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JEMS: A deep medium-band imaging survey in the Hubble Ultra-Deep Field with JWST NIRCam & NIRISS

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arxiv 2301.09780 v1 pith:RMNV6NFK submitted 2023-01-24 astro-ph.GA

classification astro-ph.GA
keywords medium-bandjwstsurveyimagingnircamnirissalphadata
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abstract

We present JEMS (JWST Extragalactic Medium-band Survey), the first public medium-band imaging survey carried out using JWST/NIRCam and NIRISS. These observations use $\sim2\mu$m and $\sim4\mu$m medium-band filters (NIRCam F182M, F210M, F430M, F460M, F480M; and NIRISS F430M & F480M in parallel) over 15.6 square arcminutes in the Hubble Ultra Deep Field (UDF), thereby building on the deepest multi-wavelength public datasets available anywhere on the sky. We describe our science goals, survey design, NIRCam and NIRISS image reduction methods, and describe our first data release of the science-ready mosaics. Our chosen filters create a JWST imaging survey in the UDF that enables novel analysis of a range of spectral features potentially across the redshift range of $0.3<z<20$, including Paschen-$\alpha$, H$\alpha$+[NII], and [OIII]+H$\beta$ emission at high spatial resolution. We find that our JWST medium-band imaging efficiently identifies strong line emitters (medium-band colors $>1$ magnitude) across redshifts $1.5<z<9.3$, most prominently H$\alpha$+[NII] and [OIII]+H$\beta$. We present our first data release including science-ready mosaics of each medium-band image available to the community, adding to the legacy value of past and future surveys in the UDF. We also describe future data releases. This survey demonstrates the power of medium-band imaging with JWST, informing future extragalactic survey strategies using JWST observations.

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Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. OpenAlex reports about 12 citations worldwide. Full citation record

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    astro-ph.GA 2026-08 conditional novelty 6.0 of 10

    Only 0.08% of low-redshift broad-line objects have SEDs resembling high-redshift Little Red Dots, yielding nine candidates, one of which is the known analogue 'The Egg'.

  3. Dust emission from the bulk of galaxies at the Epoch of Reionization

    astro-ph.GA 2024-12 conditional novelty 6.0 of 10

    Stacked ALMA data reveal tentative infrared emission from typical z=6-7 galaxies, implying lower dust attenuation and star formation rates than UV-selected samples, and only upper limits at z>7.

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