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<rdf:RDF xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:dc="http://purl.org/dc/elements/1.1/"><rdf:Description rdf:about="https://repozitorij.uni-lj.si/IzpisGradiva.php?id=163786"><dc:title>The GLASS-JWST Early Release Science Program</dc:title><dc:creator>Mascia,	Sara	(Avtor)
	</dc:creator><dc:creator>Roberts-Borsani,	Guido	(Avtor)
	</dc:creator><dc:creator>Treu,	Tommaso	(Avtor)
	</dc:creator><dc:creator>Pentericci,	Laura	(Avtor)
	</dc:creator><dc:creator>Chen,	Wenlei	(Avtor)
	</dc:creator><dc:creator>Calabrò,	Antonello	(Avtor)
	</dc:creator><dc:creator>Bradač,	Maruša	(Avtor)
	</dc:creator><dc:subject>galaxies evolution</dc:subject><dc:subject>galaxies formation</dc:subject><dc:subject>early universe</dc:subject><dc:subject>galaxies evolution</dc:subject><dc:subject>high-redshift galaxies</dc:subject><dc:subject>spectroscopic surveys</dc:subject><dc:description>We release fully reduced spectra obtained with NIRSpec onboard JWST as part of the GLASS-JWST Early Release Science Program and a follow-up Director’s Discretionary Time program 2756. From these 263 spectra of 245 unique sources, acquired with low (R = 30–300) and high dispersion (R ∼ 2700) gratings, we derive redshifts for 200 unique sources in the redshift range z = 0–10. We describe the sample selection and characterize its high completeness as a function of redshift and apparent magnitude. Comparison with independent estimates based on different methods and instruments shows that the redshifts are accurate, with 80% differing less than 0.005. We stack the GLASS-JWST spectra to produce the first high-resolution (R ∼ 2700) JWST spectral template extending in the rest frame wavelength from 2000 Å to 20 000 Å. Catalogs, reduced spectra, and template are made publicly available to the community.</dc:description><dc:date>2024</dc:date><dc:date>2024-10-10 16:53:53</dc:date><dc:type>Članek v reviji</dc:type><dc:identifier>163786</dc:identifier><dc:language>sl</dc:language></rdf:Description></rdf:RDF>
