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7 Oct 2000: FIRST -- Faint Images of the Radio Sky at Twenty-cm -- is a project designed to produce the radio equivalent of the Palomar Observatory Sky Survey over 10,000 square degrees of the North Galactic Cap. Using the NRAO Very Large Array (VLA) and an

18 Jan 2000: This new instrument offers unique opportunities for the UK/NL communities to execute high resolution, deep, wide field optical imaging surveys. ... give an indication of when new data will be available for download.

6 Oct 2000: Maximun priority is given to the zone -3º to -9º the same zone observed in San Fernando for the Astrophotographic Catalogue in order to computes proper motions using new measures of ... In 1991 the original declination glass circle was changed for a

8 Jul 2000: Villafranca Station at Villafranca del Castillo, Spain VLA Very Large Array (Radio Telescope in New Mexico) VOB Vertical Optical Branch V&V Validation and Verification WAN Wide Area Network WFC Wide

12 May 2000: INT WFS: Publications and Reports. McMahon, R.G., Walton, N.A., et al, 1999, To appear in "Instrumentation at the ING", Edited by Walton, N, Smartt, S., New Astronomy Reviews" (Elsevier ... Science). The WFS Pipeline Irwin & Lewis To appear in

23 Jan 2000: Select HKEY_LOCAL_MACHINESOFTWARELife Science Resources LtdOEM<>. Double click on OEMcode and set the new value, as described below. ... Most of the functions normally required at the telescope are on a new control panel called INFRARED next to the

13 Jan 2000: of Astronomy, Cambridge Observatory Building Meeting Room Note: The IOA, Hoyle Building is partially a building site while a new Lecture Theatre is completed, so reception is in the Observatory Building.

23 Jan 2000: New Features:. There is no remote/local switch. Sending the 'GO' command now starts a sequence directly. ... The value is returned. Parameters are changed by sending the parameter and new value separated by a space.

23 Jan 2000: Before you install your Software. If you are using a new PC with your system, it is strongly recommended you check your PC system is functioning correctly.

23 Jan 2000: It is automatically incremented on each new saved sequence. The total number of files which will be written is also shown.

23 Jan 2000: Check the 'Override settings for.' to make changes to settings, or check 'Store as.' for the creation of a new setting. ... Sequence mode. To create a new sequence of single or multi image acquisition, select the Sequence tab.

3 Nov 2000: DO THE MOSAIC OFFSET INSTEAD OF PULLING THE NEW POSITION OFFSET FROM THE CATFILE i.e. ... this will open three new windows. =setup "equinox" and let the telescope operator know what you will be using.

23 Jan 2000: File :. New : Select the New file icon to clear the image area to start a new image. ... New file Select the New file icon to clear the image area to start a new image.

23 Jan 2000: The new parameters are in five groups at end of the pixcel.ini file:. ... RUN=0 to n. A run number is inserted into each file written, the number is automatically incremented with each new sequence.

23 Jan 2000: The plot is updated with the pixels from the new image under the line selection. ... The histogram is updated with the data from the new image under the rectangle selection.

23 Jan 2000: The plot is updated with the pixels from the new image under the line selection. ... The histogram view is updated with the pixels from the new image that are contained by the rectangle selection.

26 Feb 2000: The campaign successfully found ten new SN in the required red-shift range. ... Put seeing statistics, new flats, fringe frames etc. on too and more detailed filter responses with correct overall QE.