Search Publications

A sub-Earth-mass planet orbiting Barnard's star
DOI: 10.1051/0004-6361/202451311 Bibcode: 2024A&A...690A..79G

Bouchy, F.; Rebolo, R.; Allende Prieto, C. +37 more

Context. ESPRESSO guaranteed time observations (GTOs) at the 8.2m VLT telescope were performed to look for Earth-like exoplanets in the habitable zone of nearby stars. Barnard's star is a primary target within the ESPRESSO GTO as it is the second closest neighbour to our Sun after the α Centauri stellar system. Aims. We present here a large set of…

2024 Astronomy and Astrophysics
Gaia 7
The radiative and dynamical impact of clouds in the atmosphere of the hot Jupiter WASP-43 b
DOI: 10.1051/0004-6361/202347069 Bibcode: 2024A&A...683A.231T

Millour, E.; Spiga, A.; Bézard, B. +6 more

Context. Hot Jupiters are tidally locked gaseous exoplanets that exhibit large day-night temperature contrasts. Their cooler nightsides are thought to host clouds, as has been suggested by numerous observations. However, the exact nature of these clouds, their spatial distribution, and their impact on atmospheric dynamics, thermal structure, and s…

2024 Astronomy and Astrophysics
eHST JWST 7
Planetary Nebula NGC 2818: Revealing its complex 3D morphology
DOI: 10.1093/mnras/stae1013 Bibcode: 2024MNRAS.530.3327D

Boumis, P.; Chiotellis, A.; Derlopa, S. +3 more

We carry out an advanced morpho-kinematic analysis of the Planetary Nebula (PN) NGC 2818, whose complex morphology is described by a basic bipolar component, filamentary structures and a knotty central region. We performed an upgrated 3D Morpho-kinematic (MK) model by employing the SHAPE software, combining for the first time in PNe optical 2D spa…

2024 Monthly Notices of the Royal Astronomical Society
Gaia eHST 7
An Extensive Hubble Space Telescope Study of the Offset and Host Light Distributions of Type I Superluminous Supernovae
DOI: 10.3847/1538-4357/ad12be Bibcode: 2024ApJ...961..169H

Berger, Edo; Gomez, Sebastian; Blanchard, Peter K. +1 more

We present an extensive Hubble Space Telescope rest-frame UV imaging study of the locations of Type I superluminous supernovae (SLSNe) within their host galaxies. The sample includes 65 SLSNe with detected host galaxies in the redshift range z ≈ 0.05–2. Using precise astrometric matching with SN images, we determine the distributions of the physic…

2024 The Astrophysical Journal
Gaia eHST 7
AGN STORM 2. V. Anomalous Behavior of the C IV Light Curve of Mrk 817
DOI: 10.3847/1538-4357/ad1be4 Bibcode: 2024ApJ...963..123H

Treu, Tommaso; Kaspi, Shai; Hall, Patrick B. +49 more

An intensive reverberation mapping campaign of the Seyfert 1 galaxy Mrk 817 using the Cosmic Origins Spectrograph on the Hubble Space Telescope revealed significant variations in the response of broad UV emission lines to fluctuations in the continuum emission. The response of the prominent UV emission lines changes over an ∼60 day duration, resul…

2024 The Astrophysical Journal
eHST 7
Nine lensed quasars and quasar pairs discovered through spatially extended variability in Pan-STARRS
DOI: 10.1051/0004-6361/202347598 Bibcode: 2024A&A...682A..47D

Anguita, Timo; Courbin, Frédéric; Hempel, Angela +7 more

We present the proof of concept of a method for finding strongly lensed quasars using their spatially extended photometric variability through difference imaging in cadenced imaging survey data. We applied the method to Pan-STARRS, starting with an initial selection of 14 107 Gaia multiplets with quasar-like infrared colours from WISE. We identifi…

2024 Astronomy and Astrophysics
Gaia 7
The Lyα Nondetection by JWST NIRSpec of a Strong Lyα Emitter at z = 5.66 Confirmed by MUSE
DOI: 10.3847/1538-4357/ad61db Bibcode: 2024ApJ...972..121J

Kong, Xu; Cheng, Cheng; Boyett, Kristan +6 more

The detections of Lyα emission in galaxies with redshifts above 5 are of utmost importance for constraining the cosmic reionization timeline, yet such detections are usually based on slit spectroscopy. Here we investigate the significant bias induced by slit placement on the estimate of Lyα escape fraction (

2024 The Astrophysical Journal
eHST JWST 7
Refining Galactic primordial black hole evaporation constraints
DOI: 10.1103/PhysRevD.110.123022 Bibcode: 2024PhRvD.110l3022L

Balaji, Shyam; Koechler, Jordan; Luque, Pedro De la Torre

We revisit the role of primordial black holes (PBHs) as potential dark matter (DM) candidates, particularly focusing on light asteroid-mass PBHs. These PBHs are expected to emit particles through Hawking evaporation that can generate cosmic rays (CRs), eventually producing other secondary radiations through their propagation in the Milky Way, in a…

2024 Physical Review D
XMM-Newton 7
A second view on the X-ray polarization of NGC 4151 with IXPE
DOI: 10.1051/0004-6361/202451645 Bibcode: 2024A&A...691A..29G

Bianchi, S.; Done, C.; Petrucci, P. -O. +21 more

We report on the second observing program of the active galactic nucleus NGC 4151 with simultaneous Imaging X-ray Polarimetry Explorer (IXPE; 750 ks), NuSTAR (∼60 ks), XMM-Newton (∼75 ks), and NICER (∼65 ks) pointings. NGC 4151 is the first Type-1 radio-quiet Seyfert galaxy with constrained polarization properties for the X-ray corona. Despite the…

2024 Astronomy and Astrophysics
XMM-Newton 7
Systematic KMTNet Planetary Anomaly Search. X. Complete Sample of 2017 Prime-field Planets
DOI: 10.3847/1538-3881/ad1888 Bibcode: 2024AJ....167...88R

Han, Cheongho; Udalski, Andrzej; Lee, Chung-Uk +42 more

We complete the analysis of planetary candidates found by the KMT AnomalyFinder for the 2017 prime fields that cover ∼13 deg2. We report three unambiguous planets: OGLE-2017-BLG-0640, OGLE-2017-BLG-1275, and OGLE-2017-BLG-1237. The first two of these were not previously identified, while the last was not previously published due to tech…

2024 The Astronomical Journal
Gaia 7