% TABLE1.TEX -- AASTeX sample table 1. \documentstyle[aj_pt]{article} \begin {document} % The following gobbledygook is done so that this particular table % paginates in a way that "looks nice" regardless of whether apjpt % or aj_pt styles are chosen. The \tablebreak commands that appear % after some of the lines force page breaks when the apjpt style is % selected, but act simply as line delimiters for aj_pt. \makeatletter \def\jnl@aj{AJ} \ifx\revtex@jnl\jnl@aj\let\tablebreak=\nl\fi \makeatother % From here on, the file contains tabular data as an author might % prepare it. \tablenum{1C} \begin{planotable}{rccrrrrrrccrrl} \tablewidth{0pc} \tablecaption{Early-type stars, giants and degenerates} \tablehead{ \colhead{ } & \colhead{name} & \colhead{bin.} & \colhead{} & \colhead{$\alpha$} & \colhead{2000} & \colhead{} & \colhead{$\delta$} & \colhead{} & \colhead{Src.} & \colhead{V} & \colhead {M$_V$} &\colhead{r} & \colhead{Sp}} \startdata 176&GJ 1023 A &p& 0& 54& 18.4& 69& 2& 50& 3& 9.70& 4.4& 115& G0 \nl 177&GJ 1023 B &s& 0& 54& 18.4& 69& 2& 50& 3& 10.40& 4.9& 125& G0 \nl 183&G269-061 & & 0& 56& 19.5&-28& 8& 21& 3& 10.96& 6.7& 70& K3 \nl 185&Gl 44 & & 0& 57& 20.2& -1& 48& 56& 3& 9.46& 6.2& 45& K1 \nl 188&GJ 2017 & & 0& 59& 51.5&-25& 35& 25& 3& 9.87& 4.1& 145& G0 \nl 192&GJ 2019 & & 1& 0& 37.0&-26& 38& 15& 3& 10.11& 5.6& 80& G5 \nl 198&GJ 2020 & & 1& 1& 49.2&-25& 53& 12& 3& 9.75& 2.9& 230& F2 \nl 201&RGO 2913 & & 1& 1& 54.2&-25& 45& 38& 3& 11.84& 7.8& 65& K5 \nl 228&Gl 53.3 & & 1& 9& 43.4& 35& 37& 15& 4& 2.05& 0.5& 20\tablenotemark{a}& M0 III \nl 306&BD+63 219 & & 1& 41& 9.9& 63& 48& 43& 3& 10.07& 3.9& 175& A5 \nl 387&Rob 115 & & 2& 10& 13.4& 11& 31& 58& 3& 12.72& -0.8& 5000\tablenotemark{b}& M4 III \nl 579& AC +0:641-15& & 3& 14& 20.3& 0& 39& 11& 3& 9.40& 6.7& 35\tablenotemark{b}& G3 \nl 602&LP355-65 &s& 3& 22& 52.7& 27& 8& 44& 2& 18.00& 15.6& 30\tablenotemark{c}& DC \nl 666&Wo 9124 & & 3& 44& 20.0& 24& 47& 45& 3& 10.66& 5.1& 130& K1 \nl 667&Wo 9125 & & 3& 44& 20.4& 24& 46& 21& 3& 10.81& 5.3& 125& K5 \nl 669&Wo 9127 & & 3& 44& 22.1& 24& 45& 57& 4& 11.09& 6.2& 95& G0 \nl 720&Gl 160.2 & & 4& 6& 34.7&-20& 51& 0& 3& 9.68& 7.7& 25& K4 \nl 755&Gl 168.1 & & 4& 22& 10.3& 19& 28& 59& 3& 15.04& 4.8& 450& G0\tablenotemark{d} \nl 757&LH190 & & 4& 22& 16.5& 15& 30& 44& 2& 17.00& 9.0& 100\tablenotemark{b}& M1?\tablenotemark{d} \nl 763&vA342 & & 4& 25& 0.2& 16& 59& 4& 3& 10.31& 7.0& 45& K3 \nl 820&AC+19:1513-210 & & 4& 43& 26.5& 19& 0& 18& 3& 13.40& 6.5& 240\tablenotemark{b}& G0 \nl 909&GJ 2040 & & 5& 19& 34.9& 3& 52& 24& 3& 9.86& 7.9& 25& K0 \nl 985&Gl 223.1 & & 5& 54& 34.0& -9& 23& 34& 3& 10.71& 7.7& 40& K4 \nl 1306&V518 & & 8& 18& 44.3&-15& 12& 7& 3& 9.84& 7.5& 30& K3 \nl 1314&Gl 305.1 & & 8& 23& 30.7& 21& 50& 58& 3& 9.54& 7.6& 25& K3 \nl 1354&GJ 1113 & & 8& 40& 36.7& 43& 6& 51& 3& 9.32& 7.3& 25& K2 \nl 1384&GJ 1115 & & 8& 53& 47.3& 35& 13& 21& 3& 9.30& 7.8& 20& K3 \nl 1418&GJ 1120 A &p& 9& 1& 17.5& 15& 15& 57& 3& 9.43& 7.9& 20& K4 \nl 1597&Gl 383.1 & & 10& 13& 57.3& 52& 30& 28& 3& 9.53& 7.5& 25& K2 \nl 1689&Gl 402.1 & & 10& 52& 2.6& 0& -9& 35& 3& 10.20& 6.3& 60& K0 \nl 1714&Gl 409 & & 11& 1& 57.2&-17& 57& 23& 3& 11.87& 4.8& 265& G5 \nl 1885&Gl 454.1 & & 12& 1& 7.2& -1& 43& 54& 3& 10.96& 7.5& 50& K3 \nl 1912&Wo 9394 & & 12& 12& 1.4& 13& 15& 43& 3& 10.18& 3.9& 180& F2 \nl 2034&Gl 489 & & 12& 57& 44.0&-14& 27& 47& 3& 9.12& 7.6& 20& K3 \nl 2053&Gl 499.1 & & 13& 6& 22.5& 22& 36& 56& 3& 5.60& 0.0& 130\tablenotemark{e}& M5 III \nl 2149&Gl 518.2B &s& 13& 37& 13.8& 30& 5& 12& 3& 10.51& 6.0& 80& K1 \nl 2197&GJ 1180 & & 13& 51& 59.5& 26& 38& 10& 3& 10.83& 5.5& 115& G5 \nl 2213<T 5453 & & 13& 59& 7.6&-23& 33& 28& 4& 14.93& 14.7& 11\tablenotemark{f}& DA \nl 2287&Gl 550.1 & & 14& 27& 45.3& 23& 50& 26& 3& 10.92& 7.9& 40& K4 \nl 2328&Gl 561 & & 14& 43& 19.2& 26& 44& 58& 3& 9.67& 5.4& 70& K0 \nl 2335&Gl 562 & & 14& 46& 23.3& 16& 29& 55& 3& 9.25& 8.4& 15& K4 \nl 2347<T 14398 &s& 14& 51& 2.3& 9& 43& 23& 3& 8.90& 7.1& 23\tablenotemark{c}& K4 \nl 2609&Gl 629.2A &p& 16& 34& 42.3& -4& 13& 39& 3& 9.62& 5.6& 65& F8 \nl 2656&BD+38 2847 & & 16& 50& 54.2& 38& 9& 0& 3& 10.55& 7.1& 50\tablenotemark{b}& K3 \nl 2759&AC+02:2142-173& & 17& 26& 10.6& 1& 48& 20& 3& 10.90& 5.1& 145& G0 \nl 2768&Gl 677 A &p& 17& 29& 20.1& 29& 23& 32& 3& 9.55& 7.6& 25& K3 \nl 2807&Gl 690 A &p& 17& 38& 33.9& 71& 19& 53& 3& 9.20& 7.2& 25& K4 \nl 2856&Gl 700.1C &s& 18& 3& 13.9& -8& 11& 25& 1& 9.40& 5.9& 50\tablenotemark{b}& G1 \nl \phantom{0} 3022&LP336-6 & & 19& 11& 5.9& 32& 39& 59& 3& 10.48& 0.5& 1000\tablenotemark{b}& M0 III \nl 3030&Gl 748.2A &p& 19& 14& 58.6& 2& 9& 47& 3& 10.20& 7.8& 30& K2 \nl 3309&Wo 9723 & & 21& 8& 44.0& 47& 9& 8& 1& 10.78& 6.6& 70& K2 \nl 3315&GJ 2152 & & 21& 13& 29.1& 7& 26& 13& 4& 16.17& 16.0& 11\tablenotemark{f}& DA \nl 3438&BD+32 4292A &p& 21& 55& 38.6& 33& 2& 11& 3& 10.00& 5.0& 100\tablenotemark{b}& G0 \nl 3462&AC+01:2189-92& & 22& 3& 28.6& 1& 35& 48& 3& 10.34& 5.5& 95& K1 \nl 3493&Wo 9775 & & 22& 14& 24.0& -8& 44& 38& 3& 11.85& 6.0& 150\tablenotemark{b}& K1 \nl 3495&Gl 851.4 & & 22& 14& 0.9& 57& 7& 12& 3& 9.83& 5.5& 75& K0 \nl 3555&VVO 271 & & 22& 37& 11.9& 0&-39& 1& 3& 10.50& 6.0& 80\tablenotemark{b}& G8 \nl 3585&BD+43 4306 & & 22& 47& 31.6& 44& 33& 11& 3& 9.60& 3.7& 150\tablenotemark{b}& G0 \nl 3692&Wo 9826 & & 23& 25& 55.3& 29& 11& 42& 3& 11.05& 6.5& 80& K1 \nl 3734&LP463-28 &s& 23& 38& 58.6& 21& 1& 23& 2& 16.40& 14.3& 26\tablenotemark{c}& DC \nl 3798&Wo 9848 & & 0& 1& 54.4& 26& 0& 38& 1& 11.30& 6.5& 90& K0 \nl \tablenotetext{a} {distance from CNS3;} \tablenotetext{b} {distance estimated from the spectral type;} \tablenotetext{c} {distance estimated from companion star;} \tablenotetext{d} {757: foreground reddening probably present;} \tablenotetext{e} {FS Comae - distance based on Jura \& Kleinmann's M$_K$;} \tablenotetext{f} {distance from McCook \& Sion (M$_V$, B-V) relations} \tablecomments{V magnitudes are from the CNS3; absolute magnitudes are derived using Reid \& Murray's (1991) (M$_V$, (B-V)) relation unless otherwise indicated.} \end{planotable} \end {document}