Search Results - "Bielby, R. M."

Quasar Sightline and Galaxy Evolution (QSAGE) survey – I. The galaxy environment of O vi absorbers up to z = 1.4 around PKS 0232−04 by Bielby, R M, Stott, J P, Cullen, F, Tripp, T M, Burchett, J N, Fumagalli, M, Morris, S L, Tejos, N, Crain, R A, Bower, R G, Prochaska, J X

“…ABSTRACT We present the first results from a study of O vi absorption around galaxies at z < 1.44 using data from a near-infrared grism spectroscopic Hubble…”
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Non-linearity and environmental dependence of the star-forming galaxies main sequence by 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, Floch, E Le, Magnelli, B, Mulchaey, J S, Nordon, R, Newman, J A, Poglitsch, A, Pozzi, F

“…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)…”
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The Very Large Telescope Lyman-Break Galaxy Redshift Survey – IV. Gas and galaxies at z ∼ 3 in observations and simulations by Tummuangpak, P., Bielby, R. M., Shanks, T., Theuns, T., Crighton, N. H. M., Francke, H., Infante, L.

“…We use a combination of observations and simulation to study the relationship between star-forming galaxies and the intergalactic medium at z ≈ 3. The observed…”
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Submillimetre observations of X-ray active galactic nuclei in the William Herschel Deep Field by Bielby, R. M., Hill, M. D., Metcalfe, N., Shanks, T.

“…We investigate the contribution made by active galactic nuclei (AGN) to the high-redshift, luminous, submillimetre (submm) source population using deep (≤2 mJy…”
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Anomalous SZ contribution to three-year WMAP data by Bielby, R. M., Shanks, T.

“…We first show that the new Wilkinson Microwave Anisotropy Probe (WMAP) 3-yr data confirm the detection by Myers et al. of an extended SZ signal centred on 606…”
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The evolution of star formation activity in galaxy groups by 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.

“…We study the evolution of the total star formation (SF) activity, total stellar mass (ΣM *) and halo occupation distribution (HOD) in massive haloes by using…”
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The nature of sub-millimetre galaxies I: a comparison of AGN and star-forming galaxy SED fits by Shanks, T, Ansarinejad, B, Bielby, R M, Heywood, I, Metcalfe, N, Wang, L

“…ABSTRACT High-redshift sub-millimetre galaxies (SMGs) are usually assumed to be powered by star formation. However, it has been clear for some time that…”
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Quasar Sightline and Galaxy Evolution (QSAGE) – III. The mass–metallicity and fundamental metallicity relation of z ≈ 2.2 galaxies by Stephenson, H M O, Stott, J P, Cullen, F, Bielby, R M, Amos, N, Dutta, R, Fumagalli, M, Tejos, N, Burchett, J N, Crain, R A, Prochaska, J X

“…ABSTRACT We present analysis of the mass–metallicity relation (MZR) for a sample of 67 [O iii]-selected star-forming (SF) galaxies at a redshift range of z =…”
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Quasar Sightline and Galaxy Evolution (QSAGE) survey – II. Galaxy overdensities around UV luminous quasars at z = 1–2 by Stott, J P, Bielby, R M, Cullen, F, Burchett, J N, Tejos, N, Fumagalli, M, Crain, R A, Morris, S L, Amos, N, Bower, R G, Prochaska, J X

“…ABSTRACT We demonstrate that the UV brightest quasars at z = 1–2 live in overdense environments. This is based on an analysis of deep Hubble Space Telescope…”
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The nature of sub-millimetre galaxies II: an ALMA comparison of SMG dust heating mechanisms by Ansarinejad, B, Shanks, T, Bielby, R M, Metcalfe, N, Infante, L, Murphy, D N A, Rosario, D J, Stach, S M

“…ABSTRACT We compare the contribution of active galactic nuclei (AGNs) and star formation towards dust heating in sub-mm galaxies (SMGs). We have used ALMA at…”
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The MUSE Ultra Deep Field (MUDF) – I. Discovery of a group of Lyα nebulae associated with a bright z ≈ 3.23 quasar pair by Lusso, E, Fumagalli, M, Fossati, M, Mackenzie, R, Bielby, R M, Arrigoni Battaia, F, Cantalupo, S, Cooke, R, Cristiani, S, Dayal, P, D’Odorico, V, Haardt, F, Lofthouse, E, Morris, S, Peroux, C, Prichard, L, Rafelski, M, Simcoe, R, Swinbank, A M, Theuns, T

“…ABSTRACT We present first results from Multi Unit Spectroscopic Explorer (MUSE) observations at the Very Large Telescope in the MUSE Ultra Deep Field (MUDF), a…”
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The VLT LBG Redshift Survey - I. Clustering and dynamics of ≈1000 galaxies at z≈ 3 by Bielby, R. M., Shanks, T., Weilbacher, P. M., Infante, L., Crighton, N. H. M., Bornancini, C., Bouché, N., Héraudeau, P., Lambas, D. G., Lowenthal, J., Minniti, D., Padilla, N., Petitjean, P., Theuns, T.

“…We present the initial imaging and spectroscopic data acquired as part of the Very Large Telescope (VLT) VIMOS Lyman-break galaxy Survey. UBR (or UBVI) imaging…”
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Sub-millimetre source identifications and the microjansky source population at 8.4 GHz in the William Herschel Deep Field by Heywood, I., Bielby, R. M., Hill, M. D., Metcalfe, N., Rawlings, S., Shanks, T., Smirnov, O. M.

“…Sub-millimetre observations of the William Herschel Deep Field (WHDF) using the Large Apex Bolometer Camera (LABOCA) revealed possible sub-mm counterparts for…”
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The nature of sub-millimetre galaxies I: A comparison of AGN and star-forming galaxy SED fits by Shanks, T, Ansarinejad, B, Bielby, R. M, Heywood, I, Metcalfe, N, Wang, L

“…2021MNRAS.505.1509S High redshift sub-millimetre galaxies (SMGs) are usually assumed to be powered by star-formation. However, it has been clear for some time…”
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The nature of sub-millimetre galaxies II: an ALMA comparison of SMG dust heating mechanisms by Ansarinejad, B, Shanks, T, Bielby, R. M, Metcalfe, N, Infante, L, Murphy, D. N. A, Rosario, D. J, Stach, S. M

“…We compare the contribution of Active Galactic Nuclei (AGN) and star-formation towards dust heating in sub-mm galaxies (SMGs). We have used ALMA at $0."1$…”
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Quasar Sightline and Galaxy Evolution (QSAGE) survey -- II. Galaxy overdensities around UV luminous quasars at z=1-2 by Stott, J. P, Bielby, R. M, Cullen, F, Burchett, J. N, Tejos, N, Fumagalli, M, Crain, R. A, Morris, S. L, Amos, N, Bower, R. G, Prochaska, J. X

“…2020, MNRAS, 497, 3083 We demonstrate that the UV brightest quasars at z=1-2 live in overdense environments. This is based on an analysis of deep Hubble Space…”
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The VLT LBG redshift survey – V. Characterizing the z = 3.1 Lyman α emitter population by Bielby, R. M., Tummuangpak, P., Shanks, T., Francke, H., Crighton, N. H. M., Bañados, E., González-López, Jorge, Infante, L., Orsi, A.

“…We present a survey of z ∼ 3 Lyα emitters (LAEs) within the fields of the VLT Lyman break galaxies (LBG) redshift survey. The data encompass five independent…”
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Quasar Sightline and Galaxy Evolution (QSAGE) Survey - I. The Galaxy Environment of OVI Absorbers up to z=1.4 around PKS 0232-04 by Bielby, R. M, Stott, J. P, Cullen, F, Tripp, T. M, Burchett, J, Fumagalli, M, Morris, S. L, Tejos, N, Crain, R. A, Bower, R. G, Prochaska, J. X

“…We present the first results from a study of OVI absorption around galaxies at $z<1.44$ using data from a near-infrared grism spectroscopic Hubble Space…”
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The VLT LBG redshift survey – VI. Mapping H i in the proximity of z ∼ 3 LBGs with X-Shooter by Bielby, R. M., Shanks, T., Crighton, N. H. M., Bornancini, C. G., Infante, L., Lambas, D. G., Minniti, D., Morris, S. L., Tummuangpak, P.

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The VLT LBG Redshift Survey - V. Characterising the z = 3.1 Lyman Alpha Emitter Population by Bielby, R. M, Tummuangpak, P, Shanks, T, Francke, H, Crighton, N. H. M, Bañados, E, González-López, Jorge, Infante, L, Orsi, A

“…MNRAS, 2016, 456, 4061 We present a survey of $z\sim3$ Ly$\alpha$ emitters (LAEs) within the fields of the VLT LBG Redshift Survey. The data encompasses 5…”
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