Pith. sign in

Paper Citation Record · LEDGER

Determination of neutron star radius from pulse profile modeling using profile likelihood

As of 17 August 2026, this Paper Citation Record lists 28 of 28 outbound references and 0 inbound Pith citation observations for arXiv:2607.11154.

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

pith.paper-citation-record.v1
2607.11154 v1

Coverage vector

measured 28 of 28 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-07-14T06:38:48.754265Z

measured 28 of 28 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-17T06:30:58.91139+00:00

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

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

Source: cited_works

Reference resolution

28 of 28 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved28
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

Observation 35bd1859-e23e-4f34-8a32-9c052b72aa4a · outbound

This paper cites an unresolved cited work.

Determination of neutron star radius from pulse profile modeling using profile likelihood Unresolved cited work

Reference 1

Resolution
unresolved
no resolver link, observed 2026-07-14T06:38:48.754265Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-14T06:38:48.754265Z digest=sha256:18362754cea0f4ccb1e0b2cd7a67990871bc3140ce4d0f7aac7da47c1020f94c

Observation b9cc448a-530c-4552-86b9-2b677307ee0e · outbound

This paper cites Measuring the neutron star equation of state using X-ray timing.

Determination of neutron star radius from pulse profile modeling using profile likelihood Measuring the neutron star equation of state using X-ray timing

Reference 2

Resolution
unresolved
no resolver link, observed 2026-07-14T06:38:48.754265Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-14T06:38:48.754265Z digest=sha256:6e49dc0a734f52ec684ebaba5c4da2b259d00f319cb8b1c1f295772da441d312

Observation 6df10ca7-bc9d-43f0-8b0a-3ad1e579e476 · outbound

This paper cites A NICER view of the millisecond pulsar PSR J2124$-$3358: evidence for a helium atmosphere.

Determination of neutron star radius from pulse profile modeling using profile likelihood A NICER view of the millisecond pulsar PSR J2124$-$3358: evidence for a helium atmosphere

Reference 3

Resolution
unresolved
no resolver link, observed 2026-07-14T06:38:48.754265Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-14T06:38:48.754265Z digest=sha256:a5789425c60857aed5e68111e7d7af1ce8d14d701d3b416fdb2aecaa830344f3

Observation 45aff4da-48e7-42db-a9af-1a907692923d · outbound

This paper cites Masses, Radii, and Equation of State of Neutron Stars.

Determination of neutron star radius from pulse profile modeling using profile likelihood Masses, Radii, and Equation of State of Neutron Stars

Reference 4

Resolution
unresolved
no resolver link, observed 2026-07-14T06:38:48.754265Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-14T06:38:48.754265Z digest=sha256:8d392eae24fc1b00083a3e0a55d49ff2aa01caa94aa51108b4210bda8a1bcb60

Observation b37f31ee-19d5-431b-a3c3-96616362e3df · outbound

This paper cites an unresolved cited work.

Determination of neutron star radius from pulse profile modeling using profile likelihood Unresolved cited work

Reference 5

Resolution
unresolved
no resolver link, observed 2026-07-14T06:38:48.754265Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-14T06:38:48.754265Z digest=sha256:737dc1a7f8f787cee3e992094fe4036c38b376c40c2f37e1a902c57826b570f8

Observation 4852faf0-3aea-4c2d-a2c1-160f49360167 · outbound

This paper cites Universality of the Acceleration Due to Gravity on the Surface of a Rapidly Rotating Neutron Star.

Determination of neutron star radius from pulse profile modeling using profile likelihood Universality of the Acceleration Due to Gravity on the Surface of a Rapidly Rotating Neutron Star

Reference 6

Resolution
unresolved
no resolver link, observed 2026-07-14T06:38:48.754265Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-14T06:38:48.754265Z digest=sha256:18ff280a110454121e928c9a19d642cf82eb293cdd808485bff0604b1d1e586e

Observation 5a80641a-2438-41c7-b073-1925e47faabc · outbound

This paper cites Bogdanov, G.

Determination of neutron star radius from pulse profile modeling using profile likelihood Bogdanov, G

Reference 7

Resolution
unresolved
no resolver link, observed 2026-07-14T06:38:48.754265Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-14T06:38:48.754265Z digest=sha256:89027f2c9cafe260ede1101110808fb1daebd36aad770e85885426bc54b4c7fd

Observation e70f897b-bde2-4dc9-9b2f-8da73fa349e5 · outbound

This paper cites Bayesian Methods in Cosmology.

Determination of neutron star radius from pulse profile modeling using profile likelihood Bayesian Methods in Cosmology

Reference 8

Resolution
unresolved
no resolver link, observed 2026-07-14T06:38:48.754265Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-14T06:38:48.754265Z digest=sha256:36b4554c285ced6847af06ef31f340c1cfb141e9d55999094e8c2cae3b838632

Observation 77be4a10-17fc-439c-9622-2190c0b2be58 · outbound

This paper cites Multimodal nested sampling: an efficient and robust alternative to MCMC methods for astronomical data analysis.

Determination of neutron star radius from pulse profile modeling using profile likelihood Multimodal nested sampling: an efficient and robust alternative to MCMC methods for astronomical data analysis

Reference 9

Resolution
unresolved
no resolver link, observed 2026-07-14T06:38:48.754265Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-14T06:38:48.754265Z digest=sha256:eaf885117712ded5a670c30faf490a4195b8b1e3abc1329938a23532ce74f14e

Observation 05d502cd-7a00-4813-a09d-9dab44842ae3 · outbound

This paper cites The Radius of the High-mass Pulsar PSR J0740+6620 with 3.6 yr of NICER Data.

Determination of neutron star radius from pulse profile modeling using profile likelihood The Radius of the High-mass Pulsar PSR J0740+6620 with 3.6 yr of NICER Data

Reference 10

Resolution
unresolved
no resolver link, observed 2026-07-14T06:38:48.754265Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-14T06:38:48.754265Z digest=sha256:5f22c1c1212495351327a8d2028a4618d94a56c36e4164a719a92041aed2cbb0

Observation cf3cb5ca-4584-4158-9dad-6e893b8f375b · outbound

This paper cites A More Precise Measurement of the Radius of PSR J0740+6620 Using Updated NICER Data.

Determination of neutron star radius from pulse profile modeling using profile likelihood A More Precise Measurement of the Radius of PSR J0740+6620 Using Updated NICER Data

Reference 11

Resolution
unresolved
no resolver link, observed 2026-07-14T06:38:48.754265Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-14T06:38:48.754265Z digest=sha256:af50d7371335bec699d3dd17605d7123a512417a4e213084feec196b76522fb2

Observation 39dc24a2-2b73-49c1-bb7c-2656d3cd7f7e · outbound

This paper cites Mauviard, S.

Determination of neutron star radius from pulse profile modeling using profile likelihood Mauviard, S

Reference 12

Resolution
unresolved
no resolver link, observed 2026-07-14T06:38:48.754265Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-14T06:38:48.754265Z digest=sha256:6ba661cd2510eda26c61d8abdf24607149d2ec8068ffbe74f607b9e5d93d2c2f

Observation fb9aa7b1-fd13-4484-bd63-20c984ea8c5c · outbound

This paper cites Hoogkamer, Y.

Determination of neutron star radius from pulse profile modeling using profile likelihood Hoogkamer, Y

Reference 13

Resolution
unresolved
no resolver link, observed 2026-07-14T06:38:48.754265Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-14T06:38:48.754265Z digest=sha256:5971e50b3da42922c06c3058906dc881162641f09d5c2982e443f352d128af44

Observation 6c3bd4ae-1647-4345-9319-f4568c53116d · outbound

This paper cites Bilby-MCMC: An MCMC sampler for gravitational-wave inference.

Determination of neutron star radius from pulse profile modeling using profile likelihood Bilby-MCMC: An MCMC sampler for gravitational-wave inference

Reference 14

Resolution
unresolved
no resolver link, observed 2026-07-14T06:38:48.754265Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-14T06:38:48.754265Z digest=sha256:0cae706c6147acf8b3d7ae3de14f291da57155ed047acc8a43c4d70b5cb5a610

Observation d01c0019-b24f-4989-a396-4bb1c17de286 · outbound

This paper cites UltraNest -- a robust, general purpose Bayesian inference engine.

Determination of neutron star radius from pulse profile modeling using profile likelihood UltraNest -- a robust, general purpose Bayesian inference engine

Reference 15

Resolution
unresolved
no resolver link, observed 2026-07-14T06:38:48.754265Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-14T06:38:48.754265Z digest=sha256:575a0d969a8111f02ef4ada75439b12d3bc80df14bfe86ce478e4f877f6deb3e

Observation e30f1f09-08b5-4461-81d9-9399e48d7c87 · outbound

This paper cites Comparison of Step Samplers for Nested Sampling.

Determination of neutron star radius from pulse profile modeling using profile likelihood Comparison of Step Samplers for Nested Sampling

Reference 16

Resolution
unresolved
no resolver link, observed 2026-07-14T06:38:48.754265Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-14T06:38:48.754265Z digest=sha256:17ce6ea7fc998e7b617665c0ce58492db88d8d9f34db67c257781bb399b72b8d

Observation 0fb38ac0-05ea-4990-ab1b-0fadc656ffca · outbound

This paper cites A fast test to assess the impact of marginalization in Monte Carlo analyses, and its application to cosmology.

Determination of neutron star radius from pulse profile modeling using profile likelihood A fast test to assess the impact of marginalization in Monte Carlo analyses, and its application to cosmology

Reference 17

Resolution
unresolved
no resolver link, observed 2026-07-14T06:38:48.754265Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-14T06:38:48.754265Z digest=sha256:e62a0e954ec62b0c2b522342f2d7c6c93dcea438b694fbc33e64b2b85fdb6f1c

Observation 8fc455e3-0aad-4f56-bf11-adc7f2d37bbe · outbound

This paper cites New constraint on Early Dark Energy from Planck and BOSS data using the profile likelihood.

Determination of neutron star radius from pulse profile modeling using profile likelihood New constraint on Early Dark Energy from Planck and BOSS data using the profile likelihood

Reference 18

Resolution
unresolved
no resolver link, observed 2026-07-14T06:38:48.754265Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-14T06:38:48.754265Z digest=sha256:43f99055239a55d6554f99da3b443895b74b26181fd979340aa100e8738c6f55

Observation 59edd5ca-38cd-4367-82fd-775ea69de6b1 · outbound

This paper cites New constraint on the tensor-to-scalar ratio from the $Planck$ and BICEP/Keck Array data using the profile likelihood.

Determination of neutron star radius from pulse profile modeling using profile likelihood New constraint on the tensor-to-scalar ratio from the $Planck$ and BICEP/Keck Array data using the profile likelihood

Reference 19

Resolution
unresolved
no resolver link, observed 2026-07-14T06:38:48.754265Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-14T06:38:48.754265Z digest=sha256:4e3a965312f9781373e5c15e90a4c951e83eaf9058f662c991d9e9eb2e926a1d

Observation 7275efe7-9997-41fa-895c-5597b3b83407 · outbound

This paper cites Procoli: Profiles of cosmological likelihoods.

Determination of neutron star radius from pulse profile modeling using profile likelihood Procoli: Profiles of cosmological likelihoods

Reference 20

Resolution
unresolved
no resolver link, observed 2026-07-14T06:38:48.754265Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-14T06:38:48.754265Z digest=sha256:428525f6c4447d1aef2570bf8e51a64b8c52df9b4a966cdffc92481be4831527

Observation 6cec5c39-447d-4e1b-84a9-73f7d4ae7fe1 · outbound

This paper cites Barua, S.

Determination of neutron star radius from pulse profile modeling using profile likelihood Barua, S

Reference 21

Resolution
unresolved
no resolver link, observed 2026-07-14T06:38:48.754265Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-14T06:38:48.754265Z digest=sha256:1789eff0e5895882ee61196925d1c33b9b72121adb21c5a9f5a5c9d5767ab2cb

Observation 53a55f26-9757-465c-b592-cd37c56a7809 · outbound

This paper cites Profile Likelihoods in Cosmology: When, Why and How illustrated with $\Lambda$CDM, Massive Neutrinos and Dark Energy.

Determination of neutron star radius from pulse profile modeling using profile likelihood Profile Likelihoods in Cosmology: When, Why and How illustrated with $\Lambda$CDM, Massive Neutrinos and Dark Energy

Reference 22

Resolution
unresolved
no resolver link, observed 2026-07-14T06:38:48.754265Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-14T06:38:48.754265Z digest=sha256:807fe5b29127d68c4c849b00dc9bb9d0568f8f4c2dacc235eb1af4b77c32e414

Observation 17391af8-3ecb-40b5-b6eb-f297ccade713 · outbound

This paper cites Constraints on Lorentz Invariance Violation from Gamma-ray Burst rest-frame spectral lags using Profile Likelihood.

Determination of neutron star radius from pulse profile modeling using profile likelihood Constraints on Lorentz Invariance Violation from Gamma-ray Burst rest-frame spectral lags using Profile Likelihood

Reference 23

Resolution
unresolved
no resolver link, observed 2026-07-14T06:38:48.754265Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-14T06:38:48.754265Z digest=sha256:845184c2d17f1046e5890e8b0b2cfe9f876cbeb5f628215a1da38f6ff80d19fc

Observation 0217dc19-17cf-40b4-b7f9-1f51a4083b68 · outbound

This paper cites Navas et al.

Determination of neutron star radius from pulse profile modeling using profile likelihood Navas et al

Reference 24

Resolution
unresolved
no resolver link, observed 2026-07-14T06:38:48.754265Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-14T06:38:48.754265Z digest=sha256:ebc50509bd1d7bef1a2abdfe3a20002f54efd10267f0ed2be8eee25fa7e2b555

Observation 0f55748c-d8ad-484b-a8f0-03c29f791e6d · outbound

This paper cites Atmospheres and Spectra of Strongly Magnetized Neutron Stars.

Determination of neutron star radius from pulse profile modeling using profile likelihood Atmospheres and Spectra of Strongly Magnetized Neutron Stars

Reference 25

Resolution
unresolved
no resolver link, observed 2026-07-14T06:38:48.754265Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-14T06:38:48.754265Z digest=sha256:7761c3f9d79380f70e16581bdc9701a172a1e564477c408cc08f7a95dc148c6d

Observation 8d64ed12-2124-48ca-bf34-3b83cc158e48 · outbound

This paper cites A Neutron Star with a Carbon Atmosphere in the Cassiopeia A Supernova Remnant.

Determination of neutron star radius from pulse profile modeling using profile likelihood A Neutron Star with a Carbon Atmosphere in the Cassiopeia A Supernova Remnant

Reference 26

Resolution
unresolved
no resolver link, observed 2026-07-14T06:38:48.754265Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-14T06:38:48.754265Z digest=sha256:9a727f531819c7015b46c9d51868cdb6cb7b6c1c617246834759ea4b6ca0ed3d

Observation 2a98d95e-7af8-4e46-94c4-db8bd9082485 · outbound

This paper cites an unresolved cited work.

Determination of neutron star radius from pulse profile modeling using profile likelihood Unresolved cited work

Reference 27

Resolution
unresolved
no resolver link, observed 2026-07-14T06:38:48.754265Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-14T06:38:48.754265Z digest=sha256:296ef42349da99d75841d58f46fc5b5fe9d5ccd02d43320636e590b0eae26a4f

Observation 4401e2ca-bf1e-4b1b-b77f-6411aed189b9 · outbound

This paper cites GetDist: a Python package for analysing Monte Carlo samples.

Determination of neutron star radius from pulse profile modeling using profile likelihood GetDist: a Python package for analysing Monte Carlo samples

Reference 28

Resolution
unresolved
no resolver link, observed 2026-07-14T06:38:48.754265Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-14T06:38:48.754265Z digest=sha256:19c4e9787cd7370562a9460d029f191ea90798d728ed7352d32f9eef223101d3

Pith citing papers

No inbound Pith citation observations are available.