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1. Lyα forest tomography from background galaxies: The first megaparsec-resolution large-scale structure map at z > 2

Author

Lee, KG, Hennawi, JF, Stark, C, Prochaska, JX, White, M, Schlegel, DJ, Eilers, AC, Arinyo-I-Prats, A, Suzuki, N, Croft, RAC, Caputi, KI, Cassata, P, Ilbert, O, Garilli, B, Koekemoer, AM, Le Brun, V, Fèvre, OL, Maccagni, D, Nugent, P, Taniguchi, Y, Tasca, LAM, Tresse, L, Zamorani, G, and Zucca, E

Subjects
cosmology: observations, galaxies: high-redshift, intergalactic medium, quasars: absorption lines, surveys, techniques: spectroscopic, astro-ph.CO, astro-ph.GA, Astronomy & Astrophysics, Astronomical and Space Sciences
Abstract

We present the first observations of foreground Lyα forest absorption from high-redshift galaxies, targeting 24 star-forming galaxies (SFGs) with z ∼ 2.3-2.8 within a 5′ × 14′ region of the COSMOS field. The transverse sightline separation is ∼2 h-1 Mpc comoving, allowing us to create a tomographic reconstruction of the three-dimensional (3D) Lyα forest absorption field over the redshift range 2.20 ≤ z ≤ 2.45. The resulting map covers 6 h-1 Mpc × 14 h-1 Mpc in the transverse plane and 230 h-1 Mpc along the line of sight with a spatial resolution of ≈3.5 h-1 Mpc, and is the first high-fidelity map of a large-scale structure on ∼ Mpc scales at z > 2. Our map reveals significant structures with ≳10 h-1 Mpc extent, including several spanning the entire transverse breadth, providing qualitative evidence for the filamentary structures predicted to exist in the high-redshift cosmic web. Simulated reconstructions with the same sightline sampling, spectral resolution, and signal-to-noise ratio recover the salient structures present in the underlying 3D absorption fields. Using data from other surveys, we identified 18 galaxies with known redshifts coeval with our map volume, enabling a direct comparison with our tomographic map. This shows that galaxies preferentially occupy high-density regions, in qualitative agreement with the same comparison applied to simulations. Our results establish the feasibility of the CLAMATO survey, which aims to obtain Lyα forest spectra for ∼1000 SFGs over ∼1deg2 of the COSMOS field, in order to map out the intergalactic medium large-scale structure at 〈z〉 ∼ 2.3 over a large volume (100 h-1 Mpc)3.

Published
2014

2. Euclid preparation: XXXVIII. Spectroscopy of active galactic nuclei with NISP.

Author

Euclid Collaboration, Lusso, E., Fotopoulou, S., Selwood, M., Allevato, V., Calderone, G., Mancini, C., Mignoli, M., Scodeggio, M., Bisigello, L., Feltre, A., Ricci, F., La Franca, F., Vergani, D., Gabarra, L., Le Brun, V., Maiorano, E., Palazzi, E., Moresco, M., and Zamorani, G.

Subjects
DISTRIBUTION (Probability theory), BLACK holes, ACTIVE galactic nuclei, REDSHIFT, SUPERMASSIVE black holes, ASTROPHYSICS, SPECTROMETRY, GALAXY clusters
Abstract

The statistical distribution and evolution of key properties of active galactic nuclei (AGN), such as their accretion rate, mass, and spin, remains a subject of open debate in astrophysics. The ESA Euclid space mission, launched on July 1 2023, promises a breakthrough in this field. We create detailed mock catalogues of AGN spectra from the rest-frame near-infrared down to the ultraviolet – including emission lines – to simulate what Euclid will observe for both obscured (type 2) and unobscured (type 1) AGN. We concentrate on the red grisms of the NISP instrument, which will be used for the wide-field survey, opening a new window for spectroscopic AGN studies in the near-infrared. We quantify the efficiency in the redshift determination as well as in retrieving the emission line flux of the Hα+[N II] complex, as Euclid is mainly focused on this emission line, given that it is expected to be the brightest one in the probed redshift range. Spectroscopic redshifts are measured for 83% of the simulated AGN in the interval where the Hα is visible (i.e. 0.89 <  z <  1.83 at a line flux of > 2 × 10−16 erg s−1 cm−2, encompassing the peak of AGN activity at z ≃ 1 − 1.5) within the spectral coverage of the red grism. Outside this redshift range, the measurement efficiency decreases significantly. Overall, a spectroscopic redshift iscorrectly determined for about 90% of type 2 AGN down to an emission line flux of roughly 3 × 10−16 erg s−1 cm−2, and for type 1 AGN down to 8.5 × 10−16 erg s−1 cm−2. Recovered values for black hole mass show a small offset with respect to the input values by about 10%, but the agreement is good overall. With such a high spectroscopic coverage at z <  2, we will be able to measure AGN demography, scaling relations, and clustering from the epoch of the peak of AGN activity down to the present-day Universe for hundreds of thousands of AGN with homogeneous spectroscopic information. [ABSTRACT FROM AUTHOR]

Published
2024
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3. The VVDS: Early Results on the Large Scale Structure Distribution of Galaxies out to z~1.5

Author

Le Fèvre, O., Vettolani, G., Maccagni, D., Picat, J.P., Adami, C., Arnaboldi, M., Arnouts, S., Bardelli, S., Bolzonella, M., Bondi, M., Bottini, D., Busarello, G., Cappi, A., Ciliegi, P., Contini, T., Charlot, S., Foucaud, S., Franzetti, P., Garilli, B., Gavignaud, I., Guzzo, L., Ilbert, O., Iovino, A., Le Brun, V., Marano, B., Marinoni, C., McCracken, H.J., Mathez, G., Mazure, A., Mellier, Y., Meneux, B., Merluzzi, P., Merighi, R., Paltani, S., Pellò, R., Pollo, A., Pozzetti, L., Radovich, M., Rizzo, D., Scaramella, R., Scodeggio, M., Tresse, L., Zamorani, G., Zanichelli, A., Zucca, E., Renzini, Alvio, editor, and Bender, Ralf, editor

Published
2005
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4. Metal content of the circumgalactic medium around star-forming galaxies at z ∼ 2.6 as revealed by the VIMOS Ultra-Deep Survey

Author

Méndez-Hernández, H., primary, Cassata, P., additional, Ibar, E., additional, Amorín, R., additional, Aravena, M., additional, Bardelli, S., additional, Cucciati, O., additional, Garilli, B., additional, Giavalisco, M., additional, Guaita, L., additional, Hathi, N., additional, Koekemoer, A., additional, Le Brun, V., additional, Lemaux, B. C., additional, Maccagni, D., additional, Ribeiro, B., additional, Tasca, L., additional, Tejos, N., additional, Thomas, R., additional, Tresse, L., additional, Vergani, D., additional, Zamorani, G., additional, and Zucca, E., additional

Published
2022
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5. The Vimos Vlt Deep Survey: Redshift Distribution of a I AB ≤ 24 Sample, and the Effect of Environment on Galaxy Evolution

Author

Le Fevre, Olivier, Ilbert, O., Marinoni, C., Paltani, S., Vettolani, G., Tresse, L., Zucca, E., Adami, C., Arnaboldi, M., Arnouts, S., Bardelli, S., Bolzonella, M., Bondi, M., Bongiorno, A., Bottini, D., Busarello, G., Cappi, A., Charlot, S., Ciliegi, P., Contini, T., Foucaud, S., Franzetti, P., Garilli, B., Gavignaud, I., Gregorini, L., Guzzo, L., Iovino, A., Le Brun, V., Maccagni, D., Mancini, D., Marano, B., Mathez, G., Mazure, A., McCracken, H. J., Mellier, Y., Meneux, B., Merluzzi, P., Merighi, R., Pello, R., Picat, J. P., Pollo, A., Pozzetti, L., Radovich, M., Ripepi, V., Rizzo, D., Scaramella, R., Scodeggio, M., Zamorani, G., Zanichelli, A., Block, David L., editor, Puerari, Ivânio, editor, Freeman, Kenneth C., editor, Groess, Robert, editor, and Block, Elizabeth K., editor

Published
2004
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6. Deep Redshift Surveys: The VIMOS VLT Deep Survey (Invited)

Author

Le Fevre, O., Vettolani, G., Maccagni, D., Picat, J. P., Adami, C., Arnaboldi, M., Bardelli, S., Bottini, D., Busarello, G., Cappi, A., Contini, T., Charlot, S., Garilli, B., Gavignaud, I., Guzzo, L., Ilbert, O., Iovino, A., Le Brun, V., Marinoni, C., McCracken, H. J., Mathez, G., Mazure, A., Mellier, Y., Meneux, B., Merluzi, P., Paltani, S., Pelló, R., Radovich, M., Scaramella, R., Scodeggio, M., Tresse, L., Zamorani, G., Zanichelli, A., Zucca, E., Burton, W. B., editor, Kuijpers, J. M. E., editor, van den Heuvel, E. P. J., editor, van der Laan, H., editor, Appenzeler, I., editor, Bahcall, J. N., editor, Bertola, F., editor, Cassinelli, J. P., editor, Cesarsky, C. J., editor, Engvold, O., editor, McCray, R., editor, Murdin, P. G., editor, Pacini, F., editor, Radhakrishnan, V., editor, Sato, K., editor, Shu, F. H., editor, Somov, B. V., editor, Sunyaev, R. A., editor, Tanaka, Y., editor, Tremaine, S., editor, Weiss, N. O., editor, and Plionis, Manolis, editor

Published
2004
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7. The VVDS Data‐Reduction Pipeline: Introducing VIPGI, the VIMOS Interactive Pipeline and Graphical Interface

Author

Scodeggio, M., Franzetti, P., Garilli, B., Zanichelli, A., Paltani, S., Maccagni, D., Bottini, D., Le Brun, V., Contini, T., Scaramella, R., Adami, C., Bardelli, S., Zucca, E., Tresse, L., Ilbert, O., Foucaud, S., Iovino, A., Merighi, R., Zamorani, G., Gavignaud, I., Rizzo, D., McCracken, H. J., Le Fèvre, O., Picat, J. P., Vettolani, G., Arnaboldi, M., Arnouts, S., Bolzonella, M., Cappi, A., Charlot, S., Ciliegi, P., Guzzo, L., Marano, B., Marinoni, C., Mathez, G., Mazure, A., Meneux, B., Pellò, R., Pollo, A., Pozzetti, L., and Radovich, M.

Published
2005
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8. The VIMOS Integral Field Unit: Data‐Reduction Methods and Quality Assessment

Author

Zanichelli, A., Garilli, B., Scodeggio, M., Franzetti, P., Rizzo, D., Maccagni, D., Merighi, R., Picat, J. P., Le Fèvre, O., Foucaud, S., Bottini, D., Le Brun, V., Scaramella, R., Tresse, L., Vettolani, G., Adami, C., Arnaboldi, M., Arnouts, S., Bardelli, S., Bolzonella, M., Cappi, A., Charlot, S., Ciliegi, P., Contini, T., Gavignaud, I., Guzzo, L., Ilbert, O., Iovino, A., McCracken, H. J., Marano, B., Marinoni, C., Mathez, G., Mazure, A., Meneux, B., Paltani, S., Pellò, R., Pollo, A., Pozzetti, L., Radovich, M., Zamorani, G., and Zucca, E.

Published
2005
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9. The Very Large Telescope Visible Multi‐Object Spectrograph Mask Preparation Software

Author

Bottini, D., Garilli, B., Maccagni, D., Tresse, L., Le Brun, V., Le Fèvre, O., Picat, J. P., Scaramella, R., Scodeggio, M., Vettolani, G., Zanichelli, A., Adami, C., Arnaboldi, M., Arnouts, S., Bardelli, S., Bolzonella, M., Cappi, A., Charlot, S., Ciliegi, P., Contini, T., Foucaud, S., Franzetti, P., Guzzo, L., Ilbert, O., Iovino, A., McCracken, H. J., Marano, B., Marinoni, C., Mathez, G., Mazure, A., Meneux, B., Merighi, R., Paltani, S., Pollo, A., Pozzetti, L., Radovich, M., Zamorani, G., and Zucca, E.

Published
2005
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10. Less and more IGM-transmitted galaxies from z ∼ 2.7 to z ∼ 6 from VANDELS and VUDS

Author

Thomas, R., primary, Pentericci, L., additional, Le Fèvre, O., additional, Koekemoer, A. M., additional, Castellano, M., additional, Cimatti, A., additional, Fontanot, F., additional, Gargiulo, A., additional, Garilli, B., additional, Talia, M., additional, Amorín, R., additional, Bardelli, S., additional, Cristiani, S., additional, Cresci, G., additional, Franco, M., additional, Fynbo, J. P. U., additional, Hathi, N. P., additional, Hibon, P., additional, Khusanova, Y., additional, Le Brun, V., additional, Lemaux, B. C., additional, Mannucci, F., additional, Schaerer, D., additional, Zamorani, G., additional, and Zucca, E., additional

Published
2021
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11. A test of the nature of cosmic acceleration using galaxy redshift distortions

Author

Guzzo, L., Pierleoni, M., Meneux, B., Branchini, E., Le Fevre, O., Marinoni, C., Garilli, B., Blaizot, J., De Lucia, G., Pollo, A., McCracken, H. J., Bottini, D., Le Brun, V., Maccagni, D., Picat, J. P., Scaramella, R., Scodeggio, M., Tresse, L., Vettolani, G., Zanichelli, A., Adami, C., Arnouts, S., Bardelli, S., Bolzonella, M., Bongiorno, A., Cappi, A., Charlot, S., Ciliegi, P., Contini, T., Cucciati, O., de la Torre, S., Dolag, K., Foucaud, S., Franzetti, P., Gavignaud, I., Ilbert, O., Iovino, A., Lamareille, F., Marano, B., Mazure, A., Memeo, P., Merighi, R., Moscardini, L., Paltani, S., Pello, R., Perez-Montero, E., Pozzetti, L., Radovich, M., Vergani, D., Zamorani, G., and Zucca, E.

Subjects
Red shift -- Research -- Observations, Expanding universe -- Observations -- Research, Environmental issues, Science and technology, Zoology and wildlife conservation, Observations, Research
Abstract

Author(s): L. Guzzo (corresponding author) [1, 2, 3, 4]; M. Pierleoni [3]; B. Meneux [5]; E. Branchini [6]; O. Le Fèvre [7]; C. Marinoni [8]; B. Garilli [5]; J. Blaizot [...]

Published
2008
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12. Clinical spectrum, prognosis and estimated prevalence of DNAJB11-kidney disease

Author

Huynh, V.T., Audrézet, M.-P., Sayer, J.A., Ong, A.C., Lefevre, S., Le Brun, V., Després, A., Senum, S.R., Chebib, F., Barroso-Gil, M., Patel, C., Mallett, A.J., Goel, H., Mallawaarachchi, A.C., Van Eerde, A.M., Ponlot, E., Kribs, M., Le Meur, Y., Harris, P.C., and Cornec-Le Gall, E.

Abstract

Monoallelic mutations of DNAJB11 were recently described in seven pedigrees with atypical clinical presentations of autosomal dominant polycystic kidney disease. DNAJB11 encodes one of the main cofactors of the endoplasmic reticulum chaperon BiP, a heat-shock protein required for efficient protein folding and trafficking. Here we conducted an international collaborative study to better characterize the DNAJB11-associated phenotype. Thirteen different loss-of-function variants were identified in 20 new pedigrees (54 affected individuals) by targeted next-generation sequencing, whole-exome sequencing or whole-genome sequencing. Amongst the 77 patients (27 pedigrees) now in total reported, 32 reached end stage kidney disease (range, 55-89 years, median age 75); without a significant difference between males and females. While a majority of patients presented with non-enlarged polycystic kidneys, renal cysts were inconsistently identified in patients under age 45. Vascular phenotypes, including intracranial aneurysms, dilatation of the thoracic aorta and dissection of a carotid artery were present in four pedigrees. We accessed Genomics England 100,000 genomes project data, and identified pathogenic variants of DNAJB11 in nine of 3934 probands with various kidney and urinary tract disorders. The clinical diagnosis was cystic kidney disease for eight probands and nephrocalcinosis for one proband. No additional pathogenic variants likely explaining the kidney disease were identified. Using the publicly available GnomAD database, DNAJB11 genetic prevalence was calculated at 0.85/10.000 individuals. Thus, establishing a precise diagnosis in atypical cystic or interstitial kidney disease is crucial, with important implications in terms of follow-up, genetic counseling, prognostic evaluation, therapeutic management, and for selection of living kidney donors.

Published
2020

14. Estimating the galaxy two-point correlation function using a split random catalog

Author

Gargiulo, A., Cucciati, O., Garilli, B., Scodeggio, M., Bolzonella, M., Zamorani, G., De Lucia, G., Krywult, J., Guzzo, L., Granett, B. R., de la Torre, S., Abbas, U., Adami, C., Arnouts, S., Bottini, D., Cappi, A., Franzetti, P., Fritz, A., Haines, C., Hawken, A. J., Iovino, A., Le Brun, V., Le Fèvre, O., Maccagni, D., Małek, K., Marulli, F., Moutard, T., Polletta, M., Pollo, A., Tasca, L. A. M., Tojeiro, R., Vergani, D., Zanichelli, A., Bel, J., Branchini, E., Coupon, J., Ilbert, O., Moscardini, L., Peacock, J. A., Gargiulo, A., Cucciati, O., Garilli, B., Scodeggio, M., Bolzonella, M., Zamorani, G., De Lucia, G., Krywult, J., Guzzo, L., Granett, B. R., de la Torre, S., Abbas, U., Adami, C., Arnouts, S., Bottini, D., Cappi, A., Franzetti, P., Fritz, A., Haines, C., Hawken, A. J., Iovino, A., Le Brun, V., Le Fèvre, O., Maccagni, D., Małek, K., Marulli, F., Moutard, T., Polletta, M., Pollo, A., Tasca, L. A. M., Tojeiro, R., Vergani, D., Zanichelli, A., Bel, J., Branchini, E., Coupon, J., Ilbert, O., Moscardini, L., and Peacock, J. A.

Subjects
formation [galaxies], galaxies: evolution, galaxies: formation, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics::Galaxy Astrophysics, evolution [galaxies]
Abstract

We use the unparalleled statistics of the VIPERS survey to investigate the relation between the surface mean stellar mass density Sigma = M/(2 pi R-e(2)) of massive passive galaxies (MPGs, M >= 10(11) M-circle dot) and their local environment in the redshift range 0.5 2 x 10(11) M-circle dot, we find an excess of MPGs with low Sigma and a deficit of high-Sigma MPGs in the densest regions with respect to other environments. We interpret this result as due to the migration of some high-Sigma MPGs (= 0.8 migrate to the MPG population. Here, we investigate the Sigma-delta relation of MSFGs at z >= 0.8 and find that it is consistent within 1 sigma with that of low-Sigma MPGs at z = 0.8 are consistent in terms of number and environment with being the progenitors of low-Sigma MPGs at z < 0.8.

Published
2019

15. Obscured AGN at 1.5 < z < 3.0 from the zCOSMOS-deep Survey

Author

Mignoli, M., Feltre, A., Bongiorno, A., Calura, F., Gilli, R., Vignali, C., Zamorani, G., Lilly, S. J., Le Fèvre, O., Bardelli, S., Bolzonella, M., Bordoloi, R., Le Brun, V., Caputi, K. I., Cimatti, A., Diener, C., Garilli, B., Koekemoer, A. M., Maier, C., Mainieri, V., Peng, Y., Pérez Montero, E., Silverman, J. D., Zucca, E., Mignoli, M., Feltre, A., Bongiorno, A., Calura, F., Gilli, R., Vignali, C., Zamorani, G., Lilly, S. J., Le Fèvre, O., Bardelli, S., Bolzonella, M., Bordoloi, R., Le Brun, V., Caputi, K. I., Cimatti, A., Diener, C., Garilli, B., Koekemoer, A. M., Maier, C., Mainieri, V., Peng, Y., Pérez Montero, E., Silverman, J. D., and Zucca, E.

Subjects
galaxies: active, line: formation, galaxies: evolution, galaxies: fundamental parameter, quasars: emission line, X-rays: galaxie
Abstract

Context. The physics and demographics of high-redshift obscured active galactic nuclei (AGN) is still scarcely investigated. New samples of such objects, selected with different techniques, can provide useful insights into their physical properties.Aims. With the goal to determine the properties of the gas in the emitting region of type 2 AGN, in particular, the gas metal content, we exploit predictions from photoionization models, including new parameterizations for the distance of gas distribution from the central source and internal microturbulence in the emitting clouds, to interpret rest-frame UV spectral data.Methods. We selected a sample of 90 obscured (type 2) AGN with 1.45

Published
2019

16. The VIMOS Public Extragalactic Redshift Survey (VIPERS)

Author

Gargiulo, A., Cucciati, O., Garilli, B., Scodeggio, M., Bolzonella, M., Zamorani, G., De Lucia, G., Krywult, J., Guzzo, L., Granett, B. R., de la Torre, S., Abbas, U., Adami, C., Arnouts, S., Bottini, D., Cappi, A., Franzetti, P., Fritz, A., Haines, C., Hawken, A. J., Iovino, A., Le Brun, V., Le Fèvre, O., Maccagni, D., Małek, K., Marulli, F., Moutard, T., Polletta, M., Pollo, A., Tasca, L. A. M., Tojeiro, R., Vergani, D., Zanichelli, A., Bel, J., Branchini, E., Coupon, J., Ilbert, O., Moscardini, L., Peacock, J. A., Gargiulo, A., Cucciati, O., Garilli, B., Scodeggio, M., Bolzonella, M., Zamorani, G., De Lucia, G., Krywult, J., Guzzo, L., Granett, B. R., de la Torre, S., Abbas, U., Adami, C., Arnouts, S., Bottini, D., Cappi, A., Franzetti, P., Fritz, A., Haines, C., Hawken, A. J., Iovino, A., Le Brun, V., Le Fèvre, O., Maccagni, D., Małek, K., Marulli, F., Moutard, T., Polletta, M., Pollo, A., Tasca, L. A. M., Tojeiro, R., Vergani, D., Zanichelli, A., Bel, J., Branchini, E., Coupon, J., Ilbert, O., Moscardini, L., and Peacock, J. A.

Subjects
formation [galaxies], Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics::Galaxy Astrophysics, evolution [galaxies]
Abstract

We use the unparalleled statistics of the VIPERS survey to investigate the relation between the surface mean stellar mass density Sigma = M/(2 pi R-e(2)) of massive passive galaxies (MPGs, M >= 10(11) M-circle dot) and their local environment in the redshift range 0.5 2 x 10(11) M-circle dot, we find an excess of MPGs with low Sigma and a deficit of high-Sigma MPGs in the densest regions with respect to other environments. We interpret this result as due to the migration of some high-Sigma MPGs (= 0.8 migrate to the MPG population. Here, we investigate the Sigma-delta relation of MSFGs at z >= 0.8 and find that it is consistent within 1 sigma with that of low-Sigma MPGs at z = 0.8 are consistent in terms of number and environment with being the progenitors of low-Sigma MPGs at z < 0.8.

Published
2019

17. UV and Lyα luminosity functions of galaxies and star formation rate density at the end of HI reionization from the VIMOS UltraDeep Survey (VUDS)

Author

Khusanova, Y., primary, Le Fèvre, O., additional, Cassata, P., additional, Cucciati, O., additional, Lemaux, B. C., additional, Tasca, L. A. M., additional, Thomas, R., additional, Garilli, B., additional, Le Brun, V., additional, Maccagni, D., additional, Pentericci, L., additional, Zamorani, G., additional, Amorín, R., additional, Bardelli, S., additional, Castellano, M., additional, Cassarà, L. P., additional, Cimatti, A., additional, Giavalisco, M., additional, Hathi, N. P., additional, Ilbert, O., additional, Koekemoer, A. M., additional, Marchi, F., additional, Pforr, J., additional, Ribeiro, B., additional, Schaerer, D., additional, Tresse, L., additional, Vergani, D., additional, and Zucca, E., additional

Published
2020
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22. A large population of galaxies 9 to 12 billion years back in the history of the Universe

Author

Le Fèvre, O., Paltani, S., Arnouts, S., Charlot, S., Foucaud, S., Ilbert, O., McCracken, H. J., Zamorani, G., Bottini, D., Garilli, B., Le Brun, V., Maccagni, D., Picat, J. P., Scaramella, R., Scodeggio, M., Tresse, L., Vettolani, G., Zanichelli, A., Adami, C., Bardelli, S., Bolzonella, M., Cappi, A., Ciliegi, P., Contini, T., Franzetti, P., Gavignaud, I., Guzzo, L., Iovino, A., Marano, B., Marinoni, C., Mazure, A., Meneux, B., Merighi, R., Pellò, R., Pollo, A., Pozzetti, L., Radovich, M., Zucca, E., Arnaboldi, M., Bondi, M., Bongiorno, A., Busarello, G., Gregorini, L., Lamareille, F., Mathez, G., Mellier, Y., Merluzzi, P., Ripepi, V., and Rizzo, D.

Published
2005

23. The VIMOS Public Extragalactic Redshift Survey (VIPERS)

Author

Scodeggio, M., Guzzo, L., Garilli, B., Granett, B. R., Bolzonella, M., de la Torre, S., Abbas, U., Adami, C., Arnouts, S., Bottini, D., Cappi, A., Coupon, J., Cucciati, O., Davidzon, I., Franzetti, P., Fritz, A., Iovino, Andrea, Krywult, J., Le Brun, V., Le Fèvre, O., Maccagni, D., Małek, K., Marchetti, A., Marulli, Federico, Polletta, M., Pollo, A., Tasca, L. A. M., Tojeiro, R., Vergani, D., Zanichelli, A., Bel, J., Branchini, E., DE LUCIA, Gabriella, Ilbert, O., Mccracken, H. J., Moutard, T., Peacock, J. A., Zamorani, G., Burden, A., Fumana, M., Jullo, E., Marinoni, Charles, Mellier, Y., Moscardini, L., Percival, W. J., Scodeggio, M., Guzzo, L., Garilli, B., Granett, B. R., Bolzonella, M., de la Torre, S., Abbas, U., Adami, C., Arnouts, S., Bottini, D., Cappi, A., Coupon, J., Cucciati, O., Davidzon, I., Franzetti, P., Fritz, A., Iovino, Andrea, Krywult, J., Le Brun, V., Le Fèvre, O., Maccagni, D., Małek, K., Marchetti, A., Marulli, Federico, Polletta, M., Pollo, A., Tasca, L. A. M., Tojeiro, R., Vergani, D., Zanichelli, A., Bel, J., Branchini, E., DE LUCIA, Gabriella, Ilbert, O., Mccracken, H. J., Moutard, T., Peacock, J. A., Zamorani, G., Burden, A., Fumana, M., Jullo, E., Marinoni, Charle, Mellier, Y., Moscardini, L., and Percival, W. J.

Published
2018

25. The VIMOS Public Extragalactic Redshift Survey (VIPERS)

Author

Gargiulo, A., primary, Cucciati, O., additional, Garilli, B., additional, Scodeggio, M., additional, Bolzonella, M., additional, Zamorani, G., additional, De Lucia, G., additional, Krywult, J., additional, Guzzo, L., additional, Granett, B. R., additional, de la Torre, S., additional, Abbas, U., additional, Adami, C., additional, Arnouts, S., additional, Bottini, D., additional, Cappi, A., additional, Franzetti, P., additional, Fritz, A., additional, Haines, C., additional, Hawken, A. J., additional, Iovino, A., additional, Le Brun, V., additional, Le Fèvre, O., additional, Maccagni, D., additional, Małek, K., additional, Marulli, F., additional, Moutard, T., additional, Polletta, M., additional, Pollo, A., additional, Tasca, L. A. M., additional, Tojeiro, R., additional, Vergani, D., additional, Zanichelli, A., additional, Bel, J., additional, Branchini, E., additional, Coupon, J., additional, Ilbert, O., additional, Moscardini, L., additional, and Peacock, J. A., additional

Published
2019
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26. Obscured AGN at 1.5 < 3.0 from the zCOSMOS-deep Survey

Author

Mignoli, M., primary, Feltre, A., additional, Bongiorno, A., additional, Calura, F., additional, Gilli, R., additional, Vignali, C., additional, Zamorani, G., additional, Lilly, S. J., additional, Le Fèvre, O., additional, Bardelli, S., additional, Bolzonella, M., additional, Bordoloi, R., additional, Le Brun, V., additional, Caputi, K. I., additional, Cimatti, A., additional, Diener, C., additional, Garilli, B., additional, Koekemoer, A. M., additional, Maier, C., additional, Mainieri, V., additional, Peng, Y., additional, Pérez Montero, E., additional, Silverman, J. D., additional, and Zucca, E., additional

Published
2019
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28. The VIMOS Ultra Deep Survey: The role of HI kinematics and HI column density on the escape of Lyα photons in star-forming galaxies at 2 < z < 4

Author

Guaita, L, Talia, M, Pentericci, L, Verhamme, A, Cassata, P, Lemaux, BC, Orlitova, I, Ribeiro, B, Schaerer, D, Zamorani, G, Garilli, B, Le Brun, V, Le Fèvre, O, MacCagni, D, Tasca, LAM, Thomas, R, Vanzella, E, Zucca, E, Amorin, R, Bardelli, S, Castellano, M, Grazian, A, Hathi, NP, Koekemoer, A, and Marchi, F

Subjects
ISM: kinematics and dynamics, techniques: imaging spectroscopy, galaxies: high-redshift, galaxies: star formation, scattering
Abstract

© 2017 ESO. Aims. We wish to assess the role of kinematics and neutral hydrogen column density in the escape and distribution of Lya photons. Methods. We selected a sample of 76 Lya emitting galaxies from the VIMOS Ultra Deep Survey (VUDS) at 2 = z = 4. We estimated the velocity of the neutral gas flowing out of the interstellar medium as the velocity offset, δv, between the systemic redshift (zsys) and the center of low-ionization absorption line systems (LIS). To increase the S/N of VUDS spectra, we stacked subsamples defined based on median values of their photometric and spectroscopic properties. We measured the systemic redshift from the rest-frame UV spectroscopic data using the CIII]1908 nebular emission line, and we considered SiII1526 as the highest signal-to-noise LIS line. We calculated the Lya peak shift with respect to the zsys, the EW(Lya), and the Lya spatial extension, Ext(Lya-C), from the in the 2D stacked spectra. Results. The galaxies that are faint in the rest-frame UV continuum, strong in Lya and CIII] , with compact UV morphology, and localized in an underdense environment are characterized by outflow velocities of the order of a few hundreds of km s -1 . The subsamples with smaller δv are characterized by larger Lya peak shifts, larger Ext(Lya-C), and smaller EW(Lya). In general we find that EW(Lya) anti-correlates with Ext(Lya-C) and Lya peak shift. Conclusions. We interpret these trends using a radiative-transfer shell model. The model predicts that an HI gas with a column density larger than 1020 cm -2 is able to produce Lya peak shifts larger than > 300 km s -1 . An ISM with this value of NHI would favour a large amount of scattering events, especially when the medium is static, so it can explain large values of Ext(Lya-C) and small EW(Lya). On the contrary, an ISM with a lower NHI, but large velocity outflows would lead to a Lya spatial profile peaked at the galaxy center (i.e. low values of Ext(Lya-C)) and to a large EW(Lya), as we see in our data. Our results and their interpretation via radiative-transfer models tell us that it is possible to use Lya to study the properties of the HI gas. Also, the fact that Lya emitters are characterized by large δv could give hints about their stage of evolution in the sense that they could be experiencing short bursts of star formation that push strong outflows., This work is supported by funding from the European Research Council Advanced Grant ERC–2010–AdG–268107–EARLY and by INAF Grants PRIN 2010, PRIN 2012, and PICS 2013. This work is based on data products made available at the CESAM data center, Laboratoire d’Astrophysique de Marseille, France. R.A. acknowledges support from the ERC Advanced Grant 695671 “QUENCH” and I.O. from the Czech Science Foundation grant 17-06217Y.

Published
2017
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29. The zCOSMOS survey

Author

Zucca E., Bardelli S., Bolzonella M., Zamorani G., Ilbert O., Pozzetti L., Mignoli M., Kova, #269, Lilly S., Tresse L., Tasca L., Cassata P., Halliday C., Vergani D., Caputi K., Carollo C. M., Contini T., Kneib J. P., Le Fèvre O., Mainieri V., Renzini A., Scodeggio M., Bongiorno A., Coppa G., de La Torre S., de Ravel L., Franzetti P., Garilli B., Iovino A., Kampczyk P., Knobel C., Lamareille F., Le Borgne J. F., Le Brun V., Maier C., Pellò R., Peng Y., Perez Montero E., Ricciardelli E., Silverman J. D., Tanaka M., Abbas U., Bottini D., Cappi A., Guzzo L., Koekemoer A. M., Leauthaud A., Maccagni D., Marinoni C., McCracken H. J., Meme, P., Meneux B., Oesch P., Porciani C., Scaramella R., Arnouts S., Aussel H., Capak P., Kartaltepe J., Salvato M., Sanders D., Scoville N., Taniguchi Y., Thompson D., CUCCIATI, OLGA, CIMATTI, ANDREA, MORESCO, MICHELE ENNIO MARIA, INAF - Osservatorio Astronomico di Brera (OAB), Istituto Nazionale di Astrofisica (INAF), INAF - Osservatorio Astronomico di Bologna (OABO), Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), AUTRES, 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), INAF - Osservatorio Astrofisico di Arcetri (OAA), University of Chicago, Laboratoire Astrophysique de Toulouse-Tarbes (LATT), 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), INAF- Milano, Dipartimento di Fisica, Università degli Studi di Milano-Bicocca = University of Milano-Bicocca (UNIMIB)-Università degli Studi di Milano = University of Milan (UNIMI), Institute of Astronomy [ETH Zürich], Department of Physics [ETH Zürich] (D-PHYS), Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology [Zürich] (ETH Zürich)- Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology [Zürich] (ETH Zürich), Tokai University, Istituto di Astrofisica Spaziale e Fisica cosmica - Bologna (IASF-Bo), Space Telescope Science Institute (STSci), Centre de Physique Théorique - UMR 6207 (CPT), Université de la Méditerranée - Aix-Marseille 2-Université de Provence - Aix-Marseille 1-Université de Toulon (UTLN)-Centre National de la Recherche Scientifique (CNRS), Centre de Physique Théorique - UMR 7332 (CPT), Aix Marseille Université (AMU)-Université de Toulon (UTLN)-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), Max-Planck-Institut für Astronomie (MPIA), Max-Planck-Gesellschaft, Materials & Process technology, Boeing Company [Chicago], California Institute of Technology (CALTECH), Sea Mammal Research Unit, St Andrews, Astronomy, Zucca E., Bardelli S., Bolzonella M., Zamorani G., Ilbert O., Pozzetti L., Mignoli M., Kova&#269, K., Lilly S., Tresse L., Tasca L., Cassata P., Halliday C., Vergani D., Caputi K., Carollo C. M., Contini T., Kneib J.-P., Le Fèvre O., Mainieri V., Renzini A., Scodeggio M., Bongiorno A., Coppa G., Cucciati O., de La Torre S., de Ravel L., Franzetti P., Garilli B., Iovino A., Kampczyk P., Knobel C., Lamareille F., Le Borgne J.-F., Le Brun V., Maier C., Pellò R., Peng Y., Perez-Montero E., Ricciardelli E., Silverman J. D., Tanaka M., Abbas U., Bottini D., Cappi A., Cimatti A., Guzzo L., Koekemoer A. M., Leauthaud A., Maccagni D., Marinoni C., McCracken H. J., Meme, P., Meneux B., Moresco M., Oesch P., Porciani C., Scaramella R., Arnouts S., Aussel H., Capak P., Kartaltepe J., Salvato M., Sanders D., Scoville N., Taniguchi Y., Thompson D., Università di Bologna, Dipartimento di Astronomia, 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), Centre National de la Recherche Scientifique (CNRS)-Observatoire Midi-Pyrénées (OMP), 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)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées, Università degli Studi di Milano-Bicocca [Milano] (UNIMIB)-Università degli Studi di Milano [Milano] (UNIMI), Centre National de la Recherche Scientifique (CNRS)-Université de Toulon (UTLN)-Université de Provence - Aix-Marseille 1-Université de la Méditerranée - Aix-Marseille 2, and Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC)

Subjects
Normalization (statistics), Cosmology and Nongalactic Astrophysics (astro-ph.CO), High density, FOS: Physical sciences, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Surveys, 01 natural sciences, Luminosity, [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], MORPHOLOGICAL CLASSIFICATION, 1ST EPOCH DATA, 0103 physical sciences, Astrophysics::Solar and Stellar Astrophysics, Density field, FIELD, 10. No inequality, 010303 astronomy & astrophysics, PHOTOMETRIC REDSHIFTS, Astrophysics::Galaxy Astrophysics, galaxies: statistics, Luminosity function (astronomy), Physics, REDSHIFT SURVEY, LEGACY SURVEY, 010308 nuclear & particles physics, Galaxies: evolution, Galaxies: luminosity function, mass function, Galaxies: statistics, Astronomy and Astrophysics, Space and Planetary Science, VLT DEEP SURVEY, B band, Galaxy, galaxies: luminosity function, mass function, COLOR-DENSITY RELATION, galaxies: luminosity function, mass function, DIGITAL SKY SURVEY, galaxies: evolution, Cosmic time, SURVEY COSMOS, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

(Abridged) We studied the evolution in the B band luminosity function to z~1 in the zCOSMOS 10k sample, for which both accurate galaxy classifications and a detailed description of the local density field are available. The global LF exhibits a brightening of ~0.7 mag in M* from z~0.2 to z~0.9. At low z, late types dominate at faint magnitudes, while the bright end is populated mainly by early types. At higher z, late-type galaxies evolve significantly and, at z~1, the contribution from the various types to the bright end of the LF is comparable. The evolution for early types is in both luminosity and normalization. A similar behaviour is exhibited by late types, but with an opposite trend for the normalization. Studying the role of the environment, we find that the global LF of galaxies in overdense regions has always a brighter M* and a flatter slope. In low density environments, the main contribution to the LF is from blue galaxies, while for high density environments there is an important contribution from red galaxies to the bright end. The differences between the global LF in the two environments are not due to only a difference in the relative numbers of red and blue galaxies, but also to their relative luminosity distributions: the value of M* for both types in underdense regions is always fainter than in overdense environments. The "specular" evolution of late- and early-type galaxies is consistent with a scenario where a part of blue galaxies is transformed in red galaxies with increasing cosmic time, without significant changes in the fraction of intermediate-type galaxies. The bulk of this tranformation in overdense regions probably happened before z~1, while it is still ongoing at lower z in underdense environments., Comment: 18 pages, 10 figures, A&A in press

Published
2009
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32. The VIMOS Public Extragalactic Redshift Survey (VIPERS)

Author

Vergani, D., primary, Garilli, B., additional, Polletta, M., additional, Franzetti, P., additional, Scodeggio, M., additional, Zamorani, G., additional, Haines, C. P., additional, Bolzonella, M., additional, Guzzo, L., additional, Granett, B. R., additional, de la Torre, S., additional, Abbas, U., additional, Adami, C., additional, Bottini, D., additional, Cappi, A., additional, Cucciati, O., additional, Davidzon, I., additional, De Lucia, G., additional, Fritz, A., additional, Gargiulo, A., additional, Hawken, A. J., additional, Iovino, A., additional, Krywult, J., additional, Le Brun, V., additional, Le Fèvre, O., additional, Maccagni, D., additional, Małek, K., additional, Marulli, F., additional, Pollo, A., additional, Tasca, L. A. M., additional, Tojeiro, R., additional, Zanichelli, A., additional, Arnouts, S., additional, Bel, J., additional, Branchini, E., additional, Coupon, J., additional, Ilbert, O., additional, Moutard, T., additional, and Moscardini, L., additional

Published
2018
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33. The progeny of a cosmic titan: a massive multi-component proto-supercluster in formation at z = 2.45 in VUDS

Author

Cucciati, O., primary, Lemaux, B. C., additional, Zamorani, G., additional, Le Fèvre, O., additional, Tasca, L. A. M., additional, Hathi, N. P., additional, Lee, K.-G., additional, Bardelli, S., additional, Cassata, P., additional, Garilli, B., additional, Le Brun, V., additional, Maccagni, D., additional, Pentericci, L., additional, Thomas, R., additional, Vanzella, E., additional, Zucca, E., additional, Lubin, L. M., additional, Amorin, R., additional, Cassarà, L. P., additional, Cimatti, A., additional, Talia, M., additional, Vergani, D., additional, Koekemoer, A., additional, Pforr, J., additional, and Salvato, M., additional

Published
2018
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34. The VIMOS Public Extragalactic Redshift Survey (VIPERS)

Author

Mohammad, F. G., primary, Bianchi, D., additional, Percival, W. J., additional, de la Torre, S., additional, Guzzo, L., additional, Granett, B. R., additional, Branchini, E., additional, Bolzonella, M., additional, Garilli, B., additional, Scodeggio, M., additional, Abbas, U., additional, Adami, C., additional, Bel, J., additional, Bottini, D., additional, Cappi, A., additional, Cucciati, O., additional, Davidzon, I., additional, Franzetti, P., additional, Fritz, A., additional, Iovino, A., additional, Krywult, J., additional, Le Brun, V., additional, Le Fèvre, O., additional, Małek, K., additional, Marulli, F., additional, Polletta, M., additional, Pollo, A., additional, Tasca, L. A. M., additional, Tojeiro, R., additional, Vergani, D., additional, Zanichelli, A., additional, Arnouts, S., additional, Coupon, J., additional, De Lucia, G., additional, Ilbert, O., additional, Moscardini, L., additional, and Moutard, T., additional

Published
2018
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35. The VIMOS Public Extragalactic Redshift Survey (VIPERS)

Author

Siudek, M., primary, Małek, K., additional, Pollo, A., additional, Krakowski, T., additional, Iovino, A., additional, Scodeggio, M., additional, Moutard, T., additional, Zamorani, G., additional, Guzzo, L., additional, Garilli, B., additional, Granett, B. R., additional, Bolzonella, M., additional, de la Torre, S., additional, Abbas, U., additional, Adami, C., additional, Bottini, D., additional, Cappi, A., additional, Cucciati, O., additional, Davidzon, I., additional, Franzetti, P., additional, Fritz, A., additional, Krywult, J., additional, Le Brun, V., additional, Le Fèvre, O., additional, Maccagni, D., additional, Marulli, F., additional, Polletta, M., additional, Tasca, L. A.M., additional, Tojeiro, R., additional, Vergani, D., additional, Zanichelli, A., additional, Arnouts, S., additional, Bel, J., additional, Branchini, E., additional, Coupon, J., additional, De Lucia, G., additional, Ilbert, O., additional, Haines, C. P., additional, Moscardini, L., additional, and Takeuchi, T. T., additional

Published
2018
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39. The VIMOS Public Extragalactic Redshift Survey

Author

Granett, B. R., Branchini, ENZO FRANCO, Guzzo, L., Abbas, U., Adami, C., Arnouts, S., Bel, J., Bolzonella, M., Bottini, D., Cappi, A., Coupon, J., Cucciati, O., Davidzon, I., De Lucia, G., de la Torre, S., Fritz, A., Franzetti, P., Fumana, M., Garilli, B., Ilbert, O., Iovino, A., Krywult, J., Le Brun, V., Le Fèvre, O., Maccagni, D., Małek, K., Marulli, F., Mccracken, H. J., Polletta, M., Pollo, A., Scodeggio, M., Tasca, L. A. M., Tojeiro, R., Vergani, D., Zanichelli, A., Burden, A., Di Porto, C., Marchetti, A., Marinoni, C., Mellier, Y., Moutard, T., Moscardini, L., Nichol, R. C., Peacock, J. A., Percival, W. J., Zamorani, G., Granett, B. R., Branchini, ENZO FRANCO, Guzzo, L., Abbas, U., Adami, C., Arnouts, S., Bel, J., Bolzonella, M., Bottini, D., Cappi, A., Coupon, J., Cucciati, O., Davidzon, I., De Lucia, G., de la Torre, S., Fritz, A., Franzetti, P., Fumana, M., Garilli, B., Ilbert, O., Iovino, A., Krywult, J., Le Brun, V., Le Fèvre, O., Maccagni, D., Małek, K., Marulli, F., Mccracken, H. J., Polletta, M., Pollo, A., Scodeggio, M., Tasca, L. A. M., Tojeiro, R., Vergani, D., Zanichelli, A., Burden, A., Di Porto, C., Marchetti, A., Marinoni, C., Mellier, Y., Moutard, T., Moscardini, L., Nichol, R. C., Peacock, J. A., Percival, W. J., and Zamorani, G.

Subjects
methods: statistical, large-scale structure of Universe, cosmology: observations, galaxies: statistics, cosmological parameters, methods: data analysis, observations, galaxies: statistics, cosmological parameters, methods: statistical, methods: data analysis [large-scale structure of Universe, cosmology], Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics::Galaxy Astrophysics
Abstract

Aims: Using the VIMOS Public Extragalactic Redshift Survey (VIPERS) we aim to jointly estimate the keyparameters that describe the galaxy density field and its spatial correlations in redshift space. Methods: We use the Bayesian formalism to jointly reconstruct the redshift-space galaxy density field, power spectrum, galaxy bias and galaxy luminosity function given the observations and survey selection function. The high-dimensional posterior distribution is explored using the Wiener filter within a Gibbs sampler. We validate the analysis using simulated catalogues and apply it to VIPERS data taking into consideration the inhomogeneous selection function. Results: We present joint constraints on the anisotropic power spectrum, and the bias and number density of red and blue galaxy classes in luminosity and redshift bins as well as the measurement covariances of these quantities. We find that the inferred galaxy bias and number density parameters are strongly correlated although they are only weakly correlated with the galaxy power spectrum. The power spectrum and redshift-space distortion parameters are in agreement with previous VIPERS results with the value of the growth rate fσ8 = 0.38 with 18% uncertainty at redshift 0.7.

Published
2015

40. VizieR Online Data Catalog: COSMOS photometric redshift catalog (Ilbert+, 2009)

Author

Ilbert, O., Capak, P., Salvato, M., Aussel, H., Mccracken, H. J., Sanders, D. B., Scoville, N., Kartaltepe, J., Arnouts, S., Le Floc H, E., Mobasher, B., Taniguchi, Y., Lamareille, F., Leauthaud, A., Sasaki, S., Thompson, D., Zamojski, M., Zamorani, G., Bardelli, S., Bolzonella, M., Angela Bongiorno, Brusa, M., Caputi, K. I., Carollo, C. M., Contini, T., Cook, R., Coppa, G., Cucciati, O., La Torre, S., Ravel, L., Franzetti, P., Garilli, B., Hasinger, G., Iovino, A., Kampczyk, P., Kneib, J. -P, Knobel, C., Kovac, K., Le Borgne, J. F., Le Brun, V., Fevre, O. L., Lilly, S., Looper, D., Maier, C., Mainieri, V., Mellier, Y., Mignoli, M., Murayama, T., Pello, R., Peng, Y., Perez-Montero, E., Renzini, A., Ricciardelli, E., Schiminovich, D., Scodeggio, M., Shioya, Y., Silverman, J., Surace, J., Tanaka, M., Tasca, L., Tresse, L., Vergani, D., Zucca, E., 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
Photometry, [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Redshifts, Surveys, Galaxy catalogs
Published
2017

41. The VIMOS Public Extragalactic Redshift Survey (VIPERS): The growth of structure at 0.5 < z < 1.2 from redshift-space distortions in the clustering of the PDR-2 final sample

Author

Pezzotta , A., De La Torre , S., Bel , J., Granett , B.R., Guzzo , L., Peacock , J.A., Garilli , B., Scodeggio , M., Bolzonella , M., Abbas , U., Adami , C., Bottini , D., Cappi , A., Cucciati , O., Davidzon , I., Franzetti , P., Fritz , A., Iovino , A., Krywult , J., Le Brun , V., Fèvre , O., Maccagni , D., Małek , K., Marulli , F., Polletta , M., Pollo , A., Tasca , L.A.M., Tojeiro , R., Vergani , D., Zanichelli , A., Arnouts , S., Branchini , E., Coupon , J., De Lucia , G., Koda , J., Ilbert , O., Moutard , T., Moscardini , L., 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 ), Centre de Physique Théorique - UMR 7332 ( CPT ), Aix Marseille Université ( AMU ) -Université de Toulon ( UTLN ) -Centre National de la Recherche Scientifique ( CNRS ), Joseph Louis LAGRANGE ( LAGRANGE ), Université Nice Sophia Antipolis ( UNS ), Université Côte d'Azur ( UCA ) -Université Côte d'Azur ( UCA ) -Observatoire de la Côte d'Azur, Université Côte d'Azur ( UCA ) -Centre National de la Recherche Scientifique ( CNRS ), Université de la Méditerranée - Aix-Marseille 2, Institut de recherche en astrophysique et planétologie ( IRAP ), and Université Paul Sabatier - Toulouse 3 ( UPS ) -Observatoire Midi-Pyrénées ( OMP ) -Centre National de la Recherche Scientifique ( CNRS )

Subjects
galaxies: high-redshift, cosmology: observations, [ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph], large-scale structure of Universe, galaxies: statistics
Abstract

International audience; We present measurements of the growth rate of cosmological structure from the modelling of the anisotropic galaxy clustering measured in the final data release of the VIPERS survey. The analysis is carried out in configuration space and based on measurements of the first two even multipole moments of the anisotropic galaxy auto-correlation function, in two redshift bins spanning the range 0.5

Published
2017
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42. The VIMOS Public Extragalactic Redshift Survey (VIPERS)

Author

Scodeggio, M., primary, Guzzo, L., additional, Garilli, B., additional, Granett, B. R., additional, Bolzonella, M., additional, de la Torre, S., additional, Abbas, U., additional, Adami, C., additional, Arnouts, S., additional, Bottini, D., additional, Cappi, A., additional, Coupon, J., additional, Cucciati, O., additional, Davidzon, I., additional, Franzetti, P., additional, Fritz, A., additional, Iovino, A., additional, Krywult, J., additional, Le Brun, V., additional, Le Fèvre, O., additional, Maccagni, D., additional, Małek, K., additional, Marchetti, A., additional, Marulli, F., additional, Polletta, M., additional, Pollo, A., additional, Tasca, L. A. M., additional, Tojeiro, R., additional, Vergani, D., additional, Zanichelli, A., additional, Bel, J., additional, Branchini, E., additional, De Lucia, G., additional, Ilbert, O., additional, McCracken, H. J., additional, Moutard, T., additional, Peacock, J. A., additional, Zamorani, G., additional, Burden, A., additional, Fumana, M., additional, Jullo, E., additional, Marinoni, C., additional, Mellier, Y., additional, Moscardini, L., additional, and Percival, W. J., additional

Published
2018
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43. The VIMOS Public Extragalactic Redshift Survey (VIPERS) Omega(m0) from the galaxy clustering ratio measured at z similar to 1

Author

Bel J., Marinoni C., Granett B. R., Guzzo L., Peacock J. A., Cucciati O., de la Torre S., Iovino A., Percival W. J., Steigerwald H., Abbas U., Adami C., Arnouts S., Bolzonella M., Bottini D., Cappi A., Coupon J., Davidzon I., De Lucia G., Fritz A., Franzetti P., Fumana M., Garilli B., Ilbert O., Krywult J., Le Brun V., Le Fevre O., Maccagni D., Malek K., Marulli F., McCracken H. J., Paioro L., Polletta M., Pollo A., Schlagenhaufer H., Scodeggio M., Tasca L. A. M., Tojeiro R., Vergani D., Zanichelli A., Burden A., Di Porto C., Marchetti A., Mellier Y., Moscardini L., Nichol R. C., Phleps S., Wolk M., Zamorani G., BRANCHINI, ENZO FRANCO, Bel, J., Marinoni, C., Granett, B. R., Guzzo, L., Peacock, J. A., Branchini, ENZO FRANCO, Cucciati, O., de la Torre, S., Iovino, A., Percival, W. J., Steigerwald, H., Abbas, U., Adami, C., Arnouts, S., Bolzonella, M., Bottini, D., Cappi, A., Coupon, J., Davidzon, I., De Lucia, G., Fritz, A., Franzetti, P., Fumana, M., Garilli, B., Ilbert, O., Krywult, J., Le Brun, V., Le Fevre, O., Maccagni, D., Malek, K., Marulli, F., Mccracken, H. J., Paioro, L., Polletta, M., Pollo, A., Schlagenhaufer, H., Scodeggio, M., Tasca, L. A. M., Tojeiro, R., Vergani, D., Zanichelli, A., Burden, A., Di Porto, C., Marchetti, A., Mellier, Y., Moscardini, L., Nichol, R. C., Phleps, S., Wolk, M., and Zamorani, G.

Published
2014

44. Measuring Large-Scale Structure atz∼ 1 with the VIPERS galaxy survey

Author

GUZZO, Luigi, Abbas, U., Adami, Christophe, Arnouts, Stephane, Bel, Julien, Bolzonella, M., Bottini, D., Branchini, Enzo Franco, Burden, Angela, Cappi, A., Coupon, Jean, Cucciati, O., Davidzon, Iary, de la Torre, Silvain, De Lucia, G., Di Porto, Cinzia, Franzetti, P., Fritz, Alexander, Fumana, M., GARILLI, BIANCA MARIA ROSA, Granett, B. R., Guennou, L., Hawken, A., Ilbert, O., Iovino, A., Krywult, J., Le Brun, V., Le Fevre, O., Maccagni, D., Malek, K., Marchetti, A., Marinoni, C., Marulli, F., McCracken, H. J., Mellier, Y., Moscardini, L., Nichol, R. C., Paioro, L., Peacock, J. A., Percival, W. J., Phleps, S., POLLETTA, MARIA DEL CARMEN, Pollo, A., Rota, S., Schlagenhaufer, H., SCODEGGIO, MARCO, Solarz, A., Tasca, L. A. M., Tojeiro, R., VERGANI, DANIELA, Wolk, M., Zamorani, G., and ZANICHELLI, Alessandra

Subjects
Physics, Space and Planetary Science, Scale structure, Astronomy and Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, Astrophysics::Galaxy Astrophysics, Galaxy
Abstract

The VIMOS Public Extragalactic Redshift Survey (VIPERS) is the largest redshift survey ever conducted with the ESO telescopes. It has used the Very Large Telescope to collect nearly 100,000 redshifts from the general galaxy population at 0.5

Published
2016

45. The VIMOS Public Extragalactic Redshift Survey (VIPERS)

Author

de la Torre, S., primary, Jullo, E., additional, Giocoli, C., additional, Pezzotta, A., additional, Bel, J., additional, Granett, B. R., additional, Guzzo, L., additional, Garilli, B., additional, Scodeggio, M., additional, Bolzonella, M., additional, Abbas, U., additional, Adami, C., additional, Bottini, D., additional, Cappi, A., additional, Cucciati, O., additional, Davidzon, I., additional, Franzetti, P., additional, Fritz, A., additional, Iovino, A., additional, Krywult, J., additional, Le Brun, V., additional, Le Fèvre, O., additional, Maccagni, D., additional, Małek, K., additional, Marulli, F., additional, Polletta, M., additional, Pollo, A., additional, Tasca, L. A. M., additional, Tojeiro, R., additional, Vergani, D., additional, Zanichelli, A., additional, Arnouts, S., additional, Branchini, E., additional, Coupon, J., additional, De Lucia, G., additional, Ilbert, O., additional, Moutard, T., additional, Moscardini, L., additional, Peacock, J. A., additional, Metcalf, R. B., additional, Prada, F., additional, and Yepes, G., additional

Published
2017
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46. The VIMOS Public Extragalactic Redshift Survey

Author

Hawken, A. J., primary, Granett, B. R., additional, Iovino, A., additional, Guzzo, L., additional, Peacock, J. A., additional, de la Torre, S., additional, Garilli, B., additional, Bolzonella, M., additional, Scodeggio, M., additional, Abbas, U., additional, Adami, C., additional, Bottini, D., additional, Cappi, A., additional, Cucciati, O., additional, Davidzon, I., additional, Fritz, A., additional, Franzetti, P., additional, Krywult, J., additional, Le Brun, V., additional, Le Fèvre, O., additional, Maccagni, D., additional, Małek, K., additional, Marulli, F., additional, Polletta, M., additional, Pollo, A., additional, Tasca, L. A. M., additional, Tojeiro, R., additional, Vergani, D., additional, Zanichelli, A., additional, Arnouts, S., additional, Bel, J., additional, Branchini, E., additional, De Lucia, G., additional, Ilbert, O., additional, Moscardini, L., additional, and Percival, W. J., additional

Published
2017
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47. The VIMOS Public Extragalactic Redshift Survey (VIPERS)

Author

Gargiulo, A., primary, Bolzonella, M., additional, Scodeggio, M., additional, Krywult, J., additional, De Lucia, G., additional, Guzzo, L., additional, Garilli, B., additional, Granett, B. R., additional, de la Torre, S., additional, Abbas, U., additional, Adami, C., additional, Arnouts, S., additional, Bottini, D., additional, Cappi, A., additional, Cucciati, O., additional, Davidzon, I., additional, Franzetti, P., additional, Fritz, A., additional, Haines, C., additional, Hawken, A. J., additional, Iovino, A., additional, Le Brun, V., additional, Le Fèvre, O., additional, Maccagni, D., additional, Małek, K., additional, Marulli, F., additional, Moutard, T., additional, Polletta, M., additional, Pollo, A., additional, Tasca, L. A. M., additional, Tojeiro, R., additional, Vergani, D., additional, Zanichelli, A., additional, Zamorani, G., additional, Bel, J., additional, Branchini, E., additional, Coupon, J., additional, Ilbert, O., additional, Moscardini, L., additional, and Peacock, J. A., additional

Published
2017
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48. The VIMOS Ultra Deep Survey

Author

Guaita, L., primary, Talia, M., additional, Pentericci, L., additional, Verhamme, A., additional, Cassata, P., additional, Lemaux, B. C., additional, Orlitova, I., additional, Ribeiro, B., additional, Schaerer, D., additional, Zamorani, G., additional, Garilli, B., additional, Le Brun, V., additional, Le Fèvre, O., additional, Maccagni, D., additional, Tasca, L. A. M., additional, Thomas, R., additional, Vanzella, E., additional, Zucca, E., additional, Amorin, R., additional, Bardelli, S., additional, Castellano, M., additional, Grazian, A., additional, Hathi, N. P., additional, Koekemoer, A., additional, and Marchi, F., additional

Published
2017
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49. The VIMOS Public Extragalactic Redshift Survey (VIPERS)

Author

Haines, C. P., primary, Iovino, A., additional, Krywult, J., additional, Guzzo, L., additional, Davidzon, I., additional, Bolzonella, M., additional, Garilli, B., additional, Scodeggio, M., additional, Granett, B. R., additional, de la Torre, S., additional, De Lucia, G., additional, Abbas, U., additional, Adami, C., additional, Arnouts, S., additional, Bottini, D., additional, Cappi, A., additional, Cucciati, O., additional, Franzetti, P., additional, Fritz, A., additional, Gargiulo, A., additional, Le Brun, V., additional, Le Fèvre, O., additional, Maccagni, D., additional, Małek, K., additional, Marulli, F., additional, Moutard, T., additional, Polletta, M., additional, Pollo, A., additional, Tasca, L. A. M., additional, Tojeiro, R., additional, Vergani, D., additional, Zanichelli, A., additional, Zamorani, G., additional, Bel, J., additional, Branchini, E., additional, Coupon, J., additional, Ilbert, O., additional, Moscardini, L., additional, Peacock, J. A., additional, and Siudek, M., additional

Published
2017
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50. The VIMOS Public Extragalactic Redshift Survey (VIPERS)

Author

Moresco, M., primary, Marulli, F., additional, Moscardini, L., additional, Branchini, E., additional, Cappi, A., additional, Davidzon, I., additional, Granett, B. R., additional, de la Torre, S., additional, Guzzo, L., additional, Abbas, U., additional, Adami, C., additional, Arnouts, S., additional, Bel, J., additional, Bolzonella, M., additional, Bottini, D., additional, Carbone, C., additional, Coupon, J., additional, Cucciati, O., additional, De Lucia, G., additional, Franzetti, P., additional, Fritz, A., additional, Fumana, M., additional, Garilli, B., additional, Ilbert, O., additional, Iovino, A., additional, Krywult, J., additional, Le Brun, V., additional, Le Fèvre, O., additional, Małek, K., additional, McCracken, H. J., additional, Polletta, M., additional, Pollo, A., additional, Scodeggio, M., additional, Tasca, L. A. M., additional, Tojeiro, R., additional, Vergani, D., additional, and Zanichelli, A., additional

Published
2017
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