| Autor: |
Doyon, Rene, Willott, C. J, Hutchings, John B., Sivaramakrishnan, Anand, Albert, Loic, Lafreniere, David, Rowlands, Neil, Vila, M. Begona, Martel, Andre R., LaMassa, Stephanie, Aldridge, David, Artigau, Etienne, Cameron, Peter, Chayer, Pierre, Cook, Neil J., Cooper, Rachel A., Darveau-Bernier, Antoine, Dupuis, Jean, Earnshaw, Colin, Espinoza, Nestor, Filippazzo, Joseph C., Fullerton, Alexander W., Gaudreau, Daniel, Gawlik, Roman, Goudfrooij, Paul, Haley, Craig, Kammerer, Jens, Kendall, David, Lambros, Scott D., Ignat, Luminita Ilinca, Maszkiewicz, Michael, McColgan, Ashley, Morishita, Takahiro, Ouellette, Nathalie N. -Q., Pacifici, Camilla, Philippi, Natasha, Radica, Michael, Ravindranath, Swara, Rowe, Jason, Roy, Arpita, Saad, Karl, Sohn, Sangmo Tony, Talens, Geert Jan, Thatte, Deepashri, Taylor, Joanna M., Vandal, Thomas, Volk, Kevin, Wander, Michel, Warner, Gerald, Zheng, Sheng-Hai, Zhou, Julia, Abraham, Roberto, Beaulieu, Mathilde, Benneke, Bjorn, Ferrarese, Laura, Johnstone, Doug, Kaltenegger, Lisa, Meyer, Michael R., Pipher, Judy L., Rameau, Julien, Rieke, Marcia, Salhi, Salma, Sawicki, Marcin |
| Rok vydání: |
2023 |
| Předmět: |
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| Druh dokumentu: |
Working Paper |
| Popis: |
The Near-Infrared Imager and Slitless Spectrograph (NIRISS) is the science module of the Canadian-built Fine Guidance Sensor (FGS) onboard the James Webb Space Telescope (JWST). NIRISS has four observing modes: 1) broadband imaging featuring seven of the eight NIRCam broadband filters, 2) wide-field slitless spectroscopy (WFSS) at a resolving power of $\sim$150 between 0.8 and 2.2 $\mu$m, 3) single-object cross-dispersed slitless spectroscopy (SOSS) enabling simultaneous wavelength coverage between 0.6 and 2.8 $\mu$m at R$\sim$700, a mode optimized for exoplanet spectroscopy of relatively bright ($J<6.3$) stars and 4) aperture masking interferometry (AMI) between 2.8 and 4.8 $\mu$m enabling high-contrast ($\sim10^{-3}-10^{-4}$) imaging at angular separations between 70 and 400 milliarcsec for relatively bright ($M<8$) sources. This paper presents an overview of the NIRISS instrument, its design, its scientific capabilities, and a summary of in-flight performance. NIRISS shows significantly better response shortward of $\sim2.5\,\mu$m resulting in 10-40% sensitivity improvement for broadband and low-resolution spectroscopy compared to pre-flight predictions. Two time-series observations performed during instrument commissioning in the SOSS mode yield very stable spectro-photometry performance within $\sim$10% of the expected noise. The first space-based companion detection of the tight binary star AB Dor AC through AMI was demonstrated. |
| Databáze: |
arXiv |
| Externí odkaz: |
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