pith. sign in

arxiv: astro-ph/0612759 · v1 · pith:TKGFSPHKnew · submitted 2006-12-28 · 🌌 astro-ph

A retrospective view of Miriad

R.J. Sault , P.J. Teuben , M.C.H. Wright This is my paper
classification 🌌 astro-ph
keywords miriadanalysisbeguncharacteristicsdatadata-reductiondecisionsdesign
0
0 comments X
read the original abstract

Miriad is a radio interferometry data-reduction package, designed for taking raw data through to the image analysis stage. The Miriad project, begun in 1988, is now middle-aged. With the wisdom of hindsight, we review design decisions and some of Miriad's characteristics.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 6 Pith papers

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

  1. IXPE Polarizations of the Lighthouse Pulsar, Trail, and Filament

    astro-ph.HE 2026-04 unverdicted novelty 7.0

    IXPE detects 55% polarization in the filament with EVPA aligned to the filament axis, implying ordered magnetic field and low turbulence, plus orthogonal X-ray and radio polarization in the trail.

  2. IXPE Polarizations of the Lighthouse Pulsar, Trail, and Filament

    astro-ph.HE 2026-04 accept novelty 7.0

    IXPE detects 55% polarization in the filament with B-field aligned along its axis, orthogonal X-ray and radio polarization in the trail indicating separate lepton populations, and a rotating vector model fit for the pulsar.

  3. SDSSJ110546.07+145202.4: The first long-duration radio changing-look NLS1 galaxy

    astro-ph.HE 2026-04 unverdicted novelty 7.0

    SDSSJ110546.07+145202.4 is the first known long-duration radio changing-look NLS1 galaxy whose outburst is explained by an accretion-rate change that triggered a powerful radio jet.

  4. Sub-kpc scale gas density histograms of the nearby barred spiral galaxy M83: Multi-component molecular gas structure reflecting the galactic environment

    astro-ph.GA 2026-05 unverdicted novelty 5.0

    Molecular gas in M83 consists of two log-normal density components, with the high-density component enhanced along spiral arms and more tightly linked to star formation than the low-density component.

  5. The MeerKAT Fornax Survey VII. Characterisation of the Fornax cluster's magnetic field and new insights on magnetisation in large scale systems

    astro-ph.CO 2026-04 unverdicted novelty 5.0

    Fornax cluster magnetic field follows a power-law spectrum of slope ~2.7 with central strength ~5 μG scaling as n^1.6, consistent with recent central re-amplification and trends across 17 clusters.

  6. Clusters Hiding Under Millimeter Sources (CHUMS) I: Extreme CHUMS

    astro-ph.CO 2026-05 conditional novelty 4.0

    AGN emission from central galaxies hides galaxy clusters in SZ surveys; CARMA-based subtraction recovers high-SNR detections in ACT maps for three specific clusters.