Beardmore (U. 1 Università dell'Insubria, via Valleggio 11, 22100 Como, Italy e-mail: boris. B. csv file with my fitbit activities for the past month. inaf. T. sbarufatti@brera. The data are entirely in. Boris Sbarufatti (CoI) (ESA Member) INAF - Osservatorio Astronomico di Brera Dr. Sbarufatti, V. de Pasquale (INAF-IASFPA), A. Swiftimmediately slewed to GRB 090417B and narrow-field observations began observing 387 s (XRT) and 378 s (UVOT) after the BAT trigger. A. 2 ks of Photon Counting. GCN Circ. La Parola, B. A. Sbarufatti, V. it> B. inaf. Table 3 - uploaded by Boris Sbarufatti. , Sbarufatti et al. Leicester), P. Download full-text PDF Read full-text. GCN Circ. Boris Sbarufatti at INAF-OAB/IASFPA <boris. P. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Of the two unknown sources reported by. it> B. The data comprise 1. Osborne (U. inaf. it> B. Content may be subject to copyright. The data are entirely in Photon Counting (PC. The spectrum reported by Chavushyan et al. Sbarufatti, V. Stroh (PSU), D. 7687). Fig 1 - uploaded by Boris Sbarufatti. 17398) between T+515. Page (U. 7 ks to 35. Burrows (PSU), J. Lien (GSFC/UMBC) and B. A. inaf. M. News; Events; Alumni; Faculty and Staff DirectoryTITLE: GCN CIRCULAR NUMBER: 28859 SUBJECT: GRB 201104A: Swift-XRT observations DATE: 20/11/06 17:46:49 GMT FROM: Boris Sbarufatti at PSU V. sbarufatti@brera. Leicester), A. These. Sbarufatti (INAF-OAB/IASFPA) and S. Stroh (PSU), D. , GCN circ. gamma radiation Earth & Environmental Sciences 81%. Beardmore (U Leicester), J. Sbarufatti (INAF OAB/IASF PA), V. K. Boris Sbarufatti at INAF-OAB/IASFPA <boris. it). NASA’s Swift satellite recently detected a rising tide of high-energy X-rays from a source toward the center of our Milky Way galaxy. Tohuvavohu (U Toronto) report on behalf of the Neil Gehrels Swift Observatory Team: At 13:32:56 UT, the Swift Burst Alert. Mangano (INAF IASF-PA), B. 8600,8602). Evans (U. DOI: 10. We have analyzed 14. Sbarufatti (INAF-OAB/IASFPA), S. 5 minutes. sbarufatti@brera. 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. it> S. 9603) comprising 6 ks in Photon Counting (PC) mode from T+16. D. Holland (GSFC/USRA), H. 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. inaf. it> B. The data consist of 240 s in Windowed Timing (WT) mode, starting 1603 seconds after the trigger followed. inaf. 0 ks after the BAT [email protected] ks of data of the ToO observation of GRB 080120, started on Jan 20 at 19:47 UT. A. 9 ks of XRT data for the Swift/BAT-detected burst: GRB110319B (Cummings et al. De Pasquale (MSSL) report on behalf of the Swift Team. 0 ks after the BAT trigger. Sbarufatti, V. it> B. Sbarufatti (INAF-OAB/PSU) report on behalf of the Swift Team: At 13:37:25 UT, the Swift Burst Alert Telescope (BAT) detected a peak in an image at a location near to the known. A. Y. A. GCN Circ. We report on Swift-XRT observations of GRB 081203B (Copete et al. H. D. it> B. III. 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. inaf. Oates (Uni. 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. These topic labels come from the works of this person. it> B. 9 ks of XRT data for GRB 101204A (Cummings et al. Evans (U. inaf. 4-3658 @article{Markwardt2011SwiftDA, title={Swift Detects a New Outburst of the Millisecond Accreting Pulsar SAX J1808. Leicester) report on behalf of the Swift-XRT team Swift-XRT has performed follow up observations of GRB 210218A (Sbarufatti et al. Please contact the BA by email if you require additional information regarding Swift followup of this burst. Sbarufatti (INAF-OAB/IASFPA) report on behalf of the Swift-XTR team We have analysed 4. inaf. sbarufatti@brera. Sbarufatti (PSU), K. it> S. 1086/519450 Corpus ID: 14317593; Swift Observations of GRB 070110: An Extraordinary X-Ray Afterglow Powered by the Central Engine @article{Troja2007SwiftOO, title={Swift Observations of GRB 070110: An Extraordinary X-Ray Afterglow Powered by the Central Engine}, author={Eleonora Troja and Gaspare. Evans (U. Om Sharan Salafia, Maria Edvige Ravasio, Sergio Campana, Paolo D’Avanzo, Boris Sbarufatti & Gianpiero Tagliaferri. GCN Circ. M. The data comprise 24 s in Windowed Timing (WT) mode with the. Once the X-rays fade away, we hope to measure its mass and confirm its black hole status,” said Boris Sbarufatti, an astrophysicist at Brera Observatory in Milan, Italy,. Evans (U. A. (GCN Circ. Leicester), A. Lien (GSFC/UMBC) and S. Mangano, V. 0 ks after the BAT trigger. Boris Sbarufatti at INAF-IASF-Pa <[email protected]. 9603) comprising 6 ks in Photon Counting (PC) mode from T+16. Aptekar, D. INFN - Sezione di Milano-Bicocca,. Name Institution Dr. Gehrels and Erik Andrew. inaf. inaf. J. E. ) has clearly shown that the host galaxies are massive and luminous ellipticals. inaf. Boris Sbarufatti at INAF-OAB/IASFPA <boris. 9 ks exposure. Cummings (GSFC/UMBC), N. Mangano (INAF/IASF_PA) and C. Kennea (PSU), N. P. Burrows (PSU), J. sbarufatti@brera. Of the two unknown sources reported by. Mangano (INAF/IASFPA) report on behalf of the Swift-XRT team: We have analyzed 4. Axelsson. Boris Sbarufatti at INAF-IASF-Pa <sbarufatti@ifc. edu> B. Strazzeri, O. 5 UT, 92. In 3. Boris Sbarufatti INAF, Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo, Via Ugo La Malfa 153, I-90146 Palermo, Italy E-mail: [email protected]> B. The data are entirely in Photon Counting (PC. Sbarufatti, V. it> S. The data comprise 235 s in Windowed Timing (WT). Baumgartner (GSFC/UMBC) The Swift-XRT began observing GRB 080506 (trigger=311159, Baumgartner et al. Sbarufatti, V. sbarufatti@brera. The. R. GCN Circ. 8600, 8602) 16. inaf. Melandri (INAF-OAB) and B. 6 ks to 14. De Pasquale (MSSL) report on behalf of the Swift Team. Sbarufatti, V. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Sbarufatti (PSU), A. Sbarufatti (INAF-OAB/PSU) and C. Beardmore (U. it> Sbarufatti B. 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. Evans (U. Filippenko (UC Berkeley) report that: The Katzman. 1 ks. E. Born in Chalkis, a small town near Athens, Greece, Sara Fortis never knew her father, who passed away when she was only two months old. afterglows. The Swift-BAT trigger happened while the burst position in the sky was Moon constrained for. 5 ks of Photon Counting data for GRB 110604A (Barthelmy et al. D'Avanzo (INAF-OAB), A. 10983), from 68 s to 58. it> B. GCN Circ. Amaral-Rogers (U. Boris Sbarufatti at INAF-OAB/IASFPA <boris. it> B. inaf. 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. L. The light curve shows an initial flare between. 11440), from 126. . An official website of the United States government. , GCN Circ. it> B. it> V. { "subject": "GRB 150202B: Swift/XRT afterglow confirmation", "bibcode": "2015GCN. La Parola (INAF-IASF PA) and W. ESO VLT optical spectroscopy of BL Lac objects. A. This is illustrated in. Boris Sbarufatti at INAF-IASF-Pa <sbarufatti@ifc. GCN Circ. An X-ray outburst caught by NASA’s Swift on Sept. 11813), from 27. 9 days) (Cummings, GCN Circ. Vanden Berk at PSU/Swift D. Page (U Leicester), [email protected]. Morris (GWU/GSFC) report on behalf of the Swift-XRT team: We have analysed 9. The Swift-BAT trigger happened while the burst position in the sky was Moon constrained for. Burrows (PSU), [email protected] Sbarufatti at INAF-OAB/IASFPA <boris. Boris Sbarufatti, Martina Barattini. Boris Sbarufatti (CoI) (ESA Member) INAF - Osservatorio Astronomico di Brera Dr. In the XRT field of view we detect a single faint. Leicester), J. et al. Boris Sbarufatti at INAF-IASF-Pa <[email protected] ks of XRT data for GRB 100727A (Morris et al. Massimiliano De Pasquale, Mathew J. Sbarufatti (INAF-OAB/IASFPA), J. 1K", "createdOn": 1598983743000, "circularId": 28341, "submitter": "Boris. F. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Mark Kennedy (CoI) (ESA Member). Download PDF. Burst Advocate for this burst is B. GCN Circ. GCN Circ. N. Boris Sbarufatti at INAF-OAB/IASFPA <boris. 11813), from 27. { "subject": "GRB 200901A: Swift-XRT refined Analysis", "bibcode": "2020GCN. A. Boris Sbarufatti at PSU <bxs60@psu. Here’s how you knowBoris Sbarufatti at INAF-IASF-Pa <[email protected] to main content Utility Menu. Melandri (INAF-OAB), B. Mangano, B. edu> B. 7195. Lara Nava, Ruben Salvaterra, Giancarlo Ghirlanda, Gabriele Ghisellini, Sergio Campana, Stefano Covino, Paolo D’Avanzo, Andrea Melandri, Boris Sbarufatti, Gianpiero. inaf. edu> B. Sbarufatti, V. 15029), from 53 s to 35. Mangano (INAF IASF-PA), B. Sbarufatti (INAF-OAB/PSU), M. In extremely urgent cases, after trying the Burst Advocate, you can contact the. Leicester), V. 5 ks of XRT data for GRB 100117A (De Pasquale et al. 29529). Mangano, V. Content may be subject to copyright. Swift took a second epoch of data for the LAT/IPN GRB 150202B (Axelsson et al. sbarufatti AT brera. Corpus ID: 115633452; Swift Detects a New Outburst of the Millisecond Accreting Pulsar SAX J1808. . B. GCN Circ. 9603) on 2009 July 2 at 14:15 UT, 3. Sbarufatti, B. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Melandri (INAF-OAB), V. The data are entirely in Photon Counting (PC) mode. Beardmore (U. GCN Circ. it> P. D'ai (INAF-IASFPA), A. Romano, C. Boris Sbarufatti at INAF-OAB/IASFPA <boris. 11944), from 2. Maselli (INAF-IASFPA), A. The refined position for the afterglow, obtained using the XRT-UVOT alignment and matching UVOT field sources to the USNO-B1 catalogue (see. 7828) started on 2008 May 05 at 23:49:36 UT, 97 s after the BAT trigger. Boris Sbarufatti at INAF-OAB/IASFPA <boris. it> Sbarufatti B. Mangano (INAF/IASFPA) report on behalf of the Swift-XRT team: We have analyzed 4. inaf. The data are entirely in Photon Counting (PC) mode, from T+806 s. We have analyzed 14. Y. , GCN Circ. Osborne (U. Cummings (GSFC), M. Sbarufatti (INAF-OAB/PSU) and C. Amaral-Rogers et al. Page, Silvia Zane, Alice A. Boris Sbarufatti at INAF-IASF-Pa <[email protected] ks to 35. The enhanced XRT position was given in Osborne et al. 3 ks of XRT data for GRB 100725A (Markwardt et al. Melandri (INAF-OAB), D. Lien (GSFC/UMBC) and B. GCN Circ. GCN 12064 table; GRB_name: GRB110604A: GCN_number: 12064: Detection_method: Konus-Wind Det: t_trigger: 14:49:45. edu> B. Beardmore (U. We derive here the intrinsic absorbing X–ray column densities of these GRBs making use of the Swift X–ray Telescope data. R. Sbarufatti at this conference). Leicester) and P. g. 6560 ), consisting of 150 s in Window Timing. 21822), from 63 s to 924 s after the BAT trigger. 3 ks after the BAT trigger. The data comprise 177 s in Windowed Timing (WT). La Parola (INAF-IASF Pa), T. A. it> B. P. inaf. 2009). R. it> B. { "subject": "BAT trigger 778435 is not a GRB. 5 ks to T+25. GCN Circ. D. An official website of the United States government. Oates (Uni. Holland1,2,3, Boris Sbarufatti4, Rongfeng Shens, Patricia Schady6, Jay R. Oates (Uni. Dr. Hello, today I imported a . Krimm (GSFC/USRA) The BAT data set from T-61 to T+302 sec from the recent telemetry. , GCN 12063 ), observed from 138 ks to 425 ks after the Konus-Wind. The XRT onboard Swift observed the field of GRB 090531A on 2009 June 10 and 2009 June 17, after it came outside the Moon observing contstraint, for a total exposure of 35. B. 17385, Hurley et al. Leicester) and D. De Pasquale (MSSL) report on behalf of the Swift Team. 2 ks exposure time. Sbarufatti (INAF-OAB/PSU), H. 17385, Hurley et al. Boris Sbarufatti at INAF-IASF-Pa <sbarufatti@ifc. Margutti (INAF-OAB), S. H. edu> B. 11525), from 339 s to 30. N. Sbarufatti (boris. Gropp (PSU), [email protected]. The data are entirely in [email protected]. Simpson (PSU) report on behalf of the Swift-XRT team: We have analyzed 8. A. D. Boris Sbarufatti at INAF-IASF-Pa <[email protected]> B. Sbarufatti (INAF-OAB/IASFPA), J. A. it> B. Boris Sbarufatti at PSU <[email protected] Sharan Salafia, Maria Edvige Ravasio, Sergio Campana, Paolo D’Avanzo, Boris Sbarufatti & Gianpiero Tagliaferri. D'Avanzo (INAF-OAB), J. Leicester), A. Melandri (INAF-OAB), K. inaf. Y.