Zobrazeno 1 - 10
of 7 462
pro vyhledávání: '"Ho, P. C."'
Autor:
Jiang, C. Y., Chen, B. L., Chen, K. W., Jiao, J. C., Wang, Y., Wu, Q., Zhang, N. Y., Zou, M. Y., Ho, P. -C., Bernal, O. O., Shu, L.
We report results of magnetic susceptibility, specific heat, and muon spin relaxation ($\mu$SR) measurements on the polycrystalline Ba$_6$Nd$_2$Ti$_4$O$_{17}$, a disorder-free triangular-lattice antiferromagnet. The absence of long-range magnetic ord
Externí odkaz:
http://arxiv.org/abs/2411.13070
Autor:
Kim, Donghoon, Ottesen, Jon Andre, Kumar, Ashwin, Ho, Brandon C., Bismuth, Elsa, Young, Christina B., Mormino, Elizabeth, Zaharchuk, Greg
Identifying amyloid-beta positive patients is crucial for determining eligibility for Alzheimer's disease (AD) clinical trials and new disease-modifying treatments, but currently requires PET or CSF sampling. Previous MRI-based deep learning models f
Externí odkaz:
http://arxiv.org/abs/2411.12061
Autor:
Kim, Taehyun, Kim, Minjin, Ho, Luis C., Li, Yang A., Jeong, Woong-Seob, Kim, Dohyeong, Kim, Yongjung, Lee, Bomee, Lee, Dongseob, Lee, Jeong Hwan, Pyo, Jeonghyun, Shim, Hyunjin, Son, Suyeon, Song, Hyunmi, Yang, Yujin
Future satellite missions are expected to perform all-sky surveys, thus providing the entire sky near-infrared spectral data and consequently opening a new window to investigate the evolution of galaxies. Specifically, the infrared spectral data faci
Externí odkaz:
http://arxiv.org/abs/2411.10981
Pressure injury (PI) detection is challenging, especially in dark skin tones, due to the unreliability of visual inspection. Thermography has been suggested as a viable alternative as temperature differences in the skin can indicate impending tissue
Externí odkaz:
http://arxiv.org/abs/2411.10627
We aim to constrain the average star formation associated with neutral hydrogen gas reservoirs at cosmic noon. Using a unprecedented sample of 1716 high column density Damped Ly-$\alpha$ absorbers (DLAs) from the Sloan Digital Sky Survey with log($N$
Externí odkaz:
http://arxiv.org/abs/2411.10525
Autor:
Baghel, Janhavi, Kharb, P., Hovatta, T., Ho, Luis C., Harrison, C., Lindfors, E., S., Silpa, Gulati, S.
We present polarization images with the Karl G. Jansky Very Large Array (VLA) in A and B-array configurations at 6 GHz of 7 radio-loud (RL) quasars and 8 BL Lac objects belonging to the Palomar-Green (PG) `blazar' sample. This completes our arcsecond
Externí odkaz:
http://arxiv.org/abs/2411.06937
We investigate the host galaxy properties of eight little red dots (LRDs) selected from the JWST UNCOVER survey, applying a new technique ({\tt\string GalfitS}) to simultaneously fit the morphology and spectral energy distribution using multi-band NI
Externí odkaz:
http://arxiv.org/abs/2411.04446
Autor:
Zavala, Jorge A., Bakx, Tom, Mitsuhashi, Ikki, Castellano, Marco, Calabro, Antonello, Akins, Hollis, Buat, Veronique, Casey, Caitlin M., Fernandez-Arenas, David, Franco, Maximilien, Fontana, Adriano, Hatsukade, Bunyo, Ho, Luis C., Ikeda, Ryota, Kartaltepe, Jeyhan, Koekemoer, Anton M., McKinney, Jed, Napolitano, Lorenzo, Perez-Gonzalez, Pablo G., Santini, Paola, Serjeant, Stephen, Terlevich, Elena, Terlevich, Roberto, Yung, L. Y. Aaron
We present ALMA observations on the high-redshift galaxy GHZ2 and report a successful detection of the rest-frame 88um atomic transition from doubly-ionized Oxygen at z=12.3327+/-0.0005. Based on these observations, combined with additional constrain
Externí odkaz:
http://arxiv.org/abs/2411.03593
Autor:
Yang, Tsung-Ching, Hashimoto, Tetsuya, Hsu, Tzu-Yin, Goto, Tomotsugu, Ling, Chih-Teng, Ho, Simon C. -C., Chen, Amos Y. -A., Kilerci, Ece
Measuring the Hubble constant (H$_0$) is one of the most important missions in astronomy. Nevertheless, recent studies exhibit differences between the employed methods. Fast radio bursts (FRBs) are coherent radio transients with large dispersion meas
Externí odkaz:
http://arxiv.org/abs/2411.02249
James Webb Space Telescope (JWST) has revealed a population of red and compact sources at $z \gtrsim 5$ known as "Little Red Dots" (LRDs) that are likely active galactic nuclei (AGNs). Here we present a comprehensive study of the variability of 314 L
Externí odkaz:
http://arxiv.org/abs/2411.02729