Search Publications

The Peculiar Short-duration GRB 200826A and Its Supernova
DOI: 10.3847/1538-4357/ac60a2 Bibcode: 2022ApJ...932....1R

Covino, S.; D'Avanzo, P.; Della Valle, M. +31 more

Gamma-ray bursts (GRBs) are classified into long and short events. Long GRBs (LGRBs) are associated with the end states of very massive stars, while short GRBs (SGRBs) are linked to the merger of compact objects. GRB 200826A was a peculiar event, because by definition it was an SGRB, with a rest-frame duration of ~0.5 s. However, this event was en…

2022 The Astrophysical Journal
Gaia 80
Constraining the evolution of cataclysmic variables via the masses and accretion rates of their underlying white dwarfs
DOI: 10.1093/mnras/stab3449 Bibcode: 2022MNRAS.510.6110P

Reichart, D. E.; Knigge, C.; Gänsicke, B. T. +28 more

We report on the masses (MWD), effective temperatures ($\rm{T_\mathrm{eff}}$), and secular mean accretion rates ($\langle \dot{M} \rangle$) of 43 cataclysmic variable (CV) white dwarfs, 42 of which were obtained from the combined analysis of their Hubble Space Telescope ultraviolet data with the parallaxes provided by the Early Third Da…

2022 Monthly Notices of the Royal Astronomical Society
Gaia eHST 79
High star cluster formation efficiency in the strongly lensed Sunburst Lyman-continuum galaxy at z = 2.37
DOI: 10.1051/0004-6361/202141590 Bibcode: 2022A&A...659A...2V

Zanella, A.; Brammer, G.; Castellano, M. +16 more

We investigate the strongly lensed (µ ≃ ×10 − 100) Lyman continuum (LyC) galaxy, dubbed Sunburst, at z = 2.37, taking advantage of a new accurate model of the lens. A characterization of the intrinsic (delensed) properties of the system yields a size of ≃3 sq. kpc, a luminosity of MUV = −20.3, and a stellar mass of M ≃ 109

2022 Astronomy and Astrophysics
Gaia eHST 79
A very luminous jet from the disruption of a star by a massive black hole
DOI: 10.1038/s41586-022-05465-8 Bibcode: 2022Natur.612..430A

Kulkarni, S. R.; Kilpatrick, Charles D.; Izzo, Luca +78 more

Tidal disruption events (TDEs) are bursts of electromagnetic energy that are released when supermassive black holes at the centres of galaxies violently disrupt a star that passes too close1. TDEs provide a window through which to study accretion onto supermassive black holes; in some rare cases, this accretion leads to launching of a r…

2022 Nature
eHST 79
A dusty compact object bridging galaxies and quasars at cosmic dawn
DOI: 10.1038/s41586-022-04454-1 Bibcode: 2022Natur.604..261F

Marques-Chaves, R.; Magdis, G. E.; Colina, L. +18 more

Understanding how super-massive black holes form and grow in the early Universe has become a major challenge1,2 since it was discovered that luminous quasars existed only 700 million years after the Big Bang3,4. Simulations indicate an evolutionary sequence of dust-reddened quasars emerging from heavily dust-obscured starburs…

2022 Nature
Gaia Herschel eHST 78
ARIADNE: measuring accurate and precise stellar parameters through SED fitting
DOI: 10.1093/mnras/stac956 Bibcode: 2022MNRAS.513.2719V

Jenkins, James S.; Vines, Jose I.

Accurately measuring stellar parameters is a key goal to increase our understanding of the observable Universe. However, current methods are limited by many factors, in particular, the biases and physical assumptions that are the basis for the underlying evolutionary or atmospheric models, those that these methods rely upon. Here, we introduce our…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 78
Three-dimensional extinction maps: Inverting inter-calibrated extinction catalogues
DOI: 10.1051/0004-6361/202243319 Bibcode: 2022A&A...664A.174V

Lallement, R.; Cox, N. L. J.; Vergely, J. L.

Context. Three-dimensional (3D) maps of the extinction density in the Milky Way can be built through the inversion of large catalogues of distance-extinction pairs for individual target stars. Considerable progress is currently achieved in this field through the Gaia mission. Available catalogues are based on various types of photometric or spectr…

2022 Astronomy and Astrophysics
Gaia 78
The three-year shear catalog of the Subaru Hyper Suprime-Cam SSP Survey
DOI: 10.1093/pasj/psac006 Bibcode: 2022PASJ...74..421L

Strauss, Michael A.; Takita, Satoshi; Miyatake, Hironao +15 more

We present the galaxy shear catalog that will be used for the three-year cosmological weak gravitational lensing analyses using data from the Wide layer of the Hyper Suprime-Cam (HSC) Subaru Strategic Program (SSP) Survey. The galaxy shapes are measured from the i-band imaging data acquired from 2014 to 2019 and calibrated with image simulations t…

2022 Publications of the Astronomical Society of Japan
Gaia XMM-Newton 77
Has JWST Already Falsified Dark-matter-driven Galaxy Formation?
DOI: 10.3847/2041-8213/ac9a50 Bibcode: 2022ApJ...939L..31H

Kroupa, Pavel; Haslbauer, Moritz; Haghi, Hosein +1 more

The James Webb Space Telescope (JWST) discovered several luminous high-redshift galaxy candidates with stellar masses of M * ≳ 109 M at photometric redshifts z phot ≳ 10, which allows to constrain galaxy and structure formation models. For example, Adams et al. identified the candidate ID 1514 with ${\…

2022 The Astrophysical Journal
JWST 77
CORINOS. I. JWST/MIRI Spectroscopy and Imaging of a Class 0 Protostar IRAS 15398–3359
DOI: 10.3847/2041-8213/aca289 Bibcode: 2022ApJ...941L..13Y

Lee, Jeong-Eun; Cleeves, L. Ilsedore; Bergner, Jennifer B. +13 more

The origin of complex organic molecules (COMs) in young Class 0 protostars has been one of the major questions in astrochemistry and star formation. While COMs are thought to form on icy dust grains via gas-grain chemistry, observational constraints on their formation pathways have been limited to gas-phase detection. Sensitive mid-infrared spectr…

2022 The Astrophysical Journal
JWST 76