C. Western

activity

20152019

_{2}

from 4,500 to 15,700 cm

^{- 1}

revisited with PGOPHER

60 citations · 60 across the 2 of their papers we have counts for

collaborators

3 papers

physics.chem-ph2019★ 60 cited

The spectrum of N $_{2}$ from 4,500 to 15,700 cm $^{- 1}$ revisited with PGOPHER

Colin Western, Luke Carter-Blatchford, Patrick Crozet +3

Using a reference molecular atlas to ensure self-consistency of wavelength calibration is widespread practice. Boesch \& Reiners (Astronomy \& Astrophysics 582 A43 (2015)) reported…

astro-ph.EP2018

Rotational Temperature Modeling of the Swan $Δ ν = 0$ Band Sequence in Comet 122P/de~Vico

Tyler Nelson, Anita L. Cochran, Colin Western

We modeled observations of the C $_{2}$ $d^{3} Π_{g} - a^{3} Π_{u}$ (Swan) $Δ ν = 0$ sequence observed in spectra of comet 122P/de Vico obtained with the 2.7m Harlan J. Smith…

astro-ph.SR2015

Line Strengths of Rovibrational and Rotational Transitions in the X $^{2} Π$ Ground State of OH

James S. A. Brooke, Peter F. Bernath, Colin M. Western +4

A new line list including positions and absolute intensities (in the form of Einstein $A$ values and oscillator strengths) has been produced for the OH ground X\DP\ state rovibrati…

The spectrum of N2​ from 4,500 to 15,700 cm−1 revisited with PGOPHER

Rotational Temperature Modeling of the Swan Δν=0 Band Sequence in Comet 122P/de~Vico

Line Strengths of Rovibrational and Rotational Transitions in the X2Π Ground State of OH

The spectrum of N $_{2}$ from 4,500 to 15,700 cm $^{- 1}$ revisited with PGOPHER

Rotational Temperature Modeling of the Swan $Δ ν = 0$ Band Sequence in Comet 122P/de~Vico

Line Strengths of Rovibrational and Rotational Transitions in the X $^{2} Π$ Ground State of OH