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1. spectrometer counts to kelvins
... Avg: the average value of the spectra (maybe throwing out some channels at the edges). <>:average over the spectra (throwing out points at the edges if you want). gCal(f) :- frequency dependence of the tabulated cal values. ... calInK(Avg): Scaler cal value averaged over the band. calOffSpc(Avg): cal off value averaged over the band (in spectrometer counts) . ... cntsToK(avg) = calInK(Avg) / (calDif_cnts(Avg)) . To convert a spectrum b_cnts in spectrometer counts to b_K in Kelvins using cntsToK: . ...
[ Сохраненная копия ]  Ссылки http://www.naic.edu/~phil/cals/spectrometerCntsToKelvins.html -- 19.1 Кб -- 12.06.2014
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2. XWare > APOD
... In 1572, Danish astronomer Tycho Brahe recorded the sudden appearance of a bright new star in the constellation Cassiopeia. ... Occasionally, a planet in our Solar System will pass in front of a bright star. ... Two months ago, however, Pluto and its large moon Charon passed in front of a comparatively bright triple star system known as P126. ... The picture is actually composed from two images recorded weeks apart by the Voyager 2 spacecraft during its visit to the Saturnian System in August of...
[ Сохраненная копия ]  Ссылки http://www.astronet.ru/db/xware/apod.html?page=88&d=2005-01 -- 15.7 Кб -- 12.04.2016
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3. NEAR recorded on 23 January 1998(frame 1)
Main Sections LabIR main page . ... On January 23, 1998 the space probe NEAR was on its way to its closest approach to Earth. ... However, we were able to record a series of images of the space probe shortly before the sunglint event, and we have assembled them into a movie. At the TIRGO observatory, an observation of the space probe NEAR was organized for the night of January 22-23, 1998. ... We show here a preliminary movie (MPEG format, 412kb) made from 74 frames, each lasting 5 seconds. ...
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/irlab/luna/news/near/near2.php -- 10.2 Кб -- 04.02.2013
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4. Author Query Results
... Date . ... Authors . ... 1.000 . ... Kniazev, Alexei Y.; Grebel, Eva K.; Pustilnik, Simon A.; Pramskij, Alexander G.; Kniazeva, Tamara F.; Prada, Francisco; Harbeck, Daniel . Low Surface Brightness Galaxies in the Sloan Digital Sky Survey. ... 08/2001 . ... V. The fifth list of 161 galaxies . ... IV (Kniazev+, 2001) . ... Email results to: . ... Return:  Results  Form for manual query . ... Databases queried: Astronomy/Planetary Authors: KNIAZEVA, T Start date: 00/1990 End date: 03/2004 . ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/precise/Laboratory/Publications/tkn_list.html -- 23.7 Кб -- 18.03.2004
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5. Disk Recording
... ATNF Home . About ATNF . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Australia Telescope User Committee . ... Astrophysics graduate student programs . ... Australian Square Kilometre Array Pathfinder . Murchison Radio-astronomy Observatory . ... Parkes radio telescope . Australia Telescope Compact Array . ... Visiting Parkes radio telescope . Visiting Australia Telescope Compact Array . ... Parkes radio telescope webcam . ... LBA Disk Recording . ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/vlbi/evlbi/recorder/troubleshooting.html -- 48.6 Кб -- 08.04.2016
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6. http://www.stsci.edu/documents/dhb/webvol2/c07_foserrors.fm12.html
... The fundamental internal FOS time interval is an FOS clock tick of 7.8125 ?sec duration, which is equal to 8 ticks of the HST 1.024 MHz clock. ... The engineering telemetry did record the so-called LINESTART time; that is, the precise time when the SDF told the FOS to commence sending data from the FOS memory to the SDF. ... FOS engineering telemetry, available only at STScI, provides all timing information at accuracy of FOS clock (7.8125 ?sec). ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/documents/dhb/webvol2/c07_foserrors.fm12.html -- 8.0 Кб -- 10.02.1998
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7. NPOI Lab
The visibility amplitude bias (there is also a closure phase bias, but this one is nominally corrected by the raw data averaging pipeline) is related to non-Poisson detector statistics due to after-pulsing, and to fixed pattern noise due to non-linearities in the modulation stroke. We determine the bias using so-called incoherent scans, which record data even though the delay lines are deliberately set away from the white light fringe. ... Averaging triple products.. ... Background data loaded. ...
[ Сохраненная копия ]  Ссылки http://www.eso.org/~chummel/oyster/lab/bias6.html -- 4.7 Кб -- 26.11.2007
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8. ...for the most difficult/finickity/unbelievable recorded/verified observation
. Search this album . Gallery . :: Public Events . :: Opening of Canberra Astronomical Soc's nтАж . :: ...for the most difficult/finickity/unbelievaтАж . Sidebar Left . Sidebar Top . No Sidebar . Sidebar Bottom . Sidebar Right . View full size . Title: ...for the most difficult/finickity/unbelievable recorded/verified observation of the year . File name: CAS_XmasGrand_Opening_2004_055.jpg . Dimensions: 504 x 378 px . Page: 1 2 15 16 17 18 19 20 21 22 23 24 . Powered by Gallery 3.0.9 (Chartres) . Login
[ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/gallery3/index.php/publicEvents/album45/CAS_XmasGrand_Opening_2004_055 -- 18.6 Кб -- 11.04.2016
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9. Рекорды и рекордсмены / Азбука астрономии
... Главная Астрономия Фотографии Рекорды Форум Гостевая книга . Азбука . ... Обмен кнопками/баннерами в самом . ... Азбука звездного неба / Рекорды и рекордсмены . ... Самая большая планета . Самая маленькая планета . Самая яркая планета . ... Планета с самым большим количеством лун . Самая большая луна . ... Самая большая группа солнечных пятн . ... Самая большая звезда . ... Самая яркая звезда . Звезда с самой большой светимостью . ... Звезда с самым большим собственным движением . ...
[ Сохраненная копия ]  Ссылки http://www.astro-azbuka.info/records -- 34.5 Кб -- 09.04.2016
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10. Venus transit as seen in NYC (previosly recorded) - стр. 2 - Астрономия и
... Общероссийская неделя "Астрономия на тротуаре" - 15-17 апреля . ... Практическая астрономия ? Астрономия и компьютеры (Модераторы: Deimos , Ed_Vazhorov ) ? Venus transit as seen in NYC (previosly recorded) . ... Ответ #20 : 15.06.2004 [08:40:32] ? ... Цитата: SergeyZ от 15.06.2004 [08:40:32] Братцы! ... Последнее редактирование: 15.06.2004 [13:04:40] от Vladimir Nebotov ? ...
[ Сохраненная копия ]  Ссылки http://www.astronomy.ru/forum/index.php/topic,5631.20.html -- 38.9 Кб -- 09.04.2016
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11. TESIS has recorded new sizeable mass ejections from the Sun's atmosphere
... One of this year's largest mass ejections from the Sun's atmosphere was recorded last Sunday by TESIS telescopes aboard the CORONAS-PHOTON satellite ( video - wmv 4.3 MB ). ... Over the course of a week, two gigantic solar prominences were simultaneously ejected from the surface of the Sun. ... Earth will not feel the Sun's influence either. ... The TESIS observatory ї TESIS: www.tesis.lebedev.ru . ... One of this year's largest mass ejections from the Sun's atmosphere (movie WMV, 4.3 MB) . ...
[ Сохраненная копия ]  Ссылки http://www.tesis.lebedev.ru/en/info/mass_ejection_20090614_en.php -- 10.4 Кб -- 01.10.2012
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12. APOD: 2015 May 14 - Dwarf Planet, Bright Spot
... 2015 May 14 . Dwarf Planet, Bright Spot . Image Credit: NASA , JPL-Caltech , UCLA , MPS/DLR/IDA . Explanation: Now at Ceres, Dawn's camera recorded this closer view of the dwarf planet's northern hemisphere and one of its mysterious bright spots on May 4. ... Imaged by Hubble in 2004 and then by Dawn as it approached Ceres in 2015, the bright spot itself is revealed to be made up of smaller spots of reflective material that could be exposed ice glinting in the sunlight. ... About APOD | ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/apod/ap150514.html -- 5.2 Кб -- 10.04.2016
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13. Why Asteroid 2008 TC3 Represents a Landmark - Dr David Asher, from Armagh
... A hundred years later, a handful of Tunguska-sized asteroids have been spotted by telescopes, but most remain unseen. The asteroid designated 2008 TC3 , which made the news on October 6th before colliding with the Earth on October 7th was too small to constitute a part of the "Earth impact hazard". ... 2008 TC3, for example, finally exploded in the atmosphere above Sudan . ... Wednesday, 8 October 2008 01:15 . International Year of Astronomy, Ireland National Node . ...
[ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/scholars/iya/news/asteroid_2008_tc3.html -- 14.0 Кб -- 31.12.2009
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14. Description
... rgsregions defines and constructs the various RGS event-selection regions, and adds them to the source list (see rgssources ). ... Image regions and the background region refer to the plane of dispersion versus cross-dispersion ( image plane ) and select events based on their spatial coordinates. ... The order regions refer to the plane of dispersion versus calibrated pulse-height ( energy plane ) and select events from a specific astrophysical source within a particular reflection order. ...
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/sas/5.4.1/doc/rgsregions/node3.html -- 11.1 Кб -- 10.01.2003
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15. Low Surface Brightness Galaxy Gallery
In this gallery are many images of Low Surface Brightness Galaxies which have recently been discovered and analyzed. ... The central surface brightness of this galaxy is 24.28 . Malin 2 This galaxy is another huge disk galaxy with a scale length of 15 kpc and a redshift of 15000 km/a. The high surface brightness knot in one of its spiral arms actually has the same color, luminosity and H-alpha equivalent width as the entire Large Magellanic Cloud . ... Truly it is a Low Surface Brightness Galaxy. ...
[ Сохраненная копия ]  Ссылки http://zebu.uoregon.edu/sb2.html -- 4.8 Кб -- 26.05.2000
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16. Recorder (ImageJ API)
... public static void record (java.lang.String method, int a1, int a2, int a3) . ... public static void record (java.lang.String method, java.lang.String args, int a1, int a2) . public static void record (java.lang.String method, int a1, int a2, int a3, int a4) . public static void record (java.lang.String method, int a1, int a2, int a3, int a4, int a5) . public static void record (java.lang.String method, java.lang.String path, java.lang.String args, int a1, int a2, int a3, int a4, int a5) . ...
[ Сохраненная копия ]  Ссылки http://www.astro.louisville.edu/software/astroimagej/imagej/api/ij/plugin/frame/Recorder.html -- 49.6 Кб -- 02.12.2010
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17. Results
Next: References Up: On the problem of Previous: The spectrograph design and . Figure: Fragment of the echelle spectrum of protoplanetary nebula RAFGL 618 in H . In Fig. 3 are shown fragments of the echelle spectra of the quasar S5 0014+81 ( ) obtained with the PF echelle spectrograph within the frames of the programme of study of absorption spectra of bright quasars (authors of the programme are D.A.Varshalovich and A.V.Ivanchik). ...
[ Сохраненная копия ]  Ссылки http://mavr.sao.ru/hq/ssl/PFES/node5.html -- 5.5 Кб -- 02.10.2012
[ Сохраненная копия ]  Ссылки http://www.sao.ru/hq/ssl/PFES/node5.html -- 5.5 Кб -- 01.10.2012
[ Сохраненная копия ]  Ссылки http://jet.sao.ru/hq/ssl/PFES/node5.html -- 5.5 Кб -- 01.10.2012
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18. ASP: Monster Comet Promises Big Show
... Its perihelion would occur on April 1, 1997, at which point the comet would be only 0.92 astronomical units from the Sun, just within the orbit of Earth. ... Taken in April 1993, the photo showed the comet over 13 astronomical units from the Sun, well beyond the orbit of Saturn. ... Hale, as in Comet Hale-Bopp, has written a book, Everybody's Comet (available through the ASP Catalog) and coordinated an Internet project, "Hale-Bopp: Live in the American Classroom." ... Anatomy of a comet. ...
[ Сохраненная копия ]  Ссылки http://www.astrosociety.org/edu/publications/tnl/36/comet3.html -- 11.6 Кб -- 02.10.2012
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19. Detection of unique bright radio flare of X-ray binary
... The Galactic low-mass X-ray binary GS 2023+338 was discovered during the burst on May 22, 1989 with the Japanise satellite Ginga (aka Galaxy). The flux reached 17 crabs (this unit of flux measurement is an bright X-ray source, Crab Nebula) at 10-35 keV. ... No other radio telescope worldwide carried out multi-frequency measurements. ... Upon 14 days the radio flux fell below the detection level at the RATAN-600 in relation to the decrease of the X-ray flux. ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/Doc-en/SciNews/2016/Trushkin/ -- 8.4 Кб -- 10.04.2016
[ Сохраненная копия ]  Ссылки http://mavr.sao.ru/Doc-en/SciNews/2016/Trushkin/ -- 8.4 Кб -- 10.04.2016
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20. Chandra Supernova Remnants Catalog - Instrumental Artifacts
True Color Image Gallery: Galactic SNR | Magellanic Cloud SNR . ... Chandra Proposer's Guide pile up section ] During frame readout, the ACIS CCDs take 40 microsec to (parallel) transfer the charge by one pixel. As a result of this, each frame readout, each pixel is exposed for 40 microsec to a source (plus cosmic X-ray background) at each location along its column. ... Note also that the image does not just trail, it extends along the whole column. ... Chandra Supernova Remnant Catalog . ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/ChandraSNR/note_artifacts.html -- 5.0 Кб -- 01.10.2012
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