... 1. protection of the astronomical quality of areas suitable for scientific observation of the Universe should be taken into account when developing and evaluating national and international scientific and environmental policies, with due regard to local ...
... total SFR density in the lo cal (z = 0) universe is estimated to be (0.019 ± 0.003)M ... jor techniques for determining the star formation rate (SFR) in the lo cal universe ...
... 1; module_param(howmany, int, 0); static int hello_init(void) { int i; for (i = 0; i Inserting this module with a command like: insmod ./hellop.ko howmany=2 whom=universe causes the message "hello, universe" to show up twice in the system logfile ...
... the proceedings of the conference "A Universe of dwarf galaxies", EAS Publications ... for superpowerful radio galaxies in the early universe at redshift z = 4.514 ...
... P curve is presented in diH'erential form, normalized to the expected dependence of D N on P for a static Euclidean Universe ... Here, D N/N 0 is the ratio of the observed differential source density to that expected for a static Euclidean Universe. ...
... Clark,1997 . Clark Stuart, Towards the edge of the universe. A review of modern cosmology, Wiley, 1997 Physical description xxi, 209 p. Code et al., ...