a7a8c5ea9af906

Observation 1165c6b2-9954-46a3-9e1e-351f188e0f20 · outbound

This paper cites an unresolved cited work.

Directly Imaging the Cooling Flow in the Phoenix Cluster Unresolved cited work

Reference 51

Resolution
unresolved
raw_fallback, observed 2026-08-08T04:32:45.721617Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-08-08T04:32:44.484611Z digest=sha256:7ec4eefff979622c9da6656a9e7389f04815dfa7ec549f7ba0352b5a15de619c

Observation 13708afa-1f34-4a0a-bf74-67f496da18b7 · outbound

This paper cites The Obscured Nucleus and Shocked Environment of VV 114E Revealed by JWST/MIRI Spectroscopy.

Directly Imaging the Cooling Flow in the Phoenix Cluster The Obscured Nucleus and Shocked Environment of VV 114E Revealed by JWST/MIRI Spectroscopy

Reference 52

Resolution
verified exact
local_arxiv, observed 2026-08-08T04:32:44.859059Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-08-08T04:32:44.488953Z digest=sha256:d0b4fe03b515c99b9697d8268539936b82236cdc7f2c4d4a8edc880475296951

Observation 9019e479-dbf0-440e-bc56-b77d09b0cb9f · outbound

This paper cites Wavelength Calibration and Resolving Power of the JWST MIRI Medium Resolution Spectrometer.

Directly Imaging the Cooling Flow in the Phoenix Cluster Wavelength Calibration and Resolving Power of the JWST MIRI Medium Resolution Spectrometer

Reference 53

Resolution
verified exact
local_arxiv, observed 2026-08-08T04:32:44.838544Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-08-08T04:32:44.493764Z digest=sha256:bf3158aa35af25dfdf4cb8cbaa14a18bdbfe2503b968bb02bb122446ab30c40c

Observation 859dc804-4eb6-436f-ba4e-b624669e5ee7 · outbound

This paper cites A systematic study of silicate absorption features in heavily obscured AGNs observed by Spitzer/IRS.

Directly Imaging the Cooling Flow in the Phoenix Cluster A systematic study of silicate absorption features in heavily obscured AGNs observed by Spitzer/IRS

Reference 54

Resolution
verified exact
local_arxiv, observed 2026-08-08T04:32:44.817152Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-08-08T04:32:44.498551Z digest=sha256:ca3497be0a2e57cf9e0026d0b612e345bcf5943f532714178b51203195ae8f10

Observation 69c517e9-d1d2-4bea-b3d9-6721bd40c4bb · outbound

This paper cites Spitzer Quasar and ULIRG Evolution Study (QUEST). IV. Comparison of 1-Jy Ultraluminous Infrared Galaxies with Palomar-Green Quasars.

Directly Imaging the Cooling Flow in the Phoenix Cluster Spitzer Quasar and ULIRG Evolution Study (QUEST). IV. Comparison of 1-Jy Ultraluminous Infrared Galaxies with Palomar-Green Quasars

Reference 55

Resolution
unresolved
no resolver link, observed 2026-08-08T04:32:44.503176Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-08T04:32:44.503176Z digest=sha256:d3f2e941412d516d5c5a5b51fe661a7fd86cad8c94b214bea460249dbbc61c60

Observation b2015d6d-06c1-4011-99da-176b700ba24a · outbound

This paper cites Non-linear Least Squares Fitting in IDL with MPFIT.

Directly Imaging the Cooling Flow in the Phoenix Cluster Non-linear Least Squares Fitting in IDL with MPFIT

Reference 56

Resolution
unresolved
no resolver link, observed 2026-08-08T04:32:44.507779Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-08T04:32:44.507779Z digest=sha256:7a308a19c6f4a8b8fba5f1e0dbaff731f464d1976328bc21a3ad8133dae1409a

Observation a7df365e-6651-43d6-83a8-a1d8fad14d8b · outbound

This paper cites an unresolved cited work.

Directly Imaging the Cooling Flow in the Phoenix Cluster Unresolved cited work

Reference 57

Resolution
unresolved
raw_fallback, observed 2026-08-08T04:32:45.707257Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-08-08T04:32:44.512307Z digest=sha256:a7c849bda704c5eff6f2ec0f8850aae002ae72092cc718039bf28e4269f2064c

Observation 92cef9a5-cf39-4c1f-99fe-7098ddf2238a · outbound

This paper cites CHIANTI -- an atomic database for emission lines -- Paper XVI: Version 10, further extensions.

Directly Imaging the Cooling Flow in the Phoenix Cluster CHIANTI -- an atomic database for emission lines -- Paper XVI: Version 10, further extensions

Reference 58

Resolution
unresolved
no resolver link, observed 2026-08-08T04:32:44.516817Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-08T04:32:44.516817Z digest=sha256:c1af5d6c489511f68f27248684ff8734ce35c5b8b331f7d0dae14d8c76ee4a24

Observation 96a22121-bc1a-4da9-a198-8cde0d56f09f · outbound

This paper cites The Structure of Multiphase Galactic Winds.

Directly Imaging the Cooling Flow in the Phoenix Cluster The Structure of Multiphase Galactic Winds

Reference 59

Resolution
unresolved
no resolver link, observed 2026-08-08T04:32:44.521272Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-08T04:32:44.521272Z digest=sha256:584be26570b2431530a8bf0740602205b9c9fde7c111793b12add4a2e12eeeba

Observation 6aa21f2c-00fc-409f-84ce-1ab2d08d325a · outbound

This paper cites Investigating the Narrow Line Region Dynamics in Nearby Active Galaxies.

Directly Imaging the Cooling Flow in the Phoenix Cluster Investigating the Narrow Line Region Dynamics in Nearby Active Galaxies

Reference 60

Resolution
verified exact
local_arxiv, observed 2026-08-08T04:32:44.736585Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-08-08T04:32:44.525835Z digest=sha256:fe7d1371187516559263ef6174b0fcb76580adb63d05a76c5645fc0af34bc427

Observation 97430d5f-da23-45f4-b88e-24b4f83db9af · outbound

This paper cites Linking Macro, Meso, and Micro Scales in Multiphase AGN Feeding and Feedback.

Directly Imaging the Cooling Flow in the Phoenix Cluster Linking Macro, Meso, and Micro Scales in Multiphase AGN Feeding and Feedback

Reference 61

Resolution
metadata mismatch
local_arxiv, observed 2026-08-08T04:32:44.714962Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-08-08T04:32:44.530487Z digest=sha256:48735d9d46080236ff0ea3124b741763f5a52f30cab3ddad80230c526aa234f2

Observation 583847a8-9ebd-4477-a9fc-bcd65090dd56 · outbound

This paper cites Dusty, Radiation Pressure Dominated Photoionization. II. Multi-Wavelength Emission Line Diagnostics for Narrow Line Regions.

Directly Imaging the Cooling Flow in the Phoenix Cluster Dusty, Radiation Pressure Dominated Photoionization. II. Multi-Wavelength Emission Line Diagnostics for Narrow Line Regions

Reference 62

Resolution
unresolved
no resolver link, observed 2026-08-08T04:32:44.535034Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-08T04:32:44.535034Z digest=sha256:25de69b1c48727b4145c5f3df3f001c05c57d16ad9226e7b87da8b92f23e45f6

Observation 12524a63-ac9f-4bf0-91b2-eddd06b1e940 · outbound

This paper cites The MAPPINGS III Library of Fast Radiative Shock Models.

Directly Imaging the Cooling Flow in the Phoenix Cluster The MAPPINGS III Library of Fast Radiative Shock Models

Reference 63

Resolution
unresolved
no resolver link, observed 2026-08-08T04:32:44.539652Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-08T04:32:44.539652Z digest=sha256:52cd6e6002a83bfa99707aa576ebf2dc8f646494c2837b0f952db8317bbc77e9

Observation 2b5d4ea8-3550-4bc9-9b8c-f7d20bb059ba · outbound

This paper cites Theoretical Modeling of Starburst Galaxies.

Directly Imaging the Cooling Flow in the Phoenix Cluster Theoretical Modeling of Starburst Galaxies

Reference 64

Resolution
unresolved
no resolver link, observed 2026-08-08T04:32:44.544204Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-08T04:32:44.544204Z digest=sha256:684894b42ee2fa032afae20e2dbcb217a66d69051b107ed8e9a2b5640f2779d5

Observation 7c6eb1dc-bafb-49a5-9b68-56327a957aa0 · outbound

This paper cites Very Large Array observations of the mini-halo and AGN feedback in the Phoenix cluster.

Directly Imaging the Cooling Flow in the Phoenix Cluster Very Large Array observations of the mini-halo and AGN feedback in the Phoenix cluster

Reference 65

Resolution
verified exact
local_arxiv, observed 2026-08-08T04:32:44.653384Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-08-08T04:32:44.548557Z digest=sha256:4916090d348d34706f57d47198043d1186ab019b092553106a4690884534058d

Observation 504a0a2b-8f32-4cf8-804d-67f5228cbca0 · outbound

This paper cites an unresolved cited work.

Directly Imaging the Cooling Flow in the Phoenix Cluster Unresolved cited work

Reference 66

Resolution
unresolved
raw_fallback, observed 2026-08-08T04:32:45.692957Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-08-08T04:32:44.553740Z digest=sha256:b26a22b73297bd783daca73b5bccdee8d39c2e09e280b7333c87210a3b6758e9

Observation 8e874dbe-c80b-4a8b-9236-73a10c7f12ad · outbound

This paper cites an unresolved cited work.

Directly Imaging the Cooling Flow in the Phoenix Cluster Unresolved cited work

Reference 67

Resolution
unresolved
raw_fallback, observed 2026-08-08T04:32:45.678464Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-08-08T04:32:44.558228Z digest=sha256:0d45a0323016e6dc48786772f25f4f5ae314511d858cbd9f8e5dfb5f239180ab

Observation 560a9c28-99d8-4c99-aecb-849d9ca154cb · outbound

This paper cites Numerical Study of Turbulent Mixing Layers with Non-Equilibrium Ionization Calculations.

Directly Imaging the Cooling Flow in the Phoenix Cluster Numerical Study of Turbulent Mixing Layers with Non-Equilibrium Ionization Calculations

Reference 68

Resolution
metadata mismatch
local_arxiv, observed 2026-08-08T04:32:44.632217Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-08-08T04:32:44.562764Z digest=sha256:a3fbad7869ccd5c4646ce9c88efb2948e708759d7781fa9069fcf11f6803dc4a

Observation 878b58e7-e8fd-44d3-a7d8-b966681299c4 · outbound

This paper cites title Solar System Abundances and Condensation Temperatures of the Elements.

Directly Imaging the Cooling Flow in the Phoenix Cluster title Solar System Abundances and Condensation Temperatures of the Elements

Reference 69

Resolution
verified fuzzy
raw_fallback, observed 2026-08-08T04:32:45.663910Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-08-08T04:32:44.567496Z digest=sha256:77459f301651adbc4222e1fda2e0886b481dc5c070bd61aea54aec7dee375795

Observation db4518b8-f026-44f3-911e-d9813e876a13 · outbound

This paper cites , " * write output.state after.block = add.period write newline.

Directly Imaging the Cooling Flow in the Phoenix Cluster , " * write output.state after.block = add.period write newline

Reference 70

Resolution
unresolved
no resolver link, observed 2026-08-08T04:32:44.571632Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-08T04:32:44.571632Z digest=sha256:540288d42d66bc2dc1cbf4c8eac7fb65988cf787c8800104da551f1c1eecfb89

Observation 54258ca3-c7b0-44b5-bf0b-a92ffabeda53 · outbound

This paper cites write newline.

Directly Imaging the Cooling Flow in the Phoenix Cluster write newline

Reference 71

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unresolved
no resolver link, observed 2026-08-08T04:32:44.576903Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-08T04:32:44.576903Z digest=sha256:c966aee107b05387e0e989f8867e34a33588125890a4f546c51e6056b7086f91

Pith citing papers

No inbound Pith citation observations are available.