<?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>Multicolour photometry of the cluster of galaxies Sersic 129-01</title>
	<altname type="ADC">J/MNRAS/240/785</altname>
		<altname type="CDS">J/MNRAS/240/785</altname>
		<altname type="brief">Multicolour photometry of Sersic 129-01</altname>
	<reference>
		<source>
<journal>
	<title>Multicolour photometry of the cluster of galaxies Sersic 129-01</title>
	<author>
			<initial>S</initial>
			<initial>J</initial>
			<initial>C</initial>
			<lastName>Millington</lastName></author>
	<author>
			<initial>J</initial>
			<initial>V</initial>
			<lastName>Peach</lastName></author>
	<name>Mon. Not. R. Astron. Soc.</name>
	<volume>240</volume>
	<pageno>785</pageno>
		<date>
			<year>1989</year></date>
	<bibcode>1989MNRAS.240..785M</bibcode></journal></source></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
			<keyword xlink:href="Galaxies_photometry.html">Galaxies, photometry</keyword>
			<keyword xlink:href="Redshifts.html">Redshifts</keyword>
			<keyword xlink:href="Spectra_ultraviolet.html">Spectra, ultraviolet</keyword></keywords>
	<descriptions>
				<description>
				<para>
    We describe photometry of 907 galaxies brighter than b26.25=20.5 in a
    1.83X1.83 area centred on the southern cluster Sersic 129-01 in the u,
    b, r and i bands. The slopes and zero-points of the colour-absolute
    magnitude diagrams agree well with other clusters including Coma and
    the rich cluster Shapley 8 suggesting they are independent of cluster
    environment. The (u-b) against (b-i) diagram distinguishes well
    between morphological types. The reddening we obtain by a number of
    methods disagrees with that of Griersmith (1982). The L-sig relation
    has a similar form to other clusters and when combined with data for
    Virgo leads to a relative distance modulus which agrees with that from
    Griersmith's comparison of colour-magnitude diagrams only on the
    assumption of E (B-V) = 0.15 in front of the cluster and a high value
    of Ho. A mass of 7.4X10 13 Mo is found for the elliptical dominated
    component of the cluster and (M/L)b=59.</para></description>
                        <details/></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="appendix">
	<title>ubri photometry</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>No</name>
			<definition>Identification number</definition>
			<units>---</units></field>
		<field>
			<name>Type</name>
			<definition>'?' for probable galaxies,
                         ';'       when magnitudes could not be measured
                                   due to contamination by stars</definition>
			<units>---</units></field>
		<field>
			<name>RAh</name>
			<definition>Right ascension 1950</definition>
			<units>h</units></field>
		<field>
			<name>RAm</name>
			<definition>Right ascension 1950</definition>
			<units>min</units></field>
		<field>
			<name>RAs</name>
			<definition>Right ascension 1950</definition>
			<units>s</units></field>
		<field>
			<name>DE-</name>
			<definition>Declination 1950 (sign)</definition>
			<units>---</units></field>
		<field>
			<name>DEd</name>
			<definition>Declination 1950</definition>
			<units>deg</units></field>
		<field>
			<name>DEm</name>
			<definition>Declination 1950</definition>
			<units>arcmin</units></field>
		<field>
			<name>DEs</name>
			<definition>Declination 1950</definition>
			<units>arcsec</units></field>
		<field>
			<name>Remark</name>
			<definition>'D' for double, 'E' for est.mag.</definition>
			<units>---</units></field>
		<field>
			<name>Overlap</name>
			<definition>'*' for overlapped image</definition>
			<units>---</units></field>
		<field>
			<name>b26.25</name>
			<definition>b26.25 isophotoal magnitude</definition>
			<units>mag</units></field>
		<field>
			<name>R(b26.25)</name>
			<definition>Effective radius at
                                    26.25 mag/arcsec^2 limiting isophote</definition>
			<units>arcsec</units></field>
		<field>
			<name>b-r</name>
			<definition>(b-r) equal area colour</definition>
			<units>mag</units></field>
		<field>
			<name>R(b-r)</name>
			<definition>Radius of equal area colour</definition>
			<units>arcsec</units></field>
		<field>
			<name>u-b</name>
			<definition>(u-b) equal area colour</definition>
			<units>mag</units></field>
		<field>
			<name>R(u-b)</name>
			<definition>Radius of equal area colour</definition>
			<units>arcsec</units></field>
		<field>
			<name>b-i</name>
			<definition>(b-i) equal area colour</definition>
			<units>mag</units></field>
		<field>
			<name>R(b-i)</name>
			<definition>Radius of equal area colour</definition>
			<units>arcsec</units></field></fields></tableHead>
	
	<history>
		<ingest>
	
			<creator>
				<lastName>Francois Ochsenbein</lastName>
				<affiliation>CDS</affiliation></creator>
	<date>
		<year>1993</year><month>Jan</month><day>05</day></date></ingest>
		</history>
	<identifier>J_MNRAS_240_785.xml</identifier></dataset>
