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ISR WFPC2 03-03: WFPC2 Cycle 12 Calibration Plan , Koekemoer, A. M., Heyer, I., Brammer, G., Kozhurina-Platais, V., Rhoads, J., Whitmore, B. ISR WFPC2 03-02: Toward a Multi-Wavelength Geometric Distortion Solution for WFPC2 , Kozhurina-Platais, V., Anderson, J., Koekemoer, A. M. ISR WFPC2 03-01: WFPC2 Cycle 9 Closure Report , Koekemoer, A. M., Baggett, S., Casertano, S., Gonzaga, S., Heyer, I., and the WFPC2 Group. ... ISR WFPC2 97-02: WFPC2 Cycle 5 Calibration Closure Report , Casertano and Baggett. ...

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... General information . ... Staff . Research staff . Technical, administrative & librarian staff . ... Infrared astronomy . ... Historical highlights . ... Friends of Arcetri . ... This leads to a number of technical reports which remain often unpublished in the general journals. ... 1993 Reports list. 1994 Reports list. 1995 Reports list. 1996 Reports list. 1997 Reports list. 1998 Reports list. 1999 Reports list. ... Twenty years of Arcetri Technical Reports! ...

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... Watchouts . ... In this page some issues concerning SAS and XMM-Newton data analysis are reported, along with recommended workarounds and/or solutions, and useful tricks and tips. ... If a SAS topic of interest is not reported in this page, users are invited to search in the HelpDesk database before submitting an Observation Report or contacting the XMM-Newton HelpDesk . ... Answer . ... I cannot filter on the TIME an RGS event file produced with a former SAS version. ... Am I doing something wrong?...

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... Updated 2003 December 18th . ... Updated 2003 December 15th . ... Updated 2003 December 2nd . ... Updated 2003 November 21st . ... Updated 2003 June 27th . ... Updated 2003 June 20th . ... Updated 2003 June 5th . ... Domes Restoration Project Update . Updated 2003 June 3rd . ... Updated 2003 June 2nd . ... Web Site Statistics . ... Updated 2003 January 31st . ... Updated 2003 January 27th . ... Updated 2003 January 23rd . ... Updated 2003 January 13th . ... Updated 2003 January 8th . ...

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Semiconductor Home > Products > Mixed Signal and Analog > CCD IMAGERS Family > . TC213, 1024- X 512-PIXEL CCD IMAGE SENSOR . ... The TC213 is a frame-transfer charge-coupled device (CCD) image sensor that provides very high-resolution image acquisition for image-processing applications such as robotic vision, medical X-ray analysis, and metrology. The image format measures 12.00 mm horizontally by 6.12 mm vertically; the image-area diagonal is 13.5 mm. ... 13.5-mm Image-Area Diagonal . ...

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Supernova 2009js in NGC 918 . This page is devoted to information on Supernova 2009js in NGC 918 . Basic information on this SN, including the last reported brightness, on this Supernova can be found on the main page . Information on the original web pages for many of these images can be found on the updates and links web pages. Discovered independently by Lick Observatory Supernova Search (USA) and Koichi Itagaki (Japan). ... 2009/10/11.44 . 17.2 . ... Joseph Brimacombe . ...

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If you have questions, need help, want to point out errors in this page, suggest improvements or give constructive criticisms regarding the observing system and this website, call Paulo Freire . Why CIMA? ... CIMA has become the default observing mode for pulsar observations at the Arecibo Observatory . ... The 4 Wideband Arecibo Pulsar Processors (WAPPs) have become the default back-ends for pulsar observations at the Arecibo Observatory. ... CIMA / WAPP observing page now available. ...

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. 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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... Meade Instruments Corporation . Telescopes ћ Binoculars ћ Microscopes . ... Frequently Asked Questions: LX200GPS . When I align the telescope, the alignment star is not in the viewfinder. ... After I select an object and press GOTO, the Autostar displays "Slewing.....", but does not seem to move. Is my Autostar broken? ... Can I use my Autostar II on his telescope to access my user objects? ... Choosing A Telescope . ... Copyright 2006 Meade Instruments Corporation, All Rights Reserved. ...

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NOTE: The storm sudden commencement data file was updated on 18 Feb 1998. o Revised data for 1968-1975 were taken from IAGA Bulletin No. ... Indices aa and storm sudden commencements"; see also IAGA Bulletin 39: " Supplementary Geomagnetic Data 1957-1975", including a new list of ssc's 1968-1975). ... From the monthly reports of Rapid Variations prepared by 43 magnetic observatories (see list page 121), a combined list of all events is compiled. ...

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... Next: FITS Checksum Verification Up: Data Models and Previous: A Proposed Convention . ... The FITSIO Subroutine Library has been available for 3 years, and has matured into a stable, full-featured interface for reading and writing FITS format files. ... The FITSIO subroutine library for reading and writing FITS files is now three years old and is used by many projects as the standard programming interface for accessing FITS format data files. ...

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Welcome to the home page of the ROSAT Science Data Center located at the Smithsonian Astrophysical Observatory in Cambridge, Massachusetts! We are the data support center for the ROSAT Xray orbiting observatory . The ROSAT Science Data Center is no longer active. Question about PROS or ROSAT can still be directed to hotseat or rsdc but we have limited resources to solve major problems. ... PROS User's Guide (Updated June 1998) . ... HRI Calibration Report (Updated October 1999) . ...

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... Welcome to the ADLab home page! Advanced Design Laboratory of the Special Astrophysical Observatory is concerned with research on low light level imaging and development of scientific digital imaging systems. About ADLab . ... Current project "A New Generation Multipurpose CCD Controller" . Project Contents . ... Publications on the Project . ... Other Web Sites of Interest . Created: 24 March 1998 . ... people have visited our web site. ... Copyright 1998 Advanced Design Laboratory. ...

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... It was designed to observe the solar wind approaching Earth, from a position near the Lagrangian point L1, and it is part of the International Solar-Terrestrial Physics (ISTP) Initiative . ... The original plan called for "Wind" to approach its final station over two years, undergoing two close encounters with the Moon to boost its speed. ... If however the object is moving , the encounter is not symmetric, and in the end the spacecraft may have gained or lost speed, depending on its trajectory. ...

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