Next: Calibration with the ISOPHOT Interactive Analysis (PIA) . ... ISO P HOT I nteractive A nalysis, PIA , is a scientific and calibration data analysis tool for ISOPHOT data reduction. The PIA software was designed both as a tool for use by the instrument team for calibration of the PHT instrument during and after the ISO mission, and as an interactive tool for ISOPHOT data analysis by general observers. ... PIA is entirely based on the Interactive Data Language IDL (IDL92). ...

... The Science Analysis System ( SAS ) is a collection of tasks, scripts and libraries, specifically designed to reduce and analyze data collected by the XMM-Newton observatory . ... Observation Data Files (ODF), i.e. reformatted telemetry in FITS format. ... Pipeline Processing System (PPS) products, a collection of validated, top-level scientific products including event and source lists, multiwavelength images and cross-correlation products, generated at the Survey Science Center (SSC). ...

Introduction to Reducing HST Data Part I: Introduction to Reducing HST Data . ... 1.2 Getting Data with StarView . ... 1.2.3 Marking and Retrieving Data with StarView . 1.2.4 Using StarView to Retrieve Calibration Files and Proposal Information . ... 1.2.7 Quick Data Retrieval with StarView . ... 2.2 FITS File Format . ... 2.2.2 Working with FITS Table Extensions . ... 3.4 Displaying HST Spectra . ... 3.6.3 Other References Cited in This Chapter Part II: WFPC2 Data Handbook . ...

Next: Photometric Corrections Up: Long-Slit and 1D Previous: Long-Slit and 1D . This chapter describes the long-slit љ reduction package in a general way. ... The package provides about 50 basic commands to perform the calibration and to display the results, defined in the context LONG . ... The context SPEC is a low-level context including general utility commands required by the different spectroscopy packages ECHELLE , IRSPEC and LONG . ... This interface is described in the Appendix . ...

... Science . ... Science Users Information > Observing Facilities > Instrumentation Development > VLT/Instrument Interfaces . ... APEX Visitor Instrument . ... The interfaces between the VLT Unit Telescopes and the scientific instruments to be operated at the VLT Cassegrain, Nasmyth and Coudц© foci are well defined. ... Interface and numerous other relevant information for instrument builders is available in the "Requirements for Scientific Instruments on the VLT Unit Telescopes" , ESO doc. no. ...

At Arecibo we have a variety of optical instruments that we use to study terrestrial airglow emissions. ... As a complement to the airglow instrumentation we also maintain a set of optical instruments, called lidars, used for "active" remote sensing of the atmosphere. That is, we generate our own source signal using lasers and measure the characteristics of the light scattered back from the atmosphere. ... An operations manual for the Optical Laboratories is currently under major revision. ...