Zobrazeno 1 - 10
of 281
pro vyhledávání: '"A. Debackère"'
Systematic uncertainties in the mass measurement of galaxy clusters limit the cosmological constraining power of future surveys that will detect more than $10^5$ clusters. Previously, we argued that aperture masses can be inferred more accurately and
Externí odkaz:
http://arxiv.org/abs/2205.08424
The abundance of clusters of galaxies is highly sensitive to the late-time evolution of the matter distribution, since clusters form at the highest density peaks. However, the 3D cluster mass cannot be inferred without deprojecting the observations,
Externí odkaz:
http://arxiv.org/abs/2203.16379
We quantify two main pathways through which baryonic physics biases cluster count cosmology. We create mock cluster samples that reproduce the baryon content inferred from X-ray observations. We link clusters to their counterparts in a dark matter-on
Externí odkaz:
http://arxiv.org/abs/2101.07800
The interpretation of upcoming weak gravitational lensing surveys depends critically on our understanding of the matter power spectrum on scales $k < 10 h/\mathrm{Mpc}$, where baryonic processes are important. We study the impact of galaxy formation
Externí odkaz:
http://arxiv.org/abs/1908.05765
Autor:
Littlefield, Colin, Garnavich, Peter, Kennedy, Mark R., Patterson, Joseph, Kemp, Jonathan, Stiller, Robert A., Hambsch, Franz-Josef, Heras, Teofilo Arranz, Myers, Gordon, Stone, Geoffrey, Sjoberg, George, Dvorak, Shawn, Nelson, Peter, Popov, Velimir, Bonnardeau, Michel, Vanmunster, Tonny, de Miguel, Enrique, Alton, Kevin B., Harris, Barbara, Cook, Lewis M., Graham, Keith A., Brincat, Stephen M., Lane, David J., Foster, James, Pickard, Roger, Sabo, Richard, Vietje, Brad, Lemay, Damien, Briol, John, Krumm, Nathan, Dadighat, Michelle, Goff, William, Solomon, Rob, Padovan, Stefano, Bolt, Greg, Kardasis, Emmanuel, Debackere, Andre, Thrush, Jeff, Stein, William, Coulter, Daniel, Tsehmeystrenko, Valery, Gout, Jean-Francois, Lewin, Pablo, Galdies, Charles, Fernandez, David Cejudo, Walker, Gary, Boardman Jr., James, Pellett, Emil
The intermediate polar FO Aquarii (FO Aqr) experienced its first-reported low-accretion states in 2016, 2017, and 2018, and using newly available photographic plates, we identify pre-discovery low states in 1965, 1966, and 1974. The primary focus of
Externí odkaz:
http://arxiv.org/abs/1904.11505
Autor:
Vanden Bempt, Marlies, Debackere, Koen, Demeyer, Sofie, Van Thillo, Quentin, Meeuws, Nienke, Prieto, Cristina, Provost, Sarah, Mentens, Nicole, Jacobs, Kris, Gielen, Olga, Nittner, David, Ogawa, Seishi, Kataoka, Keisuke, Graux, Carlos, Tousseyn, Thomas, Cools, Jan, Dierickx, Daan
Publikováno v:
In Blood 8 December 2022 140(23):2463-2476
Autor:
Littlefield, Colin, Garnavich, Peter, Kennedy, Mark R., Aadland, Erin, Terndrup, Donald M., Calhoun, Grace V., Callanan, Paul, Abe, Lyu, Bendjoya, Philippe, Rivet, Jean-Pierre, Vernet, David, Devogele, Maxime, Shappee, Benjamin, Holoien, Thomas, Heras, Teofilo Arranz, Bonnardeau, Michel, Cook, Michael, Coulter, Daniel, Debackere, Andre, Dvorak, Shawn, Foster, James R., Goff, William, Hambsch, Franz-Josef, Harris, Barbara, Myers, Gordon, Nelson, Peter, Popov, Velimir, Solomon, Rob, Stein, William L., Stone, Geoff, Vietje, Brad
In 2016 May, the intermediate polar FO~Aqr was detected in a low state for the first time in its observational history. We report time-resolved photometry of the system during its initial recovery from this faint state. Our data, which includes high-
Externí odkaz:
http://arxiv.org/abs/1609.01026
Autor:
Santerne, A., Hébrard, G., Lillo-Box, J., Armstrong, D. J., Barros, S. C. C., Demangeon, O., Barrado, D., Debackere, A., Deleuil, M., Mena, E. Delgado, Montalto, M., Pollacco, D., Osborn, H. P., Sousa, S. G., Abe, L., Adibekyan, V., Almenara, J. -M., André, P., Arlic, G., Barthe, G., Bendjoya, P., Behrend, R., Boisse, I., Bouchy, F., Boussier, H., Bretton, M., Brown, D. J. A., Carry, B., Cailleau, A., Conseil, E., Courcol, B., Dauchet, B., Dalouzy, J. -C., Deldem, M., Dubreuil, P., Fehrenbach, J. -M., Ferratfiat, S., Girelli, R., Gregorio, J., Jaecques, S., Kugel, F., Kirk, J., Labrevoir, O., Lachurié, J. -C., Lam, K. W. F., Guen, P. Le, Martinez, P., Maurin, L., McCormac, J., Pioppa, J-B., Quadri, U., Rajpurohit, A., Rey, J., Rivet, J. -P., Roy, R., Santos, N. C., Signoret, F., Strabla, L., Suarez, O., Toublanc, D., Tsantaki, M., Wilson, P. A., Bachschmidt, M., Colas, F., Gerteis, O., Louis, P., Mario, J. -C., Marlot, C., Montier, J., Perroud, V., Pic, V., Romeuf, D., Ubaud, S., Verilhac, D.
Publikováno v:
2016, ApJ, 825, 55
In the present paper we report the discovery of a new hot Jupiter, EPIC211089792 b, first detected by the Super-WASP observatory and then by the K2 space mission during its campaign 4. The planet has a period of 3.25d, a mass of 0.73 +/- 0.04 Mjup, a
Externí odkaz:
http://arxiv.org/abs/1601.07680
Autor:
Hanuš, J., Ďurech, J., Oszkiewicz, D. A., Behrend, R., Carry, B., Delbo', M., Adam, O., Afonina, V., Anquetin, R., Antonini, P., Arnold, L., Audejean, M., Aurard, P., Bachschmidt, M., Badue, B., Barbotin, E., Barroy, P., Baudouin, P., Berard, L., Berger, N., Bernasconi, L., Bosch, J-G., Bouley, S., Bozhinova, I., Brinsfield, J., Brunetto, L., Canaud, G., Caron, J., Carrier, F., Casalnuovo, G., Casulli, S., Cerda, M., Chalamet, L., Charbonnel, S., Chinaglia, B., Cikota, A., Colas, F., Coliac, J-F., Collet, A., Coloma, J., Conjat, M., Conseil, E., Costa, R., Crippa, R., Cristofanelli, M., Damerdji, Y., Debackere, A., Decock, A., Déhais, Q., Déléage, T., Delmelle, S., Demeautis, C., Dróżdż, M., Dubos, G., Dulcamara, T., Dumont, M., Durkee, R., Dymock, R., del Valle, A. Escalante, Esseiva, N., Esseiva, R., Esteban, M., Fauchez, T., Fauerbach, M., Fauvaud, M., Fauvaud, S., Forné, E., Fournel, C., Fradet, D., Garlitz, J., Gerteis, O., Gillier, C., Gillon, M., Giraud, R., Godard, J-P., Goncalves, R., Hamanowa, H., Hay, K., Hellmich, S., Heterier, S., Higgins, D., Hirsch, R., Hodosan, G., Hren, M., Hygate, A., Innocent, N., Jacquinot, H., Jawahar, S., Jehin, E., Jerosimic, L., Klotz, A., Koff, W., Korlevic, P., Kosturkiewicz, E., Krafft, P., Krugly, Y., Kugel, F., Labrevoir, O., Lecacheux, J., Lehký, M., Leroy, A., Lesquerbault, B., Lopez-Gonzales, M. J., Lutz, M., Mallecot, B., Manfroid, J., Manzini, F., Marciniak, A., Martin, A., Modave, B., Montaigut, R., Montier, J., Morelle, E., Morton, B., Mottola, S., Naves, R., Nomen, J., Oey, J., Ogłoza, W., Paiella, M., Pallares, H., Peyrot, A., Pilcher, F., Pirenne, J-F., Piron, P., Polinska, M., Polotto, M., Poncy, R., Previt, J. P., Reignier, F., Renauld, D., Ricci, D., Richard, F., Rinner, C., Risoldi, V., Robilliard, D., Romeuf, D., Rousseau, G., Roy, R., Ruthroff, J., Salom, P. A., Salvador, L., Sanchez, S., Santana-Ros, T., Scholz, A., Séné, G., Skiff, B., Sobkowiak, K., Sogorb, P., Soldán, F., Spiridakis, A., Splanska, E., Sposetti, S., Starkey, D., Stephens, R., Stiepen, A., Stoss, R., Strajnic, J., Teng, J-P., Tumolo, G., Vagnozzi, A., Vanoutryve, B., Vugnon, J. M., Warner, B. D., Waucomont, M., Wertz, O., Winiarski, M., Wolf, M.
Publikováno v:
A&A 586, A108 (2016)
Asteroid modeling efforts in the last decade resulted in a comprehensive dataset of almost 400 convex shape models and their rotation states. This amount already provided a deep insight into physical properties of main-belt asteroids or large collisi
Externí odkaz:
http://arxiv.org/abs/1510.07422
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