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UVES POst PipeLine Echelle Reduction (UVES_popler): For combining multiple echelle spectroscopy exposures into a single spectrum

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.gitignore
.gitignore
 
 
EW.c
EW.c
 
 
Makefile
Makefile
 
 
Makefile.bak
Makefile.bak
 
 
README.md
README.md
 
 
UVES_atmask.c
UVES_atmask.c
 
 
UVES_boxcar.c
UVES_boxcar.c
 
 
UVES_chunk_cont.c
UVES_chunk_cont.c
 
 
UVES_combine_ESPRESSOtrace.c
UVES_combine_ESPRESSOtrace.c
 
 
UVES_combine_cont.c
UVES_combine_cont.c
 
 
UVES_combine_nocont.c
UVES_combine_nocont.c
 
 
UVES_combine_region.c
UVES_combine_region.c
 
 
UVES_combine_spec.c
UVES_combine_spec.c
 
 
UVES_combsynthThAr.c
UVES_combsynthThAr.c
 
 
UVES_confit.c
UVES_confit.c
 
 
UVES_cspec_cont.c
UVES_cspec_cont.c
 
 
UVES_cspec_stats.c
UVES_cspec_stats.c
 
 
UVES_hex2dec.c
UVES_hex2dec.c
 
 
UVES_hirx_blzfit.c
UVES_hirx_blzfit.c
 
 
UVES_init_cspec.c
UVES_init_cspec.c
 
 
UVES_memspec.c
UVES_memspec.c
 
 
UVES_merge_thar.c
UVES_merge_thar.c
 
 
UVES_model_resol.c
UVES_model_resol.c
 
 
UVES_order_cont.c
UVES_order_cont.c
 
 
UVES_order_rejsigedge.c
UVES_order_rejsigedge.c
 
 
UVES_order_sigclip.c
UVES_order_sigclip.c
 
 
UVES_order_stats.c
UVES_order_stats.c
 
 
UVES_params_init.c
UVES_params_init.c
 
 
UVES_params_set.c
UVES_params_set.c
 
 
UVES_past_actions.c
UVES_past_actions.c
 
 
UVES_past_actions_AM.c
UVES_past_actions_AM.c
 
 
UVES_pgenv_init.c
UVES_pgenv_init.c
 
 
UVES_pixscal.c
UVES_pixscal.c
 
 
UVES_plot_cspec.c
UVES_plot_cspec.c
 
 
UVES_plot_cspec.new.c
UVES_plot_cspec.new.c
 
 
UVES_plot_replay.c
UVES_plot_replay.c
 
 
UVES_popler.c
UVES_popler.c
 
 
UVES_popler.h
UVES_popler.h
 
 
UVES_r1Dspec.c
UVES_r1Dspec.c
 
 
UVES_r1Dspec.temp.c
UVES_r1Dspec.temp.c
 
 
UVES_r2Dspec.c
UVES_r2Dspec.c
 
 
UVES_r2Dspec_ESOmer.c
UVES_r2Dspec_ESOmer.c
 
 
UVES_r2Dspec_KODIAQ.c
UVES_r2Dspec_KODIAQ.c
 
 
UVES_r2Dspec_espresso.c
UVES_r2Dspec_espresso.c
 
 
UVES_r2Dspec_harps.c
UVES_r2Dspec_harps.c
 
 
UVES_r2Dspec_hirx.c
UVES_r2Dspec_hirx.c
 
 
UVES_r2Dspec_hirx.pdf
UVES_r2Dspec_hirx.pdf
 
 
UVES_r2Dspec_hirx.tex
UVES_r2Dspec_hirx.tex
 
 
UVES_r2Dspec_iraf.c
UVES_r2Dspec_iraf.c
 
 
UVES_r2Dspec_iresi.c
UVES_r2Dspec_iresi.c
 
 
UVES_r2Dspec_irls.c
UVES_r2Dspec_irls.c
 
 
UVES_r2Dspec_mage.c
UVES_r2Dspec_mage.c
 
 
UVES_r2Dspec_makee.c
UVES_r2Dspec_makee.c
 
 
UVES_r2Dspec_pypeit.c
UVES_r2Dspec_pypeit.c
 
 
UVES_rFITSlist.c
UVES_rFITSlist.c
 
 
UVES_rMacmap.c
UVES_rMacmap.c
 
 
UVES_rUPLfile.c
UVES_rUPLfile.c
 
 
UVES_ratmask.c
UVES_ratmask.c
 
 
UVES_redispers.c
UVES_redispers.c
 
 
UVES_replace_envinstr.c
UVES_replace_envinstr.c
 
 
UVES_replay_control.c
UVES_replay_control.c
 
 
UVES_rescale_region.c
UVES_rescale_region.c
 
 
UVES_revwpol.c
UVES_revwpol.c
 
 
UVES_rinputfile.c
UVES_rinputfile.c
 
 
UVES_rscale.c
UVES_rscale.c
 
 
UVES_rvshift.c
UVES_rvshift.c
 
 
UVES_scale.c
UVES_scale.c
 
 
UVES_select_subspec.c
UVES_select_subspec.c
 
 
UVES_set_wavelen_scale.c
UVES_set_wavelen_scale.c
 
 
UVES_skysub.c
UVES_skysub.c
 
 
UVES_synthThAr.c
UVES_synthThAr.c
 
 
UVES_thar_sigarray.c
UVES_thar_sigarray.c
 
 
UVES_tmpfit.c
UVES_tmpfit.c
 
 
UVES_undo_lastact.c
UVES_undo_lastact.c
 
 
UVES_vhelio.c
UVES_vhelio.c
 
 
UVES_wDATfile.c
UVES_wDATfile.c
 
 
UVES_wFITSfile.c
UVES_wFITSfile.c
 
 
UVES_wUPLfile.c
UVES_wUPLfile.c
 
 
UVES_wpol.c
UVES_wpol.c
 
 
UVES_wrawFITS.c
UVES_wrawFITS.c
 
 
ast_coord.c
ast_coord.c
 
 
ast_date2epoch.c
ast_date2epoch.c
 
 
ast_date2jd.c
ast_date2jd.c
 
 
ast_epoch2jd.c
ast_epoch2jd.c
 
 
ast_jd2date.c
ast_jd2date.c
 
 
ast_jd2epoch.c
ast_jd2epoch.c
 
 
ast_mst.c
ast_mst.c
 
 
ast_precess.c
ast_precess.c
 
 
ast_rotmatrix.c
ast_rotmatrix.c
 
 
ast_vbary.c
ast_vbary.c
 
 
ast_vorbit.c
ast_vorbit.c
 
 
ast_vrotate.c
ast_vrotate.c
 
 
astron.h
astron.h
 
 
brent.c
brent.c
 
 
carray.c
carray.c
 
 
charstr.h
charstr.h
 
 
chebyshev_eval.c
chebyshev_eval.c
 
 
chixy.c
chixy.c
 
 
chixy_fixa.c
chixy_fixa.c
 
 
cmatrix.c
cmatrix.c
 
 

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UVES_popler

UVES POst PipeLine Echelle Reduction (UVES_popler): For combining multiple echelle spectroscopy exposures into a single spectrum. See http://astronomy.swin.edu.au/~mmurphy/UVES_popler.

The main analysis steps and algorithms used in UVES_popler are documented in:
Murphy M.T., Kacprzak G.G., Savorgnan G.A.D., Carswell R.F.,
The UVES Spectral Quasar Absorption Database (SQUAD) data release 1: the first 10 million seconds,
2019, Mon. Not. Roy. Astron. Soc., 482, 3458, arXiv:1810.06136 (NASA ADS: 2019MNRAS.482.3458M).
Please cite this paper when using UVES_popler.

Please also cite this software using the DOI above. For example, "Murphy M. T., 2016, UVES_popler: POst PipeLine Echelle Reduction software. doi:10.5281/zenodo.1297190".

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UVES POst PipeLine Echelle Reduction (UVES_popler): For combining multiple echelle spectroscopy exposures into a single spectrum

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