Publications (35)
Gaia Data Release 1: The archive visualisation service
A. Moitinho, A. Krone-Martins, H. Savietto +31
A Gaia DR2 view of the Open Cluster population in the Milky Way
T. Cantat-Gaudin, C. Jordi, A. Vallenari +10
Gaia Data Release 2: Catalogue validation
F. Arenou, X. Luri, C. Babusiaux +36
uvby-βphotometry of high-velocity and metal-poor stars XI. Ages of halo and old disk stars
W. J. Schuster, A. Moitinho, A. Marquez +2
Insights into the properties of the Local (Orion) spiral arm. NGC 2302: First results and description of the program
E. Costa, A. Moitinho, M. Radiszc +4
Evidence of tidal distortions and mass loss from the old open cluster NGC 6791
E. Dalessandro, P. Miocchi, G. Carraro +2
New catalogue of optically visible open clusters and candidates
W. S. Dias, B. S. Alessi, A. Moitinho +1
Gaia Data Release 1: Catalogue validation
F. Arenou, X. Luri, C. Babusiaux +42
A couple of recent developments in the structure of the outer disk of the Milky Way
G. Carraro, G. Perren, R. A. Vázquez +1
Gaia Data Release 2: Summary of the variability processing & analysis results
B. Holl, M. Audard, K. Nienartowicz +60
Blue Straggler Stars in Galactic Open Clusters and the effect of field star contamination
G. Carraro, R. A. Vazquez, A. Moitinho
NGC 2362: a Template for Early Stellar Evolution
A. Moitinho, J. Alves, N. Huelamo +1
Searching for unknown open clusters in the Tycho-2 catalog
B. S. Alessi, A. Moitinho, W. S. Dias
The intermediate-age open clusters Ruprecht 61, Czernik 32, NGC 2225 and NGC 2262
G. Carraro, G. Baume, R. Vazquez +2
Open clusters in the Third Galactic Quadrant. II. The intermediate age open clusters NGC 2425 and NGC 2635
A. Moitinho, G. Carraro, G. Baume +1
Open cluster kinematics with Gaia DR2
C. Soubiran, T. Cantat-Gaudin, M. Romero-Gómez +16
On the difference between nuclear and contraction ages
W. Lyra, A. Moitinho, N. van der Bliek +1
Characterising Open Clusters in the solar neighbourhood with the Tycho-Gaia Astrometric Solution
T. Cantat-Gaudin, A. Vallenari, R. Sordo +8
UBV(RI)_C photometry of the open clusters Be 15, Be 80, and NGC 2192
M. T. Tapia, W. J. Schuster, R. Michel +4
A photometric study of the old open clusters Berkeley 73, Berkeley 75 and Berkeley 25
G. Carraro, D. Geisler, A. Moitinho +2
Gaia Data Release 1: The variability processing & analysis and its application to the south ecliptic pole region
L. Eyer, N. Mowlavi, D. W. Evans +70
Milli-arcsecond astrophysics with VSI, the VLTI spectro-imager in the ELT era
F. Malbet, D. Buscher, G. Weigelt +49
Comments on the "Monoceros" affair
M. Lopez-Corredoira, A. Moitinho, S. Zaggia +5
UPMASK: unsupervised photometric membership assignment in stellar clusters
A. Krone-Martins, A. Moitinho
Solving the distance discrepancy for the open cluster NGC 2453. The planetary nebula NGC 2452 is not a cluster member
D. González-DÃaz, C. Moni Bidin, E. Silva-Villa +6
Gaia Data Release 1. Testing the parallaxes with local Cepheids and RR Lyrae stars
Gaia Collaboration, G. Clementini, L. Eyer +588
Spiral structure of the Third Galactic Quadrant and the solution to the Canis Major debate
A. Moitinho, R. A. Vazquez, G. Carraro +3
Gaia Data Release 2: Observational Hertzsprung-Russell diagrams
Gaia Collaboration, C. Babusiaux, F. van Leeuwen +450
NGC 2580 and NGC 2588: Two open clusters in the Third Galactic Quadrant
G. Baume, A. Moitinho, E. Giorgi +2
Age determination for 269 $Gaia$ DR2 Open Clusters
D. Bossini, A. Vallenari, A. Bragaglia +9
VSI: the VLTI spectro-imager
F. Malbet, D. Buscher, G. Weigelt +51
G0.253+0.016: a molecular cloud progenitor of an Arches-like cluster
Steven N. Longmore, Jill Rathborne, Nate Bastian +20
Gaia DR2 unravels incompleteness of nearby cluster population: New open clusters in the direction of Perseus
T. Cantat-Gaudin, A. Krone-Martins, N. Sedaghat +13
Gaia Data Release 1. Open cluster astrometry: performance, limitations, and future prospects
Gaia Collaboration, F. van Leeuwen, A. Vallenari +589
NGC 2401: A template of the Norma-Cygnus Arm's young population in the Third Galactic Quadrant
G. Baume, A. Moitinho, R. Vazquez +3