Complement to VIII/104

Source RGB_1753+441: 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 1 column 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/104/spectra
Post annotation
SPECFIND V3.0 Catalog of radio continuum spectra (Stein+, 2021) [ReadMe+ftp]
The parameters of the radio spectra[image] (1658207 rows)
img(gal)
start AladinLite

nu Name S(nu) e beam Seq a b RAJ2000 DEJ2000 MHz mJy mJy arcsec [mJy] deg deg
74 VLSSr J175323.0+440944 1.52e+03 3.0e+02 75.0000 236774 -0.06 3.14 268.3461 +44.1623 150 TGSSADR J175323.0+440947 1.02e+03 2.0e+02 25.0020 236774 -0.06 3.14 268.3459 +44.1633 151 7C 175154.00+441019.00 1.45e+03 2.9e+02 70.2000 236774 -0.06 3.14 268.3454 +44.1631 232 MY 175152.7+441016.8 8.40e+02 1.7e+02 150.0000 236774 -0.06 3.14 268.3400 +44.1713 325 WN B1751.8+4410 9.65e+02 1.9e+02 12.0000 236774 -0.06 3.14 268.3449 +44.1626 365 TXS 1751+441 8.64e+02 1.7e+02 6.0000 236774 -0.16 3.38 268.3454 +44.1629 408 B3 1751+441 7.60e+02 1.5e+02 84.0000 236774 -0.06 3.14 268.3442 +44.1661 1400 NVSS J175322+440946 7.66e+02 1.5e+02 45.0000 236774 -0.06 3.14 268.3449 +44.1629 1400 WB 1751+4410 7.81e+02 1.6e+02 120.0000 236774 -0.05 3.11 268.3492 +44.1667 2700 RGB11 J1753.4+4409 9.09e+02 1.8e+02 258.0000 236774 -0.15 3.35 268.3492 +44.1667 4850 87GB 175154.8+441031 9.98e+02 2.0e+02 138.0000 236774 -0.06 3.14 268.3487 +44.1664 4850 BWE 1751+4410 9.88e+02 2.0e+02 138.0000 236774 -0.13 3.29 268.3492 +44.1667 4850 GB6 B1751+4410 1.00e+03 2.0e+02 108.0000 236774 -0.15 3.35 268.3492 +44.1669 4850 MITG J175325+4409 1.12e+03 2.2e+02 258.0000 236774 -0.06 3.14 268.3554 +44.1536 4885 [P82a] 1751+441 8.60e+02 1.7e+02 6.0000 236774 -0.06 3.13 268.3440 +44.1627 4885 RGB 1753+441 1.00e+03 2.0e+02 4.0200 236774 -0.06 3.13 268.3443 +44.1627 5000 RGB6 J1753.4+4409 1.16e+03 2.3e+02 144.0000 236774 -0.06 3.14 268.3492 +44.1667 5000 VIPS J17533+4409 5.45e+02 1.1e+02 0.0009 236774 -0.13 3.29 268.3443 +44.1627 8400 CLASS J175322.6450+440945.680 8.10e+02 1.6e+02 0.3300 236774 -0.13 3.29 268.3443 +44.1627 8400 CRATES J175323+441001 8.10e+02 1.6e+02 6.0000 236774 -0.06 3.13 268.3444 +44.1627 8400 JVAS J1753+441 8.32e+02 1.7e+02 0.3300 236774 -0.06 3.14 268.3444 +44.1627 8400 [PK2012]8IVS 1751+441 8.00e+02 1.6e+02 0.0020 236774 0.00 2.94 268.3443 +44.1627 10700 RGB2 J1753.4+4409 9.80e+02 2.0e+02 72.0000 236774 0.03 2.87 268.3492 +44.1667 30000 [PGB2011] J1753+4409 4.23e+02 8.5e+01 72.0000 236774 -0.15 3.35 268.3446 +44.1627

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/104/waste
Post annotation
SPECFIND V3.0 Catalog of radio continuum spectra (Stein+, 2021) [ReadMe+ftp]
Source parameters based on positional cross-id[spectrum] (3570814 rows)
img(gal)
start AladinLite

nu Name S(nu) e beam Seq RAJ2000 DEJ2000 MHz mJy mJy arcsec deg deg
1400 NVSS J023802-044326 8.90e+00 1.8e+00 45.0000 -236774 039.5101 -04.7239

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