inaf. inaf. M. 10979), from 82 s to [email protected]. GCN Circ. Leicester) and P. Kennea (PSU), A. Sbarufatti (INAF-OAB/IASFPA), V. sbarufatti@brera. Sbarufatti (INAF-IASFPA), S. 4 ks, with a 1. The enhanced XRT position was given in Osborne et al. D. GCN Circ. F. 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. 0 ks after the BAT trigger. , GCN Circ 9461) at 19:26:22 UT, 3026 seconds after the BAT trigger, as soon as the burst went. , & Falomo, R. We report on Swift-XRT observations of GRB 081203B (Copete et al. Barun was a naughty child. Burst Advocate for this burst is B. Melandri (INAF-OAB), V. A. Sbarufatti (boris. We report the observations for the GRB191122A (B. Evans (U. Sbarufatti (INAF-OAB/IASFPA), J. 15029), from 53 s to 35. ESO VLT optical spectrum of RBS 1915, a X-ray selected BL Lac object. GCN Circ. sbarufatti AT brera. Page (U Leicester), [email protected]. it> B. Boris Sbarufatti at INAF-IASF-Pa <[email protected] Sbarufatti at INAF-OAB/IASFPA <boris. Here’s how you knowBoris Sbarufatti at INAF-IASF-Pa <[email protected] to main content Utility Menu. inaf. Beardmore (U Leicester), J. 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. inaf. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Mangano, B. , GCN circ. 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. Sbarufatti (INAF-OAB/PSU), P. N. , GCN [email protected] Sbarufatti at INAF-OAB/IASFPA <[email protected] is concluded that, if the X-ray source is physically associated with the optical-UV transient, then ASASSN-15lh most likely represents the tidal disruption of a main-sequence star by the most massive spinning black hole detected to date. Sbarufatti (boris. La Parola, V. inaf. Mangano (INAF IASF-Pa) report on behalf of the Swift-XRT team. Baumgartner (GSFC/UMBC) The Swift-XRT began observing GRB 080506 (trigger=311159, Baumgartner et al. Copy reference. 29529). 12335), from 82 s to 7. it> B. N. All content in this area was uploaded by Boris Sbarufatti. Evans (U. Melandri (INAF-OAB), D. Kennea (PSU), B. Breeveld, Samantha R. Kuin (UCL-MSSL), S Laha (GSFC/UMBC/CRESST) and A. Together they form a unique fingerprint. A. An extension of the sample, by B. P. Melandri (INAF-OAB), B. De Pasquale (MSSL) report on behalf of the Swift Team. 4-3658}, author={Craig B. The source has faded with respect to the initial. Mangano (INAF IASF-Pa), C. L. 1 ks. inaf. Proceedings of ScienceACCEPT & CONTINUE. Evans (U. sbarufatti@brera. , GCN Circ. D'Avanzo (INAF-OAB), V. inaf. Mangano (INAF/IASFPA) report on behalf of the Swift XRT team: Further observations of the field of GRB 110420B (Sbarufatti et al. Content may be subject to copyright. 10998), from 48 s to 39. Download. N. From: Boris Sbarufatti [v1] Thu, 28 Oct 2004 11:39:10 UTC (112 KB) Full-text links: Access Paper: Download a PDF of the paper titled ESO-VLT optical spectroscopy of BL Lac objects: I. Sbarufatti, V. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Sbarufatti (PSU), K. Perley, W. Y. Sbarufatti (INAF-OAB/IASFPA) and V. Sbarufatti (PSU), K. Boris Sbarufatti at INAF-OAB/IASFPA <boris. sbarufatti@brera. Sbarufatti (INAF/OAB-IASF Pa) reports on behalf of the Swift-XRT team: We have analysed 24 ks of XRT data for GRB 101204A (Cummings et al. GCN Circ. inaf. (INAF-IASFPA) report on behalf of the Swift Team: We have analyzed the Swift-XRT data of XRF 090702 (Paizis, et al. 6 ks in. 2 ks and T+516. , GCN Circ. Embed figure. 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. inaf. Find Boris Sbarufatti's email address, contact information, LinkedIn, Twitter, other social media and more. 2 ks of XRT data for GRB 130518B (Cummings GCN Circ. GCN Circ. GCN Circ. Siegel (PSU) report on behalf of the Swift team. (INAF-IASFPA), A. Content may be subject to copyright. 8600, 8602) 16. T. Sbarufatti (1) and 18 other authors. it> Sbarufatti B. it> B. Sbarufatti (INAF-OAB/PSU), P. A. The data consist of 240 s in Windowed Timing (WT) mode, starting 1603 seconds after the trigger followed. Sbarufatti (INAF-IASFPA), P. Mangano (INAF-IASF PA) report on behalf of the Swift-XRT team: We have analyzed the 3. Simpson (PSU) report on behalf of the Swift-XRT team: We have analyzed 8. Authors: Marco Landoni, Renato Falomo, Aldo Treves, Boris Sbarufatti. , GCN 17394 ) shows no evidence for detection of a source and only apparently random. 12335), from 82 s to 7. Siegel (PSU) report on behalf of the Swift-XRT team: We have analysed 15 ks of XRT data for GRB. Boris Sbarufatti at INAF-OAB/IASFPA <boris. inaf. 5 ks of XRT data for GRB 191019a (Simpson et al. Krimm (NSF), N. inaf. 3 ks to 32. Sbarufatti (INAF-IASF PA) report on behalf of the Swift-XRT team: The Swift-XRT observed GRB 080603B (trigger 313087, Mangano et al. La Parola, B. 6 ks in. Leicester), J. Here’s how you knowA. An official website of the United States government. Boris Sbarufatti at INAF-OAB/IASFPA <boris. 9905). A. 10983), from 68 s to 58. Evans ([email protected]> S. inaf. sample objects are given in Sbarufatti et al. Sbarufatti (boris. Burst Advocate for this burst is. , Treves, A. H. Holland 1,2,3, Boris Sbarufatti 4, Rongfeng Shen 5, Patricia Schady 6, Jay R. T. Sbarufatti (INAF-OAB/IASFPA), R. inaf. Here’s how you knowDOI: 10. The data are entirely in Photon Counting (PC. P. Gehrels and Erik Andrew. , GCN Circ. Siegel (PSU) report on behalf of the Swift-XRT team: We have analysed 15 ks of XRT data for GRB 150317A (Siegel et. T. 3 ks after the BAT trigger. Leicester) and P. In 3. Sbarufatti (INAF-OAB/IASFPA) report on behalf of the Swift-XTR team We have analysed 4. Hello, today I imported a . { "subject": "BAT trigger 778435 is not a GRB. 11944), from 2. inaf. E. csv file deleting the 1st line) but nothing (steps, sleep, etc. sbarufatti@brera. It was optically dark and has been associated with a bright star-forming galaxy at a redshift of. Copy caption. Boris Sbarufatti at INAF-IASF-Pa <[email protected] Sbarufatti at INAF-OAB/IASFPA <boris. We have analyzed 14. 14862), from 184. D. Gropp (PSU) and P. N. 21822), from 63 s to 924 s after the BAT trigger. it). edu> B. it> B. Cummings 1,3,7,. There will be no XRT or UVOT data until this time. Marshall (NASA/GSFC), A. De Pasquale (MSSL) report on behalf of the Swift Team. Sbarufatti (INAF-IASFPA), and S. it> B. 7687). inaf. Beardmore (U Leicester), J. These topic labels come from the works of this person. D'ai (INAF-IASFPA), A. 1. inaf. 2 ks of Photon Counting mode data for this burst, covering times from T+17 ks to T+ 47 ks. 9 ks exposure. R. 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. The Swift-BAT trigger happened while the burst position in the sky was Moon constrained for. Kuin (UCL-MSSL), A. 11813), from 27. inaf. D. 6 ks [email protected] ks after the trigger. 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. Beardmore (U. inaf. D Elia (ASDC), A. inaf. T reves. inaf. GCN Circ. Evans (U. K. Barthelmy (GSFC), P. Boris Sbarufatti at INAF-IASF-Pa <sbarufatti@ifc. sbarufatti AT brera. Palmer (LANL) report on behalf of the Swift-XRT team: We have analysed 6. Boris Sbarufatti at INAF-OAB/IASFPA <boris. 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. Burrows's 797 research works with 17,426 citations and 9,283 reads, including: Swift-XRT follow-up of gravitational wave triggers during the third aLIGO/Virgo observing run///// TITLE: GCN CIRCULAR NUMBER: 26346 SUBJECT: GRB 191130A: Swift-XRT observations DATE: 19/12/05 17:22:42 GMT FROM: Boris Sbarufatti at PSU B. 3 ks after the BAT trigger. inaf. Copy reference. News; Events; Alumni; Faculty and Staff Directory; Utility Menu. 9 ks after the Swift/BAT trigger. Maselli (INAF-IASFPA), A. Sbarufatti (INAF-OAB/IASFPA), S. Boris Sbarufatti (CoI) (ESA Member) Dr. III. 9 ks after the Swift/BAT trigger. 1142/9789813226609_0375 Corpus ID: 125637366; GRB 130831A: Rise and demise of a magnetar at z = 0. Boris Sbarufatti at INAF-OAB/IASFPA <boris. 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. D'Avanzo (INAF-OAB), J. T. Sbarufatti (INAF-OAB/PSU), M. In the XRT field of view we detect a single faint. Mangano (INAF/IASFPA) report on behalf of the Swift-XRT team: We have analyzed 4. The data comprise 235 s in Windowed Timing (WT). The data comprise 185 s in Windowed Timing (WT) mode (the first 7 s were taken. 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. We analyzed 3. Barthelmy (GSFC), P. B. A. A. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Leicester), V. H. sbarufatti@brera. The Astronomical Observatory of Brera; Show all 7 authors Hide. C. B. Please contact the BA by email if you require additional information regarding Swift followup of this burst. sbarufatti@brera. N. inaf. C. , GCN Circ. Sbarufatti (INAF-OAB/IASFPA) and S. " by A. 7198). B. Burrows (PSU), J. A. Ukwatta (GSFC/GWU) report on behalf of the Swift Team: We have analyzed the first 22. Melandri (INAF-OAB), D. it> P. 2 ks of XRT data for GRB 130725B (Swenson et al. Barthelmy (GSFC), P. Sbarufatti (INAF OAB/INAF IASF-PA) and C. Sbarufatti (INAF OAB/INAF IASF-PA) and C. C. GCN Circ. Boris Sbarufatti at INAF-IASF-Pa <sbarufatti@ifc. Sbarufatti (INAF-OAB/PSU), A. A. inaf. P. Burrows (PSU) report on behalf of the Swift XRT team. Swift-XRT performed further observations on the afterglow candidate announced in Sbarufatti et al. 7957) at 08:02 UT, 49 minutes after the trigger. Tohuvavohu (U Toronto) report on behalf of the Neil Gehrels Swift Observatory Team: At 13:32:56 UT, the Swift Burst Alert. Boris Sbarufatti (CoI) (ESA Member) INAF - Osservatorio Astronomico di Brera JWST Proposal 2344 (Created: Tuesday, June 13, 2023 at 2:00:38 AM Eastern Standard Time) - Overview 1. Sbarufatti (INAF OAB/INAF IASF-PA) and W. Raffaella MARGUTTI | Cited by 12,897 | of Harvard-Smithsonian Center for Astrophysics, Cambridge | Read 383 publications | Contact Raffaella MARGUTTIBoris Sbarufatti at INAF-OAB/IASFPA <boris. Kennea (PSU), A. Sbarufatti T able 1: Roma-BZCA T blazars detected in the BA T surve y . Leicester) report on behalf of the Swift-XRT team Swift-XRT has performed follow up observations of GRB 210218A (Sbarufatti et al. The enhanced XRT position was given in Osborne et al. The data comprise 9 s in Windowed Timing (WT) mode (taken while Swift was slewing. Sbarufatti (INAF-OAB/PSU) and D. 4 ks after the BAT trigger. Boris Sbarufatti. Sbarufatti (INAF-OAB/PSU), M. 17398) between T+515. La Parola (INAF-IASFPA), S. it> B. sbarufatti AT brera. Sbarufatti (INAF-OAB/IASFPA), J. 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. Sbarufatti (INAF-OAB/IASFPA) reports on behalf of the Swift-XRT team: We have analysed 6. H. (GCN 12067). Dr. Strazzeri, O. sbarufatti@brera. The XRT began observing the field at 2011-03-23 17:57:33 UT, that is T+340 ks ( 3. inaf. edu> B. (GCN Circ. Golenetskii, R. 11944) have shown that the X-ray source reported by Sbarufatti et al. A. Berger & Fox (2009) measured a redshift of z = 0. Mangano (INAF/IASF Pa), B. 10968 ), from 96 s to 25. Leicester), J. Melandri (INAF-OAB), D. FRB 20121102A: images of the bursts and the varying radio counterpart. GCN Circ. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Mangano, [email protected] Sbarufatti at INAF-OAB/IASFPA <boris. Evans (U. The data are entirely in [email protected]. Barthelmy (GSFC), [email protected] ks of Photon Counting data for GRB 110604A (Barthelmy et al. D. We have analysed 12 ks of XRT data for GRB 150801B (Sbarufatti et al. Sbarufatti and 5 other authors. N. inaf. Pagani (U. it> B. inaf. Stroh (PSU), D. 22007). An X-ray outburst caught by NASA’s Swift on Sept. Melandri (INAF. P. 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. (Feb 11, 2013) Published in: Astron. Embed figure. V. Burst Advocate for this burst is. it> B. 10979), from 82 s to 11. de Pasquale (INAF-IASFPA), A. 5 UT, 92. Mangano, V. Krimm (GSFC/USRA) The BAT data set from T-61 to T+302 sec from the recent telemetry. Y. Boris Sbarufatti Osservatorio astronomico di Brera: Milano, Lombardia, IT 2011-10-01 to 2017-07-31 | Post-Doc Employment Show more detail Source : Boris. it> B. Sbarufatti (INAF-OAB/IASFPA), R. Vanden Berk at PSU/Swift D. , GCN Circ 7790) on June 3, 14:11 UT, 173 minutes after the trigger. The data are entirely in Photon Counting (PC) mode. N. Barun Sobti’s childhood image. Sbarufatti (INAF OAB/INAF IASF-PA) , V. 11947) has not faded. Perugia Section, Via A. Please contact the BA by email if you require additional information regarding Swift followup of this burst. it> Boris Sbarufatti (INAF-OAB/PSU) reports on behalf of the Swift XRT team We have analysed 4. Sbarufatti (INAF-OAB/IASFPA) report on behalf of the Swift-XTR team We have analysed 4. it> B. Evans (U. H. We report on Swift-XRT observations of GRB 081203B (Copete et al. 17385, Hurley et al. D. , Mangano V. Axelsson. Guidorzi (INAF OAB) and D. N. 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, who currently is working. Leicester), A. M. McCauley (PSU), J. Together they form a unique [email protected]@brera. sbarufatti@brera. 9 days) (Cummings, GCN Circ. Mangano (INAF/IASF PA) and D. 7685) in Window Timing mode, 146 s after the BAT trigger. 2002) and the possible host galaxy of GRB 090417B. ] Renato Falomo; We present results of an ongoing program at the ESO VLT for spectroscopy of BL Lac objects lacking a firm redshift estimate. Johan P. , GCN 12063 ), observed from 138 ks to 425 ks after the Konus-Wind.