Search Publications

The Gaia-ESO survey: Age-chemical-clock relations spatially resolved in the Galactic disc
DOI: 10.1051/0004-6361/202142937 Bibcode: 2022A&A...660A.135V

Baratella, M.; Gilmore, G.; Montes, D. +33 more

Context. The last decade has seen a revolution in our knowledge of the Galaxy thanks to the Gaia and asteroseismic space missions and the ground-based spectroscopic surveys.
Aims: To complete this picture, it is necessary to map the ages of its stellar populations. During recent years, the dependence on time of abundance ratios involving slow…

2022 Astronomy and Astrophysics
Gaia 40
HSC-XXL: Baryon budget of the 136 XXL groups and clusters
DOI: 10.1093/pasj/psab115 Bibcode: 2022PASJ...74..175A

Oguri, Masamune; Valtchanov, Ivan; Umetsu, Keiichi +17 more

We present our determination of the baryon budget for an X-ray-selected XXL sample of 136 galaxy groups and clusters spanning nearly two orders of magnitude in mass (M500 ~ 1013-1015 M) and the redshift range 0 ≲ z ≲ 1. Our joint analysis is based on the combination of Hyper Suprime-Cam Subaru Strategic…

2022 Publications of the Astronomical Society of Japan
XMM-Newton 40
GIARPS High-resolution Observations of T Tauri stars (GHOsT). IV. Accretion properties of the Taurus-Auriga young association
DOI: 10.1051/0004-6361/202244042 Bibcode: 2022A&A...667A.124G

Munari, U.; Alcalá, J. M.; Manara, C. F. +9 more


Aims: In the framework of the GIARPS High-resolution Observations of T Tauri stars (GHOsT) project, we study the accretion properties of 37 classical T Tauri stars of the Taurus-Auriga star-forming region (SFR) with the aim of characterizing their relation with the properties of the central star, with jets and disk winds, and with the global …

2022 Astronomy and Astrophysics
Gaia 39
Classical Cepheid period-Wesenheit-metallicity relation in the Gaia bands
DOI: 10.1051/0004-6361/202142649 Bibcode: 2022A&A...659A.167R

Clementini, G.; Ripepi, V.; Molinaro, R. +7 more

Context. Classical Cepheids (DCEPs) represent a fundamental tool to calibrate the extragalactic distance scale. However, they are also powerful stellar population tracers in the context of Galactic studies. The forthcoming Data Release 3 of the Gaia mission will allow us to study, with unprecedented detail, the structure, the dynamics, and the che…

2022 Astronomy and Astrophysics
Gaia 39
First discoveries and localizations of Fast Radio Bursts with MeerTRAP: real-time, commensal MeerKAT survey
DOI: 10.1093/mnras/stac1450 Bibcode: 2022MNRAS.514.1961R

Prochaska, J. Xavier; Kramer, M.; Tejos, N. +24 more

We report on the discovery and localization of fast radio bursts (FRBs) from the MeerTRAP project, a commensal fast radio transient-detection programme at MeerKAT in South Africa. Our hybrid approach combines a coherent search with an average field-of-view (FoV) of 0.4 $\rm deg^{2}$ with an incoherent search utilizing a FoV of ~1.27 $\rm deg^{2}$ …

2022 Monthly Notices of the Royal Astronomical Society
Gaia 39
Primordial black holes and gravitational waves in hybrid inflation with chaotic potentials
DOI: 10.1016/j.nuclphysb.2022.115968 Bibcode: 2022NuPhB.98415968A

Ahmed, Waqas; Junaid, M.; Zubair, Umer

We study the formation of primordial black hole (PBH) dark matter and the generation of scalar induced secondary gravitational waves (SIGWs) in a non-supersymmetric model of hybrid inflation with chaotic (polynomial-like) potential, including one-loop radiative corrections. A radiatively corrected version of these models is entirely consistent wit…

2022 Nuclear Physics B
INTEGRAL 39
Strong constraints on primordial black hole dark matter from 16 years of INTEGRAL/SPI observations
DOI: 10.1103/PhysRevD.106.023030 Bibcode: 2022PhRvD.106b3030B

Calore, F.; Serpico, P. D.; Siegert, T. +2 more

We present a new analysis of the diffuse soft γ -ray emission toward the inner Galaxy as measured by the spectrometer aboard the INTEGRAL satellite (SPI) with 16 years of data taking. The analysis implements a spatial template fit of SPI data and an improved instrumental background model. We characterize the contribution of primordial black holes …

2022 Physical Review D
INTEGRAL 39
Water and an Escaping Helium Tail Detected in the Hazy and Methane-depleted Atmosphere of HAT-P-18b from JWST NIRISS/SOSS
DOI: 10.3847/2041-8213/ac9977 Bibcode: 2022ApJ...940L..35F

Deming, Drake; Sing, David K.; Fu, Guangwei +11 more

JWST is here. The early release observation (ERO) program provides us with the first look at the scientific data and the spectral capabilities. One of the targets from the ERO is HAT-P-18b, an inflated Saturn-mass planet with an equilibrium temperature of ~850 K. We present the NIRISS/SOSS transmission spectrum of HAT-P-18b from 0.6 to 2.8 µ…

2022 The Astrophysical Journal
eHST JWST 39
Comprehensive catalogue of the overall best distances and properties of 402 galactic novae
DOI: 10.1093/mnras/stac2900 Bibcode: 2022MNRAS.517.6150S

Schaefer, Bradley E.

I derive the overall best distances for all 402 known Galactic novae, and I collect their many properties. The centrepiece is the 74 novae with accurate parallaxes from the new Gaia data release. For the needed priors, I have collected 171 distances based on old methods (including expansion parallaxes and extinction distances). Further, I have col…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 39
Cosmological Fast Optical Transients with the Zwicky Transient Facility: A Search for Dirty Fireballs
DOI: 10.3847/1538-4357/ac8bd0 Bibcode: 2022ApJ...938...85H

Kulkarni, S. R.; Filippenko, Alexei V.; Riddle, Reed +35 more

Dirty fireballs are a hypothesized class of relativistic massive-star explosions with an initial Lorentz factor Γinit below the Γinit ~ 100 required to produce a long-duration gamma-ray burst (LGRB), but which could still produce optical emission resembling LGRB afterglows. Here we present the results of a search for on-axis …

2022 The Astrophysical Journal
INTEGRAL 39