<?xml version="1.0" encoding="UTF-8"?>
<!DOCTYPE dataset SYSTEM "http://tarantella.gsfc.nasa.gov/xml/dataset_048.dtd">
<dataset subject="astronomy" xmlns:xlink="http://www.w3.org/XML/XLink/0.9">
	<title>Galaxy populations in the distant galaxy clusters.
I. Cl0939+472 (z=0.41) and Cl0016+161 (z=0.54). I.</title>
	<altname type="ADC">J/A+AS/118/65</altname>
		<altname type="CDS">J/A+AS/118/65</altname>
		<altname type="brief">BRI &amp; redshifts in Cl0939+472 &amp; Cl0016+161</altname>
	<reference>
		<source>
<journal>
	<title>Galaxy populations in the distant galaxy clusters.
I. Cl0939+472 (z=0.41) and Cl0016+161 (z=0.54). I.</title>
	<author>
			<initial>P</initial>
			<lastName>Belloni</lastName></author>
	<author>
			<initial>H</initial>
			<initial>-J</initial>
			<lastName>Roeser</lastName></author>
	<name>Astron. Astrophys. Suppl. Ser.</name>
	<volume>118</volume>
	<pageno>65</pageno>
		<date>
			<year>1996</year></date>
	<bibcode>1996A&amp;AS..118...65B</bibcode></journal></source></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
			<keyword xlink:href="Clusters_galaxy.html">Clusters, galaxy</keyword>
			<keyword xlink:href="Redshifts.html">Redshifts</keyword></keywords>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/apj_keywords.html">
			<keyword xlink:href="galaxies_clusters_general.html">galaxies: clusters: general</keyword>
			<keyword xlink:href="galaxies_clusters_individual_(Cl_0939+479_CI_0016+161).html">galaxies: clusters: individual (Cl 0939+479, CI 0016+161)</keyword>
			<keyword xlink:href="galaxies_distances_and_redshifts.html">galaxies: distances and redshifts</keyword>
			<keyword xlink:href="galaxies_evolution.html">galaxies: evolution</keyword></keywords>
	<descriptions>
				<abstract>
					<para>
    We present results of a study of the galaxy population of Cl 0939+472
    (z=0.41) and Cl 0016+161 (z=0.54). We have used narrow-band filters
    (FWHM=~90-200A) and broad band B, R, I filters covering the range from
    3800A to 9200A obtain low resolution spectra for all galaxies brighter
    than R=22.5mag in a 5'x5' (Cl 0939+472) and a 3.5'x5' (Cl 0016+161)
    field. Template spectra for classical Hubble type and E+A galaxies
    were fitted to the low-resolution spectral energy distribution in
    order to determine the galaxies' redshift and the morphological type.
    We detected 160 cluster members in Cl 0939+472 and 100 in Cl 0016+161,
    with a success rate of about 80% in the determination of redshifts and
    corresponding classification of morphological types from spectral
    energy distributions. These results constitute a statistical
    improvement of at least a factor of 4 over the most complete study to
    date of these clusters. In particular, we provide a large sample of
    elliptical galaxies with secure membership, well suited for a study of
    evolutionary effects. The same E+A templates developed for the
    analysis of Cl 0939+472 were successful in recognizing almost all of
    the spectroscopically already known E+A galaxies in Cl 0016+161 and in
    identifying 10 new ones. Our results show that in this cluster, too,
    the fraction of E+A galaxies represents about 20% of the total galaxy
    population. This outlines the importance of taking into account
    galaxies with signs of recent star formation for a correct evaluation
    of the Butcher-Oemler effect in distant galaxy clusters.</para></abstract>
                        <details>
	<astroObjects>
		
			<astroObject><name>Cl 0939+479</name><name>ACO 851</name><position><ra>09 42.8 </ra><dec>+47 00 </dec></position></astroObject>
			<astroObject><name>Cl 0016+161</name><position><ra>00 18.5 </ra><dec>+16 26 </dec></position></astroObject></astroObjects></details></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table4">
	<title>Data of 323 objects with R>22.5mag in
                              Cl 10939+47 field</title></tableLink>
				<tableLink xlink:href="table5">
	<title>Data of 200 objects with R>22.5mag in
                              Cl 10016+161 field</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>No</name>
			<definition>Sequence number</definition>
			<units>---</units></field>
		<field>
			<name>Xpos</name>
			<definition>X coordinate</definition>
			<units>arcsec</units></field>
		<field>
			<name>Ypos</name>
			<definition>Y coordinate</definition>
			<units>arcsec</units></field>
		<field>
			<name>Rmag</name>
			<definition>R magnitude</definition>
			<units>mag</units></field>
		<field>
			<name>B-R</name>
			<definition>B-R color</definition>
			<units>mag</units></field>
		<field>
			<name>n_B-R</name>
			<definition>Note no B-R
	<footnote footnoteId="???"><para>number=1</para>
			<para>An '?' indicates objects that could not be fitted by any of the
           templates at any redshift between z=0.3 and z=0.7
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>B-I</name>
			<definition>B-I color</definition>
			<units>mag</units></field>
		<field>
			<name>n_B-I</name>
			<definition>Note no B-I
	<footnote footnoteId="???"><para>number=1</para>
			<para>An '?' indicates objects that could not be fitted by any of the
           templates at any redshift between z=0.3 and z=0.7
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>D4000</name>
			<definition>4000A-break index</definition>
			<units>---</units></field>
		<field>
			<name>zD92</name>
			<definition>Redshitf from Dressler &amp; Gunn, 1992</definition>
			<units>---</units></field>
		<field>
			<name>z</name>
			<definition>Redshift</definition>
			<units>---</units></field>
		<field>
			<name>n_z</name>
			<definition>Note on z, s = star
	<footnote footnoteId="???"><para>number=1</para>
			<para>An '?' indicates objects that could not be fitted by any of the
           templates at any redshift between z=0.3 and z=0.7
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>e_z</name>
			<definition>rms uncertainty on z</definition>
			<units>---</units></field>
		<field>
			<name>n_e_z</name>
			<definition>Note on e_z
	<footnote footnoteId="???"><para>number=1</para>
			<para>An '?' indicates objects that could not be fitted by any of the
           templates at any redshift between z=0.3 and z=0.7
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>MType</name>
			<definition>Morphological type</definition>
			<units>---</units></field></fields></tableHead>
	
	<history>
		<ingest>
	
			<creator>
				<lastName>Patricia Bauer</lastName>
				<affiliation>CDS</affiliation></creator>
	<date>
		<year>1996</year><month>Apr</month><day>12</day></date><acknowledgement>Paola Belloni &lt;belloni@usm.uni-muenchen.de></acknowledgement></ingest>
		</history>
	<identifier>J_A+AS_118_65.xml</identifier></dataset>
