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Maria
and Eric Muhlmann Award
Michael Skrutskie, University of Virginia, USA
and The 2MASS team
The
Two-Micron All Sky Survey, 2MASS, was conceived as a logical extension
of the original Two-micron Sky Survey (TMSS) carried out by Neugebauer
and Leighton in the 1960’s. Neugebauer and Leighton realized
that military development of PbS detectors for surveillance opened
up a unique opportunity to explore the sky at infrared wavelengths
four decades ago. A similar renaissance in technology stimulated
by detector development for the Hubble Space Telescope (also leveraging
military investments) in the 1990’s created an opportunity
to carry out an all-sky survey in the near infrared with sensitivity
gains of 1000-fold over the original two-micron sky survey and thus
usher in the era where infrared observations played a dominant role
in many astronomical investigations. Originally promoted by Susan
Kleinmann of the University of Massachusetts, Michael Skrutskie
became the principal investigator soon after the project's inception
and guided it to a successful completion and incremental public
release starting in 2000, improving upon the state of the art by
about three orders of magnitude.
2MASS
has revolutionized modern astronomy. Like its forerunners, the TMSS
and All Sky Survey carried out with the 48” Schmidt telescope
at Palomar Mountain, 2MASS has become an essential reference base
for modern investigations, like the Sloan Digital Sky Survey and
2dF and 6dF surveys. The major discoveries resulting from 2MASS
are:
- the
identification of an entire new class of stars, the L- and T-dwarfs,
with masses well down into the brown dwarf regime below the nuclear
burning limit for hydrogen in stars,
- characterization
of Galactic structure and its interaction with satellite galaxies
by penetrating the obscuration by dust that pervades visual observations,
- revealing
obscured star formation regions in the Galaxy that cannot be seen
at visual wavelengths owing to dust,
- the
discovery of (infra-) red quasars,
- an
accurate census of nearby galaxies,
- and
a refined understanding of the cosmic background radiation at
near-infrared wavelengths.
The
success of 2MASS is the result of years of dedication and astute
guidance from the team’s leaders. Indeed, the original concept
of 2MASS was brilliant but unable to meet its potential until Skrutskie
and his collaborators took on the management of the project. They
guided the construction of two telescopes, one each in the northern
and southern hemisphere, built dedicated instrumentation to run
remotely and automatically and return data products with a high
degree of reliability. The data processing involved an entirely
new level of sophistication in processing ground-based infrared
observations and ultimately met the goals of better than 3% photometric
accuracy, >99% completeness to a J-band magnitude of 16, and
>99.95% source reliability. Many of the achievements of this
team were judged impossible by others at the gestation of the project.
The
2MASS team advanced astronomy in exactly the manner envisioned for
the Muhlmann award, and the ASP has the privilege of bestowing the
award on the 2MASS team.
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