The following checklist must be completed after each execution
of the FEROS Daily Health Check OB and is very desirable to be
completed after morning CALOB calibrations:
Where to look
On w2p2off find the MOZILLA window (NOT the firefox window):
In this window for each DHC set and for each StanCal set there are
three TABS:
1) QC0 trends: shows BIAS mean and sd trend, FF flux in each fibre in
orders
1 & 30 trends, WLC solution RMS and number of lines in solution
trend.
In these plots the larger BLUE points represent the latest point added,
i.e.
the initialisation JUST made.
*) Check the "Last Point Date" corresponds to the data
just acquired.
*) Check that the Blue points do not deviate from the
trends.
2) DRSinit web summary of this initialisation (for comparison with the
summary). Also check that the FF ratio plots show flat lines with mean
ONE.
3) DRSinit web summary of Reference initialisation on the web server for
this Readout Mode, Binning (references for binning 2x2 do not (yet)
exist...)
Checklist
In the QC0 trend tab
Check the "Last Point Date" corresponds to the data just acquired.
In each graph of the QC0 summary movie check that the blue points
do not deviate from the trends.
In the DRSinit web summary of this initialisation tab
Visually compare with the DRSinit web summary of Reference
initialisation for obvious deviations from "normal"
Check the RMS plots, should be scattered about zero with no
obvious trend (e.g. a "S" shape is sometimes seen). RMS value and the
number of points is verified above in the QC0 verification.
In the FF ratio plots check that that ratios for each order have
amean value of unity and do not show trends, i.e. slopes (can indicate
variable flux level from one or other of the halogen lamps) or
increases or decreases at the ends of the orders (can indicate shutter
problems). In case of issue check in the web summarys of the individual
files:
From the "Bookmarks toolbar" select the "FEROS DRS" bookmark
click on the relevant date
examine the web summary plots of the individual frames, in
particular look in the flat field summaries to check that the reduced
spectra are flat with a mean of ONE any slopes shows variation in the
flux level between individual exposures which could be due either to
variable flux from the lamp or shutter problems. Such problems will
also be evident in the FF ratio plots which would should trends other
than flat lines with mean ONE.