Spectroscopic Confirmation of CEERS NIRCam-selected Galaxies at z ≃ 8-10
| dc.contributor.author | Haro, Pablo Arrabal, Dickinson, Mark, Finkelstein, Steven L., Fujimoto, Seiji, Fernandez, Vital, Kartaltepe, Jeyhan S., Jung, Intae, Cole, Justin W., Burgarella, Denis, Chworowsky, Katherine, Hutchison, Taylor A., Morales, Alexa M., Papovich, Casey, Simons, Raymond C., Amorin, Ricardo O., Backhaus, Bren E., Bagley, Micaela B., Bisigello, Laura, Calabro, Antonello, Castellano, Marco, Cleri, Nikko J., Dave, Romeel, Dekel, Avishai, Ferguson, Henry C., Fontana, Adriano, Gawiser, Eric, Giavalisco, Mauro, Harish, Santosh, Hathi, Nimish P., Hirschmann, Michaela, Holwerda, Benne W., Huertas-Company, Marc, Koekemoer, Anton M., Larson, Rebecca L., Lucas, Ray A., Mobasher, Bahram, Perez-Gonzalez, Pablo G., Pirzkal, Nor, Rose, Caitlin, Santini, Paola, Trump, Jonathan R., de la Vega, Alexander, Wang, Xin, Weiner, Benjamin J., Wilkins, Stephen M., Yang, Guang, Yung, L. Y. Aaron, Zavala, Jorge A. | |
| dc.date.accessioned | 2024-11-27T21:50:38Z | |
| dc.date.available | 2024-11-27T21:50:38Z | |
| dc.date.issued | 2023/07/01 | |
| dc.description.abstract | We present JWST/NIRSpec prism spectroscopy of seven galaxies selected from Cosmic Evolution Early Release Science (CEERS) survey NIRCam imaging with photometric redshifts z(phot) > 8. We measure emission line redshifts of z = 7.65 and 8.64 for two galaxies. For two other sources without securely detected emission lines we measure = z 9.77(-0.29)(+0.37) and 10.01 (+0.14)(-0.19) by fitting model spectral templates to the prism data, from which we detect continuum breaks consistent with Ly alpha opacity from a mostly neutral intergalactic medium. The presence of strong breaks and the absence of strong emission lines give high confidence that these two galaxies have redshifts z > 9.6, but the redshift values derived from the breaks alone have large uncertainties given the low spectral resolution and relatively low S/N of the CEERS NIRSpec prism data. The two z similar to 10 sources observed are relatively luminous (MUV < -20), with blue continua (-2.3 less than or similar to ss less than or similar to -1.9) and low dust attenuation ( A similar or equal to 0.15(- 0.1)(+ 0.3)), and at least one of them has a high stellar mass for a galaxy at that redshift ( log M-* M-circle dot similar or equal to 9.3(-0.30)(+0.2) ). Considered together with spectroscopic observations of other CEERS NIRCam-selected high-z galaxy candidates in the literature, we find a high rate of redshift confirmation and low rate of confirmed interlopers (8%). Ten out of 35 z > 8 candidates with CEERS NIRSpec spectroscopy do not have secure redshifts, but the absence of emission lines in their spectra is consistent with redshifts z > 9.6. We find that z > 8 photometric redshifts are generally in agreement (within their uncertainties) with the spectroscopic values, but also that the photometric redshifts tend to be slightly overestimated ( = 0.45 +/- 0.11), suggesting that current templates do not fully describe the spectra of veryhigh-z sources. Overall, the spectroscopy solidifies photometric redshift evidence for a high spatial density of bright galaxies at z > 8 compared to theoretical model predictions, and further disfavors an accelerated decline in the integrated UV luminosity density at z > 8. | |
| dc.identifier.doi | http://dx.doi.org/10.3847/2041-8213/acdd54 | |
| dc.identifier.issn | 2041-8205 | |
| dc.identifier.uri | https://publicacionesabiertas.userena.cl/handle/123456789/142 | |
| dc.language | English | |
| dc.publisher | IOP Publishing Ltd | |
| dc.subject | ULTRAVIOLET LUMINOSITY FUNCTIONS, HIGH REDSHIFT GALAXIES, STAR-FORMATION, JWST, I., EVOLUTION, EMISSION, CANDELS, DUST, CANDIDATES | |
| dc.title | Spectroscopic Confirmation of CEERS NIRCam-selected Galaxies at z ≃ 8-10 | |
| dc.type | Article |
