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Paper Citation Record · LEDGER

Detection of persistent helium absorption in the 91bg-like type Ia Supernova 2022an

As of 6 August 2026, this Paper Citation Record lists 12 of 12 outbound references and 0 inbound Pith citation observations for arXiv:2605.07827.

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

pith.paper-citation-record.v1
2605.07827 v1

Coverage vector

measured 12 of 12 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-05-11T01:54:24.850586Z

measured 12 of 12 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-06T06:34:29.942622+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

12 of 12 outbound references displayed

  • verified exact1
  • verified fuzzy6
  • unresolved4
  • parse uncertain0
  • malformed identifier1
  • metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

Observation 43c500db-efed-48ba-b217-6a697c14e628 · outbound

This paper cites 2026, A&A, 707, A91, doi: 10.1051/0004-6361/202555976 Barkhudaryan, L.

Detection of persistent helium absorption in the 91bg-like type Ia Supernova 2022an 2026, A&A, 707, A91, doi: 10.1051/0004-6361/202555976 Barkhudaryan, L

Reference 1

Resolution
verified exact
doi, observed 2026-05-11T01:55:51.095649Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

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Observation 961b14cc-d4b8-4ffe-b971-c1e634467fbc · outbound

This paper cites an unresolved cited work.

Detection of persistent helium absorption in the 91bg-like type Ia Supernova 2022an Unresolved cited work

Reference 2

Resolution
unresolved
raw_fallback, observed 2026-05-14T15:16:40.567313Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

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Observation 4adfd660-7cfb-468f-a189-f965c2a298df · outbound

This paper cites The basic data reduction, including bias subtraction, flat-field correction, and astrometric solu- tion, was performed using the PESSTO pipeline (Smartt et al.

Detection of persistent helium absorption in the 91bg-like type Ia Supernova 2022an The basic data reduction, including bias subtraction, flat-field correction, and astrometric solu- tion, was performed using the PESSTO pipeline (Smartt et al

Reference 3

Resolution
verified fuzzy
raw_fallback, observed 2026-05-14T15:16:40.571552Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

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Observation 28cd6bc3-15a0-4b60-a2f2-d0a967e096c0 · outbound

This paper cites We performed PSF photometry with thedaophottask inIRAF(Tody 1986, 1993).

Detection of persistent helium absorption in the 91bg-like type Ia Supernova 2022an We performed PSF photometry with thedaophottask inIRAF(Tody 1986, 1993)

Reference 4

Resolution
verified fuzzy
raw_fallback, observed 2026-05-14T15:16:40.561606Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

source=pdf_text observed=2026-05-11T01:54:24.850586Z digest=sha256:63baac0addc82d243cf3b9fb52f30f664e3a156cc4ffe95044b9ef1d31a8a971

Observation 3c58096d-19e3-42b4-ac3a-d62723e31208 · outbound

This paper cites an unresolved cited work.

Detection of persistent helium absorption in the 91bg-like type Ia Supernova 2022an Unresolved cited work

Reference 5

Resolution
unresolved
raw_fallback, observed 2026-05-14T15:16:40.565347Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

source=pdf_text observed=2026-05-11T01:54:24.850586Z digest=sha256:b11013e9fd86f48f845fe4c6e10d80eccc34192c33b102bf0c8b7d5db5ad4642

Observation a22242dd-1888-491f-98fc-33b1fbe569eb · outbound

This paper cites All these photometry procedures were performed using thepmpyeasypipeline (Chen et al.

Detection of persistent helium absorption in the 91bg-like type Ia Supernova 2022an All these photometry procedures were performed using thepmpyeasypipeline (Chen et al

Reference 6

Resolution
verified fuzzy
raw_fallback, observed 2026-05-14T15:16:40.573484Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

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Observation 85b17f3e-1c30-4a04-a0bf-0876574edcc5 · outbound

This paper cites Image Subtraction (No reference flux added).

Detection of persistent helium absorption in the 91bg-like type Ia Supernova 2022an Image Subtraction (No reference flux added)

Reference 7

Resolution
verified fuzzy
raw_fallback, observed 2026-05-14T15:16:40.581030Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

source=pdf_text observed=2026-05-11T01:54:24.850586Z digest=sha256:a83297c9ff906d8e1d2c56574abe8bafde0c88f3a7c4294dd00b756eac596650

Observation d60100a3-9d08-4e87-a1b2-d86b37c02769 · outbound

This paper cites SOAR/GHTS—SN 2022an was observed on 2022 Jan- uary 7 by the Goodman High Throughput Spectrograph (GHTS; Clemens et al.

Detection of persistent helium absorption in the 91bg-like type Ia Supernova 2022an SOAR/GHTS—SN 2022an was observed on 2022 Jan- uary 7 by the Goodman High Throughput Spectrograph (GHTS; Clemens et al

Reference 8

Resolution
verified fuzzy
raw_fallback, observed 2026-05-14T15:16:40.569242Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

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Observation d99cc60d-2b0f-41df-8094-602770c47a4e · outbound

This paper cites 400 SYZY.

Detection of persistent helium absorption in the 91bg-like type Ia Supernova 2022an 400 SYZY

Reference 9

Resolution
malformed identifier
raw_fallback, observed 2026-05-14T15:16:40.563419Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

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Observation f834e7aa-fdb2-4223-946e-c30913b70ba7 · outbound

This paper cites an unresolved cited work.

Detection of persistent helium absorption in the 91bg-like type Ia Supernova 2022an Unresolved cited work

Reference 10

Resolution
unresolved
raw_fallback, observed 2026-05-14T15:16:40.579034Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

source=pdf_text observed=2026-05-11T01:54:24.850586Z digest=sha256:b79ddfb5631660058d9ba124562c6309c4e78ef3e1ea4ffd19fed892ce427715

Observation 80629057-59c4-48c5-94fc-8bb1d0a26809 · outbound

This paper cites an unresolved cited work.

Detection of persistent helium absorption in the 91bg-like type Ia Supernova 2022an Unresolved cited work

Reference 11

Resolution
unresolved
raw_fallback, observed 2026-05-14T15:16:40.577125Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

source=pdf_text observed=2026-05-11T01:54:24.850586Z digest=sha256:3e2dab079e2992fe6cc9c25d0730b20c1794a348a725bf4e144a3d9e60fcc03d

Observation e52e6b94-2700-4fe8-920b-856ac01c7882 · outbound

This paper cites The FIRE spectrum was taken with the long-slit mode, and the data were reduced with the IDL pipelinefirehose (Simcoe et al.

Detection of persistent helium absorption in the 91bg-like type Ia Supernova 2022an The FIRE spectrum was taken with the long-slit mode, and the data were reduced with the IDL pipelinefirehose (Simcoe et al

Reference 12

Resolution
verified fuzzy
raw_fallback, observed 2026-05-14T15:16:40.575416Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

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Pith citing papers

No inbound Pith citation observations are available.