... People have been asking how cell phones transmissions affect observations done on the telescope. ... Three 50 Mhz bands centered at 1625, 1675, and 1725 Mhz were sampled once a second using the interim correlator. 2048 channels gave 48Khz resolution (after hanning smoothing). ... Each 1 second spectra was divided by this band pass correction. ... You can also see glonass at 1609, and iridium at 1620 to 1628 Mhz. dynamic spectra of the 1650-1700 Mhz band (.gif) . ... There are two frequency bands: . ...

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• lbw_crosshead_rfi_may09
• aerostat returns apr14
• gps rfi aug08

... First of all, I should say that you cannot guarantee user-mode processes to have exact control of timing because of the multi-tasking nature of Linux. ... However, for most applications using I/O ports, this does not really matter. To minimise this, you may want to nice your process to a high-priority value (see the nice(2) manual page) or use real-time scheduling (see below). ... Linux 2.x kernels have soft real time support; see the manual page for sched_setscheduler(2) for details. ...

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Using DIFX with ASKAP Chris Phillips, eVLBI Project Scientist November 2011 Murchison Radio Observatory Murchison Radio Observatory gazetted towns: 0 population: up to 160 population: 16 million ASKAP Design Goals High-dynamic range, wide field-of-view imaging Number of dishes Dish diameter Max baseline Resolution Sensitivity Speed Observing frequency Field of View Processed Bandwidth Channels Integration time Focal Plane Phased Array 36 12 ...

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• http://www.atnf.csiro.au/research/pulsar/ppta/uploads/PPTA2/stratenapsr.pdf
• User Parameters - Pipeline & job control CentralProcessor 0.11 documentation

... We can help students grasp the significance of Hubble's extremely keen eye, and learn a bit about angles and math in the process, with the following in-class activity. ... Looking through binoculars or telescopes allows us to magnify a small section of the sky. To measure sizes or distances in that small section, astronomers divide a degree into 60 smaller pieces called arcminutes, and further subdivide minutes into 60 smaller sections called arcseconds. ... 30 feet = . ... 36 seconds . ...

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... 2MASS Overview . The 2MASS Sky . Executive Summary of 2MASS Second Incremental Data Products . Point Source Catalog . Extended Source Catalog . ... Distribution Mode for 2MASS Products . Data Release Plan . ... Point Source Catalog (PSC) . Extended Source Catalog (XSC) . ... 2MASS Source Naming Convention . ... General Properties of the Data Release . ... Comparison of Achieved Performance of Second Incremental Release Catalogs with Level 1 Science Specification . ...

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• X-ray CCD Camera : C6086 Series(Hamamatsu Photonics)
• KODAK KAI Series Image Sensors
• KODAK KAF Series Image Sensors

... System for maintaining reference files and tables used to calibrate HST observational datasets. ... COSTAR: Corrective Optics Space Telescope Axial Replacement. ... Used for archiving HST data. ... Basic tool used to retrieve files from a remote system. Ask your system manager for information about using FTP. ... STARCAT: System used for retrieving archived HST data. ... STEIS: Space Telescope Electronic Information System. ... STSDAS: Space Telescope Science Data Analysis System. ...

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• Telemetry processing
• NSSC-I stored command processing
• COS Spectroscopic Observing Strategies

... Contacts . 2009: . ... We finalized the development of a facility for observations (including remote observations) of the star-shaped objects with the temporal resolution of 1 micro second. ... For contacts: G.M.Beskin ) . RATAN-600 Multi-Octave Frequency Range Overlapping Finalized. We finalized the multi-octave overlapping of the RATAN-600 frequency range from 0.75 to 18GHz with the frequency resolution of 1% using the parallel spectrum analysing complex. ... Archive . ...

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• SAO RAS home page
• Hardware sector, archive 2005

M obile A stronomical Sy stem of TE lescope- R obots MASTER-II Kislovodsk Lomonosov Moscow State University, Sternberg Astronomical Institute , Moscow Union "Optic" , Kislovodsk Solar Station Latitude = 43 o љ44'.767љN; Longitude = 42 o љ31'.417љE; Altitude = 2067љm MASTERљIIљ(8љsquareљdegress) + MASTERљVWF(VeryљWideљFieldљCameras (FOV=800 square degrees, Timeљresolutionљupљtoљ150љms, with unfiltered m_lim=14m on 5 sec. exposure, and ~10.5m with 0.15 sec) . ... 11h 38m 38.0s , -09d 59m 59s) . ...

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... Quality Control and Data Processing . ... HOME . ... UVES /UVES . ... retired : . ... This is the home page of the Quality Control and Data Processing Group (QCG) within ESO's Data Management and Operations Division (DMO). ... At ESO Headquarters in Garching, calibration data from all Paranal instruments (VLT, VLTI, survey cameras) are processed, their quality is checked and monitored. ... UVES ECHELLE data, point sources: quality-controlled, homogeneous processing of complete data stream 2000-now ....

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• ESO - Circumstellar Dynamics at High Resolution
• FLAMES/UVES Data Processing and Quality Control
• UVES & FLAMES/UVES Data Processing and Quality Control

... Skalnatґ Pleso 43, 1 ­ 2, (2014) e Mini-MegaTORTORA ­ multichannel system for wide-field optical monitoring with high temp oral resolution V. Sasyuk1 , G. Beskin2 , S. Karp ov2 , S. Bondar3 , A. Perkov3 , E. Ivanov3 , E. Katkova3 and A. Shearer4 2 Kazan Federal University, Russia Special Astrophysical Observatory of Russian Academy of Sciences, Russia 3 Insttitute for Precise Instrumentation, Russia 4 National University of Ireland, Galway, Ireland Received: November 4, 2013; Accepted: ?? ...

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• http://vo.astronet.ru/~karpov/pdf/2015_Malaga_mmt_meteors.pdf
• http://vo.astronet.ru/~karpov/pdf/2015_Terskol_mmt_meteors.pdf
• http://vo.astronet.ru/~karpov/pdf/2013_EAS_Karpov.pdf

Next: The ESO VLT CCD Detectors Software . ... Up: Instrument-Specific Software . ... The framework for data calibration and analysis of the VLT instrumentation is presented, based on the concepts of a calibration plan, pipeline calibration, quality control, and archiving of calibrated data for a ground-based observatory. ... Quality Control Pipeline provides quality assessment for instrument performance data and observing conditions, and tests the results of the Reduction Pipeline. ...

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• Doing Theoretical Astrophysics With HST's Data Processing Pipeline Software:
• ADASS 2003 Conference Proceedings
• Operating the TNG Data Handling and Archiving

... Stellar Evolution is driven entirely by the never ending battle between Pressure and Gravity . As imbalances are reached, the star is driven to find a new Energy source. ... Pressure and gravitational forces are equal, the star is stable and its core is sufficiently hot to fuse Hydrogen into Helium More about main sequence stars . ... The luminosity generated by the core fusion of Helium into Carbon is far greater than the shell luminosity associated with the fusion of Hydrogen into Helium. ...

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• What should I know for the Second Midterm?
• Astro-2 and the UIT Experiment
• Thermal History of the Universe

You can also see this page in Russian with using KOI8 (X Windows) or CP1251 (MS Windows) Cyrillic coding. The Laboratory supports the space TV experiments, mainly in the planetary exploration missions. ... Image Co-registration . ... PHOBOS mission - Martian satellites investigations. Phobos on the Martian limb, the image from Phobos-2 probe from 02/28/89. ... Russian Space Bulletin. ... Last modified at June,26 1997 Alexey Kuzmin: akuzmin@mx.iki.rssi.ru . Back to IKI home page ...

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• Auroral Images
• Lunar Orbiter 5
• Lunar Orbiter 2

XPA supports host-based access control for each XPA access point. You can enable/disable access control using the XPA_ACL environment variable. ... See XPA Access Points and Templates for more information about xpa templates. ... For example: xpaset -p xpa1 -acl "somehost -" will turn off all access control for somehost to the xpa1 access point, while: xpaset -p XPA:xpa1 -acl "beberly gs" will give beberly xpaget and xpaset access to the access point whose class is XPA and whose name is xpa1. ...

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• Source Selection
• Casio QV-* Camera info
• HEAD 2010: Chandra's Ultimate Angular Resolution

... Ranger 7 was designed to achieve a lunar impact trajectory and to transmit high-resolution photographs of the lunar surface during the final minutes of flight. ... Velocity at impact was 2.62 km/sec (1.62 miles per second). ... The television system consisted of a six slow-scan vidicon TV cameras capable of transmitting high-resolution, close-up television pictures of the lunar surface during the final minutes of flight before the spacecraft impacted the lunar surface. ...

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• prefork - Apache HTTP Server
• Ranger 9
• Ranger 8

Some radio clocks and related timekeeping gear have a pulse-per- second (PPS) signal that can be used to discipline the local clock oscillator to a high degree of precision, typically to the order less than 50 us in time and 0.1 PPM in frequency. ... Either way requires conversion of the PPS signal, usually at TTL levels, to RS232 levels, which can be done using a circuit such as described in the Gadget Box PPS Level Converter and CHU Modem page. ...

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• APOD: July 30, 1999 - The Sea of Tranquillity: 5 Seconds To Impact
• APOD: 2012 July 23 - Lightning Captured at 7207 Images per Second
• APOD: 2005 September 15 - The Nucleus of Comet Tempel 1

Target: Arcturus Date: 2010-04-15 Time: 2010:04:15 Telescope: FSQ with tandem Nikon and 85mm f/1.4 Nikor Camera: Nikon D200 Filters: None Exposure time: 10 seconds Observer: John Kielkopf Processing: John Kielkopf Processed from full range NEF data transformed to PPM and mapped to PNG with AstroImageJ. The field of view is approximately 10 degrees wide x 16 degrees high. Arcturus is near the center, and CN Boo is the bluish star just to its southeast.

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• http://www.astro.louisville.edu/shared_skies/archive/select/messier/m3/20070421/m3_r_300_stv_01_d.txt
• Shared Skies Photo Gallery
• Moore Observatory's XmCCD

... Lightning Captured at 7207 Images per Second . ... 23.07.2012 . ... Credit Copyright: Tom A. Warner , ZTResearch , www.weathervideoHD.TV Explanation: How fast is lightning? ... The above lightning stroke did not move too fast, however, for this extremely high time resolution video to resolve. Tracking at an incredible 7,207 frames per second, actual time can be seen progressing at the video bottom. ... July 2012 . ... 2011 2012 . ... NASA Web Site Statements, Warnings, and Disclaimers . ...

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• The South Pole of Asteroid Vesta
• Journal "Peremennye Zvezdy"
• XWare > APOD

This describes the exposure window used by each instrument (the graphical interface for the hub's expose command). ... To open the expose window for a given instrument, bring up that instrument's main window, then press the Expose... button along the bottom. ... The top panel shows the status of the current exposure sequence (regardless of who started it). ... File: the file name for the current exposure, or the most recent exposure if not exposing. ... Download: exposure download preferences. ...

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• ARC 3.5m | Instrumentation
• TUI:Instruments:Agile:Agile window
• Spectrographic time budget

Static Fourier spectrometers are often used for spectral measurements of the ionosphere emissions. There are two main advantages of Fourier spectrometers (FS) - large geometric factor and high spectral resolution; these parameters are two orders better than for grating spectral instruments. ... In scanning Fourier spectrometer optical and electric modulation of signal is used to avoid this problem, for static Fourier spectrometer there are no such ways. ...

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• HIGH RESOLUTION IONOSPHERIC MASS SPECTROMETER P-11
• INFRARED FOURIER-SPECTROMETER SICH-F
• TELEVISION CAMERA TVC