An introduction
Hello. I’m new around here and I thought I should introduce myself. My name is Arfon Smith and I’m the latest addition to the Galaxy Zoo team. I’ve been appointed to the role of technical lead and I’m looking forward to working with Chris in Oxford on some really exciting new stuff for future versions of Galaxy Zoo.
Galaxy Zoo is a great project and a perfect fit for my two main interests, Astronomy and Software. I have a PhD in Astrochemistry from The University of Nottingham where I studied the role that dust has to play in a variety of astrophysical environments.
More recently I have been working as a software developer at The Wellcome Trust Sanger Institute (Human Genome Project) near Cambridge. At Sanger, I’ve been working on web applications to support the high-throughput sequencing of DNA. It’s been a great experience but I’m really looking forward to being back in the astronomical community.
Anyway, that’s about all for now! For those of you interested, I’ll be blogging about some more technical aspects of the software development process going on behind the scenes at Galaxy Zoo. Look out for updates soon!
More from Chris's talk – red spirals
Chris told me in the pub yesterday that “it’s nice to give a Galaxy Zoo talk where people are already familiar with the story; it means that people already know the story.” That’s a testament to the success of your classifications — from what I’ve seen at this meeting, it seems that in just a year and a half, Galaxy Zoo has gone through evolved from a cool new strategy for doing science to a source of exciting research results. The results Chris presented about red spirals were particularly interesting. Karen Masters has blogged about these red spirals before. Spiral galaxies usually contain lots of young, blue stars, but these “red spirals” contain old, red stars. What this means is that the formation of new stars in these galaxies has been shut off. Galaxy Zoo’s contribution — your contribution — has been to show that red spirals most often live at the edge of galaxy clusters. They are clusters that have just begun to move toward the centers of clusters due to the clusters’ gravitational attraction. The attraction of the galaxy clusters has led to new star formation being shut off, but not to the shape of the galaxy changing — a process that Chris called “gentle strangulation.” The gravitational attraction is just right — enough to shut off star formation, but not enough to deform the galaxy.
Conditions Improving
I am halfway through our penultimate night and, as expected, the weather is still poor though much better than the previous night. In total it left about 2-3 feet of snow (Pic A) and for most of the day it looked as though the telescope would remain non-operational. Lots of ice had collected on the dish and the receivers. After about an hour into our scheduled run though, there was a short spell when the stars came out and the satellite images suggested the cloudy front had finally passed. The first thing needed was for the operator to get on the raised platform and knock off all the ice from the receiver (Pic B). They also heated the dish to melt the ice though this meant that our calibrations would be off for a while since the receivers basically work by measuring temperature differences. Anyhow, we got underway with some Blue Elliptical galaxies a bit later and I thought that things would pick up quickly. Unfortunately, more cloud soon moved in and it was very hard to get a good signal. I had to resort to pointing at Saturn for readings which is not ideal because Saturn is large compared with our beam and so its not great at calibrating the exact centre of the direction in which the telescope points. In any case, by the time we were taking readings it started snowing again and we had to shut down. Hopefully it will have cleared up by day break and we can get a few good readings in. I also managed to get a picture of Senor Zorro with the flash at a distance. If this isn’t the epitome of evil, then I’m not sure what is (Pic C)!
Pictures: (A) Snow, (B) Icicles and (C) Evil.
Iram Now 30cm Under!!!
The bad weather continues to badden. The telescope has now been down for about 36 hours and the first night of the blue ellipticals project has saddly gone to waste. There is atleast a foot of snow now and the dish is covered in icicles (pictured). The forecast isn’t good for tomorrow either so our best hope for results will probably be in the 5-hour stretch just before we finish on Monday!
In other news, Senor Zorro came back last night, pining at the window for more of my hard earned champagne! I thought I better include this picture as it brings out the evil in his eyes. 
IRAM 30m – 30mm Under!
We’re almost 30 hours into our observing run to examine “Molecular Gas in Merging Spirals” and virtually the whole time we’ve been shut down due to weather! Tonight we’re expecting 3cm of snow which is great news for the skiers (who seem to be enjoying perfect blue skies during the day) but disastrous for detecting CO gas from galaxies. IRAM can see through some cloud, but when the air is completely saturated with water there is no possibility of getting a clean signal. The most exciting thing to happen so far occurred last night (New Years Eve) when I left a small bottle of champagne outside in the snow to chill it for midnight GMT. When I went out to fetch it though, I found it had disappeared with a set of fox prints leading up to and then away from it! Tonight at dinner the fox (“Zorro” in Spanish) came by the dining room looking for food (the IRAM staff treat them as pets and feed them often) though I reckon it was after more of my champagne. (Pictures to follow soon – I forgot my USB cable).
Since tonight was the last night we were scheduled for the mergers, we’ll have to reapply to come back later on this year! Tomorrow we shift projects to the Blue Ellipticals thought the forecast isn’t good so we’ll probably be seeing more of IRAM soon. Great start to 2009! (Next time I’m here I’m bringing a foxhound).
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Update: Pictures of the Fox, and snow on the dish:
Happy New Year
New Year marked the start of night two of our observing run. We finished observing yesterday at just after midday – radio astronomers laugh at both sun and, in our case, cloud. The result’s weren’t great; we lost more than five hours completely to strong winds which might have been dangerous to the telescope, and the rest of the data was pretty shoddy. Not only that, but Daniel beat me soundly at first chess and then billiards.Tonight isn’t looking very good either – we’re struggling even to point the telescope at extremely bright objects – but I did at least join in with the Spanish tradition of eating twelve grapes in twelve seconds to welcome in the New Year. Let’s hope it brings us some luck.
A false start…
We’re off. Our first candidate galaxy is this rather nice system 
Before we can get to that though, we have to point the telescope at a well-known, bright source – usually an otherwise innocent and boring radio galaxy – to calibrate the system and to focus. Which is where our problems have started; the weather isn’t great (or is at least changeable) and we had trouble getting a decent focus. We ended up rotating the telescope by about 100 degrees to find a brighter standard source, and managed to focus. By the time we moved back to our galaxy, though, the wind had picked up and the telescope operator – whose concern is for the safety of the dish rather than for our observations – decided we had to stop.So we’re 90 minutes or so in, and have six minutes of useful data. It feels like it’s going to be one of those nights…
Hola from Pico Veleta
I’m sitting in what looks like a perfectly normal hotel room; bed, tv, shower and desk (with every astronomer’s essential needs – an internet connection – catered for). It’s only by opening the curtains that you might realise I’m somewhere special. Skiers are flying past in one direction, while in the other direction others are being pulled up the slopes on a chairlift. Down below the city of Granada stretches out in the foothills of the Sierra Nevada mountains. We’d worked our way through the throng earlier, looking incongruous pulling suitcases behind us among the multicoloured sportswear, on our way to use the IRAM SEO Services UK millimeter radio telescope. We’ll be looking at merging galaxies selected from the Galaxy Zoo catalogues, and then at some of the nearest blue ellipticals.IRAM is a hard working telescope – being a radio telescope we can observe right round the clock – and we’ve been allocated a shift from midnight to 12.30pm starting tonight. The skies are – at the minute – clear and so the lunch we just shared with the day crew and other observers has become dinner, and I’m off to bed. Daniel and I will be blogging throughout the run, so please do keep us company – we’ll have plenty of time to answer questions once things start running smoothly.
Getting Observing Time
If you followed the many interesting discoveries made by us all as part of the Galaxy Zoo team on the forum and the blog, you’ll have noticed that one of the most important things in astrophysics research is getting data. Unlike most other scientists, astrophysicists can’t just take a tiny galaxy into the lab and watch it evolve, perhaps feeding its (now tiny) supermassive black hole to see what happens. All we can do is observe the universe around us, and to do that, we need telescopes.
Observations are a bit like experiments. They are often designed to answer a very specific question. To take an example from Galaxy Zoo: when we first spotted the Voorwerp, and convinced ourselves that it’s real, rather than an artifact on the camera, we had to find out how far away it is by measuring its redshift and perhaps learn something about what it’s made of. To do this, we needed a spectrum, so we went about looking to obtain one. Normally, to get “time” on a telescope takes a lot of effort and waiting; in this case, we managed to convince some colleagues that the Voorwerp was exciting enough for them to forego some of their allocated time to take a peek at it.
So how do you normally get observing time? I’ll take the example of the XMM-Newton time we just got. Depending on the facility, the administrators will issue a “call for proposals” in certain intervals asking for proposals for observations. For most ground-based facilities, this will be twice a year. For many space missions, since they are harder to schedule, this may be only once a year, or even rarer. This “call” outlines the instruments of the facility, what kinds of proposals for time they will accept (lots of large proposals, no large proposals, etc.) and any technical issues proposers should be aware of.
We wanted to learn more about what physics the Voorwerp can teach us and one of the biggest questions about it is whether the supermassive black hole in IC 2497 (the spiral galaxy next to it) has really shut down, or if it is still a quasar and feeding. All indications so far are pointing towards a shutdown, but perhaps the quasar is really hidden by plenty of material in the way. So, we would like to use the X-ray vision of XMM-Newton, a 3.8 ton, bus-sized X-ray space telescope operated by the European Space Agency to take a look and see if any X-rays still get to us. Even if the quasar was highly obscured, some of the X-rays might still get through. It’s a bit like going to the doctor’s – we need an X-ray to diagnose what’s going on.
We thus sat down and wrote a proposal. The call for proposals outlines quite strictly how many pages, figures etc. you can use and what kind of information on the proposed observations they want. A proposal for observations generally consists of two parts: 1) a science justification and 2) a technical justification.
The science justification is an explanation of what you want to observe and what kind of physics you will learn from the observations. In our case, we described the discovery of the Voorwerp, how much excitement it generated with you all, and what we know about it so far. We then outlined precisely what we will learn with XMM-Newton data.
The technical justification following the science case is an explanation of why your proposed observations are really feasible. Will you really gather enough data to answer your question? Will the observations damage the telescope? Are there any other constraints? Are you (gasp!) asking for more time than you really need? All these are important. Even if you have the greatest science case, if you can’t make a convincing argument that your observations will work, you still won’t get time.
Preparing such a proposal is a lot of work. After submission (hopefully before the deadline!), the facility sends out the proposals to an anonymous panel for review (a bit like for scientific papers). This panel reads the proposals and meets somewhere for discussion. They assign each proposal a grade and so rank them. The telescope planners then approve proposals from the top until they’ve filled the available time. The remaining proposals are then rejected. This is actually the fate of most proposals. Popular facilities like XMM-Newton, Hubble or the VLTs are highly “oversubscribed”, regularly receiving five or even ten times more requests for observing time than they can give.
Astrophysicists thus spend a lot of time writing proposals in the knowledge that they’re unlikely to be accepted. Getting time is very precious and of course, every observation is an opportunity for discovery. As you can see from this description, it also takes a long time between applying for time, getting the time, and the actual observations. It’s fairly common to wait for your data for a year.
Luckily, so far Galaxy Zoo has been very successful with getting observing time….
4 Calling birds, 3 French hens, 2 Turtle Doves and 37,000 seconds of XMM-Newton Time
Just in time for the holidays, we got a little early Christmas present in our inbox. Applying for telescope time can be a large part of an astronomer’s work, and because astronomers often apply for far more time than is available, many worthy proposals don’t make it. If you’ve been following the blog, you know that in the past we were successful in getting time on facilities like Hubble, WIYN and IRAM to work on discoveries made by you all. So we were very happy to receive an email from esa confirming that we were awarded 37,000 seconds (or, in X-ray astronomer lingo 37 ksec) on the XMM-Newton space telescope.
Artist impression of XMM-Newton in space (from esa)
The title of our accepted program is: “How fast can an AGN shut down? XMM-Newton observation of IC 2497“. It’s with the piercing X-ray eyes of XMM–Newton that we hope to better understand the mystery Voorwerp. Just like at your doctor’s, X-rays in space can be a great tool to diagnose what’s going, in this case a supermassive black hole. One of the Big Questions about the Voorwerp is whether the quasar in IC 2497 (the spiral galaxy next to it) has really shut down, or whether it’s just hidden (obscured) by lots of gas and dust around it. With the help of this X-ray observation, we will hopefully be able to tell the difference between these two scenarios. When supermassive black holes feed, they emit radiation at many wavelengths, but X-rays are the most reliable measure of just how much material they really are gobbling up. The interpretation isn’t necessarily straightforward, as even X-rays can be blocked if there’s enough material in the way, but in 37 ksec (or just over 10 hours) with XMM-Newton, we should be able to tell the difference and make another step towards understanding what the Voorwerp really tells us about astrophysics.
So when do we get the data? As with all observations, it might take a while. The next cycle of observations lasts from May 2009 to April 2010…
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Update: A nice artist’s impression by Adrianus V from the forum :
