... Retrieve the list of all available HK parameter validity ranges for instrument EPN from the CAL and construct a GTI data set with name hkgti_epn.ds : hkgtigen instrument=epn withgtiset=true gtiset=hkgti_epn.ds . ... As 1. but do not consider any present validity ranges for parameters P1 , and P2 : hkgtigen instrument=epn withparameters=true except=true parameters="P1 P2" \ withgtiset=true gtiset=hkgti_epn.ds . ... IN [10,20]"\ withgtiset=true gtiset=hkgti_epn.ds . ...

... HST Phase II Proposal Instructions for Cycle 20 > Chapter 13: Wide Field Camera 3(WFC3) > 13.1 Introduction to WFC3 . ... More complete descriptions of Instrument Configurations, Modes, Apertures, Spectral Elements, Detector Characteristics, etc. are available in the WFC3 Instrument Handbook . ... Table 13.1 lists the permitted WFC3 Instrument Configurations, Operating Modes, Apertures, Spectral Elements, and Optional Parameters. ... Optional Parameters . ... See Table 13.2: Apertures for WFC3/UVIS ...

... Average resolution at altitude H=668 km . ... Swath width at H=668 km and inclination of beginning of swath 20.48 degrees . ... Resolution at H=668 км . ... Наименование параметра . ... 1 канале . ... Полоса обзора при H=668 км . ... 1-5 спектральной зоне, не более . ... 1 спектральной зоне . 0,48-0,52 мкм . ... 0,915-0,997 мкм . ... 1-4 канал . ... 1-4 каналов . ... Спектральные характеристики каналов (по уровню 0,5): . ... For more information send a mail to: info@sputnik.infospace.ru . ...

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 . ...

Purpose: IRAS instrument parameters. Category: IR File: ircc_const.c Author: P.R. Roelfsema Description: In this file the following routines are present: IRCC_ALIVE - returns 1: alive; 0: dead; -1: nonexistent IRCC_BANDET - returns band number given a detector IRCC_BANDNR - returns band number for instrument names. ... IRCC_SDET - returns SDET nr for detector number Updates: Aug 8, 1990: PRR, Creation date Sep 6, 1990: PRR, various changes Sep 10, 1990: PRR, changed device/bands to modes/bands. ...

ESO Phase 3 Data Release Description Please start from this template when preparing the documentation for your ESO Phase 3 data release. ... Finally, the release description will be published as submitted - without further editing by ESO - to support the user community in utilizing the data. ... Please indicate if this is a catalogue data release. ... Data Reduction and Calibration Please address the following questions for scientific catalogue data, particularly in case of source catalogues: . ...

... The Boolean object is an object wrapper for a boolean value. ... JavaScript 1.3: added toSource method . ... If value is omitted or is 0, -0, null, false, NaN , undefined, or the empty string ( "" ), the object has an initial value of false. All other values, including any object or the string "false" , create an object with an initial value of true. ... For Boolean objects and values, the built-in toString method returns the string "true" or "false" depending on the value of the boolean object. ...

... SphereParams Struct Reference . ... SphereParams (const float radius) . ... Definition at line 50 of file StelGeometryBuilder.hpp . ... Definition at line 103 of file StelGeometryBuilder.hpp . ... Definition at line 120 of file StelGeometryBuilder.hpp . ... Definition at line 112 of file StelGeometryBuilder.hpp . ... Definition at line 118 of file StelGeometryBuilder.hpp . ... Definition at line 110 of file StelGeometryBuilder.hpp . ... Definition at line 114 of file StelGeometryBuilder.hpp . ...

The Wideband Arecibo Pulsar Processor - File Format Page . WAPP files have three sections that appear sequentially in this order: an ASCII header description, the binary header, and finally the actual binary data. ... The WAPP realtime observation engine does not produce files larger that 2 Gbytes. At one time this represented a fundamental limit to Linux files. ... Each file will have it's own header, even when the files are simply continuations of a single observation. ... long int . ...