Zobrazeno 1 - 10
of 7 823
pro vyhledávání: '"Dye S"'
Publikováno v:
In Carbohydrate Polymers 1 June 2019 213:428-440
Publikováno v:
In Forensic Science International June 2018 287:98-107
Autor:
Bakx, Tom J. L. C., Berta, S., Dannerbauer, H., Cox, P., Butler, K. M., Hagimoto, M., Hughes, D. H., Riechers, D. A., van der Werf, P. P., Yang, C., Baker, A. J., Beelen, A., Bendo, G. J., Borsato, E., Buat, V., Cooray, A. R., Dunne, L., Dye, S., Eales, S., Gavazzi, R., Harris, A. I., Ismail, D., Ivison, R. J., Jones, B., Krips, M., Lehnert, M. D., Marchetti, L., Messias, H., Negrello, M., Neri, R., Omont, A., Perez-Fournon, I., Nanni, A., Chartab, N., Serjeant, S., Stanley, F., Tamura, Y., Urquhart, S. A., Vlahakis, C., Weiß, A., Young, A. J.
We report on deep SCUBA-2 observations at 850$\mu$m and NOEMA spectroscopic measurements at 2 mm of the environment surrounding the luminous, massive ($M_{*} \approx 2 \times 10^{11}$ M$_{\odot}$) Herschel-selected source HerBS-70. This source was re
Externí odkaz:
http://arxiv.org/abs/2404.18991
Autor:
Geach, J. E., Lopez-Rodriguez, E., Doherty, M. J., Chen, Jianhang, Ivison, R. J., Bendo, G. J., Dye, S., Coppin, K. E. K.
Magnetic fields are fundamental to the evolution of galaxies, playing a key role in the astrophysics of the interstellar medium and star formation. Large-scale ordered magnetic fields have been mapped in the Milky Way and nearby galaxies, but it is n
Externí odkaz:
http://arxiv.org/abs/2309.02034
Autor:
Berta, S., Stanley, F., Ismail, D., Cox, P., Neri, R., Yang, C., Young, A. J., Jin, S., Dannerbauer, H., Bakx, T. J., Beelen, A., Weiss, A., Nanni, A., Omont, A., van der Werf, P., Krips, M., Baker, A. J., Bendo, G., Borsato, E., Buat, V., Butler, K. M., Chartab, N., Cooray, A., Dye, S., Eales, S., Gavazzi, R., Hughes, D., Ivison, R. J., Jones, B. M., Lehnert, M., Marchetti, L., Messias, H., Negrello, M., Perez-Fournon, I., Riechers, D. A., Serjeant, S., Urquhart, S., Vlahakis, C.
Publikováno v:
A&A 678, A28 (2023)
The z-GAL survey observed 137 bright Herschel-selected targets with the IRAM NOrthern Extended Millimeter Array, with the aim to measure their redshift and study their properties. Several of them have been resolved into multiple sources. Consequently
Externí odkaz:
http://arxiv.org/abs/2307.15748
Autor:
Ismail, D., Beelen, A., Buat, V., Berta, S., Cox, P., Stanley, F., Young, A., Jin, S., Neri, R., Bakx, T., Dannerbauer, H., Butler, K., Cooray, A., Nanni, A., Omont, A., Serjeant, S., van der Werf, P., Vlahakis, C., Weiss, A., Yang, C., Baker, A. J., Bendo, G., Borsato, E., Chartab, N., Dye, S., Eales, S., Gavazzi, R., Hughes, D., Ivison, R., Krips, B. M. Jones M., Lehnert, M., Marchetti, L., Messias, H., Negrello, M., Perez-Fournon, I., Riechers, D. A., Urquhart, S.
Publikováno v:
A&A 678, A27 (2023)
(Abridged) We present the dust properties of 125 bright Herschel galaxies selected from the z-GAL survey. The large instantaneous bandwidth of NOEMA provides an exquisite sampling of the underlying dust continuum emission at 2 and 3 mm in the observe
Externí odkaz:
http://arxiv.org/abs/2307.15747
Autor:
Cox, P., Neri, R., Berta, S., Ismail, D., Stanley, F., Young, A., Jin, S., Bakx, T., Beelen, A., Dannerbauer, H., Krips, M., Lehnert, M., Omont, A., Riechers, D. A., Baker, A. J., Bendo, G., Borsato, E., Buat, V., Butler, K., Chartab, N., Cooray, A., Dye, S., Eales, S., Gavazzi, R., Hughes, D., Ivison, R., Jones, B. M., Marchetti, L., Messias, H., Nanni, A., Negrello, M., Perez-Fournon, I., Serjeant, S., Urquhart, S., Vlahakis, C., Weiss, A., van der Werf, P., Yang, C.
Publikováno v:
A&A 678, A26 (2023)
(Abridged) Using the IRAM NOEMA interferometer, we measures the redshifts of 126 bright galaxies detected in the Herschel H-ATLAS, HeLMS, and HerS surveys. We report reliable spectroscopic redshifts for a total of 124 of the Herschel-selected galaxie
Externí odkaz:
http://arxiv.org/abs/2307.15732
Autor:
Hagimoto, M., Bakx, T. J. L. C., Serjeant, S., Bendo, G. J., Urquhart, S. A., Eales, S., Harrington, K. C., Tamura, Y., Umehata, H., Berta, S., Cooray, A. R., Cox, P., De Zotti, G., Lehnert, M. D., Riechers, D. A., Scott, D., Temi, P., van der Werf, P. P., Yang, C., Amvrosiadis, A., Andreani, P. M., Baker, A. J., Beelen, A., Borsato, E., Buat, V., Butler, K. M., Dannerbauer, H., Dunne, L., Dye, S., Enia, A. F. M., Fan, L., Gavazzi, R., Gonzalez-Nuevo, J., Harris, A. I., Herrera, C. N., Hughes, D. H., Ismail, D., Ivison, R. J., Jones, B., Kohno, K., Krips, M., Lagache, G., Marchetti, L., Massardi, M., Messias, H., Negrello, M., Neri, R., Omont, A., Perez-Fournon, I., Sedgwick, C., Smith, M. W. L., Stanley, F., Verma, A., Vlahakis, C., Ward, B., Weiner, C., Weiss, A., Young, A. J.
We analyse the molecular and atomic emission lines of 71 bright Herschel-selected galaxies between redshifts 1.4 to 4.6 detected by the Atacama Large Millimetre/submillimetre Array. These lines include a total of 156 CO, [C I], and H2O emission lines
Externí odkaz:
http://arxiv.org/abs/2303.04830
Autor:
Stanley, F., Jones, B. M., Riechers, D. A., Yang, C., Berta, S., Cox, P., Bakx, T. J. L. C., Cooray, A., Dannerbauer, H., Dye, S., Hughes, D. H., Ivison, R. J., Jin, S., Lehnert, M., Neri, R., Omont, A., van der Werf, P., Weiss, A.
We present the results of a survey of CO(1-0) emission in 14 infrared luminous dusty star forming galaxies (DSFGs) at 2 < z < 4 with the NSF's Karl G. Jansky Very Large Array. All sources are detected in CO(1-0), with an ~1arcsec angular resolution.
Externí odkaz:
http://arxiv.org/abs/2301.12976
Autor:
Bendo, G. J., Urquhart, S. A., Serjeant, S., Bakx, T., Hagimoto, M., Cox, P., Neri, R., Lehnert, M. D., Dannerbauer, H., Amvrosiadis, A., Andreani, P., Baker, A. J., Beelen, A., Berta, S., Borsato, E., Buat, V., Butler, K. M., Cooray, A., De Zotti, G., Dunne, L., Dye, S., Eales, S., Enia, A., Fan, L., Gavazzi, R., González-Nuevo, J., Harris, A. I., Herrera, C. N., Hughes, D. H., Ismail, D., Jones, B. M., Kohno, K., Krips, M., Lagache, G., Marchetti, L., Massardi, M., Messias, H., Negrello, M., Omont, A., Pérez-Fournon, I., Riechers, D. A., Scott, D., Smith, M. W. L., Stanley, F., Tamura, Y., Temi, P., van der Werf, P., Verma, A., Vlahakis, C., Weiß, A., Yang, C., Young, A. J.
We present 101 and 151 GHz ALMA continuum images for 85 fields selected from Herschel observations that have 500 micron flux densities >80 mJy and 250-500 micron colours consistent with z > 2, most of which are expected to be gravitationally lensed o
Externí odkaz:
http://arxiv.org/abs/2301.02584