Search Results - "Overzier, R."

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    NO OVERDENSITY OF LYMAN-ALPHA EMITTING GALAXIES AROUND A QUASAR AT z ∼ 5.7 by Mazzucchelli, C., Bañados, E., Decarli, R., Farina, E. P., Venemans, B. P., Walter, F., Overzier, R.

    Published in The Astrophysical journal (01-01-2017)
    “…ABSTRACT Bright quasars, observed when the universe was less than one billion years old (z > 5.5), are known to host massive black holes (∼109 M ) and are…”
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    RESOLVING THE OPTICAL EMISSION LINES OF Lyα BLOB “B1” AT z = 2.38: ANOTHER HIDDEN QUASAR by OVERZIER, R A, Nesvadba, N P H, Dijkstra, M, Hatch, N A, Lehnert, M D, Villar-Martin, M, Wilman, R J, ZIRM, A W

    Published in The Astrophysical journal (10-07-2013)
    “…We have used the SINFONI near-infrared integral field unit on the Very Large Telescope to resolve the optical emission line structure of one of the brightest…”
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    The nature of faint radio galaxies at high redshifts by Saxena, A, Röttgering, H J A, Duncan, K J, Hill, G J, Best, P N, Indahl, B L, Marinello, M, Overzier, R A, Pentericci, L, Prandoni, I, Dannerbauer, H, Barrena, R

    “…ABSTRACT We present spectra and near-infrared images of a sample of faint radio sources initially selected as promising high-redshift radio galaxy (HzRG)…”
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    The MUSE 3D view of feedback in a high-metallicity radio galaxy at z = 2.9 by Silva, M, Humphrey, A, Lagos, P, Villar-Martín, M, Morais, S G, di Serego Alighieri, S, Cimatti, A, Fosbury, R, Overzier, R A, Vernet, J, Binette, L

    “…Abstract We present a detailed study of the kinematic, chemical and excitation properties of the giant Ly α emitting nebula and the giant H i absorber…”
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    VLT/SINFONI study of black hole growth in high-redshift radio-loud quasars from the CARLA survey by Marinello, M, Overzier, R A, Röttgering, H J A, Kurk, J D, De Breuck, C, Vernet, J, Wylezalek, D, Stern, D, Duncan, K J, Hatch, N, Kashikawa, N, Lin, Y-T, Nemmen, R S, Saxena, A

    “…ABSTRACT We present Very Large Telescope/Spectrograph for INtegral Field Observations in the Near Infrared (VLT/SINFONI) observations of 35 quasars at 2.1 < z…”
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    Chemodynamical properties and ages of metal-poor stars in S-PLUS by Almeida-Fernandes, F, Placco, V M, Rocha-Pinto, H J, Fernandes, M B, Limberg, G, Silva, L Beraldo e, Amarante, J A S, Perottoni, H D, Overzier, R, Schoenell, W, Ribeiro, T, Kanaan, A, Mendes de Oliveira, C

    “…ABSTRACT Metal-poor stars are key to our understanding of the early stages of chemical evolution in the Universe. New multifilter surveys, such as the Southern…”
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    Morphologies of Local Lyman Break Galaxy Analogs. II. A Comparison with Galaxies at z 2–4 in ACS and WFC3 Images of the Hubble Ultra Deep Field by Overzier, R. A, Heckman, T. M, Schiminovich, D, Basu-Zych, A, Gonçalves, T, Martin, D. C, Rich, R. M

    Published in Analytica chimica acta (20-02-2010)
    “…Previous work has shown that Lyman break galaxies (LBGs) display a range in structures (from single and compact to more clumpy and extended) that is different…”
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    The Quasar Catalogue for S-PLUS DR4 (QuCatS) and the estimation of photometric redshifts by Nakazono, L, R Valença, R, Soares, G, Izbicki, R, Ivezić, Ž, R Lima, E V, T Hirata, N S, Sodré Jr, L, Overzier, R, Almeida-Fernandes, F, Oliveira Schwarz, G B, Schoenell, W, Kanaan, A, Ribeiro, T, Mendes de Oliveira, C

    “…ABSTRACT The advent of massive broad-band photometric surveys enabled photometric redshift estimates for unprecedented numbers of galaxies and quasars. These…”
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    Deep Learning assessment of galaxy morphology in S-PLUS Data Release 1 by Bom, C R, Cortesi, A, Lucatelli, G, Dias, L O, Schubert, P, Oliveira Schwarz, G B, Cardoso, N M, Lima, E V R, Mendes de Oliveira, C, Sodre, L, Smith Castelli, A V, Ferrari, F, Damke, G, Overzier, R, Kanaan, A, Ribeiro, T, Schoenell, W

    “…ABSTRACT The morphological diversity of galaxies is a relevant probe of galaxy evolution and cosmological structure formation, but the classification of…”
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    PROBING THE ACTIVE MASSIVE BLACK HOLE CANDIDATE IN THE CENTER OF NGC 404 WITH VLBI by Paragi, Z., Frey, S., Kaaret, P., Cseh, D., Overzier, R., Kharb, P.

    Published in The Astrophysical journal (10-08-2014)
    “…Recently, Nyland et al. argued that the radio emission observed in the center of the dwarf galaxy NGC 404 originates in a low-luminosity active galactic…”
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    A SINFONI view of flies in the Spiderweb: a galaxy cluster in the making by Kuiper, E., Hatch, N. A., Miley, G. K., Nesvadba, N. P. H., Röttgering, H. J. A., Kurk, J. D., Lehnert, M. D., Overzier, R. A., Pentericci, L., Schaye, J., Venemans, B. P.

    “…The environment of the high-z radio galaxy PKS 1138−262 at z∼ 2.2 is a prime example of a forming galaxy cluster. We use deep Spectrograph for INtegral Field…”
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    The growth and assembly of a massive galaxy at z∼ 2 by Hatch, N. A., Overzier, R. A., Kurk, J. D., Miley, G. K., Röttgering, H. J. A., Zirm, A. W.

    “…We study the stellar mass assembly of the Spiderweb galaxy (MRC 1138−262), a massive z= 2.2 radio galaxy in a protocluster and the probable progenitor of a…”
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    The Millennium Run Observatory: first light by Overzier, R., Lemson, G., Angulo, R. E., Bertin, E., Blaizot, J., Henriques, B. M. B., Marleau, G.-D., White, S. D. M.

    “…Simulations of galaxy evolution aim to capture our current understanding as well as to make predictions for testing by future experiments. Simulations and…”
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    Galaxy protocluster candidates around z∼ 2.4 radio galaxies by Hatch, N. A., De Breuck, C., Galametz, A., Miley, G. K., Overzier, R. A., Röttgering, H. J. A., Doherty, M., Kodama, T., Kurk, J. D., Seymour, N., Venemans, B. P., Vernet, J., Zirm, A. W.

    “…We study the environments of six radio galaxies at 2.2 < z < 2.6 using wide-field near-infrared images. We use colour cuts to identify galaxies in this…”
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    A search for active galactic nuclei in the most extreme UV-selected starbursts using the European VLBI Network by Alexandroff, R., Overzier, R. A., Paragi, Zsolt, Basu-Zych, Antara, Heckman, Tim, Kauffmann, Guinevere, Bourke, Stephen, Lobanov, Andrei, Ptak, Andy, Schiminovich, David

    “…We have used the European very long baseline interferometry (VLBI) Network (EVN) to observe a sample of Lyman break analogues (LBAs), nearby (z < 0.3) galaxies…”
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    Diffuse UV light associated with the Spiderweb Galaxy: evidence for in situ star formation outside galaxies by Hatch, N. A., Overzier, R. A., Röttgering, H. J. A., Kurk, J. D., Miley, G. K.

    “…We present detailed images of diffuse ultraviolet (UV) intergalactic light (IGL), situated in a 60-kpc halo that surrounds the radio galaxy MRC 1138−262 at z=…”
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