... limit is agonizingly slow --- especially in the tails, where a small number of large ... from the center of the distribution, so that convergence is very slow in the tails ...
... Also large HI tail is stretching NE from SBS 1129+577 (see paper by Ekta, Chengalur and Pustilnik 2006, MNRAS, 372, 853). ... A strong tidal tail stretching to the south is seen on HI map of SDSS J1105+6022. ...
... имеет вид echo Это расчет $0: sort $2 >> $1 cat $1 а файлы "cock" и "tail" содержат соответственно cock: Это отсортированный файл: tail: 1 3 2 Тогда после вызова команды examp-1 cock tail на экране будет Это расчет examp-1: Это отсортированный файл: 1 2 3 ...
... of Sy galaxies in comparison with the above mentioned surveys (< 2 % here versus 10 % in the UM sample and 8 % in the UCM sample) and pick up only the low-luminosity tail of AGN ( possible LINERs) mainly as interlopers and second priority candidates ...
... The additive spike-like jam makes the "tails" of the distribution "heavier" which leads to different offsets for linear and rank mean estimation on the integrating interval. ...
... The redshift distribution peaks at z = 0.025, but there are about 200 powerful radio galaxies in the extended tail of the distribution which have z greater than 0.2. ...
... Do+CC'' for double sources with a central component or peak giving a well-defined position, ``H'' for a diffuse halo around a central source, and ``HT'' for a complex head-tail morphology. (2) comments in parentheses refer to the optical identification ...