Table 2
Spectroscopic observations of HR 10.
Dedicated spectroscopic campaigns | ||||||||||
---|---|---|---|---|---|---|---|---|---|---|
Dates | N | Resolution | Spectral range | Telescope/Observatory | ||||||
(nm) | spectrograph | |||||||||
2015-09 04-07 | 17 | 1.2-m Mercator Telescope/La Palma | ||||||||
2015-12 20-23 | 8 | 85 000 | 377–900 | High Efficiency and Resolution Mercator Echelle Spectrograph (HERMES) | ||||||
2016-07 12 | 1 | |||||||||
2015-10 22-23 | 3 | 48 000 | 350–920 | 2.2-m ESO-MPIA Telescope/La Silla | ||||||
Fibre-fed Extended Range Optical Echelle Spectrograph (FEROS) | ||||||||||
2017-10-05 to | ||||||||||
2018-01-03 | 10 | 2.5-m Nordic Optical Telescope (NOT)/La Palma | ||||||||
2018-11-23 to | 12 | 67 000 | 370–910 | FIbre-fed Echelle Spectrograph (FIES) | ||||||
2019-01-08 | ||||||||||
2017-10-06 to | 21 | 115 000 | 383–693 | 3.6-m Telescopio Nazionale Galileo (TNG)/La Palma | ||||||
2018-01-02 | High Accuracy Radial velocity Planet Searcher North (HARPS-N) | |||||||||
2017-07-21 to | 21 | 94 600 (VIS) | 520–960 | 3.5-m CAHA Telescope/Calar Alto | ||||||
2017-12-30 | 80 400 (NIR) | 960–1710 | Calar Alto high-Resolution search for M dwarfs with Exoearths | |||||||
with Near-infrared and optical Echelle Spectrographs (CARMENES) | ||||||||||
Observations extracted from publications or archives | ||||||||||
Dates | N | Resolution | Spectral range | Telescope/Observatory | Ref. | |||||
(line or nm) | spectrograph | |||||||||
1986-08-15 | 1 | 60 000 | Ca II K | 1.4-m Coudé Auxiliary Telescope (CAT)/La Silla | 1 | |||||
1998-10-15 | 1 | 100 000 | ESO Coudé Echelle Spectrometer (CES) | |||||||
1996-11-30 | 1 | 3.6-m Telescope/Anglo Australian Observatory | 2 | |||||||
1997-06-20 | 1 | 1 000 000 | Ca II K | Ultra High Resolution Facility (UHRF) | 2 | |||||
2005-06-15 | 1 | 3 | ||||||||
1998-10-25 | 1 | 49 000 | 380–590 | 4.2-m William Herschel Telescope/La Palma | 4 | |||||
1999-01-28 | 1 | Utrech Echelle Spectrograph (UES) | ||||||||
2004-08-28 | 1 | 2.7-m Harlan J. Smith Telescope/McDonald Observatory | ||||||||
2004-08-29 | 1 | 240 000 | Ca II K | Cross-Dispersed Echelle Spectrometer (CS21) | 3 | |||||
2005-09-15 | 1 | |||||||||
2007-06-28 | 14 | |||||||||
2007-07-11 | 6 | 360–450 | 8-m ESO–Very Large Telescope/Paranal | ESO | ||||||
2007-07-15 | 14 | 60 000 | 460–670 | Ultraviolet and Visual Echelle Spectrograph (UVES) | Archive | |||||
2007-07-26 | 34 | |||||||||
2007-07-27 | 6 | |||||||||
2010-09-01 | 3 | 336–810 | 10-m Keck I Telescope/Hawaii | Keck | ||||||
2011-12-08 | 3 | High Resolution Echelle Spectrometer (HIRES) | Archive | |||||||
2015-01-18 | 1 | |||||||||
2015-01-19 | 2 | 3.6-m ESO Telescope/La Silla | ESO | |||||||
2015-01-20 | 1 | 120 000 | 378–691 | High Accuracy Radial velocity Planet Searcher (HARPS) | Archive | |||||
2015-01-21 | 2 |
Notes. Dates of the specific nights of the campaigns are given in Table 3. “N” is the number of spectra. Data from CARMENES will be used in a forthcoming paper.
References. (1) Lagrange-Henri et al. (1990), (2) Welsh et al. (1998), (3) Redfield et al. (2007), (4) EXPORT La Palma International Time campaigns, Mora et al. (2001).
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