Table A.1
Velocity broadening upper limits and total line widths.
3.4′ RGS extraction region | 0.8′ RGS extraction region | 0.8′ free spatial broadening | ||||||
Source | 1σ a | 2σ a | FWHM c | 1σ a | 2σ a | FWHM c | 1σ b | 2σ b |
|
||||||||
2A0335+096 | 80 | 240 | 2920 ± 140 | 150 | 400 | 2240 ± 140 | 570 | 880 |
A 85 | 290 | 440 | 2100 ± 500 | 220 | 340 | 720 ± 160 | 580 | 910 |
A 133 | 280 | 440 | 1610 ± 220 | 230 | 380 | 1170 ± 140 | 980 | 1050 |
A 189 | 530 | 840 | 1980 ± 320 | 700 | 910 | 1350 ± 190 | 600 | 950 |
A 262 | 180 | 370 | 4570 ± 410 | 180 | 310 | 2340 ± 450 | 170 | 300 |
A 496 | 310 | 540 | 3150 ± 220 | 270 | 450 | 1970 ± 170 | 1250 | 1520 |
A 1795 | 610 | 990 | 2590 ± 320 | 540 | 810 | 1687 ± 320 | 2100 | 2300 |
A 1991 | 270 | 500 | 830 ± 250 | 250 | 460 | 480 ± 230 | 300 | 520 |
A 2029 | 330 | 560 | 1470 ± 700 | 410 | 690 | 720 ± 260 | 330 | 500 |
A 2052 | 190 | 420 | 2800 ± 500 | 180 | 430 | 2289 ± 220 | 570 | 910 |
A 2199 | 380 | 620 | 3800 ± 300 | 240 | 420 | 2540 ± 230 | 330 | 560 |
A 2597 | 480 | 720 | 1730 ± 270 | 300 | 510 | 1130 ± 170 | 1200 | 1300 |
A 2626 | 900 | 1500 | 3300 ± 900 | 850 | 1250 | 2440 ± 610 | 1600 | 2300 |
A 3112 | 420 | 650 | 2000 ± 170 | 270 | 450 | 1120 ± 130 | 1240 | 1390 |
A 3526 | 260 | 360 | 3930 ± 110 | 190 | 260 | 2470 ± 160 | 290 | 400 |
A 3581 | 610 | 980 | 4390 ± 220 | 410 | 670 | 2980 ± 260 | 700 | 960 |
A 4038 | 5180 | 6480 | 8100 ± 800 | 930 | 1540 | 4700 ± 750 | 2600 | 3200 |
A 4059 | 420 | 680 | 2620 ± 250 | 360 | 600 | 1860 ± 180 | 1490 | 1730 |
AS 1101 | 340 | 550 | 2650 ± 200 | 270 | 450 | 1790 ± 180 | 600 | 910 |
AWM 7 | 8000 | 10 000 | 12 600 ± 700 | 1000 | 1430 | 10 500 ± 700 | 150 | 600 |
EXO 0422 | 480 | 770 | 1520 ± 280 | 400 | 680 | 1020 ± 230 | 1300 | 1400 |
Fornax | 160 | 260 | 2500 ± 500 | 160 | 230 | 820 ± 100 | 170 | 260 |
HCG 62 | 150 | 290 | 2180 ± 190 | 140 | 270 | 1420 ± 90 | 350 | 560 |
Hydra-A | 360 | 730 | 3990 ± 400 | 550 | 920 | 2420 ± 370 | 460 | 1050 |
M 49 | 190 | 310 | 3180 ± 190 | 150 | 240 | 1350 ± 100 | 220 | 320 |
M 86 | 650 | 1100 | 7500 ± 400 | 400 | 690 | 5960 ± 490 | 390 | 660 |
M 87 | 3800 | 4100 | 5290 ± 150 | 100 | 210 | 3850 ± 150 | 170 | 470 |
M 89 | 740 | 910 | 1700 ± 180 | 710 | 900 | 1300 ± 190 | 460 | 670 |
MKW 3s | 350 | 600 | 4010 ± 570 | 360 | 590 | 2170 ± 250 | 430 | 680 |
MKW 4 | 310 | 550 | 3620 ± 330 | 360 | 580 | 2040 ± 140 | 380 | 620 |
NGC 507 | 2500 ± 1000 | 2500 ± 1500 | 6100 ± 900 | 1500 ![]() |
2800 | 4600 ± 500 | 3000 ± 1200 | 5000 |
NGC 1316 | 20 | 210 | 1770 ± 120 | 110 | 330 | 1160 ± 90 | 90 | 240 |
NGC 1404 | 250 | 390 | 1930 ± 130 | 520 | 680 | 1470 ± 130 | 540 | 650 |
NGC 1550 | 860 | 1320 | 7500 ± 700 | 890 | 1100 | 3750 ± 250 | 1130 | 1250 |
NGC 3411 | 290 | 710 | 3830 ± 360 | 610 | 1030 | 2230 ± 310 | 370 | 720 |
NGC 4261 | 160 | 300 | 760 ± 120 | 140 | 220 | 470 ± 350 | 160 | 230 |
NGC 4325 | 300 | 520 | 1570 ± 240 | 310 | 490 | 1060 ± 180 | 440 | 680 |
NGC 4374 | 120 | 250 | 1770 ± 140 | 180 | 310 | 1400 ± 490 | 160 | 280 |
NGC 4636 | 140 | 190 | 2410 ± 70 | 130 | 180 | 1660 ± 60 | 190 | 300 |
NGC 4649 | 210 | 320 | 1520 ± 80 | 130 | 250 | 1050 ± 70 | 280 | 390 |
NGC 5044 | 80 | 220 | 4170 ± 180 | 100 | 240 | 3100 ± 200 | 140 | 400 |
NGC 5813 | 100 | 140 | 4080 ± 80 | 120 | 160 | 2980 ± 120 | 110 | 160 |
NGC 5846 | 40 | 80 | 2100 ± 60 | 20 | 130 | 1670 ± 50 | 100 | 190 |
Perseus | 320 | 460 | 4950 ± 140 | 620 | 880 | 4381 ± 390 | 1000 | 1600 |
Notes.
Velocity 1σ and 2σ upper limits for the RGS spectra extracted within the 3.4′ and 0.8′ regions centered on the source emission peak. For NGC 507, we quote the best-fit velocities. The spatial line broadening was subtracted through the MOS 1 maps (see Figs. 3 and A.2 left panel).
Velocity limits for the 0.8′ region obtained by subtracting the best-fit spatial line broadening (see Sect. 4.2 and Fig. A.2 right panel).
Total (spatial + velocity) line widths with 1σ uncertainties (see Sect. 4.3).
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