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Statistical methods in weak gravitational lensing [PDF]
, 2015 This thesis studies several topics in the area of weak gravitational lensing and addresses some key statistical problems within this subject. A large part of the thesis concerns the measurement of galaxy shapes for weak gravitational lensing and the ...Kacprzak, Tcore How Many Worlds Could There Be? David Lewis and Advanced Modalizing
Analytic Philosophy, EarlyView.ABSTRACT
Advanced modalizing, namely, possibilities and necessities concerning modal space itself, is problematic for a Lewis‐style analysis of modality. A popular solution, proposed by Divers, postulates explicit semantic clauses for a collapse of advanced modalizing, to the conclusion that all such matters are, if true in the first place, both ...Lorenzo Azzano, Ciro De Florio, Aldo Frigerio +2 morewiley +1 more sourceThe S-PLUS Fornax Project (S+FP): Fornax-like clusters in cosmological hydrodynamical simulations
Astronomy & AstrophysicsContext. The Fornax cluster, the second-nearest rich galaxy cluster, constitutes a suitable laboratory to explore the evolution of galaxies in a dense environment.Zenocratti L. J., Smith Castelli A. V., De Rossi M. E., Pallero D., Artale M. C., Haack R. F., Lopes A. R., Faifer F. R., Palma D., Humire P. K., Thainá-Batista J., Schoenell W., Ribeiro T., Kanaan A., Mendes de Oliveira C. +14 moredoaj +1 more sourceBerryBox: An affordable computer vision system for postharvest phenotyping of cranberry and other small fruits
The Plant Phenome Journal, Volume 9, Issue 1, December 2026.Abstract
Fruit size, shape, color, and percent fruit rot are important quality traits for breeding cranberry (Vaccinium macrocarpon Ait.). Image analysis can be used to measure these traits, but affordable hardware for standardized image capture and integrated user‐friendly software pipelines are lacking.Jeffrey L. Neyhart, Collins Wakholi, Devin A. Rippner, John H. Price, Kayla R. Altendorf, Garett C. Heineck, Juan Zalapa, Jenyne Loarca, Gina M. Sideli +8 morewiley +1 more sourceEuclid 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 sourceThe Role of Cluster Environments in Quiescent Galaxy Stellar Halo Assembly
The Astrophysical JournalExternal interactions drive galaxy stellar mass growth and morphological evolution. As stellar halos—assembled largely via hierarchical accretion—preserve signatures of these processes, their growth probes how environment regulates galaxy evolution.Devin J. Williams, Ivana Damjanov, Marcin Sawicki, Harrison Souchereau, Lingjian Chen, Guillaume Desprez, Angelo George, Stephen Gwyn, Stéphane Arnouts +8 moredoaj +1 more sourceLyman continuum escaping from in situ formed stars in a tidal bridge at z = 3
Astronomy & AstrophysicsWe present an analysis of archival JWST NIRSpec IFS and HST imaging observations of the z = 3 Lyman continuum emitter (LCE) candidate LACES104037. We show that a nearby galaxy, denoted LACES104037-S, has a redshift offset from the main galaxy by only ...Rivera-Thorsen T. E., Le Reste A., Hayes M. J., Flury S., Saldana-Lopez A., Welch B., Choe S. C., Sharon K., Kim K., Owens M. R., Solhaug E., Dahle H., Rigby J. R., Melinder J. +13 moredoaj +1 more sourceExploring the Potential of Unmanned Aerial System‐Based Topographic Indices Maps to Evaluate Storm Drain Positioning
Journal of Flood Risk Management, Volume 19, Issue 4, December 2026.ABSTRACT
Urbanisation, climate uncertainty, and limited city budgets have heightened the need for efficient urban drainage management. While advanced hydrodynamic models assess the performance of drainage networks, they are computationally intensive, time‐consuming, and expensive.Rakhee Ramachandran, Yadira Bajón‐Fernández, Ian Truckell, Mónica Rivas Casado +3 morewiley +1 more source
