Low surface brightness galaxies in the local universe. II. Selection effects and completeness of the automated plate measuring 1 survey

D. Sprayberry; C. D. Impey; M. J. Irwin

doi:10.1086/177268

Low surface brightness galaxies in the local universe. II. Selection effects and completeness of the automated plate measuring 1 survey

D. Sprayberry, C. D. Impey, M. J. Irwin

Astronomy

Research output: Contribution to journal › Article › peer-review

27 Scopus citations

Abstract

We discuss the techniques employed for identifying low surface brightness galaxies for the Automated Plate Measuring (APM) survey. We present the method of calibrating the photometry performed from the APM scans and discuss the uncertainties associated with the calibrations. We also review the possible sources of incompleteness in the survey, and we present the results of a program of simulations to estimate the completeness as a function of galaxy parameters. Finally, we discuss the implications of the survey results and show, in particular, that the observed distribution of central surface brightnesses among all galaxies in one survey field is almost flat for μ_B(0) ≥ 23 mag arcsec^-2.

Original language	English (US)
Pages (from-to)	535-542
Number of pages	8
Journal	Astrophysical Journal
Volume	463
Issue number	2 PART I
DOIs	https://doi.org/10.1086/177268
State	Published - 1996

Keywords

Galaxies: photometry
Methods: data analysis
Surveys

ASJC Scopus subject areas

Astronomy and Astrophysics
Space and Planetary Science

Access to Document

10.1086/177268

Cite this

@article{87f3bc98e7a34b14a81042e6174d9844,

title = "Low surface brightness galaxies in the local universe. II. Selection effects and completeness of the automated plate measuring 1 survey",

abstract = "We discuss the techniques employed for identifying low surface brightness galaxies for the Automated Plate Measuring (APM) survey. We present the method of calibrating the photometry performed from the APM scans and discuss the uncertainties associated with the calibrations. We also review the possible sources of incompleteness in the survey, and we present the results of a program of simulations to estimate the completeness as a function of galaxy parameters. Finally, we discuss the implications of the survey results and show, in particular, that the observed distribution of central surface brightnesses among all galaxies in one survey field is almost flat for μB(0) ≥ 23 mag arcsec-2.",

keywords = "Galaxies: photometry, Methods: data analysis, Surveys",

author = "D. Sprayberry and Impey, {C. D.} and Irwin, {M. J.}",

year = "1996",

doi = "10.1086/177268",

language = "English (US)",

volume = "463",

pages = "535--542",

journal = "Astrophysical Journal",

issn = "0004-637X",

publisher = "IOP Publishing Ltd.",

number = "2 PART I",

}

TY - JOUR

T1 - Low surface brightness galaxies in the local universe. II. Selection effects and completeness of the automated plate measuring 1 survey

AU - Sprayberry, D.

AU - Impey, C. D.

AU - Irwin, M. J.

PY - 1996

Y1 - 1996

N2 - We discuss the techniques employed for identifying low surface brightness galaxies for the Automated Plate Measuring (APM) survey. We present the method of calibrating the photometry performed from the APM scans and discuss the uncertainties associated with the calibrations. We also review the possible sources of incompleteness in the survey, and we present the results of a program of simulations to estimate the completeness as a function of galaxy parameters. Finally, we discuss the implications of the survey results and show, in particular, that the observed distribution of central surface brightnesses among all galaxies in one survey field is almost flat for μB(0) ≥ 23 mag arcsec-2.

AB - We discuss the techniques employed for identifying low surface brightness galaxies for the Automated Plate Measuring (APM) survey. We present the method of calibrating the photometry performed from the APM scans and discuss the uncertainties associated with the calibrations. We also review the possible sources of incompleteness in the survey, and we present the results of a program of simulations to estimate the completeness as a function of galaxy parameters. Finally, we discuss the implications of the survey results and show, in particular, that the observed distribution of central surface brightnesses among all galaxies in one survey field is almost flat for μB(0) ≥ 23 mag arcsec-2.

KW - Galaxies: photometry

KW - Methods: data analysis

KW - Surveys

UR - http://www.scopus.com/inward/record.url?scp=21344470997&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=21344470997&partnerID=8YFLogxK

U2 - 10.1086/177268

DO - 10.1086/177268

M3 - Article

AN - SCOPUS:21344470997

SN - 0004-637X

VL - 463

SP - 535

EP - 542

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 2 PART I

ER -

Low surface brightness galaxies in the local universe. II. Selection effects and completeness of the automated plate measuring 1 survey

Abstract

Keywords

ASJC Scopus subject areas

Access to Document

Other files and links

Fingerprint

Cite this