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# XMM-13hr: Validation Report (FULL)

XMM-13hr: Validation Report (FULL)

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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.

 
## I. Caveats

I. Caveats

 
### I.a. Magnitude errors 

I.a. Magnitude errors

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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

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

 
## II. Flags

II. Flags

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### II.b. Outliers
There are no bands with multiple observations, we then cannot flag outliers.

II.b. Outliers

There are no bands with multiple observations, we then cannot flag outliers.