QC1 Plotter

sinfoni_sci: obsnod and obsjit science data

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Select for plotting:


1. Plot Items
X axis Y axis Item Comment
mjd_obs MJD-OBS of first raw fits frame
pro_datancom number of raw input frames
qc_frmon_meanflux mean flux ON-lamp frame
qc_frmoff_meanflux mean flux OFF-lamp frame
qc_frmdif_meanflux mean flux ON-OFF lamp
qc_frmon_maxflux max flux in ON-lamp frame
qc_frmoff_maxflux max flux in OFF-lamp frame
qc_frmdif_maxflux max flux in ON-OFF lamp
qc_frmon_npixsat number of ON-lamp saturated pixels
rtc_obs_enc_mean rtc encircled energy mean
rtc_obs_enc_std rtc encircled energy std dev
rtc_obs_fwhm_mean rtc fwhm mean
rtc_obs_fwhm_std rtc fwhm std dev
rtc_obs_l0mean rtc mean outer scale [m]
rtc_obs_l0std rtc std dev of outer scale [m]
rtc_obs_r0mean rtc mean Fried parameter [m]
rtc_obs_r0std rtc std dev of Fried parameter [m]
rtc_obs_str_mean rtc mean Strehl ratio [%]
rtc_obs_str_std rtc Strehl ratio std dev [%]
rtc_obs_t0mean rtc mean correlation time [s]
rtc_obs_t0std rtc std dev of correlation time [m]
rtc_obs_wfemean rtc mean wavefront error
rtc_obs_wfestd rtc std dev of wavefront error
qc_nreal_det number of sources detected (>3sigma) (QC script)
qc_xpos X-pos of brightest source (QC script)
qc_ypos Y-pos of brightest source (QC script)
qc_flux total flux (in ADU) within 3 sigma aperture of brightest source (QC script)
qc_iso_area total aperture area over which flux is summed (pixels^2) (QC script)
qc_net_flux net flux (in ADU): qc_flux/qc_iso_area of brightest source (QC script)
qc_spectra_peak mean flux of extracted spectrum at peak flux pixel (QC script)
qc_spectra_mean average flux of extracted spectrum (mean in fwhm) (QC script)
qc_spectra_std std dev of extracted spectrum mean flux level
qc_posang brightest source position angle (CCW along X-axis) (QC script)
qc_elong brightest source elongation (A_image/B_image) (QC script)
qc_ellip brightest source ellipticity (1 - B_image/A_image) (QC script)
qc_fwhm_dimm DIMM seeing corrected to observed airmass and IR bandpass (arcsec) (QC script)
qc_fwhm_sinfo brightest source FWHM assuming a Gaussian core (arcsec) (QC script)
qc_delta_fwhm difference (qc_fwhm_sinfo - qc_fwhm_dimm) (arcsec) (QC script)
qc_persist_danger a test if flux levels are too high (danger of persistence = 1; no persistence = 0) (QC script)
qc_Npersist total number of persistence critical pixels (QC script)
qc_temp_det detector temperature (C)
qc_temp_grat grating housing temperature (C)
qc_temp_ambi ambient temperature (C)
qc_delta_temp_det diff between sci obs and wave det temp
qc_delta_temp_grat diff between sci obs and wave grating temp
qc_delta_time delta days between sci obs and STD obs
qc_delta_am delta airmass between sci obs and STD obs

2. Filter by
det_chip_id detector id
det_ncorrs_name correlation mode name
det_dit discrete integration time
det_ndit number of averages on the chip
det_ndsamples samples
det_mindit minimum dit
det_rspeed read speed parameter
ins_grat_name grating name
ins_opti1_name preoptics name
ins_setup_id grating name
obs_prog_id observing program identification
obs_id OB identification
obs_targ_name target name
ins1_mode instrumental AO mode (NOAO, NGS, LGS)
rtc_loop_state AO loop status (OPEN or CLOSED)
rtc_loop_lgs LGS jitter loop on or off

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%

Send comments to: <qc@eso.org>