... Phase I: FUV Internal/External Wavelength Scale Monitor . ... Data . ... Phase I Proposing . ... Phase II Cycle 23 . ... Retrieving HST Data . ... Data Analysis . ... Monitoring . ... Phase I . ... ID: COS Cycle 18 Calibration - Phase I Template Last Revised: Oct 12 2010 Date Proposal ID: 12425 ( e.g . 9026) Title: FUV Internal / External Wavelength Scale Monitor PI: Cristina Oliveira Co-I(s): --------------------------------------------------------------------------- # Orbit estimates...

... Exposure Time Calculator (ETC) . ... ESO - Public Surveys . ... the recommended values to use for DIT, . ... Detector on-chip integration (DIT): seconds. to your chosen value - a separate page gives recommended values to use for DIT - for modes 1 and 2 below you may wish to start with the maximum recommended values as these will minimize the effect of read noise (a total object exposure of Y secs with DIT=X secs will produce Y/X lots of read noise) and give you a lower limit on the time needed. ...

The determination of the detector parameters is based on sets of images of a spatially uniform-illumination scene (flatfield frames) and without any illumination (dark frames), putting a plug in place of the filter, taken at a series of exposure times. ... We interleave before and after each exposure time in the series of flatfield frames a set of reference images at an exposure time of 1 sec to determine the possible temporal variation of the illumination level. ...

... Edit . ... Data archive . Main . Pulsar Groups Worldwide . ... Group . Group Members . ... Pulsar Surveys . Pulsar Catalogue . Pulsar Data Archive . PSRFITS pulsar data standard . Tasks . Tasks carried out by CASS staff . ... External Links . Pulsar Groups . edit SideBar . Page last modified on March 15, 2009, at 05:27 PM . ...

. XMM-Newton Science Analysis System . epicproc (epicproc-2.9.19) [xmmsas_20080701_1801-8.0.0] . Meta Index / Home Page / Description . An external GTI can be supplied to epicproc with the parameters withgtiset and gtiset . If the parameter applygti is further set to true (this is the default), the external GTI will be combined with the housekeeping GTI (if any, see 3.4 ) and applied to the event lists. XMM-Newton SOC/SSC -- 2008-07-02

. Search this album . Gallery . :: Astronomy Pictures . :: Images from external telescopes . Sidebar Left . Sidebar Top . No Sidebar . Sidebar Bottom . Sidebar Right . Title: Images from external telescopes . Description: Images acquired by RSAA astronomers using external telescopes NOTE: All images are copyright and must not be reproduced or mirrored in any form without written permission. NGC 1512 and NGC 1510 . Views: 1139 . Powered by Gallery 3.0.9 (Chartres) . Login

... Observing with ESO Telescopes . ... ESO-MIDAS . ... ESO Data . ... Related External Services . ESO HST Image Galleries . ... ESO Data Access Policy . ... ESO Science Newsletter . ... ESO Annual Reports . ... Seminars at ESO Santiago . ... Seminars at ESO Garching . ... ESO Telescope Bibliography . ... External routines for sky subtraction can be applied to MAPPED_ALL_SCI_LSS. After the sky subtraction the SPECPHOT_TABLE product can be used to perform the flux calibration. ...

... Charge Coupled Devices (CCD) are currently by far the most widely used type of detector in astronomy. ... After a brief introduction to the VLT Control System, the VLT CCD Detectors Control Software is presented. The VLT Control System is a distributed system consisting of a set of UNIX Workstations, dedicated to high level operations, such as coordination of sub-system activities and interface to the users, and VME-based Local Control Units (LCU), dedicated to the control of sub-systems hardware. ...

... Up: Fitting of Data Previous: Function Specification . ... C C.INPUT ARGUMENTS : C NIND INTEGER Number of independent variables C X ( NIND ) REAL Array of NIND elements with the C independent variable C NPAR INTEGER Number of parameters C PARAM ( NPAR ) DOUBLE PRECISION Array of NPAR elements with the C values of the parameters C C.OUTPUT ARGUMENTS : C Y DOUBLE PRECISION Value of the function C DERIV ( NPAR ) DOUBLE PRECISION Array of ... Array Arguments .. ...

... The spectral analysis system xspec , which is part of the XANADU software originally written for analysis of EXOSAT data, provides a larger variety of spectral models than those supported in PROS. PROS format spectral data can be input into xspec using the XANADU program proscon . Users should note that for spectral data generated in PROS 2.3 or later, the PROS program downspecrdf must be run to generate the input file to proscon . ...

This WWW form allows the user simplified access to images produced by the NRAO/VLA Sky Survey (NVSS). This service determines which NVSS image is desired based on a celestial position and returns either the image directly or a Web page with a link to the file. ... The NVSS Postage stamp (small FITS file) server can be used to obtain images with other geometries.) ... Web browsers use external viewers to display files like FITS images which they do not understand. ...

. Next: random.c Up: Piping Previous: plotter.c . /* externals.h */ #ifndef EXTERNALS #define EXTERNALS #include <stdio.h> #include <stdlib.h> #include <math.h> /* prototypes */ void StartPlot(void); void RemoveDat(void); void StopPlot(void); void PlotOne(void); void RePlot(void); #endif . Dave.Marshall@cm.cf.ac.uk . Wed Sep 14 10:06:31 BST 1994

... Conference 2009 . Conference 2011 . ... По данным ИСЗ Космос-1809, Интеркосмос-19, Космос-900 было определено кольцо ионосферных провалов, RIT, ассоциируемых с кольцом магнитосферного потока и SAR-дуги (SAR-arcs). ... Путем зондирования верхней ионосферы с ИСЗ Интеркосмос-19 был исследован новый тип провала NmF2 на низких широтах, который наблюдался преимущественно во время Декабрьского солнцестояния в экваториальной аномалии области Южного пика (смотрите Изображение 3). ...

NMW survey overview . Access image archive . ... The New Milky Way survey aims to detect bright (V<13.5) optical transients near the Galactic plane using an automated wide-field (8x6 deg.) system capable of surveying the whole Milky Way area visible from the observing site in one night. ... All images obtained during the transient search survey are available online (please use the image archive access form ). ... Images per field: . ... Images per night: . ... Milky Way imaging time: . ...

. About the beginning of 1996 I've started to collect our daily statistics. At this time we had about 30 percents load of 115Kbps line, and the life for users was quite comfortable. Based on Feb - May data the line overload had been predicted for the end of summer 1996. This prediction occured rather precise. Our link is operated over 4-wire leased line (about 5 km) and Zelax M-115 modems. The modems were found very stable and reliable.

In the current version .. ... Apogee Alta . Many SBIG cameras and filter wheels . ... FITS file format with exposure, camera, telescope, object and filter header information . Interactive image display and analysis with latest SAOimage ds9 . Interactive data processing in real time with AstroImageJ . ... XmCCD creates FITS image files with comprehensive header information and displays the images using ds9. ... Latest version 5.1 for Apogee and SBIG cameras updated June 17, 2015 . ...

... In recent years, as shown in Table 2 , the Observatory has regularly attracted external funding amounting to more than 50% of the DCAL grant-in-aid (more than 100% when the cost of external facilities used by Observatory staff is included). ... All items refer to calendar year, with the exception of DCAL Grant Income and External Grant Income which refer to the corresponding financial year (i.e. External Grant Income for 2000 refers to the financial year 2000/2001). ... Total DCAL . ... 66,000 . ...

... This example illustrates the use of external files as the source for a layer. This example creates a web page for Nikki's Diner, which is a vegan restaurant that offers tasty daily specials. The web page contains some general information about the diner, and then offers a pop-up menu that lists the days of the week. ... These files contain HTML formatted text that describes the specials for that day. ... LAYER ID="menu" LEFT=50 WIDTH=400 src="specials/sat.htm"> </LAYER> . ...

... In the presence of only uniform magnetic field B , the motion of a charged particle can be described with gyration about the guiding center and motion along the field line. ... In the precence of both magnetic and electric fields, the equation of motion for charged particle (mass m, charge q) is m d v /dt = q ( E + v x B ). ... Because v is independent of the mass and sign of the charge, it is the same for negatively and positively charged particles, and does not create electric current. ...

Astrophysical implications of external triggers, GRB030329 in particular External Triggers subgroup · · GRB astrophysics is still very uncertain Associated GW emission: even more uncertain Interpret our observations in the simplest terms Easy to re-cast in terms of specific models Provides some astrophysical context which is readily interpretable Probable: The GRB field will need GW observations to fully understand GRB progenitor astrophysics Nov 10, 2003 Frey 1 Short and Long GRBs.. ...