Paper Citation Record · LEDGER

Frequency Standard Contributions to Limitations on the Signal-to-Noise Ratio in Very Long Baseline Interferometric (VLBI) Observations

As of 5 August 2026, this Paper Citation Record lists 20 of 20 outbound references and 1 inbound Pith citation observation for arXiv:2508.19123.

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

pith.paper-citation-record.v1
2508.19123 v2

Coverage vector

measured 20 of 20 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-07-11T11:50:26.030339Z

measured 21 of 21 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-05T06:32:48.257954+00:00

measured 1 of 1 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-03T12:49:34.374829Z

measured 0 of 1 external citation measurements

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

Source: cited_works

Reference resolution

20 of 20 outbound references displayed

verified exact9
verified fuzzy10
unresolved1
parse uncertain0
malformed identifier0
metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

Observation 3f3bade3-2e52-4a9f-8242-892fd9bb6128 · outbound

This paper cites Ultra stable oscillator (USO) for deep space exploration.

Frequency Standard Contributions to Limitations on the Signal-to-Noise Ratio in Very Long Baseline Interferometric (VLBI) Observations Ultra stable oscillator (USO) for deep space exploration

Reference 1

Resolution: verified fuzzy; raw_fallback, observed 2026-05-18T21:01:52.087326Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation d65c3fc8-bd37-4002-ac47-f709379ad37f · outbound

This paper cites Each graph shows results for a different VLBI frequency: a) 90 GHz, b) 230 GHz, c) 345 GHz, and d) 630 GHz.

Frequency Standard Contributions to Limitations on the Signal-to-Noise Ratio in Very Long Baseline Interferometric (VLBI) Observations Each graph shows results for a different VLBI frequency: a) 90 GHz, b) 230 GHz, c) 345 GHz, and d) 630 GHz

Reference 2

Resolution: verified fuzzy; raw_fallback, observed 2026-05-18T21:01:52.091253Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 375a6be7-733b-4717-8505-91b39b4ea560 · outbound

This paper cites an unresolved cited work.

Frequency Standard Contributions to Limitations on the Signal-to-Noise Ratio in Very Long Baseline Interferometric (VLBI) Observations Unresolved cited work

Reference 3

Resolution: unresolved; raw_fallback, observed 2026-05-18T21:01:52.095142Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation b6001dde-af7e-4c5a-b6f9-1338b0c77b3a · outbound

This paper cites Space-qualified rubidium atomic frequency standard clocks.

Frequency Standard Contributions to Limitations on the Signal-to-Noise Ratio in Very Long Baseline Interferometric (VLBI) Observations Space-qualified rubidium atomic frequency standard clocks

Reference 4

Resolution: verified fuzzy; raw_fallback, observed 2026-05-18T21:01:52.121967Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 79995800-b653-4189-a42b-00d064a78469 · outbound

This paper cites Figure 13 shows the results of simulating clock-limited S/N from equations (38) - (42) for the currently operating high-performance space clocks.

Frequency Standard Contributions to Limitations on the Signal-to-Noise Ratio in Very Long Baseline Interferometric (VLBI) Observations Figure 13 shows the results of simulating clock-limited S/N from equations (38) - (42) for the currently operating high-performance space clocks

Reference 5

Resolution: verified fuzzy; raw_fallback, observed 2026-05-18T21:01:52.130494Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 52d24df6-7577-4733-8ee3-3fc1e3652942 · outbound

This paper cites Each graph shows results for a different VLBI frequency: a) 90 GHz, b) 230 GHz, c) 345 GHz, and d) 630 GHz.

Reference 6

Resolution: verified fuzzy; raw_fallback, observed 2026-05-18T21:01:52.117382Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 0857e6b0-f866-4299-84f6-34ee45e43a5e · outbound

This paper cites warm-cell optical clock.

Frequency Standard Contributions to Limitations on the Signal-to-Noise Ratio in Very Long Baseline Interferometric (VLBI) Observations warm-cell optical clock

Reference 7

Resolution: verified fuzzy; raw_fallback, observed 2026-05-18T21:01:52.126396Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation eb2525cf-2e99-4c91-8022-7fa132f2b63a · outbound

This paper cites The OLO is significantly better than the iodine clock and the ACES maser on short time scales, but crosses over iodine at about 20 seconds and the maser at about 100 seconds.

Frequency Standard Contributions to Limitations on the Signal-to-Noise Ratio in Very Long Baseline Interferometric (VLBI) Observations The OLO is significantly better than the iodine clock and the ACES maser on short time scales, but crosses over iodine at about 20 seconds and the maser at about 100 seconds

Reference 8

Resolution: verified fuzzy; raw_fallback, observed 2026-05-18T21:01:52.112703Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 8e9342cf-ab4a-492c-80ff-64ce5010d831 · outbound

This paper cites Each trace corresponds to the coherence function for the indicated VLBI frequency.

Frequency Standard Contributions to Limitations on the Signal-to-Noise Ratio in Very Long Baseline Interferometric (VLBI) Observations Each trace corresponds to the coherence function for the indicated VLBI frequency

Reference 9

Resolution: verified fuzzy; raw_fallback, observed 2026-05-18T21:01:52.106988Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation f068fb6a-fa9e-48c7-b13b-c43843043586 · outbound

This paper cites #+𝜈AB. Under these conditions the exponential is very nearly linear over the band and can be treated as a constant evaluated at the center frequency, 𝜈=𝜈.

Frequency Standard Contributions to Limitations on the Signal-to-Noise Ratio in Very Long Baseline Interferometric (VLBI) Observations #+𝜈AB. Under these conditions the exponential is very nearly linear over the band and can be treated as a constant evaluated at the center frequency, 𝜈=𝜈

Reference 10

Resolution: verified fuzzy; raw_fallback, observed 2026-05-18T21:01:52.102829Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 6584842c-d324-4490-b3e2-6a04449ac940 · outbound

This paper cites flicker floor.

Frequency Standard Contributions to Limitations on the Signal-to-Noise Ratio in Very Long Baseline Interferometric (VLBI) Observations flicker floor

Reference 11

Resolution: verified fuzzy; raw_fallback, observed 2026-05-18T21:01:52.098821Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 44e18914-74e3-4639-ae77-58af418f7895 · outbound

This paper cites Copyright to be transferred to the journal within 10 days of acceptance.

Frequency Standard Contributions to Limitations on the Signal-to-Noise Ratio in Very Long Baseline Interferometric (VLBI) Observations Copyright to be transferred to the journal within 10 days of acceptance

Reference 12

Resolution: verified exact; doi, observed 2026-05-18T21:01:50.670851Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 276e2f36-0b3b-4332-b48c-b54158832025 · outbound

This paper cites E., Pesce, D.

Frequency Standard Contributions to Limitations on the Signal-to-Noise Ratio in Very Long Baseline Interferometric (VLBI) Observations E., Pesce, D

Reference 13

Resolution: verified exact; doi, observed 2026-05-18T21:01:50.683347Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation d2c275f8-7f53-44c7-9806-51b8206cd7fa · outbound

This paper cites an unresolved cited work.

Frequency Standard Contributions to Limitations on the Signal-to-Noise Ratio in Very Long Baseline Interferometric (VLBI) Observations Unresolved cited work

Reference 14

Resolution: verified exact; doi, observed 2026-05-18T21:01:50.686960Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation c07512b1-07f6-4a25-8bb1-f151e7a1665f · outbound

This paper cites an unresolved cited work.

Frequency Standard Contributions to Limitations on the Signal-to-Noise Ratio in Very Long Baseline Interferometric (VLBI) Observations Unresolved cited work

Reference 15

Resolution: verified exact; doi, observed 2026-05-18T21:01:50.690942Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation ef31ed83-b068-44b8-9455-959d57aa814f · outbound

This paper cites First Very Long Baseline Interferometry Detections at 870{\mu}m.

Frequency Standard Contributions to Limitations on the Signal-to-Noise Ratio in Very Long Baseline Interferometric (VLBI) Observations First Very Long Baseline Interferometry Detections at 870{\mu}m

Reference 16

Resolution: verified exact; arxiv_id, observed 2026-05-18T21:01:50.701882Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 88da0aa1-2bea-4304-8535-8d7b60cd3217 · outbound

This paper cites High Precision Astrometric Millimeter VLBI Using a New Method for Atmospheric Calibration.

Frequency Standard Contributions to Limitations on the Signal-to-Noise Ratio in Very Long Baseline Interferometric (VLBI) Observations High Precision Astrometric Millimeter VLBI Using a New Method for Atmospheric Calibration

Reference 17

Resolution: verified exact; local_arxiv, observed 2026-05-18T21:01:50.712610Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 251e6870-ccf7-4c48-822e-7a3c94471533 · outbound

This paper cites an unresolved cited work.

Frequency Standard Contributions to Limitations on the Signal-to-Noise Ratio in Very Long Baseline Interferometric (VLBI) Observations Unresolved cited work

Reference 18

Resolution: verified exact; doi, observed 2026-05-18T21:01:50.694897Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 528c7fce-e098-4b28-9f52-c7a590d8b57f · outbound

This paper cites an unresolved cited work.

Frequency Standard Contributions to Limitations on the Signal-to-Noise Ratio in Very Long Baseline Interferometric (VLBI) Observations Unresolved cited work

Reference 19

Resolution: verified exact; arxiv_id, observed 2026-05-18T21:01:50.678038Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 6e0e15f4-b531-4302-b05e-1e1de942f35e · outbound

This paper cites https://vremya-ch.com/index.php/en/progects-en/spaceapplications-en/vch-1010-en-2/index.html.

Frequency Standard Contributions to Limitations on the Signal-to-Noise Ratio in Very Long Baseline Interferometric (VLBI) Observations https://vremya-ch.com/index.php/en/progects-en/spaceapplications-en/vch-1010-en-2/index.html

Reference 20

Resolution: verified exact; doi, observed 2026-05-18T21:01:50.706410Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Pith citing papers

Observation 3f69ca87-edd3-4b82-ae3d-c036f3be4bd8 · inbound

When the Shadow Meets Its Measure: Assessing the Feasibility of Submillimeter Black Hole Shadow Imaging in Megamaser Disk AGN cites this paper.

When the Shadow Meets Its Measure: Assessing the Feasibility of Submillimeter Black Hole Shadow Imaging in Megamaser Disk AGN Frequency Standard Contributions to Limitations on the Signal-to-Noise Ratio in Very Long Baseline Interferometric (VLBI) Observations

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-03T12:49:34.374829Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.