Zobrazeno 1 - 10
of 51
pro vyhledávání: '"Bridge, C. R."'
Autor:
Petty, S. M., Neill, J. D., Jarrett, T. H., Blain, A. W., Farrah, D. G., Rich, R. M., Tsai, C. -W., Benford, D. J., Bridge, C. R., Lake, S. E., Masci, F. J., Wright, E. L.
In the local Universe, 10% of massive elliptical galaxies are observed to exhibit a peculiar property: a substantial excess of ultraviolet emission (UVX) over what is expected from their old, red stellar populations. Several origins for the UVX have
Externí odkaz:
http://arxiv.org/abs/1307.6282
Autor:
Alexander, D. M., Stern, D., Del Moro, A., Lansbury, G. B., Assef, R. J., Aird, J., Ajello, M., Ballantyne, D. R., Bauer, F. E., Boggs, S. E., Brandt, W. N., Christensen, F. E., Civano, F., Comastri, A., Craig, W. W., Elvis, M., Grefenstette, B. W., Hailey, C. J., Harrison, F. A., Hickox, R. C., Luo, B., Madsen, K. K., Mullaney, J. R., Perri, M., Puccetti, S., Saez, C., Treister, E., Urry, C. M., Zhang, W. W., Bridge, C. R., Eisenhardt, P. R. M., Gonzalez, A. H., Miller, S. H., Tsar, C. W.
We report on the first ten identifications of sources serendipitously detected by the NuSTAR to provide the first sensitive census of the cosmic X-ray background (CXB) source population at >10 keV. We find that these NuSTAR-detected sources are ~100x
Externí odkaz:
http://arxiv.org/abs/1307.1733
Autor:
Haan, S., Armus, L., Surace, J. A., Charmandaris, V., Evans, A. S., Diaz-Santos, T., Melbourne, J. L., Mazzarella, J. M., Howell, J. H., Stierwalt, S., Kim, D. C., Vavilkin, T., Sanders, D. B., Petric, A., Murphy, E. J., Braun, R., Bridge, C. R., Inami, H.
Nuclear stellar cusps are defined as central excess light component in the stellar light profiles of galaxies and are suggested to be stellar relics of intense compact starbursts in the central ~100-500 pc region of gas-rich major mergers. Here we pr
Externí odkaz:
http://arxiv.org/abs/1306.4337
Autor:
Stierwalt, S., Armus, L., Surace, J. A., Inami, H., Petric, A. O., Diaz-Santos, T., Haan, S., Charmandaris, V., Howell, J., Kim, D. C., Marshall, J., Mazzarella, J. M., Spoon, H. W. W., Veilleux, S., Evans, A., Sanders, D. B., Appleton, P., Bothun, G., Bridge, C. R., Chan, B., Frayer, D., Iwasawa, K., Kewley, L. J., Lord, S., Madore, B. F., Melbourne, J. E., Murphy, E. J., Rich, J. A., Schulz, B., Sturm, E., U, V., Vavilkin, T., Xu, K.
The Great Observatories All-Sky LIRG Survey (GOALS) is a multiwavelength study of luminous infrared galaxies (LIRGs) in the local universe. Here we present low resolution Spitzer spectra covering 5-38um and provide a basic analysis of the mid-IR spec
Externí odkaz:
http://arxiv.org/abs/1302.4477
Autor:
Haan, S., Surace, J. A., Armus, L., Evans, A. S., Howell, J. H., Mazzarella, J. M., Kim, D. C., Vavilkin, T., Inami, H., Sanders, D. B., Petric, A., Bridge, C. R., Melbourne, J. L., Charmandaris, V., Diaz-Santos, T., Murphy, E. J., U, V., Stierwalt, S., Marshall, J. A.
We present results of Hubble Space Telescope NICMOS H-band imaging of 73 of most luminous (i.e., log[L_IR/L_0]>11.4) Infrared Galaxies (LIRGs) in the Great Observatories All-sky LIRG Survey (GOALS). This dataset combines multi-wavelength imaging and
Externí odkaz:
http://arxiv.org/abs/1012.4012
Autor:
Pérez-González, P. G., Egami, E., Rex, M., Rawle, T. D., Kneib, J. -P., Richard, J., Johansson, D., Altieri, B., Blain, A. W., Bock, J. J., Boone, F., Bridge, C. R., Chung, S. M., Clément, B., Clowe, D., Combes, F., Cuby, J. -G., Dessauges-Zavadsky, M., Dowell, C. D., Espino-Briones, N., Fadda, D., Fiedler, A. K., Gonzalez, A., Horellou, C., Ilbert, O., Ivison, R. J., Jauzac, M., Lutz, D., Pelló, R., Pereira, M. J., Rieke, G. H., Rodighiero, G., Schaerer, D., Smith, G. P., Valtchanov, I., Walth, G. L., van der Werf, P., Werner, M. W., Zemcov, M.
We present preliminary results about the detection of high redshift (U)LIRGs in the Bullet cluster field by the PACS and SPIRE instruments within the Herschel Lensing Survey (HLS) Program. We describe in detail a photometric procedure designed to rec
Externí odkaz:
http://arxiv.org/abs/1005.3823
Autor:
Zemcov, M., Rex, M., Rawle, T. D., Bock, J. J., Egami, E., Altieri, B., Blain, A. W., Boone, F., Bridge, C. R., Clement, B., Combes, F., Dowell, C. D., Dessauges-Zavadsky, M., Fadda, D., Ilbert, O., Ivison, R. J., Jauzac, M., Kneib, J. -P., Lutz, D., Pelló, R., Pereira, M. J., Pérez-González, P. G., Richard, J., Rieke, G. H., Rodighiero, G., Schaerer, D., Smith, G. P., Valtchanov, I., Walth, G. L., van der Werf, P., Werner, M. W.
The Sunyaev-Zel'dovich (SZ) effect is a spectral distortion of the cosmic microwave background as observed through the hot plasma in galaxy clusters. This distortion is a decrement in the CMB intensity for lambda > 1.3 mm, an increment at shorter wav
Externí odkaz:
http://arxiv.org/abs/1005.3824
Autor:
Rawle, T. D., Chung, S. M., Fadda, D., Rex, M., Egami, E., Pérez-González, P. G., Altieri, B., Blain, A. W., Bridge, C. R., Fiedler, A. K., Gonzalez, A. H., Pereira, M. J., Richard, J., Smail, I., Valtchanov, I., Zemcov, M., Appleton, P. N., Bock, J. J., Boone, F., Clement, B., Combes, F., Dowell, C. D., Dessauges-Zavadsky, M., Ilbert, O., Ivison, R. J., Jauzac, M., Kneib, J. -P., Lutz, D., Pelló, R., Rieke, G. H., Rodighiero, G., Schaerer, D., Smith, G. P., Walth, G. L., van der Werf, P., Werner, M. W.
We use deep, five band (100-500um) data from the Herschel Lensing Survey (HLS) to fully constrain the obscured star formation rate, SFR_FIR, of galaxies in the Bullet cluster (z=0.296), and a smaller background system (z=0.35) in the same field. Hers
Externí odkaz:
http://arxiv.org/abs/1005.3822
Autor:
Rex, M., Rawle, T. D., Egami, E., Pérez-González, P. G., Zemcov, M., Aretxaga, I., Chung, S. M., Fadda, D., Gonzalez, A. H., Hughes, D. H., Horellou, C., Johansson, D., Kneib, J. -P., Richard, J., Altieri, B., Fiedler, A. K., Pereira, M. J., Rieke, G. H., Smail, I., Valtchanov, I., Blain, A. W., Bock, J. J., Boone, F., Bridge, C. R., Clement, B., Combes, F., Dowell, C. D., Dessauges-Zavadsky, M., Ilbert, O., Ivison, R. J., Jauzac, M., Lutz, D., Omont, A., Pelló, R., Rodighiero, G., Schaerer, D., Smith, G. P., Walth, G. L., van der Werf, P., Werner, M. W., Austermann, J. E., Ezawa, H., Kawabe, R., Kohno, K., Perera, T. A., Scott, K. S., Wilson, G. W., Yun, M. S.
The Herschel Lensing Survey (HLS) takes advantage of gravitational lensing by massive galaxy clusters to sample a population of high-redshift galaxies which are too faint to be detected above the confusion limit of current far-infrared/submillimeter
Externí odkaz:
http://arxiv.org/abs/1005.3821
Autor:
Egami, E., Rex, M., Rawle, T. D., Pérez-González, P. G., Richard, J., Kneib, J. -P., Schaerer, D., Altieri, B., Valtchanov, I., Blain, A. W., Fadda, D., Zemcov, M., Bock, J. J., Boone, F., Bridge, C. R., Clement, B., Combes, F., Dowell, C. D., Dessauges-Zavadsky, M., Ilbert, O., Ivison, R. J., Jauzac, M., Lutz, D., Metcalfe, L., Omont, A., Pelló, R., Pereira, M. J., Rieke, G. H., Rodighiero, G., Smail, I., Smith, G. P., Tramoy, G., Walth, G. L., van der Werf, P., Werner, M. W.
The Herschel Lensing Survey (HLS) will conduct deep PACS and SPIRE imaging of ~40 massive clusters of galaxies. The strong gravitational lensing power of these clusters will enable us to penetrate through the confusion noise, which sets the ultimate
Externí odkaz:
http://arxiv.org/abs/1005.3820