I’m delighted to announce that after a very successful beta test period, our first non-astrophysical project, Solar Stormwatch has gone live. Our science team, led by Chris Davis, is standing by ready to receive the results of your hard work. As he explains on his post over at the SSW blog, the results are already intriguing and we’re hoping for much, much more.
I’ve been working closely with Zookeeper Geza recently, to figure out how to provide better support for those of you who are doing your own research in addition to classifying galaxies. (Stay tuned for more on that.) In addition to being the awesome, Geza has a wonderful analogy for what we are all working together to do. I’d like to share that analogy with you in story form. A few years ago, I joined a twice-weekly lunchtime basketball game with some of the science faculty at the Hopkins Gym.
Continue reading Citizen Basketball
This morning we made some major changes to the way you manage your account with Galaxy Zoo and the Zooniverse. Previously all account management (e.g. changing your email address) was done through the Galaxy Zoo site however the changes that we made this morning have moved those pages to the Zooniverse Home.
From the Zooniverse you can now manage your profile for both the projects (such as Galaxy Zoo) and also any of the Zooniverse forums. I’ve recorded a quick screencast demonstrating the changes here.
As part of the update today we also upgraded the Galaxy Zoo forum to the latest (and greatest) version of SMF. The changes we made today were made possible by the hard work of the whole Zooniverse developer team, in particular Jarod Luebbert and Pamela Gay – thanks for your help guys!
We hope you like the changes!
From Raul Jimenez, the lead author of this paper.
Dear galaxy zooers,
Our paper on the correlation of spins and past star formation was accepted today to the MNRAS. This was after a very positive and insightful referee report, which helped us make the paper stronger. next steps are to look for the effect in numerical simulations and increase the size of the observational sample. Because the above correlation is a very particular prediction of hierarchical galaxy formation, it raises the bar for alternative theories of galaxy formation to produce such effect.
Greetings. My name is Mansi Kasliwal and I am pursuing my PhD thesis at Caltech. The goal of my thesis is finding novel cosmic explosions too bright to be novae and too faint to be supernovae! The has churned out several candidates (even last night) and is counting on you all to discover some fun transients among them. Tonight, I am at the 10-m Keck telescope in Hawaii. I am using the “LRIS” spectrograph. This gigantic piece of glass is superb at thumb-printing transients. In less than 5 min, I can take a spectrum of a PTF transient and tell you what type of star blew up and what elements it was made of. The weather is predicted to be quite nice and it should be a lovely, long winter night as I’m snuggling in with my hot garcinia cambogia tea. Thank you all for joining the fun of discovering new cosmic explosions! Clear Skies and Mahalo.