Skip to main content
U.S. Department of Energy
Office of Scientific and Technical Information

First Detection of the Baryon Acoustic Oscillation (BAO) Feature in the 3-Point Correlation Function of DESI DR1 Luminous Red Galaxies

Journal Article · · No journal information
OSTI ID:3020050
 [1];  [1];  [2];  [1];  [1];  [1];  [1];  [3];  [3];  [4];  [5];  [4];  [4];  [6];  [7];  [4];  [4];  [8];  [9];  [10] more »;  [7];  [11];  [12];  [13];  [14];  [15];  [16];  [17];  [18];  [19];  [20];  [21];  [21];  [22];  [4];  [4];  [7];  [23];  [4];  [24];  [25];  [21];  [26];  [27];  [9];  [28];  [29];  [30];  [31];  [32];  [33];  [4];  [19];  [34];  [4];  [21];  [35];  [21];  [36];  [37] « less
  1. Florida U.
  2. U. Waterloo (main); Waterloo U., IQC
  3. Granada U., Theor. Phys. Astrophys.
  4. LBL, Berkeley
  5. Boston U.
  6. Milan U.; Brera Observ.
  7. University Coll. London
  8. Utah U.
  9. UNAM, Mexico
  10. Rochester U.
  11. UC, Berkeley (main); UC, Berkeley, Math. Dept.
  12. Andes U., Bogota
  13. Barcelona, IEEC; Portsmouth U., ICG; ICE, Bellaterra
  14. Virginia U.
  15. Fermilab
  16. Paris, Inst. Astrophys.; IRFU, Saclay
  17. Chicago U., KICP; Ohio State U.
  18. Queensland U.
  19. Michigan U., MCTP; Syracuse U.; Michigan U.; KEK, Tsukuba; Hiroshima Shudo U.
  20. U. Texas, Dallas
  21. Natl. Solar Observ., Tucson
  22. UC, Irvine
  23. Ohio State U.
  24. LPNHE, Paris
  25. Barcelona, IFAE; Barcelona, Autonoma U.
  26. ICREA, Barcelona; Barcelona, IFAE
  27. Siena Coll., Loudonville
  28. Pittsburgh U.
  29. Waterloo U., IQC; Perimeter Inst. Theor. Phys.; U. Waterloo (main)
  30. LBL, Berkeley; UC, Berkeley (main); UC, Berkeley, Math. Dept.
  31. Barcelona, Polytechnic U.
  32. Kansas State U.; Ilia State U.
  33. Madrid, CIEMAT
  34. Ohio U., Athens
  35. Michigan U.; KEK, Tsukuba; Hiroshima Shudo U.
  36. Tsinghua U., Beijing
  37. Beijing Observ.
We present the first detection of the 3-Point Correlation Function (3PCF) Baryon Acoustic Oscillation (BAO) signal from the DESI Data Release 1 (DR1) sample of Luminous Red Galaxies (LRGs), which contains over 2.1 million galaxies. Our analysis is based on a tree-level redshift-space bispectrum template, which is then transformed to position space using the Fast Fourier Transform on Logarithmic scales (FFTLog) algorithm. We detect the BAO feature with a significance of approximately $8.1σ$ using the EZmock covariance matrix and $8.5σ$ using the analytical covariance matrix, for the full LRG redshift range ($0.4
Research Organization:
Syracuse U.; Queensland U.; Beijing Observ.; Rochester U.; Andes U., Bogota; ICREA, Barcelona; UC, Berkeley, Math. Dept.; Paris, Inst. Astrophys.; UNAM, Mexico; IRFU, Saclay; Natl. Solar Observ., Tucson; Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States); UC, Berkeley (main); Boston U.; KEK, Tsukuba; Barcelona, Autonoma U.; Siena Coll., Loudonville; Pittsburgh U.; Hiroshima Shudo U.; Utah U.; Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States); LPNHE, Paris; U. Texas, Dallas; ICE, Bellaterra; Florida U.; Michigan U.; Tsinghua U., Beijing; Portsmouth U., ICG; UC, Irvine; Waterloo U., IQC; Granada U., Theor. Phys. Astrophys.; Ohio State U.; Michigan U., MCTP; Virginia U.; U. Waterloo (main); Barcelona, Polytechnic U.; Chicago U., KICP; Milan U.; University Coll. London; Ilia State U.; Barcelona, IFAE; Barcelona, IEEC; Kansas State U.; Perimeter Inst. Theor. Phys.; Madrid, CIEMAT; Brera Observ.; Ohio U., Athens
Sponsoring Organization:
US Department of Energy
DOE Contract Number:
89243024CSC000002
OSTI ID:
3020050
Report Number(s):
FERMILAB-PUB-26-0107-PPD; oai:inspirehep.net:3121404; arXiv:2602.16134
Journal Information:
No journal information, Journal Name: No journal information
Country of Publication:
United States
Language:
English

Similar Records

Combined tracer analysis for DESI 2024 BAO
Journal Article · Wed Aug 06 20:00:00 EDT 2025 · No journal information · OSTI ID:3019373

Related Subjects