X-ray/UVOIR Frequency-resolved Time Lag Analysis of Mrk 335 Reveals Accretion Disk Reprocessing

Kavli Affiliate: Erin Kara | First 5 Authors: Collin Lewin, Erin Kara, Edward M. Cackett, Dan Wilkins, Christos Panagiotou | Summary: UV and optical continuum reverberation mapping is powerful for probing the accretion disk and inner broad-line region. However, recent reverberation mapping campaigns in the X-ray, UV, and optical have found lags consistently longer than […]


Continue.. X-ray/UVOIR Frequency-resolved Time Lag Analysis of Mrk 335 Reveals Accretion Disk Reprocessing

The Third Fermi Large Area Telescope Catalog of Gamma-ray Pulsars

Kavli Affiliate: Maria Elena Monzani | First 5 Authors: David A. Smith, Philippe Bruel, Colin J. Clark, Lucas Guillemot, Matthew T. Kerr | Summary: We present 294 pulsars found in GeV data from the Large Area Telescope (LAT) on the Fermi Gamma-ray Space Telescope. Another 33 millisecond pulsars (MSPs) discovered in deep radio searches of […]


Continue.. The Third Fermi Large Area Telescope Catalog of Gamma-ray Pulsars

The Third Fermi Large Area Telescope Catalog of Gamma-ray Pulsars

Kavli Affiliate: Maria Elena Monzani | First 5 Authors: David A. Smith, Philippe Bruel, Colin J. Clark, Lucas Guillemot, Matthew T. Kerr | Summary: We present 294 pulsars found in GeV data from the Large Area Telescope (LAT) on the Fermi Gamma-ray Space Telescope. Another 33 millisecond pulsars (MSPs) discovered in deep radio searches of […]


Continue.. The Third Fermi Large Area Telescope Catalog of Gamma-ray Pulsars

Characterizing Gravitational Wave Detector Networks: From A$^sharp$ to Cosmic Explorer

Kavli Affiliate: Peter Fritschel | First 5 Authors: Ish Gupta, Chaitanya Afle, K. G. Arun, Ananya Bandopadhyay, Masha Baryakhtar | Summary: Gravitational-wave observations by the Laser Interferometer Gravitational-Wave Observatory (LIGO) and Virgo have provided us a new tool to explore the universe on all scales from nuclear physics to the cosmos and have the massive […]


Continue.. Characterizing Gravitational Wave Detector Networks: From A$^sharp$ to Cosmic Explorer

Characterizing Gravitational Wave Detector Networks: From A$^sharp$ to Cosmic Explorer

Kavli Affiliate: Peter Fritschel | First 5 Authors: Ish Gupta, Chaitanya Afle, K. G. Arun, Ananya Bandopadhyay, Masha Baryakhtar | Summary: Gravitational-wave observations by the Laser Interferometer Gravitational-Wave Observatory (LIGO) and Virgo have provided us a new tool to explore the Universe on all scales from nuclear physics to the cosmos and have the massive […]


Continue.. Characterizing Gravitational Wave Detector Networks: From A$^sharp$ to Cosmic Explorer

Characterizing Gravitational Wave Detector Networks: From A$^sharp$ to Cosmic Explorer

Kavli Affiliate: David H. Shoemaker | First 5 Authors: Ish Gupta, Chaitanya Afle, K. G. Arun, Ananya Bandopadhyay, Masha Baryakhtar | Summary: Gravitational-wave observations by the Laser Interferometer Gravitational-Wave Observatory (LIGO) and Virgo have provided us a new tool to explore the Universe on all scales from nuclear physics to the cosmos and have the […]


Continue.. Characterizing Gravitational Wave Detector Networks: From A$^sharp$ to Cosmic Explorer

Direct observation of chiral edge current at zero magnetic field in odd-layer MnBi$_2$Te$_4$

Kavli Affiliate: Jing Wang | First 5 Authors: Jinjiang Zhu, Yang Feng, Xiaodong Zhou, Yongchao Wang, Zichen Lian | Summary: The chiral edge current is the boundary manifestation of the Chern number of a quantum anomalous Hall (QAH) insulator. Its direct observation is assumed to require well-quantized Hall conductance, and is so far lacking. The […]


Continue.. Direct observation of chiral edge current at zero magnetic field in odd-layer MnBi$_2$Te$_4$

Colliding red giants in galactic nuclei: Shocks, jets, impact on the ISM, X- and gamma-rays, neutrinos, fusion ignition and afterglow

Kavli Affiliate: Pau Amaro Seoane | First 5 Authors: Pau Amaro Seoane, , , , | Summary: In galactic nuclei, stellar densities are so high that stars can physically collide with each other. In this work we focus on the collision of red giants and in particular on the formation of non-thermal processes through collisions […]


Continue.. Colliding red giants in galactic nuclei: Shocks, jets, impact on the ISM, X- and gamma-rays, neutrinos, fusion ignition and afterglow

Colliding red giants in galactic nuclei: Shocks, jets, impact on the ISM, X- and gamma-rays, neutrinos, fusion ignition and afterglow

Kavli Affiliate: Pau Amaro Seoane | First 5 Authors: Pau Amaro Seoane, , , , | Summary: In galactic nuclei, stellar densities are so high that stars can physically collide with each other. In this work we focus on the collision of red giants and in particular on the formation of non-thermal processes through collisions […]


Continue.. Colliding red giants in galactic nuclei: Shocks, jets, impact on the ISM, X- and gamma-rays, neutrinos, fusion ignition and afterglow