Stellar Parameters of BOSS M dwarfs in SDSS-V DR19
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2025
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| author | Qiu, Dan Johnson, Jennifer A. Liu, Chao Souto, Diogo Medan, Ilija Stringfellow, Guy S. Way, Zachary Ting, Yuan-sen Casey, Andrew R. Rojas-Ayala, Bárbara López-Valdivia, Ricardo Song, Ying-Yi Zhang, Bo Li, Jiadong Behmard, Aida Mészáros, Szabolcs Stassun, Keivan G. Fernández-Trincado, José G. |
| author_facet | Qiu, Dan Johnson, Jennifer A. Liu, Chao Souto, Diogo Medan, Ilija Stringfellow, Guy S. Way, Zachary Ting, Yuan-sen Casey, Andrew R. Rojas-Ayala, Bárbara López-Valdivia, Ricardo Song, Ying-Yi Zhang, Bo Li, Jiadong Behmard, Aida Mészáros, Szabolcs Stassun, Keivan G. Fernández-Trincado, José G. |
| contents | We utilized the Stellar LAbel Machine (SLAM), a data-driven model based on Support Vector Regression, to derive stellar parameters ([Fe/H], $T_{\rm eff}$, and $\log{g}$) for SDSS-V M dwarfs using low-resolution optical spectra (R$\sim$2000) obtained with the BOSS spectrographs. These parameters are calibrated using LAMOST F, G or K dwarf companions ([Fe/H]), and APOGEE Net ($T_{\rm eff}$ and $\log{g}$), respectively. Comparisons of SLAM predicted [Fe/H] values between two components of M+M dwarfs wide binaries show no bias but with a scatter of 0.11 dex. Further comparisons with two other works, which also calibrated the [Fe/H] of M dwarfs by using the F/G/K companions, reveal biases of -0.06$\pm$0.16 dex and 0.02$\pm$0.14 dex, respectively. The SLAM-derived effective temperatures agree well with the temperature which is calibrated by using interferometric angular diameters (bias: -27$\pm$92 K) and those of the LAMOST (bias: -34$\pm$65 K), but are systematically lower than those from an empirical relationship between the color index and $T_{\rm eff}$ by 146$\pm$45 K. The SLAM surface gravity aligns well with those of LAMOST (bias: -0.01$\pm$0.07 dex) and those derived from the stellar mass and radius (bias: -0.04$\pm$0.09 dex). Finally, we investigated a bias in [Fe/H] between SLAM and APOGEE ASPCAP. It depends on ASPCAP's [Fe/H] and $T_{\rm eff}$, we provide an equation to correct the ASPCAP metallicities. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2511_20005 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Stellar Parameters of BOSS M dwarfs in SDSS-V DR19 Qiu, Dan Johnson, Jennifer A. Liu, Chao Souto, Diogo Medan, Ilija Stringfellow, Guy S. Way, Zachary Ting, Yuan-sen Casey, Andrew R. Rojas-Ayala, Bárbara López-Valdivia, Ricardo Song, Ying-Yi Zhang, Bo Li, Jiadong Behmard, Aida Mészáros, Szabolcs Stassun, Keivan G. Fernández-Trincado, José G. Solar and Stellar Astrophysics Astrophysics of Galaxies We utilized the Stellar LAbel Machine (SLAM), a data-driven model based on Support Vector Regression, to derive stellar parameters ([Fe/H], $T_{\rm eff}$, and $\log{g}$) for SDSS-V M dwarfs using low-resolution optical spectra (R$\sim$2000) obtained with the BOSS spectrographs. These parameters are calibrated using LAMOST F, G or K dwarf companions ([Fe/H]), and APOGEE Net ($T_{\rm eff}$ and $\log{g}$), respectively. Comparisons of SLAM predicted [Fe/H] values between two components of M+M dwarfs wide binaries show no bias but with a scatter of 0.11 dex. Further comparisons with two other works, which also calibrated the [Fe/H] of M dwarfs by using the F/G/K companions, reveal biases of -0.06$\pm$0.16 dex and 0.02$\pm$0.14 dex, respectively. The SLAM-derived effective temperatures agree well with the temperature which is calibrated by using interferometric angular diameters (bias: -27$\pm$92 K) and those of the LAMOST (bias: -34$\pm$65 K), but are systematically lower than those from an empirical relationship between the color index and $T_{\rm eff}$ by 146$\pm$45 K. The SLAM surface gravity aligns well with those of LAMOST (bias: -0.01$\pm$0.07 dex) and those derived from the stellar mass and radius (bias: -0.04$\pm$0.09 dex). Finally, we investigated a bias in [Fe/H] between SLAM and APOGEE ASPCAP. It depends on ASPCAP's [Fe/H] and $T_{\rm eff}$, we provide an equation to correct the ASPCAP metallicities. |
| title | Stellar Parameters of BOSS M dwarfs in SDSS-V DR19 |
| topic | Solar and Stellar Astrophysics Astrophysics of Galaxies |
| url | https://arxiv.org/abs/2511.20005 |