Archive | June 2009

Finishing that paper II

The Galaxy Zoo AGN host galaxies paper is nearing the final draft stage.

Note to self: when converting a document from British to American spelling, do not just automatically replace all instances of `ise’ with `ize!’

Voorwerps everywhere

I’m delighted to announce that the fifth Galaxy Zoo paper – the one that discusses Hanny’s Voorwerp – has now been accepted for publication by Monthly Notices of the Royal Astronomical Society.

picture-1

It’s somewhat of a relief to say that, as it was way back in August of last year that we first submitted it. The referee was extremely thorough, catching a few stupid mistakes we’d made (as a good referee should) and in correcting these and responding to responses for clarification the paper grew from four pages to thirteen. The basic story is still the one that Bill and I outlined more than a year ago – we think we’re seeing the result of activity associated with the black hole in the nearby galaxy IC2497 which has now ceased.

Along the way, another team of astronomers have published a paper about their radio observations of the Voorwerp; I’ll blog later in the week about how we think the two sets of observations are compatible. Hopefully they’ll do the same, and we can have a discussion in public about what we do – and don’t – agree on. By coincidence, their paper is being published in the journal Astronomy & Astrophysics this week – and their image of the Voorwerp made the front cover of the printed edition. We’ll have an image of that for you as soon as anyone involved can find a printed edition – a rare thing in this internet age.

Update : Paper is now available here.

P.S. For those keeping score, our Voorwerp paper was the 5th to be submitted, but the 6th to be accepted.

Update: The pre-print is available on astro-ph now.

Questions about Cosmology?

A group of young cosmology researchers at the University of Portsmouth (where a number of Zoo people work) are trying to start a video podcast outreach project. The working title is “Our Universe” and the idea is that these would be short video podcasts, probably released on You Tube which will give some insight into how cosmologists/astronomers work as well as answer some basic questions about the science. I’ve seen a rough draft of the “pilot episode” and it’s quite fun.

One idea is that each episode would include short (ideally around 10 seconds) video or audio clips from members of the public asking questions of scientists. These can be questions about the science, or about their jobs, or whatever you want really. We were hoping that some Zooites reading this blog might be interested in helping out with this as a test run – and you might get to appear in one of the early episodes if it all works out. Be warned – if the clip is too long it’s much less likely to be useful. Short and to the point questions are what’s needed here.

So if you have a burning question to ask a cosmologist and you have the ability to make a short video (with a webcam for example) or audio clip (plus accompanying picture) of yourself asking this question that would be great. For now we’ll use the University of Portsmouth Web Shelf to share the files – if you upload something post a comment here with the URL and I’ll grab it (don’t worry it’ll expire a week after you upload it).

Thanks in advance for your help, Karen.

Finishing that paper…

When you start to write a paper for publication, you generally think that it will take a fortnight, at most. Naturally, that’s almost always a highly optimistic estimate and it can take months to get a paper into shape for submission to a journal. 

I’m currently working on the Galaxy Zoo paper dealing with the host galaxies of AGN (active galactic nuclei – accreting supermassive black holes). Your classifications from Zoo1 are making it possible for us to look at AGN host galaxies in a completely new light and, in particular, see how they’re different from galaxies whose black holes aren’t accreting at the moment. The diagrams and plots are done and the text is now mostly there (10,000 words and counting!), but some of the crucial sections are still very much in the draft stage.

I’ve circulated two earlier drafts with the team to get their comments and suggestions and I’ve mostly finished incorporating them into the text. However, as am writing up the part of the paper where I’m trying to explain what it all means, it’s becoming clear that there’s a lot that the morphologies that your classifications made possible are telling us that’s new and, to be honest, quite mystifying. 

That means that I will still have to do some more writing, thinking and discussing with experts on our team on various aspects, all of which of course take time. I started work on this paper in the autumn of 2008, and I’m still working on it.  So you can see that getting a scientific paper from an idea to something you can submit can take quite a long time, especially when you start finding things you didn’t expect. And of course, once the paper is finished and submitted to a journal, the process of peer-review begins, which in turn can take weeks, months, or even years.

Eleventh Galaxy Zoo paper submitted!

My colleagues and I are happy to say that the eleventh Galaxy Zoo paper has now been submitted to the journal Astronomy Education Review. The paper is called “Galaxy Zoo: Exploring the Motivations of Citizen Science Volunteers,” and the authors are myself, Georgia Bracey, Pamela, and Chris, Phil, Kevin, Alex, and Jan of the original Galaxy Zoo team. In addition to being the eleventh paper overall, it is also the first paper to study the Galaxy Zoo volunteer community – that is, you!

We are grateful for your collaboration with us even more than usual, because for this paper, you not only classified galaxies, but some of you agreed to give a half-hour of your time to participate in an instant message or phone interview.

As with all the other papers, this paper is being sent out by the journal’s editors to one or more anonymous “peer reviewers” – practicing education researchers who read the paper and recommend that the journal either accept or reject the paper, or (most commonly) request that the authors resubmit the paper after making some improvements. The process can sometimes go a few cycles of changing and resubmitting before the paper is finally accepted. This peer review process helps ensure that scientific studies meet quality standards as judged by the community.

You might have noticed that I haven’t talked about this research on the blog yet, as other team members have done with their research. I wish I could have shared more, but there was an important reason for saving all the explanation until after the paper was submitted. It is well-known in social science research that if the group being studied is aware of the study results, all sorts of unpredictable things can happen.

However, now that the study is over, we can and will gladly share our results. I’ll do that in a series of posts, first by giving a quick summary of what we found, then writing about the ethics of conducting research with people, then about ways to avoid bias in social science, and finally posting a detailed explanation of what we found in the study and what it means.

Now for the quick summary: based on our interviews, we identified 12 motivations that volunteers have given for participating in Galaxy Zoo – 12 reasons why people like you participate. These 12 reasons are:

Motivation (the category name we used in the paper) Description (what we said on the survey)
1. Contribute I am excited to contribute to original scientific research.
2. Learning I find the site and forums helpful in learning about astronomy.
3. Discovery I can look at galaxies that few people have seen before.
4. Community I can meet other people with similar interests.
5. Teaching I find Galaxy Zoo to be a useful resource for teaching other people.
6. Beauty I enjoy looking at the beautiful galaxy images.
7. Fun I had a lot of fun categorizing the galaxies.
8. Vastness I am amazed by the vast scale of the universe.
9. Helping I am happy to help.
10. Zoo I am interested in the Galaxy Zoo project.
11. Astronomy I am interested in astronomy.
12. Science I am interested in science.

We included these motivations in an online survey that many of you took (thanks!), and we are now analyzing the results of that survey to find out which motivations are common and which are rare.

Knowing your motivations for participating will be greatly helpful to us and to other citizen science projects by helping us understand you better. As we understand what appeals to you about Galaxy Zoo, we can design future Zoos to meet those needs and wants. So, this research is helping us create the best Zoos we can create for you.

I really enjoyed doing the interviews, and going through all your forum responses. It’s clear that many of you have many different reasons for being a part of Galaxy Zoo, and many different and eloquent ways of expressing your reasons. A few of the reasons that you gave as part of the forum discussion stuck out in my mind. One of you said “just knowing how small you are is something that’s really hard to explain.” Another said “getting to know, at least a little, some fans and professionals in the GalaxyZoo community.” Another of you said “I’m so proud to be with You, the whole project, to be a part of something bigger than wars or politics. Because science and discovering the truth are the only things that matter.” And there were many, many others.

It’s been a real pleasure getting to know so many of your reasons for being a part of this great enterprise we call Galaxy Zoo, and we’re looking forward to continuing to work with all of you!

Unveiling the Mass of Galaxies with Vera Rubin

This week I am attending a conference at Queen’s University in Kingston (Ontario, Canada) with I think the longest name I have ever seen. It’s called “A Celebration of Vera Rubin’s Life. Unveiling the Mass: Extracting an Interpreting Galaxy Masses.” I was very excited to attend this conference. Vera Rubin has always been a role model of mine (hard to avoid as a women studying galaxies) and as well as her the list of speakers includes many people who’s work I know and respect. It also has the advantage of being held in Kingston where a close friend (and fellow astronomer) from graduate school is now living with her very new baby.

This morning the introductory talks did not disappoint. We heard anecdotes from Vera Rubin about her work as a young scientist just trying to interpret the observations she was making on the rotation curves of galaxies (observations that provided the first strong evidence for dark matter in galaxies). She talked about a 1962 paper she did with students measuring the rotation curve of the Milky Way, and her regrets on not noticing that dark matter must have been present when she measured a similar “flat” rotation curve for the Andromeda galaxy 13 years later. She further impressed me by dating another anecdote (about discovering a galaxy in which the stars rotated in two directions) by the year her youngest child learned to walk (1961). Not only is Vera Rubin an incredibly successful and famous astronomer, but she managed to have 4 children (at least one of whom followed her into astronomy) during the period she did most of her famous work. Wow! I got to talk with her a little bit this morning at coffee, and she’s also a very nice person.

As well as enjoying the many talks by leaders in the field of galaxy evolution, I am presenting a poster on my work on dust reddening of Galaxy Zoo spirals which you have heard about several times before (eg. Blue Sky and Red Spirals, and from when I presented it at the 2009 European Week of Astronomy). This work has relevance to the masses of galaxies as dust is a significant source of error on estimates of the total mass of stars in a galaxy – at the simplest level dust hides the stars.

dustposter2

I was encouraged to share my poster on this blog, so if you wish to have a closer look at it you can download it (pdf). Of course this poster is aimed at explaining my work to other astronomers not to a general audience. If you have questions about it I encourage you to first look at my more general explanation of the work Blue Sky and Red Spirals and I am also happy to answer questions in the comments below.

One little details which is not explained in the poster is that the images of galaxies on both the right and left are not random. On the right I show edge-on spiral galaxies ordered from bluest (at the bottom) to reddest (at the top). On the left I show all face-on galaxies, also ordered in the same way. My definition of blue versus red comes from a measured difference in the brightness seen through 2 filters (in this case the SDSS g and z filters), so is not always obvious to the eye – also remember that it is the average colour of the whole galaxy, and some have significantly different colours in their centres to in the outskirts. However one of the interesting results coming from this work is that even though on average dust reddens galaxies as they become more inclined (as they go from face-on to edge-on) some face-on galaxies are much redder than some edge-on galaxies. This shows that while dust is important to the colour of a spiral galaxy it is clearly not the most important factor. This is very good news for those of us interested in red spirals as an evolutionary stage!

If anyone is in the Kingston area there will be a public lecture at 8pm tomorrow night given by Prof. Sandy Faber. It’s on the Queen’s Campus in the Biosciences Building, Room 1101. I include the poster below. Sandy Faber was a student of Vera Rubin’s and gave a very nice review talk this morning about her early work on dark matter during this time. I encourage you to attend if you are able – I think it will be a very nice public astronomy talk.

faber2009

Dust pathfinding with Galaxy Zoo

Now that spring classes are over, I’m catching up with lots of things. These include making color-composite images from our latest observations at the WIYN 3.5-meter telescope in Arizona done to follow up overlapping-galaxy pairs from the Forum. Here are three samples, showing how much more detail we can see with long exposures one the objects have been found from the SDSS data. In SDSS J215311.30-073533.5, the WIYN images show just the kind of thing we’re looking for – dust in spiral arms silhouetted against the light of the background galaxy. First here is the SDSS image, then the WIYN picture below it.

SDSS 2153-07 WIYN image

SDSS 2153-07 WIYN image


Read More…

Pictures from AAS

The AAS meeting just ended, and in a few minutes I’ll be giving Lucy from the Zoo Education Team a ride to Caltech, which is just down the street. Georgia sent me some photos from the three Galaxy Zoo education posters that we presented here.

Here is my poster, describing the irregular galaxies project:

Jordan's poster about the irregulars project

Here is Pamela’s poster describing the results of our survey into the reasons you participate in Galaxy Zoo:

Pamela's poster on your motivations

And, last but not least, here is Georgia’s poster describing our plans for future user testing of the Zoo 2 website:

Georgia's poster describing Zoo 2 user testing

It was a very successful meeting, and a lot of people came by the poster to ask questions or share their own results.

I’m headed back home at 11 PM tonight. It’s been a great trip, but I’m looking forward to going home!

Watch the AAS Citizen Science session now!

The International Year of Astronomy citizen science session at AAS is going on *right now*! Pamela’s team is live-streaming the session. You can see it at http://tinyurl.com/mmm5n4 .

Live from the AAS International Year of Astronomy Press Conference, part 2

11:08 AM: Pamela: “Galaxy Zoo takes long collaborator lists to a whole new level.” She’s showing a small sample of all the names from the Zoo 1 poster. Next, she’s talking about Zoo 2, and telling the story of 100 hours of astronomy challenge – 1 million galaxies in 100 hours. We thought this was an ambitious goal, but you did 2.6 million!

11:09 AM: “We now have a group of volunteers larger than the Italian Army.” Chris leaned over to me and says, “We need to update that, so we can figure out who we can invade now.” 🙂

11:11 AM: Now she’s revealing the research result – it’s the “Old Galaxies Spin in Sync” discovery that Raul Jimenez posted about yesterday. Read Raul’s post for more about that. I couldn’t reveal the result before now because there was a press embargo. Pamela is now emphasizing that star formation history is the *only* thing that matches up with galaxy spin direction.

11:13 AM: In addition to Raul’s spin result, Pamela is talking about the discoveries that are coming out of Daniel’s mergers research. She’s showing a picture of mergers divided up by your confidence of how likely it was that it was truly a merger. The biggest discovery from your merger classifications is that about 1-3% of galaxies are undergoing major mergers. Pamela: “this work would not have been possible without the participation of large numbers of Zooites.” Great job, everyone – you made this press conference possible!

11:16 AM: Now it’s question time from reporters – I’ll try to record the Zoo-related questions and answers.

11:19 AM: Question: “What’s the correlation between different Zoo members in terms of classification?” Answer: We were able to build separate samples based on agreement between Zooites, called “clean,” “cleanest,” and “superclean,” based on agreement between 60%, 80%, and 95% of Zooites.

11:24 AM: Question: “How do you account for human bias when classifying clockwise and counterclockwise spirals?” Answer: When we first noticed an extra amount of counterclockwise galaxies, we mirrored images of the galaxies. When you classified the mirrored images, you found the same excess of counterclockwise galaxies, showing that it’s a human bias rather than something strange about the universe. Now that we know about the bias, we correct for it.

That’s the end of the press conference. Later today, I’ll go back and add some links to these posts for more information. Do any of you have any questions about anything that was said here?