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Paper Citation Record · LEDGER

X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes

As of 8 August 2026, this Paper Citation Record lists 100 of 300 outbound references and 0 inbound Pith citation observations for arXiv:2606.21495.

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

pith.paper-citation-record.v1
2606.21495 v1

Coverage vector

measured 100 of 300 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-06-26T13:47:51.674362Z

measured 100 of 100 standing notices

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measured 0 of 0 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links

measured 0 of 1 external citation measurements

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Source: cited_works

Reference resolution

100 of 300 outbound references displayed

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External citation measurements

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Outbound references

Observation 70673421-94ae-416d-93dc-fe1e479e2ea3 · outbound

This paper cites Aceña and E.

X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes Aceña and E

Reference 1

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Observation 6060990a-6f05-4284-9fb2-08a3fff1d13f · outbound

This paper cites López and F.

X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes López and F

Reference 2

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Observation 53941a9d-97d8-41bd-80d5-16f6c2053ba9 · outbound

This paper cites López and J.

X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes López and J

Reference 3

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Observation 09a513df-3edc-4922-8e0d-c1d4d43430ca · outbound

This paper cites López and J.

X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes López and J

Reference 4

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Observation e5352753-1481-4e01-a2f1-6b45401bcbb7 · outbound

This paper cites Armijos-Abendaño and E.

X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes Armijos-Abendaño and E

Reference 5

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Observation 061e7597-4ef2-4589-82cc-6081aa54f2c8 · outbound

This paper cites Armijos-Abendaño and E.

X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes Armijos-Abendaño and E

Reference 6

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X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes Unresolved cited work

Reference 7

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Observation 4590375f-c66e-4b6e-91c0-b6635bb7b383 · outbound

This paper cites Freedman and Barry F.

X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes Freedman and Barry F

Reference 8

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X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes Unresolved cited work

Reference 9

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This paper cites Weigel and Kevin Schawinski and Claudio Bruderer , doi =.

X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes Weigel and Kevin Schawinski and Claudio Bruderer , doi =

Reference 10

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This paper cites Le Fevre and L Tresse and M Bethermin and Y.

X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes Le Fevre and L Tresse and M Bethermin and Y

Reference 11

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This paper cites Montero-Dorta and Francisco Prada , doi =.

X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes Montero-Dorta and Francisco Prada , doi =

Reference 12

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Observation a04285a8-a90c-4415-bbbb-2e32391e0f96 · outbound

This paper cites Blanton and John Moustakas , doi =.

X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes Blanton and John Moustakas , doi =

Reference 13

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This paper cites Croton , doi =.

X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes Croton , doi =

Reference 14

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X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes Unresolved cited work

Reference 15

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X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes Masui and Douglas Scott , doi =

Reference 16

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X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes Unresolved cited work

Reference 17

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X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes Unresolved cited work

Reference 18

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Observation 7064fe00-9d82-45a6-9ad7-dcab8094cb30 · outbound

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X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes Copi and Dominik J

Reference 19

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X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes Sánchez-Conde , doi =

Reference 20

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X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes Vernstrom and Douglas Scott and J

Reference 21

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X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes Unresolved cited work

Reference 22

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X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes Unresolved cited work

Reference 23

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X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes Unresolved cited work

Reference 24

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X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes Unresolved cited work

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X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes Unresolved cited work

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X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes Astrophysics Special issue Planck 2018 results I

Reference 27

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X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes Unresolved cited work

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X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes The rise and fall of a challenger: The Bullet Cluster in Λ cold dark matter simulations , volume =

Reference 29

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X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes Feretti and I.M

Reference 30

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X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes Story and K

Reference 31

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X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes Song and A

Reference 32

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X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes Matsuoka and N

Reference 33

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X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes Hartmann and Marco Ajello and Ramon Canal and Friedrich K

Reference 34

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X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes Unresolved cited work

Reference 35

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X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes Lisse and Andrew R

Reference 36

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X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes Unresolved cited work

Reference 37

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X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes The information content of cosmic infrared background anisotropies , volume =

Reference 38

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Observation 5af74554-931c-4364-9061-bf387a060c45 · outbound

This paper cites Kravtsov and Neal Dalal and Stefan Gottlöber , doi =.

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Observation 9b4d03a1-2d89-4bd5-91d5-ac516c089aab · outbound

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Observation a3cd21ec-df0a-4594-a034-a6a77bcb2aae · outbound

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Observation 34bc13ba-e605-486f-83e6-87fe30031573 · outbound

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Observation 4762d741-f7f2-4500-b143-3b1b4bded6b3 · outbound

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Observation 16779b3d-a041-4712-be21-a4d719c4ee1e · outbound

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Observation 858dcee5-9de3-4698-a930-4b24d0a37316 · outbound

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Observation cdfff556-3a53-47a2-bca6-0e29450ce161 · outbound

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Observation 5e1dfb7d-5976-4314-9e30-1a5ca48522f7 · outbound

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Observation c0c43a90-250e-43bc-84c7-5266da0ab737 · outbound

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Observation 9fbe928d-bcd8-4e53-af2a-437a67ca4c5c · outbound

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Observation 613c351b-a40b-47f1-96ee-5718c1c22603 · outbound

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source=arxiv_source observed=2026-06-26T13:47:51.674362Z digest=sha256:cf51eb84881a8423bc64e6f777cd06929d414611cd83a47e37745d2fa64b13f8

Observation 283ba6c0-0c91-4690-858a-f2b19f7cc4fe · outbound

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source=arxiv_source observed=2026-06-26T13:47:51.674362Z digest=sha256:e031165e670f51e63dcd24206adef0b2cf141d7bd93d20ac61d2480e4fcf78ea

Observation d0b35b7d-92d6-4202-923b-8f1f33112608 · outbound

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source=arxiv_source observed=2026-06-26T13:47:51.674362Z digest=sha256:5e93cccba3748ff9da1021c39886b33f294a10572b4054dd82675990933efa5f

Observation 304eb369-5294-4616-a9de-74f5d377f67e · outbound

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source=arxiv_source observed=2026-06-26T13:47:51.674362Z digest=sha256:0cf0590785c03efc810001126fc7a7f3701ac806fb53272e51a2c627babd9f19

Observation 9e26adb2-90b3-4c86-a281-4696dcabeb0b · outbound

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source=arxiv_source observed=2026-06-26T13:47:51.674362Z digest=sha256:2d9f5a62c73293d5403eaf7c3d4dec60b9925a421884baac73c6f15655338571

Observation 7cdaba1b-efa7-4b23-a072-ebd73030e47b · outbound

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source=arxiv_source observed=2026-06-26T13:47:51.674362Z digest=sha256:fc264d155639aab4dbd5f0df791732bf45c06088e02d6c7c58b67e79ae2abe81

Observation 6bdb405b-0433-4701-9bfc-61237dd497b3 · outbound

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source=arxiv_source observed=2026-06-26T13:47:51.674362Z digest=sha256:11fe96c7fe7ab1f07ef974cac54b89607930f77d91c2a8edf2dda1b9925a39e7

Observation 88af8d53-7b8c-46e6-be64-279b3b146377 · outbound

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source=arxiv_source observed=2026-06-26T13:47:51.674362Z digest=sha256:dbeaa79f4418ad46ce4435860f7a36cacc2acddef9735ce9aa16e0fbcccd570f

Observation 830b44c9-0941-4425-829e-69c117175eec · outbound

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source=arxiv_source observed=2026-06-26T13:47:51.674362Z digest=sha256:3c041174f8f130233fa834798842d59d84e9030c030e639acf8a60ba038bb439

Observation e416b78c-1184-4b12-aa18-fd5c29cf6fb8 · outbound

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source=arxiv_source observed=2026-06-26T13:47:51.674362Z digest=sha256:578cc252b563b43cc6a4eddbd7cb86cd3dd80d8abab2eaecf2209f7ef77e028e

Observation 991b37d7-2b6f-496b-aa72-08b51d9ef7a8 · outbound

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source=arxiv_source observed=2026-06-26T13:47:51.674362Z digest=sha256:69f17f0819e008b7730092a9c8df83e242f9e81b387b4ca9cb2163d2bf245032

Observation d3e0167d-38b9-4987-937d-b5665a86a7a0 · outbound

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Observation a9a09e08-e374-43ea-9072-a444cc908635 · outbound

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X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes X-ray clusters of galaxies as tracers of structure in the Universe , volume =

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source=arxiv_source observed=2026-06-26T13:47:51.674362Z digest=sha256:5fc4349fa42ac1b33f6158433c1e206e1f830f8b4dd9bc98cdfdd099d9d8f7ba

Observation 9add4a75-d935-47b6-9492-c95f8522dc1a · outbound

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X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes Corwin, Harold G

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Observation 66c500d8-d392-43bf-be38-1f40405a8b6f · outbound

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Observation 598f9d61-15d8-4ef2-9400-b5b0c78412d8 · outbound

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Observation f498f0fe-4b84-4d5d-83bc-3fbde6aa1c1d · outbound

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Observation 32e7a3c3-2816-41e0-921b-f9e7e9674144 · outbound

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Observation e6734ff6-40b2-4426-94aa-9d93c5e48468 · outbound

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Observation 2f88c8af-432e-482d-bd90-bd97ad1f5f57 · outbound

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Observation 6b2ac7e5-e1f0-486b-8e49-6875a2a80cf7 · outbound

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Observation ba80b145-ab5d-4e02-a98a-6bfe5853cd6b · outbound

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Observation f85e3fb3-318c-4e12-a0e1-6d087d115d0a · outbound

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source=arxiv_source observed=2026-06-26T13:47:51.674362Z digest=sha256:95090a042950ef20d147e67993072de440a5198094d3faefe083b256b4d51df4

Observation c4f8d30b-0289-4062-bda8-cafbfca90bd9 · outbound

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Observation 416662de-bb2a-4591-9a0f-ce6c42b3f9af · outbound

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source=arxiv_source observed=2026-06-26T13:47:51.674362Z digest=sha256:d9ffbc983f4d252f13ffdfc026e3a1fc3b23f9c7c9c8a84c35f3e70b377b9ac6

Observation 7a6ba9e5-d06c-420a-9686-5c22b60e4f1b · outbound

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source=arxiv_source observed=2026-06-26T13:47:51.674362Z digest=sha256:a76e3429e16e50b409eca445d0340cbc624c914c0c53a1a3de0740dc8bce371a

Observation 00637f6c-aa65-4d08-a4b8-edaf53684856 · outbound

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source=arxiv_source observed=2026-06-26T13:47:51.674362Z digest=sha256:d0739268d618673ed5a9f800516b99755dd0b2decc341d68aea692a8bdd88f2c

Observation 3754c125-b00d-4375-80c2-50871009ca7c · outbound

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Observation afdec5f8-d6df-4dea-bc12-cc8337ab2a27 · outbound

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X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes Cariddi and M

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Observation 2536f160-925a-4b50-b6db-eadcf9688975 · outbound

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X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes Lilly and Alvio Renzini and Marcella Carollo , doi =

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source=arxiv_source observed=2026-06-26T13:47:51.674362Z digest=sha256:76776de3742763511304fbd3a9e007a49aeb60dc31665584b11ebc4844c34b9b

Observation 9c785b4a-7ccf-4460-b09c-064c23b81a68 · outbound

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X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes Olave-Rojas and P

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source=arxiv_source observed=2026-06-26T13:47:51.674362Z digest=sha256:c3a9cbb7ef5f4e08d6a0c992b67ecf65ba1bbf330ec8af9b9bc0fe2126f4d27b

Observation fd204476-eacc-48cc-a77b-bfa49fae7019 · outbound

This paper cites Hennig and J.

X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes Hennig and J

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source=arxiv_source observed=2026-06-26T13:47:51.674362Z digest=sha256:33b62d6b24c9dcd968d02bb0501e11e991a9babfe9d8b55049f7e09324f2d14e

Observation 5adc81ed-e7a4-4182-8bbf-d92ae1b0b783 · outbound

This paper cites Cooper and Carlos Frenk and Adi Zolotov and Alyson M.

X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes Cooper and Carlos Frenk and Adi Zolotov and Alyson M

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source=arxiv_source observed=2026-06-26T13:47:51.674362Z digest=sha256:c84652885d7d735ba6da5a1ae785d72bab12a3f1b1cb9a5dde9db37281c01eeb

Observation a4807171-2940-4517-8b00-0648c016a59b · outbound

This paper cites an unresolved cited work.

X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes Unresolved cited work

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source=arxiv_source observed=2026-06-26T13:47:51.674362Z digest=sha256:70f37fb66e61dc1bda63a778ee258e9645acda8dd4e6579f93bbcde6006f0ec5

Observation 45164e7d-3bab-4365-84bb-a2220ad196aa · outbound

This paper cites Pasquali and R.

X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes Pasquali and R

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source=arxiv_source observed=2026-06-26T13:47:51.674362Z digest=sha256:8e6967b9b7e43871a0263d8757806d22d365d25e8af053de3176b3cfa2bec54c

Observation 8f0b87b1-215b-4e3a-9587-8e3b1d28aefc · outbound

This paper cites Investigating the projected phase space of Gaussian and non-Gaussian clusters , volume =.

X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes Investigating the projected phase space of Gaussian and non-Gaussian clusters , volume =

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source=arxiv_source observed=2026-06-26T13:47:51.674362Z digest=sha256:632b35744e66cb223d163d0f58e32c67764b42f6e76136bc584b24fee1a0a0c1

Observation f51c105d-ef8b-4af9-81db-fb39ae4043dc · outbound

This paper cites García-Lorenzo and I.

X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes García-Lorenzo and I

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source=arxiv_source observed=2026-06-26T13:47:51.674362Z digest=sha256:1015805e2611a3db429ebc5462196dd0c5df1987398da945b211d0dd957dc11c

Observation e29c472d-e4b1-40f9-844a-69a6468943a5 · outbound

This paper cites Willett and Chris J.

X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes Willett and Chris J

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source=arxiv_source observed=2026-06-26T13:47:51.674362Z digest=sha256:e0f46f0ee351c92ed26557897277623666a6f3214b60ea4ed483c413fb36d756

Observation e8db4a28-d1af-46da-b28d-7ac4c246d9cd · outbound

This paper cites Schlafly and Douglas P.

X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes Schlafly and Douglas P

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source=arxiv_source observed=2026-06-26T13:47:51.674362Z digest=sha256:aa374904ffc5ca97fdd4c9c470fb7fe1498db167d54a1ae446cd0e4a247d93f3

Observation fe15700b-3d4c-4f30-99c8-7820464cba82 · outbound

This paper cites <scp>parsec</scp> : stellar tracks and isochrones with the PAdova and TRieste Stellar Evolution Code , volume =.

X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes <scp>parsec</scp> : stellar tracks and isochrones with the PAdova and TRieste Stellar Evolution Code , volume =

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source=arxiv_source observed=2026-06-26T13:47:51.674362Z digest=sha256:d80d77f788977b3ec361775e773990fca0e779f98853b0c05ee06de95d40ccc6

Observation 5cf6dd0f-1757-4673-a2e6-282125be9850 · outbound

This paper cites an unresolved cited work.

X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes Unresolved cited work

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source=arxiv_source observed=2026-06-26T13:47:51.674362Z digest=sha256:b85373e894dbe7653ee42c5b53f171e0d40e752895b1f6bb5c485c87a719911c

Observation ff137568-64a7-42e3-9676-d9c58645bc33 · outbound

This paper cites Gratton and Gisella Clementini and Flavio Fusi Pecci , doi =.

X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes Gratton and Gisella Clementini and Flavio Fusi Pecci , doi =

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source=arxiv_source observed=2026-06-26T13:47:51.674362Z digest=sha256:10ce33fc122c466209f504826d6c06f167c32c3dccecd3d344b878da1b56f37e

Observation 488edaa9-8b45-49f5-8a9d-235050c73ca3 · outbound

This paper cites An extensive photometric catalogue of CALIFA galaxies , volume =.

X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes An extensive photometric catalogue of CALIFA galaxies , volume =

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source=arxiv_source observed=2026-06-26T13:47:51.674362Z digest=sha256:70e705bde0df31deab02592e635846fd1c7ce93be82bd9377e3b8623d97e3b93

Observation 4c47b0c6-2e91-4dca-b652-fa79687da759 · outbound

This paper cites Lotz and Joel Primack and Piero Madau , doi =.

X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes Lotz and Joel Primack and Piero Madau , doi =

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source=arxiv_source observed=2026-06-26T13:47:51.674362Z digest=sha256:9992e6d5332c21d2a5bd3d8a4953bc3541cf2ad71395c5699836f7539bfc2e91

Observation 79108439-8644-4202-b9dd-2ae59c142bb3 · outbound

This paper cites Méndez-Abreu and J.

X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes Méndez-Abreu and J

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source=arxiv_source observed=2026-06-26T13:47:51.674362Z digest=sha256:ca23d7e05142e66d1853ef3af220a30e851be84eee68ca7ad43cd7504a94d125

Observation a2aba671-5e69-47dd-b099-d1b0eb3bb2d1 · outbound

This paper cites Peng and Luis C.

X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes Peng and Luis C

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source=arxiv_source observed=2026-06-26T13:47:51.674362Z digest=sha256:e29563d6970d5936baddbbd9f93bc1d62ba9cd5cd90d1b46ce8eec715839d5a8

Observation f3382e43-e70b-413e-a3d3-778ab7164a2f · outbound

This paper cites Ellis and Christopher J.

X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes Ellis and Christopher J

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source=arxiv_source observed=2026-06-26T13:47:51.674362Z digest=sha256:fb1d6ed0b72ab59c1857e88101472a65937272d49e0a2196f916ee1e562dc172

Observation f3a3ef97-2c09-4055-b947-30a1a3bdd28f · outbound

This paper cites Martin and S.

X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes Martin and S

Reference 97

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source=arxiv_source observed=2026-06-26T13:47:51.674362Z digest=sha256:50a98fc46aef03a3ccded52398f26dd8154e60316ef632be68f962181aa2f647

Observation 8126485d-1b87-46fc-a549-03935154ade6 · outbound

This paper cites an unresolved cited work.

X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes Unresolved cited work

Reference 98

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source=arxiv_source observed=2026-06-26T13:47:51.674362Z digest=sha256:a709183afd79aabf92f0643301a5322b038eae7fd723f2a72edb19245bd80d4a

Observation bbf32c8b-6311-485b-90cc-52d24d8c9f21 · outbound

This paper cites an unresolved cited work.

X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes Unresolved cited work

Reference 99

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source=arxiv_source observed=2026-06-26T13:47:51.674362Z digest=sha256:f083b2466cabb72c42539e54987300eebc2c2c62e2bd472ba782bedb60c48815

Observation 282a614d-6571-42fe-88f0-a98a5baaa475 · outbound

This paper cites Trujillo and J.A.L.

X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG: Differences between cluster and group regimes Trujillo and J.A.L

Reference 100

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source=arxiv_source observed=2026-06-26T13:47:51.674362Z digest=sha256:c390fe71abcdab6afda2ee20f469d5f626fc8d40cd4df1d03e5301ed2eac04a1

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