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Table 1.

Summary of the EHT 2017 observations at 230 GHz.

Common B1950 J2000 Redshift z Type Volume Days (Apr. 2017) Sites BL (km) Ref.
Sagittarius A* 1742–286 J1750–2900 23024 5, 6, 7, 10, 11 all 11204 (1)
3C 279 1253–055 J1256–0547 0.538 Q 9638 5, 6, 10, 11 all 11297 (2)
M 87 1228+126 J1230+1223 0.0042 R 8846 5, 6, 10, 11 all but Y 10835 (3)
OJ 287 0851+202 J0854+2006 0.306 B 4548 5, 10, 11 all but Y 10834 (4)
Centaurus A 1322–427 J1325-4303 0.0014 R 3218 10 all but P 10749 (5)
J1924–2914 1921–293 J1924–2914 0.353 Q 2937 5, 6, 7, 10, 11 all 11091 (6)
NRAO 530 1730–130 J1733–1304 0.902 Q 1439 5, 6, 7 all 11305 (7)
3C 273 1226+023 J1229+0203 0.158 Q 642 6 all but Y 9372 (8)
1749+096 1749+096 J1751+0939 0.322 B 612 10 J, L, S, X, Z 9342
1055+018 1055+018 J1058+0133 0.89 Q 488 5, 10, 11 all but Y 8904
BL Lacertae 2200+420 J2202+4216 0.069 B 174 7 J, S, X, Z 8934
3C 84 0316+413 J0319+4130 0.0177 R 141 7 A, J, S, X, Z 9344 (9)
3C 454.3 2251+158 J2253+1608 0.859 Q 139 7 J, S, X 9382
CTA 102 2230+114 J2232+1143 1.037 Q 118 7 J, S, X 9384
J0132–1654 0130–171 J0132–1654 1.020 Q 65 6, 7 A, J, P, Y 11263
J0006–0623 0003–066 J0006–0623 0.347 B 36 7 A, J, P, Y 11211
NGC 1052 0238–084 J0241–0815 0.0049 R 20 6, 7 A, J, S, Y 5895 (10)
Cygnus X–3 2030+407 J2032+4057 X 16 5 J, S < 0.2

Notes. The names listed in column “Common” follow the convention used by the EHT, and sometimes coincide with the “B1950” or “J2000” designations. Object types: B: BL Lac object; Q: quasar; R: radio galaxy; X: X-ray binary. Sites: A = ALMA; J = JCMT; L = LMT; P = PV; S = SMA; X = APEX; Y = SPT; Z = SMT. Redshifts taken from SIMBAD (Wenger et al. 2000); Sgr A* and Cyg X–3 are galactic sources. Volume: Total number of detections; BL: Maximum projected baseline. (1) The Event Horizon Telescope Collaboration (2022a); (2) Kim et al. (2020); (3) The Event Horizon Telescope Collaboration (2019a; (4) Gómez et al. in prep.; (5) Janssen et al. (2021); (6) Issaoun et al. (2022); (7) Jorstad et al. (2023); (8) Wielgus et al. (in prep.); (9) Paraschos et al. (2024); (10) Baczko et al. (2024).

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