\magnification=900
%\input jhe.citmac
%\input jhe.defs

%--------------------------------%
%  GENERALLY USEFUL DEFINITIONS  %
%--------------------------------%
\def\nohyphen{\pretolerance 10000}
\def\singlespace{\baselineskip 12pt \lineskip 1pt \parskip 2pt plus 1 pt}
\def\mediumspace{\baselineskip 18pt \lineskip 6pt \parskip 3pt plus 5 pt}
\def\doublespace{\baselineskip 24pt \lineskip 10pt \parskip 5pt plus 10 pt}
\def\today{\number\day\enspace
     \ifcase\month\or January\or Febuary\or March\or April\or May\or
     June\or July\or August\or September\or October\or
     November\or December\fi \enspace\number\year}
\def\clock{\count0=\time \divide\count0 by 60
    \count1=\count0 \multiply\count1 by -60 \advance\count1 by \time
    \number\count0:\ifnum\count1<10{0\number\count1}\else\number\count1\fi}
\footline={\hss -- \folio\ -- \hss}
\def\draft{\headline={\hss \today \quad\quad \clock}}
%-----------%
%  SYMBOLS  %
%-----------%
\def\deg{\ifmmode^\circ\else$^\circ$\fi}
\def\solar{\ifmmode_{\mathord\odot}\else$_{\mathord\odot}$\fi}
%--------------%
%  REFERENCES  %
%--------------%
\def\jref#1 #2 #3 #4 {{\par\noindent \hangindent=3em \hangafter=1
      \advance \rightskip by 5em #1, #2, #3, #4.\par}}
\def\ref#1{{\par\noindent \hangindent=3em \hangafter=1
      \advance \rightskip by 5em #1.\par}}
%----------------------------------%
%  INCREMENTAL EQUATION NUMBERING  %
%----------------------------------%
\newcount\eqnum
\def\nexteq{\global\advance\eqnum by1 \eqno(\number\eqnum)}
\def\lasteq#1{\if)#1[\number\eqnum]\else(\number\eqnum)\fi#1}
\def\preveq#1#2{{\advance\eqnum by-#1
    \if)#2[\number\eqnum]\else(\number\eqnum)\fi}#2}
%----------%
%  TABLES  %
%----------%
\def\endtable{\endgroup}
\def\tableheight{\vrule width 0pt height 8.5pt depth 3.5pt}
{\catcode`|=\active \catcode`&=\active
    \gdef\tabledelim{\catcode`|=\active \let|=\vbar
                     \catcode`&=\active \let&=\nobar} }
\def\table{\begingroup
    \def\twidth{\hsize}
    \def\tablewidth##1{\def\twidth{##1}}
    \def\defaultheight{\vrule width 0pt height 8.5pt depth 3.5pt}
    \def\heightdepth##1{\dimen0=##1
        \ifdim\dimen0>5pt
            \divide\dimen0 by 2 \advance\dimen0 by 2.5pt
            \dimen1=\dimen0 \advance\dimen1 by -5pt
            \vrule width 0pt height \the\dimen0  depth \the\dimen1
        \else  \divide\dimen0 by 2
            \vrule width 0pt height \the\dimen0  depth \the\dimen0 \fi}
    \def\spacing##1{\def\defaultheight{\heightdepth{##1}}}
    \def\nextheight##1{\noalign{\gdef\tableheight{\heightdepth{##1}}}}
    \def\end{\cr\noalign{\gdef\tableheight{\defaultheight}}}
    \def\zerowidth##1{\omit\hidewidth ##1 \hidewidth}
    \def\hline{\noalign{\hrule}}
    \def\skip##1{\noalign{\vskip##1}}
    \def\bskip##1{\noalign{\hbox to \twidth{\vrule height##1 depth 0pt \hfil
        \vrule height##1 depth 0pt}}}
    \def\header##1{\noalign{\hbox to \twidth{\hfil ##1 \unskip\hfil}}}
    \def\bheader##1{\noalign{\hbox to \twidth{\vrule\hfil ##1
        \unskip\hfil\vrule}}}
    \def\spanloop{\span\omit \advance\mscount by -1}
    \def\extend##1##2{\omit
        \mscount=##1 \multiply\mscount by 2 \advance\mscount by -1
        \loop\ifnum\mscount>1 \spanloop\repeat \ \hfil ##2 \unskip\hfil}
    \def\vbar{&\vrule&}
    \def\nobar{&&}
    \def\hdash##1{ \noalign{ \relax \gdef\tableheight{\heightdepth{0pt}}
        \toks0={} \count0=1 \count1=0 \putout##1\end
        \toks0=\expandafter{\the\toks0 &\end} \xdef\piggy{\the\toks0} }
        \piggy}
    \let\e=\expandafter
    \def\putspace{\ifnum\count0>1 \advance\count0 by -1
        \toks0=\e\e\e{\the\e\toks0\e&\e\multispan\e{\the\count0}\hfill}
        \fi \count0=0 }
    \def\putrule{\ifnum\count1>0 \advance\count1 by 1
        \toks0=\e\e\e{\the\e\toks0\e&\e\multispan\e{\the\count1}\leaders\hrule\hfill}
        \fi \count1=0 }
    \def\putout##1{\ifx##1\end \putspace \putrule \let\next=\relax
        \else \let\next=\putout
            \ifx##1- \advance\count1 by 2 \putspace
            \else    \advance\count0 by 2 \putrule \fi \fi \next}   }
\def\tablespec#1{
    \def\vdimens{\noexpand\tableheight}
    \def\tabby{\tabskip=0pt plus100pt minus100pt}
    \def\r{&################\tabby&\hfil################\unskip}
    \def\c{&################\tabby&\hfil################\unskip\hfil}
    \def\l{&################\tabby&################\unskip\hfil}
    \edef\templ{\noexpand\vdimens ########\unskip  #1
         \unskip&########\tabskip=0pt&########\cr}
    \tabledelim
    \edef\body##1{ \vbox{
        \tabskip=0pt \offinterlineskip
        \halign to \twidth {\templ ##1}}} }
\everymath={\rm}

\def\IR{{\it IRAS }}			% IRAS
\def\fnu{$F_{\nu}$}			% fnu
\def\um{$\mu$m}		        % microns
\def\LS{$L_{\odot}$}			% L sun
\def\Lirs{${\rm log\ (L_{ir} / L_{\odot})\ }$} % Lir/Lsun
\def\Lbol{${\rm log\ (L_{bol} / L_\odot)\ }$}   % Lbol/Lsun
\def\LM{${\rm L_{ir} / M(H_2)\ }$}      % L_ir / M(H_2)
\def\LMU{${\rm \lbrack L_\odot M_\odot^{-1} \rbrack}$}  % L/M solar units
\def\Lir{${\rm L_{ir\ }}$}                % Lir
\def\s{${\rm ^{s\ }}$}                  % 's
\def\pwr #1 {$10^{#1}$}			% 10**x
\def\pwrx #1 #2 {$#1 \times$\pwr #2 }	% x*10**y
\def\il{infrared-luminous} 		% infrared-luminous
\def\fd{flux density}			% flux density
\def\lum{luminosity}			% luminosity
\def\lums{luminosities}			% luminosities
\def\EA{et al. }			% et al.
\def\arcs{$^{\prime\prime\ \ }$}			% arcsec
\def\arcm{$^{\prime\ \ }$}				% arcmin
\def\parcs{$\mskip 2mu .\!\!{^{\prime\prime}}$}	% arcsec over period
\def\parcm{$.\!{^{\prime}}$}			% arcmin over period
\def\deg{$^{\circ}$}				% deg
\def\KS{km s$^{-1}$}
\def\13CO{$^{\rm 13}$CO}
\def\12CO{$^{\rm 12}$CO}
\def\GR{$R / R_\odot$}
\def\gtapp
{\mathrel{\hbox{\raise0.3ex\hbox{$>$}\kern-0.8em\lower0.8ex\hbox{$\sim$}}}}
\def\ltapp
{\mathrel{\hbox{\raise0.3ex\hbox{$<$}\kern-0.75em\lower0.8ex\hbox{$\sim$}}}}
\def\app{$\approx$}			% IRAS
\def\lquo{\lq\lq}
\def\rquo{\rq\rq\ }
\def\IR{{\it IRAS }}			% IRAS
\def\fnu{$F_{\nu}$}			% fnu
\def\um{$\mu$m}		        % microns
\def\LS{$L_{\odot}$}			% L sun
\def\lsun{$L_{\odot}$}			% L sun
\def\Lirs{${\rm log\ (L_{ir} / L_{\odot})\ }$} % Lir/Lsun
\def\Lbol{${\rm log\ (L_{bol} / L_\odot)\ }$}   % Lbol/Lsun
\def\LM{${\rm L_{ir} / M(H_2)\ }$}      % L_ir / M(H_2)
\def\LMU{${\rm \lbrack L_\odot M_\odot^{-1} \rbrack}$}  % L/M solar units
\def\Lir{${\rm L_{ir\ }}$}                % Lir
\def\s{${\rm ^{s\ }}$}                  % 's
\def\pwr #1 {$10^{#1}$}			% 10**x
\def\pwrx #1 #2 {$#1 \times$\pwr #2 }	% x*10**y
\def\il{infrared-luminous} 		% infrared-luminous
\def\fd{flux density}			% flux density
\def\lum{luminosity}			% luminosity
\def\lums{luminosities}			% luminosities
\def\EA{et al.}			% et al.
\def\arcs{$^{\prime\prime\ \ }$}			% arcsec
\def\arcm{$^{\prime\ \ }$}				% arcmin
\def\parcs{$\mskip 2mu .\!\!{^{\prime\prime}}$}	% arcsec over period
\def\parcm{$.\!{^{\prime}}$}			% arcmin over period
\def\deg{$^{\circ}$}				% deg
\def\KS{km s$^{-1}$}
\def\ea{{\it et al.}\ }
\def\etal{{\it et al.}\ }
\def\kms{km s^{-1}}
\def \pagebottom   {\footline={\hss\tenrm\folio\hss }}
\def\ffolio{\ifnum\pageno=0        % leave page 1 blank,
{\ }  \else{\rm-- \folio\ --}      % numbers subsequent pages
\fi }
\headline={\hss\ffolio\hss} 	   % numbers at top of page, not at
				   % bottom
\footline={}			   % redefine nopagenumbers macro for
\def\nopagenumbers{\headline={}}	   % top of page numbers

%\def\repagenumbers{\headline={\hss % Turns on page numbering,
%\rm-- \folio\ --\hss}  }           % including on page 1.
%\pageno=11
\nopagenumbers

\parindent=0pt
\newdimen\digitwidth
\setbox0=\hbox{\rm0}
\digitwidth=\wd0
\catcode `?=\active
\def?{\kern\digitwidth}
\hoffset=-.3truein
\hsize=7.25truein

$$
\table\spacing{12pt}
\tablespec{\l\r\r\r\r\r\r\r\r\r\r\r\l\r\r\l\r\r\l\r\r\l}
\body{
\header{Table 1b. Integrated Flux Densities of IRAS Bright Galaxies ($5^\circ < \vert b \vert < 10^\circ$)}
\skip{5pt}
\hline
\skip{2pt}
\hline
\skip{3pt}
&Name&\extend3{RA}&\extend3{Dec}&?cz?&?D?&??m?&\extend{12}{Flux Densities}&\end
\skip{2pt}
\hline
\skip{2pt}
&&&&&&&&&&&\extend3{12\um}&\extend3{25\um}&\extend3{60\um}&\extend3{100\um}&\end
&&H&M&?S?&$^\circ$&$^\prime$&\arcs&km/s&Mpc&&S$_\nu$&$\sigma_\nu$&&
S$_\nu$&$\sigma_\nu$&&S$_\nu$&$\sigma_\nu$&&S$_\nu$&$\sigma_\nu$&&\end
&&&&&&&&&&&Jy?&mJy&?Size&Jy?&mJy&?Size&Jy?&mJy&?Size&Jy?&mJy&?Size&\end
\skip{3pt}
\hline
\skip{5pt}
&IR 01583+6807&1&58&19.8&68&07&14&3577&&-- --&0.36&26&R&0.85&35&R&6.55&147&R&13.55&325&R\end
&UGC 2789&3&31&30.6&67&23&54&:3114&&17.&0.45&33&R&0.76&28&R&5.24&87&U+&10.66&393&U\end
&IR 03582+6012&3&58&15.5&60&12&14&8997&&-- --&0.21&24&R&0.86&28&R&5.77&101&U&\#8.31&643&U\end
&IR 04271+3849&4&27&9.4&38&49&19&:5640&&-- --&\#0.31&20&R&\#0.91&48&U+&\#6.73&65&U&\#10.60&742&U\end
&IR 05083+2441&5&8&21.7&24&41&43&:6979&&-- --&0.21&35&U&0.83&51&U&6.70&92&U&\#8.86&493&U\end
&IR 05129+5128&5&12&58.8&51&28&40&:8224&&-- --&0.21&33&U&0.98&33&U&6.62&51&U&7.60&322&U\end
&IR 05223+1908&5&22&19.6&19&8&8&8867&&-- --&0.96&32&U&2.04&83&U+&\#5.61&201&R&\#11.89&1342&R\end
&MCG+08-11-002&5&36&51.2&49&40&8&:5743&&16&0.57&27&R&1.05&46&R&13.26&32&U&25.33&193&U\end
&IR 05442+1732&5&44&15.9&17&32&42&5582&&-- --&0.53&35&U+&1.79&42&R&10.27&44&U&13.40&256&U\end
&IR 06164+0311&6&16&25.3&3&11&10&2901&&13.1&1.03&29&R&0.92&29&R&8.69&52&U&25.52&470&U\end
\skip{5pt}
&IR 06478-1111&6&47&50.4&-11&11&41&:2602&&-- --&0.41&43&U&0.64&21&U+&6.14&86&U&\#9.94&1582&U\end
&ESO 491-G020&7&7&46.5&--27&29&14&2961&&13.8&0.89&36&U+&2.75&19&R&15.75&54&U&23.41&170&U\end
&ESO 492-G002&7&9&38.9&--26&37&15&2611&&13.0&0.42&20&U+&0.78&23&U+&8.15&37&U+&\#16.94&405&R\end
&ESO 428-G023&7&20&12.0&--29&8&25&3026&&13.4&0.40&22&U+&1.33&21&R&10.29&36&U&17.92&868&U\end
&ESO 428-G028&7&21&40.7&--29&57&14&2258&&14.5&0.47&23&R&0.77&19&R&6.21&26&U+&15.07&264&U\end
&IR 07251-0248&7&25&6.9&--2&48&46&:26249&&-- --&\#0.21&24&U&0.67&34&U&6.71&33&U&6.59&341&U\end
&NGC 2566&8&16&38.1&--25&20&32&1637&&11.8&1.23&26&R&4.04&27&R&24.76&51&R&38.23&173&U+\end
&IR 08355-4944&8&35&30.0&--49&44&00&:7764&&-- --&0.42&25&R&2.33&26&U&9.77&50&U&8.10&815&U\end
&ESO 432-IG006&8&42&25.0&--31&30&45&4846&&-- --&0.58&24&R&0.89&33&R&6.57&43&U+&9.54&330&U\end
&IR 09022-3615&9&2&13.3&--36&15&03&17880&&-- --&0.20&32&U&1.15&21&U&12.00&58&U&11.39&370&U\end
\skip{5pt}
&ESO 126-G002&9&12&15.8&--60&34&56&:2858&&13.6&0.49&24&U+&2.06&19&U&11.86&79&U&16.12&188&U\end
&ESO 091-G016&9&36&57.5&--63&15&37&:2162&&14.1&0.30&15&R&0.80&18&R&6.80&29&U&10.75&103&U\end
&IC 2554&10&7&30.2&--66&47&08&:1474&&12.5&1.10&22&R&2.86&22&R&17.34&35&U&36.48&269&U+\end
&ESO 093-G003&10&57&29.3&--66&3&16&:1890&&-- --&0.68&20&R&0.99&26&R&10.56&66&U+&19.13&575&U\end
&NGC 3882&11&43&36.9&--56&6&32&:1740&&13.0&0.97&28&R&2.00&25&R&20.11&115&R&34.36&509&U\end
&IR 12116-5615&12&11&41.9&--56&15&51&:8125&&-- --&0.37&24&R&1.11&23&U&9.78&103&U&11.10&440&U\end
&IR 13052-5711&13&5&14.7&--57&11&30&:6364&&-- --&0.16&24&U&0.43&25&U&8.35&74&U&\#13.40&685&U\end
&IR 13120-5453&13&12&2.3&--54&53&33&9222&&-- --&0.42&23&U&3.03&24&U&39.71&63&U&45.26&176&U\end
&ESO 173-G015&13&24&12.5&--57&13&51&3006&&-- --&1.21&27&U+&7.38&32&U+&77.52&92&U&88.80&606&U\end
&ESO 174-G005&13&58&55.4&--53&18&04&:3778&&15.8&0.20&24&R&0.46&22&R&5.29&127&U&\#6.00&1276&U\end
\skip{5pt}
&ESO 099-G004&15&20&41.7&--62&56&54&8779&&-- --&0.30&23&U&1.49&37&U+&10.86&128&U&14.95&1311&U\end
&ESO 137-G014&16&12&59.4&--58&11&20&2764&&14.8&0.29&28&R&0.98&28&U+&6.29&147&U&7.73&1723&U\end
&NGC 6156&16&30&28.2&--60&30&55&:3300&&12.3&1.22&15&R&2.73&24&R&17.55&51&R&31.13&858&U\end
&NGC 6215&16&46&47.2&--58&54&32&1560&&12.0&1.97&26&R&3.58&33&R&30.83&105&R&48.70&626&U\end
&NGC 6221&16&48&25.4&--59&8&01&:1440&&10.7&3.15&26&R&7.68&27&R&49.13&70&R&84.48&213&U+\end
&IR 17578-0400&17&57&53.5&--4&0&52&3968&&-- --&0.37&37&R&1.15&39&U&28.91&211&U+&35.16&1766&U\end
&IR 18090+0130&18&9&5.3&1&30&55&8662&&-- --&0.30&21&U&0.81&30&U&8.01&56&U&\#15.91&484&U\end
&IR 18587-1653&18&58&46.5&--16&53&45&14431&&-- --&0.09&28&U&0.34&33&U&5.51&123&U&7.07&890&U\end
&IR 19279+3534&19&27&59.4&35&34&36&4612&&-- --&0.14&30&U&0.46&21&U&5.43&92&U&9.51&324&U\end
&$\ddagger$IR 19542+1110&19&54&13.3&11&10&59&:19473&&-- --&0.08&31&R&0.75&38&R&6.29&47&U&6.78&342&U\end
\skip{5pt}
&MCG+04-48-002&20&26&26.3&25&33&53&4259&&18&0.52&22&U&1.08&26&U&10.27&61&U&18.20&212&U\end
&IR 20351+2521&20&35&9.5&25&21&11&:10102&&-- --&0.23&23&U+&0.77&17&U+&6.23&38&U&9.38&216&U\end
&IR 21101+5810&21&10&8.3&58&10&43&:11688&&-- --&0.20&25&R&0.81&14&R&8.22&65&U+&\#11.66&1097&U\end
&IR 23085+6723&23&8&33.5&67&23&22&1478&&-- --&0.44&24&U&1.96&22&U&7.46&42&U&\#9.23&872&U\end
&IR 23436+5257&23&43&37.9&52&57&20&:10121&&15.3&0.20&31&R&0.85&30&R&5.54&46&U&\#8.63&183&U\end
\hline
\skip{2pt}
\hline
}
\endtable
$$
\hskip 0.5in :\ redshifts from this paper (see text)

\hskip 0.5in \# \ uncertain flux (10--30\%) due to baseline uncertainties and/or blends

\hskip 0.5in $\ddagger$\ tentative identification of H$\alpha$+[NII]; source not listed in NED

\vfill\eject
\bye

