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Low-mass pre-main-sequence stars in the large magellanic cloud. III. Accretion rates from hubble space telescope WFPC2 observationsROMANIELLO, M; ROBBERTO, M; PANAGIA, N et al.The Astrophysical journal. 2004, Vol 608, Num 1, pp 220-228, issn 0004-637X, 9 p., 1Article

Evidence for a yellow-supergiant phase of AG CarinaeROBBERTO, M; FERRARI, A; NOTA, A et al.Astronomy and astrophysics (Berlin. Print). 1993, Vol 269, Num 1-2, pp 330-342, issn 0004-6361Article

Applications of DMDs for Astrophysical ResearchROBBERTO, M; CIMATTI, A; JACOBSEN, A et al.Proceedings of SPIE, the International Society for Optical Engineering. 2009, Vol 7210, issn 0277-786X, isbn 978-0-8194-7456-8, 72100A.1-72100A.10Conference Paper

EVIDENCE FOR A PHOTOEVAPORATED CIRCUMBINARY DISK IN ORIONROBBERTO, M; RICCI, L; DA RIO, N et al.The Astrophysical journal. 2008, Vol 687, Num 2, issn 0004-637X, L83-L86, 2Article

DMD Multi-Object Spectroscopy in Space: the EUCLID StudySPANO, P; ZAMKOTSIAN, F; MARTIN, L et al.Proceedings of SPIE, the International Society for Optical Engineering. 2009, Vol 7436, issn 0277-786X, isbn 978-0-8194-7726-2 0-8194-7726-5, 1Vol, 74360O.1-74360O.10Conference Paper

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Empirical near-infrared colors for low-mass stars and brown dwarfs in the Orion Nebula Cluster: An empirical near-infrared isochrone at ∼1 MyrSCANDARIATO, G; DA RIO, N; ROBBERTO, M et al.Astronomy and astrophysics (Berlin. Print). 2012, Vol 545, issn 0004-6361, A19.1-A19.13, 1Article

THE INITIAL MASS FUNCTION OF THE ORION NEBULA CLUSTER ACROSS THE H-BURNING LIMITDA RIO, N; ROBBERTO, M; HILLENBRAND, L. A et al.The Astrophysical journal. 2012, Vol 748, Num 1, issn 0004-637X, 14.1-14.15, 1Article

The low-mass initial mass function in the Orion nebula cluster based on HST/NICMOS III imagingANDERSEN, M; MEYER, M. R; ROBBERTO, M et al.Astronomy and astrophysics (Berlin. Print). 2011, Vol 534, issn 0004-6361, A10.1-A10.8, 1Article

The E-NIS instrument on-board the ESA Euclid Dark Energy Mission: a general view after positive conclusion of the assesment phaseVALENZIANO, L; ZERBI, F. M; DE ROSA, A et al.Proceedings of SPIE, the International Society for Optical Engineering. 2010, Vol 7731, issn 0277-786X, isbn 978-0-8194-8221-1, 77311L.1-77311L.11, 3Conference Paper

X-RAY PROPERTIES OF PROTOSTARS IN THE ORION NEBULAPRISINZANO, L; MICELA, G; WOLK, S et al.The Astrophysical journal. 2008, Vol 677, Num 1, pp 401-424, issn 0004-637X, 24 p., 1Article

The enigma of GCIRS 3 : Constraining the properties of the mid-infrared reference star of the central parsec of the Milky Way with optical long-baseline interferometryPOTT, J.-U; ECKART, A; GLINDEMANN, A et al.Astronomy and astrophysics (Berlin. Print). 2008, Vol 480, Num 1, pp 115-131, issn 0004-6361, 17 p.Article

Evidence from infrared observations of circumstellar matter around chromospherically active binariesSCALTRITI, F; BUSSO, M; FERRARI-TONIOLO, M et al.Monthly Notices of the Royal Astronomical Society. 1993, Vol 264, Num 1, pp 5-15, issn 0035-8711Article

A search for non-stellar contributions to the optical and near-IR flux of RS CVn binaries. I: The cases of TY Pyx, UV Psc, RU CncBUSSO, M; SCALTRITI, F; PERSI, P et al.Astronomy and astrophysics (Berlin. Print). 1987, Vol 183, Num 1, pp 83-90, issn 0004-6361Article