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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=sha256:1be1794cc115faa1ec7dc7541fc2c3b4973de70236d4985a685c0aad874ec8bc

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=sha256:86d6f32ab28553a2654f7576aa2fa1080ab83ad6482a39fcbf4ea05cec1d5eeb

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

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

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

Reference 3

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

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source=arxiv_source observed=2026-08-14T15:20:01.856575Z digest=sha256:e6a8df7e49056228229678cbbb5b9a8d64dd90845abf2b8758d2a1f4fc4c3320

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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Unavailable: canonical work link unavailable.

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

This paper cites an unresolved cited work.

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

Reference 5

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Unavailable: canonical work link unavailable.

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

This paper cites an unresolved cited work.

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

Reference 6

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Unavailable: canonical work link unavailable.

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

This paper cites and Gaensler, B.

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

Reference 7

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:01.884466Z digest=sha256:611d5e59ff3c8fadd41111afc1c3a422d28c7abb7875b2d5303803462199914f

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

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Unavailable: canonical work link unavailable.

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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=sha256:3ec87225de9ddd8725a5351c6352aefcc083b5615abc452d085722802baeabb2

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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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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

This paper cites and Pramod Kumar, S.

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

Reference 15

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Unavailable: canonical work link unavailable.

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

This paper cites an unresolved cited work.

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

Reference 16

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Unavailable: canonical work link unavailable.

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

This paper cites and Shenar, T.

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

Reference 17

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Unavailable: canonical work link unavailable.

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

This paper cites and Shenar, T.

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

Reference 18

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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

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

This paper cites and Falanga, M.

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

Reference 22

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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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

This paper cites and Stella, L.

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

Reference 23

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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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

This paper cites and Pavan, L.

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

Reference 24

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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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

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

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

Reference 25

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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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Source-reported events for the cited work

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

This paper cites and Bernardini, F.

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

Reference 27

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Unavailable: canonical work link unavailable.

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

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

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

Reference 28

Resolution
verified exact
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+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
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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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

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

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

Reference 30

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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

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

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

Reference 32

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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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

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

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

Reference 33

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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:b215be405c1ba503cc2e38016a0047653a2c915ac3b89c8e81ac55405e47d539

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=sha256:649917fe77f778c3be876697a8dbc0b022e33e46491468c1b01995a3f5ebd280

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=sha256:8b4e5078cadd4b9e0476cae412c049b765bf473d52010ccfd6930927c4f0d4ca

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:d624b311bb2a0b97186c08065d499db24b929b4ad8b4206f00aae4bdd166144b

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=sha256:493293cc4306ad7b671115760dc641fc3e79a95dfe590a1ebdf679de41c31e7b

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:b09082d7239324999087b4d70412ebb81aa758f308db44693b2b928818699056

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=sha256:97cb64a8ab57e001da3d803811dba5dfe6945b9c035cd44d0aab1d3a0477537b

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:f0be2cd711881be34461cb465346df9ae7edfecde0f61c69e489fde707752234

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=sha256:4447415b9c800b09eae0938e1e34a2535bd8cf0d2a90a4479e73876e02b84a4d

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=sha256:0de692a615f1a36652ce2ee4a23268a8f4949c81f75ffae36bf23359c1cbe266

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:b90542edf93a6fe1263d08aee490ec324ee64056b4f3e3549f62b14908305cc7

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=sha256:64e80217659197de1b50863a9b98524375538e2b1c3bb60749981fbaec8e9fff

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=sha256:72b45123d948e2210253c8dde858a9c89372c7fb8a771057f2645e491df39cdd

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=sha256:02975789407252f67cd0b6a2ea1c1e62810889764ca1e4c75ff876528e5e90e7

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=sha256:617e4443c010318ac9428d69c155e1fafeb694e3850f5f9a784bae3a701f48aa

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=sha256:250c3c3a3a73831ebc06404100694f2bcb9aad9ef2c8d8ba7d18ceafd8d0ddd4

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:f3afff79c96ab3d05afffd34190c2d31e61f53ba9c7368fc794fe46d34ac26dd

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=sha256:550a108972fb186ff0990d6188ba6ce08154d646cf3fbd8e509b6fb9a279d046

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=sha256:5e538af2ef8fa415e37defa252dc616f7634dfd1abe91effd91b8300a2594e6c

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=sha256:6f60ffaf5c21deac4b39b7de86948d1fba5e37014228a9df43b781f5df2606e8

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=sha256:8cadc9f62230ee7c35a7f851e45103d89280fa071bc19c5a78f1dbf8d946a631

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:b6689028598e945b20cb8770a8c21836bb5aad03a2d0309348b8a186a3090c88

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=sha256:0f0d911deb37d972a7be752b1dba192a5f5fe771a39519234fd6b6650337ff3c

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:f3494d5276b8b80dbc524891504953dc23cf6f7adb65c339d55b88952345ce09

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:c7af15ea22759e59dd9a34cea6ac9bc6f6195ca2364124ff319895193bc412f4

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=sha256:436b446ca4515db1f2fd36de3a23b8de93fb939f870c1047f8e26d691fbf0bc8

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=sha256:7851e521b2ab748ed4cc81aa575640cf30c36a0aac3e9017f791668387ce6afd

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:dcf9dc2feef866db79eb87a16cf304dffda01404fce716461da0ad040edcc29c

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=sha256:2c6c07f6f30a74e53b84d65fbce83f2f23a84d3b932ca6d894ef416c7a8619e8

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:a18699d02fdd53050a0f597c7864629aea52de268d3b55f4de29bc8aa98cc56e

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=sha256:935bc974a4e5ebf980187ccb1f4b69df67b50123e632b943f64e4c2e17a60562

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:bd7b08d6b20fd2d18eb00e7434e37337e7fabda4a844ff6ded7309cd859ecc62

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=sha256:9f915b45396198b78e4bd994c672d43175a2adac3c8341e69fb52b9904ab886c

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=sha256:421f7bd5395b8b7914922ac12e471272d1d687a9de9e22bec02cb775ad950503

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:efc5d26e08ba5c085f0404777bb704a34b2dfefbcf69838ab34265ebf6817b48

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=sha256:08dbc45996bde7cdf8c38814fc4fb3146b6a6db5de7fe3c9227fea08bb013c62

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=sha256:30ba6fdd25d80e447fd4576bfb49873154531bd834c113fc8fa967f641cf3ce1

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:a3f932480ed5474f06f910f091c1b572581164d73ea6aecd285d4cc4845fc188

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=sha256:036181c38d1dc3c766b8ae5ad4ff94ea7c1d424e638a2a691af1512cef0f271b

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=sha256:666bb6a50657d383cd4caf194dc05b879194a9f8f3c02b774f00671851e8a197

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:b1b017397e7d9d0ab21845b29491d27b1d17cfa2793e33ca320bf7906daa4a06

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:a84353c385cc8223ac262dce69c46756a58f28853c1f056928afc25643b6d64f

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:f177047025ea3edadfb0e7722d49b0b875b0ca95ec75cb9e598393ad4ff7b4d5

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=sha256:9a1549d0da4533d63acb157ccdc3f5b876b48cddbb7d7d9cf7db43ddd8e719a5

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:dfc224709f1065b3faeb147c4dfb41ca736bb8f064d56f95446a41cc6d7f013f

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:b963749da858df2520ea1f0e7bf8bb3abec29d96b3f9c6b2b8f92b57fdc0f20e

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=sha256:1a3adea8795eb8829240611a74575ead54dc64423e334bd4b31707078a776a31

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=sha256:894b17c4892b9de7f69f1ece30e00a9bcf09c2507ad786787a0a3cbb58cd0899

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:f40a4ba2ee8532870526f1676ef27fc9c4b56019a4569d158be8b8672e3193d9

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=sha256:45ace4c2eaafdbbbc9f4397fe29ac08d0bdd28d476cb4cadf71eec1a45b1ca25

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:ff0650f64e6abca29dd4e6238e2a955027441686e8b2dbd9bb87d953ea9a3f26

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=sha256:86eda4474d7bf98c16a0ae014ef6d9d2342ac95dcb6f5c00d9bc7d70ee9c7d00

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=sha256:12b8e76a6c522b6e06e310ec675602d20cc2894aa54ef2f54f40606c2aa8ca67

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:ee5ccf5508fd1644656a4e71239c38fbbc7c7a9c2e76846642a8288399eb474a

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:bd32b181d6aec6d108fa792fbce60043cff8626f034ebad6ecbeb1a90cfb513f

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:c39e29a17699a0b788ca54be0f017e40c74a2ccaee448de08c90134d09119c3b

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=sha256:4076476006084c00bdd6c4fb8c1a8210e4b06834fa82404bfd0aec79d7ed4803

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=sha256:9f9ac22c9914f700a301afac8da6140b9764d9aa4351104b0d2462519c27dfe1

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:c9f5f376e251405ed2e8272e085de0e984b8663ee1d25db9eaa92b0aa55eb43e

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:e61ef93b1e42bd62d7117b154fd7e1c117b3a989f91dee891d159b14a2f94f55

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=sha256:99ebc89fda3d30b7f8f94c64e520159249258f2dfa68d435bf8ee11b6e1fce99

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=sha256:50339604286e852bf6c17fd297b678dcd587c5fa1fd3afa4a36873c36918a547

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=sha256:9381ad77e5ed4ad3469458c84c20c13b2908531d0208fcaaf70d3ff4d421dcd8

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:cdbe1a30cbbda92501da079d8fde987611cbf85365e87c767980de7b079cb2bc

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=sha256:34dc4c5868f64063dcbc09815e084f7cea3fa0dc5fa1cbb62c3bd352f20d8c01

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:f2aef3a8e8ca8b0f81a8725523dd66a97027ef57b6f8bd88c3f8b9e9b9db5ba1

Pith citing papers

No inbound Pith citation observations are available.