Results 101 to 110 of about 284,450 (301)
Euclid preparation
Astronomy & AstrophysicsThe Cosmic Dawn Survey pre-launch catalogues cover an effective 10.13 deg2 area with uniform deep Spitzer/IRAC data (m ∼ 25 mag, 5σ), the largest area covered to these depths at IR wavelengths.Zalesky L., Weaver J. R., McPartland C. J. R., Murphree G., Valdes I., Jespersen C. K., Taamoli S., Chartab N., Allen N., Barrow S. W. J., Sanders D. B., Toft S., Mobasher B., Szapudi I., Altieri B., Amara A., Andreon S., Auricchio N., Baccigalupi C., Baldi M., Bardelli S., Battaglia P., Biviano A., Bonino D., Branchini E., Brescia M., Brinchmann J., Caillat A., Camera S., Cañas-Herrera G., Capobianco V., Carbone C., Carretero J., Casas S., Castander F. 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., Da Silva A., Degaudenzi H., De Lucia G., Di Giorgio A. M., Dole H., Dubath F., Duncan C. A. J., Dupac X., Dusini S., Ealet A., Escoffier S., Farina M., Farinelli R., Farrens S., Faustini F., Ferriol S., Finelli F., Fosalba P., Fotopoulou S., Frailis M., Franceschi E., Fumana M., George K., Gillis B., Giocoli C., Gracia-Carpio J., Grazian A., Grupp F., Gwyn S., Haugan S. V. H., Holmes W., Hook I., Hormuth F., Hornstrup A., Jahnke K., Jhabvala M., Joachimi B., Keihänen E., Kermiche S., Kiessling A., Kubik B., Kuijken K., Kümmel M., Kunz M., Kurki-Suonio H., Le Brun A. M. C., Le Mignant D., Ligori S., Lilje P. B., Lindholm V., Lloro I., Mainetti G., Maino D., Maiorano E., Mansutti O., Marggraf O., Markovic K., 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., Pedersen K., Pettorino V., Polenta G., Poncet M., Popa L. A., Pozzetti L., Raison F., Rebolo R., Renzi A., Rhodes J., Riccio G., Romelli E., Roncarelli M., Saglia R., Sakr Z., Sapone D., Sartoris B., Schewtschenko J. A., Schirmer M., Schneider P., Schrabback T., Secroun A., Sefusatti E., Seidel G., Serrano S., Simon P., Sirignano C., Sirri G., Stanco L., Starck J.-L., Steinwagner J., Tallada-Crespí P., Tavagnacco D., Taylor A. N., Teplitz H. I., Tereno I., 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., Zucca E., Bolzonella M., Bozzo E., Burigana C., Calabrese M., Di Ferdinando D., Escartin Vigo J. A., Gabarra L., Matthew S., Mauri N., Pezzotta A., Pöntinen M., Porciani C., Scottez V., Tenti M., Viel M., Wiesmann M., Akrami Y., Allevato V., Andika I. T., Anselmi S., Archidiacono M., Atrio-Barandela F., Ballardini M., Bertacca D., Bethermin M., Blanchard A., Blot L., Borgani S., Brown M. L., Bruton S., Cabanac R., Calabro A., Camacho Quevedo B., Cappi A., Caro F., Carvalho C. S., Castro T., Chary R., Cogato F., Contini T., Cooray A. R., Cucciati O., Davini S., De Paolis F., Desprez G., Díaz-Sánchez A., Di Domizio S., Diego J. M., Ferrari A. G., Finoguenov A., Ganga K., García-Bellido J., Gasparetto T., Gaztanaga E., Giacomini F., Gianotti F., Gozaliasl G., Gregorio A., Guidi M., Gutierrez C. M., Hall A., Hartley W. G., Hemmati S., Hildebrandt H., Hjorth J., Huertas-Company M., Ilbert O., Kajava J. J. E., Kang Y., Kansal V., Karagiannis D., Kirkpatrick C. C., Kruk S., Lattanzi M., Le Graet J., Legrand L., Lembo M., Leroy G., Lesgourgues J., Liaudat T. I., Loureiro A., Macias-Perez J., Maggio G., Magliocchetti M., Mancini C., Mannucci F., Maoli R., Martín-Fleitas J., Martins C. J. A. P., Maurin L., Metcalf R. B., Miluzio M., Monaco P., Moretti C., Morgante G., Murray C., Naidoo K., Natoli P., Navarro-Alsina A., Nesseris S., Paterson K., Patrizii L., Pisani A., Potter D., Risso I., Rocci P.-F., Sahlén M., Sarpa E., Schaye J., Schneider A., Schultheis M., Sciotti D., Sellentin E., Sereno M., Shankar F., Smith L. C., Stanford S. A., Tanidis K., Tao C., Testera G., Teyssier R., Tosi S., Troja A., Tucci M., Valieri C., Venhola A., Vergani D., Verza G., Vielzeuf P., Walton N. A. +305 moredoaj +1 more sourceStructural biology of ferritin nanocages
FEBS Letters, EarlyView.Ferritin is a conserved iron‐storage protein that sequesters iron as a ferric mineral core within a nanocage, protecting cells from oxidative damage and maintaining iron homeostasis. This review discusses ferritin biology, structure, and function, and highlights recent cryo‐EM studies revealing mechanisms of ferritinophagy, cellular iron uptake, and ...Eloise Mastrangelo, Flavio Di Pisawiley +1 more sourceEvolution of the Near-Infrared Tully-Fisher Relation: Constraints on the
Relationship Between the Stellar and Total Masses of Disk Galaxies since z=1
, 2005 Using a combination of Keck spectroscopy and near-infrared imaging, we
investigate the K-band and stellar mass Tully-Fisher relation for 101 disk
galaxies at 0.2 < z < 1.2, with the goal of placing the first observational
constraints on the assembly ...Andrew C. Phillips, Christopher J. Conselice, Groth E. J., Jarle Brichmann, Kevin Bundy, Motohara K., Nicole P. Vogt, Poggianti B. M., Richard S. Ellis, Tully R. B. +9 morecore +1 more sourceStellar Mass Segregation in Dark Matter Halos
The Astrophysical JournalWe study the effect of stellar mass segregation driven by collisional relaxation within the potential well of a smooth dark matter halo. This effect is of particular relevance for old stellar systems with short crossing times, where small collisional ...Raphaël Errani, Jorge Peñarrubia, Matthew G. Walker +2 moredoaj +1 more sourceStellar Masses and Radii as Constraints on Stellar Models [PDF]
International Astronomical Union Colloquium, 1993 AbstractThe current status of empirical data on stellar masses and radii of sufficient accuracy to give constraints on stellar models is reviewed. Results from the best-studied eclipsing binaries can already trace the main-sequence evolution of 1-10 M⊙ stars in considerable detail and will be even more useful when supplemented by chemical abundance ...openaire +1 more sourceTransferrin receptor 1‐mediated iron uptake supports thermogenic activation in human cervical‐derived adipocytes
FEBS Letters, EarlyView.In this study, we found that human cervical‐derived adipocytes maintain intracellular iron level by regulating the expression of iron transport‐related proteins during adrenergic stimulation. Melanotransferrin is predicted to interact with transferrin receptor 1 based on in silico analysis.Rahaf Alrifai, Mizuki Seo, Gyath Karadsheh, Fachrur Rizal Mahendra, Máté Á Demény, Ferenc Győry, János András Mótyán, László Fésüs, Endre Kristóf, Rini Arianti +9 morewiley +1 more sourceTracing Galaxy Evolution in the Nearby Universe: The Role of Dark Matter
The Astronomical JournalUsing a sample of ∼126,000 late-type galaxies (LTGs) from the Sloan Digital Sky Survey, we analyzed stellar mass as a function of the dynamical mass. Stellar masses are estimated using eight stellar population synthesis (SPS) models with constant initial A. Nigoche-Netro, P. Lagos, R. J. Diaz, E. de la Fuente, M. P. Agüero, A. Ruelas-Mayorga, S. N. Kemp, R. A. Marquez-Lugo, R. Ibarra-Nuño +8 moredoaj +1 more source
