October 14, 2002 (Monday) David Jackson, Rutherford Appleton Lab, UK . ... Fall 2000 . ... The resolution obtained is compared with the starting point, based on an optical survey, and is shown to achieve the design performance. 4:00 pm, 472 Willamette Hall . return to top . ... Amplitude analysis of the D + , D s + decays to KK p and D 0 decay to K s KK are presented using the data collected by Fermilab High Energy Photoproduction Experiment E831(FOCUS). 2:30 pm, 472 Willamette Hall . ...
... Gravitational wave search provides insights into galaxy evolution and mergers . ... galaxies . ... The double star 54 Leonis, spiral galaxy NGC 3198, and emission nebula NGC 3199 . ... Cosmic Adventures . ... A trick of perspective т?? chance alignment mimics a cosmic collision . ... While the two galaxies look as if they are in the midst of a collision, this is in fact a trick of perspective т?? the two just happen to appear in the same direction from our vantage point. ... Cosmic Origins . ...
... Indiana Jones is a registered trademark of Lucasfilm Ltd. ... There's the intrigue of the megaliths of Stonehenge, the ancient pyramids of Egypt, the earthen figures of Britain and Peru, and the bloody rituals of the Maya. ... To make sense of these great structures and sophisticated concepts, archaeologists and astronomers have pooled their talents. ... People could use these alignments to synchronize their calendars or track the exact path of a celestial object. ... Maya glyphs of Venus. ...
. Measuring/adjusting the secondary/tertiary with videogrammetry: . Place reflectors on each panel of the secondary/tertiary and then take pictures using videogrammetry. Back fit for the camera position and then find the position of each panel (angles only). Adjust each panel by turning the vertical adjustment screws at each panel corner. Iterate the measurement and adjustment. Results: . Secondary panel alignment .5 mm rms . Tertiary panel alignment .4 mm rms next previous
OptInt PmWiki : MROI Fast Tip Tilt / Tech Meet 10 . The objective of this meeting was to decide which *one or two* layouts from the four candidates (OAP, DLT, Zoom, DT - see TechMeet6 ) should be identified as preferred in the CoDR document. Taking into account at least the following: . ... If we reduce the focal length, this layout allows the baseplate to be pinned close to the camera. ... Printable View of http://www.mrao.cam.ac.uk/projects/OAS/pmwiki/pmwiki.php/MROIFastTipTilt/TechMeet10) ...
... The computer is set up so that the software for whatever camera is running and the switch box set to channel B. This allows the monitor and keyboard upstairs to operate the computer. Now the telescope can be set up. ... In the North west of the dome, there is a motor that turns the dome. The dome opens with a motor that pulls the slit back. ... Each camera had a specific alignment with the telescope. ... The lights on the roof provide a nice target to center in all three telescopes. ...
эффектов галактических и солнечных космических лучей методом наземного мониторинга ' в рам ках программы фундаментальных исследований Президиума Российской академии наук ?6 Нейтринная физика за 2006 г. В результате выполнения данного проекта осуществлялась непрерывная регистрация интенсивности КЛ на Саянском спектрографическом ... Известия РАН, серия физическая (в печати). ... Координатор http :// www . ...
Michele Bannister . Other research . ... The mutual events of Haumea . The dwarf planet Haumea is the parent of a collisional family that includes its two moons, Hi'iaka and Namaka. ... The arid and windswept McMurdo Dry Valleys of Antarctica are carpeted with the polygons of patterned ground , a geological formation that is also seen on the northern plains of the planet Mars. ... I worked to understand the influence that buried masses of ice have on the development of patterned ground. ...
... Class . ... Here is an example applet tag that launches ImageJ as an applet and passes it the URLs of two images: <applet archive="../ij.jar" code="ij.ImageJApplet.class" width=0 height=0> <param name=url1 value="http://rsb.info.nih.gov/ij/images/FluorescentCells.jpg"> <param name=url2 value="http://rsb.info.nih.gov/ij/images/blobs.gif"> </applet> To use plugins, add them to ij.jar and add entries to IJ_Props.txt file (in ij.jar) that will create commands for them in the Plugins menu, or a submenu. ...
Next: Status of the BIMA Image Pipeline . ... We describe all the steps of the standard reduction including per pixel error propagation: Bias correction, treatment of bad pixels, flatfielding, and filtering of cosmic ray events. ... We build difference images via image convolution with a technique called OIS (optimal image subtraction, Alard & Lupton 1998), proceed with PSF-fitting, relative photometry on all pixels and finally apply an automatic detection of variable sources. ...
Lessons learned from the Thirty Meter Telescope site testing Tony Travouillon Sebastian Els, Angel Otarola, Reed Riddle, Matthias Schoeck, Warren Skidmore TMT.XXX.PRE.05.0XX.DRF01 1 Introduction TMT and its Site testing. Important choice before going on site. ... Considerations during analysis of the data. TMT.XXX.PRE.05.0XX.DRF01 2 Some Background about the TMT Site Testing TMT is a 30m, segmented, RitcheyChretien telescope design. ... ASCA Cloud Cover Analysis So how do we do it in practice? ...
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Ссылки http://site2010.sai.msu.ru/static/doc/TTravouillon_TMT_site_testing_site2010.pdf -- 2354.3 Кб -- 18.10.2010 Похожие документы
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