Speaker
Description
Accurate stellar velocity dispersion measurements are of great importance for
understanding the dynamical masses, evolutionary stages, and are fundamen-
tal in studying the gravitational potential of galaxies. The accuracy of these
measurements depends on the coverage of the spectrograph, the redshift, the
signal-to-noise ratio (SNR), and the wavelength range used to perform the
measurement. To find conditions that produce accurate stellar velocity dis-
persion measurements for upcoming spectroscopic surveys (e.g., 4MOST), we
generated realistic mock spectra using the Flexible Stellar Population Synthesis
(FSPS) model for different redshifts, SNRs, and velocity dispersions. We then
performed velocity dispersion measurements using the Penalized PiXel-Fitting
(pPXF) code in different wavelength ranges between 3700 ˚A and 9000 ˚A.
| Apply for student award at which level: | PhD |
|---|---|
| Consent on use of personal information: Abstract Submission | Yes, I ACCEPT |