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95 results on '"Le Floch, E."'

1. The THESEUS space mission: science goals, requirements and mission concept

Author: Amati, L., O’Brien, P.T., Götz, D., Bozzo, E., Santangelo, A., Tanvir, N., Frontera, F., Mereghetti, S., Osborne, J. P., Blain, A., Basa, S., Branchesi, M., Burderi, L., Caballero-García, M., Castro-Tirado, A. J., Christensen, L., Ciolfi, R., De Rosa, A., Doroshenko, V., Ferrara, A., Ghirlanda, G., Hanlon, L., Heddermann, P., Hutchinson, I., Labanti, C., Le Floch, E., Lerman, H., Paltani, S., Reglero, V., Rezzolla, L., Rosati, P., Salvaterra, R., Stratta, G., and Tenzer, C.
Published: 2021
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2. Gamma ray burst studies with THESEUS

Author: Ghirlanda, G., Salvaterra, R., Toffano, M., Ronchini, S., Guidorzi, C., Oganesyan, G., Ascenzi, S., Bernardini, M. G., Camisasca, A. E., Mereghetti, S., Nava, L., Ravasio, M. E., Branchesi, M., Castro-Tirado, A., Amati, L., Blain, A., Bozzo, E., O’Brien, P., Götz, D., Le Floch, E., Osborne, J. P., Rosati, P., Stratta, G., Tanvir, N., Bogomazov, A. I., D’Avanzo, P., Hafizi, M., Mandhai, S., Melandri, A., Peer, A., Topinka, M., Vergani, S. D., and Zane, S.
Published: 2021
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3. Non-linearity and environmental dependence of the star-forming galaxies main sequence

Author: Erfanianfar, G, Popesso, P, Finoguenov, A, Wilman, D, Wuyts, S, Biviano, A, Salvato, M, Mirkazemi, M, Morselli, L, Ziparo, F, Nandra, K, Lutz, D, Elbaz, D, Dickinson, M, Tanaka, M, Altieri, MB, Aussel, H, Bauer, F, Berta, S, Bielby, RM, Brandt, N, Cappelluti, N, Cimatti, A, Cooper, MC, Fadda, D, Ilbert, O, Le Floch, E, Magnelli, B, Mulchaey, JS, Nordon, R, Newman, JA, Poglitsch, A, and Pozzi, F
Subjects: Space Sciences, Particle and High Energy Physics, Astronomical Sciences, Physical Sciences, Galaxy: evolution, Galaxy: structure, galaxies: groups: general, galaxies: haloes, galaxies: star formation, infrared: galaxies, astro-ph.GA, Astronomical and Space Sciences, Astronomy & Astrophysics, Astronomical sciences, Particle and high energy physics, Space sciences
Abstract: Using data from four deep fields (COSMOS, AEGIS, ECDFS, and CDFN), we studythe correlation between the position of galaxies in the star formation rate(SFR) versus stellar mass plane and local environment at $z10^{10.4-10.6}$ $M_{\odot}$), across all environments. At high redshift ($0.5
Published: 2016

4. The evolution of star formation activity in galaxy groups

Author: Erfanianfar, G, Popesso, P, Finoguenov, A, Wuyts, S, Wilman, D, Biviano, A, Ziparo, F, Salvato, M, Nandra, K, Lutz, D, Elbaz, D, Dickinson, M, Tanaka, M, Mirkazemi, M, Balogh, ML, Altieri, MB, Aussel, H, Bauer, F, Berta, S, Bielby, RM, Brandt, N, Cappelluti, N, Cimatti, A, Cooper, M, Fadda, D, Ilbert, O, Le Floch, E, Magnelli, B, Mulchaey, JS, Nordon, R, Newman, JA, Poglitsch, A, and Pozzi, F
Subjects: catalogues, galaxies: evolution, cosmology: observations, large-scale structure of Universe, infrared: galaxies, astro-ph.GA, Astronomical and Space Sciences, Astronomy & Astrophysics
Abstract: We study the evolution of the total star formation (SF) activity, total stellar mass (∑M*) and halo occupation distribution (HOD) in massive haloes by using one of the largest X-ray selected sample of galaxy groups with secure spectroscopic identification in the major blank field surveys (ECDFS, CDFN, COSMOS, AEGIS). We provide an accurate measurement of star formation rate (SFR) for the bulk of the star-forming galaxies using very deep mid-infrared Spitzer MIPS and far-infrared Herschel PACS observations. For undetected IR sources, we provide a well-calibrated SFR from spectral energy distribution (SED) fitting. We observe a clear evolution in the level of SF activity in galaxy groups. The total SF activity in the high-redshift groups (0.5 < z < 1.1) is higher with respect to the low-redshift (0.15 < z < 0.5) sample at any mass by 0.8 ± 0.12 dex. A milder difference (0.35 ± 0.1 dex) is observed between the low-redshift bin and the groups at z ~ 0. We show that the level of SF activity is declining more rapidly in the more massive haloes than in the more common lower mass haloes. We do not observe any evolution in the HOD and total stellar mass-halo mass relations in groups. The picture emerging from our findings suggests that the galaxy population in the most massive systems is evolving faster than galaxies in lower mass haloes, consistently with a 'halo downsizing' scenario.
Published: 2014

5. The THESEUS space mission concept: science case, design and expected performances

Author: Amati, L., O’Brien, P., Götz, D., Bozzo, E., Tenzer, C., Frontera, F., Ghirlanda, G., Labanti, C., Osborne, J.P., Stratta, G., Tanvir, N., Willingale, R., Attina, P., Campana, R., Castro-Tirado, A.J., Contini, C., Fuschino, F., Gomboc, A., Hudec, R., Orleanski, P., Renotte, E., Rodic, T., Bagoly, Z., Blain, A., Callanan, P., Covino, S., Ferrara, A., Le Floch, E., Marisaldi, M., Mereghetti, S., Rosati, P., Vacchi, A., D’Avanzo, P., Giommi, P., Piranomonte, S., Piro, L., Reglero, V., Rossi, A., Santangelo, A., Salvaterra, R., Tagliaferri, G., Vergani, S., Vinciguerra, S., Briggs, M., Campolongo, E., Ciolfi, R., Connaughton, V., Cordier, B., Morelli, B., Orlandini, M., Adami, C., Argan, A., Atteia, J.-L., Auricchio, N., Balazs, L., Baldazzi, G., Basa, S., Basak, R., Bellutti, P., Bernardini, M.G., Bertuccio, G., Braga, J., Branchesi, M., Brandt, S., Brocato, E., Budtz-Jorgensen, C., Bulgarelli, A., Burderi, L., Camp, J., Capozziello, S., Caruana, J., Casella, P., Cenko, B., Chardonnet, P., Ciardi, B., Colafrancesco, S., Dainotti, M.G., D’Elia, V., De Martino, D., De Pasquale, M., Del Monte, E., Della Valle, M., Drago, A., Evangelista, Y., Feroci, M., Finelli, F., Fiorini, M., Fynbo, J., Gal-Yam, A., Gendre, B., Ghisellini, G., Grado, A., Guidorzi, C., Hafizi, M., Hanlon, L., Hjorth, J., Izzo, L., Kiss, L., Kumar, P., Kuvvetli, I., Lavagna, M., Li, T., Longo, F., Lyutikov, M., Maio, U., Maiorano, E., Malcovati, P., Malesani, D., Margutti, R., Martin-Carrillo, A., Masetti, N., McBreen, S., Mignani, R., Morgante, G., Mundell, C., Nargaard-Nielsen, H.U., Nicastro, L., Palazzi, E., Paltani, S., Panessa, F., Pareschi, G., Pe’er, A., Penacchioni, A.V., Pian, E., Piedipalumbo, E., Piran, T., Rauw, G., Razzano, M., Read, A., Rezzolla, L., Romano, P., Ruffini, R., Savaglio, S., Sguera, V., Schady, P., Skidmore, W., Song, L., Stanway, E., Starling, R., Topinka, M., Troja, E., van Putten, M., Vanzella, E., Vercellone, S., Wilson-Hodge, C., Yonetoku, D., Zampa, G., Zampa, N., Zhang, B., Zhang, B.B., Zhang, S., Zhang, S.-N., Antonelli, A., Bianco, F., Boci, S., Boer, M., Botticella, M.T., Boulade, O., Butler, C., Campana, S., Capitanio, F., Celotti, A., Chen, Y., Colpi, M., Comastri, A., Cuby, J.-G., Dadina, M., De Luca, A., Dong, Y.-W., Ettori, S., Gandhi, P., Geza, E., Greiner, J., Guiriec, S., Harms, J., Hernanz, M., Hornstrup, A., Hutchinson, I., Israel, G., Jonker, P., Kaneko, Y., Kawai, N., Wiersema, K., Korpela, S., Lebrun, V., Lu, F., MacFadyen, A., Malaguti, G., Maraschi, L., Melandri, A., Modjaz, M., Morris, D., Omodei, N., Paizis, A., Páta, P., Petrosian, V., Rachevski, A., Rhoads, J., Ryde, F., Sabau-Graziati, L., Shigehiro, N., Sims, M., Soomin, J., Szécsi, D., Urata, Y., Uslenghi, M., Valenziano, L., Vianello, G., Vojtech, S., Watson, D., and Zicha, J.
Published: 2018
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6. Weak association between genetic markers of hyperuricemia and cardiorenal outcomes: insights from the STANISLAS study cohort with a 20-year follow-up

Author: Kanbay, Mehmet (ORCID 0000-0002-1297-0675 & YÖK ID 110580), Xhaard, C.; Le Floch, E.; Dandine-Roulland, C.; Girerd, N.; Ferreira, J.P.; Boivin, J.M.; Wagner, S.; Bacq Daian, D.; Deleuze, J.F.; Zannad, F.; Rossignol, P., School of Medicine, Kanbay, Mehmet (ORCID 0000-0002-1297-0675 & YÖK ID 110580), Xhaard, C.; Le Floch, E.; Dandine-Roulland, C.; Girerd, N.; Ferreira, J.P.; Boivin, J.M.; Wagner, S.; Bacq Daian, D.; Deleuze, J.F.; Zannad, F.; Rossignol, P., and School of Medicine
Abstract: Background: Hyperuricemia is associated with poor cardiovascular outcomes, although it is uncertain whether this relationship is causal in nature. This study aimed to: (1) assess the heritability of serum uric acid (SUA) levels, (2) conduct a genome-wide association study on SUA levels, and (3) investigate the association between certain single-nucleotide polymorphisms and target organ damage. Methods and results: the STANISLAS (Suivi Temporaire Annuel Non-Invasif de la Sante des Lorrains Assures Sociaux) study cohort is a single-center longitudinal cohort recruited between 1993 and 1995 (visit 1), with a last visit (visit 4 [V4]) performed approximate to 20 years apart. Serum lipid profile, SUA, urinary albumin/creatinine ratio, estimated glomerular filtration rate, 24-hour ambulatory blood pressure monitoring, transthoracic echocardiography, pulse wave velocity, and genotyping for each participant were assessed at V4. A total of 1573 participants were included at V4, among whom 1417 had available SUA data at visit 1. Genome-wide association study results highlighted multiple single-nucleotide polymorphisms on the SLC2A9 gene linked to SUA levels. Carriers of the most associated mutated SLC2A9 allele (rs16890979) had significantly lower SUA levels. Although SUA level at V4 was highly associated with diabetes, prediabetes, higher body mass index, CRP (C-reactive protein) levels, estimated glomerular filtration rate variation (visit 1-V4), carotid intima-media thickness, and pulse wave velocity, rs16890979 was only associated with higher carotid intima-media thickness. Conclusions: our findings demonstrate that rs16890979, a genetic determinant of SUA levels located on the SLC2A9 gene, is associated with carotid intima-media thickness despite significant associations between SUA levels and several clinical outcomes, thereby lending support to the hypothesis of a link between SUA and cardiovascular disease., Nancy Centre Hospitalier Regional Universitaire; French Ministry of Health; French National Research Agency (ANR); Contrat de Plan Etat?Lorraine and Fonds Européen de Développement Régional Lorraine; Programme Hospitalier de Recherche Clinique Inter regional 2013; Investissements d’Avenir; FIGHT?heart failure; French Plan d'Investissement d'Avenir project “Lorraine Université d’Excellence; European Union (EU); European Fibro?Targets Project; European HOMAGE project; 7th Framework Program; MEDIA project; FOCUS?MR; ERA?CVD EXPERT; Fondation de Recherche en Hypertension Artérielle
Published: 2022

7. The THESEUS space mission:science goals, requirements and mission concept

Author: Amati, L., O'Brien, P. T., Goetz, D., Bozzo, E., Santangelo, A., Tanvir, N., Frontera, F., Mereghetti, S., Osborne, J. P., Blain, A., Basa, S., Branchesi, M., Burderi, L., Caballero-Garcia, M., Castro-Tirado, A. J., Christensen, L., Ciolfi, R., De Rosa, A., Doroshenko, V. T., Ferrara, A., Ghirlanda, G., Hanlon, L., Heddermann, P., Hutchinson, Eleanor, Labanti, C., Le Floch, E., Lerman, H., Paltani, S., Reglero, Guillermo, Rezzolla, L., Rosati, P., Salvaterra, R., Stratta, G., Tenzer, C., Amati, L., O'Brien, P. T., Goetz, D., Bozzo, E., Santangelo, A., Tanvir, N., Frontera, F., Mereghetti, S., Osborne, J. P., Blain, A., Basa, S., Branchesi, M., Burderi, L., Caballero-Garcia, M., Castro-Tirado, A. J., Christensen, L., Ciolfi, R., De Rosa, A., Doroshenko, V. T., Ferrara, A., Ghirlanda, G., Hanlon, L., Heddermann, P., Hutchinson, Eleanor, Labanti, C., Le Floch, E., Lerman, H., Paltani, S., Reglero, Guillermo, Rezzolla, L., Rosati, P., Salvaterra, R., Stratta, G., and Tenzer, C.
Abstract: THESEUS, one of the two space mission concepts being studied by ESA as candidates for next M5 mission within its Comsic Vision programme, aims at fully exploiting Gamma-Ray Bursts (GRB) to solve key questions about the early Universe, as well as becoming a cornerstone of multi-messenger and time-domain astrophysics. By investigating the first billion years of the Universe through high-redshift GRBs, THESEUS will shed light on the main open issues in modern cosmology, such as the population of primordial low mass and luminosity galaxies, sources and evolution of cosmic re-ionization, SFR and metallicity evolution up to the "cosmic dawn" and across Pop-III stars. At the same time, the mission will provide a substantial advancement of multi-messenger and time-domain astrophysics by enabling the identification, accurate localisation and study of electromagnetic counterparts to sources of gravitational waves and neutrinos, which will be routinely detected in the late '20s and early '30s by the second and third generation Gravitational Wave (GW) interferometers and future neutrino detectors, as well as of all kinds of GRBs and most classes of other X/gamma-ray transient sources. Under all these respects, THESEUS will provide great synergies with future large observing facilities in the multi-messenger domain. A Guest Observer programme, comprising Target of Opportunity (ToO) observations, will expand the science return of the mission, to include, e.g., solar system minor bodies, exoplanets, and AGN.
Published: 2021

8. The THESEUS space mission concept: science case, design and expected performances

Author: Amati, L, O'Brien, P, Götz, D, Bozzo, E, Tenzer, C, Frontera, F, Ghirlanda, G, Labanti, C, Osborne, J, Stratta, G, Tanvir, N, Willingale, R, Attina, P, Campana, R, Castro-Tirado, A, Contini, C, Fuschino, F, Gomboc, A, Hudec, R, Orleanski, P, Renotte, E, Rodic, T, Bagoly, Z, Blain, A, Callanan, P, Covino, S, Ferrara, A, Le Floch, E, Marisaldi, M, Mereghetti, S, Rosati, P, Vacchi, A, D'Avanzo, P, Giommi, P, Piranomonte, S, Piro, L, Reglero, V, Rossi, A, Santangelo, A, Salvaterra, R, Tagliaferri, G, Vergani, S, Vinciguerra, S, Briggs, M, Campolongo, E, Ciolfi, R, Connaughton, V, Cordier, B, Morelli, B, Orlandini, M, Adami, C, Argan, A, Atteia, J, Auricchio, N, Balazs, L, Baldazzi, G, Basa, S, Basak, R, Bellutti, P, Bernardini, M, Bertuccio, G, Braga, J, Branchesi, M, Brandt, S, Brocato, E, Budtz-Jorgensen, C, Bulgarelli, A, Burderi, L, Camp, J, Capozziello, S, Caruana, J, Casella, P, Cenko, B, Chardonnet, P, Ciardi, B, Colafrancesco, S, Dainotti, M, D'Elia, V, De Martino, D, De Pasquale, M, Del Monte, E, Della Valle, M, Drago, A, Evangelista, Y, Feroci, M, Finelli, F, Fiorini, M, Fynbo, J, Gal-Yam, A, Gendre, B, Ghisellini, G, Grado, A, Guidorzi, C, Hafizi, M, Hanlon, L, Hjorth, J, Izzo, L, Kiss, L, Kumar, P, Kuvvetli, I, Lavagna, M, Li, T, Longo, F, Lyutikov, M, Maio, U, Maiorano, E, Malcovati, P, Malesani, D, Margutti, R, Martin-Carrillo, A, Masetti, N, Mcbreen, S, Mignani, R, Morgante, G, Mundell, C, Nargaard-Nielsen, H, Nicastro, L, Palazzi, E, Paltani, S, Panessa, F, Pareschi, G, Pe'Er, A, Penacchioni, A, Pian, E, Piedipalumbo, E, Piran, T, Rauw, G, Razzano, M, Read, A, Rezzolla, L, Romano, P, Ruffini, R, Savaglio, S, Sguera, V, Schady, P, Skidmore, W, Song, L, Stanway, E, Starling, R, Topinka, M, Troja, E, van Putten, M, Vanzella, E, Vercellone, S, Wilson-Hodge, C, Yonetoku, D, Zampa, G, Zampa, N, Zhang, B, Zhang, S, Antonelli, A, Bianco, F, Boci, S, Boer, M, Botticella, M, Boulade, O, Butler, C, Campana, S, Capitanio, F, Celotti, A, Chen, Y, Colpi, M, Comastri, A, Cuby, J, Dadina, M, De Luca, A, Dong, Y, Ettori, S, Gandhi, P, Geza, E, Greiner, J, Guiriec, S, Harms, J, Hernanz, M, Hornstrup, A, Hutchinson, I, Israel, G, Jonker, P, Kaneko, Y, Kawai, N, Wiersema, K, Korpela, S, Lebrun, V, Lu, F, Macfadyen, A, Malaguti, G, Maraschi, L, Melandri, A, Modjaz, M, Morris, D, Omodei, N, Paizis, A, Páta, P, Petrosian, V, Rachevski, A, Rhoads, J, Ryde, F, Sabau-Graziati, L, Shigehiro, N, Sims, M, Soomin, J, Szécsi, D, Urata, Y, Uslenghi, M, Valenziano, L, Vianello, G, Vojtech, S, Watson, D, Zicha, J, Amati, L., O'Brien, P., Götz, D., Bozzo, E., Tenzer, C., Frontera, F., Ghirlanda, G., Labanti, C., Osborne, J. P., Stratta, G., Tanvir, N., Willingale, R., Attina, P., Campana, R., Castro-Tirado, A. J., Contini, C., Fuschino, F., Gomboc, A., Hudec, R., Orleanski, P., Renotte, E., Rodic, T., Bagoly, Z., Blain, A., Callanan, P., Covino, S., Ferrara, A., Le Floch, E., Marisaldi, M., Mereghetti, S., Rosati, P., Vacchi, A., D'Avanzo, P., Giommi, P., Piranomonte, S., Piro, L., Reglero, V., Rossi, A., Santangelo, A., Salvaterra, R., Tagliaferri, G., Vergani, S., Vinciguerra, S., Briggs, M., Campolongo, E., Ciolfi, R., Connaughton, V., Cordier, B., Morelli, B., Orlandini, M., Adami, C., Argan, A., Atteia, J. -L., Auricchio, N., Balazs, L., Baldazzi, G., Basa, S., Basak, R., Bellutti, P., Bernardini, M. G., Bertuccio, G., Braga, J., Branchesi, M., Brandt, S., Brocato, E., Budtz-Jorgensen, C., Bulgarelli, A., Burderi, L., Camp, J., Capozziello, S., Caruana, J., Casella, P., Cenko, B., Chardonnet, P., Ciardi, B., Colafrancesco, S., Dainotti, M. G., D'Elia, V., De Martino, D., De Pasquale, M., Del Monte, E., Della Valle, M., Drago, A., Evangelista, Y., Feroci, M., Finelli, F., Fiorini, M., Fynbo, J., Gal-Yam, A., Gendre, B., Ghisellini, G., Grado, A., Guidorzi, C., Hafizi, M., Hanlon, L., Hjorth, J., Izzo, L., Kiss, L., Kumar, P., Kuvvetli, I., Lavagna, M., Li, T., Longo, F., Lyutikov, M., Maio, U., Maiorano, E., Malcovati, P., Malesani, D., Margutti, R., Martin-Carrillo, A., Masetti, N., McBreen, S., Mignani, R., Morgante, G., Mundell, C., Nargaard-Nielsen, H. U., Nicastro, L., Palazzi, E., Paltani, S., Panessa, F., Pareschi, G., Pe'er, A., Penacchioni, A. V., Pian, E., Piedipalumbo, E., Piran, T., Rauw, G., Razzano, M., Read, A., Rezzolla, L., Romano, P., Ruffini, R., Savaglio, S., Sguera, V., Schady, P., Skidmore, W., Song, L., Stanway, E., Starling, R., Topinka, M., Troja, E., van Putten, M., Vanzella, E., Vercellone, S., Wilson-Hodge, C., Yonetoku, D., Zampa, G., Zampa, N., Zhang, B., Zhang, B. B., Zhang, S., Zhang, S. -N., Antonelli, A., Bianco, F., Boci, S., Boer, M., Botticella, M. T., Boulade, O., Butler, C., Campana, S., Capitanio, F., Celotti, A., Chen, Y., Colpi, M., Comastri, A., Cuby, J. -G., Dadina, M., De Luca, A., Dong, Y. -W., Ettori, S., Gandhi, P., Geza, E., Greiner, J., Guiriec, S., Harms, J., Hernanz, M., Hornstrup, A., Hutchinson, I., Israel, G., Jonker, P., Kaneko, Y., Kawai, N., Wiersema, K., Korpela, S., Lebrun, V., Lu, F., MacFadyen, A., Malaguti, G., Maraschi, L., Melandri, A., Modjaz, M., Morris, D., Omodei, N., Paizis, A., Páta, P., Petrosian, V., Rachevski, A., Rhoads, J., Ryde, F., Sabau-Graziati, L., Shigehiro, N., Sims, M., Soomin, J., Szécsi, D., Urata, Y., Uslenghi, M., Valenziano, L., Vianello, G., Vojtech, S., Watson, D., Zicha, J., Amati, L, O'Brien, P, Götz, D, Bozzo, E, Tenzer, C, Frontera, F, Ghirlanda, G, Labanti, C, Osborne, J, Stratta, G, Tanvir, N, Willingale, R, Attina, P, Campana, R, Castro-Tirado, A, Contini, C, Fuschino, F, Gomboc, A, Hudec, R, Orleanski, P, Renotte, E, Rodic, T, Bagoly, Z, Blain, A, Callanan, P, Covino, S, Ferrara, A, Le Floch, E, Marisaldi, M, Mereghetti, S, Rosati, P, Vacchi, A, D'Avanzo, P, Giommi, P, Piranomonte, S, Piro, L, Reglero, V, Rossi, A, Santangelo, A, Salvaterra, R, Tagliaferri, G, Vergani, S, Vinciguerra, S, Briggs, M, Campolongo, E, Ciolfi, R, Connaughton, V, Cordier, B, Morelli, B, Orlandini, M, Adami, C, Argan, A, Atteia, J, Auricchio, N, Balazs, L, Baldazzi, G, Basa, S, Basak, R, Bellutti, P, Bernardini, M, Bertuccio, G, Braga, J, Branchesi, M, Brandt, S, Brocato, E, Budtz-Jorgensen, C, Bulgarelli, A, Burderi, L, Camp, J, Capozziello, S, Caruana, J, Casella, P, Cenko, B, Chardonnet, P, Ciardi, B, Colafrancesco, S, Dainotti, M, D'Elia, V, De Martino, D, De Pasquale, M, Del Monte, E, Della Valle, M, Drago, A, Evangelista, Y, Feroci, M, Finelli, F, Fiorini, M, Fynbo, J, Gal-Yam, A, Gendre, B, Ghisellini, G, Grado, A, Guidorzi, C, Hafizi, M, Hanlon, L, Hjorth, J, Izzo, L, Kiss, L, Kumar, P, Kuvvetli, I, Lavagna, M, Li, T, Longo, F, Lyutikov, M, Maio, U, Maiorano, E, Malcovati, P, Malesani, D, Margutti, R, Martin-Carrillo, A, Masetti, N, Mcbreen, S, Mignani, R, Morgante, G, Mundell, C, Nargaard-Nielsen, H, Nicastro, L, Palazzi, E, Paltani, S, Panessa, F, Pareschi, G, Pe'Er, A, Penacchioni, A, Pian, E, Piedipalumbo, E, Piran, T, Rauw, G, Razzano, M, Read, A, Rezzolla, L, Romano, P, Ruffini, R, Savaglio, S, Sguera, V, Schady, P, Skidmore, W, Song, L, Stanway, E, Starling, R, Topinka, M, Troja, E, van Putten, M, Vanzella, E, Vercellone, S, Wilson-Hodge, C, Yonetoku, D, Zampa, G, Zampa, N, Zhang, B, Zhang, S, Antonelli, A, Bianco, F, Boci, S, Boer, M, Botticella, M, Boulade, O, Butler, C, Campana, S, Capitanio, F, Celotti, A, Chen, Y, Colpi, M, Comastri, A, Cuby, J, Dadina, M, De Luca, A, Dong, Y, Ettori, S, Gandhi, P, Geza, E, Greiner, J, Guiriec, S, Harms, J, Hernanz, M, Hornstrup, A, Hutchinson, I, Israel, G, Jonker, P, Kaneko, Y, Kawai, N, Wiersema, K, Korpela, S, Lebrun, V, Lu, F, Macfadyen, A, Malaguti, G, Maraschi, L, Melandri, A, Modjaz, M, Morris, D, Omodei, N, Paizis, A, Páta, P, Petrosian, V, Rachevski, A, Rhoads, J, Ryde, F, Sabau-Graziati, L, Shigehiro, N, Sims, M, Soomin, J, Szécsi, D, Urata, Y, Uslenghi, M, Valenziano, L, Vianello, G, Vojtech, S, Watson, D, Zicha, J, Amati, L., O'Brien, P., Götz, D., Bozzo, E., Tenzer, C., Frontera, F., Ghirlanda, G., Labanti, C., Osborne, J. P., Stratta, G., Tanvir, N., Willingale, R., Attina, P., Campana, R., Castro-Tirado, A. J., Contini, C., Fuschino, F., Gomboc, A., Hudec, R., Orleanski, P., Renotte, E., Rodic, T., Bagoly, Z., Blain, A., Callanan, P., Covino, S., Ferrara, A., Le Floch, E., Marisaldi, M., Mereghetti, S., Rosati, P., Vacchi, A., D'Avanzo, P., Giommi, P., Piranomonte, S., Piro, L., Reglero, V., Rossi, A., Santangelo, A., Salvaterra, R., Tagliaferri, G., Vergani, S., Vinciguerra, S., Briggs, M., Campolongo, E., Ciolfi, R., Connaughton, V., Cordier, B., Morelli, B., Orlandini, M., Adami, C., Argan, A., Atteia, J. -L., Auricchio, N., Balazs, L., Baldazzi, G., Basa, S., Basak, R., Bellutti, P., Bernardini, M. G., Bertuccio, G., Braga, J., Branchesi, M., Brandt, S., Brocato, E., Budtz-Jorgensen, C., Bulgarelli, A., Burderi, L., Camp, J., Capozziello, S., Caruana, J., Casella, P., Cenko, B., Chardonnet, P., Ciardi, B., Colafrancesco, S., Dainotti, M. G., D'Elia, V., De Martino, D., De Pasquale, M., Del Monte, E., Della Valle, M., Drago, A., Evangelista, Y., Feroci, M., Finelli, F., Fiorini, M., Fynbo, J., Gal-Yam, A., Gendre, B., Ghisellini, G., Grado, A., Guidorzi, C., Hafizi, M., Hanlon, L., Hjorth, J., Izzo, L., Kiss, L., Kumar, P., Kuvvetli, I., Lavagna, M., Li, T., Longo, F., Lyutikov, M., Maio, U., Maiorano, E., Malcovati, P., Malesani, D., Margutti, R., Martin-Carrillo, A., Masetti, N., McBreen, S., Mignani, R., Morgante, G., Mundell, C., Nargaard-Nielsen, H. U., Nicastro, L., Palazzi, E., Paltani, S., Panessa, F., Pareschi, G., Pe'er, A., Penacchioni, A. V., Pian, E., Piedipalumbo, E., Piran, T., Rauw, G., Razzano, M., Read, A., Rezzolla, L., Romano, P., Ruffini, R., Savaglio, S., Sguera, V., Schady, P., Skidmore, W., Song, L., Stanway, E., Starling, R., Topinka, M., Troja, E., van Putten, M., Vanzella, E., Vercellone, S., Wilson-Hodge, C., Yonetoku, D., Zampa, G., Zampa, N., Zhang, B., Zhang, B. B., Zhang, S., Zhang, S. -N., Antonelli, A., Bianco, F., Boci, S., Boer, M., Botticella, M. T., Boulade, O., Butler, C., Campana, S., Capitanio, F., Celotti, A., Chen, Y., Colpi, M., Comastri, A., Cuby, J. -G., Dadina, M., De Luca, A., Dong, Y. -W., Ettori, S., Gandhi, P., Geza, E., Greiner, J., Guiriec, S., Harms, J., Hernanz, M., Hornstrup, A., Hutchinson, I., Israel, G., Jonker, P., Kaneko, Y., Kawai, N., Wiersema, K., Korpela, S., Lebrun, V., Lu, F., MacFadyen, A., Malaguti, G., Maraschi, L., Melandri, A., Modjaz, M., Morris, D., Omodei, N., Paizis, A., Páta, P., Petrosian, V., Rachevski, A., Rhoads, J., Ryde, F., Sabau-Graziati, L., Shigehiro, N., Sims, M., Soomin, J., Szécsi, D., Urata, Y., Uslenghi, M., Valenziano, L., Vianello, G., Vojtech, S., Watson, D., and Zicha, J.
Abstract: THESEUS is a space mission concept aimed at exploiting Gamma-Ray Bursts for investigating the early Universe and at providing a substantial advancement of multi-messenger and time-domain astrophysics. These goals will be achieved through a unique combination of instruments allowing GRB and X-ray transient detection over a broad field of view (more than 1sr) with 0.5–1 arcmin localization, an energy band extending from several MeV down to 0.3 keV and high sensitivity to transient sources in the soft X-ray domain, as well as on-board prompt (few minutes) follow-up with a 0.7 m class IR telescope with both imaging and spectroscopic capabilities. THESEUS will be perfectly suited for addressing the main open issues in cosmology such as, e.g., star formation rate and metallicity evolution of the inter-stellar and intra-galactic medium up to redshift ∼10, signatures of Pop III stars, sources and physics of re-ionization, and the faint end of the galaxy luminosity function. In addition, it will provide unprecedented capability to monitor the X-ray variable sky, thus detecting, localizing, and identifying the electromagnetic counterparts to sources of gravitational radiation, which may be routinely detected in the late ’20s/early ’30s by next generation facilities like aLIGO/ aVirgo, eLISA, KAGRA, and Einstein Telescope. THESEUS will also provide powerful synergies with the next generation of multi-wavelength observatories (e.g., LSST, ELT, SKA, CTA, ATHENA).
Published: 2018

9. Optimizing gravitational waves follow-up using galaxies stellar mass

Author: Ducoin, J-G, primary, Corre, D, additional, Leroy, N, additional, and Le Floch, E, additional
Published: 2020
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10. Multivariate haplotype analysis of 96 sulci opening for 15,612 UK-Biobank subjects

Author: Karkar, S., Gloaguen, A., Le Guen, Y., Pierre-Jean, Morgane, Dandine-Roulland, C., Le Floch, E., Philippe, C., Tenenhaus, A., Frouin, V., Unité Analyse et Traitement de l'Information (UNATI), Service NEUROSPIN (NEUROSPIN), Direction de Recherche Fondamentale (CEA) (DRF (CEA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Direction de Recherche Fondamentale (CEA) (DRF (CEA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Laboratoire des signaux et systèmes (L2S), Université Paris-Sud - Paris 11 (UP11)-CentraleSupélec-Centre National de la Recherche Scientifique (CNRS), Centre National de Génotypage (CNG), Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Université Paris-Saclay-Direction de Recherche Fondamentale (CEA) (DRF (CEA)), and Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)
Subjects: haplotype, multivariate analysis, [SDV.GEN.GPO]Life Sciences [q-bio]/Genetics/Populations and Evolution [q-bio.PE], [STAT.ML]Statistics [stat]/Machine Learning [stat.ML], [SDV.IB.IMA]Life Sciences [q-bio]/Bioengineering/Imaging, Imaging genetics, [INFO.INFO-BI]Computer Science [cs]/Bioinformatics [q-bio.QM]
Abstract: International audience; Imaging genetic studies of large control cohorts such as UK Biobank enable to assess the range of normal variations in brain structures. Previous studies by our group have shown that the width of several cortical sulci is associated with a variant in the upstream region of KCNK2 gene even if this effect is corrected with age. Here we propose to analyze in a multivariate setup the associations between sets of genetic variants and multiple sulci widths. The genetic variants we consider are sets of SNPs of known phase called haplotypes, taken from the upstream region of KCNK2 gene. To the best of our knowledge, multivariate analysis in imaging genetics has never been used in haplotype studies. Our method was able to recover the expected association signal and uncover new associations between imaging data and genetic variants.
Published: 2019

11. Multivariate Haplotype Analysis Of 96 Sulci Opening For 15,612 UK-Biobank Sujects

Author: Karkar, S., primary, Gloaguen, A., additional, Le Guen, Y., additional, Pierre-Jean, M., additional, Dandine-Roulland, C., additional, Le Floch, E., additional, Philippe, C., additional, Tenenhaus, A., additional, and Frouin, V., additional
Published: 2019
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12. LES EFFETS D'UN CHAUFFAGE DE TYPE CULINAIRE SUR LES PRINCIPAUX CORPS GRAS ALIMENTAIRES SES INCIDENCES PHYSIOLOGIQUES ET NUTRITIONNELLES

Author: LE FLOCH, E., ACKER, P., RAMEL, P., LANTEAUME, M.-T., and LE CLERC, A.-M.
Published: 1968

13. The Deep and Transient Universe in the SVOM Era: New Challenges and Opportunities - Scientific prospects of the SVOM mission

Author: Wei, J., Cordier, B., Antier, S., Antilogus, P., Atteia, J.-L., Bajat, A., Basa, S., Beckmann, V., Bernardini, M. G., Boissier, Samuel, Bouchet, L., Burwitz, V., Claret, A., Dai, Z.-G., Daigne, F., Deng, J., Dornic, D., Feng, H., Foglizzo, T., Gao, H., Gehrels, N., Godet, O., Goldwurm, A., Gonzalez, F., Gosset, L., Götz, D., Gouiffes, C., Grise, F., Gros, A., Guilet, J., Han, X., Huang, M., Huang, Y.-F., Jouret, M., Klotz, A., La Marle, O., Lachaud, C., Le Floch, E., Lee, W., Leroy, N., Li, L.-X., Li, S. C., Li, Z., Liang, E.-W., Lyu, H., Mercier, K., Migliori, G., Mochkovitch, R., O'Brien, P., Osborne, J., Paul, J., Perinati, E., Petitjean, P., Piron, F., Qiu, Y., Rau, A., Rodriguez, J., Schanne, S., Tanvir, N., Vangioni, E., Vergani, S., Wang, F.-Y., Wang, J., Wang, X.-G., Wang, X.-Y., Watson, A., Webb, N., Wei, J. J., Willingale, R., Wu, C., Wu, X.-F., Xin, L.-P., Xu, D., Yu, S., Yu, W.-F., Yu, Y.-W., Zhang, B., Zhang, S.-N., Zhang, Y., Zhou, X. L., Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Institut de recherche en astrophysique et planétologie (IRAP), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), 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), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Laboratoire Univers et Particules de Montpellier (LUPM), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS), Nanjing University (NJU), 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), National Astronomical Observatories [Beijing] (NAOC), Chinese Academy of Sciences [Beijing] (CAS), Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Centre National d’Études Spatiales [Paris] (CNES), Observatoire astronomique de Strasbourg (ObAS), Université de Strasbourg (UNISTRA)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Centre National d'Études Spatiales [Toulouse] (CNES), Universidad Nacional Autónoma de México = National Autonomous University of Mexico (UNAM), Laboratoire de l'Accélérateur Linéaire (LAL), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut für Astronomie und Astrophysik [Tübingen] (IAAT), Eberhard Karls Universität Tübingen = Eberhard Karls University of Tuebingen, Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Department of Physics and Astronomy [Leicester], University of Leicester, Galaxies, Etoiles, Physique, Instrumentation (GEPI), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, SVOM, Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Observatoire Midi-Pyrénées (OMP), Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS), 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), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Université de Montpellier (UM)-Université Montpellier 2 - Sciences et Techniques (UM2)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Aix Marseille Université (AMU), Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Universidad Nacional Autónoma de México (UNAM), Eberhard Karls Universität Tübingen, PSL Research University (PSL)-PSL Research University (PSL)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC), Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Centre National de la Recherche Scientifique (CNRS)-Université de Montpellier (UM)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Montpellier 2 - Sciences et Techniques (UM2), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, and PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)
Subjects: Astrophysics::High Energy Astrophysical Phenomena, [SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Astrophysics::Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Instrumentation and Methods for Astrophysics, [SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]
Abstract: To take advantage of the astrophysical potential of Gamma-Ray Bursts (GRBs), Chinese and French astrophysicists have engaged the SVOM mission (Space-based multi-band astronomical Variable Objects Monitor). Major advances in GRB studies resulting from the synergy between space and ground observations, the SVOM mission implements space and ground instrumentation. The scientific objectives of the mission put a special emphasis on two categories of GRBs: very distant GRBs at z$>$5 which constitute exceptional cosmological probes, and faint/soft nearby GRBs which allow probing the nature of the progenitors and the physics at work in the explosion. These goals have a major impact on the design of the mission: the on-board hard X-ray imager is sensitive down to 4 keV and computes on line image and rate triggers, and the follow-up telescopes on the ground are sensitive in the NIR. At the beginning of the next decade, SVOM will be the main provider of GRB positions and spectral parameters on very short time scale. The SVOM instruments will operate simultaneously with a wide range of powerful astronomical devices. This rare instrumental conjunction, combined with the relevance of the scientific topics connected with GRB studies, warrants a remarkable scientific return for SVOM. In addition, the SVOM instrumentation, primarily designed for GRB studies, composes a unique multi-wavelength observatory with rapid slew capability that will find multiple applications for the whole astronomy community beyond the specific objectives linked to GRBs. This report lists the scientific themes that will benefit from observations made with SVOM, whether they are specific GRB topics, or more generally all the issues that can take advantage of the multi-wavelength capabilities of SVOM.
Published: 2016

14. The evolution of quiescent galaxies at high redshifts (z≥ 1.4)

Author: Domínguez Sánchez H., Gruppioni C., Ilbert O., Pozzetti L., McCracken H., Capak P., Le Floch E., Salvato M., Zamorani G., Carollo C. M., Contini T., Kneib J. P., Le Fèvre O., Lilly S. J., Mainieri V., Renzini A., Scodeggio M., Bardelli S., Bolzonella M., Bongiorno A., Caputi K., Coppa G., de la Torre S., de Ravel L., Franzetti P., Garilli B., Iovino A., Kampczyk P., Knobel C., Kova, #269, Lamareille F., Le Borgne J. F., Le Brun V., Maier C., Mignoli M., Pelló R., Peng Y., Perez Montero E., Ricciardelli E., Silverman J. D., Tanaka M., Tasca L. A. M., Tresse L., Vergani D., Zucca E., POZZI, FRANCESCA, CIMATTI, ANDREA, CUCCIATI, OLGA, Domínguez Sánchez H., Pozzi F., Gruppioni C., Cimatti A., Ilbert O., Pozzetti L., McCracken H., Capak P., Le Floch E., Salvato M., Zamorani G., Carollo C. M., Contini T., Kneib J.-P., Le Fèvre O., Lilly S. J., Mainieri V., Renzini A., Scodeggio M., Bardelli S., Bolzonella M., Bongiorno A., Caputi K., Coppa G., Cucciati O., de la Torre S., de Ravel L., Franzetti P., Garilli B., Iovino A., Kampczyk P., Knobel C., Kova&#269, K., Lamareille F., Le Borgne J.-F., Le Brun V., Maier C., Mignoli M., Pelló R., Peng Y., Perez-Montero E., Ricciardelli E., Silverman J. D., Tanaka M., Tasca L. A. M., Tresse L., Vergani D., and Zucca E.
Subjects: galaxies: high-redshift, galaxies: star formation, Astrophysics::Solar and Stellar Astrophysics, Astrophysics::Earth and Planetary Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, galaxies: evolution, Astrophysics::Galaxy Astrophysics
Abstract: The goal of this work is to study the evolution of high-redshift (z≥ 1.4) quiescent galaxies over an effective area of ˜1.7 deg2 in the COSMOS field. Galaxies have been divided according to their star formation activity and the evolution of the different populations, in particular of the quiescent galaxies, has been investigated in detail. We have studied an IRAC (mag 3.6 μm < 22.0) selected sample of ˜18 000 galaxies at z≥ 1.4 in the COSMOS field with multiwavelength coverage extending from the U band to the Spitzer 24 μm one. We have derived accurate photometric redshifts (?) through a SED-fitting procedure. Other important physical parameters [masses, ages and star formation rates (SFR)] of the galaxies have been obtained using Maraston models. We have divided our sample into actively star-forming, intermediate and quiescent galaxies depending on their specific star formation rate (SSFR = SFR/M). We have computed the galaxy stellar mass function (GSMF) of the total sample and the different populations at z= 1.4-3.0. We have studied the properties of high-redshift quiescent galaxies finding that they are old (1-4 Gyr), massive (˜ 1010.65 M⊙), weakly star-forming stellar populations with low dust extinction [E(B-V) ≤ 0.15] and small e-folding time-scales (τ˜ 0.1-0.3 Gyr). We observe a significant evolution of the quiescent stellar mass function from 2.5 < z < 3.0 to 1.4 < z < 1.6, increasing by ˜1 dex in this redshift interval. We find that z˜ 1.5 is an epoch of transition of the GSMF: while the GSMF at z≳ 1.5 is dominated by the star-forming galaxies at all stellar masses, at z≲ 1.5 the contribution to the total GSMF of the quiescent galaxies is significant and becomes higher than that of the star-forming population for M≥ 1010.75 M⊙. The fraction of star-forming galaxies decreases from 60-20 per cent from z˜ 2.5-3.0 to 1.4-1.6 for M˜ 1011.0 M⊙, while the quiescent population increases from 10-50 per cent at the same redshift and mass intervals. We compare the fraction of quiescent galaxies derived with that predicted by theoretical models and find that the Kitzbichler & White model, implemented on the Millennium Simulation, is the one that better reproduces the shape of the data. Finally, we calculate the stellar mass density of the star-forming and quiescent populations as a function of redshift and find that there is already a significant number of quiescent galaxies at z > 2.5 (logρ[M⊙ Mpc-3]˜ 6), meaning that efficient star formation had to take place before that time.
Published: 2011

15. Hot-dust-poor Type 1 AGNs in the COSMOS survey

Author: Hao H., Elvis M., Civano F., LANZUISI, GIORGIO, Zamorani G., Comastri A., Bongiorno A., Impey C., Koekemoer A. M., Le Floch E., Salvato M., Sanders D., Trump J., BRUSA, MARCELLA, LUSSO, ELISABETA, VIGNALI, CRISTIAN, Hao H., Elvis M., Civano F., Lanzuisi G., Brusa M., Lusso E., Zamorani G., Comastri A., Bongiorno A., Impey C., Koekemoer A.M., Le Floch E., Salvato M., Sanders D., Trump J., and Vignali C.
Subjects: Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Earth and Planetary Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics::Galaxy Astrophysics, galaxies: evolution – quasars: general
Abstract: e report a sizable class of type 1 active galactic nuclei (AGNs) with unusually weak near-infrared (1–3μm) emission in the XMM-COSMOS type 1 AGN sample. The fraction of these “hot-dust-poor” AGNs increases with redshift from 6% at low redshift (z < 2) to 20% at moderate high redshift (2 < z < 3.5). There is no clear trend of the fraction with other parameters: bolometric luminosity, Eddington ratio, black hole mass, and X-ray luminosity. The 3 μm emission relative to the 1 μm emission is a factor of 2–4 smaller than the typical Elvis et al. AGN spectral energy distribution (SED), which indicates a “torus” covering factor of 2%–29%, a factor of 3–40 smaller than required by unified models. The weak hot dust emission seems to expose an extension of the accretion disk continuum in some of the source SEDs. We estimate the outer edge of their accretion disks to lie at (0.3–2.0) × 104 Schwarzschild radii, ∼10–23 times the gravitational stability radii. Formation scenarios for these sources are discussed.
Published: 2010

16. Massive stars formed in atomic hydrogen reservoirs: H i observations of gamma-ray burst host galaxies

Author: Michałowski, M. J., Gentile, G., Hjorth, J., Krumholz, M. R., Tanvir, N. R., Kamphuis, P., Burlon, D., Baes, M., Basa, S., Berta, S., Castro Cerón, J. M., Crosby, D., D'Elia, V., Elliott, J., Greiner, J., Hunt, L. K., Klose, S., Koprowski, M. P., Le Floch, E., Malesani, D., Murphy, T., Nicuesa Guelbenzu, A., Palazzi, E., Rasmussen, Jesper, Rossi, A., Savaglio, S., Schady, P., Sollerman, J., de Ugarte Postigo, A., Watson, D., van der Werf, P., Vergani, S. D., Xu, D., Michałowski, M. J., Gentile, G., Hjorth, J., Krumholz, M. R., Tanvir, N. R., Kamphuis, P., Burlon, D., Baes, M., Basa, S., Berta, S., Castro Cerón, J. M., Crosby, D., D'Elia, V., Elliott, J., Greiner, J., Hunt, L. K., Klose, S., Koprowski, M. P., Le Floch, E., Malesani, D., Murphy, T., Nicuesa Guelbenzu, A., Palazzi, E., Rasmussen, Jesper, Rossi, A., Savaglio, S., Schady, P., Sollerman, J., de Ugarte Postigo, A., Watson, D., van der Werf, P., Vergani, S. D., and Xu, D.
Abstract: Long gamma-ray bursts (GRBs), among the most energetic events in the Universe, are explosions of massive and short-lived stars, so they pinpoint locations of recent star formation. However, several GRB host galaxies have recently been found to be deficient in molecular gas (H2), believed to be the fuel of star formation. Moreover, optical spectroscopy of GRB afterglows implies that the molecular phase constitutes only a small fraction of the gas along the GRB line of sight. Here we report the first ever 21 cm line observations of GRB host galaxies, using the Australia Telescope Compact Array, implying high levels of atomic hydrogen (HI), which suggests that the connection between atomic gas and star formation is stronger than previously thought. In this case, it is possible that star formation is directly fuelled by atomic gas (or that the H1-to-H2 conversion is very efficient, which rapidly exhaust molecular gas), as has been theoretically shown to be possible. This can happen in low-metallicity gas near the onset of star formation because cooling of gas (necessary for star formation) is faster than the H1-to-H2 conversion. Indeed, large atomic gas reservoirs, together with low molecular gas masses, stellar, and dust masses are consistent with GRB hosts being preferentially galaxies which have very recently started a star formation episode after accreting metal-poor gas from the intergalactic medium. This provides a natural route for forming GRBs in low-metallicity environments. The gas inflow scenario is also consistent with the existence of the companion HI object with no optical counterpart ∼19 kpc from the GRB 060505 host, and with the fact that the HI centroids of the GRB 980425 and 060505 hosts do not coincide with optical centres of these galaxies, but are located close to the GRB positions.
Published: 2015

17. Voxelwise multivariate statistics and brain-wide machine learning using the full diffusion tensor

Author: Fouque, A. L., Fillard, P., Bargiacchi, A., Arnaud Cachia, Zilbovicius, M., Thyreau, B., Le Floch, E., Ciuciu, P., Duchesnay, E., Modelling brain structure, function and variability based on high-field MRI data (PARIETAL), Service NEUROSPIN (NEUROSPIN), Université Paris-Saclay-Direction de Recherche Fondamentale (CEA) (DRF (CEA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Direction de Recherche Fondamentale (CEA) (DRF (CEA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Inria Saclay - Ile de France, Institut National de Recherche en Informatique et en Automatique (Inria)-Institut National de Recherche en Informatique et en Automatique (Inria), Laboratoire de Neuroimagerie Assistée par Ordinateur (LNAO), Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Inria Saclay - Ile de France, Institut National de Recherche en Informatique et en Automatique (Inria)-Institut National de Recherche en Informatique et en Automatique (Inria)-Service NEUROSPIN (NEUROSPIN), Direction de Recherche Fondamentale (CEA) (DRF (CEA)), and Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay
Subjects: Brain Mapping, Models, Statistical, Brain, [SDV.IB.MN]Life Sciences [q-bio]/Bioengineering/Nuclear medicine, Magnetic Resonance Imaging, Diffusion Tensor Imaging, Artificial Intelligence, Child Development Disorders, Pervasive, Multivariate Analysis, Image Processing, Computer-Assisted, Humans, Child, Algorithms, Software
Abstract: International audience; In this paper, we propose to use the full diffusion tensor to perform brain-wide score prediction on diffusion tensor imaging (DTI) using the log-Euclidean framework., rather than the commonly used fractional anisotropy (FA). Indeed, scalar values such as the FA do not capture all the information contained in the diffusion tensor. Additionally, full tensor information is included in every step of the pre-processing pipeline: registration, smoothing and feature selection using voxelwise multivariate regression analysis. This approach was tested on data obtained from 30 children and adolescents with autism spectrum disorder and showed some improvement over the FA-only analysis.
Published: 2011

18. Non-linearity and environmental dependence of the star-forming galaxies main sequence

Author: Erfanianfar, G., primary, Popesso, P., additional, Finoguenov, A., additional, Wilman, D., additional, Wuyts, S., additional, Biviano, A., additional, Salvato, M., additional, Mirkazemi, M., additional, Morselli, L., additional, Ziparo, F., additional, Nandra, K., additional, Lutz, D., additional, Elbaz, D., additional, Dickinson, M., additional, Tanaka, M., additional, Altieri, M. B., additional, Aussel, H., additional, Bauer, F., additional, Berta, S., additional, Bielby, R. M., additional, Brandt, N., additional, Cappelluti, N., additional, Cimatti, A., additional, Cooper, M. C., additional, Fadda, D., additional, Ilbert, O., additional, Le Floch, E., additional, Magnelli, B., additional, Mulchaey, J. S., additional, Nordon, R., additional, Newman, J. A., additional, Poglitsch, A., additional, and Pozzi, F., additional
Published: 2015
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19. The role of massive halos in the star formation history of the Universe

Author: Popesso, P., primary, Biviano, A., additional, Finoguenov, A., additional, Wilman, D., additional, Salvato, M., additional, Magnelli, B., additional, Gruppioni, C., additional, Pozzi, F., additional, Rodighiero, G., additional, Ziparo, F., additional, Berta, S., additional, Elbaz, D., additional, Dickinson, M., additional, Lutz, D., additional, Altieri, B., additional, Aussel, H., additional, Cimatti, A., additional, Fadda, D., additional, Ilbert, O., additional, Le Floch, E., additional, Nordon, R., additional, Poglitsch, A., additional, Genel, S., additional, and Xu, C. K., additional
Published: 2015
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20. The evolution of galaxy star formation activity in massive haloes

Author: Popesso, P., primary, Biviano, A., additional, Finoguenov, A., additional, Wilman, D., additional, Salvato, M., additional, Magnelli, B., additional, Gruppioni, C., additional, Pozzi, F., additional, Rodighiero, G., additional, Ziparo, F., additional, Berta, S., additional, Elbaz, D., additional, Dickinson, M., additional, Lutz, D., additional, Altieri, B., additional, Aussel, H., additional, Cimatti, A., additional, Fadda, D., additional, Ilbert, O., additional, Le Floch, E., additional, Nordon, R., additional, Poglitsch, A., additional, and Xu, C. K., additional
Published: 2015
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21. A multiwavelength consensus on the main sequence of star-forming galaxies at z ∼ 2

Author: Rodighiero, G., primary, Renzini, A., additional, Daddi, E., additional, Baronchelli, I., additional, Berta, S., additional, Cresci, G., additional, Franceschini, A., additional, Gruppioni, C., additional, Lutz, D., additional, Mancini, C., additional, Santini, P., additional, Zamorani, G., additional, Silverman, J., additional, Kashino, D., additional, Andreani, P., additional, Cimatti, A., additional, Sánchez, H. Domínguez, additional, Le Floch, E., additional, Magnelli, B., additional, Popesso, P., additional, and Pozzi, F., additional
Published: 2014
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22. Energy Expenditure During a 160 km Endurance Race

Author: Goachet, A, primary, Loriers, A, additional, Le Floch, E, additional, and Julliand, V, additional
Published: 2014
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23. The mean star formation rate of X-ray selected active galaxies and its evolution fromz ~ 2.5: results from PEP-Herschel

Author: Rosario, D.J., primary, Santini, P., additional, Lutz, D., additional, Shao, L., additional, Maiolino, R., additional, Alexander, D.M., additional, Altieri, B., additional, Andreani, P., additional, Aussel, H., additional, Bauer, F.E., additional, Berta, S., additional, Bongiovanni, A., additional, Brandt, W.N., additional, Brusa, M., additional, Cepa, J., additional, Cimatti, A., additional, Cox, T.J., additional, Daddi, E., additional, Elbaz, D., additional, Fontana, A., additional, Förster Schreiber, N.M., additional, Genzel, R., additional, Grazian, A., additional, Le Floch, E., additional, Magnelli, B., additional, Mainieri, V., additional, Netzer, H., additional, Nordon, R., additional, Pérez Garcia, I., additional, Poglitsch, A., additional, Popesso, P., additional, Pozzi, F., additional, Riguccini, L., additional, Rodighiero, G., additional, Salvato, M., additional, Sanchez-Portal, M., additional, Sturm, E., additional, Tacconi, L.J., additional, Valtchanov, I., additional, and Wuyts, S., additional
Published: 2012
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24. Discovering associations in high dimensional imaging-genetics data: A comparison study of dimension reduction and regularisation strategies combined with partial least squares

Author: Le Floch, E., primary, Pinel, P., additional, Tenenhaus, A., additional, Trinchera, L., additional, Poline, J. B., additional, Frouin, V., additional, and Duchesnay, E., additional
Published: 2012
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25. The evolution of the star formation activity per halo mass up to redshift ~1.6 as seen byHerschel

Author: Popesso, P., primary, Biviano, A., additional, Rodighiero, G., additional, Baronchelli, I., additional, Salvato, M., additional, Saintonge, A., additional, Finoguenov, A., additional, Magnelli, B., additional, Gruppioni, C., additional, Pozzi, F., additional, Lutz, D., additional, Elbaz, D., additional, Altieri, B., additional, Andreani, P., additional, Aussel, H., additional, Berta, S., additional, Capak, P., additional, Cava, A., additional, Cimatti, A., additional, Coia, D., additional, Daddi, E., additional, Dannerbauer, H., additional, Dickinson, M., additional, Dasyra, K., additional, Fadda, D., additional, Förster Schreiber, N., additional, Genzel, R., additional, Hwang, H. S., additional, Kartaltepe, J., additional, Ilbert, O., additional, Le Floch, E., additional, Leiton, R., additional, Magdis, G., additional, Nordon, R., additional, Patel, S., additional, Poglitsch, A., additional, Riguccini, L., additional, Sanchez Portal, M., additional, Shao, L., additional, Tacconi, L., additional, Tomczak, A., additional, Tran, K., additional, and Valtchanov, I., additional
Published: 2012
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26. On the jet structure and magnetic field configuration of GRB-020813

Author: Lazzati, D., Covino, S., Grosabel, J., Rossi, E., Ghisellini, G., Rol, E., Castro-tirado, A.J., Della Valle, M., di Serego Alighieri, S., Fruchter, A.S., Fynbo, Johan Peter Uldall, Goldoni, P., Hjorth, J., Israel, G.L., Kaper, L., Kawai, N., Le Floch, E., Masetti, N., Mirabel, F., Moller, P., Ortolani, S., Palazzi, E., Pian, E., Rhoads, J., Ricker, G., Salmonson, J.D., Stella, L., Tagliaferri, G., Tanvir, N., van den Heuvel, E., Wijers, R.A.M.J., Zerbi, F.M., Castro Cerón, José María, Malesani, Daniele, Lazzati, D., Covino, S., Grosabel, J., Rossi, E., Ghisellini, G., Rol, E., Castro-tirado, A.J., Della Valle, M., di Serego Alighieri, S., Fruchter, A.S., Fynbo, Johan Peter Uldall, Goldoni, P., Hjorth, J., Israel, G.L., Kaper, L., Kawai, N., Le Floch, E., Masetti, N., Mirabel, F., Moller, P., Ortolani, S., Palazzi, E., Pian, E., Rhoads, J., Ricker, G., Salmonson, J.D., Stella, L., Tagliaferri, G., Tanvir, N., van den Heuvel, E., Wijers, R.A.M.J., Zerbi, F.M., Castro Cerón, José María, and Malesani, Daniele
Published: 2004

27. The evolution of quiescent galaxies at high redshifts (z≥ 1.4)

Author: Domínguez Sánchez, H., primary, Pozzi, F., additional, Gruppioni, C., additional, Cimatti, A., additional, Ilbert, O., additional, Pozzetti, L., additional, McCracken, H., additional, Capak, P., additional, Le Floch, E., additional, Salvato, M., additional, Zamorani, G., additional, Carollo, C. M., additional, Contini, T., additional, Kneib, J.-P., additional, Le Fèvre, O., additional, Lilly, S. J., additional, Mainieri, V., additional, Renzini, A., additional, Scodeggio, M., additional, Bardelli, S., additional, Bolzonella, M., additional, Bongiorno, A., additional, Caputi, K., additional, Coppa, G., additional, Cucciati, O., additional, de la Torre, S., additional, de Ravel, L., additional, Franzetti, P., additional, Garilli, B., additional, Iovino, A., additional, Kampczyk, P., additional, Knobel, C., additional, Kovač, K., additional, Lamareille, F., additional, Le Borgne, J.-F., additional, Le Brun, V., additional, Maier, C., additional, Mignoli, M., additional, Pelló, R., additional, Peng, Y., additional, Perez-Montero, E., additional, Ricciardelli, E., additional, Silverman, J. D., additional, Tanaka, M., additional, Tasca, L. A. M., additional, Tresse, L., additional, Vergani, D., additional, and Zucca, E., additional
Published: 2011
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28. THE LESSER ROLE OF STARBURSTS IN STAR FORMATION AT z = 2

Author: Rodighiero, G., primary, Daddi, E., additional, Baronchelli, I., additional, Cimatti, A., additional, Renzini, A., additional, Aussel, H., additional, Popesso, P., additional, Lutz, D., additional, Andreani, P., additional, Berta, S., additional, Cava, A., additional, Elbaz, D., additional, Feltre, A., additional, Fontana, A., additional, Förster Schreiber, N. M., additional, Franceschini, A., additional, Genzel, R., additional, Grazian, A., additional, Gruppioni, C., additional, Ilbert, O., additional, Le Floch, E., additional, Magdis, G., additional, Magliocchetti, M., additional, Magnelli, B., additional, Maiolino, R., additional, McCracken, H., additional, Nordon, R., additional, Poglitsch, A., additional, Santini, P., additional, Pozzi, F., additional, Riguccini, L., additional, Tacconi, L. J., additional, Wuyts, S., additional, and Zamorani, G., additional
Published: 2011
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29. A RUNAWAY BLACK HOLE IN COSMOS: GRAVITATIONAL WAVE OR SLINGSHOT RECOIL?

Author: Civano, F., primary, Elvis, M., additional, Lanzuisi, G., additional, Jahnke, K., additional, Zamorani, G., additional, Blecha, L., additional, Bongiorno, A., additional, Brusa, M., additional, Comastri, A., additional, Hao, H., additional, Leauthaud, A., additional, Loeb, A., additional, Mainieri, V., additional, Piconcelli, E., additional, Salvato, M., additional, Scoville, N., additional, Trump, J., additional, Vignali, C., additional, Aldcroft, T., additional, Bolzonella, M., additional, Bressert, E., additional, Finoguenov, A., additional, Fruscione, A., additional, Koekemoer, A. M., additional, Cappelluti, N., additional, Fiore, F., additional, Giodini, S., additional, Gilli, R., additional, Impey, C. D., additional, Lilly, S. J., additional, Lusso, E., additional, Puccetti, S., additional, Silverman, J. D., additional, Aussel, H., additional, Capak, P., additional, Frayer, D., additional, Le Floch, E., additional, McCracken, H. J., additional, Sanders, D. B., additional, Schiminovich, D., additional, and Taniguchi, Y., additional
Published: 2010
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30. PHOTOMETRIC REDSHIFT AND CLASSIFICATION FOR THEXMM-COSMOS SOURCES

Author: Salvato, M., primary, Hasinger, G., additional, Ilbert, O., additional, Zamorani, G., additional, Brusa, M., additional, Scoville, N. Z., additional, Rau, A., additional, Capak, P., additional, Arnouts, S., additional, Aussel, H., additional, Bolzonella, M., additional, Buongiorno, A., additional, Cappelluti, N., additional, Caputi, K., additional, Civano, F., additional, Cook, R., additional, Elvis, M., additional, Gilli, R., additional, Jahnke, K., additional, Kartaltepe, J. S., additional, Impey, C. D., additional, Lamareille, F., additional, Le Floch, E., additional, Lilly, S., additional, Mainieri, V., additional, McCarthy, P., additional, McCracken, H., additional, Mignoli, M., additional, Mobasher, B., additional, Murayama, T., additional, Sasaki, S., additional, Sanders, D. B., additional, Schiminovich, D., additional, Shioya, Y., additional, Shopbell, P., additional, Silverman, J., additional, Smolčić, V., additional, Surace, J., additional, Taniguchi, Y., additional, Thompson, D., additional, Trump, J. R., additional, Urry, M., additional, and Zamojski, M., additional
Published: 2008
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31. HerMES: deep number counts at 250μm, 350μm and 500μm in the COSMOS and GOODS-N fields and the build-up of the cosmic infrared background.

Author: Béthermin, M., Le Floch, E., Ilbert, O., Conley, A.s, Lagache, G., Amblard, A., Arumugam, V., Aussel, H., Berta, S., Bock, J., Boselli, A., Buat, V., Casey, C. M., Castro-Rodríguez, N., Cava, A., Clements, D. L., Cooray, A., Dowell, C. D., Eales, S., and Farrah, D.
Subjects: *REDSHIFT, *GALAXIES, *NUMERICAL analysis, *ASTROPHYSICS, *MATHEMATICAL models
Abstract: Aims. The Spectral and Photometric Imaging Receiver (SPIRE) onboard the Herschel space telescope has provided confusion limited maps of deep fields at 250 μm, 350 μm, and 500 μm, as part of the Herschel Multi-tiered Extragalactic Survey (HerMES). Unfortunately, due to confusion, only a small fraction of the cosmic infrared background (CIB) can be resolved into individually-detected sources. Our goal is to produce deep galaxy number counts and redshift distributions below the confusion limit at SPIRE wavelengths (∼20 mJy), which we then use to place strong constraints on the origins of the cosmic infrared background and on models of galaxy evolution. Methods. We individually extracted the bright SPIRE sources (>20 mJy) in the COSMOS field with a method using the positions, the flux densities, and the redshifts of the 24 μm sources as a prior, and derived the number counts and redshift distributions of the bright SPIRE sources. For fainter SPIRE sources (<20 mJy), we reconstructed the number counts and the redshift distribution below the confusion limit using the deep 24 μm catalogs associated with photometric redshift and information provided by the stacking of these sources into the deep SPIRE maps of the GOODS-N and COSMOS fields. Finally, by integrating all these counts, we studied the contribution of the galaxies to the CIB as a function of their flux density and redshift. Results. Through stacking, we managed to reconstruct the source counts per redshift slice down to ∼2 mJy in the three SPIRE bands, which lies about a factor 10 below the 5σ confusion limit. Our measurements place tight constraints on source population models. None of the pre-existing models are able to reproduce our results at better than 3-σ. Finally, we extrapolate our counts to zero flux density in order to derive an estimate of the total contribution of galaxies to the CIB, finding 10.12.32.6nW m-2sr-1, 6.5-1.6+1.7nW m-2 sr-1, and 2.8-0.8+0.9nW m-2 sr-1 at 250 μm, 350 μm, and 500 μm, respectively. These values agree well with FIRAS absolute measurements, suggesting our number counts and their extrapolation are sufficient to explain the CIB. We find that half of the CIB is emitted at z = 1.04, 1.20, and 1.25, respectively. Finally, combining our results with other works, we estimate the energy budget contained in the CIB between 8 μm and 1000 μm: 26+7-3nW m-2sr-1. [ABSTRACT FROM AUTHOR]
Published: 2012
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32. Quelques remarques sur les taillis de chênes verts : répartition, histoire, biomasse

Author: Romane, F., Floret, C., Galan, M., Grandjanny, L., Le Floch, E., Maistre, M., Perret, P., and Service irevues, irevues
Subjects: BIOMASSE FORESTIERE, RECHERCHE FORESTIERE, ECLAIRCIE, [SDV.SA.SF] Life Sciences [q-bio]/Agricultural sciences/Silviculture, forestry, QUERCUS ILEX (Chêne vert), TAILLIS, SYLVICULTURE
Published: 1988

33. Expérimentation sur l'utilisation des données Landsat pour l'étude écologique des zones arides de Tunisie (Expérience ARZOTU) : premiers résultats

Author: Long, G., Sta-M'Rad, M., Lacaze, B., Debussche, G., Le Floch, E., Pontanier, Roger, and Le Cocq, André
Subjects: SATELLITE LANDSAT, PHYTOECOLOGIE, TELEDETECTION SPATIALE
Published: 1977

34. Exemple d'utilisation des données du satellite Landsat pour l'étude des sols en zone aride (Tunisie présaharienne)

Author: Le Cocq, André, Debussche, G., Lacaze, B., Le Floch, E., and Pontanier, R.
Subjects: SATELLITE LANDSAT, SOL, TELEDETECTION SPATIALE, VEGETATION, INVENTAIRE
Published: 1977

35. The Transient High Energy Sky and Early Universe Surveyor (THESEUS)

Author: Amati, L., O Brien, P., Goetz, D., Bozzo, E., Tenzer, C., Frontera, F., Ghirlanda, G., Labanti, C., Osborne, J. P., Stratta, G., Tanvir, N., Willingale, R., Attina, P., Campana, R., Castro-Tirado, A. J., Contini, C., Fuschino, F., Gomboc, A., Hudec, R., Orleanski, P., Renotte, E., Rodic, T., Bagoly, Z., Blain, A., Callanan, P., Covino, S., Ferrara, A., Le Floch, E., Marisaldi, M., Mereghetti, S., Rosati, P., Vacchi, A., D Avanzo, P., Giommi, P., Piranomonte, S., Piro, L., Reglero, V., Rossi, A., Santangelo, A., Salvaterra, R., Tagliaferri, G., Vergani, S., Vinciguerra, S., Briggs, M., Campolongo, E., Ciolfi, R., Connaughton, V., Cordier, B., Morelli, B., Orlandini, M., Adami, C., Argan, A., Atteia, J. -L, Auricchio, N., Balazs, L., Baldazzi, G., Basa, S., Basak, R., Bellutti, P., Bernardini, M. G., Bertuccio, G., Braga, J., Branchesi, M., Brandt, S., Brocato, E., Budtz-Jorgensen, C., Bulgarelli, A., Burderi, L., Camp, J., Capozziello, S., Caruana, J., Casella, P., Cenko, B., Chardonnet, P., Ciardi, B., Colafrancesco, S., Dainotti, M. G., D Elia, V., Martino, D., Pasquale, M., Del Monte, E., Della Valle, M., Drago, A., Evangelista, Y., Feroci, M., Finelli, F., Fiorini, M., Fynbo, J., Gal-Yam, A., Gendre, B., Ghisellini, G., Grado, A., Guidorzi, C., Hafizi, M., Hanlon, L., Hjorth, J., Izzo, L., Kiss, L., Kumar, P., Kuvvetli, I., Lavagna, M., Li, T., Longo, F., Lyutikov, M., Maio, U., Maiorano, E., Malcovati, P., Malesani, D., Margutti, R., Martin-Carrillo, A., Masetti, N., Mcbreen, S., Mignani, R., Morgante, G., Mundell, C., Nargaard-Nielsen, H. U., Nicastro, L., Palazzi, E., Paltani, S., Panessa, F., Pareschi, G., Pe Er, A., Penacchioni, A. V., Pian, E., Piedipalumbo, E., Piran, T., Rauw, G., Razzano, M., Read, A., Rezzolla, L., Romano, P., Ruffini, R., Savaglio, S., Sguera, V., Schady, P., Skidmore, W., Song, L., Stanway, E., Starling, R., Topinka, M., Troja, E., Putten, M., Vanzella, E., Vercellone, S., Wilson-Hodge, C., Yonetoku, D., Zampa, G., Zampa, N., Zhang, B., Zhang, B. B., Zhang, S., Zhang, S. -N, Antonelli, A., Bianco, F., Boci, S., Boer, M., Botticella, M. T., Boulade, O., Butler, C., Campana, S., Capitanio, F., Celotti, A., Chen, Y., Colpi, M., Comastri, A., Cuby, J. -G, Dadina, M., Andrea De Luca, Dong, Y. -W, Ettori, S., Gandhi, P., Geza, E., Greiner, J., Guiriec, S., Harms, J., Hernanz, M., Hornstrup, A., Hutchinson, I., Israel, G., Jonker, P., Kaneko, Y., Kawai, N., Wiersema, K., Korpela, S., Lebrun, V., Lu, F., Macfadyen, A., Malaguti, G., Maraschi, L., Melandri, A., Modjaz, M., Morris, D., Omodei, N., Paizis, A., Pata, P., Petrosian, V., Rachevski, A., Rhoads, J., Ryde, F., Sabau-Graziati, L., Shigehiro, N., Sims, M., Soomin, J., Szecsi, D., Urata, Y., Uslenghi, M., Valenziano, L., Vianello, G., Vojtech, S., Watson, D., Zicha, J., and L. Amati, P. O’Brien, D. Goetz, E. Bozzo, C. Tenzer, F. Frontera, G. Ghirlanda, C. Labanti, J. P. Osborne, G. Stratta, N. Tanvir, R. Willingale , P. Attina, R. Campana, A.J. Castro-Tirado, C. Contini, F. Fuschino, A. Gomboc, R. Hudec, P. Orleanski, E. Renotte, T. Rodic, Z. Bagoly, A. Blain, P. Callanan, S. Covino, A. Ferrara, E. Le Floch, M. Marisaldi, S. Mereghetti, P. Rosati, A. Vacchi, P. D’Avanzo, P. Giommi, A. Gomboc, S. Piranomonte, L. Piro, V. Reglero, A. Rossi, A. Santangelo, R. Salvaterra, G. Tagliaferri, S. Vergani, S. Vinciguerra, M. Briggs, E. Campolongo, R. Ciolfi, V. Connaughton, B. Cordier, B. Morelli, M. Orlandini, C. Adami, A. Argan, J.-L. Atteia, N. Auricchio, L. Balazs, G. Baldazzi, S. Basa, R. Basak, P. Bellutti, M. G. Bernardini, G. Bertuccio, J. Braga, M. Branchesi, S. Brandt, E. Brocato, C. Budtz-Jorgensen, A. Bulgarelli, L. Burderi, J. Camp, S. Capozziello, J. Caruana, P. Casella, B. Cenko, P. Chardonnet, B. Ciardi, S. Colafrancesco, M. G. Dainotti, V. D’Elia, D. De Martino, M. De Pasquale, E. Del Monte, M. Della Valle, A. Drago, Y. Evangelista, M. Feroci, F. Finelli, M. Fiorini, J. Fynbo, A. Gal-Yam, B. Gendre, G. Ghisellini, A. Grado, C. Guidorzi, M. Hafizi, L. Hanlon, J. Hjorth, L. Izzo, L. Kiss, P. Kumar, I. Kuvvetli, M. Lavagna, T. Li, F. Longo, M. Lyutikov, U. Maio, E. Maiorano, P. Malcovati, D. Malesani, R. Margutti, A. Martin-Carrillo, N. Masetti, S. McBreen, R. Mignani, G. Morgante, C. Mundell, H. U. Nargaard-Nielsen, L. Nicastro, E. Palazzi, S. Paltani, F. Panessa, G. Pareschi, A. Pe’er, A. V. Penacchioni, E. Pian, E. Piedipalumbo, T. Piran, G. Rauw, M. Razzano, A. Read, L. Rezzolla, P. Romano, R. Ruffini, S. Savaglio, V. Sguera, P. Schady, W. Skidmore, L. Song, E. Stanway, R. Starling, M. Topinka, E. Troja, M. van Putten, E. Vanzella, S. Vercellone, C. Wilson-Hodge, D. Yonetoku, G. Zampa, N. Zampa, B. Zhang, B. B. Zhang, S. Zhang, S.-N. Zhang, A. Antonelli, F. Bianco, S. Boci, M. Boer, M. T. Botticella, O. Boulade, C. Butler, S. Campana, F. Capitanio, A. Celotti, Y. Chen, M. Colpi, A. Comastri, J.-G. Cuby, M. Dadina, A. De Luca, Y.-W. Dong, S. Ettori, P. Gandhi, E. Geza, J. Greiner, S. Guiriec, J. Harms, M. Hernanz, A. Hornstrup, I. Hutchinson, G. Israel, P. Jonker, Y. Kaneko, N. Kawai, K. Wiersema, S. Korpela, V. Lebrun, F. Lu, A. MacFadyen, G. Malaguti, L. Maraschi, A. Melandri, M. Modjaz, D. Morris, N. Omodei, A. Paizis, P. P´ata, V. Petrosian, A. Rachevski, J. Rhoads, F. Ryde, L. Sabau-Graziati, N. Shigehiro, M. Sims, J. Soomin, D. Szecsi, Y. Urata, M. Uslenghi, L. Valenziano, G. Vianello, S. Vojtech, D. Watson, J. Zicha
Subjects: Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Gamma-ray bursts, Cosmology: observations, dark ages, re-ionization, first stars, Astrophysics::Galaxy Astrophysics
Abstract: THESEUS is a space mission concept aimed at exploiting Gamma-Ray Bursts for investigating the early Universe and at providing a substantial advancement of multi-messenger and time-domain astrophysics. These goals will be achieved through a unique combination of instruments allowing GRBs and X-ray transients detection over a broad FOV (more than 1sr) with 0.5-1 arcmin localization, an energy band extending from several MeVs down to 0.3 keV and high sensitivity to transient sources in the soft X-ray domain, as well as on-board prompt (few minutes) follow-up with a 0.7 m class IR telescope with both imaging and spectroscopic capabilities. THESEUS will be perfectly suited for addressing the main open issues in cosmology such as, e.g., star formation rate and metallicity evolution of the inter-stellar and intra-galactic medium up to redshift ∼10, signatures of Pop III stars, sources and physics of re-ionization, and the faint end of the galaxy luminosity function. In addition, it will provide unprecedented capability to monitor the X-ray variable sky, thus detecting, localizing, and identifying the electromagnetic counterparts to sources of gravitational radiation, which may be routinely detected in the late '20s / early '30s by next generation facilities like aLIGO/ aVirgo, eLISA, KAGRA, and Einstein Telescope. THESEUS will also provide powerful synergies with the next generation of multi-wavelength observatories (e.g., LSST, ELT, SKA, CTA, ATHENA).

36. THE COSMOS2015 CATALOG: EXPLORING THE 1 \textless z \textless 6 UNIVERSE WITH HALF A MILLION GALAXIES

Author: Hsieh, B., Lin, L., Ilbert, O., Civano, F., Toft, S., Mccracken, H., Leauthaud, A., Taniguchi, Y., Cassata, P., Silverman, J., Vaccari, Mattia, Marchesi, S., Capak, P., Dunlop, J., Kartaltepe, J., Lilly, S., Salvato, M., Le Borgne, D., Pichon, C., Le Fevre, O., Smolcic, V., Fynbo, J., Le FlocH, E., Tasca, L., Sanders, D., Milvang-Jensen, B., Stockmann, M., Caputi, K., Aussel, H., Davidzon, I., Coupon, J., Zabl, J., Laigle, C., Scoville, N., Hasinger, G., Koekemoer, A., Chang, Y., Borgne, D., Fevre, O., FlocH, E., and Vaccari, M.
Abstract: International audience We present the COSMOS2015(24) catalog, which contains precise photometric redshifts and stellar masses for more than half a million objects over the 2deg(2) COSMOS field. Including new YJHK(s) images from the UltraVISTA-DR2 survey, Y-band images from Subaru/Hyper-Suprime-Cam, and infrared data from the Spitzer Large Area Survey with the Hyper-Suprime-Cam Spitzer legacy program, this near-infrared-selected catalog is highly optimized for the study of galaxy evolution and environments in the early universe. To maximize catalog completeness for bluer objects and at higher redshifts, objects have been detected on a chi(2) sum of the YJHK(s) and z(++) images. The catalog contains similar to 6 x 10(5) objects in the 1.5 deg(2) UltraVISTA-DR2 region and similar to 1.5 x 10(5) objects are detected in the “ultra-deep stripes” (0.62 deg(2)) at K-s \textless= 24.7 (3 sigma, 3 `, AB magnitude). Through a comparison with the zCOSMOS-bright spectroscopic redshifts, we measure a photometric redshift precision of sigma(Delta z(1) (+ zs)) = 0.007 and a catastrophic failure fraction of eta = 0.5%. At 3 \textless z \textless 6, using the unique database of spectroscopic redshifts in COSMOS, we find sigma(Delta z(1) (+ zs)) = 0.021 and eta = 13.2%. The deepest regions reach a 90% completeness limit of 10(10)M(circle dot) to z = 4. Detailed comparisons of the color distributions, number counts, and clustering show excellent agreement with the literature in the same mass ranges. COSMOS2015 represents a unique, publicly available, valuable resource with which to investigate the evolution of galaxies within their environment back to the earliest stages of the history of the universe. The COSMOS2015 catalog is distributed via anonymous ftp and through the usual astronomical archive systems (CDS, ESO Phase 3, IRSA).

37. The evolution of quiescent galaxies at high redshifts (z≥ 1.4)

Author: Domínguez Sánchez, H., Pozzi, F., Gruppioni, C., Cimatti, A., Ilbert, O., Pozzetti, L., McCracken, H., Capak, P., Le Floch, E., Salvato, M., Zamorani, G., Carollo, C. M., Contini, T., Kneib, J.-P, Le Fèvre, O., Lilly, S. J., Mainieri, V., Renzini, A., Scodeggio, M., Bardelli, S., Bolzonella, M., Bongiorno, A., Caputi, K., Coppa, G., Cucciati, O., de la Torre, S., de Ravel, L., Franzetti, P., Garilli, B., Iovino, A., Kampczyk, P., Knobel, C., Kovač, K., Lamareille, F., Le Borgne, J.-F, Le Brun, V., Maier, C., Mignoli, M., Pelló, R., Peng, Y., Perez-Montero, E., Ricciardelli, E., Silverman, J. D., Tanaka, M., Tasca, L. A. M., Tresse, L., Vergani, D., Zucca, E., Domínguez Sánchez, H., Pozzi, F., Gruppioni, C., Cimatti, A., Ilbert, O., Pozzetti, L., McCracken, H., Capak, P., Le Floch, E., Salvato, M., Zamorani, G., Carollo, C. M., Contini, T., Kneib, J.-P, Le Fèvre, O., Lilly, S. J., Mainieri, V., Renzini, A., Scodeggio, M., Bardelli, S., Bolzonella, M., Bongiorno, A., Caputi, K., Coppa, G., Cucciati, O., de la Torre, S., de Ravel, L., Franzetti, P., Garilli, B., Iovino, A., Kampczyk, P., Knobel, C., Kovač, K., Lamareille, F., Le Borgne, J.-F, Le Brun, V., Maier, C., Mignoli, M., Pelló, R., Peng, Y., Perez-Montero, E., Ricciardelli, E., Silverman, J. D., Tanaka, M., Tasca, L. A. M., Tresse, L., Vergani, D., and Zucca, E.
Abstract: The goal of this work is to study the evolution of high-redshift (z≥ 1.4) quiescent galaxies over an effective area of ∼1.7 deg2 in the COSMOS field. Galaxies have been divided according to their star formation activity and the evolution of the different populations, in particular of the quiescent galaxies, has been investigated in detail. We have studied an IRAC (mag 3.6 μm < 22.0) selected sample of ∼18 000 galaxies at z≥ 1.4 in the COSMOS field with multiwavelength coverage extending from the U band to the Spitzer 24 μm one. We have derived accurate photometric redshifts () through a SED-fitting procedure. Other important physical parameters [masses, ages and star formation rates (SFR)] of the galaxies have been obtained using Maraston models. We have divided our sample into actively star-forming, intermediate and quiescent galaxies depending on their specific star formation rate (SSFR = SFR/M). We have computed the galaxy stellar mass function (GSMF) of the total sample and the different populations at z= 1.4-3.0. We have studied the properties of high-redshift quiescent galaxies finding that they are old (1-4 Gyr), massive (〈M〉∼ 1010.65 M⊙), weakly star-forming stellar populations with low dust extinction [E(B−V) ≤ 0.15] and small e-folding time-scales (τ∼ 0.1-0.3 Gyr). We observe a significant evolution of the quiescent stellar mass function from 2.5 < z < 3.0 to 1.4 < z < 1.6, increasing by ∼1 dex in this redshift interval. We find that z∼ 1.5 is an epoch of transition of the GSMF: while the GSMF at z≳ 1.5 is dominated by the star-forming galaxies at all stellar masses, at z≲ 1.5 the contribution to the total GSMF of the quiescent galaxies is significant and becomes higher than that of the star-forming population for M≥ 1010.75 M⊙. The fraction of star-forming galaxies decreases from 60-20 per cent from z∼ 2.5-3.0 to 1.4-1.6 for M∼ 1011.0 M⊙, while the quiescent population increases from 10-50 per cent at the same redshift and mass intervals. We compare the f

38. The THESEUS space mission concept: science case, design and expected performances

Author: Amati L., O'Brien P., Götz D., Bozzo E., Tenzer C., Frontera F., Ghirlanda G., Labanti C., Osborne J., Stratta G., Tanvir N., Willingale R., Attina P., Campana R., Castro-Tirado A., Contini C., Fuschino F., Gomboc A., Hudec R., Orleanski P., Renotte E., Rodic T., Bagoly Z., Blain A., Callanan P., Covino S., Ferrara A., Le Floch E., Marisaldi M., Mereghetti S., Rosati P., Vacchi A., D'Avanzo P., Giommi P., Piranomonte S., Piro L., Reglero V., Rossi A., Santangelo A., Salvaterra R., Tagliaferri G., Vergani S., Vinciguerra S., Briggs M., Campolongo E., Ciolfi R., Connaughton V., Cordier B., Morelli B., Orlandini M., Adami C., Argan A., Atteia J., Auricchio N., Balazs L., Baldazzi G., Basa S., Basak R., Bellutti P., Bernardini M., Bertuccio G., Braga J., Branchesi M., Brandt S., Brocato E., Budtz-Jorgensen C., Bulgarelli A., Burderi L., Camp J., Capozziello S., Caruana J., Casella P., Cenko B., Chardonnet P., Ciardi B., Colafrancesco S., Dainotti M., D'Elia V., De Martino D., De Pasquale M., Del Monte E., Della Valle M., Drago A., Evangelista Y., Amati L., O'Brien P., Götz D., Bozzo E., Tenzer C., Frontera F., Ghirlanda G., Labanti C., Osborne J., Stratta G., Tanvir N., Willingale R., Attina P., Campana R., Castro-Tirado A., Contini C., Fuschino F., Gomboc A., Hudec R., Orleanski P., Renotte E., Rodic T., Bagoly Z., Blain A., Callanan P., Covino S., Ferrara A., Le Floch E., Marisaldi M., Mereghetti S., Rosati P., Vacchi A., D'Avanzo P., Giommi P., Piranomonte S., Piro L., Reglero V., Rossi A., Santangelo A., Salvaterra R., Tagliaferri G., Vergani S., Vinciguerra S., Briggs M., Campolongo E., Ciolfi R., Connaughton V., Cordier B., Morelli B., Orlandini M., Adami C., Argan A., Atteia J., Auricchio N., Balazs L., Baldazzi G., Basa S., Basak R., Bellutti P., Bernardini M., Bertuccio G., Braga J., Branchesi M., Brandt S., Brocato E., Budtz-Jorgensen C., Bulgarelli A., Burderi L., Camp J., Capozziello S., Caruana J., Casella P., Cenko B., Chardonnet P., Ciardi B., Colafrancesco S., Dainotti M., D'Elia V., De Martino D., De Pasquale M., Del Monte E., Della Valle M., Drago A., and Evangelista Y.
Abstract: © 2018 COSPAR THESEUS is a space mission concept aimed at exploiting Gamma-Ray Bursts for investigating the early Universe and at providing a substantial advancement of multi-messenger and time-domain astrophysics. These goals will be achieved through a unique combination of instruments allowing GRB and X-ray transient detection over a broad field of view (more than 1sr) with 0.5–1 arcmin localization, an energy band extending from several MeV down to 0.3 keV and high sensitivity to transient sources in the soft X-ray domain, as well as on-board prompt (few minutes) follow-up with a 0.7 m class IR telescope with both imaging and spectroscopic capabilities. THESEUS will be perfectly suited for addressing the main open issues in cosmology such as, e.g., star formation rate and metallicity evolution of the inter-stellar and intra-galactic medium up to redshift ∼10, signatures of Pop III stars, sources and physics of re-ionization, and the faint end of the galaxy luminosity function. In addition, it will provide unprecedented capability to monitor the X-ray variable sky, thus detecting, localizing, and identifying the electromagnetic counterparts to sources of gravitational radiation, which may be routinely detected in the late ’20s/early ’30s by next generation facilities like aLIGO/ aVirgo, eLISA, KAGRA, and Einstein Telescope. THESEUS will also provide powerful synergies with the next generation of multi-wavelength observatories (e.g., LSST, ELT, SKA, CTA, ATHENA).

39. The THESEUS space mission concept: science case, design and expected performances

Author: Martino Marisaldi, Enrico Bozzo, Valerie Connaughton, Dorottya Szécsi, D. Malesani, L. Maraschi, B. Cordier, P. D'Avanzo, Salvatore Capozziello, Darach Watson, C. Contini, Maryam Modjaz, Pierluigi Bellutti, M. de Pasquale, C. Guidorzi, Colleen A. Wilson-Hodge, O. Boulade, C. Adami, Y. Evangelista, A. Argan, Johan P. U. Fynbo, Y.-W. Dong, Poshak Gandhi, Allan Hornstrup, Eliana Palazzi, Andrea Bulgarelli, Andrea Comastri, E. Geza, Luciano Burderi, Giuseppe Malaguti, D. de Martino, Irfan Kuvvetli, S.-N. Zhang, Claudio Labanti, Fiamma Capitanio, Luca Izzo, Bradley Cenko, A. Melandri, Umberto Maio, Nicola Omodei, Stefano Ettori, C. Butler, S. D. Vergani, S. Zhang, Lajos G. Balázs, Patricia Schady, Federica B. Bianco, M. Branchesi, Jens Hjorth, Jochen Greiner, Felix Ryde, Jean-Gabriel Cuby, Piero Malcovati, Lorraine Hanlon, Peter G. Jonker, M. Della Valle, Elena Pian, Piotr Orleanski, Etienne Renotte, W. Skidmore, L. Sabau-Graziati, Mauro Dadina, Carl Budtz-Jørgensen, Tomaz Rodic, Giancarlo Ghirlanda, Luigi Piro, Sheila McBreen, M. Fiorini, M. Topinka, Jan Harms, Riccardo Ciolfi, Yi Chen, Giacomo Vianello, Ester Piedipalumbo, Zsolt Bagoly, Aniello Grado, Yuki Kaneko, Vito Sguera, B. Morelli, E. Le Floc'h, Luciano Rezzolla, K. Wiersema, Remo Ruffini, E. Del Monte, J. P. Osborne, M. G. Bernardini, A. Gomboc, A. De Luca, Stefano Covino, Ian Hutchinson, A. Antonelli, Enzo Brocato, Mark R. Sims, M. Razzano, Elisabetta Maiorano, Jean-Luc Atteia, J. Zicha, S. Korpela, Eros Vanzella, V. D'Elia, M. H. P. M. van Putten, Marco Feroci, Carole Mundell, A. V. Penacchioni, J. Soomin, Gabriele Ghisellini, Sandra Savaglio, N. Shigehiro, Andrea Santangelo, Antonio Martin-Carrillo, Avishay Gal-Yam, A. M. Read, Piergiorgio Casella, Giuseppe Baldazzi, B. Ciardi, Pawan Kumar, Li Song, V. Lebrun, G. Zampa, Daisuke Yonetoku, S. Vojtech, Gregor Rauw, Piero Rosati, A. J. Castro-Tirado, Bruce Gendre, Tsvi Piran, A. Rachevski, S. Basa, T. Li, Michela Uslenghi, Gianluca Morgante, Michèle Lavagna, Pascal Chardonnet, Andrew MacFadyen, Asaf Pe'er, Sandro Mereghetti, Alessandro Drago, M. Hafizi, Richard Willingale, D. Morris, Bing Zhang, Paolo Giommi, Andrea Ferrara, Mauro Orlandini, Maria Giovanna Dainotti, N. Masetti, Yuji Urata, Maxim Lyutikov, A. Vacchi, László L. Kiss, E. Campolongo, M. Boer, Lorenzo Amati, Diego Götz, Andrew Blain, M. T. Botticella, C. Tenzer, Monica Colpi, Victor Reglero, Roberto Mignani, Michael S. Briggs, Joseph Caruana, Elizabeth R. Stanway, S. Colafrancesco, Francesca Panessa, H. U. Nargaard-Nielsen, F. Lu, Giuseppe Bertuccio, A. Paizis, P. Romano, S. Vercellone, Luciano Nicastro, S. Paltani, G. Pareschi, G. Stratta, V. Petrosian, João Braga, N. Zampa, Nial Tanvir, James E. Rhoads, Raffaella Margutti, Luca Valenziano, Søren Brandt, S. Boci, Andrea Rossi, Paul J. Callanan, Annalisa Celotti, N. Kawai, René Hudec, Francesco Longo, Primo Attina, G. L. Israel, F. Fuschino, Fabio Finelli, M. Hernanz, Ruben Salvaterra, F. Frontera, P. T. O'Brien, Sergio Campana, Rupal Basak, Riccardo Campana, Eleonora Troja, Jordan Camp, Petr Páta, S. Piranomonte, G. Tagliaferri, Sylvain Guiriec, R. L. C. Starling, B. B. Zhang, Natalia Auricchio, Serena Vinciguerra, Département d'Astrophysique (ex SAP) (DAP), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Galaxies, Etoiles, Physique, Instrumentation (GEPI), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Astrophysique de Marseille (LAM), 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), Institut de recherche en astrophysique et planétologie (IRAP), Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Observatoire Midi-Pyrénées (OMP), Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Annecy-le-Vieux de Physique Théorique (LAPTH), Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), Astrophysique Relativiste Théories Expériences Métrologie Instrumentation Signaux (ARTEMIS), Université Nice Sophia Antipolis (... - 2019) (UNS), Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Agenzia Spaziale Italiana, European Commission, Czech Grant Agency, ITA, 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), 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), Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Nice Sophia Antipolis (... - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA), THESEUS, Amati, L, O'Brien, P, Götz, D, Bozzo, E, Tenzer, C, Frontera, F, Ghirlanda, G, Labanti, C, Osborne, J, Stratta, G, Tanvir, N, Willingale, R, Attina, P, Campana, R, Castro-Tirado, A, Contini, C, Fuschino, F, Gomboc, A, Hudec, R, Orleanski, P, Renotte, E, Rodic, T, Bagoly, Z, Blain, A, Callanan, P, Covino, S, Ferrara, A, Le Floch, E, Marisaldi, M, Mereghetti, S, Rosati, P, Vacchi, A, D'Avanzo, P, Giommi, P, Piranomonte, S, Piro, L, Reglero, V, Rossi, A, Santangelo, A, Salvaterra, R, Tagliaferri, G, Vergani, S, Vinciguerra, S, Briggs, M, Campolongo, E, Ciolfi, R, Connaughton, V, Cordier, B, Morelli, B, Orlandini, M, Adami, C, Argan, A, Atteia, J, Auricchio, N, Balazs, L, Baldazzi, G, Basa, S, Basak, R, Bellutti, P, Bernardini, M, Bertuccio, G, Braga, J, Branchesi, M, Brandt, S, Brocato, E, Budtz-Jorgensen, C, Bulgarelli, A, Burderi, L, Camp, J, Capozziello, S, Caruana, J, Casella, P, Cenko, B, Chardonnet, P, Ciardi, B, Colafrancesco, S, Dainotti, M, D'Elia, V, De Martino, D, De Pasquale, M, Del Monte, E, Della Valle, M, Drago, A, Evangelista, Y, Feroci, M, Finelli, F, Fiorini, M, Fynbo, J, Gal-Yam, A, Gendre, B, Ghisellini, G, Grado, A, Guidorzi, C, Hafizi, M, Hanlon, L, Hjorth, J, Izzo, L, Kiss, L, Kumar, P, Kuvvetli, I, Lavagna, M, Li, T, Longo, F, Lyutikov, M, Maio, U, Maiorano, E, Malcovati, P, Malesani, D, Margutti, R, Martin-Carrillo, A, Masetti, N, Mcbreen, S, Mignani, R, Morgante, G, Mundell, C, Nargaard-Nielsen, H, Nicastro, L, Palazzi, E, Paltani, S, Panessa, F, Pareschi, G, Pe'Er, A, Penacchioni, A, Pian, E, Piedipalumbo, E, Piran, T, Rauw, G, Razzano, M, Read, A, Rezzolla, L, Romano, P, Ruffini, R, Savaglio, S, Sguera, V, Schady, P, Skidmore, W, Song, L, Stanway, E, Starling, R, Topinka, M, Troja, E, van Putten, M, Vanzella, E, Vercellone, S, Wilson-Hodge, C, Yonetoku, D, Zampa, G, Zampa, N, Zhang, B, Zhang, S, Antonelli, A, Bianco, F, Boci, S, Boer, M, Botticella, M, Boulade, O, Butler, C, Campana, S, Capitanio, F, Celotti, A, Chen, Y, Colpi, M, Comastri, A, Cuby, J, Dadina, M, De Luca, A, Dong, Y, Ettori, S, Gandhi, P, Geza, E, Greiner, J, Guiriec, S, Harms, J, Hernanz, M, Hornstrup, A, Hutchinson, I, Israel, G, Jonker, P, Kaneko, Y, Kawai, N, Wiersema, K, Korpela, S, Lebrun, V, Lu, F, Macfadyen, A, Malaguti, G, Maraschi, L, Melandri, A, Modjaz, M, Morris, D, Omodei, N, Paizis, A, Páta, P, Petrosian, V, Rachevski, A, Rhoads, J, Ryde, F, Sabau-Graziati, L, Shigehiro, N, Sims, M, Soomin, J, Szécsi, D, Urata, Y, Uslenghi, M, Valenziano, L, Vianello, G, Vojtech, S, Watson, D, Zicha, J, Amati, L., O'Brien, P., Götz, D., Bozzo, E., Tenzer, C., Frontera, F., Ghirlanda, G., Labanti, C., Osborne, J. P., Stratta, G., Tanvir, N., Willingale, R., Attina, P., Campana, R., Castro-Tirado, A. J., Contini, C., Fuschino, F., Gomboc, A., Hudec, R., Orleanski, P., Renotte, E., Rodic, T., Bagoly, Z., Blain, A., Callanan, P., Covino, S., Ferrara, A., Le Floch, E., Marisaldi, M., Mereghetti, S., Rosati, P., Vacchi, A., D'Avanzo, P., Giommi, P., Piranomonte, S., Piro, L., Reglero, V., Rossi, A., Santangelo, A., Salvaterra, R., Tagliaferri, G., Vergani, S., Vinciguerra, S., Briggs, M., Campolongo, E., Ciolfi, R., Connaughton, V., Cordier, B., Morelli, B., Orlandini, M., Adami, C., Argan, A., Atteia, J. -L., Auricchio, N., Balazs, L., Baldazzi, G., Basa, S., Basak, R., Gian Luca, Israel, Bellutti, P., Bernardini, M. G., Bertuccio, G., Braga, J., Branchesi, M., Brandt, S., Brocato, E., Budtz-Jorgensen, C., Bulgarelli, A., Burderi, L., Camp, J., Capozziello, S., Caruana, J., Casella, P., Cenko, B., Chardonnet, P., Ciardi, B., Colafrancesco, S., Dainotti, M. G., D'Elia, V., De Martino, D., De Pasquale, M., Del Monte, E., Della Valle, M., Drago, A., Evangelista, Y., Feroci, M., Finelli, F., Fiorini, M., Fynbo, J., Gal-Yam, A., Gendre, B., Ghisellini, G., Grado, A., Guidorzi, C., Hafizi, M., Hanlon, L., Hjorth, J., Izzo, L., Kiss, L., Kumar, P., Kuvvetli, I., Lavagna, M., Li, T., Longo, F., Lyutikov, M., Maio, U., Maiorano, E., Malcovati, P., Malesani, D., Margutti, R., Martin-Carrillo, A., Masetti, N., Mcbreen, S., Mignani, R., Morgante, G., Mundell, C., Nargaard-Nielsen, H. U., Nicastro, L., Palazzi, E., Paltani, S., Panessa, F., Pareschi, G., Pe'Er, A., Penacchioni, A. V., Pian, E., Piedipalumbo, E., Piran, T., Rauw, G., Razzano, M., Read, A., Rezzolla, L., Romano, P., Ruffini, R., Savaglio, S., Sguera, V., Schady, P., Skidmore, W., Song, L., Stanway, E., Starling, R., Topinka, M., Troja, E., van Putten, M., Vanzella, E., Vercellone, S., Wilson-Hodge, C., Yonetoku, D., Zampa, G., Zampa, N., Zhang, B., Zhang, B. B., Zhang, S., Zhang, S. -N., Antonelli, A., Bianco, F., Boci, S., Boer, M., Botticella, M. T., Boulade, O., Butler, C., Campana, S., Capitanio, F., Celotti, A., Chen, Y., Colpi, M., Comastri, A., Cuby, J. -G., Dadina, M., De Luca, A., Dong, Y. -W., Ettori, S., Gandhi, P., Geza, E., Greiner, J., Guiriec, S., Harms, J., Hernanz, M., Hornstrup, A., Hutchinson, I., Israel, G., Jonker, P., Kaneko, Y., Kawai, N., Wiersema, K., Korpela, S., Lebrun, V., Lu, F., Macfadyen, A., Malaguti, G., Maraschi, L., Melandri, A., Modjaz, M., Morris, D., Omodei, N., Paizis, A., Páta, P., Petrosian, V., Rachevski, A., Rhoads, J., Ryde, F., Sabau-Graziati, L., Shigehiro, N., Sims, M., Soomin, J., Szécsi, D., Urata, Y., Uslenghi, M., Valenziano, L., Vianello, G., Vojtech, S., Watson, D., Zicha, J., 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), 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), ANR-16-CE31-0003,BEaPro,Using the most powerful explosion as probes of the high-redshift Universe(2016), Galaxies, Etoiles, Physique, Instrumentation ( GEPI ), Institut national des sciences de l'Univers ( INSU - CNRS ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Centre National de la Recherche Scientifique ( CNRS ), Laboratoire d'Astrophysique de Marseille ( LAM ), Aix Marseille Université ( AMU ) -Institut national des sciences de l'Univers ( INSU - CNRS ) -Centre National d'Etudes Spatiales ( CNES ) -Centre National de la Recherche Scientifique ( CNRS ), Institut de recherche en astrophysique et planétologie ( IRAP ), Université Paul Sabatier - Toulouse 3 ( UPS ) -Observatoire Midi-Pyrénées ( OMP ) -Centre National de la Recherche Scientifique ( CNRS ), Laboratoire d'Annecy-le-Vieux de Physique Théorique ( LAPTH ), Université Savoie Mont Blanc ( USMB [Université de Savoie] [Université de Chambéry] ) -Centre National de la Recherche Scientifique ( CNRS ), Astrophysique Relativiste Théories Expériences Métrologie Instrumentation Signaux ( ARTEMIS ), Université Nice Sophia Antipolis ( UNS ), Université Côte d'Azur ( UCA ) -Université Côte d'Azur ( UCA ) -Institut national des sciences de l'Univers ( INSU - CNRS ) -Observatoire de la Côte d'Azur, Université Côte d'Azur ( UCA ) -Centre National de la Recherche Scientifique ( CNRS ), Gotz, D., Pata, P., Szecsi, D., Department of Physics, and Amati, L. and O'Brien, P. and Götz, D. and Bozzo, E. and Tenzer, C. and Frontera, F. and Ghirlanda, G. and Labanti, C. and Osborne, J.P. and Stratta, G. and Tanvir, N. and Willingale, R. and Attina, P. and Campana, R. and Castro-Tirado, A.J. and Contini, C. and Fuschino, F. and Gomboc, A. and Hudec, R. and Orleanski, P. and Renotte, E. and Rodic, T. and Bagoly, Z. and Blain, A. and Callanan, P. and Covino, S. and Ferrara, A. and Le Floch, E. and Marisaldi, M. and Mereghetti, S. and Rosati, P. and Vacchi, A. and D'Avanzo, P. and Giommi, P. and Piranomonte, S. and Piro, L. and Reglero, V. and Rossi, A. and Santangelo, A. and Salvaterra, R. and Tagliaferri, G. and Vergani, S. and Vinciguerra, S. and Briggs, M. and Campolongo, E. and Ciolfi, R. and Connaughton, V. and Cordier, B. and Morelli, B. and Orlandini, M. and Adami, C. and Argan, A. and Atteia, J.-L. and Auricchio, N. and Balazs, L. and Baldazzi, G. and Basa, S. and Basak, R. and Bellutti, P. and Bernardini, M.G. and Bertuccio, G. and Braga, J. and Branchesi, M. and Brandt, S. and Brocato, E. and Budtz-Jorgensen, C. and Bulgarelli, A. and Burderi, L. and Camp, J. and Capozziello, S. and Caruana, J. and Casella, P. and Cenko, B. and Chardonnet, P. and Ciardi, B. and Colafrancesco, S. and Dainotti, M.G. and D'Elia, V. and De Martino, D. and De Pasquale, M. and Del Monte, E. and Della Valle, M. and Drago, A. and Evangelista, Y. and Feroci, M. and Finelli, F. and Fiorini, M. and Fynbo, J. and Gal-Yam, A. and Gendre, B. and Ghisellini, G. and Grado, A. and Guidorzi, C. and Hafizi, M. and Hanlon, L. and Hjorth, J. and Izzo, L. and Kiss, L. and Kumar, P. and Kuvvetli, I. and Lavagna, M. and Li, T. and Longo, F. and Lyutikov, M. and Maio, U. and Maiorano, E. and Malcovati, P. and Malesani, D. and Margutti, R. and Martin-Carrillo, A. and Masetti, N. and McBreen, S. and Mignani, R. and Morgante, G. and Mundell, C. and Nargaard-Nielsen, H.U. and Nicastro, L. and Palazzi, E. and Paltani, S. and Panessa, F. and Pareschi, G. and Pe'er, A. and Penacchioni, A.V. and Pian, E. and Piedipalumbo, E. and Piran, T. and Rauw, G. and Razzano, M. and Read, A. and Rezzolla, L. and Romano, P. and Ruffini, R. and Savaglio, S. and Sguera, V. and Schady, P. and Skidmore, W. and Song, L. and Stanway, E. and Starling, R. and Topinka, M. and Troja, E. and van Putten, M. and Vanzella, E. and Vercellone, S. and Wilson-Hodge, C. and Yonetoku, D. and Zampa, G. and Zampa, N. and Zhang, B. and Zhang, B.B. and Zhang, S. and Zhang, S.-N. and Antonelli, A. and Bianco, F. and Boci, S. and Boer, M. and Botticella, M.T. and Boulade, O. and Butler, C. and Campana, S. and Capitanio, F. and Celotti, A. and Chen, Y. and Colpi, M. and Comastri, A. and Cuby, J.-G. and Dadina, M. and De Luca, A. and Dong, Y.-W. and Ettori, S. and Gandhi, P. and Geza, E. and Greiner, J. and Guiriec, S. and Harms, J. and Hernanz, M. and Hornstrup, A. and Hutchinson, I. and Israel, G. and Jonker, P. and Kaneko, Y. and Kawai, N. and Wiersema, K. and Korpela, S. and Lebrun, V. and Lu, F. and MacFadyen, A. and Malaguti, G. and Maraschi, L. and Melandri, A. and Modjaz, M. and Morris, D. and Omodei, N. and Paizis, A. and Páta, P. and Petrosian, V. and Rachevski, A. and Rhoads, J. and Ryde, F. and Sabau-Graziati, L. and Shigehiro, N. and Sims, M. and Soomin, J. and Szécsi, D. and Urata, Y. and Uslenghi, M. and Valenziano, L. and Vianello, G. and Vojtech, S. and Watson, D. and Zicha, J.
Subjects: Ionization, Atmospheric Science, cosmological model, Cherenkov Telescope Array, [ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph], Astronomy, Dark age, MASSIVE SINGLE STARS, Star formation rates, Gamma ray, 01 natural sciences, Cosmology: observation, localization, law.invention, Astrophysic, Einstein Telescope, observational cosmology, law, Observational cosmology, Re-ionization, Cosmology: observations, Dark ages, First stars, Gamma-ray: bursts, LIGO, observations [Cosmology], Telescope, 010303 astronomy & astrophysics, High sensitivity, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, Multi-wavelength, energy: high, sezele, gamma-ray bursts, Aerospace Engineering, Space and Planetary Science, Astrophysics::Instrumentation and Methods for Astrophysics, imaging, star: formation, burst [Gamma-ray], observatory, Geophysics, X rays, Cosmology: observation, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, signature, Star, TIDAL DISRUPTION, Gamma-ray: burst, Astrophysics::High Energy Astrophysical Phenomena, SIMILAR-TO 6, Socio-culturale, FOS: Physical sciences, observation [Cosmology], galaxy: luminosity, X-ray astronomy: instrumentation, 7 CANDIDATE GALAXIES, Astrophysics::Cosmology and Extragalactic Astrophysics, gamma ray: burst, 114 Physical sciences, Settore FIS/03 - Fisica della Materia, X-ray, bursts [Gamma-ray], FIS/05 - ASTRONOMIA E ASTROFISICA, Settore FIS/05 - Astronomia e Astrofisica, First star, 0103 physical sciences, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], KAGRA, Instrumentation and Methods for Astrophysics (astro-ph.IM), Astrophysics::Galaxy Astrophysics, LIGHT CURVES, 010308 nuclear & particles physics, Gravitational wave, gravitational radiation, Astronomy and Astrophysics, 115 Astronomy, Space science, redshift, sensitivity, Redshift, NEUTRON-STAR MERGER, messenger, VIRGO, electromagnetic, LUMINOSITY FUNCTION, BLACK-HOLE, General Earth and Planetary Sciences, Gamma-ray burst, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract: THESEUS is a space mission concept aimed at exploiting Gamma-Ray Bursts for investigating the early Universe and at providing a substantial advancement of multi-messenger and time-domain astrophysics. These goals will be achieved through a unique combination of instruments allowing GRB and X-ray transient detection over a broad field of view (more than 1sr) with 0.5¿1 arcmin localization, an energy band extending from several MeV down to 0.3¿keV and high sensitivity to transient sources in the soft X-ray domain, as well as on-board prompt (few minutes) follow-up with a 0.7¿m class IR telescope with both imaging and spectroscopic capabilities. THESEUS will be perfectly suited for addressing the main open issues in cosmology such as, e.g., star formation rate and metallicity evolution of the inter-stellar and intra-galactic medium up to redshift 10, signatures of Pop III stars, sources and physics of re-ionization, and the faint end of the galaxy luminosity function. In addition, it will provide unprecedented capability to monitor the X-ray variable sky, thus detecting, localizing, and identifying the electromagnetic counterparts to sources of gravitational radiation, which may be routinely detected in the late ¿20s/early ¿30s by next generation facilities like aLIGO/ aVirgo, eLISA, KAGRA, and Einstein Telescope. THESEUS will also provide powerful synergies with the next generation of multi-wavelength observatories (e.g., LSST, ELT, SKA, CTA, ATHENA).© 2018 COSPAR, S.E. acknowledges the financial support from contracts ASI-INAF 1/009/10/0, NARO15 ASI-INAF 1/037/12/0 and ASI 2015-046-R.0. R.H. acknowledges GACR grant 13-33324S. S.V. research leading to these results has received funding from the European Union's Seventh Framework Programme for research, technological development and demonstration under grant agreement no 606176. D.S. was supported by the Czech grant 1601116S GA CR. Maria Giovanna Dainotti acknowledges funding from the European Union through the Marie Curie Action FP7-PEOPLE-2013-IOF, under grant agreement No. 626267 (>Cosmological Candles>).
Published: 2018

40. Weak Association Between Genetic Markers of Hyperuricemia and Cardiorenal Outcomes: Insights From the STANISLAS Study Cohort With a 20‐Year Follow‐Up

Author: Mehmet Kanbay, Constance Xhaard, Edith Le Floch, Claire Dandine‐Roulland, Nicolas Girerd, João Pedro Ferreira, Jean‐Marc Boivin, Sandra Wagner, Delphine Bacq‐Daian, Jean‐François Deleuze, Faiez Zannad, Patrick Rossignol, Koç University, Défaillance Cardiovasculaire Aiguë et Chronique (DCAC), Centre Hospitalier Régional Universitaire de Nancy (CHRU Nancy)-Institut National de la Santé et de la Recherche Médicale (INSERM)-Université de Lorraine (UL), Centre d'investigation clinique plurithématique Pierre Drouin [Nancy] (CIC-P), Centre d'investigation clinique [Nancy] (CIC), Centre Hospitalier Régional Universitaire de Nancy (CHRU Nancy)-Institut National de la Santé et de la Recherche Médicale (INSERM)-Université de Lorraine (UL)-Centre Hospitalier Régional Universitaire de Nancy (CHRU Nancy)-Institut National de la Santé et de la Recherche Médicale (INSERM)-Université de Lorraine (UL), Cardiovascular and Renal Clinical Trialists [Vandoeuvre-les-Nancy] (INI-CRCT), Institut Lorrain du Coeur et des Vaisseaux Louis Mathieu [Nancy], French-Clinical Research Infrastructure Network - F-CRIN [Paris] (Cardiovascular & Renal Clinical Trialists - CRCT ), Centre National de Recherche en Génomique Humaine (CNRGH), Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Institut de Biologie François JACOB (JACOB), Direction de Recherche Fondamentale (CEA) (DRF (CEA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA), The STANISLAS (Suivi Temporaire Annuel Non‐Invasif de la Santé des Lorrains Assurés Sociaux) study is sponsored by the Nancy Centre Hospitalier Régional Universitaire. This work is supported by the French Ministry of Health 'Programme Hospitalier de Recherche Clinique Inter regional 2013,' by the Contrat de Plan Etat‐Lorraine and Fonds Européen de Développement Régional Lorraine, and a public grant overseen by the French National Research Agency (ANR) as part of the second 'Investissements d’Avenir' program FIGHT‐heart failure (reference: ANR‐15‐RHU‐0004) and by the French Plan d'Investissement d'Avenir project 'Lorraine Université d’Excellence,' reference ANR‐15‐IDEX‐04‐LUE. It is also supported by the European Fibro‐Targets Project (grant agreement No. SP7#602904), European HOMAGE project (grant agreement No. Heart 'Omics' in Ageing, 7th Framework Program grant No. 305507), the MEDIA project (Européen 'Cooperation'–Theme 'Health'/FP7‐HEALTH‐2010‐single‐stage (reference: 261409), FOCUS‐MR (reference: ANR‐15‐CE14‐0032‐01), ERA‐CVD EXPERT (reference: ANR‐16‐ECVD‐0002‐02), and the Fondation de Recherche en Hypertension Artérielle., ANR-15-RHUS-0004,FIGHT-HF,Combattre l'insuffisance cardiaque(2015), ANR-15-IDEX-0004,LUE,Isite LUE(2015), ANR-15-CE14-0032,MR-focus,Régulation, Diagnostique et Thérapeutique ciblée du récepteur minéralocorticoïde dans le remodelage cardiaque(2015), ANR-16-ECVD-0002,EXPERT,Exploring new pathways in age-related heart diseases(2016), European Project: SP7#602904, European Project: 305507, European Project: 261409,EU FP 7 MEDIA project, Université de Lorraine (UL)-Institut National de la Santé et de la Recherche Médicale (INSERM)-Centre Hospitalier Régional Universitaire de Nancy (CHRU Nancy), Université de Lorraine (UL)-Centre Hospitalier Régional Universitaire de Nancy (CHRU Nancy)-Institut National de la Santé et de la Recherche Médicale (INSERM)-Université de Lorraine (UL)-Centre Hospitalier Régional Universitaire de Nancy (CHRU Nancy)-Institut National de la Santé et de la Recherche Médicale (INSERM), BOZEC, Erwan, Combattre l'insuffisance cardiaque - - FIGHT-HF2015 - ANR-15-RHUS-0004 - RHUS - VALID, ISITE - Isite LUE - - LUE2015 - ANR-15-IDEX-0004 - IDEX - VALID, Régulation, Diagnostique et Thérapeutique ciblée du récepteur minéralocorticoïde dans le remodelage cardiaque - - MR-focus2015 - ANR-15-CE14-0032 - AAPG2015 - VALID, Exploring new pathways in age-related heart diseases - - EXPERT2016 - ANR-16-ECVD-0002 - ERA-CVD - VALID, European Fibro‐Targets Project - SP7#602904 - INCOMING, HOMAGE (Heart Omics in Ageing consortium) - 305507 - INCOMING, The MEtabolic Road to DIAstolic Heart Failure - EU FP 7 MEDIA project - 261409 - INCOMING, Kanbay, Mehmet (ORCID 0000-0002-1297-0675 & YÖK ID 110580), Xhaard, C., Le Floch, E., Dandine-Roulland, C., Girerd, N., Ferreira, J.P., Boivin, J.M., Wagner, S., Bacq Daian, D., Deleuze, J.F., Zannad, F., Rossignol, P., and School of Medicine
Subjects: Genetic Markers, Glucose Transport Proteins, Facilitative, Hyperuricemia, Cardiovascular system and cardiology, Blood Pressure Monitoring, Ambulatory, Pulse Wave Analysis, Carotid Intima-Media Thickness, Polymorphism, Single Nucleotide, [SDV.MHEP.CSC] Life Sciences [q-bio]/Human health and pathology/Cardiology and cardiovascular system, Uric Acid, Cardiovascular disease, Genome-wide, Association study, Single-nucleotide Polymorphism, Uric acid, [SDV.MHEP.CSC]Life Sciences [q-bio]/Human health and pathology/Cardiology and cardiovascular system, Risk Factors, Humans, Cardiology and Cardiovascular Medicine, Follow-Up Studies, Genome-Wide Association Study
Abstract: Background: Hyperuricemia is associated with poor cardiovascular outcomes, although it is uncertain whether this relationship is causal in nature. This study aimed to: (1) assess the heritability of serum uric acid (SUA) levels, (2) conduct a genome-wide association study on SUA levels, and (3) investigate the association between certain single-nucleotide polymorphisms and target organ damage. Methods and results: the STANISLAS (Suivi Temporaire Annuel Non-Invasif de la Sante des Lorrains Assures Sociaux) study cohort is a single-center longitudinal cohort recruited between 1993 and 1995 (visit 1), with a last visit (visit 4 [V4]) performed approximate to 20 years apart. Serum lipid profile, SUA, urinary albumin/creatinine ratio, estimated glomerular filtration rate, 24-hour ambulatory blood pressure monitoring, transthoracic echocardiography, pulse wave velocity, and genotyping for each participant were assessed at V4. A total of 1573 participants were included at V4, among whom 1417 had available SUA data at visit 1. Genome-wide association study results highlighted multiple single-nucleotide polymorphisms on the SLC2A9 gene linked to SUA levels. Carriers of the most associated mutated SLC2A9 allele (rs16890979) had significantly lower SUA levels. Although SUA level at V4 was highly associated with diabetes, prediabetes, higher body mass index, CRP (C-reactive protein) levels, estimated glomerular filtration rate variation (visit 1-V4), carotid intima-media thickness, and pulse wave velocity, rs16890979 was only associated with higher carotid intima-media thickness. Conclusions: our findings demonstrate that rs16890979, a genetic determinant of SUA levels located on the SLC2A9 gene, is associated with carotid intima-media thickness despite significant associations between SUA levels and several clinical outcomes, thereby lending support to the hypothesis of a link between SUA and cardiovascular disease., Nancy Centre Hospitalier Regional Universitaire; French Ministry of Health; French National Research Agency (ANR); Contrat de Plan Etat?Lorraine and Fonds Européen de Développement Régional Lorraine; Programme Hospitalier de Recherche Clinique Inter regional 2013; Investissements d’Avenir; FIGHT?heart failure; French Plan d'Investissement d'Avenir project “Lorraine Université d’Excellence; European Union (EU); European Fibro?Targets Project; European HOMAGE project; 7th Framework Program; MEDIA project; FOCUS?MR; ERA?CVD EXPERT; Fondation de Recherche en Hypertension Artérielle
Published: 2022

41. Gamma ray burst studies with THESEUS

Author: Lara Nava, Gor Oganesyan, Lorenzo Amati, Diego Götz, Enrico Bozzo, Giancarlo Ghirlanda, P. T. O'Brien, M. Topinka, S. Ascenzi, M. E. Ravasio, A. Melandri, Sandro Mereghetti, A. E. Camisasca, M. Hafizi, M. Toffano, Andrew Blain, Giulia Stratta, Silvia Zane, A. I. Bogomazov, S. Ronchini, Piero Rosati, Ruben Salvaterra, E. Le Floc'h, Marica Branchesi, P. D'Avanzo, M. G. Bernardini, A. J. Castro-Tirado, S. D. Vergani, Nial R. Tanvir, J. P. Osborne, S. Mandhai, C. Guidorzi, Asaf Pe'er, Istituto Nazionale di Astrofisica, Ghirlanda, G, Salvaterra, R, Toffano, M, Ronchini, S, Guidorzi, C, Oganesyan, G, Ascenzi, S, Bernardini, M, Camisasca, A, Mereghetti, S, Nava, L, Ravasio, M, Branchesi, M, Castro-Tirado, A, Amati, L, Blain, A, Bozzo, E, O'Brien, P, Gotz, D, Le Floch, E, Osborne, J, Rosati, P, Stratta, G, Tanvir, N, Bogomazov, A, D'Avanzo, P, Hafizi, M, Mandhai, S, Melandri, A, Peer, A, Topinka, M, Vergani, S, Zane, S, Astrophysique Interprétation Modélisation (AIM (UMR7158 / UMR_E_9005 / UM_112)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), 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)-Centre National de la Recherche Scientifique (CNRS), 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), and 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)
Subjects: Gamma ray burst, Jet structure, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, Gamma ray bursts, Synchrotron radiation, Jet structure, Spectral line, Gamma ray bursts, NO, Astrophysical jet, 0103 physical sciences, Emission spectrum, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], 010306 general physics, 010303 astronomy & astrophysics, Instrumentation and Methods for Astrophysics (astro-ph.IM), Luminosity function, Astrophysics::Galaxy Astrophysics, Physics, Synchrotron radiation, Astronomy and Astrophysics, Redshift, Afterglow, Stars, Space and Planetary Science, Gamma-ray burst, Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: Gamma-ray Bursts (GRBs) are the most powerful transients in the Universe, over-shining for a few seconds all other $\gamma$-ray sky sources. Their emission is produced within narrowly collimated relativistic jets launched after the core-collapse of massive stars or the merger of compact binaries. THESEUS will open a new window for the use of GRBs as cosmological tools by securing a statistically significant sample of high-$z$ GRBs, as well as by providing a large number of GRBs at low-intermediate redshifts extending the current samples to low luminosities. The wide energy band and unprecedented sensitivity of the Soft X-ray Imager (SXI) and X-Gamma rays Imaging Spectrometer (XGIS) instruments provide us a new route to unveil the nature of the prompt emission. For the first time, a full characterisation of the prompt emission spectrum from 0.3 keV to 10 MeV with unprecedented large count statistics will be possible revealing the signatures of synchrotron emission. SXI spectra, extending down to 0.3 keV, will constrain the local metal absorption and, for the brightest events, the progenitors' ejecta composition. Investigation of the nature of the internal energy dissipation mechanisms will be obtained through the systematic study with XGIS of the sub-second variability unexplored so far over such a wide energy range. THESEUS will follow the spectral evolution of the prompt emission down to the soft X-ray band during the early steep decay and through the plateau phase with the unique ability of extending above 10 keV the spectral study of these early afterglow emission phases., Comment: Submitted to Experimental Astronomy
Published: 2021

42. Tracing the cosmic growth of supermassive black holes to z ∼ 3 with Herschel★

Author: Giovanni Cresci, G. Zamorani, Marco Scodeggio, Alessandro Cimatti, A. Feltre, P. Popesso, Ivan Delvecchio, Alvio Renzini, M. Carollo, Benjamin Magnelli, Carlotta Gruppioni, Mattia Vaccari, Douglas Scott, E. Le Floc'h, O. Le Fevre, Francesca Pozzi, Simon J. Lilly, S. Berta, Jacopo Fritz, Asantha Cooray, Dieter Lutz, J. J. Bock, Cristian Vignali, Vincenzo Mainieri, Seb Oliver, Thierry Contini, Delvecchio I., Gruppioni C., Pozzi F., Berta S., Zamorani G., Cimatti A., Lutz D., Scott D., Vignali C., Cresci G., Feltre A., Coorey A., Vaccari M., Fritz J., Le Floch E., Magnelli B., Popesso P., Oliver S., Bock J., Carollo M., Contini T., Le Fevre O., Lilly S., Mainieri V., Renzini A., and Scodeggio M.
Subjects: ULTRALUMINOUS INFRARED GALAXIES, ACTIVE GALACTIC NUCLEI, Cosmology and Nongalactic Astrophysics (astro-ph.CO), Active galactic nucleus, Astrophysics::High Energy Astrophysical Phenomena, RAY LUMINOSITY FUNCTION, nuclei [galaxies], FOS: Physical sciences, SPECTRAL ENERGY-DISTRIBUTIONS, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, galaxies [infrared], 01 natural sciences, HIGH-REDSHIFT GALAXIES, infrared: galaxies, QB0460, 0103 physical sciences, Astrophysics::Solar and Stellar Astrophysics, 010303 astronomy & astrophysics, evolution [galaxies], Astrophysics::Galaxy Astrophysics, Luminosity function (astronomy), XMM-NEWTON, Luminous infrared galaxy, Physics, Supermassive black hole, 010308 nuclear & particles physics, Star formation, Astronomy, Astronomy and Astrophysics, HUBBLE-SPACE-TELESCOPE, STAR-FORMATION HISTORY, Astrophysics - Astrophysics of Galaxies, Galaxy, Black hole, Physics and Astronomy, Space and Planetary Science, Astrophysics of Galaxies (astro-ph.GA), X-RAY, DEEP-FIELD-SOUTH, Spectral energy distribution, Astrophysics::Earth and Planetary Astrophysics, galaxies: nuclei, galaxies: evolution, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: We study a sample of Herschel-PACS selected galaxies within the GOODS-South and the COSMOS fields in the framework of the PACS Evolutionary Probe (PEP) project. Starting from the rich multi-wavelength photometric data-sets available in both fields, we perform a broad-band Spectral Energy Distribution (SED) decomposition to disentangle the possible active galactic nucleus (AGN) contribution from that related to the host galaxy. We find that 37 per cent of the Herschel-selected sample shows signatures of nuclear activity at the 99 per cent confidence level. The probability to reveal AGN activity increases for bright ($L_{\rm 1-1000} > 10^{11} \rm L_{\odot}$) star-forming galaxies at $z>0.3$, becoming about 80 per cent for the brightest ($L_{\rm 1-1000} > 10^{12} \rm L_{\odot}$) infrared (IR) galaxies at $z \geq 1$. Finally, we reconstruct the AGN bolometric luminosity function and the super-massive black hole growth rate across cosmic time up to $z \sim 3$ from a Far-Infrared (FIR) perspective. This work shows general agreement with most of the panchromatic estimates from the literature, with the global black hole growth peaking at $z \sim 2$ and reproducing the observed local black hole mass density with consistent values of the radiative efficiency $��_{\rm rad}$ ($\sim$0.07)., 20 pages, 14 figures, 1 table, accepted for publication in MNRAS
Published: 2014

43. Non-linearity and environmental dependence of the star-forming galaxies main sequence

Author: Paola Popesso, F. Ziparo, Jeffrey A. Newman, G. Erfanianfar, N. Brandt, Andrea Biviano, S. Berta, H. Aussel, Albrecht Poglitsch, D. Wilman, M. Mirkazemi, Francesca Pozzi, Benjamin Magnelli, Mark Dickinson, Raanan Nordon, E. Le Floc'h, Kirpal Nandra, O. Ilbert, D. Fadda, D. Elbaz, Alexis Finoguenov, Andrea Cimatti, John S. Mulchaey, M. C. Cooper, R. M. Bielby, Nico Cappelluti, Masaomi Tanaka, L. Morselli, Dieter Lutz, Mara Salvato, Franz E. Bauer, M. B. Altieri, Stijn Wuyts, Max-Planck-Institut für Extraterrestrische Physik (MPE), Excellence Cluster Universe, excellence cluster centre, INAF - Osservatorio Astronomico di Trieste (OAT), Istituto Nazionale di Astrofisica (INAF), Astrophysique Interprétation Modélisation (AIM (UMR7158 / UMR_E_9005 / UM_112)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), National Optical Astronomy Observatory (NOAO), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Durham University, INAF - Osservatorio Astronomico di Bologna (OABO), 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), University of Bologna/Università di Bologna, Erfanianfar, G., Popesso, P., Finoguenov, A., Wilman, D., Wuyts, S., Biviano, A., Salvato, M., Mirkazemi, M., Morselli, L., Ziparo, F., Nandra, K., Lutz, D., Elbaz, D., Dickinson, M., Tanaka, M., Altieri, M.B., Aussel, H., Bauer, F., Berta, S., Bielby, R.M., Brandt, N., Cappelluti, N., Cimatti, A., Cooper, M.C., Fadda, D., Ilbert, O., Le Floch, E., Magnelli, B., Mulchaey, J.S., Nordon, R., Newman, J.A., Poglitsch, A., Pozzi, F., 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), 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), University of Bologna, and NOAO
Subjects: Infrared: galaxie, haloes [Galaxies], FOS: Physical sciences, Astrophysics, Galaxies: groups: general, Astrophysics::Cosmology and Extragalactic Astrophysics, star formation [Galaxies], 01 natural sciences, evolution [Galaxy], Peculiar galaxy, galaxies [Infrared], Galaxy group, 0103 physical sciences, Disc, Galaxies: haloe, 010303 astronomy & astrophysics, Lenticular galaxy, Galaxy: structure, Galaxy cluster, Astrophysics::Galaxy Astrophysics, Luminous infrared galaxy, Physics, Galaxy: evolution, Galaxies: star formation, 010308 nuclear & particles physics, Astronomy, Astronomy and Astrophysics, Quasar, Astronomy and Astrophysic, Astrophysics - Astrophysics of Galaxies, groups: general [Galaxies], 13. Climate action, Space and Planetary Science, Astrophysics of Galaxies (astro-ph.GA), Elliptical galaxy, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], structure [Galaxy]
Abstract: Using data from four deep fields (COSMOS, AEGIS, ECDFS, and CDFN), we study the correlation between the position of galaxies in the star formation rate (SFR) versus stellar mass plane and local environment at $z10^{10.4-10.6}$ $M_{\odot}$), across all environments. At high redshift ( $0.5, Comment: 14 pages, 14 figures, accepted for publication in MNRAS
Published: 2016

44. The evolution of galaxy star formation activity in massive haloes

Author: D. Lutz, H. Aussel, Andrea Biviano, E. Le Floc'h, D. Fadda, G. Rodighiero, C. K. Xu, Albrecht Poglitsch, Mara Salvato, Benjamin Magnelli, D. Elbaz, A. Finoguenov, F. Ziparo, Carlotta Gruppioni, Mark Dickinson, P. Popesso, O. Ilbert, Raanan Nordon, D. Wilman, S. Berta, Francesca Pozzi, Bruno Altieri, A. Cimatti, Popesso, P., Biviano, A., Finoguenov, A., Wilman, D., Salvato, M., Magnelli, B., Gruppioni, C., Pozzi, F., Rodighiero, G., Ziparo, F., Berta, S., Elbaz, D., Dickinson, M., Lutz, D., Altieri, B., Aussel, H., Cimatti, A., Fadda, D., Ilbert, O., Le Floch, E., Nordon, R., Poglitsch, A., Xu, C.K., Max-Planck-Institut für Extraterrestrische Physik (MPE), Excellence Cluster Universe, excellence cluster centre, Astrophysique Interprétation Modélisation (AIM (UMR7158 / UMR_E_9005 / UM_112)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Astrophysique Interprétation Modélisation (AIM (UMR_7158 / UMR_E_9005 / UM_112)), and 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)
Subjects: Cosmology and Nongalactic Astrophysics (astro-ph.CO), evolution-galaxie, media_common.quotation_subject, groups, FOS: Physical sciences, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, Galaxie, galaxies: groups: general, Active phase, general-galaxie, 0103 physical sciences, Astrophysics::Solar and Stellar Astrophysics, group, clusters, luminosity function, cluster, 010303 astronomy & astrophysics, Astrophysics::Galaxy Astrophysics, mass function-galaxie, media_common, Physics, COSMIC cancer database, evolution-galaxies, 010308 nuclear & particles physics, Star formation, mass function-galaxies, Astronomy and Astrophysics, Astronomy and Astrophysic, Galaxies, Astrophysics - Astrophysics of Galaxies, Universe, Galaxy, Redshift, general-galaxies, galaxies: luminosity function, galaxies: clusters: general, mass function, general, Space and Planetary Science, Astrophysics of Galaxies (astro-ph.GA), Halo, Astrophysics::Earth and Planetary Astrophysics, Low Mass, galaxies: evolution, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: There is now a large consensus that the current epoch of the Cosmic Star Formation History (CSFH) is dominated by low mass galaxies while the most active phase at 1~1, the most IR-luminous galaxies (LIRGs and ULIRGs) are preferentially located in groups, and this is consistent with a reversal of the star-formation rate vs .density anti-correlation observed in the nearby Universe. At these redshifts, group galaxies contribute 60-80% of the CSFH, i.e. much more than at lower redshifts. Below z~1, the comoving number and SFR densities of IR-emitting galaxies in groups decline significantly faster than those of all IR-emitting galaxies. Our results are consistent with a "halo downsizing" scenario and highlight the significant role of "environment" quenching in shaping the CSFH., Comment: 14 pages, 10 figures, accepted for publication by A&A
Published: 2015

45. The evolution of star formation activity in galaxy groups

Author: Raanan Nordon, Michael C. Cooper, F. Ziparo, Alessandro Cimatti, Michael L. Balogh, D. Wilman, Stijn Wuyts, M. Mirkazemi, Andrea Biviano, Mark Dickinson, Franz E. Bauer, Benjamin Magnelli, Herve Aussel, Alexis Finoguenov, Masayuki Tanaka, Mara Salvato, E. Le Floc'h, S. Berta, Jeffrey A. Newman, N. Brandt, M. B. Altieri, D. Fadda, Kirpal Nandra, D. Elbaz, Francesca Pozzi, P. Popesso, Dieter Lutz, R. M. Bielby, Nico Cappelluti, G. Erfanianfar, Albrecht Poglitsch, John S. Mulchaey, O. Ilbert, Laboratoire d'Astrophysique de Marseille (LAM), 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), Erfanianfar, G., Popesso, P., Finoguenov, A., Wuyts, S., Wilman, D., Biviano, A., Ziparo, F., Salvato, M., Nandra, K., Lutz, D., Elbaz, D., Dickinson, M., Tanaka, M., Mirkazemi, M., Balogh, M.L., Altieri, M.B., Aussel, H., Bauer, F., Berta, S., Bielby, R.M., Brandt, N., Cappelluti, N., Cimatti, A., Cooper, M., Fadda, D., Ilbert, O., Le Floch, E., Magnelli, B., Mulchaey, J.S., Nordon, R., Newman, J.A., Poglitsch, A., Pozzi, F., 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: Infrared: galaxie, Stellar mass, Large-scale structure of Universe, Population, FOS: Physical sciences, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Halo occupation distribution, Catalogue, Cosmology: observation, galaxies [infrared], Galaxy group, Astrophysics::Solar and Stellar Astrophysics, education, observations [Cosmology], Astrophysics::Galaxy Astrophysics, catalogues, evolution [galaxies], Physics, Luminous infrared galaxy, education.field_of_study, [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph], Star formation, Astronomy, Galaxies: evolution, Astronomy and Astrophysics, Astrophysics - Astrophysics of Galaxies, Galaxy, Space and Planetary Science, Astrophysics of Galaxies (astro-ph.GA), Spectral energy distribution, Astrophysics::Earth and Planetary Astrophysics, large-scale structure of Universe
Abstract: We study the evolution of the total star formation (SF) activity, total stellar mass and halo occupation distribution in massive halos by using one of the largest X-ray selected sample of galaxy groups with secure spectroscopic identification in the major blank field surveys (ECDFS, CDFN, COSMOS, AEGIS). We provide an accurate measurement of SFR for the bulk of the star-forming galaxies using very deep mid-infrared Spitzer MIPS and far-infrared Herschel PACS observations. For undetected IR sources, we provide a well-calibrated SFR from SED fitting. We observe a clear evolution in the level of SF activity in galaxy groups. The total SF activity in the high redshift groups (0.5, Comment: Accepted for publication in MNRAS
Published: 2014

46. A multiwavelength consensus on the main sequence of star-forming galaxies at z ~ 2

Author: H. Dominguez Sanchez, Benjamin Magnelli, P. Andreani, Ivano Baronchelli, G. Zamorani, Francesca Pozzi, Carlotta Gruppioni, P. Santini, Dieter Lutz, Giulia Rodighiero, Giovanni Cresci, Alberto Franceschini, E. Daddi, Daichi Kashino, C. Mancini, P. Popesso, E. Le Floc'h, S. Berta, Andrea Cimatti, John D. Silverman, Alvio Renzini, Rodighiero, G, Renzini, A., Daddi, E., Baronchelli, I., Berta, S., Cresci, G., Franceschini, A., Gruppioni, C., Lutz, D., Mancini, C., Santini, P., Zamorani, G., Silverman, J., Kashino, D., Andreani, P., Cimatti, A., Domínguez Sánchez, H., Le Floch, E., Magnelli, B., Popesso, P., and Pozzi, F.
Subjects: Astrofísica, Cosmology and Nongalactic Astrophysics (astro-ph.CO), Infrared: galaxie, Radio galaxy, Population, FOS: Physical sciences, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Disc galaxy, 01 natural sciences, Cosmology: observation, Luminosity, 0103 physical sciences, Astrophysics::Solar and Stellar Astrophysics, education, 010303 astronomy & astrophysics, Astrophysics::Galaxy Astrophysics, Luminous infrared galaxy, Physics, education.field_of_study, 010308 nuclear & particles physics, Star formation, Astronomy, Galaxies: evolution, Astronomy and Astrophysics, Galaxies: active, Astrophysics - Astrophysics of Galaxies, Galaxy, Astronomía, Space and Planetary Science, Astrophysics of Galaxies (astro-ph.GA), Elliptical galaxy, Astrophysics::Earth and Planetary Astrophysics, Galaxies: starburst, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: We compare various star formation rate (SFR) indicators for star-forming galaxies at $1.4, Comment: Accepted for publication in MNRAS
Published: 2014

47. The role of massive halos in the Star Formation History of the Universe

Author: David Elbaz, Alexis Finoguenov, S. Berta, D. Wilman, Paola Popesso, F. Ziparo, Andrea Cimatti, Dario Fadda, Bruno Altieri, Francesca Pozzi, Shy Genel, Giulia Rodighiero, Olivier Ilbert, Mark Dickinson, Carlotta Gruppioni, E. Le Floc'h, Herve Aussel, Albrecht Poglitsch, Benjamin Magnelli, Raanan Nordon, Chun Xu, Andrea Biviano, Dieter Lutz, Mara Salvato, Excellence Cluster Universe, Technische Universität München [München] (TUM), Max-Planck-Institut für Extraterrestrische Physik (MPE), 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), Technische Universität Munchen - Université Technique de Munich [Munich, Allemagne] (TUM), Popesso, P., Biviano, A., Finoguenov, A., Wilman, D., Salvato, M., Magnelli, B., Gruppioni, C., Pozzi, F., Rodighiero, G., Ziparo, F., Berta, S., Elbaz, D., Dickinson, M., Lutz, D., Altieri, B., Aussel, H., Cimatti, A., Fadda, D., Ilbert, O., Le Floch, E., Nordon, R., Poglitsch, A., Genel, S., Xu, C.K., Astrophysique Interprétation Modélisation (AIM (UMR7158 / UMR_E_9005 / UM_112)), and Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)
Subjects: Physics, Structure formation, Galaxies: star formation, Star formation, FOS: Physical sciences, Galaxies: evolution, Astronomy and Astrophysics, Galaxies: groups: general, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Astronomy and Astrophysic, Billion years, Astrophysics - Astrophysics of Galaxies, Redshift, Accretion (astrophysics), Galaxy, Space and Planetary Science, Astrophysics of Galaxies (astro-ph.GA), Halo, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Low Mass, Astrophysics::Galaxy Astrophysics
Abstract: The most striking feature of the Cosmic Star Formation History (CSFH) of the Universe is a dramatic drop of the star formation (SF) activity, since z~1. In this work we investigate if the very same process of assembly and growth of structures is one of the major drivers of the observed decline. We study the contribution to the CSFH of galaxies in halos of different masses. This is done by studying the total SFR-halo mass-redshift plane from redshift 0 to redshift z~1.6 in a sample of 57 groups and clusters by using the deepest available mid- and far-infrared surveys conducted with Spitzer MIPS and Herschel PACS and SPIRE. Our results show that low mass groups provide a 60-80% contribution to the CSFH at z~1. Such contribution declines faster than the CSFH in the last 8 billion years to less than 10% at z50%) of very massive, highly star forming Main Sequence galaxies. Below z~1 a quenching process must take place in massive halos to cause the observed faster suppression of their SF activity. Such process must be a slow one though, as most of the models implementing a rapid quenching of the SF activity in accreting satellites significantly underpredicts the observed SF level in massive halos at any redshift. Starvation or the transition from cold to hot accretion would provide a quenching timescale of 1 Gyrs more consistent with the observations. Our results suggest a scenario in which, due to the structure formation process, more and more galaxies experience the group environment and, thus, the associated quenching process. This leads to the progressive suppression of their SF activity shaping the CSFH below z~1., 18 pages, 21 figures, accepted for publication by A&A
Published: 2014

48. The Mean Star Formation Rate of X-ray selected Active Galaxies and its Evolution from z=2.5: Results from PEP-Herschel

Author: Albrecht Poglitsch, David Elbaz, David M. Alexander, David J. Rosario, Stijn Wuyts, Marcella Brusa, Reinhard Genzel, Adriano Fontana, J. Cepa, Bruno Altieri, V. Mainieri, Linda J. Tacconi, W. N. Brandt, Herve Aussel, L. Riguccini, Francesca Pozzi, Thomas J. Cox, N. M. Förster Schreiber, Paola Popesso, Roberto Maiolino, Raanan Nordon, Mara Salvato, Franz E. Bauer, E. Sturm, P. Santini, Benjamin Magnelli, Andrea Cimatti, Giulia Rodighiero, E. Daddi, E. Le Floc'h, Dieter Lutz, Hagai Netzer, Ángel Bongiovanni, Paola Andreani, Ivan Valtchanov, S. Berta, Lijing Shao, I. Pérez Garcia, Andrea Grazian, Miguel Sánchez-Portal, Rosario D., Santini P., Lutz D., Shao L., Maiolino R., Alexander D. M., Altieri B., Andreani P., Aussel H., Bauer F. E., Berta S., Bongiovanni A., Brandt W. N., Brusa M., Cepa J., Cimatti A., Cox T. J., Daddi E., Elbaz D., Fontana A., Förster Schreiber N. M., Genzel R., Grazian A., Le Floch E., Magnelli B., Mainieri V., Netzer H., Nordon R., Pérez Garcia I., Poglitsch A., Popesso P., Pozzi F., Riguccini L., Rodighiero G., Salvato M., Sanchez-Portal M., Sturm E., Tacconi L. J., Valtchanov I., and Wuyts S.
Subjects: Physics, Active galactic nucleus, Cosmology and Nongalactic Astrophysics (astro-ph.CO), Star formation, Astrophysics::High Energy Astrophysical Phenomena, galaxies: active, infrared: galaxie, FOS: Physical sciences, Astronomy and Astrophysics, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Accretion (astrophysics), Galaxy, Uncorrelated, Redshift, Luminosity, X-rays: galaxies, Orders of magnitude (time), Space and Planetary Science, galaxies: star formation, Astrophysics::Solar and Stellar Astrophysics, Astrophysics::Galaxy Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: (Abridged) We study relationships between the SFR and the nuclear properties of X-ray selected AGNs out to z=2.5, using far-IR data in three extragalactic deep fields as part of the PACS Evolutionary Probe (PEP) program. Guided by studies of intrinsic infra-red AGN SEDs, we show that the majority of the FIR emission in AGNs is produced by cold dust heated by star-formation. We uncover characteristic redshift-dependent trends between the mean FIR luminosity (L_fir) and accretion luminosity (L_agn) of AGNs. At low AGN luminosities, accretion and SFR are uncorrelated at all redshifts, consistent with a scenario where most low-luminosity AGNs are primarily fueled by secular processes in their host galaxies. At high AGN luminosities, a significant correlation is observed between L_fir and L_agn, but only among AGNs at low and moderate redshifts (z1). This suggests that the role of mergers in SMBH-galaxy co-evolution is less important at these epochs. At all redshifts, we find essentially no relationship between L_fir and nuclear obscuration across five orders of magnitude in obscuring column density, suggesting that various different mechanisms are likely to be responsible for obscuring X-rays in active galaxies. We explain our results within a scenario in which two different modes of SMBH fueling operate among low- and high-luminosity AGNs. We postulate, guided by emerging knowledge about the properties of high redshift galaxies, that the dominant mode of accretion among high-luminosity AGNs evolves with redshift., 18 pages, 9 figures, 3 tables
Published: 2012

49. The lesser role of starbursts in star formation at $z=2$

Author: P. Andreani, P. Santini, Georgios E. Magdis, E. Le Floc'h, G. Rodighiero, Roberto Maiolino, Alvio Renzini, M. Magliocchetti, Ivano Baronchelli, Alberto Franceschini, Adriano Fontana, Antonio Cava, L. Riguccini, Linda J. Tacconi, Francesca Pozzi, Dieter Lutz, P. Popesso, Stijn Wuyts, S. Berta, G. Zamorani, E. Daddi, Albrecht Poglitsch, A. Grazian, O. Ilbert, Carlotta Gruppioni, Anna Feltre, Raanan Nordon, N. M. Förster Schreiber, Benjamin Magnelli, H. Aussel, D. Elbaz, H. J. McCracken, Reinhard Genzel, A. Cimatti, Dipartimento di Astronomia [Padova], Università degli Studi di Padova = University of Padua (Unipd), 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), Dipartimento di Fisica e Astronomia [Bologna], Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), Max-Planck-Institut für Extraterrestrische Physik (MPE), European Southern Observatory (ESO), 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), Max Planck Institute for Extraterrestrial Physics (MPE), Max-Planck-Gesellschaft, Dipartimento di Fisica [Povo], Università degli Studi di Trento (UNITN), INAF - Osservatorio Astronomico di Roma (OAR), Istituto Nazionale di Astrofisica (INAF), Istituto di Astrofisica Spaziale e Fisica cosmica - Bologna (IASF-Bo), 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), Istituto di Astrofisica Spaziale e Fisica cosmica - Roma (IASF-Roma), 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), ANR-08-JCJC-0008,UPGAL(2008), European Project: 240039,EC:FP7:ERC,ERC-2009-StG,UPGAL(2009), Universita degli Studi di Padova, 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 de Paris (UP), Rodighiero G., Daddi E., Baronchelli I., Cimatti A., Renzini A., Aussel H., Popesso P., Lutz D., Andreani P., Berta S., Cava A., Elbaz D., Feltre A., Fontana A., Förster Schreiber N. M., Franceschini A., Genzel R., Grazian A., Gruppioni C., Ilbert O., Le Floch E., Magdis G., Magliocchetti M., Magnelli B., Maiolino R., McCracken H., Nordon R., Poglitsch A., Santini P., Pozzi F., Riguccini L., Tacconi L. J., Wuyts S., Zamorani G., Dipartimento di Astronomia, 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), Università di Bologna [Bologna] (UNIBO), Departamento de Astrofisica, Universidad Complutense de Madrid [Madrid] (UCM), INAF - Osservatorio Astronomico (OAR), 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), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), and UPGAL
Subjects: Cosmology and Nongalactic Astrophysics (astro-ph.CO), FOS: Physical sciences, galaxies: starburst, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, Morphological transformation, Critical phase, [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], 0103 physical sciences, galaxies: interactions, 010303 astronomy & astrophysics, Astrophysics::Galaxy Astrophysics, Physics, 010308 nuclear & particles physics, Star formation, [SDU.ASTR.SR]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR], Conjunction (astronomy), Astronomy and Astrophysics, [PHYS.ASTR.SR]Physics [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR], Galaxy, Redshift, Space and Planetary Science, galaxies: interaction, Astrophysics::Earth and Planetary Astrophysics, galaxies: nuclei, galaxies: evolution, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: Two main modes of star formation are know to control the growth of galaxies: a relatively steady one in disk-like galaxies, defining a tight star formation rate (SFR)-stellar mass sequence, and a starburst mode in outliers to such a sequence which is generally interpreted as driven by merging. Such starburst galaxies are rare but have much higher SFRs, and it is of interest to establish the relative importance of these two modes. PACS/Herschel observations over the whole COSMOS and GOODS-South fields, in conjunction with previous optical/near-IR data, have allowed us to accurately quantify for the first time the relative contribution of the two modes to the global SFR density in the redshift interval 1.51000M(sun)/yr, off-sequence sources significantly contribute to the SFR density (46+/-20%). We conclude that merger-driven starbursts play a relatively minor role for the formation of stars in galaxies, whereas they may represent a critical phase towards the quenching of star formation and morphological transformation in galaxies., Comment: Accepted for publication in ApJ Letters
Published: 2011

50. The X-ray to optical-UV luminosity ratio of X-ray selected Type 1 AGN in XMM-COSMOS

Author: O. Le Fèvre, Andrea Comastri, Anton M. Koekemoer, Jean-Paul Kneib, Eva Schinnerer, M. Scodeggio, Fabrizio Fiore, Francesca Civano, K. Iwasawa, M. Mignoli, John D. Silverman, Mara Salvato, Roberto Gilli, F. Lamareille, D. Vergani, G. Zamorani, Jonathan R. Trump, Nico Cappelluti, Knud Jahnke, Simon J. Lilly, V. Mainieri, Bianca Garilli, Andrea Merloni, M. T. Sargent, Elisabeta Lusso, Angela Bongiorno, Cristian Vignali, Martin Elvis, Marcella Brusa, Micol Bolzonella, E. Le Floc'h, A. Iovino, 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), Lusso E., Comastri A., Vignali C., Zamorani G., Brusa M., Gilli R., Iwasawa K., Salvato M., Civano F., Elvis M., Merloni A., Bongiorno A., Trump J.R., Koekemoer A.M., Schinnerer E., Le Floch E., Cappelluti N., Jahnke K., Sargent M., Silverman J., Mainieri V., Fiore F., Bolzonella M., Le Fevre O., Garilli B., Iovino A., Kneib J.P., Lamareille F., Lilly S., Mignoli M., Scodeggio M., and Vergani D.
Subjects: Physics, Cosmology and Nongalactic Astrophysics (astro-ph.CO), [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph], Galaxies: active, Galaxy: evolution, Methods: statistical, Quasars: general, Astronomy and Astrophysics, Space and Planetary Science, 010308 nuclear & particles physics, Astrophysics::High Energy Astrophysical Phenomena, Spectral density, FOS: Physical sciences, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Type (model theory), 01 natural sciences, Redshift, Luminosity, Black hole, galaxies: active – Galaxy: evolution – quasars: general – methods: statistical, 0103 physical sciences, Spectral slope, Bolometric correction, 010303 astronomy & astrophysics, Astrophysics::Galaxy Astrophysics, Photometric redshift, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: We present a study of the X-ray to optical properties of a sample of 545 X-ray selected Type 1 AGN, from the XMM-COSMOS survey, over a wide range of redshifts ($0.04, Comment: 14 pages, 15 figures, to appear in A&A
Published: 2009

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