Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-05-22T15:40:12.948232Z
Paper Citation Record · LEDGER
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear
As of 13 August 2026, this Paper Citation Record lists 95 of 95 outbound references and 8 inbound Pith citation observations for arXiv:2505.07924.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-12T06:34:41.77262+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-06T15:29:18.279667Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-02T04:26:36.362591Z
Reference resolution
95 of 95 outbound references displayed
- verified exact1
- verified fuzzy65
- unresolved27
- parse uncertain1
- malformed identifier1
- metadata mismatch0
External citation measurements
No source-named external measurement is stored.
Outbound references
Observation fccb0541-9d72-4358-8300-a8f0ed740711 · outbound
This paper cites an unresolved cited work.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Unresolved cited work
Reference 1
- Resolution
- unresolved
- raw_fallback, observed 2026-05-22T15:41:45.946155Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 152a1cfe-92eb-4d44-8066-48ca917f215f · outbound
This paper cites an unresolved cited work.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Unresolved cited work
Reference 2
- Resolution
- unresolved
- raw_fallback, observed 2026-05-22T15:41:45.928563Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 75cb370e-0997-4afa-8888-f3c6842e33ca · outbound
This paper cites Learning the Universe.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Learning the Universe
Reference 3
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:46.125282Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation d00ebf0f-e5f8-49af-923a-4d780c6400b9 · outbound
This paper cites an unresolved cited work.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Unresolved cited work
Reference 4
- Resolution
- unresolved
- raw_fallback, observed 2026-05-22T15:41:45.966222Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 87fac8b7-0ad2-415e-b361-3b93d9b43682 · outbound
This paper cites Lin, Sub-GeV dark matter models and direct detection, inDark Matter, Les Houches Summer School 2021 (SciPost, 2022).
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Lin, Sub-GeV dark matter models and direct detection, inDark Matter, Les Houches Summer School 2021 (SciPost, 2022)
Reference 5
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:45.871370Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation e0c096a0-8df4-4d6c-8c55-32da07abdfbc · outbound
This paper cites Yu, TASI lectures: a dark matter primer, inThe Frontiers of Particle Theory(2025).
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Yu, TASI lectures: a dark matter primer, inThe Frontiers of Particle Theory(2025)
Reference 6
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:46.039889Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation e536353c-ea29-47ff-a144-500da5a1d01e · outbound
This paper cites McCabe, Astrophysical uncertainties of dark matter direct detection experiments, Phys.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear McCabe, Astrophysical uncertainties of dark matter direct detection experiments, Phys
Reference 7
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:45.898068Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 8def52b9-b62b-4af2-9050-56ff1bf7d37f · outbound
This paper cites Baxteret al., Recommended conventions for reporting results from direct dark matter searches, Eur.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Baxteret al., Recommended conventions for reporting results from direct dark matter searches, Eur
Reference 8
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:45.894167Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation dcc6bfcf-c579-4bed-b288-ec4f92409a63 · outbound
This paper cites Aalberset al., A next-generation liquid xenon observatory for dark matter and neutrino physics, J.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Aalberset al., A next-generation liquid xenon observatory for dark matter and neutrino physics, J
Reference 9
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:46.004794Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation bc605f00-0a2e-45fb-ba70-e4fc1621ddad · outbound
This paper cites Wasserman, Possibility of detecting heavy neutral fermions in the Galaxy, Phys.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Wasserman, Possibility of detecting heavy neutral fermions in the Galaxy, Phys
Reference 10
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:45.908566Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 596a223e-5b59-4bdc-a57a-b586b935f2fa · outbound
This paper cites an unresolved cited work.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Unresolved cited work
Reference 11
- Resolution
- unresolved
- raw_fallback, observed 2026-05-22T15:41:45.924944Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation ce2b15ed-dd9a-42ef-891c-416129c444cc · outbound
This paper cites Freese, J.
Reference 12
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:45.890584Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 3f1eb5cd-902b-4d4a-beeb-620d3bafe0ce · outbound
This paper cites Wojtak, E.
Reference 13
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:46.097582Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation b07729e5-a0f5-4d9b-a3cc-f647388c6add · outbound
This paper cites an unresolved cited work.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Unresolved cited work
Reference 14
- Resolution
- unresolved
- raw_fallback, observed 2026-05-22T15:41:46.094372Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation a5a5df94-4b4f-4c06-8428-b60e2053531d · outbound
This paper cites Vogelsberger, S.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Vogelsberger, S
Reference 15
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:45.858728Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation ccea1401-9f90-488b-8d31-82f5d3718e60 · outbound
This paper cites Vogelsberger, A.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Vogelsberger, A
Reference 16
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:46.055801Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 2de42cd4-db05-4930-8413-725a1d6a97d2 · outbound
This paper cites Kuhlen, N.
Reference 17
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:46.139745Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 97e527cc-7939-4937-a687-679cc555988b · outbound
This paper cites an unresolved cited work.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Unresolved cited work
Reference 18
- Resolution
- unresolved
- raw_fallback, observed 2026-05-22T15:41:46.133719Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation dfae41d2-de95-4439-952f-7185c578a716 · outbound
This paper cites Vogelsberger and J.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Vogelsberger and J
Reference 19
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:45.915265Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation b941f6ca-64ac-4751-a567-79f2203aec03 · outbound
This paper cites Bozorgnia and G.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Bozorgnia and G
Reference 20
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:46.128040Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 119eb016-fc99-4138-bb45-76a10f1cb8db · outbound
This paper cites an unresolved cited work.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Unresolved cited work
Reference 21
- Resolution
- unresolved
- raw_fallback, observed 2026-05-22T15:41:46.030627Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 0f4f091c-e3a9-4d4c-8b07-335d96bd4700 · outbound
This paper cites an unresolved cited work.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Unresolved cited work
Reference 22
- Resolution
- unresolved
- raw_fallback, observed 2026-05-22T15:41:46.149978Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 6f9c3935-4077-4ca1-a858-61b8e90d3440 · outbound
This paper cites Pillepich, M.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Pillepich, M
Reference 23
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:45.935464Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 589c56b1-8a15-4824-bb5c-58a39803f8fc · outbound
This paper cites Butsky, A.
Reference 24
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:45.956631Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation b712af78-60f5-4693-93dc-80c7b4434d3a · outbound
This paper cites Kelso, C.
Reference 25
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:46.156531Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 080cee83-c82b-4180-b066-6e3de269f52e · outbound
This paper cites an unresolved cited work.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Unresolved cited work
Reference 26
- Resolution
- unresolved
- raw_fallback, observed 2026-05-22T15:41:45.949479Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 4d6f7839-d88f-48ac-9d0c-7b66f312d571 · outbound
This paper cites Bozorgnia, F.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Bozorgnia, F
Reference 27
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:46.008076Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 63c6679e-5bed-4081-bbde-84f71f8f2e88 · outbound
This paper cites Poole-McKenzie, A.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Poole-McKenzie, A
Reference 28
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:45.994722Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 3d4ef5da-1c9f-4d83-bf48-b48ec050c61e · outbound
This paper cites Bozorgnia, A.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Bozorgnia, A
Reference 29
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:45.991497Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation e73648f1-9e4d-457e-9aa5-8c6316923aec · outbound
This paper cites Hryczuk, E.
Reference 30
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:45.952752Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation ad962999-bfda-4f14-9eff-d7c93c73e3e5 · outbound
This paper cites Nu˜nez-Casti˜neyra, E.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Nu˜nez-Casti˜neyra, E
Reference 31
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:45.963115Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation b7416461-7ce8-4ff7-ac6e-b6cb25ba01ae · outbound
This paper cites an unresolved cited work.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Unresolved cited work
Reference 32
- Resolution
- unresolved
- raw_fallback, observed 2026-05-22T15:41:46.049580Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 88f6c874-8287-4cc4-aced-a1eba544a79b · outbound
This paper cites an unresolved cited work.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Unresolved cited work
Reference 33
- Resolution
- unresolved
- raw_fallback, observed 2026-05-22T15:41:46.046574Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation eedd4904-25e5-4a9e-b826-4857e38994d6 · outbound
This paper cites Hammer, M.
Reference 34
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:46.043216Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 250386f1-13b7-4787-9b50-0972dcea0d2d · outbound
This paper cites an unresolved cited work.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Unresolved cited work
Reference 35
- Resolution
- unresolved
- raw_fallback, observed 2026-05-22T15:41:45.911878Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation e85c4abb-e848-4e8b-883a-f8fdafbc28be · outbound
This paper cites Boardman, G.
Reference 36
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:45.905040Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation e0879c8f-f7dd-4fb7-8ef3-7bc73cfbf9bc · outbound
This paper cites Tsukui, E.
Reference 37
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:46.119188Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation bb969956-d60e-4e33-87c3-4354cd2cea04 · outbound
This paper cites Nelson, A.
Reference 38
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:46.027661Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 1317100b-fdea-4547-8a29-0d45d3be1774 · outbound
This paper cites Pillepich, D.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Pillepich, D
Reference 39
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:46.078492Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation a982a84e-d392-496e-bcfa-d68904585a24 · outbound
This paper cites Helmi, C.
Reference 40
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:45.881037Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 8680f2d4-6317-4508-9a25-0ae07ef7cfb2 · outbound
This paper cites Belokurov, D.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Belokurov, D
Reference 41
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:45.887471Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 4d9b5631-d0d5-415f-b858-676a292c6c59 · outbound
This paper cites an unresolved cited work.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Unresolved cited work
Reference 42
- Resolution
- unresolved
- raw_fallback, observed 2026-05-22T15:41:45.874533Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation e23449aa-db2b-4265-b424-015cc694158e · outbound
This paper cites Aprileet al., (XENON Collaboration), Dark matter search results from a one ton-year exposure of XENON1T, Phys.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Aprileet al., (XENON Collaboration), Dark matter search results from a one ton-year exposure of XENON1T, Phys
Reference 43
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:45.877944Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 62fa17f8-373f-4b17-a5e9-31347fb0f187 · outbound
This paper cites Aprileet al., (XENON Collaboration), First dark matter search with nuclear recoils from the XENONnT Experiment, Phys.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Aprileet al., (XENON Collaboration), First dark matter search with nuclear recoils from the XENONnT Experiment, Phys
Reference 44
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:45.939204Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 226ba66d-8887-4665-9eb1-0a42c0540f38 · outbound
This paper cites Aalberset al., (LZ Collaboration), Dark matter search results from 4.2 tonne-years of exposure of the LUX-ZEPLIN (LZ) Experiment, Phys.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Aalberset al., (LZ Collaboration), Dark matter search results from 4.2 tonne-years of exposure of the LUX-ZEPLIN (LZ) Experiment, Phys
Reference 45
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:45.862753Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 5fa3cf9f-302e-4bb2-8c59-732f367cf546 · outbound
This paper cites Springel, S.
Reference 46
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:46.058930Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation c5fe898f-1945-4384-bbb0-39173a2b1e62 · outbound
This paper cites Dolag, S.
Reference 47
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:45.884071Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation b7fdbdbd-9704-43ab-98e6-c7e54ce2f0b9 · outbound
This paper cites Folsom, M.
Reference 48
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:45.918388Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation eba87a8b-8a5a-4c71-bd4a-7122afba6dfe · outbound
This paper cites Sotillo-Ramos, A.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Sotillo-Ramos, A
Reference 49
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:45.972337Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 053df00e-bf97-4112-b122-42b4621ac926 · outbound
This paper cites Pillepich, D.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Pillepich, D
Reference 50
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:46.033802Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 36a006eb-a388-4bc1-8630-3d673b4ba56a · outbound
This paper cites an unresolved cited work.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Unresolved cited work
Reference 51
- Resolution
- unresolved
- raw_fallback, observed 2026-05-22T15:41:46.113091Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation f5f4d85c-6cbd-4fe4-8a7e-2538521d7e14 · outbound
This paper cites Bovy and H.-W.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Bovy and H.-W
Reference 52
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:45.975761Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 543648b8-80cf-46b9-be87-c48583afeadf · outbound
This paper cites an unresolved cited work.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Unresolved cited work
Reference 53
- Resolution
- unresolved
- raw_fallback, observed 2026-05-22T15:41:46.106746Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 11f6a92e-3c3d-4d5f-a86a-37a0dea62b93 · outbound
This paper cites Juri´cet al., The Milky Way tomography with SDSS.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Juri´cet al., The Milky Way tomography with SDSS
Reference 54
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:46.110131Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation d5d35270-74ce-46c6-b3dc-ee219d4a4c59 · outbound
This paper cites Rix and J.
Reference 55
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:46.116031Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation b003ba1f-39b7-47ca-827a-c471db1a0732 · outbound
This paper cites Bland-Hawthorn and O.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Bland-Hawthorn and O
Reference 56
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:46.036591Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation e404e5d5-2a49-41e9-b186-3551b8add7e3 · outbound
This paper cites Varma, M.
Reference 57
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:46.085683Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 41729ee9-c0aa-4257-a5bc-bc3e81f7519f · outbound
This paper cites Rosas-Guevara, S.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Rosas-Guevara, S
Reference 58
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:46.018011Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation ace25c5f-4618-45a6-a086-ff9b5313653b · outbound
This paper cites an unresolved cited work.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Unresolved cited work
Reference 59
- Resolution
- unresolved
- raw_fallback, observed 2026-05-22T15:41:46.088574Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 4439cb5d-827d-4cb8-a305-64e801d407b7 · outbound
This paper cites Abuteret al., (GRA VITY Collaboration), Improved GRA VITY astrometric accuracy from modeling optical aberrations, Astron.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Abuteret al., (GRA VITY Collaboration), Improved GRA VITY astrometric accuracy from modeling optical aberrations, Astron
Reference 60
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:46.103653Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation fb89a41d-9215-41fc-8c50-c646534bfd33 · outbound
This paper cites Abd El Dayemet al., (GRA VITY Collaboration), Improving constraints on the extended mass distribution in the Galactic Center with stellar orbits, Astron.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Abd El Dayemet al., (GRA VITY Collaboration), Improving constraints on the extended mass distribution in the Galactic Center with stellar orbits, Astron
Reference 61
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:46.001288Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 3658a9cf-4488-4611-83f7-5bdec4f5e92f · outbound
This paper cites Binney and S.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Binney and S
Reference 62
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:46.011406Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 18ce34a3-cbf1-45e4-8608-dabb32de35e0 · outbound
This paper cites Bovy, The asymmetric drift and the Sun’s motion, inDynam- ics and Astrophysics of Galaxies(Princeton University Press, Princeton, NJ, 2026, in press.) Chap.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Bovy, The asymmetric drift and the Sun’s motion, inDynam- ics and Astrophysics of Galaxies(Princeton University Press, Princeton, NJ, 2026, in press.) Chap
Reference 63
- Resolution
- malformed identifier
- raw_fallback, observed 2026-05-22T15:41:46.024441Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 7ed83ae5-5fb9-447c-9a35-0ca28837fe8d · outbound
This paper cites Sch¨onrich, J.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Sch¨onrich, J
Reference 64
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:46.069340Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation c8220b8a-ef68-4d00-8daa-205a879a4b9f · outbound
This paper cites Kawata, J.
Reference 65
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:46.122270Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation de25dabe-d06e-4ebd-bca1-12ed06358e79 · outbound
This paper cites P ˜oder, M.
Reference 66
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:45.960193Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 762de6e3-ced6-47ee-b140-61e8c699ad3e · outbound
This paper cites Decoding the Galactic Twirl: The Downfall of Milky Way-mass Galaxies Rotation Curves in the FIRE Simulations.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Decoding the Galactic Twirl: The Downfall of Milky Way-mass Galaxies Rotation Curves in the FIRE Simulations
Reference 67
- Resolution
- verified exact
- arxiv_id, observed 2026-05-22T15:41:45.352501Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 73f24be2-f856-4680-be8d-66b9a5045293 · outbound
This paper cites an unresolved cited work.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Unresolved cited work
Reference 68
- Resolution
- unresolved
- raw_fallback, observed 2026-05-22T15:41:45.921720Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 32639951-8e9f-4b67-bdf6-8d163c7ac160 · outbound
This paper cites Wetzelet al., Public data release of the FIRE-2 cosmological zoom-in simulations of galaxy formation, Astrophys.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Wetzelet al., Public data release of the FIRE-2 cosmological zoom-in simulations of galaxy formation, Astrophys
Reference 69
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:45.979542Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 31851606-e0ea-47f5-aa76-b900f4918a51 · outbound
This paper cites Schayeet al., The EAGLE project: Simulating the evolution and assembly of galaxies and their environments, Mon.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Schayeet al., The EAGLE project: Simulating the evolution and assembly of galaxies and their environments, Mon
Reference 70
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:46.142944Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 085f5911-6fae-4a49-9044-03f409a093d3 · outbound
This paper cites an unresolved cited work.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Unresolved cited work
Reference 71
- Resolution
- unresolved
- raw_fallback, observed 2026-05-22T15:41:46.091330Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation c3ed10e7-3188-4bd9-ac85-c0945c6e69ed · outbound
This paper cites Sawala, C.
Reference 72
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:46.100563Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 8d5a749a-115e-4b38-b549-eba8eb0f4397 · outbound
This paper cites Fattahi, J.
Reference 73
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:46.153117Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 96f65fab-3bfa-442a-8668-20558515c8fc · outbound
This paper cites an unresolved cited work.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Unresolved cited work
Reference 74
- Resolution
- unresolved
- raw_fallback, observed 2026-05-22T15:41:46.066009Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 69d6caa2-520f-476e-a543-516f1cac9d0a · outbound
This paper cites Aalbers, B.
Reference 75
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:46.072776Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation e3406524-f932-405f-8bfc-c5f1b03d187b · outbound
This paper cites McCabe, The Earth’s velocity for direct detection experiments, J.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear McCabe, The Earth’s velocity for direct detection experiments, J
Reference 76
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:46.062149Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 1362bbed-8021-4bea-8b5c-8f5a2f85ae63 · outbound
This paper cites an unresolved cited work.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Unresolved cited work
Reference 77
- Resolution
- unresolved
- raw_fallback, observed 2026-05-22T15:41:46.082031Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation b4c04cb0-f836-4883-8c05-99a14794c8d1 · outbound
This paper cites Aprileet al., (XENON Collaboration), An approximate likeli- hood for nuclear recoil searches with XENON1T data, Eur.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Aprileet al., (XENON Collaboration), An approximate likeli- hood for nuclear recoil searches with XENON1T data, Eur
Reference 78
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:46.014782Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 07907b73-fd9c-47b4-b1b6-35ac1521a2eb · outbound
This paper cites an unresolved cited work.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Unresolved cited work
Reference 79
- Resolution
- unresolved
- raw_fallback, observed 2026-05-22T15:41:45.997810Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 33f761cb-1e54-46d8-9a48-75cffbc0eb03 · outbound
This paper cites an unresolved cited work.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Unresolved cited work
Reference 80
- Resolution
- unresolved
- raw_fallback, observed 2026-05-22T15:41:46.130810Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation a3b593b2-d7e1-46ae-9977-a03a4c150655 · outbound
This paper cites an unresolved cited work.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Unresolved cited work
Reference 81
- Resolution
- unresolved
- raw_fallback, observed 2026-05-22T15:41:46.160043Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 52da4ec2-ccce-4031-94e5-a1c19e41b2c3 · outbound
This paper cites an unresolved cited work.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Unresolved cited work
Reference 82
- Resolution
- unresolved
- raw_fallback, observed 2026-05-22T15:41:45.988441Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation c8a6e3c3-726a-4dbf-86f5-9562e2319d86 · outbound
This paper cites Lancaster, S.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Lancaster, S
Reference 83
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:46.075623Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation a9cbc6d0-b4cf-47ab-b49a-11fac5ff6acc · outbound
This paper cites Necib, M.
Reference 84
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:46.052924Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 9da17b30-f7a4-4aba-be41-96402617bb3a · outbound
This paper cites Fattahi, V.
Reference 85
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:45.985558Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 8de41082-4631-457b-986f-77c1eec487dd · outbound
This paper cites Iorio and V.
Reference 86
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:46.146856Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation a162ec47-acf7-41ab-b408-f72642b37318 · outbound
This paper cites Besla, A.
Reference 87
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:45.969449Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 8ed16672-7c6c-4adc-a2b2-67121b36f7c9 · outbound
This paper cites Donaldson, M.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Donaldson, M
Reference 88
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:45.982581Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 3a4b4796-753e-4d07-bb4f-bba00923362e · outbound
This paper cites Smith-Orlik, N.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Smith-Orlik, N
Reference 89
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:46.136736Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 66fc2dcc-4c03-4c94-94aa-76d68f4335bf · outbound
This paper cites an unresolved cited work.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Unresolved cited work
Reference 90
- Resolution
- unresolved
- raw_fallback, observed 2026-05-22T15:41:45.942682Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 4ef7d112-f418-4f56-afc6-ad14f7e3e841 · outbound
This paper cites an unresolved cited work.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Unresolved cited work
Reference 91
- Resolution
- unresolved
- raw_fallback, observed 2026-05-22T15:41:45.867742Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 25616302-ccd1-4fea-be56-2a685a9b79ee · outbound
This paper cites an unresolved cited work.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Unresolved cited work
Reference 92
- Resolution
- unresolved
- raw_fallback, observed 2026-05-22T15:41:45.855442Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 7c209b72-de1a-4507-bd5e-60adca550562 · outbound
This paper cites Folsom, folsomde/dm velocity distributions: v1.1, Zenodo (2025).
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Folsom, folsomde/dm velocity distributions: v1.1, Zenodo (2025)
Reference 93
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:45.932179Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 68b7253d-743a-4827-9d48-71eb3cf0757d · outbound
This paper cites an unresolved cited work.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Unresolved cited work
Reference 94
- Resolution
- parse uncertain
- raw_fallback, observed 2026-05-22T15:41:45.901526Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation a2b18a25-216a-46b5-adce-f832a7634eb7 · outbound
This paper cites Garrison-Kimmel, A.
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear Garrison-Kimmel, A
Reference 95
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-22T15:41:46.021313Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Pith citing papers
Observation af4464c6-470d-4473-b5f5-17e9c0d580ed · inbound
Sub-GeV Dark Matter Under Pressure from Direct Detection cites this paper.
Sub-GeV Dark Matter Under Pressure from Direct Detection Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear
Reference 83
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T15:29:18.279667Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 308ec77b-7544-463f-bc3e-7a64d222b6c3 · inbound
How to Build an Empirical Speed Distribution for Dark Matter in the Solar Neighborhood cites this paper.
How to Build an Empirical Speed Distribution for Dark Matter in the Solar Neighborhood Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear
Reference 32
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T08:15:43.993748Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 458c7961-0480-4f35-83ac-9a08344a9f6e · inbound
Information-theoretic astrophysical uncertainties in the effective theory of dark matter direct detection cites this paper.
Information-theoretic astrophysical uncertainties in the effective theory of dark matter direct detection Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear
Reference 101
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T11:50:42.335197Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 3304d7cc-c90c-4d2c-aa49-a894534473e0 · inbound
Implications for Primordial Black Hole Dark Matter from a Single Subsolar Mass Gravitational-wave Detection in LVK O1--O4 cites this paper.
Implications for Primordial Black Hole Dark Matter from a Single Subsolar Mass Gravitational-wave Detection in LVK O1--O4 Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear
Reference 16
- Resolution
- verified exact
- local_arxiv, observed 2026-05-15T19:50:17.417301Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 1128f67f-489c-45fe-95b5-87800b7b2120 · inbound
Dive deeper with SUBMARINE: SUB-Mev dArk matter diRect detectIon using bilayer grapheNE cites this paper.
Dive deeper with SUBMARINE: SUB-Mev dArk matter diRect detectIon using bilayer grapheNE Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear
Reference 85
- Resolution
- verified exact
- local_arxiv, observed 2026-05-11T14:46:31.405761Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 01bbd8f6-0483-4a47-b75a-5f8ddf1c89d7 · inbound
Astrophysical Uncertainties in Sub-GeV Dark Matter Detection via Single Phonon Excitations cites this paper.
Astrophysical Uncertainties in Sub-GeV Dark Matter Detection via Single Phonon Excitations Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear
Reference 67
- Resolution
- verified exact
- local_arxiv, observed 2026-07-02T04:26:36.363880Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation f55f2dda-9c72-4149-a888-00254f9b707d · inbound
Boosted Dark Matter from Sagittarius A$^\star$ cites this paper.
Boosted Dark Matter from Sagittarius A$^\star$ Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear
Reference 56
- Resolution
- verified exact
- local_arxiv, observed 2026-07-01T12:15:44.544921Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 34163f90-f933-443c-992f-0db1c4cc21a5 · inbound
Ubiquitous Corotation of Dark Matter Halos: Implications for Direct Detection cites this paper.
Ubiquitous Corotation of Dark Matter Halos: Implications for Direct Detection Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear
Reference 33
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T01:15:11.029953Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.