<?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>The Hamburg/SAO Survey for Emission-Line Galaxies.
I. A First List of 70 Galaxies.</title>
	<altname type="ADC">J/A+AS/135/511</altname>
		<altname type="CDS">J/A+AS/135/511</altname>
		<altname type="brief">The Hamburg/SAO Survey for ELGs</altname>
	<reference>
		<source>
<journal>
	<title>The Hamburg/SAO Survey for Emission-Line Galaxies.
I. A First List of 70 Galaxies.</title>
	<author>
			<initial>A</initial>
			<initial>V</initial>
			<lastName>Ugryumov</lastName></author>
	<author>
			<initial>D</initial>
			<lastName>Engels</lastName></author>
	<author>
			<initial>V</initial>
			<initial>A</initial>
			<lastName>Lipovetsky</lastName></author>
	<author>
			<initial>H</initial>
			<initial>-J</initial>
			<lastName>Hagen</lastName></author>
	<author>
			<initial>U</initial>
			<lastName>Hopp</lastName></author>
	<author>
			<initial>S</initial>
			<initial>A</initial>
			<lastName>Pustilnik</lastName></author>
	<author>
			<initial>A</initial>
			<initial>Yu</initial>
			<lastName>Kniazev</lastName></author>
	<author>
			<initial>G</initial>
			<lastName>Richter</lastName></author>
	<author>
			<initial>Yu</initial>
			<initial>I</initial>
			<lastName>Izotov</lastName></author>
	<author>
			<initial>C</initial>
			<initial>C</initial>
			<lastName>Popescu</lastName></author>
	<name>Astron. Astrophys. Suppl. Ser.</name>
	<volume>135</volume>
	<pageno>511</pageno>
		<date>
			<year>1999</year></date>
	<bibcode>1999A&amp;AS..135..511U</bibcode></journal></source>
	<related>
			<holding role="similar">J/MNRAS/246/433 :  CCD photometry + APM parameters for galaxies (Maddox+ 1990)<xlink:simple href="J/MNRAS/246/433"/></holding>
			<holding role="similar">J/A+AS/115/235 :  The Hamburg/ESO survey for bright QSOs. II. (Reimers+, 1996)<xlink:simple href="J/A+AS/115/235"/></holding>
			<holding role="similar">J/A+AS/128/507 :  The Hamburg Quasar Survey. II. (Engels+ 1998)<xlink:simple href="J/A+AS/128/507"/></holding></related></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
			<keyword xlink:href="Galaxies_spectra.html">Galaxies, spectra</keyword>
			<keyword xlink:href="Magnitudes.html">Magnitudes</keyword>
			<keyword xlink:href="Radial_velocities.html">Radial velocities</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_compact.html">galaxies: compact</keyword>
			<keyword xlink:href="galaxies_distances_and_redshifts.html">galaxies: distances and redshifts</keyword>
			<keyword xlink:href="galaxies_fundamental_parameters.html">galaxies: fundamental parameters</keyword>
			<keyword xlink:href="galaxies_starburst.html">galaxies: starburst</keyword>
			<keyword xlink:href="surveys.html">surveys</keyword></keywords>
	<descriptions>
				<description>
				<para>
    We present first results of the Hamburg/SAO Survey for Emission-Line
    Galaxies (HSS therein, SAO - Special Astrophysical Observatory,
    Russia) which is based on the digitized objective-prism photoplates
    database of the Hamburg Quasar Survey (HQS). The main goal of this
    survey is the search for emission-line galaxies (ELG) in order to
    create a new deep sample of blue compact galaxies (BCG) in a large sky
    area. Another important goal of this work is to search for new
    extremely low-metallicity galaxies. We present the first results of
    spectroscopy obtained with the 2.2m telescope at the German-Spanish
    Observatory at Calar Alto, and with the 6m telescope at the Russian
    Special Astrophysical Observatory. The primary ELG candidate selection
    criteria applied were a blue continuum (near 4000{AA}) and the
    presence of emission lines close to 5000A recognized on digitized
    prism spectra of galaxies with magnitudes in the range B =16.0-19.5.
    The spectroscopy resulted in the detection or/and quantitative
    spectral classification of 74 emission-line objects. Of them 55 are
    newly discovered, and 19 were already known as galaxies before. 11 of
    the latter have redshifts and are known ELGs. For most of the known
    galaxies emission line ratios were measured for the first time and an
    improved classification is presented. 47 objects are classified as
    BCGs, one as Sy2 galaxy, six as probable LINERs, and four as new QSOs.
    The remaining galaxies do not show significant H{beta} and
    [OIII]4959,5007{AA} emission lines, and are likely either
    low-ionization starburst or dwarf amorphous nuclear starburst
    galaxies.</para></description>
                        <details/></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table1.dat">
	<title>Coordinates, velocities, magnitudes and
                              classification of emission-line galaxies</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Name</name>
			<definition>Name of objects</definition>
			<units>---</units></field>
		<field>
			<name>RAh</name>
			<definition>Right ascension (B1950)</definition>
			<units>h</units></field>
		<field>
			<name>RAm</name>
			<definition>Right ascension (B1950)</definition>
			<units>min</units></field>
		<field>
			<name>RAs</name>
			<definition>Right ascension (B1950)</definition>
			<units>s</units></field>
		<field>
			<name>DE-</name>
			<definition>Declination sign</definition>
			<units>---</units></field>
		<field>
			<name>DEd</name>
			<definition>Declination (B1950)</definition>
			<units>deg</units></field>
		<field>
			<name>DEm</name>
			<definition>Declination (B1950)</definition>
			<units>arcmin</units></field>
		<field>
			<name>DEs</name>
			<definition>Declination (B1950)</definition>
			<units>arcsec</units></field>
		<field>
			<name>HRV</name>
			<definition>Heliocentric radial velocity</definition>
			<units>km/s</units></field>
		<field>
			<name>n_Bmag</name>
			<definition>*:  Magnitudes are taken from the APM,
                                   Maddox et al., Cat. &lt;J/MNRAS/246/433></definition>
			<units>---</units></field>
		<field>
			<name>Bmag</name>
			<definition>Magnitude in B filter</definition>
			<units>mag</units></field>
		<field>
			<name>BMAG</name>
			<definition>Absolute B-magnitude</definition>
			<units>mag</units></field>
		<field>
			<name>Type</name>
			<definition>Classification
	<footnote footnoteId="???"><para>number=1</para>
			<para>Only rough classification were done due to low S/N spectra.
          Spectral classification follows Salzer et al., 1989ApJS...70..479S
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>Names</name>
			<definition>Other names from NED</definition>
			<units>---</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table2.dat">
	<title>Parameters of emission lines of galaxies</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Obs</name>
			<definition>Note on observation
	<footnote footnoteId="???"><para>number=1</para>
			<para>*: Objects observed with the IPSC (6m telescope)
         **: Objects observed with the CCD (2.2m telescope) under poor
              photometric conditions
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>Name</name>
			<definition>Name of objects</definition>
			<units>---</units></field>
		<field>
			<name>FHb</name>
			<definition>H{beta}4861{AA} emission line observed
                                          flux</definition>
			<units>10-19W/m2</units></field>
		<field>
			<name>F[OII]/Hb</name>
			<definition>[OII]3727{AA}/Hb emission line
                                            fluxes ratio</definition>
			<units>---</units></field>
		<field>
			<name>F[OII]</name>
			<definition>[OII]3727A emission line observed flux</definition>
			<units>10-19W/m2</units></field>
		<field>
			<name>F[OIII]/Hb</name>
			<definition>[OIII]5007{AA}/Hb emission line
                                          fluxes ratio</definition>
			<units>---</units></field>
		<field>
			<name>F[OIII]</name>
			<definition>[OIII]5007A emission line observed flux</definition>
			<units>10-19W/m2</units></field>
		<field>
			<name>FHa/Hb</name>
			<definition>Emission line fluxes ratio Ha/Hb</definition>
			<units>---</units></field>
		<field>
			<name>FHa</name>
			<definition>H{alpha} emission line observed flux</definition>
			<units>10-19W/m2</units></field>
		<field>
			<name>F[NII]/Ha</name>
			<definition>[NII]6583{AA}/Ha emission line
                                          fluxes ratio</definition>
			<units>---</units></field>
		<field>
			<name>F[SII]/Ha</name>
			<definition>[SII](6716{AA}+6730{AA})/Ha emission
                                          line fluxes ratio</definition>
			<units>---</units></field>
		<field>
			<name>W[OII]</name>
			<definition>[OII]3727{AA} emission line equivalent
                                          width</definition>
			<units>0.1nm</units></field>
		<field>
			<name>WHb</name>
			<definition>H{beta} emission line equivalent width</definition>
			<units>0.1nm</units></field>
		<field>
			<name>W[OIII]</name>
			<definition>[OIII]5007{AA} emission line equivalent
                                          width</definition>
			<units>0.1nm</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table3.dat">
	<title>Coordinates, redshifts and magnitudes of QSOs</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Name</name>
			<definition>Name of objects</definition>
			<units>---</units></field>
		<field>
			<name>RAh</name>
			<definition>Right ascension (B1950)</definition>
			<units>h</units></field>
		<field>
			<name>RAm</name>
			<definition>Right ascension (B1950)</definition>
			<units>min</units></field>
		<field>
			<name>RAs</name>
			<definition>Right ascension (B1950)</definition>
			<units>s</units></field>
		<field>
			<name>DE-</name>
			<definition>Declination sign</definition>
			<units>---</units></field>
		<field>
			<name>DEd</name>
			<definition>Declination (B1950)</definition>
			<units>deg</units></field>
		<field>
			<name>DEm</name>
			<definition>Declination (B1950)</definition>
			<units>arcmin</units></field>
		<field>
			<name>DEs</name>
			<definition>Declination (B1950)</definition>
			<units>arcsec</units></field>
		<field>
			<name>z</name>
			<definition>Observed redshift</definition>
			<units>---</units></field>
		<field>
			<name>Bmag</name>
			<definition>Magnitude in B filter</definition>
			<units>mag</units></field>
		<field>
			<name>ELines</name>
			<definition>Detected emission lines</definition>
			<units>---</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table4.dat">
	<title>Galaxies without emission lines</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Name</name>
			<definition>Name of objects</definition>
			<units>---</units></field>
		<field>
			<name>RAh</name>
			<definition>Right ascension (B1950)</definition>
			<units>h</units></field>
		<field>
			<name>RAm</name>
			<definition>Right ascension (B1950)</definition>
			<units>min</units></field>
		<field>
			<name>RAs</name>
			<definition>Right ascension (B1950)</definition>
			<units>s</units></field>
		<field>
			<name>DE-</name>
			<definition>Declination sign</definition>
			<units>---</units></field>
		<field>
			<name>DEd</name>
			<definition>Declination (B1950)</definition>
			<units>deg</units></field>
		<field>
			<name>DEm</name>
			<definition>Declination (B1950)</definition>
			<units>arcmin</units></field>
		<field>
			<name>DEs</name>
			<definition>Declination (B1950)</definition>
			<units>arcsec</units></field>
		<field>
			<name>HRV</name>
			<definition>Heliocentric radial velocity</definition>
			<units>km/s</units></field>
		<field>
			<name>Bmag</name>
			<definition>Magnitude in B filter</definition>
			<units>mag</units></field>
		<field>
			<name>BMAG</name>
			<definition>Absolute B-magnitude</definition>
			<units>mag</units></field>
		<field>
			<name>ALines</name>
			<definition>Absorption lines</definition>
			<units>---</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table5.dat">
	<title>Stars positions and spectral features</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Name</name>
			<definition>Name of objects</definition>
			<units>---</units></field>
		<field>
			<name>RAh</name>
			<definition>Right ascension (B1950)</definition>
			<units>h</units></field>
		<field>
			<name>RAm</name>
			<definition>Right ascension (B1950)</definition>
			<units>min</units></field>
		<field>
			<name>RAs</name>
			<definition>Right ascension (B1950)</definition>
			<units>s</units></field>
		<field>
			<name>DE-</name>
			<definition>Declination sign</definition>
			<units>---</units></field>
		<field>
			<name>DEd</name>
			<definition>Declination (B1950)</definition>
			<units>deg</units></field>
		<field>
			<name>DEm</name>
			<definition>Declination (B1950)</definition>
			<units>arcmin</units></field>
		<field>
			<name>DEs</name>
			<definition>Declination (B1950)</definition>
			<units>arcsec</units></field>
		<field>
			<name>n_Bmag</name>
			<definition>*: Magnitudes are taken from the APM
                                       Maddox et al., Cat. &lt;J/MNRAS/246/433></definition>
			<units>---</units></field>
		<field>
			<name>Bmag</name>
			<definition>Magnitude in B filter</definition>
			<units>mag</units></field>
		<field>
			<name>Type</name>
			<definition>Spectral type of a star</definition>
			<units>---</units></field>
		<field>
			<name>Lines</name>
			<definition>Spectral features</definition>
			<units>---</units></field></fields></tableHead>
	
			<textFile xlink:href="tables.tex"><name>tables.tex</name><description><para>LaTeX version of the tables</para></description></textFile>
			<textFile xlink:href="tables.ps" type="postscript"><name>tables.ps</name><description><para>PostScript version of the tables</para></description></textFile>
	<history>
		<ingest>
	
			<creator>
				<lastName>Patricia Bauer</lastName>
				<affiliation>CDS</affiliation></creator>
	<date>
		<year>1998</year><month>Dec</month><day>03</day></date><acknowledgement>Andrew Ugryumov &lt;and@relay.sao.ru></acknowledgement></ingest>
		</history>
	<identifier>J_A+AS_135_511.xml</identifier></dataset>
