Two peculiar fast transients in a strongly lensed host galaxy

DOI: 
10.1038/s41550-018-0405-4
Publication date: 
18/04/2018
Main author: 
Rodney S.A.
IAA authors: 
Molino, A.
Authors: 
Rodney S.A., Balestra I., Bradac M., Brammer G., Broadhurst T., Caminha G.B., Chirivì G., Diego J.M., Filippenko A.V., Foley R.J., Graur O., Grillo C., Hemmati S., Hjorth J., Hoag A., Jauzac M., Jha S.W., Kawamata R., Kelly P.L., McCully C., Mobasher B., Molino A., Oguri M., Richard J., Riess A.G., Rosati P., Schmidt K.B., Selsing J., Sharon K., Strolger L.-G., Suyu S.H., Treu T., Weiner B.J., Williams L.L.R., Zitrin A.
Journal: 
Nature Astronomy
Refereed: 
Yes
Publication type: 
Article
Volume: 
2
Pages: 
324-333
Abstract: 
A massive galaxy cluster can serve as a magnifying glass for distant stellar populations, as strong gravitational lensing magnifies background galaxies and exposes details that are otherwise undetectable. In time-domain astronomy, imaging programmes with a short cadence are able to detect rapidly evolving transients, previously unseen by surveys designed for slowly evolving supernovae. Here, we describe two unusual transient events discovered in a Hubble Space Telescope programme that combined these techniques with high-cadence imaging on a field with a strong-lensing galaxy cluster. These transients were faster and fainter than any supernovae, but substantially more luminous than a classical nova. We find that they can be explained as separate eruptions of a luminous blue variable star or a recurrent nova, or as an unrelated pair of stellar microlensing events. To distinguish between these hypotheses will require clarification of the cluster lens models, along with more high-cadence imaging of the field that could detect related transient episodes. This discovery suggests that the intersection of strong lensing with high-cadence transient surveys may be a fruitful path for future astrophysical transient studies. © 2018 The Author(s).
Database: 
SCOPUS
ADS
URL: 
https://ui.adsabs.harvard.edu/#abs/2018NatAs...2..324R/abstract
ADS Bibcode: 
2018NatAs...2..324R