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Table 3.

Spectral fits for the seven soft IPs detected in S45.

Name Counts NH kTbb [eV] kTlit [eV] Fbol, bb Fbol, apec χ2
PQ Gem 3257 0 . 2 0.002 + 0.009 $ 0.2^{+0.009}_{-0.002} $ 47 5 + 4 $ 47^{+4}_{-5} $ 47 . 6 2.4 + 2.9 $ 47.6^{+2.9}_{-2.4} $ 2.8 2.0 1.23
V418 Gem 442 <  + 5 84 18 + 14 $ 84^{+14}_{-18} $ 84–88 0.14 0.2 0.51
UU Col 598 < 1 65 1 + 3 $ 65^{+3}_{-1} $ 73 9 + 20 $ 73^{+20}_{-9} $ 0.02 0.28 0.99
V667 Pup 1503 9 4 + 4 $ 9^{+4}_{-4} $ 74 8 + 9 $ 74^{+9}_{-8} $ 1.0 1.3 0.74
BG CMi 479 6 6 + 10 $ 6^{+10}_{-6} $ 60 20 + 30 $ 60^{+30}_{-20} $ 0.9 13.4 1.11
TX Col 3248 3 2 + 2 $ 3^{+2}_{-2} $ 95 12 + 14 $ 95^{+14}_{-12} $ 0.14 1.3 1.14
NY Lup 8705 9 1 + 1 $ 9^{+1}_{-1} $ 96 2 + 4 $ 96^{+4}_{-2} $ 104 23 + 21 $ 104^{+21}_{-23} $ 1.9 3.6 1.10

Notes. Here, we provide the object names and the numbers of photons registered in S45 followed by the spectral parameters. The bolometric fluxes are given in 10−11 erg cm−2 s−1, the hydrogen column density NH is given in units of 1020 cm−2. Errors given refer to 90% confidence.

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