ATNF Home . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Australia Telescope User Committee . ... Murchison Radio-astronomy Observatory . ... Parkes radio telescope . Australia Telescope Compact Array . Mopra radio telescope . ... Information & tools for observers . ... Australia Telescope Online Archive (ATOA) . ... ATCA | ... Visiting Parkes radio telescope . ... Parkes radio telescope webcam . ... The Australia Telescope National Facility Colloquium . ...

Еще в разделе: (Показать все результаты (>24230) - www.atnf.csiro.au/ )

• VLAMODE
• Package: ic

Next: Particle Background Rejection Up: Detection Efficiency Previous: Front Illumination . ... The method requires that the CCD substrate be etched from the rear towards the depletion layer boundary. The device can be illuminated through this rear surface, which has a much thinner dead layer than the electrode side. ... The corresponding detection efficiency data are presented in Figure 7, and compared with the predicted data for a 20 m thick depletion layer. ...

Еще в разделе: (Показать все результаты (>10637) - xmm.vilspa.esa.es/ )

• Description
• XMM-Newton SAS: Watchout Page
• Errors

... The Radar Decoder correlates the received signal with the code used at transmission, generating the equivalent pulse-radar signal (digital). This process greatly reduces the output data rate over directly sampling with the Radar Interface , but requires that the ephemeris be very well known, so that the bins don't smear into one another. ... The Radar Interface samples an input input signal voltage (in quadrature), and provides it as a digital output to a VME bus for processing or recording. ...

Еще в разделе: (Показать все результаты (>3861) - www.naic.edu/ )

• Boundary Conditions etc.
• Outline of the Survey Planning Process (requires investment of
• GALFA Spectrometer Board Test Procedure

... For historical reasons, it is useful to offer comparisons between the current WFPC2, and its predecessor WF/PC-1, which was returned to Earth in December 1993. Field format: WF/PC-1 contained 8 cameras and CCDs, each CCD having 800 x 800 pixels. ... Many differences derive from the fact that the WF/PC-1 CCDs were thinned, backside illuminated devices whereas the WFPC2 CCDs are thick, frontside illuminated devices. WF/PC-1 CCDs were thinned and backside illuminated. ...

Еще в разделе: (Показать все результаты (>18930) - www.stsci.edu/ )

• USC Manager Tool Design Concept page
• Warnings (JWST Pipeline routines in IDL)
• CSPICE Routines: EL2CGV_C

All stars derive their energy through the thermonuclear fusion of light elements in to heavy elements. High temperatures are required so that the mutual electrostatic repulsion of the protons in each fusing atomic nucleus is overcome. ... Elements with more protons in their nuclei require higher temperatures. ... This sequence is now shown in the animation below. ... First Step of the Proton-Proton Chain Narration . Second Step of the Proton-Proton Chain Narration . ...

Еще в разделе: (Показать все результаты (>364) - zebu.uoregon.edu/ )

• Solar Collection and Energy Transport.
• Geothermal Energy

First Name . Last Name . ... A contributed talk . A poster . ... Tentative title of your oral contribution/poster . Required if ask for a Poster or Talk . ... Required if you are member of a collaboration . Short abstract of your oral contribution/poster . Required if you ask for a Poster or Talk . Options . ... Please select additional options . ... Please check the required fields. Powered by jqueryform.com . ...

Еще в разделе: (Показать все результаты (>201) - mavr.sao.ru/ )

... It includes level converters and a optional radio modem designed to decode the radio timecode signals transmitted by the Canadian time and frequency station CHU. A complete set of schematics, PCB artwork, drill templates is in the pub/ntp/gadget.tar.Z file on ftp.udel.edu. ... One of these converts a TTL positive edge into a fixed- width pulse at EIA levels and is for use with a timecode receiver or oscillator including a TTL PPS output. ... See the schematic diagram gadget.s01 for reference. ...

Еще в разделе: (Показать все результаты (>1963) - www.sai.msu.su/ )

• Zen: SAICASTODO
• Scratchbuilt CHU Receiver
• The Network Time Protocol (NTP) Distribution

... Procedure . ... Wind Baffle Pendant Control, located in the 2.5m enclosure. Spreader Bar for wind baffle counterweights, located behind the Machine shop. ... Wind baffle frame tied to eyebolt in floor. ... Move the inner white wind baffle counterweight from the temporary mounting blocks at the front of the wind baffle frame to the standard location at the back. ... Rig the secondary truss to the overhead crane using a large shackle and 4 long nylon straps (load capacity of 1000 Lb. each). ...

Еще в разделе: (Показать все результаты (>1361) - www.apo.nmsu.edu/ )

• Procedure to Remove 2.5m Wind Baffle
• Procedure to Install the 2.5m Wind Baffle
• Procedure to Remove 2.5m Secondary Truss

... Bojan Nikolic web pages (r. 329) . ... The OOF data reduction software is made available under the terms of the GPL V2 or (at licensee?s option) latter licences. ... Also, please note that this is primarily a research system that has grown during investigation and application of the OOF technique. ... The first generation of the OOF system that I wrote was designed to work within the software package that J. S. Richer wrote for reduction of with-phase holography for the JCMT. ... Build system: . ...

Еще в разделе: (Показать все результаты (>2411) - www.mrao.cam.ac.uk/ )

• OOF Reduction Software
• Building CASA Bojan Nikolic web pages (r. 329)
• How to create a new tool in CASA Bojan Nikolic web pages (r. 329)

TOOLS OF TEST GENERATION FOR SATELLITES CONTROL PROGRAMS Andrey Tyugashev, Ekaterina Myasnikova, Elena Sopchenko S.P. Korolyov Samara State Aerospace University (National Reseach University) The paper presents a research in the field of test automation for testing spacecraft control programs. ... Programmers or designers of spacecraft systems write tests manually. ... Tests are carried out by issuing the control actions on the spacecraft and condition monitoring systems parameters of the spacecraft. ...

Еще в разделе: (Показать все результаты (>1640) - www.ssau.ru/ )

• Кучеров Александр Степанович. Публикации

... SGML . The text/html content type . In this section, we begin the specification of HTML 4.0, starting with the contract between authors, documents, users, and user agents. ... These recommendations are not normative and conformance with this specification does not depend on their realization. ... An HTML document is an SGML document that meets the constraints of this specification. ... A user is a person who interacts with a user agent to view, hear, or otherwise use a rendered HTML document. ...

Еще в разделе: (Показать все результаты (>14968) - crydee.sai.msu.ru/ )

• XFree86/OS2 Available Ported Software - Tools
• XFree86/OS2 Download Page
• Recursion

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 . ...

Еще в разделе: (Показать все результаты (>1773) - www.adass.org/ )

• The Communication of Images from New Generation Astronomical Telescopes
• NICMOS Software: An Observation Case Study
• Mixing IRAF and Starlink Applications - FIGARO under IRAF

... The perceptron structure, on the basis of which the database is built, is defined by a number of the input and output parameters and a required accuracy. ... The output perceptron data are the expansion coefficients of the scattering matrix elements in series of the generalized spherical functions. ... As the cluster structure depends on the generation conditions the expansion coefficients were averaged over 5--7 realizations of the clusters (for N . ... is the coefficient number. ...

Еще в разделе: (Показать все результаты (>215) - www.astro.spbu.ru/ )

abstract: ' Catalyst based application ' author: - 'Roberto Baglioni' build_requires: ExtUtils :: MakeMaker : '6.36' configure_requires: ExtUtils :: MakeMaker : '0' dynamic_config: 0 generated_by: 'Module::Install version 1.14 , CPAN::Meta::Converter version 2.143240' license : perl meta-spec: url: http ://module-build.sourceforge.net/META-spec-v1.4.html version : ' 1.4 ' name: visite no_index: directory: - inc requires: ...

Еще в разделе: (Показать все результаты (>9487) - www.arcetri.astro.it/ )

• http://www.arcetri.astro.it/po/visinote/MYMETA.yml
• http://www.arcetri.astro.it/irlab/doc/giano/Connecting_the_LANtronix.pdf
• Electronics

trend1d - Fit a [weighted] [robust] polynomial [or Fourier] model for y = f(x) to xy[w] data. trend1d -F < xymrw > -N [ f ] n _ model [ r ] [ xy [ w ] file ] [ -C condition _# ] [ -H [ nrec ] ] [ -I [ confidence _ level ] ] [ -V ] [ -W ] [ -: ] [ -bi [ s ][ n ] ] [ -bo [ s ] ] trend1d reads x,y [and w] values from the first two [three] columns on standard input [or xy [ w ] file ] and fits a regression model y = f(x) + e by [weighted] least squares. ... E.g., a robust quadratic model is -N 3 r . ...

Еще в разделе: (Показать все результаты (>636) - xray.sai.msu.ru/ )

Next: GOCG Pre-Observation Products . Previous: RadioAstron Mission Element Overview . ... Observation Summary File (OSF) . GRT (Ground Radio Telescope) Schedule Files . ... How: The long-term schedulers will produce two files: GSTS-file (General Space Telescope Schedule) to be used by GOCG and LTS-file for all mission elements. ... What: The RSOG will produce schedule files for all GRTs participating in a particular observation, in the format required by each GRT. ...

Еще в разделе: (Показать все результаты (>125) - www.asc.rssi.ru/ )

1.2 CCD Operations, Performance Parameters, and CCD . Transfer Curves . Low-light-level CCD performance parameters are grouped into four primary CCD operations: 1) Charge Generation (e.g. QE), 2) Charge Collection (e.g. MTF), 3) Charge Transfer (e.g. CTE), and 4) Charge Detection (e.g. Read Noise). ... Four Basic CCD Operations and Associated Performance Parameters and CCD Transfer Curves Used to Measure Performance . ... Charge Transfer Performance Parameters and CCD Transfer Curve Tests . ...

Еще в разделе: (Показать все результаты (>1809) - www.sao.ru/ )

• Required observational data
• Bias Corrections
• File Formats Required for Photometry

... SphereParams Struct Reference . ... SphereParams (const float radius) . ... Definition at line 50 of file StelGeometryBuilder.hpp . ... Definition at line 103 of file StelGeometryBuilder.hpp . ... Definition at line 120 of file StelGeometryBuilder.hpp . ... Definition at line 112 of file StelGeometryBuilder.hpp . ... Definition at line 118 of file StelGeometryBuilder.hpp . ... Definition at line 110 of file StelGeometryBuilder.hpp . ... Definition at line 114 of file StelGeometryBuilder.hpp . ...

Еще в разделе: (Показать все результаты (>2161) - astro.uni-altai.ru/ )

• Stellarium: RingParams Struct Reference

... Star Atlas . ... stars . ... Nuclear fusion of hydrogen into helium powers stars, but fusion requires a lot of energy. Where does this energy come from? ... You re in good company: This question also stumped the physicists who first tried to understand nuclear fusion in stars. In a star s core, all atomic nuclei have been separated from their electrons, so each hydrogen atom is really just a proton and thus holds a positive charge. ... Get instant access to subscriber content on Astronomy.com! ...

Еще в разделе: (Показать все результаты (>5875) - www.astronomy.com/ )

• How do neutron stars generate steady magnetic fields? | Astronomy.com
• Astronomy Insights

... Proposed location of the new generation Russian VLBI network radio telescopes Kaliningrad St. Petersburg Zelenchukskaya (Zc) Badary (Bd) Ussurijsk Working frequency bands for the new generation Russian VLBI network S X Ka 2.2 2.6 7.0 9.5 27 33 F, GHz Data acquisition parameters 4 frequency bands : 512 MHz bandwidth x 2 polarisations or 1024 MHz bandwidth x 1 polarisation 2-bit sampling ...

Еще в разделе: (Показать все результаты (>309) - www.ipa.nw.ru/ )

• http://www.ipa.nw.ru/PAGE/aspirantura/literatura/whitney.pdf
• http://www.ipa.nw.ru/conference/2002/sovet/PS/GAYAZOV.PS