Abstract

Precise calibrations are needed for high-resolution near-infrared astronomical spectrographs. We have measured the wavenumbers of over 7500 uranium emission lines and used a subset of them to make precise radial velocity measurements.

© 2011 Optical Society of America

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References

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  1. F. Kerber, G. Nave, and C. J. Sansonetti, “Th-Ar Wavelength Standards for the Near-IR,” APJSS, 178, 374–384 (2008).
    [Crossref]
  2. S. Mahadevan, L. Ramsey, A. Wolszczan, J. Wright, M. Endl, and S. Redman, “The Habitable Zone Planet Finder: A Proposed High Resolution NIR Spectrograph For The Het To Discover Low Mass Exoplanets Around M Stars” in American Astronomical Society Meeting Abstracts, 215 (2010).
  3. S. L. Redman, J. E. Lawler, G. Nave, L. W. Ramsey, and S. Mahadevan, “The infrared spectrum of uranium from 850 to 5000 nm,” (in preparation).

2010 (1)

S. Mahadevan, L. Ramsey, A. Wolszczan, J. Wright, M. Endl, and S. Redman, “The Habitable Zone Planet Finder: A Proposed High Resolution NIR Spectrograph For The Het To Discover Low Mass Exoplanets Around M Stars” in American Astronomical Society Meeting Abstracts, 215 (2010).

2008 (1)

F. Kerber, G. Nave, and C. J. Sansonetti, “Th-Ar Wavelength Standards for the Near-IR,” APJSS, 178, 374–384 (2008).
[Crossref]

Endl, M.

S. Mahadevan, L. Ramsey, A. Wolszczan, J. Wright, M. Endl, and S. Redman, “The Habitable Zone Planet Finder: A Proposed High Resolution NIR Spectrograph For The Het To Discover Low Mass Exoplanets Around M Stars” in American Astronomical Society Meeting Abstracts, 215 (2010).

Kerber, F.

F. Kerber, G. Nave, and C. J. Sansonetti, “Th-Ar Wavelength Standards for the Near-IR,” APJSS, 178, 374–384 (2008).
[Crossref]

Lawler, J. E.

S. L. Redman, J. E. Lawler, G. Nave, L. W. Ramsey, and S. Mahadevan, “The infrared spectrum of uranium from 850 to 5000 nm,” (in preparation).

Mahadevan, S.

S. Mahadevan, L. Ramsey, A. Wolszczan, J. Wright, M. Endl, and S. Redman, “The Habitable Zone Planet Finder: A Proposed High Resolution NIR Spectrograph For The Het To Discover Low Mass Exoplanets Around M Stars” in American Astronomical Society Meeting Abstracts, 215 (2010).

S. L. Redman, J. E. Lawler, G. Nave, L. W. Ramsey, and S. Mahadevan, “The infrared spectrum of uranium from 850 to 5000 nm,” (in preparation).

Nave, G.

F. Kerber, G. Nave, and C. J. Sansonetti, “Th-Ar Wavelength Standards for the Near-IR,” APJSS, 178, 374–384 (2008).
[Crossref]

S. L. Redman, J. E. Lawler, G. Nave, L. W. Ramsey, and S. Mahadevan, “The infrared spectrum of uranium from 850 to 5000 nm,” (in preparation).

Ramsey, L.

S. Mahadevan, L. Ramsey, A. Wolszczan, J. Wright, M. Endl, and S. Redman, “The Habitable Zone Planet Finder: A Proposed High Resolution NIR Spectrograph For The Het To Discover Low Mass Exoplanets Around M Stars” in American Astronomical Society Meeting Abstracts, 215 (2010).

Ramsey, L. W.

S. L. Redman, J. E. Lawler, G. Nave, L. W. Ramsey, and S. Mahadevan, “The infrared spectrum of uranium from 850 to 5000 nm,” (in preparation).

Redman, S.

S. Mahadevan, L. Ramsey, A. Wolszczan, J. Wright, M. Endl, and S. Redman, “The Habitable Zone Planet Finder: A Proposed High Resolution NIR Spectrograph For The Het To Discover Low Mass Exoplanets Around M Stars” in American Astronomical Society Meeting Abstracts, 215 (2010).

Redman, S. L.

S. L. Redman, J. E. Lawler, G. Nave, L. W. Ramsey, and S. Mahadevan, “The infrared spectrum of uranium from 850 to 5000 nm,” (in preparation).

Sansonetti, C. J.

F. Kerber, G. Nave, and C. J. Sansonetti, “Th-Ar Wavelength Standards for the Near-IR,” APJSS, 178, 374–384 (2008).
[Crossref]

Wolszczan, A.

S. Mahadevan, L. Ramsey, A. Wolszczan, J. Wright, M. Endl, and S. Redman, “The Habitable Zone Planet Finder: A Proposed High Resolution NIR Spectrograph For The Het To Discover Low Mass Exoplanets Around M Stars” in American Astronomical Society Meeting Abstracts, 215 (2010).

Wright, J.

S. Mahadevan, L. Ramsey, A. Wolszczan, J. Wright, M. Endl, and S. Redman, “The Habitable Zone Planet Finder: A Proposed High Resolution NIR Spectrograph For The Het To Discover Low Mass Exoplanets Around M Stars” in American Astronomical Society Meeting Abstracts, 215 (2010).

American Astronomical Society Meeting Abstracts (1)

S. Mahadevan, L. Ramsey, A. Wolszczan, J. Wright, M. Endl, and S. Redman, “The Habitable Zone Planet Finder: A Proposed High Resolution NIR Spectrograph For The Het To Discover Low Mass Exoplanets Around M Stars” in American Astronomical Society Meeting Abstracts, 215 (2010).

APJSS (1)

F. Kerber, G. Nave, and C. J. Sansonetti, “Th-Ar Wavelength Standards for the Near-IR,” APJSS, 178, 374–384 (2008).
[Crossref]

The infrared spectrum of uranium from 850 to 5000 nm (1)

S. L. Redman, J. E. Lawler, G. Nave, L. W. Ramsey, and S. Mahadevan, “The infrared spectrum of uranium from 850 to 5000 nm,” (in preparation).