#include <cpl.h>
#include <xsh_error.h>
#include <xsh_dfs.h>
#include <xsh_utils.h>
#include <xsh_data_pre.h>
#include <xsh_data_rec.h>
#include <xsh_data_instrument.h>
#include <xsh_data_order.h>
#include <xsh_data_dispersol.h>
#include <xsh_parameters.h>
#include <xsh_qc_handling.h>
Go to the source code of this file.
Defines | |
#define | XSH_CONCAT(A, B) A ## B |
#define | XSH_STRING(A) # A |
#define | PICKUP_NOISE_HOT_PIXEL_MAP |
#define | REGDEBUG_OPTEXTRACT 0 |
#define | XSH_DIVIDE_FLAT_THRESH 1e-10 |
#define | XSH_MULTIPLY_FLAT_THRESH 1e+30 |
#define | WAVELENGTH_PRECISION 0.00001 |
#define | SLIT_PRECISION 0.00001 |
#define | SLIT_PRECISION_IFU 0.21 |
#define | XSH_DETECT_ARCLINES_TYPE_POLY 0 |
#define | XSH_DETECT_ARCLINES_TYPE_MODEL 1 |
#define | XSH_DETECT_ARCLINES_MODE_NORMAL 0 |
#define | XSH_DETECT_ARCLINES_MODE_CORRECTED 1 |
#define | XSH_DETECT_ARCLINES_MODE_RECOVER 2 |
#define | XSH_RECTIFY_TYPE_POLY 0 |
#define | XSH_RECTIFY_TYPE_MODEL 1 |
#define | XSH_OBJPOS_NB_COL 2 |
#define | XSH_OBJPOS_COLNAME_WAVELENGTH "Wavelength" |
#define | XSH_OBJPOS_UNIT_WAVELENGTH "nm" |
#define | XSH_OBJPOS_COLNAME_SLIT "Slit" |
#define | XSH_OBJPOS_UNIT_SLIT "arcsec" |
#define | XSH_LAMBDA_DIMM 0.0000005 |
#define | XSH_SHIFTIFU_NB_COL 2 |
#define | XSH_SHIFTIFU_COLNAME_WAVELENGTH "Wavelength" |
#define | XSH_SHIFTIFU_UNIT_WAVELENGTH "nm" |
#define | XSH_SHIFTIFU_COLNAME_SHIFTSLIT "Slit_shift" |
#define | XSH_SHIFTIFU_UNIT_SHIFTSLIT "arcsec" |
#define | XSH_MATH_SQRT_2 1.4142135623730951 |
#define | REGDEBUG_GAUSSIAN 0 |
#define | REGDEBUG_BLAZE 0 |
#define | REGDEBUG_EXTRACT 0 |
#define | REGDEBUG_EXTRACT_XY 0 |
#define | REGDEBUG_SUBEXTRACT_XY 0 |
#define | REGDEBUG_EXTRACT_STD 0 |
#define | REGDEBUG_N 0 |
#define | LSTART_COLUMN_NAME "LAMBDASTART" |
#define | LEND_COLUMN_NAME "LAMBDAEND" |
#define | GUESS_TELL_MASK_RESOLUTION_UVB 9100 |
#define | GUESS_TELL_MASK_RESOLUTION_VIS 17400 |
#define | GUESS_TELL_MASK_RESOLUTION_NIR 11300 |
Enumerations | |
enum | xsh_sol_wavelength { XSH_SOLUTION_ABSOLUTE, XSH_SOLUTION_RELATIVE } |
Functions | |
cpl_frame * | xsh_bpmap_2pre (cpl_frame *bpmap, const char *prefix, xsh_instrument *inst) |
This function transform a BP map from raw to pre format. | |
void | xsh_prepare (cpl_frameset *frames, cpl_frame *bpmap, cpl_frame *mbias, const char *prefix, xsh_instrument *instr, const int pre_overscan_corr, const bool flag_neg_and_thresh_pix) |
This function transform RAW frames dataset in PRE frames dataset attaching the default bad pixel map and an error image. | |
cpl_frame * | xsh_preframe_extract (cpl_frame *frame, int xmin, int ymin, int xmax, int ymax, const char *name, xsh_instrument *instr) |
This function create a sub frame from PRE frame. the sub frame is described by a box. | |
cpl_frame * | xsh_remove_crh_multiple (cpl_frameset *rawFrames, const char *name, xsh_stack_param *stack_param, xsh_clipping_param *crh_clipping, xsh_instrument *inst, cpl_imagelist **, cpl_image **, const int save_tmp) |
cpl_frame * | xsh_compute_noise_map (cpl_imagelist *, cpl_frame *bpmap, xsh_clipping_param *, xsh_instrument *instr, cpl_frame **noisemap) |
cpl_frame * | xsh_create_master_dark (cpl_frame *bpMap, xsh_instrument *instr, cpl_parameterlist *parameters, cpl_frame *crh_frm, cpl_frame *bp_map_frm) |
cpl_frame * | xsh_create_master_dark2 (cpl_frameset *raws, xsh_stack_param *stack_param, cpl_parameterlist *drs_param, cpl_propertylist *qc_log, xsh_instrument *instr) |
cpl_frame * | xsh_compute_qc_on_master_bias (cpl_frameset *raws, cpl_frame *frame, xsh_instrument *instr, cpl_parameterlist *drs_params) |
Computes QC on a master bias frame. | |
cpl_frame * | xsh_create_master_flat (cpl_frame *frame, xsh_instrument *instr) |
cpl_frame * | xsh_create_master_flat_with_mask (cpl_frame *frame, cpl_frame *edges, xsh_instrument *instr) |
cpl_frame * | xsh_create_master_flat2 (cpl_frameset *set, cpl_frame *order_tab_cen, xsh_stack_param *stack_par, xsh_instrument *inst) |
Combine master frames. | |
cpl_frame * | xsh_create_master_dark_bpmap (cpl_frame *frame, xsh_instrument *instr) |
cpl_frame * | xsh_compute_linearity (cpl_frameset *, xsh_instrument *, xsh_clipping_param *, const int decode_bp) |
int | xsh_linear_group_by_exptime (cpl_frameset *, xsh_instrument *, double, cpl_frameset **) |
cpl_frame * | xsh_subtract_bias (cpl_frame *frame, cpl_frame *bias, xsh_instrument *instr, const char *type, const int pre_overscan_corr, const int save_tmp) |
Subtract the master bias frame from PRE frame. | |
cpl_frameset * | xsh_subtract_nir_on_off (cpl_frameset *on, cpl_frameset *off, xsh_instrument *instr) |
(NIR only) subtract the OFF set of files from the On set of files | |
cpl_frame * | xsh_subtract_dark (cpl_frame *frame, cpl_frame *dark, const char *filename, xsh_instrument *instr) |
subtract the master dark frame from PRE frame | |
cpl_frame * | xsh_divide_flat (cpl_frame *frame, cpl_frame *flat, const char *filename, xsh_instrument *instr) |
divide PRE frame with the master FLAT frame | |
cpl_frame * | xsh_multiply_flat (cpl_frame *frame, cpl_frame *flat, const char *filename, xsh_instrument *instr) |
multiply PRE frame with the master FLAT frame | |
cpl_frame * | xsh_subtract_background (cpl_frame *frame, cpl_frame *ordertable, xsh_background_param *bckg, xsh_instrument *instr, const char *prefix, cpl_frame **grid_frame, cpl_frame **frame_backg, const int save_bkg, const int save_grid, const int save_sub_bkg) |
Subtract the inter-order background from PRE frame. | |
cpl_frame * | xsh_detect_order_edge (cpl_frame *frame, cpl_frame *order_table, xsh_detect_order_param *det_param, xsh_instrument *instr) |
Detect order edges and compute polynomial description of ordermin and order max. | |
cpl_frame * | xsh_detect_continuum (cpl_frame *frame, cpl_frame *order_table, cpl_frame *spectral_format, xsh_detect_continuum_param *param, xsh_clipping_param *dcn_clipping, xsh_instrument *instr, cpl_frame **resid_frame) |
Detect order and compute polynomial description of ordermin and order max. Uses a guess order table if available. If not, tries to compute one (see function xsh_order_table_from_fmtchk). | |
cpl_frame * | xsh_order_table_from_fmtchk (xsh_pre *pre, cpl_frame *spectral_frame, xsh_detect_continuum_param *detect_param, xsh_instrument *instrument) |
void | xsh_create_map (cpl_frame *dispsol_frame, cpl_frame *ordertab_frame, cpl_frame *pre_frame, xsh_instrument *instrument, cpl_frame **wavemap_frame, cpl_frame **slitmap_frame, const char *rec_prefix) |
cpl_frame * | xsh_create_wavemap (cpl_frame *in_frame, cpl_frame *resid_frame, cpl_frame *order_frame, xsh_dispersol_param *dispersol_param, xsh_instrument *instrument) |
cpl_frame * | xsh_create_poly_wavemap (cpl_frame *pre_frame, cpl_frame *wave_tab_2d_frame, cpl_frame *order_tab_frame, cpl_frame *spectral_format_frame, xsh_dispersol_param *dispsol_par, xsh_instrument *instrument, const char *filename, cpl_frame **dispersol_frame, cpl_frame **slitmap_frame) |
void | xsh_create_model_map (cpl_frame *model_frame, xsh_instrument *instrument, const char *wave_map_tag, const char *slit_map_tag, cpl_frame **wavemap_frame, cpl_frame **slitmap_frame, const int save_tmp) |
cpl_frame * | xsh_create_order_table (cpl_frame *in_frame, cpl_frame *spectralformat_frame, cpl_frame *resid_frame, cpl_frame *arclines, xsh_detect_arclines_param *da, xsh_clipping_param *dac, xsh_instrument *instrument) |
void | xsh_detect_arclines (cpl_frame *frame, cpl_frame *theo_tab_frame, cpl_frame *arc_lines_tab_frame, cpl_frame *wave_tab_guess_frame, cpl_frame *order_tab_recov_frame, cpl_frame *config_model_frame, cpl_frame *spectralformat_frame, cpl_frame **resid_tab_orders_frame, cpl_frame **arc_lines_clean_tab_frame, cpl_frame **wave_tab_frame, cpl_frame **resid_tab_frame, xsh_sol_wavelength type, xsh_detect_arclines_param *da, xsh_clipping_param *dac, xsh_instrument *instr, const char *rec_id, const int clean_tmp, const int resid_tab_name_sw) |
detect the position on the detector of emission lines listed in a catalogue, from expected position values given by the Physical model. | |
void | xsh_detect_arclines_dan (cpl_frame *frame, cpl_frame *theo_tab_frame, cpl_frame *arc_lines_tab_frame, cpl_frame *wave_tab_guess_frame, cpl_frame *order_tab_recov_frame, cpl_frame *config_model_frame, cpl_frame *spectralformat_frame, cpl_frame **resid_tab_orders_frame, cpl_frame **arc_lines_clean_tab_frame, cpl_frame **wave_tab_frame, cpl_frame **resid_tab_frame, xsh_sol_wavelength type, xsh_detect_arclines_param *da, xsh_clipping_param *dac, xsh_instrument *instr, const char *rec_id, const int clean_tmp, const int resid_tab_name_sw) |
detect the position on the detector of emission lines listed in a catalogue, from expected position values given by the Physical model. | |
void | xsh_follow_arclines_slit (cpl_frame *inframe, cpl_frame *arclines, cpl_frame *wavesol, cpl_frame *order_table, cpl_frame *spectralformat_frame, cpl_frame *model_config_frame, cpl_frame *wavemap_frame, cpl_frame *slitmap_frame, cpl_frame *disptab_frame, xsh_follow_arclines_param *param, xsh_instrument *instrument, cpl_frame **tilt_list, cpl_frame **shift_frame) |
void | xsh_follow_arclines_ifu (cpl_frame *inframe, cpl_frame *arclines, cpl_frame *wavesol, cpl_frame *order_table, cpl_frame *spectralformat_frame, cpl_frame *model_config_frame, cpl_frame *wavemap_frame, cpl_frame *slitmap_frame, cpl_frame *disptab_frame, xsh_follow_arclines_param *follow_param, xsh_instrument *instrument, cpl_frameset *tilt_set, cpl_frame **shift_frame) |
Detect and follow arc lines. Computes center, width and tilt parameters. The position of the center of each line is computed using the wavesol table, with arguments: lambda, order and slit. lambda is taken from the arclines table, order and slit is taken from the theoretical table. | |
void | xsh_rec_slit_size (xsh_rectify_param *rectify_par, double *slit_min, int *nslit, XSH_MODE mode) |
rectify frame | |
cpl_frame * | xsh_rectify_orders (cpl_frame *sci_frame, xsh_order_list *orderlist_frame, cpl_frame *wavesol_frame, cpl_frame *model_frame, xsh_instrument *instrument, xsh_rectify_param *rectify_par, cpl_frame *spectralformat_frame, cpl_frame *disp_tab_frame, const char *res_name, const char *tag, cpl_frame **res_frame_ext, cpl_frame **res_frame_tab, int min_index, int max_index, double slit_min, int nslit, double slit_shift, cpl_frame *slitshift_tab) |
Create a grid in wavelength with the step in lambda and slit. Steps are defined in the parameters. Lambda min and max are taken from the spectralformat list. Slit min/max are hard coded. Range orders arve given. | |
cpl_frameset * | xsh_rectify_orders_ifu (cpl_frame *sci_frame, xsh_order_list *orderlist, cpl_frameset *wavesol_frameset, cpl_frameset *shift_frameset, cpl_frame *model_frame, xsh_instrument *instrument, xsh_rectify_param *rectify_par, cpl_frame *spectralformat_frame, cpl_frame *slitmap_frame, cpl_frameset **rec_frameset_ext, cpl_frameset **rec_frameset_tab, int min_index, int max_index, const char *rec_prefix) |
cpl_frame * | xsh_rectify (cpl_frame *sci_frame, cpl_frame *order_table_frame, cpl_frame *wavesol_frame, cpl_frame *model_config_frame, xsh_instrument *instrument, xsh_rectify_param *rectify_par, cpl_frame *spectral_format, cpl_frame *disp_tab_frame, const char *fname, cpl_frame **res_frame_ext, cpl_frame **res_frame_tab, const char *prefix) |
Create a grid in wavelength with the step in lambda and slit. Steps are defined in the parameters. Lambda min and max are taken from the spectralformat list. Slit min/max are hard coded. | |
cpl_frame * | shift_with_kw (cpl_frame *rec_frame, xsh_instrument *instrument, xsh_rectify_param *rectify_par, const char *fname, cpl_frame **res_frame_ext, double **ref_ra, double **ref_dec, int flag) |
This function creates a structure containing for each order the shift to be applied. | |
cpl_frame * | xsh_rectify_and_shift (cpl_frame *sci_frame, cpl_frame *orderlist_frame, cpl_frame *wavesol_frame, cpl_frame *model_frame, xsh_instrument *instrument, xsh_rectify_param *rectify_par, cpl_frame *spectralformat_frame, cpl_frame *loc_frame, cpl_frame *loc0_frame, double *throw_shift, cpl_frame *disp_tab_frame, const char *res_name, cpl_frame **res_frame_ext, cpl_frame **res_frame_tab) |
cpl_frameset * | xsh_rectify_ifu (cpl_frame *sci_frame, cpl_frame *order_table_frame, cpl_frameset *wavesol_frame_set, cpl_frameset *shiftifu_frameset, cpl_frame *model_config_frame, xsh_instrument *instrument, xsh_rectify_param *rectify_par, cpl_frame *spectral_format, cpl_frame *slitmap_frame, cpl_frameset **rec_frameset_ext, cpl_frameset **rec_frameset_tab, const char *rec_prefix) |
cpl_frame * | xsh_shift_rectified (cpl_frame *rec_frame, cpl_frame *loc_frame, cpl_frame *loc0_frame, const char *file_name, xsh_combine_nod_param *combine_nod_param, xsh_rectify_param *rectif_par, xsh_instrument *instrument, cpl_frame **res_frame_ext) |
void | xsh_compute_slitlet_center (xsh_order_list *order_list, cpl_frame *slitmap_frame, double *down, double *cen, double *up, XSH_ARM arm) |
void | xsh_get_slit_edges (cpl_frame *slitmap_frame, double *sdown, double *sup, double *sldown, double *slup, xsh_instrument *instrument) |
Trace slit edges in a master flat. | |
void | xsh_compute_slitlet_limits (cpl_frameset *shift_set, double sdown, double sldown, double slup, double sup, double slit_bin, double *slitmin_tab, int *nslit_tab, double *slitcen_tab) |
cpl_frame * | xsh_subtract_sky_single (cpl_frame *sci_frame, cpl_frame *order_table_frame, cpl_frame *slitmap_frame, cpl_frame *wavemap_frame, cpl_frame *locTable_frame, cpl_frame *mflat_frame, cpl_frame *usr_defined_break_points_frame, xsh_instrument *instrument, int nbkpts, xsh_subtract_sky_single_param *sky_par, cpl_frame **sky_spectrum, cpl_frame **sky_spectrum_eso, const char *rec_prefix, const int clean_tmp) |
Subtract the sky background for single frame. If sky_spectrum is NOT NULL it is saved as a product, of type REC. | |
cpl_frame * | xsh_add_sky_model (cpl_frame *sub_sky_frame, cpl_frame *sky_frame, xsh_instrument *instrument, const char *rec_prefix) |
cpl_frame * | xsh_localize_obj (cpl_frame *sci_frame, cpl_frame *skymask_frame, xsh_instrument *instrument, xsh_localize_obj_param *loc_obj_par, xsh_slit_limit_param *slit_limit_param, const char *fname) |
Build the localization table. | |
cpl_frameset * | xsh_localize_obj_ifu (cpl_frameset *sci_frame, cpl_frame *skymask_frame, xsh_instrument *instrument, xsh_localize_obj_param *loc_obj_par, xsh_slit_limit_param *slit_limit_param) |
cpl_frame * | xsh_extract (cpl_frame *rec_frame, cpl_frame *loc_frame, xsh_instrument *instrument, xsh_extract_param *extract_par, cpl_frame **res_frame_ext, const char *rec_prefix) |
simple 1D extraction of point source like object | |
cpl_frame * | xsh_extract_clean (cpl_frame *rec_frame, cpl_frame *loc_frame, xsh_instrument *instrument, xsh_extract_param *extract_par, xsh_interpolate_bp_param *ipol_bp, cpl_frame **res_frame_ext, const char *rec_prefix) |
simple 1D extraction of point source like object | |
cpl_frameset * | xsh_extract_ifu (cpl_frameset *rec_frame_set, cpl_frameset *loc_frame_set, xsh_instrument *instrument, xsh_extract_param *extract_par, const char *rec_prefix) |
Loop on IFU Frames to extract simple 1D (1 per slitlet). | |
cpl_frame * | xsh_abs_remove_crh_single (cpl_frame *sci_frame, xsh_instrument *instrument, xsh_remove_crh_single_param *single_par, const char *res_tag) |
cpl_frame * | xsh_remove_crh_single (cpl_frame *sci_frame, xsh_instrument *instrument, xsh_remove_crh_single_param *single_par, const char *name) |
Remove cosmic rays from a single frame. | |
cpl_frame * | xsh_merge_ord_slitlet (cpl_frame *rec_frame, xsh_instrument *instrument, int merge_par, int slitlet, const char *rec_prefix) |
Merge orders of the rectified frame using merge parameters. | |
cpl_frame * | xsh_merge_ord (cpl_frame *sci_frame, xsh_instrument *instrument, int merge, const char *rec_prefix) |
Merge orders of the rectified frame using merge parameters. | |
cpl_frameset * | xsh_merge_ord_ifu (cpl_frameset *rec_frameset, xsh_instrument *instrument, int merge_par, const char *rec_prefix) |
Merge orders of the rectified frame using merge parameters. | |
double | xsh_convert_seeing (cpl_frame *frame) |
Convert seeing keywork in mu sigma. | |
cpl_frame * | xsh_localize_ifu_slitlet (cpl_frame *merge2d_slitlet, cpl_frame *skymask_frame, int smooth_hsize, int nscales, int HF_skip, const char *resname, double cut_sigma_low, double cut_sigma_up, double cut_snr_low, double cut_snr_up, double slit_min, double slit_max, int deg, int box_hsize, xsh_instrument *instr) |
Localize center of object on a merge 2D IFU slitlet. | |
cpl_frameset * | xsh_localize_ifu (cpl_frameset *merge2d_frameset, cpl_frame *skymask_frame, xsh_localize_ifu_param *locifu_par, xsh_instrument *instrument, const char *resname) |
Localize center of object on a merge 2D IFU slitlet. | |
cpl_frame * | xsh_compute_shift_ifu_slitlet (double lambda_ref, cpl_frame *objpos_frame, cpl_frame *shiftifu_frame, double lambdaref_hsize, const char *resname) |
Compute the shift in slit between reference wavelength and others. | |
cpl_frameset * | xsh_compute_shift_ifu (double lambda_ref, double lambdaref_hsize, cpl_frameset *objpos_frameset, cpl_frameset *shiftifu_frameset, xsh_instrument *instr, const char *prefix) |
Compute the shift in slit between reference wavelength and others for all the slitlets. | |
cpl_frameset * | xsh_subtract_sky_nod (cpl_frameset *raws, xsh_instrument *instrument, int mode_fast) |
void | xsh_flat_merge_qth_d2 (cpl_frame *qth_frame, cpl_frame *qth_order_tab_frame, cpl_frame *d2_frame, cpl_frame *d2_order_tab_frame, cpl_frame *qth_bkg_frame, cpl_frame *d2_bkg_frame, cpl_frame **qth_d2_flat_frame, cpl_frame **qth_d2_bkg_frame, cpl_frame **qth_d2_order_tab_frame, xsh_instrument *instrument) |
Merge two master flat fields and order tables according the spectral format. | |
void | xsh_flat_merge_qth_d2_smooth (cpl_frame *qth_frame, cpl_frame *qth_order_tab_frame, cpl_frame *d2_frame, cpl_frame *d2_order_tab_frame, cpl_frame *qth_bkg_frame, cpl_frame *d2_bkg_frame, cpl_frame **qth_d2_flat_frame, cpl_frame **qth_d2_bkg_frame, cpl_frame **qth_d2_order_tab_frame, xsh_instrument *instrument) |
Merge two master flat fields and order tables according the spectral format. | |
cpl_frame * | xsh_flat_merge_qth_d2_tabs (cpl_frame *qth_edges_tab, cpl_frame *d2_edges_tab, xsh_instrument *instrument) |
Merge two order edges tables according the spectral format. | |
cpl_error_code | xsh_extract_clean_slice (const float *flux, const float *errs, int *qual, const double *lambda, const int ilambda, xsh_instrument *instrument, const int slit_min, const int slit_max, const int nlambda, const int nslit, const int mask_hsize, double *fluxval, double *errval, int *qualval) |
void | xsh_opt_extract (cpl_frame *sci_frame, cpl_frame *order_table_frame, cpl_frame *wavesol_frame, cpl_frame *model_frame, cpl_frame *wavemap_frame, cpl_frame *slitmap_frame, cpl_frame *loc_frame, cpl_frame *spectralformat_frame, cpl_frame *masterflat_frame, xsh_instrument *instrument, xsh_opt_extract_param *opt_extract_par, const char *rec_prefix, cpl_frame **orderext1d_frame, cpl_frame **orderoxt1d_frame, cpl_frame **orderoxt1d_eso_frame, cpl_frame **qc_subextract_frame, cpl_frame **qc_s2ddiv1d_frame, cpl_frame **qc_model_frame, cpl_frame **qc_weight_frame) |
Create a SPECTRUM 1D from a Science frame. | |
void | xsh_opt_extract_orders (cpl_frame *sci_frame, cpl_frame *orderlist_frame, cpl_frame *wavesol_frame, cpl_frame *model_frame, cpl_frame *wavemap_frame, cpl_frame *slitmap_frame, cpl_frame *loc_frame, cpl_frame *spectralformat_frame, cpl_frame *masterflat_frame, xsh_instrument *instrument, xsh_opt_extract_param *opt_extract_par, int min_index, int max_index, const char *rec_refix, cpl_frame **orderext1d_frame, cpl_frame **orderoxt1d_frame, cpl_frame **orderoxt1d_eso_frame, cpl_frame **qc_subextract_frame, cpl_frame **qc_s2ddiv1d_frame, cpl_frame **qc_model_frame, cpl_frame **qc_weight_frame) |
Create a SPECTRUM 1D from a Science frame. | |
cpl_frame * | xsh_combine_nod (cpl_frameset *frames, xsh_combine_nod_param *param, const char *fname, xsh_instrument *instrument, cpl_frame **res_frame_ext) |
cpl_frame * | xsh_create_master_bias2 (cpl_frameset *rawFrames, xsh_stack_param *stack_par, xsh_instrument *instr, const char *result_name, const int method_code) |
Creates master bias. | |
cpl_frame * | xsh_compute_slice_dist (cpl_frameset *loc_frame_set, cpl_frame *order_tab, cpl_frame *slitmap_frame, cpl_frameset *merge_frameset, double lambda, xsh_instrument *instrument) |
cpl_frame * | xsh_format (cpl_frameset *rect_frame_set, const char *result_name, xsh_instrument *instrument, const char *rec_prefix) |
cpl_frame * | xsh_cube (cpl_frameset *merge2d_frameset, xsh_instrument *instrument, const char *rec_prefix) |
Create a cube. | |
void | xsh_center_cube (cpl_frame *cube_frame, cpl_frame *sky_line_frame, int chunk_size, xsh_instrument *instrument) |
Shift a cube to center object at 0 arcsec. | |
cpl_frameset * | xsh_subtract_sky_offset (cpl_frameset *object_raws, cpl_frameset *sky_raws, int nraws, xsh_instrument *instrument) |
cpl_frame * | xsh_combine_offset (cpl_frameset *rawFrames, const char *result_name, xsh_stack_param *stack_par, xsh_instrument *instr, cpl_imagelist **list, cpl_image **crh_ima, const int save_tmp) |
cpl_frame * | xsh_compute_response (cpl_frame *rect_frame, cpl_frame *std_star_flux_frame, cpl_frame *atmos_ext_frame, cpl_frame *high_abs_tab_frame, xsh_instrument *instrument, double exptime) |
cpl_frame * | xsh_compute_response2 (cpl_frame *rect_frame, cpl_frame *std_star_flux_frame, cpl_frame *atmos_ext_frame, cpl_frame *high_abs_tab_frame, cpl_frame *tell_mod_cat_frame, xsh_instrument *instrument, double exptime, const int tell_corr) |
cpl_frame * | xsh_compute_response_ord (cpl_frame *rect_frame, cpl_frame *std_star_flux_frame, cpl_frame *atmos_ext_frame, cpl_frame *high_abs_tab_frame, xsh_instrument *instrument, double exptime) |
void | xsh_data_check_spectralformat (cpl_frame *spectralformat_frame, cpl_frame *orderlist_frame, cpl_frame *wavesol_frame, cpl_frame *model_config, xsh_instrument *instr) |
Check the borders of wavelength foreach orders in spectral format. | |
cpl_error_code | xsh_wavemap_qc (cpl_frame *frm_map, const cpl_frame *frm_tab) |
Monitor Flux level along the orders traces given by an input table. | |
cpl_error_code | xsh_wavetab_qc (cpl_frame *frm_tab, const int is_poly) |
Monitor min/max/med/avg distance between detected lines on each ordee. | |
cpl_frame * | xsh_flexcor (cpl_frame *afc_frame, cpl_frame *wave_tab_frame, cpl_frame *model_config_frame, cpl_frame *order_tab_frame, cpl_frame *attresidtab_frame, int afc_xmin, int afc_ymin, xsh_instrument *instr, cpl_frame **afc_order_tab_frame, cpl_frame **afc_model_config_frame) |
This function applies the computed shift betwwen AFC CAL and AFC ATT frame. | |
cpl_frame * | xsh_afcthetab_create (cpl_frame *wave_tab_frame, cpl_frame *model_config_frame, int order, cpl_frame *spectralformat_frame, cpl_frame *arclines_frame, int xmin, int ymin, xsh_instrument *instr, const int clean_tmp) |
Create a The tab for AFC. | |
cpl_frameset * | xsh_ifu_wavetab_create (cpl_frame *wave_tab_frame, cpl_frame *shift_tab_frame, xsh_instrument *instr) |
Create an IFU wave tab frame set. | |
cpl_frame * | xsh_calibrate_flux (cpl_frame *spectrum_frame, cpl_frame *respon_frame, cpl_frame *atmos_ext_frame, const char *fname, xsh_instrument *instrument) |
cpl_frame * | xsh_create_dispersol_physmod (cpl_frame *pre_frame, cpl_frame *order_tab_frame, cpl_frame *mod_cfg_frame, cpl_frame *wave_map_frame, cpl_frame *slit_map_frame, xsh_dispersol_param *dispsol_param, cpl_frame *spectral_format_frame, xsh_instrument *instrument, const int clean_tmp) |
cpl_frame * | xsh_compute_absorp (cpl_frame *s1d_frame, cpl_frame *telllist_frame, int filter_hsize, double threshold, xsh_instrument *instr) |
Compute the shift in slit between reference wavelength and others for all the slitlets. | |
void | xsh_mark_tell (cpl_frame *s1d_frame, cpl_frame *tellmask_frame) |
Mark telluric in spectrum. |
#define GUESS_TELL_MASK_RESOLUTION_NIR 11300 |
Definition at line 730 of file xsh_drl.h.
Referenced by xsh_compute_absorp().
#define GUESS_TELL_MASK_RESOLUTION_UVB 9100 |
Definition at line 728 of file xsh_drl.h.
Referenced by xsh_compute_absorp().
#define GUESS_TELL_MASK_RESOLUTION_VIS 17400 |
Definition at line 729 of file xsh_drl.h.
Referenced by xsh_compute_absorp().
#define LEND_COLUMN_NAME "LAMBDAEND" |
Definition at line 727 of file xsh_drl.h.
Referenced by xsh_compute_absorp().
#define LSTART_COLUMN_NAME "LAMBDASTART" |
Definition at line 726 of file xsh_drl.h.
Referenced by xsh_compute_absorp().
#define WAVELENGTH_PRECISION 0.00001 |
Definition at line 190 of file xsh_drl.h.
Referenced by theo_tab_filter(), xsh_arclist_clean_from_list(), xsh_arclist_clean_from_list_not_flagged(), xsh_the_map_lambda_order_slit_compare(), and xsh_the_map_load().
#define XSH_DETECT_ARCLINES_MODE_CORRECTED 1 |
Definition at line 228 of file xsh_drl.h.
Referenced by xsh_detect_arclines(), and xsh_detect_arclines_dan().
#define XSH_DETECT_ARCLINES_MODE_NORMAL 0 |
Definition at line 227 of file xsh_drl.h.
Referenced by xsh_detect_arclines(), and xsh_detect_arclines_dan().
#define XSH_DETECT_ARCLINES_MODE_RECOVER 2 |
Definition at line 229 of file xsh_drl.h.
Referenced by xsh_detect_arclines(), and xsh_detect_arclines_dan().
#define XSH_DETECT_ARCLINES_TYPE_MODEL 1 |
Definition at line 226 of file xsh_drl.h.
Referenced by xsh_2dmap(), xsh_detect_arclines(), xsh_detect_arclines_dan(), xsh_frame_table_resid_merge(), xsh_predict(), and xsh_resid_tab_load().
#define XSH_DETECT_ARCLINES_TYPE_POLY 0 |
Definition at line 225 of file xsh_drl.h.
Referenced by main(), xsh_2dmap(), xsh_detect_arclines(), xsh_detect_arclines_dan(), xsh_predict(), xsh_resid_tab_load(), xsh_resid_tab_log(), and xsh_resid_tab_save().
#define XSH_DIVIDE_FLAT_THRESH 1e-10 |
Definition at line 151 of file xsh_drl.h.
Referenced by xsh_divide_flat().
#define XSH_LAMBDA_DIMM 0.0000005 |
Definition at line 499 of file xsh_drl.h.
Referenced by xsh_convert_seeing().
#define XSH_MATH_SQRT_2 1.4142135623730951 |
Definition at line 566 of file xsh_drl.h.
Referenced by create_gaussian_profile(), main(), xsh_image_create_gaussian_image(), and xsh_localize_ifu_slitlet().
#define XSH_MULTIPLY_FLAT_THRESH 1e+30 |
Definition at line 155 of file xsh_drl.h.
Referenced by xsh_multiply_flat().
#define XSH_OBJPOS_COLNAME_SLIT "Slit" |
Definition at line 497 of file xsh_drl.h.
Referenced by main(), xsh_compute_shift_ifu_slitlet(), and xsh_localize_ifu_slitlet().
#define XSH_OBJPOS_COLNAME_WAVELENGTH "Wavelength" |
Definition at line 495 of file xsh_drl.h.
Referenced by main(), xsh_compute_shift_ifu_slitlet(), and xsh_localize_ifu_slitlet().
#define XSH_OBJPOS_UNIT_SLIT "arcsec" |
Definition at line 498 of file xsh_drl.h.
Referenced by xsh_localize_ifu_slitlet().
#define XSH_OBJPOS_UNIT_WAVELENGTH "nm" |
Definition at line 496 of file xsh_drl.h.
Referenced by xsh_localize_ifu_slitlet().
#define XSH_RECTIFY_TYPE_MODEL 1 |
Definition at line 378 of file xsh_drl.h.
Referenced by xsh_rectify_orders().
#define XSH_RECTIFY_TYPE_POLY 0 |
Definition at line 377 of file xsh_drl.h.
Referenced by xsh_rectify_orders().
#define XSH_SHIFTIFU_COLNAME_SHIFTSLIT "Slit_shift" |
Definition at line 517 of file xsh_drl.h.
Referenced by fill_rectified(), xsh_compute_shift_ifu_slitlet(), and xsh_shift_offsettab().
#define XSH_SHIFTIFU_COLNAME_WAVELENGTH "Wavelength" |
Definition at line 515 of file xsh_drl.h.
Referenced by fill_rectified(), and xsh_compute_shift_ifu_slitlet().
#define XSH_SHIFTIFU_UNIT_SHIFTSLIT "arcsec" |
Definition at line 518 of file xsh_drl.h.
Referenced by xsh_compute_shift_ifu_slitlet().
#define XSH_SHIFTIFU_UNIT_WAVELENGTH "nm" |
Definition at line 516 of file xsh_drl.h.
Referenced by xsh_compute_shift_ifu_slitlet().
enum xsh_sol_wavelength |
cpl_frame* xsh_compute_response | ( | cpl_frame * | spectrum_frame, | |
cpl_frame * | flux_std_star_cat_frame, | |||
cpl_frame * | atmos_ext_frame, | |||
cpl_frame * | high_abs_frame, | |||
xsh_instrument * | instrument, | |||
double | exptime | |||
) |
Compute the instrument response using the rectified frame and the Standard star flux frame. The input should include also the Master Response Function and the Athmospheric Extinction Curve. Also should be produced the Efficiency frame.
spectrum_frame | Rectified frame (1D spectrum) | |
flux_std_star_cat_frame | Standard star flux catalog frame | |
atmos_ext_frame | Atmospheric Extinction Frame | |
instrument | Instrument strcture | |
exptime | Exposure time |
< computed response frame
< Std star flux
< Std star flux
< 1d spectrum
< 1d spectrum
Definition at line 3222 of file xsh_compute_response.c.
References check, check_msg, do_compute(), INTERPOL_WSTEP_NM, STAR_MATCH_DEPSILON, xsh_add_temporary_file(), XSH_ARM_NIR, XSH_ASSURE_NOT_NULL, XSH_ATMOS_EXT, xsh_atmos_ext_list_free(), xsh_atmos_ext_list_load(), xsh_fill_high_abs_regions(), xsh_frame_product(), xsh_frame_sci_get_ra_dec_airmass(), xsh_free_frame(), xsh_free_propertylist(), xsh_free_table(), xsh_instrument_arm_tostring(), xsh_instrument_get_arm(), xsh_instrument_mode_tostring(), xsh_msg, xsh_msg_warning, xsh_parse_catalog_std_stars(), xsh_pfits_get_cdelt1(), xsh_pfits_get_crval1(), xsh_pfits_get_gain(), xsh_pfits_get_naxis1(), xsh_response_merge_obj_std_info(), xsh_spectrum_free(), xsh_spectrum_interpolate(), xsh_spectrum_load(), xsh_spectrum_resample(), xsh_spectrum_save(), xsh_star_flux_list_free(), xsh_star_flux_list_load(), and xsh_star_flux_list_save().
Referenced by xsh_util_integrate().
cpl_frame* xsh_compute_response2 | ( | cpl_frame * | obs_std_star, | |
cpl_frame * | flux_std_star_cat, | |||
cpl_frame * | atmos_ext, | |||
cpl_frame * | high_abs, | |||
cpl_frame * | tell_mod_cat, | |||
xsh_instrument * | instrument, | |||
double | exptime, | |||
const int | tell_corr | |||
) |
Compute the instrument response using the rectified frame and the Standard star flux frame. The input should include also the Master Response Function and the Athmospheric Extinction Curve. Also should be produced the Efficiency frame.
obbs_std_star | Rectified frame (1D spectrum) | |
flux_std_star_cat | Standard star flux catalog frame | |
atmos_ext | Atmospheric Extinction Frame | |
instrument | Instrument structure | |
exptime | Exposure time | |
tell_corr | apply telluric correction |
Definition at line 2874 of file xsh_compute_response.c.
References check, xsh_star_flux_list::flux, xsh_star_flux_list::lambda, xsh_star_flux_list::size, STAR_MATCH_DEPSILON, xsh_rv_ref_wave_param::wguess, xsh_add_temporary_file(), XSH_ARM_NIR, XSH_ARM_UVB, XSH_ASSURE_NOT_NULL, xsh_bspline_fit(), xsh_fill_high_abs_regions(), xsh_frame_product(), xsh_frame_sci_get_ra_dec_airmass(), xsh_free_frame(), xsh_free_propertylist(), xsh_free_table(), xsh_instrument_arm_tostring(), xsh_instrument_get_arm(), xsh_instrument_mode_tostring(), xsh_msg, xsh_msg_warning, xsh_obs_std_correct(), xsh_parse_catalog_std_stars(), xsh_pfits_get_cdelt1(), xsh_pfits_get_crval1(), xsh_pfits_get_naxis1(), xsh_response_merge_obj_std_info(), xsh_rv_ref_wave_init(), xsh_rv_ref_wave_param_create(), xsh_rv_ref_wave_param_destroy(), xsh_spectrum_interpolate_linear(), xsh_spectrum_load(), xsh_star_flux_list_divide(), xsh_star_flux_list_duplicate(), xsh_star_flux_list_extrapolate_wave_end(), xsh_star_flux_list_filter_lowpass(), xsh_star_flux_list_filter_median(), xsh_star_flux_list_free(), xsh_star_flux_list_load(), xsh_star_flux_list_load_spectrum(), xsh_star_flux_list_save(), xsh_star_flux_list_to_frame(), xsh_std_star_spectra_correlate(), xsh_table_shift_rv(), and xsh_telluric_model_eval().
Referenced by xsh_respon_slit_nod(), xsh_respon_slit_offset(), xsh_respon_slit_stare(), and xsh_util_compute_response().
cpl_frame* xsh_compute_response_ord | ( | cpl_frame * | spectrum_frame, | |
cpl_frame * | flux_std_star_cat_frame, | |||
cpl_frame * | atmos_ext_frame, | |||
cpl_frame * | high_abs_win_frame, | |||
xsh_instrument * | instrument, | |||
double | exptime | |||
) |
Compute the instrument response using the rectified frame and the Standard star flux frame. The input should include also the Master Response Function and the Athmospheric Extinction Curve. Also should be produced the Efficiency frame.
spectrum_frame | Rectified frame (1D spectrum) | |
flux_std_star_cat_frame | Standard star flux catalog frame | |
atmos_ext_frame | Atmospheric Extinction Frame | |
instrument | Instrument strcture | |
exptime | Exposure time |
< computed response frame
< Std star flux
< obj star flux
< 1d spectrum
< 1d spectrum
Definition at line 3408 of file xsh_compute_response.c.
References check, check_msg, do_compute(), INTERPOL_WSTEP_NM, STAR_MATCH_DEPSILON, xsh_add_temporary_file(), XSH_ARM_NIR, XSH_ASSURE_NOT_NULL, xsh_atmos_ext_list_free(), xsh_atmos_ext_list_load(), xsh_fill_high_abs_regions(), xsh_frame_product(), xsh_frame_sci_get_ra_dec_airmass(), xsh_free_frame(), xsh_free_propertylist(), xsh_free_table(), xsh_instrument_arm_tostring(), xsh_instrument_get_arm(), xsh_instrument_mode_tostring(), xsh_msg, xsh_msg_warning, xsh_parse_catalog_std_stars(), xsh_pfits_get_cdelt1(), xsh_pfits_get_crval1(), xsh_pfits_get_gain(), xsh_pfits_get_naxis1(), xsh_spectrum_free(), xsh_spectrum_interpolate(), xsh_spectrum_load_order(), xsh_spectrum_save_order(), xsh_star_flux_list_free(), xsh_star_flux_list_load(), and xsh_star_flux_list_save_order().
Referenced by xsh_respon_slit_nod(), xsh_respon_slit_offset(), and xsh_respon_slit_stare().
void xsh_compute_slitlet_center | ( | xsh_order_list * | order_list, | |
cpl_frame * | slitmap_frame, | |||
double * | down, | |||
double * | cen, | |||
double * | up, | |||
XSH_ARM | arm | |||
) |
cpl_frame* xsh_create_dispersol_physmod | ( | cpl_frame * | pre_frame, | |
cpl_frame * | order_tab_frame, | |||
cpl_frame * | mod_cfg_frame, | |||
cpl_frame * | wave_map_frame, | |||
cpl_frame * | slit_map_frame, | |||
xsh_dispersol_param * | dispsol_param, | |||
cpl_frame * | spectral_format_frame, | |||
xsh_instrument * | instrument, | |||
const int | clean_tmp | |||
) |
Definition at line 363 of file xsh_create_wavemap.c.
References xsh_spectralformat::absorder, xsh_instrument::binx, xsh_instrument::biny, check, xsh_spectralformat::lambda_max_full, xsh_spectralformat::lambda_min_full, lambda_step, xsh_spectralformat_list::list, xsh_spectralformat_list::size, size, slit_step, x, xsh_add_temporary_file(), XSH_ASSURE_NOT_ILLEGAL_MSG, XSH_ASSURE_NOT_NULL_MSG, xsh_debug_level_get(), XSH_DEBUG_LEVEL_MEDIUM, XSH_FREE, xsh_free_frame(), xsh_free_image(), xsh_instrument_arm_tostring(), XSH_MALLOC, xsh_model_binxy(), xsh_model_config_load_best(), xsh_model_get_xy(), xsh_msg, xsh_msg_dbg_medium, xsh_pre_free(), xsh_pre_load(), xsh_spectralformat_list_free(), xsh_spectralformat_list_load(), xsh_wavemap_list_compute_poly(), xsh_wavemap_list_create(), xsh_wavemap_list_free(), xsh_wavemap_list_save_poly(), and y.
Referenced by xsh_2dmap(), and xsh_flexcomp().
void xsh_create_map | ( | cpl_frame * | dispsol_frame, | |
cpl_frame * | ordertab_frame, | |||
cpl_frame * | pre_frame, | |||
xsh_instrument * | instrument, | |||
cpl_frame ** | wavemap_frame, | |||
cpl_frame ** | slitmap_frame, | |||
const char * | rec_prefix | |||
) |
Definition at line 78 of file xsh_create_wavemap.c.
References check, XSH_ASSURE_NOT_NULL, xsh_dispersol_list_free(), xsh_dispersol_list_load(), xsh_dispersol_list_to_slitmap(), xsh_dispersol_list_to_wavemap(), XSH_GET_TAG_FROM_ARM, xsh_pre_free(), xsh_pre_load(), XSH_SLIT_MAP_POLY, and XSH_WAVE_MAP_POLY.
Referenced by main(), xsh_check_get_map(), xsh_geom_ifu(), xsh_scired_ifu_offset(), xsh_scired_ifu_stare(), and xsh_slit_stare_get_maps().
void xsh_create_model_map | ( | cpl_frame * | model_frame, | |
xsh_instrument * | instrument, | |||
const char * | wave_map_tag, | |||
const char * | slit_map_tag, | |||
cpl_frame ** | wavemap_frame, | |||
cpl_frame ** | slitmap_frame, | |||
const int | save_tmp | |||
) |
Definition at line 127 of file xsh_create_wavemap.c.
References xsh_instrument::binx, xsh_instrument::biny, check, XSH_ASSURE_NOT_NULL, XSH_ASSURE_NOT_NULL_MSG, xsh_model_binxy(), xsh_model_config_load_best(), and xsh_model_maps_create().
Referenced by xsh_2dmap(), xsh_check_get_map(), xsh_flexcomp(), xsh_geom_ifu(), xsh_scired_ifu_offset(), xsh_scired_ifu_stare(), xsh_slit_stare_get_maps(), xsh_util_physmod(), and xsh_wavecal().
cpl_frame* xsh_create_order_table | ( | cpl_frame * | in_frame, | |
cpl_frame * | spectralformat_frame, | |||
cpl_frame * | resid_frame, | |||
cpl_frame * | arclines, | |||
xsh_detect_arclines_param * | da, | |||
xsh_clipping_param * | dac, | |||
xsh_instrument * | instrument | |||
) |
Definition at line 74 of file xsh_create_order_table.c.
References xsh_order::cenpoly, check, data_order_compare(), xsh_order::endy, xsh_resid_tab::header, xsh_spectralformat_list::list, xsh_order_list::list, xsh_detect_arclines_param::mode_iterative, xsh_pre::ny, xsh_detect_arclines_param::ordertab_deg_y, xsh_order_list::size, size, xsh_order::starty, xsh_arclist_free(), xsh_arclist_get_size(), xsh_arclist_load(), XSH_ASSURE_NOT_NULL, XSH_CALLOC, xsh_debug_level_get(), XSH_DEBUG_LEVEL_MEDIUM, XSH_FREE, xsh_free_table(), XSH_GET_TAG_FROM_ARM, xsh_msg, xsh_msg_dbg_high, xsh_msg_dbg_medium, xsh_order_list_create(), xsh_order_list_fit(), xsh_order_list_free(), xsh_order_list_get_header(), xsh_order_list_save(), XSH_ORDER_TAB_GUESS, xsh_pfits_get_date(), xsh_pfits_set_qc(), xsh_pfits_set_qc_nlinecat(), xsh_pfits_set_qc_nlinefound(), xsh_pre_free(), xsh_pre_load(), XSH_QC_MODEL_FMTCHK_DATE, xsh_reindex(), xsh_resid_tab_free(), xsh_resid_tab_get_lambda_data(), xsh_resid_tab_get_order_data(), xsh_resid_tab_get_size(), xsh_resid_tab_get_xgauss_data(), xsh_resid_tab_get_ygauss_data(), xsh_resid_tab_load(), xsh_sort(), xsh_spectralformat_list_free(), xsh_spectralformat_list_load(), XSH_SPECTRALFORMAT_TABLE_COLNAME_XMIN, xsh_spectralformat::ymax, and xsh_spectralformat::ymin.
Referenced by xsh_predict().
cpl_frame* xsh_create_poly_wavemap | ( | cpl_frame * | pre_frame, | |
cpl_frame * | wave_tab_2d_frame, | |||
cpl_frame * | order_tab_frame, | |||
cpl_frame * | spectral_format_frame, | |||
xsh_dispersol_param * | dispsol_par, | |||
xsh_instrument * | instrument, | |||
const char * | filename, | |||
cpl_frame ** | dispersol_frame, | |||
cpl_frame ** | slitmap_frame | |||
) |
Definition at line 196 of file xsh_create_wavemap.c.
References xsh_spectralformat::absorder, binx, check, xsh_spectralformat::lambda_max_full, xsh_spectralformat::lambda_min_full, lambda_step, xsh_spectralformat_list::list, xsh_wavesol::max_slit, xsh_wavesol::min_slit, xsh_spectralformat_list::size, size, slit_step, x, XSH_ASSURE_NOT_ILLEGAL_MSG, XSH_ASSURE_NOT_NULL, xsh_debug_level_get(), XSH_DEBUG_LEVEL_MEDIUM, XSH_FREE, XSH_GET_TAG_FROM_ARM, xsh_instrument_get_binx(), XSH_MALLOC, xsh_msg, xsh_msg_dbg_medium, xsh_pre_free(), xsh_pre_load(), XSH_SLIT_MAP_POLY, xsh_spectralformat_list_free(), xsh_spectralformat_list_load(), xsh_wavemap_list_compute(), xsh_wavemap_list_compute_poly(), xsh_wavemap_list_create(), xsh_wavemap_list_free(), xsh_wavemap_list_save_poly(), xsh_wavesol_eval_polx(), xsh_wavesol_eval_poly(), xsh_wavesol_free(), xsh_wavesol_load(), xsh_wavesol_set_bin_x(), xsh_wavesol_set_bin_y(), and y.
Referenced by xsh_2dmap(), and xsh_flexcomp().
cpl_frame* xsh_create_wavemap | ( | cpl_frame * | in_frame, | |
cpl_frame * | resid_frame, | |||
cpl_frame * | order_frame, | |||
xsh_dispersol_param * | dispersol_param, | |||
xsh_instrument * | instrument | |||
) |
cpl_error_code xsh_wavemap_qc | ( | cpl_frame * | frm_map, | |
const cpl_frame * | frm_tab | |||
) |
Monitor Flux level along the orders traces given by an input table.
frm_map | The input frame image whose flux is to be monitored | |
frm_tab | input frame table with order traces |
Definition at line 565 of file xsh_create_wavemap.c.
References check, XSH_ASSURE_NOT_NULL, xsh_free_image(), xsh_free_propertylist(), xsh_free_table(), XSH_QC_WMAP_WAVEC, and xsh_update_pheader_in_image_multi().
Referenced by xsh_2dmap().
cpl_error_code xsh_wavetab_qc | ( | cpl_frame * | frm_tab, | |
const int | is_poly | |||
) |
Monitor min/max/med/avg distance between detected lines on each ordee.
frm_tab | input frame table with order traces | |
is_poly | data reduction method |
Definition at line 643 of file xsh_create_wavemap.c.
References check, XSH_ASSURE_NOT_NULL, xsh_free_propertylist(), xsh_free_table(), xsh_free_vector(), xsh_msg_warning, XSH_QC_LINE_DIFAVG, XSH_QC_LINE_DIFAVG_C, XSH_QC_LINE_DIFMAX, XSH_QC_LINE_DIFMAX_C, XSH_QC_LINE_DIFMAX_ORD, XSH_QC_LINE_DIFMED, XSH_QC_LINE_DIFMED_C, XSH_QC_LINE_DIFMIN, XSH_QC_LINE_DIFMIN_C, and XSH_QC_LINE_DIFMIN_ORD.
Referenced by xsh_2dmap(), and xsh_predict().