/home/amodigli/releases/xsh/1.2.10/pso/xsh.26608/xshp/xsh/xsh_drl.h File Reference

#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_data_slice_offset.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   1
#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_MATH_SQRT_2   1.4142135623730951
#define REGDEBUG_GAUSSIAN   0
#define REGDEBUG_MODEL   0
#define REGDEBUG_BLAZE   0
#define REGDEBUG_EXTRACT   0
#define REGDEBUG_EXTRACT_XY   0
#define REGDEBUG_SUBEXTRACT   0
#define REGDEBUG_SUBEXTRACT_XY   0
#define REGDEBUG_EXTRACT_STD   1
#define REGDEBUG_WEIGHT   0
#define REGDEBUG_EXTRACT_OPT   0
#define REGDEBUG_N   0

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)
 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_clipping_param *crh_clipping, xsh_instrument *inst, cpl_imagelist **, cpl_image **)
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_parameterlist *drs_params, cpl_frame *crh_frm, cpl_frame *bp_map_frm)
cpl_frame * xsh_create_master_bias (cpl_frameset *raws, cpl_frame *frame, xsh_instrument *instr, cpl_parameterlist *parameters)
 Creates a master bias frame.
cpl_frame * xsh_create_master_flat (cpl_frame *frame, xsh_instrument *instr)
cpl_frame * xsh_create_master_bpmap (cpl_frame *frame, xsh_instrument *instr)
cpl_frame * xsh_compute_linearity (cpl_frameset *, xsh_instrument *, xsh_clipping_param *)
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)
 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)
 Subtract the 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)
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)
 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 (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 *disptab_frame, xsh_follow_arclines_param *param, double slit, double slit_min, double slit_max, const char *tag_id, int ifu_flag, xsh_instrument *instrument, cpl_frame **tilt_list, 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_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)
 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_frame *model_frame, xsh_instrument *instrument, xsh_rectify_param *rectify_par, cpl_frame *spectralformat_frame, cpl_frame *sliceoffset_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_frame *model_config_frame, xsh_instrument *instrument, xsh_rectify_param *rectify_par, cpl_frame *spectral_format, cpl_frame *slice_offset_frame, 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.
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)
 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_save_sky_model (cpl_frame *obj_frame, cpl_frame *sub_sky_frame, const char *sky_tag, xsh_instrument *instrument)
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_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, cpl_frame *wavemap_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, cpl_frame *wave_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, xsh_merge_param *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, xsh_merge_param *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, xsh_merge_param *merge_par, const char *rec_prefix)
 Merge orders of the rectified frame using merge parameters.
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_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)
 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)
 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_instrument *instr, const char *result_name)
 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_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_clipping_param *crh_clipping, xsh_instrument *instr, cpl_imagelist **list, cpl_image **crh_ima)
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_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)
 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)

Define Documentation

#define PICKUP_NOISE_HOT_PIXEL_MAP

Definition at line 52 of file xsh_drl.h.

#define REGDEBUG_BLAZE   0

Definition at line 485 of file xsh_drl.h.

#define REGDEBUG_EXTRACT   0

Definition at line 486 of file xsh_drl.h.

#define REGDEBUG_EXTRACT_OPT   0

Definition at line 492 of file xsh_drl.h.

#define REGDEBUG_EXTRACT_STD   1

Definition at line 490 of file xsh_drl.h.

#define REGDEBUG_EXTRACT_XY   0

Definition at line 487 of file xsh_drl.h.

#define REGDEBUG_GAUSSIAN   0

Definition at line 483 of file xsh_drl.h.

#define REGDEBUG_MODEL   0

Definition at line 484 of file xsh_drl.h.

#define REGDEBUG_N   0

Definition at line 493 of file xsh_drl.h.

#define REGDEBUG_OPTEXTRACT   1

Definition at line 61 of file xsh_drl.h.

#define REGDEBUG_SUBEXTRACT   0

Definition at line 488 of file xsh_drl.h.

#define REGDEBUG_SUBEXTRACT_XY   0

Definition at line 489 of file xsh_drl.h.

#define REGDEBUG_WEIGHT   0

Definition at line 491 of file xsh_drl.h.

#define SLIT_PRECISION   0.00001

Definition at line 180 of file xsh_drl.h.

#define SLIT_PRECISION_IFU   0.21

Definition at line 181 of file xsh_drl.h.

#define WAVELENGTH_PRECISION   0.00001
#define XSH_CONCAT ( A,
 )     A ## B

Definition at line 49 of file xsh_drl.h.

#define XSH_DETECT_ARCLINES_MODE_CORRECTED   1

Definition at line 217 of file xsh_drl.h.

Referenced by xsh_detect_arclines().

#define XSH_DETECT_ARCLINES_MODE_NORMAL   0

Definition at line 216 of file xsh_drl.h.

Referenced by xsh_detect_arclines().

#define XSH_DETECT_ARCLINES_MODE_RECOVER   2

Definition at line 218 of file xsh_drl.h.

Referenced by xsh_detect_arclines().

#define XSH_DETECT_ARCLINES_TYPE_MODEL   1

Definition at line 215 of file xsh_drl.h.

Referenced by xsh_detect_arclines(), and xsh_resid_tab_load().

#define XSH_DETECT_ARCLINES_TYPE_POLY   0
#define XSH_DIVIDE_FLAT_THRESH   1e-10

Definition at line 140 of file xsh_drl.h.

Referenced by xsh_divide_flat().

#define XSH_MATH_SQRT_2   1.4142135623730951

Definition at line 474 of file xsh_drl.h.

Referenced by xsh_image_create_gaussian_image().

#define XSH_MULTIPLY_FLAT_THRESH   1e+30

Definition at line 144 of file xsh_drl.h.

Referenced by xsh_multiply_flat().

#define XSH_RECTIFY_TYPE_MODEL   1

Definition at line 360 of file xsh_drl.h.

Referenced by xsh_rectify_orders().

#define XSH_RECTIFY_TYPE_POLY   0

Definition at line 359 of file xsh_drl.h.

Referenced by xsh_rectify_orders().

#define XSH_STRING (  )     # A

Definition at line 50 of file xsh_drl.h.


Enumeration Type Documentation

Enumerator:
XSH_SOLUTION_ABSOLUTE 
XSH_SOLUTION_RELATIVE 

Definition at line 220 of file xsh_drl.h.


Function Documentation

cpl_frame* xsh_compute_noise_map ( cpl_imagelist *  ,
cpl_frame *  bpmap,
xsh_clipping_param ,
xsh_instrument instr,
cpl_frame **  noisemap 
)
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.

Parameters:
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
Returns:
Frame of the computed response

< computed response frame

< Std star flux

< 1d spectrum

< 1d spectrum

Definition at line 945 of file xsh_compute_response.c.

References check, check_msg, do_compute(), INTERPOL_WSTEP_NM, STAR_MATCH_DEPSILON, 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_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_linear(), 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_respon_slit_nod(), xsh_respon_slit_offset(), xsh_respon_slit_stare(), and xsh_util_integrate().

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.

Parameters:
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
Returns:
Frame of the computed response

< computed response frame

< Std star flux

< 1d spectrum

< 1d spectrum

Definition at line 1124 of file xsh_compute_response.c.

References check, check_msg, do_compute(), INTERPOL_WSTEP_NM, STAR_MATCH_DEPSILON, 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_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(), xsh_respon_slit_stare(), and xsh_util_compute_response().

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 
)
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 
)
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 
)
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 
)
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 
)
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.

Parameters:
frm_map The input frame image whose flux is to be monitored
frm_tab input frame table with order traces
Returns:
The input frame image FITS header is updated with flux level QC parameters

Definition at line 552 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.

Parameters:
frm_tab input frame table with order traces
is_poly data reduction method
Returns:
The input frame image FITS header is updated with flux level QC parameters

Definition at line 630 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().


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