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Re: ToO for Wednesday (VX017A)

From: <shoriuch_at_email.protected>
Date: Tue, 28 May 2013 16:40:54 +1000

Cormac,

I guess SgrA* at L-band is still weaker than ambient load. DAS for 64MHz
profile for L-Band looks fine with the level between sky and ambient load.

As I told you in the separate email, 70m is only available for limited
time, i.e. 10:00-13:00 and 17:45-19:30, we should take some lisk for Tid.
The antenna is yet to return to be operational and I won't be onsite to run
this, leaving Phil Pope in ops team to run this.

Cheers,
Shinji.

On 28 May 2013 15:50, John Reynolds <John.Reynolds_at_csiro.<!--nospam-->au> wrote:

>Shinji,
>
>
>I would just play with manual attenuators to get the signal within the
>>right range.
>>
>
>That could be twice every 6 minutes, as we switch between the pulsar and
>the cal. Be nice to have some help if you're doing this.
>
>On the other hand the DAS might just be able to cope with the range,
>though SgrA* is the strongest source in the sky other than the Sun so I'm
>guessing maybe not.
>
>Cheers,
>John R
>
>
>On Tue, 28 May 2013, shinji horiuchi wrote:
>
>I would just play with manual attenuators to get the signal within the
>>right range.
>>
>>Cheers,
>>Shinji.
>>
>>
>>On 28 May 2013 14:27, James Lovell <Jim.Lovell_at_utas.<!--nospam-->edu.au> wrote:
>>
>>Some programmable attenuators would be nice at Tid. There were some ready
>>>to install when I was there. Leigh Cameron even got them working but they
>>>caused RFI (or something) so had to be removed.
>>>
>>>Maybe if Shinji could plumb the signal though the MkIV rack as this has
>>>programmable attenuators that can be controlled from the Field System.
>>>
>>>Or perhaps better to record to Mark5 and have a couple of extra
>>>procedures
>>>that are called after source changes to adjust the attenuation? Then no
>>>re-wiring is needed.
>>>
>>>Cheers,
>>>Jim
>>>
>>>
>>>
>>>
>>>On 28/05/2013, at 2:14 PM, John Reynolds <John.Reynolds_at_csiro.<!--nospam-->au>
>>>wrote:
>>>
>>>Cormac,
>>>>
>>>>some Tid time has just become available for vx017a, so I have updated
>
>>>>
>>>>Should be fun maintaining acceptable levels when switching on and off
>>>>
>>>SgrA, something that promises to be interesting at Parkes as well.
>>>
>>>>
>>>>Cheers,
>>>>John R
>>>>
>>>>On Tue, 28 May 2013, Cormac Reynolds wrote:
>>>>
>>>>hi,
>
>some Tid time has just become available for vx017a, so I have updated
>the schedule (and redistributed). Please make sure you are using the
>vex file with 'PI revision number: 2.0'. Some of the scan timings have
>changed to incorporate the slower moving antenna.
>
>thanks,
>Cormac.
>
>On 27 May 2013 18:40, Cormac Reynolds <c.reynolds_at_curtin.<!--nospam-->edu.au>
>wrote:
>
>>hi all,
>>
>>I have created a schedule for Wednesday's LBA ToO. Schedules have been
>>distributed to the telescopes and the wiki pages are in place:
>>http://www.atnf.csiro.au/vlbi/**wiki/index.php?n=LBAMay2013.**VX017A<http://www.atnf.csiro.au/vlbi/wiki/index.php?n=LBAMay2013.VX017A>
>>
>>Regards,
>>Cormac
>>
>>--
>>------------------------------**----------------------
>>Cormac Reynolds
>>Phone: +61 8 9266 3785
>>Fax: +61 8 9266 9110
>>email: c.reynolds_at_curtin.<!--nospam-->edu.au
>>------------------------------**----------------------
>>
>
>
>
>--
>------------------------------**----------------------
>Cormac Reynolds
>Phone: +61 8 9266 3785
>Fax: +61 8 9266 9110
>email: c.reynolds_at_curtin.<!--nospam-->edu.au
>------------------------------**----------------------
>
>
>>>
>>>
>>
Received on 2013-05-28 16:41:02