Table 2
BN fluxes.
| Epoch | S3.6 cm [mJy] | S1.3 mm [mJy] | Notes |
|
|
|||
| 06 Sep. 1991 | 4.61 ± 0.20 | – | a |
| Nov. 1993 to Feb. 1994 | – | 150 ± 50 | b |
| 29 Apr. 1994 | 3.73 ± 0.04 | – | c |
| 22 Jul. 1995 | 3.36 ± 0.3 | – | c |
| 21 Nov. 1996 | 3.43 ± 0.1 | – | c |
| 11 Jan. 1997 | 3.90 ± 0.07 | – | c |
| 13 Nov. 2000 | 3.83 ± 0.14 | – | a |
| 12 May 2006 | 4.78 ± 0.11 | – | a |
| Mar. 2007 | – | <34 | d |
| 19 Jan. 2012 | – | 126 ± 14 | e |
Notes. a: VLA-A archival data, 
(this paper). b: OVRO observations at 218 GHz, 
(Plambeck et al. 1995; Blake et al. 1996). c: VLA-A, (Zapata et al. 2004). d: CARMA observations at 231 GHz, 
(Friedel & Snyder 2008). e: ALMA SV data, 
(this paper). The error is determined by variations in the obtained flux with different apertures in the Bmin = 100 kλ map. The flux density has been corrected for primary beam attenuation.
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