JADES Dark Horse: demonstrating high-multiplex observations with JWST /NIRSpec dense-shutter spectroscopy in the JADES Origins Field

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Authors: Francesco D’Eugenio, Erica J Nelson, Daniel J Eisenstein, R Maiolino, Stefano Carniani, J Scholtz, Mirko Curti, Christopher N A Willmer, Andrew J Bunker, Jakob M. Helton, I Juodžbalis, Fengwu Sun
+31 more Sandro Tacchella, Santiago Arribas, Alex J Cameron, Stéphane Charlot, Emma Curtis-Lake, Kevin Hainline, Benjamin D Johnson, Brant Robertson, Christina C Williams, Chris Willott, William Baker, Jacopo Chevallard, A Lola Danhaive, Yuki Isobe, Xihan Ji, Zhiyuan Ji, Gareth C Jones, Nimisha Kumari, Tobias J. Looser, Jianwei Lyu, Eleonora Parlanti, Michele Perna, Dávid Puskás, Pierluigi Rinaldi, Charlotte Simmonds, Yang Sun, Hannah Übler, Giacomo Venturi, Joris Witstok, Zihao Wu, Yongda Zhu
Cited by: 3
References: 123

Abstract

ABSTRACT We present James Web Space Telescope/NIRSpec dense-shutter spectroscopy (DSS). This novel observing strategy with the NIRSpec/multi-shutter assembly (MSA) deliberately permits a high number of controlled spectral overlaps to reach extreme multiplex while retaining the low background of slit spectroscopy. In a single configuration over the JADES Origins Field, we opened shutters on all faint ($m_\mathrm{F444W}\lt 30$ mag) $z_{\rm phot}\gt 3$ candidates, prioritizing emission-line science and rejecting only bright continuum sources. Using 33.6 and 35.8 ks on-source in G235M and G395M, we observed a single mask with $\sim$850 sources, obtaining spectroscopic redshifts for $\sim$540 galaxies over $2.5\lesssim z \lesssim 8.9$. The per-configuration target density in DSS mode is 4–5$\times$ higher than standard no- and low-overlap MSA strategies (

Fields of Study & Subjects

Galaxies: Formation Evolution Phenomena Astronomy and Astrophysical Research Astrophysics and Star Formation Studies

Publication details

Journal / source
Monthly Notices of the Royal Astronomical Society
Publisher
Oxford University Press (OUP)
Volume
549
Issue
2
Publication date
30 April 2026
Language
EN