Results 51 to 60 of about 74,495 (201)
SpecCLIP: Aligning and Translating Spectroscopic Measurements for Stars
In recent years, large language models (LLMs) have transformed natural language understanding through vast data sets and large-scale parameterization. Inspired by this success, we present SpecCLIP, a foundation model framework that extends LLM-inspired ...
Xiaosheng Zhao +8 more
doaj +1 more source
Comparing the Host Galaxies of Type Ia, Type II and Type Ibc Supernovae
We compare the host galaxies of 902 supernovae, including SNe Ia, SNe II and SNe Ibc, which are selected by cross-matching the Asiago Supernova Catalog with the SDSS Data Release 7.
Chen, X. Y. +10 more
core +2 more sources
Open Cluster Characterization via Cross-Correlation with Spectral Library [PDF]
We present a characterization method based on spectral cross-correlation to obtain the physical parameters of the controversial stellar aggregate ESO442-SC04.
Andrés E. Piatti +8 more
core +2 more sources
A New Wide-field Infrared Survey Explorer Calibration of Stellar Mass
We derive new empirical scaling relations between Wide-field Infrared Survey Explorer (WISE) mid-IR (MIR) galaxy photometry and well-determined stellar masses from spectral energy distribution modeling of a suite of optical–infrared photometry provided ...
T. H. Jarrett +5 more
doaj +1 more source
Spectral Properties of Galaxies in Void Regions
We present a study of spectral properties of galaxies in underdense large-scale structures, voids. Our void galaxy sample (75,939 galaxies) is selected from the Sloan Digital Sky Survey (SDSS) Data Release 7 (DR7) with $\rm z < 0.107$. We find that there
Constantin, Anca +5 more
core +1 more source
CORMASS: A Compact and Efficient NIR Spectrograph for Studying Low-Mass Objects [PDF]
CorMASS (Cornell Massachusetts Slit Spectrograph) is a compact, low-resolution (R=300), double-pass prism cross-dispersed near-infrared (NIR) spectrograph in operation on the Palomar Observatory 60-inch telescope.
Colonno, M. R. +8 more
core +3 more sources
Publication in the conference proceedings of EUSIPCO, Toulouse, France ...
Cavallin, Yoann +2 more
openaire +1 more source
Near-infrared spectra of ISO selected Chamaeleon I young stellar objects
We present 0.95--2.5 micron moderate (R = 500) resolution spectra of 19 ISOCAM detected sources in the Chamaeleon I dark cloud. Thirteen of these stars are candidate very low mass members of the cloud proposed by Persi et al.
Allard +57 more
core +1 more source
A Robust Young Stellar Object Identification Method Based on Deep Learning
Young stellar objects (YSOs) represent the earliest stage in the process of star formation, offering insights that contribute to the development of models elucidating star formation and evolution.
Lei Tan +6 more
doaj +1 more source

