3D-HST WFC3-SELECTED PHOTOMETRIC CATALOGS IN THE FIVE CANDELS/3D-HST FIELDS: PHOTOMETRY, PHOTOMETRIC REDSHIFTS, AND STELLAR MASSES
Whitney Museum of American Art · Yale University · +16 more institutions
Abstract
The 3D-HST and CANDELS programs have provided WFC3 and ACS spectroscopy and photometry over 900 arcmin 2 in five fields: AEGIS, COSMOS, GOODS-North, GOODS-South, and the UKIDSS UDS field. All these fields have a wealth of publicly available imaging data sets in addition to the Hubble Space Telescope (HST) data, which makes it possible to construct the spectral energy distributions (SEDs) of objects over a wide wavelength range. In this paper we describe a photometric analysis of the CANDELS and 3D-HST HST imaging and the ancillary imaging data at wavelengths 0.3-8 m. Objects were selected in the WFC3 near-IR bands, and their SEDs were determined by carefully taking the effects of the point-spread function in…
Citation impact
- FWCI
- 50.77
- Percentile
- 100%
- References
- 108
Authors
27- RERosalind E. SkeltonCorresponding
Whitney Museum of American Art, Yale University, South African Radio Astronomy Observatory
- KEKatherine E. Whitaker
Goddard Space Flight Center, Deleted Institution
- IGIvelina G. Momcheva
Whitney Museum of American Art, Yale University
- GBGabriel B. Brammer
Space Telescope Science Institute, Université Bourgogne Franche-Comté
- PGPieter G. van Dokkum
Whitney Museum of American Art, Yale University
Topics & keywords
- Photometry (optics)
- Grism
- Wide Field Camera 3
- Hubble space telescope
- Stellar population
- Population
- Wavelength
- Imaging spectroscopy