... 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

... 739C As one part of a program to detect complete samples of active extragalactic objects, the 3.36x10^-3 sr field centered on alpha=12h04min, delta=+11deg30' (1950.0) was mapped with the Very Large Array at 1411MHz. Sixty-seven maps cover this field so that no point is more than 15arcmin from the nearest map center. ... The rms map noise is 0.030 + 0.001 mJy, and the resulting source list is complete to a map peak flux density S_p = 0.2 mJy within 25 arcmin of the field center. ...

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• Correspondence Analysis

XMM-Newton Science Analysis System Page: 1 atthkgen June 28, 2006 Abstract The task atthkgen produces a FITS le with a single bintable extension, con- taining the entire attitude information for a complete observation. ... The le will contain, along with the time (TIME), the AHF and OM attitude information (i.e. RA, Dec, position angle - AHFRA, AHFDEC, AHFPA, OMRA, OMDEC, OMPA), with NULL (`INDEF') values in all three elds indicating bad attitude quality. ... This will give many more AHF entries. ...

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• http://xmm.vilspa.esa.es/sas/8.0.0/doc/atthkgen.ps.gz
• http://xmm.vilspa.esa.es/sas/5.4.1/doc/atthkgen.ps.gz
• http://xmm.vilspa.esa.es/sas/6.1.0/doc/atthkgen.ps.gz

GHRS Side 2 Cycle 4 Calibration Plan -- 8 Ma y 1996 ID Proposal Title Total Estimated S/C Time (hours) Calibration accuracy (where applicable) Notes Results External Internal Goal Achieved 5545 GHRS Side 2 Pulse Height Analysis/ion Test--- Cycle 4 0.85 Completed 5546 GHRS Side 2 Threshold Adjustment T est--- Cycle 4 1.23 Completed 5547 GHRS Side 2 Detector Calibrations--- Cycle 4 2.22 ...

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• Echelle Grating Blaze Function Zero Points

http :// hea-www.harvard.edu / AstroStat /slog/ 2007 / change - point - problem / Weaving together Astronomy+Statistics+Computer Science+Engineering+Intrumentation, far beyond the growing borders Fri, 01 Jun 2012 18:47:52 +0000 hourly 1 http ://wordpress.org/?v=3.4 http :// hea-www.harvard.edu / AstroStat /slog/ 2007 / change - point - problem /comment-page-1/#comment-64 vlk Fri, 17 Aug 2007 22:09:06 +0000 ... Defining peaks sounds like point estimation from functional data analysis. ...

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• The AstroStat Slog Blog Archive Change Point Problem
• Comments on: [ArXiv] Complete Catalog of GRBs from BeppoSAX, July 13, 2007 By:
• SAO RSDC Home Page - RRA - PSPC

... Space Research Institute . Main . ... Main research and development work completed in 2010 and ready for implementation . Elaboration of automatic technology for analysis of abnormal changes of vegetation status based on satellite data . ... Satellite MODIS-Terra image, obtained on May, 17 2010. ... Main research and development work completed in 2009 and ready for implementation . Main research and development work completed in 2008 and ready for implementation ...

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• Main research and development work completed in 2012 and ready for
• Main research and development work completed in 2009 and ready for
• Main results of the experimental and theoretical research completed in 2011

. Next: Conclusions Up: The command line interface (TEXT CEILIDH ONLY) Previous: Advantages of the command line interface . At certain times, the teacher may close a complete course, or a unit, or an exercise. These perhaps represent parts of the course which are under development, or which must be kept unmodified for administrative reasons. Dave.Marshall@cm.cf.ac.uk . Wed Sep 14 10:06:31 BST 1994

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• Advanced Pointer Topics
• LWN: Driver porting: completion events
• Program Listings

... Each leg of a cross is +/- 3 beams and takes 60 seconds to complete. 1 pattern takes about 5 to 6 minutes to complete. For each leg fit for the main beam and the 2 sidelobes. Remove the sidelobes and then do a 2d fit to the main beam of the 4 legs. The model made after alfa was installed and the kevlar cables were installed on the feed tower in the dome: . The measured errors while making the model. The model fit to the measured errors. ...

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• http://www.naic.edu/~phil/calsbn/jan01/surfadj_jan01.html
• pntModelGradients
• Useful Stuff

... Ignacio Ugarte Urra's PhD thesis topic is the investigation of coronal bright points. In his first paper (in collaboration with Gerry Doyle and Maria Madjarska) he investigated the formation, evolution and decay of a coronal bright point via a spectroscopic analysis of its transition region counterpart and the evolution of the underlying magnetic bipole during 3 days of almost continuous observations. ... In general the bright point has a radiance 4 times higher than that of the network. ...

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• Armagh Observatory PhD Theses
• Bright Point Studies
• C.J. Butler, Research Astronomer

Up: Sky Surveys . ... The object catalogue and compressed pixel data are stored online and are accessible via the WWW. ... small area (up to 15arcmin) pixel images with attached object catalogue, . ... The primary data format is FITS for both images and binary tables of object catalogues, which enables porting of the data into established software packages. ... In this way, it is possible to browse the data by clicking on objects in the image display or the catalogue list to highlight them in both. ...

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• An Extragalactic Point Source Simulator for SIRTF Pipeline Testing
• ADASS 2002 Conference Proceedings
• The Time Interferometer: Synthesis of the Correlation Function

... Pre-university education . ... Samara region . ... University at a glance . ... A group of young scientists of Samara University under the guidance of the candidate of chemical sciences Yevgeniy Aleksandrov began to make the most extensive database in the world for the structure and physical properties of crystalline coordination polymers. ... The idea of making a database for coordination polymers already exists in the scientific community of the world. ... SAMARA STATE AEROSPACE UNIVERSITY . ...

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• Dynamic tests of the scientific equipment 'Contact' have been completed in SSAU

User Parameters - Continuum Source-finding ========================================== Source-finding is run in two ways within these scripts. ... The source-finding applies a spatially-varying signal-to-noise threshold, and fits 2D Gaussians to detected islands to create a component catalogue. ... Whether to do the source-finding with Selavy on the | ... SELAVY_NSUBX`` | ... doc:`../analysis/selavy`) | up, allowing parallel processing in the source-detection. ... doc:`../analysis/thresholds`) | ...

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• Complete ionisation of the neutral gas: why there are so few detections of
• Package: mt
• casacore: casa::ImageRegion Class Reference

... There are some generalizations of the classical Eisenbud-Levine-Khimshiashvili formula for the index of a singular point of an analytic vector field on $R^n$ to vector fields on singular varieties. ... For a variety with an isolated singularity, we define an index of a (real) 1-form on it. In the complex setting we define an index of a holomorphic 1-form on a complex isolated complete intersection singularity (icis) and express it as the dimension of a certain algebra. ...

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• Calculus-1(fall 2005)
• Conference "Combinatorial Methods in Physics and Knot Theory" (February 2005)
• Yu. Burman: Publications

Microsymposium 34, MS015, 2001 TO THE DISCOVERY OF THE "SOUTH POLE - AITKEN " BASIN. ... Head [2] and Spudis [1] suggested in their reviews that the existense of the structure identified later as the South Pole - Aitken baasin was first predicted on the basis of a relief analysis of the mountain ridges observed in the libration zone be Hartman and Kuiper [7], i.e. after the first images of the lunar far-side had been obtained. ... SOUTH POLE-AIKEN BASIN: V.I.Chikmachev et al. ...

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• http://selena.sai.msu.ru/Symposium/South%20Pole.doc
• http://selena.sai.msu.ru/Symposium/South%20Pole.pdf
• http://selena.sai.msu.ru/Rod/Publications/ms40/21_Dolitsky_etal.pdf

In this chapter we will consider two very simple but useful Web agents that I have written on Actor Prolog for my own needs. ... Let us start the Web agent. Fig. ... Start of the Web agent. The Context diagram consists of three blocks: "Logic Programming Sites", "Edit", and "Check". ... Some Web sites that are linked with the logic programming and Prolog are listed in the pulldown list (these addresses are transferred to the "Edit" block from the "Logic Programming Sites" block). ...

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• ICLP 2003, International Conference on Logic Programming, Mumbai (Bombay),...

... X-Ray Structural Analysis . ... The course introduces the basic principles of diffraction analysis of crystal atomic structure and the basic concepts of state-of-the-art atomic crystallography. ... X-ray crystal diffraction. тАЬGeometricalтАЭ theory of diffraction by three-dimensional scattering center grating. ... Systematic X-ray reflection extinction related to Bravais lattice type, screw axis, glide-reflection planes. ?аFourier synthesis as a method of crystal atomic structure analysis. ...

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• Department of Solid State Physics MIPT
• The 1st International "Siberia Open" Astronomy Olympiad

... Science . ... Science Users Information > Science Publications > Science Announcements > Completion of ALMA Early Science Cycle 1 and start of Cycle 2 . ... Observing Facilities . ... ALMA . ... The ALMA Cycle 1 Early Science observing season ended in May 2014. ... Cycle 2 science observations started on the 3 June 2014 and will extend until October 2015 with two pauses: SeptemberтАУNovember 2014 (commissioning of long baselines) and FebruaryтАУMarch 2015 (annual engineering and computing activities...

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• FORS Sec Std and Abs Phot Project
• ESO - Completion of Atacama Compact Array
• ESO - MUSE Science Verification Completed

... Two weeks ago during the launch of Atlantis, the Sun, Earth, Moon, and rocket were all properly aligned for this photogenic coincidence. ... As the Moon orbits the Earth, the half illuminated by the Sun first becomes increasingly visible, then decreasingly visible. ... NEAR Spacecraft Survives Landing on Asteroid Eros . ... Orbiting asteroid 433 Eros, 145 million miles from Earth, NASA's NEAR spacecraft has been returning stunning views as its year long mission of exploration nears completion. ...

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... In electron-positron colliders, effect of the lattice modification by opposing bunch focusing on the equilibrium radiation emittance is important at high values of the space charge parameter, so one should correctly evaluate this dynamic radiation emittance of the weak beam, which may differ a lot from the nominal emittance, already in the linear beam-beam force model. ... The linearized beam-beam force is equivalent to focusing insertion in linear lattice of the collider. ...

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DIGITAL WDC EXCHANGE FORMAT . FOR OBSERVATORY 1.0 MINUTE VALUES 1. ... DATA-1 .. DATA-60 are 1-minute values of the given element for that hour. ... Typically, digital 1-minute values received by WDCs from organizations operating automatic magnetic observatory instruments are averages of more frequendy sampled values, e.g. 10-second point samples. ... If the method used to obtain 1-minute average values is important to a user, the WDC will assist in determining the exact procedure applied. ...

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• Tethys
• Synchronous Orbit
• Maps of the Heavens