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Table 1:

List of optical, near-IR, and radio observatories contributing data to this work.
Observatory Tel. size Bands
Optical
Abastumani, Georgia 70 cm R
ARIES, India 104 cm BVRI
Armenzano, Italy 35 cm BRI
Armenzano, Italy 40 cm BVRI
Belogradchik, Bulgaria 60 cm VRI
BOOTES-2, Spain 30 cm R
Bordeaux, France 20 cm V
Calar Alto, Spaina 220 cm R
Crimean, Ukraine 70 cm BVRI
Kitt Peak (MDM), USA 130 cm UBVRI
L'Ampolla, Spain 36 cm R
Lulin (SLT), Taiwan 40 cm R
Michael Adrian, Germany 120 cm R
Mt. Lemmon, USA 100 cm BVRI
New Mexico Skies, USA 30 cm VRI
Roque (KVA), Spain 35 cm R
Roque (NOT), Spain 256 cm UBVRI
Rozhen, Bulgaria 50/70 cm BVR
Rozhen, Bulgaria 200 cm BVRI
Sabadell, Spain 50 cm R
San Pedro Martir, Mexico 84 cm R
Sobaeksan, South Korea 61 cm VRI
Sommers-Bausch, USA 61 cm VRI
St. Petersburg, Russia 40 cm BVRI
Talmassons, Italy 35 cm BVR
Teide (BRT), Spain 35 cm BVR
Torino, Italy 105 cm BVRI
Tuorla, Finland 103 cm R
Univ. of Victoria, Canada 50 cm R
Valle d'Aosta, Italy 81 cm BVRI
Near-infrared
Campo Imperatore, Italy 110 cm JHK
Roque (NOT), Spain 256 cm HK
Radio
Crimean (RT-22), Ukraine 22 m 37 GHz
Mauna Kea (SMA), USA $8 \times 6$ mb 230, 345 GHz
Medicina, Italy 32 m 5, 8, 22 GHz
Metsähovi, Finland 14 m 37 GHz
Noto, Italy 32 m 43 GHz
UMRAO, USA 26 m 4.8, 8.0, 14.5 GHz

a Calar Alto data were acquired as part of the MAPCAT (Monitoring
AGN with Polarimetry at the Calar Alto Telescopes) project.
b Radio interferometer including 8 dishes of 6 m size.

Source LaTeX | All tables | In the text

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