First Detection of the Baryon Acoustic Oscillation (BAO) Feature in the 3-Point Correlation Function of DESI DR1 Luminous Red Galaxies
Journal Article
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· No journal information
OSTI ID:3020050
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- Florida U.
- U. Waterloo (main); Waterloo U., IQC
- Granada U., Theor. Phys. Astrophys.
- LBL, Berkeley
- Boston U.
- Milan U.; Brera Observ.
- University Coll. London
- Utah U.
- UNAM, Mexico
- Rochester U.
- UC, Berkeley (main); UC, Berkeley, Math. Dept.
- Andes U., Bogota
- Barcelona, IEEC; Portsmouth U., ICG; ICE, Bellaterra
- Virginia U.
- Fermilab
- Paris, Inst. Astrophys.; IRFU, Saclay
- Chicago U., KICP; Ohio State U.
- Queensland U.
- Michigan U., MCTP; Syracuse U.; Michigan U.; KEK, Tsukuba; Hiroshima Shudo U.
- U. Texas, Dallas
- Natl. Solar Observ., Tucson
- UC, Irvine
- Ohio State U.
- LPNHE, Paris
- Barcelona, IFAE; Barcelona, Autonoma U.
- ICREA, Barcelona; Barcelona, IFAE
- Siena Coll., Loudonville
- Pittsburgh U.
- Waterloo U., IQC; Perimeter Inst. Theor. Phys.; U. Waterloo (main)
- LBL, Berkeley; UC, Berkeley (main); UC, Berkeley, Math. Dept.
- Barcelona, Polytechnic U.
- Kansas State U.; Ilia State U.
- Madrid, CIEMAT
- Ohio U., Athens
- Michigan U.; KEK, Tsukuba; Hiroshima Shudo U.
- Tsinghua U., Beijing
- 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
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