16512
收藏DataCite Commons2023-04-21 更新2025-04-15 收录
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http://esdcdoi.esac.esa.int/doi/html/data/astronomy/hst/16512.html
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资源简介：
The WFC3-IR detector photometric sensitivity is typically characterized by the measurement of isolated comma standard spectrophotometric white dwarf stars. To supplement those observations comma we seek to measure fluxes of hundreds of stars in stellar clusters over time comma to achieve higher precision than using a single star. In this program comma we propose to repeat observations from previous observations of M4 (Program 14725) to mitigate effects from different observation configurations.
提供机构：
European Space Agency
创建时间：
2023-04-21
