Zobrazeno 1 - 10
of 483
pro vyhledávání: '"Messias, H."'
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:
Carvajal, R., Matute, I., Afonso, J., Norris, R. P., Luken, K. J., Sánchez-Sáez, P., Cunha, P. A. C., Humphrey, A., Messias, H., Amarantidis, S., Barbosa, D., Cruz, H. A., Miranda, H., Paulino-Afonso, A., Pappalardo, C.
Publikováno v:
A&A 679, A101 (2023)
We developed and trained a pipeline of three machine learning (ML) models than can predict which sources are more likely to be an AGN and to be detected in specific radio surveys. Also, it can estimate redshift values for predicted radio-detectable A
Externí odkaz:
http://arxiv.org/abs/2309.11652
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:
Wong, A., Hatziminaoglou, E., Borkar, A., Popping, G., Pérez-Fournon, I., Poidevin, F., Stoehr, F., Messias, H.
The Atacama Large Millimetre/submillimetre Array (ALMA) is the world's most advanced radio interferometric facility, producing science data with an average rate of about 1 TB per day. After a process of calibration, imaging and quality assurance, the
Externí odkaz:
http://arxiv.org/abs/2305.05173
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:
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
Autor:
Urquhart, S. A., Bendo, G. J., Serjeant, S., Bakx, T., Hagimoto, M., Cox, P., Neri, R., Lehnert, M., Sedgwick, C., Weiner, C., 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., Gonzalez-Nuevo, J., Harris, A. I., Herrera, C. N., Hughes, D., Ismail, D., Ivison, R., Jin, S., Jones, B., Kohno, K., Krips, M., Lagache, G., Marchetti, L., Massardi, M., Messias, H., Negrello, M., Omont, A., Perez-Fournon, I., Riechers, D. A., Scott, D., Smith, M. W. L., Stanley, F., Tamura, Y., Temi, P., Vlahakis, C., Weiss, A., van der Werf, P., Verma, A., Yang, C., Young, A. J.
We present spectroscopic measurements for 71 galaxies associated with 62 of the brightest high-redshift submillimeter sources from the Southern fields of the Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS), while targeting 85 sources whi
Externí odkaz:
http://arxiv.org/abs/2201.07815
Autor:
Berta, S., Young, A. J., Cox, P., Neri, R., Jones, B. M., Baker, A. J., Omont, A., Dunne, L., Rosell, A. Carnero, Marchetti, L., Negrello, M., Yang, C., Riechers, D. A., Dannerbauer, H., Perez-Fournon, I., van der Werf, P., Bakx, T., Ivison, R. J., Beelen, A., Buat, V., Cooray, A., Cortzen, I., Dye, S., Eales, S., Gavazzi, R., Harris, A. I., Herrera, C. N., Hughes, D., Jin, S., Krips, M., Lagache, G., Lehnert, M., Messias, H., Serjeant, S., Stanley, F., Urquhart, S., Vlahakis, C., Weiss, A.
Publikováno v:
A&A 646, A122 (2021)
(Abridged) Exploiting the sensitivity and broad band width of NOEMA, we have studied the molecular gas and dust in the galaxy HerBS-89a, at z=2.95. High angular resolution images reveal a partial 1.0" diameter Einstein ring in the dust continuum emis
Externí odkaz:
http://arxiv.org/abs/2012.01448