1 ks. H. De Pasquale (MSSL) report on behalf of the Swift Team. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Boris Sbarufatti at INAF-IASF-Pa <[email protected] Sbarufatti at INAF-OAB/IASFPA <boris. Dr. 1 ks after the BAT trigger. A. Boris Sbarufatti Osservatorio astronomico di Brera: Milano, Lombardia, IT 2011-10-01 to 2017-07-31 | Post-Doc Employment Show more detail Source : Boris. Melandri (INAF-OAB), B. This image from Webb’s NIRCam (Near-Infrared Camera) instrument highlights GRB 230307A’s kilonova and its former home galaxy. Dive into the research topics where Boris Sbarufatti is active. Boris Sbarufatti, Martina Barattini. inaf. it> B. The enhanced XRT position was given in Osborne et al. Sbarufatti (INAF-OAB/PSU), P. Melandri (INAF-OAB), D. Sbarufatti, V. , GCN Circ. it> B. Credential Certification: Boris Sbarufatti (bxs60@psu. Sbarufatti (INAF OAB/INAF IASF-PA) and C. it> S. Evans (U. sbarufatti AT brera. The field of MMA began with the detection of neutrinos from the Sun and fromBoris Sbarufatti at INAF-IASF-Pa <[email protected]@brera. inaf. A. Sbarufatti, V. Sbarufatti, V. 9 ks to T+391. Boris. There will be no XRT or UVOT data until this time. Boris Sbarufatti at INAF-OAB/IASFPA <boris. The data comprise 8 s in Windowed Timing (WT) mode while Swift was slewing to the burst, 270 s in PC mode, a further 185 s in WT mode during a bright flare starting at T0+366 s (also seen in the BAT), with the. Bicocca & INAF-OAB) A. edu> B. D'Avanzo (INAF-OAB), V. it). Markwardt (CRESST/GSFC/UMD) report on behalf of the Swift-XRT team: We have analysed 4. The import was successful (after i edited the . 3 ks of XRT data for GRB 110915A (Holland et al. it> B. inaf. its mass and confirm its black hole status," said Boris Sbarufatti, an astrophysicist at Brera Observatory in Milan, Italy, who currently is working with other Swift team members at Penn State in. Swift immediately slewed to the target. J. , GCN Circ. it> B. Aarseth. Berger & Fox (2009) measured a redshift of z = 0. This page has only limited features, please log in for full [email protected] Sbarufatti at INAF-IASF-Pa <sbarufatti@ifc. . Giovanna Pugliese (CoI) (ESA Member) Universiteit van Amsterdam Jesse Palmerio. 29529). October 25, 2023 Source: NASA/Goddard Space Flight Center Summary: A team of scientists has used multiple space and ground-based telescopes to observe an. The BAT light curve showed a long period of emission starting 200 s before the trigger (see Figure 1). Leicester), A. , GCN 12063 ), observed from 138 ks to 425 ks after the Konus-Wind. 22007). A. The data are entirely in Photon Counting (PC. 11944), from 2. Lien (GSFC/UMBC), A. N. , Kotilainen, J. GCN Circ. U. Kennea (PSU), [email protected] peak count rate was ~7000 counts/sec (15-350 keV), at ~2 sec after the trigger. it). In extremely urgent cases, after trying the Burst Advocate,. 6 ks to 14. Sbarufatti, V. Siegel (PSU) report on behalf of the Swift team. Copy caption. inaf. Melandri (INAF-OAB) and B. Mangano, V. In extremely urgent cases, after trying the Burst Advocate, you can contact the Swift PI by phone. Melandri (INAF-OAB), D. The XRT began observing the field at 2011-03-23 17:57:33 UT, that is T+340 ks ( 3. III. Burst Advocate for this burst is B. The data are entirely in Photon Counting (PC. M. 9 ks of XRT data for the Swift/BAT-detected burst: GRB110319B (Cummings et [email protected]@inaf. Sbarufatti, V. Barthelmy (GSFC), T. Simpson (PSU) report on behalf of the Swift-XRT team: We have analyzed 8. Baumgartner (GSFC/UMBC) report on behalf of the Swift-XRT team: We have analysed 10 ks of XRT data for GRB 100725B (Baumgartner et al. F. 7828) started on 2008 May 05 at 23:49:36 UT, 97 s after the BAT trigger. Roegiers (PSU), L. Sbarufatti (PSU) report on behalf of the Neil Gehrels Swift Observatory Team: At 13:02:36 UT, the Swift Burst Alert Telescope (BAT) triggered and. Leicester), P. Sbarufatti (INAF-OAB/PSU), P. Boris Sbarufatti at INAF-IASF-Pa <sbarufatti@ifc. (2008) 1 . (2005), we estimate a redshift z = 0. Boris Sbarufatti at PSU <bxs60@psu. , Sbarufatti et al. Leicester), J. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Malesani (DARK/NBI) report on behalf of the Swift team A second epoch of observations on the ground discovered GRB 150204A (Cummings, GCN 17404 ) was performed by Swift from T+378. et al. A. Mangano, [email protected] Sbarufatti at INAF-OAB/IASFPA <boris. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Sbarufatti, V. ID Name Alt. M. Mangano (INAF-IASF Pa) report on behalf of the Swift-XRT team: Swift began observing the field of the Swift BAT Slew Survey (BATSS) GRB 081203B (Copete et al. Oates (MSSL) report on behalf of the Swift-XRT and Swift-UVOT teams We have analysed 4. Osborne (U. A. The XRT began observing the field at 2011-03-23 17:57:33 UT, that is T+340 ks ( 3. it> B. Mangano (INAF/IASF PA) and D. 3 ks to 32. Y. 11813), from 27. 6 ks in. Embed figure. Barthelmy (GSFC), P. McCauley (PSU), J. 6466 ) with total exposure time of 3. 26031), from 3. GCN Circ. Simpson (PSU) report on behalf of the Swift-XRT team: We have analyzed 8. Boris Sbarufatti at INAF-IASF-Pa <sbarufatti@ifc. 6 ks, with a 3. Cummings 1,3,7,. . GCN 7789 table; GRB_name: GRB080603A: GCN_number: 7789: Detection_method: Other: Circular_text: TITLE: GCN CIRCULAR NUMBER: 7789 SUBJECT: GRB 080603 OA candidate DATE: 08/06/03 12:02:13 GMT FROM: Ryan Chornock at UC Berkeley R. Vanden Berk at PSU/Swift D. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Sbarufatti et al. sbarufatti@brera. Leicester) and P. D. Lien (GSFC/UMBC) and S. inaf. 5 ks of Photon Counting data for GRB 110604A (Barthelmy et al. We have analyzed 14. The observation is in PC mode and consists of 1. GCN Circ. Proceedings of ScienceACCEPT & CONTINUE. The data comprise 9 s in Windowed Timing (WT) mode (taken while Swift was slewing. inaf. A. sbarufatti@brera. 5 @inproceedings{Pasquale2017GRB1R, title={GRB 130831A: Rise and demise of a magnetar at z = 0. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Evans (U. A. Evans ([email protected]> S. The data comprise 235 s in Windowed Timing (WT). A. it> V. We have analyzed 14. Boris Sbarufatti at INAF-IASF-Pa <sbarufatti@ifc. Boris Sbarufatti at INAF-OAB/IASFPA <boris. GCN Circ. Oates (MSSL) report on behalf of the Swift-XRT and Swift-UVOT teams We have analysed 4. La Parola (INAF-IASF Pa) report on behalf of the Swift-XRT team The XRT began observations of GRB 080605 (trigger=313299, Sbarufatti et al. Burst Advocate for this burst is B. inaf. L. it> B. 10968 ), from 96 s to 25. Siegel (PSU) report on behalf of the Swift-XRT team: We have analysed 15 ks of XRT data for GRB 150317A (Siegel et. A. , GCN Circ. Malesani (DARK/NBI) report on behalf of the Swift team A second epoch of observations on the ground discovered GRB 150204A (Cummings, GCN 17404 ) was performed by Swift from T+378. 7828) started on 2008 May 05 at 23:49:36 UT, 97 s after the BAT trigger. Pagani (U. We report on Swift-XRT observations of GRB 081203B (Copete et al. inaf. inaf. The best position for the X-ray afterglow is the XRT. This burst shows an uncommon drop in the X-ray light curve at about 100 ks after the trigger, with a decay slope of α 7. , GCN 7564) on 2008-04-07 at 04:25:49, ~43 hours after the trigger. Y. Gehrels and Erik Andrew. Boris Sbarufatti at INAF-OAB/IASFPA <boris. P. Using 1419 s of XRT Photon Counting mode data. it> B. Sbarufatti, V. Guidorzi (INAF OAB) and D. 18104), from 64 s to 40. GCN Circ. The data are entirely in [email protected]. Sbarufatti (INAF-OAB/IASFPA), S. A. Here’s how you knowA. Leicester), V. Sbarufatti (INAF-OAB/PSU) and M. Mangano (INAF-IASF PA) report on behalf of the Swift-XRT team: We have analyzed the 3. 8600,8602). Copy reference. The Swift-BAT trigger happened while the burst position in the sky was Moon constrained for. , GCN 7564) on 2008-04-07 at 04:25:49, ~43 hours after the trigger. it> Sbarufatti B. Sbarufatti, V. Burrows (PSU) report on behalf of the Swift XRT team. N. 5 ks of XRT data for GRB 191019a (Simpson et al. it> B. The BAT ground analysis using the data set from T-240 to T+962 s shows nothing. Boris Sbarufatti at INAF-OAB/IASFPA <boris. sbarufatti AT brera. Margutti (INAF-OAB), S. Tohuvavohu (U. sbarufatti AT brera. CO] pdf DOI cite claim. Leicester), A. ) has clearly shown that the host galaxies are massive and luminous ellipticals. Beardmore (U. Sbarufatti (PSU), K. 5 ks in Photon Counting mode. 4-3658}, author={Craig B. Sbarufatti (PSU), K. Table 1 - uploaded by Boris Sbarufatti. View publication. Download. Hello, today I imported a . Kennea (PSU), A. Hagen (PSU) report on behalf of the Swift team Swift performed a follow up observation of GRB 150418A, with a pointing in the direction of Source #1 reported by Sbarufatti et al. it> B. Astronomers have spotted a rare X-ray star explosion near the center of our Milky Way galaxy, revealing a previously unknown black hole munching on gas from a neighboring sun-like star. Y. Download. Sbarufatti (boris. Kennea (PSU), A. 6560 ), consisting of 150 s in Window Timing. 21822), from 63 s to 924 s after the BAT trigger. (GCN Circ. Boris Sbarufatti at INAF-IASF-Pa <[email protected] ks to 35. inaf. TITLE: GCN CIRCULAR NUMBER: 7195 SUBJECT: GRB080120: Swift XRT position DATE: 08/01/20 23:24:55 GMT FROM: Boris Sbarufatti at INAF-IASF-Pa B. D. Amaral-Rogers (U. inaf. In extremely urgent cases, after trying the Burst Advocate, you can contact the. The data consist of 642 s in. Mangano, B. it> B. The Swift-BAT trigger happened while the burst position in the sky was Moon constrained for. sbarufatti@brera. 9 days) (Cummings, GCN Circ. 11947) has not faded. it> B. inaf. , & Falomo, R. inaf. C. inaf. B. La Parola (INAF-IASF PA) and W. R. 4 ks after the BAT trigger. A. Perugia Section, Via A. Articles by Boris Sbarufatti on Muck Rack. Burst Advocate for this burst is B. Sbarufatti (INAF-OAB/IASFPA) reports on behalf of the Swift-XRT team: Swift performed a second target of opportunity observation of GRB 110319B on March 23, 2011. Table 2 - uploaded by Boris Sbarufatti. it> V. Leicester), V. Leicester), C. A. Markwardt (CRESST/GSFC/UMD) report on behalf of the Swift-XRT team: We have analysed 10 ks of XRT data for GRB 100724A (Markwardt et al. D. Leicester), K. Krimm (GSFC/USRA), M. 5 ks to T+25. GCN Circ. A. Evans (U. Sbarufatti, V. The relationships of the temporal variation of the model parameters to the synchronous time length and the synodic period are educed from the least square fitting model and the harmonic expressions. 10336), from 69 s to 18. H. Sbarufatti, V. Download PDF Abstract: Aims. 1 Similar Profiles; gamma ray bursts Physics & Astronomy 100%. The data are all in Photon Counting (PC) mode. The data comprise 8 s in Windowed Timing (WT) mode while Swift was slewing to the burst, 270 s in PC mode, a further 185 s in WT mode during a bright flare starting at T0+366 s (also seen in the BAT), with the. sbarufatti@brera. Received: 19 April 2006We present the analysis of the extraordinarily bright Gamma-Ray Burst (GRB) 130427A under the hypothesis that the GRB central engine is an accretion–powered magnetar. A. 5 UT, 92. Burrows, report on behalf of the Swift XRT team: We have analyzed the first 3 orbits of Swift-XRT data obtained for GRB 061126 (trigger=240766, GCN 5854). inaf. Sbarufatti (INAF-OAB/IASFPA) report on behalf of the Swift-XTR team We have analysed 4. (INAF-IASFPA), A. it> B. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Boris Sbarufatti at INAF-OAB/IASFPA <boris. directly from the image (Sbarufatti et al. Gropp (PSU), J. An official website of the United States government. (INAF-IASFPA) report on behalf of the Swift Team: We have analyzed the Swift-XRT data of XRF 090702 (Paizis, et al. 5 hours after the trigger. P. Mangano (INAF-IASFPA), report on behalf of the Swift- XRT team: Swift began observation of the XRF detected by INTEGRAL (Paizis, et al. Evans (U. Roma-BZCA T blazars in the P alermo BA T Survey B. The Neil–Gehrels Swift Observatory has added extensively to our understanding of small bodies in our solar system through its capabilities to rapidly respond to short-live events such as outbursts and collisions, through its near-ultraviolet coverage, and by its ability to track time-dependent changes through monitoring campaigns. Boris Sbarufatti at INAF-IASF-Pa <sbarufatti@ifc. new redshifts, by B. The data consist of 240 s in Windowed Timing (WT) mode, starting 1603 seconds after the trigger followed. Cummings (GSFC/UMBC), N. " by A. Leicester), K. De Pasquale (MSSL) report on behalf of the Swift Team. A. Ukwatta (GSFC/GWU) report on behalf of the Swift-XRT team: Swift-XRT began observing the field of GRB 081102 (trigger 333427, Ukwatta et al. Sbarufatti (INAF-OAB/IASFPA) and S. ] Renato Falomo; We present results of an ongoing program at the ESO VLT for spectroscopy of BL Lac objects lacking a firm redshift estimate. Sbarufatti (PSU), A. Authors: Marco Landoni, Renato Falomo, Aldo Treves, Boris Sbarufatti. Barthelmy (GSFC), [email protected] ks of Photon Counting data for GRB 110604A (Barthelmy et al. , GCN 17394 ) shows no evidence for detection of a source and only apparently random. inaf. Burrows (PSU), J. inaf. M. Here’s how you knowUsing Webb’s spectacular sensitivity, scientists captured the first mid-infrared spectrum from space of a kilonova, which marked Webb’s first direct look at an individual heavy element from such an event. Sbarufatti, V. Sbarufatti, V. GCN Circ. Boris Sbarufatti at PSU <bxs60@psu. Download a PDF of the paper titled ESO-VLT optical spectroscopy of BL Lac objects: I. Sbarufatti (INAF-OAB/IASFPA), R. A. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Boris Sbarufatti at INAF-OAB/IASFPA <boris. edu> B. Embed figure. B. GCN Circ. Mangano, V. INFN - Sezione di Milano-Bicocca, Piazza della Scienza 2, Milano (MI), Italy. , Mangano V. 2005b). Kennea (PSU), B. D. it> S. 1 Università dell'Insubria, via Valleggio 11, 22100 Como, Italy e-mail: boris. Breeveld, Samantha R.