Strategies for obtaining robust SED fitting parameters for galaxies at z~1 and z~2 in the absence of IR data
Fuente:
arXiv
Guardado en:
| Autores principales: | Osborne, Chandler, Salim, Samir |
|---|---|
| Formato: | Preprint |
| Publicado: |
2024
|
| Materias: | |
| Acceso en línea: | |
| Etiquetas: |
Agregar Etiqueta
Sin Etiquetas, Sea el primero en etiquetar este registro!
|
Ejemplares similares
Assessment of SDSS-Derived Galaxy Morphologies Using HST Imaging
por: Osborne, Chandler, et al.
Publicado: (2024)
por: Osborne, Chandler, et al.
Publicado: (2024)
A physically-motivated template set for high-z galaxy SED fitting
por: Luberto, Judah, et al.
Publicado: (2024)
por: Luberto, Judah, et al.
Publicado: (2024)
Uncertainties in high-$z$ galaxy properties inferred from SED fitting using JWST NIRCam photometry
por: Choe, Jiyoung, et al.
Publicado: (2025)
por: Choe, Jiyoung, et al.
Publicado: (2025)
Near-IR clumps and their properties in high-z galaxies with JWST/NIRCam
por: Kalita, Boris S., et al.
Publicado: (2024)
por: Kalita, Boris S., et al.
Publicado: (2024)
The properties of AGN in dwarf galaxies identified via SED fitting
por: Bichang'a, B., et al.
Publicado: (2024)
por: Bichang'a, B., et al.
Publicado: (2024)
4MOST ChANGES: Catalog of high-redshift quasar candidates (4.5 < $z$ < 7) selected with SED fitting
por: Mkrtchyan, T., et al.
Publicado: (2026)
por: Mkrtchyan, T., et al.
Publicado: (2026)
Highly Efficient Identification of Extreme Emission Line Galaxies in the Local Universe: >8000 New Green Pea Candidates at 0.12 < z < 0.36
por: Samonski, Heather, et al.
Publicado: (2025)
por: Samonski, Heather, et al.
Publicado: (2025)
A Dusty Dawn: Galactic Dust Buildup at $z\gtrsim5$
por: Choban, Caleb R., et al.
Publicado: (2024)
por: Choban, Caleb R., et al.
Publicado: (2024)
Tracing the galaxy-halo connection with galaxy clustering in COSMOS-Web from z = 0.1 to z ~ 12
por: Paquereau, Louise, et al.
Publicado: (2025)
por: Paquereau, Louise, et al.
Publicado: (2025)
AGN contribution on the morphological parameters of their host galaxies up to intermediate redshifts of z~2
por: Getachew-Woreta, Tilahun, et al.
Publicado: (2025)
por: Getachew-Woreta, Tilahun, et al.
Publicado: (2025)
Improved SED-Fitting Assumptions Result in Inside-Out Quenching at $z\sim0.5$ and Quenching at All Radii Simultaneously at $z\sim1$
por: de la Vega, Alexander, et al.
Publicado: (2025)
por: de la Vega, Alexander, et al.
Publicado: (2025)
Early galaxy evolution: The complex interstellar medium distribution of the z~7 galaxy A1689-zD1
por: Knudsen, Kirsten K., et al.
Publicado: (2025)
por: Knudsen, Kirsten K., et al.
Publicado: (2025)
The rise and fall of bars in disc galaxies from $z=1$ to $z=0$. The role of the environment
por: Rosas-Guevara, Yetli, et al.
Publicado: (2024)
por: Rosas-Guevara, Yetli, et al.
Publicado: (2024)
ProGeny II: the impact of libraries and model configurations on inferred galaxy properties in SED fitting
por: Bellstedt, Sabine, et al.
Publicado: (2024)
por: Bellstedt, Sabine, et al.
Publicado: (2024)
Simulated [CII] in high-z galaxies
por: Muñoz-Elgueta, N., et al.
Publicado: (2024)
por: Muñoz-Elgueta, N., et al.
Publicado: (2024)
The LOFAR window on star-forming galaxies and AGN - curved radio SEDs and IR-radio correlation at $0 < z < 2.5$
por: Calistro-Rivera, G., et al.
Publicado: (2017)
por: Calistro-Rivera, G., et al.
Publicado: (2017)
Metal line emission around z<1 galaxies
por: Dutta, Rajeshwari, et al.
Publicado: (2024)
por: Dutta, Rajeshwari, et al.
Publicado: (2024)
SDSS low z quasar companion galaxies
por: Bettoni, D., et al.
Publicado: (2025)
por: Bettoni, D., et al.
Publicado: (2025)
Radio properties of high-redshift galaxies at $z \geq 1$
por: Khabibullina, M., et al.
Publicado: (2024)
por: Khabibullina, M., et al.
Publicado: (2024)
Cluster candidates with massive quiescent galaxies at $z\sim2$
por: Kiyota, Tomokazu, et al.
Publicado: (2024)
por: Kiyota, Tomokazu, et al.
Publicado: (2024)
The kinematic imprinting of environmental quenching in $z<0.2$ galaxies
por: de Isídio, Natan, et al.
Publicado: (2026)
por: de Isídio, Natan, et al.
Publicado: (2026)
Probing galaxy evolution from $z=0$ to $z\simeq10$ through galaxy scaling relations in three L-Galaxies flavours
por: Vani, Akash, et al.
Publicado: (2024)
por: Vani, Akash, et al.
Publicado: (2024)
Disc asymmetry characterisation in JWST-observed galaxies at 1 < z < 4
por: Ganapathy, Ananya, et al.
Publicado: (2024)
por: Ganapathy, Ananya, et al.
Publicado: (2024)
On the ages of the stellar populations of galaxies at $z=0.1$-7
por: Martínez-García, Eric E.
Publicado: (2025)
por: Martínez-García, Eric E.
Publicado: (2025)
Dust attenuation evolution in $z \sim 2$-$12$ JWST galaxies
por: Markov, V., et al.
Publicado: (2024)
por: Markov, V., et al.
Publicado: (2024)
Probing the influence of the protocluster environment on galaxy morphology at z = 2.23
por: Golden-Marx, Emmet, et al.
Publicado: (2025)
por: Golden-Marx, Emmet, et al.
Publicado: (2025)
Blue Monsters and Dusty Descendants: Reconciling UV and IR Emission from Galaxies from z=7, up to z= 14
por: Sommovigo, Laura, et al.
Publicado: (2026)
por: Sommovigo, Laura, et al.
Publicado: (2026)
The LEGA-C galaxy survey: multiple quenching channels for quiescent galaxies at $z\sim1$
por: Nersesian, Angelos, et al.
Publicado: (2025)
por: Nersesian, Angelos, et al.
Publicado: (2025)
The eventful life of GS-z14-0, the most distant galaxy at redshift $z=14.32$
por: Ferrara, Andrea
Publicado: (2024)
por: Ferrara, Andrea
Publicado: (2024)
An independent estimate of H(z) at z = 0.5 from the stellar ages of brightest cluster galaxies
por: Loubser, S. Ilani, et al.
Publicado: (2025)
por: Loubser, S. Ilani, et al.
Publicado: (2025)
High-z stellar masses can be recovered robustly with JWST photometry
por: Cochrane, R. K., et al.
Publicado: (2024)
por: Cochrane, R. K., et al.
Publicado: (2024)
JADES -- The small blue bump in GN-z11: insights into the nuclear region of a galaxy at z=10.6
por: Ji, Xihan, et al.
Publicado: (2024)
por: Ji, Xihan, et al.
Publicado: (2024)
Physical properties of galaxies and the UV Luminosity Function from $z\sim6$ to $z\sim14$ in COSMOS-Web
por: Franco, Maximilien, et al.
Publicado: (2025)
por: Franco, Maximilien, et al.
Publicado: (2025)
Escaping ionizing photons from massive spiral galaxies at $z\sim 1$
por: Maulick, Soumil, et al.
Publicado: (2026)
por: Maulick, Soumil, et al.
Publicado: (2026)
The role of small-scale environments in the quenching of massive galaxies at $1<z<5$
por: Kakimoto, Takumi, et al.
Publicado: (2026)
por: Kakimoto, Takumi, et al.
Publicado: (2026)
A multi-wavelength investigation of spiral structures in $z > 1$ galaxies with JWST
por: Kalita, Boris S., et al.
Publicado: (2025)
por: Kalita, Boris S., et al.
Publicado: (2025)
Recent star formation in 0.5<z<1.5 quiescent galaxies
por: Rutkowski, Michael J., et al.
Publicado: (2025)
por: Rutkowski, Michael J., et al.
Publicado: (2025)
Predicting the resolved CO emission of $z=1-3$ star-forming galaxies
por: Anirudh, Ravishankar, et al.
Publicado: (2025)
por: Anirudh, Ravishankar, et al.
Publicado: (2025)
Gas excitation of post-starburst galaxies at 0.6 < z < 1.3
por: Zanella, A., et al.
Publicado: (2025)
por: Zanella, A., et al.
Publicado: (2025)
The dust emissivity index beta in infrared-bright galaxies at 1.5 < z < 4.2
por: Bendo, G. J., et al.
Publicado: (2025)
por: Bendo, G. J., et al.
Publicado: (2025)
Ejemplares similares
-
Assessment of SDSS-Derived Galaxy Morphologies Using HST Imaging
por: Osborne, Chandler, et al.
Publicado: (2024) -
A physically-motivated template set for high-z galaxy SED fitting
por: Luberto, Judah, et al.
Publicado: (2024) -
Uncertainties in high-$z$ galaxy properties inferred from SED fitting using JWST NIRCam photometry
por: Choe, Jiyoung, et al.
Publicado: (2025) -
Near-IR clumps and their properties in high-z galaxies with JWST/NIRCam
por: Kalita, Boris S., et al.
Publicado: (2024) -
The properties of AGN in dwarf galaxies identified via SED fitting
por: Bichang'a, B., et al.
Publicado: (2024)