... Meta Index / Home Page / Output Files / Classification of the patterns / Single events and recognizable . ... These are not considered as recognizable patterns. See also Sects. 9.4.2 and 9.4.5 for further details on the following counter-examples: . ... quadruple pattern . ... After the CTI and gain corrections, in the entry for the corrected amplitude, `X' will get the sum of the corrected amplitudes of all parts of the pattern, while the corrected amplitude for `x' will be ``NULL''. ...

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• Extraction and correction of an X-ray light curve for a point-like source
• Description
• XMM-Newton SAS: Watchout Page

Astronomy Discussion Forums . Forums: . ... Discussion Forums . ... Reconsidering.. Forum List | ... Post Message | ... I suggest: not that "atoms" are ultimate; but that such-and-such "defining relationships" are ultimate? ... Since we agreed elsewhere that "relationships exist"; the question is: what about ultimate relationships? ... www.astronomy.net . ... Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

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• Could This Be Considered The ... - an Astronomy Net Blackholes2 Forum Message
• I Think What You're Saying Is Not A Deeply-considered Position - an Astronomy
• How Do You Feel About Numbers? - an Astronomy Net Exploration Forum Message

Download Izmccd (~2.7 MB). Solution of problems at identification of star field. ... 2) Scale is not correct. ... In this case algorithm of identification will revise all values of scale from twice smaller up to twice greater. ... There should be more than value of the field "Number of stars in frame". ... The star field is considered identified if number of the identified stars more or equally to this value. It is necessary to set value from 4 up to value of field "Number of stars in frame". ...

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... Team . ... The main goal of observations of GRB host galaxies is accumulation of statistics of their spectroscopic and photometric properties. ... The Hubble diagram for 22 GRB host galaxies with known magnitudes and redshifts (GRB 970228, GRB 970508, GRB 970828, GRB 971214, GRB 980613, GRB 980703, GRB 990123, GRB 990510, GRB 990712, GRB 9912008, GRB 991216, GRB 000131, GRB 000210, GRB 000301C, GRB 000418, GRB 000911, GRB 000926, GRB 001109, GRB 010222, GRB 010921, GRB 011121 and GRB011211). ... 600...

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• GRB follow-up team GRB workshop 2009

The database contains references to the papers, data files and links to the Internet resources related to measurements and calculations of the optical constants in the wavelength interval from X-rays to radio domain. ... References to some useful books and reviews on the subject (e.g. the classical handbooks edited by E.D.Palik) and links to Internet collections of optical constants and personal WWW pages with related software were also placed in the database. You have arrived at our welcome page. ...

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• The 2175? feature

... The orbits as follows are considered: INTERBALL Tail Probe (IB_TAIL) & Auroral Probe (IB_AUR), GEOTAIL (NASA/ISAS), and POLAR (NASA). ... The situation investigation aim is to select the following favourable spatial positions (FSP) : . ... FSP3 : That part of the FSP1 & FSP2 time intervals, which corresponds to the magnetic conjugations of the any couple of the considered spacecraft. ... The polar diagram plot . ... The geocentric distance (GCD) of the 4 spacecraft as a function of the time. ...

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• Corrected Geomagnetic Coordinates
• Introduction to the situation investigation for IACG/ISTP Campaign # 2.
• Space Research Institute (IKI) Seminar

Next: TESTTA/CCD Up: Test Commands Previous: TESTBA/CCD . ... Test F1: Creation of the combined flat frame, using only those flat frames in the input catalogue that have exposure times falling within the allowed range. The combined flat is corrected for the bias offset. ... A combined low count flat frame corrected for the bias offset; . ... The combined low count flat field is corrected for the mean bias offset, stored in the keyword BIASMEAN , filled by the command TESTB/CCD . ...

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• Emission-line galaxies
• Documentation: LEDA: parameter: m21c
• Documentation: LEDA: raw data : flux

... Publications with ESO Data . ... The tools have been developed for ESO by a team of astronomers at the Institute for Astro- and Particle Physics at the University of Innsbruck, as part of an in-kind contribution to ESO , which includes as well a model of the sky emission and transmission spectrum at Cerro Paranal. ... Skycorr provides an advanced instrument-independent sky-correction tool that removes sky emission in science spectra by means of sky spectra taken at a different time and sky location....

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• Los Cielos de Am , The darkest sky and the two galactic hemispheres
• ESO - Request Handler FAQ
• Procedure to be followed by DMD secretary for DFS Group documentation

... There are a number of "fixes" that are important for short wavelength ATCA data, especially at the 3mm band. ... By default atfix applies the ``standard'' gain/elevation model for the antennas. ... As mentioned in Section 11.1.2 , the ATCA uses a paddle to measure an above atmosphere system temperature. ... On the night of an ATCA reconfiguration, a solution for the antenna positions is derived. ... Task atfix corrects the data for an improved antenna location solution via the dantpos parameter. ...

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• Australia Telescope National Facility
• ccontsubtract CentralProcessor 0.11 documentation
• cmodel (Model Image Generator) CentralProcessor 0.11 documentation

... Computing the true count rates for digital data. ... The following equation is used to find the count rate. x = ( raw counts / sample time ) . ... True count rates for digital data are corrected by using the first equation for a point source and the second for an extended source. a = ( y - pre_amp - darkrate ) / ( highvolt x pt_effic ) . ... True photocurrents (count rates for analog data) are corrected by the first equation for point sources and the second equation for extended sources. ...

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• HDF-S Sydney Meeting Follow-up Notes
• Time Dependence of UV Response
• F300W flat

README for XFree86 on OS/2 : Adding Variables to CONFIG.SYS . ... ETC . Set to an ETC directory. Normally, this is already set to the ETC directory of the TCP/IP code, such as SET ETC=C:\TCPIP\ETC For Warp 4 and later, this may point to the \MPTN\ directory. ... Normally you will set this variable to the same value as the HOSTNAME variable and simply add a :0.0 after it, such as SET DISPLAY=myhost:0.0 Read the X11 man page on the exact meaning of these postfixes and other options. ...

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• Checking Compatibility of Video Hardware
• Introductory Note about the release 3.3.6
• Image: The procedure is as follows: put a coin into special box, pull a cord

... Cambridge . ... Bojan Nikolic web pages home . ... Welcome to the web-log (AKA, blog) about my astronomical research. ... Some of the articles are simply commentary or pointers on others people work in astronomy and contain no original research . ... Simple smoothing of astronomical images in FITS format (April 29, 2012) . ... Talk at the University of Cambridge (November 3, 2010) . ... Introductory talk at the Kavli Institute for Cosmology, Cambridge (March 22, 2010) . ...

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• DUST: Graph Legend
• OptInt PmWiki : PmWiki / Custom InterMap
• AMI-Planck Follow-up Observation Database

... Apache HTTP Server Version 2.4 . Apache > HTTP Server > Documentation > Version 2.4 > Modules . ... Location /server-info> SetHandler server-info </Location> . You may wish to use mod_authz_host inside the <Location> directive to limit access to your server configuration information: <Location /server-info> SetHandler server-info Require host example.com </Location> . ... For example, http://your.host.example.com/server-info?config will show all configuration directives. ?<module-name> . ...

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• SDSSmosaic
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• Procedures for Observations

... Step 1: The Footprint position calculation by the magnetic field line tracing from the satellite position up to the Ionosphere by using IGRF + Tsyganenko [1987] magnetic field model (the stop trace altitude 110 km). Step 2: Tracing back from the Footprint (produced on the Step 1) to the dipole equatorial plane (by using only IGRF magnetic field model up to the geocentric distance 8 RE and dipole field model after this distance). ... Back to the description . ...

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• Sensors
• Deriving Sines and Cosines
• Current Solar Wind Conditions

The pitch, roll, and focus errors of the telescope (measured and computed in AO9 survey and tilt sensor pitch,roll ) can be corrected by using the tiedowns. ... Tiedown positions to correct the pitch,roll, focus errors versus azimuth for za 2 through 20 degrees. ... The pitch, roll, and focus errors are plotted versus azimuth for za 1 to 20 degrees (the color changes every two degrees) . ... The pitch error is on the top and the roll error is on the bottom. ... The pitch and roll errors versus za. ...

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• Appendix C. Display Device Names
• Chapter 3. Selecting and Downloading the NVIDIA Packages for Your System
• Chapter 5. Listing of Installed Components

.

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• THE HUBBLE LAW JAVA APPLET
• Forces, Masses, Acceleration and Friction

... In some cases where memory space is at a premium, it is possible to tailor the configuration to remove such features as reference clock driver support, debugging support, and so forth. ... The following lines are used in this file: . ... The DEFS_LOCAL line defines global flags that apply to all machines. Ordinarily, the only flags included are the -DDEBUG , which includes the debugging code, and -DREFCLOCK , which includes basic reference clock support. ... D_INCLUDE_BSD_SOURCE . ...

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• Building and Installing the Distribution
• APOD: October 21, 1999 - Follow The Spots
• Light Curve Templete/Observing Form For Visual SNe Observers.

Follow-up astrometry and recoveries are made with the ANU 40 inch (1.0-m) f/8 reflector at Siding Spring Observatory (IAU code 413). ... A routine follow-up of 2003 WY153 on 2003 Dec 15 became much more than routine when a faint object with unusual motion vector was found close to the target asteroid. ... During routine astrometry with the 1.0-m to improve the orbit of the Apollo asteroid 2004 CB, the asteroid was found on March 30 to have a short tail! ... Siding Spring Survey Main Page . ...

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• Naomi McClure-Grffiths
• ANU - RSAA - 5th Stromlo Symposium Registration

home publications > mercury . SEARCH ASP SITE: Match ALL words Match ANY word . ... ASP Conference Series . ... Following the Martian Coastline . ... It seems scientists and laypeople alike have wondered for quite a long time whether or not water exists on Mars. ... A second reason we should determine the sites of ancient Martian seas is that if water once existed on Mars, it is possible that conditions for life obtained on the planet in the past and possibly even persist into the present. ...

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• ASP: Robert J. Trumpler Award
• ASP: Using Multicultural Dimensions to Teach Astronomy
• ASP: Education Newswire

Next: The Stopping Radius in Up: ``Ecology'' of Magnetic Rotators Previous: The Environment of the . Now we consider qualitatively the effect of the electromagnetic field of a magnetic rotator on the accreting plasma. ... What is important is that both relativistic particles and magnetic dipole radiation will transfer their momentum and hence exert pressure on the accreting plasma. ... 2) The pressure of the accreting plasma is high enough to permit the plasma to enter the light cylinder . ...

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• Effect of the Magnetic Field
• Transferring mag to erg/cm/s
• Simple Universe