... ATNF Home . About ATNF . ... 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 . ... Australia Telescope Online Archive (ATOA) . ... Parkes | ... Australia Telescope 20GHz Survey . ... Visiting Parkes radio telescope . Visiting Australia Telescope Compact Array . ... Parkes radio telescope webcam . ...

... Near Infrared Camera and Multi-Object Spectrometer Instrument Handbook for Cycle 17 > Chapter 8: Detector Readout Modes > 8.2 Multiple-Accumulate Mode . 8.2 Multiple-Accumulate Mode . ... This mode of operation is known as Multiple-Accumulate ( MULTIACCUM ). ... See Section 8.6 for trade-offs between MULTIACCUM and ACCUM readout modes.) In most cases, MULTIACCUM mode provides the highest quality scientific data. The benefits of obtaining observations in MULTIACCUM mode fall into two areas. ...

This describes the exposure window used by each instrument (the graphical interface for the hub's expose command). ... To open the expose window for a given instrument, bring up that instrument's main window, then press the Expose... button along the bottom. ... The top panel shows the status of the current exposure sequence (regardless of who started it). ... File: the file name for the current exposure, or the most recent exposure if not exposing. ... Download: exposure download preferences. ...

Stellar Clusters are very useful laboratories for empirically studying stellar evolution. ... All cluster stars are at the same distance . All cluster stars have the same physical age . ... CM diagram Young Cluster In this case we see the Main Sequence fully represented. The blue dots represent massive stars with short main sequence lifetimes. ... Thus, identifying the most massive star which is still on the main sequence is an effective means of determining the age of a stellar cluster. ...

STEP INTO THE BLUE - MEADE INSTRUMENTS PRODUCT GUIDE . ... LX600 Series . ... LX200 Series . ... Superb optical performance coupled with time proven computerized pointing and tracking has made the LX200 ACF series a best-seller in the high-performance telescope class. ... Meade's revolutionary LS LightSwitchтДв series of telescopes use advanced technologies to do what no other consumer telescopes have done before: take all the hassle out of using a telescope. ... LX200/LX600 Level/North Sensor Array. ...

State Research Center of Genetics and Selection of Industrial Microorganisms, GosNIIGenetika, Moscow , Russia Some questions of interpretation of results for DNA-protein binding on tiling arrays October 9, 2008 3rd workshop on algorithms in Molecular Biology , Moscow , 2008 ChIP-chip technology From: http://www.tigr.org October 9, 2008 3rd workshop on algorithms in Molecular ...

Among the functions the Cluster Database supplies the tclets are usefull tool for various researches (for example, for identification of radio and of optical sources). ... Three type of object are present on the picture: . ... To place the current object under all other click on left mouse button. To remove the object click on right one. ... You can switch off/on all objects of some type by clicking on the Control window buttons: "Galaxies", "FIRST radio objects" or "NVSS radio objects". ...

The Arecibo L-band Feed Array (ALFA) is a seven feed system that allows large-scale surveys of the sky to be conducted with unprecedented sensitivity using the 305-m Arecibo telescope in Puerto Rico. ALFA, operating near 1.4 GHz, consists of a cluster of seven cooled dual-polarization feeds, a fiber-optical transmission system, and digital back-end signal processors. ... ALFA Memos . Surveys and Data Products . ALFA Contact People: . ... Spectral lines: Robert Minchin . ... R. Minchin . ...

Static Fourier spectrometers are often used for spectral measurements of the ionosphere emissions. There are two main advantages of Fourier spectrometers (FS) - large geometric factor and high spectral resolution; these parameters are two orders better than for grating spectral instruments. ... In scanning Fourier spectrometer optical and electric modulation of signal is used to avoid this problem, for static Fourier spectrometer there are no such ways. ...

Infrared Detector Array Links . ... Control Software Links . Optics Links . Micro-Optics Links . ... Optical Materials Databases . ... Atmospheric Database Links . Linux Links . ... Rockwell Science Center home page. ... Santa Barbara Research Center home page. ... CCD-World home page. ... SDSU home page. ... EPICS home page. ... Optics Society of America . ... Linux on Laptops ( local site and US home page ). ... Instrumentation Links * Gemini Project Links * Other IR Instruments ...

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... Science User Portal . ... ESO, the European Southern Observatory . ... Travel and Contacts . ... Travel to Paranal . ... ESO . ... VLT/Paranal . ... Survey Telescopes . ... Star Clusters . ... VLT Unit Telescopes Names . ... ESO 3.6-metre telescope . ... A view of the Paranal platform with the four 8.2-m VLT Unit Telescopes (UTs) and the foundations for the 1.8-m VLT Auxiliary Telescopes (ATs) that are used as the VLT Interferometer (VLTI). ... Paranal , Very Large Telescope , VLT Unit Telescopes . ...

... JavaScript version 1.3 provides the following new features and enhancements: . ... See the Client-Side JavaScript Guide for details. ... Changes to the Array object. ... The push method returns the new length of the array rather than the last element added to the array. ... Changes to the Date object. ... Added a day parameter to the setMonth method. ... Added the apply method, which allows you to apply a method of another object in the context of a different object (the calling object). ...

... Up: Telescope and Instrument Control Systems . ... The software is based on a client/server architecture and provides remote access for controlling, monitoring and troubleshooting the array. ... The server software is developed in C++ and runs on a UNIX host machine. ... This computer demonstration consists of remote observing with the Caltech Millimeter Array located at Owens Valley in California to show the feasibility and features of this software package. ... Figure 2: Array Status window. ...

... Astrophysics Group . ... Beam measurement and calibration of the SKA AAVS0 array at Lord?s Bridge using a UAV system . ... SKA AAVS0 array . ... The AAVS0 array (Aperture Array Verification System 0) is the very first SKA prototype array with 16 SKALA (SKA Log-periodic Antenna) elements developed at Cambridge University for the SKA LFAA (Low Frequency Aperture Array) instrument. ... Furthermore, the UAV measurement system has been used to very calibration strategies to correct the array beam. ...

XMM-Newton Science Analysis System Page: 1 omcos ag July 9, 2007 Abstract Applies the OM tracking history to a bad pixel map 1 Instruments/Modes Instrument Mode OM FAST OM IMAGING 2 Use pipeline processing yes interactive analysis yes 3 Description The shift and add process means that the counts observed in each pixel of an OSW image may have been accumulated in several di erent detector pixels. This task takes the OM tracking history and applies it to the map of bad pixels de ned in the CCF. ...

Astronotes Armagh Planetarium's Stellar Blog! ... Our Galaxy . ... Other Galaxies . ... Space Flight . ... When Galaxies Collide (Image credit: ALMA (ESO/NAOJ/NRAO). Visible light image: the NASA/ESA Hubble Space Telescope) . In the southern sky constellation of Corvus (the Crow), we see the Antennae Galaxies (alias NGC 4038 and 4039). ... Your email address will not be published. ... Here you will find the latest news and views from the fascinating worlds of astronomy and space exploration. ...

Instruments and Methods 129 Multi-element MMIC focal array for radio telescope V.B. Khaikin1, E.K. Ma jorova1 , Yu.N. Parijskij1, M.D. Parnes2 , R.G. Shifman2 , V.A. Dobrov2 , V.A. Volkov2, V.D. Korolkov2, S.D. Uman2 , N.A. Esepkina3 , and S.K. Kruglov3 The Special Astrophysical Observatory of Russian Academy of Sciences Karachai-Cherkessia, N.Arkhyz, 357147, Russia, E-mail: vkh@brown.nord.nw.ru Svetlana", Rezonance", Ascor", 194156, Engels pr. ... Four-element sub-array prototype is shown in Fig.2. ...

The Cartwheel Galaxy . This false-color composite image shows the Cartwheel Galaxy as seen by the Galaxy Evolution Explorer's far-ultraviolet detector (blue); the Hubble Space Telescope's Wide Field and Planetary Camera 2 in B-band visible light (green); the Spitzer Space Telescope's infrared array camera at 8 microns (red); and the Chandra X-ray Observatory's advanced CCD imaging spectrometer-S array instrument (purple). ...

Astronomy Picture of the Day . A Very Large Array of Radio Telescopes . ... 20.06.1999 . ... Credit: NRAO , NSF Explanation: Pictured above is one of the world's premiere radio astronomical observatories: The Very Large Array (VLA). ... The VLA is the most sensitive radio telescope ever, and, through interferometry , can resolve a golf ball-sized radio source 150 kilometers away (0.04 arcsec). ... Publications with keywords: radio - telescope . Publications with words: radio - telescope . ...