Summary of the CV white dwarf masses derived in this work from the analysis of the ultraviolet data and those obtained employing other methods. The systems are sorted by increasing masses.
| . | MWD (M⊙) . | . | |||||
|---|---|---|---|---|---|---|---|
| System . | Ultraviolet . | Ultraviolet . | Ultraviolet . | Optical . | Gravitational . | Radial . | References . |
| . | spectral fit . | spectral fit . | light curve . | light curve . | redshift . | velocities . | . |
| . | (this work) . | (literaturea) . | . | . | . | . | . |
| BC UMa | |$0.48^{+0.08}_{-0.09}$| | |$0.53^{+0.07}_{-0.09}$| | – | – | – | – | Gänsicke et al. (2005) |
| AX For | 0.56↑ | – | – | – | |$0.76^{+0.06}_{-0.07}$| | – | This work |
| SW UMa | |$0.61^{+0.06}_{-0.04}$| | 0.61 ± 0.6 | – | – | – | – | Gänsicke et al. (2005) |
| AM Her | |$0.63^{+0.10}_{-0.08}$| | |$0.53^{+0.10}_{-0.08}$| | – | – | – | – | Gänsicke et al. (2006) |
| LL And | |$0.7^{+0.4}_{-0.3}$| | |$0.7^{+0.4}_{-0.3}$| | – | – | – | – | Howell et al. (2002) |
| EF Peg | |$0.80^{+0.16}_{-0.17}$| | |$0.88^{+0.16}_{-0.17}$| | – | – | – | – | Howell et al. (2002) |
| WZ Sge | 0.80 ± 0.02 | – | – | – | 0.85 ± 0.04 | – | Steeghs et al. (2007) |
| DW UMa | |$0.82^{+0.03}_{-0.04}$| | – | 0.77 ± 0.07 | – | – | – | Araujo-Betancor et al. (2003) |
| GW Lib | |$0.83^{+0.08}_{-0.12}$| | – | – | – | 0.84 ± 0.02 | – | van Spaandonk et al. (2010) |
| SDSS J150722.30+523039.8 | |$0.90^{+0.10}_{-0.14}$| | – | |$0.83^{+0.19}_{-0.15}$| | 0.89 ± 0.01 | – | – | Ultraviolet light curve, this work; |
| optical light curve (Savoury et al. 2011) | |||||||
| V1108 Her | |$0.88^{+0.09}_{-0.11}$| | – | – | – | |$0.91^{+0.14}_{-0.20}$| | – | This work |
| DV UMa | |$0.96^{+0.07}_{-0.10}$| | – | – | 1.09 ± 0.03 | – | – | McAllister et al. (2019) |
| IY UMa | |$0.99^{+0.04}_{-0.03}$| | – | – | |$0.955^{+0.013}_{-0.028}$| | – | – | McAllister et al. (2019) |
| SDSS J103533.02+055158.4 | |$1.00^{+0.08}_{-0.10}$| | – | – | 0.835 ± 0.009 | – | – | Savoury et al. (2011) |
| BW Scl | |$1.007^{+0.01}_{-0.012}$| | |$1.10^{+0.03}_{-0.06}$| | – | – | – | – | Gänsicke et al. (2005) |
| IR Com | |$1.03^{+0.07}_{-0.09}$| | – | 0.989 ± 0.003 | – | 0.95 ± 0.04 | – | This work |
| U Gem | 1.16 ± 0.013 | – | – | – | – | 1.2 ± 0.05 | Echevarría, de la Fuente & Costero (2007) |
| HV Vir | |$0.87^{+0.13}_{-0.17}$| | |$1.27^{+0.13}_{-0.17}$| | – | – | – | – | Szkody et al. (2002a) |
| EG Cnc | |$1.03^{+0.04}_{-0.05}$| | |$1.28^{+0.04}_{-0.05}$| | – | – | – | – | Szkody et al. (2002a) |
| . | MWD (M⊙) . | . | |||||
|---|---|---|---|---|---|---|---|
| System . | Ultraviolet . | Ultraviolet . | Ultraviolet . | Optical . | Gravitational . | Radial . | References . |
| . | spectral fit . | spectral fit . | light curve . | light curve . | redshift . | velocities . | . |
| . | (this work) . | (literaturea) . | . | . | . | . | . |
| BC UMa | |$0.48^{+0.08}_{-0.09}$| | |$0.53^{+0.07}_{-0.09}$| | – | – | – | – | Gänsicke et al. (2005) |
| AX For | 0.56↑ | – | – | – | |$0.76^{+0.06}_{-0.07}$| | – | This work |
| SW UMa | |$0.61^{+0.06}_{-0.04}$| | 0.61 ± 0.6 | – | – | – | – | Gänsicke et al. (2005) |
| AM Her | |$0.63^{+0.10}_{-0.08}$| | |$0.53^{+0.10}_{-0.08}$| | – | – | – | – | Gänsicke et al. (2006) |
| LL And | |$0.7^{+0.4}_{-0.3}$| | |$0.7^{+0.4}_{-0.3}$| | – | – | – | – | Howell et al. (2002) |
| EF Peg | |$0.80^{+0.16}_{-0.17}$| | |$0.88^{+0.16}_{-0.17}$| | – | – | – | – | Howell et al. (2002) |
| WZ Sge | 0.80 ± 0.02 | – | – | – | 0.85 ± 0.04 | – | Steeghs et al. (2007) |
| DW UMa | |$0.82^{+0.03}_{-0.04}$| | – | 0.77 ± 0.07 | – | – | – | Araujo-Betancor et al. (2003) |
| GW Lib | |$0.83^{+0.08}_{-0.12}$| | – | – | – | 0.84 ± 0.02 | – | van Spaandonk et al. (2010) |
| SDSS J150722.30+523039.8 | |$0.90^{+0.10}_{-0.14}$| | – | |$0.83^{+0.19}_{-0.15}$| | 0.89 ± 0.01 | – | – | Ultraviolet light curve, this work; |
| optical light curve (Savoury et al. 2011) | |||||||
| V1108 Her | |$0.88^{+0.09}_{-0.11}$| | – | – | – | |$0.91^{+0.14}_{-0.20}$| | – | This work |
| DV UMa | |$0.96^{+0.07}_{-0.10}$| | – | – | 1.09 ± 0.03 | – | – | McAllister et al. (2019) |
| IY UMa | |$0.99^{+0.04}_{-0.03}$| | – | – | |$0.955^{+0.013}_{-0.028}$| | – | – | McAllister et al. (2019) |
| SDSS J103533.02+055158.4 | |$1.00^{+0.08}_{-0.10}$| | – | – | 0.835 ± 0.009 | – | – | Savoury et al. (2011) |
| BW Scl | |$1.007^{+0.01}_{-0.012}$| | |$1.10^{+0.03}_{-0.06}$| | – | – | – | – | Gänsicke et al. (2005) |
| IR Com | |$1.03^{+0.07}_{-0.09}$| | – | 0.989 ± 0.003 | – | 0.95 ± 0.04 | – | This work |
| U Gem | 1.16 ± 0.013 | – | – | – | – | 1.2 ± 0.05 | Echevarría, de la Fuente & Costero (2007) |
| HV Vir | |$0.87^{+0.13}_{-0.17}$| | |$1.27^{+0.13}_{-0.17}$| | – | – | – | – | Szkody et al. (2002a) |
| EG Cnc | |$1.03^{+0.04}_{-0.05}$| | |$1.28^{+0.04}_{-0.05}$| | – | – | – | – | Szkody et al. (2002a) |
The reported values have been corrected accounting for the temperature dependency of the mass-radius relationship and the reddening, as discussed in Section 4.1.2.
Summary of the CV white dwarf masses derived in this work from the analysis of the ultraviolet data and those obtained employing other methods. The systems are sorted by increasing masses.
| . | MWD (M⊙) . | . | |||||
|---|---|---|---|---|---|---|---|
| System . | Ultraviolet . | Ultraviolet . | Ultraviolet . | Optical . | Gravitational . | Radial . | References . |
| . | spectral fit . | spectral fit . | light curve . | light curve . | redshift . | velocities . | . |
| . | (this work) . | (literaturea) . | . | . | . | . | . |
| BC UMa | |$0.48^{+0.08}_{-0.09}$| | |$0.53^{+0.07}_{-0.09}$| | – | – | – | – | Gänsicke et al. (2005) |
| AX For | 0.56↑ | – | – | – | |$0.76^{+0.06}_{-0.07}$| | – | This work |
| SW UMa | |$0.61^{+0.06}_{-0.04}$| | 0.61 ± 0.6 | – | – | – | – | Gänsicke et al. (2005) |
| AM Her | |$0.63^{+0.10}_{-0.08}$| | |$0.53^{+0.10}_{-0.08}$| | – | – | – | – | Gänsicke et al. (2006) |
| LL And | |$0.7^{+0.4}_{-0.3}$| | |$0.7^{+0.4}_{-0.3}$| | – | – | – | – | Howell et al. (2002) |
| EF Peg | |$0.80^{+0.16}_{-0.17}$| | |$0.88^{+0.16}_{-0.17}$| | – | – | – | – | Howell et al. (2002) |
| WZ Sge | 0.80 ± 0.02 | – | – | – | 0.85 ± 0.04 | – | Steeghs et al. (2007) |
| DW UMa | |$0.82^{+0.03}_{-0.04}$| | – | 0.77 ± 0.07 | – | – | – | Araujo-Betancor et al. (2003) |
| GW Lib | |$0.83^{+0.08}_{-0.12}$| | – | – | – | 0.84 ± 0.02 | – | van Spaandonk et al. (2010) |
| SDSS J150722.30+523039.8 | |$0.90^{+0.10}_{-0.14}$| | – | |$0.83^{+0.19}_{-0.15}$| | 0.89 ± 0.01 | – | – | Ultraviolet light curve, this work; |
| optical light curve (Savoury et al. 2011) | |||||||
| V1108 Her | |$0.88^{+0.09}_{-0.11}$| | – | – | – | |$0.91^{+0.14}_{-0.20}$| | – | This work |
| DV UMa | |$0.96^{+0.07}_{-0.10}$| | – | – | 1.09 ± 0.03 | – | – | McAllister et al. (2019) |
| IY UMa | |$0.99^{+0.04}_{-0.03}$| | – | – | |$0.955^{+0.013}_{-0.028}$| | – | – | McAllister et al. (2019) |
| SDSS J103533.02+055158.4 | |$1.00^{+0.08}_{-0.10}$| | – | – | 0.835 ± 0.009 | – | – | Savoury et al. (2011) |
| BW Scl | |$1.007^{+0.01}_{-0.012}$| | |$1.10^{+0.03}_{-0.06}$| | – | – | – | – | Gänsicke et al. (2005) |
| IR Com | |$1.03^{+0.07}_{-0.09}$| | – | 0.989 ± 0.003 | – | 0.95 ± 0.04 | – | This work |
| U Gem | 1.16 ± 0.013 | – | – | – | – | 1.2 ± 0.05 | Echevarría, de la Fuente & Costero (2007) |
| HV Vir | |$0.87^{+0.13}_{-0.17}$| | |$1.27^{+0.13}_{-0.17}$| | – | – | – | – | Szkody et al. (2002a) |
| EG Cnc | |$1.03^{+0.04}_{-0.05}$| | |$1.28^{+0.04}_{-0.05}$| | – | – | – | – | Szkody et al. (2002a) |
| . | MWD (M⊙) . | . | |||||
|---|---|---|---|---|---|---|---|
| System . | Ultraviolet . | Ultraviolet . | Ultraviolet . | Optical . | Gravitational . | Radial . | References . |
| . | spectral fit . | spectral fit . | light curve . | light curve . | redshift . | velocities . | . |
| . | (this work) . | (literaturea) . | . | . | . | . | . |
| BC UMa | |$0.48^{+0.08}_{-0.09}$| | |$0.53^{+0.07}_{-0.09}$| | – | – | – | – | Gänsicke et al. (2005) |
| AX For | 0.56↑ | – | – | – | |$0.76^{+0.06}_{-0.07}$| | – | This work |
| SW UMa | |$0.61^{+0.06}_{-0.04}$| | 0.61 ± 0.6 | – | – | – | – | Gänsicke et al. (2005) |
| AM Her | |$0.63^{+0.10}_{-0.08}$| | |$0.53^{+0.10}_{-0.08}$| | – | – | – | – | Gänsicke et al. (2006) |
| LL And | |$0.7^{+0.4}_{-0.3}$| | |$0.7^{+0.4}_{-0.3}$| | – | – | – | – | Howell et al. (2002) |
| EF Peg | |$0.80^{+0.16}_{-0.17}$| | |$0.88^{+0.16}_{-0.17}$| | – | – | – | – | Howell et al. (2002) |
| WZ Sge | 0.80 ± 0.02 | – | – | – | 0.85 ± 0.04 | – | Steeghs et al. (2007) |
| DW UMa | |$0.82^{+0.03}_{-0.04}$| | – | 0.77 ± 0.07 | – | – | – | Araujo-Betancor et al. (2003) |
| GW Lib | |$0.83^{+0.08}_{-0.12}$| | – | – | – | 0.84 ± 0.02 | – | van Spaandonk et al. (2010) |
| SDSS J150722.30+523039.8 | |$0.90^{+0.10}_{-0.14}$| | – | |$0.83^{+0.19}_{-0.15}$| | 0.89 ± 0.01 | – | – | Ultraviolet light curve, this work; |
| optical light curve (Savoury et al. 2011) | |||||||
| V1108 Her | |$0.88^{+0.09}_{-0.11}$| | – | – | – | |$0.91^{+0.14}_{-0.20}$| | – | This work |
| DV UMa | |$0.96^{+0.07}_{-0.10}$| | – | – | 1.09 ± 0.03 | – | – | McAllister et al. (2019) |
| IY UMa | |$0.99^{+0.04}_{-0.03}$| | – | – | |$0.955^{+0.013}_{-0.028}$| | – | – | McAllister et al. (2019) |
| SDSS J103533.02+055158.4 | |$1.00^{+0.08}_{-0.10}$| | – | – | 0.835 ± 0.009 | – | – | Savoury et al. (2011) |
| BW Scl | |$1.007^{+0.01}_{-0.012}$| | |$1.10^{+0.03}_{-0.06}$| | – | – | – | – | Gänsicke et al. (2005) |
| IR Com | |$1.03^{+0.07}_{-0.09}$| | – | 0.989 ± 0.003 | – | 0.95 ± 0.04 | – | This work |
| U Gem | 1.16 ± 0.013 | – | – | – | – | 1.2 ± 0.05 | Echevarría, de la Fuente & Costero (2007) |
| HV Vir | |$0.87^{+0.13}_{-0.17}$| | |$1.27^{+0.13}_{-0.17}$| | – | – | – | – | Szkody et al. (2002a) |
| EG Cnc | |$1.03^{+0.04}_{-0.05}$| | |$1.28^{+0.04}_{-0.05}$| | – | – | – | – | Szkody et al. (2002a) |
The reported values have been corrected accounting for the temperature dependency of the mass-radius relationship and the reddening, as discussed in Section 4.1.2.
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