Near infrared spectroscopy of carbon dioxide I. 16O12C16O line positions

Miller, Charles E.; Brown, Linda R.

doi:10.1016/j.jms.2003.11.001

Cited by 113 publications

(107 citation statements)

References 65 publications

Supporting

Mentioning

100

Contrasting

Order By: Relevance

“…The H-band itself was defined as the atmospheric transmission window between the strong and broad water absorption bands at ∼1.4 μm and ∼1.9 μm. By far, the lowest absorption in this region is in the range of approximately 1.5-1.75 μm, although this region is punctuated by the 30013 ← 00001 and 30012 ← 00001 bands 54 of the CO 2 molecule (Miller & Brown 2004), which cover roughly the ll -1.568 1.586 and ll -1.598 1.617 μm spectral intervals, respectively (Figure 2). An initial, two-detector Figure 2.…”

mentioning

confidence: 99%

The Apache Point Observatory Galactic Evolution Experiment (APOGEE)

et al. 2017

View full text Add to dashboard Cite

The Apache Point Observatory Galactic Evolution Experiment (APOGEE), one of the programs in the Sloan Digital Sky Survey III (SDSS-III), has now completed its systematic, homogeneous spectroscopic survey sampling all major populations of the Milky Way. After a three-year observing campaign on the Sloan 2.5 m Telescope, APOGEE has collected a half million high-resolution (R ∼ 22,500), high signal-to-noise ratio (>100), infrared (1.51–1.70 μm) spectra for 146,000 stars, with time series information via repeat visits to most of these stars. This paper describes the motivations for the survey and its overall design—hardware, field placement, target selection, operations—and gives an overview of these aspects as well as the data reduction, analysis, and products. An index is also given to the complement of technical papers that describe various critical survey components in detail. Finally, we discuss the achieved survey performance and illustrate the variety of potential uses of the data products by way of a number of science demonstrations, which span from time series analysis of stellar spectral variations and radial velocity variations from stellar companions, to spatial maps of kinematics, metallicity, and abundance patterns across the Galaxy and as a function of age, to new views of the interstellar medium, the chemistry of star clusters, and the discovery of rare stellar species. As part of SDSS-III Data Release 12 and later releases, all of the APOGEE data products are publicly available.

show abstract

mentioning

confidence: 99%

The Apache Point Observatory Galactic Evolution Experiment (APOGEE)

et al. 2017

View full text Add to dashboard Cite

show abstract

“…In regions containing an insufficient number of water absorption lines, separate measurements were performed with a small quantity of a calibrating gas, CO 2 or NH 3 , in the CEA chamber. The positions of the absorption lines of CO 2 [61] were also obtained from the HITRAN database [54]. The uncertainty in the positions of CO 2 lines is quoted as being between 0.0001 and 0.001 cm -1 .…”

Section: Wavelength Calibration and Accuracymentioning

confidence: 99%

The near infrared cavity-enhanced absorption spectrum of methyl cyanide

O’Leary

Ruth

Dixneuf

et al. 2012

Journal of Quantitative Spectroscopy and Radiative Transfer

View full text Add to dashboard Cite

“…We are also planning to incorporate the ongoing high-resolution work of Miller and Brown [26] between 4000 to 9000 cm"'. It should be remarked that some of these aforementioned works will enable us to replace carbon dioxide line positions in HITRAN that were derived from observations of Venus by Mandin [25].…”

Section: Hitranmentioning

confidence: 99%

Atmospheric Absorption Parameters for Laser Propagation

Rothman¹

2005

View full text Add to dashboard Cite

Near infrared spectroscopy of carbon dioxide I. 16O12C16O line positions

Cited by 113 publications

References 65 publications

The Apache Point Observatory Galactic Evolution Experiment (APOGEE)

The Apache Point Observatory Galactic Evolution Experiment (APOGEE)

The near infrared cavity-enhanced absorption spectrum of methyl cyanide

Atmospheric Absorption Parameters for Laser Propagation

Contact Info

Product

Resources

About