... You are here: start €Ё correlator €Ё records €Ё v255j . ... correlator:records:v255j . ... Observers Wiki . ... Phase reference at low spectral resolution . ... Comments: . Plots of uncalibrated amplitude and phase against frequency . ... Plots of Amplitude and phase against frequency with fringe-fit solutions applied . ... Plots of Amplitude and phase against time with fringe-fit solutions applied . ... correlator/records/v255j.txt €§ Last modified: 2014/11/11 18:08 (external edit) . ...

... Science . ... Science Users Information > Science Publications > Science Announcements > New GIRAFFE Spectral Resolutions Characterised For All Settings . ... ESO Data . ... The spectral resolution characterisation has been completed for all grating settings and the new resolving powers are listed under the FLAMES News . ... In some settings the spectral resolution is much higher, and in almost all HR settings there is an increase of 20-30% with respect to the values before the February intervention...

... Archives . ... MADS] ARCH . ... arxiv:0906.3662] The Statistical Analysis of fMRI Data by Martin A. Lindquist . ... This review paper offers some information and guidance of statistical image analysis for fMRI data that can be expanded to astronomical image data. ... This role can range from determining the appropriate statistical method to apply to a data set, to the development of unique statistical methods geared specifically toward the analysis of fMRI data. ... Chandra Blog . ... Chandra Images...

. XMM-Newton Science Analysis System . rgsangles (rgsangles-4.6.1) [xmmsas_20060628_1801-7.0.0] . Meta Index / Home Page . This task operates on the EXPOSU0n and EVENTS tables of the merged event list . High-time resolution mode will not produce any cross dispersion columns. Keywords related to cross dispersion values are not produced in that case . There is no internal looping over multiple sources. The caller (meta task) should do the source loop. XMM-Newton SOC/SSC -- 2006-06-28

... However the exact instrument setup (slit width and central wavelength) might change depending on the desired count level (which will be close to the internally allowed global rate limit). ... 1470 Exposure Time...........................: 11x4740 S = 869 M BOP Predicted Local Count Rate for MAMA.: 0.2 count/s/low-res pixel BOP Predicted Global Count Rate for MAMA: ~220000 count/s ETC PID IDs for Count Rates.............: [see comments] Special Requirements.. ... Special needs of this proposal? ...

. Comment on J2346+0930 . See Figure 4 for an image of each component. The source was detected at 2.3 GHz by Preston et al. (1985) (correlated flux density 40 mJy) with much higher resolution. VLBApls home page . Last modified: 16 Oct 2000

... Дни открытых дверей к юбилею САО РАН (12-14 апреля 2016 г.) . Международная конференция "Dark Ages and White Nights (Spectroscopy of the CMB)" (20-24 июня 2016 г.) . ... Международная конференция MULTI-SPIN GALAXIES - 2016 (26-30 сентября 2016 г.) . Международная астрономическая конференция "Физика звезд: от коллапса до коллапса" (3-7 октября 2016 г.) Архив . ... Подробнее.. ... 10.02.16 . ... БТА в реальном времени . ... Цейсс-1000 в реальном времени . ... Последнее обновление: 22/03/2016 ...

... A preliminary analysis shows that the definition of a common format for spectra is a big challenge. ... Survey among Spectral Data Providers and Consumers 339 · Elodie: 25000 extracted Echelle spectra , resolution 42000, 4000 - 6800 ° on the fly processing options available: wavelength resampling, flux A calibration etc., total volume 50 - 100 GB · ESO/ST-ECF, 250000+ observations taken with 14 spectrographs in UV, optical, near IR; archive is rapidly growing · HEASARC: Variety of ...

Next: The STScI NICMOS Calibration Up: No Title Previous: CONICA: The high resolution . The STScI NICMOS Calibration Pipeline . Introduction . ... Dark Current Subtraction . ... Input Data . ... Scalar Background Subtraction . 2-D Background Subtraction . ... Status and Goals of the NICMOS Calibration Plan . ... Photometry . ... Photometric Performance of NICMOS . ... NICMOS Photometry. ... ST-ECF Grism Spectrum Software for NICMOS Grism Data . ... Analysis . ... STScI NICMOS Software . ...

... Cheers, -Mike Data Providers (e.g., data centers, archives) Provider Name: NOAO Collection: High Resolution Atlas of Arcturus Spectra - 0.92-5.36 microns Characteristics: 310 ASCII tables of wavenumber vs flux Storage Format: Text tables Available online: ftp://ftp.noao.edu/catalogs/arcturusatlas/ir Comments: Tables contain three flux values (arcturus spectrum, telluric spectrum and ratio) for both summer and winter observations. ... Linelists also available as text table ...

... Apache HTTP Server Version 2.4 . ... This page could be summarized with the statement: don't configure Apache HTTP Server in such a way that it relies on DNS resolution for parsing of the configuration files. If httpd requires DNS resolution to parse the configuration files then your server may be subject to reliability problems (ie. it might not start up), or denial and theft of service attacks (including virtual hosts able to steal hits from other virtual hosts). ... The "main server" Address . ...

обзор! astro-ph/0207130 . ... Author: Bertil Dorch . Comments: Invited review, IAU coll. ... В обзоре рассматривается трехмерное моделирование магнитных трубок на Солнце. ... Comments: 55 pages, 35 figures -- low resolution figures to allow upload to astro-ph High-resolution version at http://www-sgk.harvard.edu:1080/~sylvain/preprints/ . ... Comments: 6 pages, 4 figures, Astron Nachr (accepted; proceedings of "1st Potsdam Thinkshop on Sunspots and Starspots", Potsdam, Germany, May 2002) . ...

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. ...

Next: Spectral-Line Observing at AO . Spectral-Line Observing at Arecibo Observatory . ... Spectral-Line Observing at AO . INTRODUCTION to Spectral Line Observing at AO . ... OBSERVING PROCEDURES . ... Run Correlator . ... RA/Dec & Dec/RA maps . ... CORRELATOR BOARDS . INTEGRATION TIME (per Data Record) . ... USING THE AO-CONTROL GUI FOR SPECTRAL LINE OBSERVATIONS . ... DATA ANALYSIS . AO data and AIPS++ . ... Some Useful Routines for On-Line Data Analysis . ...

... 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 . ...

... ASAS 090446-5625.1 . ... ASAS 091455-6401.6 . ... ASAS 094623-3957.0 . ... ASAS 105719-5057.9 . ... ASAS 150306-6028.0 . ... ASAS 154459-6236.9 . ... ASAS 171022-5415.1 . ... ASAS 184807-3513.7 . ... ASAS 201139+1606.4 . ... TYC 8590 00384 1 = HD 302079 = ASAS 090446-5625.1 . ... TYC 8948 00036 1 = ASAS 091455-6401.6 . ... TYC 7697 03154 1 = ASAS 094623-3957.0 . ... TYC 8211 01725 1 = ASAS 105719-5057.9 . ... TYC 9020 00319 1 = ASAS 150306-6028.0 . ... TYC 9027 02560 1 = ASAS 154459-6236.9 . ...

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' / . ...

... If are the wavelet coefficients of the image I at the scale j, we have: . where are the wavelet coefficients of the PSF at the scale j . The wavelet coefficients of the image I are the product of convolution of object O by the wavelet coefficients of the PSF. To deconvolve the image, we have to minimize for each scale j: . ... The problem has not generally a unique solution, and we need to do a regularization [ 40 ]. ... We have in fact a multiresolution Tikhonov's regularization. ...

... Therefore, we see that some spectral resolution is achieved by selection of the wavelet size, and some temporal resolution follows from the location of the wavelet relative to the signal (Fig. ... Figure 6: Contour line representation of the wavelet transform for a near-continuum of durations. We can identify the individual peaks and troughs of the cosine wave as well as their frequency: this compromise between the temporal domain and the spectral domain is the hallmark of wavelet transforms. ...

Обзоры hep-ex: тематический рубрикатор . ... Comments: 49 pages, 37 figures. ... обзор hep-ex/0207093 . ... Comments: Talk presented at the XXth International Conference on Neutrino Physics and Astrophysics, May 25-30, 2002, Munich, Germany. 10 pages, 12 figures . ... Comments: 16 pages, 11 figures, Talk given at the CERN-ESA-ESO Symposium, Munich, April 2002 . ... Comments: Talk presented at La Thuile, Italy, Les Rencontres de Physique de la Vallee d'Aoste, 3-9 March 2002, 12 pages, 11 figures . ...