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EPRVIII Instrument Table

Wright, Jason; Robertson, Paul

Abstract

New PRV instruments presented at the EPRVIII Workshop.

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EPRVIII Instruments Instrument EPRVIII Presenter Date of expected first light Date of expected full capabilities Wavelength range (nm) Expected best precision Telescope name Telescope location Telescope aperture Availability Instrument paper citation(s) Very short description SALT/HRS Lisa Crause 9/2013 early 2018 370-890 TBD! Hopefully <3 m/s SALT Sutherland, South Africa ~10m SALT partnership Crause+ 2014 SPIE 9147E 6T Stabilised dual-channel (370-890 nm), fibre-fed vacuum echelle, R~70k high stability (HS) mode for PRV (double scrambler + iodine cell or simultaneous Th-Ar).! Pipeline for HS under development, but instrument designed to reach <5 m/s. MINERVA Nate McCrady 12/2015 11/2016 480-690 ~0.9 m/s MINERVA Mt Hopkins, AZ, USA 4x0.7m PI-only Swift+ 2015 JATIS 1(2) 027002 Octagonal fiber-fed, robotic, temperature and pressure stabilized, iodine cell, R=75,000 echelle spectrometer. Veloce Chris Tinney 3/2018 for “Rosso” (580-950 nm) 2020 380-950 <0.3 m/s internal sub-1m/s on sky goal AAT Coonabarabran NSW, Australia 4m Facility under preparation IFU fibre-fed temperature and pressure controlled, red wavelength R=80,000 spectroagraph. Simultaneous single-mode lasercomb and ThXe calibration. Eventually to be 350-0950nm with adition of Verde and Azzurro cameras PFS2 Johanna Teske 2/2018 mid 2018 380-690 ~0.5 m/s on sky Magellan II Las Campanas, Chile 6.5m PI-only Crane+ 2006 SPIE 6269E 31 Crane+ 2008 SPIE 7014E 79 Crane+ 2010 SPIE 7735E 53 (hopefully 2018 with upgrades!) Optical, stabilized RV spectrograph on Magellan II. I2 cal. Upgrade = octagonal fiber feed, pupil slicer, new detector with smaller pixels, R~120,000. PARAS-2 Abhijit Chakraborty 12/2019 mid 2020 380-690 0.5 m/s on sky 2.5m Telescope Mt. Abu, India 2.5m PI-only under preparation Fiber-fed, stabilized RV spectrograph (R~100000) under stabilized environment (T~0.001K at 24C; Vacuum Pressure at 0.0001mbar), double srambler, octagonal-circular fiber combination; simultaneous ThAr calibration. HARPS3 Samantha Thompson end-2019 early 2020 380-690 < 0.5 m/s Isaac Newton (INT) Roque de los Muchachos, Canary Islands, Spain 2.5m Facility Thompson+ 2016 SPIE 9908E 6F Stabilised, fibre-fed, R=115,000, 380-690nm, robotic operation, full Stokes dual-beam polarimeter in Cass adapter TOU Bo Ma 11/2016 10/2017 380-900 ~0.8 m/s on sky UF 50-inch Mt. Hopkins, AZ , USA 1.27 m PI-only Ge+ 2016 SPIE 9908E 6I Optical, 380-900nm, R~100,000, ThAr calibration. Instrument stability ~1m/s. iSHELL Bryson Cale 10/2016 10/16 1100-5300 TBD, < 5m/s IRTF Maunakea, HI, USA 3m Facility Rayner+ 2016 SPIE 9908E 84 Rayner+ 2012 SPIE 8446E 2C R-70,000, 13CH4 cell for calibration, Cassegrain mounted MINERVA-R Cullen Blake 1/2018 3/2018 820-920 <1 m/s instrumental MINERVA Mt. Hopkins, AZ, USA 0.7m PI-only Sliski+2017 - submitted R~50,000, SM fiber, UNe and etalon calibration, 0.7 meter telescope MAROON-X Andreas Seifahrt 1/2019 05/2019 500-900 <0.3 m/s internal <1 m/s on-sky Gemini North Maunakea, HI, USA 8.2m public Seifahrt+ 2016 SPIE 9908E 18 !R~80,000, fiber-fed, stabilized RV spectrograph with pupil slicer and doubler scrambler. Rb-traced etalon calibrator. Optimized for M-dwarfs iLocater Jonathan Crass Fall 2019 12/2019 971-1270 <0.4 m/s internal <0.7 m/s on-sky Large Binocular Telescope Mount Graham, AZ, USA 2x8.2m PI-only Crepp+ 2016 SPIE 9908E 19 Single-mode fiber fed stabilized NIR spectrograph (YJ band). Rb-locked etalon calibration system. PARVI Gautam Vasisht Fall 2018 Fall 2019 1250-1800 1.0 m/s (req) 0.3 m/s (goal) Hale Telescope Mt. Palomar, CA, USA 5.1m Facility None Single-mode fiber fed stabilized NIR spectrograph (JH band). EOM comb based calibration system. R~100,000. NIRPS Rene Doyon 2019 2019 970-1810 ~< 1 m/s La Silla 3.6-m La Silla, Chile 3.6m ESO/public None Stabilized YJH R=100000 fiber-fed near-IR spectrograph, AO (0.4") and high-efficiency fiber (0.9”) SPIROU Claire Moutou 3/2018 8/2018 980-2350 1 m/s CFHT Maunakea, HI, USA 3.6m Facility Donati+2017 exoplanet handbook FP-stabilized YJHK fiber-fed spectropolarimeter. R=70k. Cryogenic at 80K. HPF Sam Halverson 9/2017 11/2017 810-1290 ~1 m/s Hobby-Eberly Telescope McDonald Observatory, Texas, USA ~10m Facility Mahadevan+ 2014 SPIE 9147E 1G Stabilized z/Y/J-band NIR spectrometer with EOM frequency comb, monolithic double scrambler IRD Masashi Omiya 8/9/2017 10/2017 970-1750 1 m/s Subaru Maunakea, HI, USA 8.2m Facility Kotani+ 2014 SPIE 9147E 14 Fiber-fed stabilized NIR (Y,J,H) spectrograph for the Subaru, laser frequency comb, ultra-low thermal expansion ceramic optical components CARMENES Ansgar Reiners 10/2015 01/2016 520-1710 1 m/s Calar Alto 3.5m Calar Alto, Spain 3.5m Facility Quirrenbach+ 2014 SPIE 9147E 1F Two stabilized R~90,000 spectrographs (520-980nm, 980-1710nm), simultaneous calibration GIARPS Monica Rainer 03/2017 mid 2018 340-2450 1 m/s (visible) 3 m/s (infrared) TNG Roque de los Muchachos, Canary Islands, Spain 3.6m Public Claudi+ 2016 SPIE 9908E 3H Simultaneous observations with HARPS-N (visible, 340-690nm, R=115,000) and GIANO-B (infrared, 950-2450 nm, R=50,000) NEID Paul Robertson / Chris Schwab 1/2019 mid 2019 380-1000 ~0.3 m/s initial w/ path to 0.1 m/s 3.5m WIYN Kitt Peak, AZ, USA 3.5m Public Halverson+ 2016 SPIE 9908E 6P Schwab+ 2016 SPIE 9908E 7H Ultra-precise broadband optical spectrometer. Public accessibility, optimized for both bright and faint (read: TESS) targets. EXPRES Ryan Blackman 5/2017 (front end, vacuum enclosure), 11/2017 (science) 12/2017 380-900 <0.3 m/s Discovery Channel Telescope Happy Jack, AZ, USA 4.3m PI+Lowell Consortium Jurgenson+ 2016 SPIE 9908E 6T Fiber-fed, stabilized RV spectrograph, R=150,000, Menlo LFC, double scrambler/pupil slicer, chromatic exposure meter ESPRESSO Francesco Pepe 11/2017 1/10/2018 380-780 0.1m/s VLT Cerro Paranal, Chile (4x)8m ESO/public Pepe+ 2013 The Messenger 153, 6 Stabilized, cross-disperser, fiber-fed echelle spectrograph with high spectral resolution for ultrahigh RV precision and high-fidelity spectroscopy. Can work with either one or 4 UTs of the VLT. KPF Arpita Roy 1/2020 mid 2020 440-850 0.3m/s (goal) 0.5m/s (req) Keck I Maunakea, HI, USA 10m Facility, public Gibson+ 2016 SPIE 9908E 70 Stabilized, fiber-fed, all-Zerodur, optical spectrometer (R>85,000) providing access to faint targets, especially transiting systems, on 10m Keck aperture GCLEF Sagi Ben-Ami 2022 2023 350-950 0.1m/s GMT Las Campanas, Chile 25.4m Facility Szentgyorgyi+ 2016 SPIE 9908E 22 Stabilized, fiber-fed, composite bench, visible, multimode (R=20K, 40K and 100K), First Light GMT instrument