"eEASy" Datasets

Telescope time and observations obtained in the framework of the "eEASy" project:

(especially relevant to "eEASy" objectives of WP2)

- 8-24hrs of ALMA time (PI: M. Brusa; Cycle4 and 6, priority C - Spring 2017/2019):

   "Starbursting to quenching: feedback in the gas reservoir of a dusty QSO"

- 125 ks of XMM time (PI: M. Brusa; AO15 - December 2016):

   "XMM-Newton observations of galaxy-wide outflows: the origin of super winds"

- 6.5hrs of ALMA time (PI: M. Brusa; Cycle3, priority A - June 2016):

   "Mapping the feedback effects on the gas reservoir in a z~1.6 QSO"

- 280 hours of VLT/SINFONI time at ESO (PI: V. Mainieri; P94 - ongoing):

  "SUPER: SINFONI Survey for Unveiling the Physics and Effects of Radiative feedback"

   The aim of the program is to carry out the first statistically-sound investigation of ionised outflows in AGN host galaxies at the peak epoch of AGN and galaxy assembly, z~2, down to a resolution of 1 kpc

- 100 ks of Nustar time (through Nustar GTO/ PI: A. Comastri/G. Lanzuisi):

   "XMM-Newton observations of galaxy-wide outflows: the origin of super winds"

- 8hrs of VLT/SINFONI time at ESO (PI: M. Brusa; P94 - February 2015):

   "NGS AO-assisted SINFONI observations of a unique SF-QSO system in the key epoch of AGN-galaxy evolution"

- 6hrs of PdBI time (PI: M. Brusa; DDT - June 2014):

   "A spectacular outflow in a z~1.6 QSO"

- 8hrs of VLT/SINFONI time at ESO (PI: G. Cresci; P92 - February 2014):

  "Mapping the effects of AGN feedback in two showcase outflowing obscured QSOs"

- 3 nights of VLT/XShooter time at ESO (PI: M. Brusa; P90 - February 2013)

  "Identifying and measuring BH masses for z=1-2 obscured QSO with X-shooter"

Involvement in multiwavelength projects:

(especially relevant "eEASy" objectives of WP1, WP3 and WP4)

* Chandra-COSMOS Legacy survey (PI: Civano / Yale University & Harvard University)

* Stripe82-X survey (PI: LaMassa/Urry - Yale University)

* XXL survey (PI: Pierre), complemented by  SPIDERS and SPIDERS-pilot

* SPIDERS and SPIDERS pilot (Spectroscopic Follow-up of eROSITA sources; PI: Merloni/Nandra/Georgakakis - Max Planck Institut für Extraterrestische Physik); dedicated SDSS spectroscopic coverage of X-ray selected sources from ROSAT and XMM-Slew survey within the BOSS/SDSS_IV project

* X-UDS survey (PI: Kocevski/Hasinger - Colbie college & Institute for Astronomy Hawaii), awarded in 2015 and currently ongoing.

* CDFS and CANDELS (public fields)