... ATNF Home . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Murchison Radio-astronomy Observatory . ... Parkes radio telescope . ... Mopra radio telescope . ... Visiting Parkes radio telescope . ... Parkes radio telescope webcam . ... For example, modified Newtonian dynamics (MOND) has no relativistic extension, and so makes no firm lensing predictions, but galaxy-galaxy lensing data can be used to empirically constrain the deflection law of a MONDian point-mass. ...

... S.P. KOROLEV ROCKET AND SPACE CORPORATION ENERGIA . ... OAO RSC "Energia" . ... ISS Russian Segment . Steps of ISS Assembly . ... Five new devices of the total mass of ~42 kg (instead of 6 devices of the total mass of ~101 kg) are installed in the guidance, navigation and control system of the new series vehicle. ... liquid thermostatting of GN OC devices is provided by installation of three cold plates in the vehicle instrument module (IM); . ... 2015 JSC "S.P. Korolev RSC "Energia" . ...

... Basically, though 34 these additional modifications were initialized by study CP stellar spectra, they have quite general applications. ffl chemical elements up to Z = 82 + ffl vertical stratification of stellar atmosphere ­ chemical elements + ffl iterative abundance process + ffl horizontal stratification + ffl partition function option (Mn and Ga species) + There is no reason for the cutoff of chemical species at Z=82. ... Figure 2 illustrates vertical stratification of helium. ...

... Adds a new column for the former correction. ... Version 1.7: 26 March 1999 removed accuracyLevel=LOW Version 1.6: 10 Dec 1998 Changed dependancies for mssllib-2.0 Version 1.5: 24 August 1998 Frametime computation included - uses frametime_mod from mssllib extra parameter win_ file added necessary for frametime computation SPR 420 closed : now uses errstr Version 1.4: 16th June 1998 CAL routines commented out due to cal errors ( spr submitted) ...

Next: The Quasi--Newton Method. Up: Outline of the Previous: The Newton--Raphson Method. ... At each iteration, one computes . ... Neglecting the second derivatives matrix , we obtain the ``normal equations'' and the Gauss--Newton direction . This so--called Gauss--Newton method is intended for problems where is small. ... The algorithm implemented here is a modification of that Gauss--Newton method, that allows convergence even for rank deficient Jacobians or for large residuals. ...

This service contributes to the International Service of Geomagnetic Indices (ISGI) of the IAGA . ... The Kp numbers of the previous month are available in tabular format . ... There are available also historical and current Kp and derived indices per anonoymos FTP (see below). ... U.S.A. FTP server: ftp://ftp.ngdc.noaa.gov/STP/GEOMAGNETIC_DATA/INDICES/KP_AP/ . monthly update) . ... contains the monthly Kp / ap tables in a simple text format readable for both humans and computers (*.tab). ...

... Disk space . Access to SOGS through the firewall . ... The HST planning and scheduling computing environment primarily consists of the Unix "SOGS" cluster, which includes about 30 Sun machines and about 10 MacOSX machines. ... It has 659 Gb of disk space and uses RAID 5. ... The operational Assist and PMDB databases live on the server HAL9000 which is a Fire 480R. (Since Assist and PMDB are on the same server, cross-database queries are possible and this simplifies operations.) ... Fire V210 . ...

ImageJ with our modifications and tools for astronomy . Download ImageJ for your own computer . ... ImageJ API for developers . G ttingen ImageJ astronomical resources . University of Manitoba ImageJ plugins for observational astronomy . ImageJ is an open source Java-based image processing program developed at the National Institute of Health for medical imaging. We offer a modified version with macros and plugins for astronomical use. Last update: December 7, 2014 . ...

... 18sep08: bias for 3a/3b changed. Look at p2030 data (polA,polB summed) . 21sep08: bias for all beams changed. ... The wapps in 3 level mode take 100 MHz bw with 64usec sampling and 256 lags. alfa is centred at 1440 Mhz with the 100 Mhz 1390-1490 filter int. The total power was computed and then averaged to .1 seconds. ... Beam 6b is dead and p2030 is adding polA + polB. ... The a2010 data taken on 21sep08 was analyzed to check the stability of all the beams after the bias changes in alfa. ...