The European Space Agency's
Faint Object Camera on board NASA's Hubble Space Telescope has provided a fascinating close - up view of Supernova 1987A in the Large Magellanic Cloud.
The Einstein Cross — The European Space Agency's
Faint Object Camera on board NASA's Hubble Space Telescope has provided astronomers with the most detailed image ever taken of the gravitational lens G2237 + 0305 — sometimes referred to as the Einstein Cross.
During a servicing mission in February 2002, astronauts added the Advanced Camera for Surveys (ACS), doubling the Hubble's field of view and replacing
the Faint Object Camera, which served as the HST's telephoto lens.
Note:
The Faint Object Camera was replaced by the Advanced Camera for Surveys in 2002.
The team used
the Faint Object Camera and Spectrograph (FOCAS) mounted on the Subaru Telescope to thoroughly study the visible wavelength spectrum (Note 1) of the afterglow of a gamma - ray burst (GRB, Note 2), which is a violent explosion of a massive star.
Observations of SN 1987A with the COSTAR - corrected
Faint Object Camera.
First results from
the Faint Object Camera: SN 1987a.
Not exact matches
Scientists on the Dark Energy Survey, using one of the world's most powerful digital
cameras, have discovered eight more
faint celestial
objects hovering near our Milky Way galaxy.
To help pull in
faint objects, Chandra contains a series of nested mirrors that each funnel X-rays to a sharp focus at its narrow end, where a
camera sits.
So Anita Cochran of the University of Texas and her colleagues turned to the Hubble telescope's Wide Field / Planetary
Camera, which can spot much
fainter objects.
For example, an instrument on one satellite could block the glare of the sun or a distant star, making it possible for a
camera on the other to image
faint objects such as the sun's ghostly corona or exoplanets orbiting a star.
SOFIA's
Faint Object Infrared
Camera will examine the Milky Way's tumultuous center, star - forming regions, dust clouds, and nearby galaxies.
There are also two
cameras - one which can achieve image resolutions 10 times greater than that of even the largest Earth - based telescope, and a second which can detect an
object 50 times
fainter than anything visible from Earth.
It is one of the
faintest objects in the sky, discovered using a 25» Schmidt
camera in 1952 by G.A Shajn and V.E. Hase at the Crimean Astrophyical Observatory at Simeis (in the former U.S.S.R).
The Dragonfly Telephoto Array used 14 - centimeter state of the art telephoto lens
cameras to produce digital images of the very
faint, diffuse
objects.
Camera purchased with the support of a 2009 Shoemaker NEO Grant is now on a new telescope providing follow - up measurements for even
fainter near - Earth
objects.
Their Slow Moving
Objects survey, which lasted almost a decade, used progressively larger CCD cameras to detect faint objects moving slowly relative to background
Objects survey, which lasted almost a decade, used progressively larger CCD
cameras to detect
faint objects moving slowly relative to background
objects moving slowly relative to background stars.