Pith. sign in

Paper Citation Record · LEDGER

Optimal parameterizations for observational constraints on thawing dark energy

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 17 inbound Pith citation observations for arXiv:2504.02028.

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

pith.paper-citation-record.v1
2504.02028 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 17 of 17 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-10T06:31:04.303077+00:00

measured 17 of 17 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-08T21:04:17.889014Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-10T18:27:31.773514Z

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 7e73a534-0df9-46d4-8d35-93bfd7e2bf2e · inbound

Robustness of dark energy phenomenology across different parameterizations cites this paper.

Robustness of dark energy phenomenology across different parameterizations Optimal parameterizations for observational constraints on thawing dark energy

Reference 102

Resolution
unresolved
no resolver link, observed 2026-08-08T21:04:17.889014Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T21:04:17.889014Z digest=sha256:11b1436a57339fde344dc5adebdebd4f7d4231ee5a1f0be5a039b03138698ede

Observation 43b02178-83ce-46c2-8708-3d23c71b8c75 · inbound

Scalar field dark energy models: Current and forecast constraints cites this paper.

Scalar field dark energy models: Current and forecast constraints Optimal parameterizations for observational constraints on thawing dark energy

Reference 32

Resolution
unresolved
no resolver link, observed 2026-08-08T14:22:01.325266Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T14:22:01.325266Z digest=sha256:4d27343f5a8b906508a29292707152ebeb3c7650fa7019a6b8bef6d66574188b

Observation f2f2dc9b-efda-4c00-a789-95f414f9b268 · inbound

Examining Quintessence Models with DESI Data cites this paper.

Examining Quintessence Models with DESI Data Optimal parameterizations for observational constraints on thawing dark energy

Reference 24

Resolution
unresolved
no resolver link, observed 2026-08-07T14:30:36.968298Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T14:30:36.968298Z digest=sha256:3ca6e9aa022e778b4880855302686b50e9a4c911f2c8fe168ec099280e2e22ba

Observation 31a6a164-050c-44f7-a12f-b2c7245ccb30 · inbound

Topological defects as effective dynamical dark energy cites this paper.

Topological defects as effective dynamical dark energy Optimal parameterizations for observational constraints on thawing dark energy

Reference 45

Resolution
unresolved
no resolver link, observed 2026-08-07T04:41:33.682404Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T04:41:33.682404Z digest=sha256:1c60830fa513b75fae468d4dbb1ebc303d3773c2b8cc13d19db89b0eb533419f

Observation ec77d415-0eef-4134-84b9-77ad77664286 · inbound

Constraints on Dark Energy Models Using Late Universe Probes cites this paper.

Constraints on Dark Energy Models Using Late Universe Probes Optimal parameterizations for observational constraints on thawing dark energy

Reference 182

Resolution
unresolved
no resolver link, observed 2026-08-07T00:54:49.896395Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T00:54:49.896395Z digest=sha256:93db1b9feb13fd482c5c7052a17851098b42468339f75a77655465fcf45a3474

Observation 17e85eb2-9336-436f-a590-6a05d889c977 · inbound

Simple quintessence models in light of DESI-BAO observations cites this paper.

Simple quintessence models in light of DESI-BAO observations Optimal parameterizations for observational constraints on thawing dark energy

Reference 11

Resolution
unresolved
no resolver link, observed 2026-08-07T00:43:07.694970Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T00:43:07.694970Z digest=sha256:6276557b7f662cd68e42d4c0a739fc2ef4db0ef5afdfcd87db570a1e2399ad2e

Observation f19b9e80-699f-4186-b9c3-6d056d7fcb02 · inbound

Updated observational constraints on $\phi$CDM dynamical dark energy cosmological models cites this paper.

Updated observational constraints on $\phi$CDM dynamical dark energy cosmological models Optimal parameterizations for observational constraints on thawing dark energy

Reference 38

Resolution
unresolved
no resolver link, observed 2026-08-04T13:43:12.248748Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T13:43:12.248748Z digest=sha256:9ff1a6a34d836a8c0b6135c4f19dd2e9626e61d4e24f23fb473a26fe3438d982

Observation 26de8e1f-35a1-4c79-bc4a-13f5e84235ae · inbound

BAO miscalibration cannot rescue late-time solutions to the Hubble tension cites this paper.

BAO miscalibration cannot rescue late-time solutions to the Hubble tension Optimal parameterizations for observational constraints on thawing dark energy

Reference 289

Resolution
unresolved
no resolver link, observed 2026-08-04T12:53:56.991296Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T12:53:56.991296Z digest=sha256:594a71abb382a57a31899ef08d66482ddb102e0a821049ef716beb66392651a7

Observation 39e4e25f-f8e8-4833-84b9-73bb1cefe0e7 · inbound

Beyond CPL: Evidence for dynamical dark energy in three-parameter models cites this paper.

Beyond CPL: Evidence for dynamical dark energy in three-parameter models Optimal parameterizations for observational constraints on thawing dark energy

Reference 76

Resolution
verified exact
arxiv_id, observed 2026-05-18T10:46:16.331469Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-05-18T10:45:16.985887Z digest=sha256:9bc77c878b9bddcfd5855907f5fe9035bbf821b49b8fcc743a3bae4044faaa92

Observation 8b16577a-a290-4bfb-9445-f7f51469c443 · inbound

Observational constraints on early time non-phantom behaviour of dynamical dark energy cites this paper.

Observational constraints on early time non-phantom behaviour of dynamical dark energy Optimal parameterizations for observational constraints on thawing dark energy

Reference 76

Resolution
unresolved
no resolver link, observed 2026-08-03T14:40:55.505279Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T14:40:55.505279Z digest=sha256:24aea407cb3293d302a10809c4601f8de2487e11a25048b109b05602f16ab6ea

Observation bad880ba-6014-46b1-8964-7df785cf881a · inbound

Realizing the phantom-divide crossing with vector and scalar fields cites this paper.

Realizing the phantom-divide crossing with vector and scalar fields Optimal parameterizations for observational constraints on thawing dark energy

Reference 34

Resolution
unresolved
no resolver link, observed 2026-08-03T07:07:15.621574Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T07:07:15.621574Z digest=sha256:87061427d53566dfd1b370eb659ba5abec3b8547dbc426f279894fc43d284751

Observation de5b9e86-8c3f-41ef-ae3d-63bd81e7a58d · inbound

Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy cites this paper.

Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy Optimal parameterizations for observational constraints on thawing dark energy

Reference 43

Resolution
unresolved
no resolver link, observed 2026-07-15T14:51:12.413085Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-15T14:51:12.413085Z digest=sha256:2a5d6cd131a4bdb055cd004d479472aca0d445225232f6e1411c752dc7bf3fd1

Observation 7e3036e4-5458-44a9-94ae-34f80dfd4024 · inbound

Is the $w_0w_a$CDM cosmological parameterization evidence for dark energy dynamics partially caused by the excess smoothing of Planck PR4 CMB anisotropy data? cites this paper.

Is the $w_0w_a$CDM cosmological parameterization evidence for dark energy dynamics partially caused by the excess smoothing of Planck PR4 CMB anisotropy data? Optimal parameterizations for observational constraints on thawing dark energy

Reference 42

Resolution
verified exact
arxiv_id, observed 2026-05-13T17:38:03.001116Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-05-13T17:33:08.222231Z digest=sha256:c79492192e8f94581bd52d78533466e887493cc208f2a71460524e5cdae13e4e

Observation 58c5a19f-9581-4db0-8389-986567712019 · inbound

Breaking Free from the Swampland of Impossible Universes through the DESI Portal cites this paper.

Breaking Free from the Swampland of Impossible Universes through the DESI Portal Optimal parameterizations for observational constraints on thawing dark energy

Reference 59

Resolution
unresolved
no resolver link, observed 2026-08-02T14:29:21.096514Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-02T14:29:21.096514Z digest=sha256:6a73a9d1d2ae0127aebbc7db0160f9523e54a70ff7e5fa88111ccbb0254ec2da

Observation 8d984edd-1a20-45de-8f8c-5907f2b49b3b · inbound

Quintessential $\alpha$-attractors fit DESI cites this paper.

Quintessential $\alpha$-attractors fit DESI Optimal parameterizations for observational constraints on thawing dark energy

Reference 33

Resolution
metadata mismatch
arxiv_id, observed 2026-07-02T00:16:24.678328Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-06-28T13:29:35.220988Z digest=sha256:4c6f360bdfa404535b61b209669031701da9c0f32f6c861bba3f87569214452d

Observation ce0367a0-e7d2-4c57-85ac-9221319983dd · inbound

The Status of Single Scalar Field Dark Energy cites this paper.

The Status of Single Scalar Field Dark Energy Optimal parameterizations for observational constraints on thawing dark energy

Reference 57

Resolution
verified exact
local_arxiv, observed 2026-07-10T18:27:31.774827Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-07-10T18:19:17.740185Z digest=sha256:e119a1d997ad390cb588d70393bbad86b1381794f772cfa5c584004d433fd859

Observation cea9599a-ddd8-4d21-ae44-ea65191960ff · inbound

Phantom-divide crossing and suppressed structure growth in kinetically braided dark energy with momentum exchange cites this paper.

Phantom-divide crossing and suppressed structure growth in kinetically braided dark energy with momentum exchange Optimal parameterizations for observational constraints on thawing dark energy

Reference 42

Resolution
unresolved
no resolver link, observed 2026-08-01T15:41:41.992784Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T15:41:41.992784Z digest=sha256:4427741067e82cd3dc08c02d821da46717cab6c0b55d235dc02f139be6c61d6a