<?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>Southern and equatorial irregular variables. I. Photoelectric photometry</title>
	<altname type="ADC">J/A+AS/124/55</altname>
		<altname type="CDS">J/A+AS/124/55</altname>
		<altname type="brief">Photometry of irregular variables</altname>
	<reference>
		<source>
<journal>
	<title>Southern and equatorial irregular variables. I. Photoelectric photometry</title>
	<author>
			<initial>D</initial>
			<lastName>Cieslinski</lastName></author>
	<author>
			<initial>F</initial>
			<initial>J</initial>
			<lastName>Jablonski</lastName></author>
	<author>
			<initial>J</initial>
			<initial>E</initial>
			<lastName>Steiner</lastName></author>
	<name>Astron. Astrophys. Suppl. Ser.</name>
	<volume>124</volume>
	<pageno>55</pageno>
		<date>
			<year>1997</year></date>
	<bibcode>1997A&amp;AS..124...55C</bibcode></journal></source>
	<related>
			<holding role="similar">II/139 : General Catalog of Variable Stars, 4th Ed. (GCVS4) (Kholopov+ 1988)<xlink:simple href="II/139"/></holding>
			<holding role="similar">II/140 : New Catalogue of Suspected Variable Stars (Kukarkin+, 1982)<xlink:simple href="II/140"/></holding>
			  Booth L., Charles P.A., 1982, MNRAS 201, 25p =1982MNRAS.201p..25B
  Downes R.A., Shara M.M., 1993, PASP 105, 127 =1993PASP..105..127D
  Gregorio-Hetem J., Lepine J.R.D., Quast G.R., Torres C.A.O., de la Reza R.,
      1992, AJ 103, 549 =1992AJ....103..549G
  Kholopov P.N., et al., 1987, General Catalogue of Variable Stars-GCVS4,
      Nauka Publishing House, Moscow
  Ninger-Kosibowa S., 1955, Prace Wrocl. Tow. Naukowego Ser. B, Nr. 57
  Torres C.A.O., Quast G.R., de la Reza R., Gregorio-Hetem J., Lepine J.R.D.,
      1995, AJ 109, 2146 =1995AJ....109.2146T
  Vogt N., Bateson F.M., 1982, A&amp;AS 48, 383 =1982A&amp;AS...48..383V</related></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
			<keyword xlink:href="Photometry_Cousins.html">Photometry, Cousins</keyword>
			<keyword xlink:href="Photometry_UBVRI.html">Photometry, UBVRI</keyword>
			<keyword xlink:href="Stars_variable.html">Stars, variable</keyword></keywords>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/apj_keywords.html">
			<keyword xlink:href="stars_AGB_and_post-AGB.html">stars: AGB and post-AGB</keyword>
			<keyword xlink:href="stars_variables_general.html">stars: variables: general</keyword>
			<keyword xlink:href="surveys.html">surveys</keyword></keywords>
	<descriptions>
				<description>
				<para>
    We present the results of an optical photometric survey of 616
    irregular variables. The targets were selected among objects
    classified as L, L:, I, I:, IS and IS: in the General Catalogue of
    Variable Stars and New Catalogue of Suspected Variable Stars.</para></description>
                        <details/></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table1">
	<title>UBV(RI) photometry</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Name</name>
			<definition>Star name</definition>
			<units>---</units></field>
		<field>
			<name>HJD</name>
			<definition>Heliocentric Julian day</definition>
			<units>d</units></field>
		<field>
			<name>Vmag</name>
			<definition>V magnitude</definition>
			<units>mag</units></field>
		<field>
			<name>U-B</name>
			<definition>U-B colour index</definition>
			<units>mag</units></field>
		<field>
			<name>B-V</name>
			<definition>B-V colour index</definition>
			<units>mag</units></field>
		<field>
			<name>V-Rc</name>
			<definition>V-R_c_ colour index</definition>
			<units>mag</units></field>
		<field>
			<name>Rc-Ic</name>
			<definition>R_c_-I_c_ colour index</definition>
			<units>mag</units></field>
		<field>
			<name>e_Vmag</name>
			<definition>Uncertainty on V magnitude</definition>
			<units>mag</units></field>
		<field>
			<name>e_U-B</name>
			<definition>Uncertainty on U-B colour index</definition>
			<units>mag</units></field>
		<field>
			<name>e_B-V</name>
			<definition>Uncertainty on B-V colour index</definition>
			<units>mag</units></field>
		<field>
			<name>e_V-Rc</name>
			<definition>Uncertainty on V-R_c_ colour index</definition>
			<units>mag</units></field>
		<field>
			<name>e_Rc-Ic</name>
			<definition>Uncertainty on R_c_-I_c_ colour index</definition>
			<units>mag</units></field>
		<field>
			<name>Rem</name>
			<definition>See note
	<footnote footnoteId="???"><para>number=1</para>
			<para>*: Nights without calibration sequences (see discussion in the paper)
          1: Averaged values of magnitude and colours. Object is a Mira variable
          2: Averaged values of magnitude and colours. Object is a cataclysmic
              variable
          3: 10 arcsec optical pair. Possible contamination
          4: Classified as probable Herbig Ae/Be object in Gregorio-Hetem et al.
              (1992AJ....103..549G)
          5: 10 arcsec optical pair (~2mag weaker) included in the diaphragm
          6: Averaged values of magnitude and colours. Object is a symbiotic u
              star
          7: Suggested as Cepheid variable by Booth &amp; Charles
              (1982MNRAS.201p..25B)
          8: Object is a RV Tauri variable
          9: Optical pair (~2mag weaker) included in the diaphragm
         10: Quoted as suspected of cataclysmic variable in Vogt &amp; Bateson
              (1982A&amp;AS...48..383V) and Downes &amp; Shara (1993, Cat. &lt;V/79>)
         11: Quoted as suspected of cataclysmic variable of Z Cam type in the
              GCVS4 (kholopov et al. 1987, Cat. &lt;II/139>)
         12: Classified as T Tauri star in Torres et al. (1995AJ....109.2146T)
         13: Carbon star
         14: Optical pair. The two stars were included in the diaphragm
         15: 5 arcsec optical pair (~3mag weaker) included in the diaphragm
         16: Constant star. Possibly indicated wrongly in the finding chart of
              Ninger-Kosibowa (1955, Prace Wrocl. Tow. Naukowego Ser. B, Nr. 57)
         17: 10 arcsec optical pair. The two stars were included in the
               diaphragm
         18: 10 arcsec optical pair. Possible contamination
         19: Object is a RR Lyrae variable
         20: &lt;10 arcsec optical pair. The two objects were included in the
              diaphragm
         21: Optical pair. The two stars included in the diaphragm
         22: Object is a Be star
         23: 5 arcsec optical pair included in the diaphragm
--------------------------------------------------------------------------------
Acknowledgements: Deonisio Cieslinski &lt;deo@das.inpe.br></para></footnote></definition>
			<units>---</units></field></fields></tableHead>
	
	<history>
		<ingest>
	
			<creator>
				<lastName>Patricia Bauer</lastName>
				<affiliation>CDS</affiliation></creator>
	<date>
		<year>1996</year><month>Dec</month><day>09</day></date></ingest>
		</history>
	<identifier>J_A+AS_124_55.xml</identifier></dataset>
