**Table 1:** $\gamma$ Doradus stars candidates observed at OHP showing LPV. The first 2 columns give the HD or HIP star number (if this latter exists). Asterisked stars are both good $\gamma$ Doradus candidates and possible members of binary systems (see Sect. 5). Next columns respectively provide the number of spectra, the observation window, the mean exposure time, the mean S/N value, the number of photometric frequencies previously detected, the LPV signature, remarks about the binarity, the $v~\sin i$ value and some references $^{\dag }$ .
HD	HIP	N	Range	Exp.	S/N	Phot.	LPV	Binarity	$v~\sin i$	Ref
			[d]	[sec]					[km s^-1]
Bona fide $\gamma$ Dor stars
277	623	24	527	3500	215	3	strong		31	H99 HF01 FW03
12901	9807	5	268	2000	240	3	evident		66	H99 EA00 AC03
62454	37863	12	353	2800	240	5	in the primary	SB2	10.5 and 5	KH99
68192^*	40462	3	4	2800	220	2	weak	RV var.	95	HE99 KH99
86371^*	48830	4	348	1900	220	2	weak ?	SB2, ell. ?	11 and 6	H99 KE02
105458^*	59203	25	421	3600	200	6	evident	binary?	39	H99 HF01
108100^*	60571	5	322	2700	190	3	in the slow rot.	binary	65 and 13	BH97 HF02
164615	88272	13	379	2300	180	4	evident		65	ZR97 E98
167858^*	89601	11	366	2200	210	2	evident but small	SB	9.0	E98 AE98 H99 FW03
218396	114189	162	505	1100	250	4	evident		38	E98 ZR99
221866^*	116434	32	506	3300	220	2	in the sec.	SB2	13 and 10	H99 FW03
224638	118293	23	410	3300	200	5	evident		17	PK02
224945	159	2	346	1800	190	5			54	PK02
Prime candidates
2842^*	2510	2	346	3600	210	3	in the blue wing	maybe	77	H99 KE02 FW03
7169^*	5674	4	137	3200	210	2	in both stars	visual	90 and 8	H99 FW03
9365^*	7280	6	269	4000	200	2	weak	RV var.	69	H99 FW03 LJ89
23874^*	17826	4	5	3600	200	2	in the slow rot.	visual	90 and 9	H99 FW03
48271	32263	19	423	3400	240	6	evident		21	E98 H99 MB03
63436^*	38138	7	347	3000	190	2	in the blue wing	binary ?	66	H99 MB03
70645^*	41488	10	423	3600	230	2	evident	SB1	11	H99 MB03
80731^*	46099	11	422	3400	210	5	evident	SB1	13	H99 MB03
86358^*	48895	3	2	1800	220	2	in the slow rot.	binary	37 and 25	H99 KE02 FW03
100215^*	56275	11	422	3000	240	2	evident	SB1	13	H99 KE02 FW03
113867^*	63951	7	572	1800	210	2	weak	SB2 ?	8.5 and 110	H99 FW03
171244^*	90919	4	316	3000	200	2	very weak in the wings	binary?	50	H99 FW03
175337	92837	7	315	3300	230	2	evident	unlikely	38	H99 KE02 FW03
195068	100859	36	564	1300	240	2	evident		46	E98 H99 FW03
211699	110163	21	399	3700	210	2	evident		12	H99
Other candidates and COROT targets
44195	30154	4	345	3000	220	cst	weak ?		50	PG02
44333	30217	2	3	1400	160		in the slow rot.?	binary	160 and 15	PG02 RG02
49434	32617	92	422	850	230		in the blue wing		82	BC02
112429	63076	40	566	900	220	2	in the wings		101	E98 AE98 FW03
171834	91237	13	11	940	200	cst	very weak		65	GP02
171836	91272	3	75	3600	200	cst	observed		62	GP02
172506	91580	2	9	3100	180	var?	observed	binary ?	39	GP02
174353	-	2	8	3600	200		varying res. flux		11	H02

$^{\dag }$ AC03: Aerts et al. (2004) - AE98: Aerts et al. (1998) - BC02: Bruntt et al. (2002) - BH97: Breger et al. (1997) - E98: Eyer (1998) - EA00: Eyer & Aerts (2000) - FW03: Fekel et al. (2003) - GP02: Garrido et al. (2002) - H99: Handler (1999) - H02: Handler (2002) - HE99: Henry (1999) - HF01: Henry et al. (2001) - HF02: Henry & Fekel (2002) - KE02: Koen & Eyer (2002) - KH99: Kaye et al. (1999b) - LJ89: Liu et al. (1989) - MB03: Martín et al. (2003) - PG02: Poretti et al. (2002) - PK02: Poretti et al. (2002) - RG02: Royer et al. (2002) - ZR97: Zerbi et al. (1997) - ZR99: Zerbi et al. (1999).

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