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UKIRT Infrared Deep Sky Survey

From Wikipedia, the free encyclopedia

UKIRT Infrared Deep Sky Survey
The UKIRT telescope

The UKIRT Infrared Deep Sky Survey or UKIDSS is an astronomical survey conducted using the WFCAM wide field camera on the United Kingdom Infrared Telescope on Mauna Kea in Hawaii. Survey observations were commenced in 2005.

UKIDSS consists of five surveys covering a range of areas and depths, using various combinations of five near-infrared filters.

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  • The Most Distant Quasar Ever Discovered
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Transcription

Using ESO's flagship Very Large Telescope, along with other telescopes around the world, a team of European astronomers has discovered the most distant quasar ever recorded! By studying this blazing beacon in detail the scientists have found that we are seeing this quasar at a time when the universe was just 770 million years old. This means that the light from the quasar took 12.9 billion years to reach us. Never before has a brighter object been observed this far back into the early Universe. Quasars are very brilliant distant galaxies powered by supermassive black holes at their centres. These amazing objects have the mass of millions of suns crammed into spaces as small as our Solar System. The quasar phenomenon transforms ordinary galaxies into what astronomers have fittingly dubbed 'angry monsters' - the most luminous of all objects in the universe. And ESO's Very Large Telescope, better known as the VLT, helped to discover the farthest of these impressive objects ever observed. Back in the early Universe galaxies contained much more gas and dust than we see in them today. Gradually material was used up in the formation of stars and planets, and less was available to feed the supermassive black hole, the process that creates the impressive jets of a quasar. Objects far back in the early Universe, like the newly recorded quasar, cannot be observed in visible light. By the time it reaches our detectors on Earth the expansion of the Universe has stretched the light so much that it falls mainly into the infrared part of the spectrum. In addition, quasars in the early universe are extremely rare and so in order to find this object in the first place a team of astronomers had to spend five painstakingly years closely examining huge lists of possible objects from an infrared survey made by the UKIRT telescope - before they finally struck gold. With such an exciting discovery the team could take no chances; they had to validate their findings. Using the FORS2 instrument on the VLT, along with instruments on the Gemini North telescope, a redshift of 7.1 was confirmed. This corresponds to such an extraordinary distance that it took the light from the quasar 12.9 billion years to reach us. Despite the vast distance, the quasar's extreme brightness made it possible to identify other characteristics using the same two telescopes. It was determined that the black hole powering the quasar has a mass of about two billion times that of our own Sun. This is an extraordinary mass for an object so early in the Universe. Since current estimations say there should only be around 100 bright quasars at this distance across the entire sky, finding this object was a huge challenge. It was a great bonus that it has proved to be even more distant than the astronomers expected. This quasar is a vital probe into the early Universe and will help us understand how black holes grew just a few hundred million years after the Big Bang.

Description

UKIDSS as a large-scale near infrared survey follows 2MASS and anticipates the VISTA telescope in the Southern hemisphere. It aims to cover 7500 square degrees of the Northern sky. Four particular areas of investigation for UKIDSS are: "the coolest and nearest brown dwarfs, high-redshift dusty starburst galaxies, elliptical galaxies and galaxy clusters at redshifts 1 < z < 2, and the highest-redshift quasars, at z = 7".[1]

The UKIDSS data become available online to the ESO community immediately upon entering the WFCAM Science Archive (WSA), and are then released to the world 18 months later.

Surveys

Of the five surveys in UKIDSS, two are directed towards Galactic targets and three are optimized for extra-Galactic observations. The surveys are described here in decreasing order of area. The letters refer to spectral regions; e.g. JHK is a combination of near-infrared filters, more or less synonymous with "the near-infrared".

Large Area Survey (LAS)

The LAS (extra-Galactic) covers an area of 4000 square degrees in YJHK to a depth of K = 18.4. This area has previously been covered at optical wavelengths in the Sloan Digital Sky Survey. While the high Galactic latitudes covered by the LAS make it suitable for observations of sources outside the Milky Way, the survey also targets Galactic sources, incorporating a second pass in J to measure proper motions of nearby stars.

Galactic Plane Survey (GPS)

The GPS (Galactic) covers an area of 1800 square degrees in JHK to a depth of K=19.0, with 300 square degrees also covered through a narrow-band H2 filter. The motivation for the GPS is to obtain a clearer view of the Galactic Plane than is possible at optical wavelengths, due to absorption by material in the disk of the galaxy.

Galactic Clusters Survey (GCS)

The GCS (Galactic) covers an area of 1400 square degrees in JHK to a depth of K=18.7. The area is distributed over ten open star clusters with the aim of measuring the mass function in a variety of Galactic environments.

Deep Extragalactic Survey (DXS)

The DXS (extra-Galactic) covers an area of 35 square degrees in JK to a depth of K=21.0 with 5 square degrees also imaged in H. The survey fields are at high Galactic latitudes with low extinction, and are chosen to overlap with deep observations made at other wavelengths.

Ultra Deep Survey (UDS)

The UDS (extra-Galactic) covers an area of 0.77 square degrees within the XMM-LSS field (which is contained within the DXS) in JHK to a depth of K=23.0. This is the deepest near-infrared survey yet conducted over such an area of sky, with the aim of studying the formation and evolution of galaxies in the early Universe.

Notes

  1. ^ UKIDSS Home Page. Retrieved April 30, 2007.

External links

This page was last edited on 14 July 2021, at 17:50
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