QC1 Plotter

kmos_science_idp: QC1 values from KMOS IDP science products

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Select for plotting:


1. Plot Items
X axis Y axis Item Comment
mjd_obs MJD-OBS of (first) raw file
abmaglim limiting AB magnitude
spec_res spectral resolving power at central wavelength
sky_res FWHM effective spatial resolution [arcsec]
sky_rerr estimated error of sky_res [arcsec]
pixnoise pixel-to-pixel noise [erg/s/cm**2/Angstrom]
lambda_min minimum wavelength [nm]
lambda_max maximum wavelength [nm]
ia_fwhm seeing from active optics, corrected by airmass
ambi_req requested maximum seeing
airmass mean airmass over first exposure
exptime total exposure time (in secs)
num_sat number of saturated pixels in 1st raw frame
satlevel saturation level (ADU)
num_persistent number of pixels above persistence level
persistence_level persistence level (ADU)
tell_h2o_avg H2O column in mm from, averaged over used IFUs, from associated telluric
tell_h2o_rms H2O column in mm, standard deviation over used IFUs, from associated telluric
meas_iwv Integrated Water Vapor as measured during observation
meas_iwv_30deg Integrated Water Vapor at 30 degrees as measured during observation
delta_h2o tell_h2o_avg - meas_iwv
frac_h2o tell_h2o_avg divided by meas_iwv
deltatime_flat time difference (in days) between science and lamp flat
deltatime_tell time difference (in days) between science and telluric standard
deltaairm_tell difference in airmass between science and telluric standard
ifu_nb IFU arm number used of target
seq1_dit DIT of 1st detector
seq2_dit DIT of 2nd detector
seq3_dit DIT of 3rd detector
ncombine number of combined exposures
flag_dt_flat associated flat-field taken within 1 day (0 = yes; 1 = no)
flag_tell_qual quality of telluric correction (0 = within specs; 1 = needs double checking)
flag_all_det telluric standard for all 3 detectors (0 = yes; 1 = no)
flag_mag_source star magnitude taken from observatory OB (0 = yes; 1 = no)
flag_atm_profile actual atmospheric profile from same night (0 = yes; 1 = no)
flag_nonlin number saturated pixels (0 = less than 3500; 1 = more than 3500)
flag_sky sky method (0 = separate exposure; 1 = separate IFU; 2 = no sky)

2. Filter by
det_index detector index (1 - 3)
ifu_nb IFU arm number used of target
seq1_dit DIT of 1st detector
seq2_dit DIT of 2nd detector
seq3_dit DIT of 3rd detector
ndit number of integrations
filt1_id filter/wavelength band of arm 1
filt2_id filter/wavelength band of arm 2
filt3_id filter/wavelength band of arm 3
filt1_wlen central wavelength in nm of filter in arm 1
filt2_wlen central wavelength in nm of filter in arm 2
filt3_wlen central wavelength in nm of filter in arm 3
grat1_id grating ID of arm 1
grat2_id grating ID of arm 2
grat3_id grating ID of arm 3
grat1_wlen central wavelength of grating in arm 1
grat2_wlen central wavelength of grating in arm 2
grat3_wlen central wavelegnth of grating in arm 3
ncombine number of combined exposures
VM_SM Visitor Mode or Service Mode
ob_grade OB grade (A/B/C/D or X=unknown)
score_bit quality flags (score bits)
flag_dt_flat associated flat-field taken within 1 day (0 = yes; 1 = no)
flag_tell_qual quality of telluric correction (0 = within specs; 1 = needs double checking)
flag_all_det telluric standard for all 3 detectors (0 = yes; 1 = no)
flag_mag_source star magnitude taken from observatory OB (0 = yes; 1 = no)
flag_atm_profile actual atmospheric profile from same night (0 = yes; 1 = no)
flag_nonlin number saturated pixels (0 = less than 3500; 1 = more than 3500)
flag_sky sky method (0 = separate exposure; 1 = separate IFU; 2 = no sky)
proc_scheme processing scheme
pipe_vers pipeline version number

3. Options
time range:
for plot: From To
for statistics: From To
plot options:
y scaling for plotting: y_min y_max
x scaling for plotting: x_min x_max
special:
connect by lines mark outliers civil_dates
plot format: png gif ps
statistics options:
average none mean median least-square
error thresholds none 1 sigma 3 sigma 10%

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