activity
20182025
most citedGaia Data Release 3: Analysis of RVS spectra using the General Stellar Parametriser from spectroscopy

252 citations · 1.4k across the 35 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

23 papers · 1 filter

astro-ph.GA2025★ 1 cited

The Nearby Evolved Stars Survey III: First data release of JCMT CO-line observations

S. H. J. Wallström, P. Scicluna, S. Srinivasan +37

Low- to intermediate-mass (0.88 M) evolved stars contribute significantly to the chemical enrichment of the interstellar medium in the local Universe, making accur…

astro-ph.GA2025

Gaussian Process Methods for Very Large Astrometric Data Sets

Timothy Hapitas, Lawrence M. Widrow, Thavisha E. Dharmawardena +1

We present a novel non-parametric method for inferring smooth models of the mean velocity field and velocity dispersion tensor of the Milky Way from astrometric data. Our approach…

astro-ph.GA2025★ 4 cited

Investigating silicate, carbon, and water in the diffuse interstellar medium: the first shots from WISCI

S. T. Zeegers, Jonathan P. Marshall, Karl D. Gordon +33

The dusty interstellar medium (ISM) of the Milky Way is distributed in a complex, cloudy structure. It is fundamental to the radiation balance within the Milky Way, provides a reac…

astro-ph.GA2025

Searching for star formation towards the Eos molecular cloud

Suryansh Saxena, Thomas J. Haworth, Blakesley Burkhart +5

The Eos cloud, recently discovered in the far ultraviolet via H fluorescence, is one of the nearest known dark molecular clouds to the Sun, with a distance spanning from $\sim9…

astro-ph.GA2025

A Nearby Dark Molecular Cloud in the Local Bubble Revealed via H Fluorescence

Blakesley Burkhart, Thavisha E. Dharmawardena, Shmuel Bialy +20

A longstanding prediction in interstellar theory posits that significant quantities of molecular gas, crucial for star formation, may be undetected due to being ``dark" in commonly…

astro-ph.GA2025

Magnetic fields in the Eos Cloud: dynamically important fields in the interface between atomic and molecular gas

Janik Karoly, Kate Pattle, Blakesley Burkhart +3

The recently-discovered Eos molecular cloud, is a CO-dark, low-density cloud located at a distance of approximately 94 pc from the Sun which does not appear to have formed stars at…

astro-ph.GA2024

All-sky three-dimensional dust density and extinction Maps of the Milky Way out to 2.8 kpc

T. E. Dharmawardena, C. A. L. Bailer-Jones, M. Fouesneau +5

Three-dimensional dust density maps are crucial for understanding the structure of the interstellar medium of the Milky Way and the processes that shape it. However, constructing t…

astro-ph.GA2024★ 129 cited

Discovery of a dormant 33 solar-mass black hole in pre-release Gaia astrometry

Gaia Collaboration, P. Panuzzo, T. Mazeh +412

Gravitational waves from black-hole merging events have revealed a population of extra-galactic BHs residing in short-period binaries with masses that are higher than expected base…

astro-ph.GA2023

Gaia Focused Product Release: Spatial distribution of two diffuse interstellar bands

Gaia Collaboration, M. Schultheis, H. Zhao +15

Diffuse interstellar bands (DIBs) are absorption features seen in optical and infrared spectra of stars that are probably caused by large and complex molecules in the ISM. Here we…

astro-ph.GA2023★ 7 cited

Gaia Focused Product Release: A catalogue of sources around quasars to search for strongly lensed quasars

Gaia Collaboration, A. Krone-Martins, C. Ducourant +398

Context. Strongly lensed quasars are fundamental sources for cosmology. The Gaia space mission covers the entire sky with the unprecedented resolution of " in the optical, ma…

astro-ph.GA2022★ 18 cited

The three-dimensional structure of Galactic molecular cloud complexes out to 2.5 kpc

T. E. Dharmawardena, C. A. L. Bailer-Jones, M. Fouesneau +5

Knowledge of the three-dimensional structure of Galactic molecular clouds is important for understanding how clouds are affected by processes such as turbulence and magnetic fields…

astro-ph.GA2022★ 83 cited

Gaia DR3: Apsis III -- Non-stellar content and source classification

L. Delchambre, C. A. L. Bailer-Jones, I. Bellas-Velidis +78

Context. As part of the third Gaia data release, we present the contributions of the non-stellar and classification modules from the eighth coordination unit (CU8) of the Data Proc…

astro-ph.GA2022★ 223 cited

Gaia Data Release 3: Astrophysical parameters inference system (Apsis) I -- methods and content overview

O. L. Creevey, R. Sordo, F. Pailler +86

Gaia Data Release 3 contains a wealth of new data products for the community. Astrophysical parameters are a major component of this release. They were produced by the Astrophysica…

astro-ph.GA2022★ 252 cited

Gaia Data Release 3: Analysis of RVS spectra using the General Stellar Parametriser from spectroscopy

A. Recio-Blanco, P. de Laverny, P. A. Palicio +77

The chemo-physical parametrisation of stellar spectra is essential for understanding the nature and evolution of stars and of Galactic stellar populations. Gaia DR3 contains the pa…

astro-ph.GA2022★ 26 cited

Gaia Data Release 3: Exploring and mapping the diffuse interstellar band at 862 nm

Gaia collaboration, M. Schultheis, H. Zhao +12

Diffuse interstellar bands (DIBs) are common interstellar absorption features in spectroscopic observations but their origins remain unclear. DIBs play an important role in the lif…

astro-ph.GA2022★ 4 cited

Solid confirmation of the broad DIB around 864.8 nm using stacked Gaia-RVS spectra

H. Zhao, M. Schultheis, T. Zwitter +26

Studies of the correlation between different diffuse interstellar bands (DIBs) are important for exploring their origins. However, the Gaia-RVS spectral window between 846 and 870…

astro-ph.GA2022★ 27 cited

Astrophysical Parameters from Gaia DR2, 2MASS & AllWISE

M. Fouesneau, R. Andrae, T. Dharmawardena +3

Stellar physical and dynamical properties are essential knowledge to understanding the structure, formation, and evolution of our Galaxy. We produced an all-sky uniformly derived c…

astro-ph.GA2021★ 29 cited

Three-dimensional dust density structure of the Orion, Cygnus X,Taurus, and Perseus star-forming regions

T. E. Dharmawardena, C. A. L. Bailer-Jones, M. Fouesneau +1

Interstellar dust affects astronomical observations through absorption and reddening, yet this extinction is also a powerful tool for studying interstellar matter in galaxies. 3D r…

astro-ph.GA2021

The Nearby Evolved Stars Survey II: Constructing a volume-limited sample and first results from the James Clerk Maxwell Telescope

P. Scicluna, F. Kemper, I. McDonald +89

The Nearby Evolved Stars Survey (NESS) is a volume-complete sample of 850 Galactic evolved stars within 3\,kpc at (sub-)mm wavelengths, observed in the CO (21) and…

astro-ph.GA2020★ 8 cited

H fluxes and extinction distances for planetary nebulae in the IPHAS survey of the Northern Galactic Plane

Thavisha E. Dharmawardena, M. J. Barlow, J. E. Drew +7

We report H filter photometry for 197 northern hemisphere planetary nebulae (PNe) obtained using imaging data from the IPHAS survey. H+[N II] fluxes were measured for 46 conf…

astro-ph.GA2020★ 13 cited

Systematic errors in dust mass determinations: Insights from laboratory opacity measurements

Lapo Fanciullo, Francisca Kemper, Peter Scicluna +2

The thermal emission of dust is one of the most important tracers of the interstellar medium: multi-wavelength photometry in the far-infrared (FIR) and submillimeter (submm) can be…

astro-ph.GA2019★ 19 cited

JINGLE, a JCMT legacy survey of dust and gas for galaxy evolution studies: II. SCUBA-2 850 μm data reduction and dust flux density catalogues

Matthew W. L. Smith, Christopher J. R. Clark, Ilse De Looze +33

We present the SCUBA-2 850 component of JINGLE, the new JCMT large survey for dust and gas in nearby galaxies, which with 193 galaxies is the largest targeted survey of nearby…

astro-ph.GA2018★ 46 cited

JINGLE, a JCMT legacy survey of dust and gas for galaxy evolution studies: I. Survey overview and first results

Amelie Saintonge, Christine D. Wilson, Ting Xiao +88

JINGLE is a new JCMT legacy survey designed to systematically study the cold interstellar medium of galaxies in the local Universe. As part of the survey we perform 850um continuum…