Table 1: 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) Houk & Cowley (1975); (2) Houk (1978); (3) Houk (1982); (4) Houk & Smith-Moore (1988); (5) Houk & Swift (1999); (6) Hill (1970).
        V B-V U-B    
HD CPD/BD ASAS name N [mag] [mag] [mag] MK sp. type Notes
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


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


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


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)  


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 $^{\prime\prime}$


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}$2491 140701-6834.1 2 9.60 +0.05 - B1 III (1) ALS 3196
123077 -42$^{\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


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)  


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


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)  


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)  


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