Table 2.

Results of our search for soft X-ray flashes for the 40 novae in table 1.

Nova*N  H  DistanceU.L.N  s  §Reference for distance
(cm−2)(kpc)ave (min–max)
V2672 Oph4.18 × 102119 ± 22.51 (0.71–4.24)22Takei et al. (2014)
V5584 Sgr3.96 × 10216.3 ± 0.51.20 (0.38–3.28)134Raj et al. (2015)
V496 Sct6.81 × 10212.9 ± 0.32.22 (0.74–4.75)45Raj et al. (2012)
KT Eri5.52 × 10206.6 ± 0.81.71 (0.61–6.03)109Imamura and Tanabe (2012)
V1722 Aql9.14 × 102151.97 (0.63–6.01)112Munari et al. (2010)
V2673 Oph2.84 × 10217.41.42 (0.43–4.38)77Munari and Dallaporta (2010)
V5585 Sgr2.75 × 1021N/A1.76 (0.50–4.36)44
V2674 Oph4.12 × 102191.75 (0.67–3.96)30Munari, Dallaporta, and Ochner (2010)
V407 Cyg8.19 × 10212.71.83 (0.56–4.46)52Munari, Margoni and Stagni (1990)
V5586 Sgr9.60 × 1021N/A2.79 (1.21–5.64)23
V1311 Sco4.78 × 1021N/A1.98 (0.52–4.44)20
V1723 Aql1.23 × 102261.76 (0.49–4.97)140Weston et al. (2016)
V5587 Sgr4.09 × 1021N/A1.56 (0.30–3.67)126
V5588 Sgr5.47 × 10217.62.15 (0.65–5.67)122Munari et al. (2015)
T Pyx1.88 × 10213.5 ± 11.87 (0.43–8.19)35Schaefer (2010)
V1312 Sco5.14 × 1021N/A1.61 (0.47–4.64)118
PR Lup4.82 × 1021N/A1.25 (0.39–3.76)144
V1313 Sco4.77 × 1021N/A1.09 (0.26–3.71)55
V965 Per1.20 × 1021N/A3.56 (1.37–8.18)17
V834 Car4.98 × 1021N/A1.49 (0.38–5.09)121
V1368 Cen4.30 × 1021N/A1.37 (0.46–3.50)47
V2676 Oph3.02 × 1021N/A1.34 (0.36–3.56)89
V5589 Sgr3.35 × 1021N/A2.21 (0.47–5.85)111
V5590 Sgr2.64 × 1021N/A2.19 (0.70–5.50)107
V2677 Oph3.38 × 1021N/A3.46 (0.79–11.27)44
V1324 Sco4.35 × 10214.52.56 (0.79–6.05)47Ackermann et al. (2014)
V5591 Sgr4.27 × 1021N/A2.31 (0.61–6.59)134
V5592 Sgr1.49 × 1021N/A2.01 (0.72–5.96)93
V5593 Sgr6.54 × 1021N/A2.31 (0.66–5.97)115
V959 Mon6.29 × 10213.62.68 (0.71–9.77)118Shore et al. (2013)
V1724 Aql1.47 × 1022N/A2.49 (0.61–7.11)133
V809 Cep8.22 × 10216.51.98 (0.65–5.25)93Munari et al. (2014)
V1533 Sco7.42 × 1021N/A2.10 (0.66–4.36)84
V339 Del1.36 × 10214.22.04 (0.64–6.08)140Shore (2013)
V1830 Aql1.23 × 1022N/A3.08 (0.86–8.20)128
V556 Ser4.87 × 1021N/A2.54 (0.93–6.70)89
V1369 Cen5.84 × 10212.42.58 (0.74–8.95)83Shore et al. (2014)
V962 Cep3.30 × 1021N/A2.72 (1.11–11.86)125
V1534 Sco3.88 × 1021131.77 (0.79–4.24)22Joshi et al. (2015)
V2659 Cyg4.92 × 1021N/A2.27 (0.73–6.13)124
Nova*N  H  DistanceU.L.N  s  §Reference for distance
(cm−2)(kpc)ave (min–max)
V2672 Oph4.18 × 102119 ± 22.51 (0.71–4.24)22Takei et al. (2014)
V5584 Sgr3.96 × 10216.3 ± 0.51.20 (0.38–3.28)134Raj et al. (2015)
V496 Sct6.81 × 10212.9 ± 0.32.22 (0.74–4.75)45Raj et al. (2012)
KT Eri5.52 × 10206.6 ± 0.81.71 (0.61–6.03)109Imamura and Tanabe (2012)
V1722 Aql9.14 × 102151.97 (0.63–6.01)112Munari et al. (2010)
V2673 Oph2.84 × 10217.41.42 (0.43–4.38)77Munari and Dallaporta (2010)
V5585 Sgr2.75 × 1021N/A1.76 (0.50–4.36)44
V2674 Oph4.12 × 102191.75 (0.67–3.96)30Munari, Dallaporta, and Ochner (2010)
V407 Cyg8.19 × 10212.71.83 (0.56–4.46)52Munari, Margoni and Stagni (1990)
V5586 Sgr9.60 × 1021N/A2.79 (1.21–5.64)23
V1311 Sco4.78 × 1021N/A1.98 (0.52–4.44)20
V1723 Aql1.23 × 102261.76 (0.49–4.97)140Weston et al. (2016)
V5587 Sgr4.09 × 1021N/A1.56 (0.30–3.67)126
V5588 Sgr5.47 × 10217.62.15 (0.65–5.67)122Munari et al. (2015)
T Pyx1.88 × 10213.5 ± 11.87 (0.43–8.19)35Schaefer (2010)
V1312 Sco5.14 × 1021N/A1.61 (0.47–4.64)118
PR Lup4.82 × 1021N/A1.25 (0.39–3.76)144
V1313 Sco4.77 × 1021N/A1.09 (0.26–3.71)55
V965 Per1.20 × 1021N/A3.56 (1.37–8.18)17
V834 Car4.98 × 1021N/A1.49 (0.38–5.09)121
V1368 Cen4.30 × 1021N/A1.37 (0.46–3.50)47
V2676 Oph3.02 × 1021N/A1.34 (0.36–3.56)89
V5589 Sgr3.35 × 1021N/A2.21 (0.47–5.85)111
V5590 Sgr2.64 × 1021N/A2.19 (0.70–5.50)107
V2677 Oph3.38 × 1021N/A3.46 (0.79–11.27)44
V1324 Sco4.35 × 10214.52.56 (0.79–6.05)47Ackermann et al. (2014)
V5591 Sgr4.27 × 1021N/A2.31 (0.61–6.59)134
V5592 Sgr1.49 × 1021N/A2.01 (0.72–5.96)93
V5593 Sgr6.54 × 1021N/A2.31 (0.66–5.97)115
V959 Mon6.29 × 10213.62.68 (0.71–9.77)118Shore et al. (2013)
V1724 Aql1.47 × 1022N/A2.49 (0.61–7.11)133
V809 Cep8.22 × 10216.51.98 (0.65–5.25)93Munari et al. (2014)
V1533 Sco7.42 × 1021N/A2.10 (0.66–4.36)84
V339 Del1.36 × 10214.22.04 (0.64–6.08)140Shore (2013)
V1830 Aql1.23 × 1022N/A3.08 (0.86–8.20)128
V556 Ser4.87 × 1021N/A2.54 (0.93–6.70)89
V1369 Cen5.84 × 10212.42.58 (0.74–8.95)83Shore et al. (2014)
V962 Cep3.30 × 1021N/A2.72 (1.11–11.86)125
V1534 Sco3.88 × 1021131.77 (0.79–4.24)22Joshi et al. (2015)
V2659 Cyg4.92 × 1021N/A2.27 (0.73–6.13)124

*U Sco, V1310 Sco, V5666 Sgr, and V745 Sco listed in table 1 are removed (see text).

Total Galactic H i column density toward the source as the average of the values obtained by the Leiden/Argentine/Bonn (LAB) map (Kalberla et al. 2005) and the DL map (Dickey & Lockman 1990), calculated using the HEASARC website 〈http://heasarc.gsfc.nasa.gov/cgi-bin/Tools/w3nh/w3nh.pl〉.

90% C.L. upper limit for the flux in the 2–4 keV band for each scan in units of 10−2 counts s−1 cm−2. The average (minimum and maximum) fluxes among Ns scans are shown.

§Number of GSC scans in the searched period.

Table 2.

Results of our search for soft X-ray flashes for the 40 novae in table 1.

Nova*N  H  DistanceU.L.N  s  §Reference for distance
(cm−2)(kpc)ave (min–max)
V2672 Oph4.18 × 102119 ± 22.51 (0.71–4.24)22Takei et al. (2014)
V5584 Sgr3.96 × 10216.3 ± 0.51.20 (0.38–3.28)134Raj et al. (2015)
V496 Sct6.81 × 10212.9 ± 0.32.22 (0.74–4.75)45Raj et al. (2012)
KT Eri5.52 × 10206.6 ± 0.81.71 (0.61–6.03)109Imamura and Tanabe (2012)
V1722 Aql9.14 × 102151.97 (0.63–6.01)112Munari et al. (2010)
V2673 Oph2.84 × 10217.41.42 (0.43–4.38)77Munari and Dallaporta (2010)
V5585 Sgr2.75 × 1021N/A1.76 (0.50–4.36)44
V2674 Oph4.12 × 102191.75 (0.67–3.96)30Munari, Dallaporta, and Ochner (2010)
V407 Cyg8.19 × 10212.71.83 (0.56–4.46)52Munari, Margoni and Stagni (1990)
V5586 Sgr9.60 × 1021N/A2.79 (1.21–5.64)23
V1311 Sco4.78 × 1021N/A1.98 (0.52–4.44)20
V1723 Aql1.23 × 102261.76 (0.49–4.97)140Weston et al. (2016)
V5587 Sgr4.09 × 1021N/A1.56 (0.30–3.67)126
V5588 Sgr5.47 × 10217.62.15 (0.65–5.67)122Munari et al. (2015)
T Pyx1.88 × 10213.5 ± 11.87 (0.43–8.19)35Schaefer (2010)
V1312 Sco5.14 × 1021N/A1.61 (0.47–4.64)118
PR Lup4.82 × 1021N/A1.25 (0.39–3.76)144
V1313 Sco4.77 × 1021N/A1.09 (0.26–3.71)55
V965 Per1.20 × 1021N/A3.56 (1.37–8.18)17
V834 Car4.98 × 1021N/A1.49 (0.38–5.09)121
V1368 Cen4.30 × 1021N/A1.37 (0.46–3.50)47
V2676 Oph3.02 × 1021N/A1.34 (0.36–3.56)89
V5589 Sgr3.35 × 1021N/A2.21 (0.47–5.85)111
V5590 Sgr2.64 × 1021N/A2.19 (0.70–5.50)107
V2677 Oph3.38 × 1021N/A3.46 (0.79–11.27)44
V1324 Sco4.35 × 10214.52.56 (0.79–6.05)47Ackermann et al. (2014)
V5591 Sgr4.27 × 1021N/A2.31 (0.61–6.59)134
V5592 Sgr1.49 × 1021N/A2.01 (0.72–5.96)93
V5593 Sgr6.54 × 1021N/A2.31 (0.66–5.97)115
V959 Mon6.29 × 10213.62.68 (0.71–9.77)118Shore et al. (2013)
V1724 Aql1.47 × 1022N/A2.49 (0.61–7.11)133
V809 Cep8.22 × 10216.51.98 (0.65–5.25)93Munari et al. (2014)
V1533 Sco7.42 × 1021N/A2.10 (0.66–4.36)84
V339 Del1.36 × 10214.22.04 (0.64–6.08)140Shore (2013)
V1830 Aql1.23 × 1022N/A3.08 (0.86–8.20)128
V556 Ser4.87 × 1021N/A2.54 (0.93–6.70)89
V1369 Cen5.84 × 10212.42.58 (0.74–8.95)83Shore et al. (2014)
V962 Cep3.30 × 1021N/A2.72 (1.11–11.86)125
V1534 Sco3.88 × 1021131.77 (0.79–4.24)22Joshi et al. (2015)
V2659 Cyg4.92 × 1021N/A2.27 (0.73–6.13)124
Nova*N  H  DistanceU.L.N  s  §Reference for distance
(cm−2)(kpc)ave (min–max)
V2672 Oph4.18 × 102119 ± 22.51 (0.71–4.24)22Takei et al. (2014)
V5584 Sgr3.96 × 10216.3 ± 0.51.20 (0.38–3.28)134Raj et al. (2015)
V496 Sct6.81 × 10212.9 ± 0.32.22 (0.74–4.75)45Raj et al. (2012)
KT Eri5.52 × 10206.6 ± 0.81.71 (0.61–6.03)109Imamura and Tanabe (2012)
V1722 Aql9.14 × 102151.97 (0.63–6.01)112Munari et al. (2010)
V2673 Oph2.84 × 10217.41.42 (0.43–4.38)77Munari and Dallaporta (2010)
V5585 Sgr2.75 × 1021N/A1.76 (0.50–4.36)44
V2674 Oph4.12 × 102191.75 (0.67–3.96)30Munari, Dallaporta, and Ochner (2010)
V407 Cyg8.19 × 10212.71.83 (0.56–4.46)52Munari, Margoni and Stagni (1990)
V5586 Sgr9.60 × 1021N/A2.79 (1.21–5.64)23
V1311 Sco4.78 × 1021N/A1.98 (0.52–4.44)20
V1723 Aql1.23 × 102261.76 (0.49–4.97)140Weston et al. (2016)
V5587 Sgr4.09 × 1021N/A1.56 (0.30–3.67)126
V5588 Sgr5.47 × 10217.62.15 (0.65–5.67)122Munari et al. (2015)
T Pyx1.88 × 10213.5 ± 11.87 (0.43–8.19)35Schaefer (2010)
V1312 Sco5.14 × 1021N/A1.61 (0.47–4.64)118
PR Lup4.82 × 1021N/A1.25 (0.39–3.76)144
V1313 Sco4.77 × 1021N/A1.09 (0.26–3.71)55
V965 Per1.20 × 1021N/A3.56 (1.37–8.18)17
V834 Car4.98 × 1021N/A1.49 (0.38–5.09)121
V1368 Cen4.30 × 1021N/A1.37 (0.46–3.50)47
V2676 Oph3.02 × 1021N/A1.34 (0.36–3.56)89
V5589 Sgr3.35 × 1021N/A2.21 (0.47–5.85)111
V5590 Sgr2.64 × 1021N/A2.19 (0.70–5.50)107
V2677 Oph3.38 × 1021N/A3.46 (0.79–11.27)44
V1324 Sco4.35 × 10214.52.56 (0.79–6.05)47Ackermann et al. (2014)
V5591 Sgr4.27 × 1021N/A2.31 (0.61–6.59)134
V5592 Sgr1.49 × 1021N/A2.01 (0.72–5.96)93
V5593 Sgr6.54 × 1021N/A2.31 (0.66–5.97)115
V959 Mon6.29 × 10213.62.68 (0.71–9.77)118Shore et al. (2013)
V1724 Aql1.47 × 1022N/A2.49 (0.61–7.11)133
V809 Cep8.22 × 10216.51.98 (0.65–5.25)93Munari et al. (2014)
V1533 Sco7.42 × 1021N/A2.10 (0.66–4.36)84
V339 Del1.36 × 10214.22.04 (0.64–6.08)140Shore (2013)
V1830 Aql1.23 × 1022N/A3.08 (0.86–8.20)128
V556 Ser4.87 × 1021N/A2.54 (0.93–6.70)89
V1369 Cen5.84 × 10212.42.58 (0.74–8.95)83Shore et al. (2014)
V962 Cep3.30 × 1021N/A2.72 (1.11–11.86)125
V1534 Sco3.88 × 1021131.77 (0.79–4.24)22Joshi et al. (2015)
V2659 Cyg4.92 × 1021N/A2.27 (0.73–6.13)124

*U Sco, V1310 Sco, V5666 Sgr, and V745 Sco listed in table 1 are removed (see text).

Total Galactic H i column density toward the source as the average of the values obtained by the Leiden/Argentine/Bonn (LAB) map (Kalberla et al. 2005) and the DL map (Dickey & Lockman 1990), calculated using the HEASARC website 〈http://heasarc.gsfc.nasa.gov/cgi-bin/Tools/w3nh/w3nh.pl〉.

90% C.L. upper limit for the flux in the 2–4 keV band for each scan in units of 10−2 counts s−1 cm−2. The average (minimum and maximum) fluxes among Ns scans are shown.

§Number of GSC scans in the searched period.

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