VISCACHA papers

  1. Ferreira et al., 2025: The VISCACHA Survey – XII. SL 2: Age gap cluster in the southwestern Large Magellanic Cloud
  2. Ferreira et al., 2024: The VISCACHA Survey – XI. Benchmarking SIESTA: a new synthetic CMD fitting code
  3. Gardin et al., 2024: The VISCACHA survey - X. A fast method to build completeness maps for Magellanic Clouds star clusters
  4. Parisi et al., 2024: The VISCACHA survey - IX. The SMC southern bridge in 8D
  5. Saroon et al., 2023: The VISCACHA survey. VIII. Chemical evolution history of the Small Magellanic Cloud west halo clusters
  6. Oliveira et al., 2023: The VISCACHA survey - VII. Assembly history of the Magellanic Bridge and SMC Wing from star clusters
  7. Rodriguez et al., 2023: The VISCACHA survey - VI. Dimensional study of the structure of 82 star clusters in the Magellanic Clouds
  8. Bica et al., 2022: The VISCACHA survey - V. Rejuvenating three faint SMC clusters
  9. Dias et al., 2022b: The VISCACHA survey - IV. The SMC West Halo in 8D
  10. Dias et al., 2021: The VISCACHA survey - III. Star clusters counterpart of the Magellanic Bridge and Counter-Bridge in 8D
  11. Santos Jr. et al., 2020: The VISCACHA survey - II. Structure of star clusters in the Magellanic Clouds periphery
  12. Maia et al., 2019: The VISCACHA survey - I. Overview and first results

Data products and codes

  • Ferreira et al.: CMD fitting code, SIESTA. A synthetic CMD fitting code written in Python for determining the ages, metallicities, distances, color excesses, and binary fractions of star clusters using their decontaminated CMDs with a flexible choice of photometric bands and stellar evolution models. More in Paper XI.
  • Saroon et al.: photometric catalogs and physical parameters for 15 SMC star clusters. VizieR tables containing catalogs with the coordinates and V,I magnitudes of 15 SMC star clusters as well as ages, metallicities, distances and color excesses determined from isochrone fitting in Paper VIII.
  • Santos Jr. et al.: Structural parameters for 83 MCs star clusters. VizieR tables containing structural parameters determined in Paper II for 83 clusters in the LMC and SMC using both radial density profiles and surface brightness profiles.

Other VISCACHA or VISCACHA-related publications

  1. Drory et al., 2024: The SDSS-V Local Volume Mapper (LVM): Scientific Motivation and Project Overview
  2. de Souza et al., 2024: Ages and metallicities of stellar clusters using S-PLUS narrow-band integrated photometry: the Small Magellanic Cloud
  3. De Bórtoli et al., 2022: Ca II triplet spectroscopy of Small Magellanic Cloud red giants. VI. Analysis of chemical properties of the main body
  4. Parisi et al., 2022: Ca II Triplet Spectroscopy of Small Magellanic Cloud Red Giants. V. Abundances and Velocities for 12 Massive Clusters
  5. Dias & Parisi 2020: Panchromatic calibration of Ca II triplet luminosity dependence
  6. Dias et al., 2020: The VISCACHA survey - deep and resolved photometry of star clusters in the Magellanic Clouds
  7. Bica et al., 2020: An Updated SMC and Magellanic Bridge Catalog of Star Clusters, Associations and Related Objects
  8. Dias et al., 2019: The VISCACHA survey: an overview
  9. Dias et al., 2018: The VISCACHA survey. Age and metallicity spatial distribution of star clusters in the SMC reveals a complex tidal history
  10. Santos Jr. et al., 2018: Tidal effects on the structure of Magellanic Cloud peripheral star clusters
  11. Souza et al., 2018: The SIRIUS code: Statistical Inference of physical paRameters of sIngle and mUltiple populations in Stellar clusters

Pre-VISCACHA selected references from team members

  1. Dias et al., 2016: SMC west halo: a slice of the galaxy that is being tidally stripped?. Star clusters trace age and metallicity gradients
  2. Parisi et al., 2016: Ca II Triplet Spectroscopy of Small Magellanic Cloud Red Giants. IV. Abundances for a Large Sample of Field Stars and Comparison with the Cluster Sample
  3. Bica et al., 2015: Bridge over troubled gas: clusters and associations under the SMC and LMC tidal stresses
  4. Parisi et al., 2015: Ca II Triplet Spectroscopy of Small Magellanic Cloud Red Giants. III. Abundances and Velocities for a Sample of 14 Clusters
  5. Maia et al., 2014: Mass distribution and structural parameters of Small Magellanic Cloud star clusters
  6. Dias et al., 2014: Self-consistent physical parameters for five intermediate-age SMC stellar clusters from CMD modelling
  7. Maia et al., 2010: Characterization and photometric membership of the open cluster NGC1981
  8. Dias et al., 2010: Age and metallicity of star clusters in the Small Magellanic Cloud from integrated spectroscopy
  9. Balbinot et al., 2010: Probing the Large Magellanic Cloud age gap at intermediate cluster masses
  10. Parisi et al., 2009: Ca II Triplet Spectroscopy of Small Magellanic Cloud Red Giants. I. Abundances and Velocities for a Sample of Clusters
  11. Bica et al., 2008: A general catalogue of extended objects in the Magellanic System
  12. Bica et al., 2008: BS196: an old star cluster far from the Small Magellanic Cloud main body
  13. Kerber et al., 2007: Physical parameters of 15 intermediate-age LMC clusters from modelling of HST colour-magnitude diagrams
  14. Kerber et al., 2005: Physical parameters of rich LMC clusters from modeling of deep HST colour-magnitude diagrams
  15. Kerber et al., 2002: Analysis of colour-magnitude diagrams of rich LMC clusters: NGC 1831