From Particles to Pixels: How many particles do I really need to construct stellar kinematic mock observational measurements?

Autor: Harborne, K. E., Lagos, C. del P., Croom, S. M., van de Sande, J., Ludlow, A., Remus, R. S., Kimmig, L. C., Power, C.

This work considers the impact of resolution in the construction of mock observations of simulated galaxies. In particular, when building mock integral field spectroscopic observations from galaxy formation models in cosmological simulations, we inve

Externí odkaz: http://arxiv.org/abs/2411.03791

Rare variant in scavenger receptor BI raises HDL cholesterol and increases risk of coronary heart disease

Autor: Zanoni, P., Khetarpal, S. A., Larach, D. B., Hancock-Cerutti, W. F., Millar, J. S., Cuchel, M., DerOhannessian, S., Kontush, A., Surendran, P., Saleheen, D., Trompet, S., Cooper, R. S., Chowdhury, R., Dedoussis, G., de Faire, U., Feranil, A. B., Sheu, W. H.- H., Ferrucci, L., Freimer, N. B., Gieger, C., Sengupta, S., Grallert, H., Groop, L. C., Gudnason, V., Tanaka, T., Gyllensten, U., Hamsten, A., Erdmann, J., Harris, T. B., Shuldiner, A. R., Hingorani, A., Hirschhorn, J. N., Gravito, M. L., Wilson, J. F., Hofman, A., Hovingh, G. K., Hsiung, C. A., Humphries, S. E., Teslovich, T. M., Hunt, S. C., Hveem, K., Iribarren, C., Siegbahn, A., Groves, C. J., Nordestgaard, B. G., Njolstad, I., Jarvelin, M.-R., Jula, A., Kahonen, M., Kaprio, J., Kesaniemi, A., Kivimaki, M., Thorleifsson, G., Kooner, J. S., Hallmans, G., Koudstaal, P. J., Kuulasmaa, K., Gustafsson, S., Krauss, R. M., Kuh, D., Nielsen, S. F., Kuusisto, J., Kyvik, K. O., Laakso, M., Lakka, T. A., Hartikainen, A.-L., Lind, L., Van den Herik, E. G., Lindgren, C. M., Kanoni, S., Spector, T. D., Martin, N. G., Marz, W., McCarthy, M. I., McKenzie, C. A., Tybjaerg-Hansen, A., Assimes, T. L., Meneton, P., Metspalu, A., Moilanen, L., Morris, A. D., Ganna, A., Voight, B. F., Stefansson, K., Munroe, P. B., van Pelt, L. J., Waite, L. L., Hayward, C., Strachan, D. P., Tayo, B. O., Tremoli, E., Tuomilehto, J., Uusitupa, M., Chen, J., van Duijn, C. M., Vollenweider, P., Wallentin, L., Liu, D. J., Hernandez, D., Vedantam, S., Wareham, N. J., Jukema, J. W., Whitfield, J. B., Wolffenbuttel, B. H. R., Ordovas, J. M., Buchkovich, M. L., Boerwinkle, E., Palmer, C. N. A., Thorsteinsdottir, U., Hicks, A. A., Chasman, D. I., Rotter, J. I., Wainwright, N., Franks, P. W., Perola, M., Wong, A., Riatti, S., Mora, S., Cupples, L. A., Sandhu, M. S., Rauramaa, R., Rich, S. S., Boehnke, M., Deloukas, P., Mohlke, K. L., Wijmenga, C., Ingelsson, E., Gu, D., Roberts, R., Beckmann, J. S., Wu, Y., Peloso, G. M., Blankenberg, S., Watkins, H., Clarke, R., Collins, R., Kim, B.-J., Wild, S. H., McPherson, R., Nieminen, M. S., Barroso, I., Holm, H., O'Donnell, C., Schreiber, S., Zhang, W., Salomaa, V., Zalloua, P. A., Mannisto, S., Amouyel, P., Willemsen, G., Arveiler, D., Hung, Y.-J., Bragg-Gresham, J. L., Ferrieres, J., Muller-Nurasyid, M., Ferrario, M., Kee, F., Absher, D., Willer, C. J., Samani, N., Schunkert, H., Butterworth, A. S., Sattar, N., Wilsgaard, T., Chang, H.-Y., Howson, J. M. M., Pedersen, N. L., Di Angelantonio, E., Demirkan, A., Den Hertog, H. M., Do, R., Donnelly, L. A., Ehret, G. B., Illig, T., Esko, T., Feitosa, M. F., Ferreira, T., Been, L. F., Power, C., Fischer, K., Song, C., Fontanillas, P., Fraser, R. M., Freitag, D. F., Jones, M. R., Gurdasani, D., Heikkila, K., Hypponen, E., Isaacs, A., Jackson, A. U., Pramstaller, P. P., Johansson, A., Bolton, J. L., Young, E. H., Johnson, T., Kaleebu, P., Kaakinen, M., Kettunen, J., Kleber, M. E., Li, X., Luan, J., Lyytikainen, L.-P., Price, J. F., Magnusson, P. K. E., Mangino, M., Mihailov, E., Kastelein, J. J. P., Zhao, J. H., Bonnycastle, L. L., Montasser, M. E., Nolte, I. M., OConnell, J. R., Palmer, C. D., Petersen, A.-K., Schmidt, R. F., Sanna, S., Saxena, R., Bandinelli, S., Service, S. K., Shah, S., Adair, L. S., Shungin, D., Brambilla, P., Sidore, C., De Craen, A., Burnett, M. S., Psaty, B. M., Cesana, G., Khaw, K.-T., Dimitriou, M., Doney, A. S. F., Doring, A., Elliott, P., Epstein, S. E., Eyjolfsson, G. I., Gigante, B., Goodarzi, M. O., Quertermous, T., Kim, E., Stitziel, N. O., Volcik, K. A., Klopp, N., Komulainen, P., Kumari, M., Langenberg, C., Ford, I., Lehtimaki, T., Lin, S.-Y., Lindstrom, J., Bennett, F., Danesh, J., Loos, R. J. F., Uitterlinden, A. G., Mach, F., McArdle, W. L., Meisinger, C., Mitchell, B. D., Muller, G., Nagaraja, R., Packard, C., Narisu, N., Kathiresan, S., Nieminen, T. V. M., Bochud, M., Nsubuga, R. N., Olafsson, I., Ong, K. K., Palotie, A., Papamarkou, T., Pomilla, C., Pouta, A., Rader, D. J., Reilly, M. P., Majumder, A. a. S., Ridker, P. M., Sanghera, D. K., Boehm, B. O., Rivadeneira, F., Rudan, I., Ruokonen, A., Scharnagl, H., Seeley, J., Asiki, G., Silander, K., Stancakova, A., Stirrups, K., Swift, A. J., Saramies, J., Alam, D. S., Boomsma, D. I., Tiret, L., Strawbridge, R. J., Abecasis, G., Watson, S., Borecki, I. B., Bornstein, S. R., Bovet, P., Burnier, M., Campbell, H., Schwarz, P. E. H., Chakravarti, A., Chambers, J. C., Chen, Y.-D. I., Collins, F. S., Schmidt, E. M., Surakka, I.

Scavenger receptor BI (SR-BI) is the major receptor for high-density lipoprotein (HDL) cholesterol (HDL-C). In humans, high amounts of HDL-C in plasma are associated with a lower risk of coronary heart disease (CHD). Mice that have depleted Scarb1 (S

Externí odkaz: http://hdl.handle.net/10150/623258
http://arizona.openrepository.com/arizona/handle/10150/623258

Recovering $\lambda_R$ and $V/\sigma$ from seeing-dominated IFS data

Autor: Harborne, K. E., van de Sande, J., Cortese, L., Power, C., Robotham, A. S. G., Lagos, C. D. P., Croom, S.

Observers experience a series of limitations when measuring galaxy kinematics, such as variable seeing conditions and aperture size. These effects can be reduced using empirical corrections, but these equations are usually applicable within a restric

Externí odkaz: http://arxiv.org/abs/2006.12730

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The HI Velocity Function: a test of cosmology or baryon physics?

Autor: Chauhan, G., Lagos, C. D. P., Obreschkow, D., Power, C., Oman, K., Elahi, P. J.

Accurately predicting the shape of the HI velocity function of galaxies is regarded widely as a fundamental test of any viable dark matter model. Straightforward analyses of cosmological $N$-body simulations imply that the $\Lambda$CDM model predicts

Externí odkaz: http://arxiv.org/abs/1906.06130