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Quasi-periodic eruptions from impacts between the secondary and a rigidly precessing accretion disc in an extreme mass-ratio inspiral system
DOI: 10.1051/0004-6361/202346565 Bibcode: 2023A&A...675A.100F

Lupi, Alessandro; Miniutti, Giovanni; Giustini, Margherita +7 more

X-ray quasi-periodic eruptions (QPEs) represent a recently discovered example of extreme X-ray variability associated with supermassive black holes. These are high-amplitude bursts recurring every few hours that are detected in the soft X-ray band from the nuclei of nearby galaxies whose optical spectra lack the broad emission lines typically obse…

2023 Astronomy and Astrophysics
XMM-Newton 77
UNCOVER: Illuminating the Early Universe-JWST/NIRSpec Confirmation of z > 12 Galaxies
DOI: 10.3847/2041-8213/acfe07 Bibcode: 2023ApJ...957L..34W

Labbé, Ivo; van Dokkum, Pieter; Fujimoto, Seiji +24 more

Observations of high-redshift galaxies provide a critical direct test to the theories of early galaxy formation, yet to date, only three have been spectroscopically confirmed at z > 12. Due to strong gravitational lensing over a wide area, the galaxy cluster field A2744 is ideal for searching for the earliest galaxies. Here we present JWST/NIRS…

2023 The Astrophysical Journal
eHST JWST 76
TDCOSMO. XII. Improved Hubble constant measurement from lensing time delays using spatially resolved stellar kinematics of the lens galaxy
DOI: 10.1051/0004-6361/202345878 Bibcode: 2023A&A...673A...9S

Treu, Tommaso; Fassnacht, Christopher D.; Birrer, Simon +12 more

Strong-lensing time delays enable the measurement of the Hubble constant (H0) independently of other traditional methods. The main limitation to the precision of time-delay cosmography is mass-sheet degeneracy (MSD). Some of the previous TDCOSMO analyses broke the MSD by making standard assumptions about the mass density profile of the …

2023 Astronomy and Astrophysics
eHST 76
First Look at z > 1 Bars in the Rest-frame Near-infrared with JWST Early CEERS Imaging
DOI: 10.3847/2041-8213/acacfb Bibcode: 2023ApJ...945L..10G

Papovich, Casey; Finkelstein, Steven L.; Barro, Guillermo +45 more

Stellar bars are key drivers of secular evolution in galaxies and can be effectively studied using rest-frame near-infrared (NIR) images, which trace the underlying stellar mass and are less impacted by dust and star formation than rest-frame UV or optical images. We leverage the power of JWST CEERS NIRCam images to present the first quantitative …

2023 The Astrophysical Journal
eHST JWST 76
GA-NIFS: The ultra-dense, interacting environment of a dual AGN at z ∼ 3.3 revealed by JWST/NIRSpec IFS
DOI: 10.1051/0004-6361/202346649 Bibcode: 2023A&A...679A..89P

Maiolino, R.; Jakobsen, P.; Perna, M. +18 more

Context. LBQS 0302−0019 is a blue quasar (QSO) at z ∼ 3.3 that hosts powerful outflows and resides in a complex environment consisting of an obscured active galactic nucleus (AGN) candidate and multiple companions, all within 30 kpc in projection.
Aims: We aim to characterise this complex system using JWST NIRSpec Integral Field Spectrograph …

2023 Astronomy and Astrophysics
JWST 76
Two Massive, Compact, and Dust-obscured Candidate z ≃ 8 Galaxies Discovered by JWST
DOI: 10.3847/1538-4357/acef21 Bibcode: 2023ApJ...956...61A

Papovich, Casey; Yang, Guang; Finkelstein, Steven L. +58 more

We present a search for extremely red, dust-obscured, z > 7 galaxies with JWST/NIRCam+MIRI imaging over the first 20 arcmin2 of publicly available Cycle 1 data from the COSMOS-Web, CEERS, and PRIMER surveys. Based on their red color in F277W-F444W (~2.5 mag) and detection in MIRI/F770W (~25 mag), we identify two galaxies, COS-z8M1 an…

2023 The Astrophysical Journal
Gaia eHST JWST 76
S 5: Probing the Milky Way and Magellanic Clouds potentials with the 6D map of the Orphan-Chenab stream
DOI: 10.1093/mnras/stad551 Bibcode: 2023MNRAS.521.4936K

Lewis, Geraint F.; Erkal, Denis; Bland-Hawthorn, Joss +12 more

We present a 6D map of the Orphan-Chenab (OC) stream by combining the data from Southern Stellar Stream Spectroscopic Survey (S5) and Gaia. We reconstruct the proper motion, radial velocity, distance, on-sky track, and stellar density along the stream with spline models. The stream has a total luminosity of MV = -8.2 and meta…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 76
Ejecta from the DART-produced active asteroid Dimorphos
DOI: 10.1038/s41586-023-05811-4 Bibcode: 2023Natur.616..452L

Granvik, Mikael; Kolokolova, Ludmilla; Weaver, Harold A. +61 more

Some active asteroids have been proposed to be formed as a result of impact events1. Because active asteroids are generally discovered by chance only after their tails have fully formed, the process of how impact ejecta evolve into a tail has, to our knowledge, not been directly observed. The Double Asteroid Redirection Test (DART) miss…

2023 Nature
eHST 76
A structured jet explains the extreme GRB 221009A
DOI: 10.1126/sciadv.adi1405 Bibcode: 2023SciA....9I1405O

Kouveliotou, Chryssa; Buckley, David A. H.; Hammerstein, Erica +29 more

Long-duration gamma-ray bursts (GRBs) are powerful cosmic explosions, signaling the death of massive stars. Among them, GRB 221009A is by far the brightest burst ever observed. Because of its enormous energy ( E iso ≈ 10 55 erg) and proximity ( z ≈ 0.15), GRB 221009A is an exceptionally rare event that pushes the limits of our theories. We present…

2023 Science Advances
XMM-Newton 76
Cold Jupiters and improved masses in 38 Kepler and K2 small planet systems from 3661 HARPS-N radial velocities. No excess of cold Jupiters in small planet systems
DOI: 10.1051/0004-6361/202346211 Bibcode: 2023A&A...677A..33B

Vanderburg, A.; Poretti, E.; Sozzetti, A. +31 more

The exoplanet population characterized by relatively short orbital periods (P < 100 d) around solar-type stars is dominated by super-Earths and sub-Neptunes. However, these planets are missing in our Solar System and the reason behind this absence is still unknown. Two theoretical scenarios invoke the role of Jupiter as the possible culprit: Ju…

2023 Astronomy and Astrophysics
Gaia 75