... Apache HTTP Server Version 2.4 . Apache > HTTP Server > Documentation > Version 2.4 > Programs . ... htcacheclean is used to keep the size of mod_cache_disk 's storage within a given size limit, or limit on inodes in use. ... If one or more URLs are specified, each URL will be deleted from the cache, if present. ... Specify limit as the total disk cache size limit. ... By passing the -a or -A options to htcacheclean , the URLs within the cache will be listed as they are found, one URL per line. ...

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Next: The Clark CLEAN Up: Image Deconvolution Previous: Introduction . The CLEAN algorithm (H?gbom 1974) (A&AS 15, 417) represents the image as a number of point sources in an otherwise empty field of view. ... The H?gbom CLEAN algorithm looks for the brightest (in an absolute sense) pixel (called a CLEAN component) in a specified region in the image (called the CLEAN window which must include all the real emission in the image). ... This subtracted image is called the residual image. ...

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• Archive of VLBI Observations Majordomo List
• Programme - Abstract

... 1Fanti+ We presente the result of a seach for new Galactic sources from the BG catalogue. The observations were made with the WSRT at 1.4 GHz, using the short cuts technique. The adopted selection criteria for the observed sample are discussed in detail. ... A catalogue of the sources present in each field was produced; the relevant information about observations and reduction characteristics are given. ... The expected number of Galactic sources present in the observed sample was confirmed. ...

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• A 20 cm VLA survey of Abell clusters of galaxies
• VLSS radio survey
• A General Catalog of HI Observations of Galaxies

XLVII, 4 . 2004 520.24+520.274.3+52-17 -600 . ... 2 -600 . ... 255 2004 . ... CLEAN ( ). ... 2002 4 , 1 . ... XLVII, 4 T a, K 18000 17000 16000 15000 14000 AO 9866 (1) б) Ta, K 19000 18000 17000 16000 15000 AO 9866 (2) в) -100 0 100 t, мин -100 0 100 t, мин . ... P. 125. 11. http://www.sao.ru/hq/sun/obs_table.html. 12. http://www.sao.ru/hq/sun. ... MULTI-AZIMUTH REGIME OF OBSERVATIONS AT THE RATAN-600 SOUTHERN SECTOR WITH PERISCOPE REFLECTOR V. M. Bogod, G. N. Zhekanis, M. G. Mingaliev, and S. Kh. ...

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• GRB follow-up team
• LSFVO: Results

... Up: Algorithms . ... Iterative algorithms with non-linear constraints are very attractive in image reconstruction with only a few strip-integrated projections. We present research into various versions of the iterative CLEAN algorithm for the solution of this problem. ... where is the object brightness distribution, is the fan (dirty) beam, and is the dirty (summary) image. ... We carried out the study of TC-CLEAN applied to image reconstruction with few projections. ...

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• Determination of the Permissible Solutions Area by Image Reconstruction from a
• Image Processing of Digitized Spectral Data
• The Time Interferometer: Synthesis of the Correlation Function

We combine new Spitzer Space Telescope observations in the mid-infrared and far-infrared (FIR) with SCUBA 850 ЮМm observations to improve the measurement of dust temperatures, masses, and luminosities for 11 galaxies of the SCUBA Local Universe Galaxy Survey. ... The data presented in this paper combined with previous observations show that cold dust is present in all types of spiral galaxies and is a major contributor to their total luminosity. ... ADS Citation Query . citations = 25 . ...

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• Spitzer Sage Observations of Large Magellanic Cloud Planetary Nebulae
• Webcast Archive
• Spitzer Observations of NGC 2547: The Disk Population at 25 Million Years

... See also the NAIC spectrum management page. Note that the full ALFA band covers 1225 to 1525 MHz. ... An example was shown of the OH spectrum of an OH/IR star obtained with 3-level sampling using the present autocorrelator showing lots of ringing. ... But also, we need simple RFI removal software. ... This also relates to the issue of maximum BW: 100 or 200 MHz bandwidth? From my experience, the spectrum seems to be pretty clean out to 1225 MHz, and so there is a case for 200 MHz bandwidth. ...

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• Observation Night at the Arecibo Observatory National Astronomy and Ionosphere

Peremennye Zvezdy ( Variable Stars ) 35 , No. ... We present the results of our new observations of QS Draconis, a recently discovered double-mode high-amplitude Scuti variable, HADS(B) type. ... Our CCD observations in the Johnson bands were performed at the Tien Shan Astronomical Observatory of the V.G. Fesenkov Astrophysical Institute, at the altitude of 2750 m above the sea level. ... The finding chart (Fig. 1) identifies the variable star, comparison star, and check star. ... Fig. ...

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• Journal "Peremennye Zvezdy" > PZ: main journal.

Next: Results & Discussion Up: Coronal Hole Diagnostics out Previous: Introduction . ... The dates of the observations discussed here, their locations, pointing, slit sizes and exposure times are given in BTDW. ... Line fits are given by the dotted line. ... An estimation of the errors in the derived parameters was obtained using the GA-derived parameters as an input for a ``classical'' IDL-CURVEFIT procedure (Peter, 1999; Peter & Judge, 1999). ...

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• Armagh Observatory
• Why Asteroid 2008 TC3 Represents a Landmark - Dr David Asher, from Armagh
• A Blinker Model

The large magnetic cloud caused by coronal mass ejection at the Sun on January 6, 1997 came to the Earth at early morning on January 10 and continue to interact with Earth's magnetosphere till January 11 (see for example home page of this event prepeared by Dr. M.Peredo http://www-istp.gsfc.nasa.gov/istp/cloud_jan97/event.html ). ... During the days discussed here INTERBALL-1 satellite was in the magnetosphere (MS) near its dusk flunk - see the Fig. 1 for compearing. ...

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• Space Research Institute (IKI) Seminar
• IESP-2M Results Page

EPM-ERA2012 Lunar Ephemeris and selenodynamical parameters from LLR data(1970-2012) M.V. Vasilyev, E.I.Yagudina IAA RAS, St-Petersburg, Russia Reflector at the Moon The reflector 's positions at the Moon surface 3.5 m telescope at Apache station INTRODUCTION MODERN EPHEMERIDES: 1. ... IAA RAS, Russia-EPM-ERA2012 The present analysis of (17580) LLR observations, (time interval 1970, March - 2012, February) Model ( brief description). The dynamical model EPM-ERA has been developed by G.A. Krasinsky. ...

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• http://www.ipa.nw.ru/conference/2002/sovet/PS/FIENGA.PS
• http://www.ipa.nw.ru/conference/2002/sovet/PS/YAGUDINA.PS
• Keywords_75

... Radio emission at around 90 GHz from star-forming galaxies is expected to be strongly dominated by the free-free component due to ionising radiation from massive, short-lived, stars. We present high surface-brightness sensitivity observations at 90 GHz of the nearby star-forming galaxy Messier 66 with resolution of about 9 arcsec (corresponding to a physical scale of about 500 pc) and analyse these observations in combination with archival lower frequency radio and mid-infrared measurements. ...

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• A CLEAN-based method for mosaic deconvolution
• G109.1-1.0
• High-frequency Radio Continuum Observations of Giant Radio Galaxies

... Home Gallery Club Events AAA president Marcelo Cabrera presents AAA Amateur Astronomers Medal to Al Nagler of TeleVue Optics with AAA vice-president Susan Andreoli. ... A History of the First Forty Years of the Amateur Astronomers Association . ... AAA president Marcelo Cabrera presents AAA Amateur Astronomers Medal to Al Nagler of TeleVue Optics with AAA vice-president Susan Andreoli. by . ... 2016 Amateur Astronomers Association of New York Designed by Press Customizr Powered by . ...

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JournИes SystХmes de RИfИrence Spatio-Temporels , St Petersburg, Russia, 22-24 Septembre 2014 Optical monitoring of QSO in the framework of the Gaia space mission F. Taris (1), G. Damljanovic (2), A. Andrei (3), A. Klotz (4) , F. Vachier (5) (1) Observatoire de Paris - SyRTE, France , (2) Astronomical observatory of Belgrad, Serbia, (3) Observatorio Nacional MCT, Brasil, (4) UniversitИ de Toulouse, France (5) Observatoire de Paris ґ IMCCE, ...

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• http://www.gao.spb.ru/english/as/j2014/presentations/perepelkin.pdf
• General description of the database

THE MAIN FIELDS OF MY INTEREST ARE RELATIVISTIC GRAVITATION AND COSMOLOGY . ... The first one is cosmology more precisely the anisotropy of the CMBR (Cosmic Microwave Background Radiation) . In the last paper devoted to the mapping of the CMBR and search for anisotropy we announced the observation of the signal (Strukov et al., ... We discuss the opportunity of explanation of the current observational data in the framework of this hypothesis. ... Some of my papers I devoted to the phenomena. ...

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• COSMION-96:present state
• The Present Situation in the Galaxy
• COSMION-97:present state

... Determination of the Permissible Solutions Area by Image Reconstruction from a few Projections: Method 2ґCLEAN DSA Michail I. Agafonov Radiophysical Research Institute (NIRFI), 25 B.Pecherskaya st., Nizhny Novgorod, 603600, Russia, Eґmail: agfn@nirfi.nnov.su Abstract. ... Application The problem requires the solution of the equation G = H # F (+noise) , (1) where F (x, y) is the object brightness distribution, H(x, y) is the fan (dirty) beam, and G(x, y) is the dirty (summary) image. ...

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• http://www.stecf.org/conferences/adass/adassVII/reprints/teubenp.ps.gz
• http://www.stecf.org/conferences/adass/adassVII/reprints/monais.ps.gz
• http://www.stecf.org/conferences/adass/adassVII/reprints/dolenskym2.ps.gz

... In January 2015 using the Mini-MegaTORTORA multichannel optical sky-monitoring system with subsecond temporal resolution, the observations of comet C/2014 Q2 (Lovejoy) and asteroid 357439 2004 BL86 were carried out. ... It was put into operation in 2014. ... Comet C/2014 Q2 (Lovejoy). The 60-min-long observations with the Mini-MegaTORTORA system on Jan 19, 2015 at 16:50 UT, exposure time 30 s, BVR synchronously . ... Asteroid 357439 2004 BL86. ...

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• The Present and Future of Small and Medium Size Telescopes

The radial distribution of metallicity of star-forming galaxies in a galaxy cluster can inform us about the mass assembly and enrichment history of the galaxy cluster. ... Both galaxy clusters are cool-core clusters at redshift z т?? ... The gas-phase metallicity of star- forming galaxies in MACS1115+01 exhibit anti-correlation with projected distance т??0.15 ТБ 0.08 dex/Mpc, whereas the radial metallicity distribution of RXJ1532+30 is statistically flat (т??0.09 ТБ 0.12 dex/Mpc). ...

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• Problem Based Learning in Undergraduate Astronomy
• Most rooms clean, courtyard looking bare.
• Cleaning the drive is a difficult job.

... He made observations of a supernova (literally: nova= "new star") in 1572 (we now know that a supernova is an exploding star, not a new star). ... Brahe's meticulous observations showed that the supernova did not change positions with respect to the other stars (no parallax). ... This was early evidence against the immutable nature of the heavens, although Brahe did not interpret the absence of parallax for stars correctly, as we discuss below. Brahe made careful observations of a comet in 1577. ...

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• http://zebu.uoregon.edu/2003/ph301/age_of_the_earth.html
• http://zebu.uoregon.edu/messier/m64.txt
• Astronomy HyperText Book: Stellar Clusters

... For the Corner Method, Clean_lc was originally a FORTRAN 77 program developed by Steve Snowden and Kip Kuntz in 2005-6. ... Clean_lc's purpose is to clean a light curve by creating a histogram of rate values from the light curve, finding the most likely value assuming that to be similar to the mean of the quiescent rate, then fitting a Gaussian to a small window around that value in the histogram to determine the true mean and dispersion of the quiescent background rate. ...

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• Main loop
• Summary File specification from ODF ICD 2.4