Winer Observatory P.O. Box 797, Sonoita, Arizona 85637-0797, USA . ... The building is about 106 ft. long by 26 ft. wide and is divided into two parts: a shop area to the north, 54 ft. long by 26 ft. wide with parapet walls containing the control room, and the observatory area 52 ft. long by 26 ft. wide. ... Shop Wall Counterforts . ... The shop roof is suspended between parapet walls, that is, the walls are higher than the roof, to permit the observatory roof to roll unimpeded over the shop roof. ...

Еще в разделе: (Показать все результаты (>4) - www.winer.org/ )

• Winer Observatory Site

... Home Articles Amateur Telescope Making . ... Beyond New York City . ... Observing Resources for Amateur Astronomers - Part 1: Beginning Observers . ... A History of the First Forty Years of the Amateur Astronomers Association . ... The project of making a 17-1/2 inch telescope was made possible only with the help of many other people, most of whom are part of the?а Amateur Astronomers Association . ... 2016 Amateur Astronomers Association of New York Designed by Press Customizr Powered by . ...

Еще в разделе: (Показать все результаты (>40) - www.aaa.org/ )

• Observing Resources for Amateur Astronomers ? Part 4: Magazines and Miscellany
• Observer Reports Archive ? Amateur Astronomers Association of New York
• An Asymmetrical Mount For a 17.5? Newtonian ? Amateur Astronomers Association

... We have imaged with milliarcsecond resolution at 5 GHz 374 strong flat-spectrum radio sources north of declination -44 using the VLBA in June 1996. ... The data were processed with the NRAO AIPS software package and the Caltech Difmap package. ... The VLBApls source sample . ... Click on the J2000 IAU name (in the left column) or the alternative name (mostly B1950 IAU names, in the right column) to get more information on a source, including coordinates, redshift, VLBApls images and model components...

Еще в разделе: (Показать все результаты (>2) - www.vsop.isas.ac.jp/ )

VISTA Data Flow System: Status Jim Emerson*a, Mike Irwinb, Nigel Hamblyc b a Astronomy Unit, Queen Mary Universit y o f London, Mile End Road, London E1 4NS, UK Inst itute of Astronomy, Universit y of Cambridge, Madingley Road, Cambridge CB3 0HA, UK, c Inst itute for Astronomy, School of Phys ics, Universit y of Edinburgh, Edinburgh EH9 3HJ, UK ABSTRACT Data from two IR survey cameras UKIRT's WFCAM and ESO's VISTA can arrive at rates approaching 1.4 TB/night for of order 10 years. ...

Еще в разделе: (Показать все результаты (>6) - www.vista.ac.uk/ )

• http://www.vista.ac.uk/Files/docs/vdfs/Cal-Plan-draft_v1.4.pdf

The monitoring of the optics quality of DIMM instrument V. Kornilov, B. Safonov May 24, 2010 1 Intro duction A quantitative theory of measurement of optical turbulence (OT) with Differential Image Motion Monitor (DIMM) is based on certain priori assumptions [1]. ... Bottom: behavior of the instrumental Strehl's number for the left (triangle to the left) and right (triangle to the right) DIMM images during the period of measurement the maintenance of an additional correction factor seems superfluous. ...

Еще в разделе: (Показать все результаты (>4) - curl.sai.msu.ru/ )

... The mount is also adjustable so you can orient the axis of rotation to make it parallel with the Earth's axis of rotation (see the section on Polar Alignment). ... Locate the opening in the equatorial mount on the DEC axis. ... To mount the telescope tube: 1. ... ADJUSTING THE MOUNT FOR POLAR ALIGNMENT In order for the clock drive to track accurately, the telescope's axis of rotation must be parallel to the Earth's axis of rotation, a process known as polar alignment. ... R.A. & DEC axis ! ...

Еще в разделе: (Показать все результаты (>16) - www.princetonastronomy.org/ )

... 322, L29 ? L36 (2001) The 2dF QSO Redshift Survey ? V. The 10k catalogue S. M. Croom,1w R. J. Smith,2 B. J. Boyle,1 T. Shanks,3 N. S. Loaring,4 L. Miller4 and I. J. Lewis1 1 2 3 4 Anglo-Australian Observatory, PO Box 296, Epping, NSW 1710, Australia Liverpool John Moores University, Twelve Quays House, Egerton Wharf, Birkenhead CH41 1LD Department of Physics, University of Durham, South Road, Durham DH1 3LE Department of Physics, Oxford University, 1 Keble Road, Oxford OX1 3RH Accepted 2001 March 7....

Еще в разделе: (Показать все результаты (>3) - www.2dfquasar.org/ )

• http://www.2dfquasar.org/Papers/2002MNRAS.337..275C.pdf
• http://www.2dfquasar.org/Papers/mnr7619_1397-1418.pdf

... Printed in U.S.A. ( FACEґON GALAXIES NGC 524 AND NGC 6340 : CHEMICALLY DECOUPLED NUCLEI AND INCLINED CIRCUMNUCLEAR DISKS O. K. SILоCHENKO1 Sternberg Astronomical Institute, Moscow, 119899 ... Moscow Branch ; olga=sai.msu.su Received 1999 September 1 ; accepted 2000 May 2 ABSTRACT The central regions of the earlyґtype disk galaxies NGC 524 and NGC ... 2, 2000 FACEґON GALAXIES NGC 524 AND NGC 6340 743 emission line [N II] j6583, which is strong in the centers of NGC 524 and NGC...

Еще в разделе: (Показать все результаты (>13) - sn.sai.msu.ru/ )

• http://sn.sai.msu.ru/~sil/preprints/al75.pdf
• http://sn.sai.msu.ru/~sil/preprints/iau245sil.pdf
• http://sn.sai.msu.ru/~sil/preprints/ic3653.pdf

The low aspect ratio, or spherical tokamak Globus-M [1] has recently been built in a support of international spherical tokamak plasma investigation program. ... The survey to determine the work scope in diagnostic design for Globus-M is given in the paper. ... The next one is an advanced diagnostic set intended to supply the data on basic plasma parameters: electron temperature and density profiles, ion temperature, plasma composition, radiation profile, Zeffective. ... Magnetic Diagnostics. ...

210. http://kcor.sai.msu.ru/arXiv1102.1159.pdf