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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 2026-08-15T06:32:42.880941+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
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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=sha256:56f4b3c3f225e1dd14c1b5a1f94fdbfd4805896839c59d8116d9ee9668ec05cd

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:b3627e4a3883c35d25686352d3011f4efc0dc0ff47f2d360efa60665e2135aeb

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:f66a118230572b667cfdd5972254d798db5a5df1ae6a64eee3e7c64ecc77e237

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

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:01.878434Z digest=sha256:9d36ccf5e1b832ece14648c3f7cab4c84d0d4fd4d796c442201724973a4ce905

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

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:01.884466Z digest=sha256:e4570a7f1808730f3d53866555b9720cc423a469af9faca5c2edd719a96fce58

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:e6612fff02b0f28f3c59675370737deedc95e78e0c12758ba5655e6e548196b8

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=sha256:41ea158bc86ae2ff2cc15a0775a2f688deb8e0a2ff0e912d1fd1071ae8078a29

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

Source-reported events for the cited work

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
no resolver link, observed 2026-08-14T15:20:01.963749Z

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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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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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
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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unresolved
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.

source=arxiv_source observed=2026-08-14T15:20:02.048681Z digest=sha256:fc9f0555554c8fdb2b9fff0cd8dbe701e499e6e742f9bd97dc7a7dce9be078ab

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:b79dbebd5b0972e81ec96a06bab44572b8423ee3bcac84450bbb8d8b95c31383

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:bea307fc061d54c78239dcbf1fd82e7ecde6cd264384077e898c61bb3deecc37

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

Resolution
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:a67dd0f2b04a3c2e31f6d21d2f8f25c01a9e9eed2ed804c6d08451decd6f5397

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=sha256:3b2c4c9b4080488675683df592dcce40ec7ed573de4f6fabb093417c777a40c5

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:b8484bf3237327e8b0ff4113eadfd4aed7f6b6049a54eb0e54e2d21d0837868e

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:d8103e922c3844d566d48bcab46f9a4634b20a3b55fb845e788564cef63c238f

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=sha256:5fc2e06cb20e728d3d24d9b42161fca904899bbaefc4a95e4a7fba15ab503327

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=sha256:0f0b154a2bf0d0cac603b3bf54cfb2a6a0083f3d99c32ba7341dbeebb53dfffb

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=sha256:57c7354882456b24bd9328d4d0982670a587cb7a15c195298a55354e4a7dbcb8

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=sha256:056277c153d1ddfefb5338798dbf13cd2cba1f6ad5d9baa105a97ddfa69ec53a

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:bfd83698881fa55a87550a90e7e6cbf635f6c43350ca94e8dc0053f1de194ab5

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=sha256:1a6503cb01ec958f216c1dc5c91b2a14a56371862be1c71a3c75af67781980b8

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=sha256:1a72d37d8a9519ca09dba756d1ed27bb7759727322113a56501b20a0e10d4146

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=sha256:856eb690ecb65887c6cc0918f93d63e0690947d5ca9339fb2967b9e7fe314cc5

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=sha256:2ffae225b0b64fd13121aa9de0b92b38c0e4ebdebaf00c25ea7b49894a53a0a8

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=sha256:554ffde94a3dc7ab6fed708bcd2b59d24e01b2161c87165e80375107ea983395

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=sha256:5763cb475c44c1aa191e46180e4efd0e574aa2933f1becb3230c98477773c9f2

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:b13fe34dd016e0f295b797a2d790fae5972cba8c0ad4bd0e81ebd96c98007815

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=sha256:0e6c07e5ed5b7be1e05445e1e456319d674393762e6413b40f93ec9a4f5e641b

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=sha256:6590620f058a8de978eebb8649577828cbb39029c8be086c92fa7b73e7b86aaa

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=sha256:513b7741fd90b568e3c58eeb467bae8c4e3172d6e075b592af862bbf354ae237

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=sha256:555936965dbb4638a7798dc7bf5e07e9c880d70843089f3b0e53cd2c7eb810e9

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:a5df21c9d09fedaae6e118f32a7dbee5119a14561478785ceabcc085389fde8d

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:ae8f6c7f3d6cb8ae8a88bf393b00e6cff14f005adb49f20ca33b77fe9e241549

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:e0962fa271fb806001132766d29c4e816024f67effe5c0854f20a9309e94990c

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=sha256:5f22a2670c8c14ae3304a6d34c6ee17d87f66596648a3a495068809d5f779f45

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=sha256:3afd34dfc948d651e8da55f3210e71599fd983d6f0382ee52d17adc590adc193

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=sha256:1267ee8e9d4637c4f58eaf2dbcf8455f2b382ec799737cb63e8a283d0c60e79a

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=sha256:2da9b68630fae08de80192bafd8753da1a9c2f35f953b9518b311293b8f01b7c

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=sha256:3143d0a2ae8ba48412c7e20f72633d3e5cf1434933cd2acdc9cc8a9ba0da5aa9

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:efec88a992de80b885ddf4ad503c33f78ea171e4cbc70e565bdcb99461f36689

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:be01b8f902da0fa5a77b6dc84a99218272b379d11d1ea1a52d5d4f44ee9b4abe

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=sha256:28d891c147ee73b92bce34846466e79308c808f74cef43f84f1258e9072b9d94

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=sha256:89a4f4c9fe3640349759da0bcc04fd0a21ae2851ddbea7d99d7debd73d5de351

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=sha256:8f27139f171d88a30b4e683d4cea9be4ac72978028f22ca0d920e66ccb4a6d79

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=sha256:18fc37ab691e4949e2151947a8791726e9273ae0b8ffe9a20a28c4936179ae5e

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=sha256:2a1685ed77d58329210a4098a33494511cd082b525efb448464278a6e5fa333f

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=sha256:093f1b404ee7c10c4ba60c8cf059dc7389bfc10a55f7d678402887cf0730fcd2

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=sha256:3d236cfee5359addb0afce08ccdfa71f64e25bd9200a9f4228d5351f4cd7bda1

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:b1077816ee0a34f8a557dc78b9803989593a08c3e3e0d6835410ceac53d46668

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=sha256:50ff8425f91203fb1a55a8f334c502b994f1bd2b5120c16ee18c24bcf3644a1c

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:d08d947925efae5fb0df11bbfc0c60371114f03b56d0822c0826f360cb4a1b24

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=sha256:3f2b01c5922e927dc23d2e8a1bb03968113ec014c42697458681c31a395ae999

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:e34ca2cab5434d77f5b72adef6f083b0239a985ffbe4fe428933390fff6d7e2b

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:e2a9d5e2027daa473058232556c542003a293bf33d5089ac707c3a3ef7e71e9d

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=sha256:722122bdc84d3566aaba75e221716cbc5010f06aeec0f323b84034f81b4428a8

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:f7fd6ed023b62df28b9b76ab05cc6b1a19f647f44314de3a30d2401ba071e1da

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=sha256:6acfb1fa7ca28d4b5da486e6c3a95507ef91330a4d1ed89cba91d79b4f9e8f34

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=sha256:78b9666b101fa1cf6c156b8add234d08969f7bc6ade746ad3cab0fd4d68f3093

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=sha256:716b4ea1c33cebd90fee822e4fe24bd42f51a3599f4e5e31cc0ad58b510776e0

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=sha256:8aa707ab7697fde222f81f18d3b5790a6c5d680f21fd73571b9bc61ff5f452f1

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:b8767c844f41e2a1cf9e8bda8a6e54da72bdfc0f1789a6002e60a70b2fa0cc56

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:b2665658cb52fb13a6bd65f687d5bb6e0179d4f71a6b14ab87911d8315141ea9

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=sha256:71f99f94a27e09f6e07e33bac8eabdf786055f970a1a4ab483a1aa7f7ecbac0f

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:ba9ac01517fcdfdef97a9fee8b3cfadd7f195bd6a45747f55ab8f75e50e46e80

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=sha256:3e2a2c146072eaf67cc34486ff1dc5e4f5baba6ef3815a87bb7359aa97525fae

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:c1193d63e49470ec000482481db782a79ef5085b1936e0553b308eb5e3b1574f

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=sha256:5210489427f12ac6e39e3888626a49a6dd8c6dde591634d343d409b6e126d73c

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=sha256:3c566046414107c5054afca3b66d8583aabf61018850fab5d0c46347ef402258

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=sha256:8a73e2b2f4d914fdc9eea9ad0b49ee7f98fa76c3a7c90a56e05e2653148850da

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=sha256:8f4aff70e6330315b15f9786a8d31b7e97177c7e822b88796713a33229c2aef9

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:d50783094c4e1e9112e175c9ac742418aa8e26ab7ebe3018a46d785bf0f8b278

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:be370e17b0e6a3635d39e0392c68b4e3482b141f7b36eb7daf6b4b8bc1f50d72

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=sha256:2fe3238f08fed82b31e17ed306b2c1593564e1e04b199db28ba2756e862ab55c

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=sha256:47c4b0ac054e6e0621acc454e80bdcf8eaca6503afc0322810b573d618d88ae1

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:a4af47e1a6884ebdb537c05b8bbe518529c12ec0ad5cf57b4ab5baa4c58d33e0

Pith citing papers

No inbound Pith citation observations are available.