Pith. sign in

Paper Citation Record · LEDGER

The effects of different cooling and heating function models on a simulated analog of NGC300

As of 14 August 2026, this Paper Citation Record lists 35 of 35 outbound references and 0 inbound Pith citation observations for arXiv:2412.15324.

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

pith.paper-citation-record.v1
2412.15324 v1

Coverage vector

measured 35 of 35 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-11T11:37:18.638687Z

measured 35 of 35 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-14T06:32:32.682623+00:00

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

35 of 35 outbound references displayed

  • verified exact9
  • verified fuzzy1
  • unresolved23
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch2

External citation measurements

No source-named external measurement is stored.

Outbound references

Observation a3f5cb2b-ad2e-4740-8df6-3da51373265b · outbound

This paper cites Spitzer , Lyman ,\ 10.1086/146200 journal journal \ volume 124 ,\ pages 20 ( year 1956 ) NoStop.

The effects of different cooling and heating function models on a simulated analog of NGC300 Spitzer , Lyman ,\ 10.1086/146200 journal journal \ volume 124 ,\ pages 20 ( year 1956 ) NoStop

Reference 1

Resolution
unresolved
no resolver link, observed 2026-08-11T11:37:18.450194Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-11T11:37:18.450194Z digest=sha256:d87b90e63bc41b794148d821016ab3f771504dbcc56336e022b2f88c3f86cb50

Observation 960ee357-b897-4714-bc5a-a9af99e6c84b · outbound

This paper cites an unresolved cited work.

The effects of different cooling and heating function models on a simulated analog of NGC300 Unresolved cited work

Reference 2

Resolution
unresolved
no resolver link, observed 2026-08-11T11:37:18.456209Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-11T11:37:18.456209Z digest=sha256:d608af95880cc333de51ce4e06fa7f6ea619c49ed6bce0e5994e9a439060599d

Observation f6ae93aa-f31f-4bb8-8ef8-e7455e0ef158 · outbound

This paper cites an unresolved cited work.

The effects of different cooling and heating function models on a simulated analog of NGC300 Unresolved cited work

Reference 3

Resolution
unresolved
raw_fallback, observed 2026-08-11T11:37:19.630364Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-08-11T11:37:18.462278Z digest=sha256:c1db9d3d8e464e0fd4144070ac7ed2def2a23b9a93f100fe630b8c264b1c30a8

Observation a428f400-d473-46aa-a669-27a66ed7d901 · outbound

This paper cites an unresolved cited work.

The effects of different cooling and heating function models on a simulated analog of NGC300 Unresolved cited work

Reference 4

Resolution
unresolved
no resolver link, observed 2026-08-11T11:37:18.467676Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-11T11:37:18.467676Z digest=sha256:5a3c43e5fab4474b84af535c374a10676b5170bf003a397a2dfa7f8eb6408422

Observation de67faf7-7e65-4a2a-91cb-efaa91ca31f6 · outbound

This paper cites an unresolved cited work.

The effects of different cooling and heating function models on a simulated analog of NGC300 Unresolved cited work

Reference 5

Resolution
unresolved
no resolver link, observed 2026-08-11T11:37:18.472875Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-11T11:37:18.472875Z digest=sha256:af3a914bc5c8d871fb8ddce0d0f55719c9a2e1bb3556917964d8cbc88a666d56

Observation 48985e98-e7af-45ed-bcc8-490f67c76481 · outbound

This paper cites an unresolved cited work.

The effects of different cooling and heating function models on a simulated analog of NGC300 Unresolved cited work

Reference 6

Resolution
metadata mismatch
raw_fallback, observed 2026-08-11T11:37:19.561409Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-08-11T11:37:18.480687Z digest=sha256:502d10db72d91352265bdb32a79d86cecda4cabe4cd7fe828719ae375e2a7278

Observation 2052a2a0-b821-4efa-a87d-58dcf64338d6 · outbound

This paper cites The Physical Origin of the Stellar Initial Mass Function.

The effects of different cooling and heating function models on a simulated analog of NGC300 The Physical Origin of the Stellar Initial Mass Function

Reference 7

Resolution
unresolved
no resolver link, observed 2026-08-11T11:37:18.486705Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-11T11:37:18.486705Z digest=sha256:4834c2befd2da2a83666e2f332dec62ac42ed3fd7a1ad95f5718866942b9e87b

Observation ec1dc597-8553-416f-bee2-194676526a69 · outbound

This paper cites Photochemistry and Heating/Cooling of the Multiphase Interstellar Medium with UV Radiative Transfer for Magnetohydrodynamic Simulations.

The effects of different cooling and heating function models on a simulated analog of NGC300 Photochemistry and Heating/Cooling of the Multiphase Interstellar Medium with UV Radiative Transfer for Magnetohydrodynamic Simulations

Reference 8

Resolution
verified exact
local_arxiv, observed 2026-08-11T11:37:19.474930Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-08-11T11:37:18.492393Z digest=sha256:f582e70e03839c737a22af837555d7174ad959a0232c3207a375d39f23ed4088

Observation dddd8f4b-0593-4b2f-8641-8fc2e4f4e148 · outbound

This paper cites Scannapieco , author M.

The effects of different cooling and heating function models on a simulated analog of NGC300 Scannapieco , author M

Reference 9

Resolution
unresolved
no resolver link, observed 2026-08-11T11:37:18.497838Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-11T11:37:18.497838Z digest=sha256:d5aa4ae6b42a5df461f5139e06c6bf82d5783f842527e316cca6b35a50d9c741

Observation 1e0aae4d-f55d-4718-b33d-9a6c2fbff1fd · outbound

This paper cites \ Kim , author T.

The effects of different cooling and heating function models on a simulated analog of NGC300 \ Kim , author T

Reference 10

Resolution
verified exact
raw_fallback, observed 2026-08-11T11:37:19.369630Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-08-11T11:37:18.503089Z digest=sha256:c4fa2e700798fa766111e5c697c4a40a01b7fcc5cc9b48f1db147fdc80cd4104

Observation eea40c16-d824-4c1e-9a40-8ad74be07ff4 · outbound

This paper cites A semi-analytic model comparison: testing cooling models against hydrodynamical simulations.

The effects of different cooling and heating function models on a simulated analog of NGC300 A semi-analytic model comparison: testing cooling models against hydrodynamical simulations

Reference 11

Resolution
verified exact
local_arxiv, observed 2026-08-11T11:37:19.283630Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-08-11T11:37:18.509334Z digest=sha256:e2318b6dc9bbf6899e48e8900c7d210b80898457e38cd969e6e51b9ddfcaeb67

Observation 19e1d94f-8533-4d65-860f-78e8b28e388c · outbound

This paper cites A new gas cooling model for semi-analytical galaxy formation models.

The effects of different cooling and heating function models on a simulated analog of NGC300 A new gas cooling model for semi-analytical galaxy formation models

Reference 12

Resolution
unresolved
no resolver link, observed 2026-08-11T11:37:18.515677Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-11T11:37:18.515677Z digest=sha256:b8e46549b923e4f5d43960c893ad1614a3f5127f2596b041eefa449eedd332a9

Observation b79822b8-b4b2-4756-a5ff-0ef728f2643e · outbound

This paper cites A comparison between semi-analytical gas cooling models and cosmological hydrodynamical simulations.

The effects of different cooling and heating function models on a simulated analog of NGC300 A comparison between semi-analytical gas cooling models and cosmological hydrodynamical simulations

Reference 13

Resolution
unresolved
no resolver link, observed 2026-08-11T11:37:18.521098Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-11T11:37:18.521098Z digest=sha256:0e6469c041c4070a3265392902a29a54d9d68f3eccb21ed72e5bac114b8f7d90

Observation dd4f8a67-89ce-4842-a03d-6eb8e9e63013 · outbound

This paper cites The effects of metallicity, UV radiation and non-equilibrium chemistry in high-resolution simulations of galaxies.

The effects of different cooling and heating function models on a simulated analog of NGC300 The effects of metallicity, UV radiation and non-equilibrium chemistry in high-resolution simulations of galaxies

Reference 14

Resolution
verified exact
local_arxiv, observed 2026-08-11T11:37:19.219862Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-08-11T11:37:18.526847Z digest=sha256:9015a4b9c014dd7fe9b85d27c10cafa0a57a853335f7777298e18f9d3ea7d8d1

Observation e58f9983-61e0-4d2b-987d-d56baee45af1 · outbound

This paper cites The effect of non-equilibrium metal cooling on the interstellar medium.

The effects of different cooling and heating function models on a simulated analog of NGC300 The effect of non-equilibrium metal cooling on the interstellar medium

Reference 15

Resolution
unresolved
no resolver link, observed 2026-08-11T11:37:18.531909Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-11T11:37:18.531909Z digest=sha256:18de9f24f859c809d4481b8fbace39c1d278efc011c5fbab6467fc174cd3a28a

Observation 30c35c7e-7cac-4482-96f7-85ea8ee96c07 · outbound

This paper cites Spatial Decorrelation of Young Stars and Dense Gas as a Probe of the Star Formation-Feedback Cycle in Galaxies.

The effects of different cooling and heating function models on a simulated analog of NGC300 Spatial Decorrelation of Young Stars and Dense Gas as a Probe of the Star Formation-Feedback Cycle in Galaxies

Reference 16

Resolution
verified exact
local_arxiv, observed 2026-08-11T11:37:19.174601Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-08-11T11:37:18.537053Z digest=sha256:101f1c4406eff9182a7eef74940d9938de8ee35da0ead8d84337bc878251161f

Observation 0d03510f-75fa-4b00-9c68-15d3f078a732 · outbound

This paper cites Cooling and Heating Functions of Photoionized Gas.

The effects of different cooling and heating function models on a simulated analog of NGC300 Cooling and Heating Functions of Photoionized Gas

Reference 17

Resolution
unresolved
no resolver link, observed 2026-08-11T11:37:18.542139Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-11T11:37:18.542139Z digest=sha256:6f8c7e62d564541fc559050e15b4d23ec73f7db389d4e864c6b91815f696f890

Observation b174cb91-5d7b-445e-82fd-fae7fe2074ff · outbound

This paper cites Exploring the Dependence of Gas Cooling and Heating Functions on the Incident Radiation Field with Machine Learning.

The effects of different cooling and heating function models on a simulated analog of NGC300 Exploring the Dependence of Gas Cooling and Heating Functions on the Incident Radiation Field with Machine Learning

Reference 18

Resolution
verified exact
local_arxiv, observed 2026-08-11T11:37:19.132495Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-08-11T11:37:18.547169Z digest=sha256:a46eb0c6181b15c093f20035e11ccb61c40f729446d4404a3e31b5c92a508c42

Observation f154dcf5-3604-48a6-a4e4-a97ac5ac86f9 · outbound

This paper cites Ionized Carbon in Galaxies: The [C II] 158 $\mu$m Line as a Total Molecular Gas Mass Tracer Revisited.

The effects of different cooling and heating function models on a simulated analog of NGC300 Ionized Carbon in Galaxies: The [C II] 158 $\mu$m Line as a Total Molecular Gas Mass Tracer Revisited

Reference 19

Resolution
verified exact
local_arxiv, observed 2026-08-11T11:37:18.782141Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-08-11T11:37:18.553485Z digest=sha256:dd1c9c250f4d73e7bcb2e709e4b84c394ab3ab31b22f63dfaab10a69e8f7b237

Observation 3f05a655-7a89-4981-afdb-84e3338daf7a · outbound

This paper cites Atomic and molecular gas as traced by [C II] emission.

The effects of different cooling and heating function models on a simulated analog of NGC300 Atomic and molecular gas as traced by [C II] emission

Reference 20

Resolution
metadata mismatch
local_arxiv, observed 2026-08-11T11:37:18.754459Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-08-11T11:37:18.558346Z digest=sha256:a96faa7866040d99c8336116a6f170b4383d470c07f28fc68d7c075cb210734a

Observation a5d916b6-9a8a-44fa-86d6-b8432d8a77ea · outbound

This paper cites Line-Intensity Mapping: 2017 Status Report.

The effects of different cooling and heating function models on a simulated analog of NGC300 Line-Intensity Mapping: 2017 Status Report

Reference 21

Resolution
unresolved
no resolver link, observed 2026-08-11T11:37:18.562959Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-11T11:37:18.562959Z digest=sha256:66a1ef7a6f31a1409bcc2111653220637664b262b2ef9de3fb1dea8c9c0f1391

Observation 7a4aa7e2-0648-489c-bd6a-33823d27b7af · outbound

This paper cites an unresolved cited work.

The effects of different cooling and heating function models on a simulated analog of NGC300 Unresolved cited work

Reference 22

Resolution
unresolved
raw_fallback, observed 2026-08-11T11:37:19.612730Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-08-11T11:37:18.568167Z digest=sha256:4002b8b044d4bf565cfce0248a909e26c89f39742757b2c0443c12900e631e8a

Observation 0b57b71f-57fb-4af7-bb40-00fd8d6dc443 · outbound

This paper cites Constrained Simulations of the Real Universe: II. Observational Signatures of Intergalactic Gas in the Local Supercluster Region.

The effects of different cooling and heating function models on a simulated analog of NGC300 Constrained Simulations of the Real Universe: II. Observational Signatures of Intergalactic Gas in the Local Supercluster Region

Reference 23

Resolution
verified exact
local_arxiv, observed 2026-08-11T11:37:19.106332Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-08-11T11:37:18.572927Z digest=sha256:c6aa4df57938da3b321c921d4a6a02d9496b36469cf749665b2a2616b950d390

Observation 66a6f75d-b087-47dd-bfbe-23adf79063da · outbound

This paper cites Effects of Baryons and Dissipation on the Matter Power Spectrum.

The effects of different cooling and heating function models on a simulated analog of NGC300 Effects of Baryons and Dissipation on the Matter Power Spectrum

Reference 24

Resolution
unresolved
no resolver link, observed 2026-08-11T11:37:18.578129Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-11T11:37:18.578129Z digest=sha256:cbb4c1f5095d76b16a71d61aff42513fcf07d5d7c7b4a5eeab45998d5e74c5fd

Observation f787a32d-34dd-4a48-9daa-820120654689 · outbound

This paper cites A Simple Law of Star Formation.

The effects of different cooling and heating function models on a simulated analog of NGC300 A Simple Law of Star Formation

Reference 25

Resolution
unresolved
no resolver link, observed 2026-08-11T11:37:18.583654Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-11T11:37:18.583654Z digest=sha256:c0f4d53e4450d29965996084567b95039ce0b3c954c215d277c78db477798b62

Observation 0125f96d-9610-426c-b636-aaab946badf7 · outbound

This paper cites Non-universal star formation efficiency in turbulent ISM.

The effects of different cooling and heating function models on a simulated analog of NGC300 Non-universal star formation efficiency in turbulent ISM

Reference 26

Resolution
unresolved
no resolver link, observed 2026-08-11T11:37:18.588956Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-11T11:37:18.588956Z digest=sha256:8d993a9782828dd80de16803e1080a9ba9a5430f08368a3033faff2e06c48066

Observation e76f0d93-ede6-4fef-a747-9e976815fdcc · outbound

This paper cites an unresolved cited work.

The effects of different cooling and heating function models on a simulated analog of NGC300 Unresolved cited work

Reference 27

Resolution
unresolved
no resolver link, observed 2026-08-11T11:37:18.594507Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-11T11:37:18.594507Z digest=sha256:56b9a68373460ea94ec469608b8715413d776ac45a74898c9621b6d29ea50c81

Observation 0fd0b760-31f1-4eb3-a7a0-a3c4f666c0ee · outbound

This paper cites Environmental Dependence of the Kennicutt-Schmidt Relation in Galaxies.

The effects of different cooling and heating function models on a simulated analog of NGC300 Environmental Dependence of the Kennicutt-Schmidt Relation in Galaxies

Reference 28

Resolution
unresolved
no resolver link, observed 2026-08-11T11:37:18.599635Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-11T11:37:18.599635Z digest=sha256:429f3ee04d97f336ee8e13e3bda031631cf730779773cdfe50f5cc3a1c2e97b2

Observation 3cd9091f-0ec3-4006-9db3-edeba05a6539 · outbound

This paper cites Westmeier , author R.

The effects of different cooling and heating function models on a simulated analog of NGC300 Westmeier , author R

Reference 29

Resolution
unresolved
no resolver link, observed 2026-08-11T11:37:18.604868Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-11T11:37:18.604868Z digest=sha256:d45571159002f06ec38fa05d64b7a8d1ec411bfc3bf750e6adc3919f13f56e7b

Observation b761880b-9493-482a-83d0-da34743bdedf · outbound

This paper cites Chen \ and\ author C.

The effects of different cooling and heating function models on a simulated analog of NGC300 Chen \ and\ author C

Reference 30

Resolution
verified fuzzy
raw_fallback, observed 2026-08-11T11:37:19.595400Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-08-11T11:37:18.609627Z digest=sha256:f87534745f491a516facafa72f194eade5d49f75ba306ce08a2ceedcedab6c0d

Observation d430739e-7f4c-42c9-85d9-1d2f9f66413e · outbound

This paper cites an unresolved cited work.

The effects of different cooling and heating function models on a simulated analog of NGC300 Unresolved cited work

Reference 31

Resolution
unresolved
raw_fallback, observed 2026-08-11T11:37:19.577954Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-08-11T11:37:18.614395Z digest=sha256:37b91a2569f03fb02967866a6f359cf9f82a5c1c335e3e0ea751fb55e54cd77a

Observation 528c38ee-cec7-4895-a964-19428c58b262 · outbound

This paper cites Barinovs , author M.

The effects of different cooling and heating function models on a simulated analog of NGC300 Barinovs , author M

Reference 32

Resolution
unresolved
no resolver link, observed 2026-08-11T11:37:18.619338Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-11T11:37:18.619338Z digest=sha256:9f4c4f1ad39711b43478a251af19414da04b804035deec4f1cff5e1924cef827

Observation c58e933d-a0ab-43b1-a833-cb77f88b4c11 · outbound

This paper cites an unresolved cited work.

The effects of different cooling and heating function models on a simulated analog of NGC300 Unresolved cited work

Reference 33

Resolution
verified exact
doi, observed 2026-08-11T11:37:18.682688Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-08-11T11:37:18.626836Z digest=sha256:9334e33c9836c635e1e7a70a2373a00d075dd5fade0058f7bfab912861892076

Observation f99e5d81-891c-43f3-8289-e730ccbf1fb4 · outbound

This paper cites A Multi-Code Analysis Toolkit for Astrophysical Simulation Data.

The effects of different cooling and heating function models on a simulated analog of NGC300 A Multi-Code Analysis Toolkit for Astrophysical Simulation Data

Reference 34

Resolution
unresolved
no resolver link, observed 2026-08-11T11:37:18.632361Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-11T11:37:18.632361Z digest=sha256:e84fc607ee35306675022b2d617a5b8bdc7143b632429e01b1724225777b4d20

Observation 5a2faa9e-9247-4dfb-902e-5fb4178e847b · outbound

This paper cites Array Programming with NumPy.

The effects of different cooling and heating function models on a simulated analog of NGC300 Array Programming with NumPy

Reference 35

Resolution
unresolved
no resolver link, observed 2026-08-11T11:37:18.638687Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-11T11:37:18.638687Z digest=sha256:7e8015ef7da5799fff3ffffcd2c945463e5c6f443adc261a8edd3ac0bd91cd6d

Pith citing papers

No inbound Pith citation observations are available.