Search Results - "Le Borgne, D"

Galaxy evolution in the metric of the cosmic web by Kraljic, K., Arnouts, S., Pichon, C., Laigle, C., de la Torre, S., Vibert, D., Cadiou, C., Dubois, Y., Treyer, M., Schimd, C., Codis, S., de Lapparent, V., Devriendt, J., Hwang, H. S., Le Borgne, D., Malavasi, N., Milliard, B., Musso, M., Pogosyan, D., Alpaslan, M., Bland-Hawthorn, J., Wright, A. H.

“…Abstract The role of the cosmic web in shaping galaxy properties is investigated in the Galaxy And Mass Assembly (GAMA) spectroscopic survey in the redshift…”
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Dancing in the dark: galactic properties trace spin swings along the cosmic web by Dubois, Y., Pichon, C., Welker, C., Le Borgne, D., Devriendt, J., Laigle, C., Codis, S., Pogosyan, D., Arnouts, S., Benabed, K., Bertin, E., Blaizot, J., Bouchet, F., Cardoso, J.-F., Colombi, S., de Lapparent, V., Desjacques, V., Gavazzi, R., Kassin, S., Kimm, T., McCracken, H., Milliard, B., Peirani, S., Prunet, S., Rouberol, S., Silk, J., Slyz, A., Sousbie, T., Teyssier, R., Tresse, L., Treyer, M., Vibert, D., Volonteri, M.

“…A large-scale hydrodynamical cosmological simulation, Horizon-AGN, is used to investigate the alignment between the spin of galaxies and the cosmic filaments…”
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COSMOS2015 photometric redshifts probe the impact of filaments on galaxy properties by Laigle, C, Pichon, C, Arnouts, S, McCracken, H J, Dubois, Y, Devriendt, J, Slyz, A, Le Borgne, D, Benoit-Lévy, A, Hwang, Ho Seong, Ilbert, O, Kraljic, K, Malavasi, N, Park, Changbom, Vibert, D

“…Abstract The variation of galaxy stellar masses and colour types with the distance to projected cosmic filaments are quantified using the precise photometric…”
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Swirling around filaments: are large-scale structure vortices spinning up dark haloes? by Laigle, C, Pichon, C, Codis, S, Dubois, Y, Le Borgne, D, Pogosyan, D, Devriendt, J, Peirani, S, Prunet, S, Rouberol, S, Slyz, A, Sousbie, T

“…The kinematic analysis of dark matter and hydrodynamical simulations suggests that the vorticity in large-scale structure is mostly confined to, and…”
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Horizon-AGN virtual observatory – 1. SED-fitting performance and forecasts for future imaging surveys by Laigle, C, Davidzon, I, Ilbert, O, Devriendt, J, Kashino, D, Pichon, C, Capak, P, Arnouts, S, de la Torre, S, Dubois, Y, Gozaliasl, G, Le Borgne, D, Lilly, S, McCracken, H J, Salvato, M, Slyz, A

“…Abstract Using the light-cone from the cosmological hydrodynamical simulation horizon-AGN, we produced a photometric catalogue over 0 < z < 4 with apparent…”
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Rates and Properties of Type Ia Supernovae as a Function of Mass and Star Formation in Their Host Galaxies by Sullivan, M, Le Borgne, D, Pritchet, C. J, Hodsman, A, Neill, J. D, Howell, D. A, Carlberg, R. G, Astier, P, Aubourg, E, Balam, D, Basa, S, Conley, A, Fabbro, S, Fouchez, D, Guy, J, Hook, I, Pain, R, Palanque-Delabrouille, N, Perrett, K, Regnault, N, Rich, J, Taillet, R, Baumont, S, Bronder, J, Ellis, R. S, Filiol, M, Lusset, V, Perlmutter, S, Ripoche, P, Tao, C

“…We show that Type Ia supemovae (SNe Ia) are formed within both very young and old stellar populations, with observed rates that depend on the stellar mass and…”
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The dusty, albeit ultraviolet bright, infancy of galaxies by Devriendt, J., Rimes, C., Pichon, C., Teyssier, R., Le Borgne, D., Aubert, D., Audit, E., Colombi, S., Courty, S., Dubois, Y., Prunet, S., Rasera, Y., Slyz, A., Tweed, D.

“…The largest galaxies acquire their mass early on, when the Universe is still youthful. Cold streams violently feed these young galaxies a vast amount of fresh…”
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GOODS- HERSCHEL : STAR FORMATION, DUST ATTENUATION, AND THE FIR–RADIO CORRELATION ON THE MAIN SEQUENCE OF STAR-FORMING GALAXIES UP TO z ≃ 4 by Pannella, M, Elbaz, D, Daddi, E, Dickinson, M, Hwang, H S, Schreiber, C, Strazzullo, V, Aussel, H, Bethermin, M, Buat, V

“…We use deep panchromatic data sets in the GOODS-N field, from GALEX to the deepest Herschel far-infrared (FIR) and VLA radio continuum imaging, to explore the…”
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Galaxy merger histories and the role of merging in driving star formation at z > 1 by Kaviraj, S., Devriendt, J., Dubois, Y., Slyz, A., Welker, C., Pichon, C., Peirani, S., Le Borgne, D.

“…We use Horizon-AGN, a hydrodynamical cosmological simulation, to explore the role of mergers in the evolution of massive (M * > 1010 M⊙) galaxies around the…”
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The Galaxy Population Hosting Gamma-Ray Bursts by Savaglio, S, Glazebrook, K, Le Borgne, D

“…We present the most extensive and complete study of the properties for the largest sample (46 objects) of gamma-ray burst (GRB) host galaxies. The redshift…”
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Clustering of Supernova Ia Host Galaxies by Carlberg, R. G, Sullivan, M, Le Borgne, D, Conley, A, Howell, D. A, Perrett, K, Astier, P, Balam, D, Balland, C, Basa, S, Hardin, D, Fouchez, D, Guy, J, Hook, I, Pain, R, Pritchet, C. J, Regnault, N, Rich, J, Perlmutter, S

“…For the first time the cross-correlation between Type Ia supernova host galaxies and surrounding field galaxies is measured using the Supernova Legacy Survey…”
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The Gemini Deep Deep Survey. VII. The Redshift Evolution of the Mass-Metallicity Relation by Savaglio, S, Glazebrook, K, Le Borgne, D, Juneau, S, Abraham, R. G, Chen, H.-W, Crampton, D, McCarthy, P. J, Carlberg, R. G, Marzke, R. O, Roth, K, Jørgensen, I, Murowinski, R

“…We have investigated the mass-metallicity (M-Z) relation using galaxies at 0.4 < z < 1.0 from the Gemini Deep Deep Survey (GDDS) and Canada-France Redshift…”
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Spectroscopic ages and metallicities of stellar populations: validation of full spectrum fitting by Koleva, M., Prugniel, Ph, Ocvirk, P., Le Borgne, D., Soubiran, C.

“…Fitting whole spectra at intermediate spectral resolution (R= 1000–3000), to derive physical properties of stellar populations, appears as an optimized…”
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Dwarf Galaxy Clustering and Missing Satellites by Carlberg, R. G, Sullivan, M, Le Borgne, D

“…At redshifts around 0.1 the Canada-France-Hawaii Telescope Legacy Survey Deep fields contain some 6 X 104 galaxies spanning the mass range from 105 to 1012 M …”
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On the filamentary environment of galaxies by Gay, C., Pichon, C., Le Borgne, D., Teyssier, R., Sousbie, T., Devriendt, J.

“…The correlation between the large-scale distribution of galaxies and their spectroscopic properties at z= 1.5 is investigated using the Horizon MareNostrum…”
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The COSMOS-Web ring: in-depth characterization of an Einstein ring lensing system at z~2 by Mercier, W, Shuntov, M, Gavazzi, R, Nightingale, J. W, Arango, R, Ilbert, O, Amvrosiadis, A, Ciesla, L, Casey, C, Jin, S, Faisst, A. L, Andika, I. T, Drakos, N. E, Enia, A, Franco, M, Gillman, S, Gozaliasl, G, Hayward, C. C, Huertas-Company, M, Kartaltepe, J. S, Koekemoer, A. M, Laigle, C, Borgne, D. Le, Magdis, G, Mahler, G, Maraston, C, Martin, C. L, Massey, R, McCracken, H. J, Moutard, T, Paquereau, L, Rhodes, J. D, Robertson, B. E, Sanders, D. B, Trebitsch, M, Tresse, L, Vijayan, A. P

“…A&A 687, A61 (2024) Aims. We provide an in-depth analysis of the COSMOS-Web ring, an Einstein ring at z=2 that we serendipitously discovered in the COSMOS-Web…”
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Horizon-AGN virtual observatory - 1. SED-fitting performance and forecasts for future imaging surveys by Laigle, C, Davidzon, I, Ilbert, O, Devriendt, J, Kashino, D, Pichon, C, Capak, P, Arnouts, S, de la Torre, S, Dubois, Y, Gozaliasl, G, Borgne, D. Le, Lilly, S, McCracken, H. J, Salvato, M, Slyz, A

“…Using the ligthcone from the cosmological hydrodynamical simulation Horizon-AGN, we produced a photometric catalogue over $0<z<4$ with apparent magnitudes in…”
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A history of galaxy migrations over the Stellar Mass - SFR plane from the COSMOS-Web survey by Arango-Toro, R. C, Ilbert, O, Ciesla, L, Shuntov, M, Aufort, G, Mercier, W, Laigle, C, Franco, M, Bethermin, M, Borgne, D. Le, Dubois, Y, McCracken, H. J, Paquereau, L, Huertas-Company, M, Kartaltepe, J, Casey, C. M, Akins, H, Allen, N, Andika, I, Brinch, M, Drakos, N. E, Faisst, A, Gozaliasl, G, Harish, S, Kaminsky, A, Koekemoer, A, Kokorev, V, Liu, D, Magdis, G, Martin, C. L, Moutard, T, Rhodes, J, Rich, R. M, Robertson, B, Sanders, D. B, Sheth, K, Talia, M, Toft, S, Tresse, L, Valentino, F, Vijayan, A, Weaver, J

“…The stellar mass-star formation rate (M$_\star$ - SFR) plane is essential for distinguishing galaxy populations, but how galaxies move within this plane over…”
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Evolution of dust temperature of galaxies through cosmic time as seen by Herschel by Hwang, H. S., Elbaz, D., Magdis, G., Daddi, E., Symeonidis, M., Altieri, B., Amblard, A., Andreani, P., Arumugam, V., Auld, R., Babbedge, T., Berta, S., Blain, A., Bock, J., Bongiovanni, A., Boselli, A., Buat, V., Castro-Rodríguez, N., Cava, A., Cepa, J., Chanial, P., Chapin, E., Chary, R.-R., Cimatti, A., Clements, D. L., Conley, A., Conversi, L., Cooray, A., Dannerbauer, H., Dickinson, M., Dowell, C. D., Dunlop, J. S., Dwek, E., Eales, S., Farrah, D., Schreiber, N. Förster, Fox, M., Gear, W., Genzel, R., Gruppioni, C., Halpern, M., Hatziminaoglou, E., Isaak, K., Ivison, R. J., Jeong, W.-S., Lagache, G., Le Borgne, D., Le Floc’h, E., Lee, H. M., Lee, J. C., Lee, M. G., Levenson, L., Lu, N., Lutz, D., Madden, S., Maffei, B., Magnelli, B., Mainetti, G., Maiolino, R., Marchetti, L., Mortier, A. M. J., Nguyen, H. T., Nordon, R., O’Halloran, B., Okumura, K., Oliver, S. J., Omont, A., Page, M. J., Panuzzo, P., Papageorgiou, A., Pérez-Fournon, I., García, A. M. Pérez, Poglitsch, A., Popesso, P., Pozzi, F., Rigopoulou, D., Riguccini, L., Rizzo, D., Rodighiero, G., Roseboom, I. G., Saintonge, A., Portal, M. Sánchez, Schulz, B., Scott, D., Seymour, N., Shao, L., Shupe, D. L., Smith, A. J., Stevens, J. A., Sturm, E., Tacconi, L., Trichas, M., Tugwell, K. E., Vaccari, M., Valtchanov, I., Vieira, J. D., Vigroux, L., Wang, L., Wright, G., Zemcov, M.

“…We study the dust properties of galaxies in the redshift range 0.1 ≲z≲ 2.8 observed by the Herschel Space Observatory in the field of the Great Observatories…”
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Galaxy merger histories and the role of merging in driving star formation at z>1 by Kaviraj, S, Devriendt, J, Dubois, Y, Slyz, A, Welker, C, Pichon, C, Peirani, S, Borgne, D. Le

“…We use Horizon-AGN, a hydrodynamical cosmological simulation, to explore the role of mergers in the evolution of massive (M > 10^10 MSun) galaxies around the…”
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