Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? | Paper Citation Record

Observation 238ab969-c82b-431f-85a5-379505fa5e26 · outbound

This paper cites Shapiro and Saul A.

Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? Shapiro and Saul A

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Observation 0155f031-17fe-4ee2-9693-5d5a1d8e3fa2 · outbound

This paper cites Oertel, M.

Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? Oertel, M

Reference 2

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Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? Unresolved cited work

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This paper cites Glendenning.

Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? Glendenning

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Observation bd3e1b7b-c8c5-420a-999f-bd62a7a0de7e · outbound

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Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? Unresolved cited work

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Observation 2a4a681a-ac41-4bce-9874-f098125bb6d6 · outbound

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Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? Kouveliotou et al

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Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? Unresolved cited work

Reference 7

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Observation d28b06c0-7fa3-4b81-9b0a-3467f80bc007 · outbound

This paper cites Deformation of a magnetized neutron star.

Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? Deformation of a magnetized neutron star

Reference 8

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Observation 98d4a43e-0c85-46c4-bc96-2069a074457c · outbound

This paper cites PoS, LAT2009: 0 010, 2010.

Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? PoS, LAT2009: 0 010, 2010

Reference 9

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Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? Unresolved cited work

Reference 10

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Observation e82b7673-a4b3-45bd-960b-bdb0dd828a8c · outbound

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Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? Unresolved cited work

Reference 11

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Observation de45a3b3-a840-4214-ba4e-1e663e691419 · outbound

This paper cites \"O zel and P.

Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? \"O zel and P

Reference 12

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Observation 1a13bab1-9586-4046-a803-50e5c9efb7ec · outbound

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Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? Unresolved cited work

Reference 13

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Observation b727d6b7-7680-4882-b130-2d951b3999ef · outbound

This paper cites Huth et al.

Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? Huth et al

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This paper cites a ttil \.

Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? a ttil \

Reference 15

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Observation eaf29af9-92a4-4c4b-9515-d9b030f243c3 · outbound

This paper cites Smith, Evan J.

Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? Smith, Evan J

Reference 16

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Observation f02f0988-76e2-4a5f-8cfc-8fc02ef96677 · outbound

This paper cites an unresolved cited work.

Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? Unresolved cited work

Reference 17

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Observation d3afbd85-b345-407e-961b-7601fd65e909 · outbound

This paper cites Simultaneously constraining the neutron star equation of state and mass distribution through multimessenger observations and nuclear benchmarks.

Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? Simultaneously constraining the neutron star equation of state and mass distribution through multimessenger observations and nuclear benchmarks

Reference 18

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Observation 49514a40-7376-4d81-99eb-5b868f29f5fc · outbound

This paper cites Science, 340 0 (6131): 0 1233232, 2013.

Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? Science, 340 0 (6131): 0 1233232, 2013

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Observation 84ebf716-b0b0-4695-a744-578a6f4c2f19 · outbound

This paper cites T Cromartie et al.

Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? T Cromartie et al

Reference 20

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Observation 8a2c0985-0c6b-48e9-b293-4f84007bfbfc · outbound

This paper cites Fonseca et al.

Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? Fonseca et al

Reference 21

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Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? Unresolved cited work

Reference 22

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Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? Unresolved cited work

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Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? Unresolved cited work

Reference 26

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Observation 841a55c8-633a-4ff1-96f6-257c6f579b09 · outbound

This paper cites an unresolved cited work.

Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? Unresolved cited work

Reference 28

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Observation 09567d4c-caa0-4f00-b4bb-fb3e2ebfa170 · outbound

This paper cites Lindblom.

Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? Lindblom

Reference 29

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Observation 0084588b-2811-4706-addf-00aeb98771ad · outbound

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Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? Unresolved cited work

Reference 30

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Observation b0888636-87d7-4bf7-adad-276ac5588bd9 · outbound

This paper cites Landry and R.

Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? Landry and R

Reference 31

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Observation a5b05fa9-a0d2-4f2d-9d41-77629ec7abd4 · outbound

This paper cites Somasundaram, B.

Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? Somasundaram, B

Reference 33

Resolution: verified exact; doi, observed 2026-08-03T13:39:33.471517Z

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Observation b8c32f70-407e-4d4f-8eeb-907d4741c56e · outbound

This paper cites Hebeler, J.

Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? Hebeler, J

Reference 34

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Observation e9aa944e-0094-48cc-8569-4ea903242abd · outbound

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Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? Gandolfi, J

Reference 35

Resolution: verified exact; doi, observed 2026-08-03T13:39:33.294628Z

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Observation 2eaad6e3-fa97-417c-9083-a7b12a0ed8ce · outbound

This paper cites Keller, C.

Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? Keller, C

Reference 36

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Observation f700c3b5-cc69-4529-b3c4-29da08c20f6b · outbound

This paper cites Kurkela, P.

Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? Kurkela, P

Reference 37

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Observation c1d433f6-23da-4b0d-baa6-7e068cda9bef · outbound

This paper cites Fraga, Aleksi Kurkela, and Aleksi Vuorinen.

Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? Fraga, Aleksi Kurkela, and Aleksi Vuorinen

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Observation b80e9b44-6ac4-4856-bbb6-e0b5e93662c3 · outbound

This paper cites Fraga, Jürgen Schaffner-Bielich, and Aleksi Vuorinen.

Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? Fraga, Jürgen Schaffner-Bielich, and Aleksi Vuorinen

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Observation dc7bb804-32d3-4425-9e7e-cfd5a3bd1071 · outbound

This paper cites On the Sound Speed in Neutron Stars.

Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? On the Sound Speed in Neutron Stars

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Observation 18e570eb-ebbf-490a-98ac-11bfc6d60cfd · outbound

This paper cites I-Love-Q relations for a generic family of neutron star equations of state.

Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? I-Love-Q relations for a generic family of neutron star equations of state

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Resolution: verified exact; doi, observed 2026-08-03T13:39:32.626585Z

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Observation c056d396-50de-4efe-a645-49a5ae58b64e · outbound

This paper cites Prospect of unraveling the first-order phase transition in neutron stars with f and p _ 1 modes.

Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? Prospect of unraveling the first-order phase transition in neutron stars with f and p _ 1 modes

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Resolution: verified exact; doi, observed 2026-08-03T13:39:32.388448Z

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Observation 5a125f37-0ea1-483a-ab3d-5936ddbfec2e · outbound

This paper cites A General, Scale-independent Description of the Sound Speed in Neutron Stars.

Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? A General, Scale-independent Description of the Sound Speed in Neutron Stars

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Resolution: verified exact; doi, observed 2026-08-03T13:39:32.096553Z

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Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? Impact of large-mass constraints on the properties of neutron stars

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Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? Gorda et al

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Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? Comparison of Equations of State for Neutron Stars with First-order Phase Transitions: A Qualitative Study

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Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? Probing the Internal Structure of Neutron Stars: A Comparative Analysis of Three Different Classes of Equations of State

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Resolution: verified exact; doi, observed 2026-08-03T13:39:31.582365Z

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This paper cites Potekhin, and Dmitry G.

Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? Potekhin, and Dmitry G

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Resolution: unresolved; no resolver link, observed 2026-08-03T13:35:53.553812Z

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Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? Relativistic Hydrodynamics

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This paper cites an unresolved cited work.

Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? Unresolved cited work

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Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? On the sound velocity bound in neutron stars

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Resolution: unresolved; no resolver link, observed 2026-08-03T13:35:53.565229Z

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Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? A NICER View of the 1.4 M _ Edge-on Pulsar PSR J0614-3329

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Resolution: unresolved; no resolver link, observed 2026-08-03T13:35:53.568980Z

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Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? Rhoades and Remo Ruffini

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Resolution: unresolved; no resolver link, observed 2026-08-03T13:35:53.572653Z

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Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? Lindblom

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Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? Lattimer

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Resolution: unresolved; no resolver link, observed 2026-08-03T13:35:53.580371Z

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Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? Most, and Lukas R

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Resolution: unresolved; no resolver link, observed 2026-08-03T13:35:53.584478Z

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Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? Unresolved cited work

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Resolution: unresolved; no resolver link, observed 2026-08-03T13:35:53.588453Z

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Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? Mass Distribution and Maximum Mass of Neutron Stars: Effects of Orbital Inclination Angle

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Resolution: unresolved; no resolver link, observed 2026-08-03T13:35:53.592284Z

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Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? On the maximum mass and oblateness of rotating neutron stars with generic equations of state

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Resolution: unresolved; no resolver link, observed 2026-08-03T13:35:53.597544Z

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Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? Combustion adiabat and the maximum mass of a quark star

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Resolution: verified exact; doi, observed 2026-08-03T13:39:31.036121Z

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Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? Shock waves in (1 + 1-dimensional) curved space-time

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Resolution: verified exact; doi, observed 2026-08-03T13:39:30.731631Z

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No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

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This paper cites On the maximum compactness of neutron stars.

Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? On the maximum compactness of neutron stars

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Resolution: unresolved; no resolver link, observed 2026-08-03T13:35:53.611655Z

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Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? The Ground State of Matter at High Densities: Equation of State and Stellar Models

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Resolution: unresolved; no resolver link, observed 2026-08-03T13:35:53.615779Z

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Observation 8f016c7e-a674-4554-82f8-d858321f451f · outbound

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Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? Unresolved cited work

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Resolution: unresolved; no resolver link, observed 2026-08-03T13:35:53.620192Z

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Observation ab0864b0-5a20-443a-95c3-1910b321d257 · outbound

This paper cites CompactObject: An open-source Python package for full-scope neutron star equation of state inference.

Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? CompactObject: An open-source Python package for full-scope neutron star equation of state inference

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Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? a ttil \

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

Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? UltraNest -- a robust, general purpose Bayesian inference engine

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Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? Unresolved cited work

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Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? Riley et al

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Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? Riley et al

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Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437 4715

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This paper cites Theory of probability.

Are NICER and GW170817 constraints suggesting a compactified scenario for Neutron stars? Theory of probability

Reference 72

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