... User Guide ] Task: early Purpose: Flag data which has early/normal problems. Categories: calibration, uv analysis EARLY is a Miriad task which flags visibility data that it suspects contains early/normal problems. ... If the scatter exceeds some number of sigmas, then the data are assumed to be affected by the early/normal problem, and the entire record is flagged. ... If the signal is noise dominated, no early/normal problems can be detected, and the data will not be flagged. ...

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• Image Combination

... One possible application of a solar sail is a spacecraft to warn Earth of approaching interplanetary disturbances and shocks. ... Spacecraft that can provide such a warning are currently stationed at (or near) the Lagrangian L1 point , between the Earth and the Sun--at about 4 times the distance of the moon and 1/100 times that of the Sun. ... Because of the greater distance from Earth, the Earth's pull there is weaker, not enough to make the spacecraft match the Earth's motion around the Sun. ...

Åùå â ðàçäåëå: (Ïîêàçàòü âñå ðåçóëüòàòû (>958) - www.cosmos.ru/ )

One possible application of a solar sail is a spacecraft to warn Earth of approaching interplanetary disturbances and shocks. ... Spacecraft that can provide such a warning are currently stationed at (or near) the Lagrangian L1 point , between the Earth and the Sun--at about 4 times the distance of the moon and 1/100 times that of the Sun. ... Because of the greater distance from Earth, the Earth's pull there is weaker, not enough to make the spacecraft match the Earth's motion around the Sun. ...

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... HST . WF/PC-1 Early Acquisitions . ... Data . ... HST Overview . Overview . ... We will therefore undertake this task on your behalf. ... The task of the GO will be to provide RSB (contact person: Danny Golombek) with the x,y coordinates of their objects (usually an offset star plus the target). ... Great care should be exercised in computing the onboard acquisition exposure time for the offset star, and in selecting the aperture to avoid problems with the error in the absolute coordinates. ...

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• STIS Instrument Handbook
• Andy Fruchter's Homepage
• CL Script for Correcting Exposure Times Affected by Take Data Flag Down

... A one line summary for each source detected by the EPIC detection tasks is created. The summary information is a subset of the information given in the emldetect source list table. ... M2_BOX_ID_SRC columns). emldetect source lists from different detection runs can be merged into one summary source list. ... The cross-correlation radius can be specified by an input parameter. ... In the case of several source lists from one instrument, count rates are averaged and exposure map values are added. ...

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• Generation from In-Orbit Data
• Combined Exposure Map

... Next: Unsupervised Catalog Classification Up: Object Detection and Previous: Classification of Objects . ... Multi-resolution allows for image analysis in terms of different scales. ... This approach is used for the detection (and subsequent analysis) of globular cluster systems around elliptical galaxies, and for image characterization and object trawling in large image databases. ... The applicability of this approach to object detection in large image collections has been investigated. ...

Åùå â ðàçäåëå: (Ïîêàçàòü âñå ðåçóëüòàòû (>1993) - www.adass.org/ )

• Towards Optimal Analysis of HST Crowded Stellar Fields
• The ESO Imaging Survey Project: Status and Pipeline Software
• The SAX-LEGSPC Data Reduction and Analysis System: An Example of a Minimalist

... Building Galaxies in the Early Universe . ... Explanation: What was the very early universe like? To help find out, astronomers pointed the Hubble Space Telescope between bright nearby objects to create one of the deepest images ever -- the Hubble Ultra Deep Field (HUDF). ... A recent analysis of the HUDF focused on the smallest, faintest and most compact galaxies imaged. ... Publications with keywords: galaxies - early universe . Publications with words: galaxies - early universe . ...

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• Rosetta Approaches Comet Churyumov Gerasimenko
• Approaching the International Space Station
• XWare > APOD

... ESO is building what will be the World's largest optical telescope array, The Very Large Telescope (VLT). The VLT Project organisation is responsible for the design and construction of the Unit Telescopes, including enclosures, optics, adapter-rotators and coating unit. ... Unit Telescopes Overview - This page is outdated, an update is in process. ... Secondary mirror (M2 Unit) - This page is outdated, an update is in process. ... Coating Unit - This page is outdated, an update is in process. ...

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• ESO - Galaxy Clusters in the Early Universe
• ESO - Status of ALMA Early Science
• ESO - Completion of ALMA Early Science Cycle 1 and start of Cycle 2

... user-defined data file formats . ... better integration with a user's analysis routines To add such functionality to SAOimage, we developed the XPA Messaging System that allows X programs to define points of public access through which data and commands can be exchanged with external programs. ... We have utilized XPA to develop "SAOimage: The Next Generation" (SAOtng), an extensible image display service that can cooperate with other processes and programs. ... SAOtng help pages . ...

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• Jonathan's ASC documents
• Who is tweeting about #AAS225
• ChaMPlane

... 2014 August 11 . Rosetta Approaches Comet Churyumov-Gerasimenko . ... Explanation: What does it look like to approach a comet? Early this month humanity received a new rendition as the robotic Rosetta spacecraft went right up to -- and began orbiting -- the nucleus of Comet 67P/Churyumov-Gerasimenko. ... Later this year, Rosetta is scheduled to release the Philae lander , which will attempt to land on Comet Churyumov–Gerasimenko's periphery and harpoon itself to the surface. ... About APOD | ...

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• APOD: 2001 April 30 - Approaching the International Space Station
• APOD: 2007 September 10 - Building Galaxies in the Early Universe
• APOD: 2014 August 3 - Dark Shuttle Approaching

The multiscale analysis of heterogeneous structures is actually an important and effective tool of mathematical modeling in physics, technique and biology. ... The special year will extend the existing cooperation between French and Russian researchers in the multiscale analysis and in mathematical modeling in hemodynamics, taking into consideration the mass transport, coagulation, fluid-structure interaction and other aspects. ...

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• Functional analysis seminar (Spring 2009)
• Semiclassical Microlocal Analysis (Fall 2003)

Neptunes in the Noise: Improved Precision in Exoplanet Transit Detection AimÈe Hall , Simon Hodgkin , Gabor Kovacs and Don Pollacco 1 1 1 1 2 Institute of Astronomy, University of Cambridge 2 Department of Physics, University of Warwick Figure 2 (right): Distribution of radii of all known exoplanets (grey), with those from Kepler (green) and SuperWASP (blue) also shown. We present early results from a new analysis of raw data taken with the SuperWASP telescope[1]. ...

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• PPEUC Programme - Cosmic Microwave Background Workshop
• Astrophysics Group Galactic Á€˜hailstormÁ€™ in the early Universe
• Leverhulme Collaboration

... The distinction of our approach is in that we unite the Actor Prolog concurrent ob ject-oriented logic language [ 1,2,3] with the Structural Analysis and Design Technique (SADT) diagrams to obtain new issues in the following areas: 1. ... Graphic user interface management. ... The individual blocks of visual user interface based on the SADT diagrams are implemented by using parallel processes of Actor Prolog. ... We applied the visual programming method for logic programming of Internet agents [4]. ...

Åùå â ðàçäåëå: (Ïîêàçàòü âñå ðåçóëüòàòû (>458) - www.cplire.ru/ )

PUL VLBI Analysis Center . ... IVS : International VLBI Service for Geodesy and Astrometry . ... An IVS VLBI Analysis Center at the Central Astronomical Observatory at Pulkovo of the Russian Academy of Sciences, also widely known as Pulkovo Observatory, has been organized in September 2006. ... The center is a part of the Pulkovo EOP and Reference Systems Analysis Center (PERSAC) . ... Results of VLBI data analysis can be found at Pulkovo EOP and Reference Systems Analysis Center (PERSAC) page. ...

Åùå â ðàçäåëå: (Ïîêàçàòü âñå ðåçóëüòàòû (>271) - www.gao.spb.ru/ )

• Pulkovo EOP and Reference Systems Analysis Center (PERSAC)

... Èíôîðìàöèÿ Ðóêîâîäñòâî è ïðåïîäàâàòåëè Ìÿñíèêîâ Åâãåíèé Âàëåðüåâè÷ . ... Ïóáëèêàöèè . ... Myasnikov E.V. A Nonlinear Dimensionality Reduction Using Combined Approach to Feature Space Decomposition // CEUR Workshop Proceedings, 2015, , , 2015 ã., P. 85-95 . ... Myasnikov E.V. Application of the nonlinear dimensionality reduction method with the use of reference nodes for solving the problem of multidimensional data search // Pattern Recognition and Image Analysis. 2015. ...

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... Abstract: The present investigation is a continuation of earlier work by Hasan \& Christensen-Dalsgaard (1992) and Banerjee, Hasan \& Christensen-Dalsgaard (1995), who has examined the effects of a weak vertical magnetic field on the normal adiabatic modes of an isothermal atmosphere by combining a semi-analytic approach, based on asymptotic dispersion relations, with numerical solutions. ... It was predicted that due to strong mode coupling the eigenfrequencies in these regions become complex. ...

Åùå â ðàçäåëå: (Ïîêàçàòü âñå ðåçóëüòàòû (>1972) - star.arm.ac.uk/ )

• C.J. Butler, Research Astronomer
• Armagh Observatory Preprint No. 300
• Armagh Observatory Preprint No. 301

. NASA's New Horizons captured Pluto on July 13, 2015, when the spacecraft was 476,000 miles (768,000 kilometers) from the surface. This is the last and most detailed image sent to Earth before the spacecraftòÀÙs closest approach to Pluto. The color image has been combined with lower-resolution color information from the Ralph instrument that was acquired earlier during the day. NASA/JHUAPL/SwRI

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• Explosion of galaxy formation lit up early universe | Astronomy.com
• Green pea galaxies could help astronomers understand early universe |
• Discovery's launch will be scheduled for no earlier than February 3 |

... The large body of near infrared observations presented in Testi et al. (1997; 1998) are analysed with the aim of characterizing the young stellar clusters surrounding Herbig Ae/Be stars. The results confirm the tendency of early Be stars to be surrounded by dense clusters of lower mass "companions", while Ae stars are never found to be associated with conspicuous groups. ... Only the most massive stars (10-20Msun) are found to be associated with dense (10^3 pc^-3) stellar clusters. ...

Åùå â ðàçäåëå: (Ïîêàçàòü âñå ðåçóëüòàòû (>6243) - www.arcetri.astro.it/ )

• Early Astronauts
• Omission in earlier rate-limit...
• The Discovery and Early Study of Shoemaker-Levy 9

Next: The STScI NICMOS Calibration Up: No Title Previous: CONICA: The high resolution . The STScI NICMOS Calibration Pipeline . Introduction . ... Dark Current Subtraction . ... Input Data . ... Scalar Background Subtraction . 2-D Background Subtraction . ... Status and Goals of the NICMOS Calibration Plan . ... Photometry . ... Photometric Performance of NICMOS . ... NICMOS Photometry. ... ST-ECF Grism Spectrum Software for NICMOS Grism Data . ... Analysis . ... STScI NICMOS Software . ...

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• STScI NICMOS Software
• The Formation and Evolution of LMC Rich Star Clusters: NGC 1818

The Use of Neutrals for an Improvement of Higgs BR A Review of and an Update on Higgs BR Jan Strube, Jeffrey J. Early and James E. Brau jstrube@darkwing.uoregon.edu University of Oregon ALCPG Victoria LCWS, 2004 ­ p.1/18 Overview Review of previous analyses Battaglia (Tesla TDR) Potter, Brau, et al. ... JLC) Presentation of new approach ALCPG Victoria LCWS, 2004 ­ p.2/18 Battaglia - 1999 s =350 GeV, mH =120 GeV Two studies (cut-based): 1. CDR Ver texer 2. ...

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• Radiation Dominance in the Early Universe
• CCDs for Material Scientists
• Thermal History of the Universe