XMM-Newton Science Analysis System Page: 1 rgscombine June 28, 2006 Abstract Combines a list of spectrum les to create one combined spectrum le, and the corresponding list of response matrices and background spectrum, to create one nal response matrix and background spectrum le, for a paticular RGS instrument and spectral order. ... A list of response matrix les, as produced by rgsrmfgen or rgsproc. A list of background spectrum les as produced by rgsspectrum or rgsproc for TOTAL spectra. ...

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• http://xmm.vilspa.esa.es/sas/6.5.0/doc/rgscombine.ps.gz
• http://xmm.vilspa.esa.es/sas/7.1.0/doc/rgscombine.ps.gz
• http://xmm.vilspa.esa.es/sas/8.0.0/doc/rgscombine.ps.gz

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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• Technology / Technology / Meade Instruments
• Series / Meade Instruments
• Support / Become a Meade Dealer / Become a Meade Dealer / Meade Instruments

The Vela C region, part of the Vela complex, by ESAтАЩs Herschel space observatory. ... The image was mapped using Herschel instruments PACS and SPIRE at wavelengths of 70, 160, and 250 microns, corresponding to the blue, green, and red channels, respectively. ... Credits: ESA/PACS SPIRE Consortia, T. Hill, F. Motte, Laboratoire AIM Paris-Saclay, CEA/IRFU тАУ CNRS/INSU тАУ Uni. ...

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• Cygnus X: the cool swan glowing in flight | Astronomy.com

FGS Instrument Handbook for Cycle 24 . ... Fine Guidance Sensor Instrument Handbook for Cycle 24 > Chapter 3: FGS Science Guide > 3.4 Combining FGS Modes: Determining Stellar Masses . ... The combination of Position mode and Transfer mode observations is an effective means to derive a full orbital solution of a binary system. ... And with the parallax known (from the Position mode data), the total system mass, and hence the mass of each component, can be determined. ...

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• ACS Website
• Instrument Configuration [Config]
• STIS Instrument Handbook

. A tree for site navigation will open here if you enable JavaScript in your browser. HOME . ABOUT ST-ECF . CONTACT . The Instrument Science Reoprts written by ST-ECF members for the various Hubble instruments (STIS, ACS, WFC3) and for JWST are available at the STScI. The links below point to the location of all ISR's for the corresponding instrument or telescope. Maintained by Britt Sjoeberg <bsjoeber@eso.org> .

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• HSTPOLSIM (V1.00) --- April99 --- HSTPOLSIM (V1.00)
• stecf.impol - Package Tasks
• Near IR Astronomy with the ESO VLT

Home | ... Fisica Sanitaria | ... Amber SPG . ... The near-infrared / red focal instrument of the VLTI, called AMBER will operate between 1 and 2.5 µm in a first phase (2001-2003) with two UTs. This instrument has been designed for three beams to be able to perform images through phase closure techniques. ... The instrument has been designed to be used with two or three beams, thus enabling also the use of closure phase techniques. ... AMBER VLTI focal instrument home page . ... Simone Busoni . ...

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• Labir Instrument Page
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• FIRPO II

Displays the current status of NICFPS spectrograph and allows you to change the configuration. ... Once the instrument builders have more time with the instrument we plan to refine the controls. ... Select TUI:Save Window Positions to remember the state of this checkbutton. ... The contextual menu on each control can return that control to the current setting of the instrument. ... the current set of filters. ... Current : reset all configuration widgets to the current state of the instrument. ...

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• TUI:Instruments:Echelle:Echelle window
• TUI:TUI Menu:Log Windows
• ARC Progress Reports

SHORT DESCRIPTIONS OF INSTRUMENTS . ... Particle detector RIEP-2802 was developed and built in Russia. ... The combined Soviet-French ONCH-TBF onboard instrument had in memory modes the data only from several filter-banks in the range from 10 Hz to 16 kHz (while in the real-time telemetry modes, the measurements included 5-component wave-form data in the range 10 Hz - 1.5 kHz for 3 magnetic and 2 electric field components, or a wide-band mode in the range 10 Hz - 15 kHz, and several filter banks). ...

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• Main results of the experimental and theoretical research completed in 2010
• Lidar homepage - Instrument Information

... Right: cold gas traced by [CII] emission (red) accreting onto a primeval galaxy (green) at z=7.1 ( Maiolino et al. 2015 ) (image credit: ALMA Press Release ) . ... 2010 , Cicone, Maiolino et al. ... 2012 , Cicone, Maiolino et al. ... Right: observed distribution of the average stellar metallicities of passive and star forming galaxies in the local universe, supporting starvation/strangulation as primary quenching mechanism in low/intermediate mass galaxies ( Peng, Maiolino, Cochrane 2015 ). ...

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• OptInt PmWiki : MROI / Science Instrument Downselect
• OptInt PmWiki : Science Instrument Downselect | History
• OptInt PmWiki : Science Instrument Downselect

The VLTI Calibrator Selector Tool is a tool intended to assist in the selection of suitable interferometric calibrators for VLTI observations with MIDI and AMBER. It uses a model of the VLTI and its instruments to assess the fringe visibility, given the observed bandpass, the geometry, spectrum, and coordinates of the target and the time at which the observations are to be made. ... The tool offers an HTML/Java based interface and consists of two pages. ... The quality flag depends on LDD_chi2. ...

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• Combining the light of four VLTs for the ESPRESSO instrument | ESO
• The Very Large Telescope Project
• Combining the light of four VLTs for the ESPRESSO instrument

Astronomy Picture of the Day . ... 12.10.1996 . ... NASA/GSFC ) and The GOES Project Explanation: What alien planet's bizarre landscape lurks below these fiery-looking clouds? It's only Planet Earth , of course -- as seen on the Water Vapor Channel. Hourly, images like this one (shown in false color) are brought to you by the orbiting GOES 8 satellite's multi-channel imager . ... Bright regions correspond to high concentrations of water vapor while dark spots are relatively dry areas. ...

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• Астронет > The Water Vapor Channel
• Journal "Peremennye Zvezdy"
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... Instruments are more complicated than star catalogs, but a MIDAS table file is still useful for holding the description of an instrument. ... The main sub-table contains information about the passbands used, and the second sub-table describes the detector(s). ... Basic data for an instrument file include the passbands used (and any coding that is used to represent them in the data); the detectors used, and their properties; and general information about temperature control and optical cleanliness. ...

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• Echelle Spectra
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... Ciel Espace, le magazine qui vous guide toujours plus loin . ... Ciel Espace, nouvelle formule, c'est . des actualit–їs . ... des interviews, des portraits . les plus belles images de l'Univers d–їcrypt–їes pour vous . ... des pages consacr–їes –Љ la publication de vos photos Mais c'est aussi une vraie communaut–ї avec laquelle partager votre passion et nourrir votre curiosit–ї. Accueil Curiosity en route pour Glenelg . ... 03/02/2016 - Le Luxembourg veut exploiter les ast–їro–?des . ...

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• †Зa roule pour le prochain rover martien€а | Ciel et Espace
• Ultime retour dтАЩEndeavour | Ciel et Espace
• Discovery cтАЩest fini ! | Ciel et Espace

Minding the Gaps Joseph Lazio (NRL) G. Taylor (UNM), N. Kassim (NRL), D. Wilner (CfA) Minding the Gap Protoplanetary Disks · Protoplanetary disks are expected to be dynamic. Planetary formation ­ Planetary migration · Planets and protoplanetary disks are a major theme in nextgeneration instruments ­ ­ ­ ­ ­ ALMA ELT JWST TPF/Darwin .. ... Outlier Station Science Closing the u-v Gap · LWA station locations will be about 50­100 km from the EVLA. ... Outlier station is the next step. ...

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• The CIMA ALFA Instrument Monitor Window
• Thesis Figures
• The CIMA ALFA Instrument Status Window

Function: ircc_instrname Purpose: Returns IRAS instrument names. Category: IR File: ircc_const.c Author: P.R. Roelfsema Use: CHARACTER IRCC_INSTRNAME( OBSMODE , I integer band ) I integer IRCC_INSTRNAME Returns the name of the instrument corresponding to the observing mode and band numbers. ... Updates: Aug 8, 1990: PRR, Creation date Sep 10, 1990: PRR, Changed device to observing mode. Aug 19, 1991: PRR, Chang to make OBSMODE or BAND is 'other' work properly. ...

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• The instrument
• Links to Millimetre Telescopes, Instruments, etc.
• WALLABY - the ASKAP HI All-Sky Survey

An example of visual expert system. The program is written on Actor Prolog. -- -- (c) Alexei A. Morozov, March 19, 1999. ... Actually I wrote this program to train myself -- -- in carrying out SADT interview. ... A logical description of the blocks of the SADT model. ... The main purpose of these classes is keeping lists of cooking -- -- battery corresponding to various blocks of the SADT model. ...

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• Solartron Instruments
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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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• ADASS 2003 Conference Proceedings
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Mercury Spring 2010 Table of Contents . This artist s impression shows the transiting exoplanet Corot-9b. Credit: ESO / L. Cal ada. First Temperate Exoplanet . ... Combining observations from the CoRoT satellite and the ESO HARPS instrument, astronomers have discovered the first . ... Designated Corot-9b, the . ... If you enjoyed this excerpt from a feature article and would like to receive our quarterly Mercury magazine, we invite you to join the ASP and receive 4 issues a year. ...

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• ASP: 2009 Award Winners Press Release

... 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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• General information
• Methods and instruments, general issues

... Exposure Time Calculator (ETC) . Survey processing . ... VISTA is a 4-m class wide field survey telescope for the southern hemisphere, equipped with a near infrared camera (1.65 degree diameter field of view at VISTA's nominal pixel size) containing 67 million pixels of mean size 0.34 arcsec and available broad band filters at Z,Y,J,H,K s and a narrow band filter at 1.18 micron. A wide field visible camera, if constructed, could also be used on VISTA. ... Tile . ... ESO VISTA Public Surveys . ...

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• VISTA - Images of Camera