Zobrazeno 1 - 10
of 59
pro vyhledávání: '"Ferguson, H"'
Autor:
Vega-Ferrero, J., Huertas-Company, M., Costantin, L., Pérez-González, P. G., Sarmiento, R., Kartaltepe, J. S., Pillepich, A., Bagley, M. B., Finkelstein, S. L., McGrath, E. J., Knapen, J. H., Haro, P. Arrabal, Bell, E. F., Buitrago, F., Calabrò, A., Dekel, A., Dickinson, M., Sánchez, H. Domínguez, Elbaz, D., Ferguson, H. C., Giavalisco, M., Holwerda, B. W., Kocesvski, D. D., Koekemoer, A. M., Pandya, V., Papovich, C., Pirzkal, N., Primack, J., Yung, L. Y. Aaron
Visual inspections of the first optical rest-frame images from JWST have indicated a surprisingly high fraction of disk galaxies at high redshifts. Here we alternatively apply self-supervised machine learning to explore the morphological diversity at
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b54227202e8e8e05c9a5bdfa92f4a708
http://arxiv.org/abs/2302.07277
http://arxiv.org/abs/2302.07277
Autor:
Abratenko, P, Aduszkiewicz, A, Akbar, F, Pons, M Artero, Asaadi, J, Aslin, M, Babicz, M, Badgett, W F, Bagby, L F, Baibussinov, B, Behera, B, Bellini, V, Beltramello, O, Benocci, R, Berger, J, Berkman, S, Bertolucci, S, Bertoni, R, Betancourt, M, Bettini, M, Biagi, S, Biery, K, Bitter, O, Bonesini, M, Boone, T, Bottino, B, Braggiotti, A, Brailsford, D, Bremer, J, Brice, S J, Brio, V, Brizzolari, C, Brown, J, Budd, H S, Calaon, F, Campani, A, Carber, D, Carneiro, M, Terrazas, I Caro, Carranza, H, Casazza, D, Castellani, L, Castro, A, Centro, S, Cerati, G, Chalifour, M, Chambouvet, P, Chatterjee, A, Cherdack, D, Cherubini, S, Chithirasreemadam, N, Cicerchia, M, Cicero, V, Coan, T, Cocco, A G, Convery, M R, Copello, S, Cristaldo, E, Dange, A A, de Icaza Astiz, I, De Roeck, A, Di Domizio, S, Di Noto, L, Di Stefano, C, Di Ferdinando, D, Diwan, M, Dolan, S, Domine, L, Donati, S, Doubnik, R, Drielsma, F, Dyer, J, Dytman, S, Fabre, C, Fabris, F, Falcone, A, Farnese, C, Fava, A, Ferguson, H, Ferrari, A, Ferraro, F, Gallice, N, Garcia, F G, Geynisman, M, Giarin, M, Gibin, D, Gigli, S G, Gioiosa, A, Gu, W, Guerzoni, M, Guglielmi, A, Gurung, G, Hahn, S, Hardin, K, Hausner, H, Heggestuen, A, Hilgenberg, C, Hogan, M, Howard, B, Howell, R, Hrivnak, J, Iliescu, M, Ingratta, G, James, C, Jang, W, Jung, M, Jwa, Y-J, Kashur, L, Ketchum, W, Kim, J S, Koh, D-H, Kose, U, Larkin, J, Laurenti, G, Lukhanin, G, Marchini, S, Marshall, C M, Martynenko, S, Mauri, N, Mazzacane, A, Mcfarland, K S, Méndez, D P, Menegolli, A, Meng, G, Miranda, O G, Mladenov, D, Mogan, A, Moggi, N, Montagna, E, Montanari, C, Montanari, A, Mooney, M, Moreno-Granados, G, Mueller, J, Naples, D, Nebot-Guinot, M, Nessi, M, Nichols, T, Nicoletto, M, Norris, B, Palestini, S, Pallavicini, M, Paolone, V, Papaleo, R, Pasqualini, L, Patrizii, L, Peghin, R, Petrillo, G, Petta, C, Pia, V, Pietropaolo, F, Poirot, J, Poppi, F, Pozzato, M, Prata, M C, Prosser, A, Putnam, G, Qian, X, Rampazzo, G, Rappoldi, A, Raselli, G L, Rechenmacher, R, Resnati, F, Ricci, A M, Riccobene, G, Rice, L, Richards, E, Rigamonti, A, Rosenberg, M, Rossella, M, Rubbia, C, Sala, P, Sapienza, P, Savage, G, Scaramelli, A, Scarpelli, A, Schmitz, D, Schukraft, A, Sergiampietri, F, Sirri, G, Smedley, J S, Soha, A K, Spanu, M, Stanco, L, Stewart, J, Suarez, N B, Sutera, C, Tanaka, H A, Tenti, M, Terao, K, Terranova, F, Togo, V, Torretta, D, Torti, M, Tortorici, F, Tosi, N, Tsai, Y-T, Tufanli, S, Turcato, M, Usher, T, Varanini, F, Ventura, S, Vercellati, F, Vicenzi, M, Vignoli, C, Viren, B, Warner, D, Williams, Z, Wilson, R J, Wilson, P, Wolfs, J, Wongjirad, T, Wood, A, Worcester, E, Worcester, M, Wospakrik, M, Yu, H, Yu, J, Zani, A, Zatti, P G, Zennamo, J, Zettlemoyer, J C, Zhang, C, Zucchelli, S, Zuckerbrot, M
Publikováno v:
arXiv
European Physical Journal
INSPIRE-HEP
European Physical Journal
INSPIRE-HEP
The ICARUS collaboration employed the 760-ton T600 detector in a successful 3-year physics run at the underground LNGS laboratory, performing a sensitive search for LSND-like anomalous $\nu _e$ appearance in the CERN Neutrino to Gran Sasso beam, whic
Autor:
Yang, G., Caputi, K. I., Papovich, C., Haro, P. Arrabal, Bagley, M. B., Behroozi, P., Bell, E. F., Bisigello, L., Buat, V., Burgarella, D., Cheng, Y., Cleri, N. J., Dave, R., Dickinson, M., Elbaz, D., Ferguson, H. C., Finkelstein, S. L., Grogin, N. A., Hathi, N. P., Hirschmann, M., Holwerda, B. W., Huertas-Company, M., Hutchison, T., Iani, E., Kartaltepe, J. S., Kirkpatrick, A., Kocevski, D. D., Koekemoer, A. M., Kokorev, V., Larson, R. L., Lucas, R. A., Perez-Gonzalez, P. G., Rinaldi, P., Shen, L., Trump, J. R., de la Vega, A., Yung, L. Y. A., Zavala, J. A.
Mid-infrared observations are powerful in identifying heavily obscured Active Galactic Nuclei (AGN) which have weak emission in other wavelengths. Data from the Mid-Infrared Instrument (MIRI) onboard JWST provides an excellent opportunity to perform
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3ddc9f783f19e3fb11dadd2da366ee58
Autor:
Chary, R., Helou, G., Brammer, G., Capak, P., Faisst, A., Flynn, D., Groom, S., Ferguson, H. C., Grillmair, C., Hemmati, S., Koekemoer, A., Lee, B., Malhotra, S., Miyatake, H., Melchior, P., Momcheva, I., Newman, J., Masiero, J., Paladini, R., Prakash, A., Rusholme, B., Stickley, N. R., Smith, A., Wood-Vasey, W. M., Teplitz, H. I.
The Euclid, Rubin/LSST and Roman (WFIRST) projects will undertake flagship optical/near-infrared surveys in the next decade. By mapping thousands of square degrees of sky and covering the electromagnetic spectrum between 0.3 and 2 microns with sub-ar
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::58d09bb50ef35266d4c69957f56399fd
Autor:
Chary, R., Brammer, G., Capak, P., Dawson, W., Faisst, A., Fajardo-Acosta, S., Ferguson, H. C., Grillmair, C. J., Hemmati, S., Koekemoer, A., Lee, B., Lupton, R., Malhotra, S., Melchior, P., Momcheva, I., Newman, J., Masiero, J., Paladini, R., Prakash, A., Rhodes, J., Rusholme, B., Schneider, M., Stickley, N., Smith, A., Wood-Vasey, W. M., Berriman, G. B.
Joint survey processing (JSP) is the pixel level combination of LSST, Euclid, and WFIRST datasets. By combining the high spatial resolution of the space-based datasets with deep, seeing-limited, ground-based images in the optical bands, systematics l
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cfc9e620e973e989c86a578b6f83561f
Autor:
Foley, R. J., Koekemoer, A. M., Spergel, D. N., Bianco, F. B., Capak, P., Dai, L., Dore, O., Fazio, G. G., Ferguson, H., Filippenko, A. V., Frye, B., Galbany, L., Gawiser, E., Gronwall, C., Hathi, N. P., Hirata, C., Hounsell, R., Jha, S. W., Kim, A. G., Kelly, P. L., Kruk, J. W., Malhotra, S., Mandel, K. S., Margutti, R., Marrone, D., McQuinn, K. B. W., Melchior, P., Moustakas, L., Newman, J. A., Peek, J. E. G., Perlmutter, S., Rhodes, J. D., Robertson, B., Rubin, D., Scolnic, D., Somerville, R., Street, R., Wang, Y., Whalen, D. J., Windhorst, R. A., Wollack, E. J.
The Wide-Field Infrared Survey Telescope (WFIRST) is expected to launch in the mid-2020s. With its wide-field near-infrared (NIR) camera, it will survey the sky to unprecedented detail. As part of normal operations and as the result of multiple expec
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::52dfb2a1482564bb1d21bfd5efe56880
https://escholarship.org/uc/item/1rs528tc
https://escholarship.org/uc/item/1rs528tc
Autor:
Audcent-Ross, Fiona M., Meurer, Gerhardt R., Wong, O. I., Zheng, Z., Hanish, D., Zwaan, M. A., Bland-Hawthorn, J., Elagali, A., Meyer, M., Putman, M. E., Ryan-Webber, E. V., Sweet, S. M., Thilker, D. A., Seibert, M., Allen, R., Dopita, M. A., Doyle-Pegg, M. T., Drinkwater, M., Ferguson, H. C., Freeman, K. C., Heckman, T. M., Kennicutt, R. C., Kilborn, V. A., Kim, J. H., Knezek, P. M., Koribalski, B., Smith, R. C., Staveley-Smith, L., Webster, R. L., Werk, J. K.
For the first time both H$��$ and far-ultraviolet (FUV) observations from an HI-selected sample are used to determine the dust-corrected star formation rate density (SFRD: $\dot��$) in the local Universe. Applying the two star formation rate
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::be86ec439dfaf824d17a69c10ed7811c
Autor:
Giavalisco, M., Ferguson, H. C., Koekemoer, A. M., Dickinson, M., Alexander, D. M., Bauer, F. E., Bergeron, J., Biagetti, C., Brandt, W. N., Casertano, S., Cesarsky, C., Chatzichristou, E., Conselice, C., Stefano Cristiani, Da Costa, L., Dahlen, T., Mello, D., Eisenhardt, P., Erben, T., Fall, S. M., Fassnacht, C., Fosbury, R., Fruchter, A., Gardner, J. P., Grogin, N., Hook, R. N., Hornschemeier, A. E., Idzi, R., Jogee, S., Kretchmer, C., Laidler, V., Lee, K. S., Livio, M., Lucas, R., Madau, P., Mobasher, B., Moustakas, L. A., Nonino, M., Padovani, P., Papovich, C., Park, Y., Ravindranath, S., Renzini, A., Richardson, M., Riess, A., Rosati, P., Schirmer, M., Schreier, E., Somerville, R. S., Spinrad, H., Stern, D., Stiavelli, M., Strolger, L., Urry, C. M., Vandame, B., Williams, R., Wolf, C.
Publikováno v:
Scopus-Elsevier
CIÊNCIAVITAE
CIÊNCIAVITAE
This Special Issue of the Astrophysical Journal Letters is dedicated to presenting initial results from the Great Observatories Origins Deep Survey (GOODS) that are primarily, but not exclusively, based on multi--band imaging data obtained with the {
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::79992a6d3d3b803d6a823a7d2d89f53c
https://doi.org/10.1086/379232
https://doi.org/10.1086/379232
Autor:
Shu, X. W., Elbaz, D., Bourne, N., Schreiber, C., Wang, T., Dunlop, J. S., Fontana, A., Leiton, R., Pannella, M., Okumura, K., Michalowski, M. J., Santini, P., Merlin, E., Buitrago, F., Bruce, V. A., Amorin, R., Castellano, M., Derriere, S., Comastri, A., Cappelluti, N., Wang, J. X., Ferguson, H. C.
We present a new method to search for candidate z~>2 Herschel 500��m sources in the GOODS-North field, using a S500��m/S24��m "color deconfusion" technique. Potential high-z sources are selected against low-redshift ones from their large
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e4c657ff3877f643884d8b716af13ce5
Autor:
Wang, T., Elbaz, D., Schreiber, C., Pannella, M., Shu, X., Willner, S. P., Ashby, M. L. N., Huang, J. -S., Fontana, A., Dekel, A., Daddi, E., Ferguson, H. C., Dunlop, J., Ciesla, L., Koekemoer, A. M., Giavalisco, M., Boutsia, K., Finkelstein, S., Juneau, S., Barro, G., Koo, D. C., Micha��owski, M. J., Orellana, G., Lu, Y., Castellano, M., Bourne, N., Buitrago, F., Santini, P., Faber, S. M., Hathi, N., Lucas, R. A., P��rez-Gonz��lez, P. G.
We introduce a new color-selection technique to identify high-redshift, massive galaxies that are systematically missed by Lyman-break selection. The new selection is based on the H_{160} and IRAC 4.5um bands, specifically H - [4.5] > 2.25 mag. These
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::5832c513f6e2c129488da70be5ca8213