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Table 2

Summary of pixel sampling, objective standard deviation (σobj), and required signal-to-noise ratio (S/N) values for stellar temperature intervals considered in this study.

Pixels σobj (K) 2500–5000 K S/N req. 5000–10 000 K S/N req. σobj (K) 10 000–20 000 K S/N req. 20 000–30 000 K S/N req. 30 000–37 500 K S/N req.
2 20 1500–4660 4660–>50 000 500 800–2940 2940->50 000 >50 000
2 100 290–870 870–3570 1000 380–1490 1490–3400 3400->50 000
2 150 220–620 620–2320 1500 280–990 990–2260 2260–3210
3 20 1200–3690 3690–>50 000 500 750–2920 2920–>50 000 >50 000
3 100 280–820 820–3280 1000 300–1370 1370–2740 2740–4000
3 150 200–600 600–2070 1500 220–930 930–1800 1800–2470
4 20 1070–3460 3460–>50 000 500 710–2580 2580–>50 000 >50 000
4 100 260–800 800–2940 1000 310–1290 1290–2660 2660–3730
4 150 200–560 560–2030 1500 240–830 830–1650 1650–2290
5 20 1130–3430 3430–>50 000 500 710–2480 2480–>50 000 >50 000
5 100 240–780 780–2870 1000 340–1250 1250–2590 2590–3710
5 150 170–560 560–1990 1500 180–750 750–1610 1610–1830
6 20 1120–3350 3350–>50 000 500 620–2470 2470–>50 000 >50 000
6 100 240–730 730–2840 1000 450–1170 1170–2490 2490–3100
6 150 160–540 540–1960 1500 210–750 750–1350 1350–1680
7 20 1110–3340 3340–>50 000 500 580–2370 2370–>50 000 >50 000
7 100 230–700 700–2740 1000 330–1130 1130–2210 2210–2860
7 150 160–480 480–1880 1500 170–570 570–1120 1120–1490
8 20 1080–3220 3220–>50 000 500 530–2190 2190–4690 4690->50 000
8 100 230–650 650–2570 1000 240–970 970–1920 1920–2450
8 150 150–450 450–1620 1500 150–540 540–960 960–1270

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