Search Publications

Exploring the photometric variability of ultra-cool dwarfs with TESS
DOI: 10.1093/mnras/stad3720 Bibcode: 2024MNRAS.527.8290P

Gómez Maqueo Chew, Yilen; Segura, Antígona; Jofré, Emiliano +2 more

We present a photometric characterization of 208 ultra-cool dwarfs (UCDs) with spectral types between M4 and L4, from 20-s and 2-min cadence TESS light curves. We determine rotation periods for 87 objects ($\sim 42~{{\ \rm per\ cent}}$) and identify 778 flare events in 103 UCDs ($\sim 49.5~{{\ \rm per\ cent}}$). For 777 flaring events (correspondi…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 12
Gaia uncovers difference in B and Be star binarity at small scales: evidence for mass transfer causing the Be phenomenon
DOI: 10.1093/mnras/stad3105 Bibcode: 2024MNRAS.527.3076D

Oudmaijer, René D.; Vioque, Miguel; Dodd, Jonathan M. +2 more

Be stars make up almost 20 per cent of the B star population, and are rapidly rotating stars surrounded by a disc; however the origin of this rotation remains unclear. Mass transfer within close binaries provides the leading hypothesis, with previous detections of stripped companions to Be stars supporting this. Here, we exploit the exquisite astr…

2024 Monthly Notices of the Royal Astronomical Society
Gaia Hipparcos 12
Composition and thermal properties of Ganymede's surface from JWST/NIRSpec and MIRI observations
DOI: 10.1051/0004-6361/202347326 Bibcode: 2024A&A...681A..27B

Saur, J.; Fry, P. M.; Fletcher, L. N. +21 more

Context. We present the first spectroscopic observations of Ganymede by the James Webb Space Telescope undertaken in August 2022 as part of the proposal "ERS observations of the Jovian system as a demonstration of JWST's capabilities for Solar System science".
Aims: We aimed to investigate the composition and thermal properties of the surface…

2024 Astronomy and Astrophysics
JWST 12
The Star Formation Efficiency during Reionization as Inferred from the Hubble Frontier Fields
DOI: 10.3847/1538-4357/ad06a7 Bibcode: 2024ApJ...961...50S

Lidz, Adam; Sipple, Jackson

A recent ultraviolet luminosity function (UVLF) analysis in the Hubble Frontier Fields, behind foreground lensing clusters, has helped solidify estimates of the faint-end of the z ~ 5-9 UVLF at up to 5 mag fainter than in the field. These measurements provide valuable information regarding the role of low-luminosity galaxies in reionizing the univ…

2024 The Astrophysical Journal
JWST 12
Self-interacting Dark Matter Interpretation of Crater II
DOI: 10.3847/2041-8213/ad50cd Bibcode: 2024ApJ...968L..13Z

Yang, Daneng; Yu, Hai-Bo; Zhang, Xingyu +1 more

The satellite galaxy Crater II of the Milky Way is extremely cold and exceptionally diffuse. These unusual properties are challenging to understand in the standard model of cold dark matter. We use controlled N-body simulations to investigate the formation of Crater II in self-interacting dark matter (SIDM), where dark matter particles can scatter…

2024 The Astrophysical Journal
Gaia 12
The metal-poor atmosphere of a potential sub-Neptune progenitor
DOI: 10.1038/s41550-024-02257-0 Bibcode: 2024NatAs...8..899B

Fortney, Jonathan J.; Désert, Jean-Michel; Petigura, Erik A. +12 more

Young transiting exoplanets offer a unique opportunity to characterize the atmospheres of freshly formed and evolving planets. We present the transmission spectrum of V1298 Tau b, a 23-Myr-old warm Jupiter-sized (0.91 ± 0.05 RJ, where RJ is the radius of Jupiter) planet orbiting a pre-main-sequence star. We detect a mostly cl…

2024 Nature Astronomy
eHST 12
The rate and contribution of mergers to mass assembly from NIRCam observations of galaxy candidates up to 13.3 billion years ago
DOI: 10.1093/mnras/stae2064 Bibcode: 2024MNRAS.533.4472D

Santini, Paola; Calabrò, Antonello; Castellano, Marco +8 more

We present an analysis of the galaxy merger rate in the redshift range $4.0\lt z\lt 9.0$ (i.e. about 1.5 to 0.5 Gyr after the big bang) based on visually identified galaxy mergers from morphological parameter analysis. Our data set is based on high-resolution NIRCam…

2024 Monthly Notices of the Royal Astronomical Society
eHST JWST 12
A biconical ionised gas outflow and evidence of positive feedback in NGC 7172 uncovered by MIRI/JWST
DOI: 10.1051/0004-6361/202450262 Bibcode: 2024A&A...690A.350H

Rouan, D.; Rigopoulou, D.; Gandhi, P. +35 more

We present observations of the type-2 Seyfert NGC 7172 obtained with the medium-resolution spectrometer (MRS) of the Mid-Infrared Instrument (MIRI) on board the James Webb Space Telescope (JWST). This galaxy hosts one of the lowest ionised gas mass outflow rates (Ṁout ∼ 0.005 M yr‑1) in a sample of six active gala…

2024 Astronomy and Astrophysics
JWST 12
J-PLUS: Toward a homogeneous photometric calibration using Gaia BP/RP low-resolution spectra
DOI: 10.1051/0004-6361/202346012 Bibcode: 2024A&A...683A..29L

Hernández-Monteagudo, C.; Hernán-Caballero, A.; Carrasco, J. M. +21 more


Aims: We present the photometric calibration of the 12 optical passbands for the Javalambre Photometric Local Universe Survey (J-PLUS) third data release (DR3) comprising 1642 pointings of two square degrees each.
Methods: We selected nearly 1.5 million main sequence stars with a signal-to-noise ratio larger than ten in the 12 J-PLUS pas…

2024 Astronomy and Astrophysics
Gaia 12
High Hard X-Ray Polarization in Cygnus X-1 Confined to the Intermediate Hard State: Evidence for a Variable Jet Component
DOI: 10.3847/2041-8213/ad118d Bibcode: 2024ApJ...960L...2C

Rao, A. R.; Bhalerao, Varun; Mithun, N. P. S. +7 more

Cygnus X-1, the well-known accreting black hole system, exhibits several observational features hinting at an intricate interplay between the accretion disk, its atmosphere known as the corona, and the putative relativistic jet. It has been extensively studied using all available observational methods, including using the newly available technique…

2024 The Astrophysical Journal
INTEGRAL 12