Results 71 to 80 of about 176,448 (289)
Euclid
Astronomy & AstrophysicsContext. The performance of the Euclid system is defined in terms of image quality metrics tuned to the weak gravitational lensing cosmological probe.Anselmi A., Laureijs R., Racca G. D., Costa G., Courcould Mifsud L., Cuillandre J.-C., Gottero M., Hoekstra H., Kuijken K., Mareschi V., Miller L., Mottini S., Stramaccioni D., Altieri B., Amara A., Andreon S., Auricchio N., Baccigalupi C., Baldi M., Balestra A., Bardelli S., Bender R., Biviano A., Branchini E., Brescia M., Camera S., Cañas-Herrera G., Capobianco V., Carbone C., Carretero J., Castellano M., Castignani G., Cavuoti S., Cimatti A., Colodro-Conde C., Congedo G., Conselice C. J., Conversi L., Copin Y., Courbin F., Courtois H. M., Cropper M., Da Silva A., Degaudenzi H., De Lucia G., Dole H., Dubath F., Ducret F., Duncan C. A. J., Dupac X., Dusini S., Escoffier S., Fabricius M., Farina M., Farinelli R., Faustini F., Ferriol S., Finelli F., Fourmanoit N., Frailis M., Franceschi E., Fumana M., Galeotta S., George K., Gillis B., Giocoli C., Gracia-Carpio J., Grazian A., Grupp F., Haugan S. V. H., Hoar J., Holmes W., Hormuth F., Hornstrup A., Jahnke K., Jhabvala M., Keihänen E., Kermiche S., Kiessling A., Kohley R., Kubik B., Kunz M., Kurki-Suonio H., Le Brun A. M. C., Ligori S., Lilje P. B., Lindholm V., Lloro I., Mainetti G., Maino D., Maiorano E., Mansutti O., Marggraf O., Martinelli M., Martinet N., Marulli F., Massey R. J., Medinaceli E., Mei S., Mellier Y., Meneghetti M., Merlin E., Meylan G., Mora A., Moresco M., Moscardini L., Nakajima R., Neissner C., Nichol R. C., Niemi S.-M., Padilla C., Paltani S., Pasian F., Pedersen K., Percival W. J., Pettorino V., Pires S., Polenta G., Poncet M., Popa L. A., Raison F., Rebolo R., Renzi A., Rhodes J., Riccio G., Romelli E., Roncarelli M., Rosset C., Rossetti E., Saglia R., Sakr Z., Salvignol J.-C., Sánchez A. G., Sapone D., Sartoris B., Schirmer M., Schneider P., Schrabback T., Secroun A., Seidel G., Serrano S., Sirignano C., Sirri G., Skottfelt J., Stanco L., Steinwagner J., Tallada-Crespí P., Tavagnacco D., Taylor A. N., Teplitz H. I., Tereno I., Tessore N., Toft S., Toledo-Moreo R., Torradeflot F., Tutusaus I., Valentijn E. A., Valenziano L., Valiviita J., Vassallo T., Verdoes Kleijn G., Veropalumbo A., Wang Y., Weller J., Zacchei A., Zamorani G., Zucca E., Ballardini M., Bolzonella M., Bozzo E., Burigana C., Cabanac R., Cappi A., Escartin Vigo J. A., Gabarra L., Hartley W. G., Martín-Fleitas J., Matthew S., Mauri N., Metcalf R. B., Pezzotta A., Pöntinen M., Risso I., Scottez V., Sereno M., Tenti M., Viel M., Wiesmann M., Akrami Y., Andika I. T., Anselmi S., Archidiacono M., Atrio-Barandela F., Bertacca D., Bethermin M., Blanchard A., Blot L., Bonici M., Borgani S., Brown M. L., Bruton S., Calabro A., Camacho Quevedo B., Caro F., Carvalho C. S., Castro T., Cogato F., Conseil S., Cooray A. R., Cucciati O., Davini S., Desprez G., Díaz-Sánchez A., Diaz J. J., Di Domizio S., Diego J. M., Elkhashab M. Y., Enia A., Fang Y., Ferrari A. G., Finoguenov A., Franco A., Ganga K., García-Bellido J., Gasparetto T., Gaztanaga E., Giacomini F., Gianotti F., Gozaliasl G., Guidi M., Gutierrez C. M., Hall A., Hildebrandt H., Hjorth J., Kajava J. J. E., Kang Y., Kansal V., Karagiannis D., Kiiveri K., Kim J., Kirkpatrick C. C., Kruk S., Le Graet J., Legrand L., Lembo M., Lepori F., Leroy G., Lesci G. F., Lesgourgues J., Leuzzi L., Liaudat T. I., Liu S. J., Loureiro A., Macias-Perez J., Magliocchetti M., Mannucci F., Maoli R., Martins C. J. A. P., Maurin L., Miluzio M., Monaco P., Montoro A., Moretti C., Morgante G., Nadathur S., Naidoo K., Navarro-Alsina A., Nesseris S., Paoletti D., Passalacqua F., Paterson K., Patrizii L., Pisani A., Potter D., Quai S., Radovich M., Sacquegna S., Sahlén M., Sanders D. B., Sarpa E., Schneider A., Sciotti D., Sellentin E., Smith L. C., Tanidis K., Testera G., Teyssier R., Tosi S., Troja A., Tucci M., Valieri C., Venhola A., Vergani D., Verza G., Vielzeuf P., Walton N. A. +295 moredoaj +1 more sourceBlack Holes at Neutrino Telescopes
, 2002 In scenarios with extra dimensions and TeV-scale quantum gravity, black holes
are expected to be produced in the collision of light particles at
center-of-mass energies above the fundamental Planck scale with small impact
parameters.'t Hooft, 't Hooft, A. Ringwald, Abe, Alvarez-Muniz, Alvarez-Muniz, Amati, Amati, Amati, Amati, Amati, Amati, Anchordoqui, Anchordoqui, Andres, Antoniadis, Aref'eva, Aref'eva, Aref'eva, Argyres, Arkani-Hamed, Arkani-Hamed, Bahcall, Balkanov, Baltrusaitis, Baltrusaitis, Banks, Berezinsky, Berezinsky, Berezinsky, Bleicher, Bugaev, Casadio, Cheung, Chiba, Cornwall, Dimopoulos, Dimopoulos, Eardley, Emparan, Emparan, Emparan, Engel, Espinosa, Fabbrichesi, Fargion, Feng, Fodor, Fodor, Gandhi, Gandhi, Gelmini, Gibbs, Giddings, Giddings, Giddings, Giudice, Giudice, Goldberg, Greisen, Grieder, Groom, H. Tu, Halzen, Hawking, Hawking, Hossenfelder, Hundertmark, Kalashev, Klinkhamer, Kravchenko, Lai, Landsberg, Learned, M. Kowalski, Mannheim, Mattis, McLerran, Montaruli, Morris, Morris, Myers, Pagliarone, Park, Peskin, Plothow-Besch, Plothow-Besch, Plothow-Besch, Protheroe, Protheroe, Protheroe, Randall, Ringwald, Ringwald, Ringwald, Ringwald, Ringwald, Rizzo, Rubakov, Seckel, Tinyakov, Uehara, Voloshin, Voloshin, Voloshin, Waxman, Weiler, Yoshida, Yoshida, Yoshida, Yoshida, Zatsepin, Zavrtanik +112 morecore +1 more sourceHigh-resolution x-ray telescopes
, 2010 High-energy astrophysics is a relatively young scientific field, made
possible by space-borne telescopes. During the half-century history of x-ray
astronomy, the sensitivity of focusing x-ray telescopes-through finer angular
resolution and increased ...Brissenden, R. J., Davis, W. N., Elsner, R. F., Elvis, M., Freeman, M., Gaetz, T., Gorenstein, P., Gubarev, M. V., Jerius, D., Juda, M., Kolodziejczak, J. J., Murray, S., O'Dell, S. L., Petre, R., Podgorski, W., Ramsey, B. D., Reid, P. B., Saha, T., Schwartz, D. A., Trolier-McKinstry, S., Weisskopf, M. C., Wilke, R. H. T., Wolk, S., Zhang, W. W. +23 morecore +1 more sourceListening to Hong Kong children's perspectives through pretend play
British Educational Research Journal, EarlyView.Abstract
Quality in early childhood education and care (ECEC) has become an increasing concern in recent years. The issue has been regularly discussed by different stakeholders. However, the rising concern regarding quality in ECEC has not seriously taken into account children's perspectives.Suzannie K. Y. Leungwiley +1 more sourceHidden O‐Deglycosylation Activity Triggers O → C Rearrangement for Aryl Di‐C‐Glucoside Formation by the C‐Glycosyltransferase From Fortunella crassifolia
Biotechnology and Bioengineering, EarlyView.Here, we uncovered an unexpected O‐deglycosylation activity of the C glycosyltransferase (FcCGT), forming phloretin (1) from phloretin 2'‐O‐glucoside (2). In the presence of UDP, FcCGT catalyzes the O→C rearrangement to yield nothofagin (3). Upon additional UDP‐glucose, further C‐glycosylation occurs, forming phloretin 3',5'‐di‐C‐glucoside (4 ...Tuo Li, Annika J. E. Borg, Leo Krammer, Rolf Breinbauer, Bernd Nidetzky +4 morewiley +1 more source