NICMOS Calibration Proposals Candidates . ... STScI . ... HST Overview . ... NICMOS STScI Analysis Newsletter 25 June 2001 CONTENTS: - NICMOS NEWS + Cycle 11 Call for Proposals + NICMOS Calibration Proposals Candidates + New Version of the NICMOS Instrument Handbook + Performance of the NICMOS ETC Against Archived Data - RECENT PREPRINTS - APPENDIX: NICMOS CONTACTS ============================================================================ NICMOS NEWS ----------- ...

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• NICMOS STScI Analysis Newsletter 10
• NICMOS STScI Analysis Newsletter 7
• WFPC2 STAN

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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• On-The-Fly Re-Calibration of HST Observations
• The ISO Post-Mission Archive
• The Ground Support Facilities for the BeppoSAX Mission

... Science Users Information > Data Handling and Products > Data Reduction FAQ > Are there any pipilines available to reduce APEX bolometer data (instruments LABOCA, SABOCA Artemis)? ... APEX . ... Observing with ESO Telescopes . ... Instrument Pipelines . ... ESO Data . ... ESO Data Access Policy . ... To reduce photometric (wobbler on-off) data taken with LABOCA or SABOCA using BoA, a detailed cookbook can be found at http://www.apex-telescope.org/bolometer/laboca/reduction/BoA-woo.html . ...

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• ESO - Are there any pipelines available to reduce APEX heterodyne data
• ESO - Science Announcements
• VLTI Calibrator Selection Help Page

... On the right side you will find all exposures of each instrument: . The exposures are aligned as bars with some text information. The size of the bar is related to the duration of the exposure, and the position of each bar depend on the instrument it belongs to and the start time of the exposure. ... Note, that the duration of some exposures can be quite short, such that the text in the bar is not always readable. ... This text can be the exposure id , instrument filter , or instrument mode . ...

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• Home Page

SAI 175 anniversary . ... Moscow University . Search for in SAI Moscow University Search for in Russian astronomical resources . ... SAI Astronomical Databases . ... Browse SAI Software archive(ftp.sai.msu.su) . ASTRONET.RU - Russian Astronomical Network (available in translit also) . ... SAI Supernovae Research Group . ... Department of the Galaxy and Variable Stars (in Russian) . Sternberg Astronomical Institute Seminars . ... All-Russian Astronomical Olympiad (in Russian) . ...

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... Astrophysics Group . Graduate Research Opportunities 2016 . Available research projects/areas . ... Astrophysics Admissions Form . ... This includes active participation in the development of new instruments as well as the use of ground and space observatories. ... Further details are available at the following web site: http://www.mrao.cam.ac.uk/research/extragalactic-group-2/ . ... Our research group has a wide range of expertise in the development of receivers for radio astronomy. ...

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• Preliminary results of OOF holography at the GBT
• Preliminary results page of the new OOF Holography
• OptInt PmWiki : PmWiki / Mailing Lists

... On­The­Fly Re­Calibration of HST Observations B. Pirenne and A. Micol Space Telescope -- European Coordinating Facility, ESO, Garching, D­85748 D. Durand and S. Gaudet Canadian Astronomy Data Centre, DAO, Victoria, BC Abstract. ... On­the­fly re­calibration data flow: from request submis­ sion to data delivery. ... On­the­fly re­calibration has another advantage for our archive sites: we only need to keep the raw data and calibration reference files on­line for the process to be automatic. ...

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• http://www.stecf.org/conferences/adass/adassVII/reprints/saxtonr.ps.gz
• http://www.stecf.org/conferences/adass/adassVII/reprints/brucal.ps.gz
• http://www.stecf.org/conferences/adass/adassVII/reprints/walterr.ps.gz

... Explanations of the Observation codes and GRT codes are available. ... V codes are for AO1 experiments W codes are for AO2 experiments VS experiment codes are VSOP Survey Observations VT Test/Calibration Observations EXPNO SOURCE FRQ Corr DOY DY: DATE UT RANGE #TEL TELESCOPES W071n J0745+10 L Mitk 6 We:Jan-06 10:00 - 17:00 6 UD SH KA AT MP HO W059e J0811+01 C Socr 7 Th:Jan-07 04:00 - 14:00 10 VLBA VS10a J0842+18 C Pent 8 Fr:Jan-08 13:00 - 18:00 6 CD HO UD SH KA MP VS11r J0909+01 C ...

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• Archive of VLBI Observations Majordomo List
• e-VLBI Workshop

. Please use the following for publications and media citations: . "Based on observations obtained with Apache Point Observatory's 0.5-m Astrophysical Research Consortium Small Aperture Telescope." . List of publications based on 0.5-m observations (TBD) . for questions or comments contact archive server .

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• APO Home Page
• APO 3.5-m Users Mail Servers
• ARCSAT Observers Nightlog Form

STEP INTO THE BLUE - MEADE INSTRUMENTS PRODUCT GUIDE . ... Telescopes . LX850 Series . ... Superb optical performance coupled with time proven computerized pointing and tracking has made the LX200 ACF series a best-seller in the high-performance telescope class. ... Meade's revolutionary LS LightSwitchтДв series of telescopes use advanced technologies to do what no other consumer telescopes have done before: take all the hassle out of using a telescope. ... Coronado€о Solar . ... Spotting Scopes . ...

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• CES Media Kit / CES Media Kit / Meade Instruments
• Meade Instruments Corp. - Frequently Asked Questions
• Meade Instruments Corporation - Frequently Asked Questions

... Keywords: network interface . ... How to find : . 1) the interfaces which are available : . ... There is a structure called "struct ifnet" which is used in include/linux/route.h. struct ifnet has information like the name of the interface (e.g. le0 or sl0), as well as the status of the interface (whether up or down). ... Older versions of linux had the definition of this structure available (struct ifnet also occurs in BSD code). ... Re: Question on network interfaces by Pedro Roque . ...

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• IBIS: SolarNet Access
• The Arcetri Spectral Code - E.Landi and M.Landini (2001)
• Observing capabilities

The INTERBALL space mission ( INTERBALL-1 with its subsatellite MAGION-4 in orbits with an apogee of 30 Re, and INTERBALL-2 with its recently reactivated MAGION-5 subsatellite in orbits with an apogee of 4 Re geocentric) continue to conduct important measurements in the solar wind, magnetosheath, magnetotail, magnetopause and above the auroral region. ... Plasma Boundaries in Near-Earth Space . ... Now we announce that online ABSTRACT submission is available at the SYMPOSIUM home page . ...

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• Space Research Institute (IKI) Seminar
• Optico-electronic Instruments for the Phobos-Grunt Mission
• Submission of questions

GRANAT is the Russian x-ray sattelite launched to the high apogee orbit (200,000 km) and operated almost for 10 years (1989 -1999) , carrying out four major instruments: French SIGMA coded-mask hard x-ray telescope (30-1000 keV), Soviet ART-P coded-mask telescope (2??-60?? keV), all-sky monitor WATCH (6-150 keV), and a gamma-burst detector PHEBUS . ... Since September 1994, GRANAT is in the survey mode. ... Explore pages devoted to individual GRANAT instruments (including main scientific results): . ...

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• SXG Science Data Center
• The 6th INTEGRAL Workshop "The Obscured Universe"
• Russian Turkish 1.5-m telescope

Peremennye Zvezdy ( Variable Stars ) 26 , No. ... Moscow 119992, Russia . ... 84/32, Moscow 117997, Russia . ... Our CCD observations compared to times of minima derived from the archival photographic plates and from the NSVS and ASAS-3 data clearly show that the orbital period of the system is variable. ... The phased light curve for the light elements . ... CCD, Moscow . ... and for the current linear light elements (in excellent agreement with the NSVS, ASAS, and our CCD observations): . ...

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... For the XRBs which are highly variable the concurrent presence of the RXTE/ASM that continuously measures their X-ray spectral states invites a new and innovative program to harness the available information to facilitate detailed studies of individual systems as well as comparative studies between classes of systems. ... This will enable them to quickly decide which data are worth putting in effort to extract and further analyze. ...

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• Statistics 310hfr 2004-2005
• *qpspec* - Time Resolved Spectral Fitting
• Notes on IPC and PSPC Spectral Fitting

Why are there different versions of CIMA? Which version of CIMA should I choose? ... There is no CIMA log in my project directory --- what happened? ... If You are a normal, happy observer, You should choose the CIMA version with the highest version number, since that version contains the latest improvements and bug fixes. ... This means that programs like the data quick-look display and various ALFA instrument displays all exist in several versions just like the CIMA observing session itself. ...

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• Pilot Fast Mapping Survey
• Solar System Studies at AO
• Visitors Tourists -- The AO Optical Laboratory

... He made observations of a supernova (literally: nova= "new star") in 1572 (we now know that a supernova is an exploding star, not a new star). ... Brahe's meticulous observations showed that the supernova did not change positions with respect to the other stars (no parallax). ... This was early evidence against the immutable nature of the heavens, although Brahe did not interpret the absence of parallax for stars correctly, as we discuss below. Brahe made careful observations of a comet in 1577. ...

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• Physics 410/510 Observational Cosmology

Examples of pipeline processing . ... This page presents examples of "on the fly" processing of FITS astronomical data available on the WEB using the HyperLeda pipeline tools. ... In many cases, raw data are archived and a consisten description of the file (FITS header) allows to process them on the fly. ... This first command makes a "pre-view" display of the image. o=fa:L93111HP1/00147&z=vg . ... The result of a pipeline processing is a FITS file that you can read as a normal disk file. ...

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• NVSS radio survey
• Frequently Asked Questions - Apache HTTP Server
• Sitemap - Apache HTTP Server

... Previous: Ground Tracking Station (GTS) Products . ... GRT Log File . ... GRT Gain Curves . ... What: Co-observing GRTs will each generate a log file identical to those for ground-based VLBI experiments. ... Where: Files are placed by GRTs on their regional server ( Regional Servers for GRT logs etc ) in the sub-directory named for the month and year (e.g. may97 ) below the sub-directory named gps . ... Where: Files are placed by GRTs on their regional server ( Regional Servers for GRT logs etc ). ...

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• References and Documentation
• Список литературы и документации
• RSOG Pre-Observation Products

... 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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