most citedThe transitional gap transient AT 2018hso: new insights on the luminous red nova phenomenon

52 citations · 123 across the 4 of their papers we have counts for

collaborators

6 papers

astro-ph.IM2020

White Paper on MAAT@GTC

Francisco Prada, Robert Content, Ariel Goobar +41

MAAT is proposed as a visitor mirror-slicer optical system that will allow the OSIRIS spectrograph on the 10.4-m Gran telescopio CANARIAS (GTC) the capability to perform Integral F…

astro-ph.HE201938 cited

GRB171010A / SN2017htp: a GRB-SN at z=0.33

A. Melandri, D. B. Malesani, L. Izzo +41

The number of supernovae known to be connected with long-duration gamma-ray bursts is increasing and the link between these events is no longer exclusively found at low redshift ($…

astro-ph.HE201952 cited

The transitional gap transient AT 2018hso: new insights on the luminous red nova phenomenon

Y-Z. Cai, A. Pastorello, M. Fraser +20

Aims: AT 2018hso is a new transient showing transitional properties between those of LRNe and the class of intermediate luminosity red transients (ILRTs) similar to SN 2008S. Throu…

astro-ph.HE2019

Constraining the observer angle of the kilonova AT2017gfo associated with GW170817: Implications for the Hubble constant

S. Dhawan, M. Bulla, A. Goobar +2

There is a strong degeneracy between the luminosity distance () and the observer viewing angle (; hereafter viewing angle) of the gravitational wave (GW) source w…

astro-ph.HE2019

The long-lived Type IIn SN 2015da: Infrared echoes and strong interaction within an extended massive shell

L. Tartaglia, A. Pastorello, J. Sollerman +41

In this paper we report the results of the first four years of spectroscopic and photometric monitoring of the Type IIn supernova SN 2015da (also known as PSN J13522411+39412…

astro-ph.SR201933 cited

The Evolution of Luminous Red Nova AT 2017jfs in NGC 4470

A. Pastorello, T. -W. Chen, Y. -Z. Cai +43

We present the results of our photometric and spectroscopic follow-up of the intermediate-luminosity optical transient AT 2017jfs. At peak, the object reaches an absolute magnitude…