Malesani (DARK/NBI), S. Sbarufatti (boris. Mangano (INAF-IASFPA), report on behalf of the Swift- XRT team: Swift began observation of the XRF detected by INTEGRAL (Paizis, et al. , GCN Circ. N. , GCN Circ. Sbarufatti, V. H. 528N) in Yunnan Province, China. inaf. Sbarufatti (INAF-OAB/IASFPA), V. 5 UT, 92. Palmer (LANL), M. Boris Sbarufatti at INAF-OAB/IASFPA <boris. In 3. it> P. D. The Swift-BAT trigger happened while the burst position in the sky was Moon constrained for. The XRT began observing the field at 2011-03-23 17:57:33 UT, that is T+340 ks ( 3. Sbarufatti, V. Beardmore (U Leicester), J. B. it> B. A. 6 ks [email protected] ks after the trigger. Sbarufatti (boris. Here’s how you knowDOI: 10. Physics Department University of Perugia, and I. Sbarufatti, V. 9 days) (Cummings, GCN Circ. 1 ks after the BAT trigger. Evans (U. Beardmore (U. Once the X-rays fade away, we hope to measure its mass and confirm its black hole status,” said Boris Sbarufatti from Brera Observatory in Milan, Italy, who currently. Cummings (GSFC), M. Osborne (U. Mangano (INAF-IASF PA) on behalf of the Swift XRT team Swift XRT started a ToO observation of the INTEGRAL burst GRB080120 at 19:47 UT. it> B. GCN Circ. Page (U. 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. GCN Circ. H. Leicester), K. Leicester), A. et al. sbarufatti@brera. Sbarufatti (boris. T. D'Ai (INAF-IASFPA), D. Sbarufatti (INAF-OAB/PSU), A. sbarufatti AT brera. inaf. Mangano (INAF/IASF_PA) and C. 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. it> B. A. The data comprise 185 s in Windowed Timing (WT) mode (the first 7 s were taken. inaf. Boris Sbarufatti at PSU <bxs60@psu. edu> B. B. , GCN 12063 ), observed from 138 ks to 425 ks after the Konus-Wind. A. Boris Sbarufatti at INAF-OAB/IASFPA <boris. 13 UT on 2023-08-21, is due to misidentification of a known source during a Star Tracker Loss-of-Lock. J. D Elia (ASDC), A. inaf. it> B. An official website of the United States government. Gehrels and Erik Andrew. it> B. 10968 ), from 96 s to 25. it> B. C. GCN Circ 7794) for three orbits which consisted of 200 s of Windowed Timing mode data starting 68 s after the trigger and 990. Kennea (PSU), A. 5 hours after the trigger. 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. Melandri (INAF-OAB) and B. Swenson (PSU) report on behalf of the Swift-XRT team: We have analysed 8. Table 2 - uploaded by Boris Sbarufatti. D. 4-3658}, author={Craig B. Leicester), A. Due to a Sun observing constraint, Swift cannot slew to the BAT position until 05:00 UT on 2011 April 11. R. Stroh (PSU), D. La Parola (INAF-IASF Pa) report on behalf of the Swift-XRT team The Swift XRT began observations of the INTEGRAL burst GRB 080603A (Paizis et al. sbarufatti AT brera. B. J. Download a PDF of the paper titled ESO-VLT optical spectroscopy of BL Lac objects: I. Sbarufatti (INAF-OAB) report on behalf of the Neil Gehrels Swift Observatory Team: Swift BAT trigger 1186391 at 15:25:12. it> D. Kennea (PSU), B. Boris Sbarufatti at INAF-IASF-Pa <[email protected] Sbarufatti at INAF-OAB/IASFPA <boris. Evans (U. Since 2006 I am member of the Swift team, where I contribute as Burst Advocate, XRT Burst Specialist, Observatory Duty Scientist, XRT Duty Scientist and Science Planner,. D. , GCN circ. 0 seconds after the BAT trigger. it> B. Pagani (U. D. An official website of the United States government. et al. De Pasquale (MSSL) report on behalf of the Swift Team. The source has faded with respect to the initial. sbarufatti AT brera. These topic labels come from the works of this person. 8 ks after the BAT trigger. B. T reves. (Sbarufatti et al. Sbarufatti (INAF-IASFPA), and S. Boris Sbarufatti, Martina Barattini. it> B. Mangano, V. K. D. 2017, GCN 21032 ). P. Sbarufatti, V. There will be no XRT or UVOT data until this time. Burst Advocate for this burst is B. inaf. Leicester) report on behalf of the Swift-XRT team Swift-XRT has performed follow up observations of GRB 210218A (Sbarufatti et al. 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. sbarufatti@brera. Osborne (U. Sbarufatti (1) and 18 other authors. Evans (U. C. 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. P. Nial Rahil Tanvir (CoI) (ESA Member) Prof. Sbarufatti (INAF-OAB/PSU), H. 4 ks. Siegel (PSU) report on behalf of the Swift team: Examination of the full BAT data set for Swift trigger 629693 (Siegel et al. Mangano (INAF-IASFPA) on behalf of the Swift-XRT team. Krimm (GSFC/USRA) The BAT data set from T-61 to T+302 sec from the recent telemetry. 16, 2012, resulted from a flood of gas. 0 ks to 196. Boris Sbarufatti at INAF-OAB/IASFPA <boris. inaf. The data are entirely in Photon. , GCN Circ. . Mangano (INAF IASF-PA), B. Leicester), A. Mangano, V. (GCN Circ. P. Copy reference. Download Table | Journal of Observations from publication: European Southern Observatory Very Large Telescope Optical Spectroscopy of BL Lacertae Objects. Leicester) report on behalf of the Swift-XRT team Swift-XRT has performed follow up observations of GRB 210218A (Sbarufatti et al. Mangano, B. A. Leicester) report on behalf of the Swift-XRT team: Swift-XRT has conducted further observations of the field of the Fermi/LAT. it> B. A. Boris Sbarufatti at INAF-IASF-Pa <sbarufatti@ifc. Boris Sbarufatti at INAF-IASF-Pa <[email protected] ks of XRT data for GRB 100727A (Morris et al. 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. La Parola (INAF-IASF Pa), T. Cummings (GSFC/UMBC), report on behalf of the Swift Team. Mingo (U. , Treves, A. Mangano (INAF IASF-Pa) report on behalf of the Swift-XRT team. Holland (CRESST/USRA/GSFC) report on behalf of the Swift XRT team: We have analysed the first two orbits of XRT data of GRB 070529 (Holland et al. 17385, Hurley et al. M. inaf. Sbarufatti, V. B. Beardmore (U. Sbarufatti (PSU), A. Our earliest-time LRIS images do not cover the position of the X-ray source reported by Sbarufatti et al. it> Boris Sbarufatti (INAF-OAB/PSU) reports on behalf of the Swift XRT team We have analysed 4. it> B. L. 8600,8602). The outburst, produced by a rare X-ray nova, announced the presence of a previously unknown stellar-mass black hole. D. Oates. 6560 ), consisting of 150 s in Window Timing. 7 ks after the BAT trigger. A. Boris Sbarufatti at INAF-IASF-Pa <[email protected], the position is marginally consistent with the known X. We report redshift measurements for 12 BL Lacertae objects from a program aimed at obtaining high signal-to-noise ratio (up to ∼500) optical spectroscopy. Sbarufatti, R. Morris (GWU/GSFC) report on behalf of the Swift-XRT team: We have analysed 9. Y. Dive into the research topics where Boris Sbarufatti is active. Leicester) report on behalf of the Swift-XRT team: Swift-XRT has performed follow-up observations of the Swift/BAT-detected burst. The XRT began observing the field at 2011-03-23 17:57:33 UT, that is T+340 ks ( 3. L. Y. 7 ks after the BAT trigger. A. Burrows (PSU), J. Download. T. inaf. Sbarufatti (INAF OAB/INAF IASF-PA) and C. Melandri (INAF-OAB), D. Leicester), P. from publication: European. Leicester) report on behalf of the Swift-XRT team: Swift-XRT has performed follow-up observations of the Fermi/GBM. inaf. Sbarufatti at this conference). 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. C. inaf. 9 ks of XRT data for the Swift/BAT-detected burst: GRB110319B (Cummings et al. H. E. P. L. 3 ks of XRT data for GRB 100725A (Markwardt et al. 7957) at 08:02 UT, 49 minutes after the trigger. Lien (GSFC/UMBC) and S. inaf. View publication. 9 ks after the Swift/BAT trigger. N. Page (U. sbarufatti@brera. Starling (CoI) (ESA Member) Prof. 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. 0 ks after the BAT trigger. inaf. inaf. 1. Copy caption. Burst Advocate for this burst is B. inaf. Page (U. Sbarufatti (INAF-OAB/IASFPA), V. Swift did not slew. 1 Similar Profiles; gamma ray bursts Physics & Astronomy 100%. L. 4 ks after the BAT trigger. Dr. A. 6466 ) with total exposure time of 3. Sbarufatti B. GCN Circ. Sbarufatti (INAF-OAB/IASFPA), R. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Download. The data consist of 642 s in. A. Kennea (PSU), B. Pagani (U. GCN Circ. 5 minutes. Boris Sbarufatti at INAF-OAB/IASFPA <boris. 18104), from 64 s to 40. it> B. V. 1 ks. 7197) and by Schady & Sbarufatti (GCN Circ. A. We report on Swift XRT observations of the field of the Fermi-LAT discovered GRB 170424A (N. sbarufatti@brera. Y. Mangano (INAF-IASF PA) report on behalf of the Swift-XRT team: We have analyzed the 3. Dr. P. Mangano (INAF-IASF PA) report on behalf of the Swift-XRT team: We have analyzed the 3. A. TITLE: GCN CIRCULAR NUMBER: 26048 SUBJECT: GRB 191019A: Swift-XRT updated analysis DATE: 19/10/20 20:12:27 GMT FROM: Boris Sbarufatti at PSU B. A. Rhaana L. , GCN Circ. it> B. Sbarufatti (PSU), A. (GCN 12067). 2006) it remains one of the f ew bright sour ces. Lien (GSFC/UMBC) and B. Bicocca & INAF-OAB) A. View publication. inaf. B. In this framework, initially proposed to explain GRBs with precursor activity, the prompt emission is produced by accretion of matter onto a newly–born magnetar, and. Amaral-Rogers et al. B. Cummings (GSFC/UMBC), N. In the XRT field of view we detect a single faint. Swiftimmediately slewed to GRB 090417B and narrow-field observations began observing 387 s (XRT) and 378 s (UVOT) after the BAT trigger. This distribution has a mean value of. Boris Sbarufatti at INAF-IASF-Pa <[email protected]@brera. Boris Sbarufatti at INAF-IASF-Pa <sbarufatti@ifc. Y. These. Mangano (PSU), M. 11813), from 27. 10968 ), from 96 s to 25. The data are entirely in. A. Copy caption. 6 ks to 14. inaf. Margutti (INAF-OAB), S. 41 ± 0. H. 1 Università dell'Insubria, via Valleggio 11, 22100 Como, Italy e-mail: boris. Stamatikos (NASA/ORAU) and D. Margutti (INAF-OAB), S. 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. J. 6 ks, with a 3. Sbarufatti (INAF-OAB/PSU), M. Mangano (INAF/IASF_PA) and C. Mangano (INAF/IASFPA) report on behalf of the Swift-XRT team: We have analyzed 4. Sbarufatti (INAF-OAB/IASFPA) and S. Sbarufatti (PSU) ), J. R. inaf. it> B. 4 ks after the BAT trigger. Burst Advocate for this burst is B. Sbarufatti (boris. Sbarufatti and 5 other. , Decarli, R. Boris Sbarufatti at INAF-OAB/IASFPA <boris. H. Sbarufatti, V. This redshift is consistent with the pre viously reported imaging redshift estimate from. it>. Sbarufatti (INAF-OAB/PSU), H. 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. Sbarufatti (INAF-OAB/IASFPA), J. In extremely urgent cases, after trying the Burst Advocate,. Sbarufatti, V. 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. Mangano (INAF-IASFPA) and J. (2005), we estimate a redshift z = 0. Boris Sbarufatti at INAF-OAB/IASFPA <boris. 1 ks. Swift immediately slewed to GRB 090417B and narrow-field observations began observing 387 s (XRT) and 378 s (UVOT) after the BAT trigger. A redshift of z 0. Boris Sbarufatti at INAF-OAB/IASFPA <boris. The BAT ground analysis using the data set from T-240 to T+962 s shows nothing. Burrows (PSU), B. , GCN Circ. 5}, author={Massimiliano de Pasquale and M. 10983), from 68 s to 58. inaf.