Table 1.

List of nearby WZ Sge-type DNe.

Objectd* (pc)G   (mag)
ASASSN-14dx80.8 [80.6, 81.1]15.0
WZ Sge45.1 [45.0, 45.2]15.2
V455 And75.4 [75.1, 75.7]16.1
BW Scl94.2 [93.3, 95.0]16.3
V627 Peg99.4 [98.8, 100.1]15.7
GW Lib112.5 [111.4, 113.5]16.5
EZ Lyn145.3 [142.1, 148.6]17.8
V355 UMa149.6 [147.7, 151.5]17.4
FL Ps153.1 [150.0, 156.3]17.5
V406 Vir168.8 [164.5, 173.3]17.7
PNV J1714176.9 [172.5, 181.6]17.2
EG Cnc184.9 [175.0, 195.9]18.8
QZ Lib189.2 [178.0, 201.9]18.9
V1838 Aql201.6 [195.0, 208.7]17.9
1RXS J0232206.9 [198.8, 215.8]18.7
OV Boo§210.5 [204.4, 216.9]18.2
V624 Peg217.7 [204.1, 233.2]18.4
TCP J1815220.0 [208.6, 232.7]19.2
SSS J1222239.8 [220.5, 262.8]18.9
PNV J0309246.6 [230.8, 264.6]18.7
ASASSN-14cl261.2 [248.9, 274.9]18.2
Objectd* (pc)G   (mag)
ASASSN-14dx80.8 [80.6, 81.1]15.0
WZ Sge45.1 [45.0, 45.2]15.2
V455 And75.4 [75.1, 75.7]16.1
BW Scl94.2 [93.3, 95.0]16.3
V627 Peg99.4 [98.8, 100.1]15.7
GW Lib112.5 [111.4, 113.5]16.5
EZ Lyn145.3 [142.1, 148.6]17.8
V355 UMa149.6 [147.7, 151.5]17.4
FL Ps153.1 [150.0, 156.3]17.5
V406 Vir168.8 [164.5, 173.3]17.7
PNV J1714176.9 [172.5, 181.6]17.2
EG Cnc184.9 [175.0, 195.9]18.8
QZ Lib189.2 [178.0, 201.9]18.9
V1838 Aql201.6 [195.0, 208.7]17.9
1RXS J0232206.9 [198.8, 215.8]18.7
OV Boo§210.5 [204.4, 216.9]18.2
V624 Peg217.7 [204.1, 233.2]18.4
TCP J1815220.0 [208.6, 232.7]19.2
SSS J1222239.8 [220.5, 262.8]18.9
PNV J0309246.6 [230.8, 264.6]18.7
ASASSN-14cl261.2 [248.9, 274.9]18.2

*Distance estimated by using the parallax ϖ in Gaia DR2 and the method of Bailer-Jones et al. (2018). The left-hand values are the medians of the distance probability distributions, and the right-hand values in the brackets are the 16th and 84th percentiles.

 G magnitude in Gaia DR2.

PNV J1714 = PNV J17144255−2943481, 1RXS J0232 = 1RXS J023238.8−371812, TCP J1815 = TCP J18154219+3515598, SSS J1222 = SSS J122221.7−311523, PNV J0309 = PNV J03093063+2638031.

§Population II CV below the period minimum which showed a WZ Sge-type super-outburst.

Table 1.

List of nearby WZ Sge-type DNe.

Objectd* (pc)G   (mag)
ASASSN-14dx80.8 [80.6, 81.1]15.0
WZ Sge45.1 [45.0, 45.2]15.2
V455 And75.4 [75.1, 75.7]16.1
BW Scl94.2 [93.3, 95.0]16.3
V627 Peg99.4 [98.8, 100.1]15.7
GW Lib112.5 [111.4, 113.5]16.5
EZ Lyn145.3 [142.1, 148.6]17.8
V355 UMa149.6 [147.7, 151.5]17.4
FL Ps153.1 [150.0, 156.3]17.5
V406 Vir168.8 [164.5, 173.3]17.7
PNV J1714176.9 [172.5, 181.6]17.2
EG Cnc184.9 [175.0, 195.9]18.8
QZ Lib189.2 [178.0, 201.9]18.9
V1838 Aql201.6 [195.0, 208.7]17.9
1RXS J0232206.9 [198.8, 215.8]18.7
OV Boo§210.5 [204.4, 216.9]18.2
V624 Peg217.7 [204.1, 233.2]18.4
TCP J1815220.0 [208.6, 232.7]19.2
SSS J1222239.8 [220.5, 262.8]18.9
PNV J0309246.6 [230.8, 264.6]18.7
ASASSN-14cl261.2 [248.9, 274.9]18.2
Objectd* (pc)G   (mag)
ASASSN-14dx80.8 [80.6, 81.1]15.0
WZ Sge45.1 [45.0, 45.2]15.2
V455 And75.4 [75.1, 75.7]16.1
BW Scl94.2 [93.3, 95.0]16.3
V627 Peg99.4 [98.8, 100.1]15.7
GW Lib112.5 [111.4, 113.5]16.5
EZ Lyn145.3 [142.1, 148.6]17.8
V355 UMa149.6 [147.7, 151.5]17.4
FL Ps153.1 [150.0, 156.3]17.5
V406 Vir168.8 [164.5, 173.3]17.7
PNV J1714176.9 [172.5, 181.6]17.2
EG Cnc184.9 [175.0, 195.9]18.8
QZ Lib189.2 [178.0, 201.9]18.9
V1838 Aql201.6 [195.0, 208.7]17.9
1RXS J0232206.9 [198.8, 215.8]18.7
OV Boo§210.5 [204.4, 216.9]18.2
V624 Peg217.7 [204.1, 233.2]18.4
TCP J1815220.0 [208.6, 232.7]19.2
SSS J1222239.8 [220.5, 262.8]18.9
PNV J0309246.6 [230.8, 264.6]18.7
ASASSN-14cl261.2 [248.9, 274.9]18.2

*Distance estimated by using the parallax ϖ in Gaia DR2 and the method of Bailer-Jones et al. (2018). The left-hand values are the medians of the distance probability distributions, and the right-hand values in the brackets are the 16th and 84th percentiles.

 G magnitude in Gaia DR2.

PNV J1714 = PNV J17144255−2943481, 1RXS J0232 = 1RXS J023238.8−371812, TCP J1815 = TCP J18154219+3515598, SSS J1222 = SSS J122221.7−311523, PNV J0309 = PNV J03093063+2638031.

§Population II CV below the period minimum which showed a WZ Sge-type super-outburst.

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