\begin{table}%t1
\caption{\label{bc-new}New $\beta$~Cephei stars.  $N$ is the number of independent modes found in the ASAS-3 photometry,
the remaining columns are self-explanatory. References to the MK spectral types in the eighth column are the following:
(1) \citet{houk1}; (2) \citet{houk2}; (3) \citet{houk3}; (4)~\citet{houk4}; (5) \citet{houk5}; (6) \citet{hill70}.}
\small%\centering
\par
\begin{tabular}{rcccrrrll}
\hline \hline
& & & & \multicolumn{1}{c}{$V$} & $B-V$ & $U-B$ & &  \\
HD & CPD/BD & ASAS name & $N$ & [mag] & [mag] & [mag] & MK sp.~type& Notes \\
\hline 
 46994 & $-$25$^\circ$1525 & 063513$-$2550.4 & 1 & 7.86 & $-$0.17 & --   & B2/3 V (4) & in CMa OB2\\
 48553 & $+$02$^\circ$1369 & 064410$+$0223.5 & 1 & 9.03 & -- & -- & B2 III (5) & in the CoRoT field\\
 67600 & $-$20$^\circ$3392 & 080754$-$2109.0 & 1 & 9.18 & -- & -- & B3/5 V (4) &\\
 68962 & $-$35$^\circ$2054 & 081323$-$3618.7 & 1 & 7.34 & $+$0.15 & $-$0.65 & B2/3 V (3) &in BH 23\\
 69016 & $-$27$^\circ$2973 & 081401$-$2743.1 & 1 & 10.22 & -- & -- & B3 IV (3) &\\
 69824 & $-$48$^\circ$1585 & 081638$-$4826.2 & 1 & 9.10 & -- & -- & B4/6 V (2) &\\
 73568 & $-$44$^\circ$2824 & 083719$-$4512.5 & 2 & 8.35 & $+$0.30 & $-$0.57 & B2/3 IV (2)& in Vela OB1\\
 74339 & $-$47$^\circ$2545 & 084133$-$4801.5 & 6 & 9.30 & $+$0.14 & $-$0.67 & B2/3 II/III (2) & in IC 2395\\
 77769 & $-$46$^\circ$3350 & 090248$-$4657.9 & 1 & 9.38 & -- & -- & B3 IV (2) & in Platais 9\\
 86085 & $-$38$^\circ$3738 & 095519$-$3845.8 & 1 & 8.94 & $-$0.09 & $-$0.85 & B1 Vn (6) &halo star\\
\noalign{\medskip}
 86214 & $-$59$^\circ$1528 & 095458$-$5949.8 & 6 & 9.21 & $-$0.02 & $-$0.79 & B2 Ib (1)&\\
 86248 & $-$30$^\circ$3001 & 095633$-$3126.5 & 1 & 9.63 & $-$0.19 & $-$0.89 & B2 III (3) &high-velocity star, very distant\\
 87592 & $-$58$^\circ$1860 & 100409$-$5922.9 & 5 & 8.96 & -- & -- & B1 IV (1) & \\
 88844 & $-$60$^\circ$1765 & 101302$-$6110.7 & 2 & 8.53 & $-$0.16 & $-$0.93 & B0.5 III (1) & ALS 1453\\
 90075 & $-$59$^\circ$2079 & 102206$-$6011.2 & 1 & 8.88 & $+$0.07 & $-$0.76 & B1 II (1) & ALS 1517\\
 90987 & $-$57$^\circ$3308 & 102849$-$5746.0 & 4 & 9.64 & $+$0.13 & $-$0.70 & B1/2 III/IVp (1) & ALS 1601, in IC 2581 ?\\
 91651 & $-$59$^\circ$2214 & 103330$-$6007.7 & 2 & 8.85 & $-$0.01 & $-$0.89 & O8/9 V (1) & ALS 1647, in Car OB1\\
 92291 & $-$60$^\circ$2077 & 103756$-$6116.5 & 5 & 9.07 & $-$0.07 & $-$0.86 & B2 Ib/II (1) & ALS 1702\\
 93113 & $-$57$^\circ$3449 & 104400$-$5741.1 & 1 & 8.71 & $+$0.03 &$-$0.76 & B1/2 II/III (1) & ALS 1818\\
 93341 & $-$56$^\circ$3759 & 104524$-$5659.4 & 1 & 9.64 & $+$0.02 & $-$0.74 & B1/2 II/III (1) & ALS 1876\\
\noalign{\medskip}
 94065 & $-$61$^\circ$1905 & 105007$-$6148.3 & 5 & 8.95 & $-$0.05 & $-$0.83 & B0/1 III-IV (1) & \\
 94345 & $-$59$^\circ$2802 & 105210$-$5957.3 & 3 & 9.00 & $+$0.06 & $-$0.77 & B0/1 IV (1) & \\
 94900 & $-$59$^\circ$2859 & 105611$-$5955.8 & 1 & 9.25 & $+$0.17 & $-$0.66 & B1/2 III (1) & ALS 2034\\
 95568 & $-$61$^\circ$2021 & 110040$-$6236.9 & 2 & 9.56 & $+$0.12 & -- & O9/B0 V (1) & ALS 2084\\
 96882 & $-$60$^\circ$2553 & 110824$-$6117.1 & 1 & 9.03 & $-$0.03 & $-$0.86 & B1 II/III (1) &\\
 96901 & $-$63$^\circ$1845 & 110820$-$6436.1 & 2 & 8.87 & $+$0.20 & $-$0.62 & B1 III/IV (1) &\\
 97629 & $-$60$^\circ$2677 & 111308$-$6106.8 & 1 & 9.53 & $+$0.11 & $-$0.65 & B3/5 Ib/II (1) &  ALS 2250\\
 98260 & $-$60$^\circ$2783 & 111719$-$6130.7 & 3 & 9.70 & $+$0.26 & $-$0.63 & B1/2 Ib/II (1) & ALS 2292\\
 99024 & $-$59$^\circ$3411 & 112303$-$6031.2 & 1 & 9.66 & $+$0.03 & $-$0.77 & B2 Ib/II (1) & ALS 2327\\
 99205 & $-$69$^\circ$1537 & 112356$-$7008.0 & 2 & 9.59 & $+$0.01 & $-$0.73 & B1 III (1) & ALS 2336\\
\noalign{\medskip}
100355 & $-$61$^\circ$2391 & 113216$-$6232.8 & 3 & 9.23 & 0.00 & $-$0.67 & B2/3 III (1) &\\
101794 & $-$61$^\circ$2541 & 114225$-$6228.6 & 2 & 8.68 & $+$0.06 & $-$0.74 & B0/1 n (1) & ALS 2460, eclipsing, Be star,\\
&&&&&&&&in Stock 14\\
101838 & $-$61$^\circ$2550 & 114249$-$6233.9 & 1 & 8.42 & $+$0.02 & $-$0.81 & B0.5/1 III (1) & ALS 2463, eclipsing, in Stock 14\\
102505 & $-$69$^\circ$1588 & 114720$-$7025.0 & 2 & 9.02 & $+$0.08 & -- & B1 IV (1) & ALS 2495\\
103007 & $-$61$^\circ$2696 & 115118$-$6159.8 & 3 & 9.29 & $-$0.01 & $-$0.82 & B2/3 (III) (1)& ALS 2519\\
103320 & $-$59$^\circ$3910 & 115341$-$6016.0 & 1 & 8.82 & $-$0.03 & -- & B2 III (1) & \\
103764 & $-$61$^\circ$2814 & 115652$-$6236.6 & 1 & 9.48 & $-$0.06 & $-$0.80 & B2 II/III (1) &\\
104257 & $-$65$^\circ$1757 & 120012$-$6604.7 & 1 & 8.85 & $+$0.05 & $-$0.73 & B1/2 II/III (1) & ALS 2562\\
104465 & $-$62$^\circ$2526 & 120137$-$6333.8 & 2 & 9.07 & $-$0.05 & $-$0.81 & B2 II/III (1) & \\
104795 & $-$58$^\circ$4048 & 120400$-$5843.4 & 1 & 9.09 & $+$0.11 & -- & B2 III (1) &\\
\noalign{\medskip}
106345 & $-$67$^\circ$1921 & 121416$-$6744.4 & 1 & 9.08 & -- & -- & B2 III (1) &\\
108628 & $-$61$^\circ$3220 & 122906$-$6228.0 & 2 & 9.16 & -- & -- & B2 II (1) &\\
108769 & $-$33$^\circ$3261 & 123003$-$3429.9 & 1 & 9.03 & -- & -- & B2 III (3) & \\
110498 & $-$60$^\circ$4253 & 124316$-$6138.9 & 1 & 9.67 & $+$0.49 & $-$0.49 & B0.5 III (1) & ALS 2737, in Cen OB1\\
111377 & $-$60$^\circ$4309 & 124938$-$6057.9 & 1 & 9.52 & $+$0.13 & $-$0.68 & B2/5 II-III (1) & ALS 2775\\
111578 & $-$59$^\circ$4488 & 125057$-$6026.8 & 1 & 9.13 & $+$0.16 & $-$0.57 & B2/3 II (1) & ALS 2785\\
113013 & $-$59$^\circ$4653 & 130141$-$6026.4 & 2 & 9.40 & $+$0.12 & -- & B2 III (1) & ALS 2871\\
114444 & $-$74$^\circ$1029 & 131304$-$7518.9 & 2 & 10.32 & $-$0.02 & $-$0.80 & B1 II/III (1) & ALS 2963\\
114733 & $-$57$^\circ$5952 & 131330$-$5821.7 & 1 & 9.52 & $+$0.27 & $-$0.55 & B2/3 III (1) & ALS 2980\\
115533 & $-$61$^\circ$3586 & 131901$-$6153.7 & 1 & 10.04 & $+$0.08 & $-$0.76 & B2/5 (Ib/II) (1) & ALS 3026, Vis.~double, Sep.~6\arcsec  \\
\noalign{\medskip}
116538 & $-$51$^\circ$6048 & 132512$-$5150.5 & 1 & 7.90 & $-$0.06 & $-$0.89 & B2 Ib/II (2) &  \\
116827 & $-$61$^\circ$3706 & 132735$-$6207.1 & 2 & 9.51 & $+$0.11 & $-$0.57 & B2/5 (Vn) (1) & Be star\\
117357 & $-$61$^\circ$3760 & 133116$-$6144.0 & 2 & 9.02 & $+$0.23 & $-$0.72 & O9.5/B0 V (1) & ALS 3103, Be star\\
117687 & $-$60$^\circ$4759 & 133330$-$6126.8 & 1 & 9.33 & $+$0.12 & $-$0.71 & B2 Ib/II (1) & ALS 3115\\
117704 & $-$61$^\circ$3793 & 133337$-$6219.1 & 1 & 8.89 & $+$0.20 & $-$0.59 & B1/2 III (1) & ALS 3116, close to WR 55\\
119252 & $-$47$^\circ$6162 & 134309$-$4748.3 & 1 & 10.34 & -- & -- & B3 III (2) &\\
119910 & $-$60$^\circ$4978 & 134754$-$6053.0 & 2 & 8.31 & $-$0.07 & -- & B2 III/IV (1) &\\
122831 & $-$67$^\circ$2491 & 140701$-$6834.1 & 2 & 9.60 & $+$0.05 & -- & B1 III (1) & ALS 3196\\
\hline
123077 & $-$42$^\circ$6537 & 140637$-$4327.8 & 4 & 10.30 & $-$0.23 & -- & B2/3 II (2) &\\
126357 & $-$59$^\circ$5569 & 142709$-$5944.2 & 3 & 9.07 & $+$0.22 & $-$0.64 & B1 III (1) & ALS 3238, in NGC 5606\\
131805 & $-$73$^\circ$1416 & 150055$-$7347.7 & 1 & 8.47 & -- & -- & B5 V (1) &long-term variability superimposed\\
132320 & $-$59$^\circ$5775 & 150106$-$5953.7 & 1 & 9.40 & $+$0.31 & $-$0.53 & B1 III (1) &\\
137405 & $-$60$^\circ$5814 & 152854$-$6048.1 & 1 & 9.36 & $+$0.13 & $-$0.64 & B0.5/1 Iab (1)& ALS 3356\\
142754 & $-$40$^\circ$7155 & 155749$-$4059.8 & 1 & 8.60 & $+$0.17 & $-$0.60 & B2 III (2) &\\
145537 & $-$34$^\circ$6468 & 161255$-$3439.3 & 2 & 10.41 & $+$0.10 & $-$0.78 & B2 Ib/II (3)&\\
146442 & $-$45$^\circ$7845 & 161823$-$4550.4 & 3 & 9.04 & $+$0.30 & $-$0.51 & B2 III (2)&\\
147421 & $-$53$^\circ$7928 & 162445$-$5327.8 & 1 & 9.02 & $+$0.09 & $-$0.81 & B0 II (1)& ALS 3596\\
149100 & $-$53$^\circ$8064 & 163521$-$5338.9 & 1 & 7.19 & $-$0.06 & $-$0.76 & B2 III (1) &\\
150927 & $-$37$^\circ$6738 & 164544$-$3810.1 & 2 & 9.44 & $+$0.32 & $-$0.52 & B2/3 Ib (3)&\\
151158 & $-$42$^\circ$7512 & 164734$-$4252.7 & 1 & 8.20 & $+$0.22 & $-$0.49 & B2 Ib/II (2)& ALS 3754\\
\noalign{\medskip}
152060 & $-$41$^\circ$7683 & 165300$-$4124.5 & 2 & 9.58 & $+$0.06 & $-$0.73 & B1 III (2) &\\
152162 & $-$45$^\circ$8186 & 165354$-$4600.9 & 2 & 8.59 & $+$0.18 & -- & B2 III (2) &\\
152372 & $-$48$^\circ$8913 & 165517$-$4848.3 & 3 & 8.85 & $+$0.20 & $-$0.60 & B2 III/IV (2)&\\
153772 & $-$50$^\circ$9813 & 170400$-$5105.0 & 1 & 8.32 & $+$0.06 & $-$0.61 & B2 V (2)& in R assoc.~vdBH81a\\
154500 & $-$34$^\circ$6724 & 170721$-$3428.7 & 2 & 9.94 & $+$0.22 & $-$0.56 & B2 Iab/b (3) &\\
155407 & $-$45$^\circ$8378 & 171332$-$4527.2 & 1 & 9.52 & -- & -- & B2 II (2) &\\
156172 & $-$41$^\circ$7933 & 171800$-$4203.6 & 1 & 8.18 & $+$0.40 & $-$0.58 & O9.5/B0.5 Ia/Iab (2) & ALS 4037\\
156321 & $-$32$^\circ$4462 & 171820$-$3219.6 & 1 & 8.15 & $+$0.01 & $-$0.77 & B2 V (3)&\\
159792 & $-$46$^\circ$8786 & 173850$-$4618.9 & 3 & 9.43 & $+$0.15 & $-$0.63 & B2 II (2)&\\
161633 & $-$46$^\circ$8909 & 174900$-$4656.4 & 4 & 9.94 & $+$0.12 & $-$0.95 & B1 Iab/b (2)&\\
\noalign{\medskip}
164188 & $-$15$^\circ$4767 & 180039$-$1548.1 & 1 & 8.67 & $+$0.19 & $-$0.71 & B1 Ib/II (4)& ALS 4546\\
164741 & $-$25$^\circ$6269 & 180344$-$2518.7 & 5 & 9.03 & $+$0.31 & $-$0.55 & B2 Ib/II (4) & ALS 4590\\
165955 & $-$34$^\circ$7625 & 180958$-$3452.1 & 2 & 9.20 & $-$0.05 & $-$0.82 & B2 II/III (3) & ALS 4702, high-velocity star\\
166304 & $-$16$^\circ$4739 & 181043$-$1642.8 & 3 & 9.33 & $+$0.19 & $-$0.63 & B2 II (4) & \\
167003 & $-$33$^\circ$4963 & 181442$-$3308.5 & 4 & 8.45 & $-$0.13 & $-$0.94 & B1 Ib/II (3) & ALS 4801, V4386 Sgr, eclipsing\\
167451 & $-$13$^\circ$4897 & 181555$-$1334.5 & 1 & 8.24 & $+$0.78 & $-$0.29 & B1 Ib (4) & ALS 4844, in Ser OB1\\
168015 & $-$13$^\circ$4919 & 181822$-$1323.2 & 2 & 9.11 & $+$0.36 & -- & B3/5 II (4) & ALS 9488\\
168050 & $-$19$^\circ$6762 & 181839$-$1906.2 & 2 & 9.81 & -- & -- & B3/5 Ib (4) & eclipsing\\
168675 & $-$17$^\circ$5154 & 182143$-$1753.8 & 2 & 8.94 & $+$0.28 & -- & B2 Ib/II (4) & ALS 4964\\
168750 & $-$26$^\circ$6414 & 182221$-$2625.0 & 3 & 8.27 & $+$0.08 & $-$0.74 & B1 Ib (3) & ALS 4969\\
\noalign{\medskip}
169173 & $-$17$^\circ$5179 & 182408$-$1751.8 & 1 & 9.93 & -- & -- & B3 Ib (4) &\\
169601 & $-$17$^\circ$5192 & 182607$-$1747.3 & 3 & 9.88 & -- & -- & B0/1 Iab/b (4) &\\
171141 & $-$46$^\circ$9389 & 183516$-$4556.4 & 1 & 8.37 & $-$0.22 & $-$0.97 & B2 II/III (2) & halo star\\
171305 & $-$04$^\circ$4497 & 183416$-$0448.8 & 1 & 8.70 & $+$0.45 & -- & B2 II (5) & ALS 9749, in the CoRoT field\\
171344 & $-$13$^\circ$5039 & 183457$-$1352.2 & 1 & 9.52 & $+$0.29 & -- & B2 Ia (4) & ALS 9758\\
172140 & $-$29$^\circ$5634 & 183948$-$2920.4 & 5 & 9.95 & $-$0.05 & $-$0.89 & B1 II (3) &\\
172427 & $-$10$^\circ$4749 & 184032$-$1043.1 & 1 & 9.46 & $+$0.48 & $-$0.44 & B0.5/1 Ib (5) & ALS 9832, in Sct OB2\\
173006 & $-$05$^\circ$4737 & 184326$-$0546.8 & 1 & 10.03 & $+$0.27 & $-$0.55 & B0.5 IV (5) & ALS 9902, in the CoRoT field\\
173502 & $-$30$^\circ$5678 & 184656$-$2957.6 & 4 & 9.73 & $-$0.10 & $-$0.91 & B1/2 Ib (3) & halo star\\
178987 & $-$47$^\circ$9208 & 191259$-$4709.7 & 1 & 9.83 & -- & -- & B2 II (2) &\\
\noalign{\medskip}
180032 & $-$14$^\circ$5352 & 191531$-$1355.1 & 2 & 9.49 & $-$0.07 & -- & B2 III/IV (4) & ALS 10219\\
186610 & $-$03$^\circ$4698 & 194527$-$0309.1 & 4 & 9.67 & $-$0.01 & $-$0.77 & B2 Ib/II (5) & ALS 10480, in the CoRoT field\\
187536 & $-$28$^\circ$7032 & 195125$-$2813.5 & 1 & 9.46 & $-$0.08 & $-$0.86 & B3 II (3) &\\
\hline
\end{tabular}
%\vspace*{2mm}
\end{table}