Designing an Optimal Kilonova Search using DECam for Gravitational Wave Events

Autor: Bom, C. R., Annis, J., Garcia, A., Palmese, A., Sherman, N., Soares-Santos, M., Santana-Silva, L., Morgan, R., Bechtol, K., Davis, T., Diehl, H. T., Allam, S. S., Bachmann, T. G., Fraga, B. M. O., Garcıa-Bellido, J., Gill, M. S. S., Herner, K., Kilpatrick, C. D., Makler, M., E., F. Olivares, Pereira, M. E. S., Pineda, J., Santos, A., Tucker, D. L., Wiesner, M. P., Aguena, M., Alves, O., Bacon, D., Bernardinelli, P. H., Bertin, E., Bocquet, S., Brooks, D., Kind, M. Carrasco, Carretero, J., Conselice, C., Costanzi, M., da Costa, L. N., De Vicente, J., Desai, S., Doel, P., Everett, S., Ferrero, I., Frieman, J., Gatti, M., Gerdes, D. W., Gruen, D., Gruendl, R. A., Gutierrez, G., Hinton, S. R., Hollowood, D. L., Honscheid, K., James, D. J., Kuehn, K., Kuropatkin, N., Melchior, P., Mena-Fernandez, J., Menanteau, F., Pieres, A., Malagon, A. A. Plazas, Raveri, M., Rodriguez-Monroy, M., Sanchez, E., Santiago, B., Sevilla-Noarbe, I., Smith, M., Suchyta, E., Swanson, M. E. C., Tarle, G., To, C., Weaverdyck, N.

We address the problem of optimally identifying all kilonovae detected via gravitational wave emission in the upcoming LIGO/Virgo/KAGRA Collaboration observing run, O4, which is expected to be sensitive to a factor of $\sim 7$ more Binary Neutron Sta

Externí odkaz: http://arxiv.org/abs/2302.04878

Constraints on the Physical Properties of GW190814 through Simulations based on DECam Follow-up Observations by the Dark Energy Survey

Autor: Morgan, R., Soares-Santos, M., Annis, J., Herner, K., Garcia, A., Palmese, A., Drlica-Wagner, A., Kessler, R., Garcia-Bellido, J., Sherman, T. G. Bachmann N., Allam, S., Bechtol, K., Bom, C. R., Brout, D., Butler, R. E., Butner, M., Cartier, R., Chen, H., Conselice, C., Cook, E., Davis, T. M., Doctor, Z., Farr, B., Figueiredo, A. L., Finley, D. A., Foley, R. J., Galarza, J. Y., Gill, M. S. S., Gruendl, R. A., Holz, D. E., Kuropatkin, N., Lidman, C., Lin, H., Malik, U., Mann, A. W., Marriner, J., Marshall, J. L., Martinez-Vazquez, C. E., Meza, N., Neilsen, E., Nicolaou, C., E., F. Olivares, Paz-Chinchon, F., Points, S., Quirola, J., Rodriguez, O., Sako, M., Scolnic, D., Smith, M., Sobreira, F., Tucker, D. L., Vivas, A. K., Wiesner, M., Wood, M. L., Yanny, B., Zenteno, A., Abbott, T. M. C., Aguena, M., Avila, S., Bertin, E., Bhargava, S., Brooks, D., Burke, D. L., Rosell, A. Carnero, Kind, M. Carrasco, Carretero, J., da Costa, L. N., Costanzi, M., De Vicente, J., Desai, S., Diehl, H. T., Doel, P., Eifler, T. F., Everett, S., Flaugher, B., Frieman, J., Gaztanaga, E., Gerdes, D. W., Gruen, D., Gschwend, J., Gutierrez, G., Hartley, W. G., Hinton, S. R., Hollowood, D. L., Honscheid, K., James, D. J., Kuehn, K., Lahav, O., Lima, M., Maia, M. A. G., March, M., Miquel, R., Ogando, R. L. C., Plazas, A. A., Roodman, A., Sanchez, E., Scarpine, V., Schubnell, M., Serrano, S., Sevilla-Noarbe, I., Suchyta, E., Tarle, G.

On 14 August 2019, the LIGO and Virgo Collaborations detected gravitational waves from a black hole and a 2.6 solar mass compact object, possibly the first neutron star -- black hole (NSBH) merger. In search of an optical counterpart, the Dark Energy

Externí odkaz: http://arxiv.org/abs/2006.07385

Efficient single-photon emission from electrically driven InP quantum dots epitaxially grown on Si(001)

Autor: Wiesner, M., Schulz, W. -M., Kessler, C., Reischle, M., Rossbach, R., Jetter, M., Michler, P.

The heteroepitaxy of III-V semiconductors on silicon is a promising approach for making silicon a photonic platform for on-chip optical interconnects and quantum optical applications. Monolithic integration of both material systems is a long-time cha

Externí odkaz: http://arxiv.org/abs/1104.2144

Shot noise and conductivity at high bias in bilayer graphene: Signatures of electron-optical phonon coupling

Autor: Fay, A., Danneau, R., Viljas, J. K., Wu, F., Tomi, M. Y., Wengler, J., Wiesner, M., Hakonen, P. J.

We have studied electronic conductivity and shot noise of bilayer graphene (BLG) sheets at high bias voltages and low bath temperature $T_0=4.2$ K. As a function of bias, we find initially an increase of the differential conductivity, which we attrib

Externí odkaz: http://arxiv.org/abs/0904.4446

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