Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster | Paper Citation Record

Observation ff6fc1d0-feae-4aba-85e6-666953148ee1 · outbound

This paper cites Physical conditions of the molecular gas in metal-poor galaxies.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster Physical conditions of the molecular gas in metal-poor galaxies

Reference 1

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Observation 2a8ef883-19a6-48f8-aa2f-72476afe322d · outbound

This paper cites , keywords =.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster , keywords =

Reference 2

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Observation 536680e5-7bb7-4eb7-89e7-8d1b64ccc3c6 · outbound

This paper cites A large H{\alpha} survey at z=2.23, 1.47, 0.84 & 0.40: the 11 Gyr evolution of star-forming galaxies from HiZELS.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster A large H{\alpha} survey at z=2.23, 1.47, 0.84 & 0.40: the 11 Gyr evolution of star-forming galaxies from HiZELS

Reference 3

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Observation 5b666222-7774-4a68-8574-cfd585822324 · outbound

This paper cites Dust evolution in zoom-in cosmological simulations of galaxy formation.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster Dust evolution in zoom-in cosmological simulations of galaxy formation

Reference 4

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Observation 711f2dea-44ae-4efc-9e04-3491351bb7d6 · outbound

This paper cites HELP: The Herschel Extragalactic Legacy Project.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster HELP: The Herschel Extragalactic Legacy Project

Reference 5

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Observation 9cf0d0fc-c427-4d62-9c32-18de0e221387 · outbound

This paper cites Galaxy And Mass Assembly (GAMA): Data Release 4 and the z < 0.1 total and z < 0.08 morphological galaxy stellar mass functions.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster Galaxy And Mass Assembly (GAMA): Data Release 4 and the z < 0.1 total and z < 0.08 morphological galaxy stellar mass functions

Reference 6

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Observation 89a24fc2-c84e-48f6-8393-930154cc4860 · outbound

This paper cites The Messenger , keywords =.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster The Messenger , keywords =

Reference 7

Resolution: verified exact; doi, observed 2026-07-14T05:50:16.663675Z

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Observation 193af8e8-82a1-494c-86f2-5bd01ea62f86 · outbound

This paper cites A dusty proto-cluster surrounding the binary galaxy HerBS-70 at $z = 2.3$.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster A dusty proto-cluster surrounding the binary galaxy HerBS-70 at $z = 2.3$

Reference 8

Resolution: verified exact; local_arxiv, observed 2026-07-14T05:40:16.545409Z

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Observation 0b275e5e-3546-401b-b1e5-8661871635e6 · outbound

This paper cites Galactic Stellar and Substellar Initial Mass Function.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster Galactic Stellar and Substellar Initial Mass Function

Reference 9

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Observation 0877a96c-c130-419c-b480-9ae87096edae · outbound

This paper cites , keywords =.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster , keywords =

Reference 10

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Observation 83692667-7b3a-4f05-b7bc-440e96c268e4 · outbound

This paper cites Bright submillimeter galaxies do trace galaxy protoclusters.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster Bright submillimeter galaxies do trace galaxy protoclusters

Reference 11

Resolution: verified exact; local_arxiv, observed 2026-07-14T05:50:16.714694Z

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Observation 3083cb53-93d2-4d29-b233-521fd2b864b2 · outbound

This paper cites z-GAL -- A NOEMA spectroscopic redshift survey of bright Herschel galaxies: [I] Overview.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster z-GAL -- A NOEMA spectroscopic redshift survey of bright Herschel galaxies: [I] Overview

Reference 12

Resolution: verified exact; local_arxiv, observed 2026-07-14T05:40:16.152272Z

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Observation 86d019f6-d752-4c02-8cfb-1bef16db82fe · outbound

This paper cites A Giant Disk Galaxy Two Billion Years After The Big Bang.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster A Giant Disk Galaxy Two Billion Years After The Big Bang

Reference 13

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Observation 42e73346-e08b-4bdc-b69c-53e8f7614825 · outbound

This paper cites The quiescent population at $0.5\le z \le 0.9$: Environmental impact on the mass-size relation.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster The quiescent population at $0.5\le z \le 0.9$: Environmental impact on the mass-size relation

Reference 14

Resolution: verified exact; local_arxiv, observed 2026-07-14T05:40:16.173244Z

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Observation 32e9aab4-59ef-4366-bbaf-7a21c573790c · outbound

This paper cites Euclid Quick Data Release (Q1). Exploring galaxy morphology across cosmic time through Sersic fits.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster Euclid Quick Data Release (Q1). Exploring galaxy morphology across cosmic time through Sersic fits

Reference 15

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Observation 612307cf-a4ab-41b0-a503-95172f194c2b · outbound

This paper cites The evolution of the SFR and Sigma-SFR of galaxies in cosmic morning (4 < z < 10).

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster The evolution of the SFR and Sigma-SFR of galaxies in cosmic morning (4 < z < 10)

Reference 16

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Observation 01aca63f-b1d8-4388-9194-6d569767cc44 · outbound

This paper cites Evolution of the star formation rate surface density main sequence. Insights from a semi-analytic simulation since $z = 12$.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster Evolution of the star formation rate surface density main sequence. Insights from a semi-analytic simulation since $z = 12$

Reference 17

Resolution: verified exact; local_arxiv, observed 2026-07-14T05:40:16.481089Z

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Observation 3155969a-a005-4f68-8165-a940781d74bf · outbound

This paper cites $\Sigma_{\mathrm{SFR}}$-M* Diagram: A Valuable Galaxy Evolution Diagnostic to Complement (s)SFR-M* Diagrams.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster $\Sigma_{\mathrm{SFR}}$-M* Diagram: A Valuable Galaxy Evolution Diagnostic to Complement (s)SFR-M* Diagrams

Reference 18

Resolution: verified exact; local_arxiv, observed 2026-07-14T05:40:16.509780Z

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Observation 8cf04f78-d218-4453-99ec-0ee978843a97 · outbound

This paper cites The 700 ks Chandra Spiderweb Field I: evidence for widespread nuclear activity in the Protocluster.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster The 700 ks Chandra Spiderweb Field I: evidence for widespread nuclear activity in the Protocluster

Reference 19

Resolution: verified exact; local_arxiv, observed 2026-07-14T05:40:16.628618Z

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Observation a6526a28-a360-450e-b54c-d058d7f8d75b · outbound

This paper cites A morphological study of galaxies in ZwCl0024+1652, a galaxy cluster at redshift z $\sim$ 0.4.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster A morphological study of galaxies in ZwCl0024+1652, a galaxy cluster at redshift z $\sim$ 0.4

Reference 20

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Observation f008ac38-d919-4db2-9898-b9241b3acac0 · outbound

This paper cites JWST+ALMA reveal the ISM kinematics and stellar structure of MAMBO-9, a merging pair of DSFGs in an overdense environment at $z=5.85$.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster JWST+ALMA reveal the ISM kinematics and stellar structure of MAMBO-9, a merging pair of DSFGs in an overdense environment at $z=5.85$

Reference 21

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Observation f386950f-a472-4a83-92ff-8d4784e6672a · outbound

This paper cites COALAS III: The ATCA CO(1-0) look at the growth and death of H$\alpha$ emitters in the Spiderweb protocluster at z=2.16.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster COALAS III: The ATCA CO(1-0) look at the growth and death of H$\alpha$ emitters in the Spiderweb protocluster at z=2.16

Reference 22

Resolution: verified exact; local_arxiv, observed 2026-07-14T05:40:16.640236Z

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Observation 655f3090-d679-4373-8a16-413b0f60d496 · outbound

This paper cites Early results from GLASS-JWST. XIV: A spectroscopically confirmed protocluster 650 million years after the Big Bang.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster Early results from GLASS-JWST. XIV: A spectroscopically confirmed protocluster 650 million years after the Big Bang

Reference 23

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Observation dbb6ab5a-0fbd-49dd-87d1-cdff950164c2 · outbound

This paper cites Planck 2018 results. VI. Cosmological parameters.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster Planck 2018 results. VI. Cosmological parameters

Reference 24

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Observation 0368c65c-1ebd-4da9-8c26-c2bc551b3e98 · outbound

This paper cites an unresolved cited work.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster Unresolved cited work

Reference 25

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Observation 6c9e13a0-ef30-4974-8012-a6910914bf65 · outbound

This paper cites arXiv e-prints , keywords =.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster arXiv e-prints , keywords =

Reference 26

Resolution: verified exact; arxiv_id, observed 2026-07-14T05:40:17.158349Z

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Observation b08fdd7f-d0d2-4da7-8040-5a0cd0d4e7e3 · outbound

This paper cites arXiv e-prints , keywords =.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster arXiv e-prints , keywords =

Reference 28

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Observation d748728e-fff1-4b4d-8fbf-f2729a749397 · outbound

This paper cites What are Protoclusters? -- Defining High Redshift Galaxy Clusters and Protoclusters.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster What are Protoclusters? -- Defining High Redshift Galaxy Clusters and Protoclusters

Reference 29

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Observation 80bda089-233f-40be-8553-968a2cf3828c · outbound

This paper cites An excess of dusty starbursts related to the Spiderweb galaxy.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster An excess of dusty starbursts related to the Spiderweb galaxy

Reference 30

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Observation 32f9abc6-25a5-4878-90fe-9335d6f3a72f · outbound

This paper cites The Herschel Bright Sources (HerBS): Sample definition and SCUBA-2 observations.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster The Herschel Bright Sources (HerBS): Sample definition and SCUBA-2 observations

Reference 31

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Observation 9884488d-d126-4748-975d-fc73dab4f67a · outbound

This paper cites The Bright Extragalactic ALMA Redshift Survey (BEARS) I: redshifts of bright gravitationally-lensed galaxies from the Herschel ATLAS.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster The Bright Extragalactic ALMA Redshift Survey (BEARS) I: redshifts of bright gravitationally-lensed galaxies from the Herschel ATLAS

Reference 32

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Observation f0d317ab-8b62-4792-a291-16c539ff7dda · outbound

This paper cites , keywords =.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster , keywords =

Reference 33

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Observation 866e9263-cc0a-4f0e-a214-012dcab2795d · outbound

This paper cites Herschel-ATLAS: deep HST/WFC3 imaging of strongly lensed submillimeter galaxies.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster Herschel-ATLAS: deep HST/WFC3 imaging of strongly lensed submillimeter galaxies

Reference 34

Resolution: verified exact; local_arxiv, observed 2026-07-14T05:40:16.111025Z

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Observation dfe629ce-57e6-49f3-853b-bc3af011dc6d · outbound

This paper cites Observation of H2O in a strongly lensed Herschel-ATLAS source at z=2.3.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster Observation of H2O in a strongly lensed Herschel-ATLAS source at z=2.3

Reference 35

Resolution: verified exact; local_arxiv, observed 2026-07-14T05:40:17.173225Z

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Observation 55b4b31c-78e1-4f6d-ba96-94c6bc120508 · outbound

This paper cites GBT Zpectrometer CO(1-0) Observations of the Strongly-Lensed Submillimeter Galaxies from the Herschel ATLAS.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster GBT Zpectrometer CO(1-0) Observations of the Strongly-Lensed Submillimeter Galaxies from the Herschel ATLAS

Reference 36

Resolution: verified exact; local_arxiv, observed 2026-07-14T05:40:17.178022Z

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Observation da91e9c0-2a29-46ff-b7f3-6d5edf75655b · outbound

This paper cites Dust evolution with MUPPI in cosmological volumes.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster Dust evolution with MUPPI in cosmological volumes

Reference 37

Resolution: verified exact; local_arxiv, observed 2026-07-14T05:40:16.105820Z

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Observation 2e1b0aec-2a92-4170-9684-e354a2b8fdca · outbound

This paper cites Star Formation and Dust in the Cosmic Web.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster Star Formation and Dust in the Cosmic Web

Reference 38

Resolution: metadata mismatch; local_arxiv, observed 2026-07-14T05:40:16.116034Z

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Observation 617a6347-a1d5-4bd5-a7c4-26067367cc92 · outbound

This paper cites an unresolved cited work.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster Unresolved cited work

Reference 39

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Observation 6270a79e-6656-4d6c-919d-dcda1add0012 · outbound

This paper cites The OTELO survey: Nature and mass-metallicity relation for H$\alpha$ emitters at $z\sim\,0.4$.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster The OTELO survey: Nature and mass-metallicity relation for H$\alpha$ emitters at $z\sim\,0.4$

Reference 40

Resolution: verified exact; local_arxiv, observed 2026-07-14T05:40:17.184209Z

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Observation bba3924d-5059-4818-a5ea-6cabf489421f · outbound

This paper cites The lesser role of starbursts for star formation at z=2.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster The lesser role of starbursts for star formation at z=2

Reference 41

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Observation 59f5dbbf-65d5-4dc8-b169-caf8de799f2b · outbound

This paper cites L-GALAXIES 2020: Spatially resolved cold gas phases, star formation and chemical enrichment in galactic discs.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster L-GALAXIES 2020: Spatially resolved cold gas phases, star formation and chemical enrichment in galactic discs

Reference 42

Resolution: verified exact; local_arxiv, observed 2026-07-14T05:40:16.095426Z

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Observation 0b68af1e-1182-4b31-ad94-48009a35ee26 · outbound

This paper cites , keywords =.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster , keywords =

Reference 43

Resolution: verified exact; doi, observed 2026-07-14T05:40:17.149045Z

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Observation c3792910-8200-4a45-8b05-7a78cb739fc3 · outbound

This paper cites Properties of Early-Type, Dry Galaxy Mergers and the Origin of Massive Elliptical Galaxies.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster Properties of Early-Type, Dry Galaxy Mergers and the Origin of Massive Elliptical Galaxies

Reference 44

Resolution: verified exact; local_arxiv, observed 2026-07-14T05:40:17.193822Z

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No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation fa2d5c87-97eb-4495-834e-e7415018eec7 · outbound

This paper cites Knocking on giants' doors: I. The evolution of the dust-to-stellar mass ratio in distant dusty galaxies.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster Knocking on giants' doors: I. The evolution of the dust-to-stellar mass ratio in distant dusty galaxies

Reference 45

Resolution: verified exact; local_arxiv, observed 2026-07-14T05:40:17.199923Z

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Observation 313ca7c0-3f36-4bdf-a86a-6e5efc64192b · outbound

This paper cites Star formation quenching in massive galaxies.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster Star formation quenching in massive galaxies

Reference 46

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Observation 44102a54-9628-4e62-9fb4-05a5aa304753 · outbound

This paper cites IX: First spectroscopic confirmation of low-mass quiescent galaxies at z>2 with NIRISS.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster IX: First spectroscopic confirmation of low-mass quiescent galaxies at z>2 with NIRISS

Reference 47

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Observation 5f360fea-935e-4ddc-a2e3-224e9efebf3b · outbound

This paper cites The Dependence of Quenching upon the Inner Structure of Galaxies at 0.5<z< 0.8 in the DEEP2/AEGIS Survey.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster The Dependence of Quenching upon the Inner Structure of Galaxies at 0.5<z< 0.8 in the DEEP2/AEGIS Survey

Reference 48

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Observation b323ad35-c701-4280-8e15-f1fba09d6ffb · outbound

This paper cites What turns galaxies off? The different morphologies of star-forming and quiescent galaxies since z~2 from CANDELS.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster What turns galaxies off? The different morphologies of star-forming and quiescent galaxies since z~2 from CANDELS

Reference 49

Resolution: unresolved; no resolver link, observed 2026-07-14T05:32:07.775931Z

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Observation 40e1e9fd-153e-43b5-bb42-537fa7ad4e77 · outbound

This paper cites The Evolution of ISM Mass Probed by Dust Emission -- ALMA Observations at z = 0.3 to 2.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster The Evolution of ISM Mass Probed by Dust Emission -- ALMA Observations at z = 0.3 to 2

Reference 50

Resolution: unresolved; no resolver link, observed 2026-07-14T05:32:07.775931Z

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Observation 6a92b8ff-fd73-4ac4-82bf-834255e1971c · outbound

This paper cites The dominant role of mergers in the size evolution of massive early-type galaxies since z ~ 1.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster The dominant role of mergers in the size evolution of massive early-type galaxies since z ~ 1

Reference 51

Resolution: verified exact; local_arxiv, observed 2026-07-14T05:40:16.161982Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation b20ea1f8-6379-451f-879f-ad5454385516 · outbound

This paper cites , keywords =.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster , keywords =

Reference 52

Resolution: unresolved; no resolver link, observed 2026-07-14T05:32:07.775931Z

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Unavailable: canonical work link unavailable.

Observation 44ca2e94-9c34-4407-a1d6-be20a4494357 · outbound

This paper cites On Star Formation Rates and Star Formation Histories of Galaxies out to z ~ 3.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster On Star Formation Rates and Star Formation Histories of Galaxies out to z ~ 3

Reference 53

Resolution: unresolved; no resolver link, observed 2026-07-14T05:32:07.775931Z

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Unavailable: canonical work link unavailable.

Observation adc877c3-746c-475c-9e0a-497823fc6a7a · outbound

This paper cites Galaxy And Mass Assembly (GAMA): Panchromatic Data Release (far-UV --- far-IR) and the low-z energy budget.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster Galaxy And Mass Assembly (GAMA): Panchromatic Data Release (far-UV --- far-IR) and the low-z energy budget

Reference 54

Resolution: unresolved; no resolver link, observed 2026-07-14T05:32:07.775931Z

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Unavailable: canonical work link unavailable.

Observation 2ac732fb-182e-4477-b7bc-a4a9054bc4a1 · outbound

This paper cites Galaxy And Mass Assembly (GAMA): the G02 field, Herschel-ATLAS target selection and Data Release 3.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster Galaxy And Mass Assembly (GAMA): the G02 field, Herschel-ATLAS target selection and Data Release 3

Reference 55

Resolution: unresolved; no resolver link, observed 2026-07-14T05:32:07.775931Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 72e79b24-7e1e-4f09-bf44-a7d7d15b2529 · outbound

This paper cites Galaxy bulges and their black holes: a requirement for the quenching of star formation.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster Galaxy bulges and their black holes: a requirement for the quenching of star formation

Reference 56

Resolution: unresolved; no resolver link, observed 2026-07-14T05:32:07.775931Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7323a922-35ff-469c-abe0-dcb542e4dc5c · outbound

This paper cites Quenching timescales of galaxies in the EAGLE simulations.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster Quenching timescales of galaxies in the EAGLE simulations

Reference 57

Resolution: verified exact; local_arxiv, observed 2026-07-14T05:40:17.214051Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation ca9377ba-0655-40aa-b3b2-d3852a72eb27 · outbound

This paper cites Both starvation and outflows drive galaxy quenching.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster Both starvation and outflows drive galaxy quenching

Reference 58

Resolution: verified exact; local_arxiv, observed 2026-07-14T05:40:16.048042Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 9bcc60a8-89ec-48f4-9647-bcfa63339e49 · outbound

This paper cites Strangulation as the primary mechanism for shutting down star formation in galaxies.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster Strangulation as the primary mechanism for shutting down star formation in galaxies

Reference 59

Resolution: unresolved; no resolver link, observed 2026-07-14T05:32:07.775931Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0302cf63-a6ab-43b7-93ae-304a6c27dfa2 · outbound

This paper cites Star Formation in AEGIS Field Galaxies since z=1.1 : The Dominance of Gradually Declining Star Formation, and the Main Sequence of Star-Forming Galaxies.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster Star Formation in AEGIS Field Galaxies since z=1.1 : The Dominance of Gradually Declining Star Formation, and the Main Sequence of Star-Forming Galaxies

Reference 60

Resolution: unresolved; no resolver link, observed 2026-07-14T05:32:07.775931Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6d996142-956f-43cd-a922-8ca8168ea597 · outbound

This paper cites Dust production scenarios in galaxies at z ~ 6-8.3.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster Dust production scenarios in galaxies at z ~ 6-8.3

Reference 61

Resolution: unresolved; no resolver link, observed 2026-07-14T05:32:07.775931Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b172fd1c-0a9f-44fa-98d1-0a2badef1a22 · outbound

This paper cites Interstellar Medium and Star Formation of Starburst Galaxies on the Merger Sequence.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster Interstellar Medium and Star Formation of Starburst Galaxies on the Merger Sequence

Reference 62

Resolution: unresolved; no resolver link, observed 2026-07-14T05:32:07.775931Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fdfc45d1-dfe2-4c4f-b232-3de33d91789c · outbound

This paper cites , keywords =.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster , keywords =

Reference 63

Resolution: unresolved; no resolver link, observed 2026-07-14T05:32:07.775931Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2a829b5d-29f1-483e-b649-7847117db3f0 · outbound

This paper cites , keywords =.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster , keywords =

Reference 64

Resolution: unresolved; no resolver link, observed 2026-07-14T05:32:07.775931Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cca79f40-a81f-4409-ae24-81bfd4844fe9 · outbound

This paper cites A Survey of Atomic Carbon [C I] in High-redshift Main-Sequence Galaxies.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster A Survey of Atomic Carbon [C I] in High-redshift Main-Sequence Galaxies

Reference 65

Resolution: unresolved; no resolver link, observed 2026-07-14T05:32:07.775931Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6d33b09c-0961-4ef8-b0c3-4c6164401fde · outbound

This paper cites An ACA Survey of [CI] $^3P_1-^3P_0$, CO $J=4-3$, and Dust Continuum in Nearby U/LIRG.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster An ACA Survey of [CI] $^3P_1-^3P_0$, CO $J=4-3$, and Dust Continuum in Nearby U/LIRG

Reference 66

Resolution: verified exact; local_arxiv, observed 2026-07-14T05:40:16.653378Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation c455d550-9e7e-46b7-bc8b-e9d0ca316e5d · outbound

This paper cites Direct measurement of the [CI] luminosity to molecular gas mass conversion factor in high-redshift star-forming galaxies.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster Direct measurement of the [CI] luminosity to molecular gas mass conversion factor in high-redshift star-forming galaxies

Reference 67

Resolution: verified exact; local_arxiv, observed 2026-07-14T05:40:16.354280Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 165a458e-107f-4422-8f3a-a450994278c0 · outbound

This paper cites A Herschel Space Observatory Spectral Line Survey of Local Luminous Infrared Galaxies from 194 to 671 Microns.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster A Herschel Space Observatory Spectral Line Survey of Local Luminous Infrared Galaxies from 194 to 671 Microns

Reference 68

Resolution: verified exact; local_arxiv, observed 2026-07-14T05:40:16.700197Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 8e631aab-f551-4e3f-8d8d-900a4bf65da4 · outbound

This paper cites A fundamental plane for field star-forming galaxies.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster A fundamental plane for field star-forming galaxies

Reference 69

Resolution: unresolved; no resolver link, observed 2026-07-14T05:32:07.775931Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 83202d32-b44f-419a-94dd-a346710ec37d · outbound

This paper cites Dust continuum, CO, and [C I] 1-0 lines: self-consistent H2 mass estimates and the possibility of globally CO-dark galaxies at $z = 0.35$.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster Dust continuum, CO, and [C I] 1-0 lines: self-consistent H2 mass estimates and the possibility of globally CO-dark galaxies at $z = 0.35$

Reference 70

Resolution: verified exact; local_arxiv, observed 2026-07-14T05:40:16.709827Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 828b1b52-096c-4bb7-93d2-cce56417f8de · outbound

This paper cites On the Appearance of Thresholds in the Dynamical Model of Star Formation.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster On the Appearance of Thresholds in the Dynamical Model of Star Formation

Reference 71

Resolution: unresolved; no resolver link, observed 2026-07-14T05:32:07.775931Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ffdf0467-2238-47e4-ac63-d4d3ce395703 · outbound

This paper cites , keywords =.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster , keywords =

Reference 72

Resolution: unresolved; no resolver link, observed 2026-07-14T05:32:07.775931Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation aad1b764-8563-4797-b337-048f31807646 · outbound

This paper cites Star formation and molecular hydrogen in dwarf galaxies: a non-equilibrium view.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster Star formation and molecular hydrogen in dwarf galaxies: a non-equilibrium view

Reference 73

Resolution: verified exact; local_arxiv, observed 2026-07-14T05:40:16.357335Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 142d9dfe-d2fb-4cce-bde1-f2035495eb23 · outbound

This paper cites The relationship between dust and [CI] at z=1 and beyond.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster The relationship between dust and [CI] at z=1 and beyond

Reference 74

Resolution: verified exact; local_arxiv, observed 2026-07-14T05:40:16.417416Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation fd134e51-ce55-4f9e-8130-20d57fb4ad75 · outbound

This paper cites , keywords =.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster , keywords =

Reference 75

Resolution: unresolved; no resolver link, observed 2026-07-14T05:32:07.775931Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2301b1cf-6408-40a1-a35b-090238450050 · outbound

This paper cites The Molecular Interstellar Medium in Ultraluminous Infrared Galaxies.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster The Molecular Interstellar Medium in Ultraluminous Infrared Galaxies

Reference 76

Resolution: verified exact; local_arxiv, observed 2026-07-14T05:40:17.300007Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 5e1accab-8612-4ae6-9e6e-d8bc9d5d344f · outbound

This paper cites One star, two stars, or both? Investigating metallicity-dependant models for Gamma-Ray Burst progenitors with the IllustrisTNG simulation.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster One star, two stars, or both? Investigating metallicity-dependant models for Gamma-Ray Burst progenitors with the IllustrisTNG simulation

Reference 77

Resolution: unresolved; no resolver link, observed 2026-07-14T05:32:07.775931Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9d12be3f-094d-4a90-bf1b-d794549e652e · outbound

This paper cites Molecular gas and dust around a radio-quiet quasar at redshift 4.7.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster Molecular gas and dust around a radio-quiet quasar at redshift 4.7

Reference 78

Resolution: verified exact; local_arxiv, observed 2026-07-14T05:40:17.205211Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 9dea89ca-1df2-4f09-8ba5-c5a75aa455c3 · outbound

This paper cites , keywords =.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster , keywords =

Reference 79

Resolution: unresolved; no resolver link, observed 2026-07-14T05:32:07.775931Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2e5b82a8-3dbe-4063-809b-6f0ac1974b16 · outbound

This paper cites , keywords =.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster , keywords =

Reference 80

Resolution: unresolved; no resolver link, observed 2026-07-14T05:32:07.775931Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 004334c0-bec1-4342-b0d6-b4b0798aa7c0 · outbound

This paper cites , keywords =.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster , keywords =

Reference 81

Resolution: unresolved; no resolver link, observed 2026-07-14T05:32:07.775931Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fa51eb1e-dfae-4b84-994a-43507b6ea26a · outbound

This paper cites A Revised Host Galaxy Association for GRB 020819B: A High-Redshift Dusty Starburst, Not a Low-Redshift Gas-Poor Spiral.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster A Revised Host Galaxy Association for GRB 020819B: A High-Redshift Dusty Starburst, Not a Low-Redshift Gas-Poor Spiral

Reference 82

Resolution: unresolved; no resolver link, observed 2026-07-14T05:32:07.775931Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bdfdc482-2e91-4fdc-a374-fb9e5fc5382c · outbound

This paper cites The Swift GRB Host Galaxy Legacy Survey - II. Rest-Frame NIR Luminosity Distribution and Evidence for a Near-Solar Metallicity Threshold.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster The Swift GRB Host Galaxy Legacy Survey - II. Rest-Frame NIR Luminosity Distribution and Evidence for a Near-Solar Metallicity Threshold

Reference 83

Resolution: unresolved; no resolver link, observed 2026-07-14T05:32:07.775931Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0120eaeb-d167-44fc-840d-8bd923b0c1ae · outbound

This paper cites Connecting GRBs and ULIRGs: A Sensitive, Unbiased Survey for Radio Emission from Gamma-Ray Burst Host Galaxies at 0<z<2.5.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster Connecting GRBs and ULIRGs: A Sensitive, Unbiased Survey for Radio Emission from Gamma-Ray Burst Host Galaxies at 0<z<2.5

Reference 84

Resolution: verified exact; local_arxiv, observed 2026-07-14T05:40:17.120508Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 8ec2d55c-7204-4ede-8c7a-5010241abed3 · outbound

This paper cites New light on gamma-ray burst host galaxies with Herschel.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster New light on gamma-ray burst host galaxies with Herschel

Reference 85

Resolution: unresolved; no resolver link, observed 2026-07-14T05:32:07.775931Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9f277cd2-948d-4910-b070-ef469991bdc1 · outbound

This paper cites A Survey of Atomic Carbon at High Redshift.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster A Survey of Atomic Carbon at High Redshift

Reference 86

Resolution: verified exact; local_arxiv, observed 2026-07-14T05:40:17.125514Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 8c0be8a0-f03f-458f-a7d2-53dd440fcdf1 · outbound

This paper cites ALMA CO Observations of the Host Galaxies of Long-duration Gamma-ray Bursts. I: Molecular Gas Scaling Relations.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster ALMA CO Observations of the Host Galaxies of Long-duration Gamma-ray Bursts. I: Molecular Gas Scaling Relations

Reference 87

Resolution: verified exact; local_arxiv, observed 2026-07-14T05:40:17.145673Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation b099e8fa-5bb6-4825-b879-0353b2eb74f3 · outbound

This paper cites Dust grain growth in the interstellar medium of 5<z<6.5 quasars.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster Dust grain growth in the interstellar medium of 5<z<6.5 quasars

Reference 88

Resolution: verified exact; local_arxiv, observed 2026-07-14T05:40:17.243948Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation c21688e9-6a9a-4cf5-a6f7-9b5b48a31f05 · outbound

This paper cites Determining the stellar masses of submillimetre galaxies: the critical importance of star formation histories.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster Determining the stellar masses of submillimetre galaxies: the critical importance of star formation histories

Reference 89

Resolution: verified exact; local_arxiv, observed 2026-07-14T05:40:17.305796Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 74f2b142-0b17-4649-9de4-15c9566b8df1 · outbound

This paper cites GRB 980425 host: [CII], [OI] and CO lines reveal recent enhancement of star formation due to atomic gas inflow.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster GRB 980425 host: [CII], [OI] and CO lines reveal recent enhancement of star formation due to atomic gas inflow

Reference 90

Resolution: verified exact; local_arxiv, observed 2026-07-14T05:40:17.089665Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 1bcb4c4d-1476-4026-8ecc-1cdefee030ca · outbound

This paper cites A Detection of Molecular Gas Emission in the Host Galaxy of GRB 080517.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster A Detection of Molecular Gas Emission in the Host Galaxy of GRB 080517

Reference 91

Resolution: verified exact; local_arxiv, observed 2026-07-14T05:40:17.050554Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation b7dfaff6-8829-4aa6-b0d5-f6affde70a48 · outbound

This paper cites Two gamma-ray bursts from dusty regions with little molecular gas.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster Two gamma-ray bursts from dusty regions with little molecular gas

Reference 92

Resolution: verified exact; local_arxiv, observed 2026-07-14T05:40:17.038021Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 91b04316-59c0-4145-b9af-4c7597bc422a · outbound

This paper cites , keywords =.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster , keywords =

Reference 93

Resolution: unresolved; no resolver link, observed 2026-07-14T05:32:07.775931Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 32030e59-cf34-468c-b487-efad783ca190 · outbound

This paper cites SF2A-2005: Semaine de l'Astrophysique Francaise , year = 2005, editor =.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster SF2A-2005: Semaine de l'Astrophysique Francaise , year = 2005, editor =

Reference 94

Resolution: unresolved; no resolver link, observed 2026-07-14T05:32:07.775931Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 13fe8963-fc2e-4475-ab37-b6d827337b84 · outbound

This paper cites Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series , year = 2006, editor =.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series , year = 2006, editor =

Reference 95

Resolution: verified exact; doi, observed 2026-07-14T05:40:17.041556Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation c13c8eb3-bf8b-447f-9681-9032d2d5a3f8 · outbound

This paper cites , keywords =.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster , keywords =

Reference 96

Resolution: verified exact; doi, observed 2026-07-14T05:40:17.044981Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 92d09283-b756-486e-9318-a5fd20ab374d · outbound

This paper cites , keywords =.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster , keywords =

Reference 97

Resolution: unresolved; no resolver link, observed 2026-07-14T05:32:07.775931Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7bf33e09-0ff7-4315-a267-4eb49c3251b5 · outbound

This paper cites Mass and metallicity scaling relations of high redshift star-forming galaxies selected by GRBs.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster Mass and metallicity scaling relations of high redshift star-forming galaxies selected by GRBs

Reference 98

Resolution: verified exact; local_arxiv, observed 2026-07-14T05:40:17.084247Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 65fe1da0-17e2-4143-8ca3-c68576b4916f · outbound

This paper cites A Molecular gas rich GRB host galaxy at the peak of cosmic star formation.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster A Molecular gas rich GRB host galaxy at the peak of cosmic star formation

Reference 99

Resolution: verified exact; local_arxiv, observed 2026-07-14T05:40:17.068156Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation b1711d24-9a23-4c9a-a101-074e4b1bdc19 · outbound

This paper cites Local starburst conditions and formation of GRB 980425 / SN 1998bw within a collisional ring.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster Local starburst conditions and formation of GRB 980425 / SN 1998bw within a collisional ring

Reference 100

Resolution: verified exact; local_arxiv, observed 2026-07-14T05:40:17.095113Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 175e02e5-338a-48fa-83db-86edf5d41727 · outbound

This paper cites Relativistic supernova 2009bb exploded close to an atomic gas cloud.

Mass--size evolution and the emerging passive--density relation revealed by JWST/NIRCam in the Spiderweb protocluster Relativistic supernova 2009bb exploded close to an atomic gas cloud

Reference 101

Resolution: verified exact; local_arxiv, observed 2026-07-14T05:40:17.073385Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

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