SAO Instructor's Travels


Instructors Travels

Teaching Period 4, 2006

Posted 4 August: Sarah Maddison goes to Narrabri to do remote Mopra observing

Posted 9 August: Chris Fluke reports Preston, UK


4 August 2006: Dr Sarah Maddison goes to Narrabri to do remote Mopra observing...

My student, Annie Hughes, is working on two projects with Mopra and during August 2006 she has been awarded observing time for both of her projects. This is great, but there's a six day period where she has the telescope 24 hours a day! So she needs a bit of help with the observing :) The original plan was that I would join her at Mopra and we'd do 12 hours shifts each. But there have been plans within ATNF (ATNF = Australia Telescope National Facility, and they're the people who run the Mopra telescope) to go remote with Mopra "sometime" in 2006. After much discussion, it was decided that we would try the first remote observing with Mopra on Thursday 3 August. So rather than driving from Melbourne to Mopra (~11 hours), instead I flew to Narrarbi (~4 hours), which was much more convenient for me!

The two projects that Annie is working on are 12CO mapping of the inner regions of the Large Magellanic Cloud, and molecular mapping of the Ara OB1 molecular cloud. (For those of your studying HET608 this semester, you'll see some of Annie's data - from both of these projects - in Module 10 on radio imaging.) In my 12 hour shifts I'm doing the Ara OB1 observing, while Annie is doing the LMC observations.

We're observing Ara OB1 at 3mm using MOPS, the Mopra Spectrometer. MOPS allows us to observe multiple lines simultaneously, and we've chosen to look at the following nine lines: 12CO, 13CO, C18O, C17O, CH3OH, SO, CH3CN and two hyperfine transitions of CN. The spectral lines of these molecules all lie between 108 GHz and 115 GHz (which is within the 3mm band). If you want to learn a bit more about these molecules, see the ATNF rest frequency of spectral lines page, or the Frank Lovas' page on interstellar molecular microwave transitions website.

The Ara OB1 is part of a massive star forming region of our Milky Way galaxy at a distance of 1,300 pc. There are two massive O stars in this region, which makes it a good cloud to test theories of triggered star formation. For an optical overview of the region, see below. We're doing "on-the-fly" mapping of the region, with each of our filed measuring 5' x 5' in the sky. Below we show a NANTEN 12CO map of the Ara OB1 region, overlaid with our fields:
ESO optical image of Ara Our fields overlaying a NANTEN 12CO map

And here is our latest Mopra maps:
12CO map 13CO map
The "holes" in the maps above are being filled in right now!

I have to admit that we've had a flew 'glitches' with the observing (or at least I have - Annie is a far more experienced observer than I am!) but I don't think any of these problems have been due to the fact that we're doing remote observing. There is a webcam at Mopra, but I can't see anything right now because it's night time! So the only way we can tell if it's raining is by checking the system temperatures, which is not perfect, but on the other hand I can now walk over to the lodge and heat up my dinner which was made for me by the lovely Narrabri lodge staff earlier today :) Thanks very much to the Mopra & ATNF staff for making remote observing possible!

Postscript.... 5 August
Most of the 'glitches' discussed above had to do with the pointing. Now we know why - it was very windy last night and each time the antenna slewed, the wind knocked it about a bit! This doesn't really matter for the relatively large maps of diffuse gas we're making, but it does matter for the pointing which needs to accurately find the position of a point source. So the reason we weren't immediately finding our calibrator (an SiO maser) was because the antenna was pointing in slightly the wrong spot. And how did we discover this? Because the alarms went off! It is a bit nerve-wracking when you're happily observing away and suddenly a very loud alarm begins to sound and you can't quite work out what the problem is! The weather monitoring system had a few problems so we couldn't immediately see that the wind was gusting above 40 km/hr. We ended up stowing the dish and poor Annie lost about 5 hours of her LMC project. Today we're being very vigilant about wind monitoring!

Here's the happy observer, collecting data while the winds are calm :)


9 August 2006: Dr Chris Fluke reports from Preston, UK

As you are all aware, astronomy is a very international science, and this means that our collaborators are usually spread all over the world. One particular project that I am involved in is called the Commonwealth Cosmology Initiative. Through research linkages between Australia and the United Kingdom, we are hoping to help grow computational cosmology in Australia.

What does that all have to do with travel, I hear you ask? The answer is that I am currently travelling to meet up with one of my collaborators (former SAO instructor Prof Brad Gibson) at the University of Central Lancashire in Preston. Then, I'm off to the University of Durham, to meet some of the world's leading computational cosmologists...and also check on the progress of my postdoc, Dr Chris Power, who is spending several months back at the institution where he gained his PhD before joining Swinburne's research staff about 2 years ago.

So just what is computational cosmology? Well, it involves trying to model the Universe, particular its evolution or the growth and development of structure, by using complex computer simulations. Unfortunately it is impossible to exactly simulate the Universe - as that would require having a model for the location and motion of every single proton, electron, neutron and dark matter particle!! Instead, we make some simplifications, including often throwing away all of the "normal matter" and just looking at the effects of the dark matter.

Computational cosmology is a fairly new branch of astronomy - it has only existed since computers became available (mid 20th century), and it within the last two decades or so that it has become a mature branch of astronomy that is making valuable predictions. In fact, that is one of the best things about computational cosmology - you can choose your favourite parameters for the universe, simulate it, and then investigate what the observers might be able to see.

One of the nice things about international travel for research is that you do get to meet some of the leaders in the field, but you also get to promote your own work: and I will be giving talks on some of my research work at both Preston and Durham.

Another advantage is that you get to visit some fun places, and I was fortunate to have a chance to see the Royal Greenwich Observatory (RGO). As you can see in the somewhat shadowy "self-portrait", it was just on noon - my shadow is cast onto the prime meridian. Actually, it was 1pm local time, as the UK is currently on daylight savings/summer time.

While at the Observatory, I also witnessed the dropping of the time ball, which occurs (traditionally) at 1pm every day.

The RGO has some great display areas, particularly covering the history of time-keeping, and the attempt to find a suitable clock to allow measurements of longitude. Also on display are many of the original instruments, such as transit telescopes and mural quadrants that were used to determine the positions of stars with great accuracy. It was just a shame that photography inside the Observatory was not allowed...but probably just as well, as I might still be there!



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Monday, 19-Nov-2007 11:17:37 AEDT