Planck is not alone in this search. In early 2014, another team of astronomers presented results based on observations of the polarized CMB on a small patch of the sky performed 2010-12 with BICEP2, an experiment located at the South Pole. The team also used preliminary data from another South Pole experiment, the Keck Array.
They found something new: curly B-modes in the polarization observed over stretches of the sky a few times larger than the size of the Full Moon.
The BICEP2 team presented evidence favoring the interpretation that this signal originated in primordial gravitational waves, sparking an enormous response in the academic community and general public. However, there is another contender in this game that can produce a similar effect: interstellar dust in our galaxy, the Milky Way.
The Milky Way is pervaded by a mixture of gas and dust shining at similar frequencies to those of the CMB, and this foreground emission affects the observation of the most ancient cosmic light. Very careful analysis is needed to separate the foreground emission from the cosmic background.
Critically, interstellar dust also emits polarized light, thus affecting the CMB polarization as well.
“When we first detected this signal in our data, we relied on models for galactic dust emission that were available at the time,” says John Kovac, a principal investigator of BICEP2 at Harvard University in Massachusetts. “These seemed to indicate that the region of the sky chosen for our observations had dust polarization much lower than the detected signal.”
The two ground-based experiments collected data at a single microwave frequency, making it difficult to separate the emissions coming from the Milky Way and the background.
On the other hand, Planck observed the sky in nine microwave and submillimeter frequency channels, seven of which were also equipped with polarization-sensitive detectors. By careful analysis, these multi-frequency data can be used to separate the various contributions.
The BICEP2 team had chosen a field where they believed dust emission would be low, and thus interpreted the signal as likely to be cosmological.
However, as soon as Planck’s maps of the polarized emission from galactic dust were released, it was clear that this foreground contribution could be much higher than previously expected.
In fact, in September 2014,
Planck revealed for the first time that the polarized emission from dust is significant over the entire sky and comparable to the signal detected by BICEP2 even in the cleanest regions.
So, the Planck and BICEP2 teams joined forces, combining the satellite’s ability to deal with foregrounds using observations at several frequencies — including those where dust emission is strongest — with the greater sensitivity of the ground-based experiments over limited areas of the sky, thanks to their more recent, improved technology. By then, the full Keck Array data from 2012 and 2013 had also become available.
“This joint work has shown that the detection of primordial B-modes is no longer robust once the emission from galactic dust is removed,” says Jean-Loup Puget, principal investigator of the HFI instrument on Planck at the Institut d’Astrophysique Spatiale in Orsay, France. “So, unfortunately, we have not been able to confirm that the signal is an imprint of cosmic inflation.”