Äîêóìåíò âçÿò èç êýøà ïîèñêîâîé ìàøèíû. Àäðåñ îðèãèíàëüíîãî äîêóìåíòà : http://www.atnf.csiro.au/management/atuc/2015nov/ATUCnov2015SciOps.pdf Äàòà èçìåíåíèÿ: Tue Nov 24 01:11:34 2015 Äàòà èíäåêñèðîâàíèÿ: Sun Apr 10 09:27:00 2016 Êîäèðîâêà: Ïîèñêîâûå ñëîâà: http www.astronomy.com

Science Opera;ons
Phil Edwards | Head of Science Opera0ons
CSIRO ASTRONOMY & SPACE SCIENCE


Outline
· The user community · General issues · Parkes · ATCA · Tidbinbilla · Long Baseline Array · Call for Proposals


OPAL Users by Country (top 82%)
Country United States Users 779 600 341 293 218 195 186 153 115 109 81 % of total 21% 16% 9% 8% 6% 5% 5% 4% 3% 3% 2%



Australia Germany United Kingdom Japan Italy France China Netherlands Spain Canada

A total of 3700 users in the OPAL database (since 2006).


General issues
· The clearinghouse for informa0on on ATCA data archives is now hUp://www.atnf.csiro.au/observers/data/ ... which contains a link to the growing log of ATCA issues hUp://www.narrabri.atnf.csiro.au/observing/IssueArchive.html · How can we aUract more (and more useful) Observer Feedback? The exis0ng ques0onnaire is overdue for an overhaul. Much of the feedback falls into one of three categories:
· First-
0me observers · Regular observers with not much feedback to give · Really grumpy observers

· The numerical scale of responses allows feedback to be quan0fied, but usually the best feedback is the free format text


New support model (from Feb 2015)
· All first-
0me observers will be required to come to the SOC, and will be provided with telescope orienta0on and training sessions · The requirement for Parkes observers to return to the SOC annually will be dispensed with: the PI must ensure the observers on their team are trained and competent observers. · All ATCA observers coming to the SOC will be provided with a Friend for the dura0on of their stay. The requirement to observe from the SOC annually in order to be "remote qualified" will be retained for most ATCA observers. · Regular, competent observers (typically, people observing on at least three separate occasions or for more than 10 days per semester) can extend the 0me between their return visits by 6 months. hUp://www.atnf.csiro.au/observers/apply/ATNF-
support.html

Science Opera0ons | Page 5


Parkes visit by the Governor of NSW

His Excellency General The Honourable David Hurley AC DSC (Ret'd)


Parkes
· The 2015OCT schedule was only released through to Dec 24. The schedule for the remainder of the semester will be released later this week · There is a two-
week shutdown this & next week to run op0cal fibre to the focus cabin, and install a new rack in the focus cabin · There will be another two-
week shutdown from Feb 1--12 to remove MB20 and install the MPIfR PAF · MBCORR (and the WBC) will be decommissioned in the coming weeks · A number of receiver changes will be made during 2015OCT, and 2016APR, so that the 10cm/50cm receiver and H-
OH receiver (1.2-
1.8 GHz) will be available at 0mes during semester.

Science Opera0ons | Page 7


Parkes
· It was discovered earlier in the year that DFB spectral line data were not being normalised correctly. That is, RPFITS spectra were found to be scaled in amplitude by the system gain, essen0ally an unknown factor. · The problem was en0rely correctable but required addi0onal processing steps. The fault is now corrected and RPFITS spectra from the DFBs are now correctly normalised and calibrated.


Bi-
sta;c radar demonstra;on
This month we have been undertaking bi-static radar demonstrations: the Tidbinbilla 70m transmits at a Near Earth Asteroid at 2.1 GHz, and Parkes receives the echo

Echo from 2005 UL5, 20-nov-2015


ATCA
· A busy week was held recently at Narrabri to give the ATCA User Guide a thorough review and update: thanks to Robin Wark, Jamie Stevens, Shari Breen and Karen Lee-
Waddell · The sec0ons on RFI (1.3.2) and data flagging (4.3.5) have been significantly expanded, as requested by ATUC. · The producers of mid-
week RFI con0nue to provide some advance warning of likely episodes. · More explicit informa0on also given in Call for Proposals about RFI in the 20cm band · Two on-
line training videos available for ATCA -
-
linked from hUp://www.narrabri.atnf.csiro.au/observing/CurrentIssues.html · CABB aliasing of spectral lines in zoom mode ­ under inves0ga0on


Embracing social media?

ATUG = TLDR?


Embracing social media...

"Phasebook" !


ATCA automa;on
· Trials of unaUended observing con0nuing.
· One minor issue uncovered: the "countdown 0mer" on a dwell scan doesn't start un0l all antennas are on source and tracking.

· Automated aler0ng via SMS has been on hold. Requirements are being draled for the Solware & Compu0ng group to implement · Can implement "queue observing" rela0vely easily, though may require schedules to be made with "normal" scan mode, or in UT · "Service observing" has been offered in the past, but the preference is now for teams to find a local collaborator · Full "dynamic scheduling" would require quicker CABB mode changes, and change to observer model/support

Science Opera0ons | Page 13


ATCA Rapid Response
· It is possible to switch automa0cally in response to a trigger as soon as a valid schedule file is placed into a special directory. · There has not yet been any scoping of a system required to receive an alert and respond intelligently
· · · · · is the target above the ATCA horizon? are we in a suitable array configura0on and CABB configura0on? do we need to mosaic the field? can this NAPA displace the current observer? is a dcal required for this observa0on?

· Propose a trial limited to 4cm-
band follow-
up, with regular 4cm dcal's aler each CABB mode change & array config.


A GPU-
based replacement for CABB?
CABB is a powerful backend, that has significantly improved ATCA con0nuum sensi0vity, but
· · · · Some CABB configura0on changes take an expert an hour Not all ini0ally an0cipated zoom modes are available CABB blocks drop out at (ir)regular intervals The developers are no longer on staff

Could we improve flexibility, reliability and long term support with a GPU backend? New samplers, which talk directly to op0cal fibre Use ASKAP "redback" boards for coarse filterbank (128 MHz) and Ethernet packe0sa0on (10 GbE) Fine filterbank and cross correla0on in GPU -
Ethernet cross connect |
DIFX 2015 ­ Chris Phillips


|

DIFX 2015 ­ Chris Phillips


Costs: Total
Antennas Samplers Redback SFP Copper SFP Op0cal Server GPU NIC Switch Total 6 24 12 192 64 16 32 32 1 $120,000 $144,000 $7,680 $2,560 $128,000 $32,000 $25,600 $30,000 $489,840

http://www.atnf.csiro.au/vlbi/dokuwiki/doku.php/difx/meetings/hobart2015/agenda

|

DIFX 2015 ­ Chris Phillips


Tidbinbilla
· The 4-
channel K-
band receiver upgrade has recently been completed on the 70m. This new system supports two simultaneous beams per polarisa0on (four beams in total) across the total frequency coverage of 17 GHz to 27 GHz · It is planned to install a dual-
circular polariza0on L-
band system on DSS-
43 ~mid-
next-
year, covering 1.4 ­ 1.9 GHz · The Call for Proposals for 2016APR makes clearer the typical amounts of 0me available:
· "Access to Tidbinbilla antennas is provided through the host country agreement, which provides approximately 220 hours in total each semester, which is used for both single dish (typically 180 hours per semester) and LBA (typically 40 hours per semester) use."

· Helga Denes has taken over as ATNF Friend of Tidbinbilla


LambdaGammaBI ­ looking
Phil Edwards | Head of Science Opera0ons 20 April 2015
CSIRO ASTRONOMY & SPACE SCIENCE

up from down under

Credit to Leonid Gurvits for suggesting this title...


BI ­ looking
Phil Edwards | Head of Science Opera0ons 20 April 2015
CSIRO ASTRONOMY & SPACE SCIENCE

up from down under

...which may be more comprehensible in this format!


Long Baseline Array (VLBI)
· Correla0on of LBA data was carried out under contract by Cur0n University un0l the end of September 2015. · Correla0on has now been brought back "in-
house" and a term posi0on was adver0sed for LBA correla0on and commissioning support: Cormac Reynolds started in October · During VLBI observa0ons last week we co-
observed with the TianMa 65m telescope in Shanghai & the Kunming 20m telescope · The Mopra telescope has been mothballed for the summer while arrangements for possible future opera0ons are made · Requests for Tid 70m being made earlier, with some success · On-
line training videos for VLBI observing


Call for Proposals
Call for Proposals for 2016APR released last week: hUp://www.atnf.csiro.au/observers/apply/avail.html Proposal deadline is 5pm AEDT Tuesday December 15th. TAC procedures are outlined at www.atnf.csiro.au/management/tac/ We ask users to include their proposal codes in their publica0ons.
Science Opera0ons | Page 22


Thank you
Phil Edwards Head of Science Opera0ons t +61 2 9372 4717 E philip.edwards@csiro.au w www.atnf.csiro.au/
CSIRO ASTRONOMY AND SPACE SCIENCE