... See also ELAIS survey with VLA C.Cesarsky, L.Danese, A.Franceschini, . ... astro-ph/9812256; http://athena.ph.ic.ac.uk/pubs.html downloaded 4-May-99) B1950 coords added and (dummy) values of zero blanked out on 4-May-99 by H.Andernach A deep survey of the European Large Area ISO Survey (ELAIS) field in the southern celestial hemisphere (hereinafter S1) has been carried out with the Australia Telescope Compact Array (ATCA) at 1.4 GHz. ... Table 1: The ATCA 1.4-GHz Radio Catalog of S1 name ELAISR20_J....

... Prev . Next . comedi_get_cmd_src_mask -- streaming input/output capabilities . ... int comedi_get_cmd_src_mask (comedi_t * device, unsigned int subdevice, comedi_cmd * command); . The command capabilities of the subdevice indicated by the parameters device and subdevice are probed, and the results placed in the command structure pointed to by the parameter command. The trigger source elements of the command structure are set to the logical OR value of possible trigger sources. ...

... Solar flare activity is produced by the processes of accumulation and release of energy in an active region. ... In the framework of study of solar active regions, producing powerful flares the researchers from the RATAN-600 radio telescope have detected sources with features in the form of a sharp drop in the intensity of polarized radiation in various parts of the recorded frequency range (2-16GHz), sometimes changing the sign of polarization. ...

... Corresponding gates in each row are connected in parallel at both edges of the array. ... Other gates. ... otherwise indicated, 45 kpixels/sec and standard voltages using a dual slope CDS circuit (8 µs integration time) Minimum Format Pixel Size Imaging Area Dark current (MPP), 20° C equivalent Readout noise Front Back Full Well signal Output gain CTE per pixel Typical 512 x 512 pixels 24 µm x 24 µm 12.3 mm x 12.3 mm 50 pa/cm2 5 electrons 7 electrons 350,000 electrons 1.5 µV/ electron 0 ...