BeppoSAX is an Italian - Dutch satellite, launched late last year,
that detects gamma ray bursts and provides precise sky positions to allow ground - based telescopes to observe them.
Not exact matches
NASA's Swift satellite has found the most distant
gamma -
ray burst ever
detected.
The distance to the merger makes the source both the closest gravitational wave event
detected so far and also one of the closest
gamma -
ray burst sources ever seen.
Discovery of the
gamma -
ray «bang» from FRB 131104, the first non-radio counterpart to any FRB, was made possible by NASA's Earth - orbiting Swift satellite, which was observing the exact part of the sky where FRB 131104 occurred as the
burst was
detected by the Parkes Observatory radio telescope in Parkes, Australia.
«Swift's rapid response time enabled us to use it to rapidly search for and
detect the electromagnetic counterpart of this
gamma -
ray burst after its detection by LIGO,» said Jamie Kennea, associate research professor of astronomy and astrophysics, the leader of the Swift Science Operations Team at Swift's Mission Operations Center, located at Penn State's University Park campus.
Detectors on NASA's Swift
Gamma - Ray Burst satellite and by the Russian Konus gamma - ray instrument on board NASA's Wind satellite detected the initial burst on Marc
Gamma -
Ray Burst satellite and by the Russian Konus gamma - ray instrument on board NASA's Wind satellite detected the initial burst on Marc
Burst satellite and by the Russian Konus
gamma - ray instrument on board NASA's Wind satellite detected the initial burst on Marc
gamma -
ray instrument on board NASA's Wind satellite
detected the initial
burst on Marc
burst on March 19.
Astronomers have
detected one more clue to the origins of
gamma -
ray bursts, those highly energetic explosions that occur in distant galaxies.
But the
gamma -
ray signals produced by the August collision were 10,000 times less bright than those seen in other
detected short
gamma -
ray bursts.
Optical telescopes swung into operation and
detected a fading spot of ordinary light at the position of the
gamma -
ray burst.
The Compton
Gamma Ray Observatory (CGRO), designed to detect gamma rays from distant astrophysical objects such as neutron stars and supernova remnants, had also begun recording bright, millisecond - long bursts of gamma rays coming not from outer space but from Earth b
Gamma Ray Observatory (CGRO), designed to
detect gamma rays from distant astrophysical objects such as neutron stars and supernova remnants, had also begun recording bright, millisecond - long bursts of gamma rays coming not from outer space but from Earth b
gamma rays from distant astrophysical objects such as neutron stars and supernova remnants, had also begun recording bright, millisecond - long
bursts of
gamma rays coming not from outer space but from Earth b
gamma rays coming not from outer space but from Earth below.
Gamma - Ray Burst A far - distant object brightens suddenly and is detected first in the gamma - ray wavele
Gamma -
Ray Burst A far - distant object brightens suddenly and is
detected first in the
gamma - ray wavele
gamma -
ray wavelength.
Astronomers are furiously searching for the source of a brief
burst of
gamma rays detected by NASA's Swift space telescope on Monday.
Swift can swivel towards
gamma -
ray bursts (GRBs) in less than a minute and has
detected two short
bursts since its launch in November 2004.
This all - sky coverage lets Fermi
detect more
gamma -
ray bursts, and over a broader energy range, than any other mission.
But as she read excited messages from colleagues that a
gamma ray burst had also been
detected, «I realized this was a breakthrough event,» says Troja, an associate research scientist at the University of Maryland in College Park who works at NASA's Goddard Space Flight Center in Greenbelt in Maryland.
Swift lived up to its name on 17 January, when it
detected a bright and relatively long - lasting
gamma ray burst.
But astronomers may have pulled off an equally challenging feat:
detecting the glimmer of a supernova explosion in the fading afterglow of a titanic
gamma ray burst (GRB)-- one of the biggest type of explosions in all the cosmos.
On July 6, Lazzati's team of theorists had published a paper predicting that, contrary to earlier estimates by the astrophysics community, short
gamma -
ray bursts associated with the gravitational emission of binary neutron star coalescence could be
detected — whether or not the
gamma -
ray burst was pointing at Earth.
Seconds later, a satellite
detected a
gamma -
ray burst, and more than 70 observatories subsequently studied the aftermath in every wavelength.
If the jet is pointing towards the Earth, a
burst of
gamma -
rays is
detected.
On 6 April and 2 May 2005, Swift
detected x-
ray flares minutes after the onset of two
gamma -
ray bursts in the constellations Eridanus the River and Leo the Lion.
When
gamma -
ray bursts were first
detected by military satellites in the 1960s, nobody knew where they came from.
In the wee hours of the morning of 19 March, astronomers
detected from more than halfway across the universe a
burst of
gamma rays brighter than a hundred - billion suns — and aimed squarely at Earth.
Two seconds after the gravitational waves, orbiting telescopes
detected a powerful, short
gamma ray burst.
Reichart and Don Lamb of the University of Chicago predicted in a 2000 paper in the Astrophysical Journal that such faraway
gamma -
ray bursts could be
detected.
In March, the satellite
detected the brightest
gamma -
ray burst, which was visible to the human eye despite occurring billions of light - years away.
NASA's Swift satellite has found the most distant
gamma -
ray burst ever
detected.
LIGO was the first to
detect the signals as gravitational waves, before 70 observatories around the world joined in to watch the fireworks in the form of visible light, radio waves, X-rays and a
gamma ray burst.
Although they did not find any dark GRBs that originated in the early universe (such as the subsequently discovered GRB 090423), the astronomers were able to estimate that ancient GRBs probably account for only around 0.2 to 0.7 per cent of all
gamma -
ray bursts detected since their initial discovery.
On March 31, 2011, scientists submitted a revised paper describing how they used a supercomputer to model the formation of short
gamma -
ray bursts (GRBs) that have been
detected as lasting less than two seconds.
From the rest wavelength of the Lyman - alpha break (121.6 nm), the spectroscopic redshift of GRB 000131 was then determined to be 4.500 + / - 0.015, corresponding to a travel time of more than 90 percent of the age of the Universe and making GRB 000131 the most ancient and remote
gamma -
ray burst detected at the time — for which its age and distance could be calculated (Andersen et al, 2000).
On January 31, 2000, a brief
burst of
gamma rays was
detected by an network of satellites (Ulysses, NEAR and Konus) via the InterPlanetary Network (Hurley et al, 2000).
GRB 090423 is not only the most distant
gamma -
ray burst ever
detected, but it is also the most distant object ever
detected in the universe overall (as of April 28, 2009).
On April 23, 2009, NASA's Swift satellite
detected a 10 - second - long
burst of
gamma - rays from GRB 090423 in the western part (9:55:35 +18:9:37, J2000) of Constellation Leo — northwest of Eta and Alpha Leonis (Regulus), southwest of Gamma (Algieba) and Zeta (Adhafera) Leonis, south of Rasalas (Mu Leonis), and southeast of Algenubi (Epsilon Leonis), and northeast of Subra (Omicron Leo
gamma -
rays from GRB 090423 in the western part (9:55:35 +18:9:37, J2000) of Constellation Leo — northwest of Eta and Alpha Leonis (Regulus), southwest of
Gamma (Algieba) and Zeta (Adhafera) Leonis, south of Rasalas (Mu Leonis), and southeast of Algenubi (Epsilon Leonis), and northeast of Subra (Omicron Leo
Gamma (Algieba) and Zeta (Adhafera) Leonis, south of Rasalas (Mu Leonis), and southeast of Algenubi (Epsilon Leonis), and northeast of Subra (Omicron Leonis).
Roughly half of the GRBs
detected by NASA's Swift satellite since its 2004 launch are «dark»
gamma -
ray bursts that are not seen in visible light (and so are virtually invisible to optical telescopes).
Although GRB 000131, like other
gamma -
ray bursts, appears to have taken place in a remote «early galaxy» (or «sub-galactic clumps» of stars) that is smaller than today's luminous galaxies, astronomers found it difficult to
detect that extremely dim, sub-galactic clump of stars even with the Hubble Space Telescope, as the observed fading of the afterglow indicated that the maximum brightness of the
gamma -
ray emission was explosion was at least 10,000 times brighter than its host galaxy.
Around 4 p.m. PDT, the Swope Telescope — the oldest and smallest of a collection of four optical telescopes at Carnegie Observatories» Las Campanas Observatory in Chile —
detected a bright optical counterpart to the
gamma -
ray burst and gravitational - wave signals, in a galaxy called NGC 4993.
A couple of seconds later, a brief
burst of
gamma rays were detected by an instrument aboard the Fermi Gamma - ray Space Teles
gamma rays were
detected by an instrument aboard the Fermi
Gamma - ray Space Teles
Gamma -
ray Space Telescope.