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185 Feb 06, 2017

Fermi Gamma-ray Space Telescope identified the farthest gamma-ray blazars.

The detection of high-redshift (z>3) blazars by the Fermi Large Area Telescope (LAT) is of great astrophysical importance as they are extreme objects whose energetics remain a mystery.More importantly, high-z blazars tend to host massive black holes and can be used to constrain the space density of heavy black holes in the early Universe. The first detection with the LAT of five gamma-ray emitting blazars beyond z=3.3, has been announced and presented at the American Physical Society meeting in Washington in January 2017, and a paper describing the results has been submitted to The Astrophysical Journal Letters.

Light from the most distant object, NVSS J151002+570243 (z=4.31), began its journey to us when the universe was 1.4 billion years old. These objects have steeply falling gamma-ray spectral energy distributions and, those that have been observed in X-rays, a very hard X-ray spectrum, both typical of powerful blazars.Their Compton dominance (ratio of the inverse Compton to synchrotron peak luminosities) is also very large (> 20). All of these properties place these objects among the most extreme members of the blazar population. The radio-loudness may play a key role in rapid black hole growth in the early Universe. Fermi LAT could have detected just the tip of the iceberg, the first examples of a galaxy population that previously has not been detected in gamma rays

This research was led by researchers at the Clemson University, South Carolina, USA and at the ASI Space Science Data Center (SSDC), Rome, Italy, including D. Gasparrini (ASI SSDC and INFN). They began by searching for the most distant sources in a catalog of 1.4 million quasars, a galaxy class closely related to blazars. Because only the brightest sources can be detected at great cosmic distances, they then eliminated all but the brightest objects at radio wavelengths from the list. With a final sample of about 1,100 objects, the scientists then examined LAT data for all of them, resulting in the detection of five new gamma-ray blazars.

More details in the NASA's press release, ASI news, and in the forthcoming ApJ Letter.

185 Dec 30, 2016

50000 orbits of AGILE celebrated with the observation of an exceptional gamma-ray event

A few months before its tenth birthday in orbit, on December 19, 2016 at 06:08:53 UTC the AGILE satellite has reached the significant milestone of 50000 passes over the ASI Malindi Ground Station in Kenya with all detectors operating nominally.

AGILE is devoted to gamma-ray astrophysics, and it is also capable of detecting high energy phenomena of terrestrial nature, such as Terrestrial Gamma-ray Flashes (TGFs) revealed in the Earth equatorial regions. It is also currently at the forefront in the hunt for electromagnetic counterparts of gravitational waves.

The Italian satellite, launched on April 23, 2007 in low Earth orbit, is a small Scientific Mission of ASI, built and operated in cooperation with INAF, INFN, CIFS and with the participation of the Italian companies CGS, Thales-Alenia Space e Telespazio.

The small high-tech jewel, designed for an operative life of only two years, continues its mission with high efficiency, and it has celebrated its 50000 orbit with the observation of an exceptional gamma-ray event of extragalactic origin.



Credits: Screenshot downloaded on December 19, 2016 from the AGILEScience free app dedicated to the AGILE satellite.

As you can see from the fascinating image above, two monsters black holes at the center of the two distant active galactic nuclei CTA 102 and 3C 454.3, apparently close to each other in the AGILE sky map, made a spectacular double super-flare almost simultaneously in gamma rays.

The image was downloaded from the AGILEScience free app that enables anyone to follow in real time the latest satellite observations.

In particular, the CTA 102 source in these days was the brightest of the entire gamma-ray sky, even brighter than much closer sources within our galaxy, such as the Vela pulsar.

For more information, see also:
ASI news and INAF news (in Italian)
AGILE ATel #9743, ATel #9788, ATel #9840, ATel #9911 and references therein.

The AGILE data acquired from the ASI Malindi Ground Station are readily processed archived and managed by the SSDC/ASDC, the multi-mission ASI data center, and distributed to the PI Team alert system at INAF Bologna. The automatic alerts are analyzed daily by researchers of the AGILE team at several INAF institutes and at the ASDC itself.

185 May 02, 2016

The BeppoSAX X-Ray Astronomy Satellite (1996-2016): 20 years after the launch

The X-ray astronomy satellite BeppoSAX (Satellite per Astronomia X, "Beppo" in honor of Giuseppe Occhialini), is a project of the Italian Space Agency (ASI) with participation of the Netherlands Agency for Aerospace Programs (NIVR).

BeppoSAX was launched On 30 April 1996 and operated succesfully until 2002.

The main scientific characteristic of the BeppoSAX mission is the wide spectral coverage, ranging from 0.1 to over 200 keV, it was the first Italian satellite for the study of Astronomy High Energy.

In six years of operational life it has made 30.720 contacts with the Malindi ground station and has operated about 1.500 observations of different types of cosmic sources.

The most important result of the BeppoSAX Observatory was the discovery of the existence of the X-ray afterglows following Gamma Ray Burst (GRB) explosion. This major discovery earned Enrico Costa and other members of the BeppoSAX team several international recognitions including the "Enrico Fermi Award" 2010 (assigned to Enrico Costa and Filippo Frontera), the Descartes Prize of the European Union 2002 (shared among a group of scientists including Filippo Frontera, Enrico Costa, Luigi Piro and other members of the BeppoSAX team) and the Bruno Rossi Prize from the High Energy Astrophysics Division of the American Astronomical Society (awarded in 1998 to the BeppoSAX team and Jan van Paradijs).

The Archives of BeppoSAX data is available at the Center Scientific Data Italian Space Agency, ASI Science Data Center (ASDC), the multi-mission center founded in 2000 as an evolution of BeppoSAX SDC.

The BeppoSAX mission has inaugurated a new era for the High Energy Astrophysics, a field in which Italians have a long tradition of excellence.

For More details on BeppoSAX see:

The_BeppoSAX_Xray_Astronomy_satellite.pdf
The_BeppoSAX_publications_list.pdf

To commemorate this historic mission, the Italian Space Agency (ASI) organized on May 2, 2016 the event:

From the launch of Beppo-SAX today: twenty years of Italian successes in Space

185 Apr 06, 2016

An improved version of the ASDC 'Multi-Mission Interactive Archive for Space Science' tool is online!

The 'Multi-Mission Interactive Archive for Space Science' (MMIA2.0) is a new tool of the ASI Science Data Centre to explore its whole database. The ASDC is a repository of datasets from several space missions, exploring the Earth atmosphere, the Solar System and the Universe throughout the entire electromagnetic spectrum and other channels, such as the cosmic rays. MMIA2.0 is a user-friendly interface which allows scientists to access this all-encompassing and diverse databases. The tool has four main access tabs corresponding to the scientific topics supported at ASDC:

- Astrophysics and Cosmology. It groups all ASDC missions for the observation of the Universe. They are ordered according to the wavelengths/energies of their instruments, from Radio to Gamma-rays. Missions are selectable individually, in wavelength groups or in a specific spectral range. Observations of a single source or a sky region around a coordinate pairs can be retrieved (the default search radius is different for each selected mission).

- Exploration of the Solar System. This section provides links to the MATISSE tool by choosing the mission and the target. Once the user is on the MATISSE homepage the search can be performed by means of geographical (e.g. latitude/longitude) and geometrical (angle of observations) metadata to obtain both single- or multi-observation visualization.

- Particle Astrophysics/Cosmic Rays. It includes data from the only two magnetic spectrometers dedicated to charged cosmic rays research in space: PAMELA and AMS-02. Other experiments data will be added in the near future. Measurements of differential energy fluxes, time flux variations and solar flares, as well as fluxes of trapped particles in the Earth magnetosphere, and flux ratios are available in the database. The user can plot the data, download tables and graphs.

- Earth's Atmosphere/Terrestrial Gamma-ray Flashes. This is the newest ASDC tab. It currently gives access to data from Terrestrial Gamma-ray Flashes detected by the Minicalorimeter (MCAL) instrument on-board the AGILE satellite, and to light curves for the two TGF catalogs so far published by the AGILE Collaboration. Correlations with lightning and other Earth atmospheric parameters, and data from other missions will be included in MMIA2.0 in the near future.

The tool can be accessed from the ASDC main web page at www.asdc.asi or directly at www.asdc.asi.it/mma.html