... 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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• SUBPT User's Guide
• ACS pointing patterns
• Quasar Spectral Features at Intermediate Redshift

... 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

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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Next: HST Paper Products: A New Way to Look at HST Data . ... After providing on-the-fly re-calibration of HST data to archive users, ST-ECF has embarked on a new project aiming at grouping, cosmic ray cleaning and drizzling images taken by most HST instruments. ... The production of the missing jitter files combined with the extraction of additional engineering parameters will greatly enhance the homogeneity and the scientific value of the entire archive. ... 1995, HST Data Handbook, STScI, 107 . ...

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• An Extragalactic Point Source Simulator for SIRTF Pipeline Testing
• Zero-Points of FOS Wavelength Scales
• ADASS 2002 Conference Proceedings

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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• XIII International Astronomy Olympiad: Information before the Olympiad
• The XVIII International Astronomy Olympiad, information before Olympiad
• LHPP ISSP RAS

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

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

Magellan to Venus . ... The spacecraft carried a sophisticated imaging radar, which was used to make the most highly detailed map of Venus ever captured during its four years in orbit around Venus from 1990 to 1994. After concluding its radar mapping, Magellan also made global maps of Venus's gravity field. ... The Magellan mission was divided up into "cycles" with each cycle lasting 243 days (the time necessary for Venus to rotate once under the Magellan orbit). ... Magellan Orbiting Venus . ...

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• How to print floating point numbers from the kernel?
• FIRPO Zero Points
• IBIS - Flat Fielding

NASA JOHNSON SPACE CENTER ORAL HISTORY PROJECT BIOGRAPHICAL DATA SHEET NAME: Richard M. Mike Mullane O RAL H ISTORY: 24 January 2003 EDUCATIONAL BACKGROUND: B.S. in Military Engineering, United States Military Academy, West Point, NY, 1967 M.S. in Aeronautical Engineering, Air Force Institute of Technology, 1975 PRE- NASA EXPERIENCE: United States Air ... R. Mike Mullane, Red Sky: A Novel of Love, Space, and War (Salt Lake City, UT: Northwest Publishers, 1993). ...

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• http://www.jsc.nasa.gov/history/oral_histories/BormanF/FFB_Bio.pdf
• Astronaut Bio: Frank Borman
• Astronaut Bio: David C. Hilmers

... 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

... 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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... Izv. Acad. Nauk SSSR Ser Mat. ... Doclady Academii Nauk, 385 (2002), N 4, p. 443-449. ... Generating functions for modular graphs and Burgers's equation. ... Coloured graphs, Burgers equation and Jacobian conjecture. ... Coloured graphs, Burgers equation and Hessian conjecture. ...

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• Critical points of functions (Fall 1999)
• Critical points and reflection groups (Spring 2004)
• Hilbert schemes of points on surfaces (Fall 1997)

... Higgs, 1989; DRAO 1991. ... 12-13 RA (hours) 15-16 RA (min) 18-22 RA (sec) (XX.XX) 24-28 RA error (sec) (XX.XX) ( blank = unknown ) 30 Sign of declination 31-32 DEC (degrees) 34-35 DEC (arcmin) 37-40 DEC (arcsec) (XX.X) 42-45 DEC error (arcsec) (XX.X) ( blank = unknown ) 47 Epoch of coordinates (1=B1950, 2=J2000, 3= unknown ) 49 Type of position determination (1=rough estimate, 2=centroid, 3=peak, 4=fitted Gaussian, 5= unknown ) 51-56 Flux #1 ( variable format ) 58-62 Error in ...

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• Entry points
• The Mouse Pointer
• Source Positions

... 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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• OTHER DOCUMENTATION
• Chandra Images for G33.6+0.1
• Chandra Images for SNR J0535.4-6916

... 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

... Point sources: Pulsar inside western edge. ... TPT at 57.5 MHz (7'.2?9'.7: S=190?50 Jy). ADS . ... VLA at 327 MHz (3'.0?3'.7). ... Kassim & Weiler 1990, ApJ, 360, 184. VLA at 327 MHz (2'.8?4'.1: S=129?11 Jy), and part at 1.4 GHz (0'.9?1'.8), plus review of flux densities. ... Finley & ?gelman 1994, ApJ, 434, L25. ROSAT observations, including pulsar. ... 2006, ApJ, 636, 777. -ray observations. ... 2006, ApJ, 651, 190. X-ray observations. ... 2006, ApJ, 652, 554. ... Fermi observations. ...

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• G184.6-5.8
• G65.1+0.6
• G332.4-0.4

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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• Transferring mag to erg/cm/s
• No Title
• The ``Reflection'' Effect

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