Zobrazeno 1 - 10
of 107
pro vyhledávání: '"Clark, C. J. R."'
Autor:
Katsioli, S., Adam, R., Ade, P., Ajeddig, H., André, P., Artis, E., Aussel, H., Baes, M., Beelen, A., Benoît, A., Berta, S., Bing, L., Bourrion, O., Calvo, M., Catalano, A., Clark, C. J. R., De Looze, I., De Petris, M., Désert, F. -X., Doyle, S., Driessen, E. F. C., Ejlali, G., Galametz, M., Galliano, F., Gomez, A., Goupy, J., Hanser, C., Hughes, A., Kéruzoré, F., Kramer, C., Jones, A. P., Ladjelate, B., Lagache, G., Leclercq, S., Lestrade, J. -F., Macías-Pérez, J. F., Madden, S. C., Maury, A., Mauskopf, P., Mayet, F., Monfardini, A., Moyer-Anin, A., Muñoz-Echeverría, M., Nersesian, A., Pantoni, L., Paradis, D., Perotto, L., Pisano, G., Ponthieu, N., Revéret, V., Rigby, A. J., Ritacco, A., Romero, C., Roussel, H., Ruppin, F., Schuster, K., Sievers, A., Smith, M. W. L., Tedros, J., Tabatabaei, F., Tucker, C., Xilouris, E. M., Ysard, N., Zylka, R.
Publikováno v:
EPJ Web of conferences 293 (2024) 00026
In the framework of the IMEGIN Large Program, we used the NIKA2 camera on the IRAM 30-m telescope to observe the edge-on galaxy NGC 891 at 1.15 mm and 2 mm and at a FWHM of 11.1" and 17.6", respectively. Multiwavelength data enriched with the new NIK
Externí odkaz:
http://arxiv.org/abs/2310.04204
Autor:
Katsioli, S., Xilouris, E. M., Kramer, C., Adam, R., Ade, P., Ajeddig, H., André, P., Artis, E., Aussel, H., Baes, M., Beelen, A., Benoît, A., Berta, S., Bing, L., Bourrion, O., Calvo, M., Catalano, A., Clark, C. J. R., De Looze, I., De Petris, M., Désert, F. -X., Doyle, S., Driessen, E. F. C., Ejlali, G., Galametz, M., Galliano, F., Gomez, A., Goupy, J., Hanser, C., Hughes, A., Jones, A. P., Kéruzoré, F., Ladjelate, B., Lagache, G., Leclercq, S., Lestrade, J. -F., Macías-Pérez, J. -F., Madden, S. C., Maury, A., Mauskopf, P., Mayet, F., Monfardini, A., Muñoz-Echeverría, M., Nersesian, A., Pantoni, L., Paradis, D., Perotto, L., Pisano, G., Ponthieu, N., Revéret, V., Rigby, A. J., Ritacco, A., Romero, C., Roussel, H., Ruppin, F., Schuster, K., Sievers, A., Smith, M. W. L., Tedros, J., Tabatabaei, F., Tucker, C., Ysard, N., Zylka, R.
Publikováno v:
A&A 679, A7 (2023)
As the millimeter wavelength range remains a largely unexplored spectral region for galaxies, the IMEGIN large program aims to map the millimeter continuum emission of 22 nearby galaxies at 1.15 and 2 mm. Using the high-resolution maps produced by th
Externí odkaz:
http://arxiv.org/abs/2309.08403
Autor:
Bianchi, S., Casasola, V., Corbelli, E., Galliano, F., Magrini, L., Nersesian, A., Salvestrini, F., Baes, M., Cassara, L. P., Clark, C. J. R., De Looze, I., Jones, A. P., Madden, S. C., Mosenkov, A., Ysard, N.
Publikováno v:
A&A 664, A187 (2022)
Context: The far-infrared (FIR) and sub-millimeter (submm) emissivity of the Milky Way (MW) cirrus is an important benchmark for dust grain models. Dust masses in other galaxies are generally derived from the FIR/submm using the emission properties o
Externí odkaz:
http://arxiv.org/abs/2206.13375
Autor:
Roman-Duval, J., Jenkins, E. B., Tchernyshyov, K., Clark, C. J. R., De Cia, A., Gordon, K. D., Hamanowicz, A., Lebouteiller, V., Rafelski, M., Sandstrom, K., Werk, J., Merica-Jones, P. Yanchulova
The metallicity and gas density dependence of interstellar depletions, the dust-to-gas (D/G), and dust-to-metal (D/M) ratios have important implications for how accurately we can trace the chemical enrichment of the universe; either by using FIR dust
Externí odkaz:
http://arxiv.org/abs/2202.04765
Autor:
Scicluna, P., Kemper, F., McDonald, I., Srinivasan, S., Trejo, A., Wallström, S. H. J., Wouterloot, J. G. A., Cami, J., Greaves, J., He, Jinhua, Hoai, D. T., Kim, Hyosun, Jones, O. C., Shinnaga, H., Clark, C. J. R., Dharmawardena, T., Holland, W., Imai, H., van Loon, J. Th., Menten, K. M., Wesson, R., Chawner, H., Feng, S., Goldman, S., Liu, F. C., MacIsaac, H., Tang, J., Zeegers, S., Amada, K., Antoniou, V., Bemis, A., Boyer, M. L., Chapman, S., Chen, X., Cho, S. -H., Cui, L., Dell'Agli, F., Friberg, P., Fukaya, S., Gomez, H., Gong, Y., Hadjara, M., Haswell, C., Hirano, N., Hony, S., Izumiura, H., Jeste, M., Jiang, X., Kaminski, T., Keaveney, N., Kim, J., Kraemer, K. E., Kuan, Y. -J., Lagadec, E., Lee, C. F., Li, D., Liu, S. -Y., Liu, T., de Looze, I., Lykou, F., Maraston, C., Marshall, J. P., Matsuura, M., Min, C., Otsuka, M., Oyadomari, M., Parsons, H., Patel, N. A., Peeters, E., Pham, T. A., Qiu, J., Randall, S., Rau, G., Redman, M. P., Richards, A. M. S., Serjeant, S., Shi, C., Sloan, G. C., Smith, M. W. L., Suh, K. -W., Toalá, J. A., Uttenthaler, S., Ventura, P., Wang, B., Yamamura, I., Yang, T., Yun, Y., Zhang, F., Zhang, Y., Zhao, G., Zhu, M., Zijlstra, A. A.
The Nearby Evolved Stars Survey (NESS) is a volume-complete sample of $\sim$850 Galactic evolved stars within 3\,kpc at (sub-)mm wavelengths, observed in the CO $J = $ (2$-$1) and (3$-$2) rotational lines, and the sub-mm continuum, using the James Cl
Externí odkaz:
http://arxiv.org/abs/2110.12562
Autor:
De Looze, I., Lamperti, I., Saintonge, A., Relano, M., Smith, M. W. L., Clark, C. J. R., Wilson, C. D., Decleir, M., Jones, A. P., Kennicutt, R. C., Accurso, G., Brinks, E., Bureau, M., Cigan, P., Clements, D. L., De Vis, P., Fanciullo, L, Gao, Y., Gear, W. K., Ho, L. C., Hwang, H. S., Michalowski, M. J., Lee, J. C., Li, C., Lin, L., Liu, T., Lomaeva, M., Pan, H. -A., Sargent, M., Williams, T., Xiao, T., Zhu, M.
Scaling laws of dust, HI gas and metal mass with stellar mass, specific star formation rate and metallicity are crucial to our understanding of the buildup of galaxies through their enrichment with metals and dust. In this work, we analyse how the du
Externí odkaz:
http://arxiv.org/abs/2006.01856
Autor:
Dobbels, W., Baes, M., Viaene, S., Bianchi, S., Davies, J. I., Casasola, V., Clark, C. J. R., Fritz, J., Galametz, M., Galliano, F., Mosenkov, A., Nersesian, A., Trčka, A.
Publikováno v:
A&A 634, A57 (2020)
Dust plays an important role in shaping a galaxy's spectral energy distribution (SED). It absorbs ultraviolet (UV) to near-infrared (NIR) radiation and re-emits this energy in the far-infrared (FIR). The FIR is essential to understand dust in galaxie
Externí odkaz:
http://arxiv.org/abs/1910.06330
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:
Bianchi, S., Casasola, V., Baes, M., Clark, C. J. R., Corbelli, E., Davies, J. I., De Looze, I., De Vis, P., Dobbels, W., Galametz, M., Galliano, F., Jones, A. P., Madden, S. C., Magrini, L., Mosenkov, A., Nersesian, A., Viaene, S., Xilouris, E. M., Ysard, N.
Publikováno v:
A&A 631, A102 (2019)
Aims: We compare the far-infrared to sub-millimetre dust emission properties measured in high Galactic latitude cirrus with those determined in a sample of 204 late-type DustPedia galaxies. The aim is to verify if it is appropriate to use Milky Way d
Externí odkaz:
http://arxiv.org/abs/1909.12692
Autor:
Davies, J. I., Nersesian, A., Baes, M., Bianchi, S., Casasola, V., Cassara, L. P., Clark, C. J. R., De Looze, I., De Vis, P., Evans, R., Fritz, J., Galametz, M., Galliano, F., Jones, A. P., Lianou, S., Madden, S. C., Mosenkov, A. V., Smith, M. W. L., Verstocken, S., Viaene, S., Vika, M., Xilouris, E., Ysard, N.
We use a sub-set of the DustPedia galaxy sample (461 galaxies) to investigate the effect the environment has had on galaxies. We consider Virgo cluster and field samples and also assign a density contrast parameter to each galaxy, as defined by the l
Externí odkaz:
http://arxiv.org/abs/1904.13217