Lab . Main page News People . ASA . Master . Master net Homepage . ... Lomonosov Moscow State University Sternberg Astronomical Institute . ... MASTER . ... Lomonosov (ShOK) . ... About Space Monitoring Laboratory, scientific directions, instruments, contacts . People, who work in lab . Latest news and news archive . ... All news ...

The UV throughput of the WFPC2 degrades in a predictable way after each monthly decontamination. ... Figure 6.11 shows the photometric monitoring data for the standard star GRW+70D5824 (a white dwarf classified DA3; B-V = -0.09) in the WF3 and PC1 for the set of filters which are routinely monitored. ... Filter . ... 0.007 . ... Figure 6.12 and Figure 6.13 show the throughput decline in all four chips as a function of days since the last decontamination for the F170W filter. ... Time. ...

... Team . ... GRB mini-workshop 2006 . ... 6-meter telescope BTA: . The monitoring of gamma-ray burst afterglows and the study of their host galaxies . Monitoring of core-collapse supernovae and investigation of their host galaxies . ... Supernovae and gamma-ray bursts . ... Are some GRB host galaxies lying in galaxy clusters? ... Supernovae and gamma-ray bursts (Within the scope of the international program "Astronomy in Prielbrusiye") . ... The physics of gamma-ray bursts in the SWIFT era . ...

. Search for a cluster by name: . Otherwise, search within a radius: . RA: . Dec: . Radius (arcmin): . Download the catalogue of AMI results (FITS format)

... RADIATION AND ECOLOGICAL MONITORING . ... S.P.Korolev RSC Energia has designed and built the experimental model of automatic radiation and ecological station (ARES). ... Inspection control, including delivery of ARES to areas with high risk of ecological pollution and conduction of long-term (weeks, months) continuous observations in automatic mode; . ... Satellite data relay system. ... The control of automatic ecological control stations via satellite channel was developed in 1996-1997. ...

... We thank the Swift team for their rapid scheduling of this observation. ... 2455705.20851 V 14.15 0.03 2455707.83079 V 14.10 0.03 2455710.84028 V 13.53 0.02 2455713.64631 V 13.66 0.02 2455714.65479 V 14.11 0.03 2455714.71823 V 14.12 0.02 2455714.78596 V 14.20 0.02 2455717.39593 V 14.37 0.03 2455726.62861 V 14.83 0.04 2455727.16343 V 14.57 0.04 2455730.50586 V 14.57 0.03 2455730.57329 V 14.56 0.03 2455730.70360 V 14.66 0.04 2455738.32865 V 14.00 0.02 2455742.86146 V 14.21 ...

Astronomy Discussion Forums . Forums: . ... Discussion Forums . ... Follow Up . Forum List | Follow Ups | Post Message | ... Login to Post . ... www.astronomy.net . About Astronomy Net | Advertise on Astronomy Net | ... Unless otherwise specified, web site content Copyright 1994-2016 John Huggins All Rights Reserved . Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

... ATNF Home . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Australian Square Kilometre Array Pathfinder . Murchison Radio-astronomy Observatory . ... Parkes radio telescope . Australia Telescope Compact Array . ... Parkes | ... Visiting Parkes radio telescope . Visiting Australia Telescope Compact Array . ... Parkes radio telescope webcam . ... The follow up 21cm synthesis observations on the galaxies found by this survey are essential for a number of reasons. ...

... We present several applications of the AIPS++ environment as applied to the development of the Green Bank Telescope as well as current astrophysical problems. ... In particular, the Green Bank Telescope (GBT) project requires AIPS++ as an analysis environment. To accommodate and facilitate the GBT development, several sets of tools have been fashioned within AIPS++ at several points along the data path, from general calibration routines and data quality assessment to analysis and modeling. ...

... SMIS : Space Monitoring Information Support laboratory . Russia's Weather : State Meteorological Center Weather Forecast . Space Weather service : ACE real time solar wind data and simple geomagnetic activity forecast. ... World Fire Web : Space Research Institute (IKI) node . Sputnik : Joint project of SRC Planeta, Rosgidromet and Space Research Institute (IKI) . ... Today's Space Weather : Presented by the Space Environment Center . ... Back to the Space Research Institute Home Page ...

NEUTRON MONITOR DATA FOR JUNGFRAUJOCH AND BERN DURING THE GROUND-LEVEL SOLAR COSMIC -RAY EVENT ON 29 October 2003 R. Buetikofer and E.O. Flueckiger Physikalisches Institut, Universitaet Bern Sidlerstrasse 5, CH-3012 Bern , Switzerland This report includes information on the processing and use of the data for the ground-level solar cosmic ray event on 29 October 2003 obtained by the following three ... Section 3 of the IGY neutron monitor at Jungfraujoch is the central section. ...

... ESO Science Newsletter April 2016 . ... Follow the links or visit ESO Science Announcements to read more. ... Read more . ... The ALMA Director, on behalf of the Joint ALMA Observatory (JAO) and the partner organizations in East Asia, Europe, and North America, is pleased to announce the ALMA Cycle 4 Call for Proposals (CfP) for scientific observations to be scheduled from October 2016 to September 2017. ... Upcoming ESO or ESO-Related Workshops . ... Joint ESO, ALMA, NAOJ, NRAO Workshop. ...

Follow-up astrometry and recoveries are made with the ANU 40 inch (1.0-m) f/8 reflector at Siding Spring Observatory (IAU code 413). ... A routine follow-up of 2003 WY153 on 2003 Dec 15 became much more than routine when a faint object with unusual motion vector was found close to the target asteroid. ... During routine astrometry with the 1.0-m to improve the orbit of the Apollo asteroid 2004 CB, the asteroid was found on March 30 to have a short tail! ... Siding Spring Survey Main Page . ...

Next: Direct Monitoring of T Tauri Stars Previous: X--ray Activity and PMS Stars . Pointed EINSTEIN observations of TTs in the Taurus--Auriga star forming region (SFR) detected five serendipitous sources in the field (Feigelson & Kriss 1981 and Walter & Kuhi 1981). ... Walter (1986) called these objects naked T Tauri stars (nTTs; Walter 1986, Walter et al . ... The catalog of Herbig & Bell (1988) distinguished between cTTs and weak--lined T Tauri stars (wTTs) instead of nTTs. ...

pos_mon includes two simple gui systems which allow monitoring of the leapfrog obseving progress: the cunningly named beamtrack_plot and beampos_plot. ... If you are using the AGES account, simply type pos_mon at the command prompt . If you are not using the AGES account, start IDL (type idl at the command prompt) then enter the following commands: . ... The 'Filter' window can be modified to reflect and subselect the files containing the data for plotting. ... Don't write moronically big files. ...

... Data Analysis SAS News What is SAS? How to use SAS SAS Workshops SAS Version Changes Download and Install SAS Science Simulator (SciSim) . ... Is this going to be your first download of the SAS? ... Which version of the SAS do you intend to download? SAS version? RedHat 9 RedHat Enterprise Linux 4 RedHat Enterprise Linux 3 Fedora Core 3 SuSE 8.2 SuSE 7.3 Solaris 9 Solaris 8 Mac OS X 10.4 Mac OS X 10.2 VMWare for Windows . ... How many SAS users are going to be served through your download? ...

... The J, H and K bands are characterized by a bright background, such a background is mainly due to the emission of atmospheric lines and of thermal radiation. ... If the source cover a large fraction of the slit, spectra off-source must be observed to adequately sample the sky background. ... The on chip integration time (time spent in each position of the slit) must not exceed 40 seconds in J and H bands and 60 seconds in K band. ... We suggest a sequence of 10 for each elementary integration time. ...

Notes concerning the observations made by UKIRT for the YY Gem programme in March 1988. ... As spot modulation effects are relatively more prominent in V and flare effects in B, it was decided to monitor in K and V during eclipses and in K and B at out of eclipse phases. ... The data were corrected for extinction using the following extinction coefficients: B 0.27, V 0.10, K 0.07, J 0.10 . ... The following colour equations were derived for the UKIRT optical data using VISPHOT. ...

Next: MIDAS And the Up: Monitor and Command Previous: Monitor and Command . ... the MIDAS working directory for internal files and (optionally) private procedures: . ... On a Unix system use the option -m < mid_work > to change the default working directory, and -p or -P to run MIDAS in parallel mode љ when you start MIDAS via the command inmidas (see below). ... In NOPARALLEL mode all intermediate MIDAS files in the MIDAS startup directory are deleted when starting MIDAS via inmidas. ...

... The Science Operation Department is composed of Astronomers, Telescope Instruments Operators(TIOs) and Data Handling Administrators(DHAs). ... Astronomers have proposed several methods to quantitatively measure the amount of turbulence above the telescope, which the most common ones is Differential Image Motion Monitor (DIMM). In optical testing, the Hartmann test is the common method to test the quality of optical components. ... Hartmann mask consists of 48 lenses. ...