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X-shooter Pipeline Reference Manual 3.8.15
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#include <gsl/gsl_spline.h>#include <gsl/gsl_errno.h>#include <gsl/gsl_bspline.h>#include <gsl/gsl_multifit.h>#include <gsl/gsl_rng.h>#include <gsl/gsl_randist.h>#include <gsl/gsl_statistics.h>#include <xsh_dfs.h>#include <xsh_error.h>#include <xsh_msg.h>#include <cpl.h>#include <string.h>#include <time.h>#include <xsh_utils_table.h>#include <xsh_data_star_flux.h>#include <xsh_data_atmos_ext.h>#include <xsh_data_spectrum.h>#include <xsh_pfits.h>#include <xsh_utils.h>#include <xsh_utils_wrappers.h>#include <xsh_drl.h>#include <xsh_utils_efficiency.h>#include <xsh_efficiency_response.h>#include <xsh_utils_response.h>#include <xsh_utils_vector.h>Go to the source code of this file.
Macros | |
| #define | INTERPOL_WSTEP_NM 2 |
| #define | FILTER_MEDIAN_HSIZE 3 |
Functions | |
| static int | find_lambda_idx (double lambda, double *wave, int from, int to, double step) |
| static void | find_lambda_idx_limit (double min, double max, double *spectrum, int from, int to, double step, int *if0, int *if1) |
| static cpl_error_code | xsh_interpolate_atm_ext (xsh_star_flux_list *star_list, cpl_table *atmos_ext_tab, xsh_instrument *instrument, double **atmos_lambda, double **atmos_K) |
| static cpl_error_code | xsh_interpolate_high_abs_regions (xsh_star_flux_list *star_list, xsh_star_flux_list *resp_list, HIGH_ABS_REGION *phigh) |
| static cpl_error_code | xsh_response_crea_ascii (xsh_star_flux_list *resp_list, xsh_star_flux_list *star_list, double *lambda_spectrum, double *flux_spectrum, double *flux_added) |
| static cpl_error_code | xsh_flux_integrate_and_corr_for_badpix (int npix_in_interval, double *flux_spectrum, int *qual_spectrum, int if0, int if1, int i, double **flux_added, int *npixels, int *nbad) |
| static cpl_error_code | xsh_spectrum_correct (xsh_star_flux_list *star_list, xsh_spectrum *spectrum, double *atmos_K, XSH_ARM the_arm, double airmass, double exptime, double gain, xsh_star_flux_list **obj_list) |
| static xsh_star_flux_list * | xsh_response_calculate (xsh_star_flux_list *star_list, xsh_star_flux_list **obj_list, xsh_spectrum *spectrum, cpl_table *atmos_ext_tab, XSH_ARM the_arm, double *atmos_K, double airmass, double exptime, double gain) |
| static xsh_star_flux_list * | do_compute (xsh_star_flux_list *star_list, xsh_star_flux_list **obj_list, xsh_spectrum *spectrum, cpl_table *atmos_ext_tab, HIGH_ABS_REGION *phigh, double airmass, double exptime, double gain, xsh_instrument *instrument) |
| cpl_error_code | xsh_response_merge_obj_std_info (cpl_frame *result, xsh_star_flux_list *star_list, xsh_star_flux_list *obj_list) |
| static xsh_star_flux_list * | xsh_obs_std_correct (cpl_frame *obs_std_star, xsh_star_flux_list *ref_std_star_list, cpl_frame *atmos_ext, HIGH_ABS_REGION *phigh, xsh_instrument *instrument) |
| static cpl_error_code | xsh_std_star_spectra_to_vector_range (xsh_star_flux_list *obs_std_star_list, const double wmin, const double wmax, cpl_vector **vec_wave, cpl_vector **vec_flux) |
| cpl_error_code | xsh_sort_double_pairs (double *u1, double *u2, cpl_size n) |
| Sort an array u1 of doubles, and permute an array u2 in the same way as u1 is permuted. | |
| static cpl_error_code | xsh_select_line_core (cpl_vector *wave, cpl_vector *flux, const double wguess, const double wrange, cpl_vector **xfit, cpl_vector **yfit) |
| static double | xsh_std_star_spectra_correlate (xsh_star_flux_list *obs_std_star_list, xsh_star_flux_list *ref_std_star_list, xsh_rv_ref_wave_param *w) |
| static xsh_star_flux_list * | xsh_bspline_fit_interpol (xsh_star_flux_list *ref_std_star_list, cpl_table *resp_fit_points, HIGH_ABS_REGION *phigh, xsh_instrument *inst) |
| static xsh_star_flux_list * | xsh_bspline_fit_smooth (xsh_star_flux_list *ref_std_star_list, HIGH_ABS_REGION *phigh, xsh_instrument *inst) |
| double * | xsh_bspline_interpolate_data_at_pos (double *w_data, double *f_data, const int n_data, double *w_pos, const int n_pos) |
| double * | xsh_bspline_fit_smooth_data (double *wave, double *flux, const int size, HIGH_ABS_REGION *phigh, xsh_instrument *inst, const int fit_region) |
| double * | xsh_bspline_fit_smooth_data2 (double *wave, double *flux, const int size, HIGH_ABS_REGION *phigh, xsh_instrument *inst, const int fit_region) |
| 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 *resp_fit_points, cpl_frame *tell_mod_cat, xsh_instrument *instrument, double exptime, const int tell_corr) |
| 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) |
| 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) |
| #define FILTER_MEDIAN_HSIZE 3 |
Definition at line 81 of file xsh_compute_response.c.
| #define INTERPOL_WSTEP_NM 2 |
Definition at line 80 of file xsh_compute_response.c.
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Integrate the flux on the same sampling that the star_list, taking into account the bad pixels, apply atmos correction, and divide by the star_list table.
| star_list | Table of ref star flux |
| star_list | Table of obs obj flux |
| spectrum | 1./CPL/DOC/cpl_um_2.0.1.psD merged spectrum of standard star |
| atmos_ext_table | Atmos Extinction table |
| airmass | observed object airmass mean |
| exptime | Exposure time |
| gain | detector's gain |
| instrument | instrument arm and lamp setting |
Definition at line 1280 of file xsh_compute_response.c.
References check, exptime, instrument, xsh_star_flux_list::lambda, HIGH_ABS_REGION::lambda_max, HIGH_ABS_REGION::lambda_min, xsh_star_flux_list::size, XSH_ASSURE_NOT_NULL, XSH_FREE, xsh_instrument_get_arm(), xsh_interpolate_atm_ext(), xsh_interpolate_high_abs_regions(), xsh_msg_dbg_low, xsh_msg_dbg_medium, and xsh_response_calculate().
Referenced by xsh_compute_response(), and xsh_compute_response_ord().
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Definition at line 96 of file xsh_compute_response.c.
References step.
Referenced by xsh_interpolate_high_abs_regions().
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Definition at line 197 of file xsh_compute_response.c.
References max, step, xsh_msg_dbg_high, and xsh_msg_dbg_low.
Referenced by xsh_response_calculate().
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Definition at line 2244 of file xsh_compute_response.c.
References check, xsh_star_flux_list::flux, xsh_star_flux_list::lambda, HIGH_ABS_REGION::lambda_max, HIGH_ABS_REGION::lambda_min, xsh_star_flux_list::size, XSH_ARM_NIR, XSH_ARM_UVB, XSH_ARM_VIS, xsh_bspline_interpolate_data_at_pos(), XSH_CALLOC, XSH_FREE, xsh_free_table(), xsh_instrument_get_arm(), xsh_msg, xsh_star_flux_list_duplicate(), xsh_star_flux_list_get_flux(), and xsh_star_flux_list_get_lambda().
Referenced by xsh_compute_response2().
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Definition at line 2488 of file xsh_compute_response.c.
References xsh_star_flux_list::flux, xsh_star_flux_list::lambda, HIGH_ABS_REGION::lambda_max, HIGH_ABS_REGION::lambda_min, n, order, sigma, xsh_star_flux_list::size, x, XSH_ARM_NIR, XSH_ARM_UVB, XSH_ARM_VIS, xsh_free_table(), xsh_instrument_get_arm(), xsh_msg, xsh_star_flux_list_create(), and y.
Referenced by xsh_compute_response2().
| double * xsh_bspline_fit_smooth_data | ( | double * | wave, |
| double * | flux, | ||
| const int | size, | ||
| HIGH_ABS_REGION * | phigh, | ||
| xsh_instrument * | inst, | ||
| const int | fit_region | ||
| ) |
Definition at line 2715 of file xsh_compute_response.c.
References HIGH_ABS_REGION::lambda_max, HIGH_ABS_REGION::lambda_min, n, order, sigma, size, x, XSH_ARM_NIR, XSH_ARM_UVB, XSH_ARM_VIS, xsh_free_table(), xsh_instrument_get_arm(), xsh_msg, and y.
| double * xsh_bspline_fit_smooth_data2 | ( | double * | wave, |
| double * | flux, | ||
| const int | size, | ||
| HIGH_ABS_REGION * | phigh, | ||
| xsh_instrument * | inst, | ||
| const int | fit_region | ||
| ) |
Definition at line 2911 of file xsh_compute_response.c.
References n, order, sigma, size, x, XSH_ARM_NIR, XSH_ARM_UVB, XSH_ARM_VIS, xsh_free_table(), xsh_instrument_get_arm(), xsh_msg, and y.
| double * xsh_bspline_interpolate_data_at_pos | ( | double * | w_data, |
| double * | f_data, | ||
| const int | n_data, | ||
| double * | w_pos, | ||
| const int | n_pos | ||
| ) |
Definition at line 2664 of file xsh_compute_response.c.
References xsh_msg.
Referenced by xsh_bspline_fit_interpol(), xsh_fit_spline1(), xsh_fit_spline2(), and xsh_telluric_model_eval().
| 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 3523 of file xsh_compute_response.c.
References check, check_msg, do_compute(), exptime, instrument, 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 main(), and 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 * | resp_fit_points, | ||
| 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 3145 of file xsh_compute_response.c.
References check, xsh_star_flux_list::flux, instrument, 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_UVB, XSH_ASSURE_NOT_NULL, xsh_bspline_fit_interpol(), xsh_bspline_fit_smooth(), xsh_fill_high_abs_regions(), xsh_frame_product(), xsh_frame_sci_get_ra_dec_airmass(), xsh_frame_spectrum_save(), xsh_free_frame(), xsh_free_propertylist(), xsh_free_table(), xsh_get_basename(), 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_free(), 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_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 3709 of file xsh_compute_response.c.
References check, check_msg, do_compute(), exptime, instrument, 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().
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Definition at line 595 of file xsh_compute_response.c.
References QFLAG_GOOD_PIXEL, and XSH_ASSURE_NOT_NULL_MSG.
Referenced by xsh_response_calculate().
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Interpolate atms extinction at same sampling step as ref std star
| star_list | Table of ref star flux | |
| [in] | atmos_ext_tab | atmospheric extinction table |
| [in] | instrument | instrument arm and lamp setting |
| [out] | atmos_lambda | interpolated wave array |
| [out] | atmos_K | interpolated atmospheric extinction K |
Definition at line 237 of file xsh_compute_response.c.
References instrument, xsh_star_flux_list::lambda, xsh_star_flux_list::size, XSH_ARM_NIR, XSH_ASSURE_NOT_NULL_MSG, XSH_ATMOS_EXT_LIST_COLNAME_K, XSH_ATMOS_EXT_LIST_COLNAME_OLD, XSH_CALLOC, xsh_data_interpolate(), xsh_instrument_get_arm(), and xsh_msg_warning.
Referenced by do_compute(), and xsh_obs_std_correct().
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Interpolate high absorbtion regions
| [in] | star_list | Table of ref star flux |
| [out] | resp_list | Table of response values |
| [in] | HIGH_ABS_REGION | pointer to hight abs regions |
Definition at line 308 of file xsh_compute_response.c.
References find_lambda_idx(), xsh_star_flux_list::flux, xsh_star_flux_list::lambda, HIGH_ABS_REGION::lambda_max, HIGH_ABS_REGION::lambda_min, xsh_star_flux_list::size, XSH_ASSURE_NOT_NULL_MSG, xsh_msg, xsh_msg_dbg_low, xsh_msg_dbg_medium, and xsh_msg_debug.
Referenced by do_compute().
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Corrects the observed spectrum by gain, exptime, spectral bin size, atmospheric extinction, airmass. at the same wavelengths as the ones at which it is sampled the ref std star
| obs_std_star | Rectified frame (1D spectrum) |
| ref_std_star_list | Ref std star structure |
| atmos_ext | Atmospheric Extinction Frame |
| phigh | pointer to high abs region structure |
| instrument | Instrument structure |
< 1d spectrum
Definition at line 1423 of file xsh_compute_response.c.
References check, check_msg, exptime, instrument, XSH_ARM_NIR, XSH_ATMOS_EXT, xsh_atmos_ext_list_free(), xsh_atmos_ext_list_load(), xsh_frame_sci_get_ra_dec_airmass(), XSH_FREE, xsh_free_propertylist(), xsh_free_table(), xsh_instrument_arm_tostring(), xsh_instrument_get_arm(), xsh_interpolate_atm_ext(), xsh_msg_warning, xsh_pfits_get_airm_mean(), xsh_pfits_get_exptime(), xsh_pfits_get_gain(), xsh_spectrum_correct(), xsh_spectrum_free(), and xsh_spectrum_load().
Referenced by xsh_compute_response2().
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Definition at line 843 of file xsh_compute_response.c.
References binx, biny, check, exptime, FILTER_MEDIAN_HSIZE, find_lambda_idx_limit(), xsh_star_flux_list::flux, xsh_star_flux_list::lambda, max, xsh_star_flux_list::size, xsh_add_temporary_file(), XSH_ARM_NIR, XSH_CALLOC, xsh_debug_level_get(), XSH_DEBUG_LEVEL_LOW, xsh_flux_integrate_and_corr_for_badpix(), XSH_FREE, xsh_free_frame(), xsh_free_table(), xsh_msg_dbg_low, xsh_msg_dbg_medium, xsh_response_crea_ascii(), xsh_spectrum_get_flux(), xsh_spectrum_get_lambda_max(), xsh_spectrum_get_lambda_min(), xsh_spectrum_get_lambda_step(), xsh_spectrum_get_qual(), xsh_spectrum_get_size(), xsh_star_flux_list_create(), xsh_star_flux_list_filter_median(), and xsh_star_flux_list_save().
Referenced by do_compute().
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Integrate the flux on the same sampling that the star_list, taking into account the bad pixels, apply atmos correction, and divide by the star_list table.
| resp_list | Table of response values |
| star_list | Table of ref star flux |
| lambda_spectrum | array with lambda values |
| flux_spectrum | array with flux values |
| flux_added | array with integrated flux values |
Definition at line 543 of file xsh_compute_response.c.
References xsh_star_flux_list::flux, xsh_star_flux_list::lambda, xsh_star_flux_list::size, and XSH_ASSURE_NOT_NULL_MSG.
Referenced by xsh_response_calculate().
| cpl_error_code xsh_response_merge_obj_std_info | ( | cpl_frame * | result, |
| xsh_star_flux_list * | star_list, | ||
| xsh_star_flux_list * | obj_list | ||
| ) |
Definition at line 1362 of file xsh_compute_response.c.
References check, xsh_star_flux_list::flux, xsh_free_propertylist(), and xsh_free_table().
Referenced by xsh_compute_response(), and xsh_compute_response2().
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Definition at line 1674 of file xsh_compute_response.c.
Referenced by xsh_std_star_spectra_correlate().
| cpl_error_code xsh_sort_double_pairs | ( | double * | u1, |
| double * | u2, | ||
| cpl_size | n | ||
| ) |
Sort an array u1 of doubles, and permute an array u2 in the same way as u1 is permuted.
| [in,out] | u1 | Pointer to the first array. |
| [in,out] | u2 | Pointer to the second array. |
| n | The common length of both arrays. |
CPL_ERROR_NONE or the appropriate error code. Definition at line 1644 of file xsh_compute_response.c.
References n.
Referenced by xsh_std_star_spectra_correlate().
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This function corrects a spectrum for contributes due to atmospheric extinction, airmass,exptime,gain
| star_list | Table of ref star flux |
| spectrum | Table of observed star flux |
| atmos_K | atmospheric extinction curve |
| the_arm | observing arm |
| airmass | airmass value |
| exptime | exptime (dit*ndit) value |
| gain | gain value |
| obj_list | Table of observed star flux corrected by atmospheric extinction, airmass,exptime,gain |
Definition at line 659 of file xsh_compute_response.c.
References binx, biny, check, exptime, xsh_star_flux_list::flux, xsh_spectrum::flux_header, xsh_star_flux_list::lambda, xsh_star_flux_list::size, size, xsh_add_temporary_file(), XSH_ARM_NIR, XSH_CALLOC, XSH_FREE, xsh_free_frame(), xsh_free_table(), xsh_msg, xsh_msg_dbg_low, xsh_pfits_get_binx(), xsh_pfits_get_biny(), xsh_spectrum_get_flux(), xsh_spectrum_get_lambda_max(), xsh_spectrum_get_lambda_min(), xsh_spectrum_get_lambda_step(), xsh_spectrum_get_size(), xsh_star_flux_list_create(), and xsh_star_flux_list_save().
Referenced by xsh_obs_std_correct().
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Definition at line 1743 of file xsh_compute_response.c.
References check, xsh_star_flux_list::header, xsh_rv_ref_wave_param::ipol_hbox, xsh_rv_ref_wave_param::ipol_wmax_min, xsh_rv_ref_wave_param::ipol_wmin_max, xsh_rv_ref_wave_param::range_wmax, xsh_rv_ref_wave_param::range_wmin, xsh_rv_ref_wave_param::wguess, xsh_free_polynomial(), xsh_free_vector(), xsh_msg, xsh_pfits_get_cdelt1(), xsh_pfits_get_crval1(), xsh_pfits_get_naxis1(), xsh_polynomial_fit_1d_create(), xsh_select_line_core(), xsh_sort_double_pairs(), xsh_std_star_spectra_to_vector_range(), and xsh_vector_fit_slope().
Referenced by xsh_compute_response2().
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Definition at line 1594 of file xsh_compute_response.c.
References xsh_star_flux_list::flux, xsh_star_flux_list::lambda, xsh_star_flux_list::size, and size.
Referenced by xsh_std_star_spectra_correlate().