Complement to VIII/85A

Source PKS_J1658+0515: points from spectra and waste tables

  Postscript Figure Additional frequencies and fluxes in ν and S Data as a Table  
Adapt
Plot
nu
S
x cuts: xlog Bitmap size:
y cuts: ylog
"-c="

The 2 columns in color are computed by VizieR, and are not part of the original data.
The column SED is a link to a plot of the radio spectrum, and the column Radio+Opt is a link to an Aladin preview. The SED plot contains points from the cross-identification (spectra; red), from the waste basket (waste; yellow), and the fitted radio spectra as lines. The Aladin preview contains a DSS image together with NVSS contours (blue) and the points and associated beams of the radio spectrum (red); points and beams of the sources from the waste basket are hidden but can be made visible by clicking on the corresponding plane (yellow).
VIII/85A/spectra
Post annotation
SPECFIND V2.0 Catalog of radio continuum spectra (Vollmer+ 2009) [ReadMe+ftp]
The parameters of the radio spectra[image][spectrum] (631736 rows)
img(gal)
start AladinLite

nu Name S(nu) e beam Seq n a b RAJ2000 DEJ2000 MHz mJy mJy arcsec [mJy] deg deg
365 TXS 1656+053 2.46e+03 4.9e+02 6.00 73252 4 -0.17 3.81 254.6395 +05.2546 408 MRC 1656+053 2.34e+03 4.7e+02 120.00 73252 4 -0.20 3.90 254.6404 +05.2528 1400 NVSS J165833+051515 1.53e+03 3.1e+02 45.00 73252 4 -0.19 3.86 254.6394 +05.2543 1400 WB 1656+0519A 1.41e+03 2.8e+02 120.00 73252 4 -0.19 3.86 254.6379 +05.2536 1465 [P82] 1656+053 1.42e+03 2.8e+02 25.80 73252 4 -0.19 3.86 254.6391 +05.2545 2700 PKS J1658+0515 1.60e+03 3.2e+02 60.00 73252 4 -0.19 3.86 254.6392 +05.2544 2700 RGB11 J1658.6+0515 1.67e+03 3.3e+02 258.00 73252 4 -0.19 3.87 254.6404 +05.2531 4850 87GB 165605.3+051943 1.60e+03 3.2e+02 138.00 73252 4 -0.18 3.86 254.6379 +05.2533 4850 BWE 1656+0519A 1.44e+03 2.9e+02 138.00 73252 4 -0.20 3.90 254.6379 +05.2536 4850 GB6 B1656+0519 1.56e+03 3.1e+02 108.00 73252 4 -0.18 3.84 254.6367 +05.2542 4850 MITG J165834+0515 1.47e+03 2.9e+02 258.00 73252 4 -0.20 3.90 254.6433 +05.2511 4850 PMN J1658+0515 1.57e+03 3.1e+02 168.00 73252 4 -0.17 3.81 254.6400 +05.2569 4885 [P82a] 1656+053 1.55e+03 3.1e+02 6.00 73252 4 -0.19 3.86 254.6391 +05.2545 4885 RGB 1658+052 1.38e+03 2.8e+02 4.02 73252 4 -0.18 3.86 254.6393 +05.2546 5000 RGB6 J1658.6+0515 1.53e+03 3.1e+02 144.00 73252 4 -0.20 3.90 254.6404 +05.2531 8400 CLASS J165833.4483+051516.443 1.29e+03 2.6e+02 0.33 73252 4 -0.20 3.90 254.6393 +05.2546 8400 JVAS J1658+0515 1.33e+03 2.7e+02 0.33 73252 4 -0.19 3.85 254.6394 +05.2546 10700 RGB2 J1658.6+0515 1.30e+03 2.6e+02 72.00 73252 4 -0.18 3.84 254.6404 +05.2531

The column SED is a link to a plot of the radio spectrum, and the column Radio+Opt is a link to an Aladin preview. The SED plot contains points from the cross-identification (spectra; red), from the waste basket (waste; yellow), and the fitted radio spectra as lines. The Aladin preview contains a DSS image together with NVSS contours (blue) and the points and associated beams of the radio spectrum (red); points and beams of the sources from the waste basket are hidden but can be made visible by clicking on the corresponding plane (yellow).
VIII/85A/waste
Post annotation
SPECFIND V2.0 Catalog of radio continuum spectra (Vollmer+ 2009) [ReadMe+ftp]
Source parameters based on positional cross-id[spectrum] (1497216 rows)
img(gal)
start AladinLite

nu Name S(nu) e beam Seq RAJ2000 DEJ2000 MHz mJy mJy arcsec deg deg
365 TXS 1656+053 2.46e+03 4.9e+02 6.00 73252 254.6395 +05.2546 408 MRC 1656+053 2.34e+03 4.7e+02 120.00 73252 254.6404 +05.2528 1400 WB 1656+0519A 1.41e+03 2.8e+02 120.00 73252 254.6379 +05.2536 2700 PKS J1658+0515 1.60e+03 3.2e+02 60.00 73252 254.6392 +05.2544 4850 BWE 1656+0519A 1.44e+03 2.9e+02 138.00 73252 254.6379 +05.2536 4850 MITG J165834+0515 1.47e+03 2.9e+02 258.00 73252 254.6433 +05.2511 4885 [P82a] 1656+053 1.55e+03 3.1e+02 6.00 73252 254.6391 +05.2545 5000 RGB6 J1658.6+0515 1.53e+03 3.1e+02 144.00 73252 254.6404 +05.2531 8400 CLASS J165833.4483+051516.443 1.29e+03 2.6e+02 0.33 73252 254.6393 +05.2546

Note: For the spectrum finding algorithm, the errors have been increased by 50%