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1. The VANDELS ESO public spectroscopic survey: The spectroscopic measurements catalogue

Author

Talia, M., primary, Schreiber, C., additional, Garilli, B., additional, Pentericci, L., additional, Pozzetti, L., additional, Zamorani, G., additional, Cullen, F., additional, Moresco, M., additional, Calabrò, A., additional, Castellano, M., additional, Fynbo, J. P. U., additional, Guaita, L., additional, Marchi, F., additional, Mascia, S., additional, McLure, R., additional, Mignoli, M., additional, Pompei, E., additional, Vanzella, E., additional, Bongiorno, A., additional, Vietri, G., additional, Amorín, R. O., additional, Bolzonella, M., additional, Carnall, A. C., additional, Cimatti, A., additional, Cresci, G., additional, Cristiani, S., additional, Cucciati, O., additional, Dunlop, J. S., additional, Fontanot, F., additional, Franzetti, P., additional, Gargiulo, A., additional, Hamadouche, M. L., additional, Hathi, N. P., additional, Hibon, P., additional, Iovino, A., additional, Koekemoer, A. M., additional, Mannucci, F., additional, McLeod, D. J., additional, and Saldana-Lopez, A., additional

Published
2023
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2. COSMOS2020: UV-selected galaxies at z ≥ 7.5

Author

Kauffmann, O. B., primary, Ilbert, O., additional, Weaver, J. R., additional, McCracken, H. J., additional, Milvang-Jensen, B., additional, Brammer, G., additional, Davidzon, I., additional, Le Fèvre, O., additional, Liu, D., additional, Mobasher, B., additional, Moneti, A., additional, Shuntov, M., additional, Toft, S., additional, Casey, C. M., additional, Dunlop, J. S., additional, Kartaltepe, J. S., additional, Koekemoer, A. M., additional, Sanders, D. B., additional, and Tresse, L., additional

Published
2022
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3. The ASTRODEEP-GS43 catalogue: New photometry and redshifts for the CANDELS GOODS-South field

Author

Merlin, E., primary, Castellano, M., additional, Santini, P., additional, Cipolletta, G., additional, Boutsia, K., additional, Schreiber, C., additional, Buitrago, F., additional, Fontana, A., additional, Elbaz, D., additional, Dunlop, J., additional, Grazian, A., additional, McLure, R., additional, McLeod, D., additional, Nonino, M., additional, Milvang-Jensen, B., additional, Derriere, S., additional, Hathi, N. P., additional, Pentericci, L., additional, Fortuni, F., additional, and Calabrò, A., additional

Published
2021
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4. Low-frequency radio spectra of submillimetre galaxies in the Lockman Hole

Author

Ramasawmy, J., primary, Geach, J. E., additional, Hardcastle, M. J., additional, Best, P. N., additional, Bonato, M., additional, Bondi, M., additional, Calistro Rivera, G., additional, Cochrane, R. K., additional, Conway, J. E., additional, Coppin, K., additional, Duncan, K. J., additional, Dunlop, J. S., additional, Franco, M., additional, García-Vergara, C., additional, Jarvis, M. J., additional, Kondapally, R., additional, McCheyne, I., additional, Prandoni, I., additional, Röttgering, H. J. A., additional, Smith, D. J. B., additional, Tasse, C., additional, and Wang, L., additional

Published
2021
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5. The VANDELS ESO public spectroscopic survey

Author

Garilli, B., primary, McLure, R., additional, Pentericci, L., additional, Franzetti, P., additional, Gargiulo, A., additional, Carnall, A., additional, Cucciati, O., additional, Iovino, A., additional, Amorin, R., additional, Bolzonella, M., additional, Bongiorno, A., additional, Castellano, M., additional, Cimatti, A., additional, Cirasuolo, M., additional, Cullen, F., additional, Dunlop, J., additional, Elbaz, D., additional, Finkelstein, S., additional, Fontana, A., additional, Fontanot, F., additional, Fumana, M., additional, Guaita, L., additional, Hartley, W., additional, Jarvis, M., additional, Juneau, S., additional, Maccagni, D., additional, McLeod, D., additional, Nandra, K., additional, Pompei, E., additional, Pozzetti, L., additional, Scodeggio, M., additional, Talia, M., additional, Calabrò, A., additional, Cresci, G., additional, Fynbo, J. P. U., additional, Hathi, N. P., additional, Hibon, P., additional, Koekemoer, A. M., additional, Magliocchetti, M., additional, Salvato, M., additional, Vietri, G., additional, Zamorani, G., additional, Almaini, O., additional, Balestra, I., additional, Bardelli, S., additional, Begley, R., additional, Brammer, G., additional, Bell, E. F., additional, Bowler, R. A. A., additional, Brusa, M., additional, Buitrago, F., additional, Caputi, C., additional, Cassata, P., additional, Charlot, S., additional, Citro, A., additional, Cristiani, S., additional, Curtis-Lake, E., additional, Dickinson, M., additional, Fazio, G., additional, Ferguson, H. C., additional, Fiore, F., additional, Franco, M., additional, Georgakakis, A., additional, Giavalisco, M., additional, Grazian, A., additional, Hamadouche, M., additional, Jung, I., additional, Kim, S., additional, Khusanova, Y., additional, Le Fèvre, O., additional, Longhetti, M., additional, Lotz, J., additional, Mannucci, F., additional, Maltby, D., additional, Matsuoka, K., additional, Mendez-Hernandez, H., additional, Mendez-Abreu, J., additional, Mignoli, M., additional, Moresco, M., additional, Nonino, M., additional, Pannella, M., additional, Papovich, C., additional, Popesso, P., additional, Roberts-Borsani, G., additional, Rosario, D. J., additional, Saldana-Lopez, A., additional, Santini, P., additional, Saxena, A., additional, Schaerer, D., additional, Schreiber, C., additional, Stark, D., additional, Tasca, L. A. M., additional, Thomas, R., additional, Vanzella, E., additional, Wild, V., additional, Williams, C., additional, and Zucca, E., additional

Published
2021
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6. Extended Hα over compact far-infrared continuum in dusty submillimeter galaxies

Author

Chen, Chian-Chou, primary, Harrison, C. M., additional, Smail, I., additional, Swinbank, A. M., additional, Turner, O. J., additional, Wardlow, J. L., additional, Brandt, W. N., additional, Calistro Rivera, G., additional, Chapman, S. C., additional, Cooke, E. A., additional, Dannerbauer, H., additional, Dunlop, J. S., additional, Farrah, D., additional, Michałowski, M. J., additional, Schinnerer, E., additional, Simpson, J. M., additional, Thomson, A. P., additional, and van der Werf, P. P., additional

Published
2020
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7. The VIMOS Ultra-Deep Survey: evidence for AGN feedback in galaxies with CIII]-λ1908 Å emission 10.8 to 12.5 Gyr ago

Author

Le Fèvre, O., primary, Lemaux, B. C., additional, Nakajima, K., additional, Schaerer, D., additional, Talia, M., additional, Zamorani, G., additional, Cassata, P., additional, Garilli, B., additional, Maccagni, D., additional, Pentericci, L., additional, Tasca, L. A. M., additional, Zucca, E., additional, Amorin, R., additional, Bardelli, S., additional, Cimatti, A., additional, Giavalisco, M., additional, Guaita, L., additional, Hathi, N. P., additional, Marchi, F., additional, Vanzella, E., additional, Vergani, D., additional, and Dunlop, J., additional

Published
2019
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8. Extended Hα over compact far-infrared continuum in dusty submillimeter galaxies Insights into dust distributions and star-formation rates at z ~2.

Author

Chian-Chou Chen, Harrison, C. M., Smail, I., Swinbank, A. M., Turner, O. J., Wardlow, J. L., Brandt, W. N., Rivera, G. Calistro, Chapman, S. C., Cooke, E. A., Dannerbauer, H., Dunlop, J. S., Farrah, D., Michałowski, M. J., Schinnerer, E., Simpson, J. M., Thomson, A. P., and van der Werf, P. P.

Subjects
VERY large telescopes, STAR formation, SPECTRAL energy distribution, GALAXIES, DUST
Abstract

By using data from the Atacama Large Millimeter/submillimeter Array and near-infrared (NIR) integral field spectrographs, including both Spectrograph for INtegral Field Observations in the Near Infrared and K-band Multi Object Spectrograph on the Very Large Telescope, we investigate the two-dimensional distributions of H and rest-frame far-infrared (FIR) continuum in six submillimeter galaxies (SMGs) at z ~ 2. At a similar spatial resolution (~0: 005 FWHM; ~4.5 kpc at z = 2), we find that the half-light radius of Hα is significantly larger than that of the FIR continuum in half of the sample, and on average Hα is a median factor of 2:0 ± 0:4 larger. Having explored various ways to correct for the attenuation, we find that the attenuation-corrected Hα-based star-formation rates (SFRs) are systematically lower than the infrared (IR)-based SFRs by at least a median factor of 3 ± 1, which cannot be explained by the diαerence in half-light radius alone. In addition, we find that in 40% of cases the total V-band attenuation (AV) derived from energy balance modeling of the full ultraviolet (UV)-to-FIR spectral energy distributions (SEDs) is significantly higher than what is derived from SED modeling using only the UV-to-NIR part of the SEDs, and the discrepancy appears to increase with increasing total infrared luminosity. Finally, in considering all of our findings along with the studies in the literature, we postulate that the dust distributions in SMGs, and possibly also in less IR luminous z ~ 2 massive star-forming galaxies, can be decomposed into the following three main components: the diαuse dust heated by older stellar populations, the more obscured and extended young star-forming Hii regions, and the heavily obscured central regions that have a low filling factor but dominate the infrared luminosity in which the majority of attenuation cannot be probed via UV-to-NIR emissions. [ABSTRACT FROM AUTHOR]

Published
2020
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9. The VANDELS ESO public spectroscopic survey: Observations and first data release

Author

Pentericci, L., primary, McLure, R. J., additional, Garilli, B., additional, Cucciati, O., additional, Franzetti, P., additional, Iovino, A., additional, Amorin, R., additional, Bolzonella, M., additional, Bongiorno, A., additional, Carnall, A. C., additional, Castellano, M., additional, Cimatti, A., additional, Cirasuolo, M., additional, Cullen, F., additional, De Barros, S., additional, Dunlop, J. S., additional, Elbaz, D., additional, Finkelstein, S. L., additional, Fontana, A., additional, Fontanot, F., additional, Fumana, M., additional, Gargiulo, A., additional, Guaita, L., additional, Hartley, W. G., additional, Jarvis, M. J., additional, Juneau, S., additional, Karman, W., additional, Maccagni, D., additional, Marchi, F., additional, Marmol-Queralto, E., additional, Nandra, K., additional, Pompei, E., additional, Pozzetti, L., additional, Scodeggio, M., additional, Sommariva, V., additional, Talia, M., additional, Almaini, O., additional, Balestra, I., additional, Bardelli, S., additional, Bell, E. F., additional, Bourne, N., additional, Bowler, R. A. A., additional, Brusa, M., additional, Buitrago, F., additional, Caputi, K. I., additional, Cassata, P., additional, Charlot, S., additional, Citro, A., additional, Cresci, G., additional, Cristiani, S., additional, Curtis-Lake, E., additional, Dickinson, M., additional, Fazio, G. G., additional, Ferguson, H. C., additional, Fiore, F., additional, Franco, M., additional, Fynbo, J. P. U., additional, Galametz, A., additional, Georgakakis, A., additional, Giavalisco, M., additional, Grazian, A., additional, Hathi, N. P., additional, Jung, I., additional, Kim, S., additional, Koekemoer, A. M., additional, Khusanova, Y., additional, Le Fèvre, O., additional, Lotz, J. M., additional, Mannucci, F., additional, Maltby, D. T., additional, Matsuoka, K., additional, McLeod, D. J., additional, Mendez-Hernandez, H., additional, Mendez-Abreu, J., additional, Mignoli, M., additional, Moresco, M., additional, Mortlock, A., additional, Nonino, M., additional, Pannella, M., additional, Papovich, C., additional, Popesso, P., additional, Rosario, D. P., additional, Salvato, M., additional, Santini, P., additional, Schaerer, D., additional, Schreiber, C., additional, Stark, D. P., additional, Tasca, L. A. M., additional, Thomas, R., additional, Treu, T., additional, Vanzella, E., additional, Wild, V., additional, Williams, C. C., additional, Zamorani, G., additional, and Zucca, E., additional

Published
2018
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10. The ASTRODEEP Frontier Fields catalogues

Author

Di Criscienzo, M., primary, Merlin, E., additional, Castellano, M., additional, Santini, P., additional, Fontana, A., additional, Amorin, R., additional, Boutsia, K., additional, Derriere, S., additional, Dunlop, J. S., additional, Elbaz, D., additional, Grazian, A., additional, McLure, R. J., additional, Mármol-Queraltó, E., additional, Michalowski, M. J., additional, Mortlock, S., additional, Parsa, S., additional, and Pentericci, L., additional

Published
2017
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11. EGG: hatching a mock Universe from empirical prescriptions

Author

Schreiber, C., primary, Elbaz, D., additional, Pannella, M., additional, Merlin, E., additional, Castellano, M., additional, Fontana, A., additional, Bourne, N., additional, Boutsia, K., additional, Cullen, F., additional, Dunlop, J., additional, Ferguson, H. C., additional, Michałowski, M. J., additional, Okumura, K., additional, Santini, P., additional, Shu, X. W., additional, Wang, T., additional, and White, C., additional

Published
2017
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12. The VIMOS Ultra Deep Survey first data release: Spectra and spectroscopic redshifts of 698 objects up to zspec ~ 6 in CANDELS

Author

Tasca, L. A. M., primary, Le Fèvre, O., additional, Ribeiro, B., additional, Thomas, R., additional, Moreau, C., additional, Cassata, P., additional, Garilli, B., additional, Le Brun, V., additional, Lemaux, B. C., additional, Maccagni, D., additional, Pentericci, L., additional, Schaerer, D., additional, Vanzella, E., additional, Zamorani, G., additional, Zucca, E., additional, Amorin, R., additional, Bardelli, S., additional, Cassarà, L. P., additional, Castellano, M., additional, Cimatti, A., additional, Cucciati, O., additional, Durkalec, A., additional, Fontana, A., additional, Giavalisco, M., additional, Grazian, A., additional, Hathi, N. P., additional, Ilbert, O., additional, Paltani, S., additional, Pforr, J., additional, Scodeggio, M., additional, Sommariva, V., additional, Talia, M., additional, Tresse, L., additional, Vergani, D., additional, Capak, P., additional, Charlot, S., additional, Contini, T., additional, de la Torre, S., additional, Dunlop, J., additional, Fotopoulou, S., additional, Guaita, L., additional, Koekemoer, A., additional, López-Sanjuan, C., additional, Mellier, Y., additional, Salvato, M., additional, Scoville, N., additional, Taniguchi, Y., additional, and Wang, P. W., additional

Published
2017
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13. VIMOS Ultra-Deep Survey (VUDS): IGM transmission towards galaxies with 2.5 < z < 5.5 and the colour selection of high-redshift galaxies

Author

Thomas, R., primary, Le Fèvre, O., additional, Le Brun, V., additional, Cassata, P., additional, Garilli, B., additional, Lemaux, B. C., additional, Maccagni, D., additional, Pentericci, L., additional, Tasca, L. A. M., additional, Zamorani, G., additional, Zucca, E., additional, Amorin, R., additional, Bardelli, S., additional, Cassarà, L., additional, Castellano, M., additional, Cimatti, A., additional, Cucciati, O., additional, Durkalec, A., additional, Fontana, A., additional, Giavalisco, M., additional, Grazian, A., additional, Hathi, N. P., additional, Ilbert, O., additional, Paltani, S., additional, Pforr, J., additional, Ribeiro, B., additional, Schaerer, D., additional, Scodeggio, M., additional, Sommariva, V., additional, Talia, M., additional, Tresse, L., additional, Vanzella, E., additional, Vergani, D., additional, Capak, P., additional, Charlot, S., additional, Contini, T., additional, Cuby, J. G., additional, de la Torre, S., additional, Dunlop, J., additional, Fotopoulou, S., additional, Koekemoer, A., additional, López-Sanjuan, C., additional, Mellier, Y., additional, Salvato, M., additional, Scoville, N., additional, Taniguchi, Y., additional, and Wang, P. W., additional

Published
2017
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14. The evolving star formation rate: MBlack star relation and sSFR since z ≃ 5 from the VUDS spectroscopic survey

Author

Tasca, L. A. M., Le Fèvre, O., Hathi, N. P., Schaerer, D., Ilbert, O., Zamorani, G., Lemaux, B. C., Cassata, P., Garilli, B., Le Brun, V., Maccagni, D., Pentericci, L., Thomas, R., Vanzella, E., Zucca, E., Amorin, R., Bardelli, S., Cassarà, L. P., Castellano, M., Cimatti, A., Cucciati, O., Durkalec, A., Fontana, A., Giavalisco, M., Grazian, A., Paltani, S., Ribeiro, B., Scodeggio, M., Sommariva, V., Talia, M., Tresse, L., Vergani, D., Capak, P., Charlot, S., Contini, T., De La Torre, S., Dunlop, J., Fotopoulou, S., Koekemoer, A., López-Sanjuan, C., Mellier, Y., Pforr, J., Salvato, M., Scoville, N., Taniguchi, Y., and Wang, P. W.

Subjects
galaxies: high-redshift, Space and Planetary Science, galaxies: star formation, galaxies: formation, Astronomy and Astrophysics, galaxies: evolution
Published
2015

16. Size evolution of star-forming galaxies with 2 < 4.5 in the VIMOS Ultra-Deep Survey

Author

Ribeiro, B., primary, Le Fèvre, O., additional, Tasca, L. A. M., additional, Lemaux, B. C., additional, Cassata, P., additional, Garilli, B., additional, Maccagni, D., additional, Zamorani, G., additional, Zucca, E., additional, Amorín, R., additional, Bardelli, S., additional, Fontana, A., additional, Giavalisco, M., additional, Hathi, N. P., additional, Koekemoer, A., additional, Pforr, J., additional, Tresse, L., additional, and Dunlop, J., additional

Published
2016
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17. Effect of the star formation histories on theSFR-M∗relation atz≥ 2

Author

Cassarà, L. P., primary, Maccagni, D., additional, Garilli, B., additional, Scodeggio, M., additional, Thomas, R., additional, Le Fèvre, O., additional, Zamorani, G., additional, Schaerer, D., additional, Lemaux, B. C., additional, Cassata, P., additional, Le Brun, V., additional, Pentericci, L., additional, Tasca, L. A. M., additional, Vanzella, E., additional, Zucca, E., additional, Amorín, R., additional, Bardelli, S., additional, Castellano, M., additional, Cimatti, A., additional, Cucciati, O., additional, Durkalec, A., additional, Fontana, A., additional, Giavalisco, M., additional, Grazian, A., additional, Hathi, N. P., additional, Ilbert, O., additional, Paltani, S., additional, Ribeiro, B., additional, Sommariva, V., additional, Talia, M., additional, Tresse, L., additional, Vergani, D., additional, Capak, P., additional, Charlot, S., additional, Contini, T., additional, de la Torre, S., additional, Dunlop, J., additional, Fotopoulou, S., additional, Guaita, L., additional, Koekemoer, A., additional, López-Sanjuan, C., additional, Mellier, Y., additional, Pforr, J., additional, Salvato, M., additional, Scoville, N., additional, Taniguchi, Y., additional, and Wang, P. W., additional

Published
2016
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18. The ASTRODEEP Frontier Fields catalogues

Author

Castellano, M., primary, Amorín, R., additional, Merlin, E., additional, Fontana, A., additional, McLure, R. J., additional, Mármol-Queraltó, E., additional, Mortlock, A., additional, Parsa, S., additional, Dunlop, J. S., additional, Elbaz, D., additional, Balestra, I., additional, Boucaud, A., additional, Bourne, N., additional, Boutsia, K., additional, Brammer, G., additional, Bruce, V. A., additional, Buitrago, F., additional, Capak, P., additional, Cappelluti, N., additional, Ciesla, L., additional, Comastri, A., additional, Cullen, F., additional, Derriere, S., additional, Faber, S. M., additional, Giallongo, E., additional, Grazian, A., additional, Grillo, C., additional, Mercurio, A., additional, Michałowski, M. J., additional, Nonino, M., additional, Paris, D., additional, Pentericci, L., additional, Pilo, S., additional, Rosati, P., additional, Santini, P., additional, Schreiber, C., additional, Shu, X., additional, and Wang, T., additional

Published
2016
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19. The ASTRODEEP Frontier Fields catalogues

Author

Merlin, E., primary, Amorín, R., additional, Castellano, M., additional, Fontana, A., additional, Buitrago, F., additional, Dunlop, J. S., additional, Elbaz, D., additional, Boucaud, A., additional, Bourne, N., additional, Boutsia, K., additional, Brammer, G., additional, Bruce, V. A., additional, Capak, P., additional, Cappelluti, N., additional, Ciesla, L., additional, Comastri, A., additional, Cullen, F., additional, Derriere, S., additional, Faber, S. M., additional, Ferguson, H. C., additional, Giallongo, E., additional, Grazian, A., additional, Lotz, J., additional, Michałowski, M. J., additional, Paris, D., additional, Pentericci, L., additional, Pilo, S., additional, Santini, P., additional, Schreiber, C., additional, Shu, X., additional, and Wang, T., additional

Published
2016
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20. The VIMOS Ultra Deep Survey: Lyαemission and stellar populations of star-forming galaxies at 2 < z < 2.5

Author

Hathi, N. P., primary, Le Fèvre, O., additional, Ilbert, O., additional, Cassata, P., additional, Tasca, L. A. M., additional, Lemaux, B. C., additional, Garilli, B., additional, Le Brun, V., additional, Maccagni, D., additional, Pentericci, L., additional, Thomas, R., additional, Vanzella, E., additional, Zamorani, G., additional, Zucca, E., additional, Amorín, R., additional, Bardelli, S., additional, Cassarà, L. P., additional, Castellano, M., additional, Cimatti, A., additional, Cucciati, O., additional, Durkalec, A., additional, Fontana, A., additional, Giavalisco, M., additional, Grazian, A., additional, Guaita, L., additional, Koekemoer, A., additional, Paltani, S., additional, Pforr, J., additional, Ribeiro, B., additional, Schaerer, D., additional, Scodeggio, M., additional, Sommariva, V., additional, Talia, M., additional, Tresse, L., additional, Vergani, D., additional, Capak, P., additional, Charlot, S., additional, Contini, T., additional, Cuby, J. G., additional, de la Torre, S., additional, Dunlop, J., additional, Fotopoulou, S., additional, López-Sanjuan, C., additional, Mellier, Y., additional, Salvato, M., additional, Scoville, N., additional, Taniguchi, Y., additional, and Wang, P. W., additional

Published
2016
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21. The Lyman continuum escape fraction of galaxies atz= 3.3 in the VUDS-LBC/COSMOS field

Author

Grazian, A., primary, Giallongo, E., additional, Gerbasi, R., additional, Fiore, F., additional, Fontana, A., additional, Le Fèvre, O., additional, Pentericci, L., additional, Vanzella, E., additional, Zamorani, G., additional, Cassata, P., additional, Garilli, B., additional, Le Brun, V., additional, Maccagni, D., additional, Tasca, L. A. M., additional, Thomas, R., additional, Zucca, E., additional, Amorín, R., additional, Bardelli, S., additional, Cassarà, L. P., additional, Castellano, M., additional, Cimatti, A., additional, Cucciati, O., additional, Durkalec, A., additional, Giavalisco, M., additional, Hathi, N. P., additional, Ilbert, O., additional, Lemaux, B. C., additional, Paltani, S., additional, Ribeiro, B., additional, Schaerer, D., additional, Scodeggio, M., additional, Sommariva, V., additional, Talia, M., additional, Tresse, L., additional, Vergani, D., additional, Bonchi, A., additional, Boutsia, K., additional, Capak, P., additional, Charlot, S., additional, Contini, T., additional, de la Torre, S., additional, Dunlop, J., additional, Fotopoulou, S., additional, Guaita, L., additional, Koekemoer, A., additional, López-Sanjuan, C., additional, Mellier, Y., additional, Merlin, E., additional, Paris, D., additional, Pforr, J., additional, Pilo, S., additional, Santini, P., additional, Scoville, N., additional, Taniguchi, Y., additional, and Wang, P. W., additional

Published
2015
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22. Evolution of clustering length, large-scale bias, and host halo mass at 2 < 5 in the VIMOS Ultra Deep Survey (VUDS)

Author

Durkalec, A., primary, Le Fèvre, O., additional, Pollo, A., additional, de la Torre, S., additional, Cassata, P., additional, Garilli, B., additional, Le Brun, V., additional, Lemaux, B. C., additional, Maccagni, D., additional, Pentericci, L., additional, Tasca, L. A. M., additional, Thomas, R., additional, Vanzella, E., additional, Zamorani, G., additional, Zucca, E., additional, Amorín, R., additional, Bardelli, S., additional, Cassarà, L. P., additional, Castellano, M., additional, Cimatti, A., additional, Cucciati, O., additional, Fontana, A., additional, Giavalisco, M., additional, Grazian, A., additional, Hathi, N. P., additional, Ilbert, O., additional, Paltani, S., additional, Ribeiro, B., additional, Schaerer, D., additional, Scodeggio, M., additional, Sommariva, V., additional, Talia, M., additional, Tresse, L., additional, Vergani, D., additional, Capak, P., additional, Charlot, S., additional, Contini, T., additional, Cuby, J. G., additional, Dunlop, J., additional, Fotopoulou, S., additional, Koekemoer, A., additional, López-Sanjuan, C., additional, Mellier, Y., additional, Pforr, J., additional, Salvato, M., additional, Scoville, N., additional, Taniguchi, Y., additional, and Wang, P. W., additional

Published
2015
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23. T-PHOT: A new code for PSF-matched, prior-based, multiwavelength extragalactic deconfusion photometry

Author

Merlin, E., primary, Fontana, A., additional, Ferguson, H. C., additional, Dunlop, J. S., additional, Elbaz, D., additional, Bourne, N., additional, Bruce, V. A., additional, Buitrago, F., additional, Castellano, M., additional, Schreiber, C., additional, Grazian, A., additional, McLure, R. J., additional, Okumura, K., additional, Shu, X., additional, Wang, T., additional, Amorín, R., additional, Boutsia, K., additional, Cappelluti, N., additional, Comastri, A., additional, Derriere, S., additional, Faber, S. M., additional, and Santini, P., additional

Published
2015
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24. The evolving star formation rate:M⋆relation and sSFR sincez≃ 5 from the VUDS spectroscopic survey

Author

Tasca, L. A. M., primary, Le Fèvre, O., additional, Hathi, N. P., additional, Schaerer, D., additional, Ilbert, O., additional, Zamorani, G., additional, Lemaux, B. C., additional, Cassata, P., additional, Garilli, B., additional, Le Brun, V., additional, Maccagni, D., additional, Pentericci, L., additional, Thomas, R., additional, Vanzella, E., additional, Zucca, E., additional, Amorin, R., additional, Bardelli, S., additional, Cassarà, L. P., additional, Castellano, M., additional, Cimatti, A., additional, Cucciati, O., additional, Durkalec, A., additional, Fontana, A., additional, Giavalisco, M., additional, Grazian, A., additional, Paltani, S., additional, Ribeiro, B., additional, Scodeggio, M., additional, Sommariva, V., additional, Talia, M., additional, Tresse, L., additional, Vergani, D., additional, Capak, P., additional, Charlot, S., additional, Contini, T., additional, de la Torre, S., additional, Dunlop, J., additional, Fotopoulou, S., additional, Koekemoer, A., additional, López-Sanjuan, C., additional, Mellier, Y., additional, Pforr, J., additional, Salvato, M., additional, Scoville, N., additional, Taniguchi, Y., additional, and Wang, P. W., additional

Published
2015
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25. Stellar mass to halo mass relation from galaxy clustering in VUDS: a high star formation efficiency atz≃ 3

Author

Durkalec, A., primary, Le Fèvre, O., additional, de la Torre, S., additional, Pollo, A., additional, Cassata, P., additional, Garilli, B., additional, Le Brun, V., additional, Lemaux, B. C., additional, Maccagni, D., additional, Pentericci, L., additional, Tasca, L. A. M., additional, Thomas, R., additional, Vanzella, E., additional, Zamorani, G., additional, Zucca, E., additional, Amorín, R., additional, Bardelli, S., additional, Cassarà, L. P., additional, Castellano, M., additional, Cimatti, A., additional, Cucciati, O., additional, Fontana, A., additional, Giavalisco, M., additional, Grazian, A., additional, Hathi, N. P., additional, Ilbert, O., additional, Paltani, S., additional, Ribeiro, B., additional, Schaerer, D., additional, Scodeggio, M., additional, Sommariva, V., additional, Talia, M., additional, Tresse, L., additional, Vergani, D., additional, Capak, P., additional, Charlot, S., additional, Contini, T., additional, Cuby, J. G., additional, Dunlop, J., additional, Fotopoulou, S., additional, Koekemoer, A., additional, López-Sanjuan, C., additional, Mellier, Y., additional, Pforr, J., additional, Salvato, M., additional, Scoville, N., additional, Taniguchi, Y., additional, and Wang, P. W., additional

Published
2015
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26. The galaxy stellar mass function at 3.5 ≤z≤ 7.5 in the CANDELS/UDS, GOODS-South, and HUDF fields

Author

Grazian, A., primary, Fontana, A., additional, Santini, P., additional, Dunlop, J. S., additional, Ferguson, H. C., additional, Castellano, M., additional, Amorin, R., additional, Ashby, M. L. N., additional, Barro, G., additional, Behroozi, P., additional, Boutsia, K., additional, Caputi, K. I., additional, Chary, R. R., additional, Dekel, A., additional, Dickinson, M. E., additional, Faber, S. M., additional, Fazio, G. G., additional, Finkelstein, S. L., additional, Galametz, A., additional, Giallongo, E., additional, Giavalisco, M., additional, Grogin, N. A., additional, Guo, Y., additional, Kocevski, D., additional, Koekemoer, A. M., additional, Koo, D. C., additional, Lee, K.-S., additional, Lu, Y., additional, Merlin, E., additional, Mobasher, B., additional, Nonino, M., additional, Papovich, C., additional, Paris, D., additional, Pentericci, L., additional, Reddy, N., additional, Renzini, A., additional, Salmon, B., additional, Salvato, M., additional, Sommariva, V., additional, Song, M., additional, and Vanzella, E., additional

Published
2015
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27. Herschel unveils a puzzling uniformity of distant dusty galaxies [Letter]

Author

Elbaz, D., Hwang, H. S., Magnelli, B., Daddi, E., Aussel, H., Altieri, B., Amblard, A., Andreani, P., Arumugam, V., Auld, Robbie Richard, Babbedge, T., Berta, S., Blain, A., Bock, J., Bongiovanni, A., Boselli, A., Buat, V., Burgarella, D., Castro-Rodriguez, N., Cava, A., Cepa, J., Chanial, P., Chary, R.-R., Cimatti, A., Clements, D. L., Conley, A., Conversi, L., Cooray, A., Dickinson, M., Dominguez, H., Dowell, C. D., Dunlop, J. S., Dwek, E., Eales, Stephen Anthony, Farrah, D., Förster Schreiber, N., Fox, M., Franceschini, A., Gear, Walter Kieran, Genzel, R., Glenn, J., Griffin, Matthew Joseph, Gruppioni, C., Halpern, M., Hatziminaoglou, E., Ibar, E., Isaak, Kate Gudrun, Ivison, R. J., Lagache, G., Le Borgne, D., Le Floc'h, E., Levenson, L., Lu, N., Lutz, D., Madden, S., Maffei, B., Magdis, G., Mainetti, G., Maiolino, R., Marchetti, L., Mortier, A. M. J., Nguyen, H. T., Nordon, R., O'Halloran, B., Okumura, K., Oliver, S. J., Omont, A., Page, M. J., Panuzzo, P., Papageorgiou, Andreas, Pearson, C. P., Perez Fournon, I., Pérez García, A. M., Poglitsch, A., Pohlen, Michael, Popesso, P., Pozzi, F., Rawlings, J. I., Rigopoulou, D., Riguccini, L., Rizzo, D., Rodighiero, G., Roseboom, I. G., Rowan-Robinson, M., Saintonge, A., Sanchez Portal, M., Santini, P., Sauvage, M., Schulz, B., Scott, D., Seymour, N., Shao, L., Shupe, D. L., Smith, A. J., Stevens, J. A., Sturm, E., Symeonidis, M., Tacconi, L., Trichas, M., Tugwell, K. E., Vaccari, M., Valtchanov, I., Vieira, J., Vigroux, L., Wang, L., Ward, R., Wright, G., Xu, C. K., and Zemcov, M.

Subjects
Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Solar and Stellar Astrophysics, Astrophysics::Earth and Planetary Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics::Galaxy Astrophysics, QB
Abstract

The Herschel Space Observatory enables us to accurately measure the bolometric output of starburst galaxies and active galactic nuclei (AGN) by directly sampling the peak of their far-infrared (IR) emission. Here we examine whether the spectral energy distribution (SED) and dust temperature of galaxies have strongly evolved over the last 80% of the age of the Universe. We discuss possible consequences for the determination of star-formation rates (SFR) and any evidence for a major change in their star-formation properties. We use Herschel deep extragalactic surveys from 100 to 500 μm to compute total IR luminosities in galaxies down to the faintest levels, using PACS and SPIRE in the GOODS-North field (PEP and HerMES key programs). An extension to fainter luminosities is done by stacking images on 24 μm prior positions. We show that measurements in the SPIRE bands can be used below the statistical confusion limit if information at higher spatial resolution is used, e.g. at 24 μm, to identify “isolated” galaxies whose flux is not boosted by bright neighbors. Below z ~ 1.5, mid-IR extrapolations are correct for star-forming galaxies with a dispersion of only 40% (0.15 dex), therefore similar to z ~ 0 galaxies, over three decades in luminosity below the regime of ultra-luminous IR galaxies (ULIRGs, LIR ≥ 1012 ). This narrow distribution is puzzling when considering the range of physical processes that could have affected the SED of these galaxies. Extrapolations from only one of the 160 μm, 250 μm or 350 μm bands alone tend to overestimate the total IR luminosity. This may be explained by the lack of far-IR constraints around and above ~150 μm (rest-frame) before Herschel on those templates. We also note that the dust temperature of luminous IR galaxies (LIRGs, LIR ≥ 1011 ) around z ~ 1 is mildly colder by 10–15% than their local analogs and up to 20% for ULIRGs at z ~ 1.6 (using a single modified blackbody-fit to the peak far-IR emission with an emissivity index of β = 1.5). Above z = 1.5, distant galaxies are found to exhibit a substantially larger mid- over far-IR ratio, which could either result from stronger broad emission lines or warm dust continuum heated by a hidden AGN. Two thirds of the AGNs identified in the field with a measured redshift exhibit the same behavior as purely star-forming galaxies. Hence a large fraction of AGNs harbor coeval star formation at very high SFR and in conditions similar to purely star-forming galaxies.

Published
2010

28. A mass threshold in the number density of passive galaxies atz~ 2

Author

Sommariva, V., primary, Fontana, A., additional, Lamastra, A., additional, Santini, P., additional, Dunlop, J. S., additional, Nonino, M., additional, Castellano, M., additional, Ferguson, H., additional, McLure, R. J., additional, Galametz, A., additional, Giavalisco, M., additional, Grazian, A., additional, Lu, Y., additional, Menci, N., additional, Merson, A., additional, Paris, D., additional, Pentericci, L., additional, Somerville, R., additional, Targett, T., additional, and Koekemoer, A. M., additional

Published
2014
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29. The Hawk-I UDS and GOODS Survey (HUGS): Survey design and deepK-band number counts

Author

Fontana, A., primary, Dunlop, J. S., additional, Paris, D., additional, Targett, T. A., additional, Boutsia, K., additional, Castellano, M., additional, Galametz, A., additional, Grazian, A., additional, McLure, R., additional, Merlin, E., additional, Pentericci, L., additional, Wuyts, S., additional, Almaini, O., additional, Caputi, K., additional, Chary, R.-R., additional, Cirasuolo, M., additional, Conselice, C. J., additional, Cooray, A., additional, Daddi, E., additional, Dickinson, M., additional, Faber, S. M., additional, Fazio, G., additional, Ferguson, H. C., additional, Giallongo, E., additional, Giavalisco, M., additional, Grogin, N. A., additional, Hathi, N., additional, Koekemoer, A. M., additional, Koo, D. C., additional, Lucas, R. A., additional, Nonino, M., additional, Rix, H. W., additional, Renzini, A., additional, Rosario, D., additional, Santini, P., additional, Scarlata, C., additional, Sommariva, V., additional, Stark, D. P., additional, van der Wel, A., additional, Vanzella, E., additional, Wild, V., additional, Yan, H., additional, and Zibetti, S., additional

Published
2014
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30. Constraints on the star-formation rate ofz~ 3 LBGs with measured metallicity in the CANDELS GOODS-South field

Author

Castellano, M., primary, Sommariva, V., additional, Fontana, A., additional, Pentericci, L., additional, Santini, P., additional, Grazian, A., additional, Amorin, R., additional, Donley, J. L., additional, Dunlop, J. S., additional, Ferguson, H. C., additional, Fiore, F., additional, Galametz, A., additional, Giallongo, E., additional, Guo, Y., additional, Huang, K.-H., additional, Koekemoer, A., additional, Maiolino, R., additional, McLure, R. J., additional, Paris, D., additional, Schaerer, D., additional, Troncoso, P., additional, and Vanzella, E., additional

Published
2014
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31. Herschel PEP/HerMES: the redshift evolution (0 <= z <= 4) of dust attenuation and of the total (UV plus IR) star formation rate density

Author

Burgarella, D., Gruppioni, C., Cucciati, O., Heinis, S., Berta, S., Bethermin, M., Bock, J., Cooray, A., Dunlop, J. S., Farrah, D., Franceschini, A., Le Floc'h, E., Lutz, D., Magnelli, B., Nordon, R., Oliver, S. J., Page, M. J., Popesso, P., Pozzi, F., Riguccini, L., Vaccari, M., Viero, M., Burgarella, D., Gruppioni, C., Cucciati, O., Heinis, S., Berta, S., Bethermin, M., Bock, J., Cooray, A., Dunlop, J. S., Farrah, D., Franceschini, A., Le Floc'h, E., Lutz, D., Magnelli, B., Nordon, R., Oliver, S. J., Page, M. J., Popesso, P., Pozzi, F., Riguccini, L., Vaccari, M., and Viero, M.

Abstract

Using new homogeneous luminosity functions (LFs) in the far-ultraviolet (FUV) from VVDS and in the far-infrared (FIR) from Herschel/PEP and Herschel/HerMES, we studied the evolution of the dust attenuation with redshift. With this information, we were able to estimate the redshift evolution of the total (FUV + FIR) star formation rate density (SFRDTOT). By integrating SFRDTOT, we followed the mass building and analyzed the redshift evolution of the stellar mass density (SMD). This article aims at providing a complete view of star formation from the local Universe to z similar to 4 and, using assumptions on earlier star formation history, compares this evolution with previously published data in an attempt to draw a homogeneous picture of the global evolution of star formation in galaxies. Our main conclusions are that: 1) the dust attenuation A(FUV) is found to increase from z = 0 to z similar to 1.2 and then starts to decrease until our last data point at z = 3 : 6; 2) the estimated SFRD confirms published results to z similar to 2. At z > 2, we observe either a plateau or a small increase up to z similar to 3 and then a likely decrease up to z = 3.6; 3) the peak of AFUV is delayed with respect to the plateau of SFRDTOT and a probable origin might be found in the evolution of the bright ends of the FUV and FIR LFs; 4) using assumptions (exponential rise and linear rise with time) for the evolution of the star formation density from z = 3 : 6 to z(form) = 10, we integrated SFRDTOT and obtained a good agreement with the published SMDs.

Published
2013
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32. Herschel PEP/HerMES: the redshift evolution (0 <= z <= 4) of dust attenuation and of the total (UV plus IR) star formation rate density

Author

Physics, Burgarella, D., Gruppioni, C., Cucciati, O., Heinis, S., Berta, S., Bethermin, M., Bock, J., Cooray, A., Dunlop, J. S., Farrah, D., Franceschini, A., Le Floc'h, E., Lutz, D., Magnelli, B., Nordon, R., Oliver, S. J., Page, M. J., Popesso, P., Pozzi, F., Riguccini, L., Vaccari, M., Viero, M., Physics, Burgarella, D., Gruppioni, C., Cucciati, O., Heinis, S., Berta, S., Bethermin, M., Bock, J., Cooray, A., Dunlop, J. S., Farrah, D., Franceschini, A., Le Floc'h, E., Lutz, D., Magnelli, B., Nordon, R., Oliver, S. J., Page, M. J., Popesso, P., Pozzi, F., Riguccini, L., Vaccari, M., and Viero, M.

Abstract

Using new homogeneous luminosity functions (LFs) in the far-ultraviolet (FUV) from VVDS and in the far-infrared (FIR) from Herschel/PEP and Herschel/HerMES, we studied the evolution of the dust attenuation with redshift. With this information, we were able to estimate the redshift evolution of the total (FUV + FIR) star formation rate density (SFRDTOT). By integrating SFRDTOT, we followed the mass building and analyzed the redshift evolution of the stellar mass density (SMD). This article aims at providing a complete view of star formation from the local Universe to z similar to 4 and, using assumptions on earlier star formation history, compares this evolution with previously published data in an attempt to draw a homogeneous picture of the global evolution of star formation in galaxies. Our main conclusions are that: 1) the dust attenuation A(FUV) is found to increase from z = 0 to z similar to 1.2 and then starts to decrease until our last data point at z = 3 : 6; 2) the estimated SFRD confirms published results to z similar to 2. At z > 2, we observe either a plateau or a small increase up to z similar to 3 and then a likely decrease up to z = 3.6; 3) the peak of AFUV is delayed with respect to the plateau of SFRDTOT and a probable origin might be found in the evolution of the bright ends of the FUV and FIR LFs; 4) using assumptions (exponential rise and linear rise with time) for the evolution of the star formation density from z = 3 : 6 to z(form) = 10, we integrated SFRDTOT and obtained a good agreement with the published SMDs.

Published
2013

33. Mass assembly in quiescent and star-forming galaxies sincez≃ 4 from UltraVISTA

Author

Ilbert, O., primary, McCracken, H. J., additional, Le Fèvre, O., additional, Capak, P., additional, Dunlop, J., additional, Karim, A., additional, Renzini, M. A., additional, Caputi, K., additional, Boissier, S., additional, Arnouts, S., additional, Aussel, H., additional, Comparat, J., additional, Guo, Q., additional, Hudelot, P., additional, Kartaltepe, J., additional, Kneib, J. P., additional, Krogager, J. K., additional, Le Floc’h, E., additional, Lilly, S., additional, Mellier, Y., additional, Milvang-Jensen, B., additional, Moutard, T., additional, Onodera, M., additional, Richard, J., additional, Salvato, M., additional, Sanders, D. B., additional, Scoville, N., additional, Silverman, J. D., additional, Taniguchi, Y., additional, Tasca, L., additional, Thomas, R., additional, Toft, S., additional, Tresse, L., additional, Vergani, D., additional, Wolk, M., additional, and Zirm, A., additional

Published
2013
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34. HerschelPEP/HerMES: the redshift evolution (0 ≤z≤ 4) of dust attenuation and of the total (UV+IR) star formation rate density

Author

Burgarella, D., primary, Buat, V., additional, Gruppioni, C., additional, Cucciati, O., additional, Heinis, S., additional, Berta, S., additional, Béthermin, M., additional, Bock, J., additional, Cooray, A., additional, Dunlop, J. S., additional, Farrah, D., additional, Franceschini, A., additional, Le Floc’h, E., additional, Lutz, D., additional, Magnelli, B., additional, Nordon, R., additional, Oliver, S. J., additional, Page, M. J., additional, Popesso, P., additional, Pozzi, F., additional, Riguccini, L., additional, Vaccari, M., additional, and Viero, M., additional

Published
2013
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35. The size-luminosity relation atz = 7 in CANDELS and its implication on reionization

Author

Grazian, A., primary, Castellano, M., additional, Fontana, A., additional, Pentericci, L., additional, Dunlop, J. S., additional, McLure, R. J., additional, Koekemoer, A. M., additional, Dickinson, M. E., additional, Faber, S. M., additional, Ferguson, H. C., additional, Galametz, A., additional, Giavalisco, M., additional, Grogin, N. A., additional, Hathi, N. P., additional, Kocevski, D. D., additional, Lai, K., additional, Newman, J. A., additional, and Vanzella, E., additional

Published
2012
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36. UltraVISTA: a new ultra-deep near-infrared survey in COSMOS

Author

McCracken, H. J., primary, Milvang-Jensen, B., additional, Dunlop, J., additional, Franx, M., additional, Fynbo, J. P. U., additional, Le Fèvre, O., additional, Holt, J., additional, Caputi, K. I., additional, Goranova, Y., additional, Buitrago, F., additional, Emerson, J. P., additional, Freudling, W., additional, Hudelot, P., additional, López-Sanjuan, C., additional, Magnard, F., additional, Mellier, Y., additional, Møller, P., additional, Nilsson, K. K., additional, Sutherland, W., additional, Tasca, L., additional, and Zabl, J., additional

Published
2012
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38. AHerschelview of the far-infrared properties of submillimetre galaxies

Author

Magnelli, B., primary, Lutz, D., additional, Santini, P., additional, Saintonge, A., additional, Berta, S., additional, Albrecht, M., additional, Altieri, B., additional, Andreani, P., additional, Aussel, H., additional, Bertoldi, F., additional, Béthermin, M., additional, Bongiovanni, A., additional, Capak, P., additional, Chapman, S., additional, Cepa, J., additional, Cimatti, A., additional, Cooray, A., additional, Daddi, E., additional, Danielson, A. L. R., additional, Dannerbauer, H., additional, Dunlop, J. S., additional, Elbaz, D., additional, Farrah, D., additional, Förster Schreiber, N. M., additional, Genzel, R., additional, Hwang, H. S., additional, Ibar, E., additional, Ivison, R. J., additional, Le Floc’h, E., additional, Magdis, G., additional, Maiolino, R., additional, Nordon, R., additional, Oliver, S. J., additional, Pérez García, A., additional, Poglitsch, A., additional, Popesso, P., additional, Pozzi, F., additional, Riguccini, L., additional, Rodighiero, G., additional, Rosario, D., additional, Roseboom, I., additional, Salvato, M., additional, Sanchez-Portal, M., additional, Scott, D., additional, Smail, I., additional, Sturm, E., additional, Swinbank, A. M., additional, Tacconi, L. J., additional, Valtchanov, I., additional, Wang, L., additional, and Wuyts, S., additional

Published
2012
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40. Herschel-ATLAS: Dust temperature and redshift distribution of SPIRE and PACS detected sources using submillimetre colours

Author

Amblard, A., primary, Cooray, A., additional, Serra, P., additional, Temi, P., additional, Barton, E., additional, Negrello, M., additional, Auld, R., additional, Baes, M., additional, Baldry, I. K., additional, Bamford, S., additional, Blain, A., additional, Bock, J., additional, Bonfield, D., additional, Burgarella, D., additional, Buttiglione, S., additional, Cameron, E., additional, Cava, A., additional, Clements, D., additional, Croom, S., additional, Dariush, A., additional, de Zotti, G., additional, Driver, S., additional, Dunlop, J., additional, Dunne, L., additional, Dye, S., additional, Eales, S., additional, Frayer, D., additional, Fritz, J., additional, Gardner, Jonathan P., additional, Gonzalez-Nuevo, J., additional, Herranz, D., additional, Hill, D., additional, Hopkins, A., additional, Hughes, D. H., additional, Ibar, E., additional, Ivison, R. J., additional, Jarvis, M., additional, Jones, D. H., additional, Kelvin, L., additional, Lagache, G., additional, Leeuw, L., additional, Liske, J., additional, Lopez-Caniego, M., additional, Loveday, J., additional, Maddox, S., additional, Michałowski, M., additional, Norberg, P., additional, Parkinson, H., additional, Peacock, J. A., additional, Pearson, C., additional, Pascale, E., additional, Pohlen, M., additional, Popescu, C., additional, Prescott, M., additional, Robotham, A., additional, Rigby, E., additional, Rodighiero, G., additional, Samui, S., additional, Sansom, A., additional, Scott, D., additional, Serjeant, S., additional, Sharp, R., additional, Sibthorpe, B., additional, Smith, D. J. B., additional, Thompson, M. A., additional, Tuffs, R., additional, Valtchanov, I., additional, Van Kampen, E., additional, Van der Werf, P., additional, Verma, A., additional, Vieira, J., additional, and Vlahakis, C., additional

Published
2010
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41. Herschelunveils a puzzling uniformity of distant dusty galaxies

Author

Elbaz, D., primary, Hwang, H. S., additional, Magnelli, B., additional, Daddi, E., additional, Aussel, H., additional, Altieri, B., additional, Amblard, A., additional, Andreani, P., additional, Arumugam, V., additional, Auld, R., additional, Babbedge, T., additional, Berta, S., additional, Blain, A., additional, Bock, J., additional, Bongiovanni, A., additional, Boselli, A., additional, Buat, V., additional, Burgarella, D., additional, Castro-Rodriguez, N., additional, Cava, A., additional, Cepa, J., additional, Chanial, P., additional, Chary, R.-R., additional, Cimatti, A., additional, Clements, D. L., additional, Conley, A., additional, Conversi, L., additional, Cooray, A., additional, Dickinson, M., additional, Dominguez, H., additional, Dowell, C. D., additional, Dunlop, J. S., additional, Dwek, E., additional, Eales, S., additional, Farrah, D., additional, Förster Schreiber, N., additional, Fox, M., additional, Franceschini, A., additional, Gear, W., additional, Genzel, R., additional, Glenn, J., additional, Griffin, M., additional, Gruppioni, C., additional, Halpern, M., additional, Hatziminaoglou, E., additional, Ibar, E., additional, Isaak, K., additional, Ivison, R. J., additional, Lagache, G., additional, Le Borgne, D., additional, Le Floc'h, E., additional, Levenson, L., additional, Lu, N., additional, Lutz, D., additional, Madden, S., additional, Maffei, B., additional, Magdis, G., additional, Mainetti, G., additional, Maiolino, R., additional, Marchetti, L., additional, Mortier, A. M. J., additional, Nguyen, H. T., additional, Nordon, R., additional, O'Halloran, B., additional, Okumura, K., additional, Oliver, S. J., additional, Omont, A., additional, Page, M. J., additional, Panuzzo, P., additional, Papageorgiou, A., additional, Pearson, C. P., additional, Perez Fournon, I., additional, Pérez García, A. M., additional, Poglitsch, A., additional, Pohlen, M., additional, Popesso, P., additional, Pozzi, F., additional, Rawlings, J. I., additional, Rigopoulou, D., additional, Riguccini, L., additional, Rizzo, D., additional, Rodighiero, G., additional, Roseboom, I. G., additional, Rowan-Robinson, M., additional, Saintonge, A., additional, Sanchez Portal, M., additional, Santini, P., additional, Sauvage, M., additional, Schulz, B., additional, Scott, D., additional, Seymour, N., additional, Shao, L., additional, Shupe, D. L., additional, Smith, A. J., additional, Stevens, J. A., additional, Sturm, E., additional, Symeonidis, M., additional, Tacconi, L., additional, Trichas, M., additional, Tugwell, K. E., additional, Vaccari, M., additional, Valtchanov, I., additional, Vieira, J., additional, Vigroux, L., additional, Wang, L., additional, Ward, R., additional, Wright, G., additional, Xu, C. K., additional, and Zemcov, M., additional

Published
2010
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42. Herschel-ATLAS: Evolution of the 250 µm luminosity function out to z=0.5

Author

Dye, S., primary, Dunne, L., additional, Eales, S., additional, Smith, D. J. B., additional, Amblard, A., additional, Auld, R., additional, Baes, M., additional, Baldry, I. K., additional, Bamford, S., additional, Blain, A. W., additional, Bonfield, D. G., additional, Bremer, M., additional, Burgarella, D., additional, Buttiglione, S., additional, Cameron, E., additional, Cava, A., additional, Clements, D. L., additional, Cooray, A., additional, Croom, S., additional, Dariush, A., additional, de Zotti, G., additional, Driver, S., additional, Dunlop, J. S., additional, Frayer, D., additional, Fritz, J., additional, Gardner, Jonathan P., additional, Gomez, H. L., additional, Gonzalez-Nuevo, J., additional, Herranz, D., additional, Hill, D., additional, Hopkins, A., additional, Ibar, E., additional, Ivison, R. J., additional, Jarvis, M. J., additional, Jones, D. H., additional, Kelvin, L., additional, Lagache, G., additional, Leeuw, L., additional, Liske, J., additional, Lopez-Caniego, M., additional, Loveday, J., additional, Maddox, S., additional, Michałowski, M. J., additional, Negrello, M., additional, Norberg, P., additional, Page, M. J., additional, Parkinson, H., additional, Pascale, E., additional, Peacock, J. A., additional, Pohlen, M., additional, Popescu, C., additional, Prescott, M., additional, Rigopoulou, D., additional, Robotham, A., additional, Rigby, E., additional, Rodighiero, G., additional, Samui, S., additional, Scott, D., additional, Serjeant, S., additional, Sharp, R., additional, Sibthorpe, B., additional, Temi, P., additional, Thompson, M. A., additional, Tuffs, R., additional, Valtchanov, I., additional, van der Werf, P. P., additional, van Kampen, E., additional, and Verma, A., additional

Published
2010
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43. HerschelATLAS: The cosmic star formation history of quasar host galaxies

Author

Serjeant, S., primary, Bertoldi, F., additional, Blain, A. W., additional, Clements, D. L., additional, Cooray, A., additional, Danese, L., additional, Dunlop, J., additional, Dunne, L., additional, Eales, S., additional, Falder, J., additional, Hatziminaoglou, E., additional, Hughes, D. H., additional, Ibar, E., additional, Jarvis, M. J., additional, Lawrence, A., additional, Lee, M. G., additional, Michałowski, M., additional, Negrello, M., additional, Omont, A., additional, Page, M., additional, Pearson, C., additional, van der Werf, P. P., additional, White, G., additional, Amblard, A., additional, Auld, R., additional, Baes, M., additional, Bonfield, D. G., additional, Burgarella, D., additional, Buttiglione, S., additional, Cava, A., additional, Dariush, A., additional, de Zotti, G., additional, Dye, S., additional, Frayer, D., additional, Fritz, J., additional, Gonzalez-Nuevo, J., additional, Herranz, D., additional, Ivison, R. J., additional, Lagache, G., additional, Leeuw, L., additional, Lopez-Caniego, M., additional, Maddox, S., additional, Pascale, E., additional, Pohlen, M., additional, Rigby, E., additional, Rodighiero, G., additional, Samui, S., additional, Sibthorpe, B., additional, Smith, D. J. B., additional, Temi, P., additional, Thompson, M., additional, Valtchanov, I., additional, and Verma, A., additional

Published
2010
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44. The AGN fraction of submm-selected galaxies and contributions to the submm/mm-wave extragalactic background light

Author

Serjeant, S., primary, Negrello, M., additional, Pearson, C., additional, Mortier, A., additional, Austermann, J., additional, Aretxaga, I., additional, Clements, D., additional, Chapman, S., additional, Dye, S., additional, Dunlop, J., additional, Dunne, L., additional, Farrah, D., additional, Hughes, D., additional, Lee, H.-M., additional, Matsuhara, H., additional, Ibar, E., additional, Im, M., additional, Jeong, W.-S., additional, Kim, S., additional, Oyabu, S., additional, Takagi, T., additional, Wada, T., additional, Wilson, G., additional, Vaccari, M., additional, and Yun, M., additional

Published
2010
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46. The extended counterpart of submm source Lockman 850.1

Author

Lutz, D., primary, Dunlop, J. S., additional, Almaini, O., additional, Andreani, P., additional, Blain, A., additional, Efstathiou, A., additional, Fox, M., additional, Genzel, R., additional, Hasinger, G., additional, Hughes, D., additional, Ivison, R. J., additional, Lawrence, A., additional, Mann, R. G., additional, Oliver, S., additional, Peacock, J. A., additional, Rigopoulou, D., additional, Rowan-Robinson, M., additional, Scott, S., additional, Serjeant, S., additional, and Tacconi, L., additional

Published
2001
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47. A mass threshold in the number density of passive galaxies at z ~ 2.

Author

Sommariva, V., Fontana, A., Lamastra, A., Santini, P., Castellano, M., Galametz, A., Grazian, A., Menci, N., Paris, D., Pentericci, L., Dunlop, J. S., McLure, R. J., Targett, T., Nonino, M., Ferguson, H., Somerville, R., Giavalisco, M., Lu, Y., Merson, A., and Koekemoer, A. M.

Subjects
STELLAR mass, MILKY Way, SPECTRAL imaging, GALACTIC redshift, EVOLUTIONARY theories
Abstract

The process that quenched star formation in galaxies at intermediate and high redshifts is still the subject of considerable debate. One way to investigate this puzzling issue is to study the number density of quiescent galaxies at z ≃ 2 and its dependence on mass. Here we present the results of a new study based on very deep Ks-band imaging (with the HAWK-I instrument on the VLT) of two HST CANDELS fields (the UKIDSS Ultra-deep survey (UDS) field and GOODS-South). The new HAWK-I data (taken as part of the HUGS VLT Large Program) reach detection limits of Ks > 26 (AB mag). We have combined this imaging with the other groundbased and HST data in the CANDELS fields to select a sample of passively-evolving galaxies in the redshift range 1.4 < z < 2.5 (via the pBzK color-based selection criterion). Thanks to the depth and wide area coverage of our imaging, we have been able to extend the selection of quiescent galaxies to a magnitude fainter than previous analyses. Through extensive simulations we demonstrate, for the first time, that the observed turnover in the number of quiescent galaxies at K ⩾ 22 is not due to incompleteness, but is real. This has enabled us to establish unambiguously that the number counts of quiescent galaxies at z ≃ 2 flatten and slightly decline at magnitudes fainter than Ks ~ 22 (AB mag.), in contrast to the number density of star-forming galaxies, which continues to rise to fainter magnitudes. We show that this trend corresponds to a stellar mass threshold M* ≃ 1010.8 M☉ below which the mechanism that halts the star formation in high-redshift galaxies seems to be inefficient. We also show that, while pBzK galaxies at K < 23 are in the redshift range 1.4 < z < 2.5, as expected, at K > 23 a higher redshift population of z ≃ 3 pBzK galaxies is detected and dominates the counts at the faintest magnitudes. Finally, we compare the observed pBzK number counts with those of quiescent galaxies extracted from four different semi-analytic models. We find that only two of these models reproduce the observed trend in the number counts, even qualitatively, and that none of the models provides a statistically acceptable description of the number density of quiescent galaxies at these redshifts. We conclude that the mass function of quiescent galaxies as a function of redshift continues to present a key and demanding challenge for proposed models of galaxy formation and evolution. [ABSTRACT FROM AUTHOR]

Published
2014
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48. The Hawk-I UDS and GOODS Survey (HUGS): Survey design and deep K-band number counts.

Author

Fontana, A., Dunlop, J. S., Paris, D., Targett, T. A., Boutsia, K., Castellano, M., Galametz, A., Grazian, A., McLure, R., Merlin, E., Pentericci, L., Wuyts, S., Almaini, O., Caputi, K., Chary, R. -R., Cirasuolo, M., Conselice, C. J., Cooray, A., Daddi, E., and Dickinson, M.

Subjects
*GALACTIC evolution, *ASTRONOMICAL observations, *ASTRONOMICAL surveys, *DATA quality, *ENERGY bands
Abstract

We present the results of a new, ultra-deep, near-infrared imaging survey executed with the Hawk-I imager at the ESO VLT, of which we make all the data (images and catalog) public. This survey, named HUGS (Hawk-I UDS and GOODS Survey), provides deep, high-quality imaging in the K and Y bands over the portions of the UKIDSS UDS and GOODS-South fields covered by the CANDELS HST WFC3/IR survey. In this paper we describe the survey strategy, the observational campaign, the data reduction process, and the data quality. We show that, thanks to exquisite image quality and extremely long exposure times, HUGS delivers the deepest K-band images ever collected over areas of cosmological interest, and in general ideally complements the CANDELS data set in terms of image quality and depth. In the GOODS-S field, the K-band observations cover the whole CANDELS area with a complex geometry made of 6 different, partly overlapping pointings, in order to best match the deep and wide areas of CANDELS imaging. In the deepest region (which includes most of the Hubble Ultra Deep Field) exposure times exceed 80 hours of integration, yielding a 1 - σ magnitude limit per square arcsec of '28.0 AB mag. The seeing is exceptional and homogeneous across the various pointings, confined to the range 0.38-0.43 arcsec. In the UDS field the survey is about one magnitude shallower (to match the correspondingly shallower depth of the CANDELS images) but includes also Y-band band imaging (which, in the UDS, was not provided by the CANDELS WFC3/IR imaging). In the K-band, with an average exposure time of 13 hours, and seeing in the range 0.37-0.43 arcsec, the 1 - σ limit per square arcsec in the UDS imaging is ≃27.3 AB mag. In the Y-band, with an average exposure time ≃8 h, and seeing in the range 0.45-0.5 arcsec, the imaging yields a 1 - σ limit per square arcsec of ≃28.3 AB mag. We show that the HUGS observations are well matched to the depth of the CANDELS WFC3/IR data, since the majority of even the faintest galaxies detected in the CANDELS H-band images are also detected in HUGS. Finally we present the K-band galaxy number counts produced by combining the HUGS data from the two fields. We show that the slope of the number counts depends sensitively on the assumed distribution of galaxy sizes, with potential impact on the estimated extra-galactic background light. [ABSTRACT FROM AUTHOR]

Published
2014
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49. Constraints on the star-formation rate of z ~ 3 LBGs with measured metallicity in the CANDELS GOODS-South field.

Author

Castellano, M., Sommariva, V., Fontana, A., Pentericci, L., Santini, P., Grazian, A., Amorin, R., Donley, J. L., Dunlop, J. S., Ferguson, H. C., Fiore, F., Galametz, A., Giallongo, E., Guo, Y., Huang, K.-H., Koekemoer, A., Maiolino, R., McLure, R. J., Paris, D., and Schaerer, D.

Subjects
STAR formation, GALACTIC redshift, ULTRAVIOLET radiation, NEBULAR hypothesis, STELLAR populations
Abstract

Aims. We aim to constrain the assembly history of high-redshift galaxies and the reliability of UV-based estimates of their physical parameters from an accurate analysis of a unique sample of z ~ 3 Lyman-break galaxies (LBGs). Methods. We analyse 14 LBGs at z ~ 2.8–3.8 constituting the only sample where both a spectroscopic measurement of their metallicity and deep IR observations (CANDELS+HUGS survey) are available. Fixing the metallicity of population synthesis models to the observed values, we determine best-fit physical parameters under different assumptions about the star-formation history (SFH) and also consider the effect of nebular emission. For comparison, we determine the UV slope of the objects, and use it to estimate their SFRUV99 by correcting the UV luminosity. Results. A comparison between star-formation rate (SFR) obtained through SED-fitting (SFRfit) and the SFRUV99 shows that the latter are underestimated by a factor of 2–10, regardless of the assumed SFH. Other SFR indicators (radio, far-IR, X-ray, recombination lines) coherently indicate SFRs a factor of 2–4 larger than SFRUV99 and in closer agreement with SFRfit. This discrepancy is due to the solar metallicity implied by the usual ß - A1600 conversion factor. We propose a refined relation, appropriate for subsolar metallicity LBGs: A1600 = 5.32 + 1.99 * ß. This relation reconciles the dust-corrected UV with the SED-fitting and the other SFR indicators. We show that the fact that z ~ 3 galaxies have subsolar metallicity implies an upward revision by a factor of ~1.5–2 of the global SFRD, depending on the assumptions about the age of the stellar populations. We find very young best-fit ages (10–500 Myr) for all our objects. From a careful examination of the uncertainties in the fit and the amplitude of the Balmer break we conclude that there is little evidence of the presence of old stellar population in at least half of the LBGs in our sample, suggesting that these objects are probably caught during a huge star-formation burst, rather than being the result of a smooth evolution. [ABSTRACT FROM AUTHOR]

Published
2014
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50. Mass assembly in quiescent and star-forming galaxies since z ≃ 4 from UltraVISTA.

Author

Ilbert, O., McCracken, H. J., Le Fèvre, O., Capak, P., Dunlop, J., Karim, A., Renzini, M. A., Caputi, K., Boissier, S., Arnouts, S., Aussel, H., Comparat, J., Guo, Q., Hudelot, P., Kartaltepe, J., Kneib, J. P., Krogager, J. K., Le Floc'h, E., Lilly, S., and Mellier, Y.

Subjects
STAR formation, GALAXIES, STELLAR mass, MASS density gradients, REDSHIFT
Abstract

We estimate the galaxy stellar mass function and stellar mass density for star-forming and quiescent galaxies with 0.2 < z < 4. We construct a large, deep (Ks < 24) sample of 220 000 galaxies selected using the new UltraVISTA DR1 data release. Our analysis is based on precise 30-band photometric redshifts. By comparing these photometric redshifts with 10,800 spectroscopic redshifts from the zCOSMOS bright and faint surveys, we find a precision of σΔz/(1+z) = 0.008 at i+ < 22.5 and σΔ/(1+z) = 0.03 at 1.5 < z < 4. We derive the stellar mass function and correct for the Eddington bias. We find a mass-dependent evolution of the global and starforming populations, with the low-mass end of the mass functions evolving more rapidly than the high-mass end. This mass-dependent evolution is a direct consequence of the star formation being "quenched" in galaxies more massive than M ≳ 1010.7-10.9M⊚. For the mass function of the quiescent galaxies, we do not find any significant evolution of the high-mass end at z < 1; however we observe a clear flattening of the faint-end slope. From z ∼ 3 to z ∼ 1, the density of quiescent galaxies increases over the entire mass range. Their comoving stellar mass density increases by 1.6 dex between z ∼ 3 and z ∼ 1 and by less than 0.2 dex at z < 1. We infer the star formation history from the mass density evolution. This inferred star formation history is in excellent agreement with instantaneous star formation rate measurements at z < 1.5, while we find differences of 0.2 dex at z > 1.5 consistent with the expected uncertainties. We also develop a new method to infer the specific star formation rate from the mass function of star-forming galaxies. We find that the specific star formation rate of 1010-10.5M∼ galaxies increases continuously in the redshift range 1 < z < 4. Finally, we compare our results with a semi-analytical model and find that these models overestimate the density of low mass quiescent galaxies by an order of magnitude, while the density of low-mass star-forming galaxies is successfully reproduced. [ABSTRACT FROM AUTHOR]

Published
2013
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