Sökning: WFRF:(Olivier Anthony) > MINDS :
Fältnamn | Indikatorer | Metadata |
---|---|---|
000 | 05112naa a2200829 4500 | |
001 | oai:DiVA.org:su-231541 | |
003 | SwePub | |
008 | 240722s2024 | |||||||||||000 ||eng| | |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-2315412 URI |
024 | 7 | a https://doi.org/10.1088/1538-3873/ad34552 DOI |
040 | a (SwePub)su | |
041 | a engb eng | |
042 | 9 SwePub | |
072 | 7 | a ref2 swepub-contenttype |
072 | 7 | a art2 swepub-publicationtype |
100 | 1 | a Henning, Thomas4 aut |
245 | 1 0 | a MINDS :b The JWST MIRI Mid-INfrared Disk Survey |
264 | 1 | c 2024 |
338 | a print2 rdacarrier | |
520 | a 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 signal-to-noise ratio (∼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 PDS 70 using NIRCam imaging in the 1.87 μm narrow and the 4.8 μm medium band filter. We provide here an overview of the MINDS survey and showcase the power of the new JWST mid-IR molecular spectroscopy with the TW Hya disk spectrum where we report the detection of the molecular ion CH3+ and the robust confirmation of HCO+ earlier detected with Spitzer. | |
650 | 7 | a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe |
650 | 7 | a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng |
700 | 1 | a Kamp, Inga4 aut |
700 | 1 | a Samland, Matthias4 aut |
700 | 1 | a Arabhavi, Aditya M.4 aut |
700 | 1 | a Kanwar, Jayatee4 aut |
700 | 1 | a van Dishoeck, Ewine F.4 aut |
700 | 1 | a Güdel, Manuel4 aut |
700 | 1 | a Lagage, Pierre-Olivier4 aut |
700 | 1 | a Waelkens, Christoffel4 aut |
700 | 1 | a Abergel, Alain4 aut |
700 | 1 | a Absil, Olivier4 aut |
700 | 1 | a Barrado, David4 aut |
700 | 1 | a Boccaletti, Anthony4 aut |
700 | 1 | a Bouwman, Jeroen4 aut |
700 | 1 | a Caratti o Garatti, Alessio4 aut |
700 | 1 | a Geers, Vincent4 aut |
700 | 1 | a Glauser, Adrian M.4 aut |
700 | 1 | a Lahuis, Fred4 aut |
700 | 1 | a Mueller, Michael4 aut |
700 | 1 | a Nehmé, Cyrine4 aut |
700 | 1 | a Olofsson, Göran,d 1944-u Stockholms universitet,Institutionen för astronomi4 aut0 (Swepub:su)olofsson |
700 | 1 | a Pantin, Eric4 aut |
700 | 1 | a Ray, Tom P.4 aut |
700 | 1 | a Scheithauer, Silvia4 aut |
700 | 1 | a Vandenbussche, Bart4 aut |
700 | 1 | a Waters, L. B. F. M.4 aut |
700 | 1 | a Wright, Gillian4 aut |
700 | 1 | a Argyriou, Ioannis4 aut |
700 | 1 | a Christiaens, Valentin4 aut |
700 | 1 | a Franceschi, Riccardo4 aut |
700 | 1 | a Gasman, Danny4 aut |
700 | 1 | a Grant, Sierra L.4 aut |
700 | 1 | a Guadarrama, Rodrigo4 aut |
700 | 1 | a Jang, Hyerin4 aut |
700 | 1 | a Morales-Calderón, Maria4 aut |
700 | 1 | a Pawellek, Nicole4 aut |
700 | 1 | a Perotti, Giulia4 aut |
700 | 1 | a Rodgers-Lee, Donna4 aut |
700 | 1 | a Schreiber, Jürgen4 aut |
700 | 1 | a Schwarz, Kamber4 aut |
700 | 1 | a Tabone, Benoit4 aut |
700 | 1 | a Temmink, Milou4 aut |
700 | 1 | a Vlasblom, Marissa4 aut |
700 | 1 | a Colina, Luis4 aut |
700 | 1 | a Greve, Thomas R.4 aut |
700 | 1 | a Östlin, Göran,d 1968-u Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)ostlin |
710 | 2 | a Stockholms universitetb Institutionen för astronomi4 org |
773 | 0 | t Publications of the Astronomical Society of the Pacificg 136:5q 136:5x 0004-6280x 1538-3873 |
856 | 4 | u https://doi.org/10.1088/1538-3873/ad3455y Fulltext |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-231541 |
856 | 4 8 | u https://doi.org/10.1088/1538-3873/ad3455 |
Kungliga biblioteket hanterar dina personuppgifter i enlighet med EU:s dataskyddsförordning (2018), GDPR. Läs mer om hur det funkar här.
Så här hanterar KB dina uppgifter vid användning av denna tjänst.