True Color Image Gallery: Galactic SNR | ... nH was derived by fitting the trail of central source which is believed not to be piled-up. nH was derived from the trail of the central source . ... Statistic value = 53.6161 . ... spectrum was refitted with nH fixed at the value derived from the trail of central source. source=(xswabs * powlaw1d) . ... shell was fitted by 3 thermal plasma model with nH fixed. source=(xswabs * ((xsraymond + xsraymond) + xsraymond)) . ... Back to SNRJ 0540.1-6919 Index . ...

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• Chandra Images for SNR J0526.0-6604
• Chandra Images for G029.7-00.2
• Chandra Images for G011.2-00.3

... use frames summary class fields routine details file attributes . ... AUTHOR: Craig B. Markwardt, NASA/GSFC Code 662, Greenbelt, MD 20770 craigm@lheamail.gsfc.nasa.gov UPDATED VERSIONs can be found on my WEB PAGE: http://cow.physics.wisc.edu/~craigm/idl/idl.html . PURPOSE: Compute confidence limits for chi-square statistic . ... CALLING SEQUENCE: DELCHI = MPCHILIM(PROB, DOF, [/SIGMA, /CLEVEL, /SLEVEL ]) . ... result = mpchilim( p , dof , sigma= sigma , clevel= clevel , slevel= slevel ) . ...

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• GLSFit.pro (JWST Pipeline routines in IDL)
• generate_ramp.pro (JWST Pipeline routines in IDL)
• analyze_dark_ramp.pro (JWST Pipeline routines in IDL)

... The measured Mg2 index corresponds to a certain defined region of the object and, after systematic corrections applied to series of measurements, it is reduced to a common standard aperture (for galaxies only). The compilation of Mg2 measurements may be accessed in HyperLeda. mg2 is the Mg2 index in mag. The Mg2, as well as velocity dispersions, are standardized to an aperture r norm of 0.595 h -1 kpc, which is equivalent to an angular diameter of 3.4 arcsec at the distance of Coma. ...

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• Mean astrophysical parameters from LEDA
• Parameter estimation
• HyperLEDA documentation: parameter: vdis

... We demonstrate through numerical simulations that model parameters estimated with our technique are essentially bias-free, even when the average number of counts per bin is 1. ... The IW technique avoids such biases by estimating through successive iterations, where for each iteration, j, , and the best-fit parameters are determined by minimization of . ... In our sample, we find that the minimum values and best-fit parameters converge after about 6 iterations. ...

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• Recent Advances in Parameter Estimation in Astronomy with Poisson-Distributed

In this gallery are many images of Low Surface Brightness Galaxies which have recently been discovered and analyzed. ... The central surface brightness of this galaxy is 24.28 . Malin 2 This galaxy is another huge disk galaxy with a scale length of 15 kpc and a redshift of 15000 km/a. The high surface brightness knot in one of its spiral arms actually has the same color, luminosity and H-alpha equivalent width as the entire Large Magellanic Cloud . ... Truly it is a Low Surface Brightness Galaxy. ...

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• The Galaxy Gallery: Messier Objects

... Meta Index / Home Page This section documents the parameters recognized by this task (if any). Parameter . Mand . ... Default . Constraints . table . ... none . The table containing the columns of interest . column . ... list of strings . ... The list of columns for which statistical information is required. resultfile . ... The list of columns for which statistical information is required. ...

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... The following document provides a short instruction on the reduction of synthesis observations with the WSRT using AIPS. ... The aim of the instructions below is to provide a check list of reduction steps to be taken and of the important parameters to be set in each task. ... Please consult the AIPS Cookbook for detailed information about data reduction with AIPS (and various Banana recipes). TASK 'FITLD' . ... GETN n . ... TGET 'INDXR' . ... DOCAL 1 . ... GAINU 2 . ... IMAGRPRM 0 . ...

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• Central Processor Manager CentralProcessor 0.11 documentation
• User Parameters - Continuum Source-finding CentralProcessor 0.11 documentation
• uvfstats

... we show that the comparison between the calculated and observed numbers of the most ``fragile'' (from the point of view of the binary evolution scenario )   galactic binary types (such as X-ray low-mass X-ray binaries (LMXB), cataclysmic variables (CV),   Be-stars   with compact companions, relative number of visible binary radiopulsars   with normal and compact secondary components) impose certain constraints on the feasible initial ... Phenomenological Kick Velocity . ...

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• The Model
• The Gravimagnetic Parameter
• Initial binary parameters

... Focal reducer main parameters . Focal ratio at the 6m telescope . ... DQE (telescope+SCORPIO+CCD) . 80% in Direct Image mode . 30% in Long Slit mode . 20% in Fabry-Perot mode . Limit magnitude for images . R=26.8 (S/N=5 for Texp=1800 sec, seeing 1.5'') . Limit magnitude for low-resol. spectra . R=24.0 (S/N=10 in continuum, Texp=7200 sec) . ... Size, pixels . ... Pixel size, mkm . ... 83% Plot of the DQE . ...

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• проект SCORPIO-2: parameters
• Spectral energy distribution
• Spectrometric complex LRS

... Space flight . ... Zero Gravity . ... Characteristics of a Complex Flight: . ... Characteristics of the Reduced Gravity (Lunar Gravitation): . ... Characteristics of the Reduced Gravity (Martian Gravitation): . ... Services / Zero Gravity: General description Technical description Flight parameters Photo gallery Price . ...

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• Photo gallery: pictures of cosmonauts and participants in zero gravity flights.

... Parameters of the Moon-perturbed orbit . ... From orbits consistent with this limitation and with the date of the launch October 1, 2000 as an example, an orbit was selected with apogee directed to the North Galactic pole at the begining and rotation of orbit plane was maximized. The initial state vector is given in the inertial coordinate system in epoch J2000.0. ... The orbit has initial perigee radius Rp=7000.0 km, initial apogee radius Ra=343000.0 km and initial period T=8.453 days. ...

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• Results of measurements of SRT antenna parameters in Pushchino

... Learning set is formed on basis of the Taken' algorithm. ... For 10, 100, 200, 300 day forecast the time lag was correspondingly = 10, = 100, = 200, = 300. ... For every forecast (10, 100, 200, 300 days) ANN started k = 10 times. ... On figure, 1 it is shown the MAE and RMS statistics for 10-, 200- and 300-day forecast for Xp : M AE = 1 n i=n |f orecastav erag ei - realv aluei |, ... i=1 139 RMS 300 MAE 300 RMS 200 RMS 10 MAE 10 MAE 200 Figure 1: 10, 200, 300 day statistics for Xp forecast. ...

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• Pulkovo Observatory
• Pulkovo VLBI Analysis Center

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• Vladimir P. Reshetnikov's Home Page
• Database of Optical Properties -- Level: subpage
• Model realization and some results

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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• Tunable Kernel Parameters?
• Kernel tunable parameters
• Where are the tunable parameters of the kernel?

The pdev spectrometer dshift parameter (see layout of spectrometer scaling ) down shifts the output of the power computation before accumulating the spectral values in the 40 bit accumulators. ... As an example: a 1 second integrations at 170 MHz with: (A/D=48,pshift=0x1555, dshift=0,ashift=0) has LO feedthrough birdies close to 1.5e9. The maximum allowed value is 4e9. ... The allowable range for dshift had been computed from the spectral mean with dshift = 0 (see page 2 of the plots) . ...

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• Nominal Parameters of Galactic Plane Survey
• Alfacal
• HIPASS parameters Barnes et al (2001), Ryan-Weber et al. (2002), Zwaan et al

The starting page - The catalogues page - The list of the PUL2 fields - The list of the Pul-3(Pul-3SE) fields - The list of the PUL_ERS fields . please read short description of the access form controls . ... Right Ascension (ICRF/Tycho-2) J2000 at the central epoch of obs. (hours, minutes, seconds) (Obligatory parameter) . ... proper motion in RA (*cos(DE)) (ICRF/Tycho-2). (mas/yr) . ... Check the apropriate checkbox to output these data and radiobutton to select stars within interval. ...

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• The Pul_ERS astrometric catalogue. Data access form

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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• POLIMODEL (V1.00) --- April99 --- POLIMODEL (V1.00)
• MARKBACK (Aug99) --- nictools --- MARKBACK (Aug99)
• The Stellar Population in the NICMOS Parallel Fields

Next: Parameters Up: How to use CONSTRICTOR Previous: NPOI raw data files Contents . The parameter file contains information for CONSTRICTOR on the location of the raw data files, start and stop times, integration time, etc. ... The parameter file, YYYY-MM-DD.par , can now be created using the rawlist procedure of . ... Check beginning and tail of the listing for each file. ... Next: Parameters Up: How to use CONSTRICTOR Previous: NPOI raw data files Contents Christian Hummel 2015-04-28 ...

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• ESO - Science Announcements
• extractStat
• web4 Astroclimatology

... Thus all regions of the 0.94-2.50 micron wavelength range accessible from Mauna Kea can be recorded using five fixed angle gratings. ... Grating Angle . ... Efficiencies for the NIFS gratings are shown above. The NIFS spectrograph uses a Bouwers collimator and a refractive camera. ... With these assumptions, the NIFS system efficiency including the Gemini telescope optics but excluding the transmission of the adaptive optics system is about 0.17 e - /photon at J , and 0.22 e - /photon at H and K . ...

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• RSAA Honours Courses (2006)
• Towards a Truly Unified Model of AGN
• Claire Beech reducing data from the Melbourne Observatory

... Introduction: In the present work the morphometric parameters for 87 large martian craters [1](with diameters from 411 up to 110 kms) have been determined: depth of a crater, the relation of depth of a crater to diameter (/D), height of a rim ­ h, with the help of profiles constructed on the basis of supervision of space vehicle MGS [2].The comparison with similar morphometric parameters of large lunar craters also is fulfiled. ... 2000) Morphological Calague Of the Craters Of Mars. ...

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• http://selena.sai.msu.ru/Greg/Publications/ms40/81_Ushkin_Michael.pdf
• http://selena.sai.msu.ru/Pug/Publications/ms42/m42_60.pdf
• http://selena.sai.msu.ru/Pug/Publications/m44_70_pugacheva.pdf