A Close Look at Ly$α$ Emitters with JWST/NIRCam at $zapprox3.1$

Kavli Affiliate: Linhua Jiang | First 5 Authors: Yixiao Liu, Y. Sophia Dai, Stijn Wuyts, Jia-Sheng Huang, Linhua Jiang | Summary: We study 10 spectroscopically confirmed Ly$alpha$ emitters (LAEs) at $zapprox3.1$ in the UDS field, covered by JWST/NIRCam in the PRIMER program. All LAEs are detected in all NIRCam bands from F090W to F444W, corresponding […]


Continue.. A Close Look at Ly$α$ Emitters with JWST/NIRCam at $zapprox3.1$

A Close Look at Ly$α$ Emitters with JWST/NIRCam at $zapprox3.1$

Kavli Affiliate: Linhua Jiang | First 5 Authors: Yixiao Liu, Y. Sophia Dai, Stijn Wuyts, Jia-Sheng Huang, Linhua Jiang | Summary: We study 10 spectroscopically confirmed Ly$alpha$ emitters (LAEs) at $zapprox3.1$ in the UDS field, covered by JWST/NIRCam in the PRIMER program. All LAEs are detected in all NIRCam bands from F090W to F444W, corresponding […]


Continue.. A Close Look at Ly$α$ Emitters with JWST/NIRCam at $zapprox3.1$

Reducing hardware requirements for entanglement distribution via joint hardware-protocol optimization

Kavli Affiliate: Stephanie Wehner | First 5 Authors: Adrià Labay-Mora, Francisco Ferreira da Silva, Stephanie Wehner, , | Summary: We conduct a numerical investigation of fiber-based entanglement distribution over distances of up to 1600km using a chain of processing-node quantum repeaters. We determine minimal hardware requirements while simultaneously optimizing over protocols for entanglement generation and […]


Continue.. Reducing hardware requirements for entanglement distribution via joint hardware-protocol optimization

Axion Curvaton Model for the Gravitational Waves Observed by Pulsar Timing Arrays

Kavli Affiliate: Masahiro Kawasaki | First 5 Authors: Keisuke Inomata, Masahiro Kawasaki, Kyohei Mukaida, Tsutomu T. Yanagida, | Summary: The stochastic gravitational wave background (SGWB) recently detected by the PTA collaborations could be the gravitational waves (GWs) induced by curvature perturbations. However, primordial black holes (PBHs) might be overproduced if the SGWB is explained by […]


Continue.. Axion Curvaton Model for the Gravitational Waves Observed by Pulsar Timing Arrays

Axion Curvaton Model for the Gravitational Waves Observed by Pulsar Timing Arrays

Kavli Affiliate: Masahiro Kawasaki | First 5 Authors: Keisuke Inomata, Masahiro Kawasaki, Kyohei Mukaida, Tsutomu T. Yanagida, | Summary: The stochastic gravitational wave background (SGWB) recently detected by the PTA collaborations could be the gravitational waves (GWs) induced by curvature perturbations. However, primordial black holes (PBHs) might be overproduced if the SGWB is explained by […]


Continue.. Axion Curvaton Model for the Gravitational Waves Observed by Pulsar Timing Arrays

Structural basis of TRPV1 modulation by endogenous bioactive lipids

Kavli Affiliate: Yifan Cheng | Authors: William Randall Arnold, Adamo S Mancino, Frank R Moss III, Adam Frost, David Julius and Yifan Cheng | Summary: TRP ion channels are modulated by phosphoinositide lipids, but the underlying structural mechanisms remain unclear. The capsaicin- and heat-activated receptor, TRPV1, has served as a model for deciphering lipid modulation, […]


Continue.. Structural basis of TRPV1 modulation by endogenous bioactive lipids

Opposing, spatially-determined epigenetic forces impose restrictions on stochastic olfactory receptor choice

Kavli Affiliate: Stavros Lomvardas | Authors: Elizaveta Bashkirova, Nell Klimpert, Kevin Monahan, Christine Campbell, Jason Osinski, Longzhi Tan, Ira Schieren, Ariel Pourmorady, Rebecca Stecky, Gilad Barnea, Xiaoliang Sunney Xie, Ishmail Abdus-Saboor, Benjamin Shykind, Bianca Jones Marlin, Richard Gronostajski, Alexander Fleischmann and Stavros Lomvardas | Summary: Olfactory receptor (OR) choice represents an example of genetically hardwired […]


Continue.. Opposing, spatially-determined epigenetic forces impose restrictions on stochastic olfactory receptor choice

Systematics in the Cepheid and TRGB Distance Scales: Metallicity Sensitivity of the Wesenheit Leavitt Law

Kavli Affiliate: Wendy L. Freedman | First 5 Authors: Barry F. Madore, Wendy L. Freedman, , , | Summary: Using an updated and significantly augmented sample of Cepheid and TRGB distances to 28 nearby spiral and irregular galaxies, covering a wide range of metallicities, we have searched for evidence of a correlation of the zero-point […]


Continue.. Systematics in the Cepheid and TRGB Distance Scales: Metallicity Sensitivity of the Wesenheit Leavitt Law

First X-ray polarization measurement confirms the low black-hole spin in LMC X-3

Kavli Affiliate: Herman L. Marshall | First 5 Authors: Jiří Svoboda, Michal Dovčiak, James F. Steiner, Fabio Muleri, Adam Ingram | Summary: X-ray polarization is a powerful tool to investigate the geometry of accreting material around black holes, allowing independent measurements of the black hole spin and orientation of the innermost parts of the accretion […]


Continue.. First X-ray polarization measurement confirms the low black-hole spin in LMC X-3

First X-ray polarization measurement confirms the low black-hole spin in LMC X-3

Kavli Affiliate: Nicola Omodei | First 5 Authors: Jiří Svoboda, Michal Dovčiak, James F. Steiner, Fabio Muleri, Adam Ingram | Summary: X-ray polarization is a powerful tool to investigate the geometry of accreting material around black holes, allowing independent measurements of the black hole spin and orientation of the innermost parts of the accretion disk. […]


Continue.. First X-ray polarization measurement confirms the low black-hole spin in LMC X-3