about
Astropy: A community Python package for astronomyThe MUSE Hubble Ultra Deep Field Survey I. Survey description, data reduction, and source detectionThe MUSE Hubble Ultra Deep Field Survey. II. Spectroscopic redshifts and comparisons to color selections of high-redshift galaxiesThe MUSE Hubble Ultra Deep Field Survey VI. The faint-end of the Lyα luminosity function at 2.91 < z < 6.64 and implications for reionisationThe MUSE Hubble Ultra Deep Field Survey. VIII. Extended Lyman-{alpha} haloes around high-z star-forming galaxiesThe VIPERS Multi-Lambda Survey. I. UV and near-IR observations, multi-colour catalogues, and photometric redshiftsZAP – enhanced PCA sky subtraction for integral field spectroscopy
P50
Q56774843-0FAC0605-0D4A-4B4B-BCE5-CA4EC9CCFF06Q57712673-813F4D2F-EE49-4DEF-B9EC-76256731F8DBQ57712676-508F54D9-0ECB-424C-88AF-63DC1239EAFCQ57712681-42D8788A-736E-4565-A3DD-94A9C71007DBQ57712685-CB7A0748-E0B1-4A52-ADFA-4D774F338E66Q57712693-21E75ADE-F7E7-4357-9CCF-4F7A75711A5BQ57712696-985F7B0E-2133-482F-8CC1-76D6BC2089B0
P50
description
onderzoeker
@nl
researcher
@en
հետազոտող
@hy
name
Simon Conseil
@ast
Simon Conseil
@en
Simon Conseil
@es
Simon Conseil
@nl
type
label
Simon Conseil
@ast
Simon Conseil
@en
Simon Conseil
@es
Simon Conseil
@nl
prefLabel
Simon Conseil
@ast
Simon Conseil
@en
Simon Conseil
@es
Simon Conseil
@nl
P106
P31
P496
0000-0002-3657-4191