... 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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We present ~1000 new candidate Young Stellar Objects (YSOs) in the Large Magellanic Cloud selected from Spitzer Space Telescope data, as part of the Surveying the Agents of a Galaxy's Evolution (SAGE) Legacy program. ... The candidate YSOs were selected from the SAGE Point Source Catalog from regions of color-magnitude space least confused with other IR-bright populations. ... They are more clustered than generic point sources, as expected if star formation occurs in filamentary clouds or shells. ...

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• ACS pointing patterns
• ACS pointing

... especget (especget-1.27.7) [?? ... especget filestem=myagn srcexp="((DETX,DETY) IN circle(572,-635,800))" . backexp="((DETX,DETY) IN annulus(572,-635,1600,3200))" . ... This command line produces the files myagn_src.ds, myagn_bgd.ds, myagn_src.arf, myagn_src.rmf . The command will take quite a while to run because of the RMF generation stage . A PN observation processed with this command will take roughly twice as long as a MOS observation. ...

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• Example 3: Point source with explicit position

As an obligatory preparing for the application to participate in the IAO a short report of National Olympiad of the current year with a set of all problems used on the Olympiad has to be presented by the applicating team. ... The final minutes (protocols written in Latin or Cyrillic in form of tables) of the Olympiad (evaluating of solutions of the students participated in the last stage of the Olympiad) should be included as well. ... Historical data of the National Astronomy Olympiad: . ...

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• The XVIII International Astronomy Olympiad, information before Olympiad
• XVII International Astronomy Olympiad, information before Olympiad
• XIX International Astronomy Olympiad, information before Olympiad

Next: Available Receivers Up: The Arecibo Observatory and Previous: The Arecibo Observatory and . The main reflector of the telescope is a , 305 m (1000 ft) in diameter and 51 m (167 ft) deep. ... The system housed in the Gregorian dome provides continuous frequency coverage from 300 MHz to 10 GHz using a pair of shaped (secondary and tertiary) subreflectors, plus standard point feeds and receivers. ... Consecutive use of multiple receivers during an observing run is straightforward. ...

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• simulate 430 linefeed gain vs za
• Points of Contact
• puppi

... Up: Science Data Pipelines . ... We designed and developed a package which simulates extragalactic point source data within a given field of view and SIRTF band. ... The simulator is modular and extensible to enable multi-wavelength simulations, has been optimized by utilizing parallel processing capabilities, and will be used to test pipeline software. ... The extragalactic simulator is capable of generating large numbers of galaxies within a given patch of sky for SIRTF pipeline testing. ...

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• Enhanced HST Pointing and Calibration Accuracy: Generating HST Jitter Files at
• ADASS 2002 Conference Proceedings

The close position of main satellite and subsatellite (distance between them about 1000 km) and using the similar sets of Faraday cups (VDP and VDP-S) with high resolution measurements (up to 16 Hz for the main satellite and up to 10 Hz for the subsatellite) allow us to determine the small-scale variations of the magnetopause shape and position and to estimate the velocity of the magnetopause motion. ... Two point observation of the magnetopause motion: the INTERBALL project. ...

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• Lagrangian Points
• INTERBALL IB_TAIL last day in the topocentrical c/s of the landing point
• INTERBALL IB_TAIL landing point coordinates

... 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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• Bright Point Studies
• Solar Bright Point
• Index of /~meb/turning_point

Trace: q3c . start : q3c . ... SAI VO Projects . ... Help on Wiki search . ... dropdb q3ctest createdb q3ctest psql q3ctest /usr/local/pgsql/share/contrib/ q3c .sql psql q3ctest /usr/local/pgsql/share/contrib/pg_sphere.sql \timing on DROP TABLE running_ q3c ; DROP TABLE running_pgsphere; CREATE TABLE running_ q3c (id INT, ra FLOAT, dec FLOAT); CREATE INDEX running_ q3c _idx ON running_ q3c ( q3c _ang2ipix(ra, dec)); CREATE ... SAI VO | ... SAI MSU | ...

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... RIVER FORECAST LATEST FLOOD FORECAST AND REMARKS POINT READING STAGE GREEN NEAR 63.4 FT 64.0 FT CRESTING NEAR 65.0 FT AROUND AUBURN 300 PM MIDNIGHT TONIGHT.. ... SATSOP NEAR 33.5 FT 34.0 FT CRESTING NEAR FLOOD STAGE SATSOP 300 PM AROUND 5 PM THIS AFTERNOON NISQUALLY NEAR 12.1 FT 10.0 FT CRESTING NEAR 12.5 FT AROUND NATIONAL 230 PM 6 PM THIS EVENING. ... NEW RECORD FORECAST** *RECORD 21.57 FT ON 12/23/33 NACHES NEAR 18.5 FT 17.0 FT CRESTING NEAR 22.0 FT AROUND NACHES NOON 10 PM THIS EVENING. ...

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• http://zebu.uoregon.edu/1996/es202/fwarn.html
• http://zebu.uoregon.edu/1996/ph123/mtr.html
• Formation of the Earth's Atmosphere and Oceans

... Posts tagged ?break points? ... How would you assign orders to multivariate data? ... MADS] data depth? Tags: break points , data depth , MADS , mean , median , multivariate , nonparametric , order , parasite , quantile , robust , sort , vertebrate . ... Comment . ... Entries RSS . Comments RSS . ... vlk on [MADS] Parallel Coordinates . upvc windows on [MADS] Parallel Coordinates . ... Alfred Inselberg on [MADS] Parallel Coordinates . ... Entries (RSS) and Comments (RSS) . ...

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• Access Point Names and Templates
• Getting Common Information About Access Points
• On-Axis Point Response Functions (PRF)

... Pointers to Pointers . ... Pointers to a Function . ... We have introduced some advanced pointer issues already. This chapter brings together some topics we have briefly mentioned and others to complete our study C pointers. ... main(int argc, char **argv) . ... These are the only arguments main accepts. argc is the number of arguments typed -- including the program name. argv is an array of strings holding each command line argument -- including the program name in the first array element. ...

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• General points
• comedi_command_test
• Stream 1/0

Operations in Point operations use the pointer to query sets about points, delete points in a set, and move points. In all cases where interaction is required, pressing the right mouse button with the pointer in the drawing area cancels the operation. ... Report on a point in a set . ... Press the left mouse button. ... Press Delete point with the left mouse button to activate. ... Move the pointer to the new location and press the left mouse button again to register the point's new location. ...

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• No Title
• The ``Reflection'' Effect
• Point of view.

Next: PN3DB and NOPN3DB Up: Details of SCHED Parameters Previous: PLOT Contents . POINT is used to tell SCHED to convert this scan to a reference pointing scan. If the argument is zero (which is the value it will get if POINT is specified without an argument), all stations that are in any group and have appropriate frequencies as specified in the PEAKFILE (see also PEAKINIT ) will be used. ... POINT=-1 means don't add a pointing scan even if you can. ... None means zero. ... Example: POINT=2 . ...

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• Late Stages of Stellar Evolution
• Astrometry syllabus points
• Version 10.0

SINGULAR POINTS IN THE SOLAR CHROMOSPHERE . ... In the structure of the solar chromosphere, containing information on the configuration of the magnetic field, we have found and identified all the main types of the singular points ( see Fig. 1 ), which are known as inherent features of the 2-D vector field. ... The main types of the singular points are the node, the focus, the center, and the saddle. ... Singular point of the focus type in the solar chromosphere. ...

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• Distribution of the analyzed SEPs with different >100 MeV proton fluxes (J100)

# : macro read gauss_test.sm = loads macro into sm # : noisedemo 1000 = runs macro with 1000 pts # define N $1 set x=1,$N # dummy call to get ws dimensioned right get_hist x v ws -.5 .5 .02 set ws=ws*0 erase window 1 1 1 1 set y=x*0 limits 0 $N -.7 0.7 box ptype 1 1 # generate a lot of points to uniformly cover -0.5 to 0.5 # -and- at the same time do averages of 10 samples = pseudo-gaussian do i=1,10 { set t=random($N)-0.5 ...

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• http://www.mso.anu.edu.au/~fbriggs/WAARNEEM/gauss_test.mac
• Telescope pointing system
• Siding Spring Observatory's 2.3 m telescope (wide and high vantage point)

... With enough velocity, a spacecraft can break loose from the Earth's gravity and enter an orbit around the Sun, like that of a planet. If it then orbits the Sun with the same period as the Earth--one year--it may keep a fixed position relative to Earth. ... If the distance is just right--about 4 times the distance to the Moon or 1/100 the distance to the Sun--the spacecraft, too, will need just one year to go around the Sun, and will keep its position between the Sun and the Earth. ...

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• The Earth's Magnetosphere-- History
• Point of Agenda; Sep 1995 CONPAS workshop
• Point of Agenda; Oct. 1995 CONPAS workshop

... Accuracy of SC Launches to Geostationary Transfer Orbit and High Elliptical Orbit Using DM Type Upper Stage For a Period Since 1996. Controlled parameters of target orbits: . ... Е - eccentricity of orbit; . ... м p - perigee altitude. i - inclination of orbit to the . ... SC Type and Launch Date . ... D i,ang. Min. ... Astra 1F . ... 0.7 . ... SEA LAUNCH . LAND LAUNCH | ... LAUNCHERS | ... Official WEB-site of S.P.Korolev RSC Energia . ...

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• RSC "Energia" - Land Launch
• S.P.Korolev RSC Energia - LAND LAUNCH SYSTEM
• RSC "Energia" - History

AUTOMATED CREATION OF THE LUNAR HYPSOMETRIC MAP: TECHNIQUES OF COMPILING. ... And the second one is the database, obtained from the raster images of the Lunar Subpolar regions (higher than latitude ?60°) where brightness of each pixel depends on its height [1]. ... Due to these reasons it was necessary to develop the special 10-stage methodology of data processing and map compiling. ... The height data were obtained and the lunar hypsometric map was created according to the 10-stage methodology. ...

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• http://selena.sai.msu.ru/Rod/Publications/ms40/21_Dolitsky_etal.pdf
• Солнечное затмение 1999

GRANAT is the Russian x-ray sattelite launched to the high apogee orbit (200,000 km) and operated almost for 10 years (1989 -1999) , carrying out four major instruments: French SIGMA coded-mask hard x-ray telescope (30-1000 keV), Soviet ART-P coded-mask telescope (2??-60?? keV), all-sky monitor WATCH (6-150 keV), and a gamma-burst detector PHEBUS . ... Since September 1994, GRANAT is in the survey mode. ... Explore pages devoted to individual GRANAT instruments (including main scientific results): . ...

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• High Energy Astrophysics Department at IKI RAN