Journal
ASTROPHYSICAL JOURNAL
Volume 889, Issue 1, Pages -Publisher
IOP Publishing Ltd
DOI: 10.3847/1538-4357/ab63df
Keywords
Galaxy formation; Galaxy evolution; Galaxy dark matter halos; Circumgalactic medium; Extragalactic astronomy; Galaxy environments; Galaxy groups; Galaxy clusters
Categories
Funding
- China 973 Program [2015CB857002]
- National Science Foundation of China [11233005, 11621303, 11522324, 11421303, 11503065, 11673015, 11733004]
- CITA National Fellowship
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We present the detection of the kinetic Sunyaev-Zel'dovich effect (kSZE) signals from groups of galaxies as a function of halo mass down to Planck cosmic microwave background maps and stacking about 40,000 galaxy systems with known positions, halo masses, and peculiar velocities. The signals from groups of different mass are constrained simultaneously to take care of the projection effects of nearby halos. The total kSZE flux within halos estimated implies that the gas fraction in halos is about the universal baryon fraction, even in low-mass halos, indicating that the missing baryons are found. Various tests performed show that our results are robust against systematic effects, such as contamination by infrared/radio sources and background variations, beam size effects, and contributions from halo exteriors. Combined with the thermal Sunyaev-Zel'dovich effect, our results indicate that the missing baryons associated with galaxy groups are contained in warm-hot media with temperatures between 10(5) and 10(6) K.
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