Published July 20, 2025 | Version v3
Dataset Open

The PPO (Pre/Protostellar Objects) catalogs in W51-E and W51-IRS2 protoclusters ALMA 1.3mm and 3mm continuum images

  • 1. EDMO icon University of Florida
  • 1. University of Florida
  • 2. ROR icon Université Stendhal – Grenoble 3
  • 3. University of Concepcion
  • 4. ROR icon Université Grenoble Alpes
  • 5. ROR icon Sorbonne Université
  • 6. ROR icon Observatoire de Paris
  • 7. ROR icon Laboratoire d'Astrophysique de Bordeaux
  • 8. University of Chile
  • 9. Universitat de Barcelona Facultat de Física
  • 10. ROR icon SKA Observatory
  • 11. ROR icon Herzberg Institute of Astrophysics
  • 12. ROR icon Universidad Nacional Autónoma de México
  • 13. ROR icon Instituto Argentino de Radioastronomía
  • 14. ROR icon Université de Bordeaux
  • 15. ROR icon Universidad Nacional de Concepción
  • 16. ROR icon Yunnan University
  • 17. ROR icon National Tsing Hua University
  • 18. ROR icon National Astronomical Observatory of Japan
  • 19. ROR icon Center for Astrophysics Harvard & Smithsonian

Description

This is the full PPO catalogs extracted from W51-E and W51-IRS2 ALMA Band 3 (ALMA Cycle 5 program 2017.1.0293.S) and Band 6 (ALMA Cycle 3 program 2015.1.01596.S) continuum data. 

The detailed source identification will be described in the paper, ALMA-IMF XX: Core fragmentation in the W51 high-mass star-forming region, Yoo+25 in subm.

The files with XX_PPO1.fits are the full catalogs of Table 2 and 3 in Yoo+25. The table contains ID, RA (deg), Dec (deg), 1.3mm peak flux in Jy/beam, 3mm peak flux in Jy/beam, spectral index, spectral index error, and the spectral index group described in Sec 3.2. in Yoo+25.

"w51e" and "w51n" in XX refer to W51-E and W51-IRS2, respectively.

The files with XX_PPO2.fits are the full catalogs of Table 4 and 5 in Yoo+25. The table includes ID, the integrated flux (Jy) at 1.3mm and 3mm and their error, dust temperature in K, estimated dust mass (in Msun) assuming constant temperature and modified blackbody temperature, deconvolved size in major and minor axis in AU, and the position angle. 

The integrated flux, deconvolved size, and the position angles are estimated from TGIF (https://zenodo.org/records/13973837). 

We also provide the catalogs of unselected sources, ambiguous and low S/N in Appendix F of Yoo+25. The tables consist of four columns, RA, DEC, isdetected_b3, isdetected_b6. 

 

 

 

 

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