Найдено документов: 383023 (185 сайтов) ---- Время поиска: 0.88сек. |
Показаны документы, содержащие фрагменты текста из документа
http://www.2dfquasar.org/Papers/Dunk/wedge.html.
http://www.2dfquasar.org/Papers/Dunk/wedge.html.
1. Dunk Proceedings - 2dF QSO Redshift Survey (Completeness)
. | Front page | . | << - Number counts | Contamination - >> | . Robert J. Smith, ">rsmith@mso.anu.edu.au Last modified: Fri Sep 24 11:39:02 EST 1999 .
[
Сохраненная копия
]
Ссылки http://www.2dfquasar.org/Papers/Dunk/completeness.html -- 2.0 Кб -- 24.09.1999
Похожие документы
Похожие документы
2. http://www.stsci.edu/spst/UnixTransition/doc/get_by_cycle.py
... Otherwise, output will go to the screen. ... The -excluded_lrps will exclude proposals or visits from proposals that are in the listed LRPS. ... defaults to pi,implenetation,scheduling,completed when exetime is specified. allowed_options = [' proposals ', ' visits ', ' output =', 'detail', 'status=', 'types=', ' excluded_lrps =', ' scenario _name=', 'exectime' ] try: options, parms = spst_getopt.spst_getopt(args, allowed_options) except Exception,e: print e ...
[
Сохраненная копия
]
Ссылки http://www.stsci.edu/spst/UnixTransition/doc/get_by_cycle.py -- 8.7 Кб -- 28.02.2014
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>21310) - www.stsci.edu/ )
3. FIRPO Help 5
Last modified on March 19, 1997 by A. Richichi . ADC cards and filter/clock box. The ADC card traditionally used with FIRPO I at CA has been used also for FIRP OII in Russia. ... At the same time, the new PCMCIA ADC card (DASCard 1000) has been succesfully installed on the TM-5000 notebook, and used for instance to record the Alpha Tau occultation at Arcetri on March 14, 1997. ... In der Filter/Clock Box war durch den Transport die Leiterplatte abgegangen und hatte einige Kontakte abgerissen. ...
[
Сохраненная копия
]
Ссылки http://www.arcetri.astro.it/irlab/luna/firpo/firpo_message5.html -- 4.9 Кб -- 28.07.2005
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>9413) - www.arcetri.astro.it/ )
4. Kp Index: Classification of Days
The selection of the quietest days (Q-days) and most disturbed days (D-days) of each month is deduced from the Kp indices on the basis of three criteria for each day: . ... In order to indicate such a situation, selected days which do not satisfy certain absolute criteria are marked as follows. ... A selected disturbed day is considered not really disturbed and marked by an asterisk ( * ) if Ap less than 20. ... January 2000 - recent . January 1990 - December 1999 . ...
[
Сохраненная копия
]
Ссылки http://www.iki.rssi.ru/magbase/REFMAN/KP_INDEX/quietdst/index.htm -- 5.0 Кб -- 21.12.2007
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>1178) - www.iki.rssi.ru/ )
5. Designated Observatory Registry
The Astronomical Society of Australia has been asked by STANDARDS AUSTRALIA to compile a list of "designated" optical observatories that are valuable resources for (i) research, (ii) education and (iii)community use. The ASA is the final arbiter of whether any particular observatory is so designated. ... Status as a designated observatory will be reviewed every 2 years based on calendar year annual reports submitted in January. ... phone: 02 6125 0268 . ... Registry Number . ... Number of nights . ...
[
Сохраненная копия
]
Ссылки http://www.mso.anu.edu.au/~bessell/DOrep.html -- 9.3 Кб -- 01.10.2012
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>940) - www.mso.anu.edu.au/ )
6. VSOP Observation codes
... Observation codes for VSOP General Observing Time observations have the form . ... The first letter indicates which AO period the observation was proposed in: the letter `v' indicates the first AO period, and the letter `w' indicates the second and third AO periods. The three digits indicate the proposal number. ... For proposals with more than 26 experiments (see next item), 300 is added to the proposal code for the 27th and subsequent experiments. ...
[
Сохраненная копия
]
Ссылки http://www.atnf.csiro.au/pub/people/vlbi/vsop/www/Obscodes.html -- 4.2 Кб -- 26.12.2007
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>36535) - www.atnf.csiro.au/ )
7. http://xmm.vilspa.esa.es/sas/8.0.0/doc/ommag/ChangeLog
... Version 3.4.5 - 2005-06-28 (CB) ------------------------------- Ammended routine ommagnitude_mod in mssllib to set default polynomial coefficents to 1.0 and 0.0 (fixes SPR 3483 - mssllib version 2.43.12 has this fix) Also replaced source-list file in test directory with a more recent one to fix problem of negative magnitudes which cause a test-failure on one system. ... Adds a new column for the former correction. ... Version 2.2.2 2002-02-15 (CB) DEPEND file ammended to fix SPR 2757. ...
[
Сохраненная копия
]
Ссылки http://xmm.vilspa.esa.es/sas/8.0.0/doc/ommag/ChangeLog -- 9.1 Кб -- 06.05.2008
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>9799) - xmm.vilspa.esa.es/ )
8. The Modified Gauss--Newton Method.
Next: The Quasi--Newton Method. Up: Outline of the Previous: The Newton--Raphson Method. ... At each iteration, one computes . ... Neglecting the second derivatives matrix , we obtain the ``normal equations'' and the Gauss--Newton direction . This so--called Gauss--Newton method is intended for problems where is small. ... The algorithm implemented here is a modification of that Gauss--Newton method, that allows convergence even for rank deficient Jacobians or for large residuals. ...
[
Сохраненная копия
]
Ссылки http://www.sao.ru/precise/Midas_doc/doc/94NOV/vol1/node125.html -- 4.8 Кб -- 23.02.1996
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>3231) - www.sao.ru/ )
9. Bias-Free Parameter Estimation with Few Counts, by Iterative Chi-Squared
... We demonstrate through numerical simulations that model parameters estimated with our technique are essentially bias-free, even when the average number of counts per bin is 1. ... The IW technique avoids such biases by estimating through successive iterations, where for each iteration, j, , and the best-fit parameters are determined by minimization of . ... In our sample, we find that the minimum values and best-fit parameters converge after about 6 iterations. ...
[
Сохраненная копия
]
Ссылки http://www.adass.org/adass/proceedings/adass94/kearnsk.html -- 12.3 Кб -- 03.11.2000
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>1795) - www.adass.org/ )
10. http://hea.iki.rssi.ru/conf/hea2007/internal/templates/atom_item.tpl
<entry> <id><?=$link?>?id=<?=$number?>&db=<?=$db?></id> <author><?=$author?></author> <issued><?=$dbtime?></issued> <modified><?=$dbtime?></modified> <link rel="alternate" type="text/html" href="<?=$link?>?id=<?=$number?>&db=<?=$db?>" /> <title><![CDATA[<?=$title?>]]></title> <content type="text/html" mode="escaped"><![CDATA[<?=$abstract?>]]></content> </entry>
[
Сохраненная копия
]
Ссылки http://hea.iki.rssi.ru/conf/hea2007/internal/templates/atom_item.tpl -- 1.4 Кб -- 26.07.2007
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>992) - hea.iki.rssi.ru/ )
11. The Chandra Multiwavelength Project (ChaMP) - Science Goals
. Expect ~40 clusters, ~16 with z>0.5 . Home | Science Goals | Survey Strategy | Publications | Images & Data | Education/Outreach | Internal Page (password access only) . Date Last Modified: 22 April 2002 . Contact: Webmaster .
[
Сохраненная копия
]
Ссылки http://hea-www.harvard.edu/CHAMP/SCIENCE_GOALS/clusters.html -- 2.7 Кб -- 01.10.2012
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>4313) - hea-www.harvard.edu/ )
12. DIS Keywords
For all keywords that contain a red and a blue value, the blue value comes first. ... The full pathname, but without the trailing "b.fit" and "r.fit", that would be given to the next exposure if the basename argument is not given to the expose command. ccdHeaters=float,float . ... bluelambda2=float [M] . The center wavelength for the given grating: the 1 or 2 indicates the grating bay. The bluelambda and redlambda keywords match one set of these, depending on the position of the turret. ...
[
Сохраненная копия
]
Ссылки http://www.apo.nmsu.edu/35m_operations/DIS/DIS_Keywords.html -- 12.6 Кб -- 23.04.2003
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>728) - www.apo.nmsu.edu/ )
13. idl routines to look at dewar temps
... DWTEMPALL - INPUT ASCII DATA FROM RMALL ROUTINE. DWTEMPINP - INPUT DEWAR TEMPS FOR A YEAR . DWTEMPPLOT - PLOT DEWAR TEMPERATURES. ... EXAMPLES: To start idl: idl @phil @dwinit then print,dwtempinp(d) .. input all the data for current year print,dwtempinp(d,rcv='lbw') .. input current year lband wide only print,dwtempinp(d,year=2001,rcv='lbn') .. input lbn for year 2001 SEE ALSO: dwtempplot - to plot the data . ... DESCRIPTION: Plot the receiver dewar temperature data versus day of year. ...
[
Сохраненная копия
]
Ссылки http://www.naic.edu/~phil/dwtempdoc.html -- 9.0 Кб -- 02.02.2016
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>5885) - www.naic.edu/ )
14. http://www.eso.org/projects/dfs/team/QA-code-review-form.doc
... Readability |Check number: 1 | Description: Header existence for each |Evaluation (always/often/sometimes/| |source file and for each method, class, |never) : | ... Description: Naming conventions existence |Evaluation (always/often/sometimes/| |(variables start with lowercase, then |never) : | ... limited and commented |(always/often/sometimes/ | ... Description: Error message are formated : when an|Evaluation | error or an exception is raised, report the |(always/often/sometimes/ | ...
[
Текст
]
Ссылки http://www.eso.org/projects/dfs/team/QA-code-review-form.doc -- 128.5 Кб -- 29.09.2003
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>53993) - www.eso.org/ )
15. CurveFitter (ImageJ API)
... public class CurveFitter . ... static int . ... Field Detail public static final int STRAIGHT_LINE . ... public static final int POLY2 . ... public static final int POLY3 . ... public static final int POLY4 . ... public static final int EXPONENTIAL . ... public static final int POWER . ... public static final int LOG . ... public static final int RODBARD . ... public static final int GAMMA_VARIATE . ... public static final int LOG2 . ... public static double f (int fit, double[] p, double x) . ...
[
Сохраненная копия
]
Ссылки http://www.astro.louisville.edu/software/astroimagej/imagej/api/ij/measure/CurveFitter.html -- 34.8 Кб -- 02.12.2010
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>1496) - www.astro.louisville.edu/ )
16. Sunspots and active regions September 09, 2015
... Sun images . ... Sun flares . ... Active areas . September : 2015 . ... The following regions with sunspots can be now observed on the Sun's surface . Group number . ... Group length (in degrees) . ... Coordinates and other characteristics of active regions are issued for September 09, 2015 00:31 UT The following H-alpha plages without spots can be currently observed on the Sun's surface . ... Coordinates and other characteristics of active regions are issued for September 09, 2015 00:31 UT . ...
[
Сохраненная копия
]
Ссылки http://www.tesis.lebedev.ru/en/active_areas.html?m=9&d=9&y=2015 -- 23.4 Кб -- 11.04.2016
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>3407) - www.tesis.lebedev.ru/ )
17. http://www.izmiran.rssi.ru/~ichertok/CHAINS/ANNOUNC/971216.htm
December 16, 1997 . ... An example of the EUV chain revealed by the modified SOHO/EIT images. A complex EUV (195 A) chain or thread of December 16, 1997, consisting of several quasi-straight-line fragments between points 1-2-3-4-5 and covering a large part of the solar disk. ... A comparison of the large-scale chains and threads on two pairs of the modified SOHO/EIT (195 A; inverted) and He I (10830 A; normal) images. ... SOHO/EIT, 195 A, December 15-17, 1997 GIF Animation (1.07 MB) . ...
[
Сохраненная копия
]
Ссылки http://www.izmiran.rssi.ru/~ichertok/CHAINS/ANNOUNC/971216.htm -- 3.9 Кб -- 02.04.1999
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>632) - www.izmiran.rssi.ru/ )
18. Active To Do List
. Number . Task . Pri . Author . Created By Tool . Created On . Modified On . Completed . Modified By . Assigned To . Link To . Magic . Description
[
Сохраненная копия
]
Ссылки http://www.mrao.cam.ac.uk/~nima/_vti_pvt/_x_todo.htm -- 1.5 Кб -- 06.02.2006
[ Сохраненная копия ] Ссылки http://www.schools.keldysh.ru/sch725/_vti_pvt/_x_todo.htm -- 1.5 Кб -- 11.03.2006
Похожие документы
[ Сохраненная копия ] Ссылки http://www.schools.keldysh.ru/sch725/_vti_pvt/_x_todo.htm -- 1.5 Кб -- 11.03.2006
Похожие документы
Еще в разделе:
(Показать все результаты (>2) - genphys.phys.msu.su/ )
19. Search by subdirectory on archive XFree86/OS2
Search engine provided by WebGlimpse . String to search for: . ... Return only files modified within the last days. Maximum number of files returned: 10 50 100 1000 . Maximum number of matches per file returned: 10 30 50 500 . Maximum number of characters output per file: . ... sorted by author . sorted by date . sorted by subject . ...
[
Сохраненная копия
]
Ссылки http://crydee.sai.msu.ru/ftproot/pub/comp/os/os2/xfree86os2/html/xf86search.html -- 3.4 Кб -- 23.10.2000
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>4896) - crydee.sai.msu.ru/ )
20. Hot subdwarfs
Hot subdwarfs are hots stars with masses somewhat less than that of the Sun. ... They are known as sdB stars because their spectra are dominated by hydrogen lines. ... Normally, a red giant will switch on core helium burning without losingthe layers of hydrogen around the helium core. sdOB stars are related to sdB stars, possibly being the sdB stars which have completed core helium burning and are evolving to become white dwarfs. ... Such stars are known as PG1159 stars and DO white dwarfs. ...
[
Сохраненная копия
]
Ссылки http://star.arm.ac.uk/~csj/research/subdwarfs.html -- 6.8 Кб -- 12.06.2002
Похожие документы
Похожие документы
Еще в разделе:
(Показать все результаты (>3195) - star.arm.ac.uk/ )
Астронет | Научная сеть | ГАИШ МГУ | Поиск по МГУ | О проекте | Авторам
Комментарии, вопросы? Пишите: info@astronet.ru или сюда