Pith. sign in

REVIEW 1 cited by

Supermassive black holes from OASIS and SAURON integral-field kinematics

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 0709.2861 v1 pith:B66XCIQ4 submitted 2007-09-18 astro-ph

M. Cappellari , R. Bacon , R. L. Davies , P. T. de Zeeuw , E. Emsellem , J. Falcon-Barroso , D. Krajnovic , H. Kuntschner
show 5 more authors
R. M. McDermid R. F. Peletier M. Sarzi R. C. E. van den Bosch G. van de Ven
This is my paper
classification astro-ph
keywords blackholesintegral-fieldoasissupermassiveaccumulatedactivecurrent
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

Supermassive black holes are a key element in our understanding of how galaxies form. Most of the progress in this very active field of research is based on just ~30 determinations of black hole mass, accumulated over the past decade. We illustrate how integral-field spectroscopy, and in particular our OASIS modeling effort, can help improve the current situation.

Discussion (0). Sign in to comment.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. OpenAlex reports about 7 citations worldwide. Full citation record

  1. The Impact of Non-Gaussian Line Spread Functions on Stellar Kinematic Recovery: Consequences for Dynamical Models

    astro-ph.GA 2026-06 unverdicted novelty 5.0 of 10

    Non-Gaussian LSF shapes bias kinematic extraction from spectra; matching the LSF of templates to the target reduces dispersion bias below 1%.

Pith tools