Pith. sign in

REVIEW 3 cited by

Cosmicflows-3: Two Distance-Velocity Calculators

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 1912.07214 v1 pith:4ASB3OZ3 submitted 2019-12-16 astro-ph.CO astro-ph.GAastro-ph.IM

Cosmicflows-3: Two Distance-Velocity Calculators

Ehsan Kourkchi , Helene M. Courtois , Romain Graziani , Yehuda Hoffman , Daniel Pomarede , Edward J. Shaya , R. Brent Tully This is my paper
classification astro-ph.CO astro-ph.GAastro-ph.IM
keywords distancevelocitycalculatorscosmicflowscosmicflows-3databasederiveddistances
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
0 comments
read the original abstract

Tools are provided at the Extragalactic Distance Database website that provide relationships between the distances and velocities of galaxies based on smoothed versions of the velocity fields derived by the Cosmicflows program.

discussion (0)

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

Forward citations

Cited by 3 Pith papers

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

  1. Exploring the synergies of $[\mathrm{O\,II}]\lambda 3727$ with MUSE spectroscopy in PHANGS H II regions

    astro-ph.GA 2026-07 accept novelty 5.5

    Adding SITELLE [O II] to PHANGS-MUSE for 556 H II regions recovers known metallicity-calibration offsets, shows <0.03–0.04 dex gradient scatter for many methods, and favors [S III]/[S II] as a robust ionization tracer.

  2. New optical velocities for local galaxy candidates

    astro-ph.GA 2026-07 accept novelty 5.0

    BTA optical velocities confirm 12 new Local Volume companions (including satellites of DDO 46, NGC 2903, NGC 4826) and yield NGC 1068 group mass (2.6 ± 1.0) × 10^12 M⊙.

  3. Exploring the synergies of $[\mathrm{O\,II}]\lambda 3727$ with MUSE spectroscopy in PHANGS H II regions

    astro-ph.GA 2026-07 unverdicted novelty 5.0

    Combining [O II] doublet data with MUSE spectra creates a homogeneous H II region catalog and compares strong-line metallicity calibrations, showing low scatter in radial gradients and [S III]/[S II] as a robust ioniz...