.. _pydl.pydlspec2d: ============================================ SDSS Spectroscopic Data (`pydl.pydlspec2d`) ============================================ Introduction ++++++++++++ This package provides functionality in the SDSS idlspec2d_ package. This package is used for processing and analyzing data from the SDSS optical spectrographs. The code is thus relevant to the `SDSS Legacy`_, BOSS_ and eBOSS_ surveys. This package does *not* work with any infrared spectrograph data associated with the APOGEE-2_ survey. The primary *technical* focus of this particular implementation is the function :func:`~pydl.pydlspec2d.spec2d.combine1fiber`. This function is responsible for resampling 1D spectra onto a new wavelength solution. This allows for: 1. Shifting a spectrum from observed redshift to rest frame. 2. Coaddition of spectra of the same object, after resampling all spectra onto the same wavelength solution. The primary *scientific* motivation of implementing :func:`~pydl.pydlspec2d.spec2d.combine1fiber` is to create template spectra based on curated spectra of, *e.g.*, luminous red galaxies (LRGs). Principal Component Analysis (PCA) or other techniques may be used to construct template spectra, but putting all spectra on the same rest-frame wavelength solution is the first step. The idlspec2d package is itself divided into a number of subpackages. Below we list the subpackages and the usability of the PyDL equivalent. The readiness levels are defined as: Obsolete No point in implementing because the purpose of the code lapsed many years ago. Not Applicable (NA) No point in implementing because another built-in or numpy/scipy/astropy package completely replaces this. None Not (yet) implemented at all. Rudimentary Only a few functions are implemented. Fair Enough functions are implemented to be useful, but some are missing. Good Pretty much anything you could do with the idlspec2d code you can do with the equivalent here. ========== =============== =================================================== Subpackage Readiness Level Comments ========== =============== =================================================== apo2d None Quick extraction code for quality assurance at observation time. config None Extraction pipeline configuration parameters in object-oriented IDL. fluxfix None Flux calibration guider None Interface to guider camera. inspect None Tools for manual inspection of spectra. photoz Obsolete Photometric redshifts for SDSS objects using spectral templates. plan None Tools for planning exposures and recordings summaries of exposures. plate Obsolete Tools for designing SDSS spectroscopic plates, especially for star clusters. science None Code for science analysis of sets of 1D spectra. spec1d Fair Tools for processing 1D spectra, including redshift fitting. spec2d Fair Tools for extracting spectra from 2D images. specdb Obsolete Tests on storing spectroscopic results in SQL databases. specflat None Flat-fielding of spectroscopic 2D images. templates None Tools for constructing spectroscopic templates. testsuite None Tools for high-level quality assurance, *e.g.* comparing two reductions of the same data. ========== =============== =================================================== .. _idlspec2d: https://svn.sdss.org/public/repo/eboss/idlspec2d/trunk/ .. _`SDSS Legacy`: https://classic.sdss.org/legacy/index.html .. _BOSS: https://www.sdss.org/surveys/boss/ .. _eBOSS: https://www.sdss.org/surveys/eboss/ .. _APOGEE-2: https://www.sdss.org/surveys/apogee-2/ API +++ .. automodapi:: pydl.pydlspec2d .. automodapi:: pydl.pydlspec2d.spec1d :skip: warn, solve, Pydlspec2dException, Pydlspec2dUserWarning .. automodapi:: pydl.pydlspec2d.spec2d :skip: warn, erf, get_pkg_data_filename, smooth, iterfit, djs_maskinterp, djs_median, sdss_flagval, traceset2xy, xy2traceset, vactoair