 |
 |
Source: RA (J2000): Dec (J2000): |
3652+1354 12 36 52.764 ± 0.054 62 13 54.77 ± 0.38 |
| Delta ('') |
Ssky (µJy) |
RAB (mag) |
H+K (mag) |
SISO (µJy) |
z | Type | Log P (W/Hz) |
Rel. (%) |
Contour (sigma) |
|---|---|---|---|---|---|---|---|---|---|
| 0.3 | 8 | 22.2 | 19.5 | — | 1.355 | Irr/Merg | 23.5 | 99 | -2,2,4 |
Notes:
The galaxy counterpart is possibly either a chain galaxy or a multiple
merger, as it shows evidence for six distinct optical nuclei with blue
colors (B – V = 0.2) within about 3 arcsec of the radio emission.
The optical spectrum is dominated by very strong [OII] emission and
places the galaxy at a redshift of 1.355. If the radio emission is not
contaminated by an AGN component, then we infer a SFR 
200 M
/yr. It is similar in optical
morphology to 3641+1142.