papers
Publications (13)
astro-ph.SR2015
New Constraints on the Star Formation History of the Star Cluster NGC 1856
Matteo Correnti, Paul Goudfrooij, Thomas H. Puzia +1
astro-ph.GA2017
Extended Main Sequence Turnoffs in Intermediate-Age Star Clusters: Stellar Rotation diminishes, but does not eliminate, Age Spreads
Paul Goudfrooij, Leo Girardi, Matteo Correnti
astro-ph.SR2018
The Minimum Mass of Rotating Main Sequence Stars and its Impact on the Nature of Extended Main Sequence Turnoffs in Intermediate-Age Star Clusters in the Magellanic Clouds
Paul Goudfrooij, Leo Girardi, Andrea Bellini +3
astro-ph.SR2014
New Clues to the Cause of Extended Main Sequence Turn-Offs in Intermediate-Age Star Clusters in the Magellanic Clouds
Matteo Correnti, Paul Goudfrooij, Jason S. Kalirai +3
astro-ph.GA2012
Does the Sagittarius Stream constrain the Milky Way halo to be triaxial?
Rodrigo Ibata, Geraint F. Lewis, Nicolas F. Martin +2
astro-ph.SR2015
On the Interpretation of Sub-Giant Branch Morphologies of Intermediate-Age Star Clusters with Extended Main Sequence Turnoffs
Paul Goudfrooij, Leo Girardi, Philip Rosenfield +4
astro-ph.GA2012
Star Formation in the Starburst Cluster in NGC 3603
Matteo Correnti, Francesco Paresce, Rossella Aversa +7
astro-ph.SR2014
Extended Main Sequence Turnoffs in Intermediate-Age Star Clusters: A Correlation Between Turnoff Width and Early Escape Velocity
Paul Goudfrooij, Leo Girardi, Vera Kozhurina-Platais +9
astro-ph.SR2014
Herschel Far IR observations of the giant HII region NGC 3603
Alessandra Di Cecco, Fabiana Faustini, Francesco Paresce +2
astro-ph.SR2018
The Age of the Old Metal-Poor Globular Cluster NGC6397 Using WFC3/IR Photometry
Matteo Correnti, Mario Gennaro, Jason S. Kalirai +2
astro-ph.SR2016
Dissecting the Extended Main Sequence Turn-off of the Young Star Cluster NGC1850
Matteo Correnti, Paul Goudfrooij, Andrea Bellini +2
astro-ph.SR2016
Constraining Globular Cluster Age Uncertainties Using the IR Color-Magnitude Diagram
Matteo Correnti, Mario Gennaro, Jason S. Kalirai +2
astro-ph.GA2010
Is Palomar 1 really associated with the Canis Major overdensity?
Ivo Saviane, Lorenzo Monaco, Matteo Correnti +2