CO Ice at 30 K
| Sample Type | Ice |
|---|---|
| Components | CO |
| Ratio | 1 |
| Substrate | CsI |
| Phase / State | |
| Reference Temperature | 30 K |
| Wavenumber (cm⁻¹) | 2002.11 - 2197.88 |
| Wavelength (µm) | 4.55 - 4.995 |
Carbon monoxide (CO) ice deposited at 10 K onto a cesium iodide (CsI) substrate, then warmed up to 30 K, and held at 30 K during spectroscopic measurements.
The real (n) and imaginary (k) parts of the complex index of refraction were determined using optical measurements done at a temperature of 30 K, by infrared transmission spectroscopy from 2198 to 2002 cm⁻¹ with a resolution of 1 cm⁻¹.
More information can be found in the publication and on the OCdb contributor's page.
Any use of this data should recognize the parent publication(s):
Ehrenfreund, P., Boogert, A. C. A., Gerakines, P. A., Tielens, A. G. G. M. and van Dishoeck, E. F. (1997) 'Infrared spectroscopy of interstellar apolar ice analogs', Astronomy and Astrophysics, 328, pp. 649-669.
n/k Values
Compatible Datasets (i.e., same molecule, phase, and temperature) are marked with *
| Select | Chemical | Ratio | Phase / State | T (K) | Wavelength Min (µm) |
Wavelength Max (µm) |
Compatible | n | k | Reference |
|---|---|---|---|---|---|---|---|---|---|---|
|
|
CO | 1 | 10 | 4.547 | 4.996 | ✓ | ✓ | Ehrenfreund et al. (1997) | ||
|
|
CO | 1 | 10 | 4.577 | 4.751 | ✓ | ✓ | Hudgins et al. (1993) | ||
|
|
CO | 1 | Amorphous | 12 | 4.472 | 4.86 | ✓ | ✓ | Elsila et al. (1997) | |
|
|
CO | 1 | 12.5 | 3.846 | 5.556 | ✓ | ✓ | Baratta and Palumbo (1998) | ||
|
|
CO | 1 | 15 | 3.846 | 5.882 | ✓ | ✓ | Palumbo et al. (2006) | ||
|
|
CO | 1 | Crystalline | 25 | 3.333 | 6.667 | ✓ | ✓ | Gerakines et al. (2023) | |
|
|
CO | 1 | Crystalline | 25 | 3.333 | 6.667 | ✓ | ✓ | Gerakines et al. (2023) | |
|
|
CO | 1 | 28 | 25.005 | 1602.533 | ✓ | ✓ | Gavdush et al. (2022) | ||
|
|
CO | 1 | 28.5 | 128.989 | 21025.27 | ✓ | ✓ | Giuliano et al. (2019) | ||
|
|
CO | 1 | 31.2 | 128.9 | 21010.72 | ✓ | ✓ | Giuliano et al. (2019) | ||
|
|
CO | 1 | 33.1 | 141.964 | 1500.766 | ✓ | ✓ | Giuliano et al. (2019) |