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Paper Citation Record · LEDGER

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters

As of 5 August 2026, this Paper Citation Record lists 100 of 300 outbound references and 0 inbound Pith citation observations for arXiv:2606.23790.

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

pith.paper-citation-record.v1
2606.23790 v1

Coverage vector

measured 100 of 300 reference resolution

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Pith citing papers itemized under the disclosed page cap.

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measured 0 of 1 external citation measurements

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Source: cited_works

Reference resolution

100 of 300 outbound references displayed

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External citation measurements

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Outbound references

Observation 6f1ec3a1-c81a-4dc7-b8ee-63bd8ed2360e · outbound

This paper cites T., Done C., Smith D.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters T., Done C., Smith D

Reference 1

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Observation 0b108b1d-dea6-40ca-99e2-79e8a029e6cf · outbound

This paper cites The Second Data Release of the Sloan Digital Sky Survey.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters The Second Data Release of the Sloan Digital Sky Survey

Reference 2

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Observation d58e1d28-01d0-459f-89f4-dac3189aeba5 · outbound

This paper cites Evolution of spatially resolved star formation main sequence and surface density profiles in massive disc galaxies at $0\lesssim z \lesssim 1$: inside-out stellar mass buildup and quenching.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters Evolution of spatially resolved star formation main sequence and surface density profiles in massive disc galaxies at $0\lesssim z \lesssim 1$: inside-out stellar mass buildup and quenching

Reference 3

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Observation dd10ee1b-3a4b-426f-8f13-dbf3f8152e62 · outbound

This paper cites The Hyper Suprime-Cam SSP Survey: Overview and Survey Design.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters The Hyper Suprime-Cam SSP Survey: Overview and Survey Design

Reference 4

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Observation 69dcae83-e4cd-4925-ac1d-96e5a9de0650 · outbound

This paper cites First Data Release of the Hyper Suprime-Cam Subaru Strategic Program.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters First Data Release of the Hyper Suprime-Cam Subaru Strategic Program

Reference 5

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Observation 7b99c525-5dd7-4fcb-b2f8-cfe4d908685a · outbound

This paper cites 2019, Publ.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters 2019, Publ

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This paper cites 2022, Publ.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters 2022, Publ

Reference 7

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Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters , journal=

Reference 8

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Observation 6783c3e0-ad9f-499d-9b0c-43835d09238f · outbound

This paper cites 2020, MNRAS, 497, 581, doi: 10.1093/mnras/staa1956.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters 2020, MNRAS, 497, 581, doi: 10.1093/mnras/staa1956

Reference 9

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Observation d261aa23-c1bf-4d95-b109-d27251a57b63 · outbound

This paper cites Alberts, A.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters Alberts, A

Reference 10

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Observation bea157b2-05b8-444e-8d01-9282e39cda41 · outbound

This paper cites Star formation sustained by gas accretion.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters Star formation sustained by gas accretion

Reference 11

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Observation 4d19881a-0a68-4b1c-9e9f-43f458efa09f · outbound

This paper cites A., & Cuevas, H.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters A., & Cuevas, H

Reference 12

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This paper cites LARgE Survey. I. Dead Monsters: the Massive End of the Passive Galaxy Stellar Mass Function at Cosmic Noon.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters LARgE Survey. I. Dead Monsters: the Massive End of the Passive Galaxy Stellar Mass Function at Cosmic Noon

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Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters , keywords =

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Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters , keywords =

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Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters , keywords =

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Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters and LeBlanc , F

Reference 17

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Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters keywords =

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Observation 00edad0f-89d4-439e-84ab-d904b5bd6a9a · outbound

This paper cites Quantifying the bimodal color-magnitude distribution of galaxies.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters Quantifying the bimodal color-magnitude distribution of galaxies

Reference 19

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Observation 7ccef2cc-ec5d-4be5-a468-e3c2a9bd35fb · outbound

This paper cites The GEEC2 spectroscopic survey of Galaxy Groups at $0.8<z<1$.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters The GEEC2 spectroscopic survey of Galaxy Groups at $0.8<z<1$

Reference 20

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Observation 49bc4a19-6078-4cf2-bc99-8ecd6c35e219 · outbound

This paper cites Evidence for a change in the dominant satellite galaxy quenching mechanism at z=1.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters Evidence for a change in the dominant satellite galaxy quenching mechanism at z=1

Reference 21

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Observation 2bd6d9c0-4855-436e-9e77-e675ecd75f81 · outbound

This paper cites L., van der Burg, R.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters L., van der Burg, R

Reference 22

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Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters T., Ogilvie G

Reference 23

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Observation 70be17a7-142e-4964-b9e8-210c505b855b · outbound

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Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters The Average Star Formation Histories of Galaxies in Dark Matter Halos from z=0-8

Reference 24

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Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters The luminosities, sizes and velocity dispersions of Brightest Cluster Galaxies: Implications for formation history

Reference 25

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Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters M., Coil, A

Reference 26

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Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters 1996, A&AS, 117, 393, doi: 10.1051/aas:1996164

Reference 27

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This paper cites Clustering, host halos and environment of z$\sim$2 galaxies as a function of their physical properties.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters Clustering, host halos and environment of z$\sim$2 galaxies as a function of their physical properties

Reference 28

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Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters On the occurrence of galaxy harassment

Reference 29

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This paper cites Advanced Camera for Surveys Photometry of the Cluster RDCS1252.9-2927: The Color-Magnitude Relation at z=1.24.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters Advanced Camera for Surveys Photometry of the Cluster RDCS1252.9-2927: The Color-Magnitude Relation at z=1.24

Reference 30

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Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters Astronomical Data Analysis Software and Systems XXVII , year = 2019, editor =

Reference 31

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Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters The Hyper Suprime-Cam Software Pipeline

Reference 32

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Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters Environmental Effects on Late-Type Galaxies in Nearby Clusters

Reference 33

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This paper cites The GALEX Ultraviolet Virgo Cluster Survey (GUViCS). IV: The role of the cluster environment on galaxy evolution.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters The GALEX Ultraviolet Virgo Cluster Survey (GUViCS). IV: The role of the cluster environment on galaxy evolution

Reference 34

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Observation a05a45d0-15c6-4d2d-baa2-fedd3730943f · outbound

This paper cites keywords =.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters keywords =

Reference 35

Resolution
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Observation 379d9f6e-632e-4dbb-9b09-461aa16d697e · outbound

This paper cites keywords =.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters keywords =

Reference 36

Resolution
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Observation 3ce9d0ff-4e9f-4b7c-8bd2-daaf8a10693e · outbound

This paper cites A., De Marco O., Barlow M.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters A., De Marco O., Barlow M

Reference 37

Resolution
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arxiv_id, observed 2026-06-26T07:59:08.503247Z

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Observation 4fb673a5-cc57-4501-8cde-6a38f25dc19a · outbound

This paper cites EAZY: A Fast, Public Photometric Redshift Code.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters EAZY: A Fast, Public Photometric Redshift Code

Reference 38

Resolution
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Observation 88b4240c-3bbb-4f93-adbf-fa7a3b131495 · outbound

This paper cites doi:10.5281/zenodo.8370018 , version =.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters doi:10.5281/zenodo.8370018 , version =

Reference 39

Resolution
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Observation 0e4c2227-046c-4b43-93c3-d2d9cf41dea8 · outbound

This paper cites 2025 , month = may, version =.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters 2025 , month = may, version =

Reference 40

Resolution
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Observation 40a448fc-9fc1-4cb8-ba79-7f53380d8897 · outbound

This paper cites The Era of Star Formation in Galaxy Clusters.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters The Era of Star Formation in Galaxy Clusters

Reference 41

Resolution
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Observation fff6effc-9cce-4877-a759-3032d91cffa6 · outbound

This paper cites 2022, A&A, 661, A1, doi: 10.1051/0004-6361/202141266.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters 2022, A&A, 661, A1, doi: 10.1051/0004-6361/202141266

Reference 42

Resolution
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Source-reported events for the cited work

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Observation 60be4fcf-e135-4c96-bf06-1a93f259a418 · outbound

This paper cites Jiang, F.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters Jiang, F

Reference 43

Resolution
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arxiv_id, observed 2026-06-26T07:59:08.496962Z

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Observation 32446582-2743-4500-af72-0d320aa80270 · outbound

This paper cites The Dust Content and Opacity of Actively Star-Forming Galaxies.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters The Dust Content and Opacity of Actively Star-Forming Galaxies

Reference 44

Resolution
verified exact
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Source-reported events for the cited work

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Observation 03ee7430-3d07-4e27-b9d5-21b597089e71 · outbound

This paper cites V - A study of populations since Z approximately equal to 0.5.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters V - A study of populations since Z approximately equal to 0.5

Reference 45

Resolution
verified exact
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Source-reported events for the cited work

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Observation da15f38b-c3f4-4ef8-9d05-f88565016312 · outbound

This paper cites Astronomy and Computing , keywords =.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters Astronomy and Computing , keywords =

Reference 46

Resolution
verified exact
arxiv_id, observed 2026-06-26T07:59:08.908055Z

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Observation b3cb1e42-ce3e-418a-b31f-78d6d437f7e0 · outbound

This paper cites Galactic Stellar and Substellar Initial Mass Function.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters Galactic Stellar and Substellar Initial Mass Function

Reference 47

Resolution
verified exact
local_arxiv, observed 2026-06-26T07:59:08.525151Z

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Observation 3a0cc82d-b723-4b41-9c70-adcd02479c2e · outbound

This paper cites 2020, ApJ, 890, 7, doi: 10.3847/1538-4357/ab61fd.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters 2020, ApJ, 890, 7, doi: 10.3847/1538-4357/ab61fd

Reference 48

Resolution
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Observation 05751434-7f86-41fd-95fc-e5978b5f822f · outbound

This paper cites The dark matter haloes and the progenitors and descendants of ultramassive passive galaxies at cosmic noon.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters The dark matter haloes and the progenitors and descendants of ultramassive passive galaxies at cosmic noon

Reference 49

Resolution
verified exact
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Observation 0f03e0bb-196a-4525-92d0-715f9b8b806e · outbound

This paper cites Ancient Light from Young Cosmic Cities: Physical and Observational Signatures of Galaxy Proto-Clusters.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters Ancient Light from Young Cosmic Cities: Physical and Observational Signatures of Galaxy Proto-Clusters

Reference 50

Resolution
verified exact
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Observation 42f096cd-8756-4400-b062-2d41df37a30f · outbound

This paper cites Discovery of a large number of candidate proto-clusters traced by ~15 Mpc-scale galaxy overdensities in COSMOS.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters Discovery of a large number of candidate proto-clusters traced by ~15 Mpc-scale galaxy overdensities in COSMOS

Reference 51

Resolution
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Observation 73a8208c-5187-491f-9309-37c9b57fb803 · outbound

This paper cites Surveying Galaxy Proto-clusters in Emission: A Large-scale Structure at z=2.44 and the Outlook for HETDEX.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters Surveying Galaxy Proto-clusters in Emission: A Large-scale Structure at z=2.44 and the Outlook for HETDEX

Reference 52

Resolution
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Observation c45f93c2-b61f-48ba-adac-a2299b333bf9 · outbound

This paper cites Galaxy Protoclusters as Drivers of Cosmic Star-Formation History in the First 2 Gyr.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters Galaxy Protoclusters as Drivers of Cosmic Star-Formation History in the First 2 Gyr

Reference 53

Resolution
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Observation 2039bb7a-1a06-450c-a7c7-c43fd50cecc9 · outbound

This paper cites A direct empirical proof of the existence of dark matter.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters A direct empirical proof of the existence of dark matter

Reference 54

Resolution
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Observation 520563b7-3323-4f9e-a8a3-d6f692923d0d · outbound

This paper cites The 0.1<z<1.65 evolution of the bright end of the [OII] luminosity function.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters The 0.1<z<1.65 evolution of the bright end of the [OII] luminosity function

Reference 55

Resolution
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Observation 1ee10beb-eb6a-4960-9a7e-0fa8e3ad3b37 · outbound

This paper cites On the formation and physical properties of the Intra-Cluster Light in hierarchical galaxy formation models.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters On the formation and physical properties of the Intra-Cluster Light in hierarchical galaxy formation models

Reference 56

Resolution
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Observation a92c8cdc-fb63-4f74-9461-0b8ce59fa19d · outbound

This paper cites Semi-Analytic Model Predictions of the Galaxy Population in Proto-clusters.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters Semi-Analytic Model Predictions of the Galaxy Population in Proto-clusters

Reference 57

Resolution
verified exact
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Observation 54782422-d989-4160-9813-433df447b412 · outbound

This paper cites an unresolved cited work.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters Unresolved cited work

Reference 58

Resolution
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Source-reported events for the cited work

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Observation d8391542-9fdf-4927-8cc3-4232003d5dab · outbound

This paper cites A z=2.5 protocluster associated with the radio galaxy MRC 2104-242: star formation and differing mass functions in dense environments.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters A z=2.5 protocluster associated with the radio galaxy MRC 2104-242: star formation and differing mass functions in dense environments

Reference 59

Resolution
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Source-reported events for the cited work

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Observation 7635c988-ba72-4659-bf3f-16756d7cefe5 · outbound

This paper cites A mature galaxy cluster at z=1.58 around the radio galaxy 7C1753+6311.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters A mature galaxy cluster at z=1.58 around the radio galaxy 7C1753+6311

Reference 60

Resolution
verified exact
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Observation cadfdbce-5dc4-4288-9937-75053dbd270c · outbound

This paper cites , keywords =.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters , keywords =

Reference 61

Resolution
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Observation 776de6b7-2b3e-4669-9b6d-e9d15c7534e3 · outbound

This paper cites Mignone and Jonathan C.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters Mignone and Jonathan C

Reference 62

Resolution
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Observation accfbe66-df39-413a-81cd-c44f6da4f456 · outbound

This paper cites The Environment of Galaxies at Low Redshift.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters The Environment of Galaxies at Low Redshift

Reference 63

Resolution
verified exact
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Source-reported events for the cited work

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Observation 2487392d-ff5b-4324-ba17-112e26d6d82a · outbound

This paper cites T., Done C., Smith D.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters T., Done C., Smith D

Reference 64

Resolution
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arxiv_id, observed 2026-06-26T07:59:08.550001Z

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Observation 00c1112f-c942-48c5-b829-bee875f22cf7 · outbound

This paper cites From Voids to Coma: the prevalence of pre-processing in the local Universe.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters From Voids to Coma: the prevalence of pre-processing in the local Universe

Reference 65

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verified exact
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Source-reported events for the cited work

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source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:96002c63bfce5ac158c6cacf2dda63f05b401ddbf5a7fe27dd9adcb4f7a82cfa

Observation 65d80ee2-3b3d-4824-982d-ba0d5f8d8c4e · outbound

This paper cites A Comparative Study of Density Field Estimation for Galaxies: New Insights into the Evolution of Galaxies with Environment in COSMOS out to z~3.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters A Comparative Study of Density Field Estimation for Galaxies: New Insights into the Evolution of Galaxies with Environment in COSMOS out to z~3

Reference 66

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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:fef34f5c1307cbacf42b6f1feec7b3a780712b39c819013742ea8deb4acd98ad

Observation fb98d303-1f16-4f52-844d-72bd23e26b05 · outbound

This paper cites Effects of Local Environment and Stellar Mass on Galaxy Quenching out to z~3.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters Effects of Local Environment and Stellar Mass on Galaxy Quenching out to z~3

Reference 67

Resolution
verified exact
local_arxiv, observed 2026-06-26T07:59:08.894207Z

Source-reported events for the cited work

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Observation 8a931b27-2ef1-4462-ba6f-d3bc1593aa07 · outbound

This paper cites The VIMOS Public Extragalactic Redshift Survey (VIPERS). A precise measurement of the galaxy stellar mass function and the abundance of massive galaxies at redshifts 0.5<z<1.3.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters The VIMOS Public Extragalactic Redshift Survey (VIPERS). A precise measurement of the galaxy stellar mass function and the abundance of massive galaxies at redshifts 0.5<z<1.3

Reference 68

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Observation b0b4b8f3-1ed6-44b9-b601-7384aa3dc7df · outbound

This paper cites The COSMOS2015 galaxy stellar mass function: 13 billion years of stellar mass assembly in 10 snapshots.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters The COSMOS2015 galaxy stellar mass function: 13 billion years of stellar mass assembly in 10 snapshots

Reference 69

Resolution
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Observation 3557e1d1-8e8b-497a-a6d9-58c2646277c2 · outbound

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Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters keywords =

Reference 70

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Observation 4bb0bb66-f841-4f60-89a0-b764955a74de · outbound

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Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters keywords =

Reference 71

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Source-reported events for the cited work

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Observation 580f2a21-45cb-43f9-a65e-5bf233196ace · outbound

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Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters arXiv e-prints , keywords =

Reference 72

Resolution
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Observation bb3e4d12-a360-4d58-958c-fa62cf111b73 · outbound

This paper cites and Yang , J.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters and Yang , J

Reference 73

Resolution
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arxiv_id, observed 2026-06-26T07:59:08.904175Z

Source-reported events for the cited work

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Observation 8b171590-141f-4002-8f94-3a28154673b4 · outbound

This paper cites Mignone and Jonathan C.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters Mignone and Jonathan C

Reference 74

Resolution
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arxiv_id, observed 2026-06-26T07:59:08.569833Z

Source-reported events for the cited work

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Observation e34575e7-a9d8-4540-befd-dc6cb8ed00bb · outbound

This paper cites An analytic solution for the minimal bathtub toy model: challenges in the star-formation history of high-z galaxies.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters An analytic solution for the minimal bathtub toy model: challenges in the star-formation history of high-z galaxies

Reference 75

Resolution
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Source-reported events for the cited work

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Observation 8637c649-19b5-4707-b386-9c587f12c7ac · outbound

This paper cites A., okas E.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters A., okas E

Reference 76

Resolution
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arxiv_id, observed 2026-06-26T07:59:08.564922Z

Source-reported events for the cited work

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Observation 1c7e34fd-5d2c-4d90-a0cd-b7a1e21c5be2 · outbound

This paper cites and Yang , J.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters and Yang , J

Reference 77

Resolution
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arxiv_id, observed 2026-06-26T07:59:08.439769Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

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Observation 33be578b-19d2-435d-a451-82f0127774cb · outbound

This paper cites and Shibahashi , H.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters and Shibahashi , H

Reference 78

Resolution
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arxiv_id, observed 2026-06-26T07:59:08.868082Z

Source-reported events for the cited work

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Observation 487fba03-25e5-4dbe-b66c-583fe25a72ed · outbound

This paper cites The VLA-COSMOS 3~GHz Large Project: AGN and host-galaxy properties out to z$\lesssim$6.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters The VLA-COSMOS 3~GHz Large Project: AGN and host-galaxy properties out to z$\lesssim$6

Reference 79

Resolution
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

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Observation d014de19-55ee-4eae-90ac-9c5e5fc7768f · outbound

This paper cites COLOSSUS: A python toolkit for cosmology, large-scale structure, and dark matter halos.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters COLOSSUS: A python toolkit for cosmology, large-scale structure, and dark matter halos

Reference 80

Resolution
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Observation a60adc00-eb0b-4ece-a51f-945eb63db684 · outbound

This paper cites Proto-groups at 1.8<z<3 in the zCOSMOS-deep sample.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters Proto-groups at 1.8<z<3 in the zCOSMOS-deep sample

Reference 81

Resolution
verified exact
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Source-reported events for the cited work

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Observation b46f73ca-e558-4b19-ae17-3bb7a97fd76f · outbound

This paper cites A proto-cluster at z=2.45.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters A proto-cluster at z=2.45

Reference 82

Resolution
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Source-reported events for the cited work

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Observation 50eb9fc0-4f35-43ab-98d0-b6fb2ffc52d3 · outbound

This paper cites Galaxy shapes of Light (GaLight): a 2D modeling of galaxy images.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters Galaxy shapes of Light (GaLight): a 2D modeling of galaxy images

Reference 83

Resolution
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Source-reported events for the cited work

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Observation efb0ce79-cd4b-4264-be32-b48ccf2a371d · outbound

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Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters keywords =

Reference 84

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Observation d8b01efe-18ed-4923-b5e6-fb876d6863e9 · outbound

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Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters keywords =

Reference 85

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Observation c04afedc-7c36-436e-97e9-de6f56c09477 · outbound

This paper cites P., Norberg, P., Baldry, I.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters P., Norberg, P., Baldry, I

Reference 86

Resolution
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arxiv_id, observed 2026-06-26T07:59:08.853540Z

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Observation d0881ef4-9cc3-49f1-8abb-ec7e406ddc55 · outbound

This paper cites Jellyfish: Evidence of extreme ram-pressure stripping in massive galaxy clusters.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters Jellyfish: Evidence of extreme ram-pressure stripping in massive galaxy clusters

Reference 87

Resolution
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Observation 02e23b80-37df-4b81-91a3-e0c719889ceb · outbound

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Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters , year = 1990, month = jul, volume =

Reference 88

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Observation 7d20c8ab-5a11-4f52-862f-e51f7dab038b · outbound

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Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters and Shibahashi , H

Reference 89

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Observation 9afeed5f-65bb-4cab-803b-36836132b696 · outbound

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Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters , keywords =

Reference 90

Resolution
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Source-reported events for the cited work

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Observation 56c23b49-cae6-4f3d-8889-b800fc5c0056 · outbound

This paper cites Baryonic Features in the Matter Transfer Function.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters Baryonic Features in the Matter Transfer Function

Reference 91

Resolution
verified exact
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Observation a43ca6b9-4514-4a72-9e2e-1763a851b563 · outbound

This paper cites Power Spectra for Cold Dark Matter and its Variants.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters Power Spectra for Cold Dark Matter and its Variants

Reference 92

Resolution
verified exact
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Observation 49c1bc2d-f18c-4395-b6dd-7fc6d66744fd · outbound

This paper cites The reversal of the star formation-density relation in the distant universe.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters The reversal of the star formation-density relation in the distant universe

Reference 93

Resolution
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Observation 292a65e3-2ced-4f9c-a8ba-3f3f641980aa · outbound

This paper cites Observational Evidence of AGN Feedback.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters Observational Evidence of AGN Feedback

Reference 94

Resolution
verified exact
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Source-reported events for the cited work

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Observation 10329295-c9c3-4e8c-870c-2dbbc7fd6325 · outbound

This paper cites Halpha-Derived Star-Formation Rates For Three z ~ 0.75 EDisCS Galaxy Clusters.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters Halpha-Derived Star-Formation Rates For Three z ~ 0.75 EDisCS Galaxy Clusters

Reference 95

Resolution
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Observation d638ea3a-2934-47f6-9f09-7e6bc02fdfa6 · outbound

This paper cites Galaxy environment in the 3D-HST fields. Witnessing the onset of satellite quenching at z ~ 1-2.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters Galaxy environment in the 3D-HST fields. Witnessing the onset of satellite quenching at z ~ 1-2

Reference 96

Resolution
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Source-reported events for the cited work

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Observation e4c87682-819d-481c-8f7c-24049669c8d3 · outbound

This paper cites Pre-Processing of Galaxies before Entering a Cluster.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters Pre-Processing of Galaxies before Entering a Cluster

Reference 97

Resolution
verified exact
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Source-reported events for the cited work

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Observation 7795e278-ae33-499c-b11d-8b332722171a · outbound

This paper cites R., Smartt, S.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters R., Smartt, S

Reference 98

Resolution
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Source-reported events for the cited work

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Observation abd7c2c6-3a48-420c-8927-40412ed852a0 · outbound

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Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters keywords =

Reference 99

Resolution
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Observation c6e7b8a4-497c-4c4f-a48a-d24a7f876e91 · outbound

This paper cites The Mass Profile of the Coma Galaxy Cluster.

Anisotropic quenching beyond $z=1$ and its implications for preprocessing around high-redshift galaxy clusters The Mass Profile of the Coma Galaxy Cluster

Reference 100

Resolution
verified exact
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

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Pith citing papers

No inbound Pith citation observations are available.