Welcome to the 10C Survey website! ... The first 10C Survey results from an area of 27 sq. degrees complete to 1 mJy and 12 sq. degrees complete to 0.5 mJy have now been released. ... The first results from the survey, which is the deepest extragalactic radio source survey of any significant extent (> 0.2 sq. degrees) above 1.4 GHz, including the deep 15.7-GHz source count are contained in AMI Consortium: Davies et al. ... For each field, deep and shallow areas have been defined. ...

... The following document provides a short instruction on the reduction of synthesis observations with the WSRT using AIPS. ... The aim of the instructions below is to provide a check list of reduction steps to be taken and of the important parameters to be set in each task. ... Please consult the AIPS Cookbook for detailed information about data reduction with AIPS (and various Banana recipes). TASK 'FITLD' . ... GETN n . ... TGET 'INDXR' . ... DOCAL 1 . ... GAINU 2 . ... IMAGRPRM 0 . ...

... boolean . ... integer . ... Quadrant wait states [F1294], defines the length of the Extended Full Frame Mode frame time, typical values are 0, 3, or 5 (will be removed once complete PAH and PMH files in ODF available) . ... HK value of DTIMAUTRSTPREVAL [F1052], (will be removed once complete PAH and PMH files in ODF available) . ... CCD fine temperature [ C]: H_CE_TTMPFPFE [F1128], only active in absence of real PMH files (will be removed once complete PAH and PMH files in ODF available) . ...

Target Acquisition Reference Information . ... In almost all cases where an onboard acquisition will not work (because the object is in a crowded field, or is variable, or is a moving target), it is sufficient to use an early acquisition to get a WFPC2 or FOC image a few weeks in advance of the GHRS observation. ... Explicit BRIGHT and FAINT limits may be specified if you desire, although there is an increased risk of a failed acquisition unless you are confident of those fluxes. ... MAPs . ...

TOOLS OF TEST GENERATION FOR SATELLITES CONTROL PROGRAMS Andrey Tyugashev, Ekaterina Myasnikova, Elena Sopchenko S.P. Korolyov Samara State Aerospace University (National Reseach University) The paper presents a research in the field of test automation for testing spacecraft control programs. ... Programmers or designers of spacecraft systems write tests manually. ... Tests are carried out by issuing the control actions on the spacecraft and condition monitoring systems parameters of the spacecraft. ...

. Next: FSRQs Up: THE DEEP X-RAY RADIO Previous: Redshift Distribution . DXRBS' unique combination of a dual X-ray/radio survey method and high sensitivity has opened up important, large new regions of parameter space for both blazar sub-classes, within which a large fraction of our sample (nearly 50%) lie. This section is devoted to discussing these discoveries and their impact upon our understanding of the blazar class. љ . FSRQs . BL Lacs . Paolo Padovani . 1/5/1998

Next: Calibration Frames and Up: CCD Reductions Previous: General Overview of . ... However, apart from a few cases the keyword setting itself is not modified: principally, keywords can only be changed by the SET/CCD command. ... After (partially) having finished a CCD reduction the user may want to store the current keyword setting. ... The keyword setting can be restored by the command INIT/CCD red_table , where red_table is the reduction table containing the CCD keyword setting, previously saved. ...

... We demonstrate through numerical simulations that model parameters estimated with our technique are essentially bias-free, even when the average number of counts per bin is 1. ... The IW technique avoids such biases by estimating through successive iterations, where for each iteration, j, , and the best-fit parameters are determined by minimization of . ... In our sample, we find that the minimum values and best-fit parameters converge after about 6 iterations. ...