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Start Over Author "Furlanetto, C." Publisher oxford university press (oup)
26 results on '"Furlanetto, C."'

2. The puzzling origin of massive compact galaxies in MaNGA

Author

Schnorr-Müller, A, primary, Trevisan, M, additional, Riffel, R, additional, Chies-Santos, A L, additional, Furlanetto, C, additional, Ricci, T V, additional, Lohmann, F S, additional, Flores-Freitas, R, additional, Mallmann, N D, additional, and Alamo-Martínez, K A, additional

Published
2021
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3. Erratum: The Herschel Bright Sources (HerBS): sample definition and SCUBA-2 observations

Author

Bakx, Tom J L C, primary, Eales, S A, primary, Negrello, M, primary, Smith, M W L, primary, Valiante, E, primary, Holland, W S, primary, Baes, M, primary, Bourne, N, primary, Clements, D L, primary, Dannerbauer, H, primary, De Zotti, G, primary, Dunne, L, primary, Dye, S, primary, Furlanetto, C, primary, Ivison, R J, primary, Maddox, S, primary, Marchetti, L, primary, Michałowski, M J, primary, Omont, A, primary, Oteo, I, primary, Wardlow, J L, primary, van der Werf, P, primary, and Yang, C, primary

Published
2020
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4. Modelling high-resolution ALMA observations of strongly lensed highly star-forming galaxies detected by Herschel★

Author

Dye, S, primary, Furlanetto, C, additional, Dunne, L, additional, Eales, S A, additional, Negrello, M, additional, Nayyeri, H, additional, van der Werf, P P, additional, Serjeant, S, additional, Farrah, D, additional, Michałowski, M J, additional, Baes, M, additional, Marchetti, L, additional, Cooray, A, additional, Riechers, D A, additional, and Amvrosiadis, A, additional

Published
2018
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5. ALMA observations of lensed Herschel sources: testing the dark matter halo paradigm

Author

Amvrosiadis, A, primary, Eales, S A, additional, Negrello, M, additional, Marchetti, L, additional, Smith, M W L, additional, Bourne, N, additional, Clements, D L, additional, De Zotti, G, additional, Dunne, L, additional, Dye, S, additional, Furlanetto, C, additional, Ivison, R J, additional, Maddox, S J, additional, Valiante, E, additional, Baes, M, additional, Baker, A J, additional, Cooray, A, additional, Crawford, S M, additional, Frayer, D, additional, Harris, A, additional, Michałowski, M J, additional, Nayyeri, H, additional, Oliver, S, additional, Riechers, D A, additional, Serjeant, S, additional, and Vaccari, M, additional

Published
2018
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7. The Herschel Bright Sources (HerBS): sample definition and SCUBA-2 observations

Author

Bakx, Tom J. L. C., primary, Eales, S. A., additional, Negrello, M., additional, Smith, M. W. L., additional, Valiante, E., additional, Holland, W. S., additional, Baes, M., additional, Bourne, N., additional, Clements, D. L., additional, Dannerbauer, H., additional, De Zotti, G., additional, Dunne, L., additional, Dye, S., additional, Furlanetto, C., additional, Ivison, R. J., additional, Maddox, S., additional, Marchetti, L., additional, Michałowski, M. J., additional, Omont, A., additional, Oteo, I., additional, Wardlow, J. L., additional, van der Werf, P., additional, and Yang, C., additional

Published
2017
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8. The mean star formation rates of unobscured QSOs: searching for evidence of suppressed or enhanced star formation

Author

Stanley, F., primary, Alexander, D. M., additional, Harrison, C. M., additional, Rosario, D. J., additional, Wang, L., additional, Aird, J. A., additional, Bourne, N., additional, Dunne, L., additional, Dye, S., additional, Eales, S., additional, Knudsen, K. K., additional, Michałowski, M. J., additional, Valiante, E., additional, De Zotti, G., additional, Furlanetto, C., additional, Ivison, R., additional, Maddox, S., additional, and Smith, M. W. L., additional

Published
2017
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10. VALES I: the molecular gas content in star-forming dusty H-ATLAS galaxies up to z = 0.35

Author

Villanueva, V., primary, Ibar, E., additional, Hughes, T. M., additional, Lara-López, M. A., additional, Dunne, L., additional, Eales, S., additional, Ivison, R. J., additional, Aravena, M., additional, Baes, M., additional, Bourne, N., additional, Cassata, P., additional, Cooray, A., additional, Dannerbauer, H., additional, Davies, L. J. M., additional, Driver, S. P., additional, Dye, S., additional, Furlanetto, C., additional, Herrera-Camus, R., additional, Maddox, S. J., additional, Michałowski, M. J., additional, Molina, J., additional, Riechers, D., additional, Sansom, A. E., additional, Smith, M. W. L., additional, Rodighiero, G., additional, Valiante, E., additional, and van der Werf, P., additional

Published
2017
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11. VALES – III. The calibration between the dust continuum and interstellar gas content of star-forming galaxies

Author

Hughes, T. M., primary, Ibar, E., additional, Villanueva, V., additional, Aravena, M., additional, Baes, M., additional, Bourne, N., additional, Cooray, A., additional, Davies, L. J. M., additional, Driver, S., additional, Dunne, L., additional, Dye, S., additional, Eales, S., additional, Furlanetto, C., additional, Herrera-Camus, R., additional, Ivison, R. J., additional, van Kampen, E., additional, Lara-López, M. A., additional, Maddox, S., additional, Michałowski, M. J., additional, Oteo, I., additional, Smith, D., additional, Smith, M. W. L., additional, Valiante, E., additional, van der Werf, P., additional, Viaene, S., additional, and Xue, Y. Q., additional

Published
2017
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12. TheHerschel-ATLAS: a sample of 500 μm-selected lensed galaxies over 600 deg2

Author

Negrello, M., primary, Amber, S., additional, Amvrosiadis, A., additional, Cai, Z.-Y., additional, Lapi, A., additional, Gonzalez-Nuevo, J., additional, De Zotti, G., additional, Furlanetto, C., additional, Maddox, S. J., additional, Allen, M., additional, Bakx, T., additional, Bussmann, R. S., additional, Cooray, A., additional, Covone, G., additional, Danese, L., additional, Dannerbauer, H., additional, Fu, H., additional, Greenslade, J., additional, Gurwell, M., additional, Hopwood, R., additional, Koopmans, L. V. E., additional, Napolitano, N., additional, Nayyeri, H., additional, Omont, A., additional, Petrillo, C. E., additional, Riechers, D. A., additional, Serjeant, S., additional, Tortora, C., additional, Valiante, E., additional, Verdoes Kleijn, G., additional, Vernardos, G., additional, Wardlow, J. L., additional, Baes, M., additional, Baker, A. J., additional, Bourne, N., additional, Clements, D., additional, Crawford, S. M., additional, Dye, S., additional, Dunne, L., additional, Eales, S., additional, Ivison, R. J., additional, Marchetti, L., additional, Michałowski, M. J., additional, Smith, M. W. L., additional, Vaccari, M., additional, and van der Werf, P., additional

Published
2016
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13. Herschel-ATLAS: revealing dust build-up and decline across gas, dust and stellar mass selected samples – I. Scaling relations

Author

De Vis, P., primary, Dunne, L., additional, Maddox, S., additional, Gomez, H. L., additional, Clark, C. J. R., additional, Bauer, A. E., additional, Viaene, S., additional, Schofield, S. P., additional, Baes, M., additional, Baker, A. J., additional, Bourne, N., additional, Driver, S. P., additional, Dye, S., additional, Eales, S. A., additional, Furlanetto, C., additional, Ivison, R. J., additional, Robotham, A. S. G., additional, Rowlands, K., additional, Smith, D. J. B., additional, Smith, M. W. L., additional, Valiante, E., additional, and Wright, A. H., additional

Published
2016
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14. TheHerschel -ATLAS data release 1 – I. Maps, catalogues and number counts

Author

Valiante, E., primary, Smith, M. W. L., additional, Eales, S., additional, Maddox, S. J., additional, Ibar, E., additional, Hopwood, R., additional, Dunne, L., additional, Cigan, P. J., additional, Dye, S., additional, Pascale, E., additional, Rigby, E. E., additional, Bourne, N., additional, Furlanetto, C., additional, and Ivison, R. J., additional

Published
2016
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15. TheHerschel-ATLAS Data Release 1 – II. Multi-wavelength counterparts to submillimetre sources

Author

Bourne, N., primary, Dunne, L., additional, Maddox, S. J., additional, Dye, S., additional, Furlanetto, C., additional, Hoyos, C., additional, Smith, D. J. B., additional, Eales, S., additional, Smith, M. W. L., additional, Valiante, E., additional, Alpaslan, M., additional, Andrae, E., additional, Baldry, I. K., additional, Cluver, M. E., additional, Cooray, A., additional, Driver, S. P., additional, Dunlop, J. S., additional, Grootes, M. W., additional, Ivison, R. J., additional, Jarrett, T. H., additional, Liske, J., additional, Madore, B. F., additional, Popescu, C. C., additional, Robotham, A. G., additional, Rowlands, K., additional, Seibert, M., additional, Thompson, M. A., additional, Tuffs, R. J., additional, Viaene, S., additional, and Wright, A. H., additional

Published
2016
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16. H-ATLAS: the far-infrared properties of galaxies in and around the Coma cluster

Author

Fuller, C., primary, Davies, J. I., additional, Smith, M. W. L., additional, Valiante, E., additional, Eales, S., additional, Bourne, N., additional, Dunne, L., additional, Dye, S., additional, Furlanetto, C., additional, Ibar, E., additional, Ivison, R., additional, Maddox, S., additional, Sansom, A., additional, Michałowski, M. J., additional, and Davis, T., additional

Published
2016
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17. Revealing the complex nature of the strong gravitationally lensed system H-ATLAS J090311.6+003906 using ALMA

Author

Dye, S., primary, Furlanetto, C., additional, Swinbank, A. M., additional, Vlahakis, C., additional, Nightingale, J. W., additional, Dunne, L., additional, Eales, S. A., additional, Smail, Ian, additional, Oteo, I., additional, Hunter, T., additional, Negrello, M., additional, Dannerbauer, H., additional, Ivison, R. J., additional, Gavazzi, R., additional, Cooray, A., additional, and Werf, P. van der, additional

Published
2015
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18. Herschel-ATLAS: the surprising diversity of dust-selected galaxies in the local submillimetre Universe

Author

Clark, C. J. R., primary, Dunne, L., additional, Gomez, H. L., additional, Maddox, S., additional, De Vis, P., additional, Smith, M. W. L., additional, Eales, S. A., additional, Baes, M., additional, Bendo, G. J., additional, Bourne, N., additional, Driver, S. P., additional, Dye, S., additional, Furlanetto, C., additional, Grootes, M. W., additional, Ivison, R. J., additional, Schofield, S. P., additional, Robotham, A. S. G., additional, Rowlands, K., additional, Valiante, E., additional, Vlahakis, C., additional, Werf, P. van der, additional, Wright, A. H., additional, and de Zotti, G., additional

Published
2015
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19. A multiwavelength exploration of the [C ii]/IR ratio in H-ATLAS/GAMA galaxies out to z = 0.2

Author

Ibar, E., primary, Lara-López, M. A., additional, Herrera-Camus, R., additional, Hopwood, R., additional, Bauer, A., additional, Ivison, R. J., additional, Michałowski, M. J., additional, Dannerbauer, H., additional, van der Werf, P., additional, Riechers, D., additional, Bourne, N., additional, Baes, M., additional, Valtchanov, I., additional, Dunne, L., additional, Verma, A., additional, Brough, S., additional, Cooray, A., additional, De Zotti,  G., additional, Dye, S., additional, Eales, S., additional, Furlanetto, C., additional, Maddox, S., additional, Smith, M., additional, Steele, O., additional, Thomas, D., additional, and Valiante, E., additional

Published
2015
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20. Far-infrared observations of an unbiased sample of gamma-ray burst host galaxies

Author

Kohn, S. A., primary, Michałowski, M. J., additional, Bourne, N., additional, Baes, M., additional, Fritz, J., additional, Cooray, A., additional, de Looze, I., additional, De Zotti, G., additional, Dannerbauer, H., additional, Dunne, L., additional, Dye, S., additional, Eales, S., additional, Furlanetto, C., additional, Gonzalez-Nuevo, J., additional, Ibar, E., additional, Ivison, R. J., additional, Maddox, S. J., additional, Scott, D., additional, Smith, D. J. B., additional, Smith, M. W. L., additional, Symeonidis, M., additional, and Valiante, E., additional

Published
2015
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21. The Herschel Bright Sources (HerBS): sample definition and SCUBA-2 observations

Author

Bakx, Tom J. L. C., Eales, S. A., Negrello, M., Smith, M. W. L., Valiante, E., Holland, W. S., Baes, M., Bourne, N., Clements, D. L., Dannerbauer, H., De Zotti, G., Dunne, L., Dye, S., Furlanetto, C., Ivison, R. J., Maddox, S., Marchetti, L., Michałowski, M. J., Omont, A., Oteo, I., Wardlow, J. L., van der Werf, P., Yang, C., Bakx, Tom J. L. C., Eales, S. A., Negrello, M., Smith, M. W. L., Valiante, E., Holland, W. S., Baes, M., Bourne, N., Clements, D. L., Dannerbauer, H., De Zotti, G., Dunne, L., Dye, S., Furlanetto, C., Ivison, R. J., Maddox, S., Marchetti, L., Michałowski, M. J., Omont, A., Oteo, I., Wardlow, J. L., van der Werf, P., and Yang, C.

Abstract

We present the Herschel Bright Sources (HerBS) sample, a sample of bright, high-redshift Herschel sources detected in the 616.4 square degree H-ATLAS survey. The HerBS sample contains 209 galaxies, selected with a 500 µm flux density greater than 80 mJy and an estimated redshift greater than 2. The sample consists of a combination of HyLIRGs and lensed ULIRGs during the epoch of peak cosmic star formation. In this paper, we present SCUBA-2 observations at 850 µm of 189 galaxies of the HerBS sample, 152 of these sources were detected. We fit a spectral template to the Herschel-SPIRE and 850 µm SCUBA-2 flux densities of 22 sources with spectroscopically determined redshifts, using a two-component modified blackbody spectrum as a template. We find a cold- and hot-dust temperature of 21.29+1.35 −1.66 K and 45.80+2.88 −3.48 K, a cold-to-hot dust mass ratio of 26.62+5.61 −6.74 and a β of 1.83+0.14 −0.28. The poor quality of the fit suggests that the sample of galaxies is too diverse to be explained by our simple model. Comparison of our sample to a galaxy evolution model indicates that the fraction of lenses is high. Out of the 152 SCUBA-2 detected galaxies, the model predicts 128.4 ± 2.1 of those galaxies to be lensed (84.5%). The SPIRE 500 µm flux suggests that out of all 209 HerBS sources, we expect 158.1 ± 1.7 lensed sources, giving a total lensing fraction of 76 per cent.

22. ALMA observations of lensed Herschel sources: testing the dark matter halo paradigm

Author

Amvrosiadis, A., Eales, S. A., Negrello, M., Marchetti, L., Smith, M. W. L., Bourne, N., Clements, D. L., De Zotti, G., Dunne, L., Dye, S., Furlanetto, C., Ivison, R. J., Maddox, S. J., Valiante, E., Baes, M., Baker, A. J., Cooray, A., Crawford, S. M., Frayer, D., Harris, A., Michałowski, M. J., Nayyeri, H., Oliver, S., Riechers, D. A., Serjeant, S., Vaccari, M., Amvrosiadis, A., Eales, S. A., Negrello, M., Marchetti, L., Smith, M. W. L., Bourne, N., Clements, D. L., De Zotti, G., Dunne, L., Dye, S., Furlanetto, C., Ivison, R. J., Maddox, S. J., Valiante, E., Baes, M., Baker, A. J., Cooray, A., Crawford, S. M., Frayer, D., Harris, A., Michałowski, M. J., Nayyeri, H., Oliver, S., Riechers, D. A., Serjeant, S., and Vaccari, M.

Abstract

With the advent of wide-area submillimetre surveys, a large number of high-redshift gravitationally lensed dusty star-forming galaxies have been revealed. Because of the simplicity of the selection criteria for candidate lensed sources in such surveys, identified as those with S500 μm > 100 mJy, uncertainties associated with the modelling of the selection function are expunged. The combination of these attributes makes submillimetre surveys ideal for the study of strong lens statistics. We carried out a pilot study of the lensing statistics of submillimetre-selected sources by making observations with the Atacama Large Millimeter Array (ALMA) of a sample of strongly lensed sources selected from surveys carried out with the Herschel Space Observatory. We attempted to reproduce the distribution of image separations for the lensed sources using a halo mass function taken from a numerical simulation that contains both dark matter and baryons. We used three different density distributions, one based on analytical fits to the haloes formed in the EAGLE simulation and two density distributions [Singular Isothermal Sphere (SIS) and SISSA] that have been used before in lensing studies. We found that we could reproduce the observed distribution with all three density distributions, as long as we imposed an upper mass transition of ∼1013 M⊙ for the SIS and SISSA models, above which we assumed that the density distribution could be represented by a Navarro–Frenk–White profile. We show that we would need a sample of ∼500 lensed sources to distinguish between the density distributions, which is practical given the predicted number of lensed sources in the Herschel surveys.

23. Erratum: The Herschel Bright Sources (HerBS): sample definition and SCUBA-2 observations

Author

Bakx, Tom J L C, Eales, S A, Negrello, M, Smith, M W L, Valiante, E, Holland, W S, Baes, M, Bourne, N, Clements, D L, Dannerbauer, H, De Zotti, G, Dunne, L, Dye, S, Furlanetto, C, Ivison, R J, Maddox, S, Marchetti, L, Michałowski, M J, Omont, A, Oteo, I, Wardlow, J L, van der Werf, P, Yang, C, Bakx, Tom J L C, Eales, S A, Negrello, M, Smith, M W L, Valiante, E, Holland, W S, Baes, M, Bourne, N, Clements, D L, Dannerbauer, H, De Zotti, G, Dunne, L, Dye, S, Furlanetto, C, Ivison, R J, Maddox, S, Marchetti, L, Michałowski, M J, Omont, A, Oteo, I, Wardlow, J L, van der Werf, P, and Yang, C

24. Modelling high resolution ALMA observations of strongly lensed highly star forming galaxies detected by Herschel

Author

Dye, S., Furlanetto, C., Dunne, L., Eales, S. A., Negrello, M., Nayyeri, H., van der Werf, P. P., Serjeant, S., Farrah, D., Michałowski, M. J., Baes, M., Marchetti, L., Cooray, A., Riechers, D. A., Amvrosiadis, A., Dye, S., Furlanetto, C., Dunne, L., Eales, S. A., Negrello, M., Nayyeri, H., van der Werf, P. P., Serjeant, S., Farrah, D., Michałowski, M. J., Baes, M., Marchetti, L., Cooray, A., Riechers, D. A., and Amvrosiadis, A.

Abstract

We have modelled ∼ 0.1 arcsec resolution ALMA imaging of six strong gravitationally lensed galaxies detected by the Herschel Space Observatory. Our modelling recovers mass properties of the lensing galaxies and, by determining magnification factors, intrinsic properties of the lensed sub-millimetre sources. We find that the lensed galaxies all have high ratios of star formation rate to dust mass, consistent with or higher than the mean ratio for high redshift sub-millimetre galaxies and low redshift ultra-luminous infra-red galaxies. Source reconstruction reveals that most galaxies exhibit disturbed morphologies. Both the cleaned image plane data and the directly observed interferometric visibilities have been modelled, enabling comparison of both approaches. In the majority of cases, the recovered lens models are consistent between methods, all six having mass density profiles that are close to isothermal. However, one system with poor signal to noise shows mildly significant differences.

25. Erratum: The Herschel Bright Sources (HerBS): sample definition and SCUBA-2 observations

Author

Bakx, Tom J L C, Eales, S A, Negrello, M, Smith, M W L, Valiante, E, Holland, W S, Baes, M, Bourne, N, Clements, D L, Dannerbauer, H, De Zotti, G, Dunne, L, Dye, S, Furlanetto, C, Ivison, R J, Maddox, S, Marchetti, L, Michałowski, M J, Omont, A, Oteo, I, Wardlow, J L, van der Werf, P, Yang, C, Bakx, Tom J L C, Eales, S A, Negrello, M, Smith, M W L, Valiante, E, Holland, W S, Baes, M, Bourne, N, Clements, D L, Dannerbauer, H, De Zotti, G, Dunne, L, Dye, S, Furlanetto, C, Ivison, R J, Maddox, S, Marchetti, L, Michałowski, M J, Omont, A, Oteo, I, Wardlow, J L, van der Werf, P, and Yang, C

26. Modelling high resolution ALMA observations of strongly lensed highly star forming galaxies detected by Herschel

Author

Dye, S., Furlanetto, C., Dunne, L., Eales, S. A., Negrello, M., Nayyeri, H., van der Werf, P. P., Serjeant, S., Farrah, D., Michałowski, M. J., Baes, M., Marchetti, L., Cooray, A., Riechers, D. A., Amvrosiadis, A., Dye, S., Furlanetto, C., Dunne, L., Eales, S. A., Negrello, M., Nayyeri, H., van der Werf, P. P., Serjeant, S., Farrah, D., Michałowski, M. J., Baes, M., Marchetti, L., Cooray, A., Riechers, D. A., and Amvrosiadis, A.

Abstract

We have modelled ∼ 0.1 arcsec resolution ALMA imaging of six strong gravitationally lensed galaxies detected by the Herschel Space Observatory. Our modelling recovers mass properties of the lensing galaxies and, by determining magnification factors, intrinsic properties of the lensed sub-millimetre sources. We find that the lensed galaxies all have high ratios of star formation rate to dust mass, consistent with or higher than the mean ratio for high redshift sub-millimetre galaxies and low redshift ultra-luminous infra-red galaxies. Source reconstruction reveals that most galaxies exhibit disturbed morphologies. Both the cleaned image plane data and the directly observed interferometric visibilities have been modelled, enabling comparison of both approaches. In the majority of cases, the recovered lens models are consistent between methods, all six having mass density profiles that are close to isothermal. However, one system with poor signal to noise shows mildly significant differences.

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