(Extract from the Executive Summary) Humanity stands at the threshold of answering one of its most profound questions: Does life exist beyond Earth?
Interferometer
A Preliminary Exploration Of The Effects Of Baseline Length For The LIFE Space Mission
By aiming to find and characterise dozens of habitable exoplanets through the technique of nulling interferometry, the LIFE space mission will produce transformational science. One of the key parameters for […]
Observations Of Complex Organic Molecules In The Gas Phase Of The Interstellar Medium
Thanks to the advent of sensitive and broad bandwidth instrumentation, complex organic molecules (COMs) have been found in a wide variety of interstellar environments, not only in our Galaxy but […]
A Signal Discovery Step In Interstellar Communication
Prior work using synchronized, geographically spaced radio telescopes, and a radio interferometer, suggests that narrow-bandwidth polarized pulse pair measurements repeatedly falsify a noise-cause hypothesis, given a prior celestial direction of […]
Conducting High Frequency Radio SETI Using ALMA
The Atacama Millimeter/Submillimeter Array (ALMA) remains unparalleled in sensitivity at radio frequencies above 35 GHz.
Kilometer-baseline Interferometry: Science Drivers For The Next Generation Instrument
Infrared interferometry has seen a revolution over the last few years. The advent of GRAVITY+ is about to enable high-contrast observations, all-sky coverage and faint science up to K=21, with […]
The James Webb Interferometer: Space-based Interferometric Detections of PDS 70 b and c at 4.8 μm
We observed the planet-hosting system PDS 70 with the James Webb Interferometer, JWST’s Aperture Masking Interferometric (AMI) mode within NIRISS.
Octofitter: Fast, Flexible, and Accurate Orbit Modelling to Detect Exoplanets
As next-generation imaging instruments and interferometers search for planets closer to their stars, they must contend with increasing orbital motion and longer integration times. These compounding effects make it difficult […]
Large Interferometer For Exoplanets (LIFE): VIII. Where is the phosphine? Observing exoplanetary PH3 with a space based MIR nulling interferometer
Phosphine could be a key molecule in the understanding of exotic chemistry happening in (exo)planetary atmospheres. While it has been detected in the Solar System’s giant planets, it has not […]
Large Interferometer For Exoplanets (LIFE): VIII. Detecting Rocky Exoplanets In The Habitable Zones Of Sun-like Stars
While previous studies have shown a strong preference for a future mid-infrared nulling interferometer space mission to detect habitable zone planets around M-dwarfs, we here focus on a more conservative […]
