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Paper Citation Record · LEDGER

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs

As of 15 August 2026, this Paper Citation Record lists 100 of 279 outbound references and 0 inbound Pith citation observations for arXiv:2608.13259.

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

pith.paper-citation-record.v1
2608.13259 v1

Coverage vector

measured 100 of 279 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-14T15:20:02.445134Z

measured 100 of 100 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-14T06:32:32.682623+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 279 outbound references displayed

  • verified exact25
  • verified fuzzy0
  • unresolved75
  • parse uncertain0
  • malformed identifier0
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External citation measurements

No source-named external measurement is stored.

Outbound references

Observation fae2446f-971b-4d7d-9c84-2af1a052116f · outbound

This paper cites A natural explanation for periodic X-ray outbursts in Be/X-ray binaries.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs A natural explanation for periodic X-ray outbursts in Be/X-ray binaries

Reference 1

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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:01.842978Z digest=sha256:ca27f145ccb0e55a47b9919eeb3336876c9bb3eece4b2c50ef36fcd9a386323f

Observation 8e401dc7-16a9-430c-9944-9e4ec7b73513 · outbound

This paper cites an unresolved cited work.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs Unresolved cited work

Reference 2

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no resolver link, observed 2026-08-14T15:20:01.850963Z

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:01.850963Z digest=sha256:815179dc026ce5804e1c0c9b10c3c55b638726e65981f1497b2481999021537a

Observation 70cd2f59-e319-4e75-bc94-e4af37059a9f · outbound

This paper cites A Be-type star with a black hole companion.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs A Be-type star with a black hole companion

Reference 3

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no resolver link, observed 2026-08-14T15:20:01.856575Z

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source=arxiv_source observed=2026-08-14T15:20:01.856575Z digest=sha256:be44df5c54760f4774b13d54718ddb5a71c8bb6e7e891213f7c1a3136e96009a

Observation 54433169-5784-4af0-8a88-5ebd2b76efa1 · outbound

This paper cites A catalogue of high-mass X-ray binaries in the Galaxy: from the INTEGRAL to the Gaia era.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs A catalogue of high-mass X-ray binaries in the Galaxy: from the INTEGRAL to the Gaia era

Reference 4

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no resolver link, observed 2026-08-14T15:20:01.862870Z

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Unavailable: canonical work link unavailable.

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Observation 8f7d2704-009c-414f-a469-b7ae87ea91f0 · outbound

This paper cites an unresolved cited work.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs Unresolved cited work

Reference 5

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Unavailable: canonical work link unavailable.

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Observation c61ad9e0-9a05-4543-a71d-06edb0b63d78 · outbound

This paper cites an unresolved cited work.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs Unresolved cited work

Reference 6

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Unavailable: canonical work link unavailable.

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Observation d6f3592f-cefa-44a3-b8f2-3ca38b5f4a0d · outbound

This paper cites and Gaensler, B.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs and Gaensler, B

Reference 7

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no resolver link, observed 2026-08-14T15:20:01.884466Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:01.884466Z digest=sha256:4b39a071d2c7ab528afc9106ce7cb6662a8ca8561d7fe5e7f46e0faaea5960a2

Observation 5e8dabb0-08b6-49d9-b526-21c87a78d57c · outbound

This paper cites Gorski, M , year = 2021, month = mar, volume =.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs Gorski, M , year = 2021, month = mar, volume =

Reference 9

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no resolver link, observed 2026-08-14T15:20:01.905269Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:01.905269Z digest=sha256:54dbbdaa9d136c1b1b7444f2c16e2b831887a0bc75d448a877304e2895543c22

Observation 4edffe93-9675-4dd7-8db0-dc9b4d670eb8 · outbound

This paper cites doi:10.3847/1538-3881/abd806 , annotation =.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs doi:10.3847/1538-3881/abd806 , annotation =

Reference 10

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no resolver link, observed 2026-08-14T15:20:01.911575Z

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:01.911575Z digest=sha256:4f770123e570073e598d4c95c71e3c44fb732d8e1f823069858833f18bc7cede

Observation 87376682-9b9a-4982-9283-36fed09e33bd · outbound

This paper cites Looking at.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs Looking at

Reference 11

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Observation 4c2c45eb-0062-43de-bdb4-d865fd08e679 · outbound

This paper cites an unresolved cited work.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs Unresolved cited work

Reference 12

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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 844ea059-c2bf-49cd-9ff6-5837695b7f68 · outbound

This paper cites , author =.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs , author =

Reference 13

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Unavailable: canonical work link unavailable.

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Observation 728ed4a6-ee15-4370-9d0c-788eba0a706b · outbound

This paper cites an unresolved cited work.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs Unresolved cited work

Reference 14

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unresolved
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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation c284ddd4-5943-4901-9961-f433585b4e4a · outbound

This paper cites and Pramod Kumar, S.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs and Pramod Kumar, S

Reference 15

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Unavailable: canonical work link unavailable.

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Observation 56db500b-fc51-4423-a454-2a66542d9ae4 · outbound

This paper cites an unresolved cited work.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs Unresolved cited work

Reference 16

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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation ff52c016-fb8a-4b27-892d-3fa0f2388a85 · outbound

This paper cites and Shenar, T.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs and Shenar, T

Reference 17

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Unavailable: canonical work link unavailable.

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Observation 3abf54f3-8f54-4e6e-80ca-07c1f9d4e818 · outbound

This paper cites and Shenar, T.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs and Shenar, T

Reference 18

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unresolved
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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 35f236d1-b7a4-496e-a002-482f4c12c1d8 · outbound

This paper cites an unresolved cited work.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs Unresolved cited work

Reference 19

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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 3ade511f-9e1f-492c-9fd7-5f0a608b5d84 · outbound

This paper cites an unresolved cited work.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs Unresolved cited work

Reference 20

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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 56b87cfb-b419-49c5-86ea-43843a38784e · outbound

This paper cites Classification of 3 Accreting Binaries with.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs Classification of 3 Accreting Binaries with

Reference 21

Resolution
verified exact
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Source-reported events for the cited work

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Observation b6faf3e7-94aa-4ac6-97f0-fb0e42d0b3e1 · outbound

This paper cites and Falanga, M.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs and Falanga, M

Reference 22

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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 5a157ab1-a918-4891-9da4-637b0a665055 · outbound

This paper cites and Stella, L.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs and Stella, L

Reference 23

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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 493f2d5e-9a18-454a-9e5b-fc23a8d0da56 · outbound

This paper cites and Pavan, L.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs and Pavan, L

Reference 24

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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 3e96e729-2926-45f4-bec2-9231bedcb745 · outbound

This paper cites Supergiant fast X-ray transients as an under-luminous class of supergiant X-ray binaries.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs Supergiant fast X-ray transients as an under-luminous class of supergiant X-ray binaries

Reference 25

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Unavailable: canonical work link unavailable.

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Observation 8e6bc718-1480-44fa-82a2-79c7bc1c78c6 · outbound

This paper cites and Romano, P.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs and Romano, P

Reference 26

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no resolver link, observed 2026-08-14T15:20:02.006748Z

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Unavailable: canonical work link unavailable.

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Observation 1deb76eb-a216-49fb-8e24-2c3371b8b1cd · outbound

This paper cites and Bernardini, F.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs and Bernardini, F

Reference 27

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Unavailable: canonical work link unavailable.

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Observation 798482b8-70a2-445f-8714-a2452cac7cdd · outbound

This paper cites doi:10.1051/0004-6361/201732004 , langid =.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs doi:10.1051/0004-6361/201732004 , langid =

Reference 28

Resolution
verified exact
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

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Observation 73fed4e8-a22b-4210-9ba6-20b077d2a38a · outbound

This paper cites and Rotschild, R.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs and Rotschild, R

Reference 29

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unresolved
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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 28014304-d5ff-4fe3-a4ba-a98e8d32c834 · outbound

This paper cites and Bildsten, Lars and Rutledge, Robert E.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs and Bildsten, Lars and Rutledge, Robert E

Reference 30

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unresolved
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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 78159031-10f8-49ec-a859-c1543b7846ba · outbound

This paper cites and Liu, T.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs and Liu, T

Reference 31

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no resolver link, observed 2026-08-14T15:20:02.032747Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 19aab1ed-9d68-46f5-93d5-dd80af1298d3 · outbound

This paper cites The SRG/eROSITA All-Sky Survey: The first catalog of galaxy clusters and groups in the Western Galactic Hemisphere.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs The SRG/eROSITA All-Sky Survey: The first catalog of galaxy clusters and groups in the Western Galactic Hemisphere

Reference 32

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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation c91846d2-32fe-4fb5-bd6a-366107431dd1 · outbound

This paper cites doi:10.1051/0004-6361/201730769 , langid =.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs doi:10.1051/0004-6361/201730769 , langid =

Reference 33

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no resolver link, observed 2026-08-14T15:20:02.043444Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation a99c0205-b04a-416b-adde-7774b32cf385 · outbound

This paper cites and Gastaldello, F.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs and Gastaldello, F

Reference 34

Resolution
verified exact
doi, observed 2026-08-14T15:23:53.881846Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

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Observation c06d0347-b903-467e-822f-859a0145c349 · outbound

This paper cites and Stella, L.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs and Stella, L

Reference 36

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:02.058995Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:02.058995Z digest=sha256:dc122fe2320cae71ac5d5ffbbb0512cbf6ba6568e6f7529d0a9364ddaf27e3e0

Observation 310ce646-de81-463c-a8db-08532197e84e · outbound

This paper cites and Petrucci, P.-O.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs and Petrucci, P.-O

Reference 37

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:02.064258Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 9fb155ad-87fa-4634-811f-3c90aa6b8c32 · outbound

This paper cites Challenging Classical Paradigms: Recurrent Nova M31N 2017-01e, a BeWD system in M31?.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs Challenging Classical Paradigms: Recurrent Nova M31N 2017-01e, a BeWD system in M31?

Reference 38

Resolution
verified exact
local_arxiv, observed 2026-08-14T15:23:53.847814Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

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Observation cef5674c-c02f-49d3-a46f-214c07ee387f · outbound

This paper cites Long-term spin-down and low luminosity regime in the Be/X-ray binary pulsar GX 304-1.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs Long-term spin-down and low luminosity regime in the Be/X-ray binary pulsar GX 304-1

Reference 39

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unresolved
no resolver link, observed 2026-08-14T15:20:02.076493Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:02.076493Z digest=sha256:cb5191f070da190ea24cc69f2ebb816fc1964b61671d06056839e2235f891e0c

Observation 831fd96c-1e25-4b02-9e10-0346277cfbcb · outbound

This paper cites an unresolved cited work.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs Unresolved cited work

Reference 40

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:02.082616Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:02.082616Z digest=sha256:45ab62dd94cc39e7cd92b8548af97578c43bce794a0572cf58cce38eaf8b6c72

Observation e6181087-1cf4-4da4-a99e-7c775df8915b · outbound

This paper cites Optical and.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs Optical and

Reference 43

Resolution
verified exact
doi, observed 2026-08-14T15:23:53.804905Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-08-14T15:20:02.097156Z digest=sha256:a03c38a285d780e664ec5358172e4d018a6e70865160e8cf6cadd2848d178caa

Observation 234d72cc-99d1-4e42-94f1-abdfb5d5a0ed · outbound

This paper cites doi:10.1093/mnras/stad1991 , journal =.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs doi:10.1093/mnras/stad1991 , journal =

Reference 44

Resolution
verified exact
doi, observed 2026-08-14T15:23:53.790407Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-08-14T15:20:02.102729Z digest=sha256:b0470448584a9e8d1d2553b44096f93f466287b6bdb3cb39a9d9ac8db677117d

Observation 758e894a-eaa0-47a3-8732-cee7aaab1546 · outbound

This paper cites an unresolved cited work.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs Unresolved cited work

Reference 45

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:02.107679Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:02.107679Z digest=sha256:5b52c5f8779544aaac1d0d69f267a8f5b9914165688880926562d2b3be7491c6

Observation f4897cf8-576e-4606-a363-b9114cf32713 · outbound

This paper cites , year = 2000, month = jan, journal =.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs , year = 2000, month = jan, journal =

Reference 46

Resolution
verified exact
doi, observed 2026-08-14T15:23:53.767526Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-08-14T15:20:02.112879Z digest=sha256:bb9cbc3ec55a707578c1ce5a0fa8b91c6924174cc5d74550be2c7377a98e97cd

Observation bd03223b-749f-43e7-8e5f-8bb77d328bdb · outbound

This paper cites doi:10.1051/0004-6361/202243940 , langid =.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs doi:10.1051/0004-6361/202243940 , langid =

Reference 47

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:02.118259Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:02.118259Z digest=sha256:d983aa8a267ca795d45d9f593183099e8c112d95ceefad934f2e85739f9b54a1

Observation 44b60ce4-8dcf-497a-a6d7-1b593bcc6fd5 · outbound

This paper cites an unresolved cited work.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs Unresolved cited work

Reference 48

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:02.123219Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:02.123219Z digest=sha256:b372ca358a896543609f89e37f8d6d8d0d3bf08f95d5b37bde0d5f7203779aa4

Observation a9bcb880-e784-4bfa-9e19-22c311dffc13 · outbound

This paper cites an unresolved cited work.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs Unresolved cited work

Reference 49

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:02.128415Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:02.128415Z digest=sha256:b8eebd8b0ac0f7fad3c67b31872728d22bc4cb4b723505909a93d9f0c924985e

Observation 7f4874ef-fc6b-4269-95f7-b52b5836a077 · outbound

This paper cites an unresolved cited work.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs Unresolved cited work

Reference 50

Resolution
verified exact
doi, observed 2026-08-14T15:23:53.722349Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-08-14T15:20:02.133639Z digest=sha256:64e92d1c43c759c720e38996cf015ef7814f1927f04437e11c7a9f407c6d70bb

Observation 8b642300-8048-4497-96e4-1a0863dc64ae · outbound

This paper cites doi:10.1111/j.1365-2966.2010.16749.x , langid =.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs doi:10.1111/j.1365-2966.2010.16749.x , langid =

Reference 52

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:02.143237Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:02.143237Z digest=sha256:8e061afc963a8d8f1af2e9047948f87583a62b7e09101ae8d60edb63e19f1644

Observation 680d538f-4d48-4cc5-838e-30c3ce90f59b · outbound

This paper cites doi:10.1051/0004-6361/201935978 , langid =.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs doi:10.1051/0004-6361/201935978 , langid =

Reference 54

Resolution
verified exact
doi, observed 2026-08-14T15:23:53.708551Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-08-14T15:20:02.152481Z digest=sha256:1c307ab9c91713f7c39b066234998d69327755952aadae5ff05149a5641acd9f

Observation 70473881-9ac6-43d6-b58b-ff508fb932c4 · outbound

This paper cites , year = 1973, month = jan, volume =.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs , year = 1973, month = jan, volume =

Reference 55

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:02.157250Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:02.157250Z digest=sha256:3b1a978c16cc8f3536d67a7ac7abbfa134d660050c51be4827a3dc31e84c63ed

Observation b4f9f2db-a99e-4247-ab69-ac064537b9c5 · outbound

This paper cites doi:10.1093/mnras/191.3.599 , langid =.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs doi:10.1093/mnras/191.3.599 , langid =

Reference 56

Resolution
verified exact
doi, observed 2026-08-14T15:23:53.678153Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-08-14T15:20:02.163260Z digest=sha256:f0198ab2f84a99790d1abb6f93881a74b557d6225d00cf2f40d450dddc68e381

Observation ce5ba082-0b38-4582-bacc-9b486aed1348 · outbound

This paper cites doi:10.1093/mnras/186.4.779 , langid =.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs doi:10.1093/mnras/186.4.779 , langid =

Reference 57

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:02.167974Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:02.167974Z digest=sha256:23e9f9007de02750ddec304936468ac27e859336797d0881818d2377837e3436

Observation c629b525-210e-4c9d-8cd2-3a9e4429b1a5 · outbound

This paper cites Crust Cooling of the Neutron Star in.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs Crust Cooling of the Neutron Star in

Reference 58

Resolution
verified exact
doi, observed 2026-08-14T15:23:53.647777Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-08-14T15:20:02.172727Z digest=sha256:ba88296d851ca61b2cd29554c18e170d6034e94f00032257aafc58ea9a3cd33c

Observation 30ddde8d-3b30-40b2-95c1-13d765f09bc1 · outbound

This paper cites and Perri, M.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs and Perri, M

Reference 59

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:02.177577Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:02.177577Z digest=sha256:badb3333336cae4a6dc97626e724edb763ef3d4c774589663aacb0898b2e0565

Observation abb19f33-2125-4b7f-bb7f-826a32ed97f0 · outbound

This paper cites Gaia Uncovers Difference in.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs Gaia Uncovers Difference in

Reference 60

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:02.182979Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:02.182979Z digest=sha256:10cc188b9f1fe99116bf55aceda3c70bde9b653fe1f968596c9fb823b2f31929

Observation 45a5a037-1c22-422f-8743-cd272db4ff35 · outbound

This paper cites and Santangelo, A.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs and Santangelo, A

Reference 61

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:02.188548Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:02.188548Z digest=sha256:af075e9a0d512b4eebc6c87353e0c5176cece7f2d75cc6e314f939225a75b734

Observation e2f0da95-c16d-4022-bc6d-05a21f3870e0 · outbound

This paper cites and Ducci, L.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs and Ducci, L

Reference 62

Resolution
verified exact
doi, observed 2026-08-14T15:23:53.597841Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-08-14T15:20:02.193505Z digest=sha256:d5a61fdacd5844d9aa9c7e201b73cf7b8cf7a35782fdbe2d3509c61a63f0f313

Observation 14eab6f1-6b87-408e-843c-8b66029aa19e · outbound

This paper cites and Santangelo, A.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs and Santangelo, A

Reference 63

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:02.199486Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:02.199486Z digest=sha256:4173e7fbe150a1b9d9fc8c90828f4afac9ea580e1a0e63a069c883779ce6d8a6

Observation e71362c2-08c7-49ea-81a8-37245d1beb0a · outbound

This paper cites and Santangelo, A.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs and Santangelo, A

Reference 64

Resolution
verified exact
doi, observed 2026-08-14T15:23:53.569801Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-08-14T15:20:02.204841Z digest=sha256:07a0ecbfd27349bd23f78d3da8fbea8c523d82fe1e35ac0bb4e241fb5a35c88b

Observation 5f60c2a6-f021-4848-8abc-7fdf32279c9c · outbound

This paper cites SRGA J124404.1-632232/SRGU J124403.8-632231: a new X-ray pulsar discovered in the all-sky survey by SRG.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs SRGA J124404.1-632232/SRGU J124403.8-632231: a new X-ray pulsar discovered in the all-sky survey by SRG

Reference 65

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:02.209811Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:02.209811Z digest=sha256:f632020b30af5d207a088bf57a4539635108563035e7efd7f490ee3b22d83550

Observation 6a6ddaa5-ffba-4f60-9f1f-ab2a38373c1f · outbound

This paper cites and Romano, P.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs and Romano, P

Reference 66

Resolution
verified exact
doi, observed 2026-08-14T15:23:53.552048Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-08-14T15:20:02.214921Z digest=sha256:75e4b21296ff584b7d6ea2478018267cefb6d8c5b0de7b16f9a8530b77cecc10

Observation b7de0aa7-b8ff-42d5-ae46-c51f4e3594e6 · outbound

This paper cites Modelling the Expected Very High Energy.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs Modelling the Expected Very High Energy

Reference 67

Resolution
verified exact
doi, observed 2026-08-14T15:23:53.535815Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-08-14T15:20:02.219595Z digest=sha256:2d31a8402d9e42cd7137aa76419da498bb05eb0fc95542654ffffb2cd9c2ba2f

Observation 720d4a4d-ad36-4eb5-ad71-5783430a0676 · outbound

This paper cites and Bourban, G.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs and Bourban, G

Reference 68

Resolution
verified exact
doi, observed 2026-08-14T15:23:53.519873Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-08-14T15:20:02.224625Z digest=sha256:dade6b58377319d00957418633179f2c3ba3b796b9181a7cd8ff4c0035037fcb

Observation e52b9749-7457-4bdd-a27a-8d40eec8a953 · outbound

This paper cites Evolution towards the Critical Limit and the Origin of.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs Evolution towards the Critical Limit and the Origin of

Reference 69

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:02.229595Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:02.229595Z digest=sha256:06544bbbedc6f4b3a632f07a0382b291cd7c8bf0d16e3b2529b3ed83fc99e68c

Observation 545bec64-819f-4085-b611-4f971b0baef6 · outbound

This paper cites doi:10.1093/mnras/stab285 , journal =.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs doi:10.1093/mnras/stab285 , journal =

Reference 70

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:02.235415Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:02.235415Z digest=sha256:7aaf399dd838b887e9fdf2db2be9c60a0c55b6b484b6bf00dd4b95439551dbda

Observation cda07ac8-dbc9-4542-a2a8-50320559eba3 · outbound

This paper cites doi:10.1093/mnras/stac2422 , langid =.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs doi:10.1093/mnras/stac2422 , langid =

Reference 72

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:02.245922Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:02.245922Z digest=sha256:39729985848d58276f621bce780bb602bb47bef5c13eb5a1cd32b20850100dfd

Observation 432f28c4-574c-4f06-a92f-a12ca2e7f2a4 · outbound

This paper cites and Heinke, Craig O.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs and Heinke, Craig O

Reference 73

Resolution
verified exact
doi, observed 2026-08-14T15:23:53.463336Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-08-14T15:20:02.250481Z digest=sha256:a7b94152445c6bef0d15cc74642536fc2befed2cca84a9f237aee8b2b4b7db7d

Observation 7d98aee8-ad5e-4109-b3cd-eafe73d34b6b · outbound

This paper cites an unresolved cited work.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs Unresolved cited work

Reference 74

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:02.255530Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:02.255530Z digest=sha256:468a11ec93ab7815b4cd50739185285c809299e1fa20eb804e8df3ef249f004b

Observation 950df7c1-75c0-4ab6-a505-b9710e1dfadd · outbound

This paper cites Discovery of accretion-driven pulsations in the prolonged low X-ray luminosity state of the Be/X-ray transient GX 304-1.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs Discovery of accretion-driven pulsations in the prolonged low X-ray luminosity state of the Be/X-ray transient GX 304-1

Reference 75

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:02.260455Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:02.260455Z digest=sha256:fdb8e206f133c7921e9f6c6b49f7f93a7702f75c7d16a24ef2be008db23f2558

Observation 19209474-b8cd-44ec-8249-cb36f65d6acd · outbound

This paper cites an unresolved cited work.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs Unresolved cited work

Reference 76

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:02.265455Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:02.265455Z digest=sha256:c3850546fae287f9589bf0af56fe14a4347e1e49d4673566258a53f6c1788b68

Observation 34c43486-8474-483f-8042-a3d63727fd62 · outbound

This paper cites an unresolved cited work.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs Unresolved cited work

Reference 77

Resolution
verified exact
doi, observed 2026-08-14T15:23:53.432391Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-08-14T15:20:02.270463Z digest=sha256:8ff19daa7262ee857711850367b50aea0e3ddadf52c90499f7a7817b701ce4b6

Observation 2a6a5f01-4481-42a9-a4ee-451c1e89a593 · outbound

This paper cites High-Mass.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs High-Mass

Reference 78

Resolution
verified exact
doi, observed 2026-08-14T15:23:53.418708Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-08-14T15:20:02.275685Z digest=sha256:bcb64b6909b5129d1a364d293abbe8f3f85fe79748149d9554612c7a8573938c

Observation 5a935191-8c47-429b-8942-58acbf90e77e · outbound

This paper cites and Sguera, V.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs and Sguera, V

Reference 79

Resolution
verified exact
doi, observed 2026-08-14T15:23:53.404343Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-08-14T15:20:02.281272Z digest=sha256:8f3d316cf25761276e82216b2bdd7e80850112d52872a81477a58d1e2a41ddd1

Observation 2de33101-4f3a-4928-bae7-f6205a99c3ca · outbound

This paper cites an unresolved cited work.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs Unresolved cited work

Reference 80

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:02.286252Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:02.286252Z digest=sha256:09a7ec0ed18cbf6bdbe9b414d8433b8705b92f0bf523fcf5b7b62565e90e1316

Observation 093e1f3c-0146-4fdd-ac59-e4163dc18844 · outbound

This paper cites and Chaty, S.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs and Chaty, S

Reference 81

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:02.291052Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:02.291052Z digest=sha256:2395ee1280fcf8a62ac90c55f2370c78edba1e6bb7f68da80774e9090ce9d755

Observation a99221fd-6306-4283-b136-f08f7de95cba · outbound

This paper cites Constraints to Neutron-Star Kicks in High-Mass.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs Constraints to Neutron-Star Kicks in High-Mass

Reference 82

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:02.296151Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:02.296151Z digest=sha256:78f0a308691e2321338a2ef14b67c36a396e97340a3fecb4b54642f4459d463f

Observation 354c60a1-87be-4f3f-8e80-7c1c37679d7e · outbound

This paper cites A Catalogue of High-Mass.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs A Catalogue of High-Mass

Reference 83

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:02.301633Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:02.301633Z digest=sha256:31b6f28e718742a4c5a8565f945f278d3e88f047a356064e7d0ac49d614561ab

Observation d6cc0488-4d6d-4b6b-b64b-df9d884da14e · outbound

This paper cites an unresolved cited work.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs Unresolved cited work

Reference 84

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:02.306518Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:02.306518Z digest=sha256:fa7614454b01592c4f56541d2f5dcdcf5ace7dcc29616b81a1729c94772e7e67

Observation 8135f7cb-2b97-4dac-8215-80c905cce6a8 · outbound

This paper cites CXOU J005245.0-722844: Discovery of a Be Star / White Dwarf binary system in the SMC via a very fast, super-Eddington X-ray outburst event.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs CXOU J005245.0-722844: Discovery of a Be Star / White Dwarf binary system in the SMC via a very fast, super-Eddington X-ray outburst event

Reference 85

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:02.311711Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:02.311711Z digest=sha256:d433e8076a18ba96f4cd4cf9aa4d658d7013c4a865573e050a4dc5c6e6be3763

Observation 6c35389a-37e2-4c57-840c-22ce71b59eae · outbound

This paper cites and Lehmer, Bret D.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs and Lehmer, Bret D

Reference 86

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:02.317767Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:02.317767Z digest=sha256:bd4b96420508ad61abcffbe50dd4ddfaff3ec95bbe1819cd3e6fe5c8ffdb0227

Observation 997f49a2-00b7-4cfa-953c-09b31f906ad1 · outbound

This paper cites Low-Luminosity Observation of.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs Low-Luminosity Observation of

Reference 87

Resolution
verified exact
doi, observed 2026-08-14T15:23:53.320106Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-08-14T15:20:02.323163Z digest=sha256:2153e8b1dcfe4fe57ded52f6fbf79922755eac74f971e42e4a2a3b04ee64da4a

Observation 6f737c33-f049-482d-86dc-3928eda8aeb6 · outbound

This paper cites Gamma Cas Stars as Be + White Dwarf Binary Systems.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs Gamma Cas Stars as Be + White Dwarf Binary Systems

Reference 88

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:02.328444Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:02.328444Z digest=sha256:d42dc7b968176953202632e109c71ea9df81b6d2ab10d31ff3216e146bfa0cc6

Observation d7d3cac6-d868-4298-bba2-f2fb298fcc1c · outbound

This paper cites an unresolved cited work.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs Unresolved cited work

Reference 89

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:02.333768Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:02.333768Z digest=sha256:c190f2f16713e7b0d4468ac3d37c9a0f89c19f885a6a1f992774c6ea3fa23229

Observation 57efd1e0-ed35-4cd1-8be7-89a4a5e44877 · outbound

This paper cites doi:10.1093/mnras/sty3236 , journal =.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs doi:10.1093/mnras/sty3236 , journal =

Reference 90

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:02.339356Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:02.339356Z digest=sha256:66b1bfa603fc2af689ed81aa255de221b4c751a4a1bd3a4e011c9a820f2c868c

Observation 969a3edf-5bb9-4294-9247-a3f68446d817 · outbound

This paper cites and Ekstr.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs and Ekstr

Reference 91

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:02.344222Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:02.344222Z digest=sha256:489458b6d6448723afe89cb0f816365c0d9dc42e95ffc8d37a0af0e8fda8c103

Observation af42c885-8b21-4a36-b6f7-8fb9cec8df87 · outbound

This paper cites an unresolved cited work.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs Unresolved cited work

Reference 92

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:02.349204Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:02.349204Z digest=sha256:21903527622ff6994ecedd6813e0fdf08157e73f6c6b6060a3064248f2a349d7

Observation c54243cc-9a90-4d0a-9135-0327ea82a4fb · outbound

This paper cites and Gilfanov, M.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs and Gilfanov, M

Reference 93

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:02.354086Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:02.354086Z digest=sha256:1842870107300bada595dc114baebda3081706d1d5f941770f6eac63d52f00be

Observation 3ca0aba3-3222-419f-932b-4c1479122075 · outbound

This paper cites an unresolved cited work.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs Unresolved cited work

Reference 94

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:02.359602Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:02.359602Z digest=sha256:d5692f0837a634479163b6e4abb94b5c1f4f8e7fa1a0dd28f767658f9e22340c

Observation 3c4dfcea-9f95-41a2-9b7f-246497a788b2 · outbound

This paper cites and Gilfanov, M.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs and Gilfanov, M

Reference 95

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:02.364791Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:02.364791Z digest=sha256:8c93798fbd5c7fdbff52ac4ad413f3ed3ac965481687ab304e8cd33ee07720e5

Observation 65db6d65-3049-49b1-9b43-d4a99a41fb91 · outbound

This paper cites doi:10.1093/mnras/stz2795 , journal =.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs doi:10.1093/mnras/stz2795 , journal =

Reference 96

Resolution
verified exact
doi, observed 2026-08-14T15:23:53.254897Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-08-14T15:20:02.369996Z digest=sha256:f793685d7860d3080c8f647bf1e3b1ce4004ab4f15080739667616fec062e937

Observation e97bda3f-6ebf-42cc-9d6d-624dc3175879 · outbound

This paper cites and Sturm, R.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs and Sturm, R

Reference 97

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:02.375034Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:02.375034Z digest=sha256:7a598eeffbd8bcf62a8c3724c8cb293db1e2345d0f5f095961e1d99883a2244c

Observation 288cfff7-4b5d-4173-90f9-06401d490dad · outbound

This paper cites and Craig, William W.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs and Craig, William W

Reference 100

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:02.390754Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:02.390754Z digest=sha256:d82064dd5ebfc0680a4b376f53bb42ec465df3010b0cc2c7f0112259f40bf20b

Observation 54f018b3-38da-4ed3-900e-6eba3da7b321 · outbound

This paper cites The Single Star Path to.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs The Single Star Path to

Reference 101

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:02.395950Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:02.395950Z digest=sha256:139c782d40cd67c40e482b874c3b33d5afb48a215718ce99cbc1b265ed3411b8

Observation bbd07034-4d5e-4c8d-9ff7-fccf055297f6 · outbound

This paper cites and Langer, N.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs and Langer, N

Reference 102

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:02.401966Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:02.401966Z digest=sha256:97c8f388cad639132ddefcb9070d6ccb3b0429fef3ece11315e97acf8ee65db2

Observation 6e0bc732-dba2-4c03-8211-45269fcfe0ba · outbound

This paper cites Combined Analysis of Neutron Star Natal Kicks Using Proper Motions and Parallax Measurements for Radio Pulsars and.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs Combined Analysis of Neutron Star Natal Kicks Using Proper Motions and Parallax Measurements for Radio Pulsars and

Reference 104

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:02.412298Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:02.412298Z digest=sha256:1f3fa5c95f726f3804aa4ef3450400e6005e696f48f669d4b276820172e86a66

Observation cf922e3e-0258-4ca5-9f2b-ee30370e5fd6 · outbound

This paper cites an unresolved cited work.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs Unresolved cited work

Reference 105

Resolution
verified exact
doi, observed 2026-08-14T15:23:53.193926Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-08-14T15:20:02.417381Z digest=sha256:cf5f1432d0223f6baed908d9144b19ed6c46f213c2d302ca86c93bd85230e1ab

Observation 6f1ea731-927c-4d09-bd86-d8f737a0ffd3 · outbound

This paper cites an unresolved cited work.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs Unresolved cited work

Reference 106

Resolution
verified exact
doi, observed 2026-08-14T15:23:53.180827Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-08-14T15:20:02.422576Z digest=sha256:c694702a6d9a87d4793005e7c38eb20e0365431a2b738605c463c98c39638102

Observation 1deea75a-5e3d-4ad1-a2e8-a060dae10399 · outbound

This paper cites an unresolved cited work.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs Unresolved cited work

Reference 107

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:02.428703Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:02.428703Z digest=sha256:3fac584ab7a51af6a212e5d94493bdf1c45f48a8816ad95aa247895ae1d3ec1e

Observation 6438061a-20d8-4053-893e-928d38b8ce25 · outbound

This paper cites an unresolved cited work.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs Unresolved cited work

Reference 108

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:02.433759Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:02.433759Z digest=sha256:306a6f16a47a02c1549687922c205c39070b73abe96a2330ead94fac45e8ead9

Observation fdc921a9-473a-4aca-9e25-e58a7f4e161a · outbound

This paper cites an unresolved cited work.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs Unresolved cited work

Reference 109

Resolution
verified exact
doi, observed 2026-08-14T15:23:53.167894Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-08-14T15:20:02.438923Z digest=sha256:ad39784ef5366eba7690033d536fe15ca32e61fe285374416857f1c89e690768

Observation 6659b2f1-4cf9-4495-9664-65b60ff4d9e4 · outbound

This paper cites Effects of variability of X-ray binaries on the X-ray luminosity functions of Milky Way.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs Effects of variability of X-ray binaries on the X-ray luminosity functions of Milky Way

Reference 110

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:02.445134Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:02.445134Z digest=sha256:4152ccdadf154d36bdb3b9a3c03cfa70b4465f076e9a3d9e227386491a400416

Pith citing papers

No inbound Pith citation observations are available.