Results 121 to 130 of about 12,615 (238)
Euclid Quick Data Release (Q1)
Astronomy & AstrophysicsThe matter around galaxy clusters is distributed over several filaments, reflecting their positions as nodes in the large-scale cosmic web. The number of filaments connected to a cluster, i.e.Gouin C., Laigle C., Sarron F., Bonnaire T., Sorce J. G., Aghanim N., Magliocchetti M., Quilley L., Boldrini P., Durret F., Pichon C., Kuchner U., Malavasi N., Kraljic K., Gavazzi R., Kang Y., Stanford S. A., Awad P., Altieri B., Amara A., Andreon S., Auricchio N., Aussel H., Baccigalupi C., Baldi M., Balestra A., Bardelli S., Basset A., Battaglia P., Bernardeau F., Biviano A., Bonchi A., Branchini E., Brescia M., Brinchmann J., Camera S., Cañas-Herrera G., Capobianco V., Carbone C., Carretero J., Castellano M., Castignani G., Cavuoti S., Chambers K. C., 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 la Torre S., De Lucia G., Di Giorgio A. M., Dolding C., Dole H., Dubath F., Duncan C. A. J., Dupac X., Ealet A., Escoffier S., Fabricius M., Farina M., Faustini F., Ferriol S., Finelli F., Fotopoulou S., Frailis M., Franceschi E., Galeotta S., George K., Gillis B., Giocoli C., Gómez-Alvarez P., Gracia-Carpio J., Granett B. R., Grazian A., Grupp F., Gwyn S., Haugan S. V. H., Holmes W., Hook I. M., Hormuth F., Hornstrup A., Hudelot P., Jahnke K., Jhabvala M., Joachimi B., Keihänen E., Kermiche S., Kiessling A., Kilbinger M., Kubik B., Kümmel M., Kunz M., Kurki-Suonio H., Lahav O., Le Boulc’h Q., Le Brun A. M. C., Le Mignant D., Liebing P., Ligori S., Lilje P. B., Lindholm V., Lloro I., Mainetti G., Maino D., Maiorano E., Mansutti O., Marcin S., Marggraf O., Martinelli M., Martinet N., Marulli F., Massey R., Maurogordato S., McCracken H. J., Medinaceli E., Mei S., Mellier Y., Meneghetti M., Merlin E., Meylan G., Mora A., Moresco M., Moscardini L., Nakajima R., Neissner C., Niemi S.-M., Nightingale J. W., Padilla C., Paltani S., Pasian F., Peacock J. A., Pedersen K., Percival W. J., Pettorino V., Pires S., Polenta G., Poncet M., Popa L. A., Pozzetti L., Raison F., Rebolo R., Renzi A., Rhodes J., Riccio G., Romelli E., Roncarelli M., Rusholme B., Saglia R., Sakr Z., Sánchez A. G., Sapone D., Sartoris B., Schewtschenko J. A., Schirmer M., Schneider P., Schrabback T., Scodeggio M., Secroun A., Seidel G., Serrano S., Simon P., 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., Tsyganov A., Tutusaus I., Valenziano L., Valiviita J., Vassallo T., Verdoes Kleijn G., Veropalumbo A., Wang Y., Weller J., Zacchei A., Zamorani G., Zerbi F. M., Zucca E., Allevato V., Ballardini M., Bolzonella M., Bozzo E., Burigana C., Cabanac R., Cappi A., Di Ferdinando D., Escartin Vigo J. A., Gabarra L., Huertas-Company M., Martín-Fleitas J., Matthew S., Maturi M., Mauri N., Metcalf R. B., Pezzotta A., Pöntinen M., Porciani C., Risso I., Scottez V., Sereno M., Tenti M., Viel M., Wiesmann M., Akrami Y., Alvi S., Andika I. T., Anselmi S., Archidiacono M., Atrio-Barandela F., Balaguera-Antolinez A., Benoist C., Benson K., Bergamini P., Bertacca D., Bethermin M., Blanchard A., Blot L., Böhringer H., Brown M. L., Bruton S., Calabro A., Camacho Quevedo B., Caro F., Carvalho C. S., Castro T., Cogato F., Cooray A. R., Cucciati O., Davini S., De Paolis F., Desprez G., Díaz-Sánchez A., Diaz J. J., Di Domizio S., Diego J. M., Duc P.-A., Enia A., Fang Y., Ferrari A. G., Ferreira P. G., Finoguenov A., Fontana A., Franco A., Ganga K., García-Bellido J., Gasparetto T., Gautard V., Gaztanaga E., Giacomini F., Gianotti F., Gozaliasl G., Guidi M., Gutierrez C. M., Hall A., Hartley W. G., Hemmati S., Hernández-Monteagudo C., Hildebrandt H., Hjorth J., Kajava J. J. E., Kansal V., Karagiannis D., Kiiveri K., 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., Loureiro A., Macias-Perez J., Maggio G., Magnier E. A., Mannucci F., Maoli R., Martins C. J. A. P., Maurin L., Migliaccio M., Miluzio M., Monaco P., Montoro A., Moretti C., Morgante G., Nadathur S., Naidoo K., Navarro-Alsina A., Nesseris S., 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., Scognamiglio D., Sellentin E., Shankar F., 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., Scott D. +338 moredoaj +1 more sourceVisual Icons
Philosophy and Phenomenological Research, EarlyView.ABSTRACT
Philosophers often characterize perception as image‐like. There is little agreement, however, about what constitutes an imagistic or iconic representation. This article identifies five signature properties of iconic representations endorsed in the philosophical and scientific literature: item‐richness, feature‐richness, spatiotemporal ...Jake Quilty‐Dunnwiley +1 more sourceHerS-3: An Exceptional Einstein Cross Reveals a Massive Dark Matter Halo
The Astrophysical JournalWe present a study of HerS-3, a dusty star-forming galaxy at z _spec = 3.0607, which is gravitationally amplified into an Einstein cross with a fifth image of the background galaxy seen at the center of the cross.P. Cox, K. M. Butler, C. R. Keeton, L. Eid, E. Borsato, T. J. L. C. Bakx, R. Neri, B. M. Jones, P. Prajapati, A. J. Baker, S. Berta, A. Cooray, E. M. Corsini, L. Marchetti, A. Omont, A. Beelen, R. Gavazzi, D. Ismail, R. J. Ivison, M. Krips, M. D. Lehnert, H. Messias, D. Riechers, C. Vlahakis, A. Weiss, P. van der Werf, C. Yang +26 moredoaj +1 more sourceThe Problem of Psychonomic Harmony
Philosophy and Phenomenological Research, EarlyView.ABSTRACT
The problem of nomological harmony is the problem of explaining why the laws of nature match or apply to the states of the universe in a way that results in temporal evolution. The problem of psychophysical harmony is the problem of explaining why phenomenal states are paired with physical states and other phenomenal states in surprisingly ...Joseph C. Schmidwiley +1 more sourceDeath, Deprivation, and the Symmetry Problem
Ratio, EarlyView.ABSTRACT
According to the deprivation account of the badness of death, death is bad for the one who dies because it deprives her of goods she would otherwise have enjoyed. This view faces the so‐called symmetry problem when one considers prenatal nonexistence. Scholars have proposed various solutions to this problem, but all of them encounter their own Ryota Ishiharawiley +1 more sourceEnvironmental history of filament galaxies
Astronomy & AstrophysicsGalaxy properties, such as stellar mass and star formation rate, correlate with their position within the cosmic web. Although galaxy properties can be correlated with a specific environment at a certain cosmic epoch, they may have experienced different ...Zakharova D., De Lucia G., Vulcani B., Fontanot F., Xie L. +4 moredoaj +1 more source
