... 1 Vol = 1 Array name = ATLBA Antennas: 1:PKS 2:HOB 3:CAT 4:TD7 Sourcename = CIRCINUS : 1 Calcode = Timerange: 0/05:02:51 - 0/06:00:01 Visibility numbers 1 - 3434 Subarray = 1 Freqid = 1 ANTS 1 2 3 ------------------- 1 | ... 0 0 0 ------------------- Sourcename = CIRCINUS : 1 Calcode = Timerange: 0/06:15:47 - 0/07:15:45 Visibility numbers 4697 - 9940 Subarray = 1 Freqid = 1 ANTS 1 2 3 ------------------- 1 | ... 1 Vol = 1 Subarray = 1 Freqid = 1 ANTS 1 2 3 ------------------- 1 | ... 0 431 431 2 | ...

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• http://www.atnf.csiro.au/pub/people/vlbi/v174/v174a/corr/V174A_DT_SUM.TXT
• http://www.atnf.csiro.au/pub/people/vlbi/v176/v176b/corr/V176B_F1_DATA_SUMMARY.TXT
• http://www.atnf.csiro.au/pub/people/vlbi/vx009/corr/DT_SUM.TXT

Hide Zen home . ... GiST . ... desc') - sort intarray test =# select sort ('{1,2,3}':: int [],'desc'); sort --------- {3,2,1} (1 row) int [] sort ( int []) - sort in ascending order int [] sort _asc( int []), sort _desc( int []) - shortcuts for sort int [] uniq( int []) - returns unique elements test =# select uniq( sort ('{1,2,3,2,1}':: int [])); uniq --------- {1,2,3} (1 row) int idx( int - returns intarray - union of arguments int[] | ... Zen, 2003-2007 ...

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Last modified on November 17, 1998 by A. Richichi . An occultation of the late-type star SAO 95190 was recorded at the Calar Alto Observatory's 3.5m telescope using for the first time the Omega-Cass camera. This uses a 1024 x 1024 pixel HgCdTe array (HAWAII), which can be read-out at fast speed in a subarray. ... A movie is available (300Kb), showing a sequence of about 2.4 seconds in a 32 x 32 pixels subarray, corresponding to 9.6 x 9.6 arcseconds on the sky. ...

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• http://www.arcetri.astro.it/irlab/luna/news/3c273/index.html

Aitoff Projection showing ChaMP Fields . ... Main survey: >20 from galactic plane. ... Galactic Plane Survey: No subarray fields: reduced area and more complicated processing . ... Short exposures included except NGC galaxies . Galactic Plane Survey: > 30 ksecs . ... Galactic Plane Survey: >10% contamination by a diffuse/distributed X-ray or optical source. ... E(B-V)= (B-V) - (B-V) 0 which translates to visual extinction A V via . ... Crudely, E(B-V) can be related to Galactic latitude via . ...

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. Fig.6 Topography of 8 element MMIC feed SUBARRAY at 26-30 GHz which is being tested now . Multi-beam feed array with 10 000 receiver elements may be installed in the focal plane of the RATAN-600

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... The BIMA Data Archive at NCSA has been operating in production mode for a decade and will be reused for CARMA with enhanced search capabilities. ... This in- CARMA Data Storage, Archiving, Pipeline Processing CARMA Data Flow and Archiving 271 AIPS++ Imaging Pipeline MIRIAD NCSA Internet to Subarray #1 MS2 Dataset Mir Subarray #1 Visibilities Subarray #1 MS2 Dataset Subarray #1 Header MIRIAD Observing Program 60 sec Monitor Avg. 0.5 sec Monitor Data Metadata Subarray #1 Astr. ...

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... More so for optical, radio Ї Ї Ї Ї Ї Ї Ї LSST = Large Synoptic Survey Telescope ґ Rename to OLSST Consider RLSST ( Radio LSST) The dynamic radio sky (DRS) = SKA science area SKA specifications unprecedented blind surveys of the DRS The science is important for the known knowns There are bound to be many unknown knowns and unknown unknowns Fast and slow transients : ґ What capabilities are needed Tucson Future cm/m Telescopes 1 8/21/ ... The Dynamic Radio Sky, Cordes et al. ...

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• http://www.naic.edu/~phil/notes/idlspcproc.html

... Представлено описание 10-антенного макета многочастотного Сибирского радиогелиографа. ... The 10-antenna prototype of the multifrequency Siberian radioheliograph is described. The prototype consists of four parts: antennas with wideband front-ends, analog back-ends, digital receivers and a correlator. ... The frequency range of the prototype is from 4 to 8 GHz. ... radioheliograph, antennas with a wideband feed system, digital receivers, correlator, frequency converter. ...

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... Alta E6 Imaging area 1024 x 1024 array, 24 x 24 micron pixels (actual size) 1 MHz 16-bit digitization and 1.4 MHz 12-bit digitization to 24Mbyte camera memory 100bT Ethernet interface: up to 300 kHz throughput TCP/IP or UDP protocols DHCP or fixed IP addressing No plug in cards or external controllers Programmable , intelligent cooling to 50° C below ambient Ї Astronomy Binning up to 10 Horizontal x ... Pixel Binning Exposure Time Frame Sizes Cooling Dark Current (nom.) ...

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• http://www.apo.nmsu.edu/35m_operations/35m_manual/Instruments/NA2Guider/PDF/ESeries34x11.pdf

... Функция P?(R,r) описывает прохождение радиоволн от источника до антенны. ... Находится пик ?грязной карты?. ... Установить параметр TASK для задачи самокалибровки данных функции видности CALIB TASK 'CALIB' Просмотреть необходимые для работы задачи параметры INP Установить необходимые значения параметров INNAME* INCLASS* INSEQ* INDISK 1 Данные о функции видностинаходятся на диске 1 CALSOUR ' ' QUAL -1 CALCODE ' ' SELBAND -1 SELFREQ -1 FREQID -1 TIMERANG 0 BCHAN 1 ECHAN 0 ANTENNAS ...

11. http://www.mrao.cam.ac.uk/~bn204/alma/memo-turb/uvfits.py

12. http://star.arm.ac.uk/~ambn/yzcmi83_final.ps

13. http://www.mso.anu.edu.au/~kcf/pubs_top20/67.pdf