... DEC - As above . LII - Galactic longitude computed from the RA above . BII - Galactic latitude computed from the DEC above . M_STD_COL - The standard M magnitude that was calculated when the standard COL colour was calculated (M stands for one of the filters and COL the instrumental colour that was used - NB THE FILTERS FOR ALL COLOURS ARE THE XMM CODES LISTED EARLIER). ERR_M_STD_COL - The error of the standard M magnitude. ...

... Archives . ... Quote of the Week, Aug 31, 2007 . Aug 30th, 2007| 09:36 pm | ... From arxiv/astro-ph:0708.3758v1 . Numerical Color-Magnitude Diagram Analysis of SDSS Data and Application to the New Milky Way Satellites by J. T. A. de Jong et. al. ... A traditional CMD fitting begins with building synthetic CMDs: Completeness of SDSS Data Release 5, Hess diagram (a bivariate histogram from a CMD), and features in MATCH for CMD synthesis were taken into account. ... Chandra Blog . ...

... You are here: start €Ё correlator €Ё records €Ё v486g . ... correlator:records:v486g . ... Observers Wiki . ... Plots of uncalibrated amplitude and phase against frequency . ... Plots of uncalibrated amplitude and phase against time . ... Plots of cross-polarization amplitude and phase against frequency (not always available) . ... Plots of Amplitude and phase against frequency with fringe-fit solutions applied . ... correlator/records/v486g.txt €§ Last modified: 2016/04/08 12:19 by cormac . ...

... OOF holography home Quick Links: . ... Scans 2002+: Aperture, Residuals, Residuals (log plot) , FITS file of the calculated phase map, ASCII file of the calculated phase map, . Scans 3001+: Aperture, Residuals, Residuals (log plot) , FITS file of the calculated phase map, ASCII file of the calculated phase map, . Scans 4001+: Aperture, Residuals, Residuals (log plot) , FITS file of the calculated phase map, ASCII file of the calculated phase map, . ... Scans 3001+: Aperture . ...

Comment on the International Jubilee Symposium . ... The usefulness of the Internet as a method of holding international meetings without the expense of travel is also clear, but this new medium is not yet well established in this role. ... How can we move on with international cooperation in the World Wide Web era? I would like to suggest that NASA's Planetary Data System is a good model. ... At the same time, much might be done with older images, by scanning prints to create new digital files. ...

Please enter the lightcurve file name and period search parameters: . Lightcurve file: . ... Apply the Heliocentric correction and convert all dates to Terrestrial Time (TT)? ... Also, the Heliocentric correction cannot be applied to such lightcurves. ... This period search service is also available at the mirror sites: Mirror 1 , Mirror 2 , Mirror 3 , Mirror 4 . You may download the latest source code distribution and install the period search service at your own web server. ...

For the calibration of RATAN-600 data you will need to Download Nobeyama Fluxes (1, 2, 3.75, 9.4, 17 GHz): year 1999 2000 2001 2002 2003 . Brief description of Work Scan . Main functions of processing, realized in the program are: . ... Correction of various (not fatal) defects of data; . ... Calculating of the lower enveloping curve or an average scan from observations data for a few days; . ... COMMENT This table contains the set (TFIELDS) of 1-dimensional (TFORM# . ... AZIMUTH = 'float' / . ...

... HST . ... APT . ... HST Overview . Overview . ... Phase I Proposing . ... Cycle 24 Announcement . ... Phase II Cycle 23 . ... Documents . ... After you have brought up APT you will see a "Help" menu on the top menu bar. From here you can also bring up the documents that will help you to learn APT. Phase I: You can bring up Phase I Specific APT Training Materials to learn about using APT to submit your Phase I proposal. ... These are the same documents you will find on the HST Website. ...

. Comment on J2243-2544 . The jet extends in the opposite direction to that shown by Shen et al. (1998) at 5 GHz with about 2 times higher resolution than our image. The structure we see is confirmed by the 2.3 and the 8.4 GHz images from the VLBA Calibrators database. VLBApls home page . Last modified: 16 Oct 2000

exp. energy levels: Martin,W.C., Sugar,J., Musgrove,A., Dalton, G.R., 2000, NIST Database for Atomic Spectroscopy, Version 1.0, NIST Standard Reference Database 61. %exp. energy levels (1s2p 3P): Curdt, W., Landi, E., Wilhelm, K., Feldman, U., 2000, Phys.Rev.A, in press %Comment: the 1s2p 3P energies are calculated using the 1s2s 3S level as reference. ... Comment: 1s2p 3P1 energy has been calculated from the 1s2s 3P0 level using the NIST level separation. Thu Jul 20 13:42:29 2000 ...

The AstroGuide . ... AstroGuide | ... AstroGuide Listing . ... See many more Astronomy Listings by: Category or Alphabet . ... The software run under Windows 95, 98 NT, including Paraxial and Seidel . ... and Energy Distribution, Optical Layout, Optimization, Tolerancing etc. ... Listed Since August 20, 2005 . ... Web Site . ... Web . ... Unless otherwise specified, web site content Copyright 1994-2016 John Huggins All Rights Reserved . dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

. Next: Standard values Up: Optional stellar data Previous: Rough magnitudes . љ Up to 32 characters can be carried in an additional column, with the label COMMENT. Rein Warmels . Mon Jan 22 15:08:15 MET 1996

... About ATMoB . ... Events . ... Located in Westford, MA, less than an hour's drive from Boston. The clubhouse is maintained for members, but any non-member may visit with a member or by other prior arrangement (see the Contact Us page). The clubhouse is located on the grounds of MIT's Millstone farmhouse in Westford, MA. ... View sky above the clubhouse. ... Upcoming Clubhouse Events.. ... About the Club . ... ATMoB Club House . ... Copyright (c) Amateur Telescope Makers of Boston, Inc. ...

Peremennye Zvezdy", . ... Data . ... Our frequency analysis of this star was performed using discrete Fourier transform for the time series with an arbitrary data spacing (Deeming, 1975). ... P(1) = 0.0506318(+/-5) day (Ampl=0.0040 mag); . P(2) = 0.0377470(+/-3) day (Ampl=0.0023 mag); . P(3) = 0.0314978(+/-2) day (Ampl=0.0023 mag); . P(4) = 0.0391142(+/-3) day (Ampl=0.0018 mag); . P(5) = 0.0606147(+/-7) day (Ampl=0.0018 mag); . P(6) = 0.0396115(+/-4) day (Ampl=0.0015 mag). ...

... Natalya V. Raguzova and Sergei B. Popov . ... We present a compilative catalogue of Be/X-ray binaries and candidates in the Galaxy and in the Large and Small Magellanic Clouds. This catalogue contains 160 sources and provides information on names and spectral types of optical components, distances, on spin characteristics of neutron stars, and on orbital and X-ray properties of binary systems. ... Be/X-Ray Binaries and candidates in the Galaxy . Galactic sources: comments to the Table 1 . ...

... When creating a mosaic from a set of individual frames, the correct background offset for each frame must be determined for proper matching. In this paper we describe a method for constructing a mosaic from a set of individual frames by applying a minimization technique. ... Typically these are frames with some known defect (see ? ... Determining which frames to exclude from the final mosaic is critical, since one bad frame can create background offset errors that propagate throughout the mosaic. ...

SN 1989B Light Curve Analysis. ... In the light curve depicting their observations, definite trends are noted, here is a "thumb-nail" analysis of the the magnitude estimations of the bright SN (1989B) in the galaxy NGC 3627 (M66). ... The observations were inserted against the V magnitude templete of BL, CCD photometric data, (Wells et. al, (1994) and a color trend (B-V) histogram of the mean type Ia SN (BL)(nutemp.gif). Key Words: Amateur Observations, Supernova, Magnitude Estimates, 1989B . ...

... Science Users Information > Observing Facilities > ALMA > European ALMA Regional Centre . ... ARC Staff at ESO . ... The European ALMA Regional Centre (ARC) provides the interface between the ALMA project and the European science community. ... The central node is located at ESO Headquarters in Garching bei MУМnchen and carries the responsibility for all the core ARC activities as well as the coordination of the additional science support provided by the regional nodes and centres of expertise . ...

... Authors: Spyros Basilakos (Imperial College London) . ... Title: Populating a cluster of galaxies - I. Results at z=0 . ... Title: The Merger Rate to Redshift One from Kinematic Pairs: Caltech Faint Galaxy Redshift Survey XI . ... Title: Multi-wavelength observations of an evolved galaxy group: An endpoint of galaxy merging? ... 23 matches for the search pattern galaxy merging . The URL for this page is: http://xxx.itep.ru/find/astro-ph/1/galaxy+merging/0/1/0/past,all/0/0 www-admin@xxx.lanl.gov ...

. Back to the main page . Short introduction into wavelet analysis (A.F.Kholtygin, in russian) . Bibliography with comments