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Paper Citation Record · LEDGER

The potential broader complex linked to the key Cepheid SV Vul

As of 21 August 2026, this Paper Citation Record lists 100 of 230 outbound references and 0 inbound Pith citation observations for arXiv:2607.14007.

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

pith.paper-citation-record.v1
2607.14007 v1

Coverage vector

measured 100 of 230 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-02T03:06:04.407025Z

measured 100 of 100 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-21T06:32:19.484+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

100 of 230 outbound references displayed

  • verified exact11
  • verified fuzzy0
  • unresolved89
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

Observation d869635a-d765-4141-8b8a-2e68e0a903c8 · outbound

This paper cites Main source (Gaia Collaboration, 2022).

The potential broader complex linked to the key Cepheid SV Vul Main source (Gaia Collaboration, 2022)

Reference 1

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no resolver link, observed 2026-08-02T03:06:03.688572Z

Source-reported events for the cited work

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source=arxiv_source observed=2026-08-02T03:06:03.688572Z digest=sha256:a6e12d852566613103dc95829a09a9ac3470cc250a7095a5b14cd8751a3cb198

Observation 2f8dc370-bd17-4127-9e17-6a632edacc1f · outbound

This paper cites Discovery and description of two young open clusters in the primordial group of NGC 6871.

The potential broader complex linked to the key Cepheid SV Vul Discovery and description of two young open clusters in the primordial group of NGC 6871

Reference 2

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no resolver link, observed 2026-08-02T03:06:03.707847Z

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source=arxiv_source observed=2026-08-02T03:06:03.707847Z digest=sha256:a9c3c5167cb6d1b9a6a5e567262c686ae33b1886e536d8ac3cbe118045d27292

Observation 88befad9-e3a0-4c80-84ed-24a0998306b3 · outbound

This paper cites , year = 2015, month = aug, volume =.

The potential broader complex linked to the key Cepheid SV Vul , year = 2015, month = aug, volume =

Reference 3

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no resolver link, observed 2026-08-02T03:06:03.781030Z

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source=arxiv_source observed=2026-08-02T03:06:03.781030Z digest=sha256:26448890eeb0d2afc7406818e25b9b45eaf1c24e92c8cd566d716f70605c8bb1

Observation 54453f35-e179-4fd5-bd50-b26f7978ef6b · outbound

This paper cites Young open cluster IC 4996 and its vicinity: multicolor photometry and Gaia DR2 astrometry.

The potential broader complex linked to the key Cepheid SV Vul Young open cluster IC 4996 and its vicinity: multicolor photometry and Gaia DR2 astrometry

Reference 4

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no resolver link, observed 2026-08-02T03:06:03.936795Z

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source=arxiv_source observed=2026-08-02T03:06:03.936795Z digest=sha256:b5efdfa620e042326d2bba6bd796c3985554ec3f369181720508ad30bb8915d5

Observation e6ea3df5-3620-41d3-b157-f0be39c8f35d · outbound

This paper cites , year = 1956, month = sep, volume =.

The potential broader complex linked to the key Cepheid SV Vul , year = 1956, month = sep, volume =

Reference 5

Resolution
verified exact
doi, observed 2026-08-02T03:09:06.579483Z

Source-reported events for the cited work

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

source=arxiv_source observed=2026-08-02T03:06:03.942008Z digest=sha256:1df81d3d90cd5db4452d74c612baba3e301acec89529888d0dae4f4f363c0815

Observation 7564669d-4d54-4b6c-99aa-3c2d780da303 · outbound

This paper cites Binary Properties from Cepheid Radial Velocities (CRaV).

The potential broader complex linked to the key Cepheid SV Vul Binary Properties from Cepheid Radial Velocities (CRaV)

Reference 6

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no resolver link, observed 2026-08-02T03:06:03.946716Z

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source=arxiv_source observed=2026-08-02T03:06:03.946716Z digest=sha256:979bd43761241dbf056b8dca4431e4038928b9aa77832f4239f45a19d1f520a1

Observation eed06da1-c330-4410-8f2a-237d4a2d6b96 · outbound

This paper cites Cepheid Abundances: Multiphase Results and Spatial Gradients.

The potential broader complex linked to the key Cepheid SV Vul Cepheid Abundances: Multiphase Results and Spatial Gradients

Reference 7

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no resolver link, observed 2026-08-02T03:06:03.951449Z

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:03.951449Z digest=sha256:bed56520c5fe5a5e00963f5cb0a0a37dd878641d125acbf50e09a5601aad8ece

Observation 9592b2b2-b8cb-4910-8f6d-6af0d42dad9f · outbound

This paper cites Updated parameters of 1743 open clusters based on Gaia DR2.

The potential broader complex linked to the key Cepheid SV Vul Updated parameters of 1743 open clusters based on Gaia DR2

Reference 8

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unresolved
no resolver link, observed 2026-08-02T03:06:03.956295Z

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:03.956295Z digest=sha256:179e5c58bc4d5ed2590ba3fc73c92e495f65e5af605aa85da3adaaa65f6edfb1

Observation a291a7af-6753-4b93-878f-4a839a85435a · outbound

This paper cites Estimating distances from parallaxes. V: Geometric and photogeometric distances to 1.47 billion stars in Gaia Early Data Release 3.

The potential broader complex linked to the key Cepheid SV Vul Estimating distances from parallaxes. V: Geometric and photogeometric distances to 1.47 billion stars in Gaia Early Data Release 3

Reference 9

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no resolver link, observed 2026-08-02T03:06:03.960899Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:03.960899Z digest=sha256:fad699907fb2cec308523b5c123e2e0aad54759ae799e521b90e7aa6d76b1131

Observation e926063b-f02c-46b4-b635-daa26b3f312a · outbound

This paper cites New catalogue of optically visible open clusters and candidates.

The potential broader complex linked to the key Cepheid SV Vul New catalogue of optically visible open clusters and candidates

Reference 10

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unresolved
no resolver link, observed 2026-08-02T03:06:03.965501Z

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:03.965501Z digest=sha256:f08c4c9b5831f3075f5670b8b7d4e9cc3519999a94d01e5cf04bd517423a35a8

Observation c73fab6b-978e-4785-9d94-e67faedf90a9 · outbound

This paper cites A Multi-Band Catalog of 10978 Star Clusters, Associations and Candidates in the Milky Way.

The potential broader complex linked to the key Cepheid SV Vul A Multi-Band Catalog of 10978 Star Clusters, Associations and Candidates in the Milky Way

Reference 11

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no resolver link, observed 2026-08-02T03:06:03.970028Z

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:03.970028Z digest=sha256:426f1565d11f5fcb55a7f7ce791f7bb2cc45f1fef1963e14a3e58cebc57a831c

Observation 089146a1-4e4c-49d9-883d-60ad366a0272 · outbound

This paper cites Unveiling hidden stellar aggregates in the Milky Way: 1656 new star clusters found in Gaia EDR3.

The potential broader complex linked to the key Cepheid SV Vul Unveiling hidden stellar aggregates in the Milky Way: 1656 new star clusters found in Gaia EDR3

Reference 12

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unresolved
no resolver link, observed 2026-08-02T03:06:03.975072Z

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:03.975072Z digest=sha256:1b73baf60622bf75db825062b3d72d896ad4c81c4d5534f36805588015d8bbfd

Observation a8a11ecc-65b8-4198-9a6c-aa7731c90621 · outbound

This paper cites Binary and Grouped Open Clusters: A New Catalogue.

The potential broader complex linked to the key Cepheid SV Vul Binary and Grouped Open Clusters: A New Catalogue

Reference 13

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no resolver link, observed 2026-08-02T03:06:03.979416Z

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source=arxiv_source observed=2026-08-02T03:06:03.979416Z digest=sha256:23acc42b25a5d462aa4e90054c67a7fccaf42f4aa56e0dd8f52d6ba82423d3f2

Observation 5b77b416-87cc-451e-aad0-f43941490be8 · outbound

This paper cites Improving the open cluster census. III. Using cluster masses, radii, and dynamics to create a cleaned open cluster catalogue.

The potential broader complex linked to the key Cepheid SV Vul Improving the open cluster census. III. Using cluster masses, radii, and dynamics to create a cleaned open cluster catalogue

Reference 14

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unresolved
no resolver link, observed 2026-08-02T03:06:03.983774Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:03.983774Z digest=sha256:50e78acccc5445b87f4f555cc1198f4240c19c97ab5e3b1e8932a21c584136c1

Observation b05f2311-3102-40c4-82cf-8660df85e9ed · outbound

This paper cites Validation of the accuracy and precision of Gaia EDR3 parallaxes with globular clusters.

The potential broader complex linked to the key Cepheid SV Vul Validation of the accuracy and precision of Gaia EDR3 parallaxes with globular clusters

Reference 15

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unresolved
no resolver link, observed 2026-08-02T03:06:03.988473Z

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:03.988473Z digest=sha256:ca3571502d52ac9e003769286059bf4f1b7135a5ba8e6fb6c6343b25e0c7e003

Observation a27f08f2-6fb7-412b-bfe5-274bc364ae34 · outbound

This paper cites an unresolved cited work.

The potential broader complex linked to the key Cepheid SV Vul Unresolved cited work

Reference 16

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no resolver link, observed 2026-08-02T03:06:03.993352Z

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Observation c834d980-1c2e-49bd-89fc-a93ce3f3e27d · outbound

This paper cites An efficient approach to extract parameters from star cluster CMDs: fitCMD.

The potential broader complex linked to the key Cepheid SV Vul An efficient approach to extract parameters from star cluster CMDs: fitCMD

Reference 17

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no resolver link, observed 2026-08-02T03:06:03.997808Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:03.997808Z digest=sha256:665eb58f48690a206fe17e735aad07979114f2e1c442953d1d08474e02fd9c51

Observation 2c24c4d6-7121-4772-b6d0-f50ac9ed5577 · outbound

This paper cites , keywords =.

The potential broader complex linked to the key Cepheid SV Vul , keywords =

Reference 18

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no resolver link, observed 2026-08-02T03:06:04.002557Z

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source=arxiv_source observed=2026-08-02T03:06:04.002557Z digest=sha256:646bb7c13004e99d054efd4eb984c7bea4ddb292fb6168798a6b3f14dc9cf13b

Observation 7c760215-b9f7-4ce5-b2bb-b9a58de7a7c8 · outbound

This paper cites , keywords =.

The potential broader complex linked to the key Cepheid SV Vul , keywords =

Reference 19

Resolution
verified exact
doi, observed 2026-08-02T03:09:06.374133Z

Source-reported events for the cited work

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

source=arxiv_source observed=2026-08-02T03:06:04.006659Z digest=sha256:d55c6eecfeee07051390c05d26321efab1220839ecd6fcd59753a8e36c9a840b

Observation 851f16fa-d187-43bf-b90a-67025c6a33a5 · outbound

This paper cites Anchors for the Cosmic Distance Scale: the Cepheids U Sgr, CF Cas and CEab Cas.

The potential broader complex linked to the key Cepheid SV Vul Anchors for the Cosmic Distance Scale: the Cepheids U Sgr, CF Cas and CEab Cas

Reference 20

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no resolver link, observed 2026-08-02T03:06:04.011452Z

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source=arxiv_source observed=2026-08-02T03:06:04.011452Z digest=sha256:791ef54b56041d317af908baef3cb4705ae0a59038cef5ee414316d9940403cc

Observation c8101aea-c3ce-45cb-809a-3547bc685b1d · outbound

This paper cites A review of simulated properties and the reliability of observational catalogues.

The potential broader complex linked to the key Cepheid SV Vul A review of simulated properties and the reliability of observational catalogues

Reference 21

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no resolver link, observed 2026-08-02T03:06:04.015937Z

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source=arxiv_source observed=2026-08-02T03:06:04.015937Z digest=sha256:1116f882d762bb0ee101dd8685f3ce6dd4491953a3e21362ee89b31b8e56252b

Observation ae44c8c4-b56e-4734-8538-ed4666b1e9b6 · outbound

This paper cites 3D Morphology of Open Clusters in the Solar Neighborhood with Gaia EDR3: its Relation to Cluster Dynamics.

The potential broader complex linked to the key Cepheid SV Vul 3D Morphology of Open Clusters in the Solar Neighborhood with Gaia EDR3: its Relation to Cluster Dynamics

Reference 22

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unresolved
no resolver link, observed 2026-08-02T03:06:04.020586Z

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.020586Z digest=sha256:d21613080d0bc8c2127c4d797e493ea6de7f27488c9f8b44817ef3d2ed69aaa5

Observation e9f6acbe-0f4b-4646-9810-855e84b9256a · outbound

This paper cites YBC, a stellar bolometric corrections database with variable extinction coefficients: an application to PARSEC isochrones.

The potential broader complex linked to the key Cepheid SV Vul YBC, a stellar bolometric corrections database with variable extinction coefficients: an application to PARSEC isochrones

Reference 23

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no resolver link, observed 2026-08-02T03:06:04.025219Z

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.025219Z digest=sha256:b96d792600eb4fb02ddfca7010016d88271977408cd40ad86a8c56adcf67f260

Observation 01676722-c753-46be-94a3-939c8a636e48 · outbound

This paper cites Hunting for Neighboring Open Clusters with Gaia DR3: 101 New Open Clusters within 500 pc.

The potential broader complex linked to the key Cepheid SV Vul Hunting for Neighboring Open Clusters with Gaia DR3: 101 New Open Clusters within 500 pc

Reference 24

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unresolved
no resolver link, observed 2026-08-02T03:06:04.030500Z

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source=arxiv_source observed=2026-08-02T03:06:04.030500Z digest=sha256:a10b708ebb198caf397d30c478709ce7988948ee73b15d96c46c81ce03c05ba5

Observation d9cbc0a2-8964-4d92-b611-42d12cd4e45e · outbound

This paper cites Oxygen, sulfur, and iron radial abundance gradients of classical Cepheids across the Galactic thin disk.

The potential broader complex linked to the key Cepheid SV Vul Oxygen, sulfur, and iron radial abundance gradients of classical Cepheids across the Galactic thin disk

Reference 25

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unresolved
no resolver link, observed 2026-08-02T03:06:04.035625Z

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source=arxiv_source observed=2026-08-02T03:06:04.035625Z digest=sha256:b6cbc285bbf1f4f3ff9a162d7f0a509517284ba3426128b1205d028a3f7af8d9

Observation af62ecc2-55c0-4169-bb14-41029cd54624 · outbound

This paper cites , keywords =.

The potential broader complex linked to the key Cepheid SV Vul , keywords =

Reference 26

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unresolved
no resolver link, observed 2026-08-02T03:06:04.040488Z

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.040488Z digest=sha256:6525edaf24abfbb6718e916626585bce4de39d68a1c4723c93842b58f4140451

Observation 2e5cb2c2-b9ed-45cb-96d2-29f532392dee · outbound

This paper cites , year = 1996, month = apr, volume =.

The potential broader complex linked to the key Cepheid SV Vul , year = 1996, month = apr, volume =

Reference 27

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unresolved
no resolver link, observed 2026-08-02T03:06:04.045127Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.045127Z digest=sha256:200dbe0bb8b4ac85a3a07ffadedfee175dca228651fe8b74a506e4221b59a336

Observation 3f06fa94-2396-475c-af03-13b37fa8431e · outbound

This paper cites Open cluster dissolution rate and the initial cluster mass function in the solar neighbourhood. Modelling the age and mass distributions of clusters observed by Gaia.

The potential broader complex linked to the key Cepheid SV Vul Open cluster dissolution rate and the initial cluster mass function in the solar neighbourhood. Modelling the age and mass distributions of clusters observed by Gaia

Reference 28

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unresolved
no resolver link, observed 2026-08-02T03:06:04.049692Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.049692Z digest=sha256:66e9c04bc2d8dd338f21c11d50d1ba867f91190585cf83331b39e5320008b29c

Observation 56abe916-1d08-41b2-9bff-18dba9f26e76 · outbound

This paper cites Parameter Estimation for Open Clusters using an Artificial Neural Network with a QuadTree-based Feature Extractor.

The potential broader complex linked to the key Cepheid SV Vul Parameter Estimation for Open Clusters using an Artificial Neural Network with a QuadTree-based Feature Extractor

Reference 29

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.054662Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.054662Z digest=sha256:07c679bcfe839ec4cd5b27e20263c56e815585aa738e8c9ce2e38af84ede94dc

Observation e6465c9e-64a9-45a7-b826-f3188703b861 · outbound

This paper cites Painting a portrait of the Galactic disc with its stellar clusters.

The potential broader complex linked to the key Cepheid SV Vul Painting a portrait of the Galactic disc with its stellar clusters

Reference 30

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unresolved
no resolver link, observed 2026-08-02T03:06:04.059503Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.059503Z digest=sha256:90fb03865d3ab950d172e2b733731e05d3ba7612d74fb85316e29da198f09c4b

Observation f6c7063a-1c8a-4165-96a3-ac279eb17409 · outbound

This paper cites Open clusters housing classical Cepheids in Gaia DR3.

The potential broader complex linked to the key Cepheid SV Vul Open clusters housing classical Cepheids in Gaia DR3

Reference 31

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unresolved
no resolver link, observed 2026-08-02T03:06:04.064996Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.064996Z digest=sha256:7e6ec0827595838fb5fdd2e1d4be017aa52d9752635ccc1e563faaba40429b7d

Observation 4bc532f7-1bfe-4452-8146-fa1be50ecfbe · outbound

This paper cites Evolution of the local spiral structure of the Milky Way revealed by open clusters.

The potential broader complex linked to the key Cepheid SV Vul Evolution of the local spiral structure of the Milky Way revealed by open clusters

Reference 32

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unresolved
no resolver link, observed 2026-08-02T03:06:04.070261Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.070261Z digest=sha256:81b3ad422f7837541dbe5e57f550dcb977fa04a9c16b6c0fc53f513ea786edab

Observation 669f6075-b78d-4215-88d7-284d606be705 · outbound

This paper cites , keywords =.

The potential broader complex linked to the key Cepheid SV Vul , keywords =

Reference 33

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unresolved
no resolver link, observed 2026-08-02T03:06:04.074970Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.074970Z digest=sha256:ca51f4a70aabaebc24736c7199a651eb22bf88bdafb0e302ff8fb8bdad350678

Observation f398b109-bd92-4326-a932-bcb4bdbdbedb · outbound

This paper cites Rate of Period Change as a Diagnostic of Cepheid Properties.

The potential broader complex linked to the key Cepheid SV Vul Rate of Period Change as a Diagnostic of Cepheid Properties

Reference 34

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unresolved
no resolver link, observed 2026-08-02T03:06:04.079972Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.079972Z digest=sha256:6299bfac93812445b63418febb7bf8eeeaa8be33ea271e65549b6f2ed4b815ac

Observation 9a88984a-2b58-4410-87cf-5b665c48f586 · outbound

This paper cites , keywords =.

The potential broader complex linked to the key Cepheid SV Vul , keywords =

Reference 35

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.084727Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.084727Z digest=sha256:15e890f098cab48ae55572e82be608fdc78f0c15e9f81160bf640b28d0a212db

Observation bfa103fa-2967-4cdd-ad88-c6267075e36e · outbound

This paper cites an unresolved cited work.

The potential broader complex linked to the key Cepheid SV Vul Unresolved cited work

Reference 36

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.089598Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.089598Z digest=sha256:3876982194de38f8ba01d3e4d80a8072403fbcc695255cf8b464e1f174b8adb2

Observation 05a6bf41-8f84-4ea5-b850-86956439e9f6 · outbound

This paper cites , keywords =.

The potential broader complex linked to the key Cepheid SV Vul , keywords =

Reference 37

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.093998Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.093998Z digest=sha256:e7c4d43bf502b120aadaf2dcb9d0b3e63f51bc66a2971c6ddbec1514a18f31ee

Observation 5abab5c8-b30f-4f13-9d00-9d4154bc77a7 · outbound

This paper cites Evolutionary tracks and isochrones for low- and intermediate-mass stars: from 0.15 to 7 M_sun, and from Z=0.0004 to 0.03.

The potential broader complex linked to the key Cepheid SV Vul Evolutionary tracks and isochrones for low- and intermediate-mass stars: from 0.15 to 7 M_sun, and from Z=0.0004 to 0.03

Reference 38

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.098983Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.098983Z digest=sha256:20153100274acb879a90d96cd8069d339ecdc20cb94edf14ec3abd238c95f55f

Observation ec4c1070-6564-4c56-ac8b-5e92fd081184 · outbound

This paper cites an unresolved cited work.

The potential broader complex linked to the key Cepheid SV Vul Unresolved cited work

Reference 39

Resolution
verified exact
doi, observed 2026-08-02T03:09:06.197933Z

Source-reported events for the cited work

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

source=arxiv_source observed=2026-08-02T03:06:04.103947Z digest=sha256:a707336d7be156a6debf89a6e0ac869f325da0b116434d67bd37d2b8d6f41e10

Observation 16b5c527-8199-47d6-bb24-282988164450 · outbound

This paper cites , keywords =.

The potential broader complex linked to the key Cepheid SV Vul , keywords =

Reference 40

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.108885Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.108885Z digest=sha256:bfe141a53940fe24ee42acb59417c7bf578d6c580baf6c5d132b5a3ed0ca5457

Observation 2d69fe35-877f-4436-ae09-fc6a22b1736d · outbound

This paper cites A 0.9% Calibration of the Galactic Cepheid luminosity scale based on Gaia DR3 data of open clusters and Cepheids.

The potential broader complex linked to the key Cepheid SV Vul A 0.9% Calibration of the Galactic Cepheid luminosity scale based on Gaia DR3 data of open clusters and Cepheids

Reference 41

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.113452Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.113452Z digest=sha256:e5e49b4a3d3dcfbe84b6cc336eaa805dc90e5615f7744f391736988542dc6f10

Observation e288d7ff-99b5-4bc0-a708-06363556d067 · outbound

This paper cites Exploring a New Standard Candle for the Extragalactic Distance Scale.

The potential broader complex linked to the key Cepheid SV Vul Exploring a New Standard Candle for the Extragalactic Distance Scale

Reference 42

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.118411Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.118411Z digest=sha256:e0075c1a1d1339dd3c8033e8d2917c8657fd939eb55f033950fa9eca671fac46

Observation e4abaee0-6024-4cf0-b209-527b1b7694eb · outbound

This paper cites Classical Cepheid Pulsation Models. X. The Period-Age Relation.

The potential broader complex linked to the key Cepheid SV Vul Classical Cepheid Pulsation Models. X. The Period-Age Relation

Reference 43

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.122808Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.122808Z digest=sha256:0a761b38ae4e635f872fefb4d992dca85ececd9fc9c90f33af538889d07527c3

Observation 80626554-c49c-48a5-b517-95b4e478ec9f · outbound

This paper cites , keywords =.

The potential broader complex linked to the key Cepheid SV Vul , keywords =

Reference 44

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.127875Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.127875Z digest=sha256:343fa3f2803ce2874c593158ce75f7f4ada1bceec16e6d67dafa36102ccc14b7

Observation b1e4bb7f-43f8-49d2-8189-4069788e93ad · outbound

This paper cites On the Effect of Rotation on Populations of Classical Cepheids II. Pulsation Analysis for Metallicities 0.014, 0.006, and 0.002.

The potential broader complex linked to the key Cepheid SV Vul On the Effect of Rotation on Populations of Classical Cepheids II. Pulsation Analysis for Metallicities 0.014, 0.006, and 0.002

Reference 45

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.132227Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.132227Z digest=sha256:216894be1b51f2a1208bc8af5873ab1e16f68bd7c50f15c74a104f5c97a16b0f

Observation e7c864de-bcec-453a-846d-f070dd92f750 · outbound

This paper cites , keywords =.

The potential broader complex linked to the key Cepheid SV Vul , keywords =

Reference 46

Resolution
verified exact
doi, observed 2026-08-02T03:09:06.006230Z

Source-reported events for the cited work

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

source=arxiv_source observed=2026-08-02T03:06:04.137334Z digest=sha256:e6eb88b63eb595ba34980852d64178809b16651106bab03781c738a7dbfd136e

Observation 74b373f8-72cf-4ac0-8347-b5ec949335db · outbound

This paper cites Parallaxes and proper motions for 20 open clusters as based on the new Hipparcos catalogue.

The potential broader complex linked to the key Cepheid SV Vul Parallaxes and proper motions for 20 open clusters as based on the new Hipparcos catalogue

Reference 47

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.141877Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.141877Z digest=sha256:b6faa679c367130ca50b4cc0a0a1c23be99d8d7b651bc1bde5da99c23cbd0144

Observation fe68fbd4-273b-4057-b75c-3d4889a77cd7 · outbound

This paper cites Accurate age determinations of several nearby open clusters containing magnetic Ap stars.

The potential broader complex linked to the key Cepheid SV Vul Accurate age determinations of several nearby open clusters containing magnetic Ap stars

Reference 48

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.147217Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.147217Z digest=sha256:0a697fc77675082bc4e20205d73e93d007cc9851304f06103dea61cf602b6b64

Observation 29dc9df1-cf4b-4ea2-a839-ef963bd4e10d · outbound

This paper cites The influence of metallicity on the Leavitt Law from geometrical distances of Milky Way and Magellanic Clouds Cepheids.

The potential broader complex linked to the key Cepheid SV Vul The influence of metallicity on the Leavitt Law from geometrical distances of Milky Way and Magellanic Clouds Cepheids

Reference 49

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.151841Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.151841Z digest=sha256:10ff9f2db8558b8be4d5fc8e07fbde8480b8f0937bcd3436c1c0ad85b5400a74

Observation 55fae2a7-304b-4e19-86c0-3c2da19d6d96 · outbound

This paper cites , keywords =.

The potential broader complex linked to the key Cepheid SV Vul , keywords =

Reference 50

Resolution
verified exact
doi, observed 2026-08-02T03:09:05.834365Z

Source-reported events for the cited work

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

source=arxiv_source observed=2026-08-02T03:06:04.156726Z digest=sha256:c169e66a76076ca51a35a2c7e73caf4d87383b18c317fdaf43814a6704a6796f

Observation b3e0a4ec-5e2e-4adb-a470-1f0a48077f5e · outbound

This paper cites On the Application of Wesenheit Function in Deriving Distance to Galactic Cepheids.

The potential broader complex linked to the key Cepheid SV Vul On the Application of Wesenheit Function in Deriving Distance to Galactic Cepheids

Reference 51

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.162028Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.162028Z digest=sha256:385ebc88e46598592542f23373f290ca0e3c25b78caf4df75b3413658812b8cb

Observation fe180194-37ba-406a-9682-31681a0e23e8 · outbound

This paper cites an unresolved cited work.

The potential broader complex linked to the key Cepheid SV Vul Unresolved cited work

Reference 52

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.166933Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.166933Z digest=sha256:aca206d3299ee848831f8fe55167e7a89d481b57404c1a04311f1a7c9aecff9f

Observation 1d0fdd15-41a4-4be5-8477-8cf3a7800d1f · outbound

This paper cites A suite of classical Cepheids tied to the binary cluster Berkeley 58 \& NGC 7790.

The potential broader complex linked to the key Cepheid SV Vul A suite of classical Cepheids tied to the binary cluster Berkeley 58 \& NGC 7790

Reference 54

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.176617Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.176617Z digest=sha256:ac9977ff469f2697143b5793ba488f844cd053f11634702516122cb463553cd2

Observation 44e7c929-d078-42be-b6fb-db4f61d4e348 · outbound

This paper cites Gaia Data Release 3: Analysis of the Gaia BP/RP spectra using the General Stellar Parameterizer from Photometry.

The potential broader complex linked to the key Cepheid SV Vul Gaia Data Release 3: Analysis of the Gaia BP/RP spectra using the General Stellar Parameterizer from Photometry

Reference 55

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.183028Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.183028Z digest=sha256:1ad4aabd0e82d032a7858caa94d456fbe5a126bf642a2c2af1c973f7dfbaa844

Observation 4e69fa63-3a4a-41e6-90be-fdebc67866b5 · outbound

This paper cites an unresolved cited work.

The potential broader complex linked to the key Cepheid SV Vul Unresolved cited work

Reference 56

Resolution
verified exact
doi, observed 2026-08-02T03:09:05.630829Z

Source-reported events for the cited work

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

source=arxiv_source observed=2026-08-02T03:06:04.188757Z digest=sha256:9da515e0c7a874838e7121f04fc39805fcd1cc613bd090d131a6f6a9783ba6ab

Observation 8e4e84ac-1492-4dbd-85c2-bd13e15d7b34 · outbound

This paper cites , keywords =.

The potential broader complex linked to the key Cepheid SV Vul , keywords =

Reference 57

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.193365Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.193365Z digest=sha256:283cc4fb9257f3d287b309cf1e975ea32237917f03bbb2d0fe8d76dfd4c7833b

Observation 1163b520-8472-439d-b3ce-ebe4a0ce0e56 · outbound

This paper cites IGAPS: the merged IPHAS and UVEX optical surveys of theNorthern Galactic Plane.

The potential broader complex linked to the key Cepheid SV Vul IGAPS: the merged IPHAS and UVEX optical surveys of theNorthern Galactic Plane

Reference 58

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.198681Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.198681Z digest=sha256:2ef1d78a849c7999308be0132a000ada76e165060fd0767f4d4bf0bc609d9366

Observation 9ad3f65b-f7b7-4570-93e0-7df9308e3bf9 · outbound

This paper cites What Does the Milky Way Look Like?.

The potential broader complex linked to the key Cepheid SV Vul What Does the Milky Way Look Like?

Reference 59

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.203686Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.203686Z digest=sha256:3a2120be095063fb3973a5ef7f02794c4da37662dfe30d74e018e9949c5eb33b

Observation 0ffbd7aa-aa6f-46ab-8cc7-eb1ade387781 · outbound

This paper cites A catalog of newly identified star clusters in GAIA DR2.

The potential broader complex linked to the key Cepheid SV Vul A catalog of newly identified star clusters in GAIA DR2

Reference 60

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.208731Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.208731Z digest=sha256:72532af46e7a01242345ec3cf37cdfce2abedaf621b92f3300f0643df99d69a9

Observation bc5ef06b-19a0-4b04-9432-3680e2d18895 · outbound

This paper cites The Valuable Long-period Cluster Cepheid KQ Scorpii and other Calibration Candidates.

The potential broader complex linked to the key Cepheid SV Vul The Valuable Long-period Cluster Cepheid KQ Scorpii and other Calibration Candidates

Reference 61

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.213414Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.213414Z digest=sha256:62ef026bf491dde994003dc7f1c0c9c8fc3927da26b65def84cf8d454509f177

Observation bfa36ccf-3da1-4083-86c9-5205b0dfd1fa · outbound

This paper cites Revisiting cosmic acceleration with DESI BAO.

The potential broader complex linked to the key Cepheid SV Vul Revisiting cosmic acceleration with DESI BAO

Reference 62

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.218256Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.218256Z digest=sha256:cc32f566509929407fcd1542f792485a574a487431bed5b2a5f4e12f52c66945

Observation 76d006cb-2215-4a3c-9cad-7d97c5b366bf · outbound

This paper cites DESI 2024: Reconstructing Dark Energy using Crossing Statistics with DESI DR1 BAO data.

The potential broader complex linked to the key Cepheid SV Vul DESI 2024: Reconstructing Dark Energy using Crossing Statistics with DESI DR1 BAO data

Reference 63

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.223166Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.223166Z digest=sha256:19bffd60edbfeca7eca1fa691c20c6a1c91511f9722141b3ee2037c512c8dcb2

Observation c46fa9f7-2021-465e-bc03-7c928fa3ebed · outbound

This paper cites , keywords =.

The potential broader complex linked to the key Cepheid SV Vul , keywords =

Reference 64

Resolution
verified exact
doi, observed 2026-08-02T03:09:05.469072Z

Source-reported events for the cited work

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

source=arxiv_source observed=2026-08-02T03:06:04.228058Z digest=sha256:254413500718f3368f9207d75311c6f3e0c8466729e7c34857c449e2ec7213e2

Observation c22b1cae-90a5-439e-8d2a-3bf37029a9bb · outbound

This paper cites Cluster Cepheids with High Precision Gaia Parallaxes, Low Zeropoint Uncertainties, and Hubble Space Telescope Photometry.

The potential broader complex linked to the key Cepheid SV Vul Cluster Cepheids with High Precision Gaia Parallaxes, Low Zeropoint Uncertainties, and Hubble Space Telescope Photometry

Reference 65

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.233612Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.233612Z digest=sha256:4b1e4d53e958fe3a0eba52bb327b2ed2498565084ece7125d1b408c6a75cab31

Observation 297c5282-3384-462d-8776-9a20c7e86be0 · outbound

This paper cites , keywords =.

The potential broader complex linked to the key Cepheid SV Vul , keywords =

Reference 66

Resolution
verified exact
doi, observed 2026-08-02T03:09:05.281887Z

Source-reported events for the cited work

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

source=arxiv_source observed=2026-08-02T03:06:04.238429Z digest=sha256:265d7cef0874f5c1f1c28c8b0845a66dfe5d49f3199873f1a922c8265d90c842

Observation 90497a22-716e-42b9-9792-885f24aded33 · outbound

This paper cites , keywords =.

The potential broader complex linked to the key Cepheid SV Vul , keywords =

Reference 67

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.243262Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.243262Z digest=sha256:11c5609a86174369dbe8f780b02a9e03de8375e079d3ab2708b9830c33e3f568

Observation 7050d96f-c800-46cf-8d96-a36ea9a485b4 · outbound

This paper cites , keywords =.

The potential broader complex linked to the key Cepheid SV Vul , keywords =

Reference 68

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.247757Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.247757Z digest=sha256:772ce988eaa966b738951ebe7023f0e8f89b8d817b665e8f48af759301d339e6

Observation 9b383fb5-dd9e-4028-abe4-58cbdd1df139 · outbound

This paper cites Cluster membership for the long period Cepheid calibrator SV Vul.

The potential broader complex linked to the key Cepheid SV Vul Cluster membership for the long period Cepheid calibrator SV Vul

Reference 69

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.252685Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.252685Z digest=sha256:775a30221223edb323a40869e5d3f51d9951e0e674baff47ef768dc8dba00c22

Observation 04b26142-ec97-4513-aa61-5a6dc1d336ee · outbound

This paper cites , keywords =.

The potential broader complex linked to the key Cepheid SV Vul , keywords =

Reference 70

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.257997Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.257997Z digest=sha256:4fe5c2bc168de0a6aa7ae74c384d308195c58eb144e7637d46cb8ae20aab30d4

Observation 008cd9c5-d662-4242-b70d-7e25316f2a0a · outbound

This paper cites , keywords =.

The potential broader complex linked to the key Cepheid SV Vul , keywords =

Reference 71

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.262642Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.262642Z digest=sha256:f2f1d3ef09efb4150dbb2a7093ce4d0314b420196ff2db91d690ae1f7ddc6af8

Observation 9ba6a375-ad9e-4e20-bb05-9b86ba29f8a4 · outbound

This paper cites Catalogue of light-curve parameters and distances.

The potential broader complex linked to the key Cepheid SV Vul Catalogue of light-curve parameters and distances

Reference 72

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.266911Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.266911Z digest=sha256:eb29cc75267f3a8922cfe3930e3b3455ff3dab2d4ef5dc831dbaece210bcbeae

Observation e93453f6-fa13-4c34-a037-70f9da62557e · outbound

This paper cites The Distribution of the Elements in the Galactic Disk II. Azimuthal and Radial Variation in Abundances from Cepheids.

The potential broader complex linked to the key Cepheid SV Vul The Distribution of the Elements in the Galactic Disk II. Azimuthal and Radial Variation in Abundances from Cepheids

Reference 73

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.271275Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.271275Z digest=sha256:ef63bb74e37fd577f2de32a993357fc3de0cec8b137361a1acbc9227e5781acd

Observation e7c86dee-386a-4b95-8015-85590d0b2736 · outbound

This paper cites Astronomy Letters , year = 2013, month = jul, volume =.

The potential broader complex linked to the key Cepheid SV Vul Astronomy Letters , year = 2013, month = jul, volume =

Reference 74

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.276287Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.276287Z digest=sha256:fe19e185e813c11d3eaf09d2a9aad6882f61da69114e91ced689b27755342a3c

Observation 89b101d9-8197-4455-95a1-9b3262daa448 · outbound

This paper cites Odessa Astronomical Publications , keywords =.

The potential broader complex linked to the key Cepheid SV Vul Odessa Astronomical Publications , keywords =

Reference 75

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.280950Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.280950Z digest=sha256:c45dd5f7130d992b26c44667748ec48f1f34e082987df2622bd45db3abbaa9d2

Observation cab6c740-4b38-48ad-8f53-1465c3dfb592 · outbound

This paper cites Baade-Wesselink distances to Galactic and Magellanic Cloud Cepheids and the effect of metallicity.

The potential broader complex linked to the key Cepheid SV Vul Baade-Wesselink distances to Galactic and Magellanic Cloud Cepheids and the effect of metallicity

Reference 76

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.285621Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.285621Z digest=sha256:18f03bcdeffced9f883a0988eb90c5d935ca3867db5e6ac67a3253603a3857ab

Observation fb8b44d7-fd05-4caa-9077-7d55a8b7dd48 · outbound

This paper cites , keywords =.

The potential broader complex linked to the key Cepheid SV Vul , keywords =

Reference 77

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.290225Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.290225Z digest=sha256:f9d29668f5f2b020788f0e11c84bb5f647af9a07b8c95888b375f899c3d736cc

Observation 6fa5f06e-b564-4888-9155-43235ea2f036 · outbound

This paper cites A distance determination to the Small Magellanic Cloud with an accuracy of better than 2 percent based on late-type eclipsing binary stars.

The potential broader complex linked to the key Cepheid SV Vul A distance determination to the Small Magellanic Cloud with an accuracy of better than 2 percent based on late-type eclipsing binary stars

Reference 78

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.295108Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.295108Z digest=sha256:750f270303eca9f5ef0a59833949e686b1d18b2cdd42164f9748a2afafc33679

Observation d8c15faa-09e8-4409-9852-f081e1692245 · outbound

This paper cites arXiv e-prints , keywords =.

The potential broader complex linked to the key Cepheid SV Vul arXiv e-prints , keywords =

Reference 79

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.299870Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.299870Z digest=sha256:495b854ffa1512f8b3c7d1d8155a0ee2e5e082c02cec99bec89828c24d574223

Observation 701dbfd5-f828-4e1e-bf3d-419be7ef953c · outbound

This paper cites Astrometry with Hubble Space Telescope: A Parallax of the Fundamental Distance Calibrator delta Cephei.

The potential broader complex linked to the key Cepheid SV Vul Astrometry with Hubble Space Telescope: A Parallax of the Fundamental Distance Calibrator delta Cephei

Reference 80

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.304559Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.304559Z digest=sha256:0da578ffd423fb8335bc862c957a016bf4b09930a117d2e1fb2be629c9bd27b3

Observation c84e99f9-bf18-4443-80e8-64851b85afa0 · outbound

This paper cites Period-Luminosity Relations for Galactic Type II Cepheids in the Sloan bands.

The potential broader complex linked to the key Cepheid SV Vul Period-Luminosity Relations for Galactic Type II Cepheids in the Sloan bands

Reference 81

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.309193Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.309193Z digest=sha256:751fc402d23ac1e8e8978a6d57fbe7e0191e100e14bcddf455b74edd021e91f1

Observation 57d290d3-2a9a-4a44-b0e7-f36b300a5909 · outbound

This paper cites Blending of Cepheids in M33.

The potential broader complex linked to the key Cepheid SV Vul Blending of Cepheids in M33

Reference 82

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.314102Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.314102Z digest=sha256:59ed3be6bf82835f9f848cf651401c1f8a3c8b58bf33c4bffc2798e5849cb653

Observation 375baa95-bd62-4ff7-8b73-381f6956df0a · outbound

This paper cites Chicago-Carnegie Hubble Program (CCHP) A Multi-Wavelength Search for the Effects of Metallicity on the Cepheid Distance Scale. Part II: Theoretical Models and Synthetic Spectra.

The potential broader complex linked to the key Cepheid SV Vul Chicago-Carnegie Hubble Program (CCHP) A Multi-Wavelength Search for the Effects of Metallicity on the Cepheid Distance Scale. Part II: Theoretical Models and Synthetic Spectra

Reference 83

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.319508Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.319508Z digest=sha256:7570d6fbfe9c8ec17a4cae135f43faf4472db2cb537be2a5e1a1004eb584a87d

Observation 4254f026-0343-4c29-96e7-d31a034f84f7 · outbound

This paper cites VLT spectroscopy of blue supergiants in IC 1613.

The potential broader complex linked to the key Cepheid SV Vul VLT spectroscopy of blue supergiants in IC 1613

Reference 84

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.324304Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.324304Z digest=sha256:470135550b01b21dea6e47293596fa7764ce23cb563e7e7c1ff9b28738fcbf33

Observation 734c3536-9dcd-4c6d-803c-7bf52deb9513 · outbound

This paper cites an unresolved cited work.

The potential broader complex linked to the key Cepheid SV Vul Unresolved cited work

Reference 85

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.329376Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.329376Z digest=sha256:dc694fa3500f3f783c8aaed078758de019df240bb7b0c99eb85b31fe0e9dbc51

Observation 89f205dd-6b81-4d44-9b48-42787995c4d4 · outbound

This paper cites Red supergiant stars in IC 1613 and metallicity-dependent mixing length in the evolutionary model.

The potential broader complex linked to the key Cepheid SV Vul Red supergiant stars in IC 1613 and metallicity-dependent mixing length in the evolutionary model

Reference 86

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.333832Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.333832Z digest=sha256:fe9701f028484b4c0226e916ba94daa28a018df864c7c2a8d68df1df0766bd7b

Observation 83b6cd4b-74ea-4ee6-a930-e7c87559d035 · outbound

This paper cites Red Supergiants as Cosmic Abundance Probes: The Magellanic Clouds.

The potential broader complex linked to the key Cepheid SV Vul Red Supergiants as Cosmic Abundance Probes: The Magellanic Clouds

Reference 87

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.338882Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.338882Z digest=sha256:e89acd72d09bc0c662d9689ed661469af1b1b010e9f4af53eb56b21cfd6ed974

Observation 80fd3cd6-29f8-45dd-be95-6fbf1d523998 · outbound

This paper cites Quantitative Spectroscopy of Supergiants in the Local Group Dwarf Galaxy IC 1613: Metallicity and Distance.

The potential broader complex linked to the key Cepheid SV Vul Quantitative Spectroscopy of Supergiants in the Local Group Dwarf Galaxy IC 1613: Metallicity and Distance

Reference 88

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.344069Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.344069Z digest=sha256:f2570e668f531f3a99d81429f675fb536d2d2128525c12fcaac9a8f03cdf6433

Observation 7a00f393-859b-4c95-a789-97d87c3beded · outbound

This paper cites The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch.

The potential broader complex linked to the key Cepheid SV Vul The Chicago Carnegie Hubble Program: Improving the Calibration of SNe Ia with JWST Measurements of the Tip of the Red Giant Branch

Reference 89

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.348765Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.348765Z digest=sha256:9f9350af0c99c502573db7c6497e6603236fa2b54bf556ea78ce19eca9395d75

Observation 0976eabe-944f-4f8e-81fb-8e19597dbed2 · outbound

This paper cites The Araucaria Project. The distance to the Small Magellanic Cloud from late-type eclipsing binaries.

The potential broader complex linked to the key Cepheid SV Vul The Araucaria Project. The distance to the Small Magellanic Cloud from late-type eclipsing binaries

Reference 90

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.353787Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.353787Z digest=sha256:e7f6e4f85248afd9598fa38dcc90e360ec3c7f2d0d99f40255612f7b934aaa8c

Observation 162fda35-d76a-4654-8e61-faf0575b5c7a · outbound

This paper cites Video Memorie della Societa Astronomica Italiana , keywords =.

The potential broader complex linked to the key Cepheid SV Vul Video Memorie della Societa Astronomica Italiana , keywords =

Reference 91

Resolution
verified exact
doi, observed 2026-08-02T03:09:05.077151Z

Source-reported events for the cited work

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

source=arxiv_source observed=2026-08-02T03:06:04.359020Z digest=sha256:3279975c1345032d9afb3cfacbb74a557ab8ee190aaf54be54770f1da8a54f26

Observation c52e7d73-3d72-4197-9669-78575b1e9509 · outbound

This paper cites arXiv e-prints , keywords =.

The potential broader complex linked to the key Cepheid SV Vul arXiv e-prints , keywords =

Reference 92

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.363553Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.363553Z digest=sha256:15f6166477ff0182aead05dc716ab740ecd1d5cb5785782df6be01717740a055

Observation 56dbb827-59ed-42f4-913b-a9debd52663a · outbound

This paper cites Anchoring the Universal Distance Scale via a Wesenheit Template.

The potential broader complex linked to the key Cepheid SV Vul Anchoring the Universal Distance Scale via a Wesenheit Template

Reference 93

Resolution
verified exact
local_arxiv, observed 2026-08-02T03:09:04.862887Z

Source-reported events for the cited work

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

source=arxiv_source observed=2026-08-02T03:06:04.368222Z digest=sha256:548538ba7e230aa849066d5d9f4343f1af6ed2ec940a7bb6f8e65e396d8d0579

Observation cad75859-f7ed-4059-b782-aa709782bb1f · outbound

This paper cites The VMC Survey -- XLVIII. Classical Cepheids unveil the 3D geometry of the LMC.

The potential broader complex linked to the key Cepheid SV Vul The VMC Survey -- XLVIII. Classical Cepheids unveil the 3D geometry of the LMC

Reference 94

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.373890Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.373890Z digest=sha256:8997b08e66669b795d5ad079504178a6df923d75a3725dca10098a5ac923faab

Observation c199efb0-c8be-42bd-a240-4a700eb77c62 · outbound

This paper cites , keywords =.

The potential broader complex linked to the key Cepheid SV Vul , keywords =

Reference 95

Resolution
verified exact
doi, observed 2026-08-02T03:09:04.556686Z

Source-reported events for the cited work

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

source=arxiv_source observed=2026-08-02T03:06:04.378615Z digest=sha256:9f9ae0f0cb6966dcc3254baf2a50fb4a515998187ae871a176f93e7b0b57558d

Observation b3d70e71-eba1-4d3d-97d1-7c05512d9d3e · outbound

This paper cites The PL calibration for Milky Way Cepheids and its implications for the distance scale.

The potential broader complex linked to the key Cepheid SV Vul The PL calibration for Milky Way Cepheids and its implications for the distance scale

Reference 96

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.383161Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.383161Z digest=sha256:04a8b635d8b234f524793154dc308e826c7f982c67a938e987aa6085586e6356

Observation 5d4b27fd-dc2a-41fc-83e0-e6a25edf7824 · outbound

This paper cites , keywords =.

The potential broader complex linked to the key Cepheid SV Vul , keywords =

Reference 97

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.387960Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.387960Z digest=sha256:b68b6865244f40ec14006c5b2d062c0c951888ea0e5003ff40cbd4a7cfbe2d16

Observation 63e5cbb3-5893-45b1-ae2a-d3f288625516 · outbound

This paper cites , keywords =.

The potential broader complex linked to the key Cepheid SV Vul , keywords =

Reference 98

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.392685Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.392685Z digest=sha256:179be4296d293f1071d835543057d82f87006e94a8cf9c60deb0b8f0b8672abc

Observation ce6bbd60-1513-4931-a033-8d35e5bbe551 · outbound

This paper cites The Milky Way Cepheid Leavitt law based on Gaia DR2 parallaxes of companion stars and host open cluster populations.

The potential broader complex linked to the key Cepheid SV Vul The Milky Way Cepheid Leavitt law based on Gaia DR2 parallaxes of companion stars and host open cluster populations

Reference 99

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.397031Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.397031Z digest=sha256:836de034f08600c52adf9e692c195ccdc085cbfff09b2e10630de26f4a0b3c70

Observation 6486b369-94f7-4485-bef4-d972a5b615e7 · outbound

This paper cites A re-classification of Cepheids in the Gaia Data Release 2.

The potential broader complex linked to the key Cepheid SV Vul A re-classification of Cepheids in the Gaia Data Release 2

Reference 100

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.401795Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.401795Z digest=sha256:3d299e2ed80ca9c5bdad3e39092e98e3afd280b3bc753bdc3423ac13a68dab5a

Observation b974e5ef-dd6d-4456-ae09-0b5460558a96 · outbound

This paper cites A geometrical 1% distance to the short-period binary Cepheid V1334 Cygni.

The potential broader complex linked to the key Cepheid SV Vul A geometrical 1% distance to the short-period binary Cepheid V1334 Cygni

Reference 101

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.407025Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.407025Z digest=sha256:2b5e587f70635c50366191d0a10a3338cb01abf732c17e14e16bb09f9461b83e

Pith citing papers

No inbound Pith citation observations are available.