... They include: 4 dither patterns, 4 chop patterns, and 3 dither-chop patterns. For each of these, the observer will be able to specify, during the Phase II Proposal submission, the total number of positions desired (2 to 40), the dither size (0 to 40 arcsecs), the chop size (0 to 1800 arcsecs), and the orientation of the pattern on the sky. ... In addition, the figure number where the pattern is graphically shown is given in column 5 of Table 10.1 . ... Figure 10.3 . ... 0.0 - 1800.0 . ...

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• http://www.stsci.edu/hst/nicmos/documents/isrs/isr_013.pdf
• How to Fill Out the Pattern Parameters Form
• Chapter 8: Pointings and Patterns

... This thread contains a step-by-step recipe to extract MOS spectra of a point-like source observed in Imaging mode and to create associated response matrices, starting from a calibrated, concatenated event list (either produced with emproc or available as PPS product; here it has the assumed file name MOS.fits ). ... The users should note that the SAS metatask xmmselect allows them to interactively define source and background regions (via ds9) and to run backscale on the fly. ...

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• How to extract MOS spectra of a point-like source and associated matrices using
• How to extract PN spectra of a point-like source and associated matrices
• Point sources

... Current APO Weather . ... Search Site . ... Information for New Users . ... Technical Staff pages . Night Logs and Mailing Lists (maintained by APO) . ... Technical Documents and Database Search . ... Observer's Documentation and Procedures . ... Problem Reporting and APO Technical Documents Database Search . ... APO Drawing/Document Management Procedures . ... APO Technical Documents Database Search . Home Astrophysical Research Consortium . ... Mail Lists (maintained by APO) . ...

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• Astrophysical Research Consortium - Apache Point Observatory
• sgs summary

... 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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... This section will deal with obtaining photons within specified regions of an image. Available regions are: Annulus Box Circle Ellipse Field -- entire field Irregular region based on intensity of map... i.e. region defined by contour levels. ... The imcnts task in the xray-spatial package sums the source and background counts in specified regions, and subtracts one from the other properly normalized. ... imcnts* - Find counts in an extended region, after removing an embedded point source . ...

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• The Markers Menu
• Comments on: A test for global maximum By: hlee By: aneta
• XPA Programs

... This section gives a brief description of each of the parameters available to SCHED that are specifically for VLA observations or are especially useful for VLA observations. ... Should be provided for non-VLBI observations. ... This used to be required in order to obtain calibration data for the VLBI observations. ... FREQ: and DOPPLER Warning -- these parameters cannot be used for non-VLBI observations at the VLA since they are only used to adjust the baseband converter frequencies. ...

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• Package: iedit
• User Parameters - Continuum Source-finding CentralProcessor 0.11 documentation
• User Parameters - Bandpass Calibration CentralProcessor 0.11 documentation

... 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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• Enhanced HST Pointing and Calibration Accuracy: Generating HST Jitter Files at
• In-Orbit Calibration of the Distortion of the SOHO/LASCO-C2 Coronagraph
• Indexing and Searching Distributed Astronomical Data Archives

IRAS fluxes at 60 um and 100 um are converted in the so-called far-infrared flux according to the relation: mfir = -2.5 log(2.58 f60 + f100) + 14.75 . where f60 and f100 are IRAS fluxes at 60 m and 100 m expressed in Jansky. ... The term 14.75 comes from the zero-point chosen in RC3 (p.43, Rel. ... The factor 2.58 comes from IRAS Point Source Catalog (1988). ... Flux at other wavelengths are given in the parameters: m21 , bt , it . ... HyperLeda . ...

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• Entry points
• Mean astrophysical parameters from LEDA
• HyperLEDA documentation: parameter: multiple

. Intervals of available data are coded by blue color. To read availability charts user should know the descriptor ("name") of the KP subset of interest. Table annotations include also number of version for each subset. Plot resolution is exactly one pixel per hour. Data are considered as available if at least one data point is present during that hour.

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• AZ Key parameters, 1998
• AZ key parameters, 1996
• List of currently available KP AZ.

... Apache HTTP Server Version 2.4 . ... macro_module . ... These macros have parameters. ... macro definition within a <Macro> section, following the apache style. user defined names for the macro and its parameters. macro names are case-insensitive, like apache directives. macro parameter names are case sensitive. macro parameters must have distinct names. error on empty parameter names. redefining a macro generates a warning. macro definitions can be nested... (but what for?) . ... Use of a macro: . ...

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• Tunable Kernel Parameters?
• mod_session_crypto - Apache HTTP Server
• Program parameters

Fortran 90 properties already in CF77 . ... Only the old form (fix form) of the source code is available. ... LOGICAL Default KIND number = 8 INTEGER Default int7 int15 KIND number = 6 1 2 digits = 46 7 15 radix = 2 2 2 range = 13 2 4 huge = 70368744177663 127 32767 bit_size = 46 8 16 INTEGER int31 int46 int64 KIND number = 4 6 8 digits = 31 46 63 radix = 2 2 2 range = 9 13 18 huge = 2147483647 70368744177663 9223372036854775807 bit_size = 32 46 46 REAL half Default,single double KIND ...

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• Argument association
• Specifications
• Relationship Between Auto Chirplet FF Plane and Radon Transform

... An Association Block (AB) contains for a set of raw frames all information about associated other files. ... associated calibration products . It also hosts information about pipeline reduction (recipe name, parameters for execution). ... set of specific keys (name=value) used to group the raw input files . ... column 5: associated AB of that product (pointing to the associated calib raw files) . ... further associated information: . ... name(s) of associated further information (e.g. QC1 plots) . ...

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• POLIMPLOT (V2.00) --- November00 --- POLIMPLOT (V2.00)
• SPECPSF (V1.00) --- May00 stecf.specres --- SPECPSF (V1.00)
• Load configuration, tables, and logs

Next: Star Formation Rate and Up: No Title Previous: Calculation of Evolutionary Tracks . To start calculations, we choose the distributions of the initial binary parameters: the mass of the primary ZAMS component, , binary mass ratio, , orbital separation a . ... whereas the mass ratio distribution is not. ... The zero assumption often made is that the mass ratio distribution has a flat shape, that is binaries with a high mass ratio occur as frequently as those with equal masses. ...

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• Initial binary parameters
• Dependence on the Scenario Parameters and Initial Distributions
• Restrictions on the Scenario Parameters

Results of analysis . ... IAA EOP Service . ... EOP series are regularly submitted to the IERS, and also are available at the IAA EOP Service page. EPN coordinate time series . EUREF Permanent GPS Network (EPN) coordinate time series is computed from analysis of available EUREF weekly solutions. ... Second solution is based on independent combination of individual EPN Analysis Centers' solutions . ... USNO GPS Timing Operations . ... GPS Time Series . ... EPN : European Permanent GPS Network . ...

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... spectrum . ... sfit . ... define >macro_name< : define a macro . ... meth_range <w1> <w2>: Set wavelength range for fit . data_spectrum <name> : data in "spectrum" format . ... data_sigma <sigma> : define mean standard error in data . ... data_line_set | ... NB: synth uses multiple calls to spectrum , so various Spectrum commands may also be required. synth : find optimum fit by adjusting abundances, v turb , v sin i , and v rad . ... save <fit> : Save the spectrum and best fit from synth . ...

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• sfit help file
• lte-codes: sterne model atmospheres
• Spectrum - control

... Публикации и издания Публикации профессорско-преподавательского состава СГАУ Издания проф. Сосниной Т.Н. Biosphere: Analysis of Value Parameters . ... Besides, the ways of saving the use value and value properties of biosphere are analyzed. The expediency of transformation of two-criterion theory of value into the three- criterion theory of the balance of value, where the ecologic component performs the function of the key criterion has been founded. ... BIOSPHERE USE VALUE OF THE PRODUCT: MAIN . ...

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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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• Lecture Series 2015-2016 ? Amateur Astronomers Association of New York

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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• POLIMPLOT (V1.00) --- April99 --- POLIMPLOT (V1.00)
• MAKEPRFCORR (Nov98) --- nictools --- MAKEPRFCORR (Nov98)
• MAKEFLAT (Sep99) --- nictools --- MAKEFLAT (Sep99)

Bismuth chalcogenides (Bi 2 Se 3 , Bi 2 Te 3 ) . ... 30 30-40 mm . ... Available orientation . 0001) . ... Available dopants . any (except gases and radioactive elements) . ... Bismuth chalcogenide crystals: . ...

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• VI International Astronomy Olympiad: information available before (in Russian)
• VI International Astronomy Olympiad: information available before
• Department of Solid State Physics MIPT

The AstroGuide . ... AstroGuide | ... AstroGuide Listing . ... See many more Astronomy Listings by: Category or Alphabet . The BPAA is a non-profit amateur astronomy organization. We have constructed and operate the Edwin E. Ritchie Observatory in the Helix House at Battle Point Park. ... Listed Since February 14, 1999 . ... Web Site . ... Unless otherwise specified, web site content Copyright 1994-2016 John Huggins All Rights Reserved . dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

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• Aberrator Startesting Software, AstroGuide Listing