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P., The Astrophysical Journal, 920, 2021-10-01 00:00:00, 2021ApJ...920..129J||Intrinsic metallicity variation in the intermediate mass type II globular cluster NGC 1261, Muñoz, Cesar,Geisler, D.,Villanova, S., Monthly Notices of the Royal Astronomical Society, 506, 2021-10-01 00:00:00, 2021MNRAS.506.4676M||Investigating the Consistency of Stellar Evolution Models with Globular Cluster Observations via the Red Giant Branch Bump, Joyce, M.,Chaboyer, B., The Astrophysical Journal, 814, 2015-12-01 00:00:00, 2015ApJ...814..142J||Is helium the key parameter in the extended colour spread of the first generation stars in M3?, Tailo, M.,D'Antona, F.,Caloi, V., Monthly Notices of the Royal Astronomical Society, 486, 2019-07-01 00:00:00, 2019MNRAS.486.5895T||Isochrone fitting of Galactic globular clusters - III. 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I. Velocity Dispersion Profiles and Rotation Signals of 11 Globular Clusters, Ferraro, F. R.,Mucciarelli, A.,Lanzoni, B., The Astrophysical Journal, 860, 2018-06-01 00:00:00, 2018ApJ...860...50F||Milky Way globular cluster metallicity and low-mass X-ray binaries: the red giant influence, Vulic, N.,Barmby, P.,Gallagher, S. C., Monthly Notices of the Royal Astronomical Society, 473, 2018-02-01 00:00:00, 2018MNRAS.473.4900V||Mixed Populations in Globular Clusters: Et Tu, 47 Tuc?, Anderson, J.,Piotto, G.,King, I. 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Application to the colour-magnitude diagrams of the globular clusters 47 Tuc, NGC 6362, M 5, M 3, M 55, and M92, VandenBerg, Don A.,Casagrande, L.,Edvardsson, Bengt, Monthly Notices of the Royal Astronomical Society, 509, 2022-01-01 00:00:00, 2022MNRAS.509.4208V||Models for metal-poor stars with different initial abundances of C, N, O, Mg, and Si - III. Grids of isochrones for -2.5 ≤ [Fe/H] ≤ -0.5 and helium abundances Y = 0.25 and 0.29 at each metallicity, VandenBerg, Don A., Monthly Notices of the Royal Astronomical Society, 518, 2023-01-01 00:00:00, 2023MNRAS.518.4517V||Models of metal-poor stars with different initial abundances of C, N, O, Mg, and Si - I. Bolometric corrections derived from new MARCS synthetic spectra and their implications for observed colour-magnitude diagrams, VandenBerg, Don A.,Edvardsson, Bengt,Casagrande, L., Monthly Notices of the Royal Astronomical Society, 509, 2022-01-01 00:00:00, 2022MNRAS.509.4189V||Multiband Probabilistic Cataloging: A Joint Fitting Approach to Point-source Detection and Deblending, Feder, Richard M.,Portillo, Stephen K. N.,Daylan, Tansu, The Astronomical Journal, 159, 2020-04-01 00:00:00, 2020AJ....159..163F||Multichromatic colour-magnitude diagrams of the globular cluster NGC 6366, Campos, Fabíola,Kepler, S. O.,Bonatto, C., Monthly Notices of the Royal Astronomical Society, 433, 2013-07-01 00:00:00, 2013MNRAS.433..243C||Multiple Stellar Populations in 47 Tucanae, Milone, A. P.,Piotto, G.,Bedin, L. R., The Astrophysical Journal, 744, 2012-01-01 00:00:00, 2012ApJ...744...58M||Multiple Stellar Populations in Asymptotic Giant Branch Stars of Galactic Globular Clusters, Lagioia, E. 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Instrument
ACS, ACS/WFC, WFPC2, WFPC2/WFC
Temporal Coverage
2006-02-20T11:16:31Z/2006-08-08T04:33:27Z
Version
1.0
Mission Description
Launched in 1990, the NASA/ESA Hubble Space Telescope remains the premier UV and visible light telescope in orbit. With well over 1.6 million observations from 10 different scientific instruments, the ESA Hubble Science Archive is a treasure trove of astronomical data to be exploited.
