Paper Citation Record · LEDGER

CSST Cosmological Emulator I: Matter Power Spectrum Emulation with one percent accuracy to k = 10 h/Mpc

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:2502.11160.

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

pith.paper-citation-record.v1
2502.11160 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 6 of 6 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-11T06:34:44.6726+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T04:48:07.686518Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-06-30T15:14:47.254587Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
unresolved0
parse uncertain0
malformed identifier0
metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation aba3464c-6ec0-439e-8d2e-0f5d3eef8922 · inbound

CSST Cosmological Emulator II: Generalized Accurate Halo Mass Function Emulation cites this paper.

CSST Cosmological Emulator II: Generalized Accurate Halo Mass Function Emulation CSST Cosmological Emulator I: Matter Power Spectrum Emulation with one percent accuracy to k = 10 h/Mpc

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-07T04:48:07.686518Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 232da093-ff67-41b6-977d-47bdc3af423f · inbound

Artifacts in Halo Shapes: Imprints of the Initial Condition cites this paper.

Artifacts in Halo Shapes: Imprints of the Initial Condition CSST Cosmological Emulator I: Matter Power Spectrum Emulation with one percent accuracy to k = 10 h/Mpc

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-06T15:06:54.407449Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8a5518ee-8f58-4c6b-a444-825a206f95a9 · inbound

Extending CSST Emulator to post-DESI era cites this paper.

Extending CSST Emulator to post-DESI era CSST Cosmological Emulator I: Matter Power Spectrum Emulation with one percent accuracy to k = 10 h/Mpc

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-04T10:39:32.917085Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3716f5bb-b5ac-41ae-afcf-ddbb6cda853e · inbound

The first AKRA mass map reconstruction from HSC Y1 data cites this paper.

The first AKRA mass map reconstruction from HSC Y1 data CSST Cosmological Emulator I: Matter Power Spectrum Emulation with one percent accuracy to k = 10 h/Mpc

Reference 72

Resolution: verified exact; arxiv_id, observed 2026-05-17T22:40:23.658871Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 3f2c4e84-7091-451b-9143-fb60350316d9 · inbound

Cosmological constraints from neighbor-density-weighted marked correlation functions cites this paper.

Cosmological constraints from neighbor-density-weighted marked correlation functions CSST Cosmological Emulator I: Matter Power Spectrum Emulation with one percent accuracy to k = 10 h/Mpc

Reference 78

Resolution: verified exact; arxiv_id, observed 2026-05-25T03:30:17.354329Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation af43e219-7c79-4e8b-83c2-1cf7d8f1978a · inbound

Cosmological constraints from neighbor-density-weighted marked correlation functions cites this paper.

Cosmological constraints from neighbor-density-weighted marked correlation functions CSST Cosmological Emulator I: Matter Power Spectrum Emulation with one percent accuracy to k = 10 h/Mpc

Reference 78

Resolution: verified exact; arxiv_id, observed 2026-06-30T15:14:47.255883Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.