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A. C. Carnall

Identifiers

  • name variant A. C. Carnall 0.60 · backfill

Papers (40)

  1. The JWST EXCELS survey: Too much, too young, too fast? Ultra-massive quiescent galaxies at 3 < z < 5 astro-ph.GA · 2024 · author #1
  2. The NIRVANDELS Survey: the stellar and gas-phase mass-metallicity relations of star-forming galaxies at z = 3.5 astro-ph.GA · 2024 · author #10
  3. Quiescent or dusty? Unveiling the nature of extremely red galaxies at $z>3$ astro-ph.GA · 2024 · author #6
  4. JWST PRIMER: A new multi-field determination of the evolving galaxy UV luminosity function at redshifts $\mathbf{z \simeq 9-15}$ astro-ph.GA · 2024 · author #10
  5. The sizes of bright Lyman-break galaxies at $z\simeq3-5$ with JWST PRIMER astro-ph.GA · 2024 · author #7
  6. The ultraviolet continuum slopes of high-redshift galaxies: evidence for the emergence of dust-free stellar populations at z > 10 astro-ph.GA · 2023 · author #6
  7. The VANDELS ESO public spectroscopic survey: The spectroscopic measurements catalogue astro-ph.GA · 2023 · author #23
  8. Connecting the escape fraction of Lyman-alpha and Lyman-continuum photons in star-forming galaxies at $\mathbf{z\simeq 4-5}$ astro-ph.GA · 2023 · author #6
  9. A new measurement of the expansion history of the Universe at z=1.26 with cosmic chronometers in VANDELS astro-ph.CO · 2023 · author #7
  10. The connection between stellar mass, age and quenching timescale in massive quiescent galaxies at $z \simeq 1$ astro-ph.GA · 2023 · author #2
  11. A massive quiescent galaxy at redshift 4.658 astro-ph.GA · 2023 · author #1
  12. The abundance of $z \gtrsim 10$ galaxy candidates in the HUDF using deep JWST NIRCam medium-band imaging astro-ph.GA · 2022 · author #5
  13. The VANDELS survey: the ionizing properties of star-forming galaxies at $3 \leq z \leq 5$ using deep rest-frame ultraviolet spectroscopy astro-ph.GA · 2022 · author #9
  14. The ultraviolet continuum slopes ($\mathbf{\beta}$) of galaxies at $\mathbf{z\simeq8-16}$ from JWST and ground-based near-infrared imaging astro-ph.GA · 2022 · author #6
  15. A surprising abundance of massive quiescent galaxies at 3 < z < 5 in the first data from JWST CEERS astro-ph.GA · 2022 · author #1
  16. The evolution of the galaxy UV luminosity function at redshifts z ~ 8-15 from deep JWST and ground-based near-infrared imaging astro-ph.GA · 2022 · author #5
  17. A first look at the SMACS0723 JWST ERO: spectroscopic redshifts, stellar masses and star-formation histories astro-ph.GA · 2022 · author #1
  18. The XXL survey. XLIX. Linking the members star formation histories to the cluster mass assembly in the z=1.98 galaxy cluster XLSSC 122 astro-ph.GA · 2022 · author #5
  19. On the Simultaneous Modelling of Dust and Stellar Populations for Interpretation of Galaxy Properties astro-ph.GA · 2022 · author #3
  20. The VANDELS survey: a measurement of the average Lyman-continuum escape fraction of star-forming galaxies at z=3.5 astro-ph.GA · 2022 · author #6
  21. A combined VANDELS and LEGA-C study: the evolution of quiescent galaxy size, stellar mass and age from $\mathbf{\textit{z} = 0.6}$ to $\mathbf{\textit{z} = 1.3}$ astro-ph.GA · 2022 · author #2
  22. The stellar metallicities of massive quiescent galaxies at 1.0 < z < 1.3 from KMOS+VANDELS astro-ph.GA · 2021 · author #1
  23. The VANDELS Survey: New constraints on the high-mass X-ray binary populations in normal star-forming galaxies at 3 < z < 5.5 astro-ph.GA · 2021 · author #6
  24. The NIRVANDELS Survey: a robust detection of $\alpha$-enhancement in star-forming galaxies at $z\simeq3.4$ astro-ph.GA · 2021 · author #12
  25. The evolution of the galaxy stellar mass function over the last twelve billion years from a combination of ground-based and HST surveys astro-ph.GA · 2020 · author #5
  26. Timing the earliest quenching events with a robust sample of massive quiescent galaxies at 2 < z < 5 astro-ph.GA · 2020 · author #1
  27. The VANDELS survey: A strong correlation between Ly$\alpha$ equivalent width and stellar metallicity at $\mathbf{3\leq z \leq 5}$ astro-ph.GA · 2020 · author #4
  28. The Intergalactic medium transmission towards z>4 galaxies with VANDELS and the impact of dust attenuation astro-ph.CO · 2019 · author #8
  29. The properties of He II 1640 emitters at z ~ 2.5-5 from the VANDELS survey astro-ph.GA · 2019 · author #11
  30. The VANDELS survey: the stellar metallicities of star-forming galaxies at 2.5 < z < 5.0 astro-ph.GA · 2019 · author #8
  31. The VANDELS survey: the star-formation histories of massive quiescent galaxies at 1.0 < z < 1.3 astro-ph.GA · 2019 · author #1
  32. The VANDELS survey: the role of ISM and galaxy physical properties on the escape of Ly{\alpha} emission in z $\sim$ 3.5 star-forming galaxies astro-ph.GA · 2019 · author #9
  33. Maximising the power of deep extragalactic imaging surveys with the James Webb Space Telescope astro-ph.GA · 2019 · author #5
  34. How to measure galaxy star-formation histories I: Parametric models astro-ph.GA · 2018 · author #1
  35. The VANDELS ESO public spectroscopic survey astro-ph.GA · 2018 · author #11
  36. The VANDELS ESO public spectroscopic survey: observations and first data release astro-ph.GA · 2018 · author #9
  37. Inferring the star-formation histories of massive quiescent galaxies with BAGPIPES: Evidence for multiple quenching mechanisms astro-ph.GA · 2017 · author #1
  38. The VANDELS survey: Dust attenuation in star-forming galaxies at $\mathbf{z=3-4}$ astro-ph.GA · 2017 · author #6
  39. SpectRes: A Fast Spectral Resampling Tool in Python astro-ph.IM · 2017 · author #1
  40. Two bright z > 6 quasars from VST ATLAS and a new method of optical plus mid-infra-red colour selection astro-ph.GA · 2015 · author #1

Mentions

  • 2405.02242 #1 · arxiv_oai · confidence 0.70 A. C. Carnall
  • 2403.03171 #10 · arxiv_oai · confidence 0.70 A. C. Carnall
  • 2401.15971 #7 · arxiv_oai · confidence 0.70 A. C. Carnall
  • 2405.00774 #10 · arxiv_oai · confidence 0.70 A. C. Carnall
  • 2311.06209 #6 · arxiv_oai · confidence 0.70 A. C. Carnall
  • 2404.08052 #6 · arxiv_oai · confidence 0.70 A. C. Carnall
  • 1712.04452 #1 · arxiv_oai · confidence 0.70 A. C. Carnall
  • 2305.16387 #7 · arxiv_oai · confidence 0.70 A. C. Carnall
  • 2306.03916 #6 · arxiv_oai · confidence 0.70 A. C. Carnall
  • 2309.14436 #23 · arxiv_oai · confidence 0.70 A. C. Carnall
  • 2301.11413 #1 · arxiv_oai · confidence 0.70 A. C. Carnall
  • 2211.01351 #9 · arxiv_oai · confidence 0.70 A. C. Carnall
  • 2303.06107 #2 · arxiv_oai · confidence 0.70 A. C. Carnall
  • 2212.10126 #5 · arxiv_oai · confidence 0.70 A. C. Carnall
  • 2208.00986 #1 · arxiv_oai · confidence 0.70 A. C. Carnall
  • 2208.04914 #6 · arxiv_oai · confidence 0.70 A. C. Carnall
  • 2207.12356 #5 · arxiv_oai · confidence 0.70 A. C. Carnall
  • 2207.08778 #1 · arxiv_oai · confidence 0.70 A. C. Carnall
  • 2206.10063 #5 · arxiv_oai · confidence 0.70 A. C. Carnall
  • 2206.06379 #3 · arxiv_oai · confidence 0.70 A. C. Carnall
  • 2108.13430 #1 · arxiv_oai · confidence 0.70 A. C. Carnall
  • 2202.04088 #6 · arxiv_oai · confidence 0.70 A. C. Carnall
  • 2201.10576 #2 · arxiv_oai · confidence 0.70 A. C. Carnall
  • 2104.02624 #6 · arxiv_oai · confidence 0.70 A. C. Carnall
  • 2103.06300 #12 · arxiv_oai · confidence 0.70 A. C. Carnall
  • 2009.03176 #5 · arxiv_oai · confidence 0.70 A. C. Carnall
  • 2001.11975 #1 · arxiv_oai · confidence 0.70 A. C. Carnall
  • 2001.11063 #4 · arxiv_oai · confidence 0.70 A. C. Carnall
  • 1911.09999 #11 · arxiv_oai · confidence 0.70 A. C. Carnall
  • 1911.12532 #8 · arxiv_oai · confidence 0.70 A. C. Carnall
  • 1903.11082 #1 · arxiv_oai · confidence 0.70 A. C. Carnall
  • 1903.08593 #9 · arxiv_oai · confidence 0.70 A. C. Carnall
  • 1903.11081 #8 · arxiv_oai · confidence 0.70 A. C. Carnall
  • 1903.08169 #5 · arxiv_oai · confidence 0.70 A. C. Carnall
  • 1811.03635 #1 · arxiv_oai · confidence 0.70 A. C. Carnall
  • 1803.07373 #9 · arxiv_oai · confidence 0.70 A. C. Carnall
  • 1803.07414 #11 · arxiv_oai · confidence 0.70 A. C. Carnall
  • 1712.01292 #6 · arxiv_oai · confidence 0.70 A. C. Carnall
  • 1705.05165 #1 · arxiv_oai · confidence 0.70 A. C. Carnall
  • 1502.07748 #1 · arxiv_oai · confidence 0.70 A. C. Carnall
  • 1502.07748 #1 · backfill · confidence 0.70 A. C. Carnall

Frequent Coauthors