... NICMOS Data Handbook > Chapter 2: Data Structures > 2.5 Paper Products . 2.5 Paper Products . ... After the data from an observation have been received and processed through the STScI pipeline, PDF files ( paper products ) can be generated which summarize the data obtained The paper products are generated using the stsdas.hst_calib.paperprod task pp_dads . ... Optional Parameters : a table listing the optional parameters, other than the pattern related parameters, used in the observations. ...

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• WFC3 Data Handbook
• HDF-S Observing Strategy
• Near Infrared Camera and Multi-Object Spectrometer Instrument Handbook for

... The processing of these associated images presents new challenges to the HST data processing pipelines, which heretofore operated only on single images. ... Stage 1 (CALNICA) calibrates individual exposures without information from other members of the association. ... Stage 2 of calibration (CALNICB) only operates on associated images that have previously gone through CALNICA processing, and creates combined images for each distinct (non-overlapping) pointing within the association. ...

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• The STScI NICMOS Calibration Pipeline
• Data Quality Control at the Very Large Telescope
• A Distributed System for ``Phase II'' Proposal Preparation

Next: Miriad's Calibration Model Up: Visibility Data Concepts Previous: Visibility Data Concepts . A visibility dataset in Miriad logically consists of two parts - a stream of variables and calibration tables. ... Because source names, frequencies, observing centre etc., are stored as variables, Miriad does not distinguish between a single-source file and a file with multiple sources or frequencies, or a mosaiced observation. ...

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• THE SCHED INPUT FILES (Includes parameter lists)
• User Parameters - Bandpass Calibration CentralProcessor 0.11 documentation
• Mosaicing Observing Strategies

... Finally, the individual observations themselves are reduced, using the parameters from the extinction solution. ... That is, the extinction solution can in principle produce results if we observe extinction star 1 only in passband A and star 2 in passband B on night 1, and star 1 only in passband B and star 2 in passband A on night 2. ... Even if the passbands are linked by color terms in the extinction, the solution is possible, because we do obtain mean colors for each star. ...

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• Line parameter measurements
• Bad Pixel Correction
• How the Data is Processed

NAME ABbuilder - DFO data organization tool SYNOPSIS ABbuilder <options> where <options> are: --raw-dir directory containing raw data --cal-dir directory containing calib data --cal-ldir directory containing symbolic links to calib files --cal-list mcalib list --vcal-dir directory containing virtual products --pro-dir where pipeline products are created --ab-dir where association blocks are created --oca-rul file containing OCA rules --instrume instrument --date YYYY-MM-DD --mode { CALIB | ...

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• GOODS
• Data Flow System overview
• ESO - Phase 3 Policies for ESO Spectroscopic Public Surveys

XMM-Newton Science Analysis System Page: 1 etimeget March 18, 2004 Abstract A procedure to generate source and background time series. ... The essential input parameters are the name of the XMM events table and a selection expression for the source and optionally background areas, e.g. srcexp="((DETX,DETY) IN circle(572,-635,1340))" backexp="((DETX,DETY) IN circle(2572,-1635,1340))". ... If timebinstyle is set to intrinsic then the light curve is binned at the frame time of the observation. ...

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• http://xmm.vilspa.esa.es/sas/6.1.0/doc/etimeget.ps.gz
• Parameters
• Description

Next: ST-6 Data Collection Up: Data Acquisition Previous: Data Acquisition with . ... The tracking software is extremely important to data collection, and will be presented here. The tracking software is run from the CPU box. ... The exposure adjust will set the exposure time. ... After the drive is calibrated, the track button will set the ST-4 in a mode where it will track the star until it either loses track or the operator stops the track. ...

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• Filtering ROSAT HRI data on the basis of background level
• Structure of the Spectral Package
• The Chandra Multiwavelength Project (ChaMP)

asncombine -- Process and combine images in one or two NICMOS associations asncombine association . ... set to yes to include error planes in co-added images error. background . ... This is useful to use different background subtractions for different images. fheader . set to yes in order to multiply the background by the value of keyword "factor" in the image header. ... Set to yes to use quadrants statistics save in the image header from previous runs of asncombine. regquad1 . ...

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• The STScI NICMOS Calibration Pipeline
• MAKEASN (Nov98) --- nictools --- MAKEASN (Nov98)
• STScI NICMOS Software

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 . ...

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• CIMA Configuration Files
• VLBI at Arecibo Observatory
• Postdoctoral Research Associate in Radio Astronomy

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: . ...

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... Observing . ... Solar Observing . ... April 3 (SUN) - Solar Observing, Central Park , Manhattan . ... APRIL'S SKY . ... Lecture Series at the American Museum of Natural History The Amateur Astronomers Association is proud to present an astronomy lecture series from October through May each year for our members and the .. ... The€аAmateur Astronomers Association of New York€аwas organized in 1927 to promote the study of Astronomy, emphasizing its cultural and inspirational value. ...

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• Stanley Fertig Gallery ? Amateur Astronomers Association of New York
• Lectures ? Amateur Astronomers Association of New York
• Lecture Series 2010-2011 ? ?The History of the Universe in One Hour? by Max

Next: Program use Up: Description of program searchdup Previous: Description of program searchdup . Parameter input is done with a graphic user interface. ... Input file: Name of the input catalog file. It has to be formatted, one record per source/observation, according to the format used in the Arcetri observations and source archives. ... Minimum number of observations per source Source with less than this number of independent observations are not included in the output file . ...

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• Observing capabilities
• Arcetri Star-formation Group Research Topics
• CHIANTI atomic database

... galaxies: bulges galaxies: clusters: general galaxies: clusters: individual: . ... star formation statistics stellar content structure Cosmology ( cosmology :) cosmic background radiation ( cosmology :) cosmological parameters cosmology : miscellaneous cosmology : observations cosmology : theory ( cosmology :) dark ages, reionization, first stars ( cosmology :) dark energy ( cosmology :) dark matter ( cosmology :) diffuse radiation ( cosmology :) distance scale ( cosmology :) early Universe (...

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• Galaxy sector, archive 2012
• HD965

... SFIT is a general-purpose code designed to optimize theoretical stellar spectra to an observed spectrum. ... While the programme expects input from "stdio", it is more natural to save commands in a file (eg "sfit_input") and run the code simply by . ... If the spectra to be fitted have a filename "star_spectrum", then the best fit spectrum will be written out, together with the renormalized input spectrum, to a file called "star_spectrum.fit". ... sets up model spectrum grid (and for 2nd star) . ...

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• Armagh Astronomers to observe Ringing Star with Global Telescope
• Armagh Observatory
• Irregular Satellite Research

... New Mexico State University is seeking a technical and computer-oriented person as a Support Astronomer for nighttime astronomical observing at Apache Point Observatory (APO) with the Astrophysical Research Consortium (ARC) 3.5m Telescope. б  . ... Paper/email documents will not be accepted. ... TELESCOPE OPERATIONS SPECIALIST . ... Responsibilities include nightly operation of the 3.5m telescope and instruments, Quality monitoring the data streams and system performance and observing efficiency. ...

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• Observers Instructions for filling out the ARCSAT nightlog
• APO Telescope Documentation
• lsst.coordConv: coordConv::FK4CoordSys Class Reference

Databases (NSDC) of the Natural Planetary Satellites. ... NSDC: Database of astrometric observations of Natural Planetary Satellites . ... They are thoroughly looking for observations in different sources, creating their owndatabases which are then mostly inaccessible to other researchers. ... In the file "content" with explications, the reference is given to the data source as well as the bibliographic reference. ... Data sources. ... Why a specific bibliographic database for Natural satellites? ...

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• Data bases of Natural Satellites. Documentation. Sources

National Aeronautics and Space Administration . ... Bruce McCandless II (Captain, USN, Ret.) NASA Astronaut (former) . ... He was a member of the astronaut support crew for the Apollo 14 mission and was backup pilot for the first manned Skylab mission (SL-1/SL-2). ... A veteran of two space flights, McCandless has logged over 312 hours in space, including 4 hours of MMU flight time. ... With the completion of this flight McCandless logged 191 hours in space (including 4 hours of MMU flight time). ...

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• Astronaut Bio: Mark C. Lee 10/2006
• Astronaut Bio:Mae C. Jemison
• Astronaut Bio: Stephen K. Robinson (07/2012)

Observational data on solar activity is a basement for investigation of processes that take place on the Sun and interplanetary space, with data of long-term observations being of special importance. ... Subsection "Sunspot groups" is the catalogue of all sunspot groups that were observed in the given year. ... For every day of observation of the group the area of the group, the area of the largest spot (both areas - in millionths of solar hemisphere) and number of spots in the group are presented. ...

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• http://www.gao.spb.ru/english/personal/malkin/publ/zm12e.pdf
• Pulkovo EOP and Reference Systems Analysis Center (PERSAC)
• Pulkovo NEO Page: Observations

... IAA VLBI Analysis Center . ... First IAA SLR EOP submission to IERS Annual Report . ... Beginning of operational processing of SLR observations . ... We use several program packages for analysis mostly developed at the IAA: GROSS for processing of the SLR observations and analysis of EOP and coordinates time series, OCCAM/GROSS for computation of EOP, station coordinates, and troposphere parameters time series from the VLBI observations, GRAPE for processing of GPS observations. ...

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• LAB Ephem. Astronomy-ERA
• (Untitled)
• NAA 2013-2014 (preface)

... Fitting the observed dependence includes calculations of the polarization cross-sections averaged over particles orientation and size distribution, their normalization and the comparison of obtained dependencies with Serkowski's curve representing observational data for a chosen star. ... Variations of the polarization factors with wavelength are shown in Fig. 16 for homogeneous spheroidal particles with PF orientation. ... The distinction between prolate and oblate spheroids is also clearly seen. ...

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• AI SPbU library of scattering codes
• Database of Optical Properties -- Level: subpage