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1. The spectrum-selection window
... Figure 2: Spectrum-selection window . A spectrum region is selected by clicking the left mouse-button on the image- this position should correspond to the coordinates of the zeroth-order spectrum. ... Any spectra in the table can be viewed by clicking the left mouse-button on the appropitate row in the table, or by clicking the Display current button, after it has been selected by clicking on its number in the table. ... All the selected spectra can be deleted by clicking the Delete all button. ...
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/sas/7.1.0/doc/omgsource/node9.html -- 6.1 Кб -- 09.07.2007
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2. Alternative construction
Next: Sky Subtraction Up: Construction of Flat Previous: Standard construction . For a number of projects where very deep integrations and accurate flat fields are required, and the targets are point sources or much smaller than the frame size, the sky background itself can be used to calculate the flat field. ... Use STATISTICS/IMAGE to calculate the image median, and COMPUTE/IMAGE to divide by this to get the normalised flat field. ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/precise/Midas_doc/doc/95NOV/vol2/node660.html -- 3.7 Кб -- 23.02.1996
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3. Some Alternative Non-Linear Methods
Next: Reducing 12-mm ATCA observations Up: Combining Mosaics and Single Previous: The Non-Linear Method - . Here we describe two ad hoc methods of combining single-dish and mosaic images. ... where and are the beam volumes of the synthesised mosaic beam and the single-dish beam respectively). ... If both the interferometer primary beam and the single-dish beam are gaussian forms with widths and respectively, then you will want to add a gaussian to the mosaic beam dataset which has a width . ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/computing/software/miriad/userguide/node196.html -- 10.5 Кб -- 10.04.2016
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4. http://hea-www.harvard.edu/AstroStat/Stat310_1011/ad_20110419.pdf
... memb ers of the CAUSTIC Group www.dfg.unito.it/ricerca/caustic Cambridge, April 19th 2011 SCIENTIFIC BACKGROUND Observations of SNae : Interpretation in the CDM model Alternative cosmological models: Conformal gravity and kinematic conformal gravity GRBs as cosmological probes: Bayesian approach BAYESIAN ANALYSIS Parameter forecasts (posterior probability): Likelihood and priors ... Constitution set of Hicken et al 2009) Bayesian parameter estimation again.. ...
[ Текст ]  Ссылки http://hea-www.harvard.edu/AstroStat/Stat310_1011/ad_20110419.pdf -- 2896.9 Кб -- 19.04.2011
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5. The CIMA Alternative Drift Map Menu
. This is the CIMA alternative drift map menu: . The following is the on-line help page for alternative drift map: . You can return to the main CIMA page by clicking here .
[ Сохраненная копия ]  Ссылки http://www.naic.edu/~cima/cima_win_obs_altdrift.html -- 1.9 Кб -- 01.03.2012
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6. http://www.gao.spb.ru/english/personal/malkin/publ/zm12i.pdf
... Impact of Covariance Information on the Orientation Parameters Between Radio Source Position Catalogs, IVS 2012 General Meeting Proceedings, p.339­341 http://ivscc.gsfc.nasa.gov/publications/gm2012/sokolova.pdf Impact of Covariance Information on the Orientation Parameters Between Radio Source ... IVS Analysis Centers provide these catalogs in a standard IERS format, where together with radio source positions and other relevant information, RA/DE correlations are reported. ...
[ Текст ]  Ссылки http://www.gao.spb.ru/english/personal/malkin/publ/zm12i.pdf -- 144.7 Кб -- 08.11.2013
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7. Index
... ACQ-DIST Optional Parameter for FGS 1 , 2 . ACQTYPE Optional Parameter for STIS . Acquisition modes . ... Aperture Coordinate System . ... AFTER date Special Requirement . ... BINAXIS1, BINAXIS2 Optional Parameters for STIS 1 , 2 . ... BUFFER-TIME Optional Parameter for STIS . ... CHECKBOX Optional Parameter for STIS . ... Calibration Targets . ... CR-SPLIT Optional Parameter for STIS . ... DIFFUSE-CENTER Optional Parameter for STIS . ... GAIN Optional Parameter for STIS . ... Position . ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/documents/p2pi/HTMLjavahelpCy20/ix.html -- 54.9 Кб -- 31.05.2012
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8. http://www.mrao.cam.ac.uk/~bn204/lecture/2008/bn-l4.pdf
Statistics for Astronomy IV: Maximum Likelihood B. Nikolic b.nikolic@mrao.cam.ac.uk Astrophysics Group, Cavendish Laboratory, University of Cambridge http://www.mrao.cam.ac.uk/~bn204/lecture/astrostats.html 3 November 2008 Goals for this Lecture Maximum Likelihood Example Recap Alternatives to ML How to find the Maximum Likelihood Errors estimation in Maximum Likelihood Monte Carlo simulation Problems Outline ... or equivalently the log-likelihood log L( ). ...
[ Текст ]  Ссылки http://www.mrao.cam.ac.uk/~bn204/lecture/2008/bn-l4.pdf -- 365.4 Кб -- 10.08.2012
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9. http://scan.sai.msu.ru/lk/
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. ...
[ Сохраненная копия ]  Ссылки http://scan.sai.msu.ru/lk/ -- 6.6 Кб -- 24.12.2015
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10. Alternative Idea - an Astronomy Net Blackholes Forum Message
Blackholes Forum Message . Forums: . ... Alternative Idea . ... With the proposal of exotic super dense entities like quark stars and others including black holes, matter on the atomic level can, and most likely does, break down to its most simplist building blocks (photons, leptons, quarks, etc). ... www.astronomy.net . About Astronomy Net | ... Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...