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1,231 results on '"Serjeant, S"'

201. z -GAL:A NOEMA spectroscopic redshift survey of bright Herschel galaxies II. Dust properties

Author

Ismail, D., Beelen, A., Buat, V., Berta, S., Cox, P., Stanley, F., Young, A., Jin, S., Neri, R., Bakx, T., Dannerbauer, H., Butler, K., Cooray, A., Nanni, A., Omont, A., Serjeant, S., Van Der Werf, P., Vlahakis, C., Weiß, A., Yang, C., Baker, A. J., Bendo, G., Borsato, E., Chartab, N., Dye, S., Eales, S., Gavazzi, R., Hughes, D., Ivison, R., Jones, B. M., Krips, M., Lehnert, M., Marchetti, L., Messias, H., Negrello, M., Perez-fournon, I., Riechers, D. A., Urquhart, S., Ismail, D., Beelen, A., Buat, V., Berta, S., Cox, P., Stanley, F., Young, A., Jin, S., Neri, R., Bakx, T., Dannerbauer, H., Butler, K., Cooray, A., Nanni, A., Omont, A., Serjeant, S., Van Der Werf, P., Vlahakis, C., Weiß, A., Yang, C., Baker, A. J., Bendo, G., Borsato, E., Chartab, N., Dye, S., Eales, S., Gavazzi, R., Hughes, D., Ivison, R., Jones, B. M., Krips, M., Lehnert, M., Marchetti, L., Messias, H., Negrello, M., Perez-fournon, I., Riechers, D. A., and Urquhart, S.

Published
2023

202. The bright extragalactic ALMA redshift survey (BEARS) – II. Millimetre photometry of gravitational lens candidates.

Author

Bendo, G J, Urquhart, S A, Serjeant, S, Bakx, T, Hagimoto, M, Cox, P, Neri, R, Lehnert, M D, Dannerbauer, H, Amvrosiadis, A, Andreani, P, Baker, A J, Beelen, A, Berta, S, Borsato, E, Buat, V, Butler, K M, Cooray, A, De Zotti, G, and Dunne, L

Subjects
REDSHIFT, GALACTIC redshift, SPECTRAL energy distribution, PHOTOMETRY, GRAVITATIONAL lenses, ACTINIC flux, ASTRONOMICAL photometry
Abstract

We present 101- and 151-GHz ALMA continuum images for 85 fields selected from Herschel observations that have 500-μm flux densities >80 mJy and 250–500-μm colours consistent with z > 2, most of which are expected to be gravitationally lensed or hyperluminous infrared galaxies. Approximately half of the Herschel 500-μm sources were resolved into multiple ALMA sources, but 11 of the 15 brightest 500-μm Herschel sources correspond to individual ALMA sources. For the 37 fields containing either a single source with a spectroscopic redshift or two sources with the same spectroscopic redshift, we examined the colour temperatures and dust emissivity indices. The colour temperatures only vary weakly with redshift and are statistically consistent with no redshift-dependent temperature variations, which generally corresponds to results from other samples selected in far-infrared, submillimetre, or millimetre bands but not to results from samples selected in optical or near-infrared bands. The dust emissivity indices, with very few exceptions, are largely consistent with a value of 2. We also compared spectroscopic redshifts to photometric redshifts based on spectral energy distribution templates designed for infrared-bright high-redshift galaxies. While the templates systematically underestimate the redshifts by ∼15 per cent, the inclusion of ALMA data decreases the scatter in the predicted redshifts by a factor of ∼2, illustrating the potential usefulness of these millimetre data for estimating photometric redshifts. [ABSTRACT FROM AUTHOR]

Published
2023
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203. The bright extragalactic ALMA redshift survey (BEARS) – II. Millimetre photometry of gravitational lens candidates

Author

Bendo, G J, primary, Urquhart, S A, additional, Serjeant, S, additional, Bakx, T, additional, Hagimoto, M, additional, Cox, P, additional, Neri, R, additional, Lehnert, M D, additional, Dannerbauer, H, additional, Amvrosiadis, A, additional, Andreani, P, additional, Baker, A J, additional, Beelen, A, additional, Berta, S, additional, Borsato, E, additional, Buat, V, additional, Butler, K M, additional, Cooray, A, additional, De Zotti, G, additional, Dunne, L, additional, Dye, S, additional, Eales, S, additional, Enia, A, additional, Fan, L, additional, Gavazzi, R, additional, González-Nuevo, J, additional, Harris, A I, additional, Herrera, C N, additional, Hughes, D H, additional, Ismail, D, additional, Jones, B M, additional, Kohno, K, additional, Krips, M, additional, Lagache, G, additional, Marchetti, L, additional, Massardi, M, additional, Messias, H, additional, Negrello, M, additional, Omont, A, additional, Pérez-Fournon, I, additional, Riechers, D A, additional, Scott, D, additional, Smith, M W L, additional, Stanley, F, additional, Tamura, Y, additional, Temi, P, additional, van der Werf, P, additional, Verma, A, additional, Vlahakis, C, additional, Weiß, A, additional, Yang, C, additional, and Young, A J, additional

Published
2022
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204. QSO Environments at Intermediate Redshifts

Author

Wold, Margrethe, Lacy, Mark, Lilje, Per B., Serjeant, S., Márquez, Isabel, editor, Masegosa, Josefa, editor, del Olmo, Ascensión, editor, Lara, Lucas, editor, García, Emilio, editor, and Molina, Josefina, editor

Published
2001
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205. The bright extragalactic ALMA redshift survey (BEARS) I: redshifts of bright gravitationally lensed galaxies from the Herschel ATLAS

Author

Dye, S, Urquhart, S A, Bendo, G J, Serjeant, S, Bakx, T, Hagimoto, M, Cox, P, Neri, R, Lehnert, M, Sedgwick, C, Weiner, C, Dannerbauer, H, Amvrosiadis, A, Andreani, P, Baker, A J, Beelen, A, Berta, S, Borsato, E, Buat, V, Butler, K M, Cooray, A, De Zotti, G, Kohno, K, Dunne, L, Eales, S, Enia, A, Fan, L, Gavazzi, R, Harris, A I, Herrera, C N, Hughes, D, Ismail, D, Ivison, R, Jin, S, Jones, B, Krips, M, Lagache, G, Marchetti, L, Massardi, M, Messias, H, Negrello, M, Omont, A, Perez-Fournon, I, Riechers, D A, Scott, D, Smith, M W L, Stanley, F, Tamura, Y, Temi, P, Vlahakis, C, Werf, P, Verma, A, Yang, C, and Young, A J

Subjects
Space and Planetary Science, Astronomy and Astrophysics
Abstract

We present spectroscopic measurements for 71 galaxies associated with 62 of the brightest high-redshift submillimetre sources from the Southern fields of the Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS), while targeting 85 sources which resolved into 142. We have obtained robust redshift measurements for all sources using the 12-m Array and an efficient tuning of ALMA to optimize its use as a redshift hunter, with 73 per cent of the sources having a robust redshift identification. Nine of these redshift identifications also rely on observations from the Atacama Compact Array. The spectroscopic redshifts span a range 1.41 < z < 4.53 with a mean value of 2.75, and the CO emission line full-width at half-maxima range between 110kms−1

Published
2022

206. The bright extragalactic ALMA redshift survey (BEARS) I: Redshifts of bright gravitationally lensed galaxies from the Herschel ATLAS

Author

Urquhart, SA, Bendo, GJ, Serjeant, S, Bakx, T, Hagimoto, M, Cox, P, Neri, R, Lehnert, M, Sedgwick, C, Weiner, C, Dannerbauer, H, Amvrosiadis, A, Andreani, P, Baker, AJ, Beelen, A, Berta, S, Borsato, E, Buat, V, Butler, KM, Cooray, A, De Zotti, G, Dunne, L, Dye, S, Eales, S, Enia, A, Fan, L, Gavazzi, R, González-Nuevo, J, Harris, AI, Herrera, CN, Hughes, D, Ismail, D, Ivison, R, Jin, S, Jones, B, Kohno, K, Krips, M, Lagache, G, Marchetti, L, Massardi, M, Messias, H, Negrello, M, Omont, A, Perez-Fournon, I, Riechers, DA, Scott, D, Smith, MWL, Stanley, F, Tamura, Y, Temi, P, Vlahakis, C, Weiß, A, Van Der Werf, P, Verma, A, Yang, C, Young, AJ, Urquhart, SA, Bendo, GJ, Serjeant, S, Bakx, T, Hagimoto, M, Cox, P, Neri, R, Lehnert, M, Sedgwick, C, Weiner, C, Dannerbauer, H, Amvrosiadis, A, Andreani, P, Baker, AJ, Beelen, A, Berta, S, Borsato, E, Buat, V, Butler, KM, Cooray, A, De Zotti, G, Dunne, L, Dye, S, Eales, S, Enia, A, Fan, L, Gavazzi, R, González-Nuevo, J, Harris, AI, Herrera, CN, Hughes, D, Ismail, D, Ivison, R, Jin, S, Jones, B, Kohno, K, Krips, M, Lagache, G, Marchetti, L, Massardi, M, Messias, H, Negrello, M, Omont, A, Perez-Fournon, I, Riechers, DA, Scott, D, Smith, MWL, Stanley, F, Tamura, Y, Temi, P, Vlahakis, C, Weiß, A, Van Der Werf, P, Verma, A, Yang, C, and Young, AJ

Abstract

We present spectroscopic measurements for 71 galaxies associated with 62 of the brightest high-redshift submillimetre sources from the Southern fields of the Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS), while targeting 85 sources which resolved into 142. We have obtained robust redshift measurements for all sources using the 12-m Array and an efficient tuning of ALMA to optimize its use as a redshift hunter, with 73 per cent of the sources having a robust redshift identification. Nine of these redshift identifications also rely on observations from the Atacama Compact Array. The spectroscopic redshifts span a range 1.41 < z < 4.53 with a mean value of 2.75, and the CO emission line full-width at half-maxima range between $\rm 110\, km\, s^{-1} \lt FWHM \lt 1290\, km\, s^{-1}$ with a mean value of ∼500 km s−1, in line with other high-z samples. The derived CO(1-0) luminosity is significantly elevated relative to line-width to CO(1-0) luminosity scaling relation, which is suggestive of lensing magnification across our sources. In fact, the distribution of magnification factors inferred from the CO equivalent widths is consistent with expectations from galaxy–galaxy lensing models, though there is a hint of an excess at large magnifications that may be attributable to the additional lensing optical depth from galaxy groups or clusters.

Published
2022

207. Massive Molecular Gas Reservoir in a Luminous Submillimeter Galaxy during Cosmic Noon

Author

Liu, Bin, primary, Chartab, N., additional, Nayyeri, H., additional, Cooray, A., additional, Yang, C., additional, Riechers, D. A, additional, Gurwell, M., additional, Zhu, Zong-hong, additional, Serjeant, S., additional, Borsato, E., additional, Negrello, M., additional, Marchetti, L., additional, Corsini, E. M., additional, and van der Werf, P., additional

Published
2022
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208. The Nearby Evolved Stars Survey II: Constructing a volume-limited sample and first results from the James Clerk Maxwell Telescope

Author

Scicluna, P, primary, Kemper, F, additional, McDonald, I, additional, Srinivasan, S, additional, Trejo, A, additional, Wallström, S H J, additional, Wouterloot, J G A, additional, Cami, J, additional, Greaves, J, additional, He, Jinhua, additional, Hoai, D T, additional, Kim, Hyosun, additional, Jones, O C, additional, Shinnaga, H, additional, Clark, C J R, additional, Dharmawardena, T, additional, Holland, W, additional, Imai, H, additional, van Loon, J Th, additional, Menten, K M, additional, Wesson, R, additional, Chawner, H, additional, Feng, S, additional, Goldman, S, additional, Liu, F C, additional, MacIsaac, H, additional, Tang, J, additional, Zeegers, S, additional, Amada, K, additional, Antoniou, V, additional, Bemis, A, additional, Boyer, M L, additional, Chapman, S, additional, Chen, X, additional, Cho, S-H, additional, Cui, L, additional, Dell’Agli, F, additional, Friberg, P, additional, Fukaya, S, additional, Gomez, H, additional, Gong, Y, additional, Hadjara, M, additional, Haswell, C, additional, Hirano, N, additional, Hony, S, additional, Izumiura, H, additional, Jeste, M, additional, Jiang, X, additional, Kaminski, T, additional, Keaveney, N, additional, Kim, J, additional, Kraemer, K E, additional, Kuan, Y-J, additional, Lagadec, E, additional, Lee, C F, additional, Li, D, additional, Liu, S-Y, additional, Liu, T, additional, de Looze, I, additional, Lykou, F, additional, Maraston, C, additional, Marshall, J P, additional, Matsuura, M, additional, Min, C, additional, Otsuka, M, additional, Oyadomari, M, additional, Parsons, H, additional, Patel, N A, additional, Peeters, E, additional, Pham, T A, additional, Qiu, J, additional, Randall, S, additional, Rau, G, additional, Redman, M P, additional, Richards, A M S, additional, Serjeant, S, additional, Shi, C, additional, Sloan, G C, additional, Smith, M W L, additional, Suh, K-W, additional, Toalá, J A, additional, Uttenthaler, S, additional, Ventura, P, additional, Wang, B, additional, Yamamura, I, additional, Yang, T, additional, Yun, Y, additional, Zhang, F, additional, Zhang, Y, additional, Zhao, G, additional, Zhu, M, additional, and Zijlstra, A A, additional

Published
2022
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209. The Herschel ATLAS

Author

Eales, S., Dunne, L., Clements, D., Cooray, A., De Zotti, G., Dye, S., Ivison, R., Jarvis, M., Lagache, G., Maddox, S., Negrello, M., Serjeant, S., Thompson, M. A., Kampen, E. Van, Amblard, A., Andreani, P., Baes, M., Beelen, A., Bendo, G. J., Benford, D., Bertoldi, F., Bock, J., Bonfield, D., Boselli, A., Bridge, C., Buat, V., Burgarella, D., Carlberg, R., Cava, A., Chanial, P., Charlot, S., Christopher, N., Coles, P., Cortese, L., Dariush, A., da Cunha, E., Dalton, G., Danese, L., Dannerbauer, H., Driver, S., Dunlop, J., Fan, L., Farrah, D., Frayer, D., Frenk, C., Geach, J., Gardner, J., Gomez, H., González-Nuevo, J., González-Solares, E., Griffin, M., Hardcastle, M., Hatziminaoglou, E., Herranz, D., Hughes, D., Ibar, E., Jeong, Woong-Seob, Lacey, C., Lapi, A., Lawrence, A., Lee, M., Leeuw, L., Liske, J., López-Caniego, M., Müller, T., Nandra, K., Panuzzo, P., Papageorgiou, A., Patanchon, G., Peacock, J., Pearson, C., Phillipps, S., Pohlen, M., Popescu, C., Rawlings, S., Rigby, E., Rigopoulou, M., Robotham, A., Rodighiero, G., Sansom, A., Schulz, B., Scott, D., Smith, D. J. B., Sibthorpe, B., Smail, I., Stevens, J., Sutherland, W., Takeuchi, T., Tedds, J., Temi, P., Tuffs, R., Trichas, M., Vaccari, M., Valtchanov, I., van der Werf, P., Verma, A., Vieria, J., Vlahakis, C., and White, Glenn J.

Published
2010
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210. The bright extragalactic ALMA redshift survey (BEARS) I: redshifts of bright gravitationally lensed galaxies from the Herschel ATLAS

Author

Urquhart, S A, primary, Bendo, G J, additional, Serjeant, S, additional, Bakx, T, additional, Hagimoto, M, additional, Cox, P, additional, Neri, R, additional, Lehnert, M, additional, Sedgwick, C, additional, Weiner, C, additional, Dannerbauer, H, additional, Amvrosiadis, A, additional, Andreani, P, additional, Baker, A J, additional, Beelen, A, additional, Berta, S, additional, Borsato, E, additional, Buat, V, additional, Butler, K M, additional, Cooray, A, additional, De Zotti, G, additional, Dunne, L, additional, Dye, S, additional, Eales, S, additional, Enia, A, additional, Fan, L, additional, Gavazzi, R, additional, González-Nuevo, J, additional, Harris, A I, additional, Herrera, C N, additional, Hughes, D, additional, Ismail, D, additional, Ivison, R, additional, Jin, S, additional, Jones, B, additional, Kohno, K, additional, Krips, M, additional, Lagache, G, additional, Marchetti, L, additional, Massardi, M, additional, Messias, H, additional, Negrello, M, additional, Omont, A, additional, Perez-Fournon, I, additional, Riechers, D A, additional, Scott, D, additional, Smith, M W L, additional, Stanley, F, additional, Tamura, Y, additional, Temi, P, additional, Vlahakis, C, additional, Weiß, A, additional, van der Werf, P, additional, Verma, A, additional, Yang, C, additional, and Young, A J, additional

Published
2022
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211. A high-resolution investigation of the multiphase ISM in a galaxy during the first two billion years

Author

Dye, S, primary, Eales, S A, additional, Gomez, H L, additional, Jones, G C, additional, Smith, M W L, additional, Borsato, E, additional, Moss, A, additional, Dunne, L, additional, Maresca, J, additional, Amvrosiadis, A, additional, Negrello, M, additional, Marchetti, L, additional, Corsini, E M, additional, Ivison, R J, additional, Bendo, G J, additional, Bakx, T, additional, Cooray, A, additional, Cox, P, additional, Dannerbauer, H, additional, Serjeant, S, additional, Riechers, D, additional, Temi, P, additional, and Vlahakis, C, additional

Published
2021
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212. Close-up view of a luminous star-forming galaxy at z=2.95

Author

Berta, S., Young, A.J., Cox, P., Neri, R., Jones, B.M., Baker, A.J., Omont, A., Dunne, L., Carnero Rosell, A., Marchetti, L., Negrello, M., Yang, C., Riechers, D.A., Dannerbauer, H., Perez-Fournon, I., van der Werf, P., Bakx, T., Ivison, R.J., Beelen, A., Buat, V., Cooray, A., Cortzen, I., Dye, S., Eales, S., Gavazzi, R., Harris, A.I., Herrera, C.N., Hughes, D., Jin, S., Krips, M., Lagache, G., Lehnert, M., Messias, H., Serjeant, S., Stanley, F., Urquhart, S., and Vlahakis, C.

Abstract

Exploiting the sensitivity of the IRAM NOrthern Extended Millimeter Array (NOEMA) and its ability to process large instantaneous bandwidths, we have studied the morphology and other properties of the molecular gas and dust in the star forming galaxy, H-ATLAS J131611.5+281219 (HerBS-89a), at z = 2.95. High angular resolution (0.″3) images reveal a partial 1.″0 diameter Einstein ring in the dust continuum emission and the molecular emission lines of 12CO(9−8) and H2O(202 − 111). Together with lower angular resolution (0.″6) images, we report the detection of a series of molecular lines including the three fundamental transitions of the molecular ion OH+, namely (11 − 01), (12 − 01), and (10 − 01), seen in absorption; the molecular ion CH+(1 − 0) seen in absorption, and tentatively in emission; two transitions of amidogen (NH2), namely (202 − 111) and (220 − 211) seen in emission; and HCN(11 − 10) and/or NH(12 − 01) seen in absorption. The NOEMA data are complemented with Very Large Array data tracing the 12CO(1 − 0) emission line, which provides a measurement of the total mass of molecular gas and an anchor for a CO excitation analysis. In addition, we present Hubble Space Telescope imaging that reveals the foreground lensing galaxy in the near-infrared (1.15 μm). Together with photometric data from the Gran Telescopio Canarias, we derive a photometric redshift of zphot = 0.9−0.5+0.3 for the foreground lensing galaxy. Modeling the lensing of HerBS-89a, we reconstruct the dust continuum (magnified by a factor μ ≃ 5.0) and molecular emission lines (magnified by μ ∼ 4 − 5) in the source plane, which probe scales of ∼0.″1 (or 800 pc). The 12CO(9 − 8) and H2O(202 − 111) emission lines have comparable spatial and kinematic distributions; the source-plane reconstructions do not clearly distinguish between a one-component and a two-component scenario, but the latter, which reveals two compact rotating components with sizes of ≈1 kpc that are likely merging, more naturally accounts for the broad line widths observed in HerBS-89a. In the core of HerBS-89a, very dense gas with nH2 ∼ 107 − 9 cm−3 is revealed by the NH2 emission lines and the possible HCN(11 − 10) absorption line. HerBS-89a is a powerful star forming galaxy with a molecular gas mass of Mmol = (2.1 ± 0.4) × 1011 M⊙, an infrared luminosity of LIR = (4.6 ± 0.4) × 1012 L⊙, and a dust mass of Mdust = (2.6 ± 0.2) × 109 M⊙, yielding a dust-to-gas ratio δGDR ≈ 80. We derive a star formation rate SFR = 614 ± 59 M⊙ yr−1 and a depletion timescale τdepl = (3.4 ± 1.0) × 108 years. The OH+ and CH+ absorption lines, which trace low (∼100 cm−3) density molecular gas, all have their main velocity component red-shifted by ΔV ∼ 100 km s−1 relative to the global CO reservoir. We argue that these absorption lines trace a rare example of gas inflow toward the center of a galaxy, indicating that HerBS-89a is accreting gas from its surroundings.

Published
2021

213. Early science with the Large Millimeter Telescope: a 1.1 mm AzTEC survey of red-Herschel dusty star-forming galaxies

Author

Montaña, A, primary, Zavala, J A, additional, Aretxaga, I, additional, Hughes, D H, additional, Ivison, R J, additional, Pope, A, additional, Sánchez-Argüelles, D, additional, Wilson, G W, additional, Yun, M, additional, Cantua, O A, additional, McCrackan, M, additional, Michałowski, M J, additional, Valiante, E, additional, Arumugam, V, additional, Casey, C M, additional, Chávez, R, additional, Colín-Beltrán, E, additional, Dannerbauer, H, additional, Dunlop, J S, additional, Dunne, L, additional, Eales, S, additional, Ferrusca, D, additional, Gómez-Rivera, V, additional, Gómez-Ruiz, A I, additional, de la Luz, V H, additional, Maddox, S J, additional, Narayanan, G, additional, Omont, A, additional, Rodríguez-Montoya, I, additional, Serjeant, S, additional, Schloerb, F P, additional, Velázquez, M, additional, Ventura-González, S, additional, van der Werf, P, additional, and Zeballos, M, additional

Published
2021
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214. Close-up view of a luminous star-forming galaxy at z = 2.95

Author

Berta, S., primary, Young, A. J., additional, Cox, P., additional, Neri, R., additional, Jones, B. M., additional, Baker, A. J., additional, Omont, A., additional, Dunne, L., additional, Carnero Rosell, A., additional, Marchetti, L., additional, Negrello, M., additional, Yang, C., additional, Riechers, D. A., additional, Dannerbauer, H., additional, Perez-Fournon, I., additional, van der Werf, P., additional, Bakx, T., additional, Ivison, R. J., additional, Beelen, A., additional, Buat, V., additional, Cooray, A., additional, Cortzen, I., additional, Dye, S., additional, Eales, S., additional, Gavazzi, R., additional, Harris, A. I., additional, Herrera, C. N., additional, Hughes, D., additional, Jin, S., additional, Krips, M., additional, Lagache, G., additional, Lehnert, M., additional, Messias, H., additional, Serjeant, S., additional, Stanley, F., additional, Urquhart, S., additional, Vlahakis, C., additional, and Weiß, A., additional

Published
2021
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215. Exploring cosmic origins with CORE: Extragalactic sources in cosmic microwave background maps

Author

Zotti, G, González-Nuevo, J, Lopez-Caniego, M, Negrello, M, Greenslade, J, Hernández-Monteagudo, C, Delabrouille, J, Cai, Z, Bonato, M, Achúcarro, A, Ade, P, Allison, R, Ashdown, M, Ballardini, M, Banday, A, Banerji, R, Bartlett, J, Bartolo, N, Basak, S, Bersanelli, M, Biesiada, M, Bilicki, M, Bonaldi, A, Bonavera, L, Borrill, J, Bouchet, F, Boulanger, F, Brinckmann, T, Bucher, M, Burigana, C, Buzzelli, A, Calvo, M, Carvalho, C, Castellano, M, Challinor, A, Chluba, J, Clements, D, Clesse, S, Colafrancesco, S, Colantoni, I, Coppolecchia, A, Crook, M, D'Alessandro, G, de Bernardis, P, de Gasperis, G, Diego, J, Valentino, E, Errard, J, Feeney, S, Fernández-Cobos, R, Ferraro, S, Finelli, F, Forastieri, F, Galli, S, Génova-Santos, R, Gerbino, M, Grandis, S, Hagstotz, S, Hanany, S, Handley, W, Hervias-Caimapo, C, Hills, M, Hivon, E, Kiiveri, K, Kisner, T, Kitching, T, Kunz, M, Kurki-Suonio, H, Lagache, G, Lamagna, L, Lasenby, A, Lattanzi, M, Brun, A, Lesgourgues, J, Lewis, A, Liguori, M, Lindholm, V, Luzzi, G, Maffei, B, Mandolesi, N, Martinez-Gonzalez, E, Martins, C, Masi, S, Massardi, M, Matarrese, S, Mccarthy, D, Melchiorri, A, Melin, J, Molinari, D, Monfardini, A, Natoli, P, Notari, A, Paiella, A, Paoletti, D, Partridge, R, Patanchon, G, Piat, M, Pisano, G, Polastri, L, Polenta, G, Pollo, A, Poulin, V, Quartin, M, Remazeilles, M, Roman, M, Rossi, G, Roukema, B, Rubiño-Martín, J, Salvati, L, Scott, D, Serjeant, S, Tartari, A, Toffolatti, L, Tomasi, M, Trappe, N, Triqueneaux, S, Trombetti, T, Tucci, M, Tucker, C, Väliviita, J, de Weygaert, R, Tent, B, Vennin, V, Vielva, P, Vittorio, N, Young, K, Zannoni, M, Zotti, G. De, González-Nuevo, J., Lopez-Caniego, M., Negrello, M., Greenslade, J., Hernández-Monteagudo, C., Delabrouille, J., Cai, Z. -Y., Bonato, M., Achúcarro, A., Ade, P., Allison, R., Ashdown, M., Ballardini, M., Banday, A. J., Banerji, R., Bartlett, J. G., Bartolo, N., Basak, S., Bersanelli, M., Biesiada, M., Bilicki, M., Bonaldi, A., Bonavera, L., Borrill, J., Bouchet, F., Boulanger, F., Brinckmann, T., Bucher, M., Burigana, C., Buzzelli, A., Calvo, M., Carvalho, C. S., Castellano, M. G., Challinor, A., Chluba, J., Clements, D. L., Clesse, S., Colafrancesco, S., Colantoni, I., Coppolecchia, A., Crook, M., D'Alessandro, G., de Bernardis, P., de Gasperis, G., Diego, J. M., Valentino, E. Di, Errard, J., Feeney, S. M., Fernández-Cobos, R., Ferraro, S., Finelli, F., Forastieri, F., Galli, S., Génova-Santos, R. T., Gerbino, M., Grandis, S., Hagstotz, S., Hanany, S., Handley, W., Hervias-Caimapo, C., Hills, M., Hivon, E., Kiiveri, K., Kisner, T., Kitching, T., Kunz, M., Kurki-Suonio, H., Lagache, G., Lamagna, L., Lasenby, A., Lattanzi, M., Brun, A. Le, Lesgourgues, J., Lewis, A., Liguori, M., Lindholm, V., Luzzi, G., Maffei, B., Mandolesi, N., Martinez-Gonzalez, E., Martins, C. J. A. P., Masi, S., Massardi, M., Matarrese, S., McCarthy, D., Melchiorri, A., Melin, J. -B., Molinari, D., Monfardini, A., Natoli, P., Notari, A., Paiella, A., Paoletti, D., Partridge, R. B., Patanchon, G., Piat, M., Pisano, G., Polastri, L., Polenta, G., Pollo, A., Poulin, V., Quartin, M., Remazeilles, M., Roman, M., Rossi, G., Roukema, B. F., Rubiño-Martín, J. -A., Salvati, L., Scott, D., Serjeant, S., Tartari, A., Toffolatti, L., Tomasi, M., Trappe, N., Triqueneaux, S., Trombetti, T., Tucci, M., Tucker, C., Väliviita, J., de Weygaert, R. van, Tent, B. Van, Vennin, V., Vielva, P., Vittorio, N., Young, K., Zannoni, M., Zotti, G, González-Nuevo, J, Lopez-Caniego, M, Negrello, M, Greenslade, J, Hernández-Monteagudo, C, Delabrouille, J, Cai, Z, Bonato, M, Achúcarro, A, Ade, P, Allison, R, Ashdown, M, Ballardini, M, Banday, A, Banerji, R, Bartlett, J, Bartolo, N, Basak, S, Bersanelli, M, Biesiada, M, Bilicki, M, Bonaldi, A, Bonavera, L, Borrill, J, Bouchet, F, Boulanger, F, Brinckmann, T, Bucher, M, Burigana, C, Buzzelli, A, Calvo, M, Carvalho, C, Castellano, M, Challinor, A, Chluba, J, Clements, D, Clesse, S, Colafrancesco, S, Colantoni, I, Coppolecchia, A, Crook, M, D'Alessandro, G, de Bernardis, P, de Gasperis, G, Diego, J, Valentino, E, Errard, J, Feeney, S, Fernández-Cobos, R, Ferraro, S, Finelli, F, Forastieri, F, Galli, S, Génova-Santos, R, Gerbino, M, Grandis, S, Hagstotz, S, Hanany, S, Handley, W, Hervias-Caimapo, C, Hills, M, Hivon, E, Kiiveri, K, Kisner, T, Kitching, T, Kunz, M, Kurki-Suonio, H, Lagache, G, Lamagna, L, Lasenby, A, Lattanzi, M, Brun, A, Lesgourgues, J, Lewis, A, Liguori, M, Lindholm, V, Luzzi, G, Maffei, B, Mandolesi, N, Martinez-Gonzalez, E, Martins, C, Masi, S, Massardi, M, Matarrese, S, Mccarthy, D, Melchiorri, A, Melin, J, Molinari, D, Monfardini, A, Natoli, P, Notari, A, Paiella, A, Paoletti, D, Partridge, R, Patanchon, G, Piat, M, Pisano, G, Polastri, L, Polenta, G, Pollo, A, Poulin, V, Quartin, M, Remazeilles, M, Roman, M, Rossi, G, Roukema, B, Rubiño-Martín, J, Salvati, L, Scott, D, Serjeant, S, Tartari, A, Toffolatti, L, Tomasi, M, Trappe, N, Triqueneaux, S, Trombetti, T, Tucci, M, Tucker, C, Väliviita, J, de Weygaert, R, Tent, B, Vennin, V, Vielva, P, Vittorio, N, Young, K, Zannoni, M, Zotti, G. De, González-Nuevo, J., Lopez-Caniego, M., Negrello, M., Greenslade, J., Hernández-Monteagudo, C., Delabrouille, J., Cai, Z. -Y., Bonato, M., Achúcarro, A., Ade, P., Allison, R., Ashdown, M., Ballardini, M., Banday, A. J., Banerji, R., Bartlett, J. G., Bartolo, N., Basak, S., Bersanelli, M., Biesiada, M., Bilicki, M., Bonaldi, A., Bonavera, L., Borrill, J., Bouchet, F., Boulanger, F., Brinckmann, T., Bucher, M., Burigana, C., Buzzelli, A., Calvo, M., Carvalho, C. S., Castellano, M. G., Challinor, A., Chluba, J., Clements, D. L., Clesse, S., Colafrancesco, S., Colantoni, I., Coppolecchia, A., Crook, M., D'Alessandro, G., de Bernardis, P., de Gasperis, G., Diego, J. M., Valentino, E. Di, Errard, J., Feeney, S. M., Fernández-Cobos, R., Ferraro, S., Finelli, F., Forastieri, F., Galli, S., Génova-Santos, R. T., Gerbino, M., Grandis, S., Hagstotz, S., Hanany, S., Handley, W., Hervias-Caimapo, C., Hills, M., Hivon, E., Kiiveri, K., Kisner, T., Kitching, T., Kunz, M., Kurki-Suonio, H., Lagache, G., Lamagna, L., Lasenby, A., Lattanzi, M., Brun, A. Le, Lesgourgues, J., Lewis, A., Liguori, M., Lindholm, V., Luzzi, G., Maffei, B., Mandolesi, N., Martinez-Gonzalez, E., Martins, C. J. A. P., Masi, S., Massardi, M., Matarrese, S., McCarthy, D., Melchiorri, A., Melin, J. -B., Molinari, D., Monfardini, A., Natoli, P., Notari, A., Paiella, A., Paoletti, D., Partridge, R. B., Patanchon, G., Piat, M., Pisano, G., Polastri, L., Polenta, G., Pollo, A., Poulin, V., Quartin, M., Remazeilles, M., Roman, M., Rossi, G., Roukema, B. F., Rubiño-Martín, J. -A., Salvati, L., Scott, D., Serjeant, S., Tartari, A., Toffolatti, L., Tomasi, M., Trappe, N., Triqueneaux, S., Trombetti, T., Tucci, M., Tucker, C., Väliviita, J., de Weygaert, R. van, Tent, B. Van, Vennin, V., Vielva, P., Vittorio, N., Young, K., and Zannoni, M.

Abstract

We discuss the potential of a next generation space-borne Cosmic Microwave Background (CMB) experiment for studies of extragalactic sources. Our analysis has particular bearing on the definition of the future space project, CORE, that has been submitted in response to ESA's call for a Medium-size mission opportunity as the successor of the Planck satellite. Even though the effective telescope size will be somewhat smaller than that of Planck, CORE will have a considerably better angular resolution at its highest frequencies, since, in contrast with Planck, it will be diffraction limited at all frequencies. The improved resolution implies a considerable decrease of the source confusion, i.e. substantially fainter detection limits. In particular, CORE will detect thousands of strongly lensed high-z galaxies distributed over the full sky. The extreme brightness of these galaxies will make it possible to study them, via follow-up observations, in extraordinary detail. Also, the CORE resolution matches the typical sizes of high-z galaxy proto-clusters much better than the Planck resolution, resulting in a much higher detection efficiency; these objects will be caught in an evolutionary phase beyond the reach of surveys in other wavebands. Furthermore, CORE will provide unique information on the evolution of the star formation in virialized groups and clusters of galaxies up to the highest possible redshifts. Finally, thanks to its very high sensitivity, CORE will detect the polarized emission of thousands of radio sources and, for the first time, of dusty galaxies, at mm and sub-mm wavelengths, respectively.

Published
2018

216. A high redshift population of galaxies at the North Ecliptic Pole

Author

Barrufet, L., Pearson, C., Serjeant, S., Małek, K., Baronchelli, I., Campos-Varillas, M. C., White, G. J., Valtchanov, I., Matsuhara, H., Conversi, L., Kim, S. J., Goto, T., Oi, N., Malkan, M., Kim, H., Ikeda, H., Takagi, T., Toba, Y., and Miyaji, T.

Subjects
starburst [galaxies], galaxies [submillimeter], Astronomy & Astrophysics, evolution [galaxies], high-redshift [galaxies], Astronomical and Space Sciences
Abstract

Context. Dusty high-z galaxies are extreme objects with high star formation rates (SFRs) and luminosities. Characterising the properties of this population and analysing their evolution over cosmic time is key to understanding galaxy evolution in the early Universe.\ud \ud Aims. We select a sample of high-z dusty star-forming galaxies (DSFGs) and evaluate their position on the main sequence (MS) of star-forming galaxies, the well-known correlation between stellar mass and SFR. We aim to understand the causes of their high star formation and quantify the percentage of DSFGs that lie above the MS.\ud \ud Methods. We adopted a multi-wavelength approach with data from optical to submillimetre wavelengths from surveys at the North Ecliptic Pole to study a submillimetre sample of high-redshift galaxies. Two submillimetre selection methods were used, including: sources selected at 850 μm with the Sub-millimetre Common-User Bolometer Array 2) SCUBA-2 instrument and Herschel-Spectral and Photometric Imaging Receiver (SPIRE) selected sources (colour-colour diagrams and 500 μm risers), finding that 185 have good multi-wavelength coverage. The resulting sample of 185 high-z candidates was further studied by spectral energy distribution fitting with the CIGALE fitting code. We derived photometric redshifts, stellar masses, SFRs, and additional physical parameters, such as the infrared luminosity and active galactic nuclei (AGN) contribution.\ud \ud Results. We find that the Herschel-SPIRE selected DSFGs generally have higher redshifts (z = 2.57−0.09+0.08) than sources that are selected solely by the SCUBA-2 method (z = 1.45−0.06+0.21). We find moderate SFRs (797−50+108 M⊙ yr−1), which are typically lower than those found in other studies. We find that the different results in the literature are, only in part, due to selection effects, as even in the most extreme cases, SFRs are still lower than a few thousand solar masses per year. The difference in measured SFRs affects the position of DSFGs on the MS of galaxies; most of the DSFGs lie on the MS (60%). Finally, we find that the star formation efficiency (SFE) depends on the epoch and intensity of the star formation burst in the galaxy; the later the burst, the more intense the star formation. We discuss whether the higher SFEs in DSFGs could be due to mergers.

Published
2020

217. Piloting Citizen Science Methods to Measure Perceptions of Carbon Footprint and Energy Content of Food

Author

Armstrong, B, Bridge, G, Oakden, L, Reynolds, C, Wang, C, Panzone, LA, Rivera, XS, Kause, A, Ffoulkes, C, Krawczyk, C, Miller, G, Serjeant, S, Armstrong, B, Bridge, G, Oakden, L, Reynolds, C, Wang, C, Panzone, LA, Rivera, XS, Kause, A, Ffoulkes, C, Krawczyk, C, Miller, G, and Serjeant, S

Abstract

© Copyright © 2020 Armstrong, Bridge, Oakden, Reynolds, Wang, Panzone, Rivera, Kause, Ffoulkes, Krawczyk, Miller and Serjeant. There is a food knowledge disconnect between the food research community, and the general population. Food experts know detailed information about foods, but there is a lack of understanding about what citizens know. Citizen science has been used successfully in various fields however, is virtually absent from food research. This pilot study explores the efficacy of Zooniverse citizen science platform as a method of food citizen research, and assesses the impact of response method, food type, portion size and weight information, on estimates of carbon footprint and energy content. Estimates of the carbon footprint (grams of carbon dioxide equivalent) and energy content (Kcal) of 10 foods were measured in a 3 (Between: Response Method; multiple-choice, slider, text box) × 3 (Within: portion size; small, medium, large) × 2 (Between: weight information; present, absent) observational survey. Citizens (N = ~516, unique IP addresses) were recruited via informal email networks. Kruskal–Wallis and Chi-square analyses compared citizen estimations with validated values, and assessed the impact of the variables on estimations. The majority of carbon footprint and energy content estimates were inaccurate, with citizens typically overestimating values. We observe an unexpected correlation between carbon footprint and energy content estimates. Portion size impacts perceptions, with estimations increasing with larger portion sizes. Weight information impacts perceptions, with estimations of carbon footprint being lower, and estimates of energy content being higher when weight information is present. Input method significantly affects observed values, estimates of carbon footprint and energy content estimates were lowest using the text box, followed by the slider tool, highest estimates were given using multiple choice. Citizens are unable to accurately es

Published
2020

218. AKARI/IRC source catalogues and source counts for the IRAC Dark Field, ELAIS North and the AKARI Deep Field South

Author

Davidge, H., Serjeant, S., Pearson, C., Dryer, B., Barrufet, L., Matsuhara, Hideo, and Wada, Takehiko

Subjects
Active galactic nucleus, Cosmology and Nongalactic Astrophysics (astro-ph.CO), Stellar population, Hubble Deep Field, Infrared, FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, 01 natural sciences, methods data analysis, law.invention, infrared: galaxies, Telescope, surveys, law, 0103 physical sciences, Astrophysics::Solar and Stellar Astrophysics, Source counts, 010303 astronomy & astrophysics, Spectrograph, Astrophysics::Galaxy Astrophysics, catalogues, Physics, 010308 nuclear & particles physics, Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy and Astrophysics, Astrophysics - Astrophysics of Galaxies, Space and Planetary Science, Astrophysics of Galaxies (astro-ph.GA), Satellite, Astrophysics::Earth and Planetary Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

We present the first detailed analysis of three extragalactic fields (IRAC Dark Field, ELAIS-N1, ADF-S) observed by the infrared satellite, AKARI, using an optimised data analysis toolkit specifically for the processing of extragalactic point sources. The InfraRed Camera (IRC) on AKARI complements the Spitzer space telescope via its comprehensive coverage between 8-24 microns filling the gap between the Spitzer IRAC and MIPS instruments. Source counts in the AKARI bands at 3.2, 4.1, 7, 11, 15 and 18 microns are presented. At near-infrared wavelengths, our source counts are consistent with counts made in other AKARI fields and in general with Spitzer/IRAC (except at 3.2 microns where our counts lie above). In the mid-infrared (11 - 18 microns) we find our counts are consistent with both previous surveys by AKARI and the Spitzer peak-up imaging survey with the InfraRed Spectrograph (IRS). Using our counts to constrain contemporary evolutionary models we find that although the models and counts are in agreement at mid-infrared wavelengths there are inconsistencies at wavelengths shortward of 7 microns, suggesting either a problem with stellar subtraction or indicating the need for refinement of the stellar population models. We have also investigated the AKARI/IRC filters, and find an AGN selection criteria out to $z, Accepted for publication in MNRAS

Published
2017

219. bright extragalactic ALMA redshift survey (BEARS) I: redshifts of bright gravitationally lensed galaxies from the Herschel ATLAS.

Author

Urquhart, S A, Bendo, G J, Serjeant, S, Bakx, T, Hagimoto, M, Cox, P, Neri, R, Lehnert, M, Sedgwick, C, Weiner, C, Dannerbauer, H, Amvrosiadis, A, Andreani, P, Baker, A J, Beelen, A, Berta, S, Borsato, E, Buat, V, Butler, K M, and Cooray, A

Subjects
REDSHIFT, GALAXIES, SUBMILLIMETER astronomy, GALACTIC redshift, GALAXY clusters
Abstract

We present spectroscopic measurements for 71 galaxies associated with 62 of the brightest high-redshift submillimetre sources from the Southern fields of the Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS), while targeting 85 sources which resolved into 142. We have obtained robust redshift measurements for all sources using the 12-m Array and an efficient tuning of ALMA to optimize its use as a redshift hunter, with 73 per cent of the sources having a robust redshift identification. Nine of these redshift identifications also rely on observations from the Atacama Compact Array. The spectroscopic redshifts span a range 1.41 < z < 4.53 with a mean value of 2.75, and the CO emission line full-width at half-maxima range between |$\rm 110\, km\, s^{-1} \lt FWHM \lt 1290\, km\, s^{-1}$| with a mean value of ∼500 km s−1, in line with other high- z samples. The derived CO(1-0) luminosity is significantly elevated relative to line-width to CO(1-0) luminosity scaling relation, which is suggestive of lensing magnification across our sources. In fact, the distribution of magnification factors inferred from the CO equivalent widths is consistent with expectations from galaxy–galaxy lensing models, though there is a hint of an excess at large magnifications that may be attributable to the additional lensing optical depth from galaxy groups or clusters. [ABSTRACT FROM AUTHOR]

Published
2022
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220. IRAM 30-m-EMIR redshift search of z = 3–4 lensed dusty starbursts selected from the HerBS sample

Author

Bakx, T J L C, primary, Dannerbauer, H, primary, Frayer, D, primary, Eales, S A, primary, Pérez-Fournon, I, primary, Cai, Z-Y, primary, Clements, D L, primary, De Zotti, G, primary, González-Nuevo, J, primary, Ivison, R J, primary, Lapi, A, primary, Michałowski, M J, primary, Negrello, M, primary, Serjeant, S, primary, Smith, M W L, primary, Temi, P, primary, Urquhart, S, primary, and van der Werf, P, primary

Published
2020
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221. NOEMA redshift measurements of bright Herschel galaxies

Author

Neri, R., primary, Cox, P., additional, Omont, A., additional, Beelen, A., additional, Berta, S., additional, Bakx, T., additional, Lehnert, M., additional, Baker, A. J., additional, Buat, V., additional, Cooray, A., additional, Dannerbauer, H., additional, Dunne, L., additional, Dye, S., additional, Eales, S., additional, Gavazzi, R., additional, Harris, A. I., additional, Herrera, C. N., additional, Hughes, D., additional, Ivison, R., additional, Jin, S., additional, Krips, M., additional, Lagache, G., additional, Marchetti, L., additional, Messias, H., additional, Negrello, M., additional, Perez-Fournon, I., additional, Riechers, D. A., additional, Serjeant, S., additional, Urquhart, S., additional, Vlahakis, C., additional, Weiß, A., additional, van der Werf, P., additional, Yang, C., additional, and Young, A. J., additional

Published
2020
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222. Unveiling Cosmic Dawn: the synergetic role of space and ground-based telescopes

Author

Cuby, J.-G., Oesch, P., Cooray, A., Rhodes, J., Bremer, M., Bowler, R., Capak, P., Caputi, K., Castellano, M., Conselice, C., Cuillandre, J.-C, Dayal, P., Davidzon, I., Dunlop, J., Finkelstein, S., Fontana, A., Kashlinsky, A., Koopmans, L., Kuijken, K.H., Brun, V. le, Fèvre, O. le, Mortlock, D., Pello, R., Pentericci, l., Sahlén, M., Schneider, R., Serjeant, S., Warren, S., Astronomy, Laboratoire d'Astrophysique de Marseille (LAM), and Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)

Subjects
[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics::Galaxy Astrophysics
Abstract

Euclid and WFIRST will find thousands of galaxies and quasars above redshift 7 during the epoch of reionization. Massive spectroscopic follow-up campaigns with existing and planned near-infrared and mm facilities will be required for confirmation and physical characterization. A properly coordinated large follow-up campaign is recommended.

Published
2019

223. The case for a 'sub-millimeter SDSS': a 3D map of galaxy evolution to z 10

Author

Geach, J., Banerji, M., Bertoldi, F., Bethermin, M., Casey, C., Chen, C., Clements, D., Cicone, C., Combes, F., Conselice, C., Cooray, A., Coppin, K., Daddi, E., Dannerbauer, H., Dave, R., Doherty, M., Dunlop, J., Edge, A., Farrah, D., Franco, M., Fuller, G., Garratt, T., Gear, W., Greve, T., Hatziminaoglou, E., Hayward, C., Ivison, R., Kawabe, R., Klaassen, P., Knudsen, K., Kohno, K., Koprowski, M., Lagos, C., Magdis, G., Magnelli, B., McGee, S., Michalowski, M., Mroczkowski, T., Noroozian, O., Narayanan, D., Oliver, S., Riechers, D., Rujopakarn, W., Scott, D., Serjeant, S., Smith, M., Swinbank, M., Tamura, Y., van der Werf, P., van Kampen, E., Verma, A., Vieira, J., Wagg, J., Walter, F., Wang, L., Wootten, A., and Yun, M.

Subjects
ComputingMethodologies_IMAGEPROCESSINGANDCOMPUTERVISION, Astrophysics::Instrumentation and Methods for Astrophysics, Astrophysics::Solar and Stellar Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics::Galaxy Astrophysics
Abstract

We argue that a 'sub-millimeter SDSS' - a sensitive large-area imaging+spectroscopic survey in the sub-mm window - will revolutionize our understanding of galaxy evolution in the early Universe.

Published
2019

226. AKARI mid-infrared slitless spectroscopic survey of star-forming galaxies at z less than or similar to 0.5

Author

Malkan, M., Lee, Hyung Mok, Im, Myungshin, Kim, Ji Hoon, Pearson, Chris, Burgarella, Denis, Mazyed, F., Jeong, Woong-Seob, Diaz, Tello J., Serjeant, S., Takeuchi, T. T., Toba, Y., White, G. J., Ohyama, Youichi, Wada, Takehiko, Matsuhara, Hideo, Takagi, Toshinobu, Goto, Tomotsugu, Egami, Eiichi, Inami, Hanae, Oyabu, Shinki, Usui, Fumihiko, Imanishi, Masatoshi, Miyaji, Takamitsu, Nakagawa, Takao, Hanami, Hitoshi, and Ishigaki, Tsuyoshi

Subjects
galaxies: active, galaxies: starburst, galaxies: evolution, infrared: galaxies
Abstract

著者人数: 27名, Accepted: 2018-08-09, 資料番号: SA1180118000

Published
2018

227. The strong gravitational lens finding challenge

Author

Metcalf, R. B., primary, Meneghetti, M., additional, Avestruz, C., additional, Bellagamba, F., additional, Bom, C. R., additional, Bertin, E., additional, Cabanac, R., additional, Courbin, F., additional, Davies, A., additional, Decencière, E., additional, Flamary, R., additional, Gavazzi, R., additional, Geiger, M., additional, Hartley, P., additional, Huertas-Company, M., additional, Jackson, N., additional, Jacobs, C., additional, Jullo, E., additional, Kneib, J.-P., additional, Koopmans, L. V. E., additional, Lanusse, F., additional, Li, C.-L., additional, Ma, Q., additional, Makler, M., additional, Li, N., additional, Lightman, M., additional, Petrillo, C. E., additional, Serjeant, S., additional, Schäfer, C., additional, Sonnenfeld, A., additional, Tagore, A., additional, Tortora, C., additional, Tuccillo, D., additional, Valentín, M. B., additional, Velasco-Forero, S., additional, Verdoes Kleijn, G. A., additional, and Vernardos, G., additional

Published
2019
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228. Spectroscopic confirmation and modelling of two lensed quadruple quasars in the Dark Energy Survey public footprint

Author

Spiniello, C, primary, Sergeyev, A V, primary, Marchetti, L, primary, Tortora, C, primary, Napolitano, N R, primary, Shalyapin, V, primary, Agnello, A, primary, Getman, F I, primary, Vaccari, M, primary, Serjeant, S, primary, Koopmans, L V E, primary, Baker, A J, primary, Jarrett, T H, primary, Covone, G, primary, and Vernardos, G, primary

Published
2019
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229. Exploring Cosmic Origins with CORE: Extragalactic sources in Cosmic Microwave Background maps

Author

Zotti, G. De, González-Nuevo, J., Lopez-Caniego, M., Negrello, M., Greenslade, J., Hernández-Monteagudo, C., Delabrouille, J., Cai, Z. -Y., Bonato, M., Achúcarro, A., Ade, P., Allison, R., Ashdown, M., Ballardini, M., Banday, A. J., Banerji, R., Bartlett, J. G., Bartolo, N., Basak, S., Bersanelli, M., Biesiada, M., Bilicki, M., Bonaldi, A., Bonavera, L., Borrill, J., Bouchet, F., Boulanger, F., Brinckmann, T., Bucher, M., Burigana, C., Buzzelli, A., Calvo, M., Carvalho, C. S., Castellano, M. G., Challinor, A., Chluba, J., Clements, D. L., Clesse, S., Colafrancesco, S., Colantoni, I., Coppolecchia, A., Crook, M., D'Alessandro, G., De Bernardis, P., De Gasperis, G., Diego, J. M., Valentino, E. Di, Errard, J., Feeney, S. M., Fernández-Cobos, R., Ferraro, S., Finelli, F., Forastieri, F., Galli, S., Génova-Santos, R. T., Gerbino, M., Grandis, S., Hagstotz, S., Hanany, S., Handley, W., Hervias-Caimapo, C., Hills, M., Hivon, E., Kiiveri, K., Kisner, T., Kitching, T., Kunz, M., Kurki-Suonio, H., Lagache, G., Lamagna, L., Lasenby, A., Lattanzi, M., Brun, A. Le, Lesgourgues, J., Lewis, A., Liguori, M., Lindholm, V., Luzzi, G., Maffei, B., Mandolesi, N., Martinez-Gonzalez, E., Martins, C. J. A. P., Masi, S., Massardi, M., Matarrese, S., Mccarthy, D., Melchiorri, A., Melin, J. -B., Molinari, D., Monfardini, A., Natoli, P., Notari, A., Paiella, A., Paoletti, D., Partridge, R. B., Patanchon, G., Piat, M., Pisano, G., Polastri, L., Polenta, G., Pollo, A., Poulin, V., Quartin, M., Remazeilles, M., Roman, M., Rossi, G., Roukema, B. F., Rubiño-Martín, J. -A., Salvati, L., Scott, D., Serjeant, S., Tartari, A., Toffolatti, L., Tomasi, M., Trappe, N., Triqueneaux, S., Trombetti, T., Tucci, M., Tucker, C., Väliviita, J., De Weygaert, R. Van, Tent, B. Van, Vennin, V., Vielva, P., Vittorio, N., Young, K., Zannoni, M., D'Alessandro, Giuseppe, AstroParticule et Cosmologie ( APC - UMR 7164 ), Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ), Institut de recherche en astrophysique et planétologie ( IRAP ), Université Paul Sabatier - Toulouse 3 ( UPS ) -Observatoire Midi-Pyrénées ( OMP ) -Centre National de la Recherche Scientifique ( CNRS ), Institut d'Astrophysique de Paris ( IAP ), Université Pierre et Marie Curie - Paris 6 ( UPMC ) -Institut national des sciences de l'Univers ( INSU - CNRS ) -Centre National de la Recherche Scientifique ( CNRS ), Institut d'astrophysique spatiale ( IAS ), Université Paris-Sud - Paris 11 ( UP11 ) -Institut national des sciences de l'Univers ( INSU - CNRS ) -Centre National de la Recherche Scientifique ( CNRS ), Institut Néel ( NEEL ), Université Grenoble Alpes [Saint Martin d'Hères]-Centre National de la Recherche Scientifique ( CNRS ), Institut Lagrange de Paris, Sorbonne Universités, Laboratoire de Physique Nucléaire et de Hautes Énergies ( LPNHE ), Université Pierre et Marie Curie - Paris 6 ( UPMC ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Université Paris Diderot - Paris 7 ( UPD7 ) -Centre National de la Recherche Scientifique ( CNRS ), Laboratoire d'Astrophysique de Marseille ( LAM ), Aix Marseille Université ( AMU ) -Institut national des sciences de l'Univers ( INSU - CNRS ) -Centre National d'Etudes Spatiales ( CNES ) -Centre National de la Recherche Scientifique ( CNRS ), Laboratoire AIM, Université Paris Diderot - Paris 7 ( UPD7 ) -Centre d'Etudes de Saclay, Département de Physique des Particules (ex SPP) ( DPP ), Institut de Recherches sur les lois Fondamentales de l'Univers ( IRFU ), Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ) -Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ) -Université Paris-Saclay, Laboratoire d'Annecy-le-Vieux de Physique Théorique ( LAPTH ), Université Savoie Mont Blanc ( USMB [Université de Savoie] [Université de Chambéry] ) -Centre National de la Recherche Scientifique ( CNRS ), Laboratoire de Physique Théorique d'Orsay [Orsay] ( LPT ), Université Paris-Sud - Paris 11 ( UP11 ) -Centre National de la Recherche Scientifique ( CNRS ), CORE, AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Institut de recherche en astrophysique et planétologie (IRAP), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), Institut d'Astrophysique de Paris (IAP), Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Institut d'astrophysique spatiale (IAS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES), Cryogénie (NEEL - Cryo), Institut Néel (NEEL), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019])-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019]), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Astrophysique Interprétation Modélisation (AIM (UMR7158 / UMR_E_9005 / UM_112)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Département de Physique des Particules (ex SPP) (DPhP), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Hélium : du fondamental aux applications (NEEL - HELFA), Laboratoire d'Annecy-le-Vieux de Physique Théorique (LAPTH), Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Théorique d'Orsay [Orsay] (LPT), Université Paris-Sud - Paris 11 (UP11)-Centre National de la Recherche Scientifique (CNRS), Zotti, G, González-Nuevo, J, Lopez-Caniego, M, Negrello, M, Greenslade, J, Hernández-Monteagudo, C, Delabrouille, J, Cai, Z, Bonato, M, Achúcarro, A, Ade, P, Allison, R, Ashdown, M, Ballardini, M, Banday, A, Banerji, R, Bartlett, J, Bartolo, N, Basak, S, Bersanelli, M, Biesiada, M, Bilicki, M, Bonaldi, A, Bonavera, L, Borrill, J, Bouchet, F, Boulanger, F, Brinckmann, T, Bucher, M, Burigana, C, Buzzelli, A, Calvo, M, Carvalho, C, Castellano, M, Challinor, A, Chluba, J, Clements, D, Clesse, S, Colafrancesco, S, Colantoni, I, Coppolecchia, A, Crook, M, D'Alessandro, G, de Bernardis, P, de Gasperis, G, Diego, J, Valentino, E, Errard, J, Feeney, S, Fernández-Cobos, R, Ferraro, S, Finelli, F, Forastieri, F, Galli, S, Génova-Santos, R, Gerbino, M, Grandis, S, Hagstotz, S, Hanany, S, Handley, W, Hervias-Caimapo, C, Hills, M, Hivon, E, Kiiveri, K, Kisner, T, Kitching, T, Kunz, M, Kurki-Suonio, H, Lagache, G, Lamagna, L, Lasenby, A, Lattanzi, M, Brun, A, Lesgourgues, J, Lewis, A, Liguori, M, Lindholm, V, Luzzi, G, Maffei, B, Mandolesi, N, Martinez-Gonzalez, E, Martins, C, Masi, S, Massardi, M, Matarrese, S, Mccarthy, D, Melchiorri, A, Melin, J, Molinari, D, Monfardini, A, Natoli, P, Notari, A, Paiella, A, Paoletti, D, Partridge, R, Patanchon, G, Piat, M, Pisano, G, Polastri, L, Polenta, G, Pollo, A, Poulin, V, Quartin, M, Remazeilles, M, Roman, M, Rossi, G, Roukema, B, Rubiño-Martín, J, Salvati, L, Scott, D, Serjeant, S, Tartari, A, Toffolatti, L, Tomasi, M, Trappe, N, Triqueneaux, S, Trombetti, T, Tucci, M, Tucker, C, Väliviita, J, de Weygaert, R, Tent, B, Vennin, V, Vielva, P, Vittorio, N, Young, K, Zannoni, M, Astronomy, Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Observatoire Midi-Pyrénées (OMP), Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Université Grenoble Alpes (UGA)-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES), Astrophysique Interprétation Modélisation (AIM (UMR_7158 / UMR_E_9005 / UM_112)), Département de Physique des Particules (ex SPP) (DPP), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019]), Sorbonne Université (SU), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7), Centre National de la Recherche Scientifique (CNRS)-Université Paris-Sud - Paris 11 (UP11), Science and Technology Facilities Council (STFC), Science and Technology Facilities Council, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA), Helsinki Institute of Physics, and Department of Physics

Subjects
LENSED GALAXIES, Brightness, POLARIZATION, active galactic nuclei, CMBR experiments, galaxy evolution, galaxy surveys, POINT SOURCES, [ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph], Cosmic microwave background, galaxy evolution, Astrophysics, CMB, 01 natural sciences, Physics, Particles & Fields, law.invention, law, CMBR experiments, galaxy surveys, 010303 astronomy & astrophysics, QC, QB, Physics, COSMIC cancer database, Nuclear & Particles Physics, PLANCK, COMPACT SOURCE CATALOG, ALL-SKY SURVEY, Physical Sciences, astro-ph.CO, symbols, GALAXY FORMATION, CMBR experiment, Astrophysics - Cosmology and Nongalactic Astrophysics, RADIO-SOURCES, Cosmology and Nongalactic Astrophysics (astro-ph.CO), galaxy survey, astro-ph.GA, FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, Astronomy & Astrophysics, NO, Telescope, symbols.namesake, FIS/05 - ASTRONOMIA E ASTROFISICA, 0202 Atomic, Molecular, Nuclear, Particle And Plasma Physics, Settore FIS/05 - Astronomia e Astrofisica, active galactic nuclei, Astronomy and Astrophysics, 0103 physical sciences, Planck, Astrophysics::Galaxy Astrophysics, HERSCHEL, Science & Technology, 010308 nuclear & particles physics, Star formation, HERSCHEL-ATLAS, 115 Astronomy, Space science, Astrophysics - Astrophysics of Galaxies, Galaxy, Redshift, EVOLUTION, 0201 Astronomical And Space Sciences, LUMINOSITY FUNCTION, Astrophysics of Galaxies (astro-ph.GA), SKY, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract

Work supported in part by ASI/INAF agreement n. 2014-024-R.1 and by PRIN–INAF 2014 “Probing the AGN/galaxy co-evolution through ultra-deep and ultra-high resolution radio surveys”. JGN acknowledges financial support from the Spanish MINECO for a “Ramon y Cajal” fellowship (RYC-2013-13256) and the I+D 2015 project AYA2015-65887-P (MINECO/FEDER). CH-M acknowledges the financial support of the Spanish MINECO through I+D project AYA-2015-66211-C2-2-P. MB is supported by the Netherlands Organization for Scientific Research, NWO, through grant number 614.001.451, and by the Polish National Science Centre under contract UMO-2012/07/D/ST9/02785. CJM is supported by an FCT Research Professorship, contract reference IF/00064/2012, funded by FCT/MCTES (Portugal) and POPH/FSE (EC). GR acknowledges support from the National Research Foundation of Korea (NRF) through NRF-SGER 2014055950 funded by the Korean Ministry of Education, Science and Technology (MoEST), and from the faculty research fund of Sejong University in 2016., Zotti, G.D., González-Nuevo, J., Lopez-Caniego, M., Negrello, M., Greenslade, J., Hernández-Monteagudo, C., Delabrouille, J., Cai, Z.-Y., Bonato, M., Achúcarro, A., Ade, P., Allison, R., Ashdown, M., Ballardini, M., Banday, A.J., Banerji, R., Bartlett, J.G., Bartolo, N., Basak, S., Bersanelli, M., Biesiada, M., Bilicki, M., Bonaldi, A., Bonavera, L., Borrill, J., Bouchet, F., Boulanger, F., Brinckmann, T., Bucher, M., Burigana, C., Buzzelli, A., Calvo, M., Carvalho, C.S., Castellano, M.G., Challinor, A., Chluba, J., Clements, D.L., Clesse, S., Colafrancesco, S., Colantoni, I., Coppolecchia, A., Crook, M., D'Alessandro, G., De Bernardis, P., De Gasperis, G., Diego, J.M., Valentino, E.D., Errard, J., Feeney, S.M., Fernández-Cobos, R., Ferraro, S., Finelli, F., Forastieri, F., Galli, S., Génova-Santos, R.T., Gerbino, M., Grandis, S., Hagstotz, S., Hanany, S., Handley, W., Hervias-Caimapo, C., Hills, M., Hivon, E., Kiiveri, K., Kisner, T., Kitching, T., Kunz, M., Kurki-Suonio, H., Lagache, G., Lamagna, L., Lasenby, A., Lattanzi, M., Brun, A.L., Lesgourgues, J., Lewis, A., Liguori, M., Lindholm, V., Luzzi, G., Maffei, B., Mandolesi, N., Martinez-Gonzalez, E., Martins, C.J.A.P., Masi, S., Massardi, M., Matarrese, S., McCarthy, D., Melchiorri, A., Melin, J.-B., Molinari, D., Monfardini, A., Natoli, P., Notari, A., Paiella, A., Paoletti, D., Partridge, R.B., Patanchon, G., Piat, M., Pisano, G., Polastri, L., Polenta, G., Pollo, A., Poulin, V., Quartin, M., Remazeilles, M., Roman, M., Rossi, G., Roukema, B.F., Rubiño-Martín, J.-A., Salvati, L., Scott, D., Serjeant, S., Tartari, A., Toffolatti, L., Tomasi, M., Trappe, N., Triqueneaux, S., Trombetti, T., Tucci, M., Tucker, C., Väliviita, J., De Weygaert, R.V., Tent, B.V., Vennin, V., Vielva, P., Vittorio, N., Young, K., Zannoni, M.

Published
2016
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230. Exploring cosmic origins with CORE : Extragalactic sources in cosmic microwave background maps

Author

De Zotti, G., Gonzalez-Nuevo, J., Lopez-Caniego, M., Negrello, M., Greenslade, J., Hernandez-Monteagudo, C., Delabrouille, J., Cai, Z-Y., Bonato, M., Achucarro, A., Ade, P., Allison, R., Ashdown, M., Ballardini, M., Banday, A. J., Banerji, R., Bartlett, J. G., Bartolo, N., Basak, S., Bersanelli, M., Biesiada, M., Bilicki, M., Bonaldi, A., Bonavera, L., Borrill, J., Bouchet, F., Boulanger, F., Brinckmann, T., Bucher, M., Burigana, C., Buzzelli, A., Calvo, M., Carvalho, C. S., Castellano, M. G., Challinor, A., Chluba, J., Clements, D. L., Clesse, S., Colafrancesco, S., Colantoni, I., Coppolecchia, A., Crook, M., D'Alessandro, G., de Bernardis, P., de Gasperis, G., Diego, J. M., Di Valentino, E., Errard, J., Feeney, S. M., Fernandez-Cobos, R., Ferraro, S., Finelli, F., Forastieri, F., Galli, S., Genova-Santos, R. T., Gerbino, Martina, Grandis, S., Hagstotz, S., Hanany, S., Handley, W., Hervias-Caimapo, C., Hills, M., Hivon, E., Kiiveri, K., Kisner, T., Kitching, T., Kunz, M., Kurki-Suonio, H., Lagache, G., Lamagna, L., Lasenby, A., Lattanzi, M., Le Brun, A., Lesgourgues, J., Lewis, A., Liguori, M., Lindholm, V., Luzzi, G., Maffei, B., Mandolesi, N., Martinez-Gonzalez, E., Martins, C. J. A. P., Masi, S., Massardi, M., Matarrese, S., McCarthy, D., Melchiorri, A., Melin, J-B., Molinari, D., Monfardini, A., Natoli, P., Notari, A., Paiella, A., Paoletti, D., Partridge, R. B., Patanchon, G., Piat, M., Pisano, G., Polastri, L., Polenta, G., Pollo, A., Poulin, V., Quartin, M., Remazeilles, M., Roman, M., Rossi, G., Roukema, B. F., Rubino-Martin, J-A., Salvati, L., Scott, D., Serjeant, S., Tartari, A., Toffolatti, L., Tomasi, M., Trappe, N., Triqueneaux, S., Trombetti, T., Tucci, M., Tucker, C., Valiviita, J., van de Weygaert, R., Van Tent, B., Vennin, V., Vielva, P., Vittorio, N., Young, K., Zannoni, M., De Zotti, G., Gonzalez-Nuevo, J., Lopez-Caniego, M., Negrello, M., Greenslade, J., Hernandez-Monteagudo, C., Delabrouille, J., Cai, Z-Y., Bonato, M., Achucarro, A., Ade, P., Allison, R., Ashdown, M., Ballardini, M., Banday, A. J., Banerji, R., Bartlett, J. G., Bartolo, N., Basak, S., Bersanelli, M., Biesiada, M., Bilicki, M., Bonaldi, A., Bonavera, L., Borrill, J., Bouchet, F., Boulanger, F., Brinckmann, T., Bucher, M., Burigana, C., Buzzelli, A., Calvo, M., Carvalho, C. S., Castellano, M. G., Challinor, A., Chluba, J., Clements, D. L., Clesse, S., Colafrancesco, S., Colantoni, I., Coppolecchia, A., Crook, M., D'Alessandro, G., de Bernardis, P., de Gasperis, G., Diego, J. M., Di Valentino, E., Errard, J., Feeney, S. M., Fernandez-Cobos, R., Ferraro, S., Finelli, F., Forastieri, F., Galli, S., Genova-Santos, R. T., Gerbino, Martina, Grandis, S., Hagstotz, S., Hanany, S., Handley, W., Hervias-Caimapo, C., Hills, M., Hivon, E., Kiiveri, K., Kisner, T., Kitching, T., Kunz, M., Kurki-Suonio, H., Lagache, G., Lamagna, L., Lasenby, A., Lattanzi, M., Le Brun, A., Lesgourgues, J., Lewis, A., Liguori, M., Lindholm, V., Luzzi, G., Maffei, B., Mandolesi, N., Martinez-Gonzalez, E., Martins, C. J. A. P., Masi, S., Massardi, M., Matarrese, S., McCarthy, D., Melchiorri, A., Melin, J-B., Molinari, D., Monfardini, A., Natoli, P., Notari, A., Paiella, A., Paoletti, D., Partridge, R. B., Patanchon, G., Piat, M., Pisano, G., Polastri, L., Polenta, G., Pollo, A., Poulin, V., Quartin, M., Remazeilles, M., Roman, M., Rossi, G., Roukema, B. F., Rubino-Martin, J-A., Salvati, L., Scott, D., Serjeant, S., Tartari, A., Toffolatti, L., Tomasi, M., Trappe, N., Triqueneaux, S., Trombetti, T., Tucci, M., Tucker, C., Valiviita, J., van de Weygaert, R., Van Tent, B., Vennin, V., Vielva, P., Vittorio, N., Young, K., and Zannoni, M.

Abstract

We discuss the potential of a next generation space-borne Cosmic Microwave Background (CMB) experiment for studies of extragalactic sources. Our analysis has particular bearing on the definition of the future space project, CORE, that has been submitted in response to ESA's call for a Medium-size mission opportunity as the successor of the Planck satellite. Even though the effective telescope size will be somewhat smaller than that of Planck, CORE will have a considerably better angular resolution at its highest frequencies, since, in contrast with Planck, it will be diffraction limited at all frequencies. The improved resolution implies a considerable decrease of the source confusion, i.e. substantially fainter detection limits. In particular, CORE will detect thousands of strongly lensed high-z galaxies distributed over the full sky. The extreme brightness of these galaxies will make it possible to study them, via follow-up observations, in extraordinary detail. Also, the CORE resolution matches the typical sizes of high-z galaxy proto-clusters much better than the Planck resolution, resulting in a much higher detection efficiency; these objects will be caught in an evolutionary phase beyond the reach of surveys in other wavebands. Furthermore, CORE will provide unique information on the evolution of the star formation in virialized groups and clusters of galaxies up to the highest possible redshifts. Finally, thanks to its very high sensitivity, CORE will detect the polarized emission of thousands of radio sources and, for the first time, of dusty galaxies, at mm and sub-mm wavelengths, respectively.

Published
2018
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231. Exploring cosmic origins with CORE : Survey requirements and mission design

Author

Delabrouille, J., de Bernardis, P., Bouchet, F. R., Achucarro, A., Ade, P. A. R., Allison, R., Arroja, F., Artal, E., Ashdown, M., Baccigalupi, C., Ballardini, M., Banday, A. J., Banerji, R., Barbosa, D., Bartlett, J., Bartolo, N., Basak, S., Baselmans, J. J. A., Basu, K., Battistelli, E. S., Battye, R., Baumann, D., Benoit, A., Bersanelli, M., Bideaud, A., Biesiada, M., Bilicki, M., Bonaldi, A., Bonato, M., Borrill, J., Boulanger, F., Brinckmann, T., Brown, M. L., Bucher, M., Burigana, C., Buzzelli, A., Cabass, G., Cai, Z. -Y., Calvo, M., Caputo, A., Carvalho, C. -S., Casas, F. J., Castellano, G., Catalano, A., Challinor, A., Charles, I., Chluba, J., Clements, D. L., Clesse, S., Colafrancesco, S., Colantoni, I., Contreras, D., Coppolecchia, A., Crook, M., D'Alessandro, G., D'Amico, G., da Silva, A., de Avillez, M., de Gasperis, G., De Petris, M., de Zotti, G., Danese, L., Desert, F. -X., Desjacques, V., Di Valentino, E., Dickinson, C., Diego, J. M., Doyle, S., Durrer, R., Dvorkin, C., Eriksen, H. K., Errard, J., Feeney, S., Fernandez-Cobos, R., FineIli, F., Forastieri, F., Franceschet, C., Fuskeland, U., Galli, S., Genova-Santos, R. T., Gerbino, Martina, Giusarma, E., Gomez, A., Gonzalez-Nuevo, J., Grandis, S., Greenslade, J., Goupy, J., Hagstotz, S., Hanany, S., Handley, W., Henrot-Versille, S., Hernandez-Monteagudo, C., Hervias-Caimapo, C., Hills, M., Hindmarsh, M., Hivon, E., Hoang, D. T., Hooper, D. C., Hu, B., Keihanen, E., Keskitalo, R., Kiiveri, K., Kisner, T., Kitching, T., Kunz, M., Kurki-Suonio, H., Lagache, G., Lamagna, L., Lapi, A., Lasenby, A., Lattanzi, M., Le Brun, A. M. C., Lesgourgues, J., Liguori, M., Lindholm, V., Lizarraga, J., Luzzi, G., Macias-Perez, J. F., Maffei, B., Mandolesi, N., Martin, S., Martinez-Gonzalez, E., Martins, C. J. A. P., Masi, S., Massardi, M., Matarrese, S., Mazzotta, P., McCarthy, D., Melchiorri, A., Melin, J. -B., Mennella, A., Mohr, J., Molinari, D., Monfardini, A., Montier, L., Natoli, P., Negrello, M., Notari, A., Noviello, F., Oppizzi, F., O'Sullivan, C., Pagano, L., Paiella, A., Pajer, E., Paoletti, D., Paradiso, S., Partridge, R. B., Patanchon, G., Patil, S. P., Perdereau, O., Piacentini, F., Piat, M., Pisano, G., Polastri, L., Polenta, G., Pollo, A., Ponthieu, N., Poulin, V., Prele, D., Quartin, M., Ravenni, A., Remazeilles, M., Renzi, A., Ringeval, C., Roest, D., Roman, M., Roukema, B. F., Rubino-Martin, J. -A., Salvati, L., Scott, D., Serjeant, S., Signorelli, G., Starobinsky, A. A., Sunyaev, R., Tan, C. Y., Tartari, A., Tasinato, G., Toffolatti, L., Tomasi, M., Torrado, J., Tramonte, D., Trappe, N., Triqueneaux, S., Tristram, M., Trombetti, T., Tucci, M., Tucker, C., Urrestilla, J., Valiviita, J., Van de Weygaert, R., Van Tent, B., Vennin, V., Verde, L., Vermeulen, G., Vielva, P., Vittorio, N., Voisin, F., Wallis, C., Wandelt, B., Wehus, I. K., Weller, J., Young, K., Zannoni, M., Delabrouille, J., de Bernardis, P., Bouchet, F. R., Achucarro, A., Ade, P. A. R., Allison, R., Arroja, F., Artal, E., Ashdown, M., Baccigalupi, C., Ballardini, M., Banday, A. J., Banerji, R., Barbosa, D., Bartlett, J., Bartolo, N., Basak, S., Baselmans, J. J. A., Basu, K., Battistelli, E. S., Battye, R., Baumann, D., Benoit, A., Bersanelli, M., Bideaud, A., Biesiada, M., Bilicki, M., Bonaldi, A., Bonato, M., Borrill, J., Boulanger, F., Brinckmann, T., Brown, M. L., Bucher, M., Burigana, C., Buzzelli, A., Cabass, G., Cai, Z. -Y., Calvo, M., Caputo, A., Carvalho, C. -S., Casas, F. J., Castellano, G., Catalano, A., Challinor, A., Charles, I., Chluba, J., Clements, D. L., Clesse, S., Colafrancesco, S., Colantoni, I., Contreras, D., Coppolecchia, A., Crook, M., D'Alessandro, G., D'Amico, G., da Silva, A., de Avillez, M., de Gasperis, G., De Petris, M., de Zotti, G., Danese, L., Desert, F. -X., Desjacques, V., Di Valentino, E., Dickinson, C., Diego, J. M., Doyle, S., Durrer, R., Dvorkin, C., Eriksen, H. K., Errard, J., Feeney, S., Fernandez-Cobos, R., FineIli, F., Forastieri, F., Franceschet, C., Fuskeland, U., Galli, S., Genova-Santos, R. T., Gerbino, Martina, Giusarma, E., Gomez, A., Gonzalez-Nuevo, J., Grandis, S., Greenslade, J., Goupy, J., Hagstotz, S., Hanany, S., Handley, W., Henrot-Versille, S., Hernandez-Monteagudo, C., Hervias-Caimapo, C., Hills, M., Hindmarsh, M., Hivon, E., Hoang, D. T., Hooper, D. C., Hu, B., Keihanen, E., Keskitalo, R., Kiiveri, K., Kisner, T., Kitching, T., Kunz, M., Kurki-Suonio, H., Lagache, G., Lamagna, L., Lapi, A., Lasenby, A., Lattanzi, M., Le Brun, A. M. C., Lesgourgues, J., Liguori, M., Lindholm, V., Lizarraga, J., Luzzi, G., Macias-Perez, J. F., Maffei, B., Mandolesi, N., Martin, S., Martinez-Gonzalez, E., Martins, C. J. A. P., Masi, S., Massardi, M., Matarrese, S., Mazzotta, P., McCarthy, D., Melchiorri, A., Melin, J. -B., Mennella, A., Mohr, J., Molinari, D., Monfardini, A., Montier, L., Natoli, P., Negrello, M., Notari, A., Noviello, F., Oppizzi, F., O'Sullivan, C., Pagano, L., Paiella, A., Pajer, E., Paoletti, D., Paradiso, S., Partridge, R. B., Patanchon, G., Patil, S. P., Perdereau, O., Piacentini, F., Piat, M., Pisano, G., Polastri, L., Polenta, G., Pollo, A., Ponthieu, N., Poulin, V., Prele, D., Quartin, M., Ravenni, A., Remazeilles, M., Renzi, A., Ringeval, C., Roest, D., Roman, M., Roukema, B. F., Rubino-Martin, J. -A., Salvati, L., Scott, D., Serjeant, S., Signorelli, G., Starobinsky, A. A., Sunyaev, R., Tan, C. Y., Tartari, A., Tasinato, G., Toffolatti, L., Tomasi, M., Torrado, J., Tramonte, D., Trappe, N., Triqueneaux, S., Tristram, M., Trombetti, T., Tucci, M., Tucker, C., Urrestilla, J., Valiviita, J., Van de Weygaert, R., Van Tent, B., Vennin, V., Verde, L., Vermeulen, G., Vielva, P., Vittorio, N., Voisin, F., Wallis, C., Wandelt, B., Wehus, I. K., Weller, J., Young, K., and Zannoni, M.

Abstract

Future observations of cosmic microwave background (CMB) polarisation have the potential to answer some of the most fundamental questions of modern physics and cosmology, including: what physical process gave birth to the Universe we see today? What are the dark matter and dark energy that seem to constitute 95% of the energy density of the Universe? Do we need extensions to the standard model of particle physics and fundamental interactions? Is the ACDM cosmological scenario correct, or are we missing an essential piece of the puzzle? In this paper, we list the requirements for a future CMB polarisation survey addressing these scientific objectives, and discuss the design drivers of the CORE space mission proposed to ESA in answer to the M5 call for a medium-sized mission. The rationale and options, and the methodologies used to assess the mission's performance, are of interest to other future CMB mission design studies. CORE has 19 frequency channels, distributed over a broad frequency range, spanning the 60-600 GHz interval, to control astrophysical foreground emission. The angular resolution ranges from 2' to 18', and the aggregate CMB sensitivity is about 2 mu K.arcmin. The observations are made with a single integrated focal-plane instrument, consisting of an array of 2100 cryogenically-cooled, linearly-polarised detectors at the focus of a 1.2-m aperture cross-Dragone telescope. The mission is designed to minimise all sources of systematic effects, which must be controlled so that no more than 10(-4) of the intensity leaks into polarisation maps, and no more than about 1% of E-type polarisation leaks into B-type modes. CORE observes the sky from a large Lissajous orbit around the Sun-Earth L2 point on an orbit that offers stable observing conditions and avoids contamination from sidelobe pick-up of stray radiation originating from the Sun, Earth, and Moon. The entire sky is observed repeatedly during four years of continuous scanning, with a combination of th

Published
2018
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232. Galaxy Evolution Studies with the SPace IR Telescope for Cosmology and Astrophysics (SPICA): The Power of IR Spectroscopy

Author

Spinoglio, L., Alonso-Herrero, A., Armus, L., Baes, M., Bernard-Salas, J., Bianchi, S., Bocchio, M., Bolatto, A., Bradford, C., Braine, J., Carrera, F. J., Ciesla, L., Clements, D. L., Dannerbauer, H., Doi, Yasuo, Efstathiou, A., Egami, E., Fernandez-Ontiveros, J. A., Ferrara, A., Fischer, J., Franceschini, A., Gallerani, S., Giard, M., Gonzalez-Alfonso, E., Gruppioni, C., Guillard, P., Hatziminaoglou, E., Imanishi, M., Ishihara, Daisuke, Isobe, Naoki, Kaneda, Hidehiro, Kawada, Mitsunobu, Kohno, Kotaro, Kwon, Jungmi, Madden, S., Malkan, M. A., Marassi, S., Matsuhara, Hideo, Matsuura, M., Miniutti, G., Nagamine, K., Nagao, T., Najarro, F., Nakagawa, Takao, Onaka, Takashi, Oyabu, Shinki, Pallottini, A., Piro, L., Pozzi, F., Rodighiero, G., Roelfsema, P., Sakon, Itsuki, Santini, P., Schaerer, D., Schneider, R., Scott, D., Serjeant, S., Shibai, Hiroshi, Smith, J. -D. T., Sobacchi, E., Sturm, E., Suzuki, T., Vallini, L., van der Tak, F., Vignali, C., Yamada, Toru, Wada, Takehiko, Wang, L., 土井, 靖生, 石原, 大輔, 磯部, 直樹, 金田, 英宏, 川田, 光伸, 權, 靜美, 松原, 英雄, 中川, 貴雄, 尾中, 敬, 大薮, 進喜, 左近, 樹, 芝井, 広, 山田, 亨, 和田, 武彦, Spinoglio, L., Alonso-Herrero, A., Armus, L., Baes, M., Bernard-Salas, J., Bianchi, S., Bocchio, M., Bolatto, A., Bradford, C., Braine, J., Carrera, F. J., Ciesla, L., Clements, D. L., Dannerbauer, H., Doi, Yasuo, Efstathiou, A., Egami, E., Fernandez-Ontiveros, J. A., Ferrara, A., Fischer, J., Franceschini, A., Gallerani, S., Giard, M., Gonzalez-Alfonso, E., Gruppioni, C., Guillard, P., Hatziminaoglou, E., Imanishi, M., Ishihara, Daisuke, Isobe, Naoki, Kaneda, Hidehiro, Kawada, Mitsunobu, Kohno, Kotaro, Kwon, Jungmi, Madden, S., Malkan, M. A., Marassi, S., Matsuhara, Hideo, Matsuura, M., Miniutti, G., Nagamine, K., Nagao, T., Najarro, F., Nakagawa, Takao, Onaka, Takashi, Oyabu, Shinki, Pallottini, A., Piro, L., Pozzi, F., Rodighiero, G., Roelfsema, P., Sakon, Itsuki, Santini, P., Schaerer, D., Schneider, R., Scott, D., Serjeant, S., Shibai, Hiroshi, Smith, J. -D. T., Sobacchi, E., Sturm, E., Suzuki, T., Vallini, L., van der Tak, F., Vignali, C., Yamada, Toru, Wada, Takehiko, Wang, L., 土井, 靖生, 石原, 大輔, 磯部, 直樹, 金田, 英宏, 川田, 光伸, 權, 靜美, 松原, 英雄, 中川, 貴雄, 尾中, 敬, 大薮, 進喜, 左近, 樹, 芝井, 広, 山田, 亨, and 和田, 武彦

Abstract

著者人数: 68名

Published
2018

234. GravityCam:Wide-filed high-resolution high-cadence imaging surveys in the visible form the ground

Author

Mackay, C., Dominik, M., Steele, I. A., Snodgrass, C., Jorgensen, U. G., Skottfelt, J., Stefanov, K., Carry, B., Braga-Ribas, F., Doressoundiram, A., Ivanov, V. D., Gandhi, P., Evans, D. F., Hundertmark, M., Serjeant, S., Ortolani, S., Mackay, C., Dominik, M., Steele, I. A., Snodgrass, C., Jorgensen, U. G., Skottfelt, J., Stefanov, K., Carry, B., Braga-Ribas, F., Doressoundiram, A., Ivanov, V. D., Gandhi, P., Evans, D. F., Hundertmark, M., Serjeant, S., and Ortolani, S.

Published
2018

235. AKARI mid-infrared slitless spectroscopic survey of star-forming galaxies at z less than or similar to 0.5

Author

Ohyama, Y., Wada, T., Matsuhara, H., Takagi, T., Malkan, M., Goto, T., Egami, E., Lee, H. -M., Im, M., Kim, J. H., Pearson, C., Inami, H., Oyabu, S., Usui, F., Burgarella, D., Mazyed, F., Imanishi, M., Jeong, W. -S., Miyaji, T., Diaz Tello, J., Nakagawa, T., Serjeant, S., Takeuchi, T. T., Toba, Y., White, G. J., Hanami, H., Ishigaki, T., Ohyama, Y., Wada, T., Matsuhara, H., Takagi, T., Malkan, M., Goto, T., Egami, E., Lee, H. -M., Im, M., Kim, J. H., Pearson, C., Inami, H., Oyabu, S., Usui, F., Burgarella, D., Mazyed, F., Imanishi, M., Jeong, W. -S., Miyaji, T., Diaz Tello, J., Nakagawa, T., Serjeant, S., Takeuchi, T. T., Toba, Y., White, G. J., Hanami, H., and Ishigaki, T.

Published
2018

236. PROPERTIES OF DUST OBSCURED GALAXIES IN THE NEP-DEEP FIELD

Author

Matsuhara, H., Wada, T., Oi, N., Takagi, T., Nakagawa, T., Murata, K., Goto, T., Oyabu, S., Takeuchi, T.T., Malek, K., Solarz, A., Ohyama, Y., Miyaji, T., Krumpe, M., Lee, H.M., Im, M., Serjeant, S., Pearson, C.P., White, G.J., Malkan, M.A., Hanami, H., Ishigaki, T., Burgarella, D., Buat, V., Pollo, A., Laboratoire d'Astrophysique de Marseille (LAM), and Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)

Subjects
Luminous infrared galaxy, Physics, Hubble Deep Field, Astronomy, General Medicine, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Galaxy, ComputingMilieux_MISCELLANEOUS
Abstract

International audience

Published
2017

237. The Herschel-ATLAS: a sample of 500?m-selected lensed galaxies over 600 deg2

Author

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

Subjects
Gravitational lensing, Galaxies high-redshift, Submillimetre, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics::Galaxy Astrophysics
Abstract

We present a sample of 80 candidate strongly lensed galaxies with flux density above 100 mJy at 500 μm extracted from the Herschel Astrophysical Terahertz Large Area Survey, over an area of 600 deg2. Available imaging and spectroscopic data allow us to confirm the strong lensing in 20 cases and to reject it in one case. For other eight objects, the lensing scenario is strongly supported by the presence of two sources along the same line of sight with distinct photometric redshifts. The remaining objects await more follow-up observations to confirm their nature. The lenses and the background sources have median redshifts zL = 0.6 and zS = 2.5, respectively, and are observed out to zL = 1.2 and zS = 4.2. We measure the number counts of candidate lensed galaxies at 500 μm and compare them with theoretical predictions, finding a good agreement for a maximum magnification of the background sources in the range 10–20. These values are consistent with the magnification factors derived from the lens modelling of individual systems. The catalogue presented here provides sub-mm bright targets for follow-up observations aimed at exploiting gravitational lensing, to study with unprecedented details the morphological and dynamical properties of dusty star-forming regions in z ≳ 1.5 galaxies.

Published
2017

238. The SCUBA-2 Cosmology Legacy Survey: 850 ?m maps, catalogues and number counts

Author

Geach, J. E., Dunlop, J. S., Halpern, M., Smail, Ian, van der Werf, P., Alexander, D. M., Almaini, O., Aretxaga, I., Arumugam, V., Asboth, V., Banerji, M., Beanlands, J., Best, P. N., Blain, A. W., Birkinshaw, M., Chapin, E. L., Chapman, S. C., Chen, C-C., Chrysostomou, A., Clarke, C., Clements, D. L., Conselice, C., Coppin, K. E. K., Cowley, W. I., Danielson, A. L. R., Eales, S., Edge, A. C., Farrah, D., Gibb, A., Harrison, C. M., Hine, N. K., Hughes, D., Ivison, R. J., Jarvis, M., Jenness, T., Jones, S. F., Karim, A., Koprowski, M., Knudsen, K. K., Lacey, C. G., Mackenzie, T., Marsden, G., McAlpine, K., McMahon, R., Meijerink, R., Micha?owski, M. J., Oliver, S. J., Page, M. J., Peacock, J. A., Rigopoulou, D., Robson, E. I., Roseboom, I., Rotermund, K., Scott, Douglas, Sarjeant, S., Simpson, C., Simpson, J. M., Smith, D. J. B., Spaans, M., Stanley, F., Stevens, J. A., Swinbank, A. M., Targett, T., Thomson, A. P., Valiante, E., Wake, D. A., Webb, T. M. A., Willott, C., Zavala, J. A., Zemcov, M., and Serjeant, S.

Subjects
surveys, galaxies: high-redshift, galaxies: evolution, cosmology: observations, catalogues
Abstract

We present a catalogue of ∼3000 submillimetre sources detected (≥3.5σ) at 850 μm over ∼5 deg2 surveyed as part of the James Clerk Maxwell Telescope (JCMT) SCUBA-2 Cosmology Legacy Survey (S2CLS). This is the largest survey of its kind at 850 μm, increasing the sample size of 850 μm selected submillimetre galaxies by an order of magnitude. The wide 850 μm survey component of S2CLS covers the extragalactic fields: UKIDSS-UDS, COSMOS, Akari-NEP, Extended Groth Strip, Lockman Hole North, SSA22 and GOODS-North. The average 1σ depth of S2CLS is 1.2 mJy beam−1, approaching the SCUBA-2 850 μm confusion limit, which we determine to be σc ≈ 0.8 mJy beam−1.We measure the 850 μm number counts, reducing the Poisson errors on the differential counts to approximately 4 per cent at S850 ≈ 3 mJy. With several independent fields, we investigate field-to-field variance, finding that the number counts on 0.5◦–1◦ scales are generally within 50 per cent of the S2CLS mean for S850 > 3 mJy, with scatter consistent with the Poisson and estimated cosmic variance uncertainties, although there is a marginal (2σ) density enhancement in GOODS-North. The observed counts are in reasonable agreement with recent phenomenological and semi-analytic models, although determining the shape of the faint-end slope (S850 < 3 mJy) remains a key test. The large solid angle of S2CLS allows us to measure the bright-end counts: at S850 >10 mJy there are approximately 10 sources per square degree, and we detect the distinctive up-turn in the number counts indicative of the detection of local sources of 850 μm emission, and strongly lensed high-redshift galaxies. All calibrated maps and the catalogue are made publicly available.

Published
2017

239. AKARI mid-infrared slitless spectroscopic survey of star-forming galaxies at z ≲ 0.5

Author

Ohyama, Y., primary, Wada, T., additional, Matsuhara, H., additional, Takagi, T., additional, Malkan, M., additional, Goto, T., additional, Egami, E., additional, Lee, H.-M., additional, Im, M., additional, Kim, J.H., additional, Pearson, C., additional, Inami, H., additional, Oyabu, S., additional, Usui, F., additional, Burgarella, D., additional, Mazyed, F., additional, Imanishi, M., additional, Jeong, W.-S., additional, Miyaji, T., additional, Díaz Tello, J., additional, Nakagawa, T., additional, Serjeant, S., additional, Takeuchi, T. T., additional, Toba, Y., additional, White, G. J., additional, Hanami, H., additional, and Ishigaki, T., additional

Published
2018
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240. Ultra-red Galaxies Signpost Candidate Protoclusters at High Redshift

Author

Lewis, A. J. R., primary, Ivison, R. J., additional, Best, P. N., additional, Simpson, J. M., additional, Weiss, A., additional, Oteo, I., additional, Zhang, Z-Y., additional, Arumugam, V., additional, Bremer, M. N., additional, Chapman, S. C., additional, Clements, D. L., additional, Dannerbauer, H., additional, Dunne, L., additional, Eales, S., additional, Maddox, S., additional, Oliver, S. J., additional, Omont, A., additional, Riechers, D. A., additional, Serjeant, S., additional, Valiante, E., additional, Wardlow, J., additional, Werf, P. van der, additional, and Zotti, G. De, additional

Published
2018
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241. TheSpitzer-IRAC/MIPS Extragalactic Survey (SIMES). II. Enhanced Nuclear Accretion Rate in Galaxy Groups atz∼ 0.2

Author

Baronchelli, I., primary, Rodighiero, G., additional, Teplitz, H. I., additional, Scarlata, C. M., additional, Franceschini, A., additional, Berta, S., additional, Barrufet, L., additional, Vaccari, M., additional, Bonato, M., additional, Ciesla, L., additional, Zanella, A., additional, Carraro, R., additional, Mancini, C., additional, Puglisi, A., additional, Malkan, M., additional, Mei, S., additional, Marchetti, L., additional, Colbert, J., additional, Sedgwick, C., additional, Serjeant, S., additional, Pearson, C., additional, Radovich, M., additional, Grado, A., additional, Limatola, L., additional, and Covone, G., additional

Published
2018
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242. Exploring cosmic origins with CORE: Extragalactic sources in cosmic microwave background maps

Author

Zotti, G. De, primary, González-Nuevo, J., additional, Lopez-Caniego, M., additional, Negrello, M., additional, Greenslade, J., additional, Hernández-Monteagudo, C., additional, Delabrouille, J., additional, Cai, Z.-Y., additional, Bonato, M., additional, Achúcarro, A., additional, Ade, P., additional, Allison, R., additional, Ashdown, M., additional, Ballardini, M., additional, Banday, A.J., additional, Banerji, R., additional, Bartlett, J.G., additional, Bartolo, N., additional, Basak, S., additional, Bersanelli, M., additional, Biesiada, M., additional, Bilicki, M., additional, Bonaldi, A., additional, Bonavera, L., additional, Borrill, J., additional, Bouchet, F., additional, Boulanger, F., additional, Brinckmann, T., additional, Bucher, M., additional, Burigana, C., additional, Buzzelli, A., additional, Calvo, M., additional, Carvalho, C.S., additional, Castellano, M.G., additional, Challinor, A., additional, Chluba, J., additional, Clements, D.L., additional, Clesse, S., additional, Colafrancesco, S., additional, Colantoni, I., additional, Coppolecchia, A., additional, Crook, M., additional, D'Alessandro, G., additional, de Bernardis, P., additional, de Gasperis, G., additional, Diego, J.M., additional, Valentino, E. Di, additional, Errard, J., additional, Feeney, S.M., additional, Fernández-Cobos, R., additional, Ferraro, S., additional, Finelli, F., additional, Forastieri, F., additional, Galli, S., additional, Génova-Santos, R.T., additional, Gerbino, M., additional, Grandis, S., additional, Hagstotz, S., additional, Hanany, S., additional, Handley, W., additional, Hervias-Caimapo, C., additional, Hills, M., additional, Hivon, E., additional, Kiiveri, K., additional, Kisner, T., additional, Kitching, T., additional, Kunz, M., additional, Kurki-Suonio, H., additional, Lagache, G., additional, Lamagna, L., additional, Lasenby, A., additional, Lattanzi, M., additional, Brun, A. Le, additional, Lesgourgues, J., additional, Lewis, A., additional, Liguori, M., additional, Lindholm, V., additional, Luzzi, G., additional, Maffei, B., additional, Mandolesi, N., additional, Martinez-Gonzalez, E., additional, Martins, C.J.A.P., additional, Masi, S., additional, Massardi, M., additional, Matarrese, S., additional, McCarthy, D., additional, Melchiorri, A., additional, Melin, J.-B., additional, Molinari, D., additional, Monfardini, A., additional, Natoli, P., additional, Notari, A., additional, Paiella, A., additional, Paoletti, D., additional, Partridge, R.B., additional, Patanchon, G., additional, Piat, M., additional, Pisano, G., additional, Polastri, L., additional, Polenta, G., additional, Pollo, A., additional, Poulin, V., additional, Quartin, M., additional, Remazeilles, M., additional, Roman, M., additional, Rossi, G., additional, Roukema, B.F., additional, Rubiño-Martín, J.-A., additional, Salvati, L., additional, Scott, D., additional, Serjeant, S., additional, Tartari, A., additional, Toffolatti, L., additional, Tomasi, M., additional, Trappe, N., additional, Triqueneaux, S., additional, Trombetti, T., additional, Tucci, M., additional, Tucker, C., additional, Väliviita, J., additional, de Weygaert, R. van, additional, Tent, B. Van, additional, Vennin, V., additional, Vielva, P., additional, Vittorio, N., additional, Young, K., additional, and Zannoni, M., additional

Published
2018
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243. Exploring cosmic origins with CORE: Survey requirements and mission design

Author

Delabrouille, J., primary, de Bernardis, P., additional, Bouchet, F.R., additional, Achúcarro, A., additional, Ade, P. A. R., additional, Allison, R., additional, Arroja, F., additional, Artal, E., additional, Ashdown, M., additional, Baccigalupi, C., additional, Ballardini, M., additional, Banday, A.J., additional, Banerji, R., additional, Barbosa, D., additional, Bartlett, J., additional, Bartolo, N., additional, Basak, S., additional, Baselmans, J.J.A., additional, Basu, K., additional, Battistelli, E. S., additional, Battye, R., additional, Baumann, D., additional, Benoít, A., additional, Bersanelli, M., additional, Bideaud, A., additional, Biesiada, M., additional, Bilicki, M., additional, Bonaldi, A., additional, Bonato, M., additional, Borrill, J., additional, Boulanger, F., additional, Brinckmann, T., additional, Brown, M.L., additional, Bucher, M., additional, Burigana, C., additional, Buzzelli, A., additional, Cabass, G., additional, Cai, Z.-Y., additional, Calvo, M., additional, Caputo, A., additional, Carvalho, C.-S., additional, Casas, F.J., additional, Castellano, G., additional, Catalano, A., additional, Challinor, A., additional, Charles, I., additional, Chluba, J., additional, Clements, D.L., additional, Clesse, S., additional, Colafrancesco, S., additional, Colantoni, I., additional, Contreras, D., additional, Coppolecchia, A., additional, Crook, M., additional, D'Alessandro, G., additional, D'Amico, G., additional, Silva, A. da, additional, de Avillez, M., additional, de Gasperis, G., additional, Petris, M. De, additional, de Zotti, G., additional, Danese, L., additional, Désert, F.-X., additional, Desjacques, V., additional, Valentino, E. Di, additional, Dickinson, C., additional, Diego, J.M., additional, Doyle, S., additional, Durrer, R., additional, Dvorkin, C., additional, Eriksen, H.K., additional, Errard, J., additional, Feeney, S., additional, Fernández-Cobos, R., additional, Finelli, F., additional, Forastieri, F., additional, Franceschet, C., additional, Fuskeland, U., additional, Galli, S., additional, Génova-Santos, R.T., additional, Gerbino, M., additional, Giusarma, E., additional, Gomez, A., additional, González-Nuevo, J., additional, Grandis, S., additional, Greenslade, J., additional, Goupy, J., additional, Hagstotz, S., additional, Hanany, S., additional, Handley, W., additional, Henrot-Versillé, S., additional, Hernández-Monteagudo, C., additional, Hervias-Caimapo, C., additional, Hills, M., additional, Hindmarsh, M., additional, Hivon, E., additional, Hoang, D.T., additional, Hooper, D.C., additional, Hu, B., additional, Keihänen, E., additional, Keskitalo, R., additional, Kiiveri, K., additional, Kisner, T., additional, Kitching, T., additional, Kunz, M., additional, Kurki-Suonio, H., additional, Lagache, G., additional, Lamagna, L., additional, Lapi, A., additional, Lasenby, A., additional, Lattanzi, M., additional, Brun, A.M.C. Le, additional, Lesgourgues, J., additional, Liguori, M., additional, Lindholm, V., additional, Lizarraga, J., additional, Luzzi, G., additional, Macìas-Pérez, J.F., additional, Maffei, B., additional, Mandolesi, N., additional, Martin, S., additional, Martinez-Gonzalez, E., additional, Martins, C.J.A.P., additional, Masi, S., additional, Massardi, M., additional, Matarrese, S., additional, Mazzotta, P., additional, McCarthy, D., additional, Melchiorri, A., additional, Melin, J.-B., additional, Mennella, A., additional, Mohr, J., additional, Molinari, D., additional, Monfardini, A., additional, Montier, L., additional, Natoli, P., additional, Negrello, M., additional, Notari, A., additional, Noviello, F., additional, Oppizzi, F., additional, O'Sullivan, C., additional, Pagano, L., additional, Paiella, A., additional, Pajer, E., additional, Paoletti, D., additional, Paradiso, S., additional, Partridge, R.B., additional, Patanchon, G., additional, Patil, S.P., additional, Perdereau, O., additional, Piacentini, F., additional, Piat, M., additional, Pisano, G., additional, Polastri, L., additional, Polenta, G., additional, Pollo, A., additional, Ponthieu, N., additional, Poulin, V., additional, Prêle, D., additional, Quartin, M., additional, Ravenni, A., additional, Remazeilles, M., additional, Renzi, A., additional, Ringeval, C., additional, Roest, D., additional, Roman, M., additional, Roukema, B.F., additional, Rubiño-Martin, J.-A., additional, Salvati, L., additional, Scott, D., additional, Serjeant, S., additional, Signorelli, G., additional, Starobinsky, A.A., additional, Sunyaev, R., additional, Tan, C.Y., additional, Tartari, A., additional, Tasinato, G., additional, Toffolatti, L., additional, Tomasi, M., additional, Torrado, J., additional, Tramonte, D., additional, Trappe, N., additional, Triqueneaux, S., additional, Tristram, M., additional, Trombetti, T., additional, Tucci, M., additional, Tucker, C., additional, Urrestilla, J., additional, Väliviita, J., additional, de Weygaert, R. Van, additional, Tent, B. Van, additional, Vennin, V., additional, Verde, L., additional, Vermeulen, G., additional, Vielva, P., additional, Vittorio, N., additional, Voisin, F., additional, Wallis, C., additional, Wandelt, B., additional, Wehus, I.K., additional, Weller, J., additional, Young, K., additional, and Zannoni, M., additional

Published
2018
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244. 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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245. Spitzer Observations of the North Ecliptic Pole

Author

Nayyeri, H., primary, Ghotbi, N., additional, Cooray, A., additional, Bock, J., additional, Clements, D. L., additional, Im, M., additional, Kim, M. G., additional, Korngut, P., additional, Lanz, A., additional, Lee, H. M., additional, Lee, D. H., additional, Malkan, M., additional, Matsuhara, H., additional, Matsumoto, T., additional, Matsuura, S., additional, Nam, U. W., additional, Pearson, C., additional, Serjeant, S., additional, Smidt, J., additional, Tsumura, K., additional, Wada, T., additional, and Zemcov, M., additional

Published
2018
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246. 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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247. GravityCam: Wide-field high-resolution high-cadence imaging surveys in the visible from the ground

Author

Mackay, C., primary, Dominik, M., additional, Steele, I. A., additional, Snodgrass, C., additional, Jørgensen, U. G., additional, Skottfelt, J., additional, Stefanov, K., additional, Carry, B., additional, Braga-Ribas, F., additional, Doressoundiram, A., additional, Ivanov, V. D., additional, Gandhi, P., additional, Evans, D. F., additional, Hundertmark, M., additional, Serjeant, S., additional, and Ortolani, S., additional

Published
2018
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248. Probing the high-redshift universe with SPICA: Toward the epoch of reionisation and beyond

Author

Egami, E., primary, Gallerani, S., additional, Schneider, R., additional, Pallottini, A., additional, Vallini, L., additional, Sobacchi, E., additional, Ferrara, A., additional, Bianchi, S., additional, Bocchio, M., additional, Marassi, S., additional, Armus, L., additional, Spinoglio, L., additional, Blain, A. W., additional, Bradford, M., additional, Clements, D. L., additional, Dannerbauer, H., additional, Fernández-Ontiveros, J. A., additional, González-Alfonso, E., additional, Griffin, M. J., additional, Gruppioni, C., additional, Kaneda, H., additional, Kohno, K., additional, Madden, S. C., additional, Matsuhara, H., additional, Najarro, F., additional, Nakagawa, T., additional, Oliver, S., additional, Omukai, K., additional, Onaka, T., additional, Pearson, C., additional, Perez-Fournon, I., additional, Pérez-González, P. G., additional, Schaerer, D., additional, Scott, D., additional, Serjeant, S., additional, Smith, J. D., additional, van der Tak, F. F. S., additional, Wada, T., additional, and Yajima, H., additional

Published
2018
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250. Galaxy Evolution Studies with the &ITSPace IR Telescope for Cosmology and Astrophysics&IT (&ITSPICA&IT) : The Power of IR Spectroscopy

Author

Spinoglio, L., Alonso-Herrero, A., Armus, L., Baes, M., Bernard-Salas, J., Bianchi, S., Bocchio, M., Bolatto, A., Bradford, C., Braine, J., Carrera, F. J., Ciesla, L., Clements, D. L., Dannerbauer, H., Doi, Y., Efstathiou, A., Egami, E., Fernandez-Ontiveros, J. A., Ferrara, A., Fischer, J., Franceschini, A., Gallerani, S., Giard, M., Gonzalez-Alfonso, E., Gruppioni, C., Guillard, P., Hatziminaoglou, E., Imanishi, M., Ishihara, D., Isobe, N., Kaneda, H., Kawada, M., Kohno, K., Kwon, J., Madden, S., Malkan, M. A., Marassi, S., Matsuhara, H., Matsuura, M., Miniutti, G., Nagamine, K., Nagao, T., Najarro, F., Nakagawa, T., Onaka, T., Oyabu, S., Pallottini, A., Piro, L., Pozzi, F., Rodighiero, G., Roelfsema, P., Sakon, I., Santini, P., Schaerer, D., Schneider, R., Scott, D., Serjeant, S., Shibai, H., Smith, J. -DT., Sobacchi, E., Sturm, E., Suzuki, T., Vallini, Livia, van der Tak, F., Vignali, C., Yamada, T., Wada, T., Wang, L., Spinoglio, L., Alonso-Herrero, A., Armus, L., Baes, M., Bernard-Salas, J., Bianchi, S., Bocchio, M., Bolatto, A., Bradford, C., Braine, J., Carrera, F. J., Ciesla, L., Clements, D. L., Dannerbauer, H., Doi, Y., Efstathiou, A., Egami, E., Fernandez-Ontiveros, J. A., Ferrara, A., Fischer, J., Franceschini, A., Gallerani, S., Giard, M., Gonzalez-Alfonso, E., Gruppioni, C., Guillard, P., Hatziminaoglou, E., Imanishi, M., Ishihara, D., Isobe, N., Kaneda, H., Kawada, M., Kohno, K., Kwon, J., Madden, S., Malkan, M. A., Marassi, S., Matsuhara, H., Matsuura, M., Miniutti, G., Nagamine, K., Nagao, T., Najarro, F., Nakagawa, T., Onaka, T., Oyabu, S., Pallottini, A., Piro, L., Pozzi, F., Rodighiero, G., Roelfsema, P., Sakon, I., Santini, P., Schaerer, D., Schneider, R., Scott, D., Serjeant, S., Shibai, H., Smith, J. -DT., Sobacchi, E., Sturm, E., Suzuki, T., Vallini, Livia, van der Tak, F., Vignali, C., Yamada, T., Wada, T., and Wang, L.

Abstract

IR spectroscopy in the range 12-230 mu m with the SPace IR telescope for Cosmology and Astrophysics (SPICA) will reveal the physical processes governing the formation and evolution of galaxies and black holes through cosmic time, bridging the gap between the James Webb Space Telescope and the upcoming Extremely Large Telescopes at shorter wavelengths and the Atacama Large Millimeter Array at longer wavelengths. The SPICA, with its 2.5-m telescope actively cooled to below 8 K, will obtain the first spectroscopic determination, in the mid-IR rest-frame, of both the star-formation rate and black hole accretion rate histories of galaxies, reaching lookback times of 12 Gyr, for large statistically significant samples. Densities, temperatures, radiation fields, and gas-phase metallicities will be measured in dust-obscured galaxies and active galactic nuclei, sampling a large range in mass and luminosity, from faint local dwarf galaxies to luminous quasars in the distant Universe. Active galactic nuclei and starburst feedback and feeding mechanisms in distant galaxies will be uncovered through detailed measurements of molecular and atomic line profiles. The SPICA's large-area deep spectrophotometric surveys will provide mid-IR spectra and continuum fluxes for unbiased samples of tens of thousands of galaxies, out to redshifts of z similar to 6., QC 20200422

Published
2017
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