TY - JOUR 
A1 - Inserra, Cosimo
AU - Nichol, Robert C.
AU - Scovacricchi, Dario
AU - Amiaux, Jerome
AU - Brescia, Massimo
AU - Burigana, Carlo
AU - Cappellaro, Enrico
AU - Carvalho, C. Sofia
AU - Cavuoti, Stefano
AU - Conforti, Vito
AU - Cuillandre, Jean Charles
AU - Silva, Antonio da
AU - Toledo Moreo, Rafael
T1 - Euclid: Superluminous supernovae in the Deep Survey
Y1 - 2018
SN - 0004-6361
UR - http://hdl.handle.net/10317/7763
AB - Context. In the last decade, astronomers have found a new type of supernova called superluminous supernovae (SLSNe) due to their high peak luminosity and long light-curves. These hydrogen-free explosions (SLSNe-I) can be seen to z ~ 4 and therefore, offer the possibility of probing the distant Universe.

Aims. We aim to investigate the possibility of detecting SLSNe-I using ESA’s Euclid satellite, scheduled for launch in 2020. In particular, we study the Euclid Deep Survey (EDS) which will provide a unique combination of area, depth and cadence over the mission.

Methods. We estimated the redshift distribution of Euclid SLSNe-I using the latest information on their rates and spectral energy distribution, as well as known Euclid instrument and survey parameters, including the cadence and depth of the EDS. To estimate the uncertainties, we calculated their distribution with two different set-ups, namely optimistic and pessimistic, adopting different star formation densities and rates. We also applied a standardization method to the peak magnitudes to create a simulated Hubble diagram to explore possible cosmological constraints.

Results. We show that Euclid should detect approximately 140 high-quality SLSNe-I to z ~ 3.5 over the first five years of the mission (with an additional 70 if we lower our photometric classification criteria). This sample could revolutionize the study of SLSNe-I at z > 1 and open up their use as probes of star-formation rates, galaxy populations, the interstellar and intergalactic medium. In addition, a sample of such SLSNe-I could improve constraints on a time-dependent dark energy equation-of-state, namely w(a), when combined with local SLSNe-I and the expected SN Ia sample from the Dark Energy Survey.

Conclusions. We show that Euclid will observe hundreds of SLSNe-I for free. These luminous transients will be in the Euclid data-stream and we should prepare now to identify them as they offer a new probe of the high-redshift Universe for both astrophysics and cosmology.
KW - Arquitectura y Tecnología de Computadoras
KW - Surveys
KW - Supernovae
KW - Cosmology
KW - 21 Astronomía y Astrofísica
LA - eng
PB - EDP Sciences
ER -