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1. The NGC 2903 ALFA Survey
... Observing blocks for Nov-Dec 2004 . Observing Schedule Preparation Martha's instructions for setting up a Schedule File for Observations . ... Observer's Log (web form) . Results (web log file) . ... Log of Dec strip status for line observations . Log of Dec strip status for continuum observations. ... Memo explaining the Fixed Azimuth Drift Mapping mode for ALFA. ... Phil's RFI pages (see in particular the problem of the drifting birdie ). ... Judith's NGC 2903 project web page . ...
[ Сохраненная копия ]  Ссылки http://www.naic.edu/~ngc2903/ -- 4.0 Кб -- 05.03.2005
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2. http://www.stsci.edu/documents/dhb/web/c29_wfpc2data.fm3.html
... Because of the need to schedule observations as efficiently as possible, the order in which exposures are executed may be different from the order in which they appear in the observer's Phase II submission-unless an explicit special requirement dictates otherwise. ... Data files can then be associated with the corresponding exposure line in the Phase II proposal by comparing exposure information in the Phase II proposal with data file header keywords. ... Time_Per_Exposure . ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/documents/dhb/web/c29_wfpc2data.fm3.html -- 8.4 Кб -- 17.11.1997
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3. Observations and Results
... 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 . Mopra radio telescope . ... Visiting Parkes radio telescope . Visiting Australia Telescope Compact Array . ... Parkes radio telescope webcam . ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pasa/14_1/barnes/paper/node2.html -- 51.2 Кб -- 08.04.2016
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4. XMM-Newton Satellite Position
... News Latest News News Archive Newsletter Quarterly Status Report . ... Data Analysis SAS News What is SAS? ... Archive, Pipeline & Catalogues XMM-Newton Science Archive Pipeline Processing System Observation Data Status Time Correlation Fix Serendipitous Source Catalogue OM Serendipitous Source Catalogue Slew Survey Catalogue Latest Slew Results Browsing Interface for RGS Data Live Radiation Monitor Plots Radiation Monitor Files . ... Please refresh your browser to update the satellite position. ...
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/external/xmm_science/sat_pos/ -- 12.9 Кб -- 09.04.2016
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5. ESO - La Silla Science Operations
... Science Users Information > Observing Facilities > La Silla Facilities > La Silla Science Operations . ... La Silla News . ... Internal Pages . La Silla Science Operations Department (LSO) is part of the La Silla Paranal Observatory and is in charge of the operations of the telescopes on La Silla. ... In the La Silla Science Operation pages, you should find all the information you need for your observations from the time you have an idea of observations until when you finish processing your data. ...
[ Сохраненная копия ]  Ссылки http://www.eso.org/sci/facilities/lasilla/sciops.html -- 27.2 Кб -- 10.04.2016
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6. http://www.adass.org/adass/proceedings/adass03/reprints/P1-29.pdf
... The results are used in quasireal time by the observing process, but also as input by hardware quality control, by the dynamical scheduler, and by the Science Pipeline. Among processing operations are the calibration of the atmospheric absorption, of phase radiometric correction, of pointing scans, of phase and amplitude reference measurements, .. ... Using the last few measurements, we will determine a provisional amplitude calibration curve (to be also used by the Quick Look pipeline). ...
[ Текст ]  Ссылки http://www.adass.org/adass/proceedings/adass03/reprints/P1-29.pdf -- 109.0 Кб -- 27.08.2004
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7. (Untitled)
... For each observed position the table contains designation of object as in file of observations, the time of observation, the number and name/ preliminary designation of minor planet supposedly identical with observed object, the values of O – C (observed position minus computed one) in right ascension and declination expressed in arcsec, the difference O – C between observed magnitude and computed one, the code of observatory in the Observatory list (see Observatories section). ...
[ Сохраненная копия ]  Ссылки http://www.ipa.nw.ru/PAGE/FUNDAMENTAL/LSBSS/winample_guide/user248j.htm -- 2.3 Кб -- 10.04.2016
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Еще в разделе: (Показать все результаты (>1494) - www.ipa.nw.ru/ )

8. Results of follow-up spectroscopy
Next: Emission-line galaxies Up: The Hamburg/SAO Survey for Previous: Data reduction . In total 217 candidates were observed during the January - June, 1995, of which 34 objects were observed with the 6m telescope, 183 objects with the Calar Alto 2.2m telescope, and 4 with both instruments. ... For 11 of the known ELGs we measure emission line ratios and make quantitative classification. ... Emission-line galaxies . ... Objects without emission lines . Absorption-line galaxies . ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/precise/Laboratory/Publications/1999/HSSI/TEXT/node7.html -- 4.8 Кб -- 24.11.1998
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9. Observers Instructions for filling out the ARCSAT nightlog
... The schedule assigned id (example: AS05) for your observing program. ... Use the time you started using the telescope including when you started taking calibrations. The time you opened for on sky observations can be entered later in the activity log. UTC End Time: . ... Focus Log: . ... The focus position can be obtained under the Telescope column of the System Status in ACP or from the run log. ... When all fields are filled out press this button to email the log to the ARCSAT and community. ...
[ Сохраненная копия ]  Ссылки http://www.apo.nmsu.edu/Telescopes/ARCSAT/ObservingAids/nightlogInstructions.html -- 5.9 Кб -- 16.05.2014
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10. http://www.asc.rssi.ru/RadioAstron/meetings/telecon/dec13_2011.pdf
MINUTES of the RadioAstron Teleconference on December 13, 2011 Yu.Yu. ... IOC status update M. Popov informed the participants on the current IOC results. ... Kovalev added: we continue to observe pulsars and spectral line sources in radiointerferometer mode but only with spacecraft and we are also going to observing pulsars soon with space-ground baselines. ... Kovalev: It is fringe-fitting result. ... In RAFS05 we replace it with K-band observing (maser source Ori KL ­ spectral lines ~100000Jy). ...
[ Текст ]  Ссылки http://www.asc.rssi.ru/RadioAstron/meetings/telecon/dec13_2011.pdf</