Lockman-SpReSO: a deep OSIRIS spectroscopic survey

Bibcode
2020sea..confE..43G
González-Otero, M.; Padilla Torres, C. P.; Cepa, J.(Instituto de Astrofísica de Canarias, Universidad de La Laguna, Spain) [Staff ULL]; Lockman-SpReSO Team
Bibliographical reference

Contributions to the XIV.0 Scientific Meeting (virtual) of the Spanish Astronomical Society

Advertised on:
7
2020
Number of authors
4
IAC number of authors
3
Citations
0
Refereed citations
0
Description
Lockman-SpReSO is a deep optical spectroscopic survey of a complete sample of galaxies previously observed at the greatest depth in X-ray, far infrared, and sub-millimeter, using, respectively, XMM-Newton, Spitzer, Herschel, and radio observations covering the central 24 x 24 arcmin2 of the Lockman Hole field. The main scientific objective is to study the spectroscopic properties of a complete, magnitude-limited sample (∼18 < R(AB) < 24.5) of the optical counterparts of far-infrared galaxies, aiming for determining the evolution of fundamental parameters such as extinction, star formation rate and gas metallicity and their infrared biases. The survey observations are in their final phase. The procedures for the analysis of spectra are currently being tested and refined. This presentation shows the results obtained so far.
Type
Non-refereed

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