Precise Near-Infrared Radial Velocities

Peter Plavchan; Peter Gao; Jonathan Gagne; Elise Furlan; Carolyn Brinkworth; Michael Bottom; Angelle Tanner; Guillem Anglada-Escude; Russel White; Cassy Davison; Sean Mills; Chas Beichman; John Asher Johnson; David Ciardi; Kent Wallace; Bertrand Mennesson; Gautam Vasisht; Lisa Prato; Stephen Kane; Sam Crawford; Tim Crawford; Keeyoon Sung; Brian Drouin; Sean Lin; Stephanie Leifer; Joe Catanzarite; Todd Henry; Kaspar Von Braun; Bernie Walp; Claire Geneser; Nick Ogden; Andrew Stufflebeam; Garrett Pohl; Joe Regan

doi:10.1017/S1743921315006468

Precise Near-Infrared Radial Velocities

Peter Plavchan, Peter Gao, Jonathan Gagne, Elise Furlan, Carolyn Brinkworth, Michael Bottom, Angelle Tanner, Guillem Anglada-Escude, Russel White, Cassy Davison, Sean Mills, Chas Beichman, John Asher Johnson, David Ciardi, Kent Wallace, Bertrand Mennesson, Gautam Vasisht, Lisa Prato, Stephen Kane, Sam CrawfordTim Crawford, Keeyoon Sung, Brian Drouin, Sean Lin, Stephanie Leifer, Joe Catanzarite, Todd Henry, Kaspar Von Braun, Bernie Walp, Claire Geneser, Nick Ogden, Andrew Stufflebeam, Garrett Pohl, Joe Regan

Research output: Contribution to journal › Article › peer-review

Abstract

We present the results of two 2.3 μm near-infrared (NIR) radial velocity (RV) surveys to detect exoplanets around 36 nearby and young M dwarfs. We use the CSHELL spectrograph (R ∼ 46,000) at the NASA InfraRed Telescope Facility (IRTF), combined with an isotopic methane absorption gas cell for common optical path relative wavelength calibration. We have developed a sophisticated RV forward modeling code that accounts for fringing and other instrumental artifacts present in the spectra. With a spectral grasp of only 5 nm, we are able to reach long-term radial velocity dispersions of ∼20-30 m s^-1 on our survey targets.

Original language	English
Pages (from-to)	286-287
Number of pages	2
Journal	Proceedings of the International Astronomical Union
Volume	10
DOIs	https://doi.org/10.1017/S1743921315006468
State	Published - 2015
Externally published	Yes

Keywords

instrumentation: spectrographs
techniques: radial velocities

Access to Document

10.1017/S1743921315006468

Cite this

Plavchan, P., Gao, P., Gagne, J., Furlan, E., Brinkworth, C., Bottom, M., Tanner, A., Anglada-Escude, G., White, R., Davison, C., Mills, S., Beichman, C., Johnson, J. A., Ciardi, D., Wallace, K., Mennesson, B., Vasisht, G., Prato, L., Kane, S., ... Regan, J. (2015). Precise Near-Infrared Radial Velocities. Proceedings of the International Astronomical Union, 10, 286-287. https://doi.org/10.1017/S1743921315006468

@article{d36130cebe3a4f5c9b6b9a88e19ec51c,

title = "Precise Near-Infrared Radial Velocities",

abstract = "We present the results of two 2.3 μm near-infrared (NIR) radial velocity (RV) surveys to detect exoplanets around 36 nearby and young M dwarfs. We use the CSHELL spectrograph (R ∼ 46,000) at the NASA InfraRed Telescope Facility (IRTF), combined with an isotopic methane absorption gas cell for common optical path relative wavelength calibration. We have developed a sophisticated RV forward modeling code that accounts for fringing and other instrumental artifacts present in the spectra. With a spectral grasp of only 5 nm, we are able to reach long-term radial velocity dispersions of ∼20-30 m s-1 on our survey targets.",

keywords = "instrumentation: spectrographs, techniques: radial velocities",

author = "Peter Plavchan and Peter Gao and Jonathan Gagne and Elise Furlan and Carolyn Brinkworth and Michael Bottom and Angelle Tanner and Guillem Anglada-Escude and Russel White and Cassy Davison and Sean Mills and Chas Beichman and Johnson, \{John Asher\} and David Ciardi and Kent Wallace and Bertrand Mennesson and Gautam Vasisht and Lisa Prato and Stephen Kane and Sam Crawford and Tim Crawford and Keeyoon Sung and Brian Drouin and Sean Lin and Stephanie Leifer and Joe Catanzarite and Todd Henry and \{Von Braun\}, Kaspar and Bernie Walp and Claire Geneser and Nick Ogden and Andrew Stufflebeam and Garrett Pohl and Joe Regan",

note = "Publisher Copyright: {\textcopyright} 2016 International Astronomical Union.",

year = "2015",

doi = "10.1017/S1743921315006468",

language = "English",

volume = "10",

pages = "286--287",

journal = "Proceedings of the International Astronomical Union",

issn = "1743-9213",

publisher = "Cambridge University Press",

}

Plavchan, P, Gao, P, Gagne, J, Furlan, E, Brinkworth, C, Bottom, M, Tanner, A, Anglada-Escude, G, White, R, Davison, C, Mills, S, Beichman, C, Johnson, JA, Ciardi, D, Wallace, K, Mennesson, B, Vasisht, G, Prato, L, Kane, S, Crawford, S, Crawford, T, Sung, K, Drouin, B, Lin, S, Leifer, S, Catanzarite, J, Henry, T, Von Braun, K, Walp, B, Geneser, C, Ogden, N, Stufflebeam, A, Pohl, G & Regan, J 2015, 'Precise Near-Infrared Radial Velocities', Proceedings of the International Astronomical Union, vol. 10, pp. 286-287. https://doi.org/10.1017/S1743921315006468

TY - JOUR

T1 - Precise Near-Infrared Radial Velocities

AU - Plavchan, Peter

AU - Gao, Peter

AU - Gagne, Jonathan

AU - Furlan, Elise

AU - Brinkworth, Carolyn

AU - Bottom, Michael

AU - Tanner, Angelle

AU - Anglada-Escude, Guillem

AU - White, Russel

AU - Davison, Cassy

AU - Mills, Sean

AU - Beichman, Chas

AU - Johnson, John Asher

AU - Ciardi, David

AU - Wallace, Kent

AU - Mennesson, Bertrand

AU - Vasisht, Gautam

AU - Prato, Lisa

AU - Kane, Stephen

AU - Crawford, Sam

AU - Crawford, Tim

AU - Sung, Keeyoon

AU - Drouin, Brian

AU - Lin, Sean

AU - Leifer, Stephanie

AU - Catanzarite, Joe

AU - Henry, Todd

AU - Von Braun, Kaspar

AU - Walp, Bernie

AU - Geneser, Claire

AU - Ogden, Nick

AU - Stufflebeam, Andrew

AU - Pohl, Garrett

AU - Regan, Joe

PY - 2015

Y1 - 2015

N2 - We present the results of two 2.3 μm near-infrared (NIR) radial velocity (RV) surveys to detect exoplanets around 36 nearby and young M dwarfs. We use the CSHELL spectrograph (R ∼ 46,000) at the NASA InfraRed Telescope Facility (IRTF), combined with an isotopic methane absorption gas cell for common optical path relative wavelength calibration. We have developed a sophisticated RV forward modeling code that accounts for fringing and other instrumental artifacts present in the spectra. With a spectral grasp of only 5 nm, we are able to reach long-term radial velocity dispersions of ∼20-30 m s-1 on our survey targets.

AB - We present the results of two 2.3 μm near-infrared (NIR) radial velocity (RV) surveys to detect exoplanets around 36 nearby and young M dwarfs. We use the CSHELL spectrograph (R ∼ 46,000) at the NASA InfraRed Telescope Facility (IRTF), combined with an isotopic methane absorption gas cell for common optical path relative wavelength calibration. We have developed a sophisticated RV forward modeling code that accounts for fringing and other instrumental artifacts present in the spectra. With a spectral grasp of only 5 nm, we are able to reach long-term radial velocity dispersions of ∼20-30 m s-1 on our survey targets.

KW - instrumentation: spectrographs

KW - techniques: radial velocities

UR - https://www.scopus.com/pages/publications/84956494630

U2 - 10.1017/S1743921315006468

DO - 10.1017/S1743921315006468

M3 - Article

AN - SCOPUS:84956494630

SN - 1743-9213

VL - 10

SP - 286

EP - 287

JO - Proceedings of the International Astronomical Union

JF - Proceedings of the International Astronomical Union

ER -

Precise Near-Infrared Radial Velocities

Abstract

Keywords

Access to Document

Other files and links

Fingerprint

Cite this