GZ Quench: Classification Complete – Now the Real Fun Begins!
Congratulations all! We’ve completed Phase 1 of Galaxy Zoo Quench! Over 1600 people lent us their time and pattern-recognition skills to complete the needed 120,000 classifications. Thank you!
Now is when GZ Quench gets really fun, interesting, and totally different from past projects. We’re not stopping with classifications; we’re helping our volunteers to go all the way… from soup to nuts, as some like to say.
Phase 2 begins today and will run for the next few weeks*, with our science team supporting you, our esteemed Zooniverse volunteers, in the data analysis and discussion.
We’ll be using the results from our classifications of the 3002 post-quenched galaxies + 3002 control galaxies to address the following questions: What causes the star formation in these galaxies to be quenched? What role do galaxy mergers play in galaxy evolution? Join us in exploring these questions, being a part of the scientific process, and contributing to our understanding of this dynamic phase of galaxy evolution!
Luckily, we have great tools to help make this phase accessible to anyone, no matter your background.
- Quenchtalk.galaxyzoo.org – our discussion forum within which there are already really interesting and exciting conversations happening between Zooites and the science team. This forum allows us to share knowledge, pursue interesting results, collaboratively make sense of interesting plots, and determine which results to include in our article.
- Tools.zooniverse.org – our online data visualization environment, which helps you play with the data and look for trends. Click here for the blog post and to watch the GZ google hangout describing Tools and the Quench Tools tutorial.
- Authorea.com – the online article writing platform we’ll be using to collaboratively write the GZ Quench article, to be submitted to a professional journal. This is the same online environment that a group of over 100 CERN physicists are using to write their articles.
We can’t stress enough that you do not need prior background or knowledge to take part in this next phase. Each of you brings useful skills to the project – asking questions, communication, critical thinking, organization, leadership, consensus building, intuition, etc. Through Quench Talk, we’ll help you apply those skills in this context, and enable you to get your feet wet experiencing the full process of science.
Have questions about the project? Ask us on Twitter (@galaxyzoo), Facebook, or within Quench Talk.
*Science timelines often subject to a factor of two uncertainty. We’ll do our best to keep on track, at the same time expecting the unexpected (all part of the fun of doing science!).
Using Galaxy Zoo Classifications – a Casjobs Example
As Kyle posted yesterday, you can now download detailed classifications from Galaxy Zoo 2 for more than 300,000 galaxies via the Sloan Digital Sky Survey’s “CasJobs” – which is a flexible SQL-based interface to the databases. I thought it might be helpful to provide some example queries to the data base for selecting various samples from Galaxy Zoo.
This example will download what we call a volume limited sample of Galaxy Zoo 2. Basically what this means is that we attempt to select all galaxies down to a fixed brightness in a fixed volume of space. This avoids biases which can be introduced because we can see brighter galaxies at larger distances in a apparent brightness limited sample like Galaxy Zoo (which is complete to an r-band magnitude of 17 mag if anyone wants the gory details).
So here it is. To use this you need to go to CasJobs (make sure it’s the SDSS-III CasJobs and not the one for SDSS-I and SDSS-II which is a separate page and only includes SDSS data up to Data Release 7), sign up for a (free) account, and paste these code bits into the “Query” tab. I’ve included comments in the code which explain what each bit does.
-- Select a volume limited sample from the Galaxy Zoo 2 data set (which is complete to r=17 mag). -- Also calculates an estimate of the stellar mass based on the g-r colours. -- Uses DR7 photometry for easier cross matching with the GZ2 sample which was selected from DR7. -- This bit of code tells casjobs what columns to download from what tables. -- It also renames the columns to be more user friendly and does some maths -- to calculate absolute magnitudes and stellar masses. -- For absolute magnitudes we use M = m - 5logcz - 15 + 5logh, with h=0.7. -- For stellar masses we use the Zibetti et al. (2009) estimate of -- M/L = -0.963+1.032*(g-i) for L in the i-band, -- and then convert to magnitude using a solar absolute magnitude of 4.52. select g.dr7objid, g.ra, g.dec, g.total_classifications as Nclass, g.t01_smooth_or_features_a01_smooth_debiased as psmooth, g.t01_smooth_or_features_a02_features_or_disk_debiased as pfeatures, g.t01_smooth_or_features_a03_star_or_artifact_debiased as pstar, s.z as redshift, s.dered_u as u, s.dered_g as g, s.dered_r as r, s.dered_i as i, s.dered_z as z, s.petromag_r, s.petromag_r - 5*log10(3e5*s.z) - 15.0 - 0.7745 as rAbs, s.dered_u-s.dered_r as ur, s.dered_g-s.dered_r as gr, (4.52-(s.petromag_i- 5*log10(3e5*s.z) - 15.0 - 0.7745))/2.5 + (-0.963 +1.032*(s.dered_g-s.dered_i)) as Mstar -- This tells casjobs which tables to select from. from DR10.zoo2MainSpecz g, DR7.SpecPhotoAll s -- This tells casjobs how to match the entries in the two tables where g.dr7objid = s.objid and -- This is the volume limit selection of 0.01<z<0.06 and Mr < -20.15 s.z < 0.06 and s.z > 0.01 and (s.petromag_r - 5*log10(3e5*s.z) - 15 - 0.7745) < -20.15 --This tells casjobs to put the output into a file in your MyDB called gz2volumelimit into MyDB.gz2volumelimit
Once you have this file in your MyDB, you can go into it and make plots right in the browser. Click on the file name, then the “plot” tab, and then pick what to plot. Colour-magnitude diagrams are interesting – to make one, you would plot “rabs” on the X-axis and “ur” (or “gr”) on the yaxis. There will be some extreme outliers in the colour, so put in limits (for u-r a range of 1-3 will work well). The resulting plot (which you will have to wait a couple of minutes to be able to download) should look something like this:
Or if you want to explore the GZ classifications, how about plotting “psmooth” (which is approximately the fraction of people viewing a galaxy who thought it was smooth) against the colour.
That plot would look something like this:
Which reveals the well known relationship between colour and morphology – that redder galaxies are much more likely to be ellipticals (or “smooth” in the GZ2 language) than blue ones.
You can learn more about SQL and the many things you could do with CasJobs at the Help Page (and then come back and tell me how simple my query example was!).
This example only downloads the very first answer from the GZ2 classification tree – there’s obviously a lot more in there to explore.
(Note that at the time of posting the DR10 server seemed to be struggling – perhaps over demand. I’m sure it will be fixed soon and this will then work.)
SDSS Data Release 10 and Galaxy Zoo 2
Since the original launch of the Sloan Digital Sky Survey (SDSS) in 2000, the data from the project has been released to the public on a timescale of every year or two. These Data Releases include both new observations from the telescope, as well as refinements to old data based on improving the processing and reduction routines.
Today, Sloan announced that Data Release 10 (DR10) is now available to both the general astronomy community and to the public. It contains the first release of spectra from the APOGEE experiment, which has been observing tens of thousands of red giant stars in the Milky Way. It also includes new data from BOSS, which has been measuring redshifts for distant galaxies in order to measure cosmological parameters and study structure formation.
The original data from Galaxy Zoo was included in the SDSS Data Release 8. That’s quite important for a couple of reasons. It makes it much easier for scientists to use the GZ data, since SDSS uses this as the input for their own database, called CasJobs. This database enables matching of morphologies to other properties of the galaxies that SDSS measures, such as color or size. It also provides one of the main means of access to the data for people who aren’t members of the Galaxy Zoo team. Finally, it’s a validation that your GZ classifications have become a core data product of the survey, and something which is worth preserving and sharing as widely as possible.
In DR10, we’re happy to announce that data from Galaxy Zoo 2 is available for the first time. The reduction and description of the data is covered in a recent paper, which received a very favorable referee report a couple of weeks ago and will be resubmitted soon. We’ll share the paper as soon as it’s been formally accepted. The GZ2 data will also be hosted on our own site within Galaxy Zoo in the near future.
Please check out DR10 if you’re interested in peeking at the GZ2 data – do acknowledge both Willett et al. (GZ2) and Ahn et al. (DR10) if you end up using it, though. Congratulations to the SDSS team on this new release!
Next GZ (Tools!) Hangout: Wednesday 24th July, 20:30 GMT
With the Quench project well underway and the start of the next phase of the project around the corner, it’s time for another hangout — this time with a focus on using the new Zoo Tools data analysis suite to work with Quench data!
We’ll start at 15:30 CDT (Chicago), which is 13:30 PDT, 16:30 EDT, 20:30 GMT, 21:30 BST, 22:30 CET, and 23:30 CAT. That’s getting a bit late for Europe and Africa, but if you can’t make the hangout on the day, don’t worry, we’ll post the recording of it as soon as possible.
Have questions? Post them here or tweet at us (@galaxyzoo). Just before the hangout starts, we’ll embed the video here so you can watch from the blog. And feel free to try out tools.zooniverse.org (and check out the Zooniverse blog post about it) beforehand!
The best way to send us a comment during the live hangout is to tweet at us, but you can also leave a comment on this blog post, or on Google Plus, Facebook or YouTube, which we’ll also try to keep an eye on. See you soon!
Note: if you’d prefer a text-based tutorial, check out this Zooniverse blog post.
Zoo Tools: A New Way to Analyze, View and Share Data
Your Galaxy Zoo data can be explored using our new Zoo Tools site. It’s currently in beta (meaning it’s not perfect!) but if you’re interested in plotting and sharing data, you should give it a try.
Since the very first days of Galaxy Zoo, our projects have seen amazing contributions from volunteers who have gone beyond the main classification tasks. Many of these examples have led to scientific publications, including Hanny’s Voorwerp, the ‘green pea’ galaxies, and the circumbinary planet PH1b.
One common thread that runs through the many positive experiences we’ve had with the volunteers is the way in which they’ve interacted more deeply with the data. In Galaxy Zoo, much of this has been enabled by linking to the Sloan SkyServer website, where you can find huge amounts of additional information about galaxies on the site (redshift, spectra, magnitudes, etc). We’ve put in similar links on other projects now, linking to the Kepler database on Planet Hunters, or data on the location and water conditions in Seafloor Explorer.
The second part of this that we think is really important, however, is providing…
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Galaxy Zoo Quench: A New Kind of Citizen Science
Yesterday, we launched a new Galaxy Zoo side-project: Quench. Read all about it in this Zooniverse blog post:
A new ‘mini’ project went live yesterday called Galaxy Zoo Quench. This project involves new images of 6,004 galaxies drawn from the original Galaxy Zoo. As usual, everyone is invited to come and classify these galaxies, but this project has a twist that makes it special! We hope to take citizen science to the next level by providing the opportunity to take part in the entire scientific process – everything from classifying galaxies to analyzing results to collaborating with astronomers to writing a scientific article!
Galaxy Zoo Quench is examining a sample of galaxies that have recently and abruptly quenched their star formation. These galaxies are aptly named Post-Quenched Galaxies. They provide an ideal laboratory for studying galaxy evolution. So that’s exactly what we want to do: with the help of the Zooniverse community. We hope you’ll join us as we try out a new kind of citizen science project…
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Galaxy Zoo Quench – Experience the Full Scientific Process
Experience Science from Beginning to End! Classify, Analyze, Discuss, and Collaboatively Write an Article!
Galaxy Zoo and other Zooniverse projects have given thousands the opportunity to contribute to scientific research. It’s time to take the role of volunteers to the next level. For the next two months*, this new Galaxy Zoo Quench project provides the opportunity to take part in the ENTIRE scientific process – everything from classifying galaxies to analyzing results to collaborating with astronomers to writing a scientific article!
Galaxy Zoo Quench will examine a sample of galaxies that have recently and abruptly quenched their star formation. These galaxies are aptly named Post-Quenched Galaxies. They provide an ideal laboratory for studying how galaxies evolve from blue, star-forming spiral galaxies to red, non-star-forming elliptical galaxies. Using the more than a million galaxies in the Sloan Digital Sky Survey, we identified ~3000 post-quenched galaxies. By classifying these galaxies and analyzing the results, we will explore the mechanisms that quenched their star formation and investigate the role of post-quenched galaxies in galaxy evolution.

The entire process of classifying, analyzing, discussing, and writing the article will take place over an 8 week period*, beginning July 18th. After classifying the galaxies, volunteers will use the tools available within Zooniverse to plot the data and look for trends. Through reading articles and interaction in Talk, volunteers will gain background information. Throughout, they’ll discuss with the science team their interpretation of the results. At the end of the process, volunteers and the science team will collaboratively write a 4-page Astrophysical Journal article.

What causes the star formation in these galaxies to be quenched? How do interactions impact galaxy evolution? What is the fate of our Milky Way? Join us this Summer (or Winter if you’re below the equator!) in exploring these questions, being a part of the scientific process, and contributing to our understanding of this dynamic phase of galaxy evolution!

CLICK HERE TO PARTICIPATE!
We’ll be sharing more details about this project during the next Galaxy Zoo Hangout, on Monday, July 15th at 14:00 CST / 19:00 GMT / 20:00 BST. Have questions about the project? Post them here or tweet at us (@galaxyzoo). Just before the Hangout starts, we’ll embed the video here so you can watch from the blog.
The best way to send us a comment during the live Hangout is through twitter (@galaxyzoo). You can also leave a comment on this blog post, or on Google Plus, Facebook or YouTube. See you soon!
Update: here’s the hangout (and the mp3 version)!
*Note: science timelines often subject to a factor of two uncertainty. We’ll do our best to keep on track, at the same time expecting the unexpected (all part of the fun of doing science!).
Zooniverse Live Chat
This just in: join the Zooniverse (including Galaxy Zoo) for a live hangout tomorrow from Chicago!
A small team of scientists and developers from across the Zooniverse are gathered at Adler Planetarium in Chicago this week to pitch and work on ideas for advanced tools for some of your favorite Zooniverse projects. Our goal is to come up with some tools and experiences that will help the Zooniverse volunteers further explore, beyond the scope of the main classification interfaces, the rich datasets behind the projects in new and different ways. As part of the three days of hacking, there will be a live chat with representatives from Galaxy Zoo, Planet Hunters, Snapshot Serengeti, and Planet Four (as well as a special guest or two) tomorrow Thursday July 11th at 2pm CDT ( 3 pm EDT, 8 pm BST). We’ll also give you an inside peek into the US Zooniverse Headquarters on the floor of the Adler Planetarium where much of the coding and…
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Updates to Talk
The good news: the developers are currently hard at work migrating Talk to the latest version, which has many improvements over the old version. When the update is finished, the Talk home page will contain lots more information about each new post (including thumbnails!), the discussions should be easier to navigate, and the collections will be easier to navigate and manage — just for a start. We’ve been looking forward to this upgrade for a while, and once it’s completed it will make discussions of your discoveries even better.
The bad news: Talk will be down for a few hours while the upgrade actually takes place. And, as with any significant update that includes changing the way your favorite website appears on a page, it may take some getting used to. But hang in there and you’ll find your way around. Also, please feel free to ask questions, either here or on Talk itself. (Also also, thanks for bearing with us.)
The other good news: The main classification site isn’t affected at all — so you can still classify galaxies to your heart’s content, without interruption!
How to Translate Galaxy Zoo
Not too long ago we announced that Galaxy Zoo has gone open source – along with several other Zooniverse projects. Part of that announcement was that it is now possible for anyone to translate the Galaxy Zoo website into their own language and have that pulled back into the main site. We love translation at the Zooniverse! Using GitHub (our code repository) means we can open up the translation process to everyone.
I’ve been answering a lot of emails about how this process works so I thought I would outline a tutorial here on the blog. To get started go to: https://github.com/zooniverse/Galaxy-Zoo/tree/master/public/locales and download the .json file corresponding to your language. If there is not yet one there you have two options:
- Clone the app locally from GitHub and run the translate.rb file in root
- If step 1 doesn’t make any sense then contact rob@zooniverse.org and we can create the file for you.
These JSON files are tree structures of strings in “key”: “value” pairs that contain all the translatable text on Galaxy Zoo. You need to translate just the values , which are the parts after the colon (:) shown in bold in the example chunk of the file below.
{
“zooniverse”: {
“browser_check”: {
“wont_work”: “This site probably won’t work until you update your browser.”,
“recommended”: “We recommend using <a href=\”http://www.mozilla.org/firefox/\” target=\”_blank\”>Mozilla Firefox</a> or <a href=\”http://www.google.com/chrome\” target=\”_blank\”>Google Chrome</a>.”,
“ie”: “If you use <a href=\”http://www.microsoft.com/windows/internet-explorer/\” target=\”_blank\”>Microsoft Internet Explorer</a>, make sure you’re running the latest version.”,
“chrome_frame”: “If you can’t install the latest Internet Explorer, try <a href=\”http://google.com/chromeframe\” target=\”_blank\”>Chrome Frame</a>!”,
“dismiss”: “Dismiss”
},
…
You do not translate the parts before the colon as these are the keys that are used to identify each string. so in the example you do not translate “zooniverse”, “browser_check”, “won’t_work, “recommended”, “ie”, “chrome_frame” or “dismiss”. Here’s the Spanish version of the above segment of the file:
{
“zooniverse”: {
“browser_check”: {
“wont_work”: “Es probable que este sitio no funcione hasta que actualices tu navegador.”,
“recommended”: “Te recomendamos usar <a href=\”http://www.mozilla.org/firefox/\” target=\”_blank\”>Mozilla Firefox</a> o <a href=\”http://www.google.com/chrome\” target=\”_blank\”>Google Chrome</a>.”,
“ie”: “Si utilizas <a href=\”http://www.microsoft.com/windows/internet-explorer/\” target=\”_blank\”>Microsoft Internet Explorer</a>, asegúrate que estés usando la última versión.”,
“chrome_frame”: “Si no puedes instalar la última versión de Internet Explorer, intenta usar <a href=\”http://google.com/chromeframe\” target=\”_blank\”>Chrome Frame</a>!”,
“dismiss”: “Dismiss”
},
…
Note that any quotation marks need to be escaped i.e. ” becomes \” – these files have to be valid JSON and there is a handy online tool for validating this at http://jsonlint.com/ – here you can paste in the whole file and it will tell you where there are any formatting errors if you have any.
There is very little scope for doing language-specific formatting on the website. This means that if text is too long when it’s been translated it may run off the page or be cut-off on the screen. Because of this, you need to keep the translated strings to approximately the same length. If this causes issues let us know. To test out the translation and see how it looks, which you’re welcome to do ant any time, you can either email your current file to rob@zooniverse.org or run the Galaxy Zoo app locally by cloning it from GitHub (https://github.com/zooniverse/Galaxy-Zoo/).
We also have an email list for Zooniverse Translators. If you’d like to join it in order to ask questions of other translators and hear about other projects you might want to translate then email rob@zooniverse.org. If you are planning on doing a translation it would be worth joining the list to coordinate with other translators in your language.
NOTE: If you’re familiar with GitHub, you can clone the Galaxy Zoo repo, create a local JSON file for your language and just submit a Pull Request when you’re ready. You can find the translation-creator script here.
When your translation is complete will find find an astronomer somewhere in the world who speaks your language, in order to double-check (peer-review!) the new text and give feedback. This is done to ensure that the site is still conveying the original meaning and acts as a good error-checking mechanism.
Good luck with your translation, and thank you! Hopefully we can open up Galaxy Zoo to many more people around the world.







