<?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 ATCA/VLA OH 1612 MHz survey. I. Observations of the Galactic Bulge Region</title>
	<altname type="ADC">J/A+AS/122/79</altname>
		<altname type="CDS">J/A+AS/122/79</altname>
		<altname type="brief">Galactic Bulge Region OH 1612MHz survey. I.</altname>
	<reference>
		<source>
<journal>
	<title>The ATCA/VLA OH 1612 MHz survey. I. Observations of the Galactic Bulge Region</title>
	<author>
			<initial>M</initial>
			<initial>N</initial>
			<lastName>Sevenster</lastName></author>
	<author>
			<initial>J</initial>
			<initial>M</initial>
			<lastName>Chapman</lastName></author>
	<author>
			<initial>H</initial>
			<initial>J</initial>
			<lastName>Habing</lastName></author>
	<author>
			<initial>N</initial>
			<initial>E</initial>
			<initial>B</initial>
			<lastName>Killeen</lastName></author>
	<author>
			<initial>M</initial>
			<lastName>Lindqvist</lastName></author>
	<name>Astron. Astrophys. Suppl. Ser.</name>
	<volume>122</volume>
	<pageno>79</pageno>
		<date>
			<year>1997</year></date>
	<bibcode>1997A&amp;AS..122...79S</bibcode></journal></source></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
			<keyword xlink:href="Masers.html">Masers</keyword>
			<keyword xlink:href="Radio_lines.html">Radio lines</keyword></keywords>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/apj_keywords.html">
			<keyword xlink:href="Galaxy_center.html">Galaxy: center</keyword>
			<keyword xlink:href="Galaxy_stellar_content.html">Galaxy: stellar content</keyword>
			<keyword xlink:href="radio_lines_stars.html">radio lines: stars</keyword>
			<keyword xlink:href="stars_AGB_and_post-AGB.html">stars: AGB and post-AGB</keyword>
			<keyword xlink:href="surveys.html">surveys</keyword>
			<keyword xlink:href="techniques_image_processing.html">techniques: image processing</keyword></keywords>
	<descriptions>
				<abstract>
					<para>
    We present observations of the region between |l|&lt;=10{deg} and
    |b|&lt;=3{deg} in the OH 1612.231MHz line, taken in 1993 October and
    November with the Australia Telescope Compact Array. The region was
    systematically searched for OH/IR stars and was covered completely
    with 539 pointing centres separated by 30'. The size of the dataset
    calls for a special reduction technique that is fast, reliable and
    minimizes the output (positions and velocities of possible stars
    only). Having developed such a reduction method we found 307 OH masing
    objects, 145 of which are new detections. Out of these, 248 have a
    standard double-peaked spectral profile, 55 a single-peaked profile
    and 4 have nonstandard or irregular profiles. In this article we
    analyse the data statistically and give classifications and
    identifications with known sources where possible. The astrophysical,
    kinematical, morphological and dynamical properties of subsets of the
    data will be addressed in future articles. These observations are part
    of a larger survey, covering |l|&lt;=45{deg} and |b|&lt;=3{deg}, with the
    Australia Telescope Compact Array and the Very Large Array. The
    electronic version of this paper, that includes table and spectra, can
    be obtained from http://www.ed-phys.fr.</para></abstract>
                        <details/></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table1">
	<title>Compact OH-maser sources</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>No</name>
			<definition>Source number</definition>
			<units>---</units></field>
		<field>
			<name>Name</name>
			<definition>Source name (based on galactic longitude
                                 and latitude)</definition>
			<units>---</units></field>
		<field>
			<name>Type</name>
			<definition>Spectrum type</definition>
			<units>---</units></field>
		<field>
			<name>RAh</name>
			<definition>Right ascension J2000</definition>
			<units>h</units></field>
		<field>
			<name>RAm</name>
			<definition>Right ascension J2000</definition>
			<units>min</units></field>
		<field>
			<name>RAs</name>
			<definition>Right ascension J2000</definition>
			<units>s</units></field>
		<field>
			<name>DE-</name>
			<definition>Declination sign</definition>
			<units>---</units></field>
		<field>
			<name>DEd</name>
			<definition>Declination J2000</definition>
			<units>deg</units></field>
		<field>
			<name>DEm</name>
			<definition>Declination J2000</definition>
			<units>arcmin</units></field>
		<field>
			<name>DEs</name>
			<definition>Declination J2000</definition>
			<units>arcsec</units></field>
		<field>
			<name>Delta</name>
			<definition>Position scatter</definition>
			<units>arcsec</units></field>
		<field>
			<name>R</name>
			<definition>Offset from pointing centre</definition>
			<units>arcmin</units></field>
		<field>
			<name>VL</name>
			<definition>Velocity blue-shifted peak</definition>
			<units>km/s</units></field>
		<field>
			<name>VH</name>
			<definition>Velocity red-shifted peak</definition>
			<units>km/s</units></field>
		<field>
			<name>VC</name>
			<definition>Velocity central star</definition>
			<units>km/s</units></field>
		<field>
			<name>VE</name>
			<definition>Outflow velocity shell</definition>
			<units>km/s</units></field>
		<field>
			<name>SL</name>
			<definition>Flux density blue-shifted peak</definition>
			<units>Jy</units></field>
		<field>
			<name>SH</name>
			<definition>Flux density red-shifted peak</definition>
			<units>Jy</units></field>
		<field>
			<name>Rms</name>
			<definition>Rms noise in empty cubes</definition>
			<units>mJy</units></field>
		<field>
			<name>Ref</name>
			<definition>Number reference for previous detection</definition>
			<units>---</units></field>
		<field>
			<name>IRAS</name>
			<definition>Name of nearest IRAS point source &lt;II/125></definition>
			<units>---</units></field>
		<field>
			<name>N</name>
			<definition>Distance to nearest IRAS PS as fraction of IRAS
                                 error ellipse</definition>
			<units>---</units></field></fields></tableHead>
	
			<textFile xlink:href="table1.tex"><name>table1.tex</name><description><para>LaTeX version of table1</para></description></textFile>
	<history>
		<ingest>
	
			<creator>
				<lastName>M.N. Sevenster</lastName>
				<affiliation>Sterrewacht Leiden, NL</affiliation></creator>
	<date>
		<year>1996</year><month>Jul</month><day>19</day></date></ingest>
		</history>
	<identifier>J_A+AS_122_79.xml</identifier></dataset>
