... When I display the weight map generated for my final drizzled image (or any of the single drizzled images as well), there seem to be representations of the objects in my science image. ... Most likely you need to refine the parameters that are set during the driz_cr step which detects cosmic rays in each of your science frames. ... I've calculated refined offsets between my science images but when I supply MultiDrizzle with the delta shifts the final image is not aligned properly. ...

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• http://www.stsci.edu/hst/nicmos/documents/isrs/isr_98_010.pdf
• Results
• Herschel Images and Results for the Magellanic Clouds

... The eboxdetect task has two different modes of operation: (1) local detection and (2) map detection. eboxdetect is first run in local mode. The local mode source lists serves as input for task esplinemap which creates background maps (one per energy band for each EPIC instrument) which are then used to run eboxdetect in map mode. ... In both modes, source searching is only performed in the area of the images which is marked by an optional detection mask created by task emask . ...

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• Algorithm

... Three different techniques for averaging have been introduced. ... The average functions mentioned above will normally produce a result frame whose world coordinates are the intersection of the father frames' world coordinates. ... Averaging statistically consistent values --- љ This command differs somewhat from the purely mathematical functions of the previous two commands in the sense that it tries to anticipate some of the astronomical content of the input data frames. ...

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• Sky Subtraction
• Results and Discussion
• Flat-Fielding

Next: Acknowledgements Up: World Wide Web version Previous: Page contents . ... Part of the table and a cartoon figure of the track calculated for the default set of the initial parameters are shown in Fig. 1 and 2. In the future, we intend to made available calculations of a large number of binary systems assuming different intial distributions, chemical composition, etc., to construct a "Galaxy at will", as well as various interface facilities. ... Fri Jun 21 19:17:07 MSD 1996 ...

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• Results of calculations
• Introduction
• ADS Abstract Service Results

... 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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• A Method for Minimizing Background Offset Errors When Creating Mosaics
• Towards Optimal Analysis of HST Crowded Stellar Fields
• ADASS 2003 Conference Proceedings

... Data . AAS 221 . AAS 219 . ... The first thing to note is that Twitter does not guarantee to return all matching Tweets, whatever method is used (unless you have direct access to their "fire hose", which I don't). ... This should result in the same results as my REST-based search (method 2), since the volume of Tweets was probably not enough to cause this site to miss Tweets based on their collection strategy . ... A search for the tag #aas219 (case insensitive) using the Twitter REST API . ...

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• *xflux, hxflux* - Calculation of X-ray Flux
• Stars with Less Secure Periods
• Calculation of Extinction from Optical Colors

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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• ST-ECF Grism Spectrum Software for NICMOS Grism Data
• The Formation and Evolution of LMC Rich Star Clusters: NGC 1818

Some recent results ( see ) attracted the attentions of astronomers working on field which could benefits from photon counting techniques with high speed and spatial resolutions as adaptive optics. ... Fasti has been designed to be fast and largerly configurable. ... The data rate attined in the best case (30 Mhz), give no impossible load to the digital acquisition in the photon counting mode, since data are 1 bit only, they can be parallelized, giving a maximum speed of about 940.000 32 bit word/sec. ...

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• NICMOS3 Detector for Spectroscopy
• IBIS - Flat Fielding
• Comet Shoemaker-Levy 9

... Status of the numerical solutions and validation 2. ... Coupling of "solid" Earth components, e.g. core ­ mantle (Dehant et al.) ... Consistent relativistic formulation of Earth rotation (Gerlach, Klioner, Soffel) Status of the numerical solutions - 2 · The results from numerical solutions suffer from ­ Simplified solid Earth models ­ Incomplete Earth system models or neglecting of certain parts or neglecting of certain coupling mechanisms ­ Methodological limitations of computations...

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• http://www.gao.spb.ru/english/personal/malkin/publ/zm03d.pdf
• http://www.gao.spb.ru/english/personal/malkin/publ/zm03e.pdf
• http://www.gao.spb.ru/english/as/j2014/presentations/bezmenov.pdf

. Minsk bibliography on light scattering . Related Internet resources . (under construction) . Here we will give links to such Internet resources as follows: . SCATLIB . contains lists of references to papers devoted to calculations of light scattering by particles of different shapes . and so on. To homepage . © 1990,2001 Victor Babenko (Bibliography compiling) . © 2001 Serge Beletsky (Design & Programming) . E-mail: serge@cyteg.com . Last updated: 2001/10/30

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• Query Results from Astronomy Database
• Model realization and some results
• Introduction

The beam pattern and the polarization characteristics . of the radio telescope RATAN-600 . The Mueller matrix elements was computed via formulas [1]: . ... The BP were computed by the aperture method, proceeding from the fild distribution in the aperture of the primary mirror. The components of the main and cross-polarization components of the electric field in the vertical aperture of the primary mirror was computed in Frenel diffraction approximation. ...

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• Results scientific researchs 7
• Description of algorithm
• shmidt_e

Next: Pilot Survey Up: Minutes of the 1st Previous: GALFA Surveys . ... The minimum integration time required to achieve a given mass sensitivity scales as distance to 4th power so the depth of survey increases only as t int to the 1/4. ... To predict what ALFA might see for several surveys, I have performed a set of simulations governed by the following: . ... ZOA survey: Assuming integration time of 300 sec, covering 10 (more than pulsar survey suggested), within the AO limits . ...

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• Arecibo Galaxy Environment Survey (AGES)
• HIDEEP and HIJASS Results
• testing radar dataking 31oct13

HI source finding: 2 novel approaches ATNF, December 2010 Outline · Background · What is source finding? ... Motivation for developing new HI source finding methods · Novel source finding methods · · · · General idea Iterative 3-D median smoothing Characterised noise method Wavelet method · Summary Background What is source finding? ... 3-D median smoothing: Purpose · Goal: Reduce noise while preserving shape · Particularly edges · Median works because it's non-linear · Consider this, Iter. ...

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• http://www.atnf.csiro.au/research/Astro2008/Postings/Daniel_Yardley.pdf
• The completeness and reliability of threshold and false-discovery-rate source
• Weighting

Results of calculation of O – C can be saved and printed with the help of usual means of Windows. ... Saving and printing results . It should be taken in mind that the type of extension that is actual in default of specifications is “.ocr” ( O – C results ). ... NOTE : Paper size different from A4 is not recommended: in this case the part of data can be out of print area. If printer resolution is lower then 300 dpi then problems can occur when printintig text in Portrait mode. ...

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... The experience of determination of the link between radio sources and dynamical reference frames is presented. To obtain this connection we used a series of very long baseline interferometry (VLBI) observations of the spacecraft Phobos-2 and angularly nearby quasars. ... The dynamical reference frame is determined by equator and equinox of these ephemerides. ... References . ... The relative orientation of the radio and dynamical reference frames can be described by a sequence of three rotations . ...

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• Computing dispersive atmospheric delay with AATM Bojan Nikolic web pages (r.
• Astrophysics Group Fringes and Power Spectra from COAST
• Preliminary results of OOF holography at the GBT

SOME RESULTS FROM INTMINS . The experiment can be performed when the electron beam (instrument ISTOCHNIK ) and plasma blobs (instrument ARIEL ) are injected approximately along or perpendicular to the Earth's magnetic field. ... The pulses of frequency of 1000 Hz will generate EM waves and its harmonics. ... To increase the electron gun pulse duration up to D t = 0.5 f -1 ( D t = 5x10 -4 s) and to stabilise their frequency as good as possible. ... Back to the INTMINS Main Page ...

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• FM-3I Instrument
• Comet Shoemaker-Levy 9
• Field-aligned potential drops [Oulu]

... A three-cell test section roughly representative of the primary mirror was provided for this test by the Steward Mirror Lab. ... Additionally, the tests are intended to determine relative airflow vs. pressure drop characteristics for each of the air flow patterns so the results can be evaluated both as a function of flow rate and of pressure drop along the flow path. ... The bottom (top as installed) was cut out so it could close the chamber for heating and be removed for the cooling tests. ...

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• Deforming Plug-plates
• Astigmatism II
• Untitled Document

Past Maria and Eric Muhlmann Award recipients . ... The Maria and Eric Muhlmann Award of the ASP is given annually for recent significant observational results made possible by innovative advances in astronomical instrumentation, software, or observational infrastructure. ... Nominations . ... Letters of nomination must be received in the office of the Astronomical Society of the Pacific on or before 1 January of 2013 . ... The Award . ... Submitting Nominations . ... Maria and Eric Muhlmann Award . ...

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• ASP: Light Pollution
• ASP: Richard Berry CCD Workshop
• ASP: Using Multicultural Dimensions to Teach Astronomy

THE PHOTOMETRIC RESEARCHS OF THE MERCURY'S SURFACE BY MEANS OF DIGITAL MODELS. ... The surface brightness of Mercury was measured Danjon (1933, 1949, 1953) and Harris (1961) in phase angle 3o-123o. The analysis of the various data of the integral photometric gives the results of determination of the main photometric constants for Mercury. ... THE PHOTOMETRIC RESEARCHS OF THE MERCURY'S SURFACE: S.G. Pugacheva The surface brightness of the Mercurian images was established on the geologic map Mercury. ...

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• http://selena.sai.msu.ru/Pug/Publications/Pugacheva%20LPS%2041.pdf
• http://selena.sai.msu.ru/Bus/Publications/m44_14_busarev_etal.pdf

... S.P. KOROLEV ROCKET AND SPACE CORPORATION ENERGIA . ... OAO RSC "Energia" . ... Company's History . ... History . Brief History of Rocket and Space Technology . ... Project History . ISS Russian Segment . Steps of ISS Assembly . ... Chronology of Extravehicular Activity . ISS 45/46 . ... Rocket Space Complexes . ... Automatic Space Systems . Universal Space Platform . ... History of flights . ... Man in space | ... Work station" set. ... 2015 JSC "S.P. Korolev RSC "Energia" . ...

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