Differences between revisions 3 and 4
⇤ ← Revision 3 as of 2025-08-17 13:06:22 →
Size: 714
Editor: NikaBolometer
Comment:
← Revision 4 as of 2025-08-17 13:07:21 → ⇥
Size: 669
Editor: NikaBolometer
Comment:
Deletions are marked like this. Additions are marked like this.
Line 7: Line 7:
 * '''Visibility of targets:'''


   - Planets, secondary flux calibrators and bright QSOs. The latter's favorites for being the brightest in this epoch are 1641+399, 2251+1058 (3C454), 2230+114, 1749+096, 2200+420, 3C84 (0316+413).[[http://sma1.sma.hawaii.edu/callist/callist.html|Updated fluxes]]		  * Planets, secondary flux calibrators and bright QSOs. The latter's favorites for being the brightest in this epoch are 1641+399, 2251+1058 (3C454), 2230+114, 1749+096, 2200+420, 3C84 (0316+413).[[http://sma1.sma.hawaii.edu/callist/callist.html|Updated fluxes]]
Line 15: Line 12:

  - Selected targets for "deep field" observations:
  * Selected targets for "deep field" observations:

Back to the NIKA2 Run 75 main page

Sources

  • Extensive catalogs and astro scripts can be reached at the ~/PaKo/202503/ folder in the NIKA2 commissioning account.

  • Planets, secondary flux calibrators and bright QSOs. The latter's favorites for being the brightest in this epoch are 1641+399, 2251+1058 (3C454), 2230+114, 1749+096, 2200+420, 3C84 (0316+413).Updated fluxes

    • [ATTACH]

  • Selected targets for "deep field" observations:

    • [ATTACH]

ListOfAstroTargetNika2Run75 (last edited 2025-10-10 08:08:13 by NikaBolometer)