Search Publications

The star-forming and ionizing properties of dwarf z 6-9 galaxies in JADES: insights on bursty star formation and ionized bubble growth
DOI: 10.1093/mnras/stae1857 Bibcode: 2024MNRAS.533.1111E

Chevallard, Jacopo; Carniani, Stefano; Bunker, Andrew J. +37 more

Reionization is thought to be driven by faint star-forming galaxies, but characterizing this population has long remained very challenging. Here, we utilize deep nine-band JADES (JWST Advanced Deep Extragalactic Survey)/NIRCam (Near-Infrared Camera) imaging to study the star-forming and ionizing properties of 756 $z\sim 6-9$ galaxies, including hu…

2024 Monthly Notices of the Royal Astronomical Society
eHST JWST 133
The galaxy UV luminosity function at z ≃ 11 from a suite of public JWST ERS, ERO, and Cycle-1 programs
DOI: 10.1093/mnras/stad3471 Bibcode: 2024MNRAS.527.5004M

Cullen, F.; McLure, R. J.; Dunlop, J. S. +8 more

We present a new determination of the evolving galaxy ultraviolet (UV) luminosity function (LF) over the redshift range 9.5 < z < 12.5 based on a wide-area (>250 arcmin2) data set of JWST NIRCam near-infrared imaging assembled from 13 public JWST surveys. Our relatively large-area search allows us to uncover a sample of 61 robu…

2024 Monthly Notices of the Royal Astronomical Society
eHST JWST 110
JWST PRIMER: a new multifield determination of the evolving galaxy UV luminosity function at redshifts z ≃ 9 - 15
DOI: 10.1093/mnras/stae2037 Bibcode: 2024MNRAS.533.3222D

Bowler, R. A. A.; Cullen, F.; McLure, R. J. +18 more

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 combination of several major Cycle-1 JWST imaging programmes - Public Release IMaging for Extragalactic Research, JWS…

2024 Monthly Notices of the Royal Astronomical Society
Gaia eHST JWST 99
Galaxy build-up in the first 1.5 Gyr of cosmic history: insights from the stellar mass function at z 4-9 from JWST NIRCam observations
DOI: 10.1093/mnras/stae1891 Bibcode: 2024MNRAS.533.1808W

Pérez-González, Pablo G.; Santini, Paola; Dickinson, Mark +28 more

Combining the public JWST/NIRCam imaging programs CEERS, PRIMER, and JADES, spanning a total area of $\sim 500\, {\rm arcmin}^2$, we obtain a sample of $\gt $30 000 galaxies at $z_{\rm phot}\sim 4\!-\!9$ that allows us to perform a complete, rest-optical-selected census of the galaxy population at $z\gt 3$. Comparing the stellar mass $M_*$ and the…

2024 Monthly Notices of the Royal Astronomical Society
Gaia eHST JWST 78
EPOCHS VI: the size and shape evolution of galaxies since z 8 with JWST Observations
DOI: 10.1093/mnras/stad3597 Bibcode: 2024MNRAS.527.6110O

Conselice, C. J.; Adams, N. J.; Li, Q. +8 more

We present the results of a size and structural analysis of 1395 galaxies at 0.5 ≤ z ≲ 8 with stellar masses log (M*/M)> 9.5 within the James Webb Space Telescope Public CEERS field that overlaps with the Hubble Space Telescope Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey EGS observations. We use GALFIT …

2024 Monthly Notices of the Royal Astronomical Society
Gaia eHST JWST 71
The UV continuum slopes of early star-forming galaxies in JADES
DOI: 10.1093/mnras/stae800 Bibcode: 2024MNRAS.529.4087T

Chevallard, Jacopo; Carniani, Stefano; Bunker, Andrew J. +22 more

The power-law slope of the rest-ultraviolet (UV) continuum (fλ ∝ λβ) is a key metric of early star-forming galaxies, providing one of our only windows into the stellar populations and physical conditions of z ≳ 10 galaxies. Expanding upon previous studies with limited sample sizes, we leverage deep imaging from the JWST Advan…

2024 Monthly Notices of the Royal Astronomical Society
eHST JWST 71
Extreme emission line galaxies detected in JADES JWST/NIRSpec - I. Inferred galaxy properties
DOI: 10.1093/mnras/stae2430 Bibcode: 2024MNRAS.535.1796B

Charlot, Stéphane; Chevallard, Jacopo; Maseda, Michael V. +33 more

Extreme emission line galaxies (EELGs) exhibit large equivalent widths (EW) in their rest-optical emission lines ([O III]$\lambda 5007$ or H $\alpha$ rest-frame EW

2024 Monthly Notices of the Royal Astronomical Society
eHST JWST 57
The ultraviolet continuum slopes of high-redshift galaxies: evidence for the emergence of dust-free stellar populations at z > 10
DOI: 10.1093/mnras/stae1211 Bibcode: 2024MNRAS.531..997C

Bowler, R. A. A.; Cullen, F.; McLure, R. J. +11 more

We present an analysis of the ultraviolet (UV) continuum slopes (β) for a sample of 172 galaxy candidates at 8 < zphot < 16 selected from a combination of JWST NIRCam imaging and COSMOS/UltraVISTA ground-based near-infrared imaging. Focusing primarily on a new sample of 121 galaxies at ⟨z⟩ ≃ 11 selected from ≃ 320 arcmin2

2024 Monthly Notices of the Royal Astronomical Society
eHST JWST 56
Fundamental scaling relationships revealed in the optical light curves of tidal disruption events
DOI: 10.1093/mnras/stad3001 Bibcode: 2024MNRAS.527.2452M

Ingram, Adam; van Velzen, Sjoert; Hammerstein, Erica +4 more

We present fundamental scaling relationships between properties of the optical/UV light curves of tidal disruption events (TDEs) and the mass of the black hole that disrupted the star. We have uncovered these relations from the late-time emission of TDEs. Using a sample of 63 optically selected TDEs, the latest catalogue to date, we observed flatt…

2024 Monthly Notices of the Royal Astronomical Society
eHST 44
Insight from JWST/Near Infrared Camera into galaxy overdensities around bright Lyman-alpha emitters during reionization: implications for ionized bubbles at z 9
DOI: 10.1093/mnras/stae516 Bibcode: 2024MNRAS.529..855W

Charlot, Stéphane; Chen, Zuyi; Stark, Daniel P. +4 more

Several studies have detected Lyman-alpha (Ly Α) from bright ($M_{\small UV}\lesssim -21.5$) galaxies during the early stages of reionization despite the significantly neutral intergalactic medium. To explain these detections, it has been suggested that z > 7 Ly Α emitters (LAEs) inhabit physical Mpc (pMpc)-scale ionized regions powered by over…

2024 Monthly Notices of the Royal Astronomical Society
eHST JWST 42