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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 16 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 2026-08-15T06:32:42.880941+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
  • metadata mismatch0

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:d51bf52f77bfe0a59d435ecb980c7571215b52dc6c040fa23c75cda370e4f31b

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=sha256:445374053bf90fd14f50765e670c0f863aa33bafe7e48ef67f148e58aabcd8d4

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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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:01.856575Z digest=sha256:b2b32634fe8461152932626a2ca3e8aba08168afd57014e4e7110a13412fdd85

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:01.862870Z digest=sha256:1fe7b3a34ff0fbecfa88186854e3e0e568bee077685c210ee06129f359788823

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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no resolver link, observed 2026-08-14T15:20:01.869655Z

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:01.869655Z digest=sha256:0908cde47b23da0b185973620f2c2fa76becbb583e9f5b8eee4ff138f652c44a

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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no resolver link, observed 2026-08-14T15:20:01.878434Z

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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=sha256:6aff2f898de5977017b49cf12515d3fb4e2452676a9dfd5c174d1887cb72ff9f

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=sha256:34615a59c26ac55317afb2caab9519ea1d81ec76fe55bcc906c5b673ceebb60e

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:01.911575Z digest=sha256:e0834357712c85e875d6d22a7c538eae6d3148531b95dabd412b543412317e51

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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Unavailable: canonical work link unavailable.

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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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Source-reported events for the cited work

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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Source-reported events for the cited work

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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no resolver link, observed 2026-08-14T15:20:01.958205Z

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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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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

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

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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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unresolved
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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.

source=arxiv_source observed=2026-08-14T15:20:02.006748Z digest=sha256:472931f91012071db0ecb9725781216e727091e9addad32979b286291cc7bbf8

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
doi, observed 2026-08-14T15:23:53.939373Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+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
no resolver link, observed 2026-08-14T15:20:02.021685Z

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

Resolution
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

Resolution
unresolved
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 2026-08-15T06:32:42.880941+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.

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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.

source=arxiv_source observed=2026-08-14T15:20:02.064258Z digest=sha256:2d8f55347a74c1edfbe00e4957f8576d5a1e3be8c10c19e3c4018d904632390e

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 2026-08-15T06:32:42.880941+00:00.

source=arxiv_source observed=2026-08-14T15:20:02.070418Z digest=sha256:da671c66eca6c6aa73dfca064617ac55f3a201a4f411c6cb22c10ceafdb1a113

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:acd54e6571fc37270746f169ea642bf5dc1a1e23335219634d0da19b014a0380

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=sha256:4ae1414eac1fad21bccdc1d9aa5a34f23a33dafbfe97df122055054ffb7e5efc

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 2026-08-15T06:32:42.880941+00:00.

source=arxiv_source observed=2026-08-14T15:20:02.097156Z digest=sha256:106e3b7c480a606ec82a6be030eb832b785beb981bb398360f37880315339dcf

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 2026-08-15T06:32:42.880941+00:00.

source=arxiv_source observed=2026-08-14T15:20:02.102729Z digest=sha256:2c65cba9476ddf95bfc1cecf1747509202e1e34d59664a6afcd402065323a094

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:a7157deb66de96b8c8e2979d318f2ec887deae4559e95fa3b8caeafaeebbef17

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 2026-08-15T06:32:42.880941+00:00.

source=arxiv_source observed=2026-08-14T15:20:02.112879Z digest=sha256:598ee4deac25e0da8a0aac512fa7ddd55238a88562ec3660d0c487cadb1276b8

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:ebb0d4dcac519b8d99eccaf32fbe4bf1f9bc749aef641693ee26818e5b39623e

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=sha256:5778abdaa78cd9a27cb1cb72a791146089a1777f864667306c21c64de6b3b654

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=sha256:149bae2912907d33a9cc8bac2a6721d01b14e5b0296048aea63284e5483fd2ec

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 2026-08-15T06:32:42.880941+00:00.

source=arxiv_source observed=2026-08-14T15:20:02.133639Z digest=sha256:b740664885eeee8116a57bcd0d7f7a574bf286dbdfe58e7fcbefd4e69e365be2

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=sha256:84561014b9d965f37bfb2543d98c240a137808b2fe4e40582b9dacbf33375abc

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 2026-08-15T06:32:42.880941+00:00.

source=arxiv_source observed=2026-08-14T15:20:02.152481Z digest=sha256:e8f574f47f125135161ee8b7187b5285adf8e9ab3845b6e006fa02fbf3d92a5c

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:e18130ff1d077aef855eff91718411afe8ac5643e143a46b48fc048b2d106d68

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 2026-08-15T06:32:42.880941+00:00.

source=arxiv_source observed=2026-08-14T15:20:02.163260Z digest=sha256:61c9f46c32329974c3734dfd942143b7b140c8aac7f5d4052d7d29cedab264e3

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:a7f6d4213f61cca2aaaaa767bbecab2d5e886f07bec8fc9a5714a215e4b99c2c

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 2026-08-15T06:32:42.880941+00:00.

source=arxiv_source observed=2026-08-14T15:20:02.172727Z digest=sha256:711154d5aeb3bb487b71fd413bc12e772fd7800b8192076bfeddebf4c00bef4e

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:f3ddbb9eb3e697fc9b3cc6f498d5609e4ad0521acbf70cd4f658bea7cc8885f3

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=sha256:33de9ea4f531eb596a97e13e0b73f5dc8be31e015989bf6d46ad04f7261f624d

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:d30aea685efd64be10b91521b311d2188dd1fddc250baa4cce77f166ab1e1f9a

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 2026-08-15T06:32:42.880941+00:00.

source=arxiv_source observed=2026-08-14T15:20:02.193505Z digest=sha256:e40e7a377a3526139d31975d6f6db4ff159ebaab766009acd47630e4f3024379

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=sha256:920c2d409616d2dae2d7b12ae257444e29305bf8b073f4d19642be0585762ed7

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 2026-08-15T06:32:42.880941+00:00.

source=arxiv_source observed=2026-08-14T15:20:02.204841Z digest=sha256:e522b5cce426bfe356af939f16e2ec823671a15cf4bec2033d256a76a1e3ed84

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:d0346ecb2a15c7f2ad9169122e431ff6cb108bebbdcd365782cba628f1f2520a

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 2026-08-15T06:32:42.880941+00:00.

source=arxiv_source observed=2026-08-14T15:20:02.214921Z digest=sha256:4c958fb1814b449f27da977aae963e00a3fbe80812599a2882b3b8eccbcb6e4b

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 2026-08-15T06:32:42.880941+00:00.

source=arxiv_source observed=2026-08-14T15:20:02.219595Z digest=sha256:034463768d18a6cebb506d161f5856920ad6490ae0db2fc3a56865a1775d829a

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 2026-08-15T06:32:42.880941+00:00.

source=arxiv_source observed=2026-08-14T15:20:02.224625Z digest=sha256:69d9a6ee90ab7d1ab918ae33b2abb9158bc0a029ac7e9873e7cb3bbd56fdf1d8

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:ec2b00dc685a14d93f73bf2d25125323d0d4f0e8e17c272bedd9925f89c6c91e

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=sha256:33efe1283ec87480dbd3a014bbcfb52e4e0f96685dfe273cbc988e509362968c

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:b2408efcccb6fdd58d0602507b060b9a54a76b0acdeec24eca950ecc48cd30b6

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 2026-08-15T06:32:42.880941+00:00.

source=arxiv_source observed=2026-08-14T15:20:02.250481Z digest=sha256:164ef442d7c111d44d20386241df422f6c5f33ba66b8a06f89466de8dea4699a

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=sha256:02c9ca5967c70f89bb87e59f1cd04cc9abc534dce89893b2c8fa0514e7cd3f84

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:e3087d1002eb1e897861a4f27dccbf54dc12a49e04d7ad60dc25a635f762572e

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:da0dc3d153fbeb6d41bfdae9d9c3b78c2ea028fc843ccd615570d73fd51c8dc6

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 2026-08-15T06:32:42.880941+00:00.

source=arxiv_source observed=2026-08-14T15:20:02.270463Z digest=sha256:5db43c2b5f38bfa9c75e4d7e7e4a507a70c1d6fc19a6ff8eb3a2a03f531feb68

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 2026-08-15T06:32:42.880941+00:00.

source=arxiv_source observed=2026-08-14T15:20:02.275685Z digest=sha256:d9cc9d26558062b42437be006a7390931f7807b87272e5d7e1c29e9f86dda275

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 2026-08-15T06:32:42.880941+00:00.

source=arxiv_source observed=2026-08-14T15:20:02.281272Z digest=sha256:4c470cb8c1e5cc2ea5c3df5d95508b77739ef7373e6e9f033d220934caaa906d

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:c00ecabaebf3f23cda764ff653b8d6f80663bdeda7129d63e7ee0482624fb787

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=sha256:60b07a9a4da0255046289d48300b0d3dec458e655ba0aee8815234c89d0a85b6

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=sha256:554da9b256cad02bbcc23d83d0246a15cf938ef585dfc203dd5a3249f446a5fe

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=sha256:050acddd4da5a6004273378c2d0390e2982ad8c98df35f2ce9e42c07d661c476

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=sha256:8cddc264f10585f87c9e42f56103e36c83daccb5eb94e1672d604eae4b1b9a49

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=sha256:6e657eaf82fb3a57f03dd25b6bb36d8b6072020a4a39f015f40a50f23f5635bf

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:bacfb628bf94e8e3418545d62c85f39fbd4be1da7b3313a9bacd634343d032f6

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 2026-08-15T06:32:42.880941+00:00.

source=arxiv_source observed=2026-08-14T15:20:02.323163Z digest=sha256:8e45e2a5f24e33cc9b2e8be165223a588649e35beaec0f3d73db3122ff157c97

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=sha256:7a1f4fe54fdb729fd6cfdf39b6d9974bc9af8ccb519dbfb97609485b7e74478a

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=sha256:9f194087ee66d57c433e1da46ea71547eead8d15eccf2fde65cdb135c84a3ca6

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=sha256:5aafb22f59defc6596cd52d212ef327cc4e3c29db1abcbe176b5f49add6a8ce3

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=sha256:9631e981d41115af027cd58af11ee16eb3537034d3478802cdff44419b4b6a99

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=sha256:4b100caca2c61d2f5fb0fc79e0487e31f70a549767f2327efc08a4f344d1bb37

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=sha256:8f0f0ebdad2c677a78abb1bebc39e6ae5ea49461d6aca8e3b372f030ce2fbb10

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=sha256:50f184b7d96cdb447da890227217260f5e4edff00ce5788bd19386a8124d5e21

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=sha256:634287c91af8fdc9a4ff83158c5c16d03c9198e5aea616d54e527ffe1d27645e

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 2026-08-15T06:32:42.880941+00:00.

source=arxiv_source observed=2026-08-14T15:20:02.369996Z digest=sha256:09f1aeef9dc6c15262dd3a6105d67dc6ed3618941ed5b856da9de8cc05fedc9a

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=sha256:314f1f24c5b48d831e1b9c8657a586ca490a98b6427ff2d3ebccfe4748e56d84

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=sha256:3306c45e74fbcf5511106f4d9a7dcd1914806a3d4536c7d36b9a449649e8ba6b

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=sha256:0cac72ed2af96d96156d0f142dc50cfb1032292c3ac322ac775b8a057c4d4a44

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:b28018eda1ea8fd4cc16c2159f3e003ee151ffba942433efe4d2ac7593f4118d

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=sha256:4cadf5d7a23d910724fd2d42157e6e8eb649a3117e97021cc8ab9cc2d28a699b

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 2026-08-15T06:32:42.880941+00:00.

source=arxiv_source observed=2026-08-14T15:20:02.417381Z digest=sha256:4e0ebe25059f862ed1a5764acc5768254ca436be3c69cde2e79129cba18bf758

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 2026-08-15T06:32:42.880941+00:00.

source=arxiv_source observed=2026-08-14T15:20:02.422576Z digest=sha256:43c41b7cc5758111c7ccd72ab11206c6049de5f1a9b96e3a8a118a1c9476c814

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:c1f8ece9c8c497ee79b4d0b3225885f1763eaa397e2325c30935d6e36b4d867b

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:accb048e8c709a96e6e793b937d72069723599d7d7f203ba4fbd33822ac7b02f

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 2026-08-15T06:32:42.880941+00:00.

source=arxiv_source observed=2026-08-14T15:20:02.438923Z digest=sha256:b8a9aedb62e09d4cd686684bc090682277cce7119da5195f60f4b8afc541a064

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:b6fd045a5e4d82859042f179e6ac49e7f3a436d7b66127bdbbd86ff2e634396a

Pith citing papers

No inbound Pith citation observations are available.