4 research outputs found
An update to the MARVEL data set and ExoMol line list for ¹²C₂
The spectrum of dicarbon (C_{2}) is important in astrophysics and for spectroscopic studies of plasmas and flames. The C_{2} spectrum is characterized by many band systems with new ones still being actively identified; astronomical observations involve eight of these bands. Recently, Furtenbacher et al. presented a set of 5699 empirical energy levels for {12}^C_{2}, distributed among 11 electronic states and 98 vibronic bands, derived from 42 experimental studies and obtained using the MARVEL (Measured Active Rotational-Vibrational Energy Levels) procedure. Here, we add data from 13 new sources and update data from 5 sources. Many of these data sources characterize high-lying electronic states, including the newly detected 3 {3}^Π_{g} state. Older studies have been included following improvements in the MARVEL procedure that allow their uncertainties to be estimated. These older works in particular determine levels in the C {1}^Π_{g} state, the upper state of the insufficiently characterized Deslandres–d’Azambuja (C {1}^Π_{g}–A {1}^Π_{u}) band. The new compilation considers a total of 31 323 transitions and derives 7047 empirical (MARVEL) energy levels spanning 20 electronic and 142 vibronic states. These new empirical energy levels are used here to update the 8states C_{2} ExoMol line list This updated line list is highly suitable for high-resolution cross-correlation studies in astronomical spectroscopy of, for example, exoplanets, as 99.4 per cent of the transitions with intensities over 10^{−18} cm molecule^{−1} at 1000 K have frequencies determined by empirical energy levels
MARVEL Analysis of the Measured High-Resolution Rovibronic Spectra of 90Zr16O
Zirconium oxide(ZrO) is an important astrophysical molecule that defines the
S-star classification class for cool giant stars. Accurate, empirical
rovibronic energy levels, with associated labels and uncertainties, are
reported for 9 low-lying electronic states of the diatomic 90Zr16O molecule.
These 8088 empirical energy levels are determined using the Marvel (Measured
Active Rotational-Vibrational Energy Levels) algorithm with 23 317 input
assigned transition frequencies, 22 549 of which were validated. A
temperature-dependent partition function is presented alongside updated
spectroscopic constants for the 9 low-lying electronic states
MARVEL Analysis of the Measured High-resolution Rovibronic Spectra of (ZrO)-Zr-90-O-16
Zirconium oxide (ZrO) is an important astrophysical molecule that defines the S-star classification class for cool
giant stars. Accurate, empirical rovibronic energy levels, with associated labels and uncertainties, are reported for
nine low-lying electronic states of the diatomic 90 16 Zr O molecule. These 8088 empirical energy levels are
determined using the Measured Active Rotational-Vibrational Energy Levels algorithm with 23,317 input assigned
transition frequencies, 22,549 of which were validated during this study. A temperature-dependent partition
function is presented alongside updated spectroscopic constants for the nine low-lying electronic states