Table 3
Example of entries in the source catalogue for the 54 direction-independent calibrated images.
Source ID | RA | σRA | Dec | σDEC | Speak | σSpeak | Sint | σSint | Resolved | RMS | Type | Mosaic | |||||
(σRA,tot) | (σDEC,tot) | (σSpeak,tot) | (σSint,tot) | noise | ID | ||||||||||||
(°) | (″) | (°) | (″) | (mJy/beam) | (mJy/beam) | (mJy) | (mJy) | (mJy) | |||||||||
|
|||||||||||||||||
ILTJ104322.7+473446.5 | 160.8445 | 0.7 (1.8) | 47.5796 | 0.7 (1.8) | 8.0 | 0.5 (1.7) | 9.2 | 0.8 (2.0) | U | 0.5 | C | P3 | |||||
ILTJ105059.3+515054.5 | 162.7473 | 1.7 (2.4) | 51.8485 | 1.6 (2.3) | 3.4 | 0.4 (0.8) | 5.2 | 0.7 (1.2) | U | 0.4 | S | P4 | |||||
ILTJ110856.6+480024.4 | 167.2356 | 0.6 (1.8) | 48.0068 | 0.5 (1.8) | 17.0 | 0.5 (3.4) | 38.0 | 0.7 (7.6) | R | 0.5 | S | P7 | |||||
ILTJ123820.5+533450.5 | 189.5856 | 0.9 (1.9) | 53.5807 | 1.1 (2.0) | 16.7 | 1.5 (3.6) | 17.5 | 2.5 (4.3) | U | 1.5 | S | P29 | |||||
ILTJ112629.2+532151.7 | 171.6216 | 1.2 (2.1) | 53.3644 | 1.7 (2.4) | 3.3 | 0.5 (0.8) | 3.4 | 0.8 (1.0) | U | 0.5 | S | P12 | |||||
ILTJ115132.5+471429.2 | 177.8854 | 1.4 (2.2) | 47.2414 | 2.0 (2.6) | 9.0 | 1.2 (2.2) | 11.5 | 2.0 (3.1) | U | 1.2 | S | P15 | |||||
ILTJ124209.0+555428.1 | 190.5377 | 4.9 (5.1) | 55.9078 | 2.0 (2.6) | 2.8 | 0.4 (0.7) | 13.0 | 0.5 (2.6) | R | 0.4 | S | P191+55 | |||||
ILTJ124003.6+574429.8 | 190.0152 | 1.4 (2.2) | 57.7416 | 1.2 (2.1) | 11.3 | 1.3 (2.6) | 14.1 | 2.0 (3.5) | U | 1.2 | S | P191+55 | |||||
ILTJ132112.1+574121.3 | 200.3005 | 2.1 (2.7) | 57.6892 | 2.5 (3.0) | 5.3 | 0.9 (1.4) | 8.2 | 1.4 (2.1) | U | 0.8 | C | P200+55 | |||||
ILTJ151613.0+505206.5 | 229.0541 | 0.7 (1.9) | 50.8685 | 0.8 (1.9) | 6.5 | 0.5 (1.4) | 6.8 | 0.8 (1.6) | U | 0.5 | S | P227+50 | |||||
ILTJ150730.3+501951.5 | 226.8761 | 0.8 (1.9) | 50.3310 | 1.0 (2.0) | 4.4 | 0.4 (1.0) | 4.1 | 0.7 (1.1) | U | 0.4 | S | P227+50 | |||||
ILTJ150506.2+505458.1 | 226.2760 | 0.7 (1.8) | 50.9161 | 0.8 (1.9) | 8.9 | 0.6 (1.9) | 10.1 | 0.9 (2.2) | U | 0.6 | S | P227+50 | |||||
ILTJ142842.4+481322.7 | 217.1767 | 1.1 (2.0) | 48.2230 | 1.3 (2.2) | 5.0 | 0.5 (1.1) | 6.8 | 0.8 (1.6) | U | 0.5 | S | P217+47 | |||||
ILTJ140150.1+460845.3 | 210.4587 | 1.6 (2.3) | 46.1459 | 1.6 (2.3) | 3.3 | 0.4 (0.8) | 4.3 | 0.7 (1.1) | U | 0.4 | S | P210+47 | |||||
ILTJ135725.8+484433.4 | 209.3577 | 1.3 (2.1) | 48.7426 | 1.3 (2.1) | 3.0 | 0.3 (0.7) | 4.0 | 0.5 (0.9) | U | 0.3 | S | P210+47 | |||||
ILTJ143733.8+563232.0 | 219.3909 | 0.8 (1.9) | 56.5422 | 0.4 (1.8) | 16.8 | 0.6 (3.4) | 37.0 | 0.8 (7.5) | R | 0.6 | S | P218+55 | |||||
ILTJ151911.5+512419.0 | 229.7978 | 1.9 (2.6) | 51.4053 | 2.5 (3.0) | 4.3 | 0.6 (1.1) | 7.7 | 0.9 (1.8) | U | 0.6 | S | P227+53 | |||||
ILTJ150703.0+540008.3 | 226.7625 | 0.9 (1.9) | 54.0023 | 0.9 (1.9) | 7.6 | 0.6 (1.6) | 10.6 | 0.9 (2.3) | U | 0.5 | S | P227+53 | |||||
ILTJ132723.5+464943.9 | 201.8478 | 0.8 (1.9) | 46.8289 | 0.8 (1.9) | 6.2 | 0.4 (1.3) | 7.8 | 0.7 (1.7) | U | 0.4 | S | P39 | |||||
ILTJ111612.8+555350.7 | 169.0535 | 0.5 (1.8) | 55.8974 | 0.6 (1.8) | 8.9 | 0.4 (1.8) | 10.5 | 0.7 (2.2) | U | 0.4 | S | P169+55 | |||||
ILTJ122630.6+531346.8 | 186.6274 | 0.5 (1.8) | 53.2297 | 0.5 (1.8) | 8.8 | 0.4 (1.8) | 10.1 | 0.6 (2.1) | U | 0.3 | S | P25 |
Notes. The entire catalogue contains over 44 000 sources. The entries in the catalogue are as follows: source identifier (ID), J2000 right ascension (RA), J2000 declination (Dec), peak brightness (Speak), integrated flux density (Sint), a flag indicating whether the source is resolved (R) or unresolved (U), the local noise at the position of the source (RMS noise), the type of source (where “S” indicates an isolated source that is fit with a single Gaussian; “C” represents sources that are fit by a single Gaussian but are within an island of emission that also contains other sources; and “M” is used for sources that are extended and fitted with multiple Gaussians), and the mosaic identifier. The right ascension, declination, peak brightness, and integrated flux density are assigned both a formal error from the source fitting and a total error that accounts for the 1.7″ astrometric uncertainty and the 20% flux uncertainty.
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