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Today’s telescopes study the sky across the electromagnetic spectrum.
Each part of the spectrum tells us different things about the Universe,
giving us more pieces of the cosmic jigsaw puzzle.
The most powerful telescopes on the ground and in space
have joined forces over the last decade
in a unique observing campaign, known as GOODS,
which reaches across the spectrum and deep back into cosmic time.
This is the ESOcast!
Cutting-edge science and life behind the scenes of ESO,
the European Southern Observatory.
Exploring the ultimate frontier with our host Dr J, a.k.a. Dr Joe Liske.
Hello and welcome to this very special “multicast”.
We’ll be exploring a unique collaboration
between some of the world’s most powerful telescopes both
on the ground and in space.
Now, to do this, we’ve set up a similar collaboration between
the ESOcast, the Hubblecast,
the Spitzer Space Telescope’s “Hidden Universe” and
the Chandra X-Ray Observatory’s “Beautiful Universe”.
I’m Megan Watzke for the Beautiful Universe from the Chandra X-ray Center
And I’m Dr Robert Hurt for Hidden Universe from NASA Spitzer Science Center
It’s the combination of deep observations from many different telescopes
that makes this project so important.
The longer a telescope spends looking at a target,
the more sensitive the observations become, and the deeper we can look into space.
But to get the full picture of what’s happening in the Universe,
astronomers also need observations at a range of different wavelengths,
requiring different telescopes.
These are the key ideas behind the Great Observatories Origins Deep Survey,
or GOODS for short.
The GOODS project unites the world’s most advanced observatories,
these include ESO’s Very Large Telescope,
the NASA/ESA Hubble Space Telescope,
the Spitzer Space Telescope,
the Chandra X-ray Observatory and many more,
each making extremely deep observations
of the distant Universe, across the electromagnetic spectrum.
By combining their powers and observing the same piece of sky,
the GOODS observatories are giving us a unique view of the formation
and evolution of galaxies across cosmic time,
and mapping the history of the expansion of the Universe.
Now, this is not the first time that telescopes
have been used to give us extremely deep views of the cosmos.
For example, the Hubble Deep Field is a very deep image
of a small region of sky in the northern constellation of Ursa Major.
This revealed thousands of distant galaxies
despite the fact that the whole field is actually only a tiny speck of sky,
about the size of a grain of sand held at arm’s length.
Now, with GOODS, many different observatories
have brought their powers to bear on two larger targets,
one centred on the original Hubble Deep Field in the northern sky,
and one centred on a different deep target,
the Chandra Deep Field South, in the southern sky.
The main GOODS fields are each 30 times larger than the Hubble Deep Field,
and additional observations cover an area the size of the full Moon.
These areas of the sky were already some of the most extensively explored,
and so the combination of existing archival data with the many new, dedicated observations
gives us an unprecedented view of the history of galaxies.
At ESO’s Very Large Telescope on Cerro Paranal, the 8.2-metre-diameter giants
were used for a total of almost 100 nights of dedicated observations.
The telescopes made images of the region both in near-infrared light,
and on the boundary between visible light and ultraviolet light.
At these short wavelengths, only telescopes on exceptional sites
such as the VLT’s Cerro Paranal
have a chance to observe through the Earth’s atmosphere.
The NASA/ESA Hubble Space Telescope observed
the GOODS regions at optical and near-infrared wavelengths,
in order to detect distant star-forming galaxies among other things.
Now, Hubble spent a total of five days observing the fields,
spread over five repeat visits.
Each of these was separated from the previous one by about 45 days.
Now, by spreading out the observations like this,
Hubble was able to watch out for new supernovae appearing over the months,
providing key information for studying the expansion and the acceleration of the Universe
due to the mysterious dark energy.
But it wasn’t just Hubble making space-based observations for GOODS…
NASA’s Spitzer Space Telescope imaged the GOODS regions
in near- and mid-infrared light for five days,
at wavelengths up to 30 times longer than the Hubble observations.
These longer wavelengths are important for revealing distant galaxies
whose light may be obscured by cosmic dust,
or stretched by the expansion of the Universe, making them invisible to Hubble.
For these distant galaxies, the Spitzer images also tell astronomers about their age
and their total mass of stars — complementary information to the data from Hubble.
Now, let’s move from the infrared to much shorter wavelengths…
Also in orbit, the Chandra X-Ray Observatory had already observed the GOODS field
in many long observations taken over the course of a year.
The Chandra images are the deepest X-ray images ever taken,
and detected more than 200 X-ray sources
believed to be supermassive black holes in the centres of young galaxies.
The X-rays are produced by extremely hot interstellar gases
falling into the black holes.
These multiwavelength observations identified tens of thousands of galaxies.
To get a full understanding of the history and development of galaxies
over the vast stretch of the Universe’s history,
we need to be able to pin down their distances more precisely,
to fix them in cosmic time.
As these galaxies are so far away,
the light waves we see from them today
started their journey up to about 13 billion years ago,
and because the Universe has been expanding since the Big ***,
back then the Universe was less than one seventh of its current size.
During the billions of years of the light’s journey,
its wavelength has been stretched as the fabric of space has expanded.
This effect is known as “redshift”
because, for example, light that was originally blue or ultraviolet in colour
is shifted to longer and redder wavelengths.
Back on the ground, astronomers used spectrographs
on ESO’s Very Large Telescope
to capture the spectra of galaxies,
spreading out their light like the colours of the rainbow.
Now, the spectra allow astronomers to measure
the redshifts of the galaxies, and hence, their distances.
An extensive campaign produced redshifts
for almost 3000 galaxies in the GOODS fields.
Now, with this knowledge, we can place the galaxies
at their distances along a vast cone of space,
stretching out from our own vantage point
like a searchlight beam into the cosmos.
We can take an amazing journey
through kind of a tunnel towards the edge of the Universe.
In some places, the galaxies cluster together,
forming structures which are up to tens of millions of light years in scale.
Thanks to GOODS and other surveys of the same region,
these areas of the sky are uniquely well studied
with high resolution, deep observations
across a wide wavelength range,
plus there is more to come.
For example, the Atacama Pathfinder Experiment telescope, or APEX,
has spent a total of 300 hours — nearly two full weeks —
imaging the region at submillimetre wavelengths,
from its high site on the 5000-metre-altitude plateau of Chajnantor
in the Chilean Andes.
Observations at these wavelengths
are ideal for finding the redshifted light
of distant dusty galaxies in the very early Universe.
Because of the longer wavelength of its submillimetre light,
the APEX image is not as sharp as the visible light and infrared images.
However, thanks to the deep Spitzer images,
as well as images made at radio wavelengths,
we can match up and identify the objects found by APEX
with galaxies seen at other wavelengths.
The submillimetre light glow
reveals that hundreds of stars are being formed per year in these galaxies.
In the next couple of years,
ALMA, the Atacama Large Millimeter/submillimeter Array,
currently under construction on the same plateau as APEX,
will begin its first science observations.
Also observing at submillimetre wavelengths,
it will have much greater sensitivity than APEX,
and resolution even better than Hubble.
ALMA will revolutionise our understanding of the early Universe
by revealing many more distant, dust-obscured galaxies
that cannot be seen at all by visible light and infrared telescopes.
These projects are an excellent example of how great observatories
are joining together, across the electromagnetic spectrum,
to give us a more complete view of galaxies over the history of the Universe.
Already, astronomers have written over 400 papers based on these data,
with even more in the pipeline!
And on top of that, the observations of the GOODS fields will continue in the future.
These patches of the sky will be prime targets for the next generation of telescopes
both on the ground and in space,
and astronomers around the world will use these data
to learn new things about the Universe for many years to come.
Saying goodbye to our friends at the other observatories,
this is Dr J signing off for the ESOcast and the Hubblecast…
This is Dr Robert Hurt signing off for the Hidden Universe and the Spitzer Science Center,
reminding you there’s a hidden Universe just waiting to be discovered.
And this is Megan Watzke
signing off for the Chandra X-ray Observatory and the Beautiful Universe.
Join me again next time for another cosmic adventure,
which I’m sure will surprise us beyond our wildest imagination.
This was a multicast from:
ESOcast, Hubblecast, Hidden Universe, Beautiful Universe
ESOcast is produced by ESO, the European Southern Observatory.
ESO, the European Southern Observatory, is the pre-eminent intergovernmental science and technology organisation in astronomy,
designing, constructing and operating the world’s most advanced ground-based telescope
The Atacama Large Millimeter/submillimeter Array (ALMA), an international astronomy facility,
is a partnership of Europe, North America and East Asia in cooperation with the Republic of Chile.
APEX is a collaboration between the Max-Planck-Institut für Radioastronomie,
the European Southern Observatory, and the Onsala Space Observatory.
Transcription by ESO ; translation by —
Now that you've caught up with ESO,
head 'out of this world' with Hubble.
The Hubblecast highlights the latest discoveries of the world´s most recognized and prized space observatory,
the NASA/ESA Hubble Space Telescope