Pith. sign in

REVIEW 1 cited by

Measuring the Evolution of the NuSTAR Detector Gains

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 2206.04058 v3 pith:Y7ZHIXHP submitted 2022-06-08 astro-ph.IM astro-ph.HE

Brian Grefenstette , Murray Brightman , Hannah P. Earnshaw , Karl Forster , Kristin K. Madsen , Hiromasa Miyasaka This is my paper · ORCID
classification astro-ph.IMastro-ph.HE
keywords gainnustaranalysiscaldbdetectorsdocumentbuildscalibration
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

The memo describes the methods used to track the long-term gain variations in the NuSTAR detectors. It builds on the analysis presented in Madsen et al. (2015) using the deployable calibration source to measure the gain drift in the NuSTAR CdZnTe detectors. This is intended to be a live document that is periodically updated as new entries are required in the NuSTAR gain CALDB files. This document covers analysis up through late-2024 and the gain v011 CALDB file released in version 20240226.

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. Resolving SLX 1744-299 and SLX 1744-300 in the hard X-ray band: implications for their ultracompact nature

    astro-ph.HE 2026-06 unverdicted novelty 6.0 of 10

    NuSTAR resolves SLX 1744-299 and SLX 1744-300 in hard X-rays, yielding low luminosities that favor ultracompact orbital periods below 90-155 min via disc instability model comparison.

Pith tools