Zobrazeno 1 - 10
of 24
pro vyhledávání: '"Meyers, J."'
Autor:
collaboration, CCAT-Prime, Aravena, M., Austermann, J. E., Basu, K., Battaglia, N., Beringue, B., Bertoldi, F., Bigiel, F., Bond, J. R., Breysse, P. C., Broughton, C., Bustos, R., Chapman, S. C., Charmetant, M., Choi, S. K., Chung, D. T., Clark, S. E., Cothard, N. F., Crites, A. T., Dev, A., Douglas, K., Duell, C. J., Dunner, R., Ebina, H., Erler, J., Fich, M., Fissel, L. M., Foreman, S., Gallardo, P. A., Gao, J., García, Pablo, Giovanelli, R., Golec, J. E., Groppi, C. E., Haynes, M. P., Henke, D., Hensley, B., Herter, T., Higgins, R., Hlozek, R., Huber, A., Huber, Z., Hubmayr, J., Jackson, R., Johnstone, D., Karoumpis, C., Keating, L. C., Komatsu, E., Li, Y., Magnelli, B., Matthews, B. C., Mauskopf, P., McMahon, J. J., Meerburg, P. D., Meyers, J., Muralidhara, V., Murray, N. W., Niemack, M. D., Nikola, T., Okada, Y., Puddu, R., Riechers, D. A., Rosolowsky, E., Rossi, K., Rotermund, K., Roy, A., Sadavoy, S. I., Schaaf, R., Schilke, P., Scott, D., Simon, R., Sinclair, Adrian K., Sivakoff, G. R., Stacey, G. J., Stutz, Amelia M., Stutzki, J., Tahani, M., Thanjavur, K., Timmermann, R. A., Ullom, J. N., van Engelen, A., Vavagiakis, E. M., Vissers, M. R., Wheeler, J. D., White, S. D. M., Zhu, Y., Zou, B.
We present a detailed overview of the science goals and predictions for the Prime-Cam direct detection camera/spectrometer being constructed by the CCAT-prime collaboration for dedicated use on the Fred Young Submillimeter Telescope (FYST). The FYST
Externí odkaz:
http://arxiv.org/abs/2107.10364
Autor:
Jarvis, M., Bernstein, G. M., Amon, A., Davis, C., Léget, P. F., Bechtol, K., Harrison, I., Gatti, M., Roodman, A., Chang, C., Chen, R., Choi, A., Desai, S., Drlica-Wagner, A., Gruen, D., Gruendl, R. A., Hernandez, A., MacCrann, N., Meyers, J., Navarro-Alsina, A., Pandey, S., Plazas, A. A., Secco, L. F., Sheldon, E., Troxel, M. A., Vorperian, S., Wei, K., Zuntz, J., Abbott, T. M. C., Aguena, M., Allam, S., Avila, S., Bhargava, S., Bridle, S. L., Brooks, D., Rosell, A. Carnero, Kind, M. Carrasco, Carretero, J., Costanzi, M., da Costa, L. N., De Vicente, J., Diehl, H. T., Doel, P., Everett, S., Flaugher, B., Fosalba, P., Frieman, J., García-Bellido, J., Gaztanaga, E., Gerdes, D. W., Gutierrez, G., Hinton, S. R., Hollowood, D. L., Honscheid, K., James, D. J., Kent, S., Kuehn, K., Kuropatkin, N., Lahav, O., Maia, M. A. G., March, M., Marshall, J. L., Melchior, P., Menanteau, F., Miquel, R., Ogando, R. L. C., Paz-Chinchón, F., Rykoff, E. S., Sanchez, E., Scarpine, V., Schubnell, M., Serrano, S., Sevilla-Noarbe, I., Smith, M., Suchyta, E., Swanson, M. E. C., Tarle, G., Varga, T. N., Walker, A. R., Wester, W., Wilkinson, R. D., Collaboration, DES
Publikováno v:
2021MNRAS.501.1282J
We introduce a new software package for modeling the point-spread function (PSF) of astronomical images, called Piff (PSFs In the Full FOV), which we apply to the first three years (known as Y3) of the Dark Energy Survey (DES) data. We describe the r
Externí odkaz:
http://arxiv.org/abs/2011.03409
Autor:
Hanany, S., Alvarez, M., Artis, E., Ashton, P., Aumont, J., Aurlien, R., Banerji, R., Barreiro, R. B., Bartlett, J. G., Basak, S., Battaglia, N., Bock, J., Boddy, K. K., Bonato, M., Borrill, J., Bouchet, F., Boulanger, F., Burkhart, B., Chluba, J., Chuss, D., Clark, S., Cooperrider, J., Crill, B. P., De Zotti, G., Delabrouille, J., Di Valentino, E., Didier, J., Dore, O., Eriksen, H. K., Errard, J., Essinger-Hileman, T., Feeney, S., Filippini, J., Fissel, L., Flauger, R., Fuskeland, U., Gluscevic, V., Gorski, K. M., Green, D., Hensley, B., Herranz, D., Hill, J. C., Hivon, E., Hlozek, R., Hubmayr, J., Johnson, B. R., Jones, W., Jones, T., Knox, L., Kogut, A., Lopez-Caniego, M., Lawrence, C., Lazarian, A., Li, Z., Madhavacheril, M., Melin, J. B., Meyers, J., Murray, C., Negrello, M., Novak, G., O'Brient, R., Paine, C., Pearson, T., Pogosian, L., Pryke, C., Puglisi, G., Remazeilles, M., Rocha, G., Schmittfull, M., Scott, D., Shirron, P., Stephens, I., Sutin, B., Tomasi, M., Trangsrud, A., van Engelen, A., Vansyngel, F., Wehus, I. K., Wen, Q., Xu, S., Young, K., Zonca, A.
The Probe of Inflation and Cosmic Origins (PICO) is a proposed probe-scale space mission consisting of an imaging polarimeter operating in frequency bands between 20 and 800 GHz. We describe the science achievable by PICO, which has sensitivity equiv
Externí odkaz:
http://arxiv.org/abs/1908.07495
Autor:
Stacey, G. J., Aravena, M., Basu, K., Battaglia, N., Beringue, B., Bertoldi, F., Bond, J. R., Breysse, P., Bustos, R., Chapman, S., Chung, D. T., Cothard, N., Erler, J., Fich, M., Foreman, S., Gallardo, P., Giovanelli, R., Graf, U. U., Haynes, M. P., Herrera-Camus, R., Herter, T. L., Hložek, R., Johnstone, D., Keating, L., Magnelli, B., Meerburg, D., Meyers, J., Murray, N., Niemack, M., Nikola, T., Nolta, M., Parshley, S. C., Riechers, D., Schilke, P., Scott, D., Stein, G., Stevens, J., Stutzki, J., Vavagiakis, E. M., Viero, M. P.
We present the detailed science case, and brief descriptions of the telescope design, site, and first light instrument plans for a new ultra-wide field submillimeter observatory, CCAT-prime, that we are constructing at a 5600 m elevation site on Cerr
Externí odkaz:
http://arxiv.org/abs/1807.04354
Autor:
Rubin, D., Aldering, G., Amanullah, R., Barbary, K., Dawson, K. S., Deustua, S., Faccioli, L., Fadeyev, V., Fakhouri, H. K., Fruchter, A. S., Gladders, M. D., de Jong, R. S., Koekemoer, A., Krechmer, E., Lidman, C., Meyers, J., Nordin, J., Perlmutter, S., Ripoche, P., Schlegel, D. J., Spadafora, A., Suzuki, N., Project, The Supernova Cosmology
NICMOS 2 observations are crucial for constraining distances to most of the existing sample of z > 1 SNe Ia. Unlike the conventional calibration programs, these observations involve long exposure times and low count rates. Reciprocity failure is know
Externí odkaz:
http://arxiv.org/abs/1502.01026
Autor:
Meyers, J. E., Burchat, P. R.
Current and future imaging surveys will measure cosmic shear with a statistical precision that demands a deeper understanding of potential systematic biases in galaxy shape measurements than has been achieved to date. We investigate the effects of us
Externí odkaz:
http://arxiv.org/abs/1402.5101
Autor:
Nordin, J., Rubin, D., Richard, J., Rykoff, E., Aldering, G., Amanullah, R., Atek, H., Barbary, K., Deustua, S., Fakhouri, H. K., Fruchter, A. S., Goobar, A., Hook, I., Hsiao, E. Y., Huang, X., Kneib, J. -P., Lidman, C., Meyers, J., Perlmutter, S., Saunders, C., Spadafora, A. L., Suzuki, N.
Publikováno v:
MNRAS 440, 2742-2754 (2014)
Using three magnified Type Ia supernovae (SNe Ia) detected behind CLASH clusters, we perform a first pilot study to see whether standardizable candles can be used to calibrate cluster mass maps created from strong lensing observations. Such calibrati
Externí odkaz:
http://arxiv.org/abs/1312.2576
The importance of major mergers in the build up of stellar mass in brightest cluster galaxies at z=1
Autor:
Lidman, C., Iacobuta, G., Bauer, A. E., Barrientos, L. F., Cerulo, P., Couch, W. J., Delaye, L., Demarco, R., Ellingson, E., Faloon, A. J., Gilbank, D., Huertas-Company, M., Mei, S., Meyers, J., Muzzin, A., Noble, A., Nantais, J., Rettura, A., Rosati, P., Sanchez-Janssen, R., Strazzullo, V., Webb, T. M. A., Wilson, G., Yan, R., Yee, H. K. C.
Recent independent results from numerical simulations and observations have shown that brightest cluster galaxies (BCGs) have increased their stellar mass by a factor of almost two between z~0.9 and z~0.2. The numerical simulations further suggest th
Externí odkaz:
http://arxiv.org/abs/1305.0882
Autor:
Meyers, J., Aldering, G., Barbary, K., Barrientos, L. F., Brodwin, M., Dawson, K. S., Deustua, S., Doi, M., Eisenhardt, P., Faccioli, L., Fakhouri, H. K., Fruchter, A. S., Gilbank, D. G., Gladders, M. D., Goldhaber, G., Gonzalez, A. H., Hattori, T., Hsiao, E., Ihara, Y., Kashikawa, N., Koester, B., Konishi, K., Lidman, C., Lubin, L., Morokuma, T., Oda, T., Perlmutter, S., Postman, M., Ripoche, P., Rosati, P., Rubin, D., Rykoff, E., Spadafora, A., Stanford, S. A., Suzuki, N., Takanashi, N., Tokita, K., Yasuda, N.
Using the sample of Type Ia supernovae (SNe Ia) discovered by the Hubble Space Telescope (HST) Cluster Supernova Survey and augmented with HST-observed SNe Ia in the GOODS fields, we search for correlations between the properties of SNe and their hos
Externí odkaz:
http://arxiv.org/abs/1201.3989
Autor:
Barbary, K., Aldering, G., Amanullah, R., Brodwin, M., Connolly, N., Dawson, K. S., Doi, M., Eisenhardt, P., Faccioli, L., Fadeyev, V., Fakhouri, H. K., Fruchter, A. S., Gilbank, D. G., Gladders, M. D., Goldhaber, G., Goobar, A., Hattori, T., Hsiao, E., Huang, X., Ihara, Y., Kashikawa, N., Koester, B., Konishi, K., Kowalski, M., Lidman, C., Lubin, L., Meyers, J., Morokuma, T., Oda, T., Panagia, N., Perlmutter, S., Postman, M., Ripoche, P., Rosati, P., Rubin, D., Schlegel, D. J., Spadafora, A. L., Stanford, S. A., Strovink, M., Suzuki, N., Takanashi, N., Tokita, K., Yasuda, N.
We present a measurement of the volumetric Type Ia supernova (SN Ia) rate out to z ~ 1.6 from the Hubble Space Telescope Cluster Supernova Survey. In observations spanning 189 orbits with the Advanced Camera for Surveys we discovered 29 SNe, of which
Externí odkaz:
http://arxiv.org/abs/1110.6442