_version_ 1866914714469007360
author Henning, Thomas
Kamp, Inga
Samland, Matthias
Arabhavi, Aditya M.
Kanwar, Jayatee
van Dishoeck, Ewine F.
Guedel, Manuel
Lagage, Pierre-Olivier
Waelkens, Christoffel
Abergel, Alain
Absil, Olivier
Barrado, David
Boccaletti, Anthony
Bouwman, Jeroen
Garatti, Alessio Caratti o
Geers, Vincent
Glauser, Adrian M.
Lahuis, Fred
Nehme, Cyrine
Olofsson, Goeran
Pantin, Eric
Ray, Tom P.
Vandenbussche, Bart
Waters, L. B. F. M.
Wright, Gillian
Christiaens, Valentin
Franceschi, Riccardo
Gasman, Danny
Guadarrama, Rodrigo
Jang, Hyerin
Morales-Calderon, Maria
Pawellek, Nicole
Perotti, Giulia
Rodgers-Lee, Donna
Schreiber, Juergen
Schwarz, Kamber
Tabone, Benoit
Temmink, Milou
Vlasblom, Marissa
Colina, Luis
Greve, Thomas R.
Oestlin, Goeran
author_facet Henning, Thomas
Kamp, Inga
Samland, Matthias
Arabhavi, Aditya M.
Kanwar, Jayatee
van Dishoeck, Ewine F.
Guedel, Manuel
Lagage, Pierre-Olivier
Waelkens, Christoffel
Abergel, Alain
Absil, Olivier
Barrado, David
Boccaletti, Anthony
Bouwman, Jeroen
Garatti, Alessio Caratti o
Geers, Vincent
Glauser, Adrian M.
Lahuis, Fred
Nehme, Cyrine
Olofsson, Goeran
Pantin, Eric
Ray, Tom P.
Vandenbussche, Bart
Waters, L. B. F. M.
Wright, Gillian
Christiaens, Valentin
Franceschi, Riccardo
Gasman, Danny
Guadarrama, Rodrigo
Jang, Hyerin
Morales-Calderon, Maria
Pawellek, Nicole
Perotti, Giulia
Rodgers-Lee, Donna
Schreiber, Juergen
Schwarz, Kamber
Tabone, Benoit
Temmink, Milou
Vlasblom, Marissa
Colina, Luis
Greve, Thomas R.
Oestlin, Goeran
contents The study of protoplanetary disks has become increasingly important with the Kepler satellite finding that exoplanets are ubiquitous around stars in our galaxy and the discovery of enormous diversity in planetary system architectures and planet properties. High-resolution near-IR and ALMA images show strong evidence for ongoing planet formation in young disks. The JWST MIRI mid-INfrared Disk Survey (MINDS) aims to (1) investigate the chemical inventory in the terrestrial planet-forming zone across stellar spectral type, (2) follow the gas evolution into the disk dispersal stage, and (3) study the structure of protoplanetary and debris disks in the thermal mid-IR. The MINDS survey will thus build a bridge between the chemical inventory of disks and the properties of exoplanets. The survey comprises 52 targets (Herbig Ae stars, T Tauri stars, very low-mass stars and young debris disks). We primarily obtain MIRI/MRS spectra with high S/N (~100-500) covering the complete wavelength range from 4.9 to 27.9 μm. For a handful of selected targets we also obtain NIRSpec IFU high resolution spectroscopy (2.87-5.27 μm). We will search for signposts of planet formation in thermal emission of micron-sized dust - information complementary to near-IR scattered light emission from small dust grains and emission from large dust in the submillimeter wavelength domain. We will also study the spatial structure of disks in three key systems that have shown signposts for planet formation, TW Hya and HD 169142 using the MIRI coronagraph at 15.5 μm and 10.65 μm respectively and PDS70 using NIRCam imaging in the 1.87 μm narrow and the 4.8 μm medium band filter. ...
format Preprint
id arxiv_https___arxiv_org_abs_2403_09210
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle MINDS: The JWST MIRI Mid-INfrared Disk Survey
Henning, Thomas
Kamp, Inga
Samland, Matthias
Arabhavi, Aditya M.
Kanwar, Jayatee
van Dishoeck, Ewine F.
Guedel, Manuel
Lagage, Pierre-Olivier
Waelkens, Christoffel
Abergel, Alain
Absil, Olivier
Barrado, David
Boccaletti, Anthony
Bouwman, Jeroen
Garatti, Alessio Caratti o
Geers, Vincent
Glauser, Adrian M.
Lahuis, Fred
Nehme, Cyrine
Olofsson, Goeran
Pantin, Eric
Ray, Tom P.
Vandenbussche, Bart
Waters, L. B. F. M.
Wright, Gillian
Christiaens, Valentin
Franceschi, Riccardo
Gasman, Danny
Guadarrama, Rodrigo
Jang, Hyerin
Morales-Calderon, Maria
Pawellek, Nicole
Perotti, Giulia
Rodgers-Lee, Donna
Schreiber, Juergen
Schwarz, Kamber
Tabone, Benoit
Temmink, Milou
Vlasblom, Marissa
Colina, Luis
Greve, Thomas R.
Oestlin, Goeran
Earth and Planetary Astrophysics
The study of protoplanetary disks has become increasingly important with the Kepler satellite finding that exoplanets are ubiquitous around stars in our galaxy and the discovery of enormous diversity in planetary system architectures and planet properties. High-resolution near-IR and ALMA images show strong evidence for ongoing planet formation in young disks. The JWST MIRI mid-INfrared Disk Survey (MINDS) aims to (1) investigate the chemical inventory in the terrestrial planet-forming zone across stellar spectral type, (2) follow the gas evolution into the disk dispersal stage, and (3) study the structure of protoplanetary and debris disks in the thermal mid-IR. The MINDS survey will thus build a bridge between the chemical inventory of disks and the properties of exoplanets. The survey comprises 52 targets (Herbig Ae stars, T Tauri stars, very low-mass stars and young debris disks). We primarily obtain MIRI/MRS spectra with high S/N (~100-500) covering the complete wavelength range from 4.9 to 27.9 μm. For a handful of selected targets we also obtain NIRSpec IFU high resolution spectroscopy (2.87-5.27 μm). We will search for signposts of planet formation in thermal emission of micron-sized dust - information complementary to near-IR scattered light emission from small dust grains and emission from large dust in the submillimeter wavelength domain. We will also study the spatial structure of disks in three key systems that have shown signposts for planet formation, TW Hya and HD 169142 using the MIRI coronagraph at 15.5 μm and 10.65 μm respectively and PDS70 using NIRCam imaging in the 1.87 μm narrow and the 4.8 μm medium band filter. ...
title MINDS: The JWST MIRI Mid-INfrared Disk Survey
topic Earth and Planetary Astrophysics
url https://arxiv.org/abs/2403.09210