GIARPS@TNG: GIANO-B and HARPS-N together for a wider wavelength range spectroscopy

被引：53

作者：

Claudi, R. ^{[1
]}

Benatti, S. ^{[1
]}

Carleo, I. ^{[1
,2
]}

Ghedina, A. ^{[3
]}

Guerra, J. ^{[3
]}

Micela, G. ^{[4
]}

Molinari, E. ^{[3
,5
]}

Oliva, E. ^{[6
]}

Rainer, M. ^{[7
]}

Tozzi, A. ^{[6
]}

Baffa, C. ^{[6
]}

Baruffolo, A. ^{[1
]}

Buchschacher, N. ^{[8
]}

Cecconi, M. ^{[3
]}

Cosentino, R. ^{[3
]}

Fantinel, D. ^{[1
]}

Fini, L. ^{[6
]}

Ghinassi, F. ^{[3
]}

Giani, E. ^{[6
]}

Gonzalez, E. ^{[4
]}

Gonzalez, M. ^{[3
]}

Gratton, R. ^{[1
]}

Harutyunyan, A. ^{[3
]}

Hernandez, N. ^{[3
]}

Lodi, M. ^{[3
]}

Malavolta, L. ^{[2
]}

Maldonado, J. ^{[4
]}

Origlia, L. ^{[9
]}

Sanna, N. ^{[6
]}

Sanjuan, J. ^{[3
]}

Scuderi, S. ^{[10
]}

Seemann, U. ^{[11
]}

Sozzetti, A. ^{[12
]}

Perez Ventura, H. ^{[3
]}

Hernandez Diaz, M. ^{[3
]}

Galli, A. ^{[3
]}

Gonzalez, C. ^{[3
]}

Riverol, L. ^{[3
]}

Riverol, C. ^{[3
]}

机构：

[1] INAF, Astron Observ Padova, Padua, Italy

[2] Univ Padua, Dept Phys & Astron, Padua, Italy

[3] INAF, Fdn Galileo Galilei, Brena Baja, Spain

[4] INAF, Astrophys Observ Palermo, Palermo, Italy

[5] INAF IASF, Milan, Italy

[6] INAF, Astrophys Observ Arcetri, Florence, Italy

[7] INAF, Astron Observ Brera, Merate, Italy

[8] Univ Geneva, Geneva, Switzerland

[9] INAF, Astron Observ Bologna, Bologna, Italy

[10] INAF, Astrophys Observ Catania, Catania, Italy

[11] Georg August Univ Gottingen, Inst Astrophys, Gottingen, Germany

[12] Astrophys Observ Torino, Pino Torinese, Italy

来源：

EUROPEAN PHYSICAL JOURNAL PLUS | 2017年 / 132卷 / 08期

关键词：

GROUND-BASED DETECTION; EXOPLANET HD 209458B; EXTRASOLAR PLANET; TRANSMISSION SPECTRUM; HOT JUPITER; RADIAL-VELOCITIES; SECONDARY ECLIPSE; THERMAL EMISSION; ATMOSPHERE; WATER;

D O I：

10.1140/epjp/i2017-11647-9

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

Since 2012, thanks to the installation of the high-resolution echelle spectrograph in the optical range HARPS-N, the Italian telescope TNG (La Palma) became one of the key facilities for the study of the extrasolar planets. In 2014 TNG also offered GIANO to the scientific community, providing a near-infrared (NIR) cross-dispersed echelle spectroscopy covering 0.97-2.45 mu m at a resolution of 50000. GIANO, although designed for direct light-feed from the telescope at the Nasmyth-B focus, was provisionally mounted on the rotating building and connected via fibers to only available interface at the Nasmyth-A focal plane. The synergy between these two instruments is particularly appealing for a wide range of science cases, especially for the search of exoplanets around young and active stars and the characterisation of their atmosphere. Through the funding scheme "WOW" (a Way to Others Worlds), the Italian National Institute for Astrophysics (INAF) proposed to position GIANO at the focal station for which it was originally designed and the simultaneous use of these spectrographs with the aim to achieve high-resolution spectroscopy in a wide wavelength range (0.383-2.45 mu m) obtained in a single exposure, giving rise to the project called GIARPS (GIANO-B & HARPS-N). Because of its characteristics, GIARPS can be considered the first and unique worldwide instrument providing not only high resolution in a large wavelength band, but also a high-precision radial velocity measurement both in the visible and in the NIR arm, since in the next future GIANO-B will be equipped with gas absorption cells.

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