Luigi Mancini

Associate Professor in Astrophysics
Contacts

Hello, welcome to my home page.
I am an Associate Professor working at the Department of Physics of the University of Rome Tor Vergata. I am also affiliated with the Max Planck Institute for Astronomy in Heidelberg (MPIA) and the INAF Astrophysical Observatory of Turin (OATo). My current research is mainly focused on the search for new Extrasolar Planets and their physical characterization.

I am involved in several collaborations, including:

  • HATSouth, which uses a network of identical, fully automated wide-field telescopes, for detecting new transiting exoplanets;
  • GAPS, which is undertaking a challenging observational program to characterize the global architectural properties of exoplanetary systems, by using the high-resolution spectrograph HARPS-N;
  • CARMENES, which is carrying out a survey of 300 late-type main-sequence stars with the goal of detecting low-mass planets in their habitable zones;
  • MiNDSTEp, which exploits the technique of gravitational microlensing to study the population of planets in the Galaxy.
  • I have also participated in several programs aimed to confirm the planetary nature of a subset of Kepler and K2 candidates via radial-velocity follow-up observations, and I am now working on TESS data. I also collaborate with SuperWASP e QES contributing with photometric follow-up observations of their planet candidates.

We discovered TOI-1853b, which is the most dense Neptune-size planet in the known Galaxy thanks to TESS data and precise radial-velocity measurements with HARPS-N at the TNG.

I was a member of the JWST (James Webb Space Telescope) Transiting Exoplanet Community Early Release Science program, whose goal was to understand the limitations and capabilities of the JWST instruments and provide the scientific community with the technical skills to analyze JWST data, in particular those concerning the study of the atmospheres of transiting exoplanets. The aim was not only to demonstrate JWST's ability to obtain precise measurements of the chemical composition of the atmospheres of transiting planets but also to test the various instrumental modalities, which are currently used to study a wide variety of exoplanets, from the hot and giant ones up to the more temperate and terrestrial ones. A little over a month after the first data collected by the James Webb Space Telescope, the Transiting Exoplanet Early Release Science Team unequivocally detected carbon dioxide in the atmosphere of the exoplanet WASP-39b. In 2023, we achieved another first: an extremely detailed molecular and chemical portrait of the skies of the exoplanet WASP-39b. Among the unprecedented revelations, there is the first detection in an exoplanetary atmosphere of sulfur dioxide, a molecule produced by chemical reactions triggered by highly energetic radiation from the planet's parent star. Other atmospheric constituents detected by the JWST include sodium, potassium and water vapour, confirming previous observations from space and ground-based telescopes, as well as finding additional traces of water, at longer wavelengths, that had never been seen Before. The JWST also saw carbon monoxide and carbon dioxide, the latter at higher resolution, providing double the data reported by its previous observations. These results have been described in a series of papers published by Nature (Volume 614 Issue 7949). 

 

I am also a member of the Exo-Earth Discovery and Exploration Network (EDEN), which aims to find habitable planets within 50 light years. Actually, a large part of the exoplanet community is focussing on the neighbours of the Solar system, not only for the obvious observational reasons but also in the spirit of future exploration, because the closest planets will be the only ones that can be reached by the human being on a historical scale.

I am leading an observational program to accurately measure the characteristics of known exoplanet systems hosting close-in transiting giant planets. Our study is based on high-quality photometric follow-up observations of transit events with an array of medium-class telescopes, which are located in both the northern and the southern hemispheres. High photometric precision is achieved through the telescope-defocussing technique. The data are then reduced and analyzed homogeneously for estimating the orbital and physical parameters of both the planets and their parent stars. We also make use of multi-band imaging cameras for probing planetary atmospheres via the transmission-photometry technique. In some cases, we adopt a two-site observational strategy for collecting simultaneous light curves of individual transits, which is the only reliable method for truly distinguishing a real astrophysical signal from systematic noise.

I am the main organizer of the Advanced School on Exoplanetary Science, whose first four editions took place in Vietri sul Mare (Italy) in May 2015, 2017, 2019 (ASES3) and 2023 (ASES4)

 Lecture Notes of ASES1: Methods of Detecting Exoplanets

Lecture Notes of ASES2: Astrophysics of Exoplanetary Atmospheres

Lecture Notes of ASES3: Demographics of Exoplanetary Systems

The complete list of my publications is powered by the Astrophysics Data System

 

Selected list of my publications in high impact Scientific Journals

  • Inhomogeneous terminators on the exoplanet WASP-39 b
    • N. Espinoza, M. E. Steinrueck, J. Kirk, et al., Nature 632, 1017 (2024) -- Link
  • A benchmark JWST near-infrared spectrum for the exoplanet WASP-39 b
    • A. Carter, E. M. May, N. Espinoza, et al., Nature Astronomy 8, 1008 (2024) -- Link
  • Nightside clouds and disequilibrium chemistry on the hot Jupiter WASP-43b
    • T. J. Bell, N. Crouzet, P. E. Cubillos, et al., Nature Astronomy 8, 879 (2024) -- Link
  • Sulfur dioxide in the mid-infrared transmission spectrum of WASP-39b
    • D. Powell, A. D. Feinstein, E. K. H. Lee, et al., Nature 626, 979 (2024) -- Link
  • A super-massive Neptune-sized planet
    • L. Naponiello, L. Mancini, A. Sozzetti, et al., Nature 622, 255 (2023) -- Link
  • A broadband thermal emission spectrum of the ultra-hot Jupiter WASP-18b
    • L.-P. Coulombe, B. Benneke, R. Challener, et al., Nature 620, 292 (2023) -- Link
  • Early Release Science of the exoplanet WASP-39b with JWST NIRISS
    • A. D. Feinstein, M. Radica, L. Welbanks, et al., Nature 614, 670 (2023) -- Link
  • Early Release Science of the exoplanet WASP-39b with JWST NIRSpec G395H
    • L. Alderson, H. R. Wakeford, M. K. Alam, et al., Nature 614, 664 (2023) -- Link
  • Early Release Science of the exoplanet WASP-39b with JWST NIRSpec PRISM
    • Z. Rustamkulov, D. K. Sing, S. Mukherjee, et al., Nature 614, 659 (2023) -- Link
  • Early Release Science of the exoplanet WASP-39b with JWST NIRCam
    • E.-M. Ahrer, K. B. Stevenson, M. Mansfield, et al., Nature 614, 653 (2023) -- Link
  • Identification of carbon dioxide in an exoplanet atmosphere
    • JWST Transiting Exoplanet Community Early Release Science Team, Nature 614, 649 (2023) -- Link
  • A giant exoplanet orbiting a very-low-mass star challenges planet formation models
    • J. C. Morales, A. J. Mustill, I Ribas, et al., Science 365, 1441 (2019) -- Link

 

Selected list of my publications in high impact factor Astrophysics Journals

  • An inner eccentric sub-Neptune and an outer sub-Neptune-mass candidate around BD+00 444
    • L. Naponiello, A. S. Bonomo, L. Mancini, et al., Astronomy & Astrophysics 693, A7 (2025) -- Link
  • Star-spot activity, orbital obliquity, transmission spectrum, physical properties, and transit time variations of the HATS-2 planetary system
    • F. Biagiotti, L. Mancini, L., J. Southworth, et al., Astronomy & Astrophysics 685, A131 (2024) -- Link
  • A puffy and warm Neptune-sized planet and an outer Neptune-mass candidate orbiting the solar-type star TOI-1422
    • L. Naponiello, L. Mancini, M. Damasso, et al., Astronomy & Astrophysics 667, A8 (2022) -- Link
  • Measurement of the Rossiter-McLaughlin effect and revising the physical and orbital parameters of the HAT-P-15, HAT-P-17, HAT-P-21, HAT-P-26, HAT-P-29 eccentric planetary systems
    • L. Mancini, M. Esposito, E. Covino, et al., Astronomy & Astrophysics 664, A162 (2022) -- Link
  • The ultra-hot-Jupiter KELT-16 b: dynamical evolution and atmospheric properties
    • L. Mancini, J. Southworth, L. Naponiello, et al., Monthly Notices of the Royal Astronomical Society 509, 1447 (2022) -- Link
  • An Isolated Stellar-mass Black Hole Detected through Astrometric Microlensing
    • K. C. Sahu, J. Anderson, S. Casertano, et al., The Astrophysical Journal 933, 83 (2022) -- Link
  • The highly inflated giant planet WASP-174b
    • L. Mancini, P. Sarkis, Th. Henning, et al., Astronomy & Astrophysics 633, A30 (2020) -- Link
  • Two temperate Earth-mass planet candidates around Teegarden's Star
    • M. Zechmeister, S. Dreizler, I. Ribas, et al., Astronomy & Astrophysics 627, A49 (2019) -- Link
  • Physical properties and transmission spectrum of the WASP-74 planetary system from multiband photometry
    • L. Mancini, J. Southworth, P. Mollière, et al., Monthly Notices of the Royal Astronomical Society 485, 5168 (2019) -- Link
  • Measurement of the Rossiter-McLaughlin effect of transiting planetary systems HAT-P-3, HAT-P-12, HAT-P-22, WASP-39, and WASP-60
    • L. Mancini, M. Esposito, E. Covino, et al., Astronomy & Astrophysics 613, A41 (2018) -- Link
  • HATS-50b through HATS-53b: Four Transiting Hot Jupiters Orbiting G-type Stars Discovered by the HATSouth Survey
    • Th. Henning, L. Mancini, P. Sarkis, et al., The Astronomical Journal 155, 79 (2018) -- Link
  • Detection of the Atmosphere of the 1.6 M⊕ Exoplanet GJ 1132 b
    • J. Southworth, L. Mancini, N. Madhusudhan, et al., The Astronomical Journal 153, 191 (2017) -- Link
  • Orbital alignment and star-spot properties in the WASP-52 planetary system
    • L. Mancini, J. Southworth, G. Raia, et al., Monthly Notices of the Royal Astronomical Society, Volume 465, 843 (2017) -- Link
  • An optical transmission spectrum of the transiting hot Jupiter in the metal-poor WASP-98 planetary system
    • L. Mancini, M. Giordano, P. Mollière, et al., Monthly Notices of the Royal Astronomical Society, Volume 461, 1053 (2016) -- Link
  • 197 Candidates and 104 Validated Planets in K2’s First Five Fields
    • I. J. M. Crossfield, D. R. Ciardi, E. A. Petigura, et al., The Astrophysical Journal Supplement Series 226, 7 (2016) -- Link
  • An optical transmission spectrum of the giant planet WASP-36 b
    • L. Mancini, J. Kemmer, J. Southworth, et al., Monthly Notices of the Royal Astronomical Society, Volume 459, 1393 (2016) -- Link
  • Kepler-539: A young extrasolar system with two giant planets on wide orbits and in gravitational interaction
    • L. Mancini, J. Lillo-Box, J. Southworth, et al., Astronomy & Astrophysics 590, A112 (2016) -- Link
  • Rotation periods and astrometric motions of the Luhman 16AB brown dwarfs by high-resolution lucky-imaging monitoring
    • L. Mancini, P. Giacobbe, S. P. Littlefair, et al., Astronomy & Astrophysics 584, A104 (2015) -- Link
  • HATS-13b and HATS-14b: two transiting hot Jupiters from the HATSouth survey
    • L. Mancini, J. D. Hartman, K. Penev, et al., Astronomy & Astrophysics 580, A63 (2015) -- Link
  • Observations of the Rossiter-McLaughlin effect and characterisation of the transiting planetary systems HAT-P-36 and WASP-11/HAT-P-10
    • L. Mancini, M. Esposito, E. Covino, et al., Astronomy & Astrophysics 579, A136 (2015) -- Link
  • Physical properties, star-spot activity, orbital obliquity and transmission spectrum of the Qatar-2 planetary system from multicolour photometry
    • L. Mancini, J. Southworth, S. Ciceri, et al., Monthly Notices of the Royal Astronomical Society, Volume 443, 2391 (2014) -- Link
  • Physical properties of the WASP-67 planetary system from multi-colour photometry
    • L. Mancini, J. Southworth, S. Ciceri, et al., Astronomy & Astrophysics 568, A127 (2014) -- Link
  • Physical properties and transmission spectrum of the WASP-80 planetary system from multi-colour photometry
    • L. Mancini, J. Southworth, S. Ciceri, et al., Astronomy & Astrophysics 562, A126 (2014) -- Link
  • Physical properties, transmission and emission spectra of the WASP-19 planetary system from multi-colour photometry
    • L. Mancini, S. Ciceri, G. Chen, et al., Monthly Notices of the Royal Astronomical Society, Volume 436, 2 (2013) -- Link
  • Physical properties of the WASP-44 planetary system from simultaneous multi-colour photometry
    • L. Mancini, N. Nikolov, J. Southworth, et al., Monthly Notices of the Royal Astronomical Society, Volume 430, 2932 (2013) -- Link
  • A lower radius and mass for the transiting extrasolar planet HAT-P-8 b
    • L. Mancini, J. Southworth, S. Ciceri, et al., Astronomy & Astrophysics 551, A11 (2013) -- Link
  • Observing Gravitational Lensing Effects by Sgr A* with GRAVITY
    • V. Bozza & L. Mancini, The Astrophysical Journal 753, 56 (2012) -- Link
  • The scaling relation between the mass of supermassive black holes and the kinetic energy of random motions of the host galaxies
    • L. Mancini & A. Feoli, Astronomy & Astrophysics 537, A48 (2012) -- Link
  • Microlensing towards the Large Magellanic Cloud: self-lensing for OGLE-II and OGLE-III
    • S. Calchi Novati & L. Mancini, Monthly Notices of the Royal Astronomical Society, Volume 416, 1292 (2011) -- Link
  • A Hertzsprung-Russell-like Diagram for Galaxies: The M • Versus M Gσ2 Relation
    • A. Feoli & L. Mancini, The Astrophysical Journal 703, 1502 (2009) -- Link
  • Gravitational Lensing of Stars Orbiting the Massive Black Hole in the Galactic Center
    • V. Bozza & L. Mancini, The Astrophysical Journal 696, 701 (2009) -- Link
  • Microlensing towards the LMC revisited by adopting a non-Gaussian velocity distribution for the sources
    • L. Mancini, Astronomy & Astrophysics 496, 465 (2009) -- Link
  • Gravitational Lensing of Stars in the Central Arcsecond of Our Galaxy
    • V. Bozza & L. Mancini, The Astrophysical Journal 627, 790 (2005) -- Link
  • LMC self-lensing from a new perspective
    • L. Mancini & S. Calchi Novati, Ph. Jetzer, G. Scarpetta, Astronomy & Astrophysics 427, 61 (2004) -- Link
  • Gravitational Lensing by Black Holes: A Comprehensive Treatment and the Case of the Star S2
    • V. Bozza & L. Mancini, The Astrophysical Journal 611, 1045 (2004) -- Link
  • Time Delay in Black Hole Gravitational Lensing as a Distance Estimator
    • V. Bozza & L. Mancini, General Relativity and Gravitation 36, 435 (2004) -- Link
  • Microlensing of strongly interacting binary systems
    • V. Bozza & L. Mancini, Astronomy & Astrophysics 394, L47 (2002) -- Link
  • Microlensing towards the Large Magellanic Cloud
    • Ph. Jetzer, L. Mancini, G. Scarpetta, Astronomy & Astrophysics 393, 129 (2002) -- Link
  • Microlensing by compact objects associated with gas clouds
    • V. Bozza, Ph. Jetzer, L. Mancini, G. Scarpetta, Astronomy & Astrophysics 382, 6 (2002) -- Link
...
Teaching in the Physics Department
ID Course Name Semester Length CFU
Astrophysical Techniques Second 14 Weeks 8
Exoplanets First 14 Weeks 6