HUGS: UltraDeep near-IR coverage of GOODS-S and UDS

Data, Data Release

What is HUGS: the deepest K-band survey ever. HUGS (an acronym for Hawk- I UDS and GOODS Survey) is a ultra–deep IR imaging survey executed with the Hawk-I imager at the VLT, that observed in the K and Y bands the UDS and GOODS-South fields covered by the CANDELS...

New simulated Herschel images available

Data Release, news, Simulations

As a first release of simulated data, we make here available a new set of Herschel simulated data. They carefully mimics the quality, size and depth of the Herschel images in GOODS-S at 100,160,250,350 and 500um. They are optimally designed to test Herschel source...

CONVPHOT

Software

Description of CONVPHOT CONVPHOT (De Santis et al. 2007) is a C code developed at INAF‐OAR that can compute background for each source and subtract it on-the-fly. The convolution is performed via straight pixel-­‐by-­‐pixel summation. Cutouts, templates, and also...

TFIT

Software

Description of TFIT TFIT (Laidler et al. 2007) was initially conceived and written by C. Papovich in 1999 as a C++ code.In its latest version, TFIT consists of a Python envelop performing the entirety of tasks, except for the fitting core routine, which is based on...

A CANDELS – GOODS – HERSCHEL SCIENCE MEETING

Uncategorized

The Spectral Energy Distribution of high redshift galaxies: lessons learned and open questions. Sexten Center for Astrophysics January 26‐30 2015 Aim of the workshop This workshop is organized under the auspices of the ASTRODEEP project and is devoted to discuss what...