Zobrazeno 1 - 10
of 1 018
pro vyhledávání: '"Maddox, S"'
We present a self-consistent cross-calibration of the three main molecular gas mass tracers in galaxies, the $\rm ^{12}CO$(1-0), [CI]($^3P_1$-$^3P_0$) lines, and the submm dust continuum emission, using a sample of 407 galaxies, ranging from local di
Externí odkaz:
http://arxiv.org/abs/2208.01622
Autor:
Ward, B. A., Eales, S. A., Pons, E., Smith, M. W. L., McMahon, R. G., Dunne, L., Ivison, R. J., Maddox, S. J., Negrello, M.
In this paper we present the third data release (DR3) of the Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS). We identify likely near-infrared counterparts to submillimetre sources in the South Galactic Pole (SGP) field using the VISTA V
Externí odkaz:
http://arxiv.org/abs/2202.07687
Publikováno v:
2021 MNRAS 501 2537
We present ALMA observations of a small but statistically complete sample of twelve 250 micron selected galaxies at $z=0.35$ designed to measure their dust submillimeter continuum emission as well as their CO(1-0) and atomic carbon [CI](3P1-3P0) spec
Externí odkaz:
http://arxiv.org/abs/2111.09067
Publikováno v:
MNRAS Volume 505, Issue 3, 2021, Pages 3228-3246
We build a rigorous statistical framework to provide constraints on the chemical and dust evolution parameters for nearby late-type galaxies with a wide range of gas fractions ($3\%
Externí odkaz:
http://arxiv.org/abs/2107.03382
Autor:
Montaña, A., Zavala, J. A., Aretxaga, I., Hughes, D. H., Ivison, R. J., Pope, A., Sánchez-Argüelles, D., Wilson, G. W., Yun, M., Cantua, O. A., McCrackan, M., Michałowski, M. J., Valiante, E., Arumugam, V., Casey, C. M., Chávez, R., Colín-Beltrán, E., Dannerbauer, H., Dunlop, J. S., Dunne, L., Eales, S., Ferrusca, D., Gómez-Rivera, V., Gómez-Ruiz, A. I., de la Luz, V. H., Maddox, S. J., Narayanan, G., Omont, A., Rodríguez-Montoya, I., Serjeant, S., Schloerb, F. P., Velázquez, M., Ventura-González, S., van der Werf, P., Zeballos, M.
We present LMT/AzTEC 1.1mm observations of $\sim100$ luminous high-redshift dusty star-forming galaxy candidates from the $\sim600\,$sq.deg $Herschel$-ATLAS survey, selected on the basis of their SPIRE red far-infrared colours and with $S_{500\mu\rm
Externí odkaz:
http://arxiv.org/abs/2106.03286
Autor:
Bonavera, L., González-Nuevo, J., Cueli, M. M., Ronconi, T., Migliaccio, M., Dunne, L., Lapi, A., Maddox, S. J., Negrello, M.
Publikováno v:
A&A 639, A128 (2020)
Context. As recently demonstrated, high-z submillimetre galaxies (SMGs) are the perfect background sample for tracing the mass density profiles of galaxies and clusters (baryonic and dark matter) and their time-evolution through gravitational lensing
Externí odkaz:
http://arxiv.org/abs/2006.09185
Autor:
Maddox, S. J., Dunne, L.
We describe the method used to detect sources for the Herschel-ATLAS survey. The method is to filter the individual bands using a matched filter, based on the point-spread function (PSF) and confusion noise, and then form the inverse variance weighte
Externí odkaz:
http://arxiv.org/abs/2002.10840
Autor:
Dunne, L., Zhang, Z., de Vis, P., Clark, C. J. R., Oteo, I., Maddox, S. J., Cigan, P., de Zotti, G., Gomez, H. L., Ivison, R. J., Rowlands, K., Smith, M. W. L., van der Werf, P., Vlahakis, C., Millard, J. S.
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 2018, 479, p.1221-1239
The Herschel-ATLAS unbiased survey of cold dust in the local Universe is dominated by a surprising population of very blue (FUV-K < 3.5), dust-rich galaxies with high gas fractions (f_HI = M_HI/(M*+M_HI)>0.5)). Dubbed `Blue and Dusty Gas Rich Sources
Externí odkaz:
http://arxiv.org/abs/1910.04596
Autor:
Amvrosiadis, A., Valiante, E., Gonzalez-Nuevo, J., Maddox, S. J., Negrello, M., Eales, S. A., Dunne, L., Wang, L., van Kampen, E., De Zotti, G., Smith, M. W. L., Andreani, P., Greenslade, J., Tai-An, C., Michałowski, M. J.
We present measurements of the angular correlation function of sub-millimeter (sub-mm) galaxies (SMGs) identified in four out of the five fields of the Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS) - GAMA-9h, GAMA-12h, GAMA-15h and NGP
Externí odkaz:
http://arxiv.org/abs/1811.02870