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54. Perspektiven – Ein zukunftsweisendes 'Health-Systems-Science'-Modul

Author

Krapp, N, Wild, V, and Rotthoff, T

Subjects
ddc: 610, Medicine and health
Abstract

Fragestellung/Zielsetzung: Im kompetenzorientierten Modellstudiengang Humanmedizin der Medizinischen Fakultät Augsburg setzt sich das Modul „Perspektiven“ gemäß der Empfehlungen des Wissenschaftsrates [ref:1] das Ziel einen „integrativen Blick auf die [zum vollständigen Text gelangen Sie über die oben angegebene URL]

Published
2021
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56. The VANDELS ESO public spectroscopic survey

Author

Garilli, B., Mclure, R., Pentericci, L., Franzetti, P., Gargiulo, A., Carnall, A., Cucciati, O., Iovino, A., Amorin, R., Bolzonella, M., Bongiorno, A., Castellano, M., Cimatti, A., Cirasuolo, M., Cullen, F., Dunlop, J., Elbaz, D., Finkelstein, S., Fontana, A., Fontanot, F., Fumana, M., Guaita, L., Hartley, W., Jarvis, M., Juneau, S., Maccagni, D., Mcleod, D., Nandra, K., Pompei, E., Pozzetti, L., Scodeggio, M., Talia, M., Calabrò, A., Cresci, G., Fynbo, J., Hathi, N., Hibon, P., Koekemoer, A., Magliocchetti, M., Salvato, M., Vietri, G., Zamorani, G., Almaini, O., Balestra, I., Bardelli, S., Begley, R., Brammer, G., Bell, E., Bowler, R., Brusa, M., Buitrago, F., Caputi, C., Cassata, P., Charlot, S., Citro, A., Cristiani, S., Curtis-Lake, E., Dickinson, M., Fazio, G., Ferguson, H., Fiore, F., Franco, M., Georgakakis, A., Giavalisco, M., Grazian, A., Hamadouche, M., Jung, I., Kim, S., Khusanova, Y., Le Fèvre, O., Longhetti, M., Lotz, J., Mannucci, F., Maltby, D., Matsuoka, K., Mendez-Hernandez, H., Mendez-Abreu, J., Mignoli, M., Moresco, M., Nonino, M., Pannella, M., Papovich, C., Popesso, P., Roberts-Borsani, G., Rosario, D., Saldana-Lopez, A., Santini, P., Saxena, A., Schaerer, D., Schreiber, C., Stark, D., Tasca, L., Thomas, R., Vanzella, E., Wild, V., Williams, C., Zucca, E., 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), Astrophysique Interprétation Modélisation (AIM (UMR_7158 / 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-Saclay-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), 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]Physics [physics], [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], surveys, cosmology: observations, galaxies: fundamental parameters, Astrophysics::Cosmology and Extragalactic Astrophysics, galaxies: distances and redshifts, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], galaxies: statistics, catalogs, Astrophysics::Galaxy Astrophysics
Abstract

International audience; VANDELS is an ESO Public Spectroscopic Survey designed to build a sample of high-signal-to-noise ratio, medium-resolution spectra of galaxies at redshifts between 1 and 6.5. Here we present the final Public Data Release of the VANDELS Survey, comprising 2087 redshift measurements. We provide a detailed description of sample selection, observations, and data reduction procedures. The final catalogue reaches a target selection completeness of 40% at i AB = 25. The high signal-to-noise ratio of the spectra (above 7 in 80% of the spectra) and the dispersion of 2.5 Å allowed us to measure redshifts with high precision, the redshift measurement success rate reaching almost 100%. Together with the redshift catalogue and the reduced spectra, we also provide optical mid-infrared photometry and physical parameters derived through fitting the spectral energy distribution. The observed galaxy sample comprises both passive and star forming galaxies covering a stellar mass range of 8.3 < Log( M * / M ⊙ ) < 11.7.

Published
2021

57. DRG: Ethik vs. Ökonomie?

Author

Wild, V, Pfister, E, Biller-Andorno, N, and University of Zurich

Subjects
170 Ethics, 10222 Institute of Biomedical Ethics and History of Medicine, 610 Medicine & health, ddc:610, 10001 Center for Ethics
Published
2021

58. The VANDELS ESO public spectroscopic survey:Final data release of 2087 spectra and spectroscopic measurements

Author

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

Abstract

VANDELS is an ESO Public Spectroscopic Survey designed to build a sample of high-signal-to-noise ratio, medium-resolution spectra of galaxies at redshifts between 1 and 6.5. Here we present the final Public Data Release of the VANDELS Survey, comprising 2087 redshift measurements. We provide a detailed description of sample selection, observations, and data reduction procedures. The final catalogue reaches a target selection completeness of 40% at i(AB)=25. The high signal-to-noise ratio of the spectra (above 7 in 80% of the spectra) and the dispersion of 2.5 angstrom allowed us to measure redshifts with high precision, the redshift measurement success rate reaching almost 100%. Together with the redshift catalogue and the reduced spectra, we also provide optical mid-infrared photometry and physical parameters derived through fitting the spectral energy distribution. The observed galaxy sample comprises both passive and star forming galaxies covering a stellar mass range of 8.3

Published
2021

59. MOONS : the new Multi-Object Spectrograph for the VLT

Author

MOONS, Rees, P., Evans, C., Atkinson, D., Tojeiro, R., Wild, V., and University of St Andrews. School of Physics and Astronomy

Subjects
Astrophysics::Instrumentation and Methods for Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics::Earth and Planetary Astrophysics, 3rd-DAS, Astrophysics::Galaxy Astrophysics
Abstract

MOONS is the new Multi-Object Optical and Near-infrared Spectrograph currently under construction for the Very Large Telescope (VLT) at ESO. This remarkable instrument combines, for the first time, the collecting power of an 8-m telescope, 1000 fibres with individual roboticp ositioners, and both low- and high-resolution simultaneous spectral coverage across the 0.64–1.8 μm wavelength range. This facility will provide the astronomical community with a powerful, world-leading instrument able to serve a wide range of Galactic, extragalactic and cosmological studies. Construction is now proceeding full steam ahead and this overview article presents some of the science goals and the technical description of the MOONS instrument. More detailed information on the MOONS surveys is provided in the other dedicated articles in this Messenger issue. Publisher PDF

Published
2020

60. Justice: a key consideration in health policy and systems research ethics

Author

Pratt, B, Wild, V, Barasa, E, Kamuya, D, Gilson, L, Hendl, T, Molyneux, S, Pratt, B, Wild, V, Barasa, E, Kamuya, D, Gilson, L, Hendl, T, and Molyneux, S

Abstract

Health policy and systems research (HPSR) is increasingly being funded and conducted worldwide. There are currently no specific guidelines or criteria for the ethical review and conduct of HPSR. Academic debates on HPSR ethics in the scholarly literature can inform the development of guidelines. Yet there is a deficiency of academic bioethics work relating tojusticein HPSR. This gap is especially problematic for a field like HPSR, which can entail studies that intervene in ways affecting the social and health system delivery structures of society. In this paper, we call for interpreting the principle of justice in a more expansive way in developing and reviewing HPSR studies (relative to biomedical research). The principle requires advancing health equity and social justice at population or systems levels. Drawing on the rich justice literature from political philosophy and public health ethics, we propose a set of essential justice considerations to uphold this principle. These considerations are relevant for research funders, researchers, research ethics committees, policymakers, community organisations and others who are active in the HPSR field.

Published
2020

63. Less than the sum of its parts: the dust-corrected H α luminosity of star-forming galaxies explored at different spatial resolutions with MaNGA and MUSE

Author

Vale Asari, N, primary, Wild, V, additional, de Amorim, A L, additional, Werle, A, additional, Zheng, Y, additional, Kennicutt, R, additional, Johnson, B D, additional, Galametz, M, additional, Pellegrini, E W, additional, Klessen, R S, additional, Reissl, S, additional, Glover, S C O, additional, and Rahner, D, additional

Published
2020
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64. Timing the earliest quenching events with a robust sample of massive quiescent galaxies at 2 &lt; z &lt; 5

Author

Carnall, A C, primary, Walker, S, primary, McLure, R J, primary, Dunlop, J S, primary, McLeod, D J, primary, Cullen, F, primary, Wild, V, primary, Amorin, R, primary, Bolzonella, M, primary, Castellano, M, primary, Cimatti, A, primary, Cucciati, O, primary, Fontana, A, primary, Gargiulo, A, primary, Garilli, B, primary, Jarvis, M J, primary, Pentericci, L, primary, Pozzetti, L, primary, Zamorani, G, primary, Calabro, A, primary, Hathi, N P, primary, and Koekemoer, A M, primary

Published
2020
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66. ДЕКСТРАНОВЫЕ, ЛЕВАНОВЫЕ И ЛЕВАНОПОДОБНЫЕ СЛИЗИ В САХАРОВАРЕНИИ

Author

WILD, V. and MOISCH, U.

Subjects
СКОРОСТЬ ФИЛЬТРОВАНИЯ, MUCOUS POLYSACCHARIDES, LEVAN-LIKE MUCUS, АНТИСЕПТИРУЮЩИЕ ПРЕПАРАТЫ, ФЕРМЕНТЫ, DEXTRAN, ЛЕВАН, ДЕКСТРАН, СЛИЗИСТЫЕ ПОЛИСАХАРИДЫ, ANTISEPTIC DRUGS, FILTRATION RATE, ЛЕВАНОПОДОБНЫЕ СЛИЗИ, LEVAN, ENZYMES
Abstract

В статье представлены данные о многообразии слизистых субстанций, которые обнаруживаются на сахарных предприятиях вследствие их бактериологического поражения. С целью борьбы со слизеобразованием предлагаются комплексные ферменто-антисептирующие вспомогательные препараты «Декстрасепт 1», «Дефеказа» и «Фильтраза», которые позволяют улучшить технологическое качество сахаросодержащих потоков и стабилизировать работу экстракционного и очистительного отделений сахарных заводов. The article presents data on the diversity of mucous substances that are found in sugar factories as a result of their bacteriological damage. In order to combat mucus formation, complex enzyme-antiseptic technological auxiliary products «Dextrasept 1», «Defekaza» and «Filtraza» are offered, which allow improving the technological quality of sugar-containing streams and stabilizing the work of the extraction and refining departments of sugar factories.

Published
2019
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67. The VANDELS ESO public spectroscopic survey

Author

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

Subjects
surveys, galaxies: high-redshift, galaxies: star formation, Astrophysics::Solar and Stellar Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, galaxies: evolution, Astrophysics::Galaxy Astrophysics
Abstract

VANDELS is a uniquely deep spectroscopic survey of high-redshift galaxies with the VIMOS spectrograph on ESO’s Very Large Telescope (VLT). The survey has obtained ultradeep optical (0.48 < λ < 1.0 μm) spectroscopy of ≃2100 galaxies within the redshift interval 1.0 ≤ z ≤ 7.0, over a total area of ≃0.2 deg2 centred on the CANDELS Ultra Deep Survey and Chandra Deep Field South fields. Based on accurate photometric redshift pre-selection, 85 per cent of the galaxies targeted by VANDELS were selected to be at z ≥ 3. Exploiting the red sensitivity of the refurbished VIMOS spectrograph, the fundamental aim of the survey is to provide the high-signal-to-noise ratio spectra necessary to measure key physical properties such as stellar population ages, masses, metallicities, and outflow velocities from detailed absorption-line studies. Using integration times calculated to produce an approximately constant signal-to-noise ratio (20 < tint< 80 h), the VANDELS survey targeted: (a) bright star-forming galaxies at 2.4 ≤ z ≤ 5.5, (b) massive quiescent galaxies at 1.0 ≤ z ≤ 2.5, (c) fainter star-forming galaxies at 3.0 ≤ z ≤ 7.0, and (d) X-ray/Spitzer-selected active galactic nuclei and Herschel-detected galaxies. By targeting two extragalactic survey fields with superb multiwavelength imaging data, VANDELS will produce a unique legacy data set for exploring the physics underpinning high-redshift galaxy evolution. In this paper, we provide an overview of the VANDELS survey designed to support the science exploitation of the first ESO public data release, focusing on the scientific motivation, survey design, and target selection.

Published
2018

68. The VANDELS ESO spectroscopic survey

Author

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

Subjects
high-redshift [Galaxies], QC Physics, NDAS, Astrophysics::Solar and Stellar Astrophysics, QB Astronomy, Astrophysics::Cosmology and Extragalactic Astrophysics, Surveys, evolution [Galaxies], star formation [Galaxies], Astrophysics::Galaxy Astrophysics, QC, QB
Abstract

VANDELS is a uniquely-deep spectroscopic survey of high-redshift galaxies with the VIMOS spectrograph on ESO’s Very Large Telescope (VLT). The survey has obtained ultra-deep optical (0.48 < λ < 1.0 μm) spectroscopy of ≃2100 galaxies within the redshift interval 1.0 ≤ z ≤ 7.0, over a total area of ≃ 0.2 deg2 centred on the CANDELS UDS and CDFS fields. Based on accurate photometric redshift pre-selection, 85% of the galaxies targeted by VANDELS were selected to be at z ≥ 3. Exploiting the red sensitivity of the refurbished VIMOS spectrograph, the fundamental aim of the survey is to provide the high signal-to-noise ratio spectra necessary to measure key physical properties such as stellar population ages, masses, metallicities and outflow velocities from detailed absorption-line studies. Using integration times calculated to produce an approximately constant signal-to-noise ratio (20 < tint < 80 hours), the VANDELS survey targeted: a) bright star-forming galaxies at 2.4 ≤ z ≤ 5.5, b) massive quiescent galaxies at 1.0 ≤ z ≤ 2.5, c) fainter star-forming galaxies at 3.0 ≤ z ≤ 7.0 and d) X-ray/Spitzer-selected active galactic nuclei and Herschel-detected galaxies. By targeting two extragalactic survey fields with superb multi-wavelength imaging data, VANDELS will produce a unique legacy data set for exploring the physics underpinning high-redshift galaxy evolution. In this paper we provide an overview of the VANDELS survey designed to support the science exploitation of the first ESO public data release, focusing on the scientific motivation, survey design and target selection. Postprint

Published
2018

69. ОБОСНОВАНИЕ ПРИМЕНЕНИЯ ФЕРМЕНТО-АНТИСЕПТРИУЮЩИХ ПРЕПАРАТОВ ПРИ ПЕРЕРАБОТКЕ ДЕФЕКТНОЙ СВЁКЛЫ

Author

WILD, V. and MOISCH, U.

Subjects
LEUCONOSTOC, DEFECTIVE SUGAR BEET, СЛИЗИСТЫЙ БАКТЕРИОЗ, COLLOID SUBSTANCES, DEXTRAN, ЛЕВАН, MUCOUS BACTERIOSIS, ДЕКСТРАН, КОЛЛОИДНЫЕ ВЕЩЕСТВА, ENZYME-ANTISEPTIC DRUGS, ФЕРМЕНТО-АНТИСЕПТИРУЮЩИЕ ПРЕПАРАТЫ, ДЕФЕКТНАЯ САХАРНАЯ СВЁКЛА, ЛЕЙКОНОСТОК, LEVAN
Abstract

В статье представлены данные многолетних наблюдений, позволяющих выявить три основных типа дефектности свёклы (лейконостковое поражение, поражение слизистым бактериозом и гнилостное поражение), которые наиболее часто встречаются на предприятиях Российской Федерации. Для каждого конкретно типа сырьевой дефектности представлено обоснование использования определённого ассортимента ферменто-антисептирующих препаратов. Применение препаратов «Декстрасепт 1» или «Бетасепт А и Б» совместно с «Декстрасепт 2» или «Дефеказа» в промышленных условиях позволило надёжно подавить инфицирование сахаросодержащих потоков и исключить накопление в них слизеобразующих веществ (декстрана, левана и коллоидных веществ), что привело к улучшению технико-экономических и качественных показателей сахарных заводов, перерабатывающих свёклу с пониженными технологическими качествами.The article presents the data of long-term observations, which allow to identify the 3 main types of defect in beet (leuconostoc, mucous bacterial infection and putrefaction), which are most often encountered at the enterprises of the Russian Federation. For each specific type of raw defectiveness, the rationale for using a certain range of enzyme-antiseptic drugs is presented. The use of «Dextrasept 1» or «Betasept A and B» preparations together with «Dextrasept 2» or «Defecasa» in industrial conditions made it possible to reliably suppress the infection of sugar-containing streams and exclude the accumulation of mucus-forming substances (dextran, levan and colloid substances) to improve the technical, economic and quality indicators of sugar factories that process beets with reduced technological qualities.

Published
2018
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71. Stellar Populations of over 1000 z ̃ 0.8 Galaxies from LEGA-C: Ages and Star Formation Histories from D n 4000 and Hδ

Author

Wu, P., van der Wel, A., Gallazzi, A., Bezanson, R., Pacifici, C., Straatman, C., Franx, M., Barišić, I., Bell, E., Brammer, G., Calhau, J., Chauke, P., van Houdt, J., Maseda, M., Muzzin, A., Rix, H., Sobral, D., Spilker, J., van de Sande, J., van Dokkum, P., and Wild, V.

Abstract

Drawing from the LEGA-C data set, we present the spectroscopic view of the stellar population across a large volume- and mass-selected sample of galaxies at large look-back time. We measure the 4000 Å break (D n 4000) and Balmer absorption line strengths (probed by Hδ) from 1019 high-quality spectra of z = 0.6-1.0 galaxies with M * = 2 × 1010 M ☉ to 3 × 1011 M ☉. Our analysis serves as a first illustration of the power of high-resolution, high signal-to-noise ratio continuum spectroscopy at intermediate redshifts as a qualitatively new tool to constrain galaxy formation models. The observed D n 4000-EW(Hδ) distribution of our sample overlaps with the distribution traced by present-day galaxies, but z ̃ 0.8 galaxies populate that locus in a fundamentally different manner. While old galaxies dominate the present-day population at all stellar masses >2 × 1010 M ☉, we see a bimodal D n 4000-EW(Hδ) distribution at z ̃ 0.8, implying a bimodal light-weighted age distribution. The light-weighted age depends strongly on stellar mass, with the most massive galaxies >1 × 1011 M ☉ being almost all older than 2 Gyr. At the same time, we estimate that galaxies in this high-mass range are only ̃3 Gyr younger than their z ̃ 0.1 counterparts, at odds with purely passive evolution given a difference in look-back time of >5 Gyr; younger galaxies must grow to >1011 M ☉ in the meantime, or small amounts of young stars must keep the light-weighted ages young. Star-forming galaxies at z ̃ 0.8 have stronger Hδ absorption than present-day galaxies with the same D n 4000, implying larger short-term variations in star formation activity.

Published
2018

72. The CALIFA view on stellar angular momentum across the Hubble sequence

Author

Falcón-Barroso, J., primary, van de Ven, G., additional, Lyubenova, M., additional, Mendez-Abreu, J., additional, Aguerri, J. A. L., additional, García-Lorenzo, B., additional, Bekeraité, S., additional, Sánchez, S. F., additional, Husemann, B., additional, García-Benito, R., additional, González Delgado, R. M., additional, Mast, D., additional, Walcher, C. J., additional, Zibetti, S., additional, Zhu, L., additional, Barrera-Ballesteros, J. K., additional, Galbany, L., additional, Sánchez-Blázquez, P., additional, Singh, R., additional, van den Bosch, R. C. E., additional, Wild, V., additional, Bland-Hawthorn, J., additional, Cid Fernandes, R., additional, de Lorenzo-Cáceres, A., additional, Gallazzi, A., additional, Marino, R. A., additional, Márquez, I., additional, Peletier, R. F., additional, Pérez, E., additional, Pérez, I., additional, Roth, M. M., additional, Rosales-Ortega, F. F., additional, Ruiz-Lara, T., additional, Wisotzki, L., additional, and Ziegler, B., additional

Published
2019
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73. The VANDELS survey: the star-formation histories of massive quiescent galaxies at 1.0 &lt; z &lt; 1.3

Author

Carnall, A C, primary, McLure, R J, additional, Dunlop, J S, additional, Cullen, F, additional, McLeod, D J, additional, Wild, V, additional, Johnson, B D, additional, Appleby, S, additional, Davé, R, additional, Amorin, R, additional, Bolzonella, M, additional, Castellano, M, additional, Cimatti, A, additional, Cucciati, O, additional, Gargiulo, A, additional, Garilli, B, additional, Marchi, F, additional, Pentericci, L, additional, Pozzetti, L, additional, Schreiber, C, additional, Talia, M, additional, and Zamorani, G, additional

Published
2019
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75. Galaxy And Mass Assembly (GAMA): The mechanisms for quiescent galaxy formation at z < 1

Author

Rowlands, K., Wild, V., Bourne, N., Bremer, M., Brough, S., Driver, S. P., Hopkins, A. M., Owers, M. S., Phillipps, S., Pimbblet, K., Sansom, Anne E, Wang, L., Alpaslan, M., Bland-Hawthorn, J., Colless, M., Holwerda, B. W., Taylor, E. N., Rowlands, K., Wild, V., Bourne, N., Bremer, M., Brough, S., Driver, S. P., Hopkins, A. M., Owers, M. S., Phillipps, S., Pimbblet, K., Sansom, Anne E, Wang, L., Alpaslan, M., Bland-Hawthorn, J., Colless, M., Holwerda, B. W., and Taylor, E. N.

Abstract

One key problem in astrophysics is understanding how and why galaxies switch off their star formation, building the quiescent population that we observe in the local Universe. From the Galaxy And Mass Assembly and VIsible MultiObject Spectrograph Public Extragalactic Redshift surveys, we use spectroscopic indices to select quiescent and candidate transition galaxies. We identify potentially rapidly transitioning post-starburst (PSB) galaxies and slower transitioning green-valley galaxies. Over the last 8 Gyr, the quiescent population has grown more slowly in number density at high masses ({M}_\ast >10^{11}{M_{&sun;}) than at intermediate masses ({M}_\ast >10^{10.6}{M_{&sun;}). There is evolution in both the PSB and green-valley stellar mass functions, consistent with higher mass galaxies quenching at earlier cosmic times. At intermediate masses ({M}_\ast >10^{10.6}{M_{&sun;}), we find a green-valley transition time-scale of 2.6 Gyr. Alternatively, at z ~ 0.7, the entire growth rate could be explained by fast-quenching PSB galaxies, with a visibility time-scale of 0.5 Gyr. At lower redshift, the number density of PSBs is so low that an unphysically short visibility window would be required for them to contribute significantly to the quiescent population growth. The importance of the fast-quenching route may rapidly diminish at z < 1. However, at high masses ({M}_\ast >10^{11}{M_{&sun;}), there is tension between the large number of candidate transition galaxies compared to the slow growth of the quiescent population. This could be resolved if not all high-mass PSB and green-valley galaxies are transitioning from star forming to quiescent, for example if they rejuvenate out of the quiescent population following the accretion of gas and triggering of star formation, or if they fail to completely quench their star formation.

Published
2018

76. Migration: a core public health ethics issue

Author

Wild, V, Dawson, A, Wild, V, and Dawson, A

Abstract

© 2018 The Royal Society for Public Health Objectives: In this article, we outline the link between migration, public health and ethics. Study design: Discussing relevant arguments about migration from the perspective of public health and public health ethics. Methods: Critical review of theories and frameworks, case-based analysis and systematic identification and discussion of challenges. Results: Migration is a core issue of public health ethics and must take a case-based approach: seeking to identify the specific ethical dimensions and vulnerabilities in each particular context. Public health as a practice, built upon the core value of justice, requires the protection and promotion of migrants' well-being (even if this produces tension with immigration services). Ethical analysis should take all phases of migration into account: before, during and after transit. We argue that migration policies, at least as they relate to migrants' well-being, should be founded upon a shared humanity, respect for human rights and on the idea that effective public health cannot and should not be confined within the borders and to the citizens of any host country. Conclusions: We make the case for migration to be seen as a core issue of public health ethics.

Published
2018

77. The VANDELS ESO public spectroscopic survey:Observations and first data release

Author

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

Published
2018

78. Stellar kinematics across the Hubble sequence in the CALIFA survey: general properties and aperture corrections

Author

Falc��n-Barroso, J., Lyubenova, M., van de Ven, G., M��ndez-Abreu, J., Aguerri, J. A. L., Garc��a-Lorenzo, B., Bekeraite, S., S��nchez, S. F., Husemann, B., Garc��a-Benito, R., Mast, D., Walcher, C. J., Zibetti, S., Barrera-Ballesteros, J. K., Galbany, L., S��nchez-Bl��zquez, P., Singh, R., Bosch, R. C. E. van den, Wild, V., Zhu, L., Bland-Hawthorn, J., Fernandes, R. Cid, de Lorenzo-C��ceres, A., Gallazzi, A., Delgado, R. M. Gonz��lez, Marino, R. A., M��rquez, I., P��rez, E., P��rez, I., Roth, M. M., Rosales-Ortega, F. F., Ru��z-Lara, T., Wisotzki, L., Ziegler, B., collaboration, the CALIFA, Astronomy, Ministerio de Economía y Competitividad (España), European Commission, European Research Council, and University of St Andrews. School of Physics and Astronomy

Subjects
Astrofísica, POTSDAM MULTIAPERTURE SPECTROPHOTOMETER, Ciencias Físicas, structure [Galaxies], Astrophysics, Kinematics, 01 natural sciences, Hubble sequence, purl.org/becyt/ford/1 [https], elliptical and lenticular [Galaxies], Range (statistics), QB Astronomy, EARLY-TYPE GALAXIES, EMISSION-LINE KINEMATICS, galaxies: elliptical and lenticular, 010303 astronomy & astrophysics, QC, galaxies: kinematics and dynamics, QB, Physics, Basis (linear algebra), kinematics and dynamics [Galaxies], Velocity dispersion, Galaxies: elliptical and lenticular, cD, stucture [Galaxies], FIELD AREA SURVEY, symbols, galaxies: structure, galaxies: evolution, CIENCIAS NATURALES Y EXACTAS, Stellar kinematics, galaxies: spiral, Aperture, FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, elliptical and lenticular, cD [Galaxies], PUBLIC DATA RELEASE, cD, symbols.namesake, ELLIPTIC GALAXIES, 0103 physical sciences, galaxies: formation, Astrophysics::Galaxy Astrophysics, LENTICULAR GALAXIES, spiral [Galaxies], 010308 nuclear & particles physics, DAS, Astronomy and Astrophysics, purl.org/becyt/ford/1.3 [https], evolution [Galaxies], Astrophysics - Astrophysics of Galaxies, formation [Galaxies], SAURON PROJECT, Galaxy, Astronomía, QC Physics, Space and Planetary Science, Astrophysics of Galaxies (astro-ph.GA), DIGITAL SKY SURVEY, SIGHT VELOCITY DISTRIBUTIONS
Abstract

J. Falcón-Barroso et. al., We present the stellar kinematic maps of a large sample of galaxies from the integral-field spectroscopic survey CALIFA. The sample comprises 300 galaxies displaying a wide range of morphologies across the Hubble sequence, from ellipticals to late-type spirals. This dataset allows us to homogeneously extract stellar kinematics up to several effective radii. In this paper, we describe the level of completeness of this subset of galaxies withrespect to the full CALIFA sample, as well as the virtues and limitations of the kinematic extraction compared to other well-known integral-field surveys. In addition, we provide averaged integrated velocity dispersion radial profiles for different galaxy types, which are particularly useful to apply aperture corrections for single aperture measurements or poorly resolved stellar kinematics of high-redshift sources. The work presented in this paper sets the basis for the study of more general properties of galaxies that will be explored in subsequent papers of the survey.© ESO, 2016., J.F.-B. from grant AYA2013-48226-C3-1-P from the Spanish Ministry of Economy and Competitiveness (MINECO). J.F.-B. and G.v.d.V. from the FP7 Marie Curie Actions of the European Commission, via the Initial Training Network DAGAL under REA grant agreement number 289313. J.M.-A. and V.W. acknowledge support from the European Research Council Starting Grant (SEDMorph P.I. V. Wild). P.S.-B. acknowledge financial support from the BASAL CATA Center for Astrophysics and Associated Technologies through grant PFB-06. R.M.G.D. from grant AYA2014-57490-P. R.G.-B, R.M.G.D. and E.P. acknowledge support from the project JA-FQM-2828. C.J.W. acknowledges support through the Marie Curie Career Integration Grant 303912. L.G. from the Ministry of Economy, Development, and Tourism's Millennium Science Initiative through grant IC120009 awarded to The Millennium Institute of Astrophysics (MAS), and CONICYT through FONDECYT grant 3140566. I.M. from grant AYA2013-42227-P.

Published
2017

79. Сезон 2016 года: слизистый бактериоз

Author

WILD, V. and MOISCH, U.

Subjects
жомопрессовая вода, декстраназа, диффузионный сок, dextranase, dextran, colloidal substances, pulp-press water, Leuconostoc mesenteroides, декстран, diffusion juice, коллоидные вещества, антисептирующие препараты, antiseptic drugs
Abstract

В статье представлены данные об особенностях микробиологического поражения свёклосахарных предприятий слизистым бактериозом в сезон 2016 г. В целях эффективной борьбы с этой инфекцией апробирован и рекомендован комплексный антисептирующий препарат «Декстрасепт 1 и 2», эффективно уничтожающий лейконосток и декстрановые слизи. The article presents data on the peculiarities of microbiological defeat of sugar beet enterprises with mucous bacteriosis in the season of 2016. In order to effectively combat this infection, a complex antiseptic drug «Dextrasept 1 and 2» effectively destroying leuconostoc and dextran mucus was tested and recommended

Published
2017
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80. ОСОБЕННОСТИ ПЕРЕРАБОТКИ ДЕФЕКТНОЙ СВЁКЛЫ

Author

WILD, V. and MOISCH, U.

Subjects
LEUCONOSTOC MESENTEROIDES, DEFECTIVE SUGAR BEET, АНТИСЕПТИРУЮЩИЕ ПРЕПАРАТЫ, ФЕРМЕНТЫ, СЛИЗИСТЫЙ БАКТЕРИОЗ, COLLOIDAL SUBSTANCES, LEUCONOSTOCMESENTEROIDES, DEXTRAN, MUCOUS BACTERIOSIS, ДЕКСТРАН, КОЛЛОИДНЫЕ ВЕЩЕСТВА, ANTISEPTIC DRUGS, ДЕФЕКТНАЯ САХАРНАЯ СВЁКЛА, ENZYMES
Abstract

В статье представлены данные о микробиологическом и биохимическом составах свёклы, поражённой слизистым бактериозом и лейконостоковой инфекцией, и об особенностях её переработки. Показано, что использование ферменто-антисептирующего комплекса препаратов «Декстрасепт 1» («Бетасепт А и Б») и «Декстрасепт 2», которые устраняют посторонние микроорганизмы и продукты их жизнедеятельности, позволяет значительно улучшить технико-экономические показатели сахарных заводов, перерабатывающих свёклу с пониженными технологическими качествами.The article presents data on the microbiological and biochemical composition of beets affected by mucous bacteriosis and Leuconostoc infection and on the peculiarities of its processing. It is shown that the use of the enzyme-antiseptic complex of preparations «Dextrasept 1» («Betasept A and B») and «Dextrasept 2», which eliminate foreign microorganisms and products of their vital activity, allows to significantly improve the technical and economic indicators of sugar refineries processing beets with reduced technological qualities.

Published
2017
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81. Timing the earliest quenching events with a robust sample of massive quiescent galaxies at 2 < z < 5.

Author

Carnall, A C, Walker, S, McLure, R J, Dunlop, J S, McLeod, D J, Cullen, F, Wild, V, Amorin, R, Bolzonella, M, Castellano, M, Cimatti, A, Cucciati, O, Fontana, A, Gargiulo, A, Garilli, B, Jarvis, M J, Pentericci, L, Pozzetti, L, Zamorani, G, and Calabro, A

Abstract

We present a sample of 151 massive (M * > 1010 M⊙) quiescent galaxies at 2 < z < 5, based on a sophisticated Bayesian spectral energy distribution fitting analysis of the CANDELS UDS and GOODS-South fields. Our sample includes a robust sub-sample of 61 objects for which we confidently exclude low-redshift and star-forming solutions. We identify 10 robust objects at z > 3, of which 2 are at z > 4. We report formation redshifts, demonstrating that the oldest objects formed at z > 6; however, individual ages from our photometric data have significant uncertainties, typically ∼0.5 Gyr. We demonstrate that the UVJ colours of the quiescent population evolve with redshift at z > 3, becoming bluer and more similar to post-starburst galaxies at lower redshift. Based upon this, we construct a model for the time evolution of quiescent galaxy UVJ colours, concluding that the oldest objects are consistent with forming the bulk of their stellar mass at z  ∼ 6–7 and quenching at z  ∼ 5. We report spectroscopic redshifts for two of our objects at z  = 3.440 and 3.396, which exhibit extremely weak Ly α emission in ultra-deep VANDELS spectra. We calculate star formation rates based on these line fluxes, finding that these galaxies are consistent with our quiescent selection criteria, provided their Ly α escape fractions are >3 and >10 per cent, respectively. We finally report that our highest redshift robust object exhibits a continuum break at λ ∼ 7000 Å in a spectrum from VUDS, consistent with our photometric redshift of |$z_\mathrm{phot}=4.72^{+0.06}_{-0.04}$|⁠. If confirmed as quiescent, this object would be the highest redshift known quiescent galaxy. To obtain stronger constraints on the times of the earliest quenching events, high-SNR spectroscopy must be extended to z  ≳ 3 quiescent objects. [ABSTRACT FROM AUTHOR]

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

Author

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

Published
2018
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83. SDSS-IV MaNGA: spatially resolved star formation histories and the connection to galaxy physical properties

Author

Rowlands, K, primary, Heckman, T, additional, Wild, V, additional, Zakamska, N L, additional, Rodriguez-Gomez, V, additional, Barrera-Ballesteros, J, additional, Lotz, J, additional, Thilker, D, additional, Andrews, B H, additional, Boquien, M, additional, Brinkmann, J, additional, Brownstein, J R, additional, Hwang, H-C, additional, and Smethurst, R, additional

Published
2018
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87. The origins of post-starburst galaxies at z < 0.05

Author

Pawlik, M M, primary, Taj Aldeen, L, additional, Wild, V, additional, Mendez-Abreu, J, additional, Lahén, N, additional, Johansson, P H, additional, Jimenez, N, additional, Lucas, W, additional, Zheng, Y, additional, Walcher, C J, additional, and Rowlands, K, additional

Published
2018
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88. Rejoinder to Karen Lutfey Spencer

Author

Wild, V., Drewniak, D.P., Sauer, C.G., Krones, T., Wild, V., Drewniak, D.P., Sauer, C.G., and Krones, T.

Abstract

Contains fulltext : 161248.pdf (publisher's version ) (Closed access), Refers to: Karen Lutfey Spencer, What is the future of research on medical decision making? (And is it bright?): A response to Drewniak and colleagues, Social Science & Medicine, Volume 168, November 2016, Pages 175-177. http://dx.doi.org/10.1016/j.socscimed.2016.09.017

Published
2017

89. CALIFA, the Calar Alto Legacy Integral Field Area survey

Author

Sanchez, Sébastien, García-Benito, R., Zibetti, S., Walcher, C., Husemann, B., Mendoza, M., Galbany, L., Falcón-Barroso, J., Mast, D., Aceituno, J., Aguerri, J., Alves, J., Amorim, A., Ascasibar, Y., Barrado-Navascues, D., Barrera-Ballesteros, J., Bekeraitè, S., Bland-Hawthorn, J., Cano Díaz, M., Cid Fernandes, R., Cavichia, O., Cortijo, C., Dannerbauer, H., Demleitner, M., Díaz, A., Dettmar, R., de Lorenzo-Cáceres, A., del Olmo, A., Galazzi, A., García-Lorenzo, B., Gil de Paz, A., González Delgado, R., Holmes, L., Iglesias-Paramo, J., Kehrig, C., Kelz, A., Kennicutt, R., Kleemann, B., Lacerda, E., López Fernández, R., López Sánchez, A., Lyubenova, M., Marino, R., Márquez, I., Mendez-Abreu, J., Mollá, M., Monreal-Ibero, A., Ortega Minakata, R., Torres-Papaqui, J., Perez, Emile, Rosales-Ortega, F., Roth, M., Sánchez-Blázquez, P., Schilling, U., Spekkens, K., Vale Asari, N., van den Bosch, R., van de Ven, G., Vilchez, J., Wild, V., Wisotzki, L., Yildirim, A., Ziegler, B., Laboratoire de l'intégration, du matériau au système (IMS), Centre National de la Recherche Scientifique (CNRS)-Institut Polytechnique de Bordeaux-Université Sciences et Technologies - Bordeaux 1, Instituto de Astrofísica de Andalucía (IAA), Consejo Superior de Investigaciones Científicas [Madrid] (CSIC), INAF - Osservatorio Astrofisico di Arcetri (OAA), Istituto Nazionale di Astrofisica (INAF), Department of Physics [Pittsburgh], Carnegie Mellon University [Pittsburgh] (CMU), Instituto Dom Luiz, Universidade de Lisboa (ULISBOA), Laboratory for Systems, Instrumentation and Modeling in Science and Technology for Space and the Environment (University of Lisbon and University of Beira Interior), CRLCC Val d'Aurelle - Paul Lamarque, Astrophysique Interprétation Modélisation (AIM (UMR_7158 / UMR_E_9005 / UM_112)), 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), Heidelberg Univ, Astron Rechen Inst, Zentrum Astron, Heidelberg, Germany, Astronomisches Institut der Ruhr-Universität Bochum, Ruhr-Universität Bochum [Bochum], 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), Laboratoire Avancé de Spectroscopie pour les Intéractions la Réactivité et l'Environnement - UMR 8516 (LASIRE), Institut de Chimie du CNRS (INC)-Université de Lille-Centre National de la Recherche Scientifique (CNRS)-Centrale Lille Institut (CLIL), Galaxies, Etoiles, Physique, Instrumentation (GEPI), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Princeton University, Departamento de FisicaTeorica e IFT-UAM/CSIC, Universidad Autonoma de Madrid (UAM), Departamento de Tecnociencias,Centro de Ciencias Aplicadas y Desarrollo Tecnologico, Universidad Nacional Autonoma de Mexico, Universidad Nacional Autónoma de México (UNAM), Leibniz-Institut für Astrophysik Potsdam (AIP), European Southern Observatory (ESO), Millennium Institute of Astrophysics, Universidad de Chile, Instituto de Astrofisica de Canarias (IAC), Consejo Nacional de Investigaciones Científicas y Técnicas [Buenos Aires] (CONICET), Centro Astronómico Hispano Alemán, Observatorio de Calar Alto (CAHA), University of Vienna [Vienna], Departamento Física [Florianópolis], Universidade Federal de Santa Catarina = Federal University of Santa Catarina [Florianópolis] (UFSC), Department of Physics and Astronomy [Baltimore], Johns Hopkins University (JHU), Sydney Institute for Astronomy (SIfA), The University of Sydney, Universidade Federal de Itajubá, SUPA School of Physics and Astronomy [University of St Andrews], University of St Andrews [Scotland]-Scottish Universities Physics Alliance (SUPA), Universidad de Granada (UGR), Departamento de Astrofisica y Ciencias de la Atmósfera, Universidad Complutense de Madrid = Complutense University of Madrid [Madrid] (UCM), Royal Military College of Canada (RMCC), Royal Military College of Canada, Institute of Astronomy [Cambridge], University of Cambridge [UK] (CAM), Departamento de Física [Universidade Federal de Santa Catarina], Kapteyn Astronomical Institute [Groningen], University of Groningen [Groningen], Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology [Zürich] (ETH Zürich), Centro de Investigaciones Energéticas Medioambientales y Tecnológicas [Madrid] (CIEMAT), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS), Observatório do Valongo/UFRJ [Rio de Janeiro], Universidade Federal do Rio de Janeiro (UFRJ), Universidad de Guanajuato, ANR-12-BS05-0016,STILISM,Structure du Milieu Interstellaire Local par Inversion(2012), European Project: 326466,EC:FP7:PEOPLE,FP7-PEOPLE-2012-CIG,STEMAGE(2013), European Project: 289313,EC:FP7:PEOPLE,FP7-PEOPLE-2011-ITN,DAGAL(2012), European Project: 267251,EC:FP7:PEOPLE,FP7-PEOPLE-2010-COFUND,ASTROFIT(2011), European Project: 306299,EC:FP7:ERC,ERC-2012-StG_20111012,SEDMORPH(2012), European Project: 303912,EC:FP7:PEOPLE,FP7-PEOPLE-2011-CIG,SFEHG(2012), European Project: 612701,EC:FP7:PEOPLE,FP7-PEOPLE-2013-IRSES,SELGIFS(2013), Université Sciences et Technologies - Bordeaux 1-Institut Polytechnique de Bordeaux-Centre National de la Recherche Scientifique (CNRS), Consejo Superior de Investigaciones Científicas [Spain] (CSIC), 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), Laboratoire de Spectrochimie Infrarouge et Raman - UMR 8516 (LASIR), Centre National de la Recherche Scientifique (CNRS)-Université de Lille, PSL Research University (PSL)-PSL Research University (PSL)-Centre National de la Recherche Scientifique (CNRS), Universidad Nacional Autónoma de México = National Autonomous University of Mexico (UNAM), Universidad de Chile = University of Chile [Santiago] (UCHILE), Universidad Autónoma de Madrid (UAM), Universität Heidelberg [Heidelberg] = Heidelberg University, and Universidad de Granada = University of Granada (UGR)

Subjects
[PHYS]Physics [physics], Galaxies: fundamental parameters, Techniques: imaging spectroscopy, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], techniques: spectroscopic, ComputingMilieux_MISCELLANEOUS
Abstract

International audience; This paper describes the Third Public Data Release (DR3) of the Calar Alto Legacy Integral Field Area (CALIFA) survey. Sciencegrade quality data for 667 galaxies are made public, including the 200 galaxies of the Second Public Data Release (DR2). Data were obtained with the integral-field spectrograph PMAS/PPak mounted on the 3.5m telescope at the Calar Alto Observatory. Three different spectral setups are available, i) a low-resolution V500 setup covering the wavelength range 3745–7500 Å (4240-7140 Å unvignetted) with a spectral resolution of 6.0 Å (FWHM), for 646 galaxies, ii) a medium-resolution V1200 setup covering the wavelength range 3650–4840 Å (3650-4620 Å unvignetted) with a spectral resolution of 2.3 Å (FWHM), for 484 galaxies, and iii) the combination of the cubes from both setups (called COMBO), with a spectral resolution of 6.0 Å and a wavelength range between 3700-7500 Å (3700-7140 Å unvignetted), for 446 galaxies. The Main Sample, selected and observed according to the CALIFA survey strategy covers a redshift range between 0.005 and 0.03, spans the color-magnitude diagram and probes a wide range of stellar mass, ionization conditions, and morphological types. The Extension Sample covers several types of galaxies that are rare in the overall galaxy population and therefore not numerous or absent in the CALIFA Main Sample. All the cubes in the data release were processed using the latest pipeline, which includes improved versions of the calibration frames and an even further improved image reconstruction quality. In total, the third data release contains 1576 datacubes, including ∼1.5 million independent spectra. It is available at http://califa.caha.es/DR3.

Published
2016

90. The 2dF Galaxy Redshift Survey: the nature of the relative bias between galaxies of different spectral type

Author

Conway, E, Maddox, S, Wild, V, Peacock, JA, Hawkins, E, Norberg, P, Madgwick, DS, Baldry, IK, Baugh, CM, Hawthorn, JB, Bridges, T, Cannon, R, Cole, S, Colless, M, Collins, C, Couch, W, Dalton, G, De Propris, R, Driver, SP, Efstathiou, G, Ellis, RS, Frenk, CS, Glazebrook, K, Jackson, C, Jones, B, Lahav, O, Lewis, I, Lumsden, S, Percival, W, Peterson, BA, Sutherland, W, Taylor, K, and Team, 2

Subjects
Physics, Field galaxy, Large-scale structure of Universe, Astronomy and Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, Surveys, Scale invariance, Type (model theory), Redshift survey, Measure (mathematics), Galaxies : distances and redshifts, Galaxy, distances and redshifts, Galaxies : statistics, Large-scale structure of Universe [Surveys, Galaxies], Goodness of fit, Space and Planetary Science, Log-normal distribution
Abstract

Monthly Notices of the Royal Astronomical Society, 356 (2), ISSN:0035-8711, ISSN:1365-2966, ISSN:1365-8711

Published
2016

91. Morpho-kinematic properties of field S0 bulges in the CALIFA survey

Author

Méndez-Abreu, J., primary, Aguerri, J. A. L., additional, Falcón-Barroso, J., additional, Ruiz-Lara, T., additional, Sánchez-Menguiano, L., additional, de Lorenzo-Cáceres, A., additional, Costantin, L., additional, Catalán-Torrecilla, C., additional, Zhu, L., additional, Sánchez-Blazquez, P., additional, Florido, E., additional, Corsini, E. M., additional, Wild, V., additional, Lyubenova, M., additional, van de Ven, G., additional, Sánchez, S. F., additional, Bland-Hawthorn, J., additional, Galbany, L., additional, García-Benito, R., additional, García-Lorenzo, B., additional, Delgado, R. M. González, additional, López-Sánchez, A. R., additional, Marino, R. A., additional, Márquez, I., additional, Ziegler, B., additional, and collaboration, the CALIFA, additional

Published
2017
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92. Galaxy And Mass Assembly (GAMA): The mechanisms for quiescent galaxy formation at z < 1

Author

Rowlands, K., primary, Wild, V., additional, Bourne, N., additional, Bremer, M., additional, Brough, S., additional, Driver, S. P., additional, Hopkins, A. M., additional, Owers, M. S., additional, Phillipps, S., additional, Pimbblet, K., additional, Sansom, A. E., additional, Wang, L., additional, Alpaslan, M., additional, Bland-Hawthorn, J., additional, Colless, M., additional, Holwerda, B. W., additional, and Taylor, E. N., additional

Published
2017
Full Text
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94. Non-Invasive Beurteilung der Chemokin Receptor 4 (CXCR4) Expression in Gastroenteropankreatischen Neuroendokrinen Tumoren

Author

Weich, A, additional, Werner, RA, additional, Higuchi, T, additional, Schmid, JS, additional, Schirbel, A, additional, Lassmann, M, additional, Wild, V, additional, Rudelius, M, additional, Kudlich, T, additional, Herrmann, K, additional, Scheurlen, M, additional, Buck, AK, additional, Kropf, S, additional, Wester, HJ, additional, and Lapa, C, additional

Published
2017
Full Text
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95. Two-dimensional multi-component photometric decomposition of CALIFA galaxies

Author

Méndez-Abreu, J., primary, Ruiz-Lara, T., additional, Sánchez-Menguiano, L., additional, de Lorenzo-Cáceres, A., additional, Costantin, L., additional, Catalán-Torrecilla, C., additional, Florido, E., additional, Aguerri, J. A. L., additional, Bland-Hawthorn, J., additional, Corsini, E. M., additional, Dettmar, R. J., additional, Galbany, L., additional, García-Benito, R., additional, Marino, R. A., additional, Márquez, I., additional, Ortega-Minakata, R. A., additional, Papaderos, P., additional, Sánchez, S. F., additional, Sánchez-Blazquez, P., additional, Spekkens, K., additional, van de Ven, G., additional, Wild, V., additional, and Ziegler, B., additional

Published
2017
Full Text
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96. Tracing kinematic (mis)alignments in CALIFA merging galaxies

Author

Barrera-Ballesteros, J., García-Lorenzo, B., Falcón-Barroso, J., van de Ven, G., Lyubenova, M., Wild, V., Méndez-Abreu, J., Sanchez, Sébastien, Marquez, I., Masegosa, J., Monreal-Ibero, A., Ziegler, B., Del Olmo, A., Verdes-Montenegro, L., García-Benito, R., Husemann, B., Mast, D., Kehrig, C., Iglesias-Paramo, J., Marino, R., Aguerri, J., Walcher, C., Vílchez, J., Bomans, D., Cortijo-Ferrero, C., González Delgado, R., Bland-Hawthorn, J., McIntosh, D., Bekeraitė, S., Laboratoire de l'intégration, du matériau au système (IMS), Université Sciences et Technologies - Bordeaux 1 (UB)-Institut Polytechnique de Bordeaux-Centre National de la Recherche Scientifique (CNRS), Galaxies, Etoiles, Physique, Instrumentation (GEPI), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Instituto de Astrofísica de Andalucía (IAA), Consejo Superior de Investigaciones Científicas [Madrid] (CSIC), 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), Laboratoire de Cosmologie, Astrophysique Stellaire & Solaire, de Planétologie et de Mécanique des Fluides (CASSIOPEE), Université Nice Sophia Antipolis (1965 - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Ruhr-Universität Bochum [Bochum], The University of Sydney, Centre National de la Recherche Scientifique (CNRS)-Institut Polytechnique de Bordeaux-Université Sciences et Technologies - Bordeaux 1, Université Nice Sophia Antipolis (... - 2019) (UNS), and Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS)

Subjects
[PHYS]Physics [physics], [SDU]Sciences of the Universe [physics], [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], ComputingMilieux_MISCELLANEOUS
Abstract

International audience

Published
2015

97. CALIFA, the Calar Alto Legacy Integral Field Area survey

Author

García-Benito, R., Zibetti, S., Sanchez, Sébastien, Husemann, B., de Amorim, A., Castillo-Morales, A., Cid Fernandes, R., Ellis, S., Falcón-Barroso, J., Galbany, L., Gil de Paz, A., González Delgado, R., Lacerda, E., Lopez-Fernandez, R., de Lorenzo-Cáceres, A., Lyubenova, M., Marino, R., Mast, D., Mendoza, M., Perez, Emile, Vale Asari, N., Aguerri, J., Ascasibar, Y., Bekerait*error*ė, S., Bland-Hawthorn, J., Barrera-Ballesteros, J., Bomans, D., Cano-Díaz, M., Catalán-Torrecilla, C., Cortijo, C., Delgado-Inglada, G., Demleitner, M., Dettmar, R.-J., Díaz, A., Florido, E., Gallazzi, A., García-Lorenzo, B., Gomes, J., Holmes, L., Iglesias-Paramo, J., Jahnke, K., Kalinova, V., Kehrig, C., Kennicutt, R., López-Sánchez, Á., Márquez, I., Masegosa, J., Meidt, S., Mendez-Abreu, J., Mollá, M., Monreal-Ibero, A., Morisset, C., del Olmo, A., Papaderos, P., Pérez, I., Quirrenbach, A., Rosales-Ortega, F., Roth, M., Ruiz-Lara, T., Sánchez-Blázquez, P., Sánchez-Menguiano, L., Singh, R., Spekkens, K., Stanishev, V., Torres-Papaqui, J., van de Ven, G., Vilchez, J., Walcher, C., Wild, V., Wisotzki, L., Ziegler, B., Alves, J., Barrado, D., Quintana, J., Aceituno, J., Instituto de Astrofísica de Andalucía (IAA), Consejo Superior de Investigaciones Científicas [Madrid] (CSIC), INAF - Osservatorio Astrofisico di Arcetri (OAA), Istituto Nazionale di Astrofisica (INAF), Laboratoire de l'intégration, du matériau au système (IMS), Université Sciences et Technologies - Bordeaux 1 (UB)-Institut Polytechnique de Bordeaux-Centre National de la Recherche Scientifique (CNRS), Department of Physics [Pittsburgh], Carnegie Mellon University [Pittsburgh] (CMU), Laboratoire de Cosmologie, Astrophysique Stellaire & Solaire, de Planétologie et de Mécanique des Fluides (CASSIOPEE), Université Nice Sophia Antipolis (1965 - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Philippine General Hospital, Interactions moléculaires et réactivité chimique et photochimique (IMRCP), Institut de Chimie de Toulouse (ICT), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut de Chimie du CNRS (INC)-Centre National de la Recherche Scientifique (CNRS)-Institut National Polytechnique (Toulouse) (Toulouse INP), Université de Toulouse (UT)-Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Institut Ecologie et Environnement (INEE), Centre National de la Recherche Scientifique (CNRS)-Centre National de la Recherche Scientifique (CNRS)-Fédération de Recherche Fluides, Energie, Réacteurs, Matériaux et Transferts (FERMAT), Institut National des Sciences Appliquées - Toulouse (INSA Toulouse), Institut National des Sciences Appliquées (INSA)-Université de Toulouse (UT)-Institut National des Sciences Appliquées (INSA)-Université de Toulouse (UT)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Centre National de la Recherche Scientifique (CNRS)-Institut National Polytechnique (Toulouse) (Toulouse INP), Université de Toulouse (UT)-Institut National des Sciences Appliquées - Toulouse (INSA Toulouse), Institut National des Sciences Appliquées (INSA)-Université de Toulouse (UT)-Institut National des Sciences Appliquées (INSA)-Centre National de la Recherche Scientifique (CNRS)-Centre National de la Recherche Scientifique (CNRS), The University of Sydney, Ruhr-Universität Bochum [Bochum], CRLCC Val d'Aurelle - Paul Lamarque, Universität Heidelberg [Heidelberg] = Heidelberg University, Astronomisches Institut der Ruhr-Universität Bochum, 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), Max-Planck-Institut für Astronomie (MPIA), Max-Planck-Gesellschaft, Galaxies, Etoiles, Physique, Instrumentation (GEPI), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Plateforme d’Investigation Technologique [Centre d’Investigation Clinique 1432 module Plurithématique - Dijon] (PIT), Cognition, Action, et Plasticité Sensorimotrice [Dijon - U1093] (CAPS), Université de Bourgogne (UB)-Institut National de la Santé et de la Recherche Médicale (INSERM)-Université de Bourgogne (UB)-Institut National de la Santé et de la Recherche Médicale (INSERM)-Centre d'Investigation Clinique 1432 (Dijon) - Module Plurithématique : Périnatalité Cancérologie Handicap et Ophtalmologie (CIC-P803), Université de Bourgogne (UB)-Direction Générale de l'Organisation des Soins (DGOS)-Institut National de la Santé et de la Recherche Médicale (INSERM)-Direction Générale de l'Organisation des Soins (DGOS)-Institut National de la Santé et de la Recherche Médicale (INSERM), Centre IRMf de Marseille, Université de la Méditerranée - Aix-Marseille 2, Departamento de FisicaTeorica e IFT-UAM/CSIC, Universidad Autónoma de Madrid (UAM), Institute for Plasma Research [Gandhinagar], Instituto Superior Técnico, Universidade Técnica de Lisboa (IST), Fundaçao Cearense de Meteorologia e Recursos Hidricos, Departamento de Astrofisica [Madrid], Centro de Astrobiologia [Madrid] (CAB), Instituto Nacional de Técnica Aeroespacial (INTA)-Consejo Superior de Investigaciones Científicas [Madrid] (CSIC)-Instituto Nacional de Técnica Aeroespacial (INTA)-Consejo Superior de Investigaciones Científicas [Madrid] (CSIC), Université Sciences et Technologies - Bordeaux 1-Institut Polytechnique de Bordeaux-Centre National de la Recherche Scientifique (CNRS), Université Nice Sophia Antipolis (... - 2019) (UNS), Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Chimie du CNRS (INC)-Institut de Chimie de Toulouse (ICT-FR 2599), Institut National Polytechnique (Toulouse) (Toulouse INP), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Institut de Chimie du CNRS (INC)-Institut National Polytechnique (Toulouse) (Toulouse INP), Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD), Heidelberg Univ, Astron Rechen Inst, Zentrum Astron, Heidelberg, Germany, and Universidad Autonoma de Madrid (UAM)

Subjects
[PHYS]Physics [physics], [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], ComputingMilieux_MISCELLANEOUS
Abstract

International audience

Published
2015

99. Übersicht über empirische Untersuchungen zu DRG und Managed Care in den USA

Author

Wild, V, Pfister, E, Biller-Andorno, N; https://orcid.org/0000-0001-7661-1324, Wild, V ( V ), Pfister, E ( E ), Biller-Andorno, N ( N ), Bastami, S, Wild, V, Pfister, E, Biller-Andorno, N; https://orcid.org/0000-0001-7661-1324, Wild, V ( V ), Pfister, E ( E ), Biller-Andorno, N ( N ), and Bastami, S

Published
2011

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