OSIRIS large guaranteed time programs

A. Bongiovanni; M. Ramón-Pérez; A. M. Pérez García; E. J. Alfaro; H. O. Castañeda; M. Cerviño; J. Gallego; J. J. González; J. I. González-Serrano; M. A. Lara-López; R. Pérez-Martínez; I. Pintos-Castro; M. Sánchez-Portal; J. Bland-Hawthorn; D. H. Jones

OSIRIS large guaranteed time programs

A. Bongiovanni, M. Ramón-Pérez, A. M. Pérez García, E. J. Alfaro, H. O. Castañeda, M. Cerviño, J. Gallego, J. J. González, J. I. González-Serrano, M. A. Lara-López, R. Pérez-Martínez, I. Pintos-Castro, M. Sánchez-Portal, J. Bland-Hawthorn, D. H. Jones

Escuela Superior de Física y Matemáticas (ESFM)

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › peer-review

Abstract

The status of OTELO and Lockman SpReSO surveys, the two large guaranteed time programs currently under way using OSIRIS at the 10.4m GTC is presented. The OTELO project, designed to detect the main optical emission lines from Ha to Lyα at redshifts from 0.4 through 7, is the deepest emission line survey to date, with unprecedented sensitivity in the detection of small equivalent widths. Lockman SpReSO is aimed to obtaining optical spectra, up to 24.5 AB magnitudes, in the central 24×24 square arcminutes of the Lockman Hole field, which has been observed with ROSAT and XMM-Newton at the highest depth. Lockman SpReSO mainly targets Far Infrared sources detected with the Herschel Space Observatory.

Original language	English
Title of host publication	Proceedings of the 12th Scientific Meeting of the Spanish Astronomical Society - Highlights of Spanish Astrophysics IX, SEA 2016
Editors	S. Arribas, A. Alonso-Herrero, F. Figueras, C. Hernandez-Monteagudo, A. Sanchez-Lavega, S. Perez-Hoyos
Publisher	SEA
Pages	76-87
Number of pages	12
ISBN (Electronic)	9788461789313
State	Published - 2016
Event	12th Scientific Meeting of the Spanish Astronomical Society - Highlights of Spanish Astrophysics IX, SEA 2016 - Bilbao, Spain Duration: 18 Jul 2016 → 22 Jul 2016

Publication series

Name	Proceedings of the 12th Scientific Meeting of the Spanish Astronomical Society - Highlights of Spanish Astrophysics IX, SEA 2016

Conference

Conference	12th Scientific Meeting of the Spanish Astronomical Society - Highlights of Spanish Astrophysics IX, SEA 2016
Country/Territory	Spain
City	Bilbao
Period	18/07/16 → 22/07/16

Cite this

Bongiovanni, A., Ramón-Pérez, M., Pérez García, A. M., Alfaro, E. J., Castañeda, H. O., Cerviño, M., Gallego, J., González, J. J., González-Serrano, J. I., Lara-López, M. A., Pérez-Martínez, R., Pintos-Castro, I., Sánchez-Portal, M., Bland-Hawthorn, J., & Jones, D. H. (2016). OSIRIS large guaranteed time programs. In S. Arribas, A. Alonso-Herrero, F. Figueras, C. Hernandez-Monteagudo, A. Sanchez-Lavega, & S. Perez-Hoyos (Eds.), Proceedings of the 12th Scientific Meeting of the Spanish Astronomical Society - Highlights of Spanish Astrophysics IX, SEA 2016 (pp. 76-87). (Proceedings of the 12th Scientific Meeting of the Spanish Astronomical Society - Highlights of Spanish Astrophysics IX, SEA 2016). SEA.

Bongiovanni, A. ; Ramón-Pérez, M. ; Pérez García, A. M. et al. / OSIRIS large guaranteed time programs. Proceedings of the 12th Scientific Meeting of the Spanish Astronomical Society - Highlights of Spanish Astrophysics IX, SEA 2016. editor / S. Arribas ; A. Alonso-Herrero ; F. Figueras ; C. Hernandez-Monteagudo ; A. Sanchez-Lavega ; S. Perez-Hoyos. SEA, 2016. pp. 76-87 (Proceedings of the 12th Scientific Meeting of the Spanish Astronomical Society - Highlights of Spanish Astrophysics IX, SEA 2016).

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abstract = "The status of OTELO and Lockman SpReSO surveys, the two large guaranteed time programs currently under way using OSIRIS at the 10.4m GTC is presented. The OTELO project, designed to detect the main optical emission lines from Ha to Lyα at redshifts from 0.4 through 7, is the deepest emission line survey to date, with unprecedented sensitivity in the detection of small equivalent widths. Lockman SpReSO is aimed to obtaining optical spectra, up to 24.5 AB magnitudes, in the central 24×24 square arcminutes of the Lockman Hole field, which has been observed with ROSAT and XMM-Newton at the highest depth. Lockman SpReSO mainly targets Far Infrared sources detected with the Herschel Space Observatory.",

author = "A. Bongiovanni and M. Ram{\'o}n-P{\'e}rez and {P{\'e}rez Garc{\'i}a}, {A. M.} and Alfaro, {E. J.} and Casta{\~n}eda, {H. O.} and M. Cervi{\~n}o and J. Gallego and Gonz{\'a}lez, {J. J.} and Gonz{\'a}lez-Serrano, {J. I.} and Lara-L{\'o}pez, {M. A.} and R. P{\'e}rez-Mart{\'i}nez and I. Pintos-Castro and M. S{\'a}nchez-Portal and J. Bland-Hawthorn and Jones, {D. H.}",

note = "Publisher Copyright: {\textcopyright} 2016 Proceedings of the 12th Scientific Meeting of the Spanish Astronomical Society - Highlights of Spanish Astrophysics IX, SEA 2016. All rights reserved.; 12th Scientific Meeting of the Spanish Astronomical Society - Highlights of Spanish Astrophysics IX, SEA 2016 ; Conference date: 18-07-2016 Through 22-07-2016",

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series = "Proceedings of the 12th Scientific Meeting of the Spanish Astronomical Society - Highlights of Spanish Astrophysics IX, SEA 2016",

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editor = "S. Arribas and A. Alonso-Herrero and F. Figueras and C. Hernandez-Monteagudo and A. Sanchez-Lavega and S. Perez-Hoyos",

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Bongiovanni, A, Ramón-Pérez, M, Pérez García, AM, Alfaro, EJ, Castañeda, HO, Cerviño, M, Gallego, J, González, JJ, González-Serrano, JI, Lara-López, MA, Pérez-Martínez, R, Pintos-Castro, I, Sánchez-Portal, M, Bland-Hawthorn, J & Jones, DH 2016, OSIRIS large guaranteed time programs. in S Arribas, A Alonso-Herrero, F Figueras, C Hernandez-Monteagudo, A Sanchez-Lavega & S Perez-Hoyos (eds), Proceedings of the 12th Scientific Meeting of the Spanish Astronomical Society - Highlights of Spanish Astrophysics IX, SEA 2016. Proceedings of the 12th Scientific Meeting of the Spanish Astronomical Society - Highlights of Spanish Astrophysics IX, SEA 2016, SEA, pp. 76-87, 12th Scientific Meeting of the Spanish Astronomical Society - Highlights of Spanish Astrophysics IX, SEA 2016, Bilbao, Spain, 18/07/16.

OSIRIS large guaranteed time programs. / Bongiovanni, A.; Ramón-Pérez, M.; Pérez García, A. M. et al.
Proceedings of the 12th Scientific Meeting of the Spanish Astronomical Society - Highlights of Spanish Astrophysics IX, SEA 2016. ed. / S. Arribas; A. Alonso-Herrero; F. Figueras; C. Hernandez-Monteagudo; A. Sanchez-Lavega; S. Perez-Hoyos. SEA, 2016. p. 76-87 (Proceedings of the 12th Scientific Meeting of the Spanish Astronomical Society - Highlights of Spanish Astrophysics IX, SEA 2016).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › peer-review

TY - GEN

T1 - OSIRIS large guaranteed time programs

AU - Bongiovanni, A.

AU - Ramón-Pérez, M.

AU - Pérez García, A. M.

AU - Alfaro, E. J.

AU - Castañeda, H. O.

AU - Cerviño, M.

AU - Gallego, J.

AU - González, J. J.

AU - González-Serrano, J. I.

AU - Lara-López, M. A.

AU - Pérez-Martínez, R.

AU - Pintos-Castro, I.

AU - Sánchez-Portal, M.

AU - Bland-Hawthorn, J.

AU - Jones, D. H.

PY - 2016

Y1 - 2016

N2 - The status of OTELO and Lockman SpReSO surveys, the two large guaranteed time programs currently under way using OSIRIS at the 10.4m GTC is presented. The OTELO project, designed to detect the main optical emission lines from Ha to Lyα at redshifts from 0.4 through 7, is the deepest emission line survey to date, with unprecedented sensitivity in the detection of small equivalent widths. Lockman SpReSO is aimed to obtaining optical spectra, up to 24.5 AB magnitudes, in the central 24×24 square arcminutes of the Lockman Hole field, which has been observed with ROSAT and XMM-Newton at the highest depth. Lockman SpReSO mainly targets Far Infrared sources detected with the Herschel Space Observatory.

AB - The status of OTELO and Lockman SpReSO surveys, the two large guaranteed time programs currently under way using OSIRIS at the 10.4m GTC is presented. The OTELO project, designed to detect the main optical emission lines from Ha to Lyα at redshifts from 0.4 through 7, is the deepest emission line survey to date, with unprecedented sensitivity in the detection of small equivalent widths. Lockman SpReSO is aimed to obtaining optical spectra, up to 24.5 AB magnitudes, in the central 24×24 square arcminutes of the Lockman Hole field, which has been observed with ROSAT and XMM-Newton at the highest depth. Lockman SpReSO mainly targets Far Infrared sources detected with the Herschel Space Observatory.

UR - http://www.scopus.com/inward/record.url?scp=85088168805&partnerID=8YFLogxK

M3 - Contribución a la conferencia

AN - SCOPUS:85088168805

T3 - Proceedings of the 12th Scientific Meeting of the Spanish Astronomical Society - Highlights of Spanish Astrophysics IX, SEA 2016

SP - 76

EP - 87

BT - Proceedings of the 12th Scientific Meeting of the Spanish Astronomical Society - Highlights of Spanish Astrophysics IX, SEA 2016

A2 - Arribas, S.

A2 - Alonso-Herrero, A.

A2 - Figueras, F.

A2 - Hernandez-Monteagudo, C.

A2 - Sanchez-Lavega, A.

A2 - Perez-Hoyos, S.

PB - SEA

T2 - 12th Scientific Meeting of the Spanish Astronomical Society - Highlights of Spanish Astrophysics IX, SEA 2016

Y2 - 18 July 2016 through 22 July 2016

ER -

Bongiovanni A, Ramón-Pérez M, Pérez García AM, Alfaro EJ, Castañeda HO, Cerviño M et al. OSIRIS large guaranteed time programs. In Arribas S, Alonso-Herrero A, Figueras F, Hernandez-Monteagudo C, Sanchez-Lavega A, Perez-Hoyos S, editors, Proceedings of the 12th Scientific Meeting of the Spanish Astronomical Society - Highlights of Spanish Astrophysics IX, SEA 2016. SEA. 2016. p. 76-87. (Proceedings of the 12th Scientific Meeting of the Spanish Astronomical Society - Highlights of Spanish Astrophysics IX, SEA 2016).

OSIRIS large guaranteed time programs

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