Search Results - "Barrufet, L."

Reionization Era Bright Emission Line Survey: Selection and Characterization of Luminous Interstellar Medium Reservoirs in the z > 6.5 Universe by Bouwens, R. J., Smit, R., Schouws, S., Stefanon, M., Bowler, R., Endsley, R., Gonzalez, V., Inami, H., Stark, D., Oesch, P., Hodge, J., Aravena, M., da Cunha, E., Dayal, P., Looze, I. de, Ferrara, A., Fudamoto, Y., Graziani, L., Li, C., Nanayakkara, T., Pallottini, A., Schneider, R., Sommovigo, L., Topping, M., van der Werf, P., Algera, H., Barrufet, L., Hygate, A., Labbé, I., Riechers, D., Witstok, J.

“…Abstract The Reionization Era Bright Emission Line Survey (REBELS) is a cycle-7 ALMA Large Program (LP) that is identifying and performing a first…”
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The ALMA REBELS Survey: cosmic dust temperature evolution out to z ∼ 7 by Sommovigo, L, Ferrara, A, Pallottini, A, Dayal, P, Bouwens, R J, Smit, R, da Cunha, E, De Looze, I, Bowler, R A A, Hodge, J, Inami, H, Oesch, P, Endsley, R, Gonzalez, V, Schouws, S, Stark, D, Stefanon, M, Aravena, M, Graziani, L, Riechers, D, Schneider, R, van der Werf, P, Algera, H, Barrufet, L, Fudamoto, Y, Hygate, A P S, Labbé, I, Li, Y, Nanayakkara, T, Topping, M

“…ABSTRACT ALMA observations have revealed the presence of dust in the first generations of galaxies in the Universe. However, the dust temperature Td remains…”
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The ALMA REBELS Survey. Epoch of Reionization giants: Properties of dusty galaxies at z ≈ 7 by Ferrara, A, Sommovigo, L, Dayal, P, Pallottini, A, Bouwens, R J, Gonzalez, V, Inami, H, Smit, R, Bowler, R A A, Endsley, R, Oesch, P, Schouws, S, Stark, D, Stefanon, M, Aravena, M, da Cunha, E, De Looze, I, Fudamoto, Y, Graziani, L, Hodge, J, Riechers, D, Schneider, R, Algera, H S B, Barrufet, L, Hygate, A P S, Labbé, I, Li, C, Nanayakkara, T, Topping, M, van der Werf, P

“…ABSTRACT We analyse FIR dust continuum measurements for 14 galaxies (redshift z ≈ 7) in the ALMA Reionization Era Bright Emission Line Survey (REBELS) Large…”
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Unveiling the nature of infrared bright, optically dark galaxies with early JWST data by Barrufet, L, Oesch, P A, Weibel, A, Brammer, G, Bezanson, R, Bouwens, R, Fudamoto, Y, Gonzalez, V, Gottumukkala, R, Illingworth, G, Heintz, K E, Holden, B, Labbe, I, Magee, D, Naidu, R P, Nelson, E, Stefanon, M, Smit, R, van Dokkum, P, Weaver, J R, Williams, C C

“…ABSTRACT Over the last few years, both Atacama Large Millimeter/submillimeter Array (ALMA) and Spitzer observations have revealed a population of likely…”
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Normal, dust-obscured galaxies in the epoch of reionization by Fudamoto, Y., Oesch, P. A., Schouws, S., Stefanon, M., Smit, R., Bouwens, R. J., Bowler, R. A. A., Endsley, R., Gonzalez, V., Inami, H., Labbe, I., Stark, D., Aravena, M., Barrufet, L., da Cunha, E., Dayal, P., Ferrara, A., Graziani, L., Hodge, J., Hutter, A., Li, Y., De Looze, I., Nanayakkara, T., Pallottini, A., Riechers, D., Schneider, R., Ucci, G., van der Werf, P., White, C.

“…Over the past decades, rest-frame ultraviolet (UV) observations have provided large samples of UV luminous galaxies at redshift ( z ) greater than 6 (refs. 1 –…”
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The ALMA REBELS Survey: the first infrared luminosity function measurement at z  ∼ 7 by Barrufet, L, Oesch, P A, Bouwens, R, Inami, H, Sommovigo, L, Algera, H, da Cunha, E, Aravena, M, Dayal, P, Ferrara, A, Fudamoto, Y, Gonzalez, V, Graziani, L, Hygate, A P S, de Looze, I, Nanayakkara, T, Pallottini, A, Schneider, R, Stefanon, M, Topping, M, van der Werf, P

“…ABSTRACT We present the first observational infrared luminosity function (IRLF) measurement in the Epoch of Reionization (EoR) based on a ultraviolet…”
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The ALMA REBELS Survey: Average [C ii] 158 μm Sizes of Star-forming Galaxies from z ∼ 7 to z ∼ 4 by Fudamoto, Y., Smit, R., Bowler, R. A. A., Oesch, P. A., Bouwens, R., Stefanon, M., Inami, H., Endsley, R., Gonzalez, V., Schouws, S., Stark, D., Algera, H. S. B., Aravena, M., Barrufet, L., da Cunha, E., Dayal, P., Ferrara, A., Graziani, L., Hodge, J. A., Hygate, A. P. S., Inoue, A. K., Nanayakkara, T., Pallottini, A., Pizzati, E., Schneider, R., Sommovigo, L., Sugahara, Y., Topping, M., van der Werf, P., Bethermin, M., Cassata, P., Dessauges-Zavadsky, M., Ibar, E., Faisst, A. L., Fujimoto, S., Ginolfi, M., Hathi, N., Jones, G. C., Pozzi, F., Schaerer, D.

“…Abstract We present the average [C ii ] 158 μ m emission line sizes of UV-bright star-forming galaxies at z ∼ 7. Our results are derived from a stacking…”
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Linking UV spectral properties of MUSE Ly α emitters at z ≳ 3 to Lyman continuum escape by Kramarenko, I G, Kerutt, J, Verhamme, A, Oesch, P A, Barrufet, L, Matthee, J, Kusakabe, H, Goovaerts, I, Thai, T T

“…ABSTRACT The physical conditions giving rise to high escape fractions of ionizing radiation (LyC fesc) in star-forming galaxies – most likely protagonists of…”
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Unveiling the hidden Universe with JWST: the contribution of dust-obscured galaxies to the stellar mass function at z ~ 3 – 8 by Gottumukkala, R, Barrufet, L, Oesch, P A, Weibel, A, Allen, N, Alcalde Pampliega, B, Nelson, E J, Williams, C C, Brammer, G, Fudamoto, Y, González, V, Heintz, K E, Illingworth, G, Magee, D, Naidu, R P, Shuntov, M, Stefanon, M, Toft, S, Valentino, F, Xiao, M

“…ABSTRACT With the advent of JWST, we can probe the rest-frame optical emission of galaxies at $z\gt 3$ with high sensitivity and spatial resolution, making it…”
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JWST PRIMER: a new multifield determination of the evolving galaxy UV luminosity function at redshifts z ≃ 9 – 15 by Donnan, C T, McLure, R J, Dunlop, J S, McLeod, D J, Magee, D, Arellano-Córdova, K Z, Barrufet, L, Begley, R, Bowler, R A A, Carnall, A C, Cullen, F, Ellis, R S, Fontana, A, Illingworth, G D, Grogin, N A, Hamadouche, M L, Koekemoer, A M, Liu, F -Y, Mason, C, Santini, P, Stanton, T M

“…ABSTRACT We present a new determination of the evolving galaxy ultraviolet (UV) luminosity function (LF) over the redshift range $8.5< z< 15.5$ using a…”
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Unveiling the main sequence to starburst transition region with a sample of intermediate redshift luminous infrared galaxies by Hogan, L, Rigopoulou, D, García-Burillo, S, Alonso-Herrero, A, Barrufet, L, Combes, F, García-Bernete, I, Magdis, G E, Pereira-Santaella, M, Thatte, N, Weiß, A

“…ABSTRACT We present a CO(3−2) study of four systems composed of six (ultra) luminous infrared galaxies (U/LIRGs), located at 0.28 <z < 0.44, that straddle the…”
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The NOEMA observations of GN-z11: constraining the neutral interstellar medium and dust formation in the heart of cosmic reionization at z = 10.6 by Fudamoto, Y, Oesch, P A, Walter, F, Decarli, R, Carilli, C L, Ferrara, A, Barrufet, L, Bouwens, R, Dessauges-Zavadsky, M, Nelson, E J, Dannerbauer, H, Illingworth, G, Inoue, A K, Marques-Chaves, R, Pérez-Fournon, I, Riechers, D A, Schaerer, D, Smit, R, Sugahara, Y, van der Werf, P

“…ABSTRACT We present results of dust continuum and [C ii]$\, 158\, {\rm \mu m}$ emission line observations of a remarkably UV luminous (MUV = −21.6) galaxy at z…”
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The NIRVANDELS survey: the stellar and gas-phase mass-metallicity relations of star-forming galaxies at z = 3.5 by Stanton, T M, Cullen, F, McLure, R J, Shapley, A E, Arellano-Córdova, K Z, Begley, R, Amorín, R, Barrufet, L, Calabrò, A, Carnall, A C, Cirasuolo, M, Dunlop, J S, Donnan, C T, Hamadouche, M L, Liu, F Y, McLeod, D J, Pentericci, L, Pozzetti, L, Sanders, R L, Scholte, D, Topping, M W

“…ABSTRACT We present determinations of the gas-phase and stellar metallicities of a sample of 65 star-forming galaxies at $z \simeq 3.5$ using rest-frame…”
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The ALMA REBELS survey: obscured star formation in massive Lyman-break galaxies at z= 4–8 revealed by the IRX–β and M⋆ relations by Bowler, R A A, Inami, H, Sommovigo, L, Smit, R, Algera, H S B, Aravena, M, Barrufet, L, Bouwens, R, da Cunha, E, Cullen, F, Dayal, P, De Looze, I, Dunlop, J S, Fudamoto, Y, Mauerhofer, V, McLure, R J, Stefanon, M, Schneider, R, Ferrara, A, Graziani, L, Hodge, J A, Nanayakkara, T, Palla, M, Schouws, S, Stark, D P, van der Werf, P P

“…ABSTRACT We investigate the degree of dust obscured star formation in 49 massive (log10(M⋆/M⊙) > 9) Lyman-break galaxies (LBGs) at z = 6.5–8 observed as part…”
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The JWST EXCELS survey: too much, too young, too fast? Ultra-massive quiescent galaxies at 3 < z < 5 by Carnall, A C, Cullen, F, McLure, R J, McLeod, D J, Begley, R, Donnan, C T, Dunlop, J S, Shapley, A E, Rowlands, K, Almaini, O, Arellano-Córdova, K Z, Barrufet, L, Cimatti, A, Ellis, R S, Grogin, N A, Hamadouche, M L, Illingworth, G D, Koekemoer, A M, Leung, H -H, Lovell, C C, Pérez-González, P G, Santini, P, Stanton, T M, Wild, V

“…ABSTRACT We report ultra-deep, medium-resolution spectroscopic observations for four quiescent galaxies with log$_{10}(M_*/\mathrm{M_\odot })\gt 11$ at $3 \lt…”
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The ALMA REBELS Survey: discovery of a massive, highly star-forming, and morphologically complex ULIRG at z = 7.31 by Hygate, A P S, Hodge, J A, da Cunha, E, Rybak, M, Schouws, S, Inami, H, Stefanon, M, Graziani, L, Schneider, R, Dayal, P, Bouwens, R J, Smit, R, Bowler, R A A, Endsley, R, Gonzalez, V, Oesch, P A, Stark, D P, Algera, H S B, Aravena, M, Barrufet, L, Ferrara, A, Fudamoto, Y, Hilhorst, J H A, De Looze, I, Nanayakkara, T, Pallottini, A, Riechers, D A, Sommovigo, L, Topping, M W, van der Werf, P

“…ABSTRACT We present Atacama Large Millimeter/Submillimeter Array (ALMA) [C ii] and ∼158 $\rm \mu m$ continuum observations of REBELS-25, a massive,…”
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Erratum: “Identification of Single Spectral Lines in Large Spectroscopic Surveys Using UMLAUT: an Unsupervised Machine-learning Algorithm Based on Unbiased Topology” (2021, ApJS, 257, 67) by Baronchelli, I., Scarlata, C. M., Rodríguez-Muñoz, L., Bonato, M., Morselli, L., Vaccari, M., Carraro, R., Barrufet, L., Henry, A., Mehta, V., Rodighiero, G., Baruffolo, A., Bagley, M., Battisti, A., Colbert, J., Dai, Y. S., De Pascale, M., Dickinson, H., Malkan, M., Mancini, C., Rafelski, M., Teplitz, H. I.

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AKARI/IRC source catalogues and source counts for the IRAC Dark Field, ELAIS North and the AKARI Deep Field South by Davidge, H., Serjeant, S., Pearson, C., Matsuhara, H., Wada, T., Dryer, B., Barrufet, L.

“…Abstract We present the first detailed analysis of three extragalactic fields (IRAC Dark Field, ELAIS-N1, ADF-S) observed by the infrared satellite, AKARI,…”
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The Spitzer-IRAC/MIPS Extragalactic Survey (SIMES). II. Enhanced Nuclear Accretion Rate in Galaxy Groups at z ∼ 0.2 by Baronchelli, I., Rodighiero, G., Teplitz, H. I., Scarlata, C. M., Franceschini, A., Berta, S., Barrufet, L., Vaccari, M., Bonato, M., Ciesla, L., Zanella, A., Carraro, R., Mancini, C., Puglisi, A., Malkan, M., Mei, S., Marchetti, L., Colbert, J., Sedgwick, C., Serjeant, S., Pearson, C., Radovich, M., Grado, A., Limatola, L., Covone, G.

“…For a sample of star-forming galaxies in the redshift interval 0.15 < z < 0.3, we study how both the relative strength of the active galactic nucleus (AGN)…”
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A GMRT 610 MHz radio survey of the North Ecliptic Pole (NEP, ADF-N) / Euclid Deep Field North by White, Glenn J, Barrufet, L, Serjeant, S, Pearson, C P, Sedgwick, C, Pal, S, Shimwell, T W, Sirothia, S K, Chiu, P, Oi, N, Takagi, T, Shim, H, Matsuhara, H, Patra, D, Malkan, M, Kim, H K, Nakagawa, T, Malek, K, Burgarella, D, Ishigaki, T

“…ABSTRACT This paper presents a 610 MHz radio survey covering 1.94 deg$^2$ around the North Ecliptic Pole (NEP), which includes parts of the ${\it AKARI}$…”
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