An Extreme-precision Radial-velocity Pipeline: First Radial Velocities from EXPRES

被引:51
作者
Petersburg, Ryan R. [1 ,2 ]
Ong, J. M. Joel [2 ]
Zhao, Lily L. [2 ]
Blackman, Ryan T. [2 ]
Brewer, John M. [2 ,3 ]
Buchhave, Lars A. [4 ]
Cabot, Samuel H. C. [2 ]
Davis, Allen B. [2 ]
Jurgenson, Colby A. [2 ,5 ]
Leet, Christopher [2 ]
McCracken, Tyler M. [2 ,6 ]
Sawyer, David [2 ,7 ]
Sharov, Mikhail [8 ]
Tronsgaard, Rene [4 ]
Szymkowiak, Andrew E. [1 ,2 ]
Fischer, Debra A. [2 ]
机构
[1] Yale Univ, Dept Phys, 217 Prospect St, New Haven, CT 06511 USA
[2] Yale Univ, Dept Astron, 52 Hillhouse Ave, New Haven, CT 06511 USA
[3] San Francisco State Univ, Dept Phys & Astron, 1600 Holloway Ave, San Francisco, CA 94132 USA
[4] Tech Univ Denmark, Natl Space Inst, DTU Space, Elektrovej 328, DK-2800 Lyngby, Denmark
[5] Ohio State Univ, Dept Astron, 4055 McPherson Lab,140 West 18th Ave, Columbus, OH 43210 USA
[6] Ball Aerosp & Technol Corp, 1600 Commerce St, Boulder, CO 80301 USA
[7] Lowell Observ, 1400 West Mars Hill Rd, Flagstaff, AZ 86001 USA
[8] Boston Univ, Dept Astron, 725 Commonwealth Ave, Boston, MA 02215 USA
基金
美国国家科学基金会;
关键词
High-resolution spectroscopy; Radial velocity; Astronomy data analysis; Observational astronomy; EXTRACTION;
D O I
10.3847/1538-3881/ab7e31
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The EXtreme-PREcision Spectrograph (EXPRES) is an environmentally stabilized, fiber-fed, R = 137,500, optical spectrograph. It was recently commissioned at the 4.3 m Lowell Discovery Telescope near Flagstaff, Arizona. The spectrograph was designed with a target radial-velocity (RV) precision of 30 cm s(-1). In addition to instrumental innovations, the EXPRES pipeline, presented here, is the first on-sky, optical, fiber-fed spectrograph to employ many novel techniques-including an "extended flat" fiber used for wavelength-dependent quantum efficiency characterization of the CCD, a flat-relative optimal extraction algorithm, chromatic barycentric corrections, chromatic calibration offsets, and an ultra-precise laser frequency comb for wavelength calibration. We describe the reduction, calibration, and RV analysis pipeline used for EXPRES and present an example of our current sub-meter-per-second RV measurement precision, which reaches a formal, single-measurement error of 0.3 m s(-1) for an observation with a per-pixel signal-to-noise ratio of 250. These velocities yield an orbital solution on the known exoplanet host 51 Peg that matches literature values with a residual rms of 0.895 m s(-1).
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页数:14
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