Pith. sign in

REVIEW 1 cited by

Pulsar Science with the SKA

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 1711.01910 v1 pith:MX7YWCUP submitted 2017-11-06 astro-ph.IM

E. F. Keane This is my paper · ORCID
classification astro-ph.IM
keywords pulsarsciencewilladvancesalreadyarraybeamedbriefly
verification ladder T0 review T1 audit T2 compute T3 formal

Signed reviews

No signed human review yet.

0 comments
read the original abstract

The Square Kilometre Array (SKA) will be sensitive enough to discover all of the pulsars in the Milky Way that are beamed towards Earth. Already in the initial deployment, SKA Phase 1, it will make significant advances in pulsar science. In these proceedings I briefly overview what the SKA is, and describe its pulsar search and timing capabilities.

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. A Square Kilometre Array Pulsar Census

    astro-ph.HE 2026-07 conditional novelty 5.5 of 10

    Composite SKA-Low + Mid Band 1/2 all-sky surveys with AA* yield ~10k slow pulsars and ~800 MSPs; AA4 yields ~20% more, rising to ~1300 MSPs if Mid coverage is broadened.

Pith tools