Pith. sign in

REVIEW 1 cited by

The Southern Wide-field Gamma-ray Observatory

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 2309.04577 v1 pith:43EMQPIL submitted 2023-09-08 hep-ex astro-ph.HE

Ruben Conceição (for the SWGO collaboration) This is my paper · ORCID
classification hep-exastro-ph.HE
keywords observatorysoutherndetectorsgammagamma-rayhemisphereprojectrays
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

The Southern Wide-field Gamma-ray Observatory (SWGO) is an R&D project to plan and design the next observatory to detect gamma rays in the Southern hemisphere. The experiment, planned to be placed at an altitude greater than 4400 m, is primarily based on water Cherenkov detectors units and is expected to measure gamma rays from a few hundred GeV up to the PeV scale. SWGO will complement CTA and the existing ground-based particle detectors of the Northern Hemisphere, namely HAWC and LHAASO, having a rich science programme. The collaboration is highly invested in evaluating different detector and array configurations, prototyping, and site search. In this presentation, I shall present an overview of the project's activities, achievements and future plans.

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. Constraints on Ultra-heavy DM from TeV-PeV gamma-ray diffuse measurements

    astro-ph.HE 2025-09 conditional novelty 5.0 of 10

    HAWC and LHAASO diffuse gamma-ray data, modeled with prompt, inverse-Compton, absorption, and astrophysical background, produce the strongest constraints on decaying ultra-heavy dark matter above ~100 TeV.

Pith tools