We present continued radio and X-ray follow-up observations of PTF11qcj, a highly energetic broad-lined Type Ic supernova (SN), with a radio peak luminosity comparable to that of the gamma-ray burst (GRB) associated SN 1998bw. The latest radio observations, carried out with the Karl G. Jansky Very Large Array, extend up to similar to 5 yr after the PTF11qcj optical discovery. The radio light curve shows a double-peak profile, possibly associated with density variations in the circumstellar medium (CSM), or with the presence of an off-axis GRB jet. Optical spectra of PTF11qcj taken during both peaks of the radio light curve do not show the broad Ha features typically expected from H-rich circumstellar interaction. Modeling of the second radi...
Over the last few years our understanding of local Type Ibc supernovae and their connection to long-...
Of the cosmological gamma-ray bursts, GRB 011121 has the lowest redshift, z = 0.36. More importantly...
The identification of type Ib/c supernovae as GRB progenitors is motivated by the association of GRB...
We present continued radio and X-ray follow-up observations of PTF11qcj, a highly energetic broad-li...
We present the discovery, classification, and extensive panchromatic (from radio to X-ray) follow-up...
We present the discovery, classification, and extensive panchromatic (from radio to X-ray) follow-up...
We present High Sensitivity Array and enhanced Multi-Element Remotely Linked Interferometer Network ...
Long duration gamma-ray bursts are a rare subclass of stripped-envelope core-collapse supernovae tha...
We present the discovery, classification, and extensive panchromatic (from radio to X-ray) follow-up...
We report extensive radio and X-ray observations of SN 2003bg, whose spectroscopic evolution shows a...
We present optical, radio, and X-ray observations of SN 2020bvc (=ASASSN-20bs, ZTF 20aalxlis), a nea...
We present the discovery and follow-up observations of a broad-line Type Ic supernova (SN), PTF 10bz...
Long duration γ-ray bursts are a rare subclass of stripped-envelope core-collapse supernovae (SNe) t...
Long duration γ-ray bursts are a rare subclass of stripped-envelope core-collapse supernovae (SNe) t...
Of the cosmological gamma-ray bursts, GRB 011121 has the lowest redshift, z = 0.36. More importantly...
Over the last few years our understanding of local Type Ibc supernovae and their connection to long-...
Of the cosmological gamma-ray bursts, GRB 011121 has the lowest redshift, z = 0.36. More importantly...
The identification of type Ib/c supernovae as GRB progenitors is motivated by the association of GRB...
We present continued radio and X-ray follow-up observations of PTF11qcj, a highly energetic broad-li...
We present the discovery, classification, and extensive panchromatic (from radio to X-ray) follow-up...
We present the discovery, classification, and extensive panchromatic (from radio to X-ray) follow-up...
We present High Sensitivity Array and enhanced Multi-Element Remotely Linked Interferometer Network ...
Long duration gamma-ray bursts are a rare subclass of stripped-envelope core-collapse supernovae tha...
We present the discovery, classification, and extensive panchromatic (from radio to X-ray) follow-up...
We report extensive radio and X-ray observations of SN 2003bg, whose spectroscopic evolution shows a...
We present optical, radio, and X-ray observations of SN 2020bvc (=ASASSN-20bs, ZTF 20aalxlis), a nea...
We present the discovery and follow-up observations of a broad-line Type Ic supernova (SN), PTF 10bz...
Long duration γ-ray bursts are a rare subclass of stripped-envelope core-collapse supernovae (SNe) t...
Long duration γ-ray bursts are a rare subclass of stripped-envelope core-collapse supernovae (SNe) t...
Of the cosmological gamma-ray bursts, GRB 011121 has the lowest redshift, z = 0.36. More importantly...
Over the last few years our understanding of local Type Ibc supernovae and their connection to long-...
Of the cosmological gamma-ray bursts, GRB 011121 has the lowest redshift, z = 0.36. More importantly...
The identification of type Ib/c supernovae as GRB progenitors is motivated by the association of GRB...