Search Publications

Unveiling the population of dual and lensed active galactic nuclei at sub-arcsec separations
DOI: 10.1038/s41550-022-01761-5 Bibcode: 2022NatAs...6.1185M

Marconi, A.; Pancino, E.; Nardini, E. +12 more

All cosmological models of structure formation predict the existence of a widespread population of dual supermassive black holes in-spiralling inside their common host galaxy, eventually merging and giving rise to intense gravitational waves. These systems can be identified as dual active galactic nuclei (AGNs) at kiloparsec separations, but only …

2022 Nature Astronomy
Gaia eHST 47
A pair of sub-Neptunes transiting the bright K-dwarf TOI-1064 characterized with CHEOPS
DOI: 10.1093/mnras/stab3799 Bibcode: 2022MNRAS.511.1043W

Lester, Kathryn V.; Charnoz, Sébastien; Triaud, Amaury H. M. J. +132 more

We report the discovery and characterization of a pair of sub-Neptunes transiting the bright K-dwarf TOI-1064 (TIC 79748331), initially detected in the Transiting Exoplanet Survey Satellite (TESS) photometry. To characterize the system, we performed and retrieved the CHaracterising ExOPlanets Satellite (CHEOPS), TESS, and ground-based photometry, …

2022 Monthly Notices of the Royal Astronomical Society
CHEOPS Gaia 47
The population of hot subdwarf stars studied with Gaia. IV. Catalogues of hot subluminous stars based on Gaia EDR3
DOI: 10.1051/0004-6361/202243337 Bibcode: 2022A&A...662A..40C

Geier, S.; Pelisoli, I.; Culpan, R. +3 more

In light of substantial new discoveries of hot subdwarfs by ongoing spectroscopic surveys and the availability of the Gaia mission Early Data Release 3 (EDR3), we compiled new releases of two catalogues of hot subluminous stars: The data release 3 (DR3) catalogue of the known hot subdwarf stars contains 6616 unique sources and provides multi-band …

2022 Astronomy and Astrophysics
Gaia 47
The K2 Galactic Archaeology Program Data Release 3: Age-abundance Patterns in C1-C8 and C10-C18
DOI: 10.3847/1538-4357/ac2c83 Bibcode: 2022ApJ...926..191Z

Lewis, Geraint F.; Vanderburg, Andrew; Chaplin, William J. +28 more

We present the third and final data release of the K2 Galactic Archaeology Program (K2 GAP) for Campaigns C1-C8 and C10-C18. We provide asteroseismic radius and mass coefficients, κ R and κ M , for ~19,000 red giant stars, which translate directly to radius and mass given a temperature. As such, K2 GAP DR3 represents the l…

2022 The Astrophysical Journal
Gaia 47
The atmosphere and architecture of WASP-189 b probed by its CHEOPS phase curve
DOI: 10.1051/0004-6361/202142400 Bibcode: 2022A&A...659A..74D

Alonso, R.; Deleuil, M.; Erikson, A. +83 more

Context. Gas giants orbiting close to hot and massive early-type stars can reach dayside temperatures that are comparable to those of the coldest stars. These `ultra-hot Jupiters' have atmospheres made of ions and atomic species from molecular dissociation and feature strong day-to-night temperature gradients. Photometric observations at different…

2022 Astronomy and Astrophysics
CHEOPS Gaia 47
The PLATO field selection process. I. Identification and content of the long-pointing fields
DOI: 10.1051/0004-6361/202142256 Bibcode: 2022A&A...658A..31N

Heras, A. M.; Deleuil, M.; Rauer, H. +26 more

PLAnetary Transits and Oscillations of stars is an ESA M-class satellite planned for launch by the end of 2026 and dedicated to the wide-field search of transiting planets around bright and nearby stars, with a strong focus on discovering habitable rocky planets hosted by solar-like stars. The choice of the fields to be pointed at is a crucial tas…

2022 Astronomy and Astrophysics
Gaia 47
The complex time and energy evolution of quasi-periodic eruptions in eRO-QPE1
DOI: 10.1051/0004-6361/202243259 Bibcode: 2022A&A...662A..49A

Salvato, M.; Buchner, J.; Nandra, K. +8 more

Quasi-periodic eruptions (QPEs) are recurrent X-ray bursts found in the nuclei of low-mass galaxies. Their trigger mechanism is still unknown, but recent models involving one or two stellar-mass companions around the central massive (≈105 − 106 M) black hole have gathered significant attention. While these models …

2022 Astronomy and Astrophysics
XMM-Newton 47
Being KLEVER at cosmic noon: Ionized gas outflows are inconspicuous in low-mass star-forming galaxies but prominent in massive AGN hosts
DOI: 10.1093/mnras/stac1026 Bibcode: 2022MNRAS.513.2535C

Maiolino, Roberto; Cresci, Giovanni; Jones, Gareth C. +13 more

We investigate the presence of ionized gas outflows in a sample of 141 main-sequence star-forming galaxies at 1.2 < z < 2.6 from the KLEVER (KMOS Lensed Emission Lines and VElocity Review) survey. Our sample covers an exceptionally wide range of stellar masses, 8.1 < log (M/M) < 11.3, pushing outflow studies int…

2022 Monthly Notices of the Royal Astronomical Society
eHST 47
Dark dimension, the swampland, and the dark matter fraction composed of primordial black holes
DOI: 10.1103/PhysRevD.106.086001 Bibcode: 2022PhRvD.106h6001A

Anchordoqui, Luis A.; Antoniadis, Ignatios; Lüst, Dieter

Very recently, it was suggested that combining the swampland program with the smallness of the dark energy and confronting these ideas to experiment lead to the prediction of the existence of a single extra dimension (dubbed the dark dimension) with characteristic length scale in the micron range. We show that the rate of Hawking radiation slows d…

2022 Physical Review D
INTEGRAL 46
The X-Ray and Radio Loud Fast Blue Optical Transient AT2020mrf: Implications for an Emerging Class of Engine-driven Massive Star Explosions
DOI: 10.3847/1538-4357/ac7a41 Bibcode: 2022ApJ...934..104Y

Kulkarni, S. R.; Chandra, Poonam; Perley, Daniel A. +9 more

We present AT2020mrf (SRGe J154754.2+443907), an extra-galactic (z = 0.1353) fast blue optical transient (FBOT) with a rise time of t g,rise = 3.7 days and a peak luminosity of M g,peak = -20.0. Its optical spectrum around peak shows a broad (v ~ 0.1c) emission feature on a blue continuum (T ~ 2 × 104 K), which b…

2022 The Astrophysical Journal
Gaia XMM-Newton 46