[ CATS home ] [ Back to CATS list ] [ ftp ] . 2000ApJS..131..335Rutledge+ . Division of Physics, Mathematics and Astronomy MS 220-47, California Institute of Technology, Pasadena, CA 91107 rutledge@srl.caltech.edu, rb@astro.caltech.edu, prince@srl.caltech.edu

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• Source Detections
• Source Positions
• Explanatory Supplement to the 2MASS Second Incremental Data Release

... Read in data: Fill (x, y, count) data records: Binned mode: x,y: image pixel coordinates count: number of events in pixel Single photon mode: x,y: event coordinates count:=1 Feed data records, background maps, and exposure maps into Maximum Likelihood PSF fitting algorithm: Use Marquarth-algorithm to minimize likelihood function of multi-source PSF fit. Remove sources from fit which do not significantly improve goodness of fit (required improvement in likelihood specified by parameter). ...

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• Auto selection of Prime source.
• Source matching

You can also see this page in Russian with using KOI8 (X Windows) or CP1251 (MS Windows) Cyrillic coding. The Laboratory supports the space TV experiments, mainly in the planetary exploration missions. ... Image Co-registration . ... PHOBOS mission - Martian satellites investigations. Phobos on the Martian limb, the image from Phobos-2 probe from 02/28/89. ... Russian Space Bulletin. ... Last modified at June,26 1997 Alexey Kuzmin: akuzmin@mx.iki.rssi.ru . Back to IKI home page ...

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• Additional Space Physics Resources
• Plasma source [Oulu]

index . ... CentralProcessor 0.11 documentation . The source-finding and analysis package supports analysis of processed radio synthesis observations, including source detection and extraction, profile fitting, and writing to the database. This package is a reimplementation of the source-finding algorithms of Duchamp, with an emphasis on the processing of ASKAP-scale data sets, and providing the functionality required by the Survey Science Projects. ... Selavy Basics . ...

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• The completeness and reliability of threshold and false-discovery-rate source
• Source Fitting and Positions
• User Parameters - Continuum Source-finding CentralProcessor 0.11 documentation

... This paper describes the main algorithms used by the Einstein Level One processing to create the exposure masks and the background maps for Einstein IPC images, and how these algorithms were recreated in the IRAF environment. Our goal was to recreate the algorithms used by the Level One Processing to create exposure masks and background maps for Einstein Image Proportional Counter (IPC) data (cf. sections 2.5 and 2.7 of Harnden et al. ...

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• An Extragalactic Point Source Simulator for SIRTF Pipeline Testing
• A New PROS Task for Calculating HRI Source Intensities or Upper Limits
• QPSIM: An IRAF/PROS Tool for Source Simulation

... Stellar Evolution is driven entirely by the never ending battle between Pressure and Gravity . As imbalances are reached, the star is driven to find a new Energy source. ... Pressure and gravitational forces are equal, the star is stable and its core is sufficiently hot to fuse Hydrogen into Helium More about main sequence stars . ... The luminosity generated by the core fusion of Helium into Carbon is far greater than the shell luminosity associated with the fusion of Hydrogen into Helium. ...

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• Energy and the Environment: Resources for a Networked World
• Nuclear Waste Disposal

... Archives . ... Quote of the Week, July 12, 2007 . ArXiv] Complete Catalog of GRBs from BeppoSAX, July 13, 2007 . Jul 13th, 2007| 07:24 pm | ... From arxiv/astro-ph: 0707.1611 Probabilistic Cross-Identification of Astronomical Sources by Budavari and Szalay . As multi-wave length studies become more popular, various source matching methodologies have been discussed. ... Are there any power related studies on source matching statistics? ... Chandra Blog . ... Stat S/W Resources . ...

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• Source Subtraction
• The AstroStat Slog source detection
• *imexamine* - General analysis of image containing many sources

... Our Java and Python software runs anywhere on Windows, Mac, and Linux . ... Alsvid - Algorithms for visualization and processing of image data with Python . Our observatory software . PyDome - Astronomical dome control in Python . ... Software archive . ... XEphem for visual access to astronomical data and remote telescope operation (Linux and Mac OS X) . ... SAOImage DS9 for astronomical data visualization (Linux, Mac OS X, and Windows) . ... G ttingen ImageJ astronomical resources . ...

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lsst.tcc љ 1.2.2-3-g89ecb63 . ... Files . ... python . tcc . cmd . process.py . ... 7 љ # dict of process name: tune attribute name, tccActor timer attribute name, tccActor method . ... 14 љ_DidCheck = False . ... 16 љ def process (tccActor, userCmd): . ... 19 љ @param[in,out] tccActor tcc actor . ... 51 љ tccActor.writeToUsers(msgCode, msgStr, cmd=userCmd) . ... tcc.cmd.process.process . ... Definition: process.py:16 . ... Generated on Mon Sep 14 2015 15:25:37 for lsst.tcc by љ 1.8.5 ...

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• lsst.tcc: python/tcc/base/loadOldObjData.py Source File
• lsst.tcc: python/tcc/mov/fullSlew.py Source File
• lsst.tcc: python/tcc/base/testUtils.py Source File

... WFPC2 ETC for Point Sources - v4.0 . Home . ... Data . ... WFPC2 Home . ... Instrument Home . WFPC2 History . ... Calibration . Calibration Home . ... LRF Data . ... Data Analysis . Data Analysis Home . Data Analysis Library . ... Line: Ly 1216 C IV 1550 He II 1640 C III 1907 Mg II 2800 0 II 3727 Ne III 3869 H 4340 0 III 4363 He II 4686 H 4861 0 III 4959 0 III 5007 N II 5755 He I 5876 0 I 6300 N II 6548 H 6563 N II 6583 S II 6716 S II 6731 S III 9531 Specify Z Vel. : (units) . ...

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• WFPC2 Photometry SYNPHOT Resources
• Discovery and Analysis of 21 ѕ®m Feature Sources in the Magellanic Clouds
• WFPC2 ETC for Point Sources + Background - v4.0

... The data was taken over many days with the same source in more than one file. ... You want to convert the data to kelvins (this is galactic work) and then average all the scans for each source. ... input each onscan, average, and then scale to kelvins . place all of the averaged scans in an array, when done with the file, store this array in an idl save file for this day. ... Average together scans of the same source and then baseline them. input all of the daily save files into a single array . ...

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• a2488 dps the 800Mhz rcvr.
• a2400_dps
• a2584

... During the analysis of the surveys carried out on RATAN-600, it was found that almost one fifth of the detected sources shows significant radio flux variations. ... We used the data from "Cold" radio surveys carried out with RATAN-600 in 1980-1994 to search for radio sources with significant flux variability. ... On possibility of detection of variable sources using the data of Cold surveys carried out on RATAN-600. ... Detection of Variable Sources Using the Data of "Cold" Surveys. ...