Pith. sign in

Paper Citation Record · LEDGER

A new determination of supernova rates and a comparison with indicators for galactic star formation

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:astro-ph/9904225.

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

pith.paper-citation-record.v1
astro-ph/9904225 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-08T06:32:00.761636+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T00:06:25.011406Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

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

External citation measurements

102
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 3568f184-5f3c-4447-81c7-b1204d600657 · inbound

The power of binaries on stripped-envelope supernovae across metallicity: uniform progenitor parameter space and persistently low ejecta masses, but subtype diversity cites this paper.

The power of binaries on stripped-envelope supernovae across metallicity: uniform progenitor parameter space and persistently low ejecta masses, but subtype diversity A new determination of supernova rates and a comparison with indicators for galactic star formation

Reference 31

Resolution
unresolved
no resolver link, observed 2026-08-05T14:41:22.226935Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-05T14:41:22.226935Z digest=sha256:7fdc342b2ad835d0978b60475960d837cea9984bc0ea0612c70798ca4e9a7c4d

Observation e9071e2b-bd8d-4cf1-8972-2a354843b04b · inbound

Are Local Group Dwarf Spheroidal Galaxies the First Safe Planet-hosting Environments? cites this paper.

Are Local Group Dwarf Spheroidal Galaxies the First Safe Planet-hosting Environments? A new determination of supernova rates and a comparison with indicators for galactic star formation

Reference 14

Resolution
unresolved
no resolver link, observed 2026-08-05T12:25:20.964552Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-05T12:25:20.964552Z digest=sha256:6ccd0c30a8a5cfac61860999d0a62a96555be53317475d4705d6b3dafca1f5ab

Observation f2b4e055-d1d5-40fc-91c9-166772c941ed · inbound

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models cites this paper.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models A new determination of supernova rates and a comparison with indicators for galactic star formation

Reference 297

Resolution
verified exact
local_arxiv, observed 2026-05-21T02:13:55.664640Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

source=arxiv_source observed=2026-05-21T02:13:20.739968Z digest=sha256:a4da3fc9e30e24e3f96a74743f94fa51c335406cd4678c32f8add3d8ae289508

Observation ae6819d3-765d-4b84-a1ea-0b9ab8ffbe1d · inbound

The impact of stellar binaries and star cluster dynamics on pair-instability supernovae cites this paper.

The impact of stellar binaries and star cluster dynamics on pair-instability supernovae A new determination of supernova rates and a comparison with indicators for galactic star formation

Reference 42

Resolution
verified exact
local_arxiv, observed 2026-06-29T02:43:03.592487Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

source=arxiv_source observed=2026-06-29T02:34:47.715528Z digest=sha256:8dfb35526a617047adf99e007845a309347141c4da78dae5b53f81778686ce9a

Observation 3b85cfa2-60aa-49f8-b4c4-0363e3d3c7e8 · inbound

The mass-dependent interplay of active galacitc nuclei and supernova feedback in shaping the $L_{\rm X}$--$T$ relation of early-type galaxies cites this paper.

The mass-dependent interplay of active galacitc nuclei and supernova feedback in shaping the $L_{\rm X}$--$T$ relation of early-type galaxies A new determination of supernova rates and a comparison with indicators for galactic star formation

Reference 29

Resolution
unresolved
no resolver link, observed 2026-08-06T00:06:25.011406Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T00:06:25.011406Z digest=sha256:44b4ccc8310c1665a37d96b88c380c4452d4e74cc0ae4c2d2738047ae22766cf