... HST . WF/PC-1 Instrument Science Reports . ... Missions . ... Data . ... Annual Reports . ... Hubble Heritage Project . Future Missions and . ... Missions Office . ... HST Peer Review Process . Hubble Fellowships . Science Blog . ... HST Overview . Overview . ... Servicing Missions . ... Cycle 24 Announcement . Cycle 23 Results . ... Mid Cycle Submission . ... Phase II Cycle 23 . ... Reporting Problems . Retrieving HST Data . ... HST Science Year in Review . ...

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• GHRS Instrument Science Report 074
• WFPC2 Technical Instrument Reports (TIRs)
• WFPC2 ISR Abstract

... The SIRTF Science Center is developing two Web-based tools that will be used during operations. One tool is for Quality Analysis. ... The basic design requirements for the QA tool are (1) that it provide an easy way of looking at all the data, observation by observation, and (2) that it provide an easy way to specify status and comments for each observation. ... The data accessed by this tool consists of meta-data in the central database as well as the actual data files in the archive. ...

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• The ESO VLT CCD Detectors Software
• ADASS 2003 Conference Proceedings
• Calibration and Performance Control for the VLT Instrumentation

XMM-Newton Science Analysis System Page: 1 omthconv August 16, 2005 Abstract Converts OM tracking-history data into tracking-star count-rates time series 1 Instruments/Modes Instrument Mode OM TRACKING 2 Use pipeline processing yes interactive analysis yes 3 Description In order to perform accurate tracking throughout an exposure, software onboard the Optical Monitor(OM) selects n (up to 10) guide stars visible within the FOV and monitors their position and counts during the exposure. ...

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• http://xmm.vilspa.esa.es/sas/7.1.0/doc/omthconv.ps.gz
• http://xmm.vilspa.esa.es/sas/7.0.0/doc/omthconv.ps.gz
• http://xmm.vilspa.esa.es/sas/8.0.0/doc/omthconv.ps.gz

Next: INTRODUCTION . ... This article presents the Quality Control system of the Very Large Telescope. ... After a presentation of the QC levels and their implementation for the VLT, the paper discusses the usage of instrument models. ... On the other hand the observatory can control the instrumental configuration, test data analysis procedures, and provide calibration solutions with the help of instrument models. ... Quality Control . ... Instrument models for calibration and quality control . ...

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• Data Flow System overview
• Trend analysis
• ESO - Phase 2 Instrument Overview Table

IXth IAGA Workshop on Geomagnetic Observatory Instruments, Data Acquisition and Processing, . ... REAL-TIME MONITORING OF THE GEOMAGNETIC FIELD VARIATIONS . AND GEOMAGNETIC DATA BASES IN IZMIRAN . ... The digital variometers were introduced on Soviet magnetic observatories since 1975 in the frame of US-USSR experiment with ATS-6 satellite. ... The regular digital registration of the geomagnetic field variations was introduced in Moscow magnetic observatory of IZMIRAN since May 1991. ...

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• Environment Monitoring Information Systems

... The Science Operation Department is composed of Astronomers, Telescope Instruments Operators(TIOs) and Data Handling Administrators(DHAs). ... Astronomers have proposed several methods to quantitatively measure the amount of turbulence above the telescope, which the most common ones is Differential Image Motion Monitor (DIMM). In optical testing, the Hartmann test is the common method to test the quality of optical components. ... Hartmann mask consists of 48 lenses. ...

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... ATNF Home . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Murchison Radio-astronomy Observatory . ... Parkes radio telescope . ... Visiting Parkes radio telescope . ... Parkes radio telescope webcam . ... Long-term Monitoring of Molonglo Calibrators . ... Before and after every 12 hour synthesis observation, the Molonglo Observatory Synthesis Telescope (MOST) measures the flux densities of 5 compact extragalactic radio sources, chosen from a list of 55 calibrators. ...

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• A Cloud Monitoring System for Remote Sites
• Science with NIFS, Australia's First Gemini Instrument
• Near-Infrared Integral-Field Spectrograph (NIFS): An Instrument Proposed for

. The ALFA instrument monitor window is a big window showing all ALFA engineering parameters (with the exception of the ALFA motor). The 'Open motor control window' button opens the ALFA motor control window . You can return to the main CIMA page by clicking here .

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• The CIMA ALFA Instrument Status Window
• The CIMA ALFA Observation Monitor Window

SN 1989B Light Curve Analysis. ... In the light curve depicting their observations, definite trends are noted, here is a "thumb-nail" analysis of the the magnitude estimations of the bright SN (1989B) in the galaxy NGC 3627 (M66). ... The observations were inserted against the V magnitude templete of BL, CCD photometric data, (Wells et. al, (1994) and a color trend (B-V) histogram of the mean type Ia SN (BL)(nutemp.gif). Key Words: Amateur Observations, Supernova, Magnitude Estimates, 1989B . ...

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... Abstract (txt) . ... Xiao-li Meng (Harvard U) . ... presentation (pdf) . ... web page: astrostatistics.psu.edu/stat05.html . ... H. Kang (Department of Statistics, Harvard University), D. van Dyk (Department of Statistics, University of California at Irvine), V. Kashyap (Harvard-Smithsonian Center for Astrophysics), A. Connors (Eureka Scientific) . ... Poster (ps) . Poster (pdf) . ... Y. Yu, X.L. Meng (Dept. of Statistics, Harvard Univ.) ... Y. Yu (Dept. of Statistics, Harvard Univ.) ...

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• Special Session on AstroStatistics at HEAD 2013
• Topics in AstroStatistics
• Spectral Analysis

... In the framework of a collaboration between ESO and OAT concerning the development of a data reduction pipeline and the related quality control subsystems software for UVES/VLT, a detailed feasibil­ ity study is being performed on the basis of data extracted from the EMMI/NTT archive. ... Overview It is ESO policy to perform data reduction for VLT instruments in ``pipeline'' mode, either at the observing premises or at headquarters. ... The work has been carried out under ESO Contract No. ...

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• Status and Goals of the NICMOS Calibration Plan
• VLT First Light
• Near IR Astronomy with the ESO VLT

... On-board Integrated submm spectrometer for atmosphere monitoring and radio astronomy V.P. Koshelets, P.N. Dmitriev, A.B. Ermakov, L.V. Filippenko, A.V. Khudchenko, N.V. Kinev, O.S. Kiselev, A.S. Sobolev, M.Yu. ... In particular we have developed integrated receiver for novel balloon borne instrument TELIS (Terahertz Limb Sounder) [5]. ... TELIS is designed to be a compact, lightweight instrument capable of providing broad spectral coverage, high spectral resolution and long flight duration. ...

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• http://www.cplire.ru/html/lab234/pubs/2011_07a.pdf
• http://www.cplire.ru/html/lab234/pubs/2014_27.pdf
• Solartron Instruments

Lab . Main page News People . ASA . Master . Master net Homepage . ... Lomonosov Moscow State University Sternberg Astronomical Institute . ... MASTER . ... Lomonosov (ShOK) . ... About Space Monitoring Laboratory, scientific directions, instruments, contacts . People, who work in lab . Latest news and news archive . ... Gamma-Ray Bursts observations . Theory of Gamma-Ray Burst formation . ... MASTER (Global Robotic optical monitoring system) . ... All news ...

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To appear in "Fourth Workshop on Robotic Autonomous Observatories (2015)"RevMexAA(SC) MASSIVE PHOTOMETRY OF LOW-ALTITUDE ARTIFICIAL SATELLITES ON MINI-MEGATORTORA S. Karpov, 1, 3 E. Katkova,2 G. Beskin, 1, 3 A. Biryukov3,4 S. Bondar,2 E. Davydov5 E. Ivanov,2 A. Perkov,2 V. Sasyuk3 RESUMEN Favor de prop orcionar un resumen en espanol. ... The nine-channel Mini-MegaTORTORA (MMT-9) optical widefield monitoring system with high temporal resolution system is in operation since June 2014. ...

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• http://vo.astronet.ru/~karpov/pdf/2015_Malaga_mmt_meteors.pdf
• http://vo.astronet.ru/~karpov/pdf/2015_Malaga_mmt.pdf

Reloading smiswww.iki.rssi.ru ...

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• XV-TRACKER

Workshop on geometric analysis and spectral theory . ... On a class of random walks on groups with infinite number of generators". ... Optimal transportation, weak flows and very degenerate elliptic PDE's". ... Singular solutions to fully nonlinear elliptic equations". ... I will give some hints on how this conjecture is related to minimal surface theory and I will describe some flatness results for non local equations on one hand and on elliptic equations on riemannian manifolds on the other hand. ...

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• Workshop on geometric analysis and spectral theory. Schedule

... One of the instruments, the Troughton equatorial telescope, is maintained at constant temperature and relative humidity, to reduce the rate of deterioration. ... 3.1 Troughton Equatorial Telescope . Figure 1 shows the equatorial telescope constructed by J E Troughton of London and which was erected in the west dome of Armagh Observatory in 1795. ... Troughton, J. E.: c.1790, Instructions for Adjusting the Troughton Equatorial Telescope, Armagh Observatory Archives , M17.2, 3pp. ...

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• Abstract
• Abstract 218
• Abstract 200

... Space Science Education . ... Particle detectors networks for the Fundamental Physics, Space Weather and Education . ... A network of middle to low latitude particle detectors called SEVAN (Space Environmental Viewing and Analysis Network) is planned in the framework of the International Heliophysical Year (IHY), to improve fundamental research of the space weather conditions and provide possibilities to perform short and long-term forecasts of the dangerous consequences of the space storms. ...

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ICC/Hub Software Overview Requirements · · · · Monitor and control the instrument's robotics. ... Design · · Computer and software is in the computer room, named the ICC, which means Instrument Control Computer. Instrument's robotics and telemetry uses smart Ethernet I/O devices. ... Filter wheel changes for a variety of different wheel types (mix of filter sizes and number of filters in a wheel). ... Imager Robotics and Telemetry Requirements · · · · · · Stepper motor for filter wheel. ...

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• http://www.apo.nmsu.edu/arc35m/Instruments/GIFS/APO-GIFS_Factsheet.pdf
• TUI:Introduction
• APO Job Announcements

Next: Summary of reduction Up: Echelle Reduction Previous: Saving the Data . In the present version we will be concerned with the standard configuration of CASPEC, the Cassegrain Echelle Spectrograph which is in operation at the Cassegrain focus of the ESO 3.6 m telescope. ... In its standard configuration CASPEC uses a a 31.6 lines/mm echelle grating together with a 300 lines/mm grating cross disperser. ... The table shows the change in resolution with the order number. Table: Resolution . ...

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• Molonglo deep sky survey
• Radio patrol survey by Gregory and Taylor
• ESO-MIDAS Users Guide Overview