τ Boo b Archives

Orbital phase coverage for the observations of τ Boo b. The orbital phase was calculated using the ephemeris from Wang & Ford (2011) and is relative to periastron of τ Boo b. The LOFAR and NenuFAR observations are labeled in red and orange, respectively. The original LOFAR observations were taken between February 18, 2017 and March 25, 2017. The τ Boo LOFAR observations with the tentative detections are displayed as large dark-blue rectangles. The tentative detection of burst emission was seen on February 18, 2017 and the slow emission was seen on March 6, 2017. An arbitrary number of days was placed between the 2020 and 2017 observations for clarity. -- astro-ph.EP

Follow-up Radio Observations Of The τ Boötis Exoplanetary System: Preliminary Results From NenuFAR

by Keith CowingOctober 10, 2023October 10, 2023

Studying the magnetic fields of exoplanets will provide valuable information about their interior structures, atmospheric properties (escape and dynamics), and potential habitability.

τ Boo b

Follow-up Radio Observations Of The τ Boötis Exoplanetary System: Preliminary Results From NenuFAR

How A Deep-sea Protein Adapts To An Extreme Environment

Fingerprints Inside Our Sun Could Reveal If It Once Swallowed A Planet

Climates Of Gl 514 b

Cosmic Radiation at Flight Altitudes Rises When the Sun Is Less Active

The History Of Enzyme Evolution Embedded In Metabolism