## Its mission is to measure sizes of known transiting exoplanets orbiting bright and nearby stars, but it will also have significant capability for asteroseismology, collecting high-cadence photometry with precision similar to that of Kepler and TESS (Moya et al.

Editorial: The Future of Asteroseismology

## Planetary materials orbiting white dwarf stars reveal the ultimate fate of the planets of the Solar System and all known transiting exoplanets.

The Search for Planet and Planetesimal Transits of White Dwarfs with the Zwicky Transient Facility.

## Young transiting exoplanets (< 100 Myr) provide crucial insight into atmospheric evolution via photoevaporation.

H-alpha and Ca II Infrared Triplet Variations During a Transit of the 23 Myr Planet V1298 Tau c

## Young transiting exoplanets (<100 Myr) provide crucial insight into atmospheric evolution via photoevaporation.

H-alpha and Ca ii Infrared Triplet Variations During a Transit of the 23 Myr Planet V1298 Tau c

## We establish limits for transiting exoplanets around both α Cen A and B using transit signal injection and recovery tests.

Transit Search for Exoplanets around Alpha Centauri A and B with ASTERIA

## with hours of high-cadence exposure time each night, is designed to find the rare events that require all-sky monitoring, including transiting exoplanets around exotic stars like white dwarfs and hot subdwarfs, stellar activity of all types within our galaxy, nearby supernovae, and other transient events such as gamma ray bursts and gravitational-wave electromagnetic counterparts.

Building the Evryscope: Hardware Design and Performance

## Measurements of the transmission spectra, dayside emission, and phase curves of transiting exoplanets, as well as the emission spectrum and light curves of directly imaged exoplanets and brown dwarfs have shown that aerosols are distributed inhomogeneously in exoplanet atmospheres, with aerosol distributions varying significantly with planet equilibrium temperature and gravity.

Aerosols in Exoplanet Atmospheres

## Spectroscopy of transiting exoplanets can be used to investigate their atmospheric properties and habitability.

A nearby transiting rocky exoplanet that is suitable for atmospheric investigation

## We present a new implementation of the commonly used Box-fitting Least Squares (BLS) algorithm, for the detection of transiting exoplanets in photometric data.

Sparse Box-fitting Least Squares

## Accurate measurements of these effects in transiting exoplanets could be used to test GR and to gain information about the planetary interiors.

Detecting general relativistic orbital precession in transiting hot Jupiters

10.1109/CONIT51480.2021.9498407

## Over 4000 such transiting exoplanets have been identified since the mission commenced in 2007.

Analysis of Kepler Objects of Interest using Machine Learning for Exoplanet Identification

## It is the first mission dedicated to measuring the chemical composition and thermal structures of the atmospheres of hundreds of transiting exoplanets, enabling planetary science far beyond the boundaries of our own Solar System.

The Ariel Instrument Control Unit

## During its 4-year mission, Ariel will observe the atmospheres of a large and diversified population of transiting exoplanets.

Determination of stellar parameters for Ariel targets: a comparison analysis between different spectroscopic methods

## Thousands of transiting exoplanets have already been detected orbiting a wide range of host stars, including the first planets that could potentially be similar to Earth.

Finding Signs of Life in Transits: High-resolution Transmission Spectra of Earth-line Planets around FGKM Host Stars

## In recent years, a vast increase in spectroscopic observations of transiting exoplanets has for the first time allowed us to search for broad trends in their atmospheric properties.

The curse of clouds

## <p>Multi-band photometric transit observations or low resolution spectroscopy (spectro-photometry) are normally used to retrieve the broadband transmission spectra of transiting exoplanets in order to assess the chemical composition of their atmospheres.

Retrieving the transmission spectrum of HD 209458b usingCHOCOLATE: a new Chromatic Doppler Tomography technique

## We present high-precision photometric observations of the transiting exoplanets HAT-P-40b and HAT-P-51b by the Rozhen 2-m telescope.

New observations and transit solutions of the inflated exoplanets HAT-P-40b and HAT-P-51b

## To increase the sample size of future atmospheric characterization efforts, we build on the planetary infrared excess (PIE) technique that has been proposed as a means to detect and characterize the thermal spectra of transiting and non-transiting exoplanets using sufficiently broad wavelength coverage to uniquely constrain the stellar and planetary spectral components from spatially unresolved observations.

Retrieving Exoplanet Atmospheres Using Planetary Infrared Excess: Prospects for the Night Side of WASP-43 b and Other Hot Jupiters

## Young transiting exoplanets (< 100 Myr) provide crucial insight into atmospheric evolution via photoevaporation.

H-alpha and Ca II Infrared Triplet Variations During a Transit of the 23 Myr Planet V1298 Tau c

## Young transiting exoplanets (<100 Myr) provide crucial insight into atmospheric evolution via photoevaporation.

H-alpha and Ca ii Infrared Triplet Variations During a Transit of the 23 Myr Planet V1298 Tau c

## In this work we used the available TESS data, multi-color photometry data obtained with theMulticolor Simultaneous Camera for studying Atmospheres of Transiting exoplanets 2 (MuSCAT2) and literature data to calculate the period change rate of WASP-43b and to improve its precision, and to refine the parameters of the WASP-43 planetary system.

Is the orbit of the exoplanet WASP-43b really decaying? TESS and MuSCAT2 observations confirm no detection

## Its mission is to measure sizes of known transiting exoplanets orbiting bright and nearby stars, but it will also have significant capability for asteroseismology, collecting high-cadence photometry with precision similar to that of Kepler and TESS (Moya et al.

Editorial: The Future of Asteroseismology

## We find the random scheduler leads to a more biased, less accurate, and less precise, estimation of the mass of the transiting exoplanets.

Scheduling strategies for the ESPRESSO follow-up of TESS targets

## Currently, in-depth atmospheric characterization of transiting exoplanets entails the use of spectrographs on large telescopes, requiring significant observing time to study each planet.

On the Utility of Transmission Color Analysis i: Differentiating Super-Earths and Sub-Neptunes

## We establish limits for transiting exoplanets around both α Cen A and B using transit signal injection and recovery tests.

Transit Search for Exoplanets around Alpha Centauri A and B with ASTERIA

## The planet was detected using photometric data from the Transiting Exoplanet Survey Satellite and followed up with observations from the Las Cumbres Observatory and the Antarctica Search for Transiting ExoPlanets program.

TOI-1231 b: A Temperate, Neptune-sized Planet Transiting the Nearby M3 Dwarf NLTT 24399

10.1016/j.newast.2021.101693

## , is applied to NASA’s Transiting Exoplanets Survey Satellite (TESS) dataset to identify exoplanetary candidates.

Automated identification of transiting exoplanet candidates in NASA Transiting Exoplanets Survey Satellite (TESS) data with machine learning methods

## The Transiting Exoplanet Survey Satellite (TESS) mission measured light from stars in ∼75% of the sky throughout its 2 yr primary mission, resulting in millions of TESS 30-minute-cadence light curves to analyze in the search for transiting exoplanets.

Identifying Planetary Transit Candidates in TESS Full-frame Image Light Curves via Convolutional Neural Networks

## We report the discovery and characterization of 7 transiting exoplanets from the HATNet survey.

HAT-P-58b -- HAT-P-64b: Seven Planets Transiting Bright Stars

## Finally, we present a retrieval analysis of a population of transiting exoplanets, focusing on those observed in transmission with the HST WFC3/G141 grism.

The pyrat bay framework for exoplanet atmospheric modelling: a population study of Hubble/WFC3 transmission spectra

## A mid-infrared instrument (Mid-Infrared Spectrometer and Camera Transit spectrometer) will measure the spectra of transiting exoplanets in the 2.

Origins Space Telescope: baseline mission concept

10.1051/0004-6361/202141097

## We identify 14 first time X-ray detections of transiting exoplanets that are subject to irradiation levels known to cause observable evaporation signatures in other exoplanets, which makes them suitable targets for follow-up observations.

Exoplanet X-ray irradiation and evaporation rates with eROSITA

## In the search for life in the cosmos, transiting exoplanets are currently our best targets.

Past, present and future stars that can see Earth as a transiting exoplanet.

## Some of these may already be host stars to known exoplanet systems or may become so with the progress of the TESS mission that is expected to discover 10,000 nearby transiting exoplanets in the upcoming decade.

LRP2020: The Opportunity of Young Nearby Associations with the Advent of the Gaia Mission

## For years, scientists have used data from NASA's Kepler Space Telescope to look for and discover thousands of transiting exoplanets.

Identifying Exoplanets with Deep Learning II: Two New Super-Earths Uncovered by a Neural Network in K2 Data

## Planetary materials orbiting white dwarf stars reveal the ultimate fate of the planets of the Solar System and all known transiting exoplanets.

The Search for Planet and Planetesimal Transits of White Dwarfs with the Zwicky Transient Facility.

## High-resolution Doppler spectroscopy is a powerful tool for identifying molecular species in the atmospheres of both transiting and non-transiting exoplanets.

Doppler tomography as a tool for detecting exoplanet atmospheres

## WASP-12b is one of the most well-studied transiting exoplanets, as its highly-inflated radius and its 1.

Storms or systematics? The changing secondary eclipse depth of WASP-12b

## Ultracool dwarfs have emerged as key targets for searches of transiting exoplanets.

Evolutionary Models for Ultracool Dwarfs

## In this work, we perform statistical eccentricity studies of transiting exoplanets using transit durations measured via Kepler combined with precise and accurate stellar radii from the California-Kepler Survey and Gaia.

The California-Kepler Survey. VIII. Eccentricities of Kepler Planets and Tentative Evidence of a High-metallicity Preference for Small Eccentric Planets

## 64 m^2 Atmospheric Remote-sensing Exoplanet Large-survey (ARIEL) survey of ~1000 transiting exoplanets will build on the legacies of NASA's Kepler and Transiting Exoplanet Survey Satellite (TESS), and complement the James Webb Space Telescope (JWST) by placing its high-precision exoplanet observations into a large, statistically significant planetary population context.

Constraining Exoplanet Metallicities and Aerosols with the Contribution to ARIEL Spectroscopy of Exoplanets (CASE)

10.1051/0004-6361/201936259

## The system of HD219134 hosts two transiting exoplanets and at least two additional non-transiting exoplanets.

From the stellar properties of HD219134 to the internal compositions of its transiting exoplanets

## We present here the first release of the open-source python package ExoTETHyS, which aims to provide a stand-alone set of tools for modeling spectro-photometric observations of the transiting exoplanets.

The ExoTETHyS package: Tools for Exoplanetary Transits around Host Stars.

## Transiting exoplanets allow measurements of the planetary radius and mass, providing information on the physical structure of the planet.

First observation of a planetary transit with the SPARC4 CCD: improved parameters for HATS-24b

## The technique of transmission spectroscopy allows us to constrain the chemical composition of the atmospheres of transiting exoplanets.

High-resolution transmission spectroscopy of four hot inflated gas giant exoplanets

## with hours of high-cadence exposure time each night, is designed to find the rare events that require all-sky monitoring, including transiting exoplanets around exotic stars like white dwarfs and hot subdwarfs, stellar activity of all types within our galaxy, nearby supernovae, and other transient events such as gamma ray bursts and gravitational-wave electromagnetic counterparts.

Building the Evryscope: Hardware Design and Performance

## The photometric precision, monitoring baselines, and rapid, even sampling rates required by modern satellites designed for detecting the signal of transiting exoplanets are ideally suited to a large number of applications in high-energy astrophysics.

The Vast Potential of Exoplanet Satellites for High-Energy Astrophysics

## They share characteristics of both brown dwarfs and transiting exoplanets, and therefore are critical for connecting atmospheric characterizations for these objects.

Cloud Atlas: High-contrast Time-resolved Observations of Planetary-mass Companions

## This deficiency can be addressed by performing phase-resolved spectroscopy -- continuous spectroscopic observations of a planet's entire orbit about its host star -- of transiting exoplanets.

Observing exoplanets in the near-infrared from a high altitude balloon platform

## Observations from the Kepler and K2 missions have provided the astronomical community with unprecedented amounts of data to search for transiting exoplanets and other astrophysical phenomena.

K2-288Bb: a small temperate planet in a low-mass binary system discovered by citizen scientists

## Our demonstrated infrared photometric performance opens up new avenues for ground-based observations of transiting exoplanets previously thought to be restricted to space-based investigation.

Diffuser-Assisted Infrared Transit Photometry for Four Dynamically Interacting \textit{Kepler} Systems

## Transiting exoplanets have been approved for 78.

Transmission Spectroscopy of WASP-79b from 0.6 to 5.0 $\mu$m

## We argue that the little dippers are consistent with transits of star-grazing exocomets, and speculate that they are signposts of massive non-transiting exoplanets driving the close-approach orbits.

The little dippers : transits of star-grazing exocomets?

10.1051/0004-6361/201935276

## We apply, for the first time, the Transit Least Squares (TLS) algorithm to search for new transiting exoplanets.

Transit least-squares survey - I. Discovery and validation of an Earth-sized planet in the four-planet system K2-32 near the 1:2:5:7 resonance

## The detection of periodic signals from transiting exoplanets is often impeded by extraneous aperiodic photometric variability, either intrinsic to the star or arising from the measurement process.

AutoRegressive Planet Search: Methodology

## We searched for variables and candidate transiting exoplanets.

A PSF-based Approach to TESS High quality data Of Stellar clusters (PATHOS) - I. Search for exoplanets and variable stars in the field of 47 Tuc

## Finally we provide a formula useful to optimize the trade-off between precision and duration of observations of transiting exoplanets.

An Independent Analysis of the Spitzer/IRAC Phase Curves of WASP43 b

## The mission will be devoted to observing spectroscopically in the infrared a large population of warm and hot transiting exoplanets (temperatures from ~500 K to ~3000 K) in our nearby Galactic neighborhood, opening a new discovery space in the field of extrasolar planets and enabling the understanding of the physics and chemistry of these far away worlds.

an integrated payload design for the atmospheric remote-sensing infrared exoplanet large-survey (ARIEL): results from phase A and forward look to phase B1