Archive | November 2009

Want to work with the Galaxy Zoo team?

The Zoo team is expanding once again, and we’re advertising jobs in Oxford and Chicago.

The Oxford job would be suitable for a postdoc who wants to do science with the Zoo, and get involved in the technical side of things. The job advert is here.

The two Chicago positions are for education researchers, based at the Adler planetarium. The adverts for these two positions are here.

Hope to be working with you soon…

Chris

Galaxy Zoo: Mergers – A personal perspective

Now that the launch of Galaxy Zoo: Understanding Cosmic Mergers has been completed, I wanted to give a personal perspective on this project.

For me, this project started twenty years ago  when I was in graduate school.    In my dissertation work, I  modeling the tidal features of interacting galaxies.  I wrote a Fortran code for doing some of this modeling work.   You would set up a run, and then wait hours to see the result.   If it didn’t match, you had to wait hours for the next attempt.

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The worst part about the modeling process was getting the “final” result.   Even if you got a close match, you never knew if you had actually found the best match.  It was always possible that a completely different set of parameters was the real solution, and you had just made a mistake.    Even with good fits, you couldn’t tell if you really had arrived at the ‘right’ solution.

Our understanding of galaxy collisions has been limited by the lack of dynamical models.  For example, we know that some galaxy collisions have very high star formation rates.   We also know that almost all extreme star burst galaxies (Ultra-luminous infrared galaxies) have undergone some type of collision.   Why isn’t this sort of reaction the inevitable result of a merger?   It seemed like the answer was always out of reach – unless we can understand the dynamics of lots of collisions.

The java applet developed for Mergers by Anthony Holincheck is the direct descendent of the old Fortran code.  Now you can run the same kind of simulations I ran for my dissertation in fractions of a second.    When Anthony and I first resurrected this code, we immediately tried using a Genetic Algorithm help us converge on the final solution.   It didn’t work.   We couldn’t reliably teach the computers how to recognize a good match.   We could run a few hundred thousand simulations per day, but we never knew if we got the right results.

The idea of using volunteers to help us happened a few years ago.   It was crazy and impractical to imagine volunteers helping out with a project like this.   Even so, a group of us proposed to do.  Of course, our proposal got shot down.  After all, there was no way that this type of thing would work.  How would you recruit such volunteers?

About a year later, I started talking with some of the team from Galaxy Zoo.    You – the volunteers of Galaxy Zoo-  have made the impossible possible.   With your help, we can create the models we need to understand the histories of hundreds of galaxy collisions.   These models will be more reliable than any a single scientist could create.    This result alone would incredibly important.   However, by carefully analyzing your inputs, we eventually hope to train the computers to do thousands of more models.   This kind of man/machine partnership is being planned for a number of future data projects, where computers need help learning how to be scientists.     We will never discover future Voorwerpen or new Peas without your help.   However, in return, we will also never make you do busy work that a machine can do.

Your efforts on the Zoo projects have created a new the way to do science.     This is nothing less than a transformation in how we look at data, analysis, and computing.

Of course, that’s just a personal perspective.

I just posted a new target for you to try.  We are going to be doing updates at 1600 GMT everyday. even Thanksgiving.  Of course, we will keep the old targets live for a week so you can go and revisit them.   This one is a repeat from some of the beta tests.   Getting a perfect model is hard, but getting close is easy.  We didn’t want to make things too difficult – at least for now.   Be assured, we will be kicking up a notch over the next days and weeks.

-John

Mergers Update

We have just changed the target on the Galaxy Zoo Mergers page (http://mergers.galaxyzoo.org).  The new system has a broken ring and a nearby companion.  It’s a very pretty system, and it seems to be a bit easier to model than the first one we posted.  For all the systems we are putting up as challenges, we do a quick run ourselves to see if we can find any solutions that might be on-track.   Although we found a few solutions right away, we don’t know if they are the best ones or if they are unique.  Of course, that’s why we need your help.

We are going to be updating the target daily.  Every day, we should will have a new cosmic collision for you to help us model.

If you can spend 10 minutes to quickly weed out the obvious bad ones on 20-30 screens, it would be a great help to us!   The more clicks we have, the better we constrain the collision.   Make sure you hit save when you are done looking at the images!  Although we automatically back up some clicks, we don’t want to lose any of your data.

Thanks for all you do.

– John Wallin, Computational Scientist/Astronomer

Galaxy Zoo: Understanding Cosmic Mergers

Starting at midnight 11/24, our new site ‘Galaxy Zoo: Understanding Cosmic Mergers’ went on-line as a new project in Galaxy Zoo. In Mergers, we are working to understand the cosmic collisions that lead to galaxy mergers. Every day we will have a new target galaxy that we need your help to model. Based on the basic input parameters that we provide, a Java applet running in your browser will simulate some possible collision scenarios. Computers don’t do a good job comparing simulations and real astronomical images, so we need your help to find out which simulations are the most similar to the real galaxy collision.

Working on Mergers will require some patience. Some of the collisions we are trying to model are rarer than others, so don’t get discouraged. In some cases, you will need to look at a few hundred images to get your first close match. Just remember, you aren’t looking for perfection. Just try to find a simulation that has some of the unusual and unique tidal features of the target galaxy. When you found something close, you might want to go further and “enhance” the image to make even a better match. The more data we have on these galactic collisions, the more we can narrow down the input parameters that caused these systems to form. You can be the most helpful by looking at a lot of images and then select the best of the best through the evaluate mode of the applet. This will happen automatically when you have selected eight possible merger images.

My graduate student Anthony Holincheck and I have been working on this project for a long time, and are very excited to see it see it launch today. We want to thank all the Zooites that participated in our beta test. Zooites rock! Of course, thanks also go out to Arfon, Chris, Lucy, Nancy, Geza, and Mark in their work in the development. Without all of your help, this project would not be possible. Our team will be adding more features in the coming weeks and months, so please stay tuned.

As I write this blog, we are T-5 hours before the full launch of our site. I cannot help but be humbled by the incredible dedication of the Zooites. With your help, we are going to model the dynamics of hundreds of galaxy collisions. This effort will help us connect the dynamics of galaxy collision to the star formation rates in galaxies. Thank you for your on-going support Galaxy Zoo!

– John Wallin – Computational Scientist/Astronomer

Leaving La Silla

Our pea hunting observing run is over and, as you will have gathered from previous posts, it has gone very well. We travelled back from La Silla to Santiago last night, for another brief stay at the ESO Guesthouse. Now I’m about to get on the plane back to the UK.

We are thrilled with how well the run has gone. I’ve done a rough analysis of the data already and we’ve already started drafting the paper presenting the results! I’ll do a more careful analysis once I get back to the office, but early indications are that we’ve got a nice collection of higher redshift objects that are very similar to the fascinating SDSS Peas that were discovered on the Galaxy Zoo forum, and an almost perfect technique for finding more! I’ll keep you posted as our work progresses.

Technical problems

The Chilean Pea hunt continues…

You may have noticed the Galaxy Zoo blog was down over the weekend. Well, it wasn’t the only one to be experiencing technical difficulties. On Sunday night we unfortunately lost four hours of observing time to technical gremlins. First we tried to use a new filter, which resulted in a nice 10 minute exposure of nothing. After a trip to the telescope to look around inside the instrument, the support staff worked out the problem: the filter was mislabelled on the computer. With that figured out, we changed to the correct filter and carried on – only to be stopped in our tracks again a couple of hours later by the whole telescope control system crashing! This time it took three hours of methodical troubleshooting to fix the problem, apparently some problem with a power lead. By then the night was almost over.

Read More…

She's an Astronomer: Julia Wilkinson

Julia Wilkinson (Jules)

Julia Wilkinson (Jules)

Julia Wilkinson (aka Jules) manages an Advice Centre in Manchester by day and is an amateur astronomer by night – out with her telescopes or binoculars if it’s a clear, starry night or inside with Galaxy Zoo or an astronomy book if it’s cloudy. Julia has a degree in Economics and has also studied music and has a house full of musical instruments that she fully intends to find time to play again one day! A more recent interest is astrophotography and one or two of her photos have appeared on the forum’s astrophotography thread. Enticed into astronomy having grown up with the Apollo Moon programme she has always regretted not studying sciences at school but spurred on by her involvement in Galaxy Zoo she now studies science and particularly astronomy with the Open University.

Read More…

Peas please me

Well, at the start of the night we were a bit nervous that none of our objects would turn out to be Peas. Fortunately, by the end of the night our quick looks at the data indicate that four of the seven i-Pea candidates that we managed to observe are emission line objects at the redshift we expected our selection to give, i.e. they are Peas! That’s about as good a success rate as we dared hope for.

The night hasn’t been without its difficulties. The seeing (how blurry the atmosphere makes our images) wasn’t great for most of the night, and it has turned out to be hard to actually find our targets because they are so faint. Those issues combined meant that we didn’t get through as many candidates as we hoped for, but we are still happy with the collection we got.

Right now, time for a quick breakfast then some sleep before trying to net some more Peas tomorrow night.

Here we go…

The continuing adventures of the Pea hunting trip to Chile

We’ve spent the afternoon finalising our target selection, preparing our observing strategy, and taking calibrations. The sun has now set and we’re already pointing in the right direction for our first target. In a few minutes time we will start our observations. We begin with a standard star, which will be used to calibrate the spectra of our main targets. The we are on to our first Pea candidate.

The SDSS Peas that Carrie studied were green in the SDSS colour images because they were bright in the r-band, actually the red region of the visible spectrum. On this occasion we are looking for similar object that are a bit further away, so we expect them to be very bright in the i-band (further into the red) ar the z-band (on the border between red and the near infrared). Tonight we are observing the i-bright objects, and hopefully we will get through about a dozen of them. The weather looks good, so fingers crossed.

Anyway, better concentrate on the observing.

On the mountain

The continuing adventures of the Pea hunting trip to Chile

An hour’s flight from Santiago to La Serena, followed by a 2 hour drive, and we arrived at La Silla in time for a tasty lunch (notable lack of peas, though). We then had a meeting with our support astronomer to check our plans for the upcoming observing run and make sure we had filled in all the necessary forms. He also kindly gave us a tour of the three biggest telescopes, including the NTT which we will be using. I’ve been here a couple of times before, but always using the NTT, so it was nice to see the other main telescopes, and get some great views from their dome catwalks.

View of the La Silla landscape from my room

View of the La Silla landscape from my room

The landscape around La Silla is red, arid and lumpy. Dry red soil strewn with small rocks, covering many hills of different sizes which appear to be piled on top of one another to form larger peaks. Although this is the edge of a desert, the landscape is dotted by small bushes, though many look more like collections of twigs than living plants.

La Silla observatory was set up in the early Sixties. Like other sites from the same era, such as La Palma, Kitt Peak and Siding Spring, it sports a collection of telescope enclosures of various shapes and sizes. Although the traditional dome is most common, it seems the discerning enclosure has an element of squareness, the degree of which varies with construction date like a fashion.

The telescopes here have apertures varying from half a metre to 3.6 metres. Although the atmospheric conditions at La Silla are very good, they weren’t considered exceptional enough to site the latest generation of 8 metre telescopes here. Instead ESO chose to develop a new observatory at Paranal. When you’re pushing technological and scientific limits, and spending the amount of money that requires, you need to be very careful choosing your site to maximise the quantity and quality of observations that are possible. As science has advanced and typical astronomical observations have become more challenging, the numerous small telescopes around the world are being used less and less. In fact, most of the domes on La Silla are either empty or contain telescopes that are no longer in routine service.

Visiting astronomers usually arrive on the mountain at least one night before their observations begin, to prepare final details and adjust to nocturnal working. We actually have two full days and nights here before we start using the telescope. That will give us plenty of time to review and refine our initial list of targets, although we will certainly still need to adapt our plans once we start taking data. We’ve now got our list of high priority targets organised, and tomorrow we’ll decide upon other interesting objects that it would be useful to observe, if everything else is going well.