MUSELET (for MUSE Line Emission Tracker) is a simple SExtractor-based python tool to detect emission lines in a datacube. It has been developed by Johan Richard (firstname.lastname@example.org), with help from Johany Martinez (CRAL) and Laure Piqueras (CRAL).
MUSELET uses SExtractor (Bertin & Arnouts 1996, http://www.astromatic.net/software/sextractor) to detect line emission in narrow-band images created from the cube. It then merges all detections in a single catalog, separating the emission lines linked with continuum sources detected in the white light images from the isolated emission lines. It then tries to estimate the redshift from multiple emission lines.
MUSELET takes as an input a MUSE DATACUBE (fits format), and works in 3 steps:
STEP 1: creation of white light, color and narrow band images.
MUSELET will first create a variance-weighted white light image as well as R,G,B images based on 1/3 of the wavelength range each. The code will then go through the wavelength axis and create one narrow band image at each wavelength plane. The narrow band image is based on a line-weighted (spectrally) average of 5 wavelength planes in the cube (so 5x1.25 Angstroms wide). The continuum is estimated from 2 spectral medians of ~ 25 Angstroms each on the blue and red side of the narrow band region. The size of the continuum region can be adjusted with the optional parameter delta (in number of wavelength planes, default=20).
These narrow band images are created in the
nb/directory. If not present it will be created.
STEP 2: MUSELET will run SExtractor using the
default.nnwparameter files in the current and
nb/directory. If not present default parameter files are created. These files can be used to control SExtractor. Alternatively, it is possible to supply SExtractor command line options via the “sex_config=” and “sex_config_nb” keywords.
STEP 3: The code will merge all SExtractor catalogs and will return separate emission lines linked with continuum objects from the rest. For each of these catalogs, MUSELET will estimate a redshift based on multiple emission lines. Emission lines are merged spatially to the same source based on the “radius” parameter (in pixels, default radius=4). The redshifts are estimated from emission line catalogs
emlines(all emission lines) and
emlines_small(list of brightest emission lines). These files are 2 columns (name and wavelength) and can be adjusted to one’s needs.
- The code will produce:
These are written to the current directory (or the working directory if specified via the “workdir” keyword)
SExtractor (“sex” or “sextractor” binary file in your $PATH).
MUSELET is run through the following commands in MPDAF:
>>> from mpdaf.sdetect import muselet >>> muselet('DATACUBE.fits')
Optionally, one can provide the starting step (2 or 3) in order to only redo one part of the script. For instance, assuming the narrow-band images are already created:
>>> muselet('DATACUBE.fits', step=2)
Optionally, one can provide the size of the continuum region to subtract on each side of the narrow-band images:
>>> # only 15 wavelength planes in continuum estimate >>> muselet('DATACUBE.fits', delta=15)
The output detection catalogs can be opened as a
>>> from mpdaf.sdetect import Catalog >>> cat_lines = Catalog.read('lines.fit') >>> cat_objects = Catalog.read('objects.fit')
and or as a
>>> from mpdaf.sdetect import SourceList >>> sources_lines = SourceList.from_path('lines') >>> sources_objects = SourceList.from_path('objects')
mpdaf.sdetect.Source files can be open:
>>> from mpdaf.sdetect import Source >>> src_line = Source.from_file('lines/lines-0001.fits') >>> src_object = Source.from_file('objects/objects-0001.fits')
Finally it is possible to interact easily in topcat between the muselet catalog and a MUSE datacube opened in ds9. To do so one has to select the “Activation Action” menu and put the following custom code:
>>> exec("topcat_show_ds9",toString(RA),toString(DEC),toString(LBDA_OBS)) for the catalog of lines or >>> exec("topcat_show_ds9",toString(RA),toString(DEC),toString(LBDA_OBS001)) for the catalog of objects
The shell script
topcat_show_ds9 (inspired by Benjamin Clement) is
installed with MPDAF and should be in your path.