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The host galaxy of the short GRB 050709
Ana Nicuesa Guelbenzu, Sylvio Klose, Patricia Schady, Jochen Greiner, D.H. Hartmann, Leslie Hunt, Benjamin Magnelli, Nicola Masetti, Michal Michalowski, Eliana Palazzi, Andrea Rossi, Mark Wieringa, Bringfried Stecklum
Jun 30, 2021
The host of the short gamma-ray burst (GRB) 050709 is a morphologically disturbed low-luminous galaxy. At a redshift of z = 0.16, it belongs to one of the cosmologically nearest short-GRB hosts identified to date. Consequently...
The host galaxy of the short GRB 050709
Ana Nicuesa Guelbenzu, Sylvio Klose, Patricia Schady, Jochen Greiner, D.H. Hartmann, Leslie Hunt, Benjamin Magnelli, Nicola Masetti, Michal Michalowski, Eliana Palazzi, Andrea Rossi, Mark Wieringa, Bringfried Stecklum
Jun 30, 2021
The host of the short gamma-ray burst (GRB) 050709 is a morphologically disturbed low-luminous galaxy. At a redshift of z = 0.16, it belongs to one of the cosmologically nearest short-GRB hosts identified to date. Consequently...
A Comprehensive Study of the Radio Properties of Brightest Cluster Galaxies
M. T. Hogan, A. C. Edge, J. Hlavacek-Larrondo, K. J. B. Grainge, S. L. Hamer, E. K. Mahony, H. R. Russell, A. C. Fabian, B. R. McNamara, R. J. Wilman
Oct 21, 2015
We examine the radio properties of the Brightest Cluster Galaxies (BCGs) in a large sample of X-ray selected galaxy clusters comprising the Brightest Cluster Sample (BCS), the extended BCS (eBCS) and ROSAT-ESO Flux Limited X-ray...
A Comprehensive Study of the Radio Properties of Brightest Cluster Galaxies
M. T. Hogan, A. C. Edge, J. Hlavacek-Larrondo, K. J. B. Grainge, S. L. Hamer, E. K. Mahony, H. R. Russell, A. C. Fabian, B. R. McNamara, R. J. Wilman
Oct 21, 2015
We examine the radio properties of the Brightest Cluster Galaxies (BCGs) in a large sample of X-ray selected galaxy clusters comprising the Brightest Cluster Sample (BCS), the extended BCS (eBCS) and ROSAT-ESO Flux Limited X-ray...
Star formation efficiency along the radio jet in Centaurus A
Centaurus A is the most nearby powerful AGN, widely studied at all wavelengths. Molecular gas has been found in the halo at a distance of ~20 kpc from the galaxy centre, associated with HI shells. The molecular gas lies inside...
Large-amplitude late-time radio variability in GRB 151027B
J. Greiner, Jan Bolmer, M. H. Wieringa, Alexander van der Horst, D. Petry, S. Schulze, Fabian Knust, ger de Bruyn, T. Krühler, P. Wiseman, S. Klose, Corentin Delvaux, John F. Graham, D. A. Kann, A. Moin, Ana Nicuesa Guelbenzu, P. Schady, S. Schmidl, Tassilo Schweyer, Mohit Tanga, S. J. Tingay, Hendrik Van Eerten, K. Varela
Jun 01, 2018
Context: Deriving physical parameters from gamma-ray burst afterglow observations remains a challenge, even now, 20 years after the discovery of afterglows. The main reason for the lack of progress is that the peak of the...
Star formation efficiency along the radio jet in Centaurus A
Centaurus A is the most nearby powerful AGN, widely studied at all wavelengths. Molecular gas has been found in the halo at a distance of ~20 kpc from the galaxy centre, associated with HI shells. The molecular gas lies inside...
Large-amplitude late-time radio variability in GRB 151027B
J. Greiner, Jan Bolmer, M. H. Wieringa, Alexander van der Horst, D. Petry, S. Schulze, Fabian Knust, ger de Bruyn, T. Krühler, P. Wiseman, S. Klose, Corentin Delvaux, John F. Graham, D. A. Kann, A. Moin, Ana Nicuesa Guelbenzu, P. Schady, S. Schmidl, Tassilo Schweyer, Mohit Tanga, S. J. Tingay, Hendrik Van Eerten, K. Varela
Jun 01, 2018
Context: Deriving physical parameters from gamma-ray burst afterglow observations remains a challenge, even now, 20 years after the discovery of afterglows. The main reason for the lack of progress is that the peak of the...
Multi-messenger Observations of a Binary Neutron Star Merger
LIGO Scientific Collaboration, Virgo Collaboration, GBM Fermi, INTEGRAL, IceCube Collaboration, AstroSat Cadmium Zinc Telluride Imager Team, IPN Collaboration, The Insight-Hxmt Collaboration, ANTARES Collaboration, The Swift Collaboration, AGILE Team, The 1M2H Team, The Dark Energy Camera GW-EM Collaboration, the DES Collaboration, The DLT40 Collaboration, GRAWITA, GRAvitational Wave Inaf TeAm, The Fermi Large Area Telescope Collaboration, ATCA, Australia Telescope Compact Array, ASKAP, Australian SKA Pathfinder, Las Cumbres Observatory Group, OzGrav, DWF, AST3, CAASTRO Collaborations, The VINROUGE Collaboration, MASTER Collaboration, J-GEM, GROWTH, JAGWAR, NRAO Caltech-, TTU-NRAO, NuSTAR Collaborations, Pan-STARRS, The MAXI Team, TZAC Consortium, KU Collaboration, Nordic Optical Telescope, ePESSTO, GROND, Texas Tech University, SALT Group, TOROS, Transient Robotic Observatory of the South Collaboration, The BOOTES Collaboration, MWA, Murchison Widefield Array, The CALET Collaboration, IKI-GW Follow-up Collaboration, H. E. S. S. Collaboration, LOFAR Collaboration, LWA, Long Wavelength Array, HAWC Collaboration, The Pierre Auger Collaboration, ALMA Collaboration, Euro VLBI Team, Pi of the Sky Collaboration, The Chandra Team at McGill University, DFN, Desert Fireball Network, ATLAS, High Time Resolution Universe Survey, RIMAS, RATIR, SKA South Africa/MeerKAT, Hendrik Van Eerten
Oct 16, 2017
On 2017 August 17 a binary neutron star coalescence candidate (later designated GW170817) with merger time 12:41:04 UTC was observed through gravitational waves by the Advanced LIGO and Advanced Virgo detectors. The Fermi...
Multi-messenger Observations of a Binary Neutron Star Merger
LIGO Scientific Collaboration, Virgo Collaboration, GBM Fermi, INTEGRAL, IceCube Collaboration, AstroSat Cadmium Zinc Telluride Imager Team, IPN Collaboration, The Insight-Hxmt Collaboration, ANTARES Collaboration, The Swift Collaboration, AGILE Team, The 1M2H Team, The Dark Energy Camera GW-EM Collaboration, the DES Collaboration, The DLT40 Collaboration, GRAWITA, GRAvitational Wave Inaf TeAm, The Fermi Large Area Telescope Collaboration, ATCA, Australia Telescope Compact Array, ASKAP, Australian SKA Pathfinder, Las Cumbres Observatory Group, OzGrav, DWF, AST3, CAASTRO Collaborations, The VINROUGE Collaboration, MASTER Collaboration, J-GEM, GROWTH, JAGWAR, NRAO Caltech-, TTU-NRAO, NuSTAR Collaborations, Pan-STARRS, The MAXI Team, TZAC Consortium, KU Collaboration, Nordic Optical Telescope, ePESSTO, GROND, Texas Tech University, SALT Group, TOROS, Transient Robotic Observatory of the South Collaboration, The BOOTES Collaboration, MWA, Murchison Widefield Array, The CALET Collaboration, IKI-GW Follow-up Collaboration, H. E. S. S. Collaboration, LOFAR Collaboration, LWA, Long Wavelength Array, HAWC Collaboration, The Pierre Auger Collaboration, ALMA Collaboration, Euro VLBI Team, Pi of the Sky Collaboration, The Chandra Team at McGill University, DFN, Desert Fireball Network, ATLAS, High Time Resolution Universe Survey, RIMAS, RATIR, SKA South Africa/MeerKAT, Hendrik Van Eerten
Oct 16, 2017
On 2017 August 17 a binary neutron star coalescence candidate (later designated GW170817) with merger time 12:41:04 UTC was observed through gravitational waves by the Advanced LIGO and Advanced Virgo detectors. The Fermi...