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THE AGE OF THE YOUNG BULGE-LIKE POPULATION IN THE STELLAR SYSTEM TERZAN 5: LINKING THE GALACTIC BULGE TO THE HIGH-Z UNIVERSE

  • Authors: F. R. Ferraro, D. Massari, E. Dalessandro, B. Lanzoni, L. Origlia, R. M. Rich, and A. Mucciarelli

2016 The Astrophysical Journal 828 75.

  • Provider: AAS Journals

Caption: Figure 2.

Double MS-To of Terzan 5 in different CMDS. Upper left: the (H, J–H) CMD obtained from data secured with the infrared channel of the HST Wide Field Camera 3 (WFC3). Upper right: the (K, V–K) CMD obtained by combining the K-band laser AO-assisted images secured with Keck-NIRC2 and I-band images obtained with HST-ACS. Bottom left: the (I, V–I) CMD obtained with the HST-ACS. Bottom right: the (K, I–K) CMD obtained by combining K-band AO-assisted VLT observations with the deep I-band image obtained with HST-ACS. All the CMDs have been corrected for internal differential reddening and they refer to different regions of the system (see Figure 1).

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