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Table 9:

All short period sdBV stars published to date.
Name Survey name mV \ensuremath {T_{\rm {eff}}} \ensuremath{\log g} \ensuremath{\log y} C $P_{\rm range}$ $A_{\rm max}$ $N_{\rm P}$ References
    mag kK dex dex   s mma    
V361 Hya EC 14026-2647 15.3 34.7 6.10 ... G2 134-144 12 2 1,4
EO Cet PB 8783 12.3 35.7 5.70 ... F0 94-136 9 7 2,4
UX Sex EC 10228-0905 15.9 33.5 6.00 ... G2 140-152 14 3 3,4
V4640 Sgr EC 20117-4014 12.5 34.8 5.87 ... F5 137-158 4 3 4
UY Sex PG 1047+003 13.5 33.2 5.80 -2.00 a,b 104-175 10 18 5,k1
NY Vir PG 1336-018 13.5 31.3 5.60 -2.93 M5 97-205 10 28 6,k2,v2
V2203 Cyg KPD 2109+4401 13.4 31.8 5.79 -2.23 a 182-213 9 8 7,z1,h1
V338 Ser PG 1605+072 12.8 32.3 5.25 -2.53 a 350-573 64 50 8,12
KL UMa Feige 48 13.5 29.5 5.50 -2.93 WD 343-379 6 4 9,h1,o2
DT Lyn PG 0911+456 14.6 31.9 5.77 -2.55 a 149-192 7 7 10,r5
KY UMa PG 1219+534 13.2 34.3 5.95 -1.50 a,b 128-149 9 4 10,h1
AQ Col EC 05217-3914 15.6 31.3 5.76 -3.00 ... 215-218 8 8 11,r3
V1405 Ori KUV 04421+1416 15.1 32.0 5.72 -2.50 dM 185-232 20 7 11,r4
V2214 Cyg KPD 1930+2752 13.8 35.2 5.61 -1.50 WD 145-332 5 44 13,g1
LM Dra PG 1618+563B 13.5 33.9 5.80 -1.60 F3c 108-144 6 2 14,r3
DV Lyn HS 0815+4243 16.1 33.7 5.95 -2.10 ... 126-131 7 2 15
V384 Peg HS 2149+0847 16.5 35.6 5.90 -1.80 ... 142-159 11 5 15
V391 Peg HS 2201+2610 13.6 29.3 5.40 -3.00 Pl 347-351 10 3 15,s1
LS Dra HS 1824+5745 15.6 33.1 6.00 -1.52 ... 139 5 1 16,r1
V387 Peg HS 2151+0857 16.5 34.5 6.10 -1.37 F-K 129-151 4 5 16,r1
V429 And HS 0039+4302 15.1 32.4 5.70 -2.20 a 182-235 8 4 16
V1636 Ori HS 0444+0458 15.4 33.8 5.60 -1.85 a 137-168 13 2 16
EK Psc PG 0014+067 16.3 34.1 5.77 -1.68 b 137-169 3 13 17,c1,v1
EP Psc PG 2303+019 16.2 35.3 5.74 -1.70 MS? 128-145 16 3 18
QQ Vir PG 1325+101 13.8 34.8 5.81 -1.65 a,b 94-168 26 14 18,t1,s2
DW Lyn HS 0702+6043 14.7 28.4 5.35 -2.70 a 363-384 22 2 19,s3
V1078 Her PG 1613+426 14.1 34.4 5.97 -1.65 a 144 5 1 20
PG 0048+091 ... 14.3 34.2 5.69 -3.00 F5 90-192 6 28 $^{21,r3,\ddag }$
PG 0154+182 ... 15.3 35.8 5.80 -1.67 G-K 110-164 10 6 $^{21,r1,\ddag }$
J1717+5805 ... 16.7 34.4 5.75 -1.80 G9 137-144 6 2 $^{22,\dag }$
Balloon 090100001 ... 11.8 29.4 5.33 -2.54 a,b 178-356 60 3 23,o1
PG 1419+081 ... 14.9 33.3 5.85 -1.80 G5 143 7 1 $^{24,\dag }$
J1445+0002 ... 17.4 35.9 5.75 -1.60 G0 120-142 8 3 $^{24,\dag }$
J1642+4252 ... 15.7 32.4 5.80 -2.00 G0 130-138 3 2 $^{24,\dag }$
EC 09582-1137 PG 0958-116 15.2 34.8 5.79 -1.68 a 136-169 8 5 25,r6
EC 11583-2708 ... 14.4 ... ... ... MS 114-149 3 4 25
EC 20338-1925 BPS CS 22880-18 15.6 35.5 5.75 -1.71 a 135-168 27 5 $^{25,\ddag }$
RAT J0455+1305 ... 17.2 29.2 5.20 ... ... 363-374 19 2 26,b1
PG 1657+416 ... 15.9 32.2 5.80 -1.60 G5 125-143 4 5 $^{27,\dag }$
2M0415+0154 ... 14.0 34.0 5.80 -1.60 a,b 144-149 6 3 28
EC 01541-1409 ... 12.2 37.1 5.71 -1.21 a 78-146 10 6 $^{29,\ddag }$
EC 22221-3152 ... 13.4 35.1 5.85 -1.47 a 84-176 9 10 $^{29,\ddag }$
JL 166 ... 15.0 34.4 5.75 -0.80 MS 97-167 4 10 30
CS 1246 CS 124636.2-631549 14.6 28.5 5.46 -2.00 b 372 35 1 31
HE 0230-4323 ... 13.8 31.6 5.60 -2.58 dM 282-310 8 3 32,l1
HE 2151-1001 ... 15.6 35.0 5.70 -1.60 MS 126-128 3 2 $^{\dag ,l1}$
HS 2125+1105 ... 16.3 32.5 5.76 -1.86 a 136-146 4 1 $^{\dag ,l1}$
PG 1033+201 ... 15.4 31.5 ... ... F9 146-171 5 2 $^{\dag ,a1}$
HE 1450-0957 EC 14507-0957 15.3 34.6 5.79 -1.29 MS 118-139 7 3 $^{\dag ,l1}$

Notes. Pulsators discovered by our survey are listed with their names in bold face, and hybrid DW Lyn type pulsators in italics. C gives the class of the companion, where available, and the notes in that column mark: (a) no IR excess from 2MASS or SDSS photometry; (b) no detectable RV variations on a time-scale of hours or days; (c) the F3 companion to LM Dra is separated by 3.7'', but it is unclear whether the subdwarf itself is single. $P_{\rm range}$ gives the range of periods observed, excluding marginal detections, harmonics and g-modes, $A_{\rm max}$gives the highest amplitude reported, and $N_{\rm P}$ the number of independent periods reported.

References. Discovery papers: 1 Kilkenny et al. (1997); 2 Koen et al. (1997); 3 Stobie et al. (1997a); 4 O'Donoghue et al. (1997); 5 Billeres et al. (1997); O'Donoghue et al. (1998); 6 Kilkenny et al. (1998); 7 Koen (1998); Billeres et al. (1998); 8 Koen et al. (1998a); 9 Koen et al. (1998b); 10 Koen et al. (1999b); 11 Koen et al. (1999a); 12 Kilkenny et al. (1999); 13 Billéres et al. (2000); 14 silvotti00; 15 ostensen01a; 16 ostensen01b; 17 Brassard et al. (2001); 18 silvotti02a; 19 Dreizler et al. (2002); 20 Bonanno et al. (2003); 21 Koen et al. (2004); 22 solheim04; Aerts et al. (2006); 23 Oreiro et al. (2004); 24 solheim06; 25 Kilkenny et al. (2006); 26 Ramsay et al. (2006); 27 oreiro07; 28 oreiro09; 29 Kilkenny et al. (2009); 30 Barlow et al. (2009); 31 Barlow et al. (2010); 32 Koen (2007); Kilkenny (priv.comm.); $^{\dag }$this paper. Supplementary data: a1 Allard et al. (1994); b1 Baran & Fox Machado (2010); c1 Charpinet et al. (2005); g1 Geier et al. (2007); h1 Heber et al. (2000); k1 Kilkenny et al. (2002); k2 Kilkenny et al. (2003); l1 Lisker et al. (2005); o1 Oreiro et al. (2005); o2 O'Toole et al. (2004); r1 Reed et al. (2006); r2 Reed et al. (2007a); r3 Reed et al. (2007b); r4 Reed et al. (2010); r5 Randall et al. (2007); r6 Randall et al. (2009b); s1 Silvotti et al. (2007,2002a); s2 Silvotti et al. (2006); s3 Schuh et al. (2006); t1 Telting & Østensen (2004); v1 Vuckovic et al. (2006); v2 Vuckovic et al. (2007); z1 Zhou et al. (2006); $^\ddag $ Our determination of \ensuremath {T_{\rm {eff}}}, \ensuremath{\log g}and \ensuremath{\log y}.


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