The transient mid-infrared sky: Revealing the enshrouded births,
deaths and afterlives of stars through cosmic time
The growth of mass in stars and supermassive black holes (SMBHs) underpins every
area of astrophysics. It is now becoming increasingly clear that short-lived transient
outbursts caused by eruptive mass transfer episodes likely dominate the growth
processes. Yet, direct observations remain severely limited either due to their
intrinsically red emission, or absorption due to intervening dust and gas which make
these phenomena invisible in optical/X-ray time domain surveys. In this talk, I will
present the WISE transient pipeline -- a novel effort aimed at a systematic all-sky
census of the dynamic mid-infrared sky using more than a decade of data from the
NEOWISE space mission. Utilizing the highest spatial resolution images together with
state-of-the art image subtraction algorithms, we have created a statistically
complete sample of 15 million infrared transients in NEOWISE data.
Embarking on a large ground-based follow-up program, I will present results
from multi-wavelength characterization of the brightest mid-infrared
transients, revealing i) a complete census of proto-stellar growth through
transient outbursts, ii) a new class of dust obscured stellar mergers in low mass
stars, iii) new insights into the fiery fates of close planetary systems, iv)
missed tidal disruption events by SMBHs in nearby galaxies and iv) highly
variable accretion outbursts in Active Galactic Nuclei in the near and distant
universe.
The Transient Mid-infrared Sky Revealing the Enshrouded Births