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Paper Citation Record · LEDGER

The Planck High Frequency Instrument, a 3rd generation CMB experiment, and a full sky submillimeter survey

As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/0308075.

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

pith.paper-citation-record.v1
astro-ph/0308075 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 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 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T11:12:53.077373Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-26T07:49:08.559474Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 9196f81b-7d7a-4d1f-b3a5-5905f0646f96 · inbound

CAPMAP: A New Instrument to Measure the E-mode CMB Polarization on Angular Scales of 4 arcmin to 40 arcmin cites this paper.

CAPMAP: A New Instrument to Measure the E-mode CMB Polarization on Angular Scales of 4 arcmin to 40 arcmin The Planck High Frequency Instrument, a 3rd generation CMB experiment, and a full sky submillimeter survey

Reference 91

Resolution
unresolved
no resolver link, observed 2026-08-12T11:12:53.077373Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-12T11:12:53.077373Z digest=sha256:41f79b45bf4f0d50128cd74783f8f491ad370ba84513590d3ed106305d4aada5

Observation 31b9c0e4-c55d-4dc9-8e88-76200045f92e · inbound

Characterising magnetic fields at the onset of star cluster formation: From giant molecular clouds to infrared dark clumps cites this paper.

Characterising magnetic fields at the onset of star cluster formation: From giant molecular clouds to infrared dark clumps The Planck High Frequency Instrument, a 3rd generation CMB experiment, and a full sky submillimeter survey

Reference 94

Resolution
verified exact
local_arxiv, observed 2026-06-26T07:49:08.560756Z

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=2026-07-11T11:50:26.030339Z digest=sha256:a49917e4b16b77b43a745216a517379fec4e151a7b45449c54880eafd71e277b