Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Constraining the Low-Mass Slope of the Star Formation Sequence at 0.5<z<2.5
As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:1407.1843.
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 2026-07-12T01:44:24.704352Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-10T17:27:26.011828Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
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- 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 9da4c007-0c81-4acc-b927-fc3c13c9c0d2 · inbound
Spider-Webb: enhanced star formation in low-mass galaxies within the Spiderweb protocluster revealed by JWST Pa$\beta$ narrow-band imaging cites this paper.
Spider-Webb: enhanced star formation in low-mass galaxies within the Spiderweb protocluster revealed by JWST Pa$\beta$ narrow-band imaging Constraining the Low-Mass Slope of the Star Formation Sequence at 0.5<z<2.5
Reference 28
- Resolution
- verified exact
- local_arxiv, observed 2026-05-21T04:43:58.020478Z
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 10e6cf13-8217-4a00-b228-b0a8a2ea56bd · inbound
Can current models predict the local black hole merger rate? cites this paper.
Can current models predict the local black hole merger rate? Constraining the Low-Mass Slope of the Star Formation Sequence at 0.5<z<2.5
Reference 286
- Resolution
- verified exact
- local_arxiv, observed 2026-06-28T13:02:10.525032Z
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 33bbbdee-a5e5-4774-b879-1e6109ab7d28 · inbound
MSA-3D: Rotation Curves and Dark Matter Fractions at z~0.5-1.7 with JWST/NIRSpec cites this paper.
MSA-3D: Rotation Curves and Dark Matter Fractions at z~0.5-1.7 with JWST/NIRSpec Constraining the Low-Mass Slope of the Star Formation Sequence at 0.5<z<2.5
Reference 20
- Resolution
- verified exact
- local_arxiv, observed 2026-06-29T04:03:05.616670Z
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 3b880d5d-f8b9-4240-b009-21f1e0dfea55 · inbound
A MIGHTEE robust measurement of the star formation rate-radio correlation cites this paper.
A MIGHTEE robust measurement of the star formation rate-radio correlation Constraining the Low-Mass Slope of the Star Formation Sequence at 0.5<z<2.5
Reference 3
- Resolution
- unresolved
- no resolver link, observed 2026-07-12T01:44:24.704352Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 0a5eb498-f928-42fd-b28e-2c2f4c9bc09b · inbound
Compact Objects Merging with Stars as an Origin of Ultra-Long Gamma-Ray Bursts and Luminous Fast Blue Optical Transients cites this paper.
Compact Objects Merging with Stars as an Origin of Ultra-Long Gamma-Ray Bursts and Luminous Fast Blue Optical Transients Constraining the Low-Mass Slope of the Star Formation Sequence at 0.5<z<2.5
Reference 223
- Resolution
- verified exact
- local_arxiv, observed 2026-07-10T17:27:26.013477Z
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.