GA-NIFS: JWST/NIRSpec IFS view of the z~3.5 galaxy GS5001 and its close environment at the core of a large-scale overdensity
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| Formato: | Preprint |
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2024
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| author | Lamperti, Isabella Arribas, Santiago Perna, Michele Del Pino, Bruno Rodríguez Circosta, Chiara Pérez-González, Pablo G. Bunker, Andrew J. Carniani, Stefano Charlot, Stéphane D'Eugenio, Francesco Maiolino, Roberto Übler, Hannah Willott, Chris J. Bertola, Elena Böker, Torsten Cresci, Giovanni Curti, Mirko Jones, Gareth C. Kumari, Nimisha Parlanti, Eleonora Scholtz, Jan Venturi, Giacomo |
| author_facet | Lamperti, Isabella Arribas, Santiago Perna, Michele Del Pino, Bruno Rodríguez Circosta, Chiara Pérez-González, Pablo G. Bunker, Andrew J. Carniani, Stefano Charlot, Stéphane D'Eugenio, Francesco Maiolino, Roberto Übler, Hannah Willott, Chris J. Bertola, Elena Böker, Torsten Cresci, Giovanni Curti, Mirko Jones, Gareth C. Kumari, Nimisha Parlanti, Eleonora Scholtz, Jan Venturi, Giacomo |
| contents | We present JWST NIRSpec observations in IFS mode of the galaxy GS5001 at redshift z=3.47, the central member of a candidate protocluster in the GOODS-S field. The data cover a field of view (FoV) of 4''$\times$4'' (~$30\times30$~kpc$^2$) and were obtained as part of the GA-NIFS GTO program. The observations include both high (R~2700) and low (R~100) spectral resolution data, spanning the rest-frame wavelength ranges 3700-6780A and 1300-11850A, respectively. We analyse the spatially resolved ionised gas kinematics and interstellar medium properties, including obscuration, gas metallicity, excitation, ionisation parameter, and electron density. In addition to the main galaxy (GS5001), the NIRSpec FoV covers three components in the south, with velocities blue-shifted by -150 km/s with respect to the main galaxy, and another source in the north redshifted by ~200 km/s. Optical line ratio diagnostics indicate star formation ionisation and electron densities of ~500 cm$^{-3}$ across all sources in the FoV. The gas-phase metallicity in the main galaxy is 12+log(O/H) $= 8.45\pm0.04$, and slightly lower in the companions (12+log(O/H)$ = 8.34-8.42$), consistent with the mass-metallicity relation at $z\sim3$. We find peculiar line ratios (high log [NII]/H$α$, low log [OIII]/H$β$) in the northern part of GS5001. These could be attributed to either higher metallicity, or to shocks resulting from the interaction of the main galaxy with the northern source. We identify a spatially resolved outflow in the main galaxy, with an extension of about 3 kpc. We find maximum outflow velocities of ~400 km/s, an outflow mass of $(1.7\pm0.4)\times 10^8$ M$_{\odot}$, a mass outflow rate of $23\pm5$ M$_{\odot}$ yr$^{-1}$ and a mass loading factor of 0.23. These properties are compatible with star formation being the driver of the outflow. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2406_10348 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | GA-NIFS: JWST/NIRSpec IFS view of the z~3.5 galaxy GS5001 and its close environment at the core of a large-scale overdensity Lamperti, Isabella Arribas, Santiago Perna, Michele Del Pino, Bruno Rodríguez Circosta, Chiara Pérez-González, Pablo G. Bunker, Andrew J. Carniani, Stefano Charlot, Stéphane D'Eugenio, Francesco Maiolino, Roberto Übler, Hannah Willott, Chris J. Bertola, Elena Böker, Torsten Cresci, Giovanni Curti, Mirko Jones, Gareth C. Kumari, Nimisha Parlanti, Eleonora Scholtz, Jan Venturi, Giacomo Astrophysics of Galaxies We present JWST NIRSpec observations in IFS mode of the galaxy GS5001 at redshift z=3.47, the central member of a candidate protocluster in the GOODS-S field. The data cover a field of view (FoV) of 4''$\times$4'' (~$30\times30$~kpc$^2$) and were obtained as part of the GA-NIFS GTO program. The observations include both high (R~2700) and low (R~100) spectral resolution data, spanning the rest-frame wavelength ranges 3700-6780A and 1300-11850A, respectively. We analyse the spatially resolved ionised gas kinematics and interstellar medium properties, including obscuration, gas metallicity, excitation, ionisation parameter, and electron density. In addition to the main galaxy (GS5001), the NIRSpec FoV covers three components in the south, with velocities blue-shifted by -150 km/s with respect to the main galaxy, and another source in the north redshifted by ~200 km/s. Optical line ratio diagnostics indicate star formation ionisation and electron densities of ~500 cm$^{-3}$ across all sources in the FoV. The gas-phase metallicity in the main galaxy is 12+log(O/H) $= 8.45\pm0.04$, and slightly lower in the companions (12+log(O/H)$ = 8.34-8.42$), consistent with the mass-metallicity relation at $z\sim3$. We find peculiar line ratios (high log [NII]/H$α$, low log [OIII]/H$β$) in the northern part of GS5001. These could be attributed to either higher metallicity, or to shocks resulting from the interaction of the main galaxy with the northern source. We identify a spatially resolved outflow in the main galaxy, with an extension of about 3 kpc. We find maximum outflow velocities of ~400 km/s, an outflow mass of $(1.7\pm0.4)\times 10^8$ M$_{\odot}$, a mass outflow rate of $23\pm5$ M$_{\odot}$ yr$^{-1}$ and a mass loading factor of 0.23. These properties are compatible with star formation being the driver of the outflow. |
| title | GA-NIFS: JWST/NIRSpec IFS view of the z~3.5 galaxy GS5001 and its close environment at the core of a large-scale overdensity |
| topic | Astrophysics of Galaxies |
| url | https://arxiv.org/abs/2406.10348 |