The (supermassive black hole mass, MBH)–(bulge stellar mass, M, sph*) relation is,
obviously, derived using two quantities. We endeavor to provide accurate values for the …

Modern astronomy has been rapidly increasing our ability to see deeper into the Universe,
acquiring enormous samples of cosmic populations. Gaining astrophysical insights from …

Current observational evidence suggests that all large galaxies contain globular clusters
(GCs), while the smallest galaxies do not. Over what galaxy mass range does the transition …

One of the primary goals for the upcoming James Webb Space Telescope is to observe the
first galaxies. Predictions for planned and proposed surveys have typically focused on …

Two of the main problems encountered in the development and accurate validation of
photometric redshift (photo-z) techniques are the lack of spectroscopic coverage in the …

Galaxy stellar mass is known to be monotonically related to the size of the galaxy's globular
cluster (GC) population for Milky Way sized and larger galaxies. However, the relation …

Star formation rate (SFR) distributions of galaxies are often assumed to be bimodal with
modes corresponding to star-forming and quiescent galaxies, respectively. Both classes of …

The measurement of Hubble constant (H 0) is clearly a very important task in astrophysics
and cosmology. Based on the principle of minimization of the information loss, we propose a …

Aims. We intended to quantify the impact of stellar multiplicity on the presence and
properties of exoplanets. Methods. We investigated all exoplanet host stars at less than 100 …

Bayesian inference gets its name from Bayes's theorem, expressing posterior probabilities
for hypotheses about a data generating process as the (normalized) product of prior …