Zobrazeno 1 - 10
of 124
pro vyhledávání: '"Zamojski M"'
Autor:
Dessauges-Zavadsky, M., Zamojski, M., Rujopakarn, W., Richard, J., Sklias, P., Schaerer, D., Combes, F., Ebeling, H., Rawle, T. D., Egami, E., Boone, F., Clément, B., Kneib, J. -P., Nyland, K., Walth, G.
Publikováno v:
A&A 605, A81 (2017)
We report on the galaxy MACSJ0032-arc at z=3.6314 discovered during the Herschel Lensing snapshot Survey of massive galaxy clusters, and strongly lensed by the cluster MACSJ0032.1+1808. The successful detections of its rest-frame UV, optical, FIR, mi
Externí odkaz:
http://arxiv.org/abs/1610.08065
Autor:
Schaerer, D., Boone, F., Jones, T., Dessauges-Zavadsky, M., Sklias, P., Zamojski, M., Cava, A., Richard, J., Ellis, R., Rawle, T. D., Egami, E., Combes, F.
Publikováno v:
A&A 576, L2 (2015)
Our objectives are to determine the properties of the interstellar medium (ISM) and of star-formation in typical star-forming galaxies at high redshift. Following up on our previous multi-wavelength observations with HST, Spitzer, Herschel, and the P
Externí odkaz:
http://arxiv.org/abs/1502.03842
Autor:
Dessauges-Zavadsky, M., Zamojski, M., Schaerer, D., Combes, F., Egami, E., Swinbank, A. M., Richard, J., Sklias, P., Rawle, T. D., Rex, M., Kneib, J. -P., Boone, F., Blain, A.
Publikováno v:
A&A 577, A50 (2015)
To extend the molecular gas measurements to typical star-forming galaxies (SFGs) with SFR < 40 Msun yr^{-1} and M* < 2.5x10^{10} Msun at z~1.5-3, we have observed CO emission with the IRAM Plateau de Bure Interferometer and 30m telescope for five str
Externí odkaz:
http://arxiv.org/abs/1408.0816
Autor:
Schaerer, D., Boone, F., Zamojski, M., Staguhn, J., Dessauges-Zavadsky, M., Finkelstein, S., Combes, F.
Publikováno v:
A&A 574, A19 (2015)
We have targeted two recently discovered Lyman break galaxies (LBGs) to search for dust continuum and [CII] 158 micron line emission. The strongly lensed z~6.8 LBG A1703-zD1 behind the galaxy cluster Abell 1703, and the spectroscopically confirmed z=
Externí odkaz:
http://arxiv.org/abs/1407.5793
Autor:
Rawle, T. D., Egami, E., Bussmann, R. S., Gurwell, M., Ivison, R. J., Boone, F., Combes, F., Danielson, A. L. R., Rex, M., Richard, J., Smail, I., Swinbank, A. M., Altieri, B., Blain, A. W., Clement, B., Dessauges-Zavadsky, M., Edge, A. C., Fazio, G. G., Jones, T., Kneib, J. -P., Omont, A., Perez-Gonzalez, P. G., Schaerer, D., Valtchanov, I., van der Werf, P. P., Walth, G., Zamojski, M., Zemcov, M.
We present Submillimeter Array (SMA) [CII] 158um and Jansky Very Large Array (JVLA) $^{12}$CO(1-0) line emission maps for the bright, lensed, submillimeter source at $z=5.2430$ behind Abell 773: HLSJ091828.6+514223 (HLS0918). We combine these measure
Externí odkaz:
http://arxiv.org/abs/1310.4090
Autor:
Sklias, P., Zamojski, M., Schaerer, D., Dessauges-Zavadsky, M., Egami, E., Rex, M., Rawle, T., Richard, J., Boone, F., Simpson, J. M., Smail, I., van der Werf, P., Altieri, B., Kneib, J. P.
Multi-wavelength, optical to IR/sub-mm observations of 5 strongly lensed galaxies identified by the Herschel Lensing Survey, plus two well-studied lensed galaxies, MS1512-cB58 and the Cosmic Eye, for which we also provide updated Herschel measurement
Externí odkaz:
http://arxiv.org/abs/1310.2655
Autor:
Boone, F., Clément, B., Richard, J., Schaerer, D., Lutz, D., Weiß, A., Zemcov, M., Egami, E., Rawle, T. D., Walth, G. L., Kneib, J. -P., Combes, F., Smail, I., Swinbank, A. M., Altieri, B., Blain, A. W., Chapman, S., Dessauges-Zavadsky, M., Ivison, R. J., Knudsen, K. K., Omont, A., Pello, R., Pérez-González, P. G., Valtchanov, I., van der Werf, P., Zamojski, M.
In the course of our 870um APEX/LABOCA follow up of the Herschel Lensing Survey we have detected a source in AS1063 (RXC J2248.7-4431), that has no counterparts in any of the Herschel PACS/SPIRE bands, it is a Herschel 'drop-out' with S_870/S_500>0.5
Externí odkaz:
http://arxiv.org/abs/1308.6707
Autor:
Elvis, M., Hao, H., Civano, F., Brusa, M., Salvato, M., Bongiorno, A., Capak, P., Zamorani, G., Comastri, A., Jahnke, K., Lusso, E., Mainieri, V., Trump, J. R., Ho, L. C., Aussel, H., Cappelluti, N., Cisternas, M., Frayer, D., Gilli, R., Hasinger, G., Huchra, J. P., Impey, C. D., Koekemoer, A. M., Lanzuisi, G., Floc'h, E. Le, Lilly, S. J., Liu, Y., McCarthy, P., McCracken, H. J., Merloni, A., Roeser, H. J., Sanders, D. B., Sargent, M., Scoville, N., Schinnerer, E., Schiminovich, D., Silverman, J., Taniguchi, Y., Vignali, C., Urry, C. M., Zamojski, M. A., Zatloukal, M.
The "Cosmic Evolution Survey" (COSMOS) enables the study of the Spectral Energy Distributions (SEDs) of Active Galactic Nuclei (AGN) because of the deep coverage and rich sampling of frequencies from X-ray to radio. Here we present a SED catalog of 4
Externí odkaz:
http://arxiv.org/abs/1209.1478
Autor:
Boone, F., Schaerer, D., Pello, R., Lutz, D., Weiss, A., Egami, E., Smail, I., Rex, M., Rawle, T., Ivison, R., Laporte, N., Beelen, A., Combes, F., Blain, A. W., Richard, J., Kneib, J. -P., Zamojski, M., Dessauges-Zavadsky, M., Altieri, B., van der Werf, P., Swinbank, M., Perez-Gonzalez, P. G., Clement, B., Nordon, R., Magnelli, B., Menten, K. M.
The spectral energy distributions (SED) of dusty galaxies at intermediate redshift may look similar to very high redshift galaxies in the optical/near infrared (NIR) domain. This can lead to the contamination of high redshift galaxy searches based on
Externí odkaz:
http://arxiv.org/abs/1108.2406
Autor:
Brusa, M., Civano, F., Comastri, A., Miyaji, T., Salvato, M., Zamorani, G., Cappelluti, N., Fiore, F., Hasinger, G., Mainieri, V., Merloni, A., Bongiorno, A., Capak, P., Elvis, M., Gilli, R., Hao, H., Jahnke, K., Koekemoer, A. M., Ilbert, O., Floc'h, E. Le, Lusso, E., Mignoli, M., Schinnerer, E., Silverman, J. D., Treister, E., Trump, J. D., Vignali, C., Zamojski, M., Aldcroft, T., Aussel, H., Bardelli, S., Bolzonella, M., Cappi, A., Caputi, K., Contini, T., Finoguenov, A., Fruscione, A., Garilli, B., Impey, C. D., Iovino, A., Iwasawa, K., Kampczyk, P., Kartaltepe, J., Kneib, J. P., Knobel, C., Kovac, K., Lamareille, F., Leborgne, J-F., Brun, V. Le, Fevre, O. Le, Lilly, S. J., Maier, C., McCracken, H. J., Pello, R., Peng, Y-J, Perez-Montero, E., de Ravel, L., Sanders, D., Scodeggio, M., Scoville, N. Z., Tanaka, M., Taniguchi, Y., Tasca, L., de la Torre, S., Tresse, L., Vergani, D., Zucca, E.
We report the final optical identifications of the medium-depth (~60 ksec), contiguous (2 deg^2) XMM-Newton survey of the COSMOS field. XMM-Newton has detected ~800 X-ray sources down to limiting fluxes of ~5x10^{-16}, ~3x10^{-15}, and ~7x10^{-15} er
Externí odkaz:
http://arxiv.org/abs/1004.2790