Macros
#define	REGDEBUG_FULL 0

#define	new_bp 1

#define	SLIT_FRAC_STEP 50

Functions
cpl_frame *	xsh_hdrl_remove_crh_single (cpl_frame frm, xsh_instrument instrument, xsh_remove_crh_single_param crh_single_par, const char ftag)

static double	compute_shift_with_localization (cpl_frame loc_frame, cpl_frame loc0_frame)

static double	compute_shift_with_kw (cpl_propertylist header, xsh_rectify_param rectify_par, double ref_ra, double ref_dec, int flag)

static cpl_frame *	xsh_shift (cpl_frame rec_frame, xsh_instrument instrument, const char fname, double slit_shift, cpl_frame *res_frame_ext)

static void	xsh_frame_set_shiftifu_ref (cpl_propertylist header, cpl_frame shift_frame)

static void	xsh_rec_list_rectify (xsh_rec_list rec_list, int iorder, int irec, xsh_pre sci_pre, cpl_image var_img, double fx, double fy, double radius, cpl_vector profile, cpl_vector *profile2, double mult)

static void	fill_rectified (xsh_pre pre_sci, xsh_rec_list rec_list, int idx, xsh_wavesol wavesol, xsh_xs_3 model_config, xsh_instrument instrument, xsh_dispersol_list disp_list, float slit_min, float slit_max, double lambda_min, int skip_low, int skip_up, xsh_rectify_param rectify_par, double slit_shift, cpl_frame slit_shiftab_frame)
	Fill the rectified structure for one order with the corresponding flux, using the wavelength solution.

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_rec_slit_size (xsh_rectify_param rectify_par, double slit_min, int *nslit, XSH_MODE mode)
	rectify frame

static void	adjust_lambdas (xsh_spectralformat_list spec_list, xsh_rectify_param rectify_par)

cpl_frame *	xsh_rectify (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 disp_tab_frame, const char res_name, cpl_frame res_frame_ext, cpl_frame res_frame_tab, const char rec_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 *	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 orderlist_frame, cpl_frameset wavesol_frameset, cpl_frameset shiftifu_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, const char rec_prefix)

cpl_frame *	xsh_rectify_orders (cpl_frame sci_frame, xsh_order_list orderlist, 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.

static void	xsh_get_shift_ref (cpl_frameset set, double down, double cen, double up)

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_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 res_frameset_ext, cpl_frameset res_frameset_tab, int min_index, int max_index, const char rec_prefix)

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_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)

Variables
static cpl_vector *	rec_profile = NULL

static cpl_vector *	err_profile = NULL

Detailed Description

Function ...

Macro Definition Documentation

◆ new_bp

#define new_bp 1

Definition at line 71 of file xsh_rectify.c.

◆ REGDEBUG_FULL

#define REGDEBUG_FULL 0

Definition at line 48 of file xsh_hdrl_functions.c.

◆ SLIT_FRAC_STEP

#define SLIT_FRAC_STEP 50

Definition at line 78 of file xsh_rectify.c.

Function Documentation

◆ adjust_lambdas()

static void adjust_lambdas	(	xsh_spectralformat_list *	spec_list,
		xsh_rectify_param *	rectify_par
	)

static

Definition at line 788 of file xsh_rectify.c.

References xsh_spectralformat::lambda_max, xsh_spectralformat::lambda_min, xsh_spectralformat_list::list, max, xsh_rectify_param::rectif_bin_lambda, xsh_spectralformat_list::size, step, and xsh_msg_dbg_high.

Referenced by xsh_rectify_orders().

◆ compute_shift_with_kw()

static double compute_shift_with_kw	(	cpl_propertylist *	header,
		xsh_rectify_param *	rectify_par,
		double **	ref_ra,
		double **	ref_dec,
		int	flag
	)

static

Definition at line 1887 of file xsh_rectify.c.

References check, M_PI, XSH_ASSURE_NOT_NULL, XSH_MALLOC, xsh_msg, xsh_msg_dbg_high, xsh_pfits_get_b_dec_cumoffset(), xsh_pfits_get_b_dec_reloffset(), xsh_pfits_get_b_ra_cumoffset(), xsh_pfits_get_b_ra_reloffset(), xsh_pfits_get_dec_cumoffset(), xsh_pfits_get_posang(), and xsh_pfits_get_ra_cumoffset().

Referenced by shift_with_kw().

◆ compute_shift_with_localization()

static double compute_shift_with_localization	(	cpl_frame *	loc_frame,
		cpl_frame *	loc0_frame
	)

static

This function creates a structure containing for each order the shift to be applied.

Parameters

loc_frame	Localization of the current rectified frame
loc0_frame	Localization of the reference frame (first A frame)

Definition at line 1708 of file xsh_rectify.c.

References xsh_localization::cenpoly, check, XSH_ASSURE_NOT_NULL, xsh_localization_free(), xsh_localization_load(), xsh_msg, and xsh_msg_dbg_medium.

Referenced by xsh_rectify_and_shift().

◆ fill_rectified()

static void fill_rectified	(	xsh_pre *	pre_sci,
		xsh_rec_list *	rec_list,
		int	idx,
		xsh_wavesol *	wavesol,
		xsh_xs_3 *	model_config,
		xsh_instrument *	instrument,
		xsh_dispersol_list *	disp_list,
		float	slit_min,
		float	slit_max,
		double	lambda_min,
		int	skip_low,
		int	skip_up,
		xsh_rectify_param *	rectify_par,
		double	slit_shift,
		cpl_frame *	slit_shiftab_frame
	)

static

Fill the rectified structure for one order with the corresponding flux, using the wavelength solution.

Parameters

[in]	pre_sci	Science Frame (in PRE format)
[in]	rec_list	Rectified structure pointer (to fill)
[in]	idx	Index in the rec_list
[in]	wavesol	Wave Solution structure pointer
[in]	model_config	model configuration structure
[in]	instrument	instrument arm structure
[in]	disp_list	dispersion structure
[in]	slit_min	min slit value
[in]	slit_max	max slit value
[in]	lambda_min	min lambda value
[in]	skip_low	amount of points to skip on low slice
[in]	skip_up	amount of points to skip on up slice
[in]	rectify_par	rectify parameter
[in]	slit_shift	shift nod position on slit

Definition at line 371 of file xsh_rectify.c.

References assure, xsh_instrument::binx, xsh_instrument::biny, check, convert_data_to_bin(), err_profile, instrument, xsh_rectify_param::kernel_type, xsh_rec::lambda, xsh_dispersol::lambda_poly, xsh_dispersol_list::list, xsh_rec_list::list, order, rec_profile, xsh_rectify_param::rectif_bin_lambda, xsh_rectify_param::rectif_bin_space, xsh_rectify_param::rectif_radius, xsh_rec::slit, xsh_dispersol::slit_poly, XSH_ASSURE_NOT_NULL, XSH_CALLOC, xsh_data_interpolate(), xsh_debug_level_get(), XSH_DEBUG_LEVEL_MEDIUM, XSH_FREE, xsh_free_image(), xsh_free_polynomial(), xsh_free_vector(), xsh_model_get_xy(), xsh_msg_dbg_low, xsh_pre_get_errs(), xsh_rec_list_get_lambda(), xsh_rec_list_get_nlambda(), xsh_rec_list_get_nslit(), xsh_rec_list_get_order(), xsh_rec_list_get_slit(), xsh_rec_list_rectify(), XSH_SHIFTIFU_COLNAME_SHIFTSLIT, XSH_SHIFTIFU_COLNAME_WAVELENGTH, XSH_TABLE_FREE, XSH_TABLE_LOAD, xsh_wavesol_eval_polx(), and xsh_wavesol_eval_poly().

Referenced by xsh_rectify_orders().

◆ shift_with_kw()

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.

Parameters

[in]	rec_frame	Science Frame. The kwywords are taken from the header.
[in]	instrument	Instrument structure
[in]	rectify_par	Rectification parameters
[in]	fname	filename
[out]	res_frame_ext	resampled frame in ESO format
[out]	ref_ra	RA of reference frame
[out]	ref_dec	DEG of reference frame
[in]	flag	flag

Returns: resampled frame in DRL frame

Definition at line 1974 of file xsh_rectify.c.

References check, compute_shift_with_kw(), instrument, XSH_ASSURE_NOT_NULL, xsh_free_frame(), xsh_free_propertylist(), xsh_msg, xsh_pfits_get_rectify_bin_space(), xsh_round_double(), and xsh_shift().

Referenced by main(), xsh_nod_rectify_and_shift_with_key(), and xsh_shift_rectified().

◆ xsh_compute_slitlet_limits()

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
	)

Computes with the OFFSET_TAB frameset the slitlet limits in order to build the IFU cube

Parameters

[in]	shift_set	The OFFSET_TAB frameset
[in]	sdown	Limit down of the slit
[in]	sldown	Limit down of the central slitlet
[in]	slup	Limit up of then central slitlet
[in]	sup	Limit up of the slit
[in]	slit_bin	the slit binning use in rectify process
[in,out]	slitmin_tab	The compute position of the lower limit of each slitlet
[in,out]	nslit_tab	The number of bins of each slitlet
[in,out]	slitcen_tab	The center of each slitlet

Definition at line 1372 of file xsh_rectify.c.

References check, XSH_ASSURE_NOT_NULL, xsh_get_shift_ref(), xsh_msg, and xsh_msg_dbg_medium.

Referenced by main(), and xsh_rectify_orders_ifu().

◆ xsh_frame_set_shiftifu_ref()

static void xsh_frame_set_shiftifu_ref	(	cpl_propertylist *	header,
		cpl_frame *	shift_frame
	)

static

Definition at line 1332 of file xsh_rectify.c.

References check, XSH_ASSURE_NOT_NULL, xsh_free_propertylist(), xsh_pfits_get_shiftifu_lambdaref(), xsh_pfits_get_shiftifu_slitref(), xsh_pfits_set_shiftifu_lambdaref(), and xsh_pfits_set_shiftifu_slitref().

Referenced by xsh_rectify_orders().

◆ xsh_get_shift_ref()

static void xsh_get_shift_ref	(	cpl_frameset *	set,
		double *	down,
		double *	cen,
		double *	up
	)

static

Definition at line 1291 of file xsh_rectify.c.

References check, XSH_ASSURE_NOT_NULL, xsh_free_propertylist(), and xsh_pfits_get_shiftifu_slitref().

Referenced by xsh_compute_slitlet_limits().

◆ xsh_get_slit_edges()

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.

Parameters

[in]	slitmap_frame	slit map frame
[in]	sdown	down SLIT trace estimate
[in]	sup	upp SLIT trace estimate
[in]	sldown	down IFU slice estimate
[in]	slup	down IFU slice estimate
[in]	instrument	instrument arm setting

Definition at line 671 of file xsh_rectify.c.

References check, instrument, MAX_SLIT, MIN_SLIT, SLITLET_CEN_CENTER, XSH_ASSURE_NOT_NULL, xsh_error_reset, xsh_free_propertylist(), xsh_instrument_get_mode(), XSH_MODE_IFU, xsh_msg, xsh_msg_warning, xsh_pfits_get_slitmap_median_edglo(), xsh_pfits_get_slitmap_median_edgup(), xsh_pfits_get_slitmap_median_sliclo(), and xsh_pfits_get_slitmap_median_slicup().

Referenced by main(), xsh_compute_slice_dist(), xsh_follow_arclines_ifu(), xsh_opt_extract_orders(), and xsh_rectify_orders_ifu().

◆ xsh_hdrl_remove_crh_single()

cpl_frame * xsh_hdrl_remove_crh_single	(	cpl_frame *	frm,
		xsh_instrument *	instrument,
		xsh_remove_crh_single_param *	crh_single_par,
		const char *	ftag
	)

◆ xsh_rec_list_rectify()

static void xsh_rec_list_rectify	(	xsh_rec_list *	rec_list,
		int	iorder,
		int	irec,
		xsh_pre *	sci_pre,
		cpl_image *	var_img,
		double	fx,
		double	fy,
		double	radius,
		cpl_vector *	profile,
		cpl_vector *	profile2,
		double	mult
	)

static

Definition at line 188 of file xsh_rectify.c.

References check, nx, ny, QFLAG_MISSING_DATA, QFLAG_OUTSIDE_DATA_RANGE, XSH_ASSURE_NOT_NULL, xsh_msg_dbg_high, xsh_pre_get_data(), xsh_pre_get_errs(), xsh_pre_get_nx(), xsh_pre_get_ny(), xsh_pre_get_qual(), xsh_rec_list_get_data1(), xsh_rec_list_get_errs1(), and xsh_rec_list_get_qual1().

Referenced by fill_rectified().

◆ xsh_rec_slit_size()

void xsh_rec_slit_size	(	xsh_rectify_param *	rectify_par,
		double *	slit_min,
		int *	nslit,
		XSH_MODE	mode
	)

rectify frame

Parameters

[in]	rectify_par	parameters structure to control rectification
[out]	slit_min	min slit value
[out]	nslit	number of slit sampling points
[in]	mode	mode to control if we are in slit mode

Definition at line 758 of file xsh_rectify.c.

References MAX_SLIT, MIN_SLIT, mode, xsh_rectify_param::rectif_bin_space, xsh_rectify_param::rectify_full_slit, slit_step, XSH_ASSURE_NOT_NULL, XSH_MODE_SLIT, xsh_msg, and xsh_msg_warning.

Referenced by main(), xsh_rectify(), and xsh_rectify_and_shift().

◆ xsh_rectify()

cpl_frame * xsh_rectify	(	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 *	disp_tab_frame,
		const char *	res_name,
		cpl_frame **	res_frame_ext,
		cpl_frame **	res_frame_tab,
		const char *	rec_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.

Parameters

sci_frame	The input Science frame after sky subtaraction
orderlist_frame	The input Order Table Frame
wavesol_frame	The input Wavesolution frame
model_frame	The input model frame
instrument	Pointer to instrument description structure
rectify_par	Parameters for rectification
spectralformat_frame	The frame for the spectral format
disp_tab_frame	The dispersion table frame (for flux conservation)
res_name	The file name of the resampled frame
res_frame_ext	The resampled frame in ESO format
res_frame_tab	A table associated to the resampled frame
rec_prefix	The recipe prefix (to build proper products PRO.CATG)

Returns: Rectified frame

Definition at line 867 of file xsh_rectify.c.

References check, instrument, XSH_ASSURE_NOT_NULL, XSH_GET_TAG_FROM_ARM, XSH_MODE_SLIT, XSH_ORDER2D, xsh_order_list_free(), xsh_order_list_load(), xsh_rec_slit_size(), and xsh_rectify_orders().

Referenced by xsh_absorp(), xsh_nod_rectify_and_shift_with_key(), xsh_respon_slit_offset(), xsh_respon_slit_stare(), xsh_scired_slit_nod_accurate(), xsh_scired_slit_offset(), xsh_scired_slit_stare(), and xsh_slit_stare_correct_crh_and_sky().

◆ xsh_rectify_and_shift()

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
	)

This function rectify AND shift the input frame. The shift is calculated for each order and later used in the fill_rectify function.

Parameters

sci_frame	Science Frame (PRE format)
orderlist_frame	Order table
wavesol_frame	Wave table (can be NULL)
model_frame	Model Frame (can be NULL)
instrument	Instrument structure
rectify_par	Rectify parameters
spectralformat_frame	Spectral format table frame
loc_frame	Localization of this frame
loc0_frame	Localization of the reference frame (first A frame)
throw_shift	shift in nod throw
disp_tab_frame	Dispersion table
res_name	Result frame name
res_frame_ext	Ext result frame
res_frame_tab	Ext result frame table

Returns: The rectified (and shifted) frame

Definition at line 928 of file xsh_rectify.c.

References check, compute_shift_with_localization(), instrument, xsh_rectify_param::rectif_bin_space, XSH_ASSURE_NOT_NULL, xsh_free_frame(), xsh_free_propertylist(), XSH_GET_TAG_FROM_ARM, XSH_MODE_SLIT, xsh_msg, XSH_ORDER2D, xsh_order_list_free(), xsh_order_list_load(), xsh_rec_slit_size(), xsh_rectify_orders(), xsh_round_double(), and xsh_shift().

Referenced by xsh_scired_slit_nod_accurate().

◆ xsh_rectify_ifu()

cpl_frameset * xsh_rectify_ifu	(	cpl_frame *	sci_frame,
		cpl_frame *	orderlist_frame,
		cpl_frameset *	wavesol_frameset,
		cpl_frameset *	shiftifu_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,
		const char *	rec_prefix
	)

Definition at line 1014 of file xsh_rectify.c.

References check, instrument, XSH_ASSURE_NOT_NULL, xsh_order_list_free(), xsh_order_list_load(), xsh_rectify_orders_ifu(), and XSH_REGDEBUG.

Referenced by xsh_geom_ifu(), xsh_scired_ifu_offset(), and xsh_scired_ifu_stare().

◆ xsh_rectify_orders()

cpl_frame * xsh_rectify_orders	(	cpl_frame *	sci_frame,
		xsh_order_list *	orderlist,
		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.

Parameters

sci_frame	The input Science frame after sky subtaraction
orderlist	The input Order Table Frame
wavesol_frame	The input Wavesolution frame
model_frame	The input model frame
instrument	Pointer to instrument description structure
rectify_par	Parameters for rectification
spectralformat_frame	spectral format table
disp_tab_frame	disp tab frame
res_name	resampled frame filename
tag	resampled frame tag
res_frame_ext	resampled frame in ESO format
res_frame_tab	resampled frame in ESO format table
min_index	min index
max_index	max index
slit_min	slit min
nslit	number of slit sampling points
slit_shift	shift of nod position on slit

Returns: Rectified frame

Definition at line 1079 of file xsh_rectify.c.

References xsh_spectralformat::absorder, adjust_lambdas(), assure, check, xsh_rectify_param::conserve_flux, xsh_pre::data, xsh_pre::data_header, xsh_instrument::decode_bp, fill_rectified(), xsh_rec_list::header, instrument, xsh_spectralformat::lambda_max, xsh_spectralformat::lambda_min, xsh_rec_list::list, xsh_spectralformat_list::list, n, xsh_rec::nlambda, xsh_rec::nslit, xsh_rec_list::nslit, order, xsh_pre::qual, xsh_rectify_param::rectif_bin_lambda, xsh_rectify_param::rectif_bin_space, xsh_rectify_param::rectif_kernel, xsh_rectify_param::rectif_radius, xsh_rec_list::size, size, xsh_rec::slit, xsh_rec_list::slit_max, xsh_rec_list::slit_min, xsh_add_temporary_file(), XSH_ASSURE_NOT_ILLEGAL, XSH_ASSURE_NOT_NULL, xsh_baryvel(), xsh_dispersol_list_free(), xsh_dispersol_list_load(), xsh_error_msg, xsh_frame_set_shiftifu_ref(), xsh_free_mask(), xsh_instrument_arm_tostring(), xsh_model_config_load_best(), xsh_model_temperature_update_frame(), xsh_msg, xsh_msg_dbg_high, xsh_msg_dbg_medium, xsh_pre_free(), xsh_pre_load(), XSH_QC_VRAD_BARYCOR, XSH_QC_VRAD_BARYCOR_C, XSH_QC_VRAD_HELICOR, XSH_QC_VRAD_HELICOR_C, xsh_qual_to_cpl_mask(), xsh_rec_list_create(), xsh_rec_list_free(), xsh_rec_list_save(), xsh_rec_list_save2(), xsh_rec_list_save_table(), xsh_rec_list_set_data_size(), xsh_rec_list_update_header(), XSH_RECTIFY_TYPE_MODEL, XSH_RECTIFY_TYPE_POLY, xsh_round_double(), xsh_spectralformat_list_free(), xsh_spectralformat_list_load(), xsh_wavesol_free(), and xsh_wavesol_load().

Referenced by main(), xsh_rectify(), xsh_rectify_and_shift(), and xsh_rectify_orders_ifu().

◆ xsh_rectify_orders_ifu()

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 **	res_frameset_ext,
		cpl_frameset **	res_frameset_tab,
		int	min_index,
		int	max_index,
		const char *	rec_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.

Parameters

[in]	sci_frame	Science frame after sky subtaraction
[in]	orderlist	Order traces structure
[in]	wavesol_frameset	Input Wavesolution frameset (containing the 3 slitlet wave solution: DOWN, CEN, UP)
[in]	model_frame	physical model cfg table frame
[in]	instrument	Pointer to instrument description structure
[in]	rectify_par	Parameters for rectification
[in]	spectralformat_frame	The frame for the spectral format
[in]	sliceoffset_frame	frame with measured offsets of each IFU slices
[in]	slitmap_frame	The SLIT MAP Image Frame
[out]	res_frameset_ext	resampled frame in ESO format
[out]	res_frameset_tab	resampled frame in ESO format (tab)
[in]	min_index	min index
[in]	max_index	max index
[in]	rec_prefix	recipe prefix (for proper PRO.CATG values)

Returns: Rectified frame

Definition at line 1514 of file xsh_rectify.c.

References CENTER_IFU_SLITLET, check, instrument, LOWER_IFU_SLITLET, xsh_rectify_param::rectif_bin_space, UPPER_IFU_SLITLET, XSH_ASSURE_NOT_NULL, XSH_CMP_INT, xsh_compute_slitlet_limits(), xsh_get_slit_edges(), XSH_GET_TAG_FROM_ARM, xsh_msg, and xsh_rectify_orders().

Referenced by xsh_rectify_ifu().

◆ xsh_shift()

static cpl_frame * xsh_shift	(	cpl_frame *	rec_frame,
		xsh_instrument *	instrument,
		const char *	fname,
		double	slit_shift,
		cpl_frame **	res_frame_ext
	)

static

◆ xsh_shift_rectified()

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
	)

This function is used to shift a rectified frame to the position of the first frame (nodding observation). The shift is calculated either by using the localization table of the current and the first frame, or by using the NODTHROW, RELOFFSET and CUMOFFSET Keywords available in the header of the rectified frame.

Parameters

[in]	rec_frame	Input rectified frame to be shifted
[in]	loc_frame	Localization frame used (or not) for shifting
[in]	loc0_frame	Localization of reference frame used (or not) for shifting
[in]	combine_nod_param	Parameters
[in]	rectif_par	rectify parameters
[in]	instrument	Instrument structure
[out]	res_frame_ext	resampled frame in ESO format

Returns: The shifted frame

Definition at line 2108 of file xsh_rectify.c.

References check, instrument, shift_with_kw(), XSH_ASSURE_NOT_NULL, and xsh_msg.

Variable Documentation

◆ err_profile

cpl_vector* err_profile = NULL

static

Definition at line 81 of file xsh_rectify.c.

Referenced by fill_rectified().

◆ rec_profile

cpl_vector* rec_profile = NULL

static

Definition at line 80 of file xsh_rectify.c.

Referenced by fill_rectified(), xsh_efficiency_compute(), xsh_util_efficiency(), and xsh_util_efficiency2d().

Macros

Functions

Variables

Detailed Description

Macro Definition Documentation

◆ new_bp

◆ REGDEBUG_FULL

◆ SLIT_FRAC_STEP

Function Documentation

◆ adjust_lambdas()

◆ compute_shift_with_kw()

◆ compute_shift_with_localization()

◆ fill_rectified()

◆ shift_with_kw()

◆ xsh_compute_slitlet_limits()

◆ xsh_frame_set_shiftifu_ref()

◆ xsh_get_shift_ref()

◆ xsh_get_slit_edges()

◆ xsh_hdrl_remove_crh_single()

◆ xsh_rec_list_rectify()

◆ xsh_rec_slit_size()

◆ xsh_rectify()

◆ xsh_rectify_and_shift()

◆ xsh_rectify_ifu()

◆ xsh_rectify_orders()

◆ xsh_rectify_orders_ifu()

◆ xsh_shift()

◆ xsh_shift_rectified()

Variable Documentation

◆ err_profile

◆ rec_profile