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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 7.

PSFs of the HDUV data. The left panels show stamps of the F275W (top) and F336W (bottom) PSFs. Images are 5″ on a side. The right panels compare the PSF-enclosed flux with the B435-band PSF, as well as with the theoretically determined TinyTim PSFs of the corresponding WFC3/UVIS filters. The PSFs for the two fields are very consistent with each other.

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