Zobrazeno 1 - 10
of 471
pro vyhledávání: '"F. Olivares"'
Autor:
C. R. Bom, J. Annis, A. Garcia, A. Palmese, N. Sherman, M. Soares-Santos, L. Santana-Silva, R. Morgan, K. Bechtol, T. Davis, H. T. Diehl, S. S. Allam, T. G. Bachmann, B. M. O. Fraga, J. García-Bellido, M. S. S. Gill, K. Herner, C. D. Kilpatrick, M. Makler, F. Olivares E., M. E. S. Pereira, J. Pineda, A. Santos, D. L. Tucker, M. P. Wiesner, M. Aguena, O. Alves, D. Bacon, P. H. Bernardinelli, E. Bertin, S. Bocquet, D. Brooks, M. Carrasco Kind, J. Carretero, C. Conselice, M. Costanzi, L. N. da Costa, J. De Vicente, S. Desai, P. Doel, S. Everett, I. Ferrero, J. Frieman, M. Gatti, D. W. Gerdes, D. Gruen, R. A. Gruendl, G. Gutierrez, S. R. Hinton, D. L. Hollowood, K. Honscheid, D. J. James, K. Kuehn, N. Kuropatkin, P. Melchior, J. Mena-Fernández, F. Menanteau, A. Pieres, A. A. Plazas Malagón, M. Raveri, M. Rodriguez-Monroy, E. Sanchez, B. Santiago, I. Sevilla-Noarbe, M. Smith, E. Suchyta, M. E. C. Swanson, G. Tarle, C. To, N. Weaverdyck
Publikováno v:
The Astrophysical Journal, Vol 960, Iss 2, p 122 (2024)
We address the problem of optimally identifying all kilonovae detected via gravitational-wave emission in the upcoming LIGO/Virgo/KAGRA observing run, O4, which is expected to be sensitive to a factor of ∼7 more binary neutron star (BNS) alerts tha
Externí odkaz:
https://doaj.org/article/516ae8285e4f46a1a1df07455197d577
Autor:
Greiner, J., Krühler, T., Bolmer, J., Klose, S., Afonso, P. M. J., Elliott, J., Filgas, R., Graham, J. F., Kann, D. A., Knust, F., Yoldaş, A. Küpcü, Nardini, M., Guelbenzu, A. M. Nicuesa, Estay, F. Olivares, Rossi, A., Schady, P., Schweyer, T., Sudilovsky, V., Varela, K., Wiseman, P.
A dedicated gamma-ray burst (GRB) afterglow observing program was performed between 2007 and 2016 with GROND, a seven-channel optical and near-infrared imager at the 2.2m telescope of the Max-Planck Society at ESO/La Silla. In this first of a series
Externí odkaz:
http://arxiv.org/abs/2410.14441
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
Autor:
Rybicki, K. A., Wyrzykowski, Ł., Bachelet, E., Cassan, A., Zieliński, P., Gould, A., Novati, S. Calchi, Yee, J. C., Ryu, Y. -H., Gromadzki, M., Mikołajczyk, P., Ihanec, N., Kruszyńska, K., Hambsch, F. -J., Zoła, S., Fossey, S. J., Awiphan, S., Nakharutai, N., Lewis, F., E., F. Olivares, Hodgkin, S., Delgado, A., Breedt, E., Harrison, D. L., vanLeeuwen, M., Rixon, G., Wevers, T., Yoldas, A., Udalski, A., Szymański, M. K., Soszyński, I., Pietrukowicz, P., Kozłowski, S., Skowron, J., Poleski, R., Ulaczyk, K., Mróz, P., Iwanek, P., Wrona, M., Street, R. A., Tsapras, Y., Hundertmark, M., Dominik, M., Beichman, C., Bryden, G., Carey, S., Gaudi, B. S., Henderson, C., Shvartzvald, Y., Zang, W., Zhu, W., Christie, G. W., Green, J., Hennerley, S., McCormick, J., Monard, L. A. G., Natusch, T., Pogge, R. W., Gezer, I., Gurgul, A., Kaczmarek, Z., Konacki, M., Lam, M. C., Maskoliunas, M., Pakstiene, E., Ratajczak, M., Stankeviciute, A., Zdanavicius, J., Ziółkowska, O.
We present the photometric analysis of Gaia19bld, a high-magnification ($A\approx60$) microlensing event located in the southern Galactic plane, which exhibited finite source and microlensing parallax effects. Due to a prompt detection by the Gaia sa
Externí odkaz:
http://arxiv.org/abs/2112.01613
Autor:
DES Collaboration, Garcia, A., Morgan, R., Herner, K., Palmese, A., Soares-Santos, M., Annis, J., Brout, D., Vivas, A. K., Drlica-Wagner, A., Santana-Silva, L., Tucker, D. L., Allam, S., Wiesner, M., García-Bellido, J., Gill, M. S. S., Sako, M., Kessler, R., Davis, T. M., Scolnic, D., E., F. Olivares, Paz-Chinchón, F., Sherman, N., Conselice, C., Chen, H., Foley, R. J., Doctor, Z., Horvath, J., Howell, D. A., Kilpatrick, C. D., Casares, J., Cooke, J., Rest, 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., Costanzi, M., da Costa, L. N., Desai, S., Diehl, H. T., Dietrich, J. P., Doel, P., Everett, S., Flaugher, B., Fosalba, P., Friedel, D., Frieman, J., Gaztanaga, E., Gerdes, D. W., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hinton, S. R., Hollowood, D. L., Honscheid, K., James, D. J., Kuehn, K., Kuropatkin, N., Lahav, O., Lima, M., Maia, M. A. G., March, M., Marshall, J. L., Menanteau, F., Miquel, R., Ogando, R. L. C., Plazas, A. A., Romer, A. K., Roodman, A., Sanchez, E., Scarpine, V., Schubnell, M., Serrano, S., Sevilla-Noarbe, I., Smith, M., Suchyta, E., Swanson, M. E. C., Tarle, G., Thomas, D., Varga, T. N., Walker, A. R., Weller, J.
We present the results from a search for the electromagnetic counterpart of the LIGO/Virgo event S190510g using the Dark Energy Camera (DECam). S190510g is a binary neutron star (BNS) merger candidate of moderate significance detected at a distance o
Externí odkaz:
http://arxiv.org/abs/2007.00050
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
Autor:
Melandri, A., Malesani, D. B., Izzo, L., Japelj, J., Vergani, S. D., Schady, P., Carracedo, A. Sagues, Postigo, A. de Ugarte, Anderson, J. P., Barbarino, C., Bolmer, J., Breeveld, A., Calissendorff, P., Campana, S., Cano, Z., Carini, R., Covino, S., D'Avanzo, P., D'Elia, V., della Valle, M., De Pasquale, M., Fynbo, J. P. U., Gromadzki, M., Hammer, F., Hartmann, D. H., Heintz, K. E., Inserra, C., Jakobsson, P., Kann, D. A., Kotilainen, J., Maguire, K., Masetti, N., Nicholl, M., E., F. Olivares, Pugliese, G., Rossi, A., Salvaterra, R., Sollerman, J., Stone, M. B., Tagliaferri, G., Tomasella, L., Thone, C. C., Xu, D., Young, D. R.
The number of supernovae known to be connected with long-duration gamma-ray bursts is increasing and the link between these events is no longer exclusively found at low redshift ($z \lesssim 0.3$) but is well established also at larger distances. We
Externí odkaz:
http://arxiv.org/abs/1910.14160
Autor:
Prentice, S. J., Ashall, C., James, P. A., Short, L., Mazzali, P. A., Bersier, D., Crowther, P. A., Barbarino, C., Chen, T. -W., Copperwheat, C. M., Darnley, M. J., Denneau, L., Elias-Rosa, N., Fraser, M., Galbany, L., Gal-Yam, A., Harmanen, J., Howell, D. A., Hosseinzadeh, G., Inserra, C., Kankare, E., Karamehmetoglu, E., Lamb, G. P., Limongi, M., Maguire, K., McCully, C., E., F. Olivares, Piascik, A. S., Pignata, G., Reichart, D. E., Reynolds, A. Rest T., Rodríguez, Ó., Saario, J. L. O., Schulze, S., Smartt, S. J., Smith, K. W., Sollerman, J., Stalder, B., Sullivan, M., Taddia, F., Valenti, S., Vergani, S. D., Williams, S. C., Young, D. R.
We present observations and analysis of 18 stripped-envelope supernovae observed during 2013 -- 2018. This sample consists of 5 H/He-rich SNe, 6 H-poor/He-rich SNe, 3 narrow lined SNe Ic and 4 broad lined SNe Ic. The peak luminosity and characteristi
Externí odkaz:
http://arxiv.org/abs/1812.03716
Autor:
Förster, F., Moriya, T. J., Maureira, J. C., Anderson, J. P., Blinnikov, S., Bufano, F., Cabrera-Vives, G., Clocchiatti, A., de Jaeger, Th., Estévez, P. A., Galbany, L., González-Gaitán, S., Gräfener, G., Hamuy, M., Hsiao, E., Huentelemu, P., Huijse, P., Kuncarayakti, H., Martínez-Palomera, J., Medina, G., E., F. Olivares, Pignata, G., Razza, A., Reyes, I., Martín, J. San, Smith, R. C., Vera, E., Vivas, A. K., Postigo, A. de Ugarte, Yoon, S. -C., Ashall, C., Fraser, M., Gal-Yam, A., Kankare, E., Guillou, L. Le, Mazzali, P. A., Walton, N. A., Young, D. R.
Publikováno v:
Nature Astronomy, 2018
Type II supernovae (SNe) originate from the explosion of hydrogen-rich supergiant massive stars. Their first electromagnetic signature is the shock breakout, a short-lived phenomenon which can last from hours to days depending on the density at shock
Externí odkaz:
http://arxiv.org/abs/1809.06379
Autor:
Gutiérrez, C. P., Anderson, J. P., Sullivan, M., Dessart, L., González-Gaitán, S., Galbany, L., Dimitriadis, G., Arcavi, I., Bufano, F., Chen, T. -W., Dennefeld, M., Gromadzki, M., Haislip, J. B., Hosseinzadeh, G., Howell, D. A., Inserra, C., Kankare, E., Leloudas, G., Maguire, K., McCully, C., Morrell, N., E., F. Olivares, Pignata, G., Reichart, D. E., Reynolds, T., Smartt, S. J., Sollerman, J., Taddia, F., Takáts, K., Terreran, G., Valenti, S., Young, D. R.
We present an analysis of a new sample of type II core-collapse supernovae (SNe II) occurring within low-luminosity galaxies, comparing these with a sample of events in brighter hosts. Our analysis is performed comparing SN II spectral and photometri
Externí odkaz:
http://arxiv.org/abs/1806.03855