The infra-red dual imaging and spectrograph for SPHERE: design and performance

By K. Dohlen, Maud Langlois, M. Saisse, L. Hill, A. Origné, M. Jacquet, C. Fabron, J. Blanc, M. Llored, M. Carle and 6 more. Astronomical Telescopes + Instrumentation, 2008

192 citations recorded by the source corpus.

Subfields: Atomic and Molecular Physics, and Optics, Computational Mechanics, Instrumentation

View Paper: https://www.semanticscholar.org/paper/66a3385ec7887db9de48eab244131eb495b3b563

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In Atomic and Molecular Physics, and Optics

1. B. Bowler
2. R. Galicher
3. S. Udry
4. Th. Henning
5. F. Allard
6. T. Birnstiel
7. R. Teague
8. S. Desidera

In Computational Mechanics

1. B. Bowler
2. S. Udry
3. Th. Henning
4. R. Gratton
5. T. Birnstiel
6. S. Desidera
7. Sascha P. Quanz

In Instrumentation

1. B. Bowler
2. C. Mordasini
3. Th. Henning
4. R. Gratton
5. R. van Boekel
6. T. Birnstiel
7. David Mouillet
8. Anne-Marie Lagrange

Citations in the corpus

• Disks around T Tauri Stars with SPHERE (DARTTS-S). I. SPHERE/IRDIS Polarimetric Imaging of Eight Prominent T Tauri Disks (2018, methodology): “All our observations were carried out with SPHERE/IRDIS (Infra-Red Dual Imaging and Spectrograph, Dohlen et al. 2008) in Dual Polarization Imaging mode (DPI, Langlois et al. 2014; de Boer et al. 2019; van Holstein et al. 2019).”
• Photometric characterization of exoplanets using angular and spectral differential imaging (2010, methodology): “SPHERE will also incorporate a differential imager named IRDIS (InfraRed Dual Imaging Spectrograph, Dohlen et al. 2008) that will provide simultaneous images at two close wavelengths in either one of its 5 different filter pairs over the Y to Ks bands.”
• Imaging Extrasolar Giant Planets (2016, background): “IRDIS (Dohlen et al. 2008) offers classical and dual-band imaging (Vigan et al. 2010), dual-polarization imaging (Langlois et al. 2014), and long-slit spectroscopy (Vigan et al. 2008); IFS provides low-resolution (R∼30–50) integral field spectroscopy spanning 0.95–1.65 µm (Claudi et al. 2008); and Z”
• Three Radial Gaps in the Disk of TW Hydrae Imaged with SPHERE (2016, methodology): “Two of the subinstruments of SPHERE were used: the Zürich Imaging POLarimeter (ZIMPOL, Schmid et al. 2012) in field stabilized (P2) mode, and the Infra-Red Dual-beam Imaging and Spectroscopy instrument (IRDIS, Dohlen et al. 2008; Langlois et al. 2014) in Dual-band Polarimetric Imaging (DPI) mode.”
• Discovery of a planetary-mass companion within the gap of the transition disk around PDS 70 (2018, methodology): “During the nights of March 25, 2016, and July 31, 2017, we obtained two datasets of PDS 70 with the IRDIS instrument (Dohlen et al. 2008) in PDI mode (Langlois et al. 2014) using the J-band (λJ = 1.25 µm).”