Add to ORKGWe present deep ground-based {\it B} and {\it R} observations of 12 fields in the Small Magellanic Cloud (SMC). The resulting color-magnitude diagrams (CMDs) reach the oldest main-sequence (MS) turnoff at M$_{R
We use the SMASH survey to obtain unprecedented deep photometry reaching downto the oldest main sequ...
Colour–magnitude diagrams are presented for the first time for L32, L38, K28 (L43), K44 (L68) and L1...
Context. The supergiant ionized shell SMC-SGS 1 (DEM 167), which is located in the outer Wing of the...
Publicación ISIWe present ground-based B-and R-band color-magnitude diagrams (CMDs) reaching the old...
We present a progress report of a project to study the quantitative star formation history (SFH) in ...
We introduce the SMC in space and time, a large coordinated space and ground-based program to study ...
We use the SMASH survey to obtain unprecedented deep photometry reaching down to the oldest main-seq...
We present CCD photometry in the Washington C and T1 filters for six star clusters (B 34, NGC 256, N...
We present deep color-magnitud diagrams (CMDs) reaching the oldest main-sequence turnoffs for 12 fie...
We present the spatially-resolved star formation and chemical enrichment history of the Small Magell...
We recover the spatially resolved star formation history across the entire main body and Wing of the...
We recover the spatially resolved star formation history across the entire main body and Wing of the...
The periphery of the Small Magellanic Cloud (SMC) can unlock important information regarding galaxy ...
Deep HST/ACS photometry of the young cluster NGC 602, located in the remote low density "wing" of th...
We present the results of the age and metallicity estimates for the unprecedented data base of some ...
We use the SMASH survey to obtain unprecedented deep photometry reaching downto the oldest main sequ...
Colour–magnitude diagrams are presented for the first time for L32, L38, K28 (L43), K44 (L68) and L1...
Context. The supergiant ionized shell SMC-SGS 1 (DEM 167), which is located in the outer Wing of the...
Publicación ISIWe present ground-based B-and R-band color-magnitude diagrams (CMDs) reaching the old...
We present a progress report of a project to study the quantitative star formation history (SFH) in ...
We introduce the SMC in space and time, a large coordinated space and ground-based program to study ...
We use the SMASH survey to obtain unprecedented deep photometry reaching down to the oldest main-seq...
We present CCD photometry in the Washington C and T1 filters for six star clusters (B 34, NGC 256, N...
We present deep color-magnitud diagrams (CMDs) reaching the oldest main-sequence turnoffs for 12 fie...
We present the spatially-resolved star formation and chemical enrichment history of the Small Magell...
We recover the spatially resolved star formation history across the entire main body and Wing of the...
We recover the spatially resolved star formation history across the entire main body and Wing of the...
The periphery of the Small Magellanic Cloud (SMC) can unlock important information regarding galaxy ...
Deep HST/ACS photometry of the young cluster NGC 602, located in the remote low density "wing" of th...
We present the results of the age and metallicity estimates for the unprecedented data base of some ...
We use the SMASH survey to obtain unprecedented deep photometry reaching downto the oldest main sequ...
Colour–magnitude diagrams are presented for the first time for L32, L38, K28 (L43), K44 (L68) and L1...
Context. The supergiant ionized shell SMC-SGS 1 (DEM 167), which is located in the outer Wing of the...