Search Results - "Meneux, B."

Understanding the shape of the galaxy two-point correlation function at z ≃ 1 in the COSMOS field by de la Torre, S., Guzzo, L., Kovač, K., Porciani, C., Abbas, U., Meneux, B., Carollo, C. M., Contini, T., Kneib, J. P., Le Fèvre, O., Lilly, S. J., Mainieri, V., Renzini, A., Sanders, D., Scodeggio, M., Scoville, N., Zamorani, G., Bardelli, S., Bolzonella, M., Bongiorno, A., Caputi, K., Coppa, G., Cucciati, O., de Ravel, L., Franzetti, P., Garilli, B., Iovino, A., Kampczyk, P., Knobel, C., Koekemoer, A. M., Lamareille, F., Le Borgne, J.-F., Le Brun, V., Maier, C., Mignoli, M., Pelló, R., Peng, Y., Perez-Montero, E., Ricciardelli, E., Silverman, J., Tanaka, M., Tasca, L., Tresse, L., Vergani, D., Welikala, N., Zucca, E., Bottini, D., Cappi, A., Cassata, P., Cimatti, A., Fumana, M., Ilbert, O., Leauthaud, A., Maccagni, D., Marinoni, C., McCracken, H. J., Memeo, P., Nair, P., Oesch, P., Pozzetti, L., Presotto, V., Scaramella, R.

“…We investigate how the shape of the galaxy two-point correlation function as measured in the zCOSMOS survey depends on local environment, quantified in terms…”
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Bias in the estimation of global luminosity functions by Ilbert, O., Tresse, L., Arnouts, S., Zucca, E., Bardelli, S., Zamorani, G., Adami, C., Cappi, A., Garilli, B., Le Fèvre, O., Maccagni, D., Meneux, B., Scaramella, R., Scodeggio, M., Vettolani, G., Zanichelli, A.

“…We discuss a bias present in the calculation of the global luminosity function (LF) which occurs when analysing faint galaxy samples. This effect exists as a…”
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The Very Large Telescope Visible Multi‐Object Spectrograph Mask Preparation Software by Bottini, D., Garilli, B., Maccagni, D., Tresse, L., Le Brun, V., Le Fèvre, O., Picat, J. P., Scaramella, R., Scodeggio, M., Vettolani, G., Zanichelli, A., Adami, C., Arnaboldi, M., Arnouts, S., Bardelli, S., Bolzonella, M., Cappi, A., Charlot, S., Ciliegi, P., Contini, T., Foucaud, S., Franzetti, P., Guzzo, L., Ilbert, O., Iovino, A., McCracken, H. J., Marano, B., Marinoni, C., Mathez, G., Mazure, A., Meneux, B., Merighi, R., Paltani, S., Pollo, A., Pozzetti, L., Radovich, M., Zamorani, G., Zucca, E.

“…VIMOS (Visible Multi‐Object Spectrograph) is a multiobject imaging spectrograph installed at the VLT (Very large Telescope) at the ESO (European Southern…”
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The VIMOS Integral Field Unit: Data‐Reduction Methods and Quality Assessment by Zanichelli, A., Garilli, B., Scodeggio, M., Franzetti, P., Rizzo, D., Maccagni, D., Merighi, R., Picat, J. P., Le Fèvre, O., Foucaud, S., Bottini, D., Le Brun, V., Scaramella, R., Tresse, L., Vettolani, G., Adami, C., Arnaboldi, M., Arnouts, S., Bardelli, S., Bolzonella, M., Cappi, A., Charlot, S., Ciliegi, P., Contini, T., Gavignaud, I., Guzzo, L., Ilbert, O., Iovino, A., McCracken, H. J., Marano, B., Marinoni, C., Mathez, G., Mazure, A., Meneux, B., Paltani, S., Pellò, R., Pollo, A., Pozzetti, L., Radovich, M., Zamorani, G., Zucca, E.

“…With the new generation of spectrographs, integral field spectroscopy is becoming a widely used observational technique. The Integral Field Unit (IFU) of the…”
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The Environments of Active Galactic Nuclei within the zCOSMOS Density Field by Silverman, J. D, Kovač, K, Knobel, C, Lilly, S, Bolzonella, M, Lamareille, F, Mainieri, V, Brusa, M, Cappelluti, N, Peng, Y, Hasinger, G, Zamorani, G, Scodeggio, M, Contini, T, Carollo, C. M, Jahnke, K, Kneib, J.-P, Le Fevre, O, Bardelli, S, Bongiorno, A, Brunner, H, Caputi, K, Civano, F, Comastri, A, Coppa, G, Cucciati, O, de la Torre, S, de Ravel, L, Elvis, M, Finoguenov, A, Fiore, F, Franzetti, P, Garilli, B, Gilli, R, Griffiths, R, Iovino, A, Kampczyk, P, Koekemoer, A, Le Borgne, J.-F, Le Brun, V, Maier, C, Mignoli, M, Pello, R, Perez Montero, E, Ricciardelli, E, Tanaka, M, Tasca, L, Tresse, L, Vergani, D, Vignali, C, Zucca, E, Bottini, D, Cappi, A, Cassata, P, Marinoni, C, McCracken, H. J, Memeo, P, Meneux, B, Oesch, P, Porciani, C, Salvato, M

“…The impact of environment on active galactic nucleus (AGN) activity up to z ~ 1 is assessed by utilizing a mass-selected sample of galaxies from the 10k…”
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An overview of the lightning and atmospheric electricity observations collected in southern France during the HYdrological cycle in Mediterranean EXperiment (HyMeX), Special Observation Period 1 by Defer, E, Pinty, J.-P, Coquillat, S, Martin, J.-M, Prieur, S, Soula, S, Richard, E, Rison, W, Krehbiel, P, Thomas, R, Rodeheffer, D, Vergeiner, C, Malaterre, F, Pedeboy, S, Schulz, W, Farges, T, Gallin, L.-J, Ortéga, P, Ribaud, J.-F, Anderson, G, Betz, H.-D, Meneux, B, Kotroni, V, Lagouvardos, K, Roos, S, Ducrocq, V, Roussot, O, Labatut, L, Molinié, G

“…The PEACH project (Projet en Electricité Atmosphérique pour la Campagne HyMeX – the Atmospheric Electricity Project of the HyMeX Program) is the atmospheric…”
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The power spectrum from the angular distribution of galaxies in the CFHTLS-Wide fields at redshift ∼0.7 by Granett, B. R., Guzzo, L., Coupon, J., Arnouts, S., Hudelot, P., Ilbert, O., McCracken, H. J., Mellier, Y., Adami, C., Bel, J., Bolzonella, M., Bottini, D., Cappi, A., Cucciati, O., de la Torre, S., Franzetti, P., Fritz, A., Garilli, B., Iovino, A., Krywult, J., Le Brun, V., Le Fevre, O., Maccagni, D., Malek, K., Marulli, F., Meneux, B., Paioro, L., Polletta, M., Pollo, A., Scodeggio, M., Schlagenhaufer, H., Tasca, L., Tojeiro, R., Vergani, D., Zanichelli, A.

“…We measure the real-space galaxy power spectrum on large scales at redshifts 0.5-1.2 using optical colour selected samples from the Canada-France-Hawaii…”
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The VIMOS-VLT Deep Survey: evolution in the halo occupation number since z similar to 1 by Abbas, U, de la Torre, S, Le Fevre, O, Guzzo, L, Marinoni, C, Meneux, B, Pollo, A, Zamorani, G, Bottini, D, Garilli, B, Le Brun, V, Maccagni, D, Scaramella, R, Scodeggio, M, Tresse, L, Vettolani, G, Zanichelli, A, Adami, C, Arnouts, S, Bardelli, S, Bolzonella, M, Cappi, A, Charlot, S, Ciliegi, P, Contini, T, Foucaud, S, Franzetti, P, Gavignaud, I, Ilbert, O, Iovino, A, Lamareille, F, McCracken, HJ, Marano, B, Mazure, A, Merighi, R, Paltani, S, Pello, R, Pozzetti, L, Radovich, M, Vergani, D, Zucca, E, Bondi, M, Bongiorno, A, Brinchmann, J, Cucciati, O, de Ravel, L, Gregorini, L, Perez-Montero, E, Mellier, Y, Merluzzi, P

“…We model the evolution of the mean galaxy occupation of dark matter haloes over the range 0.1 < z < 1.3, using the data from the VIMOS-VLT Deep Survey. The…”
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The power spectrum from the angular distribution of galaxies in the CFHTLS-Wide fields at redshift similar to 0.7 by Granett, B R, Guzzo, L, Coupon, J, Arnouts, S, Hudelot, P, Ilbert, O, McCracken, HJ, Mellier, Y, Adami, C, Bel, J, Bolzonella, M, Bottini, D, Cappi, A, Cucciati, O, de la Torre, S, Franzetti, P, Fritz, A, Garilli, B, Iovino, A, Krywult, J, Le Brun, V, Le Fevre, O, Maccagni, D, Malek, K, Marulli, F, Meneux, B, Paioro, L, Polletta, M, Pollo, A, Scodeggio, M, Schlagenhaufer, H, Tasca, L, Tojeiro, R, Vergani, D, Zanichelli, A

“…We measure the real-space galaxy power spectrum on large scales at redshifts 0.5-1.2 using optical colour selected samples from the Canada-France-Hawaii…”
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The power spectrum from the angular distribution of galaxies in the CFHTLS-Wide fields at redshift \tilde0.7 by Krywult, J., Le Brun, V., Le Fevre, O., Maccagni, D., Malek, K., Marulli, F., Meneux, B., Paioro, L., Polletta, M., Pollo, A., Scodeggio, M., Schlagenhaufer, H., Tasca, L., Tojeiro, R., Vergani, D., Zanichelli, A., Granett, B.~r., Guzzo, L., Coupon, J., Arnouts, S., Hudelot, P., Ilbert, O., Mccracken, H.~j., Mellier, Y., Adami, C., Bel, Julien, Bolzonella, M., Bottini, D., Cappi, A., Cucciati, O., Torre, S. de La, Franzetti, P., Fritz, A., Garilli, B., Iovino, A.

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The power spectrum from the angular distribution of galaxies in the CFHTLS-Wide fields at redshift ∼0.7: The galaxy power spectrum at z ∼ 0.7 by Granett, B. R., Guzzo, L., Coupon, J., Arnouts, S., Hudelot, P., Ilbert, O., McCracken, H. J., Mellier, Y., Adami, C., Bel, J., Bolzonella, M., Bottini, D., Cappi, A., Cucciati, O., de la Torre, S., Franzetti, P., Fritz, A., Garilli, B., Iovino, A., Krywult, J., Le Brun, V., Le Fevre, O., Maccagni, D., Malek, K., Marulli, F., Meneux, B., Paioro, L., Polletta, M., Pollo, A., Scodeggio, M., Schlagenhaufer, H., Tasca, L., Tojeiro, R., Vergani, D., Zanichelli, A.

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The nonlinear biasing of the 10k zCOSMOS galaxies up to z~1 by Kovac, K., Porciani, C., Lilly, S. J., Marinoni, Christian, Guzzo, L., Cucciati, O., Zamorani, G., Iovino, A., Oesch, P., Bolzonella, M., Peng, Y., Meneux, B., Zucca, E., Bardelli, S., Carollo, C. M., Contini, T., Kneib, J. -P., Fevre, O. Le, Mainieri, V., Renzini, A., Scodeggio, M., Bongiorno, A., Caputi, K., Coppa, G., de La Torre, S., de Ravel, L., Finoguenov, A., Franzetti, P., Garilli, B., Kampczyk, P., Knobel, C., Lamareille, F., Borgne, J. -F. Le, Brun, V. Le, Maier, C., Mignoli, M., Pello, R., Montero, E. Perez, Pozzetti, L., Ricciardelli, E., Silverman, J. D., Tanaka, M., Tasca, L. A. M., Tresse, L., Vergani, D., Abbas, U., Bottini, D., Cappi, A., Cassata, P., Cimatti, Alessandro, Fumana, M., Koekemoer, A. M., Leauthaud, A., Maccagni, D., Mccracken, H. J., Memeo, P., Scaramella, R., Scoville, N. Z.

“…We use the overdensity field reconstructed in the volume of the COSMOS area to study the nonlinear biasing of the zCOSMOS galaxies. The galaxy overdensity…”
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The zCOSMOS-Bright survey: the clustering of early and late galaxy morphological types since z approximately equal to 1 by de la Torre, S, Le FA"vre, O, Porciani, C, Guzzo, L, Meneux, B, Abbas, U, Tasca, L, Carollo, C M, Contini, T, Kneib, JaP, Lilly, S J, Mainieri, V, Renzini, A, Scodeggio, M, Zamorani, G, Bardelli, S, Bolzonella, M, Bongiorno, A, Caputi, K, Coppa, G, Cucciati, O, de Ravel, L, Franzetti, P, Garilli, B, Halliday, C, Iovino, A, Kampczyk, P, Knobel, C, Koekemoer, A M, KovaA, K, Lamareille, F, Le Borgne, JaF, Le Brun, V, Maier, C, Mignoli, M, Pello, R, Peng, Y, PerezaMontero, E, Ricciardelli, E, Silverman, J, Tanaka, M, Tresse, L, Vergani, D, Zucca, E, Bottini, D, Cappi, A, Cassata, P, Cimatti, A, Leauthaud, A, Maccagni, D, Marinoni, C, McCracken, HJ, Memeo, P, Oesch, P, Pozzetti, L, Scaramella, R

“…We measure the spatial clustering of galaxies as a function of their morphological type at z[sime] 0.8, for the first time in a deep redshift survey with full…”
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The zCOSMOS-Bright survey: the clustering of early and late galaxy morphological types since z≃ 1: The zCOSMOS-Bright survey by de la Torre, S., Le Fèvre, O., Porciani, C., Guzzo, L., Meneux, B., Abbas, U., Tasca, L., Carollo, C. M., Contini, T., Kneib, J.-P., Lilly, S. J., Mainieri, V., Renzini, A., Scodeggio, M., Zamorani, G., Bardelli, S., Bolzonella, M., Bongiorno, A., Caputi, K., Coppa, G., Cucciati, O., de Ravel, L., Franzetti, P., Garilli, B., Halliday, C., Iovino, A., Kampczyk, P., Knobel, C., Koekemoer, A. M., 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., Tanaka, M., Tresse, L., Vergani, D., Zucca, E., Bottini, D., Cappi, A., Cassata, P., Cimatti, A., Leauthaud, A., Maccagni, D., Marinoni, C., McCracken, H. J., Memeo, P., Oesch, P., Pozzetti, L., Scaramella, R.

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Understanding the shape of the galaxy two-point correlation function at z ≃ 1 in the COSMOS field: Two-point correlations in the COSMOS field by De La Torre, S., Guzzo, L., Kovač, K., Porciani, C., Abbas, U., Meneux, B., Carollo, C. M., Contini, T., Kneib, J. P., Le Fèvre, O., Lilly, S. J., Mainieri, V., Renzini, A., Sanders, D., Scodeggio, M., Scoville, N., Zamorani, G., Bardelli, S., Bolzonella, M., Bongiorno, A., Caputi, K., Coppa, G., Cucciati, O., De Ravel, L., Franzetti, P., Garilli, B., Iovino, A., Kampczyk, P., Knobel, C., Koekemoer, A. M., Lamareille, F., Le Borgne, J.-F., Le Brun, V., Maier, C., Mignoli, M., Pelló, R., Peng, Y., Perez-Montero, E., Ricciardelli, E., Silverman, J., Tanaka, M., Tasca, L., Tresse, L., Vergani, D., Welikala, N., Zucca, E., Bottini, D., Cappi, A., Cassata, P., Cimatti, A., Fumana, M., Ilbert, O., Leauthaud, A., Maccagni, D., Marinoni, C., McCracken, H. J., Memeo, P., Nair, P., Oesch, P., Pozzetti, L., Presotto, V., Scaramella, R.

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Understanding the shape of the galaxy two-point correlation function at z ≃ 1 in the COSMOS field by de la Torre, S., Guzzo, L., Kovač, K., Porciani, C., Abbas, U., Meneux, B., Carollo, C. M., Contini, T., Kneib, J. P., Le Fèvre, O., Lilly, S. J., Mainieri, V., Renzini, A., Sanders, D., Scodeggio, M., Scoville, N., Zamorani, G., Bardelli, S., Bolzonella, M., Bongiorno, A., Caputi, K., Coppa, G., Cucciati, O., de Ravel, L., Franzetti, P., Garilli, B., Iovino, A., Kampczyk, P., Knobel, C., Koekemoer, A. M., Lamareille, F., Le Borgne, J.-F., Le Brun, V., Maier, C., Mignoli, M., Pelló, R., Peng, Y., Perez-Montero, E., Ricciardelli, E., Silverman, J., Tanaka, M., Tasca, L., Tresse, L., Vergani, D., Welikala, N., Zucca, E., Bottini, D., Cappi, A., Cassata, P., Cimatti, A., Fumana, M., Ilbert, O., Leauthaud, A., Maccagni, D., Marinoni, C., McCracken, H. J., Memeo, P., Nair, P., Oesch, P., Pozzetti, L., Presotto, V., Scaramella, R.

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The VIMOS-VLT Deep Survey: evolution in the halo occupation number since z∼ 1: VVDS: evolution in the HON over z = 0-1.3 by Abbas, U., De La Torre, S., Le Fèvre, O., Guzzo, L., Marinoni, C., Meneux, B., Pollo, A., Zamorani, G., Bottini, D., Garilli, B., Le Brun, V., Maccagni, D., Scaramella, R., Scodeggio, M., Tresse, L., Vettolani, G., Zanichelli, A., Adami, C., Arnouts, S., Bardelli, S., Bolzonella, M., Cappi, A., Charlot, S., Ciliegi, P., Contini, T., Foucaud, S., Franzetti, P., Gavignaud, I., Ilbert, O., Iovino, A., Lamareille, F., McCracken, H. J., Marano, B., Mazure, A., Merighi, R., Paltani, S., Pellò, R., Pozzetti, L., Radovich, M., Vergani, D., Zucca, E., Bondi, M., Bongiorno, A., Brinchmann, J., Cucciati, O., De Ravel, L., Gregorini, L., Perez-Montero, E., Mellier, Y., Merluzzi, P.

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High-Precision Lightning Detection in Thailand by Saduankkarn, K., Moehrlein, M., Meneux, B., Betz, Hans D.

“…In recent years a modern lightning detection network has been installed all over Thailand. It is a LINET system that exploits the VLF/LF frequency regime and…”
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THE OPTICAL SPECTRA OF SPITZER 24 Delta mm GALAXIES IN THE COSMIC EVOLUTION SURVEY FIELD. II. FAINT INFRARED SOURCES IN THE zCOSMOS-BRIGHT 10k CATALOG by Caputi, K I, Lilly, S J, Aussel, H, Le Floc'h, E, Sanders, D, Maier, C, Frayer, D, Carollo, C M, Contini, T, Kneib, J-P, Le Fevre, O, Mainieri, V, Renzini, A, Scodeggio, M, Scoville, N, Zamorani, G, Bardelli, S, Bolzonella, M, Bongiorno, A, Coppa, G, Cucciati, O, de la Torre, S, de Ravel, L, Franzetti, P, Garilli, B, Ilbert, O, Iovino, A, Kampczyk, P, Kartaltepe, J, Knobel, C, Kovac, K, Lamareille, F, Le Borgne, J-F, Le Brun, V, Mignoli, M, Peng, Y, Perez-Montero, E, Ricciardelli, E, Salvato, M, Silverman, J, Surace, J, Tanaka, M, Tasca, L, Tresse, L, Vergani, D, Zucca, E, Abbas, U, Bottini, D, Capak, P, Cappi, A, Cassata, P, Cimatti, A, Elvis, M, Hasinger, G, Koekemoer, A M, Leauthaud, A, MacCagni, D, Marinoni, C, McCracken, H, Memeo, P, Meneux, B, Oesch, P, Pello, R, Porciani, C, Pozzetti, L, Scaramella, R, Scarlata, C, Schiminovich, D, Taniguchi, Y, Zamojski, M

“…We have used the zCOSMOS-bright 10k sample to identify 3244 Spitzer/MIPS 24 Delta *mm-selected galaxies with 0.06 mJy < S 24 Delta *mm 0.50 mJy and I AB <…”
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The Dependence of Star Formation Activity on Stellar Mass Surface Density and Sersic Index in zCOSMOS Galaxies at 0.5 by Maier, C., Lilly, S. J., Zamorani, G., Scodeggio, M., Lamareille, F., Contini, T., Sargent, M. T., Scarlata, C., Oesch, P., Carollo, C. M., Fevre, O. Le, Renzini, A., Kneib, J. -P., Mainieri, V., 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., Kovac, K., Borgne, J. -F. Le, Brun, V. Le, Mignoli, M., Pello, R., Peng, Y., Montero, E. Perez, Ricciardelli, E., Silverman, J. D., Tanaka, M., Tasca, L., Tresse, L., Vergani, D., Zucca, E., Abbas, U., Bottini, D., Cappi, A., Cassata, P., Cimatti, Alessandro, Fumana, M., Guzzo, L., Halliday, C., Leauthaud, A., Maccagni, D., Marinoni, Christian, Mccracken, H. J., Memeo, P., Meneux, B., Porciani, C., Pozzetti, L., Scaramella, R., Walcher, J.

“…In order to try to understand the internal evolution of galaxies and relate this to the global evolution of the galaxy population, we present a comparative…”
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