WebFirst, load the dust map (do this only once): >>> import sfdmap >>> dustmap = sfdmap.SFDMap("/path/to/dust/maps") Now, for each SN you wish to fit, get the amount of dust at the SN location and set the mwebv model parameter appropriately. For example, if the SN is located at RA=42.8 degrees, Dec=0 degrees: WebThe map has a spatial angular resolution, depending on latitude, between 3 and 9 arcmin and covers the entire Xuyi Schmidt Telescope Photometric Survey of the Galactic Anticentre (XSTPS-GAC) survey area of over 6000 deg 2 for Galactic longitude 140 < l < 240 deg and latitude -60 < b < 40 deg.
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WebOct 31, 2016 · A minimal, fast, MIT-licensed Python module for getting E (B-V) values from Schlegel, Finkbeiner & Davis (1998) dust map FITS files. >>> import sfdmap >>> m = sfdmap.SFDMap () >>> m.ebv ( 100 ., 40 .) # Get E (B-V) value at RA=100 degrees, Dec=40 degrees 0.10739716819557897 Install Requirements: numpy and a FITS reader (either … WebThis service gives the Galactic dust reddening for a line of sight, returning a reddening map, the corresponding 100 micron intensity, and dust temperature, along with statistics for … ctb-o
dustmaps documentation — dustmaps v1.0.4 documentation
WebDec 13, 2024 · Our method produces not only a map of the 3D distribution of dust reddening, but also a catalog of distances, reddenings, and types for 799 million stars. Our 3D dust map may be accessed at doi: 10.7910/DVN/2EJ9TX, while our catalog of stellar parameters may be accessed at doi: 10.7910/DVN/AV9GXO. Webv1.1 Gas and Dust Python Calculator For more information about how to use this package see README Latest version published 3 years ago License: BSD-3-Clause-Clear PyPI GitHub Copy Ensure you're using the healthiest python packages Snyk scans all the packages in your projects for vulnerabilities and http://argonaut.skymaps.info/usage ears csbg