D. Content may be subject to copyright. Sbarufatti (INAF-OAB/IASFPA) reports on behalf of the Swift-XRT team: We have analysed 6. The Swift-BAT trigger happened while the burst position in the sky was Moon constrained for. Axelsson. , GCN Circ. 3 ks of XRT data for GRB 100725A (Markwardt et al. it> B. 17722). Sbarufatti (INAF-OAB/IASFPA) reports on behalf of the Swift-XRT team: We have analysed 6. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Mangano (INAF/IASF PA) and D. Cummings (GSFC), M. it> B. Mangano (INAF/IASFPA) report on behalf of the Swift-XRT team: We have analyzed 4. Burrows (PSU) and P. GCN Circ. P. Sbarufatti (PSU) report on behalf of. Boris Sbarufatti at INAF-OAB/IASFPA <boris. A. arXiv:astro-ph/0508200v1 9 Aug 2005. News; Events; Alumni; Faculty and Staff Directory; Utility Menu. inaf. it> B. Evans (U. La Parola, B. B. Boris Sbarufatti at INAF-IASF-Pa <[email protected] ks of XRT data for GRB 100727A (Morris et al. 7195. it> B. Burrows (PSU), J. Sbarufatti, R. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Sbarufatti, V. H. Sbarufatti (PSU), A. sbarufatti AT brera. 4 ks, with a 1. Mangano (INAF/IASF_PA) and C. Boris Sbarufatti at INAF-IASF-Pa <[email protected] ks of XRT data for GRB 100727A (Morris et al. 10336), from 69 s to 18. 2 ks of XRT data for GRB 130725B (Swenson et al. 8462) at 17:46:11. 11525), from 339 s to 30. 10968 ), from 96 s to 25. H. A. 8 ks after the BAT trigger. Barthelmy (GSFC) report on behalf of the Swift team: UVOT took a finding chart exposure of 100. (INAF-IASFPA) report on behalf of the Swift Team: We have analyzed the Swift-XRT data of XRF 090702 (Paizis, et al. D. D'Avanzo (INAF-OAB) and P. (INAF-IASFPA) report on behalf of the Swift Team: We have analysed the first six orbits of Swift-XRT data obtained from GRB 090417B (trigger 349450; Sbarufatti, et al. Boris Sbarufatti at INAF-OAB/IASFPA <boris. The data comprise 235 s in Windowed Timing (WT). D Elia (ASDC), A. Melandri (INAF-OAB), D. Swift did not slew. Leicester), V. 5 UT, 92. A. Tohuvavohu (U Toronto) report on behalf of the Neil Gehrels Swift Observatory Team: At 13:32:56 UT, the Swift Burst Alert. Page (U. GCN Circ. Download. , GCN 12063 ), observed from 138 ks to 425 ks after the Konus-Wind. Boris Sbarufatti (CoI) (ESA Member) INAF - Osservatorio Astronomico di Brera Dr. ) has clearly shown that the host galaxies are massive and luminous ellipticals. C. Perley, W. 21822), from 63 s to 924 s after the BAT trigger. directly from the image (Sbarufatti et al. TITLE: GCN CIRCULAR NUMBER: 28307 SUBJECT: GRB 200829A: Swift detection of a burst with an optical afterglow DATE: 20/08/29 14:18:33 GMT FROM: Boris Sbarufatti at PSU M. Boris Sbarufatti; Aldo Treves; Renato Falomo; The HST snapshot imaging survey of 110 BL Lac objects (Urry et al. The BAT light curve showed a long period of emission starting 200 s before the trigger (see Figure 1). it). The data consist of 642 s in. M. Melandri (INAF-OAB), D. The. D. it Stefano Ciprini 1. Krimm (GSFC/USRA), M. The data comprise 9 s in Windowed Timing (WT) mode (taken while Swift was slewing. 12335), from 82 s to 7. 528N) in Yunnan Province, China. A. The Swift Burst Alert Telescope (BAT) triggered on the high mass X-ray binary IGR J16418-4532 on 2021 September 18 at07:58:20 UT (image trigger 1073821). , GCN 7564) on 2008-04-07 at 04:25:49, ~43 hours after the trigger. GCN Circ. B. Boris Sbarufatti at INAF-IASF-Pa <[email protected], the position is marginally consistent with the known X. Leicester), J. 11429), from 51. 6 ks in. Barun was a naughty child. Cummings (GSFC), M. sbarufatti AT brera. Boris Sbarufatti at INAF-OAB/IASFPA <boris. 9 ks exposure. 5 hours after the trigger. Dr. 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. Pascoli, I-06123 Perugia, Italy 2. it> B. A. Cummings (GSFC/UMBC), report on behalf of the Swift Team. Boris Sbarufatti at PSU <bxs60@psu. Cummings (GSFC/UMBC), N. 11944), from 2. inaf. 2 ks exposure time. Sbarufatti (INAF OAB/INAF IASF-PA) , V. The Astronomical Observatory of Brera; Show all 7 authors Hide. 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. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Sbarufatti (INAF OAB/IASF PA), V. it> B. Boris Sbarufatti at PSU <bxs60@psu. it> B. The data are all in Photon Counting (PC) mode. 29529). B. Holland (GSFC/USRA), H. B. 145 (2013) 114 • e-Print: 1302. inaf. sbarufatti@brera. The XRT began observing the field at 2011-03-23 17:57:33 UT, that is T+340 ks ( 3. 15029), from 53 s to 35. Leicester) report on behalf of the Swift-XRT team: Swift-XRT has conducted further observations of the field of the Fermi/LAT. K. Leicester), V. inaf. 5 ks to T+25. Leicester) report on behalf of the Swift-XRT team Swift-XRT has performed follow up observations of GRB 210218A (Sbarufatti et al. Mangano (INAF-IASF PA) report on behalf of the Swift-XRT team: We have analyzed the 3. it> B. Leicester), P. 2017, GCN 21032 ). sbarufatti@uninsubria. Maselli (INAF-IASFPA), A. 1000° Circular_text: TITLE: GCN CIRCULAR NUMBER: 17385 SUBJECT: GRB 150202B: Fermi-LAT detection DATE: 15/02/03 08:25:40 GMT FROM: Magnus Axelsson at Stockholm U. L. Boris Sbarufatti at INAF-OAB/IASFPA <boris. N. Sbarufatti and 5 other. 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. Leicester) report on behalf of the Swift-XRT team Swift-XRT has performed follow up observations of GRB 210218A (Sbarufatti et al. (GCN Circ. P. Holland (CRESST/USRA/GSFC) report on behalf of the Swift-XRT team: We have analysed 3. inaf. 1 ks. Sbarufatti, V. A. 11944), from 2. In extremely urgent cases, after trying the Burst Advocate, you can contact the. Lien (GSFC/UMBC) and B. edu> B. GCN Circ. A. The data are entirely in [email protected]. GCN Circ. Krimm (GSFC/USRA), M. GCN Circ. Detailed description of the adopted techniques and results are reported in Sbarufatti et al. GCN Circ. 9 days) (Cummings, GCN Circ. , 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. de Pasquale (INAF-IASFPA), A. A complete sample of bright Swift Gamma–ray Bursts (GRBs) has been recently selected by Salvaterra et al. Krimm (GSFC/USRA) The BAT data set from T-61 to T+302 sec from the recent telemetry. Leicester), J. sbarufatti@brera. Catalano, Boris Sbarufatti. 4 ks after the BAT trigger. , GCN Circ. inaf. 12335), from 82 s to 7. edu> B. (GCN Circ. , GCN Circ. it> B. (GCN 6891) due to the large offset between the initial BAT position and XRT position. Stephen T. Boris Sbarufatti at INAF-OAB/IASFPA <boris. 2 ks to 383. Sbarufatti, V. it> B. D'Avanzo (INAF-OAB), A. B. inaf. , GCN circ. D'ai (INAF-IASFPA), A. We present observations of GRB 130831A and its afterglow obtained with Swift, Chandra, and multiple ground-based observatories. D'Avanzo (INAF-OAB) and P. it> V. D'Ai (INAF-IASFPA), A. Mangano (INAF IASF-Pa) report on behalf of the Swift-XRT team. ", "bibcode": "2017GCN. Copy reference. Rhaana L. inaf. sbarufatti@brera. sbarufatti@brera. Sbarufatti (INAF-OAB/PSU) report on behalf of the Swift Team: At 11:10:45 UT, the Swift Burst Alert Telescope (BAT) triggered and located GRS 1716-249/GRO J1719-24/V2293 Oph. { "subject": "GRB 130725B - UVOT-enhanced XRT position", "bibcode": "2013GCN. 14862), from 184. Chornock, D. g. 12335), from 82 s to 7. Mangano, V. Imaging redshifts of BL Lac ob jects. Roma-BZCA T blazars in the P alermo BA T Survey B. An official website of the United States government. Dr. inaf. 11525), from 339 s to 30. 22010. Sbarufatti (INAF-OAB/IASFPA), J. Boris Sbarufatti at INAF-IASF-Pa <[email protected] Sbarufatti. ] 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, V. Boris Sbarufatti at INAF-IASF-Pa <[email protected] ks to 35. 7 ks after the trigger. derived absolute magnitudes of the host galaxies are consistent with the distribution of M R of BL Lac hosts given. . We have analyzed 14. Boris Sbarufatti at INAF-OAB/IASFPA <boris. 29529). , Ciprini, S. La Parola (INAF-IASFPA), S. It was optically dark and has been associated with a bright star-forming galaxy at a redshift of. Sbarufatti (INAF/OAB - IASF Pa) report on behalf of the Swift-XRT team: We have analysed 4. The data are entirely in Photon. Download scientific diagram | Spectral decomposition for objects RBS 1752 and RBS 1915. Assuming the standard relativistic fireball model forSkip to main content Utility Menu. Fynbo (CoI) (ESA Member) University of Copenhagen, Niels Bohr Institute Dr. Sbarufatti (INAF OAB/IASF PA), V. The data comprise 24 s in Windowed Timing (WT) mode with the. Burrows (PSU) and P. We report the observations for the GRB191122A (B. Oates (Uni. We report on Swift-XRT observations of GRB 081203B (Copete et al. 2 ks of XRT data for GRB 130725B (Swenson et al. Leicester) and K. sbarufatti@brera. 11440), from 126. Sbarufatti (INAF-OAB/PSU) and 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 (INAF-OAB/IASFPA), R. it> B. Sbarufatti (INAF-OAB/PSU), M. An official website of the United States government. The data consist of 642 s in. and III respectively , where the criteria of selec-Boris Sbarufatti at INAF-OAB/IASFPA <boris. Gropp (PSU), J. Sbarufatti, V. GCN Circ. inaf. A. inaf. inaf. De Pasquale (MSSL) report on behalf of the Swift Team. sbarufatti@brera. it> B. A. The import was successful (after i edited the . H. [email protected] Sbarufatti at INAF-OAB/IASFPA <boris. GCN Circ. P. Cummings 1,3,7,. 8 ks after the BAT trigger. A. N. it> B. 4 ks. Mangano (INAF-IASFPA) on behalf of the Swift-XRT team. 4 ks after the BAT trigger. 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/PSU) report on behalf of the Swift Team: At 08:58:20 UT, the Swift Burst Alert Telescope (BAT) triggered and located GRB 160123A (trigger=671447). 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. Sbarufatti (PSU), P. T reves. 5 ks of XRT data for GRB 110420B (Sbarufatti et al. D. Palmer (LANL) report on behalf of the Swift-XRT team: We have analysed 6. Mangano, V. Boris Sbarufatti at INAF-OAB/IASFPA <boris. The Swift Burst Alert Telescope (BAT) triggered on the. Sbarufatti (INAF-OAB/IASFPA) report on behalf of the Swift-XTR team We have analysed 4. Swift took a second epoch of data for the LAT/IPN GRB 150202B (Axelsson et al. inaf. R. A redshift of z 0. Sbarufatti (INAF-OAB/PSU) and C. H. " Reply replyAstronomers 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. Leicester), J. Sbarufatti (boris. it> Sbarufatti B. Markwardt (CRESST/GSFC/UMD) report on behalf of the Swift-XRT team: We have analysed 4. 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. Content may be subject to copyright. Sbarufatti (INAF-OAB/IASFPA) reports on behalf of the Swift-XRT team: We have analysed 6. Leicester), K. 17722). Boris Sbarufatti was quoted saying: "The pattern we're seeing is observed in X-ray novae where the central object is a black hole. The data comprise 1. C. A. Margutti (INAF/OAB) and M. 9 ks of XRT data for the Swift/BAT-detected burst: GRB110319B (Cummings et al. Boris Sbarufatti at INAF-OAB/IASFPA <boris. M. 0 seconds after the BAT trigger. it> B. , Kotilainen, J. Leicester) report on behalf of the Swift-XRT team: Swift-XRT has performed follow-up observations of the Fermi/LAT-detected burst. it> B. A. 5 ks of XRT data for GRB 191019a (Simpson et al. 7 ks after the BAT trigger. Boris Sbarufatti at INAF-OAB/IASFPA <boris. De Pasquale (MSSL) report on behalf of the Swift Team. Boris Sbarufatti at INAF-OAB/IASFPA <boris. R. An Extension of the Sample | We. D'Avanzo (INAF-OAB), J. Maselli (INAF-IASFPA), A. 3 ks of XRT data for GRB 110915A (Holland et al. Articles by Boris Sbarufatti on Muck Rack. Sbarufatti (INAF-OAB/PSU) and C. inaf. , GCN circ. GCN Circ. Sbarufatti (PSU) reports on behalf of the Swift-XRT team: We have analysed 831 s of XRT data for GRB 170906B (Sbarufatti et al. Sbarufatti, B. (Sbarufatti et al. Ralph A. Melandri (INAF-OAB), B. Sbarufatti (INAF OAB/INAF IASF-PA) and C. Om Sharan Salafia, Maria Edvige Ravasio, Sergio Campana, Paolo D’Avanzo, Boris Sbarufatti & Gianpiero Tagliaferri. sbarufatti@brera. inaf. The BAT ground analysis using the data set from T-240 to T+962 s shows nothing. 5 ks of XRT data for GRB 110420B (Sbarufatti et al. Mangano (INAF-IASFPA), report on behalf of the Swift- XRT team: Swift began observation of the XRF detected by INTEGRAL (Paizis, et al. Kennea (PSU), A. Leicester) report on behalf of the Swift-XRT team: Swift-XRT has performed follow. 3 ks after the BAT trigger. of Warwick) report on behalf of the Swift team: We report on further analysis of BAT trigger 778435/possible GRB 171013A (Sbarufatti et al. sbarufatti@brera. L. Due to an observing constraint, Swift will not slew until T0+40. sbarufatti AT brera. Cummings (GSFC/UMBC), report on behalf of the Swift Team. Sbarufatti (PSU), A.