Galaxy formation and evolution

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Lyman-alpha spectroscopy of extreme [O iii] emitting galaxies at z ≃ 2-3: implications for Lyα visibility and LyC leakage at z > 6

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 503:3 (2021) 4105-4117

Authors:

Mengtao Tang, Daniel P Stark, Jacopo Chevallard, Stéphane Charlot, Ryan Endsley, Enrico Congiu
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The VLA Frontier Field Survey: A Comparison of the Radio and UV/Optical Size of 0.3 ≲ z ≲ 3 Star-forming Galaxies

The Astrophysical Journal American Astronomical Society 910:2 (2021) 106

Authors:

EF Jiménez-Andrade, EJ Murphy, I Heywood, I Smail, K Penner, E Momjian, M Dickinson, L Armus, TJW Lazio
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The VLA Frontier Fields Survey: Deep, High-resolution Radio Imaging of the MACS Lensing Clusters at 3 and 6 GHz

The Astrophysical Journal American Astronomical Society 910:2 (2021) 105

Authors:

I Heywood, EJ Murphy, EF Jiménez-Andrade, L Armus, WD Cotton, C DeCoursey, M Dickinson, TJW Lazio, E Momjian, K Penner, I Smail, OM Smirnov
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Structured variational inference for simulating populations of radio galaxies

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 503:3 (2021) 3351-3370

Authors:

David J Bastien, Anna MM Scaife, Hongming Tang, Micah Bowles, Fiona Porter
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The VANDELS ESO public spectroscopic survey: final data release of 2087 spectra and spectroscopic measurements

Astronomy and Astrophysics EDP Sciences 647 (2021) A150

Authors:

B Garilli, R McLure, L Pentericci, P Franzetti, A Gargiulo, A Carnall, O Cucciati, A Iovino, R Amorin, M Bolzonella, A Bongiorno, M Castellano, A Cimatti, M Cirasuolo, F Cullen, J Dunlop, D Elbaz, S Finkelstein, A Fontana, F Fontanot, M Fumana, L Guaita, W Hartley, M Jarvis, S Juneau, D Maccagni, D McLeod, K Nandra, E Pompei, L Pozzetti, M Scodeggio, M Talia, A Calabro, G Cresci, Jpu Fynbo, Np Hathi, P Hibon, Am Koekemoer, M Magliocchetti, M Salvato, G Vietri, G Zamorani, O Almaini, I Balestra, S Bardelli, R Begley, G Brammer, Ef Bell, Raa Bowler, M Brusa

Abstract:

VANDELS is an ESO Public Spectroscopic Survey designed to build a sample of high-signal-to-noise ratio, medium-resolution spectra of galaxies at redshifts between 1 and 6.5. Here we present the final Public Data Release of the VANDELS Survey, comprising 2087 redshift measurements. We provide a detailed description of sample selection, observations, and data reduction procedures. The final catalogue reaches a target selection completeness of 40% at iAB = 25. The high signal-to-noise ratio of the spectra (above 7 in 80% of the spectra) and the dispersion of 2.5 Å allowed us to measure redshifts with high precision, the redshift measurement success rate reaching almost 100%. Together with the redshift catalogue and the reduced spectra, we also provide optical mid-infrared photometry and physical parameters derived through fitting the spectral energy distribution. The observed galaxy sample comprises both passive and star forming galaxies covering a stellar mass range of 8.3 < Log(M∗/M⊙) < 11.7.
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