Source Summary Page: G043.1616+00.0120
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CORNISH 5 GHz Radio Continuum Data
Annotations: Green =
current source, White = high-reliability sources (≥ 7σ),
Yellow = 6 to 7σ sources, Red = 5 to 6σ sources.
Click within 10'' of any source with σ > 6 to
open its data summary page in a new window.
CORNISH Catalogue Entry
Source Name |
Source Type |
RA (J2000) |
Dec (J2000) |
Flux(mJy) |
Peak(mJy/bm) |
RMS Noise(mJy/bm) |
Angular Size(arcsec) |
Sigma |
LikelyArtefact? |
G043.1616+00.0120 |
Unclassified |
19:10:12.69 |
09:05:58.75 |
28.14 |
9.55 |
1.80 |
2.57 |
5.7 |
Unclassified |
Uncertainties: |
Confidence:-- |
0.309'' |
0.444'' |
7.93 |
1.99 |
  |
0.421 |
  |
  |
Click on the "likely artefact" edit the source artefact status or
the "source type" to classify the source type.
CORNISH Catalogue Flags:
In cluster?a |
Yes |
Near survey edge?b |
No |
High-noise region?c |
Yes |
High 5σ density?d |
Yes |
Near bright source?e |
No |
Smooth Weighting?f |
Yes |
Overlap 5σ?g |
No |
Overlap 7σ?h |
No |
Nearest 5σ source |
G043.1527+00.0133(d = 32.3'') |
Nearest 7σ source |
G043.1652+00.0129(d = 13.2'') |
|
|
|
|
Notes:
a Source is within 12'' of another source.
b Source is within 2' of the survey edge.
c Source is in a region with a RMS-noise greater than
0.45 mJy/beam
d Region contains greater than 7 detections of 5 to 7-sigma
sources.
e Source is within 3' of another source which has a peak
flux density greater than 500 mJy/beam.
f Source is within the half-power primary beam-width of a
field which was imaged using the smoothed weighting scheme.
g One or more 5σ to 7σ source overlaps with the current
source.
h One or more 7σ+ sources overlaps with the current
source.
The large-scale CORNISH environment
Density map of sources above 5σ.
Below is density-map of source counts above 5σ summed under a
circle of radius 8-arcmin. Regions showing locally elevated source counts
likely contain greater numbers of spurious sources and should be inspected
carefully. The position of the current source is marked with a cross.
Notes:
The map above is sampled in 2x2 arcminute bins (pixels) whose greyscale
intensity is scaled to the number of sources detected within a radius of
eight arcminutes. Only the local ten-degree region of the
Galactic plane is plotted.
Notes:
The histogram above plots the distribution of source-density
values measured over the whole survey area (as per the density map
immediately above). The red line illustrates the value of the current
source. If this lies in the upper wing of the distribution the source is
more likely to be an artefact.
Large CORNISH images and cone-searches
Click on the links below to cutout large CORNISH mosaics or
perform preset cone-searches.
Other Radio Data
MAGPIS Radio Continuum Data
No matching MAGPIS radio data
NVSS 1.4 GHz Radio Continuum Data
Use the form below to query the NVSS postage stamp server.
The default settings open a postscript contour map, centered on the
position of the CORNISH source. The resolution of NVSS is 45''.
Infrared Data
UKIDSS Near-Infrared Data
No matching UKIDSS near-IR data
GLIMPSE Mid-Infrared Data
Notes:
The Spitzer GLIMPSE (Galactic Legacy Infrared Mid-Plane Survey
Extraordinaire) data have been obtained from the IPAC IR science archive and converted into Equatorial
J2000 format. HII regions and PNe appear as red sources in the RGB image
on the left. The environment of HII regions generally exhibits extended
emission from poly-aromatic hydrocarbons in the 8-micron images.
GLIMPSE point source catalogue matches
There are no GLIMPSE point source catalogue matches within a
radius of 2''.
WISE Mid-Infrared Data
Notes:
The NASA WISE (Wide Field Survey Infrared Explorer) data have
been obtained from the IPAC IR science archive and converted into Equatorial
J2000 format. HII regions and PNe appear as red sources in the RGB image
on the left.
MIPSGAL Mid/Far-Infrared Data
Notes:
The 24 and 70-micron
MIPSGAL
survey data was downloaded from the IPAC IR science archive and converted into Equarorial
J2000 coordinatres. The standard 70-micron images contain significant
artefacts. A 'filtered' version is also available which have had some artefact corrections applied and also emission on
large scales removed.