<?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>Fifth Fundamental Catalogue (FK5) Part I</title>
	<altname type="ADC">1149A</altname>
		<altname type="CDS">I/149A</altname>
		<altname type="brief">Fifth Fundamental Catalogue</altname>
	<reference>
		<source>
<other>
	<title>Fifth Fundamental Catalogue (FK5) Part I</title>
	<author>
			<initial>W</initial>
			<lastName>Fricke</lastName></author>
	<author>
			<initial>H</initial>
			<lastName>Schwan</lastName></author>
	<author>
			<initial>T</initial>
			<lastName>Lederle</lastName></author>
	<author>
			<initial>U</initial>
			<lastName>Bastian</lastName></author>
	<author>
			<initial>R</initial>
			<lastName>Bien</lastName></author>
	<author>
			<initial>G</initial>
			<lastName>Burkhardt</lastName></author>
	<author>
			<initial>B</initial>
			<lastName>du Mont</lastName></author>
	<author>
			<initial>R</initial>
			<lastName>Hering</lastName></author>
	<author>
			<initial>R</initial>
			<lastName>Jaehrling</lastName></author>
	<author>
			<initial>H</initial>
			<lastName>Jahreiss</lastName></author>
	<author>
			<initial>S</initial>
			<lastName>Roeser</lastName></author>
	<author>
			<initial>H</initial>
			<initial>M</initial>
			<lastName>Schwerdtfeger</lastName></author>
	<author>
			<initial>H</initial>
			<initial>G</initial>
			<lastName>Walter</lastName></author>
	<name>Veroeff. Astron. Rechen-Institut Heidelb. No. 32</name>
	<publisher>???</publisher>
	<city>???</city>
	
		<date>
			<year>1988</year></date>
	<bibcode>1988VeARI..32....1F</bibcode></other></source>
	<related>
			<holding role="similar">I/175 : FK5, Part II (Extension).<xlink:simple href="I/175"/></holding>
			   Argelander, F. W. A. 1859-62, Bonner Sternverzeichniss, erste bis
      dritte Sektion, Astronomischen Beobachtungen auf der Sternwarte der
      Koeniglichen Rhein., Friedrich-Wilhelms-Universitaet zu Bonn, Baende
      3-5   (Catalog &lt;I/122>)
   Boss, B. 1937, General Catalogue of 33342 Stars for the Epoch 1950,
      Carnegie Institution of Washington Pub. 468 (Washington, Carnegie
      Institution of Washington) (Catalog &lt;I/113>)
   Cannon, A. J., &amp; Pickering, E. C. 1918-24, The Henry Draper
      Catalogue, Ann. Astron. Obs. Harvard College, 91-99
      (Catalog &lt;III/135>)
   Corbin, T. E. 1978, in IAU Colloquium 48, Modern Astrometry, ed. F. V.
      Prochazka &amp; R. H. Tucker (Vienna, University Obs.), p. 505
      (Catalog &lt;I/72>)
   Fricke, W., &amp; Kopff, A. 1963, Fourth Fundamental Katalog (FK4),
      Veroeff. Astron. Rechen-Inst. Heidelb. No. 10. (Catalog &lt;I/15>)
   Fricke, W., Schwan, H., &amp; Lederle, T. (in collaboration with
      Bastian, U., Bien, R., Burkhardt, G., du Mont, B., Hering, R.,
      Jaehrling, R., Jahreiss, H., Roeser, S., Schwerdtfeger, H. M., &amp;
      Walter, H. G.) 1988, Fifth Fundamental Catalogue (FK5), Part I. The
      Basic Fundamental Stars, Veroeff. Astron. Rechen-Institut Heidelb.
      No. 32  (Catalog &lt;I/149>)
   Gill, D., &amp; Kapteyn, J. C. 1895-1900, Cape Photographic
      Durchmusterung, Ann. Cape Obs., 3 (1895, Part I: zones -18 deg. to
      -37 deg.); 4 (1897, Part II: zones -38 deg. to -52 deg.); 5 (1900,
      Part III: zones -53 deg. to -89 deg.)   (Catalog &lt;I/108>)
   Kuestner, F. 1903, Bonner Durchmusterung des Noerdlichen Himmels,
      zweite berichtigte Auflage, Bonn Universitaets Sternwarte (Bonn, A.
      Marcus und E. Weber's Verlag) (Catalog &lt;I/122>)
   Lieske, J. H. 1979, Astron. &amp; Astroph., 73, 282   (=1979A&amp;A....73..282L)
   Nicolet, B. 1975, Catalogue of Measurements in the Cape UBV
      Photometry on Magnetic Tape, Astron. &amp; Astroph. Supp., 22, 239
      (Catalog &lt;II/27>)
   Nicolet, B. 1978, Catalogue of Homogeneous Data in the UBV
      Photoelectric Photometric System, Astron. &amp; Astroph. Supp., 34, 1
      (=1978A&amp;AS...34....1N)
   Schoenfeld, E. 1886, Bonner Sternverzeichniss, vierte Sektion,
      Astronomische Beobachtungen auf der Sternwarte der Koeniglichen
      Rheinischen Friedrich-Wilhelms-Universitaet zu Bonn, 8, Part IV
      (Bonn, Adolph Marcus Verlag)  (Catalog &lt;I/119>)
   Scott, F. P., &amp; Smith, C. A., Jr. 1971, Comparison of the SAO and
      AGK3R Star Catalogues, in Conference on Photographic Astrometric
      Techniques, ed. H. K. Eichhorn, NASA CR-1825
   Smith, C. A., Corbin, T. E., Hughes, J. A., Jackson, E. S.,
      Krutskaya, E. V., Polozhentsev, A. D., Polozhentsev, D. D., Yagudin,
      L. I., &amp; Zverev, M. S. 1990, in IAU Symposium No. 141, Inertial
      Coordinate System on the Sky, ed. J. H. Lieske &amp; V. K. Abalakin
      (Dordrecht, Reidel), p. 457 (Catalog &lt;I/138>)
   Thome, J. M. 1892-1932, Cordoba Durchmusterung,
      Resultados del Observatorio Nacional Argentino, 16 (1892, Part I:
      -22 deg. to -32 deg.); 17 (1894, Part II: -32 deg. to -42 deg.); 18
      (1900, Part III: -42 deg. to -52 deg.); 21 (Part I) (1914, Part IV,
      -52 deg. to -62 deg.); 21 (Part II) (1932, Part V: -62 deg. to
      -90 deg.)  (Catalog &lt;I/114>)</related></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
			<keyword xlink:href="Proper_motions.html">Proper motions</keyword>
			<keyword xlink:href="Positional_data.html">Positional data</keyword></keywords>
	<descriptions>
				<abstract>
					<para>
    The Basic Fifth Fundamental Catalogue (FK5) Part I provides improved
    mean positions and proper motions for the 1535 classical fundamental
    stars that had been included in the FK3 and FK4 catalogs. The machine
    version of the catalog contains the positions and proper motions of
    the Basic FK5 stars for the epochs and equinoxes J2000.0 and B1950.0,
    the mean epochs of individual observed right ascensions and
    declinations used to determine the final positions, the mean errors of
    the final positions and proper motions for the reported epochs, and
    ancillary data such as magnitudes, spectral types, parallaxes, radial
    velocities, and cross identifications to other catalog designations.</para></abstract>
			<details>
			<para>
    The Basic FK5 is the successor to the FK4 (Fricke &amp; Kopff 1963) and
    contains the 1535 classical fundamental stars used to define the
    latter system. It represents a revision of the FK4 and results from
    the determination of systematic and individual corrections to the mean
    positions and proper motions of the FK4, the elimination of the error
    in the FK4 equinox, and the introduction of the IAU (1976) system of
    astronomical constants. About 300 catalogs providing star positions
    obtained from throughout the world are included in the FK5. This
    document should be used only to supplement the information contained
    in the source reference. The latter should be consulted for more
    detailed information regarding the motivation for construction of the
    FK5, the determination of its equator and equinox, the expressions for
    general precession, a discussion of the FK5 system, systematic
    differences between the FK4 and FK5, the transformation of
    observational catalogs to the FK5 system and to the reference system
    J2000.0, and more thorough descriptions of the data contained in the
    FK5 catalog.</para></details></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="catalog.dat">
	<title>The FK5 catalog</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>FK5</name>
			<definition>FK5 number
	<footnote>
			<para>
   These numbers have remained the same from the FK3 and FK4 (Catalog &lt;I/15>).
   The user should note that the file is ordered by FK5 number, which
   means that the stars are arranged neither by right ascension nor by
   declination.</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>RAh</name>
			<definition>Right ascension, hours,
                                              Equinox=J2000, Epoch=J2000</definition>
			<units>h</units></field>
		<field>
			<name>RAm</name>
			<definition>Right ascension minutes (J2000.0)</definition>
			<units>min</units></field>
		<field>
			<name>RAs</name>
			<definition>Right ascension seconds (J2000.0)
	<footnote>
			<para>
   The terms of elliptic aberration have been eliminated from the mean
   positions. The B1950.0 data have been computed from the J2000.0 data
   using a procedure described in the source reference (Fricke et al. 1988)
   based on the IAU (1976) system of astronomical constants (see also
   Lieske 1979).</para></footnote></definition>
			<units>s</units></field>
		<field>
			<name>pmRA</name>
			<definition>Proper motion in RA (J2000.0)</definition>
			<units>s/ha</units></field>
		<field>
			<name>DE-</name>
			<definition>Sign of declination (Dec) (J2000.0)</definition>
			<units>---</units></field>
		<field>
			<name>DEd</name>
			<definition>Declination degrees (J2000.0)</definition>
			<units>deg</units></field>
		<field>
			<name>DEm</name>
			<definition>Declination arcminutes (J2000.0)</definition>
			<units>arcmin</units></field>
		<field>
			<name>DEs</name>
			<definition>Declination arcseconds (J2000.0)</definition>
			<units>arcsec</units></field>
		<field>
			<name>pmDE</name>
			<definition>Proper motion in DE (J2000.0)</definition>
			<units>arcsec/ha</units></field>
		<field>
			<name>RAh1950</name>
			<definition>Right ascension, hours
                                              Equinox=B1950, Epoch=B1950</definition>
			<units>h</units></field>
		<field>
			<name>RAm1950</name>
			<definition>Right ascension minutes (B1950.0)</definition>
			<units>min</units></field>
		<field>
			<name>RAs1950</name>
			<definition>Right ascension seconds (B1950.0)</definition>
			<units>s</units></field>
		<field>
			<name>pmRA1950</name>
			<definition>Proper motion in RA (B1950.0)</definition>
			<units>s/ha</units></field>
		<field>
			<name>DE-1950</name>
			<definition>Sign of declination (B1950.0)</definition>
			<units>---</units></field>
		<field>
			<name>DEd1950</name>
			<definition>Declination degrees (B1950.0)</definition>
			<units>deg</units></field>
		<field>
			<name>DEm1950</name>
			<definition>Declination arcminutes (B1950.0)</definition>
			<units>arcmin</units></field>
		<field>
			<name>DEs1950</name>
			<definition>Declination arcseconds (B1950.0)</definition>
			<units>arcsec</units></field>
		<field>
			<name>pmDE1950</name>
			<definition>Proper motion in DE (B1950.0)</definition>
			<units>arcsec/ha</units></field>
		<field>
			<name>EpRA-1900</name>
			<definition>Mean Epoch of observed RA
	<footnote>
			<para>
   Mean epoch (-1900.0) of the individual observed right ascensions and
   declinations.</para></footnote></definition>
			<units>a</units></field>
		<field>
			<name>e_RAs</name>
			<definition>Mean error in RA
	<footnote>
			<para>
   The mean errors of the positions at the mean epoch and of the
   corresponding proper-motion components, as obtained from the solution of
   the normal equations within the derivations of individual positions and
   proper motions. (These mean errors do not include those of the FK5
   system and of the equinox and equator.)</para></footnote></definition>
			<units>ms</units></field>
		<field>
			<name>e_pmRA</name>
			<definition>Mean error in pmRA</definition>
			<units>ms/ha</units></field>
		<field>
			<name>EpDE-1900</name>
			<definition>Mean Epoch of observed DE</definition>
			<units>a</units></field>
		<field>
			<name>e_DEs</name>
			<definition>Mean error in Declination</definition>
			<units>carcsec</units></field>
		<field>
			<name>e_pmDE</name>
			<definition>Mean error in pmDE</definition>
			<units>carcsec/ha</units></field>
		<field>
			<name>Vmag</name>
			<definition>V magnitude
	<footnote>
			<para>
   Photoelectric magnitudes on the UBV system, as taken from the catalogs
   of Nicolet (1975, 1978). Variability is indicated by a flag in byte 129.
   For physical double stars, the magnitudes of the brighter components are
   given (both are given in the published catalog).</para></footnote></definition>
			<units>mag</units></field>
		<field>
			<name>n_Vmag</name>
			<definition>Magnitude flag
	<footnote>
			<para>
   Where magnitude ranges are given in the published catalog, the brighter
   magnitude is given and byte 129 contains an upper case "V". A lower case
   "v" is present if there is variability and that letter is present in the
   published catalog (amplitude exceeds 0.3mag). A "D" code indicates that
   the magnitudes of two close components are given as a footnote in the
   published catalog. Only the first of the two is contained in the
   magnitude field of the machine-readable catalog.</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>SpType</name>
			<definition>Spectral type(s)
	<footnote>
			<para>
   A one-dimensional spectral type taken from the FK4 catalog. These types
   are from the Henry Draper Catalogue (Cannon &amp; Pickering 1918-24). For
   binary and multiple systems where spectral types are known for more than
   one component, a second spectral type may be given following a plus
   sign.</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>plx</name>
			<definition>Parallax
	<footnote>
			<para>
   Trigonometric parallax if known (blank otherwise). These data are
   taken from a preliminary version of the new Yale parallax catalog
   (van Altena, Lee, &amp; Hoffleit, in preparation). Negative parallaxes
   present in the Yale catalog have been omitted here because they are
   of no use in computing apparent places from the mean positions.</para></footnote></definition>
			<units>arcsec</units></field>
		<field>
			<name>RV</name>
			<definition>Radial velocity
	<footnote>
			<para>
   Radial Velocity if known (blank otherwise)</para></footnote></definition>
			<units>km/s</units></field>
		<field>
			<name>AGK3R</name>
			<definition>AGK3R number (Catalog &lt;I/72>)</definition>
			<units>---</units></field>
		<field>
			<name>SRS</name>
			<definition>SRS number (Catalog &lt;I/138>)</definition>
			<units>---</units></field>
		<field>
			<name>HD</name>
			<definition>HD number (Catalog &lt;III/135>)</definition>
			<units>---</units></field>
		<field>
			<name>DM</name>
			<definition>DM identifier
	<footnote>
			<para> the prefixes are
   BD:  Bonner Durchmusterung (Argelander 1859-62, Kuestner 1903)
   SD:  Southern Durchmusterung (Schoenfeld 1886)
   CD:  Cordoba Durchmusterung (Thome 1892-1932)
   CP:  Cape Photographic Durchmusterung (Gill &amp; Kapteyn 1895-1900)
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>GC</name>
			<definition>GC number (Catalog &lt;I/113>)</definition>
			<units>---</units></field></fields></tableHead>
	
	<history>
		<ingest>
	
			<creator>
				<lastName>Nancy G. Roman</lastName>
				<affiliation>ADC/SSDOO</affiliation></creator>
			<creator>
				<lastName>rev. Francois Ochsenbein</lastName>
				<affiliation>CDS</affiliation></creator>
	<date>
		<year>1995</year><month>Jun</month><day>13</day></date><acknowledgement>Dr. H. Schwan kindly supplied the original and revised versions of the
   on magnetic tape and colleagues at the Astronomisches Rechen-Institut
   generously reviewed a draft copy of the original documentation prior to
   its final release for distribution with machine-readable copies of the
   catalog, and Dr. Schwan returned comments and corrections. Appreciation
   is expressed to Dr. William M. Owen Jr. of JPL for supplying the
   machine-readable FK4, DM cross index that was used to insert DM numbers
   into the original version of the FK5 catalog.</acknowledgement></ingest>
		
		<revisions>
	<revision>
		<creator>
			<lastName>UNKNOWN</lastName></creator>
		<date><year>UNKNOWN</year></date>
		<para>   The following format changes were made by W. H. Warren Jr. (with Dr.
   Schwan's concurrence):
      The DM identifiers, which were single-digit numerical codes, were
         changed to the literal codes.
      Plus signs were added to the trigonometric-parallax data, even though
         no negative parallaxes are included in the catalog, to indicate
         that negative parallaxes are possible.
      Multiple blanks between data fields were removed, as were blanks
         beyond the end of each record, to decrease the logical record
         length from 220 bytes to 190 bytes.</para></revision></revisions></history>
	<identifier>I_149A.xml</identifier></dataset>
