Table 2: Upper limits ( $1 \sigma$ and $3 \sigma$ ) for the projected rotational velocities of the stars from Paper I. $1 \sigma$ limits have not been published previously.
WD White dwarf $v \sin i$ (km s^-1) $v \sin i$ (km s^-1)

$1 \sigma$ $3 \sigma$

0352+096 HZ 4 <13 <21

0406+169 LB 227 <20 <28

0421+162 VR 7 <8 <18

0425+168 VR 16 <18 <26

0431+125 HZ 7 $\rm 15^{+7}_{-5}$ <35

0438+108 HZ 14 <14 <28

0836+197 LB 5893 <22 <43

0837+199 LB 393 <9 <29

0413-077 40 Eri B < 1 < 8

0726+393 LP207-7 <7 <18

1143+321 G148-7 <2 <12

1314+293 HZ43 <11 <29

1911+135 G142-B2B <2 <9

**Table 2:** Upper limits ( $1 \sigma$ and $3 \sigma$ ) for the projected rotational velocities of the stars from Paper I. $1 \sigma$ limits have not been published previously.
WD	White dwarf	$v \sin i$ (km s^-1)	$v \sin i$ (km s^-1)
		$1 \sigma$	$3 \sigma$
0352+096	HZ 4	<13	<21
0406+169	LB 227	<20	<28
0421+162	VR 7	<8	<18
0425+168	VR 16	<18	<26
0431+125	HZ 7	$\rm 15^{+7}_{-5}$	<35
0438+108	HZ 14	<14	<28
0836+197	LB 5893	<22	<43
0837+199	LB 393	<9	<29
0413-077	40 Eri B	< 1	< 8
0726+393	LP207-7	<7	<18
1143+321	G148-7	<2	<12
1314+293	HZ43	<11	<29
1911+135	G142-B2B	<2	<9

Source LaTeX | All tables | In the text

	1 Introduction
	2 Atmospheric parameters and stellar masses
	3 Model atmospheres and spectral analysis
	4 Projected rotational velocities
	5 Discussion
	References