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)