Complement to VIII/85A

Source 7C_004527.69+400532.00: 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
74 VLSS J0048.2+4021 6.81e+03 1.4e+03 79.98 1757 5 -0.93 5.62 012.0546 +40.3647 151 7C 004527.69+400532.00 3.69e+03 7.4e+02 70.20 1757 5 -0.93 5.62 012.0538 +40.3647 178 4C +40.03 3.40e+03 1.0e+03 690.00 1757 5 -0.93 5.62 012.0463 +40.4017 232 MY 004527.8+402146.4 2.67e+03 5.3e+02 150.00 1757 5 -0.93 5.62 012.0542 +40.3629 325 WN B0045.4+4005 2.12e+03 4.2e+02 12.00 1757 5 -0.93 5.62 012.0543 +40.3654 408 B2.3 0045+40 1.95e+03 3.9e+02 0.00 1757 5 -0.93 5.62 012.0504 +40.3650 408 B3 0045+400 1.73e+03 3.5e+02 84.00 1757 5 -0.93 5.62 012.0546 +40.3639 1400 NVSS J004812+402152 6.12e+02 1.2e+02 45.00 1757 5 -0.93 5.62 012.0539 +40.3646 1400 WB 0045+4005 6.67e+02 1.3e+02 120.00 1757 5 -0.93 5.63 012.0546 +40.3639 4730 B3a 0045+400 1.61e+02 3.2e+01 168.00 1757 5 -0.93 5.62 012.0547 +40.3641 4850 87GB 004527.9+400530 1.86e+02 3.7e+01 138.00 1757 5 -0.91 5.58 012.0546 +40.3642 4850 BWE 0045+4005 1.39e+02 2.8e+01 138.00 1757 5 -0.93 5.63 012.0546 +40.3639 4850 GB6 B0045+4005 1.75e+02 3.5e+01 108.00 1757 5 -0.90 5.55 012.0533 +40.3661 4850 MITG J004811+4022 1.28e+02 2.6e+01 258.00 1757 5 -0.93 5.62 012.0479 +40.3742 10600 B3VLA 74 6.70e+01 1.3e+01 69.00 1757 5 -0.93 5.62 012.0533 +40.3647

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
74 VLSS J0048.2+4021 6.81e+03 1.4e+03 79.98 1757 012.0546 +40.3647 151 7C 004527.69+400532.00 3.69e+03 7.4e+02 70.20 1757 012.0538 +40.3647 178 4C +40.03 3.40e+03 1.0e+03 690.00 1757 012.0463 +40.4017 232 MY 004527.8+402146.4 2.67e+03 5.3e+02 150.00 1757 012.0542 +40.3629 325 WN B0045.4+4005 2.12e+03 4.2e+02 12.00 1757 012.0543 +40.3654 365 TXS 0045+400 1.31e+03 2.6e+02 6.00 -1757 012.0544 +40.3647 408 B2.3 0045+40 1.95e+03 3.9e+02 0.00 1757 012.0504 +40.3650 1400 NVSS J004815+402341 2.39e+01 4.8e+00 45.00 -1757 012.0652 +40.3949 1400 WB 0045+4005 6.67e+02 1.3e+02 120.00 1757 012.0546 +40.3639 4730 B3a 0045+400 1.61e+02 3.2e+01 168.00 1757 012.0547 +40.3641 4850 87GB 004527.9+400530 1.86e+02 3.7e+01 138.00 1757 012.0546 +40.3642 4850 MITG J004811+4022 1.28e+02 2.6e+01 258.00 1757 012.0479 +40.3742 10600 B3VLA 74 6.70e+01 1.3e+01 69.00 1757 012.0533 +40.3647

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