Astronet Поиск по астрономическим сайтам English Russian
       
        Точная форма слов   О проекте   Сайты   Справка
Найдено документов: 92396 (153 сайтов) ---- Время поиска: 0.26сек.   

1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | След.

Показаны документы, содержащие фрагменты текста из документа
http://www.mrao.cam.ac.uk/ALLSMOG/Data_download/tab3.txt.

1. Comments on Individual Table Columns
... 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. ...
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/sas/6.1.0/doc/omsrclistcomb/node7.html -- 3.8 Кб -- 22.11.2004
Похожие документы
Еще в разделе: (Показать все результаты (>10038) - xmm.vilspa.esa.es/ )

2. http://www.arcetri.astro.it/irlab/luna/firpo/check.ps
... (FIRPO-TIRGO) w/error AR, Sun Aug 24 10:34:33 MET DST 1997 ############################################################# Sp:K4 irc10007 J 1.509 0.028 irc10007 J 1.65+/- 0.06 [ 0.05 ] 0.14 0.09 irc10007 H 0.961 0.006 irc10007 H 1.03+/- 0.04 [ 0.04 ] 0.07 0.05 irc10007 K 0.606 0.040 irc10007 K 0.85+/- 0.05 [ 0.03 ] 0.24 0.09 Sp:M2 irc10024 J 2.099 0.028 irc10024 J 2.31+/- 0.04 [ ...
[ Текст ]  Ссылки http://www.arcetri.astro.it/irlab/luna/firpo/check.ps -- 14.9 Кб -- 28.07.2005
Похожие документы

3. clstats
... User Guide ] Task: clstats Purpose: Calculate dispersions, masses, etc for each clump from clfind file Categories: utility The mass is calculated in the following way; we define X such that, X * (sum T) * delv = column density of molecular hydrogen in units of 10^20 cm-2 which implies that to convert to a mass, multiply by 10^20 * meanmol * m(H_2) * Area Key : in file name of data cube (no default ) ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/computing/software/miriad/doc/clstats.html -- 3.3 Кб -- 10.04.2016
Похожие документы

4. http://star.arm.ac.uk/~ambn/abstract224.html
Using Ly alpha line profiles generated from a grid of M dwarf model atmospheres we calculate the attenuation factor [i.e. Ly alpha (obs)/ Ly alpha (intrin)] due to the interstellar medium as a function of hydrogen column density. ... The major uncertainty in this work has been the interstellar hydrogen column density, emphasizing the need for further work in this area and in particular an accurate model of its variation in all directions. ...
[ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/~ambn/abstract224.html -- 1.9 Кб -- 18.09.1996
Похожие документы
Еще в разделе: (Показать все результаты (>1045) - star.arm.ac.uk/ )

5. Determination of atmospheric parameters and calculation of chemical composition
... We cannot use for this purpose equivalent widths and profiles of HI lines (well known criteria of atmospheric conditions for normal supergiants), since these lines are strongly distorted in the spectrum of IRAS04296 as seen in Fig. ... Figure: Upper: iron abundance FeI (circles) and FeII (crosses) calculated for IRAS04296+3429 with model parameters , and using lines with different excitation potentials EP of a low level; bottom: the same as a function of the equivalent width W . ...
[ Сохраненная копия ]  Ссылки http://mavr.sao.ru/hq/ssl/IRAS04296/node7.html -- 28.8 Кб -- 02.10.2012
[ Сохраненная копия ]  Ссылки http://www.sao.ru/hq/ssl/IRAS04296/node7.html -- 28.8 Кб -- 01.10.2012
[ Сохраненная копия ]  Ссылки http://jet.sao.ru/hq/ssl/IRAS04296/node7.html -- 28.8 Кб -- 01.10.2012
Похожие документы
Еще в разделе: (Показать все результаты (>715) - jet.sao.ru/ )

6. Long description of example of cell background calculation
This diagram shows the six superimposed "layers" of the CSS table model. This diagram illustrates the algorithm for calculating a cell's final background. ... The diagram shows how, looking down on the six rectangles, one may compute the background color of each cell. ... A cell without a background color in the top layer is depicted as a "window" onto the lower layers, which give its final background color. ...
[ Сохраненная копия ]  Ссылки http://crydee.sai.msu.ru/~vab/html.doc/css2/images/longdesc/tbl-layers-desc.html -- 2.3 Кб -- 02.05.1998
Похожие документы
Еще в разделе: (Показать все результаты (>478) - crydee.sai.msu.ru/ )

7. *xflux, hxflux* - Calculation of X-ray Flux
Next: *upspecrdf, downspecrdf* - Transform Up: Spectral Analysis Previous: *grid_plot* - Plot Results . The conversion of count rate to flux depends on the intrinsic spectrum of the source, so xflux must be used in conjunction with fit . Fit generates a table of the best fit intrinsic spectrum ( _int.tab extension). xflux uses this table to calculate either the integrated flux between two energy limits or the flux density at a specific energy. ... This produces ``..._obs.tab'' file. ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/PROS/PUG/node159.html -- 10.7 Кб -- 01.10.2012
Похожие документы
Еще в разделе: (Показать все результаты (>1120) - hea-www.harvard.edu/ )

8. CALSPEC
CALSPEC: 2004 June 15 . ... CDBS Files of the Flux Standards with Columns in Order of Preference(1) ------------------------------------------------------------------------------- Star name V B-V CDBS name Model STIS FOS+Oke IUE+Oke (1) (2) (3) (4) (5) (6) (7) (8) AGK+81D266 11.94 -0.34 AGK_81D266 _ STIS_001 _ 005 ALPHA-LYR 0.03 0.00 ALPHA_LYR _STIS_002 _004 BD+17D4708 9.47 0.44 BD_17D4708 _ STIS_001 BD+25D4655 9.69 -0.31 BD_25D4655 _002 BD+28D4211 10.51 -0.34 BD_28D4211 _ STIS_001 _ FOS_003 _ ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/instruments/observatory/cdbs/calspec.html -- 8.7 Кб -- 15.06.2004
Похожие документы

9. A New PROS Task for Calculating HRI Source Intensities or Upper Limits
... Next: The PROS Big Up: Software Systems Previous: Data Reduction Software . ... The srcinten task provides PROS users with a tool to compute count rates for point sources in the ROSAT High Resolution Imager (HRI). ... Corrected upper limits are cited at locations where the count rate falls below the source detection threshold. ... Srcinten is a new PROS task that computes and applies the above correction factors to the net counts in a user-specified aperture. ...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass94/chenj.html -- 11.4 Кб -- 03.11.2000
Похожие документы
Еще в разделе: (Показать все результаты (>738) - www.adass.org/ )

10. Stars proper motions in NGC7063 open cluster
... The first column gives the star identification number, followed by X, Y positions in mm. The zero point of these offsets is star number 1 which lies at 21:24:20.52 +36:30:25.6 (equator and equinox 2000). Next are relative proper motions (muX and muY) and their errors (ex and ey) in 10**4 arcsec/yr, followed by calculated V magnitudes. The final column gives the calculated membership probabilities in percent. ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/groups/cluster/cl/ngc7063/ -- 2.1 Кб -- 22.12.2007
Похожие документы
Еще в разделе: (Показать все результаты (>1153) - www.sai.msu.su/ )

11. mcfile
... The less then 5 degree value of the relative geocentric angular distance between the footprints of the SC is used as a criterion of the magnetic conjugation. ... On the last column of the file is shown the magnetic field model version ( MOD IOPT ) used during magnetic mapping. ... The difference between CMLT values of the Sat.1 and Sat.2 (see as well column 11) . ... dcorlat = dla (deg) . The difference between CORLAT values of the Sat.1 and Sat.2 (see as well column 12) . ... AnD (deg) . ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/vprokhor/descr/multcnjf.htm -- 8.0 Кб -- 21.04.2000
[ Сохраненная копия ]  Ссылки http://www.cosmos.ru/vprokhor/descr/multcnjf.htm -- 8.0 Кб -- 21.04.2000
Похожие документы
Еще в разделе: (Показать все результаты (>864) - www.cosmos.ru/ )

12. Солнечное Обозрение - Среднегодичные индексы солнечной активности NGDC
... Индексы солнечной активности . ... Наблюдения NGDC . Солнечные регионы . ... Среднегодичные индексы солнечной активности . Визуальные индексы солнечной активности по версии Национального центра геофизических данных . ... 0.06 . ...
[ Сохраненная копия ]  Ссылки http://www.alexeyryback.ru/ru/ngdc.htm -- 15.1 Кб -- 03.02.2016
Похожие документы

13. http://xray.sai.msu.ru/~ivan/gmt/man/pshistogram.html
pshistogram - Bin data and plot histograms pshistogram file -Jx xscale [/ yscale ] -W bin _ width [ -2 ] [ -A ] [ -B tickinfo ] [ -C ] [ -E azimuth / elevation ] [ -G fill ] [ -H[ nrec ] ] [ -I[o] ] [ -K ] [ -L pen ] ... [r] ] [ -S ] [ -U[ / dx / dy / ][ label ] ] [ -V ] [ -X x - shift ] [ -Y y - shift ] [ -Z type ] [ -c copies ] [ -bi[s][ n ] ] pshistogram reads the first column from file [or standard input ] and calculates ... L Draw bar outline using the specified pen thickness. ...
[ Сохраненная копия ]  Ссылки http://xray.sai.msu.ru/~ivan/gmt/man/pshistogram.html -- 7.9 Кб -- 19.03.1999
Похожие документы

14. Image Arithmetic
... AVERAGE/AVERAGE Compute simple average of all pixels in a subimage . AVERAGE/COLUMN Compute average of image columns . AVERAGE/IMAGE Calculate the average of images . AVERAGE/ROW Compute average of image rows . ... COMPUTE/COLUMN Perform arithmetic expression on image column . COMPUTE/IMAGE Compute arithmetic expression of images . COMPUTE/PIXEL Perform arithmetic operations on images using . ... COMPUTE/ROW Compute arithmetic expression on image scan lines . COMPUTE/.. ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/precise/Midas_doc/doc/95NOV/vol2/node433.html -- 3.0 Кб -- 23.02.1996
Похожие документы

15. http://www.gao.spb.ru/english/as/j2014/presentations/medvedev.pdf
... Variation of systematic errors for USNO A2 (in mas per year) 23 .914 0.082 0.250 0.418 0.586 0.753 0.921 1.089 1.257 1.425 1.593 4 4. 3. 3. 3. 3. 3. 3. 3. 3. 3. 15 ± 7± 1± 3± 3± 10 ± 10 ± 11 ± 6± 10 ± 12 ± and their errors USNO UCAC USNO UCAC A2.0 2 3 B1.0 4 (1998) (2006) (2003) (2012) 37 27 11 4 732 529 778 501 050 078 775 387 (34 610 829) (17 209 447) (9 744 401) () Distribution of observations ( ...
[ Текст ]  Ссылки http://www.gao.spb.ru/english/as/j2014/presentations/medvedev.pdf -- 697.5 Кб -- 24.11.2014
Похожие документы

16. http://www.naic.edu/~tghosh/a1863/calnotes
... Here is another interesting aspect of the A1863 data. ... The delta columns show the difference between the entries in the current row and the previous row: *AST* *Cal * *delta AST* *delta Cal * 67856 0.05 68302 0.02 446 -0.03 68749 -0.01 447 -0.03 69197 -0.04 448 -0.03 69643 -0.05 446 -0.01 70090 -0.02 447 0.02 70538 0.01 448 0.03 70985 0.04 447 0.03 71954 0.04 969 0.01 The time intervals are very evenly spaced at about 7min27sec with fairly consistent steps. ...
[ Сохраненная копия ]  Ссылки http://www.naic.edu/~tghosh/a1863/calnotes -- 3.2 Кб -- 20.04.2005
Похожие документы

17. http://zebu.uoregon.edu/~uochep/talks/talks07/cluster.pdf
... SiD workshop, Fermilab, April 9-11 2007 April 9, 2007 Nick Sinev, SiD design Workshop, Fermilab 1 Topics 1. ... What and how was simulated What and was One column clusters effects Accepted background density Hit reconstruction efficiency Hit efficiency How to improve efficiency Conclusions April 9, 2007 Nick Sinev, SiD design Workshop, Fermilab 2 What is this April 9, 2007 Nick Sinev, SiD design Workshop, Fermilab 3 Marty's idea Shift charge in neighboring columns in opposite directions. ...
[ Текст ]  Ссылки http://zebu.uoregon.edu/~uochep/talks/talks07/cluster.pdf -- 591.4 Кб -- 28.06.2007
Похожие документы

18. Отчет Золотухина Ивана (лето 2001г.)
... ОТЧЕТЫ СТУДЕНТОВ О ПРАКТИКЕ В САО . Лето 2001 года . ОТЧЕТ . ... Золотухина Ивана . ... 0.07 . ...
[ Сохраненная копия ]  Ссылки http://heritage.sai.msu.ru/otchet/leto2001/Zolotuhin/Zolotuhin3.html -- 62.0 Кб -- 11.05.2007
Похожие документы
Еще в разделе: (Показать все результаты (>27) - heritage.sai.msu.ru/ )

19. Vertical Structure, figures
... R P is the perigalactic radius and R a , the apogalactic radius. Z max is the maximum deviation of the star from the Galactic plane. THe dotted curve shows the position of the Galactic plane. The hatched horizontal band shows schematically the band in Z , where the probability of that location of the star was calculated. The vertical band shows the width of the column in which we reconstruct the star distribution in Z . ... next figure | previous figure . ...
[ Сохраненная копия ]  Ссылки http://ip.rsu.ru/~marsakov/paper2/p2fg4_1.htm -- 2.3 Кб -- 02.02.2007
Похожие документы
Еще в разделе: (Показать все результаты (>54) - ip.rsu.ru/ )

20. DUST: Dust::AttSlab Class Reference
... Classes . ... Class List . Class Hierarchy . Class Members . Dust :: AttSlab . include < attslab.hxx > . Collaboration diagram for Dust::AttSlab: . ... AttSlab ( RadField *InputRF, BNLib::UnaryDD *AbsXSect) . RadField * . MkRF (double n) . Calculate the attenuated radiation field as a function of column density . RadField * Dust::AttSlab::MkRF . double . ... Return the radiation field at column density n into the slab . ... attslab.hxx . attslab.cxx . ...
[ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/~bn204/devman/dust/classDust_1_1AttSlab.html -- 5.0 Кб -- 11.07.2008
Похожие документы

1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | След.


Астронет | Научная сеть | ГАИШ МГУ | Поиск по МГУ | О проекте | Авторам

Комментарии, вопросы? Пишите: info@astronet.ru или сюда

Rambler's Top100 RFBR Яндекс цитирования