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View article: True spin-orbit obliquities distribution: data-driven confirmation of no clustering of misaligned planets
True spin-orbit obliquities distribution: data-driven confirmation of no clustering of misaligned planets Open
Context. True spin-orbit obliquities Ψ offer valuable insights into the evolutionary history of exoplanetary systems. Previous studies have suggested that exoplanets tend to occupy either aligned or perpendicular orbits. However, recent re…
View article: The radio flare and multi-wavelength afterglow of the short GRB 231117A: energy injection from a violent shell collision
The radio flare and multi-wavelength afterglow of the short GRB 231117A: energy injection from a violent shell collision Open
We present the early radio detection and multi-wavelength modeling of the short gamma-ray burst (GRB) 231117A at redshift $z=0.257$. The Australia Telescope Compact Array automatically triggered a 9-hour observation of GRB 231117A at 5.5 a…
View article: SVOM GRB 250314A at z $\simeq$ 7.3: an exploding star in the era of reionization
SVOM GRB 250314A at z $\simeq$ 7.3: an exploding star in the era of reionization Open
Most long Gamma-ray bursts originate from a rare type of massive stellar explosion. Their afterglows, while rapidly fading, can be initially extremely luminous at optical/near-infrared wavelengths, making them detectable at large cosmologi…
View article: JWST reveals a supernova following a gamma-ray burst at z $\simeq$ 7.3
JWST reveals a supernova following a gamma-ray burst at z $\simeq$ 7.3 Open
The majority of energetic long-duration gamma-ray bursts (GRBs) are thought to arise from the collapse of massive stars, making them powerful tracers of star formation across cosmic time. Evidence for this origin comes from the presence of…
View article: From precursor to afterglow: The complex evolution of GRB 210312B
From precursor to afterglow: The complex evolution of GRB 210312B Open
Context. Long gamma-ray bursts (GRBs) are characterized by a brief gamma-ray flash followed by a longer-lasting multiwavelength afterglow. The basic mechanism is largely understood, and the early afterglow evolution often shows complex fea…
View article: From data extraction to data-driven dynamic modeling for cobots: A method using multi-objective optimization
From data extraction to data-driven dynamic modeling for cobots: A method using multi-objective optimization Open
View article: The brightest GRB ever detected: GRB 221009A as a highly luminous event at <i>z</i> = 0.151
The brightest GRB ever detected: GRB 221009A as a highly luminous event at <i>z</i> = 0.151 Open
Context. The extreme luminosity of gamma-ray bursts (GRBs) makes them powerful beacons, thus effective probes of the distant Universe. The most luminous bursts are typically detected at moderate and high redshift, where the volume for seei…
View article: Varying linear polarisation in the dust-free gamma-ray burst 210610B
Varying linear polarisation in the dust-free gamma-ray burst 210610B Open
Context. Long gamma-ray bursts (GRBs) are produced by the collapse of some very massive stars, that emit ultra-relativistic jets. When the jets collide with the interstellar medium they decelerate and generate the so-called afterglow emiss…
View article: The host of GRB 171205A in 3D -- A resolved multiwavelength study of a rare grand-design spiral GRB host
The host of GRB 171205A in 3D -- A resolved multiwavelength study of a rare grand-design spiral GRB host Open
Long GRB hosts at z<1 are usually low-mass, low metallicity star-forming galaxies. Here we present the until now most detailed, spatially resolved study of the host of GRB 171205A, a grand-design barred spiral galaxy at z=0.036. Our analys…
View article: Interactive simulations as a tool for logistics and maintenance of IFMIF-DONES
Interactive simulations as a tool for logistics and maintenance of IFMIF-DONES Open
View article: An efficient workflow for virtual reality simulation of maintenance tasks in IFMIF-DONES
An efficient workflow for virtual reality simulation of maintenance tasks in IFMIF-DONES Open
This work has been carried out within the framework of the EURO-fusion Consortium and has received funding from the Euratom research and training program under grant agreement No. 101052200. The views and opinions expressed herein do not n…
View article: Observing the inner parsec-scale region of candidate neutrino-emitting blazars
Observing the inner parsec-scale region of candidate neutrino-emitting blazars Open
Context. Many questions concerning the nature of astrophysical counterparts of high-energy neutrinos remain unanswered. There is increasing evidence of a connection between blazar jets and neutrino events, with the flare of the γ -ray blaz…
View article: The science case and challenges of space-borne sub-millimeter interferometry
The science case and challenges of space-borne sub-millimeter interferometry Open
View article: Unravelling the Innermost Jet Structure of OJ 287 with the First GMVA+ALMA Observations
Unravelling the Innermost Jet Structure of OJ 287 with the First GMVA+ALMA Observations Open
We present the first very-long-baseline interferometric (VLBI) observations of the blazar OJ287 carried out jointly with the Global Millimeter VLBI Array (GMVA) and the phased Atacama Large Millimeter/submillimeter Array (ALMA) at 3.5 mm o…
View article: An integrative methodology based on protein-protein interaction networks for identification and functional annotation of disease-relevant genes applied to channelopathies
An integrative methodology based on protein-protein interaction networks for identification and functional annotation of disease-relevant genes applied to channelopathies Open
View article: Top-quark physics at the CLIC electron-positron linear collider
Top-quark physics at the CLIC electron-positron linear collider Open
© 2019, The Author(s). The Compact Linear Collider (CLIC) is a proposed future high-luminosity linear electron-positron collider operating at three energy stages, with nominal centre-of-mass energies s = 380 GeV, 1.5 TeV, and 3 TeV. Its ai…
View article: Joint direct estimation of 3D geometry and 3D motion using spatio\n temporal gradients
Joint direct estimation of 3D geometry and 3D motion using spatio\n temporal gradients Open
Conventional image motion based structure from motion methods first compute\noptical flow, then solve for the 3D motion parameters based on the epipolar\nconstraint, and finally recover the 3D geometry of the scene. However, errors\nin opt…
View article: Low-mass dark matter search using ionization signals in XENON100
Low-mass dark matter search using ionization signals in XENON100 Open
We perform a low-mass dark matter search using an exposure of 30 kg$\\times$yr with the XENON100 detector. By dropping the requirement of a scintillation signal and using only the ionization signal to determine the interaction energy, we l…
View article: Search for displaced vertices arising from decays of new heavy particles in 7 TeV pp collisions at ATLAS
Search for displaced vertices arising from decays of new heavy particles in 7 TeV pp collisions at ATLAS Open
View article: Top physics at high-energy lepton colliders
Top physics at high-energy lepton colliders Open
A summary is presented of the workshop "top physics at linear colliders" that was held at IFIC Valencia from the 30th of June to the 3rd July 2015. We present an up-to-date status report of studies into the potential for top quark physics …
View article: A new jet reconstruction algorithm for lepton colliders
A new jet reconstruction algorithm for lepton colliders Open
In experiments at future lepton colliders at the energy frontier (ILC, CLIC), high-performance reconstruction of jets is crucial for precision measurements of the interactions and properties of the Higgs boson and top quark. We present a s…
View article: Physics reach of the XENON1T dark matter experiment
Physics reach of the XENON1T dark matter experiment Open
The XENON1T experiment is currently in the commissioning phase at the Laboratori Nazionali del Gran Sasso, Italy. In this article we study the experiment's expected sensitivity to the spin-independent WIMP-nucleon interaction cross section…
View article: Lowering the radioactivity of the photomultiplier tubes for the XENON1T dark matter experiment
Lowering the radioactivity of the photomultiplier tubes for the XENON1T dark matter experiment Open
The low-background, VUV-sensitive 3-inch diameter photomultiplier tube R11410 has been developed by Hamamatsu for dark matter direct detection experiments using liquid xenon as the target material. We present the results from the joint eff…
View article: A precise characterisation of the top quark electro-weak vertices at the ILC
A precise characterisation of the top quark electro-weak vertices at the ILC Open
\n Top quark production in the process $$e^+e^- \\rightarrow t\\bar{t}$$ at a future linear electron positron collider with polarised beams is a powerful tool to determine indirectly the scale of new physics. The presented study, based on …
View article: Search for Event Rate Modulation in XENON100 Electronic Recoil Data
Search for Event Rate Modulation in XENON100 Electronic Recoil Data Open
We have searched for periodic variations of the electronic recoil event rate in the (2-6) keV energy range recorded between February 2011 and March 2012 with the XENON100 detector, adding up to 224.6 live days in total. Following a detaile…
View article: A robust jet reconstruction algorithm for high-energy lepton colliders
A robust jet reconstruction algorithm for high-energy lepton colliders Open
View article: Exclusion of leptophilic dark matter models using XENON100 electronic recoil data
Exclusion of leptophilic dark matter models using XENON100 electronic recoil data Open
Limiting unknows in the dark side Our knowledge of the inventory of stuff that makes up our universe amounts to a humbling 5%. The rest consists of either dark energy (~70%) or dark matter (~25%). Using atom interferometry, Hamilton et al.…
View article: A precise characterisation of the top quark electro-weak vertices at the ILC
A precise characterisation of the top quark electro-weak vertices at the ILC Open
Top quark production in the process $e^+e^- \to t\bar{t}$ at a future linear electron positron collider with polarised beams is a powerful tool to determine indirectly the scale of new physics. The presented study, based on a detailed simu…
View article: EVN: Present and Future
EVN: Present and Future Open