Paper Citation Record · LEDGER

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies

As of 16 August 2026, this Paper Citation Record lists 100 of 153 outbound references and 4 inbound Pith citation observations for arXiv:2509.00148.

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

pith.paper-citation-record.v1
2509.00148 v1

Coverage vector

measured 100 of 153 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-05T13:58:33.901526Z

measured 104 of 104 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-16T06:30:59.297886+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-05T13:58:27.414316Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-03T11:38:04.903312Z

Reference resolution

100 of 153 outbound references displayed

verified exact6
verified fuzzy0
unresolved94
parse uncertain0
malformed identifier0
metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

Observation 72102513-267a-4062-9355-bfa219e15378 · outbound

This paper cites S., Aguilar, G., et al.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies S., Aguilar, G., et al

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:21.557309Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fd0635fe-1f2d-435a-bd8f-a12634e36810 · outbound

This paper cites 2025, arXiv e-prints, arXiv:2508.18097.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies 2025, arXiv e-prints, arXiv:2508.18097

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:21.634086Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d4525166-6909-489c-bdfb-6e00ee8d8fae · outbound

This paper cites 2018, PASJ, 70, S4, doi: 10.1093/pasj/psx066.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies 2018, PASJ, 70, S4, doi: 10.1093/pasj/psx066

Reference 3

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:21.681810Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7e051f11-8483-4414-90bf-ca73a44d0e9d · outbound

This paper cites E., Leja, J., et al.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies E., Leja, J., et al

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:21.747757Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 306ab1d5-fbce-463d-b426-ddd9afb3047e · outbound

This paper cites 2016a, ApJ, 827, 106, doi: 10.3847/0004-637X/827/2/106.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies 2016a, ApJ, 827, 106, doi: 10.3847/0004-637X/827/2/106

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:21.873274Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 76b9c222-aba1-499e-b4fe-c49abe0a1f62 · outbound

This paper cites L., Rich, J.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies L., Rich, J

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:21.995582Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a585231e-7feb-427e-afc0-0df3dc5b76eb · outbound

This paper cites 2017, ApJ, 843, 9, doi: 10.3847/1538-4357/aa72eb.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies 2017, ApJ, 843, 9, doi: 10.3847/1538-4357/aa72eb

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:22.045922Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 71128489-0319-47e6-83bc-9cd8742d6667 · outbound

This paper cites T., et al.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies T., et al

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:22.222748Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation be17f14c-300a-4606-97f1-f7ced67dd96a · outbound

This paper cites 2025, ApJ, 978, 90, doi: 10.3847/1538-4357/ad8b30 Astropy Collaboration, Robitaille, T.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies 2025, ApJ, 978, 90, doi: 10.3847/1538-4357/ad8b30 Astropy Collaboration, Robitaille, T

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:22.332641Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 56297b70-d998-4fec-a501-201677b12288 · outbound

This paper cites I., & Xavier Prochaska, J.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies I., & Xavier Prochaska, J

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:22.496771Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 40ba8082-ac47-4c73-b52d-580c6e181829 · outbound

This paper cites D., et al.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies D., et al

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:22.629604Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 13227382-c31b-4966-a30d-e3a6fc507e50 · outbound

This paper cites an unresolved cited work.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies Unresolved cited work

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:22.765662Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7ea2beb4-30df-4a96-8c6e-ffbd28838fd4 · outbound

This paper cites X., et al.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies X., et al

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:22.921379Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 18c80a92-647f-4173-adcf-c8a6f8c2c0fb · outbound

This paper cites H., Hearin, A.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies H., Hearin, A

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:23.013325Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1ee9025e-0d73-4f2a-8a8c-342d7056f93d · outbound

This paper cites B., & Ellis, R.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies B., & Ellis, R

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:23.097353Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 50c43ef9-fed2-4674-8893-31a348c1bab4 · outbound

This paper cites 2021, ApJL, 909, L11, doi: 10.3847/2041-8213/abe6a6.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies 2021, ApJL, 909, L11, doi: 10.3847/2041-8213/abe6a6

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:23.203808Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9ec19acb-7da9-4e8f-ba88-d685a7b062f8 · outbound

This paper cites L., et al.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies L., et al

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:23.295236Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fe191108-4dcf-4d70-a504-8e39924ebda7 · outbound

This paper cites G., Kriek, M., Suess, K.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies G., Kriek, M., Suess, K

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:23.415273Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 21916c16-a112-434e-85c5-97e1f43393a8 · outbound

This paper cites G., Slob, M., Kriek, M., et al.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies G., Slob, M., Kriek, M., et al

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:23.513538Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ab5c7fc1-ec0f-4425-9e6a-00e0ef60f4ca · outbound

This paper cites S., Suess, K.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies S., Suess, K

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:23.633024Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 51f98bf1-fb1f-4b37-bb93-929a38b6261b · outbound

This paper cites D., Wolfire, M., & Leroy, A.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies D., Wolfire, M., & Leroy, A

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:23.739323Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4341af0f-2360-4b00-a900-e0b21356523f · outbound

This paper cites 2015, A&A, 575, A56, doi: 10.1051/0004-6361/201425078.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies 2015, A&A, 575, A56, doi: 10.1051/0004-6361/201425078

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:23.866397Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e12809a7-5b0b-4dd8-8ee2-4fc9da0865df · outbound

This paper cites N., Whitaker, K.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies N., Whitaker, K

Reference 23

Resolution: verified exact; doi, observed 2026-08-05T14:03:29.443251Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation f1882277-ba13-4ee8-b54a-7678b08dba40 · outbound

This paper cites C., McLure, R.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies C., McLure, R

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:24.094145Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9e3a3822-6971-4684-ae0e-93880524570c · outbound

This paper cites C., McLeod, D.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies C., McLeod, D

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:24.144678Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 26d76cb4-e867-4424-8996-22d7341110e0 · outbound

This paper cites C., McLure, R.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies C., McLure, R

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:24.219318Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 982324b5-69a9-4407-aac1-70e11be57ac3 · outbound

This paper cites C., Cullen, F., McLure, R.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies C., Cullen, F., McLure, R

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:24.288934Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 39438e87-df39-4b09-8628-6553c58329f5 · outbound

This paper cites 2022, Publications of the Astronomical Society of the Pacific, 134, 114501, doi: 10.1088/1538-3873/ac9642.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies 2022, Publications of the Astronomical Society of the Pacific, 134, 114501, doi: 10.1088/1538-3873/ac9642

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:24.368684Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 006d2d72-a02b-49c2-92d6-d8bf5908e773 · outbound

This paper cites 2003, PASP, 115, 763, doi: 10.1086/376392.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies 2003, PASP, 115, 763, doi: 10.1086/376392

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:24.493322Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fb0c426f-3aed-4f4b-a2b5-799d08306aab · outbound

This paper cites an unresolved cited work.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies Unresolved cited work

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:24.595038Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8ce5f180-93b5-4f20-b1f6-474a73ba65a5 · outbound

This paper cites 2016, ApJ, 823, 102, doi: 10.3847/0004-637X/823/2/102.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies 2016, ApJ, 823, 102, doi: 10.3847/0004-637X/823/2/102

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:24.721260Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6735b820-1c4c-4c58-9c7b-7271f0a3140a · outbound

This paper cites an unresolved cited work.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies Unresolved cited work

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:24.841307Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c98ae625-ffbe-479f-832e-cec0d52eaaf8 · outbound

This paper cites E., & White, M.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies E., & White, M

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:24.961539Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7aa0800d-084d-4e12-8a0a-476ae9023f0f · outbound

This paper cites R., Brammer, G., Heintz, K.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies R., Brammer, G., Heintz, K

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:25.114565Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 68128ee9-4140-4e9d-aa10-1d4508dadd17 · outbound

This paper cites A., Greene, J., Ma, C.-P., et al.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies A., Greene, J., Ma, C.-P., et al

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:25.392439Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation eb306567-5a7d-49f5-a44a-e65f8ecb1c35 · outbound

This paper cites 2006, MNRAS, 368, 2, doi: 10.1111/j.1365-2966.2006.10145.x.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies 2006, MNRAS, 368, 2, doi: 10.1111/j.1365-2966.2006.10145.x

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:25.508657Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9782bc40-e135-4ed5-bb1b-d4fdf9c0bfbf · outbound

This paper cites Quenching Through Tidal Gas Removal: Molecular Gas and Star Formation in Tidal Tails of z ~ 0.7 Post-Starburst Galaxies.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies Quenching Through Tidal Gas Removal: Molecular Gas and Star Formation in Tidal Tails of z ~ 0.7 Post-Starburst Galaxies

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:25.657893Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 962f4a36-9572-4cb3-b00e-7fcea93f1546 · outbound

This paper cites 2016, ApJS, 222, 8, doi: 10.3847/0067-0049/222/1/8.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies 2016, ApJS, 222, 8, doi: 10.3847/0067-0049/222/1/8

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:25.749468Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d7b823cb-25b8-4685-9c49-9a6d39c41a6c · outbound

This paper cites T., Dale, D.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies T., Dale, D

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:25.889694Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5abd1fe3-81d6-4543-b4f0-1a7c059d0cfe · outbound

This paper cites an unresolved cited work.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies Unresolved cited work

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:25.994630Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2d5ee9fc-fcf0-48da-ae6e-afcae37b76ae · outbound

This paper cites A., Baes, M., Bourne, N., et al.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies A., Baes, M., Bourne, N., et al

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:26.325998Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 48f48392-abfe-4cea-8c53-b5227d8ee89a · outbound

This paper cites 2024, The Open Journal of Astrophysics, 7, 121, doi: 10.33232/001c.127779.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies 2024, The Open Journal of Astrophysics, 7, 121, doi: 10.33232/001c.127779

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:26.489555Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 79bca719-1cd5-4afa-934f-a31fdd42593c · outbound

This paper cites 2025, The Open Journal of Astrophysics, 8, 12, doi: 10.33232/001c.129235 Falc´ on-Barroso, J., S´ anchez-Bl´ azquez, P., Vazdekis, A., et al.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies 2025, The Open Journal of Astrophysics, 8, 12, doi: 10.33232/001c.129235 Falc´ on-Barroso, J., S´ anchez-Bl´ azquez, P., Vazdekis, A., et al

Reference 45

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:26.637302Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0aefee4f-1061-49a1-a7e7-9434bc846af4 · outbound

This paper cites 2015, MNRAS, 446, 1939, doi: 10.1093/mnras/stu2207 Ferr´ e-Mateu, A., Trujillo, I., Mart ´ ın-Navarro, I., et al.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies 2015, MNRAS, 446, 1939, doi: 10.1093/mnras/stu2207 Ferr´ e-Mateu, A., Trujillo, I., Mart ´ ın-Navarro, I., et al

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:26.790325Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3211fb3e-6c30-400d-8a90-6d3b0e99f291 · outbound

This paper cites 2025, ApJ, 979, 94, doi: 10.3847/1538-4357/ad900f.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies 2025, ApJ, 979, 94, doi: 10.3847/1538-4357/ad900f

Reference 47

Resolution: verified exact; doi, observed 2026-08-05T14:03:29.132069Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation 9c0bd099-1f0f-4434-a220-55b5251f3742 · outbound

This paper cites D., Yang, Y., Zabludoff, A., et al.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies D., Yang, Y., Zabludoff, A., et al

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:26.999914Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ad5372fa-2d26-4b18-80f3-77fc5c886b14 · outbound

This paper cites D., Yang, Y., Zabludoff, A.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies D., Yang, Y., Zabludoff, A

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:27.081261Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f7f6f175-7899-470a-be45-68a1a8b3861c · outbound

This paper cites D., Smercina, A., Rowlands, K., et al.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies D., Smercina, A., Rowlands, K., et al

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:27.155989Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation dcd13b6a-a9ac-443a-903a-712bb4b213a0 · outbound

This paper cites J., et al.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies J., et al

Reference 51

Resolution: verified exact; doi, observed 2026-08-05T14:03:28.962736Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation dfe931b7-a1e1-4b2e-bc9a-5cc834ecb590 · outbound

This paper cites E., Hickox, R.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies E., Hickox, R

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:27.475355Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a8f77161-ecf1-4d89-917a-ed47b8017412 · outbound

This paper cites E., Tremonti, C., Diamond-Stanic, A.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies E., Tremonti, C., Diamond-Stanic, A

Reference 54

Resolution: verified exact; doi, observed 2026-08-05T14:03:28.795714Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation 13ca28b8-beae-47d4-a04b-59430c2a1de5 · outbound

This paper cites 2017, Nature, 544, 71, doi: 10.1038/nature21680.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies 2017, Nature, 544, 71, doi: 10.1038/nature21680

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:27.685576Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 53a9f483-9fad-4986-a9d1-cbd3b56be1c4 · outbound

This paper cites 2024, Nature, 628, 277, doi: 10.1038/s41586-024-07191-9.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies 2024, Nature, 628, 277, doi: 10.1038/s41586-024-07191-9

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:27.814393Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a7e26f32-70b9-4b1f-8e9c-320322abdfd2 · outbound

This paper cites 2018, Nature Astronomy, 2, 239, doi: 10.1038/s41550-017-0352-5.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies 2018, Nature Astronomy, 2, 239, doi: 10.1038/s41550-017-0352-5

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:27.952624Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5f39fb26-1e94-4835-9e6b-48290f5b3411 · outbound

This paper cites The Prime Focus Spectrograph Galaxy Evolution Survey.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies The Prime Focus Spectrograph Galaxy Evolution Survey

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:28.043615Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c76c4224-9f89-4e6f-a844-c933f5636ab8 · outbound

This paper cites E., Murphy, J.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies E., Murphy, J

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:28.130606Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1ff4fab4-84d8-435e-b142-f7f6a45e42ce · outbound

This paper cites E., Setton, D., Bezanson, R., et al.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies E., Setton, D., Bezanson, R., et al

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:28.251462Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4a20cbfa-7754-4d17-925b-1914af8949c7 · outbound

This paper cites J., Abergel, A., Abreu, A., et al.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies J., Abergel, A., Abreu, A., et al

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:28.354081Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 51becfa1-5499-4aec-b4e2-98fd271d341b · outbound

This paper cites C., Lanz, L., Ashby, M.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies C., Lanz, L., Ashby, M

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:28.528257Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fa676974-df73-43dd-a8e7-569a2593fd0f · outbound

This paper cites 2013, ApJS, 208, 19, doi: 10.1088/0067-0049/208/2/19.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies 2013, ApJS, 208, 19, doi: 10.1088/0067-0049/208/2/19

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:28.642640Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ce9470a2-b56f-4b9d-8d4c-b2c050d77c8b · outbound

This paper cites F., Hernquist, L., Cox, T.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies F., Hernquist, L., Cox, T

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:28.728321Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 227e8f07-49ca-4416-8f25-62a05f9b8541 · outbound

This paper cites F., Somerville, R.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies F., Somerville, R

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:28.824352Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f75c536b-106c-4fd0-acba-60d7e95ab7cf · outbound

This paper cites E., et al.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies E., et al

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:28.909834Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d4556509-746e-4548-8c0a-cc6a9c520af9 · outbound

This paper cites an unresolved cited work.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies Unresolved cited work

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:29.035288Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b80f217f-dfbf-4517-b634-8c1493c5c14f · outbound

This paper cites 2017, Bd-J/Prospector: Initial Release, v0.1, Zenodo, doi: 10.5281/zenodo.1116491.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies 2017, Bd-J/Prospector: Initial Release, v0.1, Zenodo, doi: 10.5281/zenodo.1116491

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:29.156388Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 973731b2-7e48-4720-9341-e6856fadc870 · outbound

This paper cites 2021, dfm/python-fsps: python-fsps v0.4.0, v0.4.0, Zenodo, doi: 10.5281/zenodo.4577191.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies 2021, dfm/python-fsps: python-fsps v0.4.0, v0.4.0, Zenodo, doi: 10.5281/zenodo.4577191

Reference 69

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:29.249992Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1898dba8-7cae-45a3-8598-1b756cc7d05e · outbound

This paper cites an unresolved cited work.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies Unresolved cited work

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:29.375415Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e34bed84-ac97-4b65-ada4-15264c65c2cf · outbound

This paper cites 1998, ApJ, 498, 541, doi: 10.1086/305588 Kereˇ s, D., Katz, N., Weinberg, D.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies 1998, ApJ, 498, 541, doi: 10.1086/305588 Kereˇ s, D., Katz, N., Weinberg, D

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:29.479979Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7ebfbc03-e415-4f38-bec2-d99ff68590e8 · outbound

This paper cites 2013, ApJL, 775, L16, doi: 10.1088/2041-8205/775/1/L16.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies 2013, ApJL, 775, L16, doi: 10.1088/2041-8205/775/1/L16

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:29.665193Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 08cf5826-1bd7-4832-a9b8-564fd1a67283 · outbound

This paper cites 2010, ApJL, 722, L64, doi: 10.1088/2041-8205/722/1/L64.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies 2010, ApJL, 722, L64, doi: 10.1088/2041-8205/722/1/L64

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:29.790914Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation eaeec8e1-e111-45cd-ae59-b5c286fbd7a7 · outbound

This paper cites G., et al.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies G., et al

Reference 74

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:29.907974Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4b312d29-9157-4258-8df8-cf683923bf68 · outbound

This paper cites M., Steidel, C.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies M., Steidel, C

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:30.043844Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b2b7a20f-0e2c-4f4c-ac5a-d1ae8d36a61d · outbound

This paper cites D., Conroy, C., & van Dokkum, P.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies D., Conroy, C., & van Dokkum, P

Reference 76

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:30.198217Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 96b4dc37-1bde-4b0e-bdc0-3307a7e1ec15 · outbound

This paper cites 2017, ApJ, 837, 170, doi: 10.3847/1538-4357/aa5ffe.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies 2017, ApJ, 837, 170, doi: 10.3847/1538-4357/aa5ffe

Reference 77

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:30.385173Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 936aa06c-8f35-41fc-bf48-1f29a47cb9a5 · outbound

This paper cites D., Conroy, C., et al.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies D., Conroy, C., et al

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:30.485938Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 67404173-cd9c-4757-9c24-860a1ebd955c · outbound

This paper cites S., Ting, Y.-S., et al.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies S., Ting, Y.-S., et al

Reference 79

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:30.687991Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d067f5e5-295a-4cab-9399-85a5ffa81c77 · outbound

This paper cites 2022, ApJ, 938, 63, doi: 10.3847/1538-4357/ac8b7d.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies 2022, ApJ, 938, 63, doi: 10.3847/1538-4357/ac8b7d

Reference 80

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:30.815161Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 490a5046-283a-4582-a948-b35f7473d50d · outbound

This paper cites E., Gobat, R., Valentino, F., et al.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies E., Gobat, R., Valentino, F., et al

Reference 81

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:30.899364Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 890df98f-542f-4534-8e0c-1a8f35e2f0bf · outbound

This paper cites T., Almaini, O., Wild, V., et al.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies T., Almaini, O., Wild, V., et al

Reference 82

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:31.014764Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bfaac8dd-8c32-4aa0-a08a-c65a637d308b · outbound

This paper cites an unresolved cited work.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies Unresolved cited work

Reference 83

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:31.101465Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9aba9b5c-b83c-46bb-874e-5d4395a1eed9 · outbound

This paper cites 2009, ApJ, 707, 250, doi: 10.1088/0004-637X/707/1/250.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies 2009, ApJ, 707, 250, doi: 10.1088/0004-637X/707/1/250

Reference 84

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:31.217175Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f3412878-1339-42c4-9c4e-bf7142e087ae · outbound

This paper cites S., Marchesini, D.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies S., Marchesini, D

Reference 85

Resolution: verified exact; doi, observed 2026-08-05T13:58:41.849002Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation b05d3b30-4dcc-4ab5-b820-2d7f2abb79ad · outbound

This paper cites The Herschel/PACS Point Source Catalogue Explanatory Supplement.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies The Herschel/PACS Point Source Catalogue Explanatory Supplement

Reference 86

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:31.421286Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 221c3996-2b5b-449b-a829-f8f27eb14954 · outbound

This paper cites Excavating The Ruins: an Ancient $z=2.675$ Galaxy Which Formed in the First 500 Myr.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies Excavating The Ruins: an Ancient $z=2.675$ Galaxy Which Formed in the First 500 Myr

Reference 87

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:31.524959Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 30c390af-edc1-4831-8d4d-989f153ce27a · outbound

This paper cites M., Alatalo, K., Blitz, L., et al.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies M., Alatalo, K., Blitz, L., et al

Reference 88

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:31.649232Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a5afa4a5-94b2-4149-b217-34354699154a · outbound

This paper cites 2023, arXiv e-prints, arXiv:2310.20572, doi: 10.48550/arXiv.2310.20572.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies 2023, arXiv e-prints, arXiv:2310.20572, doi: 10.48550/arXiv.2310.20572

Reference 89

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:31.740137Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e2af2f0d-6502-4fac-80a1-ec0f0773fd3b · outbound

This paper cites M., Ivezi´ c,ˇZ., & Elitzur, M.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies M., Ivezi´ c,ˇZ., & Elitzur, M

Reference 91

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:32.028455Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation af4293c9-4eca-4dcd-a7b1-f02e209c42d0 · outbound

This paper cites A., Rowlands, K., Alatalo, K., et al.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies A., Rowlands, K., Alatalo, K., et al

Reference 92

Resolution: verified exact; doi, observed 2026-08-05T13:58:41.473514Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation 50cc49d9-6034-4a6e-82fb-7ab205412e4a · outbound

This paper cites 2023, ApJ, 953, 119, doi: 10.3847/1538-4357/acd54a —.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies 2023, ApJ, 953, 119, doi: 10.3847/1538-4357/acd54a —

Reference 93

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:32.352945Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bb2e3089-233a-47fa-ab0f-ad9df1b2269c · outbound

This paper cites A., Ho, S., & Ross, N.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies A., Ho, S., & Ross, N

Reference 94

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:32.458534Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f7f0e147-da7c-43da-9fad-d1591128839f · outbound

This paper cites L., Riedinger, J.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies L., Riedinger, J

Reference 95

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:32.544499Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5d4cc9a1-9736-4dfe-8fe5-d20d3ded9372 · outbound

This paper cites M., & Wu, H.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies M., & Wu, H

Reference 96

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:32.646900Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 63234804-e047-4942-9c94-88beb9696e86 · outbound

This paper cites 2010, A&A, 518, L2, doi: 10.1051/0004-6361/201014535.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies 2010, A&A, 518, L2, doi: 10.1051/0004-6361/201014535

Reference 97

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:32.859688Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation aea397e9-6d24-40bc-a036-24c1a8850868 · outbound

This paper cites H., Kriek, M., Brammer, G.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies H., Kriek, M., Brammer, G

Reference 98

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:32.987308Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a641c8ed-bd0c-46a4-b06e-a515cdbf68a6 · outbound

This paper cites 2019, A&A, 625, A65, doi: 10.1051/0004-6361/201935222.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies 2019, A&A, 625, A65, doi: 10.1051/0004-6361/201935222

Reference 99

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:33.130104Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f0de8fb2-54b9-45d2-a58b-19af4e39f132 · outbound

This paper cites 2015, MNRAS, 448, 258, doi: 10.1093/mnras/stu2714.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies 2015, MNRAS, 448, 258, doi: 10.1093/mnras/stu2714

Reference 100

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:33.339408Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4ac1999a-b7de-4a5d-9d9a-e6fd46f62831 · outbound

This paper cites 2018, MNRAS, 473, 1168, doi: 10.1093/mnras/stx1903.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies 2018, MNRAS, 473, 1168, doi: 10.1093/mnras/stx1903

Reference 101

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:33.463118Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e17c8191-2b0d-43f0-a9ce-c5962bbd4716 · outbound

This paper cites T., Daddi, E., Bournaud, F., et al.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies T., Daddi, E., Bournaud, F., et al

Reference 103

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:33.726528Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8ad98cc2-cd9f-4080-b635-4c545c8f77a4 · outbound

This paper cites 2021, ApJ, 919, 134, doi: 10.3847/1538-4357/ac0f7f.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies 2021, ApJ, 919, 134, doi: 10.3847/1538-4357/ac0f7f

Reference 104

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:33.847459Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7436f7db-08e5-4ce0-bec0-3bf7f4be522b · outbound

This paper cites M., Simmons, B.

SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies M., Simmons, B

Reference 105

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:33.901526Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Pith citing papers

Observation 9ddd6d92-ddff-4240-b30e-11446e0eeda8 · inbound

Meet the Neighbors: Gas Rich "Buddy Galaxies" are Common Around Recently Quenched Massive Galaxies in the SQuIGG$\vec{L}$E Survey cites this paper.

Meet the Neighbors: Gas Rich "Buddy Galaxies" are Common Around Recently Quenched Massive Galaxies in the SQuIGG$\vec{L}$E Survey SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-05T13:58:27.414316Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5f34edb7-0718-4177-a669-08c9ddf8f38b · inbound

Sparks: The Magellan/FIRE survey from starburst to post-starburst cites this paper.

Sparks: The Magellan/FIRE survey from starburst to post-starburst SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies

Reference 93

Resolution: verified exact; arxiv_id, observed 2026-05-10T14:25:29.938795Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation c6cb2918-3170-4147-b8f3-7b004ba32dc9 · inbound

A Possible Protocluster of Galaxies Serendipitously Discovered in the Field of an Intermediate-Redshift Post-starburst Galaxy cites this paper.

A Possible Protocluster of Galaxies Serendipitously Discovered in the Field of an Intermediate-Redshift Post-starburst Galaxy SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies

Reference 17

Resolution: verified exact; arxiv_id, observed 2026-05-11T13:16:02.838854Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation 9965b9c6-8dae-4d4e-8d85-0c620d0e216d · inbound

Quenching of Star Formation in Massive Galaxies cites this paper.

Quenching of Star Formation in Massive Galaxies SQuIGG$\vec{L}$E: Buried star formation cannot explain the rapidly fading CO(2-1) luminosity in massive, $z\sim0.7$ post-starburst galaxies

Reference 275

Resolution: metadata mismatch; arxiv_id, observed 2026-07-03T11:38:04.904758Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.