Student or educator? Sign up with your school email and get 6 months of Pro free.
Cited by 584

The DOI matches its Crossref record.

A standard stellar spectral sequence in the red/near-infrared - Classes K5 to M9

Kirkpatrick, J. D., Henry, Todd J., McCarthy, Donald W., Jr.·1991·The Astrophysical Journal Supplement Series

Abstract

Spectra of 39 K and M dwarf spectroscopic standards, as well as 38 secondary standards, are shown from 6300 to 9000 A. This sequence of 77 spectra ranges from K5 V to M9 and has been classified on the Boeshaar system. Spectra of 14 giant and higher luminosity star are presented from 6900 to 9000 A, along with two miscellaneous spectra. Also given is an extensive list of atomic and molecular features found in the spectra of late K and M stars of all luminosity classes. From the spectral slopes and the strengths of the red/near-infrared spectral features it is possible to distinguish giants from dwarfs and to classify M dwarfs of all spectral subclasses. The library of spectra has been used to construct a spectral class versus mass relation which allows mass estimates to be made based upon a dwarf's spectral class alone. The relation is based on eight objects having both well-determined masses and spectral types.

Overview

The claims and statistics of this paper haven’t been checked yet.

Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.

A few free checks a day · papers already verified open instantly · results are public

Integrity signals

Registry

Crossref · 10.1086/191611

Cites

Statistics

Verification

Claims the paper makes

The claims and statistics of this paper haven’t been checked yet.

Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.

A few free checks a day · papers already verified open instantly · results are public

Self-check

Percentages, sums and reported differences re-computed from the paper’s own numbers.

The self-check needs the paper’s full text.

Citations

Cited by

See all 584

Metadata

Authors
Kirkpatrick, J. D., Henry, T. J., & McCarthy, D. W., Jr.
Venue
The Astrophysical Journal Supplement Series
Published
1991-11
Volume
77
Pages
417
ISSN
  • 0067-0049 (ISSN-L)
  • 1538-4365
OpenAlex
W1970076709
Cited by
584
References
0
Type
conference abstract
Language
en
Open access
closed

About these checks

Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.

Statistics and arithmetic are recomputed, not judged.

Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.

What counts as a claim ›How we measure confidence ›How we check this ›

Are you an author, or do you see a problem with this page? Request a review

How to cite

Cite CoChat for the checks on this page, and the paper for its own findings.

This page
CoChat. (2026). Citation check: A standard stellar spectral sequence in the red/near-infrared - Classes K5 to M9. https://app.cochat.ai/papers/10.1086/191611
The paper
Kirkpatrick, J. D., Henry, T. J., & McCarthy, D. W., Jr. (1991). A standard stellar spectral sequence in the red/near-infrared - Classes K5 to M9. The Astrophysical Journal Supplement Series. https://doi.org/10.1086/191611

Data sources

Bibliographic data: Semantic Scholar, OpenAlex, Crossref.

Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.