Table 8: References of the compiled effective temperatures for CP stars. The different groups of peculiar stars discussed in the text are separated by horizontal lines.
HD/DM $\overline{T}_{\rm eff}$ [K] Ref. HD/DM $\overline{T}_{\rm eff}$ [K] Ref.
27 628 7210(90) (1) a; (2) d+ 171 247 12 170 (21) d+
27 749 7340(180) (1) a; (2),(5) d+; (3),(4) d 171 782 11 500 (26) c+
27 962 9070(210) (2) d+; (6) d; (7) bd+ 173 650 10 000(1410) (18) b; (25) d+
28 226 7450 (2) d+ 175 744 12 620(140) (23),(24) a
28 355 7950 (2) d+ 176 232 7730(140) (18) b; (28) bd+; (38) a; (51) b+
28 527 8000(100) (1) a; (2) d+ 183 806 9940(190) (22) b+; (52) bd
28 546 7640(140) (1) a; (2) d+ 188 041 8580(550) (3) d; (18) b; (22) b+
29 140 7940 (2) d+ 191 742 8300 (53) c+
29 499 7690 (2) d+ 192 678 9000 (27) e
30 210 8100 (2) d+ 196 502 8900(360) (25) d+; (26) c+; (28) bd+
33 204 7650 (2) d+ 201 601 7780(130) (3) d; (18) b; (20),(28) bd+
33 254 7760(190) (1) a; (2) d+     (22) b+; (37) a; (50) d+
58 142 9500 (7) bd+ 203 932 7450 (54) d+
67 523 6700 (8) a 204 411 8510(170) (20),(28),(55) bd+; (38) a
78 362 7220(230) (2),(5) d+ 212 385 9200 (22) b+
94 334 10 030 (9) d+ 215 441 14 000 (26) c+
95 418 9600(10) (10) b; (11) bd+ 217 522 6750 (50) d+
95 608 8950(430) (2) d+; (12) bd 220 825 9200(80) (32),(38) a
97 633 9250(180) (10) b; (13) a 221 006 13 260(20) (23),(24) a
141 795 8420 (14) bd 223 640 12 240(210) (18) b; (23),(24) a
162 132 8800 (15) d+    
173 648 8160 (12) bd 358 13 830(40) (56) cd+; (70) bd+
182 564 9130 (11) bd+ 4335 12 000 (3) d
188 728 9530 (9) d+ 27 295 11 850(210) (3) d; (28) bd
189 849 7820(110) (2) d+; (16) d; (17) bd+ 27 376 12 300 (42) a
196 724 10 200 (14) bd 33 904 12 160(210) (3) d; (28) bd; (32) a
206 088 7640 (18) b 35 497 13 320(100) (10) b; (28) bd
209 625 7820(100) (2) d+; (3) d; (17) bd+ 35 548 11 500 (3) d
213 320 10 130 (14) bd 58 661 13 200 (3) d
214 994 9590(20) (3) d; (10) b; (19) bd 77 350 10 250 (28) bd
    78 316 13 040(230) (23) a; (28) bd; (58) c+
8441 9200 (20) bd+ 89 822 10 950(70) (25) d+; (59) bd+
9484 10 200 (21) d+ 106 625 12 130 (28) bd
12 098 7800 (22) b+ 143 807 10 930(460) (3) d; (60) bd
12 767 13 000(340) (21) d+; (23),(24) a 144 206 11 740(300) (28) bd; (61) b+
15 089 8280(40) (25) d+; (26) c+ 145 389 11 690(160) (3) d; (28) bd
18 610 8100 (22) b+ 147 550 10 200 (28) bd
19 832 12 430(360) (26) c+; (27) e; (28) bd+ 159 082 11 300 (15) d+
23 387 8250 (26) c+ 190 229 13 190(440) (3) d; (28) bd
24 155 13 780(70) (23),(24) a    
24 712 7290(60) (29) d; (30) d+ 4382 13 400 (3) d
25 823 12 720(200) (26) c+; (27) e; (31) d 19 400 13 000 (62) e
26 571 11 750 (26) c+ 23 408 11 900(990) (62) e, (63) bd
27 309 11 930(250) (26) c+; (27) e 49 606 13 500 (62) e
32 549 9730 (32) a 51 688 12 500 (62) e
34 452 13 830(810) (26) c+; (27) e 144 661 15 000 (62) e
37 470 13 000 (26) c+ 144 667 12 900(70) (64),(65) d+
37 808 12 890(200) (23),(24) a; (33) d+ 144 844 12 430(460) (26) c+; (62) e
40 312 10 180(200) (26) c+; (27) e; (32) a; (34) bd+ 202 671 13 150(70) (62) e; (66) d+
43 819 10 930(290) (20) bd+; (23),(24) a; (26) c+ 224 926 14 000 (42) a
60 435 8100 (22) b+    
62 140 7800(140) (22) b+; (25) d+ 21 699 16 000 (67) d+
65 339 8170(150) (25) d+; (26) c+; (27) e 22 470 13 760(250) (23),(42) a; (62) e
71 866 9000 (25) d+ 22 920 14 100(260) (21) d+; (42) a; (62) e
75 445 7700 (22) b+ 28 843 14 830(150) (23),(42) a; (62) e
81 009 8250(350) (25) d+; (35) b 37 058 19 610 (23) a
90 569 10 500 (25) d+ 49 333 15 810(120) (23),(42) a; (62) e
92 664 14 300(90) (23),(24) a; (26) c+ 62 712 13 530(240) (23),(24),(42) a
94 427 7500 (25) d+ 74 196 13 950(350) (42) a; (62) e
108 662 10 330(570) (18) b; (25) d+; (26) c+; (28) bd+ 79 158 13 250(70) (27) e; (68) cd+
108 945 8700(240) (18) b; (25) d+; (26) c+; (27) e 90 264 14 600 (42) a
    (28) bd+; (36) a c+ 109 026 15 500 (42) a
110 066 9030(60) (20) bd+; (22) b+; (25) d+ 137 509 12 680(110) (42) a; (69) d+
111 133 9850(220) (18) b; (25) d+ 142 301 15 860(150) (23),(42) a; (62) e
112 185 9350(290) (25) d+; (28) bd+; (32),(37) a 142 990 17 700(1130) (42) a; (62) e
112 413 11 210(360) (26) c+; (37),(38) a; (39) b+; (40) bd+ 143 699 15 490(410) (23),(42) a
115 708 7760(350) (25) d+; (29) d 144 334 14 760(380) (23),(42) a; (62) e
116 114 7850(210) (22) b+; (25) d+ 146 001 13 790(300) (23),(42) a
118 022 9460(410) (18) b; (25) d+; (26) c+; (28) bd+ 162 374 15 900(280) (42) a; (62) e
    (32) a; (41) ac+ 175 362 16 790(620) (23),(24) a; (62) e
120 198 10 080(330) (26) c+; (27) e; (28) bd+ 217 833 15 450 (67) d+
124 224 12 540(300) (23),(24),(32),(42) a; (26) c+; (28) bd+    
125 248 9650(260) (25) d+; (26) c+; (27) e; (41) a c+ 5737 13 970(400) (42) a; (66) d+; (70) b+
126 515 9500 (25) d+ 125 823 18 940(500) (23),(42) a; (62) e
128 898 7660(340) (43) d+; (44) e    
133 029 10 880(300) (26) c+; (27) e; (28),(45) bd+ -27 3748 23 000 (71) d+
133 792 9300(140) (46),(47) d+ -46 4639 22 500 (71) d+
133 880 10 700(60) (23),(24) a -62 2124 26 000 (71) d+
134 305 8200 (25) d+ 36 485 18 000 (71) d+
137 909 8340(360) (18) b; (22) b+; (25) d+; (28) bd+ 37 017 18 950(640) (42) a; (71) d+
137 949 7530(40) (22) b+; (25) d+ 37 479 22 500(710) (62) e; (71) d+
140 160 9120(60) (18) b; (28) bd+; (38) a 37 776 22 270(640) (42) a; (62) e; (71) d+
144 897 11 250 (48) d+ 58 260 19 000(0) (42) a; (62) e; (71) d+
148 112 9220(160) (18) b; (38) a 60 344 22 500(2120) (62) e; (71) d+
149 822 10 750 (28) bd+ 64 740 22 270(1100) (42) a; (62) e; (71) d+
151 525 9240(130) (18) b; (38) a 66 522 18 000 (71) d+
152 107 8730(230) (25) d+; (26) c+; (41) ac+ 92 938 15 000 (71) d+
153 882 9450(580) (18) b; (25) d+; (28) bd+ 96 446 20 950(640) (42) a; (71) d+
155 102 9000 (15) d+ 108 483 19 200 (71) d+
157 751 11 300 (49) d+ 133 518 18 250(1060) (42) a; (71) d+
166 473 7850(210) (22) b+; (50) d+ 260 858 18 000 (71) d+
168 733 13 320 (23) a 264 111 21 700(990) (62) e; (71) d+
170 973 10 740(20) (10) b; (28) bd+      
(1) Smalley (1993); (2) Smalley & Dworetsky (1993); (3) Allen (1977); (4) Cayrel et al. (1991); (5) van't Veer-Menneret & Mégessier (1996); (6) Liubimkov & Savanov (1983); (7) Adelman (1994b); (8) Ramírez & Meléndez (2005); (9) Caliskan & Adelman (1997); (10) Morossi & Malagnini (1985); (11) Adelman 1996; (12) Adelman et al. (1999); (13) Glushneva (1985); (14) Adelman & Albayrak (1998); (15) Catanzaro (2006); (16) Takeda (1984); (17) Adelman et al. (1997); (18) Wolff (1967); (19) Adelman (1988); (20) Adelman et al. (1995); (21) Leone & Manfre (1996); (22) Ryabchikova et al. (2004b); (23) Lanz (1985); (24) Mégessier (1988); (25) Babel (1994); (26) Lipski & Stepien (2008); (27) Stepien & Dominiczak (1989); (28) Adelman & Rayle (2000); (29) Wade (1997); (30) Ryabchikova et al. (1997); (31) Bolcal et al. (1987); (32) Glushneva (1987); (33) Leone et al. (1993); (34) van Rensbergen et al. (1984); (35) Wade et al. (2000); (36) Monier & Mégessier (1992); (37) Shallis & Blackwell (1979); (38) Shallis et al. (1985); (39) Ryabchikova et al. (1999a); (40) Kochukhov et al. (2002); (41) Monier (1992); (42) Hunger & Groote (1999); (43) Kupka et al. (1996); (44) Bruntt et al. (2008); (45) López-García & Adelman (1999); (46) Ryabchikova et al. (2004a); (47) Kochukhov et al. (2006); (48) Ryabchikova et al. (2006); (49) Hubrig & Nesvacil (2007); (50) Gelbmann (1998); (51) Ryabchikova et al. (2000); (52) Kearsley & Wegner (1978); (53) Kato & Sadakane (1999); (54) Gelbmann et al. (1997); (55) Ryabchikova et al. (2005); (56) Derman (1982); (57) Ryabchikova et al. (1999b); (58) Zoechling & Muthsam (1987); (59) Adelman (1994a); (60) Adelman (1989); (61) Zavala et al. (2007); (62) Cidale et al. (2007); (63) Mon et al. (1981); (64) Catanzaro et al. (2004); (65) Castelli & Hubrig (2007); (66) Leone & Manfre (1997); (67) Glagolevskij et al. (2006); (68) Wade et al. (2006); (69) Kochukhov (2006); (70) López-García et al. (2001); (71) Zboril et al. (1997)
a: Infrared Flux Method; b: fitting models to visual energy distribution; c: fitting models to total energy distribution; d: (Balmer) line profile fitting; e: methods as described in Sect. 2. The + sign indicates that models different to solar ones were used or the solar model is justified according to abundance analysis or tests as described in the respective reference. References using the same method are combined.

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