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Emission-line spectroscopy in NGC 891
The observed scale heights of extraplanar diffuse ionized gas (eDIG) layers exceed their thermal scale heights by a factor of a few in the Milky Way and other nearby edge-on... -
Extremely metal-poor galaxies in SDSS. II.
Extremely metal-poor (XMP) galaxies are defined to have a gas-phase metallicity smaller than a tenth of the solar value (12+log[O/H]<7.69). They are uncommon, chemically and... -
Star-forming z~2.1 galaxy metallicities
We explore the evolution of the Stellar Mass-Star Formation Rate (SFR)-Metallicity relation using a set of 256 COSMOS and GOODS galaxies in the redshift range 1.90<z<2.35.... -
Stacked spectra of SDSS star forming galaxies
The relation between galaxy stellar mass and gas-phase metallicity is a sensitive diagnostic of the main processes that drive galaxy evolution, namely cosmological gas inflow,... -
Spectroscopic survey of bright white dwarfs
We have conducted a spectroscopic survey of over 1300 bright (V<=17.5), hydrogen-rich white dwarfs based largely on the last published version of the McCook & Sion... -
Infrared absorbance of water H_2_O/H_2_O_2_ ice
Recent surface chemistry experiments have shown that the hydrogenation of molecular oxygen on interstellar dust grains is a plausible formation mechanism, via hydrogen peroxide... -
NIR spectroscopy of five dwarf galaxies
We present near-infrared (NIR) spectroscopic observations of five blue compact dwarf (BCD) galaxies, II Zw 40, Mrk 71, Mrk 930, Mrk 996, and SBS 0335-052E. The NIR spectra which... -
VIRUS-P spectroscopy of NGC 5194
We investigate the relation between the star formation rate (SFR) surface density ({Sigma}SFR) and the mass surface density of gas ({Sigma}gas) in NGC 5194 (a.k.a. M51a,... -
Line-strength indices for 74 early-type galaxies
We present line-strength measurements for 74 early-type galaxies in the core of the Coma cluster reaching down to velocity dispersions, {sigma}, of 30km/s. The index-{sigma}... -
Mid-IR spectrum of star-forming galaxies
We present a sample of low-resolution 5-38um Spitzer IRS spectra of the inner few square kiloparsecs of 59 nearby galaxies spanning a large range of star formation properties. A... -
Spectrophotometry in NGC 5253
We present echelle spectrophotometry of the blue compact dwarf galaxy NGC 5253 obtained with the VLT UVES. We have measured the intensities of a large number of permitted and... -
Wolf-Rayet galaxies in the SDSS
We use a large sample of 174 Wolf-Rayet (W-R) galaxies drawn from the Sloan Digital Sky Survey to study whether and how the slope of the stellar initial mass function depends on... -
Fundamental manifold of spheroids
We present a unifying empirical description of the structural and kinematic properties of all spheroids embedded in dark matter halos. We find that the intracluster stellar... -
Stellar mass in disk-dominated galaxies
We investigate the correlations among stellar mass (M), disk scale length (R_d_), and rotation velocity at 2.2 disk scale lengths (V_2.2_) for a sample of 81 disk-dominated... -
Line indices for 124 early-type galaxies
The aim of this paper is to set constraints on the epochs of early-type galaxy formation through the "archaeology" of the stellar populations in local galaxies. Using our models... -
HST observations of carbon in spiral galaxies
We present measurements of the gas-phase abundance ratio C/O in six H II regions in the spiral galaxies M101 and NGC 2403, based on ultraviolet spectroscopy using the Faint... -
Line strengths and gradients in S0 galaxies
Line strengths and their gradients in Mg, Fe, and HBeta have been determined for a sample of 20 S0 galaxies in order to study the stellar populations of their bulges and disks... -
LAMOST/SP_Ace DR1 catalog
We present a new analysis of the LAMOST DR1 survey spectral database performed with the code SP_Ace, which provides the derived stellar parameters Teff, logg, [Fe/H], and... -
Stellar nuclei and bulges of nearby S0 galaxies
I analyze statistics of the stellar population properties for stellar nuclei and bulges of nearby lenticular galaxies in different environments by using panoramic spectral data... -
Precision spectrophotometry at the level of 0.1%
Accurate relative spectrophotometry is critical for many science applications. Small wavelength-scale residuals in the flux calibration can significantly impact the measurements...