activity
20222026
most citedJWST MIRI/MRS in-flight absolute flux calibration and tailored fringe correction for unresolved sources

51 citations · 51 across the 4 of their papers we have counts for

collaborators

5 papers

astro-ph.GA2026

JWST observations of the planetary nebula NGC 6302 IV: PAH spectral characteristics, formation and evolution

Nicholas Clark, Els Peeters, Jan Cami +29

Polycyclic aromatic hydrocarbons (PAHs) and carbonaceous dust have been observed in Oxygen-rich planetary nebulae (PNe), yet their formation and evolution in these environments is…

astro-ph.GA2026

The Stellar Population of NGC 346 in the Small Magellanic Cloud with JWST

J. Jaspers, P. Kavanagh, G. De Marchi +13

NGC 346 is a massive star-forming region located at a distance of 62 kpc, in the Small Magellanic Cloud (SMC). Due to its low metallicity (Z 1/5 Z), it is an…

astro-ph.GA2026

Detection of CO ice in the planetary nebula NGC 6302

Charmi Bhatt, Simon W. Cao, Jan Cami +20

Using JWST/MIRI observations, we report the detection of CO ice in the dusty torus of the planetary nebula NGC 6302, an environment generally considered hostile to fragile mole…

astro-ph.GA2025

Detection of CH3+ in the O-rich planetary nebula NGC 6302

Charmi Bhatt, Jan Cami, Els Peeters +33

Planetary nebulae are sites where ejected stellar material evolves into complex molecules, but the precise physical conditions and chemical routes that govern these processes are u…

astro-ph.IM2022★ 51 cited

JWST MIRI/MRS in-flight absolute flux calibration and tailored fringe correction for unresolved sources

D. Gasman, I. Argyriou, G. C. Sloan +18

The MRS is one of the four observing modes of JWST/MIRI. Using JWST in-flight data of unresolved (point) sources, we can derive the MRS absolute spectral response function (ASRF) s…