Mar 18, 2023 | Gamma-ray rebrightening of the blazar PKS 0402-362 detected by AGILE New ATel issued: ATel #15952 (C. Pittori et al.). |
Mar 09, 2023 | GRB 230307A: AGILE/MCAL analysis New GCN issued: GCN #33444 (C. Casentini et al.). |
Mar 09, 2023 | GRB 230308A: AGILE/MCAL detection New GCN issued: GCN #33435 (C. Casentini et al.). |
Mar 07, 2023 | GRB 230307A: AGILE/MCAL detection New GCN issued: GCN #33412 (C. Casentini et al.). |
Feb 18, 2023 | GRB 230217A: AGILE/MCAL detection New GCN issued: GCN #33343 (C. Casentini et al.). |
Feb 15, 2023 | Gamma-ray activity of the blazar PKS 0402-362 detected by AGILE New ATel issued: ATel #15905 (A. Bulgarelli et al.). |
Feb 15, 2023 | GRB 230209B: AGILE detection New GCN issued: GCN #33325 (C. Casentini et al.). |
Feb 07, 2023 | GRB 230207B: AGILE detection of a burst New GCN issued: GCN #33296 (C. Casentini et al.). |
Feb 05, 2023 | GRB 230204B: AGILE detection New GCN issued: GCN #33272 (C. Casentini et al.). |
Jan 10, 2023 | AGILE detection of gamma-ray activity from blazar 4C 29.45 New ATel issued: ATel #15853 (A. Di Piano et al.). |
Jan 04, 2023 | GRB 230104A: AGILE/MCAL detection New GCN issued: GCN #33148 (A. Ursi et al.). |
Jan 02, 2023 | GRB 230102A: AGILE/MCAL detection New GCN issued: GCN #33138 (A. Ursi et al.). |
Dec 27, 2022 | GRB 221226A: AGILE detection New GCN issued: GCN #33113 (G. Panebianco et al.). |
Dec 22, 2022 | GRB 221221A: AGILE detection New GCN issued: GCN #33093 (C. Casentini et al.). |
Dic 21, 2022 | AGILE detection of increasing gamma-ray activity of blazar PKS 1424-418 New ATel issued: ATel #15818 (F. Verrecchia et al.). |
Nov 30, 2022 | AGILE detection of renewed Gamma-ray activity from 3C 454.3 New ATel issued: ATel #15782 (G. Panebianco et al.). |
Nov 28, 2022 | GRB 221126A: AGILE detection New GCN issued: GCN #32992 (C. Casentini et al.). |
Nov 19, 2022 | Ongoing gamma-ray flare from the PKS 0805-07 detected by AGILE New ATel issued: ATel #15768 (A. Bulgarelli et al.). |
Oct 29, 2022 | GRB 221028A: AGILE detection New GCN issued: GCN #32885 (A. Ursi et al.). |
Oct 29, 2022 | GRB 221027A: AGILE detection New GCN issued: GCN #32884 (A. Ursi et al.). |
Oct 26, 2022 | GRB 221023A: AGILE/GRID analysis New GCN issued: GCN #32856 (F. Verrecchia et al.). |
Oct 24, 2022 | GRB 221023A: AGILE detection of a burst New GCN issued: GCN #32825 (A. Ursi et al.). |
Oct 23, 2022 | GRB 221022B: AGILE detection New GCN issued: GCN #32822 (C. Casentini et al.). |
Oct 19, 2022 | AGILE detection of a burst from SGR J1935+2154 reported by VZLUSAT-2 New GCN issued: GCN #32801 (C. Casentini et al.). |
Oct 18, 2022 | AGILE detection of the 2022 October 17 burst from SGR J1935+2154 reported by Konus-Wind New GCN issued: GCN #32796 (F. Verrecchia et al.). |
Oct 18, 2022 | AGILE detection of short X-ray flaring activity contemporary to SGR J1935+2154 reported bursts New GCN issued: GCN #32789 (C. Casentini et al.). |
Oct 11, 2022 | GRB 221009A/Swift J1913.1+1946: AGILE-GRID detection New ATel issued: ATel #15662 (G. Piano et al.). |
Oct 10, 2022 | GRB 221009A (Swift J1913.1+1946): AGILE/GRID detection New GCN issued: GCN #32657 (A. Ursi et al.). |
Oct 10, 2022 | GRB 221009A (Swift J1913.1+1946): AGILE/MCAL detection New GCN issued: GCN #32650 (A. Ursi et al.). |
Sep 22, 2022 | SSDC Solar System group at EPSC 2022 This week Edoardo Rognini and Veronica Camplone are at the European Planetary Science Congress in Granada, Spain, with the work "Mercury exploration with MATISSE tool". The combination of a thermophysical model and the capability of selecting data basing upon geological maps, makes MATISSE a very powerful tool for the study of the first planet of the solar system. A capability that would become crucial with the ESA-JAXA BepiColombo mission approximating its scientific phase. |
Sep 10, 2022 | GRB 220910A: AGILE detection New GCN issued: GCN #32540 (A. Ursi et al.). |
Jul 31, 2022 | Gamma-ray rebrightening of the blazar PKS 1424-418 detected by AGILE New ATel issued: ATel #15533 (F. Verrecchia et al.). |
Jul 25, 2022 | Ongoing gamma-ray flare from the blazar PKS 1424-418 detected by AGILE New ATel issued: ATel #15527 (G. Piano et al.). |
Jul 22, 2022 | AGILE news AGILE, PUBLISHED THE FIRST ARTICLE ABOUT THE "NEW YEAR'S BURST" The first article about the GRB 220101A, the exceptionally energetic "New Year's Burst", has been published by AGILE on July, 15, 2022 (Ursi et al., ApJ 933, 2022). Few hours after the midnight of January 1, 2022, several satellites devoted to high-energy astrophysics, including AGILE had greeted the beginning of the new year by revealing what is probably the most energetic Gamma-Ray Burst (GRB) ever reported in the history of the observations of these phenomena, i.e., the GRB 220101A. In its 15 years activity, AGILE has already had the opportunity to reveal some particularly intense GRBs, such as the GRB 080916C and the GRB 160625B, but these events are quite rare. GRB 220101A took place more than 12 billion light years away, at the time when the Universe was just about 1.3 billion years old, and its equivalent isotropic energy is the highest ever reconstructed for a GRB. This record-breaking energy has drawn a great deal of attention from the scientific community in a short time. In the following days, more than twenty GCN communications were released, reporting observations carried out by other space missions and by astronomical ground-based observatories. AGILE data provide a first characterization of the prompt phase of this GRB, which corresponds to the emission of high-energy radiation in the initial shocks taking place within the central engine. The different detectors onboard the satellite, whose energy coverage ranges from the X-ray (SuperAGILE 20-60 keV) to the gamma-ray (AGILE-MCAL 0.4-100 MeV) band, allowed to provide a first comprehensive overview of the temporal evolution and the energetics of this event. Using AGILE data together with public data from the Swift satellite, it was also possible to study also the so-called "afterglow" emission, that is, the delayed emission at lower energies, produced by the interactions of the initial shocks with the surrounding interstellar medium. This analysis allows to obtain interesting information regarding the environment in which such energetic event took place. NEW AGILE TGF CATALOG UPDATE UP TO DECEMBER 31, 2021 AGILE confirms itself as an exceptional instrument, not only for the observation of cosmic phenomena, but it continues to give fundamental contribution also for the observation of high-energy phenomena from the Earth, such as the Terrestrial Gamma-Ray Flashes (TGFs) (A. Lindanger et al. 2020; C. Maiorana et al. 20209). Recently all TGFs seen by AGILE up to 31 December 2021 have been published as an interacting SSDC web page, including details and additional information compared to the original publications of the third TGF catalog in 2020. Additional links: ASI news (in Italian): https://www.asi.it/2022/07/agile-pubblicato-il-primo-studio-sul-grb-di-capodanno/ ASI news (in English): https://www.asi.it/en/2022/07/agile-published-the-first-article-about-the-new-years-burst/ |
Jul 15, 2022 | GRB 220715A: AGILE/MCAL detection New GCN issued: GCN #32401 (A. Ursi et al.). |
Jun 30, 2022 | GRB 220624A: AGILE/GRID refined analysis New GCN issued: GCN #32303 (F. Verrecchia et al.). |
Jun 24, 2022 | GRB 220624A: AGILE/GRID analysis New GCN issued: GCN #32261 (F. Verrecchia et al.). |
Jun 24, 2022 | GRB 220624A: AGILE detection New GCN issued: GCN #32259 (A. Ursi et al.). |
Jun 23, 2022 | GRB 220623A: AGILE detection New GCN issued: GCN #32247 (A. Ursi et al.). |
Jun 06, 2022 | Paper about SSDC activities for LICIACube published A paper describing the role of SSDC in the LICIACube mission has been recently published on the Planetary Science Journal. Led by Angelo Zinzi, coordinator of Solar System Exploration activities in SSDC, the paper focuses on the preparation of the mission Science Operations Center (SOC), hosted and managed by SSDC. The LICIACube SOC is in charge of processing and archiving the data. Raw images will be calibrated using algorithms developed by INAF. Both raw and calibrated images will be archived following the PDS4 standard, so that, after the proprietary period lasting 9 months from the DART impact on Dimorphos, they can be publicly released straightaway. The paper also describes how the SSDC MATISSE webtool is being adapted to fully exploit LICIACube images, main changes including new geological functionalities and a new thermophysical model, best suited for small, rubble-pile asteroids. |
May 27, 2022 | GRB 220527A: AGILE detection New GCN issued: GCN #32129 (A. Ursi et al.). |
May 11, 2022 | GRB 220511A: AGILE detection New GCN issued: GCN #32021 (A. Ursi et al.). |
Apr 30, 2022 | GRB 220430A: AGILE detection New GCN issued: GCN #31975 (A. Ursi et al.). |
Apr 23, 2022 | GRB 220423A: AGILE detection New GCN issued: GCN #31938 (A. Ursi et al.). We notice that today, April 23rd 2022, is the 15th anniversary of the AGILE launch. The AGILE instrument has been flawlessly operating in orbit since then. We take this opportunity to thank ASI, the AGILE scientific Team and the ground segment team for their committment to the excellence of the mission (GCN #31939 , M. Tavani et al.). |
Apr 06, 2022 | AGILE confirmation of the gamma-ray flaring activity from the FSRQ 3C 345 New ATel issued: ATel #15314 (F. Verrecchia et al.). |
Mar 23, 2022 | GRB 220323A: AGILE/MCAL detection New GCN issued: GCN #31784 (A. Ursi et al.). |
Mar 10, 2022 | GRB 220308A: AGILE detection New GCN issued: GCN #31733 (A. Ursi et al.). |
Mar 09, 2022 | Mercury NASA MESSENGER's images on MATISSE Last week an update on the MATISSE webtool, made it possible to search and retrieve calibrated images from the NASA MESSENGER MDIS-NAC camera using the NASA ODE REST protocol. This is a crucial addition, taken into account the thermophysical model already available for Mercury and the work on the geological units planned to be released in the next months. All these new functionalities could be of major interest for the study of Mercury, in preparation for the ESA-JAXA BepiColombo mission, presently on its way to starting orbiting the planet in 2025, making MATISSE a useful tool for data exploitation. |