NOAO >   Observing Info >   Approved Programs >   2018A-0056

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Program Information for 2018A-0056


PI: J Ignacio Gonzalez Serrano, Universidad de Cantabria, gserrano@ifca.unican.es
Address: Instituto de Fisica de Cantabria, Avda. de los Castos s/n, Santander, Cantabria 39005 Spain

CoI: J Gonzalez-Gonzalez, Institute of Astronomy, UNAM
CoI: C Padilla-Torres, TNG
CoI: A Bongiovanni, Instituto de Astrofisica de Canarias
CoI: Jordi Cepa, Instituto de Astrofisica de Canarias

Title: Spectroscopy of bright FIR sources in the Lockman Hole field

Abstract: This proposal is aimed to carry out a spectroscopic study of extragalactic sources in the central $24times 24$ sq. arcmin. of the Lockman Hole field, which has been observed with ROSAT, XMM-Newton at the highest depth. Within the selected objects, optical counterparts (up to $Rc=20.6$) of X-ray, Spitzer-24$mu $m prior sources on PEP- Herschel scans, and non-studied radio-galaxies will be specifically targeted. Some of the goals of the survey include studying the evolution of SFR and efficiencies, optical versus FIR extinction, metallicities, stellar populations, and specific members of high- redshift objects such as obscured AGN, SMG and ULIRG. Data to be obtained will complement the spectra of fainter targets ($21<Rc<24.5$) currently being obtained by the team using the guaranteed time of OSIRIS in MOS mode (200 hours) in the framework of the Lockman-SpReSo survey at the 10m GTC telescope. The complete catalogue will be public as soon as all data are available.

Program Type: Standard/Extragalactic

Scheduled Nights:
Run 1 (2018A):  WIYN/HYDR -- 1n on May 07 - May 08 2018


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NOAO >   Observing Info >   Approved Programs >   2018A-0056

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