Quantitative relationship between the trajectories of CMEs and evolution of their magnetic fields

Quantitative spectral analysis of early B-type supergiants in the Sculptor galaxy NGC 300

Quantitative spectral classification based on photoelectric spectrum scanner measurements of F-K stars.

Quantitative spectroscopic analysis of and distance to SN1999em

Quantitative spectroscopic criteria for the classification of pre-main sequence low-mass stars.

Quantitative Spectroscopy of 24 A supergiants in the Sculptor galaxy NGC 300: Flux weighted gravity luminosity relationship, metallicity and metallicity gradient

Quantitative spectroscopy of B supergiants in the Galaxy, the LMC and the SMC. I - The B0.5 IA supergiants Kappa Orionis, SK - 68 deg 41 and SK 159

Quantitative Spectroscopy of BA-type Supergiants

Quantitative Spectroscopy of Blue Supergiant Stars in the Disk of M81: Metallicity, Metallicity Gradient and Distance

Quantitative spectroscopy of close binary stars

Quantitative Spectroscopy of O Stars at Low Metallicity. O Dwarfs in NGC 346

Quantitative Spectroscopy of Starburst and Quasar Emission Line Regions

Quantitative Spectroscopy of Supergiants

Quantitative Spectroscopy of Supernovae for Dark Energy Studies

Quantitative spectroscopy of the HeI cluster in the Galactic center.

Quantitative Spektralanalyse des B2-Riesensterns Gamma Orionis

Quantitative Stellar Spectral Classification. II. Early Type Stars

Quantitative Stellar Spectral Classification. III. Spectral Resolution

Quantitative Stellar Spectral Classification. IV. Application to the Open Cluster IC 2391

Quantitative studies of the Far-UV, UV and optical spectra of late O and early B-type supergiants in the Magellanic Clouds