Drop Out Movie
A short movie showing how the observed spectrum of star-forming galaxies changes as we observe it at higher and higher redshift. Redshift is denoted here in this movie as "z". Note how the break in the spectrum shifts to redder and redder wavelengths as a result of this redshifting effect. To be able to identify galaxies at the highest redshifts (and thus near the beginning of the universe), it is necessary to be able to measure the fluxes of sources at near-infrared wavelengths (>1 micron). High-redshift galaxies are frequently found by noting a significant break in the spectrum as seen through a set of discrete filters.
The XDF Assembly Movie
A time lapsed sequence showing the assembly of 10 years of Hubble ACS/WFC and WFC3/IR observations and over 3000 images used in creating the eXtreme Deep Field
High resolution version with no music and full size (1520x1520). Download (163MB)
The XDF Paper
The XDF team has published a paper titled "The HST eXtreme Deep Field XDF: Combining all ACS and WFC3/IR Data on the HUDF Region into the Deepest Field Ever" discussing the methods used to produce the XDF dataset.
The paper can be downloaded at arXiv.org
The XDF Data Release v1.0
The XDF team has release the XDF v1.0 data products on the MAST HST data archive. These data include all optical and infrared data taken by Hubble covering the original Hubble Ultra-Deep Field (HUDF) program.
The data can be downloaded from the MAST High Level Science Products page XDF Data Release 1.0
Download the XDF Poster
The XDF Poster - Black Background
The XDF Poster - White Background
Hubble Goes to the eXtreme to Assemble Farthest Ever View of the Universe
Like photographers assembling a portfolio of best shots, astronomers have assembled a new, improved portrait of mankind's deepest-ever view of the universe.
Called the eXtreme Deep Field, or XDF, the photo was assembled by combining 10 years of NASA Hubble Space Telescope photographs taken of a patch of sky at the center of the original Hubble Ultra Deep Field. The XDF is a small fraction of the angular diameter of the full Moon.
The Hubble Ultra Deep Field is an image of a small area of space in the constellation Fornax, created using Hubble Space Telescope data from 2003 and 2004. By collecting faint light over many hours of observation, it revealed thousands of galaxies, both nearby and very distant, making it the deepest image of the universe ever taken at that time.
The new full-color XDF image reaches much fainter galaxies, and includes very deep exposures in red light from Hubble's new infrared camera, enabling new studies of the earliest galaxies in the universe. The XDF contains about 5,500 galaxies even within its smaller field of view. The faintest galaxies are one ten-billionth the brightness of what the human eye can see.
Magnificent spiral galaxies similar in shape to our Milky Way and the neighboring Andromeda galaxy appear in this image, as do the large, fuzzy red galaxies where the formation of new stars has ceased. These red galaxies are the remnants of dramatic collisions between galaxies and are in their declining years. Peppered across the field are tiny, faint, more distant galaxies that were like the seedlings from which today's striking galaxies grew. The history of galaxies — from soon after the first galaxies were born to the great galaxies of today, like our Milky Way — is laid out in this one remarkable image.
Hubble pointed at a tiny patch of southern sky in repeat visits (made over the past decade) for a total of 50 days, with a total exposure time of 2 million seconds. More than 2,000 images of the same field were taken with Hubble's two premier cameras — the Advanced Camera for Surveys and the Wide Field Camera 3, which extends Hubble's vision into near-infrared light — and combined to make the XDF.
"The XDF is the deepest image of the sky ever obtained and reveals the faintest and most distant galaxies ever seen. XDF allows us to explore further back in time than ever before," said Garth Illingworth of the University of California at Santa Cruz, principal investigator of the Hubble Ultra Deep Field 2009 (HUDF09) program.
The universe is 13.7 billion years old, and the XDF reveals galaxies that span back 13.2 billion years in time. Most of the galaxies in the XDF are seen when they were young, small, and growing, often violently as they collided and merged together. The early universe was a time of dramatic birth for galaxies containing brilliant blue stars extraordinarily brighter than our Sun. The light from those past events is just arriving at Earth now, and so the XDF is a "time tunnel into the distant past." The youngest galaxy found in the XDF existed just 450 million years after the universe's birth in the big bang.
Before Hubble was launched in 1990, astronomers could barely see normal galaxies to 7 billion light-years away, about halfway across the universe. Observations with telescopes on the ground were not able to establish how galaxies formed and evolved in the early universe.
Hubble gave astronomers their first view of the actual forms and shapes of galaxies when they were young. This provided compelling, direct visual evidence that the universe is truly changing as it ages. Like watching individual frames of a motion picture, the Hubble deep surveys reveal the emergence of structure in the infant universe and the subsequent dynamic stages of galaxy evolution.
The infrared vision of NASA's planned James Webb Space Telescope (Webb telescope) will be aimed at the XDF. The Webb telescope will find even fainter galaxies that existed when the universe was just a few hundred million years old. Because of the expansion of the universe, light from the distant past is stretched into longer, infrared wavelengths. The Webb telescope's infrared vision is ideally suited to push the XDF even deeper, into a time when the first stars and galaxies formed and filled the early "dark ages" of the universe with light.
||Hubble eXtreme Deep Field (XDF)
||R.A. 3h 32m 38s.5, Dec. -27° 47' 00"
||ACS/WFC and WFC3/IR
||July 2002 to March 2012
|Total Exposure Time
||22.5 days (2 million seconds)
|Number of Exposures
||2062 (1501 ACS/WFC and 561 WFC3/IR)
XDF resulted from the realization in late 2011 that all the data taken over the last ten years with the Advanced Camera and the Wide Field Camera 3 on the Hubble UltraDeep Field had not been combined into a single extremely deep image.
In discussions in late 2011 with an influential congressman, while doing the JWST Congressional hearing, Garth Illingworth realized that the HUDF images and posters found in many congressional offices, and used as educational materials across the country, were those from 2004. Our HUDF "deepest image" was out of date, even though it still looked good. A large number of new images had been taken since 2004. Hubble (and JWST) really needed a new "deepest" image for digital displays and a new poster to adorn walls all around the country.
The Hubble UltraDeep Field (HUDF) was observed in 2003 with the then-new Hubble Advanced Camera (ACS) that had been placed into Hubble in 2002 by the Shuttle astronauts during the servicing mission SM3B. The ACS HUDF was released as a public image in 2004. The new infrared Wide Field Camera 3 (WFC3) was added to Hubble in 2009 by the Shuttle astronauts in the final Hubble servicing mission (SM4). The HUDF was observed as part of the HUDF09 program in 2009 as one of the first set of images taken by the new infrared camera of WFC3 (WFC3/IR). These first observations were released as the HUDF09 image in early 2010. The HUDF09 observations were finally finished in winter 2011. The most distant, earliest galaxy seen, UDFj-39546284, was found in 2010 in the HUDF09 image (seen 13.2 billion years ago or just 450 million years after the Big Bang).
The HUDF and HUDF09 have been released individually, but a combined image of ALL the images ever taken on the ultradeep field had not been done. Over the last decade twelve different programs had taken data in this region, dominated by the original HUDF, the HUDF09 and the more recent CANDELS data.
After discussions with members of the HUDF09 team we decided to collect and process all the data for an "everything on the HUDF" image. An initial discussion with Space Telescope Science Institute (STScI) confirmed for us that this was an idea worth pursuing. We started the assembly of all the images in early winter 2012.
The images came from different cameras with different orientations and different amounts of overlap. Since very large numbers of individual images were involved, the processing and cross-checking involved a lot of effort and time. Refining the software and testing procedures, and assembling, checking and testing the co-added images, was a lengthy and time consuming task involving Dan Magee, Pascal Oesch and Rychard Bouwens that continued through the spring of 2012.
The image was finally ready by early summer 2012. Detailed communications with STScI regarding an image release ensued. Plans were developed for a number of products, in addition to the color image of the XDF. The products included a fly-through of the galaxies, explanatory images and text, and educational posters. The image was named the eXtreme Deep Field (XDF) from a name developed and used earlier by the HUDF09 team in a proposal. Given that the combined image involved 10 years of data from numerous programs, and that it represented a stunning achievement of Hubble — the "deepest image of the sky ever taken" — the updated name seemed most appropriate.
Given the length of time needed to develop all the release products, the schedule of summer vacations by key people and the focused media attention on the Mars Curiosity Rover landing in August 2012, the release was tentatively scheduled for September 2012. The final date chosen to fit with development of the data products and other NASA press releases was September 25, 2012.
The XDF includes ALL data taken by Hubble on the small patch of sky first imaged as the Hubble Ultra-Deep Field (HUDF). These images were taken over a decade from mid-2002 through to mid-2012. The XDF is an exposure of 2 million seconds total from Hubble's two premier cameras, the Advanced Camera (ACS) and the Wide Field Camera 3 (WFC3). ACS flew on the Shuttle to Hubble in 2002 on servicing mission SM3B, while the Wide Field Camera 3 (WFC3) flew to Hubble in 2009 on the final Hubble Shuttle mission (SM4).
The original HUDF data demonstrated the power of Hubble’s new ACS camera in 2004. The original HUDF contributes, by time, a little more that half to the XDF, but only contains data in the optical ("visible") region of the spectrum. In 2009 and 2010, the HUDF09 project took images towards the red end of the spectrum in the near-infrared with the new WFC3/IR camera. These new data doubled the waveband coverage and enabled exploration of a new realm of the most distant galaxies for the first time. The HUDF09 field with WFC3/IR and ACS contributed around a quarter of the data by time to XDF. The HUDF and HUDF09 fields are shown in the first and second panels of the “Hubble Dataset Used to Build Up the XDF” figure.
The XDF/HUDF09 team then took ALL the other data on this region taken by numerous programs (listed on the next page) and combined it through a very laborious and careful series of steps into one incredibly deep image, the eXtreme Deep Field (XDF). These data fall at many locations and orientations and much careful checking was needed to make sure all the Hubble ACS and WFC3 images could be properly aligned and added together. The contributions from these other programs comprised nearly a quarter of the time, of which the largest was the CANDELS images from ACS and WFC3. The numerous images are shown in third panel of the “Hubble Dataset Used to Build Up the XDF” figure.
The XDF was then assembled using data from every image over the last decade from ACS and the WFC3 (the orange region in the fourth panel of the “Hubble Dataset Used to Build Up the XDF” figure). XDF reaches back 13.2 billion years, to just 450 million years after the Big Bang. The history of galaxies — from soon after the first galaxies were born to the appearance of the great galaxies of today, like our Milky Way — is laid out in this one remarkable image.
The XDF combined image goes incredibly faint. The combined image XDF reaches to approximately one ten-billionth of what the eye can see. In astronomer-speak, XDF reaches to ∼30.7 AB magnitude for a 5 sigma detection of a point source (like a star) corrected to total magnitude (uncorrected the 5 sigma limit is 31.2 AB mag). This is equivalent to a 1 sigma noise fluctuation of 32.9 AB mag, as measured directly in a 0.33" aperture.
The XDF is such an important field that it will be imaged in the future and more data will be added. Two Hubble programs have recently obtained the first deep data in the ultra-violet (PID 12534) from WFC3/UVIS, and deeper imaging in the near-infrared (PID 12498) from WFC3/IR. The ultra-violet imaging complements the redder XDF and is being used by astronomers to study galaxies at later times when they are in transition to galaxies like today’s galaxies (including our Milky Way and Andromeda). After the latter, near-infrared WFC3/IR data set (PID 12498) becomes publicly available by the end of 2012, the XDF can be pushed deeper by an additional 20%.
Programs Used to Make the XDF
||The Deceleration Test from Treasury Type Ia Supernovae at Redshifts 1.2 to 1.6
||The Great Observatories Origins Deep Survey: Imaging with ACS
||Cosmic Shear - with ACS Pure Parallel Observations
||ACS Default (Archival) Pure Parallel Program
||The Grism-ACS Program for Extragalactic Science (GRAPES)
||The Ultra Deep Field with ACS (HUDF)
||The Ultra Deep Field with ACS (HUDF)
||Probing Acceleration Now with Supernovae (PANS)
||Tracing the Emergence of the Hubble Sequence Among the Most Luminous and Massive Galaxies
||Probing Acceleration Now with Supernovae (PANS)
||Probing Evolution And Reionization Spectroscopically (PEARS)
||Panchromatic WFC3 survey of galaxies at intermediate z: Early Release Science program for Wide Field Camera 3 (ERS)
||Galaxies at z~7-10 in the Reionization Epoch: Luminosity Functions to <0.2L* from Deep IR Imaging of the HUDF and HUDF05 Fields (HUDF09)
||Cosmic Assembly Near-IR Deep Extragalactic Legacy Survey — GOODS-South Field, Non-SNe-Searched Visits (CANDELS)
||Cosmic Assembly Near-IR Deep Extragalactic Legacy Survey — GOODS-South Field, Early Visits of SNe Search (CANDELS)
||Galaxy Assembly and the Evolution of Structure over the First Third of Cosmic Time - III (CANDELS)
||Supernova Follow-up for MCT (CANDELS)
||3D-HST: A Spectroscopic Galaxy Evolution Treasury (3DHST)
Hubble Datasets Used to Build-up the XDF
This sequence shows how the XDF was built up from the numerous exposures that have been made over the HUDF field.
The original HUDF ACS/WFC (optical) data taken from 2003-2004
The HUDF09 WFC3/IR (infrared) data taken from 2009-2011
The additional ACS/WFC and WFC3/IR data taken over the last decade
The orange region show the XDF which combines all ACS/WFC and WFC3/IR data taken from 2002-2012
The first image of the sequence shows the original HUDF data from the ACS. By fraction of the total time the original HUDF contributes over 50% to the XDF, but only contains data in the optical ("visible") region of the spectrum. In 2009, the HUDF09 project took images towards the red end of the spectrum in the near-infrared with the new WFC3/IR camera. These new data doubled the waveband coverage and enabled exploration of a new realm of the most distant galaxies for the first time. The second image of the sequence shows the HUDF09 field with WFC3/IR and ACS that contributed around a quarter of the data by time to XDF.
Finally, the XDF/HUDF09 team took ALL the other data on this region taken by numerous programs and combined it through a very laborious and careful series of steps into one incredibly deep image, the eXtreme Deep Field (XDF). As the third image shows the data falls at many locations and orientations and much careful checking was needed to make sure all the Hubble ACS and WFC3 images could be properly aligned and added together. The contributions came from ten other programs that comprised about 20% of the time, of which the largest was the CANDELS images from ACS and WFC3.
Finally, in the fourth image of the sequence the XDF is shown as the orange region where the contribution of every image over the last decade from ACS and WFC3 has been included.
The XDF combined image goes incredibly faint. It reaches to approximately one ten-billionth of what the eye can see (in astronomer-speak it reaches to ~30.7 AB magnitude for a 5 sigma detection total magnitude).
What XDF is Compared to HUDF and HUDF09?
XDF takes ALL the data that has been taken on the HUDF field between 2002 and 2012 - this means HUDF, HUDF09, CANDELS, and many other programs. No other release has done this. This makes the deepest image from HST ever, with the widest spectral coverage image from HST on the HUDF. An example galaxy spectrum is shown. This example is a galaxy that is invisible to the Advanced Camera for Surveys. It is so distant that its light has been shifted to the red so far by the expansion of the universe that it is only seen in the infrared with the Wide Field Camera 3. This example galaxy is seen about 12.8 billion years ago, just 800 million years after the Big Bang.
What is Hubble's Distance Limit?
As galaxies get more distant their light is "redshifted" by the expansion of the universe. Ultimately the galaxy light moves so far to the red that it becomes invisible to Hubble's cameras. This effect is shown here. The most distant galaxy found in the HUDF09 image, UDFj-39546284, is seen 13.21 billion years ago and is at "redshift" 10.4 (represented by "z" as in z∼10.4). The light from UDFj-39546284 appears just in the reddest filter H160 of the WFC3/IR camera on Hubble, as shown in the figure below. The ability of Hubble to see even more distant galaxies gets quickly worse. By "redshift" 11.4, just 50 million years earlier, or 13.26 billion years ago, the light from a galaxy is only partially visible to Hubble in the reddest filter (a hypothetical example galaxy at 11.4 is shown in the figure). Even though a z∼11.4 galaxy is just 50 million years closer to the Big Bang, it is a lot fainter and a lot harder for Hubble to see. Since galaxies are getting rapidly fainter at earlier times, "redshift" z∼11 or so is around the practical limit for Hubble.
Galaxies closer to the Big Bang than about redshift 11, or 400 million years from the Big Bang, cannot be seen by Hubble and will require James Webb Space Telescope to see the "first galaxies".