
AGN surveys to study galaxy evolution along cosmic times
... • Mid-IR excess: Spinoglio & Malkan (1989) first found that there is a spectral interval (7-12 μm) at which the absorption of the original continuum is balanced by the thermal emission, because dust absorbs the continuum at short wavelengths and re-emit it in the FIR. This balance allows the non-ther ...
... • Mid-IR excess: Spinoglio & Malkan (1989) first found that there is a spectral interval (7-12 μm) at which the absorption of the original continuum is balanced by the thermal emission, because dust absorbs the continuum at short wavelengths and re-emit it in the FIR. This balance allows the non-ther ...
Cosmology and Particle Physics
... Figure 3: (a) Andromeda is the closest large galaxy, at 2 million light years distance, and is very similar to our Milky Way. The blue regions harbor young and emerging stars, while dark streaks are vast clouds of gas and dust. A smaller satellite galaxy is clearly visible. (b) The box indicates wha ...
... Figure 3: (a) Andromeda is the closest large galaxy, at 2 million light years distance, and is very similar to our Milky Way. The blue regions harbor young and emerging stars, while dark streaks are vast clouds of gas and dust. A smaller satellite galaxy is clearly visible. (b) The box indicates wha ...
Document
... De Zeeuw will start by explaining the technological advances that have shaped the course of astronomy from the days of Galileo, when the telescope replaced the naked eye as man’s instrument for studying the skies. Subsequent refinement of this instrument has involved such major innovations as the sw ...
... De Zeeuw will start by explaining the technological advances that have shaped the course of astronomy from the days of Galileo, when the telescope replaced the naked eye as man’s instrument for studying the skies. Subsequent refinement of this instrument has involved such major innovations as the sw ...
galaxies and stars - Valhalla High School
... • The Milky Way is the galaxy in which our solar system is located. • A galaxy is a giant structure that contains billions of stars. • The farther away a galaxy is from us, the faster it is moving. • It takes 2 million years for light from the Andromeda galaxy to reach earth. • Astronomers have cla ...
... • The Milky Way is the galaxy in which our solar system is located. • A galaxy is a giant structure that contains billions of stars. • The farther away a galaxy is from us, the faster it is moving. • It takes 2 million years for light from the Andromeda galaxy to reach earth. • Astronomers have cla ...
from z=0 to z=1
... ratio (attenuation) for UV galaxies. For IR (24m) selected galaxies at z~0.6, no evidence is found for evolution of either the stellar mass or the IR/UV ratio for given LIR. 8. Both IR and UV evolve significantly from z=0 to z=1, and the ratio IR/UV increases by ~ 4. This is consistent with the ...
... ratio (attenuation) for UV galaxies. For IR (24m) selected galaxies at z~0.6, no evidence is found for evolution of either the stellar mass or the IR/UV ratio for given LIR. 8. Both IR and UV evolve significantly from z=0 to z=1, and the ratio IR/UV increases by ~ 4. This is consistent with the ...
Universe, Dark Energy and Dark Matter
... Milne and W. H. McCrea. This wonderful possibility is caused by the following thing. A spherically-symmetrical material shell cannot produce any gravitational field in the whole inner cavity and the space-time must be flat. The Universe does not contain such huge spherical regions but we can imagine ...
... Milne and W. H. McCrea. This wonderful possibility is caused by the following thing. A spherically-symmetrical material shell cannot produce any gravitational field in the whole inner cavity and the space-time must be flat. The Universe does not contain such huge spherical regions but we can imagine ...
ASTR 300 Stars and Stellar Systems Fall 2011
... astronomers sometimes put their telescopes in deep valleys? (Chapt. 6, Review Question 4) Optical astronomers hope to get above as much of the atmosphere as possible. For radio astronomers, interference from man-made radio signals is a major problem. Putting a radio telescope in a deep valley may sh ...
... astronomers sometimes put their telescopes in deep valleys? (Chapt. 6, Review Question 4) Optical astronomers hope to get above as much of the atmosphere as possible. For radio astronomers, interference from man-made radio signals is a major problem. Putting a radio telescope in a deep valley may sh ...
File 11 - School of Astronomy, IPM
... • Early type galaxies (built of old stars and little gas or dust) appear smooth and plain • Spiral galaxies show arms bursting with areas of active star formation, and disks rich in gas and dust. • Also while most stars in a spiral rotate in the same direction within its central plane, yielding a hi ...
... • Early type galaxies (built of old stars and little gas or dust) appear smooth and plain • Spiral galaxies show arms bursting with areas of active star formation, and disks rich in gas and dust. • Also while most stars in a spiral rotate in the same direction within its central plane, yielding a hi ...
Here
... The dust in nearby interstellar cloud blocks out the optical light from background stars. ...
... The dust in nearby interstellar cloud blocks out the optical light from background stars. ...
the universe
... Scientists have gathered a lot of evidence and information about the universe. They have used their observations to develop a theory called the Big Bang. The theory states that about 13,700 million years ago all the matter in the universe was concentrated into a single incredibly tiny point. This be ...
... Scientists have gathered a lot of evidence and information about the universe. They have used their observations to develop a theory called the Big Bang. The theory states that about 13,700 million years ago all the matter in the universe was concentrated into a single incredibly tiny point. This be ...
Sample pages 1 PDF
... elements) was considered a wide-field instrument. In 2003 a camera called Megacam began operating; it has .18 000/2 pixels and images a square degree of the sky at a sampling rate of 0:00 2 in a single exposure. Such a camera produces roughly 100 GB of data every night, the reduction of which requir ...
... elements) was considered a wide-field instrument. In 2003 a camera called Megacam began operating; it has .18 000/2 pixels and images a square degree of the sky at a sampling rate of 0:00 2 in a single exposure. Such a camera produces roughly 100 GB of data every night, the reduction of which requir ...
the universe
... Scientists have gathered a lot of evidence and information about the universe. They have used their observations to develop a theory called the Big Bang. The theory states that about 13,700 million years ago all the matter in the universe was concentrated into a single incredibly tiny point. This be ...
... Scientists have gathered a lot of evidence and information about the universe. They have used their observations to develop a theory called the Big Bang. The theory states that about 13,700 million years ago all the matter in the universe was concentrated into a single incredibly tiny point. This be ...
One World, One Sky Planetarium Show Field Trip - Science in Pre-K
... look directly at the sun! It is so bright it can burn your eyes. Can you ever see the moon in the day time? Look for the moon. If you find it, notice what shape it is. Can you draw the shape of the moon? Discuss: If the sun is a star, why does it appear different from other stars in the sky? (We ...
... look directly at the sun! It is so bright it can burn your eyes. Can you ever see the moon in the day time? Look for the moon. If you find it, notice what shape it is. Can you draw the shape of the moon? Discuss: If the sun is a star, why does it appear different from other stars in the sky? (We ...
PRIMARY SOURCE from Starry Messenger
... the form and construction of which I shall first briefly explain, as well as the occasion of its having been devised. Afterwards I shall relate the story of the observations I have made. . . . We have now briefly recounted the observations made thus far with regard to the moon. . . . There remains the ...
... the form and construction of which I shall first briefly explain, as well as the occasion of its having been devised. Afterwards I shall relate the story of the observations I have made. . . . We have now briefly recounted the observations made thus far with regard to the moon. . . . There remains the ...
Physics Observing The Universe
... • Because it orbits the Earth in the same direction as the Earth rotates. So by the time the Earth rotates enough for a static object to have gotten all the way to the opposite horizon, the Moon hasn't quite gotten there yet because it was moving with the Earth's rotation a little. ...
... • Because it orbits the Earth in the same direction as the Earth rotates. So by the time the Earth rotates enough for a static object to have gotten all the way to the opposite horizon, the Moon hasn't quite gotten there yet because it was moving with the Earth's rotation a little. ...
script
... into the universe of galaxies beyond. As we journey outward to distant galaxies we discover a surprising fact: the distant galaxies look much different than the galaxies closer to our Milky Way. Why is this? As it turns out, the light from these distant galaxies takes a much longer time to reach us ...
... into the universe of galaxies beyond. As we journey outward to distant galaxies we discover a surprising fact: the distant galaxies look much different than the galaxies closer to our Milky Way. Why is this? As it turns out, the light from these distant galaxies takes a much longer time to reach us ...
The Universe - Smithsonian Education
... second to reach us. This slight time lag was observed in the transmission of images from the astronauts to ground control. Light-year measurement allows us to pack vast numbers into manageable units. It also helps us to think in terms of age. As the Moon landings showed, nothing in space comes to us ...
... second to reach us. This slight time lag was observed in the transmission of images from the astronauts to ground control. Light-year measurement allows us to pack vast numbers into manageable units. It also helps us to think in terms of age. As the Moon landings showed, nothing in space comes to us ...
Revision Guide (Unit 2 Module 5) - Pearson Schools and FE Colleges
... Hubble’s law clearly shows that the universe is not static; it is expanding. This can help to explain Olbers’ ideas. Hubble showed that distant galaxies are moving very fast. Very distant galaxies will have large redshifts, so that their light will be shifted out of the visible region of the spectru ...
... Hubble’s law clearly shows that the universe is not static; it is expanding. This can help to explain Olbers’ ideas. Hubble showed that distant galaxies are moving very fast. Very distant galaxies will have large redshifts, so that their light will be shifted out of the visible region of the spectru ...
February 2015 - Hermanus Astronomy
... Way form, but most galaxies in the universe are faint, distant dwarf galaxies," said Principal Investigator David Nidever of the University of Michigan. "The Magellanic Clouds are two of the few nearby dwarf galaxies, and SMASH is able to map out and study the structures in them like no other survey ...
... Way form, but most galaxies in the universe are faint, distant dwarf galaxies," said Principal Investigator David Nidever of the University of Michigan. "The Magellanic Clouds are two of the few nearby dwarf galaxies, and SMASH is able to map out and study the structures in them like no other survey ...
Name - MIT
... a main-belt asteroid has an apparent magnitude of +6, a Kuiper Belt Object has an apparent magnitude of +17, a Trojan asteroid has an apparent magnitude of +14, and Pluto has an apparent magnitude of +15. Which object is faintest in the sky? A) B) C) D) E) ...
... a main-belt asteroid has an apparent magnitude of +6, a Kuiper Belt Object has an apparent magnitude of +17, a Trojan asteroid has an apparent magnitude of +14, and Pluto has an apparent magnitude of +15. Which object is faintest in the sky? A) B) C) D) E) ...
New Directions
... the Universe was not known He therefore looked at only stars in the MW and saw that there was no obvious expansion or contraction *With a nod to Dr. Barbara Ryden ...
... the Universe was not known He therefore looked at only stars in the MW and saw that there was no obvious expansion or contraction *With a nod to Dr. Barbara Ryden ...
Hubble Deep Field

The Hubble Deep Field (HDF) is an image of a small region in the constellation Ursa Major, constructed from a series of observations by the Hubble Space Telescope. It covers an area 2.5 arcminutes across, about one 24-millionth of the whole sky, which is equivalent in angular size to a 65 mm tennis ball at a distance of 100 metres. The image was assembled from 342 separate exposures taken with the Space Telescope's Wide Field and Planetary Camera 2 over ten consecutive days between December 18 and December 28, 1995.The field is so small that only a few foreground stars in the Milky Way lie within it; thus, almost all of the 3,000 objects in the image are galaxies, some of which are among the youngest and most distant known. By revealing such large numbers of very young galaxies, the HDF has become a landmark image in the study of the early universe, with the associated scientific paper having received over 900 citations by the end of 2014.Three years after the HDF observations were taken, a region in the south celestial hemisphere was imaged in a similar way and named the Hubble Deep Field South. The similarities between the two regions strengthened the belief that the universe is uniform over large scales and that the Earth occupies a typical region in the Universe (the cosmological principle). A wider but shallower survey was also made as part of the Great Observatories Origins Deep Survey. In 2004 a deeper image, known as the Hubble Ultra-Deep Field (HUDF), was constructed from a few months of light exposure. The HUDF image was at the time the most sensitive astronomical image ever made at visible wavelengths, and it remained so until the Hubble Extreme Deep Field (XDF) was released in 2012.