Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-08-11T13:27:26.097886Z
Paper Citation Record · LEDGER
How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations
As of 13 August 2026, this Paper Citation Record lists 100 of 137 outbound references and 1 inbound Pith citation observation for arXiv:2412.13182.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-12T06:34:41.77262+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-10T04:15:20.585894Z
A source-named dated measurement, never combined with another source.
Source: cited_works
Reference resolution
100 of 137 outbound references displayed
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External citation measurements
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Outbound references
Observation 1d456a20-126e-4667-ad11-60fe32ba3469 · outbound
This paper cites , " * write output.state after.block = add.period write newline.
How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations , " * write output.state after.block = add.period write newline
Reference 1
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This paper cites write newline.
Reference 2
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Observation 72e92c17-bf02-4af5-b060-ab7661963999 · outbound
This paper cites T., Bower, R.
Reference 3
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Observation 25ef4224-5f52-48d6-9ab2-e07e9f7c70b4 · outbound
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Reference 4
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Observation 18e925a8-d5c0-49a6-95e8-969feddc97c2 · outbound
This paper cites R., et al.
Reference 5
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Observation 3e4bb584-85a6-4edc-bffd-cacdc3711334 · outbound
This paper cites 2022, , 663, L6.
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Observation 49de837e-f552-43f6-a7d8-3dc564dd783a · outbound
This paper cites Anisotropic thermal conduction in galaxy clusters with MHD in Gadget.
How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations Anisotropic thermal conduction in galaxy clusters with MHD in Gadget
Reference 8
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Observation 82edf7ab-13e8-44ed-bc2a-3f084d628e60 · outbound
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Reference 9
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Observation 242328d9-a538-4673-92a9-144f1f8f6ccb · outbound
This paper cites M., Lim, P.
Reference 10
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Observation 5a4a2cd2-dc2d-4363-bbb0-3698f3899558 · outbound
This paper cites E., Bulbul, E., Clerc, N., et al.
How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations E., Bulbul, E., Clerc, N., et al
Reference 11
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Observation cd3f38f2-3aea-4dfd-9fa4-cd3a450c7fce · outbound
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How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations E., Bulbul, E., Ghirardini, V., et al
Reference 12
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How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations Unresolved cited work
Reference 13
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Observation 2e81a3dd-81c1-4157-afc4-642b2267a892 · outbound
This paper cites J., Kannan , R., Vogelsberger , M., et al.
How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations J., Kannan , R., Vogelsberger , M., et al
Reference 14
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Observation 7bbeba1d-2b8a-4749-a800-498775859753 · outbound
This paper cites J., Kay, S.
Reference 15
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Observation b8bac64d-a324-441a-b824-6c7aeee557cf · outbound
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How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations J., Vogelsberger, M., Kannan, R., et al
Reference 16
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Observation aa7be21c-302c-48fc-b4d8-30afb658a17c · outbound
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How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations M., Murante, G., Arth, A., et al
Reference 17
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Observation 4339435f-b72b-4e59-8f32-9c799d20fec0 · outbound
This paper cites 2016, The Astrophysical Journal, 827, 112.
How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations 2016, The Astrophysical Journal, 827, 112
Reference 18
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Observation 1e0da41c-312f-45b9-b4ab-2bec2c613fc0 · outbound
This paper cites 2012, Monthly Notices of the Royal Astronomical Society, 420, 3545.
How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations 2012, Monthly Notices of the Royal Astronomical Society, 420, 3545
Reference 19
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Observation 257ee5fb-75a0-4a22-a2f0-9f7ee68802dd · outbound
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How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations 2018 a , , 481, 2213
Reference 21
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Observation 2aa449a4-ece0-4599-bc43-97220d349b77 · outbound
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Reference 22
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Observation 0e962e71-2643-4930-8fb4-88352b1f5791 · outbound
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Reference 23
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Observation f6e6ac7a-e9ab-4999-95a5-6bfbbbe30908 · outbound
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How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations Unresolved cited work
Reference 24
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Observation afc97c9a-b770-452f-a97e-678abbce2df8 · outbound
This paper cites On the Self-Similar Appearance of Galaxy Clusters in X-rays.
How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations On the Self-Similar Appearance of Galaxy Clusters in X-rays
Reference 25
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Observation 55a56f8b-ab85-4106-9308-34d61315dc66 · outbound
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How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations Unresolved cited work
Reference 26
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Observation a1960147-eb29-4989-8fcd-fab00abd2e91 · outbound
This paper cites 1952, Monthly Notices of the Royal Astronomical Society, 112, 195.
How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations 1952, Monthly Notices of the Royal Astronomical Society, 112, 195
Reference 27
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Observation e6535d76-83cb-434d-890e-4d665ce7c03e · outbound
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Reference 28
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Reference 29
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Observation ca705b35-4511-41ca-b8d2-f3f3ab13dc7b · outbound
This paper cites 2004, Monthly Notices of the Royal Astronomical Society, 348, 1078.
How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations 2004, Monthly Notices of the Royal Astronomical Society, 348, 1078
Reference 30
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Reference 31
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How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations Unresolved cited work
Reference 32
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How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations W., Donahue, M., Voit, G
Reference 33
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How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations W., Donahue, M., Voit, G
Reference 34
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How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations 2003, Publications of the Astronomical Society of the Pacific, 115, 763
Reference 35
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How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations 2007, Astronomy & Astrophysics, 466, 805
Reference 36
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Observation fd175197-814e-4dcf-9d79-ca67f9df601d · outbound
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How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations 2022, Astronomy & Astrophysics, 661, A11
Reference 37
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Observation 9c4a7744-5fa4-434d-933a-6e410904cd3c · outbound
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How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations u ggen, M., Kaiser, C., B \
Reference 38
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This paper cites 2005, Monthly Notices of the Royal Astronomical Society: Letters, 363, L91.
How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations 2005, Monthly Notices of the Royal Astronomical Society: Letters, 363, L91
Reference 39
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Observation 0ea835b7-6063-4499-a160-5def7d5a5848 · outbound
This paper cites First M87 Event Horizon Telescope Results. VIII. Magnetic Field Structure near The Event Horizon.
How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations First M87 Event Horizon Telescope Results. VIII. Magnetic Field Structure near The Event Horizon
Reference 40
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Observation 146157ac-551e-4a77-8aee-6a0278c81c29 · outbound
This paper cites 2018, Publications of the Astronomical Society of Japan, 70, 9.
How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations 2018, Publications of the Astronomical Society of Japan, 70, 9
Reference 41
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Observation bc1f1e1d-2de8-4f1c-9225-9046c6fd0e46 · outbound
This paper cites Full-sky photon simulation of clusters and active galactic nuclei in the soft X-rays for eROSITA.
How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations Full-sky photon simulation of clusters and active galactic nuclei in the soft X-rays for eROSITA
Reference 42
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Observation 22419506-e0d5-48d5-956c-9bd30bec8943 · outbound
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Observation b6952743-0c09-467d-82df-c111ded8fa28 · outbound
This paper cites J., D’Aloisio, A., & Natarajan, P.
How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations J., D’Aloisio, A., & Natarajan, P
Reference 44
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Observation c99f880d-c4a9-433b-90f4-cb0de2693034 · outbound
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Reference 45
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Observation d1d4fdd5-2497-4d03-abb3-38fc1382e200 · outbound
This paper cites 2005, nature, 433, 604.
How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations 2005, nature, 433, 604
Reference 46
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Observation 7b1f5ae7-4aff-4f78-9ded-860f0b206618 · outbound
This paper cites 2015, IAU General Assembly, 29, 2250156.
How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations 2015, IAU General Assembly, 29, 2250156
Reference 47
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Observation dc900171-0a6d-4e68-b3b4-917d185c20d9 · outbound
This paper cites 2004, The Astrophysical Journal, 606, L97.
How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations 2004, The Astrophysical Journal, 606, L97
Reference 48
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Observation f0721f3c-0bc7-4226-aabe-233b3d918574 · outbound
This paper cites 2017, Galaxies, 5, 35.
How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations 2017, Galaxies, 5, 35
Reference 49
- Resolution
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Observation f7039c86-7bce-4b3f-b0c2-5fbd3fabcdb7 · outbound
This paper cites 2005, Monthly Notices of the Royal Astronomical Society, 364, 753.
How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations 2005, Monthly Notices of the Royal Astronomical Society, 364, 753
Reference 50
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Observation 0e9e0864-b1b8-4539-93fe-4c6869abdbbc · outbound
This paper cites M., & O’Sullivan, E.
Reference 51
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Observation 3c41360a-ff65-4a7c-921a-a9eb94d4138d · outbound
This paper cites 2019, Astronomy and Astrophysics, 621, A40.
How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations 2019, Astronomy and Astrophysics, 621, A40
Reference 52
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Observation 84b66d6e-1103-4add-90e3-0ffe2c407774 · outbound
This paper cites 2003, Monthly Notices of the Royal Astronomical Society, 344, L27.
How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations 2003, Monthly Notices of the Royal Astronomical Society, 344, L27
Reference 53
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 385ae79d-b901-4d44-9057-2f76b595a76f · outbound
This paper cites an unresolved cited work.
How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations Unresolved cited work
Reference 54
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Source-reported events for the cited work
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Observation 751afda4-f37d-4dc4-b05e-bc33709c82b6 · outbound
This paper cites 2010, Monthly Notices of the Royal Astronomical Society, 401, 1670.
How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations 2010, Monthly Notices of the Royal Astronomical Society, 401, 1670
Reference 55
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Unavailable: canonical work link unavailable.
Observation 9e142095-fdcc-419c-9feb-71e8238e31bc · outbound
This paper cites S., et al.
Reference 56
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T13:27:25.882389Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d249e9fd-2faf-48a5-8e1c-9ef383e93d59 · outbound
This paper cites an unresolved cited work.
How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations Unresolved cited work
Reference 57
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T13:27:25.887039Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 56209aab-aa83-4f51-babb-d0c26a2c03d8 · outbound
This paper cites J., & Pimbblet, K.
Reference 58
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T13:27:25.891901Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 2fef8dfd-e28b-4d41-9ecc-ab25ee5c9786 · outbound
This paper cites an unresolved cited work.
How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations Unresolved cited work
Reference 59
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T13:27:25.896255Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation b8fd2536-24a6-4b98-8fc9-9161212b4cf7 · outbound
This paper cites AGN jet power and feedback characterised by Bondi accretion in brightest cluster galaxies.
How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations AGN jet power and feedback characterised by Bondi accretion in brightest cluster galaxies
Reference 60
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-08-11T13:27:26.386542Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation d0d33b41-a8c1-422d-879e-b51da70cc2de · outbound
This paper cites 2016, Publications of the Astronomical Society of Japan, 68, 26.
How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations 2016, Publications of the Astronomical Society of Japan, 68, 26
Reference 61
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T13:27:25.905803Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation b8bca731-299e-41e5-ac86-e6d6f2f8bbaa · outbound
This paper cites 2013, Astronomische Nachrichten, 334, 394.
How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations 2013, Astronomische Nachrichten, 334, 394
Reference 62
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T13:27:25.911285Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 483a1d4d-b662-42a6-ad5c-740e4f09d06a · outbound
This paper cites L., et al.
Reference 63
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T13:27:25.916212Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e6f31f8a-85e1-46cb-90fc-890f6be745da · outbound
This paper cites E., Bulbul, E., et al.
How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations E., Bulbul, E., et al
Reference 64
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-11T13:27:27.637412Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 286e9021-f620-4c84-a7ee-b05e885e821b · outbound
This paper cites 2022, Astrophysics Source Code Library, ascl.
How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations 2022, Astrophysics Source Code Library, ascl
Reference 65
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-11T13:27:27.620019Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 2564595e-a3f3-40e6-a855-fb72d09b126f · outbound
This paper cites H., Zaritsky, D., & Zabludoff, A.
How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations H., Zaritsky, D., & Zabludoff, A
Reference 66
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-11T13:27:27.599337Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 72b94e3a-aa45-483f-969b-103928cdd842 · outbound
This paper cites & Mathews, W.
Reference 67
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-11T13:27:27.577475Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 2cc02d6a-9e27-45ab-8b56-a2730b0b2315 · outbound
This paper cites J., Dolag , K., & Liu , J.
How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations J., Dolag , K., & Liu , J
Reference 68
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-11T13:27:27.557603Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 96bbf416-f48a-42e2-8818-457036b0d8c7 · outbound
This paper cites 2001, Clusters of galaxies and the high redshift universe observed in X-rays.
How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations 2001, Clusters of galaxies and the high redshift universe observed in X-rays
Reference 69
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-11T13:27:27.532281Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 404ceebe-56a1-47bc-a8c1-692ad4421715 · outbound
This paper cites 2017, Monthly Notices of the Royal Astronomical Society, 470, 166.
How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations 2017, Monthly Notices of the Royal Astronomical Society, 470, 166
Reference 70
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-11T13:27:27.513189Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 9b10ce03-3943-4ed8-963c-7774eaf5385c · outbound
This paper cites R., Millman, K.
Reference 71
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T13:27:25.954683Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation eaf3adda-3186-46f8-9ce4-761bc5e1c1df · outbound
This paper cites 2014, Monthly Notices of the Royal Astronomical Society, 442, 2304.
How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations 2014, Monthly Notices of the Royal Astronomical Society, 442, 2304
Reference 72
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T13:27:25.959621Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation caf86a93-0399-4f63-8b9b-83904477f0a0 · outbound
This paper cites S., Donahue, M., Hicks, A., & Barthelemy, R.
How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations S., Donahue, M., Hicks, A., & Barthelemy, R
Reference 73
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-11T13:27:27.467122Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 6ec17835-bbe5-4599-9387-c9fe3a50176e · outbound
This paper cites 2017, The Astrophysical Journal, 837, 51.
How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations 2017, The Astrophysical Journal, 837, 51
Reference 74
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-11T13:27:27.448480Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation ceed75eb-3123-419d-b519-053f2541e56c · outbound
This paper cites & Lyttleton, R.
Reference 75
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-11T13:27:27.429993Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 99aa5265-ea70-4c15-9d00-7be87a4500f2 · outbound
This paper cites & Dale, D.
Reference 76
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-11T13:27:27.412078Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 6a17fdd3-e9c5-4e8e-bf0f-764e98dc94a3 · outbound
This paper cites 2016, Monthly Notices of the Royal Astronomical Society, 457, 4340.
How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations 2016, Monthly Notices of the Royal Astronomical Society, 457, 4340
Reference 77
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-11T13:27:27.394303Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation b419b874-73c2-4a04-b6c8-7c7602d677d6 · outbound
This paper cites M., Dunkley, J., et al.
How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations M., Dunkley, J., et al
Reference 78
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T13:27:25.988634Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 489524ff-984c-4a98-ab63-4dafb1eb9637 · outbound
This paper cites 2013, Astronomy & Astrophysics, 555, A66.
How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations 2013, Astronomy & Astrophysics, 555, A66
Reference 79
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-11T13:27:27.366662Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation d342022d-cbaf-4ce8-9728-6444a1b1782f · outbound
This paper cites M., McCarthy, I.
Reference 80
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-11T13:27:27.349965Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 34f8fbdf-1765-4e3a-aaf8-efc4633a8021 · outbound
This paper cites 2024, Astronomy & Astrophysics.
How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations 2024, Astronomy & Astrophysics
Reference 81
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-11T13:27:27.333945Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 74d8d293-d40b-4a29-b672-a7b4754513e0 · outbound
This paper cites 2022, Astronomy & Astrophysics, 661, A2.
How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations 2022, Astronomy & Astrophysics, 661, A2
Reference 82
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-11T13:27:27.317867Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation c2ac934f-62bf-4631-ac92-9db8d9a4d15a · outbound
This paper cites 2020, The Astrophysical Journal, 892, 102.
How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations 2020, The Astrophysical Journal, 892, 102
Reference 83
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-11T13:27:27.302833Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 0a6cddcc-7fa8-4534-9527-0e84a2353331 · outbound
This paper cites Detecting Galaxy Groups and AGNs populating the local Universe in the eROSITA era.
How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations Detecting Galaxy Groups and AGNs populating the local Universe in the eROSITA era
Reference 84
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T13:27:26.021555Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 99195edb-3ff1-4975-bbb7-02130dc794b5 · outbound
This paper cites 2012, Monthly Notices of the Royal Astronomical Society, 421, 1583.
How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations 2012, Monthly Notices of the Royal Astronomical Society, 421, 1583
Reference 85
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-11T13:27:27.285847Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 4a4609d3-d423-4fc5-847b-d9ff2d6910f1 · outbound
This paper cites 2004, Monthly Notices of the Royal Astronomical Society, 354, 10.
How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations 2004, Monthly Notices of the Royal Astronomical Society, 354, 10
Reference 86
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-11T13:27:27.270917Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 4d20d283-f16c-4a4f-8d20-50e40770ec77 · outbound
This paper cites G., Babul, A., Bower, R.
How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations G., Babul, A., Bower, R
Reference 87
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-11T13:27:27.254324Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 47cb7e48-c5f4-4c49-b4d8-4c3e20b19282 · outbound
This paper cites an unresolved cited work.
How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations Unresolved cited work
Reference 88
- Resolution
- unresolved
- raw_fallback, observed 2026-08-11T13:27:27.235562Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 8ec21338-3d29-4e8d-95cd-a6fc99c44d7b · outbound
This paper cites A., Vikhlinin , A., et al.
How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations A., Vikhlinin , A., et al
Reference 89
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-11T13:27:27.218449Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation db22aea7-78b5-4590-857d-6be8d237b73b · outbound
This paper cites 2018, The Astrophysical Journal, 858, 45.
How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations 2018, The Astrophysical Journal, 858, 45
Reference 90
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-11T13:27:27.202315Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 0d95ac43-15f6-4cda-9aa1-4044b1f4cdc2 · outbound
This paper cites M., Burns, J.
Reference 91
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-11T13:27:27.184868Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation c4811d49-fb5c-46e7-ba2d-b3f1c48e09c7 · outbound
This paper cites V., & Vikhlinin, A.
Reference 92
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-11T13:27:27.169220Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation abcebf1d-d693-4e92-85be-eb2f9300174a · outbound
This paper cites an unresolved cited work.
How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations Unresolved cited work
Reference 93
- Resolution
- unresolved
- raw_fallback, observed 2026-08-11T13:27:27.152460Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 1eb61324-866e-42b9-b1e4-b2596d3192f9 · outbound
This paper cites 2014, Monthly Notices of the Royal Astronomical Society, 438, 2341.
How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations 2014, Monthly Notices of the Royal Astronomical Society, 438, 2341
Reference 94
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-11T13:27:27.136513Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 967aeec6-e4be-439d-8090-7a13a452d753 · outbound
This paper cites 2022, Astronomy & Astrophysics, 661, A13.
How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations 2022, Astronomy & Astrophysics, 661, A13
Reference 95
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-11T13:27:27.119583Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 581a7d07-d9b3-401d-b164-9d2f4892a8b8 · outbound
This paper cites 2003, The Astrophysical Journal, 590, 207.
How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations 2003, The Astrophysical Journal, 590, 207
Reference 96
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-11T13:27:27.102615Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 78b96444-d939-4ae3-95be-a49f1b95cbf8 · outbound
This paper cites 2013, , 431, 1487.
Reference 97
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-11T13:27:27.087593Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation e89da3b6-51d2-42ec-ab4e-3db675b83670 · outbound
This paper cites & Quilis, V.
Reference 98
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-11T13:27:27.068711Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation e65a2e72-970d-4181-bd24-59b138318a03 · outbound
This paper cites B., Babul, A., McCarthy, I.
How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations B., Babul, A., McCarthy, I
Reference 99
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-11T13:27:27.050720Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation c9572cb2-d0b3-4633-8d23-588c4417d40e · outbound
This paper cites an unresolved cited work.
How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations Unresolved cited work
Reference 100
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T13:27:26.097886Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Pith citing papers
Observation c5ed870b-69d4-41c1-bb70-4a840fa519d5 · inbound
Average soft X-ray surface brightness profile of massive galaxy clusters in Magneticum simulations cites this paper.
Average soft X-ray surface brightness profile of massive galaxy clusters in Magneticum simulations How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations
Reference 21
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T04:15:20.585894Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.