Complement to VIII/85A

Source MY_144103.5+404424.1: 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
232 MY 144103.5+404424.1 1.22e+03 2.4e+02 150.00 106693 4 -0.43 4.19 220.7492 +40.7400 325 WN B1441.0+4057 1.74e+03 3.5e+02 12.00 106693 4 -0.55 4.62 220.7473 +40.7415 365 TXS 1441+409 1.51e+03 3.0e+02 6.00 106693 4 -0.55 4.62 220.7467 +40.7414 408 B3 1441+409 1.68e+03 3.4e+02 84.00 106693 4 -0.55 4.62 220.7475 +40.7431 1400 FIRST J144259.3+404428 9.68e+02 1.9e+02 5.00 106693 4 -0.43 4.19 220.7471 +40.7413 1400 NVSS J144259+404429 9.63e+02 1.9e+02 45.00 106693 4 -0.43 4.19 220.7472 +40.7414 1400 WB 1441+4057 9.23e+02 1.8e+02 120.00 106693 4 -0.63 4.81 220.7463 +40.7478 4850 87GB 144102.4+405726 3.94e+02 7.9e+01 138.00 106693 4 -0.55 4.63 220.7446 +40.7456 4850 BWE 1441+4057 3.22e+02 6.4e+01 138.00 106693 4 -0.63 4.81 220.7463 +40.7478 4850 GB6 B1441+4057 3.01e+02 6.0e+01 108.00 106693 4 -0.55 4.63 220.7458 +40.7456

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
151 6C 144103+405714 1.38e+03 2.8e+02 252.00 -106693 220.7479 +40.7422 151 7C 144103.20+405709.00 1.48e+03 3.0e+02 70.20 -106693 220.7475 +40.7408 232 MY 144103.5+404424.1 1.22e+03 2.4e+02 150.00 106693 220.7492 +40.7400 325 WN B1441.0+4057 1.74e+03 3.5e+02 12.00 106693 220.7473 +40.7415 365 TXS 1441+409 1.51e+03 3.0e+02 6.00 106693 220.7467 +40.7414 408 B3 1441+409 1.68e+03 3.4e+02 84.00 106693 220.7475 +40.7431 1400 FIRST J144250.7+404510 1.10e+00 2.0e-01 5.00 -106693 220.7116 +40.7530 1400 FIRST J144256.5+404527 1.60e+00 3.0e-01 5.00 -106693 220.7357 +40.7578 1400 FIRST J144259.3+404428 9.68e+02 1.9e+02 5.00 106693 220.7471 +40.7413 1400 FIRST J144305.1+404429 1.40e+00 3.0e-01 5.00 -106693 220.7713 +40.7415 1400 WB 1441+4057 9.23e+02 1.8e+02 120.00 106693 220.7463 +40.7478 4730 B3a 1441+409 3.28e+02 6.6e+01 168.00 -106693 220.7475 +40.7431 4850 87GB 144102.4+405726 3.94e+02 7.9e+01 138.00 106693 220.7446 +40.7456 4850 GB6 B1441+4057 3.01e+02 6.0e+01 108.00 106693 220.7458 +40.7456 4885 RGB 1442+407 3.01e+02 6.0e+01 4.02 -106693 220.7472 +40.7414 5000 RGB6 J1443.0+4044 3.67e+02 7.3e+01 144.00 -106693 220.7421 +40.7458 8460 [FPD2001b]b 197 2.12e+02 4.2e+01 0.20 -106693 220.7469 +40.7413 10600 B3VLA 939 1.44e+02 2.9e+01 69.00 -106693 220.7470 +40.7411

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