2023PASP..135i8001D


Query : 2023PASP..135i8001D

2023PASP..135i8001D - Publ. Astron. Soc. Pac., 135, part no 9, 8001 (2023/September-0)

The Near Infrared Imager and Slitless Spectrograph for the James Webb Space Telescope. I. Instrument Overview and In-flight Performance.

DOYON R., WILLOTT C.J., HUTCHINGS J.B., SIVARAMAKRISHNAN A., ALBERT L., LAFRENIERE D., ROWLANDS N., VILA M.B., MARTEL A.R., LAMASSA S., ALDRIDGE D., ARTIGAU E., CAMERON P., CHAYER P., COOK N.J., COOPER R.A., DARVEAU-BERNIER A., DUPUIS J., EARNSHAW C., ESPINOZA N., FILIPPAZZO J.C., FULLERTON A.W., GAUDREAU D., GAWLIK R., GOUDFROOIJ P., HALEY C., KAMMERER J., KENDALL D., LAMBROS S.D., IGNAT L.I., MASZKIEWICZ M., McCOLGAN A., MORISHITA T., OUELLETTE N.N.-Q., PACIFICI C., PHILIPPI N., RADICA M., RAVINDRANATH S., ROWE J., ROY A., ROY N., SAAD K., SOHN S.T., TALENS G.J., TOUAHRI D., THATTE D., TAYLOR J.M., VANDAL T., VOLK K., WANDER M., WARNER G., ZHENG S.-H., ZHOU J., ABRAHAM R., BEAULIEU M., BENNEKE B., FERRARESE L., JAYAWARDHANA R., JOHNSTONE D., KALTENEGGER L., MEYER M.R., PIPHER J.L., RAMEAU J., RIEKE M., SALHI S. and SAWICKI M.

Abstract (from CDS):

The Near-Infrared Imager and Slitless Spectrograph (NIRISS) is the science module of the Canadian-built Fine Guidance Sensor 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 at a resolving power of ∼150 between 0.8 and 2.2 μm, (3) single-object cross-dispersed slitless spectroscopy (SOSS) enabling simultaneous wavelength coverage between 0.6 and 2.8 μm at R ∼ 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 μm enabling high-contrast (∼10–3 - 10–4) imaging at angular separations between 70 and 400 mas 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 ∼2.5 μm 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 ∼10% of the expected noise. The first space-based companion detection of the tight binary star AB Dor AC through AMI was demonstrated.

Abstract Copyright: © 2023. The Author(s). Published by IOP Publishing Ltd on behalf of the Astronomical Society of the Pacific (ASP). All rights reserved

Journal keyword(s): Space vehicle instruments - Astronomical instrumentation

Simbad objects: 13

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Number of rows : 13
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 NAME LMC G 05 23 34.6 -69 45 22     0.4     ~ 19090 0
2 LHA 120-N 133 PN 05 24 20.7467383224 -70 05 01.601773404 15.939 16.236 15.368 15.120 16.556 [WC4/5] 88 0
3 V* AB Dor C LM* 05 28 44.83 -65 26 54.9           M8: 71 0
4 V* AB Dor TT* 05 28 44.8712165880 -65 26 55.199147208 8.259 7.856 6.999 6.496 5.993 K0V 1080 0
5 HD 37093 * 05 31 08.2590174816 -65 07 42.083399712   10.70 9.25     K5(III) 16 0
6 UCAC4 117-011267 * 06 28 02.0014566936 -66 37 38.095571100   11.979   10.708   ~ 9 0
7 CPD-66 562 * 06 31 36.6171205438 -66 21 47.605754007   11.344 10.511     ~ 11 0
8 TWA 33 Y*? 11 39 33.8249537040 -30 40 00.365859300   16.71 15.06 14.85   M5.5e 39 0
9 PG 1657+344 WD* 16 58 51.1124739360 +34 18 53.321336856   16.12       DA.9 70 0
10 BD+38 2917 Em* 17 20 27.8781604680 +38 14 31.908984936   10.41 9.99     F5V 88 1
11 BD+38 2917b Pl 17 20 27.8781604680 +38 14 31.908984936           ~ 95 1
12 BD+60 1753 * 17 24 52.2753625128 +60 25 50.749843296   9.72 9.65     A1V 42 0
13 LAWD 87 WD* 21 32 16.2327040616 +00 15 14.399267982 13.717 14.634 14.674 14.675 14.676 DB4 195 1

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