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1060:, in April 2012. Orbital predictions several days earlier indicated that the two satellites were expected to occupy the same point in space within 30 milliseconds of each other. On 3 April, telescope operators decided to stow the satellite's high-gain parabolic antenna, rotate the solar panels out of the way and to fire Fermi's rocket thrusters for one second to move it out of the way. Even though the thrusters had been idle since the telescope had been placed in orbit nearly five years earlier, they worked correctly and potential disaster was thus avoided.
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628:, associate administrator for Science at NASA Headquarters, launched a public competition 7 February 2008, closing 31 March 2008, to rename GLAST in a way that would "capture the excitement of GLAST's mission and call attention to gamma-ray and high-energy astronomy ... something memorable to commemorate this spectacular new astronomy mission ... a name that is catchy, easy to say and will help make the satellite and its mission a topic of dinner table and classroom discussion".
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1097:. This improved understanding led to two major improvements: gamma-rays that had been missed by previous analysis were detected and the direction they arrived from was determined with greater accuracy. The impact of the latter is to sharpen Fermi LAT's vision as illustrated in the figure on the right. Pass 8 also delivers better energy measurements and a significantly increased effective area. The entire mission dataset was reprocessed.
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fluctuation or an Earth albedo transient on a 1-second timescale. A rebuttal of this follow-up analysis, however, pointed out that the independent group misrepresented the analysis of the original Fermi GBM Team paper and therefore misconstrued the results of the original analysis. The rebuttal reaffirmed that the false coincidence probability is calculated empirically and is not refuted by the independent analysis.
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failed to move as instructed in one direction. On 27 March, the satellite was placed at a fixed angle relative to its orbit to maximize solar power. The next day the GBM instrument was turned back on. On 2 April, operators turned LAT on and it resumed operations on 8 April. Alternative observation strategies are being developed due to power and thermal requirements.
1400:
telescope's all-sky SPI-ACS instrument indicated that any energy emission in gamma-rays and hard X-rays from the event was less than one millionth of the energy emitted as gravitational waves, concluding that "this limit excludes the possibility that the event is associated with substantial gamma-ray
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On 16 March 2018 one of Fermi's solar arrays quit rotating, prompting a transition to "safe hold" mode and instrument power off. This was the first mechanical failure in nearly 10 years. Fermi's solar arrays rotate to maximize the exposure of the arrays to the Sun. The motor that drives that rotation
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are responsible for gamma-ray background radiation. The potential for a tremendous discovery awaits if ordinary sources are determined to be irresponsible, in which case the cause may be anything from self-annihilating dark matter to entirely new chain reactions among interstellar particles that have
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For almost all event classes, Version P8R2 had a residual background that was not fully isotropic. This anisotropy was traced to cosmic-ray electrons leaking through the ribbons of the Anti-Coincidence
Detector and a set of cuts allowed rejection of these events while minimally impacting acceptance.
612:
Both science instruments underwent environmental testing, including vibration, vacuum, and high and low temperatures to ensure that they can withstand the stresses of launch and continue to operate in space. They were integrated with the spacecraft at the
General Dynamics ASCENT facility in Gilbert,
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has theorised that if a massive star is rapidly rotating, the centrifugal force produced during its collapse will lead to the formation of a rotating bar that breaks into two dense clumps of matter with a dumbbell configuration that becomes a black hole binary, and at the end of the star's collapse
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These improvements have the greatest impact on both the low and high ends of the range of energy Fermi LAT can detect - in effect expanding the energy range within which LAT can make useful observations. The improvement in the performance of Fermi LAT due to Pass 8 is so dramatic that this software
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are not responsible for most gamma-ray background radiation. Though active galactic nuclei do produce some of the gamma-ray radiation detected here on Earth, less than 30% originates from these sources. The search now is to locate the sources for the remaining 70% or so of all gamma-rays detected.
1080:
Comparison of two Fermi LAT views of the same region in the constellation Carina. The first comes from an older analysis, termed Pass 7, while the second shows the improvements with Pass 8. Both images contain the same number of gamma rays. In the foreground plot, the tall spikes represent greater
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Computers operating both the LAT and GBM and most of the LAT's components were turned on 24 June 2008. The LAT high voltage was turned on 25 June, and it began detecting high-energy particles from space, but minor adjustments were still needed to calibrate the instrument. The GBM high voltage was
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Study better than ever before how concentrations of visible and ultraviolet light change over time. The mission should easily detect regions of spacetime where gamma-rays interacted with visible or UV light to make matter. This can be seen as an example of E=mc working in reverse, where energy is
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space telescope also did not detect a gamma-ray counterpart of the event. A follow-up analysis of the Fermi report by an independent group, released in June 2016, purported to identify statistical flaws in the initial analysis, concluding that the observation was consistent with a statistical
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that carries the instruments. It travels in a low, circular orbit with a period of about 95 minutes. Its normal mode of operation maintains its orientation so that the instruments will look away from the Earth, with a "rocking" motion to equalize the coverage of the sky. The view of the
1442:
On 17 August 2017, Fermi Gamma-Ray Burst
Monitor software detected, classified, and localized a gamma-ray burst which was later designated as GRB 170817A. Six minutes later, a single detector at Hanford LIGO registered a gravitational-wave candidate which was consistent with a binary
1101:
update is sometimes called the cheapest satellite upgrade in history. Among numerous advances, it allowed for a better search for
Galactic spectral lines from dark matter interactions, analysis of extended supernova remnants, and to search for extended sources in the Galactic plane.
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In June 2015, the Fermi LAT Collaboration released "Pass 8 LAT data". Iterations of the analysis framework used by LAT are called "passes" and at launch Fermi LAT data was analyzed using Pass 6. Significant improvements to Pass 6 were included in Pass 7 which debuted in August 2011.
987:. On 4 June 2008, after several previous delays, launch status was retargeted for 11 June at the earliest, the last delays resulting from the need to replace the Flight Termination System batteries. The launch window extended from 15:45 to 17:40 UTC daily, until 7 August 2008.
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Ackermann, M.; Ajello, M.; Albert, A.; Anderson, B.; Atwood, W. B.; Baldini, L.; Barbiellini, G.; Bastieri, D.; Bellazzini, R. (1 June 2015). "Updated search for spectral lines from
Galactic dark matter interactions with pass 8 data from the Fermi Large Area Telescope".
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was awarded to Bill Atwood, Peter
Michelson and the Fermi LAT team "for enabling, through the development of the Large Area Telescope, new insights into neutron stars, supernova remnants, cosmic rays, binary systems, active galactic nuclei and gamma-ray bursts."
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had concluded that the primary goals were "all achievable with the all-sky scanning mode of observing". Fermi switched to "sky survey mode" on 26 June 2008 so as to begin sweeping its field of view over the entire sky every three hours (every two orbits).
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At the flare's peak, the LAT detected gamma rays with two billion times the energy of visible light, or about four billion electron volts (GeV), easily setting a record for the highest-energy light ever detected during or immediately after a solar
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which produce detectable tiny pulses of electric charge. Researchers can combine information from several layers of this tracker to determine the path of the particles. After passing through the tracker, the particles enter the
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Black hole mergers of the type thought to have produced the gravitational wave event are not expected to produce gamma-ray bursts, as stellar-mass black hole binaries are not expected to have large amounts of orbiting matter.
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Gamma-ray skyβs activity during a year of observations from
February 2022 to February 2023 captured by the Large Area Telescope (LAT) aboard Fermi Gamma-ray Space Telescope. The pulsing circles represent a subset of the light
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event and with a positional uncertainty region overlapping that of the LIGO observation. The Fermi team calculated the odds of such an event being the result of a coincidence or noise at 0.22%. However, observations from the
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predict that it may not. Search for gamma rays emanating from former black holes that once exploded, providing yet another potential step toward the unification of quantum mechanics and general relativity. Determine whether
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distant above and below the galactic center. The galaxy's diffuse gamma-ray fog hampered prior observations, but the discovery team led by D. Finkbeiner, building on research by G. Dobler, worked around this problem.
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concentrations of gamma rays and correspond to brightness. Pass 8 provides more accurate directions for incoming gamma rays, so more of them fall closer to their sources, creating taller spikes and a sharper image.
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Atwood, W.; Albert, A.; Baldini, L.; Tinivella, M.; Bregeon, J.; Pesce-Rollins, M.; SgrΓ², C.; Bruel, P.; Charles, E. (1 March 2013). "Pass 8: Toward the Full
Realization of the Fermi-LAT Scientific Potential".
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with one of the highest energy outputs yet recorded. This included detection of a gamma-ray over 94 billion electron volts (GeV). This broke Fermi's previous record detection, by over three times the amount.
1546:"Gamma-ray bursts are so bright we can see them from billions of light-years away, which means they occurred billions of years ago, and we see them as they looked then", stated Charles Meegan of NASA's
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radiation, directed towards the observer." If the signal observed by the Fermi GBM was associated with GW150914, SPI-ACS would have detected it with a significance of 15 sigma above the background. The
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was recorded by the Fermi telescope. This burst is notable as having "the largest apparent energy release yet measured". The explosion had the power of about 9,000 ordinary supernovae, and the
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are on the sides of the spacecraft to view all of the sky which is not blocked by the Earth. The design is optimized for good resolution in time and photon energy, and is sensitive from
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crystals to measure the total energy of the particles. The LAT's field of view is large, about 20% of the sky. The resolution of its images is modest by astronomical standards, a few
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Study energy spectra and variability of wavelengths of light coming from blazars so as to determine the composition of the black hole jets aimed directly at Earth -- whether they are
1651:. SLAC also hosts the LAT Instrument Science Operations Center, which supports the operation of the LAT during the Fermi mission for the LAT scientific collaboration and for NASA.
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crystals with sensitivity from 150 keV to 30 MeV), and can detect gamma-ray bursts in that energy range across the whole of the sky not occluded by the Earth.
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it triggers a gamma-ray burst. Loeb suggests that the 0.4 second delay is the time it took the gamma-ray burst to cross the star, relative to the gravitational waves.
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ranked this mission as a top priority. Many new possibilities and discoveries are anticipated to emerge from this single mission and greatly expand our view of the
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1417:. It was detected on 1 January 2015 at 15:23:35 UT by the Gamma-ray Burst Monitor on board the Fermi Gamma-ray Space Telescope, along with detections by the
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Data from the instruments are available to the public through the Fermi
Science Support Center web site. Software for analyzing the data is also available.
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instruments will sweep out across most of the sky about 16 times per day. The spacecraft can also maintain an orientation that points to a chosen target.
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1725:) that "confirmed that short gamma-ray bursts are produced by binary neutron star mergers and enabled a global multi-wavelength follow-up campaign."
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On 30 April 2013, NASA revealed that the telescope had narrowly avoided a collision a year earlier with a defunct Cold War-era Soviet spy satellite,
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Study gamma-ray bursts with an energy range several times more intense than ever before so that scientists may be able to understand them better.
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naturally split into smaller photons, as predicted by quantum mechanics and already achieved under controlled, man-made experimental conditions.
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Bruel, P.; Burnett, T. H.; Digel, S. W.; Johannesson, G.; Omodei, N.; Wood, M. (26 October 2018). "Fermi-LAT improved Pass~8 event selection".
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Scientists estimate a very high possibility for new scientific discoveries, even revolutionary discoveries, emerging from this single mission.
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Ackermann, M.; Ajello, M.; Baldini, L.; Ballet, J.; Barbiellini, G.; Bastieri, D.; Bellazzini, R.; Bissaldi, E.; Bloom, E. D. (1 July 2017).
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Every detection by the Fermi LAT since its launch, was reexamined with the latest tools to learn how the LAT detector responded to both each
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530:, and government agencies in France, Germany, Italy, Japan, and Sweden, becoming the most sensitive gamma-ray telescope on orbit, succeeding
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for their work in developing the theoretical framework underpinning the many exciting pulsar results from Fermi Gamma-ray Space
Telescope.
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as well as other underground detectors. The potential for a tremendous discovery in this area is possible over the next several years.
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Education and public outreach are important components of the Fermi project. The main Fermi education and public outreach website at
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479:. Its main instrument is the Large Area Telescope (LAT), with which astronomers mostly intend to perform an all-sky survey studying
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are underlined. Launch failures are marked with the β sign. Payloads deployed from other spacecraft are (enclosed in parentheses).
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1179:. Overall, GRB 080916C had "the greatest total energy, the fastest motions, and the highest initial-energy emissions" ever seen.
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also turned on 25 June, but the GBM still required one more week of testing/calibrations before searching for gamma-ray bursts.
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1721:, the first unambiguous and completely independent discovery of an electromagnetic counterpart to a gravitational wave signal (
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1710:, Douglas Finkeiner and Meng Su "for their discovery, in gamma rays, of the large unanticipated Galactic structure called the
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Gamma-ray radiation (greater than 1 Gev) detected over the entire sky; brighter areas are more radiation (five year study by
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satellite in the 1990s. Several countries produced the components of the LAT, who then sent the components for assembly at
499:. Another instrument aboard Fermi, the Gamma-ray Burst Monitor (GBM; formerly GLAST Burst Monitor), is being used to study
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2970:"Search for Extended Sources in the Galactic Plane Using Six Years of Fermi-Large Area Telescope Pass 8 Data above 10 GeV"
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Fermi gained its new name in 2008: On 26 August 2008, GLAST was renamed the "Fermi Gamma-ray Space Telescope" in honor of
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Launches are separated by dots ( β’ ), payloads by commas ( , ), multiple names for the same satellite by slashes ( / ).
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and discovered that such flashes can produce 100 trillion positrons, far more than scientists had previously expected.
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3680:"On the Interpretation of the Fermi-GBM Transient Observed in Coincidence with LIGO Gravitational-wave Event GW150914"
1700:
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1227:
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570:(20 MeV to 300 GeV), with a field of view of about 20% of the sky; it may be thought of as a sequel to the
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Fermi reported that its GBM instrument detected a weak gamma-ray burst above 50 keV, starting 0.4 seconds after the
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Probe dark matter (e.g. by looking for an excess of gamma rays from the center of the Milky Way) and early Universe.
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Fermi includes two scientific instruments, the Large Area Telescope (LAT) and the Gamma-ray Burst Monitor (GBM).
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bands only, a first for its kind. This new pulsar sweeps the Earth every 316.86 milliseconds and is about 4,600
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Nigro, Cosimo (1 December 2015). "Fermi-LAT analysis of extended supernova remnants with the new pass 8 data".
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so as to possibly solve how they are produced. Study how pulsars generate winds of interstellar particles.
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1447:, occurring 2 seconds before the GRB 170817A event. This observation was "the first joint detection of
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Savchenko, V.; Ferrigno, C.; Mereghetti, S.; Natalucci, L.; Bazzano, A.; et al. (April 2016).
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Connaughton, V.; Burns, E.; Goldstein, A.; Briggs, M. S.; Zhang, B.-B.; et al. (July 2016).
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2005:
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Tavani, M.; Pittori, C.; Verrecchia, F.; Bulgarelli, A.; Giuliani, A.; et al. (July 2016).
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The 2018 prize was awarded to Colleen Wilson-Hodge and the Fermi GBM team for the detection of
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NASA designed the mission with a five-year lifetime, with a goal of ten years of operations.
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1997:
1889:"An Astro-Particle Physics Partnership Exploring the High Energy Universe - List of funders"
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In early 2012, Fermi/GLAST observed the highest energy light ever seen in a solar eruption.
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The Gamma-ray Burst Monitor (GBM) (formerly GLAST Burst Monitor) detects sudden flares of
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Gamma- and X-ray bubbles at the Milky Way galaxy center: Top: illustration; Bottom: video.
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upper limits on gamma-ray emission associated with the gravitational wave event GW150914"
2837:"FSSC: Fermi Data Β» Data Analysis Β» LAT Data Analysis Β» Using Pass 8 Data"
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offers gateways to resources for students, educators, scientists, and the public. NASA's
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After presenting an overview of the Fermi instrumentation and goals, Jennifer Carson of
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4092:"2018 Bruno Rossi Prize: Top High-Energy Prize Awarded to Gamma-ray Burst Monitor Team"
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Connaughton, V.; Burns, E.; Goldstein, A.; Briggs, M. S.; et al. (January 2018).
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of the Milky Way was found in data from the Fermi telescope. This is now known as the
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2009:
1861:"NASA's GLAST Burst Monitor Team Hard at Work Fine-Tuning Instrument and Operations"
1195:. The source of this surplus is not known. Suggestions include self-annihilation of
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at an altitude of 550 km (340 mi), and at an inclination of 28.5 degrees.
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GLAST launch as pictured by a space-based infrared sensor, looking down at the Earth
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Provide new data to help improve upon existing theoretical models of our own galaxy.
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jet of material ejected in the blast must have moved at a minimum of 99.9999% the
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GLAST received some minor modifications to its computer software on 23 June 2008.
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4021:"Astronomers Honored for Excellence in Research, Education, Writing & More"
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3768:"The Afterglow and Early-Type Host Galaxy of the Short GRB 150101B at z=0.1343"
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Carson, Jennifer (March 2007). "GLAST: physics goals and instrument status".
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4069:"2014 Rossi prize awarded to Douglas Finkbeiner, Tracy Slatyer, and Meng Su"
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1413:, 1.7 billion light years away from Earth, may be analogous to the historic
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1218:. This determination fulfills one of the stated missions for this project.
722:) from their presumed gamma burst signatures (Hawking Radiation component).
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The key scientific objectives of the Fermi mission have been described as:
659:
2104:"Spacecraft Overview Presentation for the GLAST LAT Collaboration Meeting"
6918:
6791:
6723:
6689:
6527:
6497:
6478:
6436:
6410:
5850:
5786:
5627:
5339:
5100:
5000:
4992:
4896:
4833:
4644:
4507:
4333:
4325:
3654:"NASA's Big Mistake: LIGO's Merging Black Holes Were Invisible After All"
2768:
1966:
Atwood, W. B.; et al. (June 2009). "The Large Area Telescope on the
1722:
1582:
1578:
1554:
1448:
1430:
1414:
1397:
996:
959:
757:
753:
731:
531:
519:
220:
17:
995:
Launch occurred successfully on 11 June 2008 at 16:05 UTC aboard a
6984:
6929:
6883:
6879:
6830:
6801:
6588:
6582:
6533:
6492:
6426:
6416:
6397:
6356:
6324:
6073:
6004:
5842:
5491:
5451:
5347:
5258:
5250:
5242:
5234:
5226:
5218:
4936:
4920:
4888:
3133:"Fermi Observations of High-Energy Gamma-Ray Emission from GRB 080916C"
1749:
1574:
904:
896:
3223:"Physicists revive hunt for dark matter in the heart of the Milky Way"
3197:"Most Extreme Gamma-ray Blast Ever, Seen By Fermi Gamma-ray Telescope"
3166:
2823:"NASA's Fermi Celebrates Five Years in Space, Enters Extended Mission"
1210:
In February 2010, it was announced that Fermi-LAT had determined that
6970:
6960:
6836:
6733:
6719:
6539:
6464:
6421:
6406:
6367:
6329:
6177:
5914:
5770:
5483:
5427:
5395:
5387:
5310:
5290:
4880:
4857:
4756:
4732:
4571:
4398:
4358:
4235:
4147:
3856:"Electromagnetic Counterparts to Black Hole Mergers Detected by LIGO"
3590:
Greiner, J.; Burgess, J. M.; Savchenko, V.; Yu, H.-F. (August 2016).
2732:
2261:
1589:. These charged particles pass through interleaved layers of silicon
1200:
1140:
932:
908:
834:
794:
764:
738:
563:
492:
3742:"Black Hole Mergers Might Actually Make Gamma-Ray Bursts, After All"
1667:(E/PO) group operates the Fermi education and outreach resources at
1187:
In 2009, a surplus of gamma rays from a spherical region around the
4165:
3959:
3874:
3784:
3696:
3608:
3549:
3490:
3425:
3314:. Harvard-Smithsonian Center for Astrophysics. Release No. 2010-22.
3312:"Astronomers Find Giant, Previously Unseen Structure in our Galaxy"
3041:
2986:
2898:
2023:
Harrington, J. D.; Harris, David; Cominsky, Lynn (26 August 2008).
1304:
were detected around our galaxy, the Milky Way. The bubbles, named
1139:
The first major discovery came when the space telescope detected a
6483:
6372:
6147:
6142:
5945:
5882:
5802:
5739:
5734:
5729:
5724:
5719:
5714:
5704:
5635:
5499:
5459:
5411:
5403:
5371:
5363:
4968:
4341:
4160:
3409:"Fermi GBM Observations of LIGO Gravitational-wave Event GW150914"
3348:"NASA's Fermi Catches Thunderstorms Hurling Antimatter into Space"
3330:"NASA's Fermi Detects the Highest-Energy Light From a Solar Flare"
2868:
2064:
2025:"NASA Renames Observatory for Fermi, Reveals Entire Gamma-Ray Sky"
1984:
1529:
1483:
1470:
1462:
1376:
1352:
1121:
1075:
1006:. Spacecraft separation took place about 75 minutes after launch.
965:
953:
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642:
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314:
304:
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1838:
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with energy from about 20 million to about 300 billion
6187:
6137:
6095:
6068:
5988:
5579:
4984:
4668:
3917:"Did a Gamma Ray Burst Accompany LIGO's Gravity Wave Detection?"
2312:
2200:"NASA Calls for Suggestions to Re-Name Future Telescope Mission"
1640:
1392:
1105:
This selection was used to create the P8R3 version of LAT data.
802:
535:
523:
175:
Stowed: 2.8 Γ 2.5 m (9.2 Γ 8.2 ft)
72:
6266:
4169:
4128:
3827:"LIGO's black holes may have lived and died inside a huge star"
4122:
4023:(Press release). American Astronomical Society. Archived from
3943:"Multi-messenger Observations of a Binary Neutron Star Merger"
3383:"NASA's Fermi Captures Dynamic Gamma-Ray Sky in New Animation"
2122:"NASA's General Dynamics-Built GLAST Satellite Launched Today"
1614:
1358:
865:
857:
596:
Advanced Information Systems (formerly Spectrum Astro and now
515:
3533:"AGILE Observations of the Gravitational Wave Event GW150914"
3081:"Fermi Telescope Makes First Big Discovery: Gamma Ray Pulsar"
903:
Test better than ever before certain established theories of
124:
4116:
886:, complementing similar experiments already planned for the
581:
The GBM consists of 14 scintillation detectors (twelve
2634:"GLAST Spacecraft Arrives in Florida to Prepare for Launch"
1068:
In August 2013 Fermi started its 5-year mission extension.
1660:
1613:
for the highest-energy photons and about 3 degrees at 100
3310:
Aguilar, David A.; Pulliam, Christine (9 November 2010).
1553:
The Gamma-ray Burst Monitor has detected gamma rays from
686:
To understand the mechanisms of particle acceleration in
4047:"NASA Goddard Astrophysicist Wins Prize for Pulsar Work"
2729:"The GLAST Mission: GLAST Overview, orbital information"
585:
crystals for the 8 keV to 1 MeV range and two
27:
Space telescope for gamma-ray astronomy launched in 2008
3267:. Fermi Gamma-ray Space Telescope. NASA. Archived from
2609:. Fermi Gamma-ray Space Telescope. NASA. Archived from
2582:. Fermi Gamma-ray Space Telescope. NASA. Archived from
2555:. Fermi Gamma-ray Space Telescope. NASA. Archived from
2528:. Fermi Gamma-ray Space Telescope. NASA. Archived from
2501:. Fermi Gamma-ray Space Telescope. NASA. Archived from
2474:. Fermi Gamma-ray Space Telescope. NASA. Archived from
2447:. Fermi Gamma-ray Space Telescope. NASA. Archived from
2420:. Fermi Gamma-ray Space Telescope. NASA. Archived from
2393:. Fermi Gamma-ray Space Telescope. NASA. Archived from
2366:. Fermi Gamma-ray Space Telescope. NASA. Archived from
801:
than ever before so as to broaden our understanding of
1941:"RE7/FERMI : The Fermi Gamma-ray Space Telescope"
2703:"Expendable Launch Vehicle Status Report: ELV-060608"
2343:
NASA β Scientists Predict Major Discoveries for GLAST
1569:
using technology similar to that used in terrestrial
1387:
GRB coincident with gravitational wave event GW150914
3292:"NASA's Fermi Probes "Dragons" of the Gamma-ray Sky"
2046:
Meegan, Charles; et al. (September 2009). "The
6953:
6902:
6845:
6775:
6703:
6668:
6603:
6548:
6445:
6381:
6343:
6317:
6201:
6056:
5957:
5926:
5179:
5036:
4873:
4776:
4591:
4482:
4316:
4271:
4210:
4203:
3368:"NASA's Fermi, Swift See 'Shockingly Bright' Burst"
2258:"The GLAST Mission: GLAST Overview, mission length"
1635:). The LAT is a bigger and better successor to the
1357:
GRB 130427A before and after in more than 100
1341:Fermi telescope has observed and detected numerous
882:Search for evidence that dark matter is made up of
424:
416:
409:
391:
383:
373:
363:
353:
343:
333:
323:
313:
303:
293:
283:
273:
263:
258:
240:
227:
216:
200:
195:
179:
171:
163:
153:
148:
136:
Elapsed: 16 years, 3 months, 16 days
130:
120:
107:
86:
68:
58:
46:
1565:The Large Area Telescope (LAT) detects individual
2124:(Press release). General Dynamics. Archived from
1253:Milky Way Gamma- and X-ray emitting Fermi bubbles
522:7920-H rocket. The mission is a joint venture of
2607:"Scientists Predict Major Discoveries for GLAST"
4161:Fermi's 14-Year Time-Lapse of the Gamma-Ray Sky
2303:
2301:
1438:GRB 170817A signals a multi-messenger transient
1323:
1147:remnant that appeared to emit radiation in the
979:On 4 March 2008, the spacecraft arrived at the
833:Study better than ever before whether ordinary
701:sky: unidentified sources and diffuse emission.
3250:"NASA's Fermi Closes on Source of Cosmic Rays"
2808:"The Day NASA's Fermi Dodged a 1.5-ton Bullet"
2648:"Tracking Station β Worldwide launch schedule"
1453:electromagnetic radiation from a single source
6278:
4181:
3766:Fong, Wen-fai; et al. (30 August 2018).
3592:"On the Fermi-GBM Event 0.4 s after GW150914"
2696:
2694:
663:Anticipated first year of operations timeline
620:GLAST renamed Fermi Gamma-ray Space Telescope
514:, was launched on 11 June 2008 at 16:05
510:Fermi, named for high-energy physics pioneer
8:
558:The LAT is an imaging gamma-ray detector (a
32:
3941:Abbott, B. P.; et al. (October 2017).
3341:
3339:
2632:Diller, George; Gutro, Rob (4 March 2008).
2240:"First Light for the Fermi Space Telescope"
1771:
1769:
1767:
1765:
1409:In October 2018, astronomers reported that
1317:Highest energy light ever seen from the Sun
852:converted into mass, in the early universe.
6285:
6271:
6263:
4207:
4188:
4174:
4166:
4002:"NASA's Newest Space Telescope Blasts Off"
3305:
3303:
3301:
1130:, constructed from photons detected by LAT
922:contends that it does, yet some models in
864:Study better than ever before how our own
437:
406:
98:
31:
3976:
3958:
3891:
3873:
3801:
3783:
3713:
3695:
3625:
3607:
3566:
3548:
3507:
3489:
3442:
3424:
3156:
3040:
3003:
2985:
2897:
2867:
2767:
2063:
1983:
3361:
3359:
3357:
3323:
3321:
3294:. Fermi Gamma-ray Space Telescope. NASA.
2109:. NASA. 23 October 2002. 1196-EB-R43864.
1337:Terrestrial gamma-ray flash observations
1302:two gamma-ray and X-ray emitting bubbles
1300:In November 2010, it was announced that
907:, such as whether the speed of light in
7056:Spacecraft launched by Delta II rockets
4150:by NASA's Marshall Space Flight Center
3849:
3847:
3381:Kazmierczak, Jeanette (14 March 2023).
3131:Abdo, A. A.; et al. (March 2009).
2224:. NASA. 8 February 2008. Archived from
1835:"FGST: Fermi Gamma-ray Space Telescope"
1761:
1163:In September 2008, the gamma-ray burst
1159:Greatest gamma-ray burst energy release
2242:. NASA. 26 August 2008. Archived from
1245:, and yet-to-be explained dark matter
704:Determine the high-energy behavior of
4125:by NASA's Goddard Space Flight Center
2756:Journal of Physics: Conference Series
2678:"GLAST Mission: Coverage Latest News"
1782:. NASA. February 2008. Archived from
1577:hit thin metal sheets, converting to
1557:generated in powerful thunderstorms.
7:
4154:Gamma-ray Burst Monitor publications
4071:. Harvard University. 8 January 2014
3265:"Cosmic Rays and Supernova Remnants"
2526:"Solar System: Sun, Moon, and Earth"
1649:SLAC National Accelerator Laboratory
1232:In March 2010 it was announced that
1126:Cycle of pulsed gamma rays from the
1045:SLAC National Accelerator Laboratory
884:weakly interacting massive particles
635:, a pioneer in high-energy physics.
461:Gamma-ray Large Area Space Telescope
50:Gamma-ray Large Area Space Telescope
3248:Reddy, Francis (16 February 2010).
3079:Atkinson, Nancy (17 October 2008).
2148:"Currently Available Data Products"
550:Fermi on Earth, solar arrays folded
397:23 February 2016, 04:46:22 UTC
4019:Fienberg, Rick (18 January 2011).
3346:Reddy, Francis (10 January 2011).
1687:In 2013, the prize was awarded to
1206:Cosmic rays and supernova remnants
714:Search for evaporating primordial
528:United States Department of Energy
25:
6219:List of proposed space telescopes
4905:Nancy Grace Roman Space Telescope
4141:Large Area Telescope publications
3947:The Astrophysical Journal Letters
3861:The Astrophysical Journal Letters
3684:The Astrophysical Journal Letters
3596:The Astrophysical Journal Letters
3477:The Astrophysical Journal Letters
3116:. 18 October 2008. Archived from
2821:Reddy, Francis (21 August 2013).
1693:Leland Stanford Junior University
1365:On 27 April 2013, Fermi detected
1260:Galactic gamma- and X-ray bubbles
1214:act as enormous accelerators for
289:6,912.9 km (4,295.5 mi)
6247:
6246:
3915:Gough, Evan (18 February 2016).
3825:Woo, Marcus (16 February 2016).
3263:Naeye, Robert (23 August 2007).
2605:Naeye, Robert (23 August 2007).
2578:Naeye, Robert (23 August 2007).
2524:Naeye, Robert (23 August 2007).
2497:Naeye, Robert (23 August 2007).
2470:Naeye, Robert (23 August 2007).
2443:Naeye, Robert (23 August 2007).
2416:Naeye, Robert (23 August 2007).
2362:Naeye, Robert (23 August 2007).
2315:. 28 August 2008. Archived from
1911:"Recognized Experiments at CERN"
1875:"Fermi Solar Flare Observations"
1277:
1266:
1183:Galactic Center gamma ray excess
1001:Cape Canaveral Air Force Station
805:. Study the pulsed emissions of
495:, other high-energy sources and
38:
5126:Nautilus Deep Space Observatory
4148:Gamma-ray Burst Monitor website
4094:. American Astronomical Society
4000:Coulter, Dauna (11 June 2008).
3328:Reddy, Francis (11 June 2012).
3290:Reddy, Francis (2 March 2010).
3108:"New kind of pulsar discovered"
1968:Fermi Gamma-Ray Space Telescope
1945:The CERN Experimental Programme
1602:, which consists of a stack of
983:payload processing facility in
911:remains constant regardless of
449:Fermi Gamma-ray Space Telescope
387:7.59 km/s (4.72 mi/s)
33:Fermi Gamma-ray Space Telescope
2701:Diller, George (6 June 2008).
2551:Woo, Marcus (23 August 2007).
2389:Berry, Dana (23 August 2007).
2309:"Q&A on the GLAST Mission"
1915:The CERN Scientific Committees
1777:"GLAST Science Writer's Guide"
827:Gamma-ray background radiation
793:Study younger, more energetic
728:National Academies of Sciences
534:. The project is a recognized
110:
1:
6229:List of heliophysics missions
3366:Reddy, Francis (3 May 2013).
3056:Chou, Felicia (30 May 2018).
2580:"Testing Fundamental Physics"
2364:"Blazars and Active Galaxies"
2120:Smith, Carol (10 June 2008).
1665:Education and Public Outreach
1655:Education and public outreach
1645:Compton Gamma Ray Observatory
1343:terrestrial gamma-ray flashes
1030:LAT/GBM computers operational
576:Compton Gamma Ray Observatory
319:543.6 km (337.8 mi)
309:525.9 km (326.8 mi)
167:4,303 kg (9,487 lb)
4135:Large Area Telescope website
3854:Loeb, Abraham (March 2016).
2222:"Name that Space Telescope!"
2178:Fermi Science Support Center
2152:Fermi Science Support Center
2002:10.1088/0004-637X/697/2/1071
1585:pairs, via a process termed
1548:Marshall Space Flight Center
1222:Background gamma ray sources
920:general theory of relativity
7051:Spacecraft launched in 2008
6209:Great Observatories program
3893:10.3847/2041-8205/819/2/L21
3803:10.3847/1538-4357/833/2/151
3627:10.3847/2041-8205/827/2/L38
3509:10.3847/2041-8205/820/2/L36
2082:10.1088/0004-637X/702/1/791
1701:Goddard Space Flight Center
1633:very-high-energy gamma rays
1423:Swift Observatory Satellite
1419:Burst Alert Telescope (BAT)
1308:, extend about 25 thousand
1228:Gamma-ray burst progenitors
7082:
5700:Orbiting Solar Observatory
3568:10.3847/2041-8205/825/1/L4
3444:10.3847/2041-8205/826/1/L6
2916:10.1103/PhysRevD.91.122002
2786:10.1088/1742-6596/60/1/020
2472:"The Gamma-ray Background"
2050:Gamma-ray Burst Monitor".
2027:. NASA. Release no. 08-214
1837:. Stanford. Archived from
1735:Galactic Center GeV excess
1495:very-high-energy gamma ray
1467:Instruments on-board Fermi
1225:
1193:Galactic Center GeV excess
1064:Extended mission 2013β2018
562:instrument) which detects
7006:
6252:Category:Space telescopes
6242:
3772:The Astrophysical Journal
3537:The Astrophysical Journal
3413:The Astrophysical Journal
2974:The Astrophysical Journal
2052:The Astrophysical Journal
1972:The Astrophysical Journal
1109:Solar array drive failure
1004:Space Launch Complex 17-B
604:, designed and built the
436:
405:
401:
254:
250:
191:
187:
144:
140:
81:U.S. Department of Energy
54:
37:
6214:List of space telescopes
3978:10.3847/2041-8213/aa91c9
3715:10.3847/2041-8213/aaa4f2
3005:10.3847/1538-4357/aa775a
2391:"GLAST Gamma-ray Bursts"
1745:List of gamma-ray bursts
1631:(from medium up to some
1475:Fermi is sensitive from
1016:low-Earth circular orbit
7036:Sonoma State University
4049:. NASA. 4 February 2013
3158:10.1126/science.1169101
2202:. NASA. 7 February 2008
1706:The 2014 prize went to
1669:Sonoma State University
1661:http://glast.sonoma.edu
1617:. It is sensitive from
1501:Gamma-ray Burst Monitor
1072:Pass 8 software upgrade
868:produces gamma rays in
459:), formerly called the
420:Gamma-ray Burst Monitor
5540:HEAO-2 (Einstein Obs.)
4004:. NASA. Archived from
2810:. NASA. 30 April 2013.
2731:. NASA. Archived from
2705:. NASA. Archived from
2260:. NASA. Archived from
1917:. CERN. Archived from
1497:
1468:
1383:
1362:
1334:
1237:Possibilities include
1234:active galactic nuclei
1131:
1082:
1022:Software modifications
971:
963:
958:GLAST launch aboard a
688:active galactic nuclei
676:
664:
656:
551:
489:active galactic nuclei
471:being used to perform
245:United Launch Alliance
5161:Space Solar Telescope
3058:"Fermi Status Update"
1863:. NASA. 28 July 2008.
1571:particle accelerators
1474:
1466:
1380:
1356:
1239:star forming galaxies
1167:in the constellation
1125:
1079:
969:
957:
888:Large Hadron Collider
752:(a) a combination of
670:
662:
655:Video: What is Fermi?
654:
549:
264:Reference system
149:Spacecraft properties
7046:Gamma-ray telescopes
6301:Orbital launches in
6234:List of planetariums
5136:NRO donation to NASA
3120:on 11 February 2009.
2499:"The Early Universe"
2339:NASA β Fermi Science
1591:microstrip detectors
1561:Large Area Telescope
962:rocket, 11 June 2008
838:yet to be conceived.
690:(AGN), pulsars, and
428:Large Area Telescope
134:Planned: 5-10 years
5930:(Mission completed)
4212:Radio and Microwave
3969:2017ApJ...848L..12A
3884:2016ApJ...819L..21L
3794:2016ApJ...833..151F
3740:(2 February 2018).
3706:2018ApJ...853L...9C
3618:2016ApJ...827L..38G
3559:2016ApJ...825L...4T
3500:2016ApJ...820L..36S
3435:2016ApJ...826L...6C
3271:on 25 November 2010
3149:2009Sci...323.1688A
3143:(5922): 1688β1693.
2996:2017ApJ...843..139A
2955:2015PhDT.......142N
2908:2015PhRvD..91l2002A
2841:fermi.gsfc.nasa.gov
2778:2007JPhCS..60..115C
2532:on 26 February 2021
2451:on 19 November 2010
2424:on 8 September 2018
2397:on 25 November 2010
2370:on 25 November 2010
2348:25 May 2017 at the
2074:2009ApJ...702..791M
1994:2009ApJ...697.1071A
1445:neutron star merger
1199:or a population of
1014:Fermi resides in a
985:Titusville, Florida
940:Unknown discoveries
473:gamma-ray astronomy
355:Argument of perigee
204:11 June 2008, 16:05
125:Fermi.GSFC.NASA.gov
63:Gamma-ray astronomy
34:
5867:Suzaku (Astro-EII)
5692:OAO-3 (Copernicus)
5676:Mikhailo Lomonosov
5524:Hinotori (Astro-A)
5131:New Worlds Mission
3229:. 12 November 2019
3203:. 19 February 2009
2709:on 22 October 2008
2559:on 13 January 2012
2445:"Milky Way Galaxy"
2128:on 27 October 2017
1841:on 7 December 2022
1815:. 23 February 2016
1789:on 8 November 2016
1498:
1469:
1384:
1363:
1212:supernova remnants
1132:
1083:
972:
964:
692:supernova remnants
677:
665:
657:
574:instrument on the
552:
538:experiment (RE7).
487:phenomena such as
475:observations from
259:Orbital parameters
208:2008-06-11UTC16:05
7018:
7017:
6522:CUTE-1.7 + APD II
6260:
6259:
6158:SIM & SIMlite
5532:Hisaki (SPRINT-A)
5492:Hakucho (CORSA-b)
5051:Astro-1 Telescope
4869:
4868:
2886:Physical Review D
2586:on 31 August 2008
2246:on 17 March 2010.
1681:Bruno Rossi Prize
1539:(a medium-energy
1286:
1052:Collision avoided
924:quantum mechanics
716:micro black holes
652:
587:bismuth germanate
469:space observatory
445:
444:
432:
431:
16:(Redirected from
7073:
7061:CERN experiments
7041:Space telescopes
6914:Shiyan Weixing 3
6536:
6530:
6524:
6518:
6512:
6506:
6500:
6306:
6305:
6304:
6287:
6280:
6273:
6264:
6250:
6249:
6049:
6045:Hitomi (Astro-H)
6041:
6033:
6025:
6017:
6009:
6001:
5993:
5985:
5977:
5969:
5950:
5942:
5931:
5919:
5911:
5903:
5895:
5887:
5879:
5871:
5863:
5855:
5847:
5839:
5831:
5823:
5815:
5807:
5799:
5791:
5783:
5775:
5767:
5759:
5751:
5696:
5688:
5680:
5672:
5664:
5656:
5648:
5640:
5632:
5624:
5616:
5608:
5600:
5592:
5584:
5576:
5568:
5560:
5552:
5544:
5536:
5528:
5520:
5512:
5504:
5496:
5488:
5480:
5472:
5464:
5456:
5448:
5440:
5432:
5424:
5416:
5408:
5400:
5392:
5384:
5376:
5368:
5360:
5352:
5344:
5336:
5328:
5320:
5295:
5287:
5279:
5271:
5263:
5255:
5247:
5239:
5231:
5223:
5215:
5207:
5199:
5191:
5029:
5021:
5013:
5005:
4997:
4989:
4981:
4973:
4965:
4957:
4949:
4941:
4933:
4925:
4917:
4909:
4901:
4893:
4885:
4862:
4854:
4846:
4838:
4830:
4822:
4814:
4806:
4798:
4790:
4779:or unclassified)
4769:
4761:
4753:
4745:
4737:
4729:
4721:
4713:
4705:
4697:
4689:
4681:
4673:
4665:
4657:
4649:
4641:
4633:
4625:
4617:
4609:
4584:
4576:
4568:
4560:
4552:
4544:
4536:
4528:
4524:Hinode (Solar-B)
4520:
4512:
4504:
4496:
4475:
4467:
4459:
4451:
4443:
4435:
4427:
4419:
4415:Hinode (Solar-B)
4411:
4403:
4395:
4387:
4379:
4371:
4363:
4355:
4347:
4338:
4330:
4309:
4301:
4293:
4285:
4264:
4256:
4248:
4240:
4232:
4224:
4208:
4197:Space telescopes
4190:
4183:
4176:
4167:
4137:at Stanford.edu
4104:
4103:
4101:
4099:
4087:
4081:
4080:
4078:
4076:
4065:
4059:
4058:
4056:
4054:
4043:
4037:
4036:
4034:
4032:
4016:
4010:
4009:
4008:on 17 June 2008.
3997:
3991:
3990:
3980:
3962:
3938:
3932:
3931:
3929:
3927:
3912:
3906:
3905:
3895:
3877:
3851:
3842:
3841:
3839:
3837:
3822:
3816:
3815:
3805:
3787:
3763:
3757:
3756:
3754:
3752:
3734:
3728:
3727:
3717:
3699:
3675:
3669:
3668:
3666:
3664:
3646:
3640:
3639:
3629:
3611:
3587:
3581:
3580:
3570:
3552:
3528:
3522:
3521:
3511:
3493:
3463:
3457:
3456:
3446:
3428:
3404:
3398:
3397:
3395:
3393:
3378:
3372:
3371:
3363:
3352:
3351:
3343:
3334:
3333:
3325:
3316:
3315:
3307:
3296:
3295:
3287:
3281:
3280:
3278:
3276:
3260:
3254:
3253:
3245:
3239:
3238:
3236:
3234:
3219:
3213:
3212:
3210:
3208:
3193:
3187:
3186:
3160:
3128:
3122:
3121:
3104:
3098:
3097:
3095:
3093:
3076:
3070:
3069:
3067:
3065:
3053:
3047:
3046:
3044:
3032:
3026:
3025:
3007:
2989:
2965:
2959:
2958:
2942:
2936:
2935:
2901:
2880:
2874:
2873:
2871:
2858:
2852:
2851:
2849:
2847:
2833:
2827:
2826:
2818:
2812:
2811:
2804:
2798:
2797:
2771:
2769:astro-ph/0610960
2751:
2745:
2744:
2742:
2740:
2735:on 9 August 2007
2725:
2719:
2718:
2716:
2714:
2698:
2689:
2688:
2686:
2684:
2674:
2668:
2667:
2665:
2663:
2654:. Archived from
2644:
2638:
2637:
2629:
2623:
2622:
2620:
2618:
2602:
2596:
2595:
2593:
2591:
2575:
2569:
2568:
2566:
2564:
2548:
2542:
2541:
2539:
2537:
2521:
2515:
2514:
2512:
2510:
2494:
2488:
2487:
2485:
2483:
2467:
2461:
2460:
2458:
2456:
2440:
2434:
2433:
2431:
2429:
2413:
2407:
2406:
2404:
2402:
2386:
2380:
2379:
2377:
2375:
2359:
2353:
2335:
2329:
2328:
2326:
2324:
2319:on 25 April 2009
2305:
2296:
2295:
2293:
2291:
2280:
2274:
2273:
2271:
2269:
2264:on 9 August 2007
2254:
2248:
2247:
2236:
2230:
2229:
2228:on 2 April 2010.
2218:
2212:
2211:
2209:
2207:
2196:
2190:
2189:
2187:
2185:
2170:
2164:
2163:
2161:
2159:
2144:
2138:
2137:
2135:
2133:
2117:
2111:
2110:
2108:
2100:
2094:
2093:
2067:
2043:
2037:
2036:
2034:
2032:
2020:
2014:
2013:
1987:
1978:(2): 1071β1102.
1963:
1957:
1956:
1954:
1952:
1937:
1931:
1930:
1928:
1926:
1907:
1901:
1900:
1898:
1896:
1885:
1879:
1878:
1871:
1865:
1864:
1857:
1851:
1850:
1848:
1846:
1831:
1825:
1824:
1822:
1820:
1805:
1799:
1798:
1796:
1794:
1788:
1781:
1773:
1720:
1630:
1623:
1538:
1527:
1511:gamma ray bursts
1492:
1481:
1332:
1288:
1287:
1270:
1243:galactic mergers
1216:cosmic particles
1135:Pulsar discovery
950:Mission timeline
815:Milky Way galaxy
775:Gamma-ray bursts
706:gamma-ray bursts
653:
602:Gilbert, Arizona
598:Orbital Sciences
594:General Dynamics
501:gamma-ray bursts
441:
412:
407:
305:Perigee altitude
211:
209:
196:Start of mission
158:General Dynamics
131:Mission duration
112:
103:
102:
96:
42:
35:
21:
7081:
7080:
7076:
7075:
7074:
7072:
7071:
7070:
7021:
7020:
7019:
7014:
7009:
7002:
6949:
6898:
6841:
6771:
6699:
6664:
6599:
6544:
6532:
6526:
6520:
6514:
6508:
6502:
6496:
6441:
6377:
6339:
6313:
6312:
6302:
6300:
6299:
6297:
6291:
6261:
6256:
6238:
6224:X-ray telescope
6197:
6079:Constellation-X
6052:
6047:
6039:
6031:
6023:
6015:
6007:
5999:
5991:
5983:
5975:
5967:
5953:
5948:
5940:
5929:
5928:
5922:
5917:
5915:Yokoh (Solar-A)
5909:
5901:
5893:
5885:
5883:Tenma (Astro-B)
5877:
5869:
5861:
5853:
5845:
5837:
5829:
5821:
5813:
5805:
5797:
5789:
5781:
5773:
5765:
5757:
5749:
5694:
5686:
5678:
5670:
5662:
5654:
5646:
5644:LISA Pathfinder
5638:
5630:
5622:
5614:
5606:
5598:
5590:
5582:
5574:
5566:
5558:
5550:
5542:
5534:
5526:
5518:
5510:
5502:
5500:HALCA (MUSES-B)
5494:
5486:
5478:
5476:Ginga (Astro-C)
5470:
5462:
5454:
5446:
5438:
5430:
5422:
5414:
5406:
5398:
5390:
5382:
5374:
5366:
5358:
5350:
5342:
5334:
5326:
5318:
5293:
5285:
5277:
5269:
5261:
5253:
5245:
5237:
5229:
5221:
5213:
5205:
5197:
5195:Akari (Astro-F)
5189:
5175:
5032:
5027:
5019:
5011:
5003:
4995:
4987:
4979:
4971:
4963:
4955:
4947:
4939:
4931:
4923:
4915:
4907:
4899:
4891:
4883:
4865:
4860:
4852:
4844:
4836:
4828:
4820:
4812:
4804:
4796:
4788:
4778:
4777:Other (particle
4772:
4767:
4759:
4751:
4743:
4735:
4727:
4719:
4711:
4703:
4695:
4687:
4679:
4671:
4663:
4655:
4647:
4639:
4631:
4623:
4615:
4607:
4587:
4582:
4574:
4566:
4558:
4550:
4542:
4534:
4526:
4518:
4510:
4502:
4494:
4478:
4473:
4465:
4457:
4449:
4441:
4433:
4425:
4417:
4409:
4401:
4393:
4385:
4377:
4369:
4361:
4353:
4345:
4336:
4328:
4312:
4307:
4299:
4291:
4283:
4267:
4262:
4254:
4246:
4238:
4230:
4222:
4199:
4194:
4113:
4108:
4107:
4097:
4095:
4090:Watzke, Megan.
4089:
4088:
4084:
4074:
4072:
4067:
4066:
4062:
4052:
4050:
4045:
4044:
4040:
4030:
4028:
4027:on 23 June 2019
4018:
4017:
4013:
3999:
3998:
3994:
3940:
3939:
3935:
3925:
3923:
3914:
3913:
3909:
3853:
3852:
3845:
3835:
3833:
3824:
3823:
3819:
3765:
3764:
3760:
3750:
3748:
3736:
3735:
3731:
3677:
3676:
3672:
3662:
3660:
3652:(3 June 2016).
3648:
3647:
3643:
3589:
3588:
3584:
3530:
3529:
3525:
3465:
3464:
3460:
3406:
3405:
3401:
3391:
3389:
3380:
3379:
3375:
3365:
3364:
3355:
3345:
3344:
3337:
3327:
3326:
3319:
3309:
3308:
3299:
3289:
3288:
3284:
3274:
3272:
3262:
3261:
3257:
3247:
3246:
3242:
3232:
3230:
3227:www.science.org
3221:
3220:
3216:
3206:
3204:
3195:
3194:
3190:
3130:
3129:
3125:
3106:
3105:
3101:
3091:
3089:
3078:
3077:
3073:
3063:
3061:
3055:
3054:
3050:
3034:
3033:
3029:
2967:
2966:
2962:
2944:
2943:
2939:
2882:
2881:
2877:
2860:
2859:
2855:
2845:
2843:
2835:
2834:
2830:
2820:
2819:
2815:
2806:
2805:
2801:
2753:
2752:
2748:
2738:
2736:
2727:
2726:
2722:
2712:
2710:
2700:
2699:
2692:
2682:
2680:
2676:
2675:
2671:
2661:
2659:
2652:Spaceflight Now
2646:
2645:
2641:
2631:
2630:
2626:
2616:
2614:
2604:
2603:
2599:
2589:
2587:
2577:
2576:
2572:
2562:
2560:
2550:
2549:
2545:
2535:
2533:
2523:
2522:
2518:
2508:
2506:
2505:on 1 March 2021
2496:
2495:
2491:
2481:
2479:
2469:
2468:
2464:
2454:
2452:
2442:
2441:
2437:
2427:
2425:
2418:"Neutron Stars"
2415:
2414:
2410:
2400:
2398:
2388:
2387:
2383:
2373:
2371:
2361:
2360:
2356:
2350:Wayback Machine
2336:
2332:
2322:
2320:
2307:
2306:
2299:
2289:
2287:
2282:
2281:
2277:
2267:
2265:
2256:
2255:
2251:
2238:
2237:
2233:
2220:
2219:
2215:
2205:
2203:
2198:
2197:
2193:
2183:
2181:
2174:"Data Analysis"
2172:
2171:
2167:
2157:
2155:
2146:
2145:
2141:
2131:
2129:
2119:
2118:
2114:
2106:
2102:
2101:
2097:
2045:
2044:
2040:
2030:
2028:
2022:
2021:
2017:
1965:
1964:
1960:
1950:
1948:
1939:
1938:
1934:
1924:
1922:
1921:on 13 June 2019
1909:
1908:
1904:
1894:
1892:
1887:
1886:
1882:
1873:
1872:
1868:
1859:
1858:
1854:
1844:
1842:
1833:
1832:
1828:
1818:
1816:
1809:"Fermi - Orbit"
1807:
1806:
1802:
1792:
1790:
1786:
1779:
1775:
1774:
1763:
1758:
1731:
1718:
1689:Roger W. Romani
1677:
1657:
1625:
1618:
1587:pair production
1563:
1533:
1522:
1503:
1487:
1476:
1461:
1440:
1389:
1371:gamma-ray burst
1351:
1339:
1333:
1330:
1319:
1298:
1297:
1296:
1295:
1291:
1290:
1289:
1278:
1273:
1272:
1271:
1262:
1261:
1255:
1230:
1224:
1208:
1189:Galactic Center
1185:
1161:
1137:
1120:
1111:
1074:
1066:
1054:
1041:
1039:Sky survey mode
1032:
1024:
1012:
997:Delta 7920H-10C
993:
977:
952:
928:quantum gravity
743:active galaxies
708:and transients.
643:
641:
622:
560:pair-conversion
544:
477:low Earth orbit
410:
315:Apogee altitude
285:Semi-major axis
221:Delta II 7920-H
207:
205:
183:1,500 W average
135:
97:
92:
28:
23:
22:
15:
12:
11:
5:
7079:
7077:
7069:
7068:
7063:
7058:
7053:
7048:
7043:
7038:
7033:
7023:
7022:
7016:
7015:
7011:Crewed flights
7007:
7004:
7003:
7001:
7000:
6987:
6982:
6973:
6968:
6963:
6957:
6955:
6951:
6950:
6948:
6947:
6945:Progress M-01M
6942:
6926:
6921:
6916:
6906:
6904:
6900:
6899:
6897:
6896:
6891:
6886:
6877:
6867:
6862:
6855:
6849:
6847:
6843:
6842:
6840:
6839:
6834:
6822:
6809:
6804:
6799:
6794:
6789:
6779:
6777:
6773:
6772:
6770:
6769:
6748:
6743:
6736:
6727:
6707:
6705:
6701:
6700:
6698:
6697:
6692:
6687:
6682:
6672:
6670:
6666:
6665:
6663:
6662:
6657:
6652:
6627:
6618:
6613:
6607:
6605:
6601:
6600:
6598:
6597:
6585:
6580:
6563:
6558:
6552:
6550:
6546:
6545:
6543:
6542:
6537:
6486:
6481:
6476:
6467:
6462:
6457:
6449:
6447:
6443:
6442:
6440:
6439:
6434:
6429:
6424:
6419:
6414:
6411:Spacelab MD002
6394:
6385:
6383:
6379:
6378:
6376:
6375:
6370:
6365:
6353:
6347:
6345:
6341:
6340:
6338:
6337:
6335:Ekspress AM-33
6332:
6327:
6321:
6319:
6315:
6314:
6308:
6293:
6292:
6290:
6289:
6282:
6275:
6267:
6258:
6257:
6255:
6254:
6243:
6240:
6239:
6237:
6236:
6231:
6226:
6221:
6216:
6211:
6205:
6203:
6199:
6198:
6196:
6195:
6190:
6185:
6180:
6175:
6170:
6165:
6160:
6155:
6150:
6145:
6140:
6135:
6130:
6125:
6120:
6115:
6110:
6105:
6098:
6093:
6088:
6081:
6076:
6071:
6066:
6060:
6058:
6054:
6053:
6051:
6050:
6042:
6034:
6026:
6018:
6010:
6002:
5994:
5986:
5978:
5970:
5961:
5959:
5955:
5954:
5952:
5951:
5943:
5934:
5932:
5924:
5923:
5921:
5920:
5912:
5904:
5896:
5888:
5880:
5872:
5864:
5856:
5848:
5840:
5832:
5824:
5816:
5808:
5800:
5792:
5784:
5776:
5768:
5760:
5752:
5744:
5743:
5742:
5737:
5732:
5727:
5722:
5717:
5712:
5707:
5697:
5689:
5681:
5673:
5665:
5657:
5649:
5641:
5633:
5625:
5617:
5609:
5601:
5593:
5585:
5577:
5569:
5561:
5553:
5545:
5537:
5529:
5521:
5513:
5505:
5497:
5489:
5481:
5473:
5465:
5457:
5449:
5441:
5433:
5425:
5417:
5409:
5401:
5393:
5385:
5377:
5369:
5361:
5356:Compton (CGRO)
5353:
5345:
5337:
5329:
5321:
5308:
5307:
5306:
5301:
5288:
5283:ASCA (Astro-D)
5280:
5272:
5264:
5256:
5248:
5240:
5232:
5224:
5216:
5208:
5200:
5192:
5183:
5181:
5177:
5176:
5174:
5173:
5168:
5163:
5158:
5153:
5148:
5143:
5138:
5133:
5128:
5123:
5118:
5113:
5108:
5103:
5098:
5093:
5088:
5086:Hypertelescope
5083:
5078:
5073:
5068:
5066:Fresnel Imager
5063:
5058:
5053:
5048:
5042:
5040:
5034:
5033:
5031:
5030:
5022:
5014:
5006:
4998:
4990:
4982:
4974:
4966:
4958:
4950:
4942:
4934:
4926:
4918:
4910:
4902:
4894:
4886:
4877:
4875:
4871:
4870:
4867:
4866:
4864:
4863:
4855:
4847:
4839:
4831:
4823:
4815:
4807:
4799:
4791:
4782:
4780:
4774:
4773:
4771:
4770:
4762:
4754:
4746:
4738:
4730:
4722:
4714:
4706:
4701:Max Valier Sat
4698:
4690:
4682:
4674:
4666:
4658:
4650:
4642:
4637:HXMT (Insight)
4634:
4629:Einstein Probe
4626:
4618:
4613:Chandra (AXAF)
4610:
4601:
4599:
4589:
4588:
4586:
4585:
4577:
4569:
4561:
4553:
4545:
4537:
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2636:. NASA. 04-08.
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4131:at Sonoma.edu
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2553:"Dark Matter"
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2473:
2466:
2463:
2450:
2446:
2439:
2436:
2423:
2419:
2412:
2409:
2396:
2392:
2385:
2382:
2369:
2365:
2358:
2355:
2351:
2347:
2344:
2340:
2334:
2331:
2318:
2314:
2310:
2304:
2302:
2298:
2285:
2284:"The Mission"
2279:
2276:
2263:
2259:
2253:
2250:
2245:
2241:
2235:
2232:
2227:
2223:
2217:
2214:
2201:
2195:
2192:
2179:
2175:
2169:
2166:
2153:
2149:
2143:
2140:
2127:
2123:
2116:
2113:
2105:
2099:
2096:
2091:
2087:
2083:
2079:
2075:
2071:
2066:
2061:
2057:
2053:
2049:
2042:
2039:
2026:
2019:
2016:
2011:
2007:
2003:
1999:
1995:
1991:
1986:
1981:
1977:
1973:
1969:
1962:
1959:
1946:
1942:
1936:
1933:
1920:
1916:
1912:
1906:
1903:
1890:
1884:
1881:
1876:
1870:
1867:
1862:
1856:
1853:
1840:
1836:
1830:
1827:
1814:
1813:Heavens Above
1810:
1804:
1801:
1785:
1778:
1772:
1770:
1768:
1766:
1762:
1755:
1751:
1748:
1746:
1743:
1741:
1738:
1736:
1733:
1732:
1728:
1726:
1724:
1715:
1713:
1712:Fermi bubbles
1709:
1708:Tracy Slatyer
1704:
1702:
1698:
1697:Alice Harding
1694:
1690:
1685:
1682:
1674:
1672:
1670:
1666:
1662:
1654:
1652:
1650:
1646:
1642:
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1634:
1629:
1622:
1616:
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1601:
1596:
1592:
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1576:
1572:
1568:
1560:
1558:
1556:
1551:
1549:
1544:
1542:
1537:
1531:
1526:
1520:
1519:scintillators
1516:
1512:
1508:
1500:
1496:
1491:
1485:
1480:
1473:
1465:
1458:
1456:
1454:
1450:
1449:gravitational
1446:
1437:
1435:
1432:
1426:
1424:
1421:on board the
1420:
1416:
1412:
1407:
1404:
1399:
1394:
1386:
1379:
1375:
1372:
1368:
1360:
1355:
1348:
1346:
1344:
1336:
1327:
1322:
1316:
1314:
1311:
1307:
1306:Fermi bubbles
1303:
1269:
1252:
1250:
1248:
1244:
1240:
1235:
1229:
1221:
1219:
1217:
1213:
1205:
1203:
1202:
1198:
1194:
1190:
1182:
1180:
1178:
1174:
1170:
1166:
1158:
1156:
1154:
1150:
1146:
1143:in the CTA 1
1142:
1134:
1129:
1124:
1117:
1115:
1108:
1106:
1102:
1098:
1096:
1092:
1087:
1078:
1071:
1069:
1063:
1061:
1059:
1051:
1049:
1046:
1038:
1036:
1029:
1027:
1021:
1019:
1017:
1009:
1007:
1005:
1002:
998:
990:
988:
986:
982:
974:
968:
961:
956:
949:
944:
943:
939:
938:
934:
929:
925:
921:
918:
914:
910:
906:
902:
901:
898:
894:
893:
889:
885:
881:
880:
876:
875:
871:
867:
863:
862:
859:
856:
855:
850:
849:
846:
842:
841:
836:
832:
831:
828:
825:
824:
820:
819:
816:
813:
812:
808:
804:
800:
796:
792:
791:
788:
787:Neutron stars
785:
784:
780:
779:
776:
773:
772:
766:
762:
759:
755:
751:
750:
748:
747:
744:
740:
737:
736:
735:
733:
729:
721:
717:
713:
710:
707:
703:
700:
696:
693:
689:
685:
684:
683:
680:
674:
669:
661:
638:
636:
634:
629:
627:
619:
617:
614:
610:
607:
603:
599:
595:
588:
584:
583:sodium iodide
580:
577:
573:
569:
568:electronvolts
565:
561:
557:
556:
555:
548:
541:
539:
537:
533:
529:
525:
521:
517:
513:
508:
506:
502:
498:
494:
490:
486:
482:
481:astrophysical
478:
474:
470:
466:
462:
458:
454:
450:
440:
435:
427:
423:
419:
415:
408:
404:
400:
396:
394:
390:
386:
382:
379:15.10 rev/day
378:
376:
372:
368:
366:
362:
358:
356:
352:
348:
346:
342:
338:
336:
332:
328:
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312:
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95:
91:
89:
85:
82:
78:
74:
71:
67:
64:
61:
57:
53:
49:
45:
41:
36:
30:
19:
7066:Enrico Fermi
7031:Astrophysics
7010:
6980:Eutelsat W2M
6928:
6859:Soyuz TMA-13
6857:
6824:
6787:Huan Jing 1B
6783:Huan Jing 1A
6738:
6730:Superbird-C2
6710:
6655:OSTM/Jason-2
6650:Orbcomm FM41
6646:Orbcomm FM40
6642:Orbcomm FM39
6638:Orbcomm FM38
6634:Orbcomm FM37
6630:Orbcomm FM29
6615:
6587:
6454:Soyuz TMA-12
6452:
6396:
6389:
6355:
6100:
6083:
5927:Hibernating
5679:(2016β2019?)
5222:(1962, 1964)
5121:Nano-JASMINE
4945:NEO Surveyor
4861:(since 2006)
4853:(since 2020)
4845:(since 1995)
4837:(since 2019)
4829:(since 2017)
4821:(since 2008)
4813:(since 2015)
4805:(since 2015)
4797:(since 2011)
4789:(since 1997)
4768:(since 1999)
4760:(since 2024)
4752:(since 2023)
4744:(since 2022)
4736:(since 2012)
4728:(since 2017)
4720:(since 2018)
4712:(since 2009)
4704:(since 2017)
4696:(since 2004)
4688:(since 2024)
4680:(since 2019)
4672:(since 2021)
4664:(since 2020)
4656:(since 2008)
4652:
4648:(since 2002)
4640:(since 2017)
4632:(since 2024)
4624:(since 2015)
4616:(since 1999)
4608:(since 2015)
4583:(since 2004)
4575:(since 2006)
4567:(since 2020)
4559:(since 2008)
4551:(since 1995)
4543:(since 2010)
4535:(since 2013)
4527:(since 2006)
4519:(since 2021)
4511:(since 2015)
4503:(since 2022)
4495:(since 2023)
4474:(since 2018)
4466:(since 2004)
4458:(since 2008)
4450:(since 1995)
4442:(since 2010)
4434:(since 2001)
4426:(since 2013)
4418:(since 2006)
4410:(since 1990)
4402:(since 2005)
4394:(since 2013)
4386:(since 2021)
4378:(since 2023)
4370:(since 2015)
4362:(since 2019)
4354:(since 2021)
4346:(since 2013)
4337:(since 2015)
4329:(since 2018)
4308:(since 2009)
4300:(since 2008)
4292:(since 2001)
4284:(since 2022)
4263:(since 2024)
4255:(since 1994)
4247:(since 2018)
4239:(since 2006)
4231:(since 2020)
4223:(since 2018)
4096:. Retrieved
4085:
4073:. Retrieved
4063:
4051:. Retrieved
4041:
4029:. Retrieved
4025:the original
4014:
4006:the original
3995:
3950:
3946:
3936:
3924:. Retrieved
3920:
3910:
3865:
3859:
3834:. Retrieved
3830:
3820:
3775:
3771:
3761:
3749:. Retrieved
3745:
3732:
3687:
3683:
3673:
3661:. Retrieved
3657:
3644:
3599:
3595:
3585:
3540:
3536:
3526:
3481:
3475:
3469:
3461:
3416:
3412:
3402:
3390:. Retrieved
3386:
3376:
3285:
3273:. Retrieved
3269:the original
3258:
3243:
3231:. Retrieved
3226:
3217:
3205:. Retrieved
3200:
3191:
3140:
3136:
3126:
3118:the original
3111:
3102:
3090:. Retrieved
3084:
3074:
3062:. Retrieved
3051:
3030:
2977:
2973:
2963:
2947:Ph.D. Thesis
2946:
2940:
2889:
2885:
2878:
2856:
2844:. Retrieved
2840:
2831:
2816:
2802:
2759:
2755:
2749:
2737:. Retrieved
2733:the original
2723:
2711:. Retrieved
2707:the original
2681:. Retrieved
2672:
2660:. Retrieved
2656:the original
2651:
2642:
2627:
2615:. Retrieved
2611:the original
2600:
2588:. Retrieved
2584:the original
2573:
2561:. Retrieved
2557:the original
2546:
2534:. Retrieved
2530:the original
2519:
2507:. Retrieved
2503:the original
2492:
2480:. Retrieved
2476:the original
2465:
2453:. Retrieved
2449:the original
2438:
2426:. Retrieved
2422:the original
2411:
2399:. Retrieved
2395:the original
2384:
2372:. Retrieved
2368:the original
2357:
2333:
2321:. Retrieved
2317:the original
2288:. Retrieved
2278:
2266:. Retrieved
2262:the original
2252:
2244:the original
2234:
2226:the original
2216:
2204:. Retrieved
2194:
2182:. Retrieved
2177:
2168:
2156:. Retrieved
2151:
2142:
2130:. Retrieved
2126:the original
2115:
2098:
2055:
2051:
2047:
2041:
2029:. Retrieved
2018:
1975:
1971:
1967:
1961:
1949:. Retrieved
1944:
1935:
1923:. Retrieved
1919:the original
1914:
1905:
1893:. Retrieved
1883:
1869:
1855:
1843:. Retrieved
1839:the original
1829:
1817:. Retrieved
1812:
1803:
1791:. Retrieved
1784:the original
1716:
1705:
1686:
1678:
1658:
1607:scintillator
1564:
1552:
1545:
1515:solar flares
1509:produced by
1504:
1441:
1427:
1408:
1390:
1364:
1340:
1324:
1320:
1305:
1299:
1247:interactions
1231:
1209:
1186:
1173:relativistic
1162:
1138:
1112:
1103:
1099:
1088:
1084:
1067:
1055:
1042:
1033:
1025:
1013:
999:rocket from
994:
978:
895:Fundamental
870:solar flares
725:
697:Resolve the
681:
678:
675:: 2009β2013)
672:
633:Enrico Fermi
630:
623:
615:
611:
592:
553:
512:Enrico Fermi
509:
505:solar flares
485:cosmological
464:
460:
456:
452:
448:
446:
365:Mean anomaly
295:Eccentricity
154:Manufacturer
76:
59:Mission type
29:
6998:Kosmos 2449
6994:Kosmos 2448
6990:Kosmos 2447
6966:Kosmos 2446
6924:Kosmos 2445
6820:Kosmos 2444
6816:Kosmos 2243
6812:Kosmos 2442
6712:Trailblazer
6695:Kosmos 2441
6685:EchoStar XI
6680:ProtoStar 1
6660:Kosmos 2440
6574:Kosmos 2439
6570:Kosmos 2438
6566:Kosmos 2437
6489:Cartosat-2A
6474:Star One C2
6403:KibΕ ELM-PS
6390:Jules Verne
6040:(2014β2015)
5992:(2012β2013)
5958:Lost/Failed
5949:(1998β2010)
5941:(1998β2005)
5918:(1991β2001)
5910:(2001β2010)
5894:(1970β1973)
5886:(1983β1985)
5878:(1975β1980)
5870:(2005β2015)
5862:(2003β2020)
5854:(2011β2019)
5846:(1979β1985)
5838:(1975β1979)
5830:(1972β1973)
5822:(1992β2004)
5814:(1995β2012)
5806:(1990β1999)
5798:(2002β2018)
5790:(1983β1984)
5782:(2009β2013)
5766:(2006β2016)
5695:(1972β1981)
5687:(1968β1973)
5671:(1996β1997)
5663:(2003β2019)
5655:(2015β2017)
5647:(2015β2017)
5639:(1997β2002)
5631:(1990β2001)
5623:(2009β2018)
5615:(1996β2004)
5607:(1978β1996)
5599:(1996β1998)
5591:(1995β1996)
5567:(1989β1993)
5559:(2000β2008)
5551:(1979β1981)
5543:(1978β1982)
5535:(2013β2023)
5527:(1981β1991)
5519:(2009β2013)
5511:(1977β1979)
5503:(1997β2005)
5495:(1979β1985)
5487:(1989β1998)
5479:(1987β1991)
5471:(1990β1992)
5463:(2003β2013)
5455:(1987β2001)
5447:(1999β2007)
5439:(1992β2001)
5431:(1983β1986)
5420:Explorer 11
5391:(2017β2019)
5383:(1989β1993)
5375:(1975β1982)
5367:(2006β2013)
5359:(1991β2000)
5351:(2003β2008)
5343:(1996β2003)
5335:(1974β1976)
5327:(1983β1991)
5286:(1993β2000)
5278:(1973β1974)
5270:(2017β2019)
5262:(1979β1982)
5254:(1974β1980)
5246:(1971β1972)
5238:(1967β1969)
5214:(1962β1972)
5206:(1993β2005)
5198:(2006β2011)
5190:(2007β2024)
4484:Ultraviolet
4119:at NASA.gov
4098:13 February
4053:13 February
3926:19 February
3836:17 February
3751:14 February
3275:16 November
3092:16 November
2617:16 November
2590:16 November
2563:16 November
2536:16 November
2509:16 November
2482:16 November
2455:16 November
2428:16 November
2401:16 November
2374:16 November
2206:10 February
1819:23 February
1793:23 February
1740:GRB 160625B
1719:GRB 170817A
1675:Rossi Prize
1611:arc minutes
1600:calorimeter
1482:, a medium
1459:Instruments
1411:GRB 150101B
1367:GRB 130427A
1349:GRB 130427A
1310:light-years
1197:dark matter
1165:GRB 080916C
1153:light-years
1128:Vela pulsar
1118:Discoveries
1093:and to the
1058:Kosmos 1805
877:Dark matter
497:dark matter
411:Instruments
375:Mean motion
325:Inclination
228:Launch site
201:Launch date
164:Launch mass
7025:Categories
6985:Fengyun 2E
6976:Hot Bird 9
6884:Shijian 6F
6880:Shijian 6E
6826:Shenzhou 7
6716:NanoSail-D
6690:SAR-Lupe 5
6625:TΓΌrksat 3A
6611:ChinaSat 9
6583:Fengyun 3A
6437:SAR-Lupe 4
6432:DirecTV-11
5899:Vanguard 3
5211:Alouette 1
5056:AstroSat-2
4765:XMM-Newton
4281:James Webb
4031:5 December
3960:1710.05833
3953:(2). L12.
3875:1602.04735
3868:(2). L21.
3785:1608.08626
3778:(2): 151.
3697:1801.02305
3609:1606.00314
3602:(2). L38.
3550:1604.00955
3491:1602.04180
3484:(2). L36.
3426:1602.03920
3207:13 January
3042:1810.11394
2987:1702.00476
2980:(2): 139.
2899:1506.00013
2184:26 October
2158:26 October
2132:26 October
2031:27 October
1970:Mission".
1951:21 January
1925:21 January
1756:References
1595:ionization
1593:, causing
1567:gamma rays
1528:(a medium
1507:gamma-rays
1095:background
917:Einstein's
913:wavelength
626:Alan Stern
606:spacecraft
268:Geocentric
241:Contractor
172:Dimensions
6894:Venesat-1
6831:Banxing-1
6807:Galaxy 19
6776:September
6724:Explorers
6621:Skynet 5C
6578:Yubileiny
6561:Galaxy 18
6516:Compass-1
6470:Vinasat-1
6325:Thuraya 3
6102:Eddington
6057:Cancelled
5564:Hipparcos
4977:Spektr-UV
4834:Mini-EUSO
4826:ISS-CREAM
4677:Spektr-RG
4597:Gamma-ray
4492:Aditya-L1
4383:Hayabusa2
4260:Queqiao 2
4204:Operating
3987:217162243
3902:119161672
3690:(1). L9.
3636:118576283
3543:(1): L4.
3419:(1). L6.
3022:119187437
3014:0004-637X
2924:1550-7998
2869:1303.3514
2337:See also
2090:118396838
2065:0908.0450
1985:0902.1089
1679:The 2011
1626:300
1555:positrons
1541:gamma-ray
1488:300
1149:gamma ray
1145:supernova
981:Astrotech
975:Prelaunch
799:Milky Way
763:(b) only
758:positrons
754:electrons
699:gamma-ray
613:Arizona.
518:aboard a
339:95.33 min
278:Low Earth
212: UTC
94:2008-029A
88:COSPAR ID
18:Fermi LAT
6971:Yaogan 5
6961:Yaogan 4
6954:December
6919:Astra 1M
6903:November
6792:GeoEye-1
6528:Delfi-C3
6498:AAUSat-2
6362:Columbus
6344:February
6153:Sentinel
5851:Spektr-R
5787:RELIKT-1
5628:Kristall
5516:Herschel
5340:BeppoSAX
5101:JEM-EUSO
5096:iWF-MAXI
5038:Proposed
5001:LiteBIRD
4993:Spektr-M
4717:MinXSS-2
4645:INTEGRAL
4508:Astrosat
4334:Astrosat
4273:Infrared
3812:10530229
3577:29097240
3470:INTEGRAL
3453:41946613
3392:22 March
3175:19228997
2739:9 August
2346:Archived
2323:29 April
2290:9 August
2268:9 August
2010:26361978
1895:9 August
1729:See also
1723:GW170817
1619:20
1583:positron
1579:electron
1534:40
1431:Avi Loeb
1415:GW170817
1398:INTEGRAL
1329:β
1201:pulsars.
960:Delta II
835:galaxies
732:Universe
542:Overview
532:INTEGRAL
520:Delta II
467:), is a
384:Velocity
299:0.001282
69:Operator
6930:STS-126
6889:COSMO-3
6846:October
6802:Nimiq-4
6767:Trochia
6594:KibΕ PM
6589:STS-124
6534:SEEDS-2
6493:Rubin-8
6484:GIOVE-B
6427:USA-201
6417:USA-200
6398:STS-123
6357:STS-122
6318:January
6202:Related
6113:FINESSE
6091:Destiny
6074:Astro-G
6037:Tsubame
6029:Astro-E
6005:ABRIXAS
5859:Spitzer
5843:Solwind
5795:R/HESSI
5755:Orion 2
5747:Orion 1
5452:Kvant-1
5348:CHIPSat
5311:Astro-2
5291:Astro-1
5267:ASTERIA
5259:Ariel 6
5251:Ariel 5
5243:Ariel 4
5235:Ariel 3
5227:Ariel 2
5219:Ariel 1
5180:Retired
5171:THESEUS
5156:Solar-D
5151:PhoENiX
4996:(2030+)
4953:JASMINE
4921:Xuntian
4889:SPHEREx
4874:Planned
4423:NEOSSat
4318:Optical
4244:Queqiao
4075:16 June
3965:Bibcode
3880:Bibcode
3790:Bibcode
3724:3513893
3702:Bibcode
3614:Bibcode
3555:Bibcode
3518:3463753
3496:Bibcode
3431:Bibcode
3370:. NASA.
3350:. NASA.
3332:. NASA.
3252:. NASA.
3183:7821247
3167:1357451
3145:Bibcode
3137:Science
3064:19 June
2992:Bibcode
2951:Bibcode
2932:6260348
2904:Bibcode
2846:3 April
2825:. NASA.
2794:2226430
2774:Bibcode
2070:Bibcode
1990:Bibcode
1750:eROSITA
1575:Photons
1523:8
1477:8
1382:curves.
933:photons
905:physics
897:physics
797:in the
795:pulsars
765:protons
739:Blazars
639:Mission
624:NASA's
564:photons
493:pulsars
455:, also
369:229.00Β°
359:131.16Β°
235:SLC-17B
206: (
121:Website
109:SATCAT
6939:PSSC-1
6837:Ratsat
6763:Choros
6751:Tachys
6734:AMC-21
6720:PRESat
6704:August
6676:Badr-6
6540:Amos-3
6510:CanX-6
6504:CanX-2
6465:C/NOFS
6460:ICO G1
6422:AMC-14
6407:Dextre
6373:Kizuna
6368:Thor 5
6330:TecSAR
6310:2009 β
6295:β 2007
6178:TAUVEX
6085:Darwin
6064:Aelita
6048:(2016)
6032:(2000)
6024:(1999)
6016:(1996)
6013:HETE-1
6008:(1999)
6000:(1965)
5984:(1976)
5976:(1970)
5968:(1966)
5902:(1959)
5819:SAMPEX
5779:Planck
5774:(2018)
5771:PicSat
5763:PAMELA
5758:(1973)
5750:(1971)
5652:MinXSS
5620:Kepler
5583:(1983)
5575:(2024)
5556:HETE-2
5548:HEAO-3
5508:HEAO-1
5484:Granat
5428:EXOSAT
5423:(1961)
5415:(2010)
5407:(2008)
5399:(1993)
5388:CXBN-2
5324:Astron
5319:(1995)
5294:(1990)
5230:(1964)
5203:ALEXIS
5111:LUVOIR
5061:EXCEDE
5028:(2035)
5020:(2035)
5017:Athena
5012:(2033)
5004:(2032)
4988:(2030)
4980:(2030)
4972:(2029)
4964:(2028)
4956:(2028)
4948:(2027)
4940:(2027)
4932:(2027)
4924:(2026)
4916:(2026)
4908:(2026)
4900:(2026)
4897:K-EUSO
4892:(2025)
4884:(2025)
4881:PETREL
4858:STEREO
4794:AMS-02
4757:XPoSat
4733:NuSTAR
4572:STEREO
4516:Hibari
4407:Hubble
4399:HiRISE
4375:Euclid
4367:DSCOVR
4359:CHEOPS
4236:STEREO
3985:
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3746:Forbes
3722:
3663:9 June
3658:Forbes
3634:
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3113:Cosmos
3060:. NASA
3020:
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2792:
2713:9 June
2683:4 June
2662:4 June
2286:. SLAC
2180:. NASA
2154:. NASA
2088:
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1947:. CERN
1891:. SLAC
1517:. Its
1169:Carina
1155:away.
1141:pulsar
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349:29.29Β°
335:Period
329:25.58Β°
274:Regime
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6446:April
6382:March
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6143:OSO J
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5973:OAO-B
5965:OAO-1
5946:TRACE
5891:Uhuru
5835:SAS-C
5827:SAS-B
5803:ROSAT
5740:OSO 8
5735:OSO 7
5730:OSO 6
5725:OSO 5
5720:OSO 4
5715:OSO 3
5710:OSO B
5705:OSO 1
5684:OAO-2
5636:LEGRI
5572:ILO-X
5468:Gamma
5460:GALEX
5412:EPOXI
5404:EPOCh
5372:Cos-B
5364:CoRoT
5299:BBXRT
5187:AGILE
5166:THEIA
5141:ORBIS
5091:ILO-1
5076:HabEx
5071:FOCAL
5046:Arcus
5009:Taiji
4969:ARIEL
4913:PLATO
4810:DAMPE
4802:CALET
4749:XRISM
4725:NICER
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4661:GECAM
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4621:DAMPE
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4556:SOLAR
4500:ASO-S
4463:Swift
4455:SOLAR
4351:CHASE
4342:BRITE
4297:SOLAR
3983:S2CID
3955:arXiv
3898:S2CID
3870:arXiv
3808:S2CID
3780:arXiv
3720:S2CID
3692:arXiv
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3604:arXiv
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3449:S2CID
3421:arXiv
3233:4 May
3179:S2CID
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3018:S2CID
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2006:S2CID
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6118:GEMS
6108:FAME
6096:EChO
6069:AOSO
6021:WIRE
5989:CXBN
5938:SWAS
5907:WMAP
5811:RXTE
5660:MOST
5612:IXAE
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5580:IRAS
5444:FUSE
5436:EUVE
5380:COBE
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5106:LUCI
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4471:TESS
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4252:Wind
4220:NCLE
4100:2018
4077:2016
4055:2018
4033:2017
3928:2016
3838:2016
3753:2018
3665:2016
3394:2023
3387:NASA
3277:2010
3235:2023
3209:2010
3171:PMID
3163:OSTI
3094:2010
3066:2018
3010:ISSN
2920:ISSN
2848:2019
2741:2007
2715:2008
2685:2008
2664:2008
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2565:2010
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2484:2010
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2208:2008
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2160:2017
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1927:2020
1897:2007
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1821:2016
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