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The 2dF Galaxy Redshift Survey: galaxy luminosity functions per spectral type

Identifieur interne : 000870 ( Main/Curation ); précédent : 000869; suivant : 000871

The 2dF Galaxy Redshift Survey: galaxy luminosity functions per spectral type

Auteurs : Darren S. Madgwick ; Ofer Lahav ; Ivan K. Baldry ; Carlton M. Baugh ; Joss Bland-Hawthorn ; Terry Bridges ; Russell Cannon ; Shaun Cole ; Matthew Colless ; Chris Collins ; Warrick Couch ; Gavin Dalton ; Roberto De Propris ; Simon P. Driver ; George Efstathiou ; Richard S. Ellis ; Carlos S. Frenk ; Karl Glazebrook ; Carole Jackson ; Ian Lewis ; Stuart Lumsden ; Steve Maddox ; Peder Norberg ; John A. Peacock ; Bruce A. Peterson ; Will Sutherland ; Keith Taylor

Source :

RBID : ISTEX:C1169FF42A088114CF688BDF25EBC48D4916F2D4

English descriptors

Abstract

We calculate the optical bJ luminosity function (LF) of the 2dF Galaxy Redshift Survey (2dFGRS) for different subsets defined by their spectral properties. These spectrally selected subsets are defined using a new parameter, η, which is a linear combination of the first two projections derived from a Principal Component Analysis. This parameter η identifies the average emission‐ and absorption‐line strength in the galaxy rest frame spectrum, and hence is a useful indicator of the present star formation. We use a total of 75 000 galaxies in our calculations, chosen from a sample of high signal‐to‐noise ratio, low‐redshift galaxies observed before 2001 January. We find that there is a systematic steepening of the faint‐end slope (α) as one moves from passive (α=‐0.54) to active (α=‐1.50) star‐forming galaxies, and that there is also a corresponding faintening of the rest frame characteristic magnitude M*‐5 log10(h) (from −19.6 to −19.2). We also show that the Schechter function provides a poor fit to the quiescent (Type 1) LF for very faint galaxies [M b J‐5 log10(h) fainter than −16.0], perhaps suggesting the presence of a significant dwarf population. The LFs presented here give a precise confirmation of the trends seen previously in a much smaller preliminary 2dFGRS sample, and in other surveys. We also present a new procedure for determining self‐consistent k‐corrections, and investigate possible fibre‐aperture biases.

Url:
DOI: 10.1046/j.1365-8711.2002.05393.x

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ISTEX:C1169FF42A088114CF688BDF25EBC48D4916F2D4

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Darren S. Madgwick
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Ofer Lahav
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Ivan K. Baldry
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Carlton M. Baugh
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Joss Bland-Hawthorn
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Terry Bridges
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Russell Cannon
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Shaun Cole
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Matthew Colless
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Chris Collins
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Warrick Couch
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Gavin Dalton
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Roberto De Propris
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Simon P. Driver
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George Efstathiou
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Richard S. Ellis
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Carlos S. Frenk
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Karl Glazebrook
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Carole Jackson
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Ian Lewis
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Stuart Lumsden
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Steve Maddox
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Peder Norberg
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Bruce A. Peterson
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Will Sutherland
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Keith Taylor
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<name sortKey="Efstathiou, George" sort="Efstathiou, George" uniqKey="Efstathiou G" first="George" last="Efstathiou">George Efstathiou</name>
<affiliation>
<mods:affiliation>Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA,</mods:affiliation>
<wicri:noCountry code="subField"></wicri:noCountry>
</affiliation>
</author>
<author>
<name sortKey="Ellis, Richard S" sort="Ellis, Richard S" uniqKey="Ellis R" first="Richard S." last="Ellis">Richard S. Ellis</name>
<affiliation>
<mods:affiliation>Department of Astronomy, Caltech, Pasadena, CA 91125, USA,</mods:affiliation>
<wicri:noCountry code="subField"></wicri:noCountry>
</affiliation>
</author>
<author>
<name sortKey="Frenk, Carlos S" sort="Frenk, Carlos S" uniqKey="Frenk C" first="Carlos S." last="Frenk">Carlos S. Frenk</name>
<affiliation>
<mods:affiliation>Department of Physics, South Road, Durham DH1 3LE,</mods:affiliation>
<wicri:noCountry code="subField"></wicri:noCountry>
</affiliation>
</author>
<author>
<name sortKey="Glazebrook, Karl" sort="Glazebrook, Karl" uniqKey="Glazebrook K" first="Karl" last="Glazebrook">Karl Glazebrook</name>
<affiliation>
<mods:affiliation>Department of Physics and Astronomy, Johns Hopkins University, Baltimore, MD 21218‐2686, USA,</mods:affiliation>
<wicri:noCountry code="subField"></wicri:noCountry>
</affiliation>
</author>
<author>
<name sortKey="Jackson, Carole" sort="Jackson, Carole" uniqKey="Jackson C" first="Carole" last="Jackson">Carole Jackson</name>
<affiliation>
<mods:affiliation>Research School of Astronomy and Astrophysics, The Australian National University, Weston Creek, ACT 2611, Australia,</mods:affiliation>
<wicri:noCountry code="subField"></wicri:noCountry>
</affiliation>
</author>
<author>
<name sortKey="Lewis, Ian" sort="Lewis, Ian" uniqKey="Lewis I" first="Ian" last="Lewis">Ian Lewis</name>
<affiliation>
<mods:affiliation>Anglo‐Australian Observatory, PO Box 296, Epping, NSW 2121, Australia,</mods:affiliation>
<wicri:noCountry code="subField"></wicri:noCountry>
</affiliation>
</author>
<author>
<name sortKey="Lumsden, Stuart" sort="Lumsden, Stuart" uniqKey="Lumsden S" first="Stuart" last="Lumsden">Stuart Lumsden</name>
<affiliation>
<mods:affiliation>Department of Physics, University of Leeds, Woodhouse Lane, Leeds LS2 9JT,</mods:affiliation>
<wicri:noCountry code="subField"></wicri:noCountry>
</affiliation>
</author>
<author>
<name sortKey="Maddox, Steve" sort="Maddox, Steve" uniqKey="Maddox S" first="Steve" last="Maddox">Steve Maddox</name>
<affiliation>
<mods:affiliation>School of Physics and Astronomy, University of Nottingham, Nottingham NG7 2RD</mods:affiliation>
<wicri:noCountry code="subField">2RD</wicri:noCountry>
</affiliation>
</author>
<author>
<name sortKey="Norberg, Peder" sort="Norberg, Peder" uniqKey="Norberg P" first="Peder" last="Norberg">Peder Norberg</name>
<affiliation>
<mods:affiliation>Department of Physics, South Road, Durham DH1 3LE,</mods:affiliation>
<wicri:noCountry code="subField"></wicri:noCountry>
</affiliation>
</author>
<author>
<name sortKey="Peacock, John A" sort="Peacock, John A" uniqKey="Peacock J" first="John A." last="Peacock">John A. Peacock</name>
<affiliation>
<mods:affiliation>Institute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ</mods:affiliation>
<wicri:noCountry code="subField">3HJ</wicri:noCountry>
</affiliation>
</author>
<author>
<name sortKey="Peterson, Bruce A" sort="Peterson, Bruce A" uniqKey="Peterson B" first="Bruce A." last="Peterson">Bruce A. Peterson</name>
<affiliation>
<mods:affiliation>Research School of Astronomy and Astrophysics, The Australian National University, Weston Creek, ACT 2611, Australia,</mods:affiliation>
<wicri:noCountry code="subField"></wicri:noCountry>
</affiliation>
</author>
<author>
<name sortKey="Sutherland, Will" sort="Sutherland, Will" uniqKey="Sutherland W" first="Will" last="Sutherland">Will Sutherland</name>
<affiliation>
<mods:affiliation>Institute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ</mods:affiliation>
<wicri:noCountry code="subField">3HJ</wicri:noCountry>
</affiliation>
</author>
<author>
<name sortKey="Taylor, Keith" sort="Taylor, Keith" uniqKey="Taylor K" first="Keith" last="Taylor">Keith Taylor</name>
<affiliation>
<mods:affiliation>Department of Astronomy, Caltech, Pasadena, CA 91125, USA,</mods:affiliation>
<wicri:noCountry code="subField"></wicri:noCountry>
</affiliation>
</author>
</analytic>
<monogr></monogr>
<series>
<title level="j">Monthly Notices of the Royal Astronomical Society</title>
<idno type="ISSN">0035-8711</idno>
<idno type="eISSN">1365-2966</idno>
<imprint>
<publisher>Blackwell Science Ltd</publisher>
<pubPlace>Oxford, UK</pubPlace>
<date type="published" when="2002-06">2002-06</date>
<biblScope unit="volume">333</biblScope>
<biblScope unit="issue">1</biblScope>
<biblScope unit="page" from="133">133</biblScope>
<biblScope unit="page" to="144">144</biblScope>
</imprint>
<idno type="ISSN">0035-8711</idno>
</series>
<idno type="istex">C1169FF42A088114CF688BDF25EBC48D4916F2D4</idno>
<idno type="DOI">10.1046/j.1365-8711.2002.05393.x</idno>
<idno type="ArticleID">MNR5393</idno>
</biblStruct>
</sourceDesc>
<seriesStmt>
<idno type="ISSN">0035-8711</idno>
</seriesStmt>
</fileDesc>
<profileDesc>
<textClass>
<keywords scheme="KwdEn" xml:lang="en">
<term>galaxies: distances and redshifts</term>
<term>galaxies: elliptical and lenticular, cD</term>
<term>galaxies: evolution</term>
<term>galaxies: formation</term>
<term>galaxies: stellar content</term>
</keywords>
</textClass>
<langUsage>
<language ident="en">en</language>
</langUsage>
</profileDesc>
</teiHeader>
<front>
<div type="abstract" xml:lang="en">We calculate the optical bJ luminosity function (LF) of the 2dF Galaxy Redshift Survey (2dFGRS) for different subsets defined by their spectral properties. These spectrally selected subsets are defined using a new parameter, η, which is a linear combination of the first two projections derived from a Principal Component Analysis. This parameter η identifies the average emission‐ and absorption‐line strength in the galaxy rest frame spectrum, and hence is a useful indicator of the present star formation. We use a total of 75 000 galaxies in our calculations, chosen from a sample of high signal‐to‐noise ratio, low‐redshift galaxies observed before 2001 January. We find that there is a systematic steepening of the faint‐end slope (α) as one moves from passive (α=‐0.54) to active (α=‐1.50) star‐forming galaxies, and that there is also a corresponding faintening of the rest frame characteristic magnitude M*‐5 log10(h) (from −19.6 to −19.2). We also show that the Schechter function provides a poor fit to the quiescent (Type 1) LF for very faint galaxies [M b J‐5 log10(h) fainter than −16.0], perhaps suggesting the presence of a significant dwarf population. The LFs presented here give a precise confirmation of the trends seen previously in a much smaller preliminary 2dFGRS sample, and in other surveys. We also present a new procedure for determining self‐consistent k‐corrections, and investigate possible fibre‐aperture biases.</div>
</front>
</TEI>
</record>

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