Can I read The UNCOVER Survey: First Release of Ultradeep JWST/NIRSpec PRISM spectra for ~700 galaxies from z~0.3-13 in Abell 2744 on EtoBox?

The UNCOVER Survey: First Release of Ultradeep JWST/NIRSpec PRISM spectra for ~700 galaxies from z~0.3-13 in Abell 2744 by Price, Sedona H.; Bezanson, Rachel; Labbe, Ivo; Furtak, Lukas J.; de Graaff, Anna; Greene, Jenny E.; Kokorev, Vasily; Setton, David J.; Suess, Katherine A.; Brammer, Gabriel; Cutler, Sam E.; Leja, Joel; Pan, Richard; Wang, Bingjie; Weaver, John R.; Whitaker, Katherine E.; Atek, Hakim; Burgasser, Adam J.; Chemerynska, Iryna; Dayal, Pratika; Feldmann, Robert; Schreiber, Natascha M. Förster; Fudamoto, Yoshinobu; Fujimoto, Seiji; Glazebrook, Karl; Goulding, Andy D.; Khullar, Gourav; Kriek, Mariska; Marchesini, Danilo; Maseda, Michael V.; Miller, Tim B.; Muzzin, Adam; Nanayakkara, Themiya; Nelson, Erica; Oesch, Pascal A.; Shipley, Heath; Smit, Renske; Taylor, Edward N.; van Dokkum, Pieter; Williams, Christina C.; Zitrin, Adi is a scholarly article available to read on EtoBox.

What is The UNCOVER Survey: First Release of Ultradeep JWST/NIRSpec PRISM spectra for ~700 galaxies from z~0.3-13 in Abell 2744 about?

We present the design and observations of low resolution JWST/NIRSpec PRISM spectroscopy from the Ultradeep NIRSpec and NIRCam ObserVations before the Epoch of Reionization (UNCOVER) Cycle 1 JWST Treasury program. Targets are selected using JWST/NIRCam photometry from UNCOVER and other programs, and cover a wide range of categories and redshifts to ensure the legacy value of the survey. These categories include the first galaxies at $z\gtrsim10$, faint galaxies during the Epoch of Reionization ($z\sim6-8$), high redshift AGN ($z\gtrsim6$), Population III star candidates, distant quiescent and dusty galaxies ($1\lesssim{}z\lesssim 6$), and filler galaxies sampling redshift--color--magnitude space from z~0.1-13. Seven NIRSpec MSA masks across the extended Abell 2744 cluster were observed, along with NIRCam parallel imaging in 8 filters (F090W, F115W, F150W, F200W, F277W, F356W, F410M, F444W, F480M) over a total area of ~26 arcmin$^2$, overlapping existing HST coverage from programs including the Hubble Frontier Fields and BUFFALO. We successfully observed 553 objects down to $m_{\mathrm{F444W}}\sim30\mathrm{AB}$, and by leveraging mask overlaps, we reach total on-target exposure time

Author

Price, Sedona H.; Bezanson, Rachel; Labbe, Ivo; Furtak, Lukas J.; de Graaff, Anna; Greene, Jenny E.; Kokorev, Vasily; Setton, David J.; Suess, Katherine A.; Brammer, Gabriel; Cutler, Sam E.; Leja, Joel; Pan, Richard; Wang, Bingjie; Weaver, John R.; Whitaker, Katherine E.; Atek, Hakim; Burgasser, Adam J.; Chemerynska, Iryna; Dayal, Pratika; Feldmann, Robert; Schreiber, Natascha M. Förster; Fudamoto, Yoshinobu; Fujimoto, Seiji; Glazebrook, Karl; Goulding, Andy D.; Khullar, Gourav; Kriek, Mariska; Marchesini, Danilo; Maseda, Michael V.; Miller, Tim B.; Muzzin, Adam; Nanayakkara, Themiya; Nelson, Erica; Oesch, Pascal A.; Shipley, Heath; Smit, Renske; Taylor, Edward N.; van Dokkum, Pieter; Williams, Christina C.; Zitrin, Adi

Published

2024

Language

EN