Improving baryon acoustic oscillation measurement with the combination of cosmic voids and galaxies


Por: Zhao, Cheng, Chuang, Chia-Hsun, Kitaura, Francisco-Shu, Liang, Yu, Pellejero-Ibanez, Marcos, Tao, Charling, Vargas-Magaa, Mariana, Variu, Andrei, Yepes, Gustavo

Publicada: 1 ene 2020
Resumen:
We develop a methodology to optimize the measurement of baryon acoustic oscillation (BAO) from a given galaxy sample. In our previous work, we demonstrated that one can measure BAO from tracers in underdense regions (voids). In this study, we combine the overdense and underdense tracers (galaxies and voids) to obtain better constraints on the BAO scale. To this end, we modify the de-wiggled BAO model with an additional parameter to describe both the BAO peak and the underlying exclusion pattern of void 2PCFs. We show that after applying BAO reconstruction to galaxies, the BAO peak scale of both galaxies and voids are unbiased using the modified model. Furthermore, we use a new 2PCF estimator for a multitracer analysis with galaxies and voids. In simulations, the joint sample improves by about 10 per cent the constraint for the post-reconstruction BAO peak position compared to the result from galaxies alone, which is equivalent to an enlargement of the survey volume by 20 per cent. Applying this method to the BOSS DR12 data, we have an 18 per cent improvement for the low-z sample (0.2 < z< 0.5), but a worse constraint for the high-z sample (0.5 < z < 0.75), which is consistent with statistical fluctuations for the current survey volume. Future larger samples will give more robust improvements due to less statistical fluctuations.

Filiaciones:
Zhao, Cheng:
 Ecole Polytech Fed Lausanne, Lab Astrophys, Observ Sauverny, CH-1290 Versoix, Switzerland

 Tsinghua Univ, Tsinghua Ctr Astrophys THCA, Beijing 100084, Peoples R China

 Tsinghua Univ, Dept Phys, Beijing 100084, Peoples R China

 Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China

Chuang, Chia-Hsun:
 Stanford Univ, Kavli Inst Particle Astrophys & Cosmol, Stanford, CA 94305 USA

 Stanford Univ, Phys Dept, Stanford, CA 94305 USA

 Leibniz Inst Astrophys Potsdam AIP, Sternwarte 16, D-14482 Potsdam, Germany

Kitaura, Francisco-Shu:
 IAC, C Via Lactea S-N, E-38200 Tenerife, Spain

 Univ La Laguna, Dept Astrofis, E-38206 Tenerife, Spain

Liang, Yu:
 Tsinghua Univ, Tsinghua Ctr Astrophys THCA, Beijing 100084, Peoples R China

 Tsinghua Univ, Dept Phys, Beijing 100084, Peoples R China

Pellejero-Ibanez, Marcos:
 IAC, C Via Lactea S-N, E-38200 Tenerife, Spain

 Univ La Laguna, Dept Astrofis, E-38206 Tenerife, Spain

Tao, Charling:
 Tsinghua Univ, Tsinghua Ctr Astrophys THCA, Beijing 100084, Peoples R China

 Tsinghua Univ, Dept Phys, Beijing 100084, Peoples R China

 Univ Aix Marseille, CPPM, CNRS, IN2P3, Case 907, F-13288 Marseille 9, France

Vargas-Magaa, Mariana:
 Univ Nacl Autonoma Mexico, Inst Fis, Apdo Postal 20-364, Mexico City, DF, Mexico

Variu, Andrei:
 Ecole Polytech Fed Lausanne, Lab Astrophys, Observ Sauverny, CH-1290 Versoix, Switzerland

Yepes, Gustavo:
 Univ Autonoma Madrid, Fac Ciencias, Dept Fis Teor, Modulo 8, E-28049 Madrid, Spain
ISSN: 00358711
Editorial
WILEY-BLACKWELL, COMMERCE PLACE, 350 MAIN ST, MALDEN 02148, MA USA, Reino Unido
Tipo de documento: Article
Volumen: 491 Número: 3
Páginas: 4554-4572
WOS Id: 000512306500109
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