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1. Tilt and Sag Coefficients: 14 Apr 2000
On April 14, 2000 UT a series of Shack-Hartmann measurements were made at varying altitudes. ... The tilts and sags shown are those given by the normal Shack-Hartmann analysis. ... Without this feedback, off-telescope tests showed positioning errors on the order of 10 arcseconds in the secondary mirror position. ... Tilt M2 Bk by X" . ... The coefficients m1 through m3 need to be added to those that are currently in the TCC to correct for the secondary translation with respect to the primary. ...
[ Сохраненная копия ]  Ссылки http://www.apo.nmsu.edu/users/morgan/APO/SH_measurements/altitude.sweeps/apr.14.00.init_meas/report.html -- 9.8 Кб -- 29.03.2003
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2. FIRPO Zero Points
Main Sections LabIR main page . ... 1.2 m. 2.2 m. --------------------------- ------------------------------ J H K L J H K JUN 93 0.8 0.9 0.6 20 DEC 93 1.10 1.43 0.94 0.20 22 DEC 93 1.15 0.81 23 DEC 93 1.40 1.45 1.00 0.58 18 FEB 94 1.30 1.25 0.95 0.44 16 JUL 94 4.1 24 OCT 94 6.5 6.8 4.1 25 OCT 94 5.6 6.0 3.8 JAN 95 0.5 0.52 0.35 OCT 95 8.7 5.4 JUN 96 1.87 1.70 1.18 (note: new feedback) AUG 96 20 SEP 96 0.79 0.72 0.55 (yet another feedback, 70cm clear mirror) 24 SEP 96 0.87 0.77 0.57 .. ...
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/irlab/luna/firpo/firpo_zp.php -- 9.1 Кб -- 03.02.2013
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3. Western end of main hall, now clear.
... Gallery . ... Western end of main hall, now clear. Sidebar Left . Sidebar Top . No Sidebar . Sidebar Bottom . Sidebar Right . ... Title: Western end of main hall, now clear. Description: NOTE: All images and movies are copyright and must not be reproduced or mirrored in any form without written permission. ... NOTE: All images and movies are copyright and must not be reproduced or mirrored in any form without written permission. Powered by Gallery 3.0.9 (Chartres) . ...
[ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/gallery3/index.php/reconstruction/album36/DSCN1064 -- 31.0 Кб -- 10.04.2016
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4. XMM-Newton SAS: Feedback
... Help . Before you report a problem you should check if it has already been reported in the help desk's SAS archive . If you decide to report a problem, then you can do so via the Observation Report (OR) form. Shortly thereafter you will be contacted by the XMM-Newton help desk . ... In most cases you'll be asked to send the following information, so you may consider enclosing it right away in your report (not all items apply in all cases): . ... Information about the CCF in use . ...
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/sas/7.0.0/feedback/ -- 4.0 Кб -- 01.10.2012
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5. ATNF Future Operations: Community Feedback
... ATNF Home . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Murchison Radio-astronomy Observatory . ... Parkes radio telescope . ... Parkes | ... Future ATNF Operations (Version 1) was released on the web in February 2008. During March and early April 2008 we visited universities around Australia to discuss the future operations plans with the Australian user community. ... Web forum feedback on ATNF Future Operations (Version 1) . ... Future ATNF Operations: Overview . ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/observers/planning/feedback.html -- 48.6 Кб -- 08.04.2016
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6. Feedback in the Magellanic Clouds
... Feedback in the Magellanic Clouds . ... Missions . ... Monday, October 5-Wednesday, October 7, 2015 . The goal of this workshop is to bring together the communities studying feedback in the Magellanic Clouds on both stellar and galactic scales. As the nearest gas-rich dwarf galaxies, the Magellanic Clouds offer a superb opportunity for studying the radiative, chemical, and mechanical feedback from star formation at high spatial resolution. ... October 5, 2015: Workshop begins . ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/institute/conference/fimc -- 15.5 Кб -- 10.04.2016
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7. Cyles and Feedback Loops I
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[ Сохраненная копия ]  Ссылки http://zebu.uoregon.edu/1999/ph161/l7.html -- 3.8 Кб -- 21.01.1999
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8. Index of /ftproot/pub/comp/hardware/wd/mirror
. Parent Directory .description .mirror . 32bda.com . 32pack.exe . INDEX.TXT . allstar.exe . caviar.exe . chkbios.exe . coretst.exe . dmpatch.exe . ezdrive.exe . fhook.exe . getcmos.exe . ispfmt2.exe . overlay.exe . parkide.exe . titan.exe . typed.exe . wd_clear.exe . wd_diag.exe . wdatide.exe . wdcdrv26.com . wdfmtp.exe . wdtblchk.exe . win31.exe
[ Сохраненная копия ]  Ссылки http://crydee.sai.msu.ru/ftproot/pub/comp/hardware/wd/mirror/ -- 2.4 Кб -- 12.04.2016
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9. ESO - User Support Department Feedback Campaign
... Observatory . ... Science . User Portal . ... Science Users Information > Science Publications > Science Announcements > User Support Department Feedback Campaign . ... Science Users Information . Observing Facilities . ... Observing with ESO Telescopes . ... Data Handling and Products . ... Science Data Products Forum . ... ESO Data . ... The User Support Department (USD) invites principal investigators and their Phase 2 delegates to participate in the most recent user feedback campaign. ...
[ Сохраненная копия ]  Ссылки http://www.eso.org/sci/publications/announcements/sciann15014.html -- 23.2 Кб -- 10.04.2016
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10. Be/X-ray binaries and candidates
... Natalya V. Raguzova and Sergei B. Popov . ... We present a compilative catalogue of Be/X-ray binaries and candidates in the Galaxy and in the Large and Small Magellanic Clouds. This catalogue contains 160 sources and provides information on names and spectral types of optical components, distances, on spin characteristics of neutron stars, and on orbital and X-ray properties of binary systems. ... Be/X-Ray Binaries and candidates in the Galaxy . Galactic sources: comments to the Table 1 . ...
[ Сохраненная копия ]  Ссылки http://xray.sai.msu.ru/~raguzova/BeXcat/ -- 5.8 Кб -- 09.01.2015
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11. http://www.mrao.cam.ac.uk/~tm419/downloads/Graduate_student_poster.pdf
The FR Divide in Radio Galaxies through Environmental Interactions T. Maciel (Astrophysics Group) tm419@cam.ac.uk , P. Alexander (Astrophysics Group) Radio -Loud Galaxies · Galaxies which are dominated by their radio emission (10MHz -100GHz) and show extended morphology: - Jets Active Galactic Nuclei -Lobes powered by (AGN) -Hotspots -Central black hole -Accretion disc -Strong B fields -Dusty torus Chandra X-Ray image of Perseus cluster with VLA ... Right: FRII galaxy 3C175 at 5GHz. ...
[ Текст ]  Ссылки http://www.mrao.cam.ac.uk/~tm419/downloads/Graduate_student_poster.pdf -- 2276.9 Кб -- 26.04.2013
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