PKS 1502+036 is a narrow-line Seyfert galaxy located in the constellation of Virgo. The redshift of the object has been estimated as (z) 0.408 and it was first discovered as a quasar with a flat radio spectrum by astronomers in 1997. It is described as radio-loud.
Description PKS 1502+036 is shown to be a gamma-ray emitting object, with one powerful flare displayed in late 2015 after a long period of low-activity with a measured low flux of 4.5×10−8 photon cm−2 s−1. By the time the flare reached a daily peak flux on December 20, 2015, the source had an estimated flux of (237±71)×10−8 photon cm−2 s−1 on a three-hour timescale which in turn, corresponds to a measured isotropic luminosity of (7.3±2.1)×1047 erg s−1. No signs of spectral changes were accompanying the flare, although an increase in optical, ultraviolet and X-ray activity was noted for the object. During intra-night optical monitoring, the source displayed short-term optical variability between April 21 and May 11, 2018, with a brightness change of 0.1 magnitude. The source of PKS 1502+036 is classified as compact double. When imaged with Very Long Baseline Array (VLBA) at 15 GHz, it has an extended radio structure indicative of a core-jet morphology, with radio emission being dominated by a compact radio core that is shown having low fractional polarization and a weak jet-like feature extending out by three milliarcseconds. A weak component with a separation of 3.05 milliarcseconds from its core, appears present in the source which was found undetected through previous observations. The radio spectrum of the source is classified as inverted. Near-infrared imaging obtained by Very Large Telescope, found PKS 1502+036 is an elliptical galaxy based on its surface brightness profile described by a combination of bulge and a nuclear component modelling. There is also a presence of an extended structure in a form of bright spots with position angles between 270 and 370 degrees indicative of galaxy mergers. On the other side of the galaxy center, a more dim extended bar-like structure is seen going from east-southeast to north direction. The supermassive black hole mass for the galaxy has been estimated as7×108 M☉ based on its near-infrared bulge luminosity. There is a close companion near the galaxy, however it isn't interacting with it.
References
External links PKS 1502+036 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images PKS 1502+036 on SIMBAD PKS 1502+036 on HyperLeda


