Pith. sign in

Paper Citation Record · LEDGER

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

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

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

pith.paper-citation-record.v1
2608.13259 v1

Coverage vector

measured 100 of 279 reference resolution

Typed states for the displayed outbound observations.

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

measured 100 of 100 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-14T06:32:32.682623+00:00

measured 0 of 0 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links

measured 0 of 1 external citation measurements

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

Source: cited_works

Reference resolution

100 of 279 outbound references displayed

  • verified exact25
  • verified fuzzy0
  • unresolved75
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

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

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

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

Reference 1

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:01.842978Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:01.842978Z digest=sha256:dc70cc2fd5db4bc618ee331573bdb76151d74e003e2fe6a3797267585eaf64c6

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

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:01.850963Z digest=sha256:3d80f836efe27482f58fe32eaf32138a1a1253579c8244cc9b98730a56a6f1ab

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

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:01.856575Z digest=sha256:a6f32c80ce9fbc786c23b923da6de69158cc93c1faf73e9b4050ea676dd2e562

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

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:01.862870Z digest=sha256:2f9cb819e12b4c02602345b1feda7e2e07a3c86083ff25d62e492c2c594262b3

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

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:01.869655Z digest=sha256:e5f93a2f47a0f92aa69686028faf19a6212504418ec61ccac332e01411879862

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

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:01.878434Z digest=sha256:6490a8ddcf9a3eaa7afc9b90a26fb48acf5488c9252a43f4c329853b22803388

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

Resolution
unresolved
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=sha256:9bb2bca997fc34aa58617594e162a04207983d57643bf4fac8711ff80579a49d

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

Resolution
unresolved
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=sha256:95bf8278031fba9f0970e66c36c698a6fd08768fd38c2ef15dcc18a40f762597

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

Resolution
unresolved
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:aa96ac1c94f0ebd1da438ddf2bebe4ed5551fd1c8bfdd16a4b75fd67d450df71

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

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:01.917449Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:01.917449Z digest=sha256:b18968fc73bed6707e1890c815095ca340eddb3ac3f593145af34b2fee3a464b

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

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:01.923923Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:01.923923Z digest=sha256:9f69ccf3e2675ce941d191de08418b852d930fffa5625d9d78aae1f1940d616c

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

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:01.930408Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:01.930408Z digest=sha256:76e6cfef2935dd8ca6e6beef92fba450a24b190657cfd928e237c2ade6275402

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

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:01.936054Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:01.936054Z digest=sha256:88853d4daa251a4a2865359525270e765971ce75beea7b7f17323a6b2b758de9

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

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:01.941364Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:01.941364Z digest=sha256:e1757b5f12f75f901ab1659589926bee442f690943098b984cc21ab57148f6e4

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

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:01.948556Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:01.948556Z digest=sha256:45d65d68b6ae43e090eadb90b32d3e55b597e6ad2219127668c3b3254da29bbd

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

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:01.958205Z digest=sha256:5d9cee2f6414e37456956211414de9d663a4dd0fc29366be8c1ad0c06acef55c

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

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:01.963749Z digest=sha256:000334d31ae01a7d3a228e8826651458eae8435855d5fefafa8a61d660ac469d

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

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:01.968942Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:01.968942Z digest=sha256:7a40dada486307dcc3d8325292f85971eb16a9ed79330a4c0a198c77356c4cc6

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

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:01.974399Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:01.974399Z digest=sha256:13f01309d2949e0e48f1e9df32387174c06c694f5e8cecddc7f53955f7057113

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
doi, observed 2026-08-14T15:23:53.998374Z

Source-reported events for the cited work

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

source=arxiv_source observed=2026-08-14T15:20:01.979548Z digest=sha256:bb56b11b29c9ab82801ef994118cfb4fa0ec4ce55168305407307b2940358aa7

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

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:01.984822Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:01.984822Z digest=sha256:c60fed226c463967a15a0ab98095fbfe1c6c690f35285c9f3ecc9949c610168e

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

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:01.990054Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:01.990054Z digest=sha256:c5ef45947484f87e82bed7b957880bdde3a7812d6d7b7549fd93a85c60fea04d

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

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:01.995234Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:01.995234Z digest=sha256:73d5632167d0b5f0adb476946f8c254c2cf5fb369279b5fab12415bf06a502f8

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

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:02.001311Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:02.001311Z digest=sha256:dcc8a261aeee274eaca0ac2c4ce3673eb7bfe679001ec29d5d34045d1699c8a1

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

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:02.006748Z digest=sha256:8a1a625c6e80104431f312c31c213012032ddb8d17c20ecd26d376603b91bdf6

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

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:02.011617Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:02.011617Z digest=sha256:7735c88e6ac493c3950cb51bee62b9d7efc12dc8d0efc637ab6c86cb7401488e

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 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-08-14T15:20:02.016605Z digest=sha256:e2b387a2fe15ef837f18c40d976ec908c99a58c4242f892a5fc81783c0c39ea3

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

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:02.021685Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:02.021685Z digest=sha256:ba9b6851b214ce3f70c848439a109619a86122a7578e3a1dccf65a1574c90da5

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
no resolver link, observed 2026-08-14T15:20:02.027134Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:02.027134Z digest=sha256:1d8e6a5e5f68c26d8b4af47a01139630cb1b2df1c7a4c4563e553a9b480aa362

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.

source=arxiv_source observed=2026-08-14T15:20:02.032747Z digest=sha256:fe162873ade27106b67de581b2cb2270564a82907b61db09d7a3a82725841326

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

Resolution
unresolved
no resolver link, observed 2026-08-14T15:20:02.037804Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:02.037804Z digest=sha256:0c6a42af6167a1fedc64c7ebf4301dfffed0bf7f8f96379d08c5e9f4c99ddc7e

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

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:02.043444Z digest=sha256:6fea57292c0427d90ecdadd0a870d655e2995f8dad9e4eb1d9d86ce36fff24ea

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

This paper cites and Gastaldello, F.

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

Reference 34

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

Source-reported events for the cited work

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

source=arxiv_source observed=2026-08-14T15:20:02.048681Z digest=sha256:f25f2f049c517d7e7d8e79c0292df76670d7b0ac7ba6bc75f4076b45df584a22

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

This paper cites and Stella, L.

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

Reference 36

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T15:20:02.058995Z digest=sha256:4545e62cd260c71b4ce4a573b388614ab3aaa24a76da33bf1fd079eeca4669e0

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:c1ba6fd091986524f5a74d69f67d676a0a2a6b6d0eb80f35e809fb08ad31d19c

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

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

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

Reference 38

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

Source-reported events for the cited work

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

source=arxiv_source observed=2026-08-14T15:20:02.070418Z digest=sha256:16411b36019453811c1e7dd84d398001bcefa55c85a5ced529c9bf4a2da5a73c

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=sha256:0a12ebfbdd60f5f4348a4b4ad8cedeaf43d54d87833d20e951ebecc6497bdaf7

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:d681c518681c6f41d87ae73d2d94441e7a90fbd91ddde1eb8259b38bbbf8182f

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

This paper cites Optical and.

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

Reference 43

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

Source-reported events for the cited work

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

source=arxiv_source observed=2026-08-14T15:20:02.097156Z digest=sha256:5d5755925693bd46dc89d5fc95a2a12d931af4f1d12ab8b36143d8d5eb566162

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

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

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

Reference 44

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

Source-reported events for the cited work

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

source=arxiv_source observed=2026-08-14T15:20:02.102729Z digest=sha256:5b176e2d7574b5f4590c9340d55d19daf884d2ba23ba1ba935e9881c3effe925

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=sha256:848182ef51eee3cde52653326f61554480508fe06002d4e3ca5968146fd1ede5

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

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

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

Reference 46

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

Source-reported events for the cited work

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

source=arxiv_source observed=2026-08-14T15:20:02.112879Z digest=sha256:959c151dfa0a8562cee083caa7ade870169568a2ccead777b2fe3af63abef10b

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:f0475afc5da24475bb7bc711a001dc61cff60744fcc53000a9732d84610ddc5c

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=sha256:68eb95b2bf3d97b458e17d5c549bee388a12ba85d438293180ef1fbf63acce37

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:c3ff30df285b65db2c584b9a2d9d628bf236e53548c0ebfe1b52939600f6d35b

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

This paper cites an unresolved cited work.

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

Reference 50

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

Source-reported events for the cited work

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

source=arxiv_source observed=2026-08-14T15:20:02.133639Z digest=sha256:f4c5fd325570c520ac86de1b0bb02760230a1687263183ba394057eeb55e65c0

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:ec0ff12aac2536c9dc953b9dc53421448530aec53bb59e3dd4a7d76cc9a647ce

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

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

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

Reference 54

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

Source-reported events for the cited work

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

source=arxiv_source observed=2026-08-14T15:20:02.152481Z digest=sha256:876a3f2ec9c2db28330efdf067ab61327ba1b71e73ccfd5e620d9109d78346f4

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=sha256:2bfd41bd64109c986721e5bfc4eb1bb5589b7838fe33eb8ed482e3b87520a935

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

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

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

Reference 56

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

Source-reported events for the cited work

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

source=arxiv_source observed=2026-08-14T15:20:02.163260Z digest=sha256:eb21d2da7aa60995e8e66bc4e40612937f45fd178ab3f79b053fc5604021b73a

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:c2458674ae903cc6fe2f895198549f74f849f0c24fb6f78e26772d2bfc2eca01

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

This paper cites Crust Cooling of the Neutron Star in.

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

Reference 58

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

Source-reported events for the cited work

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

source=arxiv_source observed=2026-08-14T15:20:02.172727Z digest=sha256:d42b1415aa9bac8915dc06d2fc120a7679983a4190a57bfe518b6fb41b6bbbef

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=sha256:575150db3d4c2173b595a22fa01a1f897a699d110cc745190c74831cc0690983

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=sha256:432350d24ab03a4d803b7e7c516f84ca3e9104fdbbd1943e8ffc3c81f1be43fa

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:dce2168d45567a87cd10c4ffd99f85276b755aed5a54606a0c2157e58810f6f1

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

This paper cites and Ducci, L.

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

Reference 62

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

Source-reported events for the cited work

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

source=arxiv_source observed=2026-08-14T15:20:02.193505Z digest=sha256:6e002f6de0a33fcdf9e4e401868e250fbf627924dc25f8b5e2a2f6830cb3b94d

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=sha256:50e525740282c35d343053591e7e6b799db1d6445c06cdb8d400e2d167b6a3b8

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

This paper cites and Santangelo, A.

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

Reference 64

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

Source-reported events for the cited work

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

source=arxiv_source observed=2026-08-14T15:20:02.204841Z digest=sha256:6e35b0e6d59d004e4b3bab0f3dfa869da7bd1d443fcdb5a18333f089ae42602d

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=sha256:261999f69a0e88a7dd15eb876607a7c96db550a88c54cad4f958cd0d106db579

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

This paper cites and Romano, P.

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

Reference 66

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

Source-reported events for the cited work

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

source=arxiv_source observed=2026-08-14T15:20:02.214921Z digest=sha256:8e14d3eed840b22e3f948fceb38dcf2fd5cdc6adaac138039ee402a59ae24c66

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

This paper cites Modelling the Expected Very High Energy.

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

Reference 67

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

Source-reported events for the cited work

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

source=arxiv_source observed=2026-08-14T15:20:02.219595Z digest=sha256:4854d13359424c03f861ca6b87701953e3565b8d30714ea212b9bdfd35a4f5b4

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

This paper cites and Bourban, G.

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

Reference 68

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

Source-reported events for the cited work

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

source=arxiv_source observed=2026-08-14T15:20:02.224625Z digest=sha256:94593b28e404386cd3e670caaa6936b7090764d340539c6c7da84083bc9810e5

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:ef12c9278477b17ddaffafcf702d0b125e06ba2bd7548cf87e81f725f810a22f

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=sha256:9649d166b9876725aefe8597a503b12612d35115ce84b1ac9441129a428ca884

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=sha256:8688c25a369933abf2472b76489c4f0f60c9dae363f37f9358e6a911dcc7a692

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

This paper cites and Heinke, Craig O.

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

Reference 73

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

Source-reported events for the cited work

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

source=arxiv_source observed=2026-08-14T15:20:02.250481Z digest=sha256:fb5369d3e5ca9e7c770a529bbb21f0078e23fadb34dae43129b0750ff67389e5

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=sha256:7443992ea48541c01ba75d11a8440af0dfce28bc03ed227709f064c7b1f4ec35

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:bad24ae83f3cb084a2a8b721838023a9f51e6b3c2f7088f5dfe7b05b0ffd72d5

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:e2e8e2bd958b55a7adfd66d2632290c2544a8f6e0ca911241ef9ed2bbf88b0a5

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

This paper cites an unresolved cited work.

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

Reference 77

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

Source-reported events for the cited work

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

source=arxiv_source observed=2026-08-14T15:20:02.270463Z digest=sha256:d4b52c2597026a1ab4b9fe8d82a1f4355c799bc107ad8db1f34ee2a64dae0d9e

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

This paper cites High-Mass.

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

Reference 78

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

Source-reported events for the cited work

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

source=arxiv_source observed=2026-08-14T15:20:02.275685Z digest=sha256:ecf747b70e24c9762c39245ad03b15fb4421ebd47d01a4ef37921b97ac808309

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

This paper cites and Sguera, V.

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

Reference 79

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

Source-reported events for the cited work

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

source=arxiv_source observed=2026-08-14T15:20:02.281272Z digest=sha256:38f7ead00c7d2bf3ef92cf927bf034c88e414ddfa2671cd64ab809d7a4dbac22

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:a051884488b45dc591c5fbd9335e09f6048941ef806746b98fc878fe23672fea

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=sha256:955ec473e8cacfab6744c14d4c49772e7c2b96b3b2f445b8ed189225e8345cd4

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=sha256:97870fd4a441ae48935bcad67a6f37eb99551da5f0de5e72173220666a9cba0c

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=sha256:63a30088f9d1756f5020d468f821a355e97749bdba261c268f4970aba9e42daa

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=sha256:056016b81ed49697e4d4287c95c6bdb657dc464aed886855902f7bda3b7d5d44

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:f73da9ebccdd78c88ef4bae85b3486bc512be6aa802eab030bb34cde89475af8

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=sha256:58ab98c00591d4fe63b5082521d0f384777de29d886aa883110f7cc949556cfa

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

This paper cites Low-Luminosity Observation of.

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

Reference 87

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

Source-reported events for the cited work

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

source=arxiv_source observed=2026-08-14T15:20:02.323163Z digest=sha256:4311994a7ad467dc5f14d5ce07e6998316b5dfd429d4187f106942d348eca721

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:eb82c476693b97b3f3eaf20001e14bf7142d0a71a31f8ab8197a74216cc1437b

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:c7844443411f13f9ec3da36d00553686a8d62d68faac8b20459d56ada55142b0

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:acd96ce90bba60fdcdabbf09218dd4c3d0785a053c2f994cc2d2f2dc8addbf24

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=sha256:983451d1761ec6d065cdcf242a7ad508ececeee5735253a9308b1eca95c75bc8

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=sha256:3c0a4f7f0fdfdf2401b8bc45b7b5f3c906b5902bdfa81dea7ef24a8f596165d1

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=sha256:14f8acc491535594c68f7217c1fa370df145e2cfe754ff12ae0a2d3fb65c342c

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:a217c51c7b5588ce67cd5a685224d445e0fa961a48cd6c0817b66805b1715169

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=sha256:2ae55be1567e45d89c9d5c88f2191ab87f6b46d896090bad2ac7258807e92f0e

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

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

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

Reference 96

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

Source-reported events for the cited work

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

source=arxiv_source observed=2026-08-14T15:20:02.369996Z digest=sha256:4883bf1a05927600c5fc0c1be6bc1d47900698c1980e62839a6779dd227a6f77

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=sha256:3ae70b3b883eeb348af823d54c8e75a312d1a38b231296f16a8f729ad42610d6

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=sha256:16576091562c5ebb466d9773fe34d16c24e4f5a0f9e25f15c35410b9de926e1b

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:dd1f2f80655718eb98b030e99b71fcf097ccf0d496b0158a63da16d20148419e

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=sha256:47b59543a2ad8b079542a36c28e648c3a47c9af8742ece6cceb76fa9ef0444ea

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=sha256:9b2b5cf446ada08a94cd0badb40b0fa74010275e078e1cbd3d35bf743df08e9f

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

This paper cites an unresolved cited work.

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

Reference 105

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

Source-reported events for the cited work

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

source=arxiv_source observed=2026-08-14T15:20:02.417381Z digest=sha256:88b439c1843cd4e639f3657e4205b80ff1e97932db8c1ca2b2cbd0962983cbf2

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

This paper cites an unresolved cited work.

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

Reference 106

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

Source-reported events for the cited work

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

source=arxiv_source observed=2026-08-14T15:20:02.422576Z digest=sha256:9070886a91be4ced9e7690819a8f7151e2496f2773e127c2ed2bc9fa90f124b2

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:ece739d0954c03369c408f67eaabf5106ef11b93219f22d321f0e9336c4b3021

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=sha256:97e383447c5dc827050c759e3ccf572af82c157ad02de5eb1799279ea445fd72

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

This paper cites an unresolved cited work.

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

Reference 109

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

Source-reported events for the cited work

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

source=arxiv_source observed=2026-08-14T15:20:02.438923Z digest=sha256:27bc81abafb277ec97723f4a8429eac7e81efb795c2f630ed9ddda8dc4cc3713

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:ba0b6bccdb3e09e16b5604d2a1a754ca09be8840b4680cb28e27a50b028ce9ce

Pith citing papers

No inbound Pith citation observations are available.