Galaxy Zoo Supernovae - Header Image

Frequently Asked Questions

Q: Why can't computers do the job?

A: The automatic PTF will find us plenty of candidates, but that doesn't mean that everything it finds will be a supernova. Even the best camera and analysis system will make mistakes, and objects like asteroids will get in the way and confuse us. The best way to make the selection is to review candidates by eye — and that's where you come in.

Q: Why are the images so poor?

A: In order for us to be successful, we need a survey that can cover galaxies very quickly. Rather than spending time getting a pretty picture, PTF takes the minimum depth image required to capture a supernova and moves on. This trade off between image quality and the number of galaxies you can get through is just something we have to live with.

Q: What happens if I discover a supernova?

A: The first step is to get confirmation of the discovery. We're currently using a mix of old and new data, both of which are useful for science but only some of which might lead to a confirmable discovery. If we can get confirmation, we'll do that for you — the first step is to take any object that has been marked as a supernova and quickly show it to many other Zooites. Our team at the WHT will follow as many highly ranked candidates as they can — keep your fingers crossed for clear skies. If we're successful, we'll make sure that those that spotted it get the appropriate credit.

Q: Can I redo a classification?

A: It is not possible to redo a classification, as we want each one to be independent. Allowing classifications to be replaced would open up the possibility of classifiers discussing objects and changing their classifications to agree with one another. This would reduce our ability to understand the uncertainties on the classifications. However, don't worry about our final results: each candidate will have been looked at by many people, so on average the classification is likely to be correct, and occasional mistakes don't matter.

Q: What if I get the answer wrong?

A: We show multiple people the same images so that a mistake shouldn't matter too much. Just relax and give it your best shot.

Q: What happens after this run on the WHT is done?

We'll be taking down the site for a short period so we can review how things went and tweak a few knobs behind the scenes. The PTF is just getting started, and we hope to make Zooite classification a regular part of how they handle their data. In the meantime, you could always classify a few galaxies over here.

Q: How can we find out how the observers following up our discoveries are getting on?

Keep an eye on the Galaxy Zoo Blog for all the updates.

Q: Why can't I find out more about the galaxies we're looking at?

This is a first attempt at a Galaxy Zoo Supernova Hunt; we'll add more features as the site expands. We also need to be careful that you (and our friends at PTF) get the credit you deserve; publishing the full coordinates of a galaxy straight away would allow other astronomers to get ahead of us.

Q: Why are there are extra stars in the reference image that disappear entirely in the subtraction?

A: This is a fluke of the way the images are produced; the reference image is the result of adding several normal images together, so fainter objects will appear here. We take this into account when creating the subtraction image, so that only true changes show up.

Q: Why are you showing us old data? Shouldn't you use the latest?

A: The PTF telescope on Palomar Mountain has been affected by the recent forest fires in Southern California. The telescope is fine, but ash from the fires is hanging in the air and it's very important it doesn't get on the mirror. Instead, we're using our WHT time to do a systematic survey of older candidates, which will lead to us being able to work out the rate.

Q: What happens after this run on the WHT is done?

A: Other observers will be heading to other telescopes. Whenever there's a need for observations, we'll call on Galaxy Zoo volunteers to help.

Q:In MySN, why do some of the candidates selected for follow up have poor ratings? Some of them don't look like supernovae!

A:We use information from our friends at the Palomar Transient Factory to determine if a candidate has been selected for follow-up or not. As suggested in the name, the PTF team are interested not only in supernovae but in all transients, including asteroids and variable stars. Currently we can't tell if they followed it up because they thought is was a supernova, or because it was something else that looked interesting. This is something we hope to fix in the near future.

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