<?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 MIT-Green Bank (MG) 5 GHz survey</title>
	<altname type="ADC">8052A</altname>
		<altname type="CDS">VIII/52A</altname>
		<altname type="brief">The MIT-Green Bank 5GHz Survey</altname>
	<reference>
		<source>
<journal>
	<title>The MIT-Green Bank (MG) 5 GHz survey</title>
	<author>
			<initial>C</initial>
			<initial>L</initial>
			<lastName>Bennett</lastName></author>
	<author>
			<initial>C</initial>
			<initial>R</initial>
			<lastName>Lawrence</lastName></author>
	<author>
			<initial>B</initial>
			<initial>F</initial>
			<lastName>Burke</lastName></author>
	<author>
			<initial>J</initial>
			<initial>N</initial>
			<lastName>Hewitt</lastName></author>
	<author>
			<initial>J</initial>
			<lastName>Mahoney</lastName></author>
	<name>Astrophys. J. Suppl. Ser.</name>
	<volume>61</volume>
	<pageno>1</pageno>
		<date>
			<year>1986</year></date>
	<bibcode>1986ApJS...61....1B</bibcode></journal>
<journal>
	<title>The MIT-Green Bank (MG) 5 GHz survey</title>
	<author>
			<initial>G</initial>
			<initial>I</initial>
			<lastName>Langston</lastName></author>
	<author>
			<initial>M</initial>
			<initial>B</initial>
			<lastName>Heflin</lastName></author>
	<author>
			<initial>S</initial>
			<initial>R</initial>
			<lastName>Conner</lastName></author>
	<author>
			<initial>J</initial>
			<lastName>Lehar</lastName></author>
	<author>
			<initial>C</initial>
			<initial>L</initial>
			<lastName>Carrilli</lastName></author>
	<author>
			<initial>B</initial>
			<initial>F</initial>
			<lastName>Burke</lastName></author>
	<name>Astrophys. J. Suppl. Ser.</name>
	<volume>72</volume>
	<pageno>621</pageno>
		<date>
			<year>1990</year></date>
	<bibcode>1990ApJS...72..621L</bibcode></journal>
<journal>
	<title>The MIT-Green Bank (MG) 5 GHz survey</title>
	<author>
			<initial>M</initial>
			<lastName>Griffith</lastName></author>
	<author>
			<initial>G</initial>
			<lastName>Langston</lastName></author>
	<author>
			<initial>M</initial>
			<lastName>Heflin</lastName></author>
	<author>
			<initial>S</initial>
			<lastName>Conner</lastName></author>
	<author>
			<initial>J</initial>
			<lastName>Lehar</lastName></author>
	<author>
			<initial>B</initial>
			<lastName>Burke</lastName></author>
	<name>Astrophys. J. Suppl. Ser.</name>
	<volume>74</volume>
	<pageno>129</pageno>
		<date>
			<year>1990</year></date>
	<bibcode>1990ApJS...74..129G</bibcode></journal>
<journal>
	<title>The MIT-Green Bank (MG) 5 GHz survey</title>
	<author>
			<initial>M</initial>
			<lastName>Griffith</lastName></author>
	<author>
			<initial>G</initial>
			<lastName>Langston</lastName></author>
	<author>
			<initial>M</initial>
			<lastName>Heflin</lastName></author>
	<author>
			<initial>S</initial>
			<lastName>Conner</lastName></author>
	<author>
			<initial>B</initial>
			<lastName>Burke</lastName></author>
	<name>Astrophys. J. Suppl. Ser.</name>
	<volume>75</volume>
	<pageno>801</pageno>
		<date>
			<year>1991</year></date>
	<bibcode>1991ApJS...75..801G</bibcode></journal></source>
	<related>
			<holding role="similar">VIII/14 : 87GB Radio Sources 4.85 GHz (Gregory, Condon 1991)
   A 4.85 GHz sky survey. (Condon+ 1994) =1994AJ....107.1829C
   90GB 4.85 GHz Sky Maps (Condon+ 1995) =1995ADIL...JC...06C<xlink:simple href="VIII/14"/></holding>
			  Condon, J. J., and Broderick, J. J. 1985, AJ, 90, 2540 =1985AJ.....90.2540C
  Douglas, J. N., Bash, F. N., Torrence, G. W., and Wolfe, C. 1980, The Texas
    Survey: Preliminary +18 deg Strip (Univ. Texas Pub. Astr. No. 17).
    =1980PAUTx..17....1D</related></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
			<keyword xlink:href="Radio_continuum.html">Radio continuum</keyword>
			<keyword xlink:href="Radio_sources.html">Radio sources</keyword></keywords>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/apj_keywords.html">
			<keyword xlink:href="radio_sources_general.html">radio sources: general</keyword>
			<keyword xlink:href="radio_sources_identifications.html">radio sources: identifications</keyword></keywords>
	<descriptions>
				<description>
				<para>
    The MIT-Green Bank 5 GHz survey catalog was produced from four separate
    surveys with the National Radio Astronomy Observatory (NRAO) 91m transit
    telescope (Bennett et al., 1986ApJS...61....1 (MG1);  Langston et al.,
    1990ApJS...72..621 (MG2);  Griffith et al., 1990ApJS...74..129 (MG3);
    Griffith et al. 1991ApJS...75..801 (MG4)).  The sky coverage of the
    various surveys is 00h &lt; RA &lt; 24h, -00d30'13" &lt; DECB &lt; +19d29'47" for MG1;
    04h &lt; RAJ &lt; 21h, +17.0d &lt; DECJ &lt; +39d09' for MG2; 16h30m &lt; RAB &lt; 05h,
    +17d &lt; DECB &lt; +39d09' for MG3; and 15h30m &lt; RAB &lt; 02h30m; +37.00d &lt; DECB
    &lt; +50d58'48" for MG4; where RAB and DECB refer to B1950 coordinates, and
    RAJ and DECJ refer to J2000 coordinates.  The catalog contains 20344
    sources detected with a signal-to-noise ratio greater than 5 and 3836
    possible detections (MG1) with a signal-to-noise ratio less than 5.
    Spectral indices are computed for MG1 sources also identified in the
    Texas 365 MHz survey (Douglas et al. 1980), and for MG1-MG4 sources also
    identified in the NRAO 1400 MHz Survey (Condon and Broderick 1985).</para><para>    Notice:
    Original names were expanded by H.Andernach to MGn_Jhhmmss+ddmm, as
    suggested by Glen Langston on 25-Mar-1998 in reply to an inquiry by the
    IAU TG on Designations.</para></description>
                        <details/></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="mg1to4.dat">
	<title>MG1-4 source list</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Name</name>
			<definition>Source name
	<footnote>
			<para>
     sources with signal-to-noise ratios less than 5 are listed as 'MG1s...'</para></footnote></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>l_Flux</name>
			<definition>Flux density limit flag
	<footnote>
			<para>
     blank if 'Flux' is actual flux density
     '>' if 'Flux' is lower limit on flux density (MG1 fluxes over 5 Jy
       are listed as "> 5000" due to receiver saturation.)</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>Flux</name>
			<definition>Green Bank flux density at 4.830 or 4.775 GHz</definition>
			<units>mJy</units></field>
		<field>
			<name>n_Flux</name>
			<definition>Flux note flag
	<footnote>
			<para>
     blank if frequency is 4.830 GHz (MG2-4)
     '*' if frequency is 4.775 GHz (MG1)</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>l_S/N</name>
			<definition>Signal-to-noise limit flag
	<footnote>
			<para>
     blank if 'S/N' is actual signal-to-noise
     '>' if 'S/N' is lower limit on signal-to-noise (MG1 S/N values over
       100 are listed as ">99.9".)</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>S/N</name>
			<definition>Signal-to-noise ratio of the detection, or
                                  lower limit on signal-to-noise.</definition>
			<units>---</units></field>
		<field>
			<name>G</name>
			<definition>Group containing the source
	<footnote>
			<para>
     G is defined by the north or south survey detecting the source
       and the source location in the survey.
     Sources with b > +10 deg and detected in the south, north, or both
       surveys are assigned to groups 0, 1, 2.
     Sources lying in regions observed only once or at low Galactic
       latitude |b| &lt; 10 deg, and detected in the south, north, or both
       surveys are assigned to groups 3, 4, or 5.
     Sources in the region observed twice but with b &lt; -10 deg and
       detected in south, north, or both surveys, are assigned to
       groups 6, 7, or 8.</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>alpha</name>
			<definition>The spectral index of the source, where
                                    Flux {prop.to.} {nu}^alpha^</definition>
			<units>---</units></field>
		<field>
			<name>n_alpha</name>
			<definition>Spectral index note flag
	<footnote>
			<para>
     blank if spectral index derived using NRAO 1400 MHz and 4.830 GHz
       observations (MG2-4)
     "*" if derived using Texas 365 MHz and 4.775 GHz observations (MG1)
</para></footnote></definition>
			<units>---</units></field></fields></tableHead>
	
	<history>
		<ingest>
	
			<creator>
				<lastName>Tom Sodroski</lastName>
				<affiliation>SSDOO/ADC</affiliation></creator>
	<date>
		<year>1999</year><month>Apr</month><day>30</day></date><acknowledgement>This catalog was originally compiled by Dr. Heinz Andernach at the
  Universidad de Guanajuato.</acknowledgement></ingest>
		</history>
	<identifier>VIII_52A.xml</identifier></dataset>
