Details on Acronym: FWKK | |
| FWKK | (Fomalont+Windhorst+Kristian+Kellerman) |
| ***** | Avoid the usage of FWKK, prefer 15V |
| Origin | of the Acronym: L = Found in the literature |
Details on Acronym: 15V | |
| 15V | (15th VLA survey)= (FWKK) |
| Write: | <<15V NNa>> |
| N: | 94+2 |
| Object: | (Rad) (SIMBAD class: Radio = Radio Source) |
| Note: | Nomenclature introduced by Fomalont et al. in the style of Cambridge, Westerbork, Penticton, for sources discovered with the VLA. 1V to 14V have not been used formerly. 16V and 17V appear in ref. 1993ApJ...405..498W. Subsequent observations at 1.5 GHz, field of area 1.5x10-5 sr centered at alpha = 14h16m and Dec = 52.7deg (1950). The range of angular size detectable is between 0".3 to 100". 62 sources compiled with a peak flux density at 5 GHz greater than 16 microJy at 8" resolution and a typical positional accuracy of 0".2. Maps. |
| Ref: | =1991AJ....102.1258F |
| by | FOMALONT E.B. , WINDHORST R.A., KRISTIAN J.A., KELLERMANN K.I. |
| Astron. J., 102, 1258-None (1991) | |
| The micro-Jansky radio source population at 5 GHz. | |
| o | Table 4: <15V NN> (Nos 1-94) |
| Ref: | =1995MNRAS.276.1085H |
| by | HAMMER F. , CRAMPTON D., LILLY S.J., LE FEVRE O., KENET T. |
| Mon. Not. R. Astron. Soc., 276, 1085-1100 (1995) | |
| The Canada-France redshift survey - VII. Optical counterparts of microjansky radio sources. | |
| o | Table 1, col.(1): <15V NNa> (Nos 26a, 26b). Table 1, col.(3): <CFRS 14.NNNN> N=37. |
| Origin | of the Acronym: A = Assigned by the author(s) |