Table 2:

Light curve classification of 64 X-ray pulsars observed atenergies below 10 keV.

Name	a	Pulsesb	B03c	Ref.
XMMU J004723.7-731226	263	1		1
AX J0049-729	74.7	1	1	2
AX J0049-732	9.1	1	1	3
AX J0049.5-7323	756	1		4
2E 0050.1-7247	8.9	1	1	5
RX J0051.3-7216	91	2		6
AX J0051-733	323	1	1	7
AX J0051.6-7311	172	1		8
SMC X-3	7.8	1		9
XTE J0052-725	82.5	1		9
XTE J0052-723	4.78	2		10
CXOU J005323.8-722715	138	1		9
RX J0053.8-7226	46.6	1		11
XTE J0054-720	168	1		12
CXOU J005455.6-724510	500	1		9,13
RX J0054.9-7226	59	1		14
XMMU J005517.9-723853	702	1		13
CXOU J005527.9-721058	34.1	2		9
XMMU J005605.2-722200	140	2		14
AX J0057.4-7325	101	1		15
CXOU J005736.2-721934	563	1		9,18
RX J0057.8-7207	152	1		14
AX J0058-720	281	2	2	14,16
1XMMU J005921.0-722317	202	1		1
RX J0059.2-7138	2.76	1	1	17
CXOU J010043.1-721134d	8.02	2		1
CXOU J010102.7-720658	304	1		18
RX J0101.3-7211	452	1		14
XTE J0103-728	6.85	2		19
SAX J0103.2-7209	345	1	1	20
RX J0103.6-7201	1323	2		21
J0105-721	3.34	1		5
XTE J0111.2-7317	30.9	2	1	22
RX J0440.9+4431	202	1	1	23
RX J0502.9-6626	4.06	2	1	24
RX J0529.8-6556	69	1	1	25
XMMU J053011.2-655122	272	2		26
EXO 053109-6609.2	13.7	2		26
1A 0538-66	0.069	2	2	27
1SAX J0544.1-710	96	2	1	28
SAX J0635.2+0533	0.034	1	1	29
RX J0648.1-4419	13.2	1	1	30
RX J0720.4-3125	8.39	1	1	31
RX J1037.5-5647	860	2	1	23
1E 1048.1-5937d	6.44	1	1	32
IGR J11215-5952	187	2		33
IGR J11435-6109	162	2		34
2RXP J130159.6-635806	710	1		35
1SAX J1324.4-6200	171	1	1	36
1SAX J1452.8-5949	437	1	1	37
2S 1553-54(2)	9.3	2	2	38
IGR J16320-4751	1300	2		39
IGR J16465-4507	228	1		40
CXOU J164710.2-455216d	10.6	2		41
AX J170006-4157	715	1	1	42
AX J1740.1-2847	730	2		43
AX J1749.2-2725	220	1	1	44
XTE J1810-197	5.54	1		45
AX 1820.5-1434	152	2		46
XTE J1829-098	7.8	1		47
AX J1841.0-0536	4.74	1 (flat)		48
1E 1841-045d	11.8	1		49
AX J1845.0-0300d	7.0	1	1	50
SAX J2239.3+6116	1247	1		51

Notes. ^(a) Pulsar spin period (s). ^(b) Number of pulses in the profile. ^(c) Classification by B03. ^(d) Magnetars.

References. (1) Majid et al. (2004); (2) Yokogawa et al. (1999); (3) Ueno et al. (2000); (4) Yokogawa et al. (2000b); (5) Israel et al. (1997a); (6) Yokogawa et al. (2000a); (7) Imanishi et al. (1999); (8) Yokogawa et al. (2000d); (9) Edge et al. (2004); (10) Laycock et al. (2003); (11) Laycock et al. (2005); (12) Yokogawa et al. (2001); (13) Haberl et al. (2004a); (14) Sasaki et al. (2003); (15) Yokogawa et al. (2000e); (16) Tsujimoto et al. (1999); (17) Kohno et al. (2000); (18) Macomb et al. (2003); (19) Haberl & Pietsch (2008); (20) Israel et al. (2000); (21) Haberl & Pietsch (2005); (22) Yokogawa et al. (2000c); (23) Reig & Roche (1999a); (24) Schmidtke et al. (1995); (25) Haberl et al. (1997); (26) Haberl et al. (2003); (27) Skinner et al. (1982); (28) Cusumano et al. (1998); (29) Cusumano et al. (2000); (30) Israel et al. (1997b); (31) Haberl et al. (2004b); (32) Seward et al. (1986); (33) Sidoli et al. (2007); (34) in't Zand & Heise (2004); (35) Chernyakova et al. (2005); (36) Angelini et al. (1998); (37) Oosterbroek et al. (1999); (38) Kelley et al. (1983); (39) Lutovinov et al. (2005b); (40) Lutovinov et al. (2005a); (41) Israel et al. (2007); (42) Torii et al. (1999); (43) Sakano et al. (2000); (44) Torii et al. (1998a); (45) Halpern & Gotthelf (2005); (46) Kinugasa et al. (1998); (47) Halpern & Gotthelf (2007); (48) Bamba et al. (2001); (49) Morii et al. (2003); (50) Torii et al. (1998b); (51) in't Zand et al. (2001b).