-
HST photometry in the wing of the SMC
We have used the Wide Field Planetary Camera 2 (WFPC2) on the Hubble Space Telescope to image a star field in the wing of the Small Magellanic Cloud (SMC), near the HII region... -
UBVRI photometry of SMC star clusters
We present age measurements for 195 star clusters in the Small Magellanic Cloud based on comparison of integrated colors measured from the Magellanic Clouds Photometric Survey... -
Magellanic Clouds Photometric Survey: the LMC
We present our catalog of U, B, V, and I stellar photometry of the central 64deg^2^ area of the Large Magellanic Cloud. Internal and external astrometric and photometric tests... -
MACHO LMC first-overtone RR Lyrae variables
Shapes of RR Lyrae light curves can be described in terms of Fourier coefficients that past research has linked with physical characteristics such as luminosity, mass, and... -
UBVR(UIT) photometry of O and OB stars in SMC
The distribution of N, the number of OB stars per association or cluster, appears to follow a universal power-law form (N)^-2^ in the local universe. We evaluate the... -
Star formation history of SMC
We present the spatially resolved star formation and chemical enrichment history of the Small Magellanic Cloud (SMC) across the entire central 4{deg}x4.5{deg} area of the main... -
Magellanic Clouds Photometric Survey: the SMC
We present our catalog of U, B, V, and I stellar photometry of the central 18{deg}^2^ area of the Small Magellanic Cloud. We combine our data with the Two Micron All Sky Survey... -
New SMC planetary nebulae
Using the ESO 2.2m telescope with the 8Kx8K mosaic CCD, we have surveyed 2.8deg^2^ (~1.6{deg}x1.7{deg}) of the Small Magellanic Cloud (SMC) to search for faint planetary nebulae... -
LMC far-ultraviolet imaging
We present an analysis of the deepest pure UV observations with the highest angular resolution ever performed, a set of 12 exposures with the Hubble Space Telescope (HST) Wide... -
Magellanic clouds ultraviolet observations
The catalog is derived from wide-field far-ultraviolet (FUV; 1300-1800{AA}) images of the Large and Small Magellanic Clouds (LMC, SMC) obtained by the Ultraviolet Imaging... -
UV Observations of the SMC
A mosaic of four UIT (Ultraviolet Imaging Telescope) far-UV (FUV) ({lambda}(eff)=1620{AA}) images, with derived stellar and H II region photometry, is presented for most of the... -
New star clusters in the Magellanic system
The Magellanic System (MS) encompasses the nearest neighbors of the Milky Way, the Large (LMC) and Small (SMC) Magellanic Clouds, and the Magellanic Bridge (MBR). This system... -
OGLE Magellanic Clouds anomalous Cepheids
We present a collection of 250 anomalous Cepheids (ACs) discovered in the OGLE-IV fields toward the Large (LMC) and Small Magellanic Cloud (SMC). The LMC sample is an extension... -
OGLE3 Magellanic Clouds High proper motion stars
We present the results of a search for High Proper Motion (HPM) stars, i.e., the ones with pm>100mas/yr, in the direction to the Magellanic Clouds. This sky area was not... -
LMC Cepheids in OGLE and MACHO data
Pulsation period of Cepheids should change as stars evolve through the instability strip. Rates of these changes found by other authors based on the decades-long O−C diagrams... -
OGLE high proper motion stars towards MC
We present a catalog of high proper motion (HPM) stars detected in the foreground of central parts of the Magellanic Clouds. The Catalog contains 2161 objects in the 4.5 square... -
OGLE Multiple Cluster Candidates in LMC
We present 100 multiple cluster candidates selected from the OGLE catalog of star clusters in the Large Magellanic Cloud. Statistical analysis shows that the significant... -
OGLE LMC star clusters
We present results of age determination based on the standard procedure of isochrone fitting for about 600 star clusters younger than about 1.2Gyr from the central parts of the... -
OGLE LMC BVI photometry
We present the BVI photometric maps of the Large Magellanic Cloud. They contain BVI photometry and astrometry of more than 7 million stars from the central parts of the LMC. The... -
OGLE LMC & SMC Cepheids VI photometry
We present Cepheids located in the close neighborhood of star clusters from the Magellanic Clouds. 204 and 132 such stars were found in the LMC and SMC, respectively. The lists...
