Paper Citation Record · LEDGER

First mid-infrared detection and modeling of a flare from Sgr A*

As of 10 August 2026, this Paper Citation Record lists 12 of 12 outbound references and 2 inbound Pith citation observations for arXiv:2501.07415.

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

pith.paper-citation-record.v1
2501.07415 v1

Coverage vector

measured 12 of 12 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-10T20:47:15.534746Z

measured 14 of 14 standing notices

One-hop event checks from named stored sources.

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

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-03T03:08:21.806849Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-21T13:10:10.295630Z

Reference resolution

12 of 12 outbound references displayed

verified exact0
verified fuzzy10
unresolved2
parse uncertain0
malformed identifier0
metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

Observation 9364881c-1edf-4ce9-9eab-af35bda941ca · outbound

This paper cites Strongly magnetized accretion with low angular momentum produces a weak jet.

First mid-infrared detection and modeling of a flare from Sgr A* Strongly magnetized accretion with low angular momentum produces a weak jet

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-10T20:47:15.439757Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6b3b0cc2-3232-4ce5-bd04-9f73ffbc5068 · outbound

This paper cites Axis labels are in pixel number with pixel angular sizes given in the text.

First mid-infrared detection and modeling of a flare from Sgr A* Axis labels are in pixel number with pixel angular sizes given in the text

Reference 4

Resolution: verified fuzzy; raw_fallback, observed 2026-08-10T20:47:15.875144Z

Source-reported events for the cited work

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

Observation 4ecf5473-e827-4ffc-8b84-acfde970e079 · outbound

This paper cites (C5) 16 No particle escape term (Blumenthal & Gould 1970; Dodds-Eden et al.

First mid-infrared detection and modeling of a flare from Sgr A* (C5) 16 No particle escape term (Blumenthal & Gould 1970; Dodds-Eden et al

Reference 6

Resolution: verified fuzzy; raw_fallback, observed 2026-08-10T20:47:15.752291Z

Source-reported events for the cited work

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

Observation fb0c377c-64c0-4734-8869-91d8175704de · outbound

This paper cites 2023; Lemoine.

First mid-infrared detection and modeling of a flare from Sgr A* 2023; Lemoine

Reference 7

Resolution: verified fuzzy; raw_fallback, observed 2026-08-10T20:47:15.732419Z

Source-reported events for the cited work

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

Observation b155fc63-dce0-459a-b0e3-336ab015935d · outbound

This paper cites longitude.

First mid-infrared detection and modeling of a flare from Sgr A* longitude

Reference 8

Resolution: verified fuzzy; raw_fallback, observed 2026-08-10T20:47:15.707246Z

Source-reported events for the cited work

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

Observation 8ee5a375-b6fb-4670-8302-ae19b41c3103 · outbound

This paper cites an unresolved cited work.

First mid-infrared detection and modeling of a flare from Sgr A* Unresolved cited work

Reference 10

Resolution: unresolved; raw_fallback, observed 2026-08-10T20:47:15.657164Z

Source-reported events for the cited work

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

Observation 224c7373-984e-491f-90b3-633fcf033ff5 · outbound

This paper cites In the absence of astrometric or polarimetric measurements of the flare, the orbital parameters of the flare are poorly constrained.

First mid-infrared detection and modeling of a flare from Sgr A* In the absence of astrometric or polarimetric measurements of the flare, the orbital parameters of the flare are poorly constrained

Reference 20

Resolution: verified fuzzy; raw_fallback, observed 2026-08-10T20:47:15.622083Z

Source-reported events for the cited work

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

Observation b1c9e91c-dda0-476c-a7b8-e42f41405dc8 · outbound

This paper cites We therefore set p = 2, which gives the canonically observed NIR spectral slope Fν,NIR ∝ ν−0.5 (e.g., Hornstein et al.

First mid-infrared detection and modeling of a flare from Sgr A* We therefore set p = 2, which gives the canonically observed NIR spectral slope Fν,NIR ∝ ν−0.5 (e.g., Hornstein et al

Reference 104

Resolution: verified fuzzy; raw_fallback, observed 2026-08-10T20:47:15.638152Z

Source-reported events for the cited work

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

Observation 7bf419d6-3abb-4938-98e8-d3d15b708c95 · outbound

This paper cites Haubois et al.

First mid-infrared detection and modeling of a flare from Sgr A* Haubois et al

Reference 2011

Resolution: verified fuzzy; raw_fallback, observed 2026-08-10T20:47:15.841802Z

Source-reported events for the cited work

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

Observation f1dc40d6-bb8d-4560-918a-9d84fb6e6b02 · outbound

This paper cites We used a standard setup of 32 “walkers” and started the sampling chain at a region visually perceived as a good fit.

First mid-infrared detection and modeling of a flare from Sgr A* We used a standard setup of 32 “walkers” and started the sampling chain at a region visually perceived as a good fit

Reference 2013

Resolution: verified fuzzy; raw_fallback, observed 2026-08-10T20:47:15.685559Z

Source-reported events for the cited work

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

Observation cfdd5756-9864-4170-b555-2115300ff8c7 · outbound

This paper cites 2023; Lemoine 2023).

First mid-infrared detection and modeling of a flare from Sgr A* 2023; Lemoine 2023)

Reference 2023

Resolution: verified fuzzy; raw_fallback, observed 2026-08-10T20:47:15.771405Z

Source-reported events for the cited work

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

Observation 87278713-5ba3-405c-bebc-3dbc583d5de9 · outbound

This paper cites 2020, 2023).

First mid-infrared detection and modeling of a flare from Sgr A* 2020, 2023)

Reference 2024

Resolution: verified fuzzy; raw_fallback, observed 2026-08-10T20:47:15.813459Z

Source-reported events for the cited work

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

Pith citing papers

Observation 00519de5-5497-4f05-83fb-c132c90f51b6 · inbound

Polarization Signatures of Inspiraling Hotspots around Kerr Black Holes cites this paper.

Polarization Signatures of Inspiraling Hotspots around Kerr Black Holes First mid-infrared detection and modeling of a flare from Sgr A*

Reference 8

Resolution: verified exact; arxiv_id, observed 2026-05-21T13:10:10.297731Z

Source-reported events for the cited work

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

Observation 462d28b1-53d9-4b4b-a6e7-3999a543516c · inbound

Polarization Signatures of Inspiraling Hotspots around Kerr Black Holes cites this paper.

Polarization Signatures of Inspiraling Hotspots around Kerr Black Holes First mid-infrared detection and modeling of a flare from Sgr A*

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-03T03:08:21.806849Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.