Zobrazeno 1 - 10
of 14 937
pro vyhledávání: '"HENRY, G."'
Autor:
Burri, Corinna, Hua, Nelson, Sanchez, Dario Ferreira, Hu, Wenxiang, Bell, Henry G., Venturini, Rok, Huang, Shih-Wen, McConnell, Aidan G., Dizdarevic, Faris, Mraz, Anze, Svetin, Damjan, Lipovsek, Benjamin, Topic, Marko, Kazazis, Dimitrios, Aeppli, Gabriel, Grolimund, Daniel, Ekinci, Yasin, Mihailovic, Dragan, Gerber, Simon
In transition metal dichalcogenides a plethora of emergent states arise from competing electron-electron and electron-phonon interactions. Among these, the non-volatile metallic 'hidden' state of 1T-TaS2 can be induced from its insulating equilibrium
Externí odkaz:
http://arxiv.org/abs/2411.04830
Autor:
McGhee, Henry G., Thompson, Henry J., Thompson, James, Zhang, Yu, Wyatt, Adam S., Springate, Emma, Chapman, Richard T., Horke, Daniel A., Minns, Russell S., Ingle, Rebecca A., Parkes, Michael A.
The presence of two chlorine atoms in 1,2-dichloroethene allows for isomerisation around the double bond. This isomerisation can lead to rich photochemistry. We present a time-resolved pump-probe photoelectron spectroscopy measurement on both the cis
Externí odkaz:
http://arxiv.org/abs/2410.14322
Autor:
Rast, R. G., Jones, C. E., Carciofi, A. C., Suffak, M. W., Silva, A. C. F., Henry, G. W., Tycner, C.
We examine the evolution of the disk surrounding the Be star in the highly eccentric binary system $\delta$ Scorpii over its three most recent periastron passages. $V$-band and $B-V$ photometry, along with H$\alpha$ spectroscopy are combined with a n
Externí odkaz:
http://arxiv.org/abs/2404.14504
Autor:
Day, Peter K., Cothard, Nicholas F., Albert, Christopher, Foote, Logan, Kane, Elijah, Eom, Byeong H., Thakur, Ritoban Basu, Janssen, Reinier M. J., Beyer, Andrew, Echternach, Pierre, van Berkel, Sven, Hailey-Dunsheath, Steven, Stevenson, Thomas R., Dabironezare, Shahab, Baselmans, Jochem J. A., Glenn, Jason, Bradford, C. Matt, Leduc, Henry G.
We report measurements characterizing the performance of a kinetic inductance detector array designed for a wavelength of 25 microns and very low optical background level suitable for applications such as a far-infrared instrument on a cryogenically
Externí odkaz:
http://arxiv.org/abs/2404.10246
Autor:
Ramanathan, Karthik, Wen, Osmond, Aralis, Taylor, Thakur, Ritoban Basu, Bumble, Bruce, Chang, Yen-Yung, Day, Peter K., Eom, Byeong Ho, LeDuc, Henry G., Sandoval, Brandon J., Stephenson, Ryan, Golwala, Sunil R.
Microwave Kinetic Inductance Detectors (MKIDs) have been demonstrated as capable phonon sensors when coupled to crystalline substrates, and have been proposed as detectors for next-generation rare-event searches such as for the direct detection of da
Externí odkaz:
http://arxiv.org/abs/2402.05419
Autor:
Sypkens, Sasha, Minutolo, Lorenzo, Patel, Sahil, Knehr, Emanuel, Walter, Alexander B., Leduc, Henry G., Narváez, Lautaro, Chamberlin, Ralph, Jamison-Hooks, Tracee, Shaw, Matthew D., Day, Peter K., Korzh, Boris
This work culminates in a demonstration of an alternative Frequency Domain Multiplexing (FDM) scheme for Superconducting Nanowire Single-Photon Detectors (SNSPDs) using the Kinetic inductance Parametric UP-converter (KPUP) made out of NbTiN. There ar
Externí odkaz:
http://arxiv.org/abs/2401.17454
Autor:
Perido, Joanna, Day, Peter K., Beyer, Andrew D., Cothard, Nicholas F., Hailey-Dunsheath, Steven, Leduc, Henry G., Eom, Byeong H., Glenn, Jason
The Balloon Experiment for Galactic INfrared Science (BEGINS) is a concept for a sub-orbital observatory that will operate from $\lambda$ = 25-250 $\mu$m to characterize dust in the vicinity of high-mass stars. The mission's sensitivity requirements
Externí odkaz:
http://arxiv.org/abs/2312.17378
Autor:
Heidari, N., Boisse, I., Hara, N. C., Wilson, T. G., Kiefer, F., Hébrard, G., Philipot, F., Hoyer, S., Stassun, K. G., Henry, G. W., Santos, N. C., Acuña, L., Almasian, D., Arnold, L., Astudillo-Defru, N., Attia, O., Bonfils, X., Bouchy, F., Bourrier, V., Collet, B., Cortés-Zuleta, P., Carmona, A., Delfosse, X., Dalal, S., Deleuil, M., Demangeon, O. D. S., Díaz, R. F., Dumusque, X., Ehrenreich, D., Forveille, T., Hobson, M. J., Jenkins, J. S., Jenkins, J. M., Lagrange, A. M., Latham, D. W., Larue, P., Liu, J., Moutou, C., Mignon, L., Osborn, H. P., Pepe, F., Rapetti, D., Rodrigues, J., Santerne, A., Segransan, D., Shporer, A., Sulis, S., Torres, G., Udry, S., Vakili, F., Vanderburg, A., Venot, O., Vivien, H. G., Vines, J. I.
Publikováno v:
A&A 681, A55 (2024)
Transiting planets with orbital periods longer than 40 d are extremely rare among the 5000+ planets discovered so far. The lack of discoveries of this population poses a challenge to research into planetary demographics, formation, and evolution. Her
Externí odkaz:
http://arxiv.org/abs/2311.13513