Risultati della ricerca - Lin, R.

The sensitivity of fixed-bed biological perchlorate removal to changes in operating conditions and water quality characteristics di Brown, J., Snoeyink, V., Raskin, L., Lin, R

Landau free energy and the absence of spontaneous magnetization of the one-dimensional Ising model di Zheng, Z. F., Lin, R. K., Zhang, J. M.

Testo

HiLoTs: High-Low Temporal Sensitive Representation Learning for Semi-Supervised LiDAR Segmentation in Autonomous Driving di Lin, R. D., Weng, Pengcheng, Wang, Yinqiao, Ding, Han, Han, Jinsong, Wang, Fei

Testo

Magnetic properties of binary alloys Ni1-xMox and Ni1-yCuy close to critical concentrations di Lin, R. -Z., Hsu, C. -H., Liu, E. -P., Chen, W. -T., Huang, C. -L.

Testo

A Complete Analysis of Subgiant Stellar Systems III: Hip70868 di Elgendy, Hoda E., Al-Wardat, Mashhoor A., Haboubi, Hassan B., Benchi, Lin R., Hussein, Abdallah M., Elmehdi, Hussein M.

Testo

Non-Fermi-liquid behavior in a ferromagnetic heavy fermion system CeTi$_{1-x}$V$_{x}$Ge$_{3}$ di Lin, R. -Z., Jin, H., Klavins, P., Chen, W. -T., Chang, Y. -Y., Chung, C. -H., Taufour, V., Huang, C. -L.

Testo

SIP-IFVM: Efficient time-accurate magnetohydrodynamic model of the corona and coronal mass ejections di Wang, H. P., Guo, J. H., Yang, L. P., Poedts, S., Zhang, F., Lani, A., Baratashvili, T., Linan, L., Lin, R., Guo, Y.

Testo

PRISMS. U37126, a very blue, ISM-naked starburst at z=10.255 with nearly 100% Lyman continuum escape fraction di Marques-Chaves, R., Álvarez-Márquez, J., Colina, L., Kendrew, S., Abdurro'uf, Blanco-Prieto, C., Boogaard, L. A., Castellano, M., Caputi, K. I., Crespo-Gomez, A., Fontana, A., Fudamoto, Y., Fujimoto, S., García-Marín, M., Harikane, Y., Harish, S., Hashimoto, T., Hsiao, T., Iani, E., Inoue, A. K., Langeroodi, D., Lin, R., Melinder, J., Napolitano, L., Ostlin, G., Pérez-González, P. G., Prieto-Jiménez, C., Rinaldi, P., Del Pino, B. Rodríguez, Santini, P., Sugahara, Y., Varo-O'ferral, A., Wright, G., Zavala, J.

Testo

PRISMS. UNCOVER-26185, a metal-poor SFG at z=10.05 with no evidence for a X-ray-luminous AGN di Álvarez-Márquez, J., Colina, L., Crespo-Gomez, A., Kendrew, S., Zavala, J., Marques-Chaves, R., Prieto-Jiménez, C., Abdurro'uf, Blanco-Prieto, C., Boogaard, L. A., Castellano, M., Fontana, A., Fudamoto, Y., Fujimoto, S., García-Marín, M., Harikane, Y., Harish, S., Hashimoto, T., Hsiao, T., Iani, E., Inoue, A. K., Langeroodi, D., Lin, R., Melinder, J., Napolitano, L., Ostlin, G., Pérez-González, P. G., Rinaldi, P., Del Pino, B. Rodríguez, Santini, P., Sugahara, Y., Treu, T., Varo-O'ferral, A., Wright, G.

Testo