We present data on the extinction distribution in M33, as derived in the article 'Extinction Distributions in Nearby Star-resolved Galaxies. I. M33' by Yuxi Wang, Yi Ren, Jian Gao, Bingqiu Chen, and Y
> 4542s grade 3 time, for which we ask for an upgrade > is to be transferred from rchini.prostata a multiwavelength isophot study is proposed to measure the ir energy distributions of a sample o
We request time to observe 270 pulsars on a regular basis in order to achieve three main science goals. The first is to understand pulsars: how do they spin down and what disrupts this process, how an
