Zobrazeno 1 - 10
of 2 539
pro vyhledávání: '"Novak, M A"'
Autor:
Nasrallah, S., Santos-Cottin, D., Mardele, F. Le, Mohelsky, I., Wyzula, J., Aksamovic, L., Sacer, P., Barrett, J. W. H., Galloway, W., Rigaux, K., Guo, F., Puppin, M., Zivkovic, I., Dil, J. H., Novak, M., Barisic, N., Homes, C. C., Orlita, M., Akrap, Ana
In this study, we identify EuCd2X2 (for X = P, As, Sb) as a series of magnetic semiconductors. We examine how the band gap of the series responds to X changing from phosphorus (P), to arsenic (As), and finally antimony (Sb). We characterize the sampl
Externí odkaz:
http://arxiv.org/abs/2409.18722
Autor:
Tolj, D., Reddy, P., Živković, I., Akšamović, L., Soh, J. R., Komȩdera, K., Biało, I., Kumar, C. M. N., Ivšić, T., Novak, M., Zaharko, O., Ritter, C., La Grange, T., Tabiś, W., Batistić, I., Forró, L., Rønnow, H. M., Sunko, D. K., Barišić, N.
Murunskite (K$_2$FeCu$_3$S$_4$) is a bridging compound between the only two known families of high-temperature superconductors. It is a semiconductor like the parent compounds of cuprates, yet isostructural to metallic iron-pnictides. Moreover, like
Externí odkaz:
http://arxiv.org/abs/2406.17108
Autor:
Santos-Cottin, D., Mohelský, I., Wyzula, J., Mardelé, F. Le, Kapon, I., Nasrallah, S., BarišIć, N., Živković, I., Soh, J. R., Guo, F., Rigaux, K., Puppin, M., Dil, J. H., Gudac, B., Rukelj, Z., Novak, M., Kuzmenko, A. B., Homes, C. C., Dietl, Tomasz, Orlita, M., Akrap, Ana
Publikováno v:
Phys. Rev. Lett. 131, 186704 (2023)
EuCd$_2$As$_2$ is now widely accepted as a topological semimetal in which a Weyl phase is induced by an external magnetic field. We challenge this view through firm experimental evidence using a combination of electronic transport, optical spectrosco
Externí odkaz:
http://arxiv.org/abs/2301.08014
Autor:
Mardelé, F. Le, Wyzula, J., Mohelsky, I., Nasrallah, S., Loh, M., David, S. Ben, Toledano, O., Tolj, D., Novak, M., Eguchi, G., Paschen, S., Barišić, N., Chen, J., Kimura, A., Orlita, M., Rukelj, Z., Akrap, A., Santos-Cottin, D.
TlBiSSe is a rare realization of a 3D semimetal with a conically dispersing band that has an optical response which is well isolated from other contributions in a broad range of photon eneries. We report optical and magneto-optical spectroscopy on th
Externí odkaz:
http://arxiv.org/abs/2301.06389
Autor:
Amadio, G., Apostolakis, J., Buncic, P., Cosmo, G., Dosaru, D., Gheata, A., Hageboeck, S., Hahnfeld, J., Hodgkinson, M., Morgan, B., Novak, M., Petre, A. A., Pokorski, W., Ribon, A., Stewart, G. A., Vila, P. M.
Making general particle transport simulation for high-energy physics (HEP) single-instruction-multiple-thread (SIMT) friendly, to take advantage of accelerator hardware, is an important alternative for boosting the throughput of simulation applicatio
Externí odkaz:
http://arxiv.org/abs/2209.15445
Autor:
Delvecchio, I., Daddi, E., Sargent, M. T., Aird, J., Mullaney, J. R., Magnelli, B., Elbaz, D., Bisigello, L., Ceraj, L., Jin, S., Kalita, B. S., Liu, D., Novak, M., Prandoni, I., Radcliffe, J. F., Spingola, C., Zamorani, G., Allevato, V., Rodighiero, G., Smolcic, V.
Publikováno v:
A&A 668, A81 (2022)
Mapping the average AGN luminosity across galaxy populations and over time encapsulates important clues on the interplay between supermassive black hole (SMBH) and galaxy growth. This paper presents the demography, mean power and cosmic evolution of
Externí odkaz:
http://arxiv.org/abs/2209.12585
[Abridged] To understand the role of the galaxy group environment on galaxy evolution, we present a study of radio luminosity functions (RLFs) of group galaxies based on the VLA-COSMOS 3 GHz Large Project. The radio-selected sample of 7826 COSMOS gal
Externí odkaz:
http://arxiv.org/abs/2204.02082
Autor:
Wyzula, J., Lu, X., Santos-Cottin, D., Mukherjee, D. K., Mohelsky, I., Mardele, F. Le, Novak, J., Novak, M., Sankar, R., Krupko, Y., Piot, B. A., Lee, W. -L., Akrap, A., Potemski, M., Goerbig, M. O., Orlita, M.
Publikováno v:
Advanced Science 2105720 (2022)
Optical response of crystalline solids is to a large extent driven by excitations that promote electrons among individual bands. This allows one to apply optical and magneto-optical methods to determine experimentally the energy band gap - a fundamen
Externí odkaz:
http://arxiv.org/abs/2110.07266
Autor:
Seelos, Frank P., Seelos, Kimberly D., Murchie, Scott L., Novak, M. Alexandra Matiella, Hash, Christopher D., Morgan, M. Frank, Arvidson, Raymond E., Aiello, John, Bibring, Jean-Pierre, Bishop, Janice L., Boldt, John D., Boyd, Ariana R., Buczkowski, Debra L., Chen, Patrick Y., Clancy, R. Todd, Ehlmann, Bethany L., Frizzell, Katelyn, Hancock, Katie M., Hayes, John R., Heffernan, Kevin J., Humm, David C., Itoh, Yuki, Ju, Maggie, Kochte, Mark C., Malaret, Erick, McGovern, J. Andrew, McGuire, Patrick, Mehta, Nishant L., Moreland, Eleanor L., Mustard, John F., Nair, A. Hari, Núñez, Jorge I., O'Sullivan, Joseph A., Packer, Liam L., Poffenbarger, Ryan T., Poulet, Francois, Romeo, Giuseppe, Santo, Andrew G., Smith, Michael D., Stephens, David C., Toigo, Anthony D., Viviano, Christina E., Wolff, Michael J.
Publikováno v:
In Icarus 1 September 2024 419
Autor:
Pensabene, A., Decarli, R., Bañados, E., Venemans, B., Walter, F., Bertoldi, F., Fan, X., Farina, E. P., Li, J., Mazzucchelli, C., Novak, M., Riechers, D., Rix, H. -W., Strauss, M. A., Wang, R., Weiß, A., Yang, J., Yang, Y.
Publikováno v:
A&A 652, A66 (2021)
We present a multi-line survey of the interstellar medium (ISM) in two $z>6$ quasar (QSO) host galaxies, PJ231-20 ($z=6.59$) and PJ308-21 ($z=6.23$), and their two companion galaxies. Observations were carried out using the Atacama Large (sub-)Millim
Externí odkaz:
http://arxiv.org/abs/2105.09958