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20002026
most citedGaia Early Data Release 3: The astrometric solution

1.2k citations · 8.4k across the 156 of their papers we have counts for

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16 papers · 1 filter

astro-ph.GA2020★ 35 cited

The VMC Survey -- XL. Three-dimensional structure of the Small Magellanic Cloud as derived from red clump stars

B. L. Tatton, J. Th. van Loon, M. -R. L. Cioni +12

Galaxy interactions distort the distribution of baryonic matter and can affect star formation. The nearby Magellanic Clouds are a prime example of an ongoing galaxy interaction pro…

astro-ph.IM2020★ 1.2k cited

Gaia Early Data Release 3: The astrometric solution

L. Lindegren, S. A. Klioner, J. Hernández +94

Gaia Early Data Release 3 (Gaia EDR3) contains results for 1.812 billion sources in the magnitude range G = 3 to 21 based on observations collected by the European Space Agency Gai…

astro-ph.SR2020★ 340 cited

Gaia Early Data Release 3: The Gaia Catalogue of Nearby Stars

Gaia Collaboration, R. L. Smart, L. M. Sarro +420

We produce a clean and well-characterised catalogue of objects within 100\,pc of the Sun from the \G\ Early Data Release 3. We characterise the catalogue through comparisons to the…

astro-ph.GA2020★ 39 cited

The Second Data Release of the Survey of the MAgellanic Stellar History (SMASH)

David L. Nidever, Knut Olsen, Yumi Choi +32

The Large and Small Magellanic Clouds (LMC and SMC) are the largest satellite galaxies of the Milky Way and close enough to allow for a detailed exploration of their structure and…

astro-ph.GA2020★ 33 cited

Gaia view of a stellar sub-structure in front of the Small Magellanic Cloud

Abinaya O. Omkumar, Smitha Subramanian, Florian Niederhofer +6

Recent observational studies identified a foreground stellar sub-structure traced by red clump (RC) stars (~ 12 kpc in front of the main body) in the eastern regions of the Small M…

astro-ph.GA2020★ 15 cited

The intrinsic reddening of the Magellanic Clouds as traced by background galaxies -- II. The Small Magellanic Cloud

Cameron P. M. Bell, Maria-Rosa L. Cioni, A. H. Wright +23

We present a map of the total intrinsic reddening across ~34 deg of the Small Magellanic Cloud (SMC) derived using optical () and near-infrared (IR; …

astro-ph.GA2020

MOONS Surveys of the Milky Way and its Satellites

O. A. Gonzalez, A. Mucciarelli, L. Origlia +37

The study of resolved stellar populations in the Milky Way and other Local Group galaxies can provide us with a fossil record of their chemo-dynamical and star-formation histories…

astro-ph.SR2020★ 175 cited

Constraining the thermally pulsing asymptotic giant branch phase with resolved stellar populations in the Large Magellanic Cloud

Giada Pastorelli, Paola Marigo, Léo Girardi +18

Reliable models of the thermally pulsing asymptotic giant branch (TP-AGB) phase are of critical importance across astrophysics, including our interpretation of the spectral energy…

astro-ph.GA2020

SMASHing the low surface brightness SMC

Pol Massana, Noelia E. D. Noël, David L. Nidever +22

The periphery of the Small Magellanic Cloud (SMC) can unlock important information regarding galaxy formation and evolution in interacting systems. Here, we present a detailed stud…

astro-ph.GA2020★ 26 cited

The VMC survey -- XXXIX: Mapping metallicity trends in the Small Magellanic Cloud using near-infrared passbands

Samyaday Choudhury, Richard de Grijs, Stefano Rubele +7

We have derived high spatial resolution metallicity maps covering 42 deg across the Small Magellanic Cloud (SMC) in an attempt to understand its metallicity distribution…

astro-ph.GA2020★ 39 cited

The Large Magellanic Cloud stellar content with SMASH: I. Assessing the stability of the Magellanic spiral arms

T. Ruiz-Lara, C. Gallart, M. Monelli +23

The Large Magellanic Cloud (LMC) is the closest and most studied example of an irregular galaxy. Among its principal defining morphological features, its off-centred bar and single…

astro-ph.GA2020★ 33 cited

The VMC survey -- XXXVIII. Proper motion of the Magellanic Bridge

Thomas Schmidt, Maria-Rosa L. Cioni, Florian Niederhofer +14

The Magellanic Clouds are a nearby pair of interacting dwarf galaxies and satellites of the Milky Way. Studying their kinematic properties is essential to understanding their origi…

astro-ph.SR2020★ 19 cited

The VMC Survey -- XXXVII. Pulsation periods of dust enshrouded AGB stars in the Magellanic Clouds

M. A. T. Groenewegen, A. Nanni, M. -R. L. Cioni +9

(abridged)Variability is a key property of stars on the asymptotic giant branch (AGB). Their pulsation period is related to the luminosity and mass-loss rate of the star. The long-…

astro-ph.SR2020★ 6 cited

The VMC survey -- XXXVI. Young stellar variability in the Large Magellanic Cloud

Viktor Zivkov, Joana M. Oliveira, Monika G. Petr-Gotzens +11

Studies of young stellar objects (YSOs) in the Galaxy have found that a significant fraction exhibit photometric variability. However, no systematic investigation has been conducte…

astro-ph.SR2020

VMC J021140.41-735320.4 -- an extremely red L dwarf candidate member of the AB Doradus young moving group

Ralf-Dieter Scholz, Lydia Pangsy, Maria-Rosa L. Cioni

We report the discovery of VMC J021140.41-735320.4, a faint ( mag) and extremely red ( mag, mag, mag) high proper motion object in front…

astro-ph.IM2020★ 11 cited

Probabilistic fibre-to-target assignment algorithm for multi-object spectroscopic surveys

E. Tempel, P. Norberg, T. Tuvikene +22

Context. Several new multi-object spectrographs are currently planned or under construction that are capable of observing thousands of Galactic and extragalactic objects simultaneo…