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Master catalogue used: __master_catalogue_xmm-13hr_20180201.fits__<br>
Number of rows: 38,629
<br>
Surveys included:<br>
| Survey | Telescope / Instrument | Filters (detection band in bold) | Location |
|---------------|------------------------|:---------------------------------:|-----------------|
| Legacy Survey | BASS | grz | dmu0_LegacySurvey |
| UHS | UKIRT | J | dmu0_UHS |
__NB: On XMM-13hr, there are no bands with multiple observations. We then cannot flag outliers or look for difference in aperture correction between point-source and extended objects for different surveys.<br>
Also, there are no sources, with "weird" magnitude or magnitude error, to flag in this field.__
Master catalogue used: master_catalogue_xmm-13hr_20180201.fits
Number of rows: 38,629
Surveys included:
Survey | Telescope / Instrument | Filters (detection band in bold) | Location |
---|---|---|---|
Legacy Survey | BASS | grz | dmu0_LegacySurvey |
UHS | UKIRT | J | dmu0_UHS |
NB: On XMM-13hr, there are no bands with multiple
observations. We then cannot flag outliers or look for difference in
aperture correction between point-source and extended objects for
different surveys.
Also, there are no sources, with "weird" magnitude or magnitude error, to flag in this field.
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At faint magnitudes (mag > 24), __Legacy Survey__ have very large errors on the __aperture and total__ magnitude (at mag > 27). These objects may be unreliable for science puposes.<br>
<img src="help_plots/XMM-13hr_magVSmagerr_BASS_g_mag_total.png" />
At faint magnitudes (mag > 24), Legacy Survey have very large errors on the aperture and total magnitude (at mag > 27). These objects may be unreliable for science puposes.
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### I.b. Aperture corrections
There are no bands with multiple observations, we then cannot look for difference in aperture correction between point-source and extended objects for different surveys
There are no bands with multiple observations, we then cannot look for difference in aperture correction between point-source and extended objects for different surveys
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### II.b. Outliers
There are no bands with multiple observations, we then cannot flag outliers.
There are no bands with multiple observations, we then cannot flag outliers.