FITS file containing galactic reddening information for 450406 Healpix pixels at N_side 256. The data was produced by analyzing the photometry of ~50 million stars from the Pan-STARRS 1 Survey. Please see the related publication for details regarding the analysis and data set (currently under review at ApJ - metadata will be updated with link to publication when available)
Context. The details of how galaxies have evolved over cosmological times are imprinted in their sta...
We present measurements of reddening due to dust using the colors of stars in the Sloan Digital Sky ...
International audienceContext. Three-dimensional maps of the Galactic interstellar medium are genera...
We present a new 3D map of interstellar dust reddening, covering three quarters of the sky (declinat...
International audienceWe present a new 3D map of interstellar dust reddening, covering three quarter...
We present a map of the dust reddening to 4.5 kpc derived from Pan-STARRS1 stellar photometry. The m...
We present a new 3D map of interstellar dust reddening, covering three quarters of the sky (declinat...
We present the attempts to measure dust reddening in the Galactic anti-center region using colors of...
A three-dimensional map of dust reddening, covering the three quarters of the sky surveyed by the Pa...
A three-dimensional map of dust reddening, covering the three quarters of the sky surveyed by the Pa...
We present a method to infer reddenings and distances to stars based only on their broad-band photom...
The mystery of Canis Major overdensity is addressed. We discuss concurrent methods and their limitat...
We present a simple but effective technique for measuring angular variation in R V across the sky. W...
We present measurements of dust reddening using the colors of stars with spectra in the Sloan Digita...
We present a new large-scale, HI-based reddening map that covers 40% of the sky. We publish two dif...
Context. The details of how galaxies have evolved over cosmological times are imprinted in their sta...
We present measurements of reddening due to dust using the colors of stars in the Sloan Digital Sky ...
International audienceContext. Three-dimensional maps of the Galactic interstellar medium are genera...
We present a new 3D map of interstellar dust reddening, covering three quarters of the sky (declinat...
International audienceWe present a new 3D map of interstellar dust reddening, covering three quarter...
We present a map of the dust reddening to 4.5 kpc derived from Pan-STARRS1 stellar photometry. The m...
We present a new 3D map of interstellar dust reddening, covering three quarters of the sky (declinat...
We present the attempts to measure dust reddening in the Galactic anti-center region using colors of...
A three-dimensional map of dust reddening, covering the three quarters of the sky surveyed by the Pa...
A three-dimensional map of dust reddening, covering the three quarters of the sky surveyed by the Pa...
We present a method to infer reddenings and distances to stars based only on their broad-band photom...
The mystery of Canis Major overdensity is addressed. We discuss concurrent methods and their limitat...
We present a simple but effective technique for measuring angular variation in R V across the sky. W...
We present measurements of dust reddening using the colors of stars with spectra in the Sloan Digita...
We present a new large-scale, HI-based reddening map that covers 40% of the sky. We publish two dif...
Context. The details of how galaxies have evolved over cosmological times are imprinted in their sta...
We present measurements of reddening due to dust using the colors of stars in the Sloan Digital Sky ...
International audienceContext. Three-dimensional maps of the Galactic interstellar medium are genera...
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