|All-Sky Automated Survey for Supernovae|
What is ASAS-SN?
The sky is big: even in the present day, only human eyes fully survey the sky for the transient, variable and violent events that are crucial probes of the nature and physics of our Universe. We plan to change that with our "All-Sky Automated Survey for Supernovae" (ASAS-SN or "Assassin") project, which will (eventually) automatically survey the entire visible sky every night down to about 17th magnitude, more than 10,000 times deeper than human eye. Such a project is guaranteed to result in many important discoveries, some of them potentially transformative to the field of astrophysics.
At this point we have
We started real-time reduction and analysis of "Brutus" four-telescope data in December 2013 and we are already making discoveries:
ASASSN-13dn (December 2013). SN Type II in SDSS J125258.03+322444.3. V=15.7, about 100 Mpc away. This is only our second non-Type Ia supernova, out of 15 discovered so far, and at absolute V magnitude of approx. -19.3 it is very luminous.
We started real-time reduction and analysis of "Brutus" two-telescope data in April 2013 and we had a number of exciting discoveries:
ASASSN-13cb: Extreme (delta V~9 mag) M-dwarf Flare (August 2013).
ASASSN-13an (SN 2013da): Our first supernova! (June 2013) SN Type Ia.
AGN Outburst and Dramatic Seyfert Type Change in NGC 2617; see also ATel #5103, #5059 and #5039 (April/May 2013)
Generally we are posting our real-time discoveries using ATel, so if you interested in being notified of our results, you should subscribe to that useful service, and also see our ASAS-SN Transients page.
We are not yet fully "All-Sky", but we are getting there, see below where our discoveries announced so far are located on the sky:
José Luis Prieto (Princeton);
At LCOGT: M. Dubberley, M. Elphick, S. Foale, E. Hawkins, D. Mullens, W. Rosing, R. Ross, Z. Walker;
Joseph Brimacombe (Coral Towers Observatory);
David Bersier (LJMU).
A crucial part of our project is the follow-up effort with bigger telescopes to get confirmation imaging (Brutus has 7.5" pixels) and spectroscopy. Sometimes a space-based telescope is needed: outburst of the AGN in NGC 2617 has been monitored by Swift. A number of people have kindly contributed their own telescope time to help us in our effort, which we most appreciate! Here are the names of our collaborators on ASAS-SN results annouced so far: S. Adams (Ohio State), A. Campillay (Las Campanas Observatory), C. Choi (Seoul National University), C. Contreras (Las Campanas Observatory), C. Copperwheat (LJMU), G. De Rosa (Ohio State), M. Dietrich (Ohio University), M. Fausnaugh (Ohio State), D. Grupe (Penn State), D. Gifford (University of Michigan), M. Giustini (XMM-Newton Science Operation Centre), C. Gonzalez (Las Campanas Observatory), A. Goulding (CfA), K. Hainline (Dartmouth), R. Hickox (Dartmouth), R. Hounsell (STScI), D. Howell (LCOGT), E. Hsiao (Las Campanas Observatory), M. Im (Seoul National University), S. Komossa (Max-Planck Institut fur Radioastronomie), M. Koss (IfA), P. Lira (U. Chile), K. Leighly (University of Oklahoma), S. Mathur (Ohio Sate), N. Morrell (LCO), A. Mosquera (Ohio State), D. Mudd (Ohio State), J. Nugent (University of Oklahoma), B. Peterson (Ohio State), M. Phillips (Carnegie Observatories), R. Pogge (Ohio State), J. Rich (Carnegie Observatories), D. Sand (Texas Tech University), S. Schmidt (Ohio State), A. Sheffield (Columbia), S. Starrfield (ASU), M. Wagner (LBTO), E. Woodward (U. Minnesota), S. Valenti (LCOGT), S. Villanueva (Ohio State), Y. Yoon (Seoul National University), Y. Zu (Pittsburgh).
So when you get an e-mail or a phone-call from us, asking to collaborate on a new exciting ASAS-SN target, we hope you will say "yes"!
Our team makes ASAS-SN a success, but we also need excellent hardware to aid us in our ultimate goal of studying real-time variability of the entire sky:
To achieve large field of view with a very stable and uniform point-spread-function (PSF) across the field, we use Nikon AF-S NIKKOR 400mm f/2.8G ED VR AF lenses. We had high expectations for these lenses and were not disappointed: we obtain very stable and sharp images for many nights in a row. This is crucial for the image subtraction method, which we employ to detect transients, to work best.
Since we are using relatively small telescopes (lenses), we cannnot afford to waste many photons. As our detectors we have selected ProLine PL230 CCD cameras from FLI, with back-iluminated E2V sensors, giving us high QE, low-noise and fast readout (and of course they are electrically cooled). To cover several thousand square degrees each night, we take many hundreds of images nightly, and we have been very happy with the reliability of our cameras.