Search Publications

Charting the Galactic Acceleration Field. II. A Global Mass Model of the Milky Way from the STREAMFINDER Atlas of Stellar Streams Detected in Gaia DR3
DOI: 10.3847/1538-4357/ad382d Bibcode: 2024ApJ...967...89I

Bianchini, Paolo; Malhan, Khyati; Martin, Nicolas F. +17 more

We present an atlas and follow-up spectroscopic observations of 87 thin stream-like structures detected with the STREAMFINDER algorithm in Gaia DR3, of which 28 are new discoveries. Here, we focus on using these streams to refine mass models of the Galaxy. Fits with a double-power-law halo with the outer power-law slope set to ‑β h = …

2024 The Astrophysical Journal
Gaia 44
Strong constraints on the gravitational law from Gaia DR3 wide binaries
DOI: 10.1093/mnras/stad3393 Bibcode: 2024MNRAS.527.4573B

Mieske, Steffen; Famaey, Benoit; Ibata, Rodrigo +4 more

We test Milgromian dynamics (MOND) using wide binary stars (WBs) with separations of 2-30 kAU. Locally, the WB orbital velocity in MOND should exceed the Newtonian prediction by $\approx 20~{{\ \rm per\ cent}}$ at asymptotically large separations given the Galactic external field effect (EFE). We investigate this with a detailed statistical analys…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 44
GA-NIFS: The core of an extremely massive protocluster at the epoch of reionisation probed with JWST/NIRSpec
DOI: 10.1051/0004-6361/202348824 Bibcode: 2024A&A...688A.146A

Pérez-González, Pablo G.; Charlot, Stéphane; Chevallard, Jacopo +24 more

Context. The SPT0311-58 system resides in a massive dark-matter halo at z ∼ 6.9. It hosts two dusty galaxies (E and W) with a combined star formation rate (SFR) of ∼3500 M yr−1, mostly obscured and identified by the rest-frame IR emission. The surrounding field exhibits an overdensity of submillimetre sources, making it a ca…

2024 Astronomy and Astrophysics
Gaia eHST JWST 44
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
Quaia, the Gaia-unWISE Quasar Catalog: An All-sky Spectroscopic Quasar Sample
DOI: 10.3847/1538-4357/ad1328 Bibcode: 2024ApJ...964...69S

Hogg, David W.; Rix, Hans-Walter; Eilers, Anna-Christina +4 more

We present a new, all-sky quasar catalog, Quaia, that samples the largest comoving volume of any existing spectroscopic quasar sample. The catalog draws on the 6,649,162 quasar candidates identified by the Gaia mission that have redshift estimates from the space observatory's low-resolution blue photometer/red photometer spectra. This initial samp…

2024 The Astrophysical Journal
Gaia 44
Identification of a transition from stochastic to secular star formation around z = 9 with JWST
DOI: 10.1051/0004-6361/202348091 Bibcode: 2024A&A...686A.128C

Magnelli, B.; Daddi, E.; Elbaz, D. +6 more

Star formation histories (SFHs) of early galaxies (6 < z < 12) have been found to be highly stochastic in both simulations and observations, while at z≲6 the presence of a main sequence (MS) of star-forming galaxies implies secular processes at play. In this work we characterise the SFH variability of early galaxies as a function of their st…

2024 Astronomy and Astrophysics
JWST 43
Chasing the impact of the Gaia-Sausage-Enceladus merger on the formation of the Milky Way thick disc
DOI: 10.1093/mnrasl/slad033 Bibcode: 2024MNRAS.528L.122C

Ting, Yuan-Sen; Grand, Robert J. J.; Fragkoudi, Francesca +8 more

We employ our Bayesian Machine Learning framework BINGO (Bayesian INference for Galactic archaeOlogy) to obtain high-quality stellar age estimates for 68 360 red giant and red clump stars present in the 17th data release of the Sloan Digital Sky Survey, the APOGEE-2 high-resolution spectroscopic survey. By examining the denoised age-met…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 43
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
Ionizing properties of galaxies in JADES for a stellar mass complete sample: resolving the cosmic ionizing photon budget crisis at the Epoch of Reionization
DOI: 10.1093/mnras/stae2537 Bibcode: 2024MNRAS.535.2998S

Maiolino, R.; Johnson, B. D.; Willott, C. +26 more

We use NIRCam imaging from the JWST Advanced Deep Extragalactic Survey (JADES) to study the ionizing properties of a sample of 14 652 galaxies at $3 \le z_{\rm {phot}} \le 9$, 90 per cent complete in stellar mass down to log(M

2024 Monthly Notices of the Royal Astronomical Society
eHST JWST 42
New insight on the nature of cosmic reionizers from the CEERS survey
DOI: 10.1051/0004-6361/202347884 Bibcode: 2024A&A...685A...3M

Kartaltepe, J. S.; Dickinson, M.; Finkelstein, S. L. +30 more

The Epoch of Reionization (EoR) began when galaxies grew in abundance and luminosity, so their escaping Lyman continuum (LyC) radiation started ionizing the surrounding neutral intergalactic medium (IGM). Despite significant recent progress, the nature and role of cosmic reionizers are still unclear: in order to define them, it would be necessary …

2024 Astronomy and Astrophysics
eHST JWST 42