<?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>Global mapping B-band photometry of a complete sample of Fornax and Virgo
early-type galaxies</title>
	<altname type="ADC">J/A+AS/106/199</altname>
		<altname type="CDS">J/A+AS/106/199</altname>
		<altname type="brief">'Global mapping' B-band photometry of a complete</altname>
	<reference>
		<source>
<journal>
	<title>Global mapping B-band photometry of a complete sample of Fornax and Virgo
early-type galaxies</title>
	<author>
			<initial>N</initial>
			<lastName>Caon</lastName></author>
	<author>
			<initial>M</initial>
			<lastName>Capaccioli</lastName></author>
	<author>
			<initial>M</initial>
			<lastName>D'Onofrio</lastName></author>
	<name>Astron. Astrophys. Suppl. Ser.</name>
	<volume>106</volume>
	<pageno>199</pageno>
		<date>
			<year>1994</year></date>
	<bibcode>1994A&amp;AS..106..199C</bibcode></journal></source></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/apj_keywords.html">
			<keyword xlink:href="galaxies_fundamental_parameters.html">galaxies: fundamental parameters</keyword>
			<keyword xlink:href="galaxies_elliptical_and_lenticular_cD.html">galaxies: elliptical and lenticular, cD</keyword>
			<keyword xlink:href="photometry.html">photometry</keyword></keywords>
	<descriptions>
				<abstract>
					<para>
   We present the B-band surface photometry of 19 early-type galaxies of the
   Virgo cluster, and of 28 galaxies of the same morphological type belonging
   to the Fornax clusters, obtained through the 'global mapping' technique
   which couples CCD and photographic plates. Taking into account 33 galaxies
   already studied by Caon et al. (1990) with the same methodology, the Virgo
   sample of early-type galaxies is now 80% complete down to B_T_=14. The
   Fornax sample is 95% complete down to B_T_=15. The geometric and
   photometric properties of the total sample of 80 galaxies are derived
   measuring accurate light profiles, ellipticities, position angles and
   Fourier coefficients of the isophotes. The main sources of errors of the
   'global mapping' procedure are reviewed and the effects of seeing discussed.
   Global galaxian parameters such as total luminosity, effective radius, and
   effective surface brightness, are computed for the whole sample in a
   homogeneous way. Our goal is to create an unbiased set of data to be used
   for investigating the process of galaxy formation and evolution.</para></abstract>
                        <details/></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="tablea">
	<title>B-band photometry</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Name</name>
			<definition>Object name</definition>
			<units>---</units></field>
		<field>
			<name>D^1/4</name>
			<definition>Distance at power 1/4 from center</definition>
			<units>arcsec</units></field>
		<field>
			<name>B(maj)</name>
			<definition>Surface brightness along the major
                                           axis (folded)</definition>
			<units>mag/arcsec2</units></field>
		<field>
			<name>B(min)</name>
			<definition>Surface brightness along the minor
                                           axis (folded)</definition>
			<units>mag/arcsec2</units></field>
		<field>
			<name>Eps</name>
			<definition>Ellipticity</definition>
			<units>---</units></field>
		<field>
			<name>PA</name>
			<definition>Position angle</definition>
			<units>deg</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="tableb">
	<title>B-band photometry</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Name</name>
			<definition>Object name</definition>
			<units>---</units></field>
		<field>
			<name>D^1/4</name>
			<definition>Distance at power 1/4 from center</definition>
			<units>arcsec</units></field>
		<field>
			<name>B(maj)SW</name>
			<definition>Surface brightness along the major axis
                                          (side as coded)</definition>
			<units>mag/arcsec2</units></field>
		<field>
			<name>B(maj)NE</name>
			<definition>Surface brightness along the major axis
                                          (side as coded)</definition>
			<units>mag/arcsec2</units></field>
		<field>
			<name>B(min)SE</name>
			<definition>Surface brightness along the minor axis
                                          (side as coded)</definition>
			<units>mag/arcsec2</units></field>
		<field>
			<name>B(min)NW</name>
			<definition>Surface brightness along the minor axis
                                          (side as coded)</definition>
			<units>mag/arcsec2</units></field>
		<field>
			<name>Eps</name>
			<definition>Ellipticity</definition>
			<units>---</units></field>
		<field>
			<name>PA</name>
			<definition>Position angle
                                           (measured from N through E)</definition>
			<units>deg</units></field></fields></tableHead>
	
	<history>
		<ingest>
	
			<creator>
				<lastName>Patricia Bauer</lastName>
				<affiliation>CDS</affiliation></creator>
	<date>
		<year>1994</year><month>Mar</month><day>21</day></date></ingest>
		</history>
	<identifier>J_A+AS_106_199.xml</identifier></dataset>
