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Home All issues Volume 502 / No 1 (July IV 2009) A&A, 502 1 (2009) 67-84 Full HTML
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Table 1:

Original list of targets for the MIDI SDT and GTO programme on AGN.
Galaxy Alternative       D $\Delta(1~{\rm pc})$ Coudé guide star $F_{11.9~{\rm\mu m}}$
name name RA (J2000) Dec (J2000) type [Mpc] [mas] $\psi$ [''] V [mag] [Jy]
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10)
NGC 253   $00\;47\;32.82$ $-25\;17\;19.6$ HII 3 60 none 2.04
NGC 1068 M 77 $02\;42\;40.70$ $-00\;00\;48.0$ Sy 2 14 14 57 17  
NGC 1365   $03\;33\;36.38$ $-36\;08\;25.7$ Sy 1.8 18 11 65 15 0.61
IRAS 05189-2524 LEDA 17155 $05\;21\;01.40$ $-25\;21\;45.3$ Sy 2 170 1.2 none 0.55
MCG-05-23-016 ESO 434-G040 $09\;47\;40.19$ $-30\;56\;56.4$ Sy 2 35 6 22 15 0.65
Mrk 1239   $09\;52\;19.10$ $-01\;36\;43.5$ Sy 1.5 80 2.5 54 15 0.64
NGC 3256   $10\;27\;51.24$ $-43\;54\;13.9$ HII 40 5 32 15 0.55
NGC 3281   $10\;31\;52.10$ $-34\;51\;13.3$ Sy 2 45 5 22 16 0.63
NGC 3783   $11\;39\;01.71$ $-37\;44\;19.0$ Sy 1 40 5 45 17 0.59
NGC 4151   $12\;10\;32.63$ $+39\;24\;20.7$ Sy 1.5 14 15 none  
3C 273   $12\;29\;06.70$ $+02\;03\;08.6$ QSO 650 0.3 53 14 0.35
Centaurus A NGC 5128 $13\;25\;27.62$ $-43\;01\;08.8$ FR I 4 54 44 13 1.22
IC 4329A ESO 445-G050 $13\;49\;19.35$ $-30\;18\;34.4$ Sy 1.2 65 3.1 58 17 0.35
Mrk 463E   $13\;56\;02.89$ $+18\;22\;18.2$ Sy 1/2 200 1.0 none 0.34
Circinus ESO 097-G013 $14\;13\;09.95$ $-65\;20\;21.2$ Sy 2 4 50 50 12 9.70
NGC 5506 Mrk 1376 $14\;13\;14.88$ $-03\;12\;27.7$ Sy 1.9 25 8 none 0.91
NGC 7469 Mrk 1514 $23\;03\;15.68$ $+08\;52\;26.3$ Sy 1.2 65 3.1 13 15 0.41
NGC 7582   $23\;18\;23.63$ $-42\;22\;13.1$ Sy 2 22 10 54 17 0.67
Notes: the columns are: (1) the name of the galaxy used in this paper; (2) an alternative name for the galaxy; (3) and (4) the coordinates of the nucleus used for the MIDI observations or, if no observations were carried out, the 2MASS coordinates; (5) the galaxy type (from NED); (6) the distance to Earth assuming $H_{0}=73~{\rm km}~{\rm s}^{-1}~{\rm Mpc}^{-1}$; (7) the angular size corresponding to $1~{\rm pc}$ in the target; (8) the angular distance $\psi$ and (9) the visual magnitude V of the best Coudé guide star (if present); (10) the flux at $11.9~{\rm\mu m}$from Raban et al. (2008).

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