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http://hea-www.harvard.edu/AstroStat/Stat310_0910/xx_20100420.pdf.
http://hea-www.harvard.edu/AstroStat/Stat310_0910/xx_20100420.pdf.
1. pdev_birdies_25jun07
... On 11mar08 a sine wave was injected into the pdev baseband mixers to measure the mixer and pdev A/D levels. ... Onset of compression. 7dbm input, 9 dbm output , 15 dbm attenuation. ... A 9 dbm output will generate a sine wave with an amplitude of 2047 A/D counts. -8dbm input, 9 dbm output, 0 dbm attenuation. ... with 15 db attenuation, the mixer input is 7 dbm, H3-5 amp needs to output 22.5 dbm . with 0 db attenuation , the mixer input is -15 dbm, the H3-5 amp needs to output 22.5 dbm. ...
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Ссылки http://www.naic.edu/~phil/hardware/pdev/mixer/mixerlevels.html -- 7.2 Кб -- 25.04.2008
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2. The AstroStat Slog ICA
... I happened to observe a surge of principle component analysis (PCA) and independent component analysis (ICA) applications in astronomy. ... Category: Algorithms , arXiv , Astro , Cross-Cultural , Data Processing , Jargon | ... Algorithms arXiv Astro Bad AstroStat Bayesian CHASC Cross-Cultural Data Processing Fitting Frequentist Galaxies gamma-ray High-Energy Imaging Jargon Job Languages MC MCMC Meta Methods Misc News Nuggets Objects Optical Physics Quotes Spectral Stars Stat Timing Uncertainty X-ray...
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Ссылки http://hea-www.harvard.edu/AstroStat/slog/groundtruth.info/AstroStat/slog/tag/ica/index.html -- 29.3 Кб -- 01.03.2014
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3. ФОРМАТ ЗАПИСИ В БАЗЕ ДАННЫХ НА CD-ROM
ФОРМАТ ЗАПИСИ В БАЗЕ ДАННЫХ НА CD-ROM BYTE MNEM CONTEXT 1 - 2 NR Record length in bytes (usually 416) 3 - 6 STCOD IAGA station code, 3 letters, 4th arbitrary 7 - 9 CMP order of the components in data block, 3 10 letters and space 11 SC scaling factor, multiply all data and base values by X (SC=0 X=1, SC=1.. ... Components code: D,I-in 0.1'; H,F,X,Y,Z in nT; E-magnetic east component perpendicular to H in nT; Usually data recorded as XYZ. ... Digital geomagnetic data base for VIKING period. ...
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Ссылки http://www.iki.rssi.ru/magbase/HTML/MAGFORM.HTM -- 4.2 Кб -- 03.07.2001
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4. Dust Attenuation in Late-Type Galaxies. I. Effects on Bulge and Disk Components
We present results of new Monte Carlo calculations made with the DIRTY code of radiative transfer of stellar and scattered radiation for a dusty giant late-type galaxy like the Milky Way, which illustrate the effect of the attenuation of stellar light by internal dust on the integrated photometry of the individual bulge and disk components. ... In addition, we find that the structure of the dusty ISM affects more sensitively the observed magnitudes than the observed colors of both bulge and disk. ...
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Ссылки http://www.stsci.edu/~kgordon/papers/2004ApJ...617.1022P.html -- 4.5 Кб -- 21.01.2016
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5. How DFS components access databases
... DpmkSpace (part of SAS) . Cdb server (part of calibDB, in Garching only . Dpserver (part of SA, in Garching only) More about P2PP checks to be performed when installing/configuring it. Go to top of page . More about OT-tcl/tk checks to be performed when installing/configuring it. ... More about Java-OT checks to be performed when installing/configuring it. ...
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Ссылки http://www.eso.org/projects/dfs/team/DFS-NEW-SYBASE-access-DB.html -- 42.8 Кб -- 08.08.2007
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6. Gadget Box PPS Level Converter and CHU Modem
... It includes level converters and a optional radio modem designed to decode the radio timecode signals transmitted by the Canadian time and frequency station CHU. A complete set of schematics, PCB artwork, drill templates is in the pub/ntp/gadget.tar.Z file on ftp.udel.edu. ... One of these converts a TTL positive edge into a fixed- width pulse at EIA levels and is for use with a timecode receiver or oscillator including a TTL PPS output. ... See the schematic diagram gadget.s01 for reference. ...
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Ссылки http://www.sai.msu.su/~er/xntp/gadget.html -- 6.3 Кб -- 21.12.2007
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7. odnh3
... User Guide ] Task: odnh3 Purpose: Ammonia analysis program Categories: map combination, map manipulation ODNH3 is a MIRIAD task that creates optical depth and rotational temperature maps from ammonia maps. Ammonia J,K=(1,1) emission has five hyperfine components, one main hyperfine component, two inner hyperfine components, and two outer hyperfine components. ... Key: map1 Input map, main hyperfine component map of the J,K=(1,1) level. No default. ... Key: region Standard keyword region. ...
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Ссылки http://www.atnf.csiro.au/computing/software/miriad/doc/odnh3.html -- 3.5 Кб -- 10.04.2016
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8. Inference of Coefficients for Use in Phase Correction
... OOF software . ... Memos . ... Raw data . ... We present a Bayesian approach to calculating the coefficients that convert the outputs of ALMA 183 GHz water-vapour radiometers into estimates of path fluctuations that can be used to correct the observed interferometric visibilities. ... Please note that the files"COPYING" in each of the distribution packages have GPL listed but it is in fact LGPL which applies. ... This is the raw data from the SMA used in the analysis shown in Section 4 of the memo. ...
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Ссылки http://www.mrao.cam.ac.uk/~bn204/mk2/alma/memo-infer.html -- 14.3 Кб -- 25.11.2009
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9. MSSA results
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Ссылки http://lnfm1.sai.msu.ru/~tempus/science/MSSA/ -- 2.4 Кб -- 28.09.2012
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10. http://mavr.sao.ru/hq/lizm/conferences/pdf/1987/1987_p27-p30.pdf
... For every level we have plotted the dependence between width and Lande factor and obtained the linear regression parameters: the inclination, the zero Lande factor line width and the correlation. ... Fig. 1. presents a model components, the intensity of which decreases (b) line with 10 and increases (c) to the center of spectral line (the field is 12 k6s). ... Our results show strong dependencies of line width on the level of width measurements. ...
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Ссылки http://mavr.sao.ru/hq/lizm/conferences/pdf/1987/1987_p27-p30.pdf -- 41.5 Кб -- 24.02.2010
[ Текст ] Ссылки http://www.sao.ru/hq/lizm/conferences/pdf/1987/1987_p27-p30.pdf -- 41.5 Кб -- 24.02.2010
[ Текст ] Ссылки http://jet.sao.ru/hq/lizm/conferences/pdf/1987/1987_p27-p30.pdf -- 41.5 Кб -- 24.02.2010
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[ Текст ] Ссылки http://www.sao.ru/hq/lizm/conferences/pdf/1987/1987_p27-p30.pdf -- 41.5 Кб -- 24.02.2010
[ Текст ] Ссылки http://jet.sao.ru/hq/lizm/conferences/pdf/1987/1987_p27-p30.pdf -- 41.5 Кб -- 24.02.2010
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11. http://www.adass.org/adass/proceedings/adass03/reprints/P4-27.pdf
... The existing package features many applications which are required for the next generation telescopes under development (e.g., multi-field, multi-scale, and wide field imaging algorithms, full primary beam Stokes I,Q,U,V imaging, automated and interactive statistical data editing, flexible calibration and self-calibration based on the telescope measurement equation; we highlight some of this functionality and discuss the future directions for the applications and underlying technology. ...
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Ссылки http://www.adass.org/adass/proceedings/adass03/reprints/P4-27.pdf -- 253.5 Кб -- 27.08.2004
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12. Software Maintenance Manual
... Created: 23 February 2001 . ... SOFTWARE MAINTENANCE MANUAL . ... 9 January 2001 . ... Note: in the final document, the table of contents will be to third level] . The Software Maintenance Manual describes the procedures for installation and maintenance of the software for the Gemini Near-infrared Integral Field Spectrograph (NIFS). ... Section 19.4.3 of the document “Programmatic Requirements for Gemini Instrumentation Development” states the requirements for the Software Maintenance Manual . ...
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Ссылки http://www.mso.anu.edu.au/nifs/manuals/man0003.htm -- 139.3 Кб -- 06.09.2001
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13. http://www.arcetri.astro.it/igm50/talks_all/grossi.pdf
... HI mass fractions Comparison samples HeViCS bright galaxy Catalogue(BGC) Davies+2012 Average scaling relations for HI-normal and extremely HI-deficient galaxies in H3 survey (Gavazzii+ 2013 ) Dwarf galaxy survey (DGS) Madden+ 2013 KINGFISH Kennicutt 2011 Specific star formation rates Schiminovich +2007 Comparison samples HeViCS bright galaxy Catalogue(BGC) Davies+2012 Dwarf galaxy survey (DGS) Madden+ 2013 KINGFISH Kennicutt 2011 Dust ...
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Ссылки http://www.arcetri.astro.it/igm50/talks_all/grossi.pdf -- 2009.2 Кб -- 17.06.2015
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14. Introduction
Next: stecf.cplucy - Enhanced Two-channel Up: The ``stecf" IRAF Layered Previous: The ``stecf" IRAF Layered . For many years the ST-ECF has developed IRAF tasks and packages for HST and related data analysis. ... To allow wider and more efficient distribution and to bring all components to a uniform level of quality and documentation we have decided to combine these components into a standard-format IRAF package to be called ``stecf''. ...
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Ссылки http://www.stecf.org/software/IRAFtools/stecf-iraf/adass99/P2-21/node1.html -- 3.8 Кб -- 06.06.2006
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15. USS radio sources
... (Roettgering+, 1994) ============================================================================ Samples of ultra-steep spectrum radio sources ROETTGERING H.J.A., LACY M., MILEY G.K., CHAMBERS K.C., SAUNDERS R. 15mJy z: A bright serendipitous source in the VLA field ---------------------------------------------------------------------------- Notes on individual sources : 0141+356 A serendipitous double ... 1718+630 Component '1' serendipitous or related to double radio source? ...
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Ссылки http://www.sao.ru/cats/doc/USS_Rottgering.html -- 10.9 Кб -- 18.03.2015
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16. User-level errors and warnings
... Meta Index / Home Page / Errors . ... warning . ... For instance, if the PROPOSAL information record is missing the user can add a fake one to the SOSF without this having any effect on the data reduction. corrective action: Continue. ... For a certain exposure in the ODF one of the parameters was not found in the housekeeping data. ... RGS, EPN, OM : the current exposure is found to contain more than one distinct calibration mode. corrective action: In the summary file: MODE = UNDEFINED . ... error...
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Ссылки http://xmm.vilspa.esa.es/sas/8.0.0/doc/odfingest/node16.html -- 15.0 Кб -- 01.07.2008
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17. "STP Data" STP Data
... Minute Values of Geomagnetic Field Components . ... AA 1868 - Present (3 hourly and daily) (monthly) (yearly) (Lists and histograms of geomagnetic disturbance and Solar Sunspots) KP_AP 1932 - Present (3 hourly and daily) (Lists and histograms of geomagnetic disturbance and Solar Sunspots) AE_HV 1957-75, 78-88 (hourly) AE_MIN 1978-881-6;198903;1990-94 (minute) DST 1957 - Present (hourly) PC 1975 - Present (15-minute) AMANAS 1959 - Present (3 hourly and daily) KMKNKS 1983 - Present (3 hourly) . ...
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Ссылки http://www.wdcb.ru/stp/welcome.shtml -- 11.9 Кб -- 18.01.2010
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18. A Simple Example With a Single Chirp Component
... In this first example, we allow an object to fall onto a small radar unit . The resulting Time-Frequency distribution is shown as a contour plot in Fig. 8 (a). Figure: FIGURE GOES SOMEWHERE IN THIS GENERAL VICINITY . ... Its density plot appears as an image in Fig. ... The response has a very high peak, as evidenced from Fig. ...
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Ссылки http://crydee.sai.msu.ru/~vab/Wavelet.rsc/Chirplet.dir/node20.html -- 3.8 Кб -- 15.04.1998
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19. http://www.iki.rssi.ru/conf/2009elw/presentations/presentations_pdf/session7/ManagadzeN_ELW.pdf
... It can · · obtain ice sample from 20 cm or deeper surface layer, then melt it and extract biomass from the ice surface water by filtration; Laser TOF MS for the measurements of element composition of the biomass; Gas TOF MS for the detection of: 1) volatile components, generated at the heating of biomass sample (closed window mode); 2) secondary ions , emitted from ice matrix by the influence of energetic magnetosphere ... Spectrum of yeast sample. ... Laser TOF MS 6. ...
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Ссылки http://www.iki.rssi.ru/conf/2009elw/presentations/presentations_pdf/session7/ManagadzeN_ELW.pdf -- 1581.2 Кб -- 02.03.2009
[ Текст ] Ссылки http://www.cosmos.ru/conf/2009elw/presentations/presentations_pdf/session7/ManagadzeN_ELW.pdf -- 1581.2 Кб -- 02.03.2009
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[ Текст ] Ссылки http://www.cosmos.ru/conf/2009elw/presentations/presentations_pdf/session7/ManagadzeN_ELW.pdf -- 1581.2 Кб -- 02.03.2009
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20. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BDE9464D1-325C-49E6-8A3A-2F90299E3BB5%7D
. This illustration shows the discovery that the outer Milky Way is a really a mixture of two distinct components rotating in opposite directions. The inner component of the Galaxy's halo spins clockwise with the galaxy's rotation at about 50,000 miles per hour. The outer component rotates counterclockwise to the galaxy at 100,000 miles per hour. SDSS-II, Masashi Chiba, Tohoku University, Japan
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BDE9464D1-325C-49E6-8A3A-2F90299E3BB5%7D -- 3.6 Кб -- 10.04.2016
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