Latest Images
Top row: TPD of 13CO (m/z = 29) used to calcula...
Top two rows: the temperature-programmed desorp...
Top panels: variation of the IR features throug...
Top panels: variation of the IR features throug...
The temporal behavior of CO2 (top panel), CO (m...
The infrared spectral bands of CO2 (left), CO (...
Top: the three 15N2 TPD curves from the three r...
A summary of the CO and N2 reported in various ...
The TPD of 13CO (m/z = 29 top row) and 15N2 (m/...
The temporal behavior of CO2 (top panel), CO (m...
A summary of the CO and N2 formed following irr...
A summary of the CO and N2 formed following ele...
The temporal behavior of CO2 (top panel), CO (m...
A summary of the CO and N2 formed following irr...
Top: the change in the spectral features throug...
The infrared spectral bands of CO2 (left), CO (...
The infrared spectra of various ices throughout...
LX–M* relations for observed and simulated BGGs...
Top panels: BGG redshift distributions. Simulat...
BGG stellar mass distributions illustrated by n...
BGG sSFR distributions. The top panel depicts t...
BGG mass-weighted stellar age (Agew) distributi...
sSFR–M* relations for samples of BGGs with ...
BGG quenched fractions. BGGs are considered que...
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