[evlatests] Nothing but noise!
Bryan Butler
bbutler at nrao.edu
Wed May 30 16:42:56 EDT 2007
this is the famed yin-yang mode?
On 5/30/07 14:31, Rick Perley wrote:
> I used 4.5 hours of free 'Dynamic Time' last night to do a deep
> integration at L-band on a random background field.
>
> Setup: BW = 12.5 MHz. Mode = '4'. This gives 16 channels, each
> of 781 kHz, for each of the four parallel hand correlations.
> Integration time was set to 3.33 seconds.
> Calibration: I observed 3C286 once every 15 minutes, for one minute.
>
> Bandpass solutions (with Hanning smoothing on, to reduce the Gibb's
> oscillations) were done for every calibrator observation.
>
> Straightforward gain calibration (2-point) was then done. The usual
> flagging was done to remove bad antennas and visibilites. In general,
> the data were of excellent quality. 27 antennas worked (but not all of
> them well).
>
> The randomly chosen field was at: RA = 13 30 00, Dec = 28 00 00.
> (The strong sources 3C286 and 3C287 were each about 2.5 degrees away).
> Afterwards, I checked the NVSS map archive, to find that I had put the
> beam in a remarkable 'hole' -- virtually no sources within the primary
> beam! (I checked because my first image returned rather fewer sources
> than I expected to see!)
>
> Imaging Results:
>
> I made many images, with single channels, and blocks of channels,
> with one IF and both IFs, of selected fields, and of the whole primary
> beam (this takes a long time -- my machine is still laboring away ...).
> But one result is very clear:
>
> ********* There are no artifacts of any kind, at any place, in any
> channel, in any images ********
>
> The full-beam, both-IF, 13 channel (channels 2 through 14) image is
> showing dozens of sources at the few-mJy level (and less), with rms
> noise levels below 100 microJy. The sources are clean and sharp. Tests
> with EVLA only and VLA only subsets show the same sky, with noise levels
> more or less in inverse proportion to the number of antennas available.
>
> All looks completely normal to me.
>
> Specific EVLA problems (and there are a few!) will be described in a
> subsequent report.
>
>
>
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