... Forms . ... This page explains how you can embed input forms into wiki pages. ... Forms processing can be found in the Cookbook (see below). ... input text name value size= n :) (: input hidden name value :) (: input password name value :) (: input search name value :) (: input number name value min=x max=y step=z:) (: input email name value :) (: input url name value :) (: input date name value :) (: input radio name value label checked=checked:) (: ...

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• Keyin Free-format Input
• Prefixes for input of spatial positions

... Operations of the Hubble Space Telescope (HST) require the creation of stable and efficient observation schedules in an environment where inputs to the plan can change daily. ... The long term scheduler, the main focus of this paper, provides approximate 4-8 week plan windows for observations. ... The long term scheduler as implemented within the Spike software system provides support for achieving stable observations schedules. ...

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• MOSS Training
• Correcting ETC Calculations of CCD Spectral Observations for CTE Effects
• CSPICE Routines: ET2UTC_C

... SUN MOON MERCURY VENUS MARS, JUPITER SATURN . Sun . ... The Sun's Heartbeat . ... Can a 0.2-second pulse from a magnetar put out as much energy as the Sun does in 250,000 years? ... A giant magnetar flare is incredibly bright and emits as much radiation energy as the Sun does in hundreds of thousands of years. Get instant access to subscriber content on Astronomy.com! ... Much more! ... If you are already registered on Astronomy.com, please log in below. ...

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• I read that once every second, somewhere in the universe a massive star ends
• New Horizons is about to pass Pluto at 9 miles per second Why won't it stop? |
• Mark Hanson | Astronomy.com

After averaging the point data, we should pay attention first to the astrometry, i.e. the quality of the delay data and the station coordinates. ... Plot FDL_O-C, that is the observed minus calculated FDL delays, versus time. ... The reference station can actually be changed in the Calibrate|Astrometry|SOLVE menu. ... This figure shows the residual delays for station 2 after solving for station coordinates, using the widget displayed in the lower right of the figure. ... Back to tour page . ...

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• Astrometry procedures
• ESO - neon-2006
• VLTI Calibrator Selection Help Page

... The input file is formatted in plain text as an unordered sequence of time-interval descriptions. Each non-empty line describes an interval, which may be simple or periodic, and good or bad. All intervals are bounded by a non-negative start and stop time. ... Periodic intervals break each period into two phase-segments, one good and the other bad, both having positive duration. ... timeref 2001-12-20T01:02:03 timesystem TT 100 0 # Good time extends from timeref + 100s onward . ...

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• Astrometric alignment of the input source coordinates
• Input

Next: Retrieving demonstration and Up: Echelle Reduction Method Previous: Echelle Reduction Method . ... User data is a set of echelle images, observed with the same instrument configuration, including a wavelength calibration image ( WLC ), a flat field image ( FLAT ) and astronomical objects OBJ . Optionally, this set will include standard stars ( STD ) to be used in the absolute or relative flux calibration, and dark images ( DARK ). ... Rotation of input frames. ...

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• Input and Output
• The random selected sample
• Input Data

... 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. ...

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... Tables for transformation from universal to sidereal time scale. Explanations. This page contains three little tables headed Hours Minutes Seconds respectively. Each the table have two columns: first of them is input column where time in whole time units of universal time is given, and second of them is output column where hours:minutes:seconds of sidereal time is presented. ... Example: transform 02 h 12 m 22.00 s from universal to sidereal time. ...

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• Explanations to tables for transformation from sidereal to universal time.

An extra leap second has to be inserted at the end of 2008, so this is how you should count down on New Year's Eve to celebrate the start of the International Year of Astronomy according to Irish astronomers. The extra second is needed to bring the uniform measure of time used by physicists using atomic clocks back into nearly exact agreement with time as measured by the rotation of the Earth. ... There will be national and international events organized throughout the year to mark the occasion. ...

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• SCL Sfit SLV Commands
• Three 6th classes at St Marks School Tallaght attended my second Solar System
• Amateur Astronomer Becomes Second Ever to Discover Asteroid from Ireland, After

Peremennye Zvezdy", . ... GSC 04232-02059, NSVS 3145727, NSVS 3145773, NSVS 3173757 . ... 13.1-13.6 (R, NSVS); . ... To combine our unfiltered photometry with publicly available NSVS (Wozniak et al., 2004; http://skydot.lanl.gov/nsvs/nsvs.php) data, we shifted the zero point of our light curve to match its magnitude at maximum light to the magnitude at maximum of the NSVS light curve. ... Light Curve . The light curve of GSC 4232-02059 in the magnitude scale of NSVS 3145773. ...

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• XWare > APOD

This file gives some hints on setting up the ABPP for pulsar observations and taking data. ... ABPP will always choose the largest bandwidth possible given the RF and the DM of the pulsar. ... The simplest way to control the WAPP datataking program is via tha datataking GUI shown below. ... As soon as the PC echos back to the gui in the ABPP LOG, that it is, in fact, taking data, you will see this reflected in the gui by the pink "SETTING UP MACHINE" being replaced by a green "DATATAKING ACTIVE". ...

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• p12mProg: 12m control program
• pdev_birdies_25jun07
• puppi software

U.S. NAVAL OBSERVATORY WASHINGTON, D.C. 20392-5420 July 23, 1998 No. 64 TIME SERVICE ANNOUNCEMENT SERIES 14 UTC TIME STEP 1. The International Earth Rotation Service (IERS) has announced the introduction of a time step to occur at the end of December, 1998. ... Coordinated Universal Time (UTC) will be retarded by 1.0s so that the sequence of dates of the UTC markers will be: 1998 December 31 23h 59m 59s 1998 December 31 23h 59m 60s 1999 January 01 0h 0m 0s 3. ... Time Service Dept., ...

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• The ALMA project
• Educator's Guide to Spotting the Shuttle
• Algorithm

... Mark C. Lee (Colonel, USAF, Ret.) NASA Astronaut (former) . ... EDUCATION: Graduated from Viroqua High School, Viroqua, Wisconsin, in 1970; received a bachelor of science degree in civil engineering from the U.S. Air Force Academy in 1974, and a master of science degree in mechanical engineering from Massachusetts Institute of Technology in 1980. ... NASA EXPERIENCE: Lee was selected as an astronaut candidate by NASA in May 1984. ... Lee retired from NASA and the Air Force effective July 1, 2001. ...

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... After the best fit is obtained, the confidence limits on two parameters can be obtained by running search_grid . This task calculates a grid of values for a given input model. ... Then search_grid will select the last dataset used (from pkgpars ), will use the best fit from the last run of fit (the null string ``'' at the model prompt will always select the best fit from the _prd.tab file), and will place the results in a _grd.tab file with the same root as the observed file. ...

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• Limiting Energy Channels Input to the Fit
• Features of the PROS software
• *tvmark* - Mark pixel positions on the display

... This year's eclipse is unique in duration. ... Although, at the present time, there are 6 solar observatories belonging to leading space agencies in orbit around the Earth, the eclipse of 22 July, 2009, will only be seen by two of them: the Russian CORONAS-PHOTON satellite equipped with TESIS telescopes and Japan's HINODE satellite fitted with an XRT space telescope. ... TESIS will be the first of the two devices (and the very first on Earth) to witness the solar eclipse. ...

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... Operations of the Hubble Space Telescope (HST) require the creation of stable and efficient observation schedules in an environment where inputs to the plan can change daily. ... A process and software architecture is presented which achieves stable and efficient observation schedules by dividing the task into long term and short term components. ... However, the resulting long range plan would be unstable as unscheduled observations in a week bin would have to be rescheduled. ...

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• Modeling Scattered Light in the HST Faint Object Spectrograph
• Electronic Submission of HST Phase I Observing Proposals
• On the Need for Input Data Control in Pipeline Reductions

... Bojan Nikolic web pages home . ... The goal here is to make a publication quality image of the sky with the coordinates labelled in the standard Right Accession/Declination units. ... Use the PGTBOX function which knows how to label the coordinate box in time units . ... тАЬINTтАЭ To draw tick marks and label them (тАЬIтАЭ so that the ticks are inverted, i.e., going outside the box) . ... Ensure that the matrix representing the coordinate system of the image is correct when calling PGIMAG . ...

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• OptInt PmWiki : PmWiki / Forms
• OptInt PmWiki : Forms
• Bojan Nikolic -- Input format for Out-Of-Focus (OOF) holography software

Comedi Documentation . ... Right to the source: #include <stdio.h> /* for printf() */ #include <comedilib.h> int subdev = 0; /* change this to your input subdevice */ int chan = 0; /* change this to your channel */ int range = 0; /* more on this later */ int aref = AREF_GROUND; /* more on this later */ int main(int argc,char *argv[]) { comedi_t *it; lsampl_t data; it=comedi_open("/dev/comedi0"); comedi_data_read(it,subdev,chan,range,aref,&data); printf("%d\n",data); return 0; } . ...

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• V.Shergin's Home Page
• INPUT - поля ввода в формах
• Fabry-Perot Interferometer: Gallery Old

psmask - To clip or mask areas of no data on a map psmask [ xyzfile ] -I dx [ m|c ][/ dy [ m|c ]] -J parameters -R west / east / south / north [ r ] [ -B tickinfo ] [ -D dumpfile ] [ -E ... radius [ k ] ] [ -T ] [ -U [/ dx / dy /][ label ] ] [ -V ] [ -X x - shift ] [ -Y y - shift ] [ -c copies ] [ -: ] [ -bi [ s ][ n ] ] psmask -C [ -K ] [ -O ] psmask reads a (x,y,z) file [or standard ... Je lon0 / lat0 / scale (Equidistant). Jf lon0 / lat0 / horizon / scale (Gnomonic). ...

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• http://xray.sai.msu.ru/~ivan/gmt/man/psclip.html
• http://xray.sai.msu.ru/~ivan/gmt/man/triangulate.html
• http://xray.sai.msu.ru/~ivan/gmt/man/spectrum1d.html

... Note on Filters: . ... NGC 3351 is a mostly face-on late type spiral galaxy. It is marked by a bar like feature in its central regions and a strong inner ring of star formation. ... The galaxy was imaged through the A1,B1 and B5 filters over a total exposure time of 1936 seconds. ... The galaxy was imaged through the A1 filter for 450 seconds and the B1 filter for 1084 seconds. ... The galaxy was imaged through the A1 and V1 filters over a total exposure time of 1200 seconds. ...

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• Avgvel