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19962022
most citedBVRI Light Curves for 22 Type Ia Supernovae

758 citations · 2.6k across the 42 of their papers we have counts for

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Showing 2006Show all

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astro-ph2006★ 22 cited

The extended star formation history of the star cluster NGC 2154 in the Large Magellanic Cloud

Gustavo Baume, Giovanni Carraro, Edgardo Costa +2

The color-magnitude diagram (CMD) of the intermediate-age Large Magellanic Cloud (LMC) star cluster NGC 2154 and its adjacent field, has been analyzed using Padova stellar models t…

astro-ph2006★ 20 cited

Photometry of the five marginally studied open clusters Collinder 74, Berkeley 27, Haffner 8, NGC 2509 and VdB-Hagen 4

Giovanni Carraro, Edgardo Costa

The stellar populations in the outer Galactic disk are nowadays a subject of wide interest. To contribute to a better picture of this part of the Galaxy, we have studied the nature…

astro-ph2006★ 501 cited

The Solar Neighborhood XVII: Parallax Results from the CTIOPI 0.9m Program -- Twenty New Members of the RECONS 10 Parsec Sample

Todd J. Henry, Wei-Chun Jao, John P. Subasavage +4

Astrometric measurements for 25 red dwarf systems are presented, including the first definitive trigonometric parallaxes for 20 systems within 10 pc of the Sun, the horizon of the…

astro-ph2006★ 2 cited

Old Main-Sequence Turnoff Photometry in the SMC

Noelia E. D. Noel, Carme Gallart, Edgardo Costa +1

We present ground-based {\it B} and {\it R}-band color-magnitude diagrams (CMDs) of unprecedented depth for twelve fields in the Small Magellanic Cloud (SMC). They reach the oldest…

astro-ph2006★ 28 cited

Photometry of seven overlooked open clusters in the First and Fourth Galactic Quadrants

Giovanni Carraro, Kenneth A. Janes, Edgardo Costa +1

CCD BVI photometry is presented for 7 previously unstudied star clusters projected toward the inner side of the Galaxy: Trumpler 23, Lynga 3, Collinder 307, Ruprecht 134, ESO552SC1…

astro-ph2006★ 19 cited

The Proper Motion of the Large Magellanic Cloud: A Reanalysis

Mario H. Pedreros, Edgardo Costa, Rene A. Mendez

We have determined the proper motion (PM) of the Large Magellanic Cloud (LMC) relative to four background quasi-stellar objects, combining data from two previous studies made by ou…