ABSTRACT A non-negligible fraction of binary neutron star mergers are expected to form
long-lived neutron star remnants, dramatically altering the multimessenger signatures of a …

We present the results from a multiyear radio campaign of the superluminous supernova
(SLSN) SN 2017ens, which yielded the earliest radio detection of an SLSN to date at the …

Context. SN 2020qlb (ZTF20abobpcb) is a hydrogen-poor superluminous supernova (SLSN-
I) that is among the most luminous (maximum M g=− 22.25 mag) and that has one of the …

We present new radio and optical data, including very-long-baseline interferometry, as well
as archival data analysis, for the luminous, decades-long radio transient FIRST J141918. 9+ …

Fast-rotating pulsars and magnetars have been suggested as the central engines of
superluminous supernovae (SLSNe) and fast radio bursts, and this scenario naturally …

Optical imaging polarimetry was conducted on the hydrogen poor superluminous supernova
2020znr during three phases after maximum light (≈+ 34 d,+ 288 d, and+ 289 d). After …

Abridged-Stars with ZAMS masses between 140 and $260 M_\odot $ are thought to explode
as pair-instability supernovae (PISNe). During their thermonuclear runaway, PISNe can …

Stars with zero-age main sequence masses between 140 and 260 M⊙ are thought to
explode as pair-instability supernovae (PISNe). During their thermonuclear runaway, PISNe …

Stars with zero-age main sequence masses between 140 and 260 M⊙ are thought to
explode as pair-instability supernovae (PISNe). During their thermonuclear runaway, PISNe …

Optical imaging polarimetry was conducted on the hydrogen poor superluminous supernova
SN2020znr during 3 phases after maximum light (≈+ 34 days,+ 288 days and+ 289 days) …