Zobrazeno 71 - 80
of 56 524
pro vyhledávání: '"Laird A"'
Autor:
Zhou, Yifan, Sanghi, Aniket, Bowler, Brendan P., Wu, Ya-Lin, Close, Laird M., Long, Feng, Ward-Duong, Kimberly, Zhu, Zhaohuan, Kraus, Adam L., Follette, Katherine B., Bae, Jaehan
Accreting protoplanets enable the direct characterization of planet formation. As part of a high-contrast imaging search for accreting planets with the Hubble Space Telescope (HST) Wide Field Camera 3, we present H$\alpha$ images of AB Aurigae (AB Au
Externí odkaz:
http://arxiv.org/abs/2207.06525
Previous work has largely considered the fairness of image captioning systems through the underspecified lens of "bias." In contrast, we present a set of techniques for measuring five types of representational harms, as well as the resulting measurem
Externí odkaz:
http://arxiv.org/abs/2206.07173
Autor:
Williams, M., Laird, A. M., Choplin, A., Adsley, P., Davids, B., Greife, U., Hudson, K., Hutcheon, D., Lennarz, A., Ruiz, C.
The efficiency of the slow neutron-capture process in massive stars is strongly influenced by neutron-capture reactions on light elements. At low metallicity, $^{16}$O is an important neutron absorber, but the effectiveness of $^{16}$O as a light-ele
Externí odkaz:
http://arxiv.org/abs/2206.06016
Autor:
Frost-Schenk, J., Adsley, P., Laird, A. M., Longland, R., Angus, C., Barton, C., Choplin, A., Diget, C. Aa., Hirschi, R., Marshall, C., Chaves, F. Portillo, Setoodehnia, K.
Massive stars are crucial to galactic chemical evolution for elements heavier than iron. Their contribution at early times in the evolution of the Universe, however, is unclear due to poorly constrained nuclear reaction rates. The competing $^{17}$O(
Externí odkaz:
http://arxiv.org/abs/2206.04167
Autor:
Haffert, Sebastiaan Y., Close, Laird M., Hedglen, Alexander D., Males, Jared R., Kautz, Maggie, Bouchez, Antonin H., Demers, Richard, Quiros-Pacheco, Fernando, Sitarski, Breann N., Van Gorkom, Kyle, Long, Joseph D., Guyon, Olivier, Schatz, Lauren, Miller, Kelsey, Lumbres, Jennifer, Rodack, Alex, Knight, Justin M.
The next generation of Giant Segmented Mirror Telescopes (GSMT) will have large gaps between the segments either caused by the shadow of the mechanical structure of the secondary mirror (E-ELT and TMT) or intrinsically by design (GMT). These gaps are
Externí odkaz:
http://arxiv.org/abs/2206.03615
Autor:
Hedglen, Alexander D., Close, Laird M., Haffert, Sebastiaan Y., Males, Jared R., Kautz, Maggie, Bouchez, Antonin H., Demers, Richard, Quiros-Pacheco, Fernando, Sitarski, Breann N., Guyon, Olivier, Van Gorkom, Kyle, Long, Joseph D., Lumbres, Jennifer, Schatz, Lauren, Miller, Kelsey, Rodack, Alex, Knight, Justin M.
The Giant Magellan Telescope (GMT) design consists of seven circular 8.4-m diameter mirror segments that are separated by large > 30 cm gaps, creating the possibility of fluctuations in optical path differences due to flexure, segment vibrations, win
Externí odkaz:
http://arxiv.org/abs/2206.03614
Autor:
Balmer, William O., Follette, Katherine B., Close, Laird M., Males, Jared R., De Rosa, Robert J., Redai, Jéa I. Adams, Watson, Alex, Weinberger, Alycia J., Morzinski, Katie M., Morales, Julio, Ward-Duong, Kimberly, Pueyo, Laurent
Publikováno v:
The Astronomical Journal, Volume 164 (2022), Issue 1, id.29, 23 pp
Companions embedded in the cavities of transitional circumstellar disks have been observed to exhibit excess luminosity at H$\alpha$, an indication that they are actively accreting. We report 5 years (2013-2018) of monitoring of the position and H$\a
Externí odkaz:
http://arxiv.org/abs/2206.00687
Autor:
Schatz, H., Reyes, A. D. Becerril, Best, A., Brown, E. F., Chatziioannou, K., Chipps, K. A., Deibel, C. M., Ezzeddine, R., Galloway, D. K., Hansen, C. J., Herwig, F., Ji, A. P., Lugaro, M., Meisel, Z., Norman, D., Read, J. S., Roberts, L. F., Spyrou, A., Tews, I., Timmes, F. X., Travaglio, C., Vassh, N., Abia, C., Adsley, P., Agarwal, S., Aliotta, M., Aoki, W., Arcones, A., Aryan, A., Bandyopadhyay, A., Banu, A., Bardayan, D. W., Barnes, J., Bauswein, A., Beers, T. C., Bishop, J., Boztepe, T., Côté, B., Caplan, M. E., Champagne, A. E., Clark, J. A., Couder, M., Couture, A., de Mink, S. E., Debnath, S., deBoer, R. J., Hartogh, J. den, Denissenkov, P., Dexheimer, V., Dillmann, I., Escher, J. E., Famiano, M. A., Farmer, R., Fisher, R., Fröhlich, C., Frebel, A., Fryer, C., Fuller, G., Ganguly, A. K., Ghosh, S., Gibson, B. K., Gorda, T., Gourgouliatos, K. N., Graber, V., Gupta, M., Haxton, W., Heger, A., Hix, W. R., Ho, W C. G., Holmbeck, E. M., Hood, A. A., Huth, S., Imbriani, G., Izzard, R. G., Jain, R., Jayatissa, H., Johnston, Z., Kajino, T., Kankainen, A., Kiss, G. G., Kwiatkowski, A., La Cognata, M., Laird, A. M., Lamia, L., Landry, P., Laplace, E., Launey, K. D., Leahy, D., Leckenby, G., Lennarz, A., Longfellow, B., Lovell, A. E., Lynch, W. G., Lyons, S. M., Maeda, K., Masha, E., Matei, C., Merc, J., Messer, B., Montes, F., Mukherjee, A., Mumpower, M., Neto, D., Nevins, B., Newton, W. G., Nguyen, L. Q., Nishikawa, K., Nishimura, N., Nunes, F. M., O'Connor, E., O'Shea, B. W., Ong, W-J., Pain, S. D., Pajkos, M. A., Pignatari, M., Pizzone, R. G., Placco, V. M., Plewa, T., Pritychenko, B., Psaltis, A., Puentes, D., Qian, Y-Z., Radice, D., Rapagnani, D., Rebeiro, B. M., Reifarth, R., Richard, A. L., Rijal, N., Roederer, I. U., Rojo, J. S., K, J. S, Saito, Y., Schwenk, A., Sergi, M. L., Sidhu, R. S., Simon, A., Sivarani, T., Skúladóttir, Á., Smith, M. S., Spiridon, A., Sprouse, T. M., Starrfield, S., Steiner, A. W., Strieder, F., Sultana, I., Surman, R., Szücs, T., Tawfik, A., Thielemann, F., Trache, L., Trappitsch, R., Tsang, M. B., Tumino, A., Upadhyayula, S., Martínez, J. O. Valle, Van der Swaelmen, M., Vázquez, C. Viscasillas, Watts, A., Wehmeyer, B., Wiescher, M., Wrede, C., Yoon, J., Zegers, R G. T., Zermane, M. A., Zingale, M.
Nuclear Astrophysics is a field at the intersection of nuclear physics and astrophysics, which seeks to understand the nuclear engines of astronomical objects and the origin of the chemical elements. This white paper summarizes progress and status of
Externí odkaz:
http://arxiv.org/abs/2205.07996
Publikováno v:
Phys. Rev. B 106, 125407 (2022)
We theoretically investigate exciton-polaritons in a two-dimensional (2D) semiconductor heterostructure, where a static magnetic field is applied perpendicular to the plane. To explore the interplay between magnetic field and a strong light-matter co
Externí odkaz:
http://arxiv.org/abs/2205.06952
Autor:
Laird, John E.
This paper is the recommended initial reading for a functional overview of Soar, version 9.6. It includes an abstract overview of the architectural structure of Soar including its processing, memories, learning modules, their interfaces, and the repr
Externí odkaz:
http://arxiv.org/abs/2205.03854