AAS Journals
Published November 23, 2024 | Version v1
Dataset Open

Dataset for "From Halos to Galaxies. X: Decoding Galaxy SEDs with Physical Priors and Accurate Star Formation History Reconstruction"

Creators

  • 1. Department of Astronomy, School of Physics, Peking University, 5 Yiheyuan Road, Beijing 100871, China
  • 2. Kavli Institute for Astronomy and Astrophysics, Peking University, Beijing 100871, China
  • 3. Institute for Computational Cosmology, Department of Physics, Durham University, South Road, Durham, DH1 3LE, UK
  • 4. Centre for Extragalactic Astronomy, Department of Physics, Durham University, South Road, Durham DH1 3LE, UK
  • 5. INAF--Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio 5, I-35122 Padova, Italy
  • 6. INAF--Osservatorio Astrofisico di Arcetri, Largo Enrico Fermi 5, I-50125 Firenze, Italy
  • 7. Department of Astronomy, University of Massachusetts, Amherst MA 01003, USA
  • 8. Department of Astronomy, School of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai 200240, China
  • 9. Tsung-Dao Lee Institute, and Shanghai Key Laboratory for Particle Physics and Cosmology, Shanghai Jiao Tong University, Shanghai 200240, China
  • 10. CAS Key Laboratory for Research in Galaxies and Cosmology, Department of Astronomy, University of Science and Technology of China, Hefei, Anhui 230026, China
  • 11. School of Astronomy and Space Science, University of Science and Technology of China, Hefei 230026, China
  • 12. School of Astronomy and Space Science, Nanjing University, Nanjing 210093, People's Republic of China
  • 13. Cavendish Laboratory, University of Cambridge, 19 J.J. Thomson Avenue, Cambridge, CB3 0HE, UK
  • 14. Kavli Institute for Cosmology, University of Cambridge, Madingley Road, Cambridge, CB3 0HA, UK
  • 15. Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, UK
  • 16. School of Physics and Electronics, Hunan University, Changsha 410082, China
  • 17. Center for Astronomy and Astrophysics and Department of Physics, Fudan University, 2005 Songhu Road, Shanghai 200438, China

Description

This deposit contains the data related to the manuscript "From Halos to Galaxies. X: Decoding Galaxy SEDs with Physical Priors and Accurate Star Formation History Reconstruction" submitted to the Astrophysical Journal. It includes the basic SDSS identifier, stellar mass, star formation rate, fractional formation time, and their errors. A detailed description can be found in Table 1 of the manuscript.

The data is stored in a CSV file. It can be read with standard data analysis packages like Pandas in Python. 

This deposit has also be updated to include a machine-readable table that follows the standards of the AAS Journals and Vizier (datafile1_ApJ57534.mrt). More information on this standard can be found in the AAS or CDS documentation. This format can be read in Python with packages like astropy. 

Files

data_release.csv

Files (144.7 MB)

Name Size Download all
md5:d041d5429ec7262e3a6a01b421cc04ae
66.9 MB Preview Download
md5:4a3869e19a541e043998e19cdfbdaeee
77.8 MB Download

Additional details

Related works

Is supplement to
Preprint: arXiv:2408.07749 (arXiv)