Zobrazeno 1 - 10
of 66
pro vyhledávání: '"pez, A"'
In recent times, the Scalar Field Dark Matter (SFDM) model (also called Fuzzy, Wave, Ultralight dark matter model) has received much attention due to its success in describing dark matter on both cosmological and galactic scales. Several challenges o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::46f84fe816f21f453bfb6e228270fb25
http://arxiv.org/abs/2203.13218
http://arxiv.org/abs/2203.13218
Autor:
Ohashi, Satoshi, Codella, Claudio, Sakai, Nami, Chandler, Claire J., Ceccarelli, Cecilia, Alves, Felipe, Fedele, Davide, Hanawa, Tomoyuki, Dur��n, Aurora, Favre, C��cile, L��pez-Sepulcre, Ana, Loinard, Laurent, Mercimek, Seyma, Murillo, Nadia M., Podio, Linda, Zhang, Yichen, Aikawa, Yuri, Balucani, Nadia, Bianchi, Eleonora, Bouvier, Mathilde, Busquet, Gemma, Caselli, Paola, Caux, Emmanuel, Charnley, Steven, Choudhury, Spandan, Cuello, Nicolas, De Simone, Marta, Dulieu, Francois, Evans, Lucy, Feng, Siyi, Fontani, Francesco, Francis, Logan, Hama, Tetsuya, Herbst, Eric, Hirano, Shingo, Hirota, Tomoya, Imai, Muneaki, Isella, Andrea, J��menez-Serra, Izaskun, Johnstone, Doug, Kahane, Claudine, Gal, Romane Le, Lefloch, Bertrand, Maud, Luke T., Maureira, Maria Jose, Menard, Francois, Miotello, Anna, Moellenbrock, George, Mori, Shoji, Nakatani, Riouhei, Nomura, Hideko, Oba, Yasuhiro, O'Donoghue, Ross, Okoda, Yuki, Ospina-Zamudio, Juan, Oya, Yoko, Pineda, Jaime, Rimola, Albert, Sakai, Takeshi, Segura-Cox, Dominique, Shirley, Yancy, Svoboda, Brian, Taquet, Vianney, Testi, Leonardo, Vastel, Charlotte, Viti, Serena, Watanabe, Naoki, Watanabe, Yoshimasa, Witzel, Arezu, Xue, Ci, Zhao, Bo, Yamamoto, Satoshi
We report a study of the low-mass Class-0 multiple system VLA 1623AB in the Ophiuchus star-forming region, using H$^{13}$CO$^+$ ($J=3-2$), CS ($J=5-4$), and CCH ($N=3-2$) lines as part of the ALMA Large Program FAUST. The analysis of the velocity fie
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6e22562fec4f5937745bde2766d55ab5
http://arxiv.org/abs/2201.07334
http://arxiv.org/abs/2201.07334
Autor:
MAGIC Collaboration, Acciari, V. A., Ansoldi, S., Antonelli, L. A., Engels, A. Arbet, Artero, M., Asano, K., Baack, D., Babi��, A., Baquero, A., de Almeida, U. Barres, Barrio, J. A., Batkovi��, I., Gonz��lez, J. Becerra, Bednarek, W., Bellizzi, L., Bernardini, E., Bernardos, M., Berti, A., Besenrieder, J., Bhattacharyya, W., Bigongiari, C., Biland, A., Blanch, O., Bonnoli, G., Bo��njak, ��., Busetto, G., Carosi, R., Ceribella, G., Cerruti, M., Chai, Y., Chilingarian, A., Cikota, S., Colak, S. M., Colombo, E., Contreras, J. L., Cortina, J., Covino, S., D'Amico, G., D'Elia, V., Da Vela, P., Dazzi, F., De Angelis, A., De Lotto, B., Delfino, M., Delgado, J., Mendez, C. Delgado, Depaoli, D., Di Pierro, F., Di Venere, L., Espi��eira, E. Do Souto, Prester, D. Dominis, Donini, A., Dorner, D., Doro, M., Elsaesser, D., Ramazani, V. Fallah, Fattorini, A., Ferrara, G., Fonseca, M. V., Font, L., Fruck, C., Fukami, S., L��pez, R. J. Garc��a, Garczarczyk, M., Gasparyan, S., Gaug, M., Giglietto, N., Giordano, F., Gliwny, P., Godinovi��, N., Green, J. G., Green, D., Hadasch, D., Hahn, A., Heckmann, L., Herrera, J., Hoang, J., Hrupec, D., H��tten, M., Inada, T., Inoue, S., Ishio, K., Iwamura, Y., Jim��nez, I., Jormanainen, J., Jouvin, L., Kajiwara, Y., Karjalainen, M., Kerszberg, D., Kobayashi, Y., Kubo, H., Kushida, J., Lamastra, A., Lelas, D., Leone, F., Lindfors, E., Lombardi, S., Longo, F., L��pez-Coto, R., L��pez-Moya, M., L��pez-Oramas, A., Loporchio, S., Fraga, B. Machado de Oliveira, Maggio, C., Majumdar, P., Makariev, M., Mallamaci, M., Maneva, G., Manganaro, M., Mannheim, K., Maraschi, L., Mariotti, M., Mart��nez, M., Mazin, D., Menchiari, S., Mender, S., Mi��anovi��, S., Miceli, D., Miener, T., Minev, M., Miranda, J. M., Mirzoyan, R., Molina, E., Moralejo, A., Morcuende, D., Moreno, V., Moretti, E., Neustroev, V., Nigro, C., Nilsson, K., Nishijima, K., Noda, K., Nozaki, S., Ohtani, Y., Oka, T., Otero-Santos, J., Paiano, S., Palatiello, M., Paneque, D., Paoletti, R., Paredes, J. M., Pavleti��, L., Pe��il, P., Perennes, C., Persic, M., Moroni, P. G. Prada, Prandini, E., Priyadarshi, C., Puljak, I., Rhode, W., Rib��, M., Rico, J., Righi, C., Rugliancich, A., Saha, L., Sahakyan, N., Saito, T., Sakurai, S., Satalecka, K., Saturni, F. G., Schleicher, B., Schmidt, K., Schweizer, T., Sitarek, J., ��nidari��, I., Sobczynska, D., Spolon, A., Stamerra, A., Strom, D., Strzys, M., Suda, Y., Suri��, T., Takahashi, M., Tavecchio, F., Temnikov, P., Terzi��, T., Teshima, M., Tosti, L., Truzzi, S., Tutone, A., Ubach, S., van Scherpenberg, J., Vanzo, G., Acosta, M. Vazquez, Ventura, S., Verguilov, V., Vigorito, C. F., Vitale, V., Vovk, I., Will, M., Wunderlich, C., Zari��, D., de Palma, F., D'Ammando, F., Barnacka, A., Sahu, D. K., Hodges, M., Hovatta, T., Kiehlmann, S., Max-Moerbeck, W., Readhead, A. C. S., Reeves, R., Pearson, T. J., L��hteenm��ki, A., Bj��rklund, I., Tornikoski, M., Tammi, J., Suutarinen, S., Hada, K., Niinuma, K.
Publikováno v:
Monthly notices of the Royal Astronomical Society 510(2), 2344-2362 (2022). doi:10.1093/mnras/stab3454
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society
V. A. Acciari et al.
We report multiwavelength observations of the gravitationally lensed blazar QSO B0218+357 in 2016–2020. Optical, X-ray, and GeV flares were detected. The contemporaneous MAGIC observations do not show significant very high
We report multiwavelength observations of the gravitationally lensed blazar QSO B0218+357 in 2016–2020. Optical, X-ray, and GeV flares were detected. The contemporaneous MAGIC observations do not show significant very high
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b37ea4c1b08287ba9fdc299a50253174
Autor:
L��pez-Guti��rrez, Martha M., Bravo-Alfaro, Hector, van Gorkom, Jacqueline H., Durret, Forence, Caretta, C��sar A.
We study complete sample of spiral galaxies brighter than M$_{\mathrm{B}} \sim$-18.4 in three Abell clusters: A85 ($z=\,$0.055), A496 ($z=\,$0.033) and A2670 ($z=\,$0.076). This work is based on a large volume limited, blind Hi-survey (21cm, NRAO-VLA
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8450193c150f12d99abd1affbd779f8f
http://arxiv.org/abs/2108.12495
http://arxiv.org/abs/2108.12495
Autor:
Spinoso, Daniele, Orsi, Alvaro, L��pez-Sanjuan, Carlos, Bonoli, Silvia, Viironen, Kerttu, Izquierdo-Villalba, David, Sobral, David, Gurung-L��pez, Siddhartha, Hern��n-Caballero, Antonio, Ederoclite, Alessandro, Varela, Jes��s, Overzier, Roderik, Miralda-Escud��, Jordi, Muniesa, David J., Alcaniz, Jailson, Angulo, Raul E., Cenarro, A. Javier, Crist��bal-Hornillos, David, Dupke, Renato A., Hern��ndez-Monteagudo, Carlos, Mar��n-Franch, Antonio, Moles, Mariano, Sodr��, Laerte, V��zquez-Rami��, H��ctor
We present the photometric determination of the bright-end (L_Lya>10^43.5 erg/s) of the Lya luminosity function (LF) within four redshifts windows in the interval 2.210^43.3 erg/s) Lya-emitting candidates. We test our selection with two spectroscopic
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1b93a5fd378b280abb6031a4a073edb5
Autor:
Cedr��s, Bernab��, Bongiovanni, ��ngel, Cervi��o, Miguel, Nadolny, Jakub, Cepa, Jordi, de Diego, Jos�� A., Garc��a, Ana Mar��a P��rez, Gallego, Jes��s, Lara-L��pez, Maritza A., S��nchez-Portal, Miguel, Gonz��lez-Serrano, J. Ignacio, Alfaro, Emilio J., Mart��nez, Roc��o Navarro, Mart��nez, Ricardo P��rez, Gonz��lez, J. Jes��s, Torres, Carmen P. Padilla, Casta��eda, H��ctor O., Gonz��lez, Mauro
In this paper, we aim to study the main properties and luminosity function (LF) of the [OII] emitters detected in the OTELO survey in order to characterise the star formation processes in low-mass galaxies at $z\sim1.43$ and to constrain the faint-en
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f86f2cc9ed09b53ed86f8aedd990ab28
http://arxiv.org/abs/2103.03645
http://arxiv.org/abs/2103.03645
Autor:
Hu, Weida, Wang, Junxian, Infante, Leopoldo, Rhoads, James E., Zheng, Zhen-Ya, Yang, Huan, Malhotra, Sangeeta, Barrientos, L. Felipe, Jiang, Chunyan, Gonz��lez-L��pez, Jorge, Prieto, Gonzalo, Perez, Lucia A., Hibon, Pascale, Galaz, Gaspar, Coughlin, Alicia, Harish, Santosh, Kong, Xu, Kang, Wenyong, Khostovan, Ali Ahmad, Pharo, John, Valdes, Francisco, Wold, Isak, Walker, Alistair R., Zheng, XianZhong
Protoclusters, the progenitors of the most massive structures in the Universe, have been identified at redshifts of up to 6.6. Besides exploring early structure formation, searching for protoclusters at even higher redshifts is particularly useful to
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::9454e716b19d17599ccb985a0c4e5412
Autor:
Wold, Isak G. B., Malhotra, Sangeeta, Rhoads, James, Wang, Junxian, Hu, Weida, Perez, Lucia A., Zheng, Zhen-Ya, Khostovan, Ali Ahmad, Walker, Alistair R., Barrientos, L. Felipe, Gonz��lez-L��pez, Jorge, Harish, Santosh, Infante, Leopoldo, Jiang, Chunyan, Pharo, John, Moya-Sierralta, Crist��bal, Bauer, Franz E., Galaz, Gaspar, Valdes, Francisco, Yang, Huan
We present a new measurement of the Ly$��$ luminosity function at redshift $z=6.9$, finding moderate evolution from $z=5.7$ that is consistent with a fully or largely ionized $z\sim7$ intergalactic medium. Our result is based on four fields of th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::cab9773b0b7b93c16df411bf159ad8b4
Autor:
Watson, Peter J., Davies, Roger L., Brough, Sarah, Croom, Scott M., D'Eugenio, Francesco, Glazebrook, Karl, Groves, Brent, L��pez-S��nchez, ��ngel R., van de Sande, Jesse, Scott, Nicholas, Vaughan, Sam P., Walcher, Jakob, Bland-Hawthorn, Joss, Bryant, Julia J., Goodwin, Michael, Lawrence, Jon S., Lorente, Nuria P. F., Owers, Matt S., Richards, Samuel
We present a new set of index-based measurements of [$��$/Fe] for a sample of 2093 galaxies in the SAMI Galaxy Survey. Following earlier work, we fit a global relation between [$��$/Fe] and the galaxy velocity dispersion $��$ for red sequ
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e547d2a1494619fd53e74fda1e3f411e
Recent studies of warp kinematics using Gaia DR2 data have produced detections of warp precession for the first time, which greatly exceeds theoretical predictions of models. However, this detection assumes a warp model derived for a young population
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::799f2d527273b6175f20a094c670746a