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HDUV: The Hubble Deep UV Legacy Survey

  • Authors: P. A. Oesch, M. Montes, N. Reddy, R. J. Bouwens, G. D. Illingworth, D. Magee, H. Atek, C. M. Carollo, A. Cibinel, M. Franx, B. Holden, I. Labbé, E. J. Nelson, C. C. Steidel, P. G. van Dokkum, L. Morselli, R. P. Naidu, and S. Wilkins

2018 The Astrophysical Journal Supplement Series 237 12.

  • Provider: AAS Journals

Caption: Figure 2.

The HST imaging filter set in the two HDUV survey fields. Combining the data of the two workhorse cameras on HST, WFC3, and ACS, these fields are now covered with 11-band data spanning a wavelength range from ∼0.25–1.7 μm at an excellent spatial resolution of 100–160 mas. The black line represents the spectrum of a typical Lyman break galaxy at z = 2, which can be selected thanks to the HDUV data.

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