Search Publications

MIDIS: The Relation between Strong (Hβ + [O III]) Emission, Star Formation, and Burstiness around the Epoch of Reionization
DOI: 10.3847/1538-4357/ad4eb2 Bibcode: 2024ApJ...969..159C

Nørgaard-Nielsen, H. U.; Östlin, G.; Güdel, M. +25 more

We investigate the properties of strong (Hβ + [O III]) emitters before and after the end of the "Epoch of Reionization" from z = 8 to z = 5.5. We make use of ultradeep JWST/NIRCam imaging in the parallel field (P2) of the MIRI Deep Imaging Survey (MIDIS) in the Hubble eXtreme Deep Field (H-XDF), in order to select prominent (Hβ + [O III]) emitters…

2024 The Astrophysical Journal
eHST JWST 22
Lyman continuum leaker candidates at z ∼ 3-4 in the HDUV based on a spectroscopic sample of MUSE LAEs
DOI: 10.1051/0004-6361/202346656 Bibcode: 2024A&A...684A..42K

Oesch, P. A.; Illingworth, G. D.; Verhamme, A. +15 more

Context. In recent years, a number of Lyman continuum (LyC) leaker candidates have been found at intermediate redshifts, providing insight into how the Universe was reionised at early cosmic times. There are now around 100 known LyC leakers at all redshifts, which enables us to analyse their properties statistically.
Aims: Here, we identify n…

2024 Astronomy and Astrophysics
eHST 22
JWST MIRI Detections of Hα and [O III] and a Direct Metallicity Measurement of the z = 10.17 Lensed Galaxy MACS0647‑JD
DOI: 10.3847/1538-4357/ad6562 Bibcode: 2024ApJ...973...81H

Costantin, Luca; Hutchison, Taylor A.; Larson, Rebecca L. +30 more

JWST spectroscopy has revolutionized our understanding of galaxies in the early Universe. Covering wavelengths up to 5.3 µm, NIRSpec can detect rest-frame optical Hα emission lines out to z = 7 and [O III] to z = 9.5. Observing these lines in more distant galaxies requires longer wavelength spectroscopy with MIRI. Here we present MIRI Medium…

2024 The Astrophysical Journal
eHST JWST 22
Probing orbits of stellar mass objects deep in galactic nuclei with quasiperiodic eruptions. II. Population analysis
DOI: 10.1103/PhysRevD.110.083019 Bibcode: 2024PhRvD.110h3019Z

Pan, Zhen; Zhou, Cong; Huang, Lei +2 more

Quasiperiodic eruptions (QPEs) are intense repeating soft x-ray bursts with recurrence times about a few hours to a few weeks from galactic nuclei. Though the debates on the origin of QPEs have not completely settled down, more and more analyses favor the interpretation that QPEs are the result of collisions between a stellar mass object (a stella…

2024 Physical Review D
XMM-Newton 22
Abundant hydrocarbons in the disk around a very-low-mass star
DOI: 10.1126/science.adi8147 Bibcode: 2024Sci...384.1086A

Waters, L. B. F. M.; Olofsson, G.; Kamp, I. +40 more

Very-low-mass stars (those less than 0.3 solar masses) host orbiting terrestrial planets more frequently than other types of stars. The compositions of those planets are largely unknown but are expected to relate to the protoplanetary disk in which they form. We used James Webb Space Telescope mid-infrared spectroscopy to investigate the chemical …

2024 Science
XMM-Newton JWST 22
Emission lines due to ionizing radiation from a compact object in the remnant of Supernova 1987A
DOI: 10.1126/science.adj5796 Bibcode: 2024Sci...383..898F

Fox, O. D.; Blommaert, J. A. D. L.; Larsson, J. +31 more

The nearby Supernova 1987A was accompanied by a burst of neutrino emission, which indicates that a compact object (a neutron star or black hole) was formed in the explosion. There has been no direct observation of this compact object. In this work, we observe the supernova remnant with JWST spectroscopy, finding narrow infrared emission lines of a…

2024 Science
Gaia JWST 22
The Star-forming Main Sequence in JADES and CEERS at z > 1.4: Investigating the Burstiness of Star Formation
DOI: 10.3847/1538-4357/ad8ba4 Bibcode: 2024ApJ...977..133C

Shapley, Alice E.; Reddy, Naveen A.; Sanders, Ryan L. +5 more

We have used public JWST/NIRSpec and JWST/NIRCam observations from the CEERS and JADES surveys in order to analyze the star-forming main sequence (SFMS) over the redshift range 1.4 ≤ z < 7. We calculate the star formation rates (SFRs) of the galaxy sample using three approaches: Balmer line luminosity, spectral energy distribution (SED) fitting…

2024 The Astrophysical Journal
eHST JWST 22
Galaxy Quenching at the High Redshift Frontier: A Fundamental Test of Cosmological Models in the Early Universe with JWST-CEERS
DOI: 10.3847/1538-4357/ad0a98 Bibcode: 2024ApJ...961..163B

Maiolino, Roberto; Conselice, Christopher J.; Bluck, Asa F. L. +10 more

We present an analysis of the quenching of star formation in massive galaxies (M * > 109.5 M ) within the first 0.5–3 Gyr of the Universe's history utilizing JWST-CEERS data. We utilize a combination of advanced statistical methods to accurately constrain the intrinsic dependence of quenching in a multidimensio…

2024 The Astrophysical Journal
eHST JWST 22
Young Star Clusters Dominate the Production of Detached Black Hole–Star Binaries
DOI: 10.3847/1538-4357/ad2f2c Bibcode: 2024ApJ...965...22D

Breivik, Katelyn; Rodriguez, Carl L.; Di Carlo, Ugo Niccolò +1 more

The recent discovery of two detached black hole–star (BH–star) binaries from Gaia's third data release has sparked interest in understanding the formation mechanisms of these systems. We investigate the formation of these systems by dynamical processes in young star clusters (SCs) and via isolated binary (IB) evolution, using a combination of dire…

2024 The Astrophysical Journal
Gaia 22
Effect of Extinction on Quasar Luminosity Distances Determined from UV and X-Ray Flux Measurements
DOI: 10.3847/1538-4357/ad11dc Bibcode: 2024ApJ...961..229Z

Zajaček, Michal; Czerny, Bożena; Khadka, Narayan +4 more

In Khadka et al., a sample of X-ray-detected reverberation-mapped quasars was presented and applied for the comparison of cosmological constraints inferred using two well-established relations in active galactic nuclei—the X-ray/UV luminosity (L X –L UV) relation and the broad-line region radius–luminosity (R–L) relation. L …

2024 The Astrophysical Journal
XMM-Newton 22