Pith. sign in

REVIEW 1 cited by

SCORPIO at the 6-m telescope: current state and perspectivies for spectroscopy of galactic and extragalactic objects

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 1106.2020 v2 pith:DC4ZHF7G submitted 2011-06-10 astro-ph.IM astro-ph.COastro-ph.GA

SCORPIO at the 6-m telescope: current state and perspectivies for spectroscopy of galactic and extragalactic objects

V.L. Afanasiev , A.V Moiseev (Special Astrophysical Observatory , Russia) This is my paper
classification astro-ph.IM astro-ph.COastro-ph.GA
keywords observationsscorpiospectroscopytelescopebeencarriedcollectedconsidered
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
0 comments
read the original abstract

A significant part of observations by Russian 6-m telescope is carried out using SCORPIO multi-mode focal reducer. A lot of scientific data have been collected using observations in direct imaging, slit spectroscopy and Fabry-Perot interferometry modes during the past ten years. Some results of these observations are considered in this review. We are also present a short description of a new generation instrument named SCORPIO-2.

discussion (0)

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

Forward citations

Cited by 1 Pith paper

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

  1. 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⊙.