sbarufatti@brera. The data comprise 9 s in Windowed Timing (WT) mode (taken while Swift was slewing. Crossref. it> B. We have analyzed 14. View publication. Download. A. N. it> B. S. Sbarufatti (INAF OAB/INAF IASF-PA) and W. 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 (PSU) reports on behalf of the Swift-XRT team: We have analysed 831 s of XRT data for GRB 170906B (Sbarufatti et al. Leicester) report on behalf of the Swift-XRT team: Swift-XRT has conducted further observations of the field of the MAXI-detected burst. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Page (U. 345 that is broadly similar to the Milky Way. Kennea (PSU), A. it). Boris Sbarufatti at INAF-OAB/IASFPA <boris. Gropp (PSU), [email protected]. A. (GCN Circ. 2005b). 10979), from 82 s to [email protected]. D'Ai (INAF-IASFPA), A. it> B. La Parola, B. Boris Sbarufatti at INAF-OAB/IASFPA <boris. , 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. Maselli (INAF-IASFPA), A. Copy caption. 11813 ). The XRT began observing the field at 2011-03-23 17:57:33 UT, that is T+340 ks ( 3. Sbarufatti, V. The light curve shows an initial flare between. 5 ks of XRT data for GRB 110420B (Sbarufatti et al. Leicester) report on behalf of the Swift-XRT team: Swift-XRT has performed follow-up observations of the. , GCN 17394 ) shows no evidence for detection of a source and only apparently random. inaf. Detailed description of the adopted techniques and results are reported in Sbarufatti et al. 5 minutes. 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). Sbarufatti (INAF-OAB/PSU), M. Content may be subject to copyright. sbarufatti@brera. The enhanced XRT position was given in Osborne et al. sbarufatti@brera. Mangano (INAF/IASF_PA) and C. D'Avanzo (INAF-OAB), A. 5 ks of Photon Counting data for GRB 110604A (Barthelmy et al. A. The data are entirely in Photon. 2009) and identified it as an SDSS galaxy (Strauss et al. edu> B. (GCN Circ. Sbarufatti (INAF-OAB/PSU) and D. Mark Kennedy (CoI) (ESA Member). 21822), from 63 s to 924 s after the BAT trigger. Leicester) and K. Download full-text PDF Read full-text. M. Beardmore (U. An official website of the United States government. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Krimm (GSFC/USRA) The BAT data set from T-61 to T+302 sec from the recent telemetry. 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. ///// TITLE: GCN CIRCULAR NUMBER: 5856 SUBJECT: GRB 061126: Swift/UVOT Afterglow Detection DATE: 06/11/26 09:53:47 GMT FROM: Daniel E. Maselli (INAF-IASFPA), A. An X-ray outburst caught by NASA’s Swift on Sept. Sbarufatti (INAF-OAB/IASFPA) and S. 26031), from 3. " by A. 17398) between T+515. 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. Kennea (PSU), A. Sbarufatti (PSU), A. Om Sharan Salafia, Maria Edvige Ravasio, Sergio Campana, Paolo D’Avanzo, Boris Sbarufatti & Gianpiero Tagliaferri. 1 ks after the BAT trigger. Content may be subject to copyright. La Parola, B. Boris Sbarufatti at INAF-IASF-Pa <[email protected] Sbarufatti at INAF-OAB/IASFPA <boris. (GCN Circ. Perley, W. , GCN circ. sbarufatti@brera. 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. The data are all in Photon Counting (PC) mode. 11525), from 339 s to 30. Page (U. 5 UT, 92. 666 UTC: Circular_text: TITLE: GCN CIRCULAR NUMBER: 12064 SUBJECT: Konus-Wind observation of GRB 110604A DATE: 11/06/06 14:36:17 GMT FROM: Dmitry Frederiks at Ioffe Institute S. P. There will be no XRT or UVOT data until this time. GCN Circ. Together they form a unique [email protected]@brera. it> B. B. Download. Lara Nava, Ruben Salvaterra, Giancarlo Ghirlanda, Gabriele Ghisellini, Sergio Campana, Stefano Covino, Paolo D’Avanzo, Andrea Melandri, Boris Sbarufatti, Gianpiero. The best position for the X-ray afterglow is the XRT. inaf. Axelsson. sbarufatti@brera. 8 ks after the BAT trigger. Mangano, B. Boris Sbarufatti at INAF-OAB/IASFPA <boris. UT on 2009 Apr17 (Sbarufatti et al. 9 ks of data of the ToO observation of GRB 080120, started on Jan 20 at 19:47 UT. B. inaf. 3 ks to 32. 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. 10979), from 82 s to 11. A. Fogli freschi d'inchiostro; Dita D'Inchiostro's Club; Passato; Mappe d'InchiostroJ. Boris Sbarufatti at INAF-OAB/IASFPA <boris. A. inaf. Boris Sbarufatti at INAF-OAB/IASFPA <boris. J. 9 ks to T+391. Boris. Palmer (LANL), M. Page (U. 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. A. Perugia Section, Via A. D. 17429. 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. Leicester), P. In 3. it> B. We fit the continuum by a power law after correction for the host. N. it> B. Leicester) and P. 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. News; Events; Alumni; Faculty and Staff Directory2 dark and has been convincingly associated with a bright star-forming galaxy at a redshift of 0. GCN Circ. Marshall (NASA/GSFC), A. Y. 18104), from 64 s to 40. Leicester), A. Romano, C. La Parola, [email protected]° decl: 59. Maselli (INAF-IASFPA) and P. Gehrels (GSFC), S. Sbarufatti (INAF-OAB/IASFPA), R. Kennea (PSU), A. Dr. P. Sbarufatti, V. A. inaf. Sbarufatti (INAF OAB/IASF PA), V. The import was successful (after i edited the . 4 ks after the BAT trigger. Giovanna Pugliese (CoI) (ESA Member) Universiteit van Amsterdam Jesse Palmerio. 9603) on 2009 July 2 at 14:15 UT, 3. A. Romano, C. (Sbarufatti et al. sbarufatti@brera. B. – 2 – cannot be explained by high redshift, incomplete observations, or unusual physics in the production of the afterglow. Leicester) report on behalf of the Swift XRT team. GCN Circ. it> D. Sbarufatti, R. 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. The data consist of 240 s in Windowed Timing (WT) mode, starting 1603 seconds after the trigger followed. inaf. sbarufatti@brera. , Veronesi, A. Melandri (INAF-OAB), B. 0 ks after the BAT trigger. Y. 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. Sbarufatti (INAF-OAB/IASFPA), J. A. sbarufatti@brera. Boris Sbarufatti at INAF-OAB/IASFPA <boris. N. Boris Sbarufatti at INAF-IASF-Pa <[email protected] ks of XRT data for GRB 100727A (Morris et al. T. Sbarufatti, V. 1 ks. 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. C. GCN Circ. D. 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, V. 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. N. GCN Circ. 10968 ), from 96 s to 25. Boris Sbarufatti at INAF-OAB/IASFPA <boris. V. , GCN 12063 ), observed from 138 ks to 425 ks after the Konus-Wind. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Pagine. inaf. 4-3658}, author={Craig B. it>. Burrows (PSU), J. sbarufatti AT brera. it> P. The data comprise 24 s in Windowed Timing (WT) mode with the. de Pasquale (INAF-IASFPA), A. Once the X-rays fade away, we hope to measure its mass and confirm its black hole status,” said Dr Boris Sbarufatti, an astrophysicist at Brera Observatory in Milan, Italy, who currently is working with other Swift team. Starling (CoI) (ESA Member) University of. Burrows (PSU), J. P. Cummings (GSFC/UMBC), report on behalf of the Swift Team. inaf. inaf. 9 ks of XRT data for the Swift/BAT-detected burst: GRB110319B (Cummings et al. inaf. , GCN 17394 ) shows no evidence for detection of a source and only apparently random. ] Renato Falomo; We present results of an ongoing program at the ESO VLT for spectroscopy of BL Lac objects lacking a firm redshift estimate. Kennea (PSU), N. Boris Sbarufatti at INAF-IASF-Pa <sbarufatti@ifc. inaf. Melandri (INAF-OAB) and B. Swift did not slew. , GCN 7564) on 2008-04-07 at 04:25:49, ~43 hours after the trigger. D. 1S", "createdOn": 1374845329000, "circularId": 15038, "submitter": "Boris. Overview; Fingerprint; Abstract. Pascoli, I-06123 Perugia, Italy 2. Stroh (PSU), D. Sbarufatti, V. it>. , GCN Circ 9461) at 19:26:22 UT, 3026 seconds after the BAT trigger, as soon as the burst went. , GCN 7564) on 2008-04-07 at 04:25:49, ~43 hours after the trigger. it> B. Download PDF Abstract: Aims. Sbarufatti (INAF-OAB/IASFPA) report on behalf of the Swift-XTR team We have analysed 4. Sbarufatti (INAF-OAB/PSU), J. Burst Advocate for this burst is. T. Evans (U. Roegiers (PSU), L. Kennea (PSU), K. Sbarufatti. Malesani (DARK/NBI), S. Guidorzi (Univ. . Evans (U. Omodei et al. A. Holland (CRESST/USRA/GSFC) report on behalf of the Swift-XRT team: We have analysed 3. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Vanden Berk (PSU), B. Siegel (PSU) report on behalf of the Swift-XRT team: We have analysed 15 ks of XRT data for GRB 150317A (Siegel et. 5 ks in Photon Counting mode. 1 Larger Context A major frontier in the study of astronomical sources is the development of multi-messenger as-tronomy (MMA). We have analyzed 14. R. GCN Circ 7794) for three orbits which consisted of 200 s of Windowed Timing mode data starting 68 s after the trigger and 990. sbarufatti@brera. Markwardt (CRESST/GSFC/UMD) report on behalf of the Swift-XRT team: We have analysed 4. The BAT ground analysis using the data set from T-240 to T+962 s shows nothing. new redshifts, by B. The analysis of the initial. Boris Sbarufatti at INAF-OAB/IASFPA <boris. The data are entirely in [email protected]. Roma-BZCA T blazars in the P alermo BA T Survey B. La Parola, V. The data are entirely in Photon Counting (PC. (2011). 9 ks of XRT data for GRB 101204A (Cummings et al. 4 ks after the BAT trigger. D Elia (ASDC), A. H. U. Sbarufatti (INAF-OAB/PSU), H. Markwardt and Span and David M. Swift took a second epoch of data for the LAT/IPN GRB 150202B (Axelsson et al. Mingo (U. Sbarufatti (INAF-OAB/IASFPA), V. We report on Swift-XRT observations of GRB 081203B (Copete et al. it). D. Boris Sbarufatti at INAF-OAB <boris. Mangano, V. Swenson (PSU) report on behalf of the Swift-XRT team: We have analysed 8. , Mangano V. H. Leicester), K. Download PDF. Sbarufatti, V. Embed figure. Leicester), M. A. View publication. inaf. Sbarufatti (PSU), A. sbarufatti@brera. Sbarufatti (INAF OAB/INAF IASF-PA) and C. (INAF-IASFPA) and T. This is illustrated in. C. In 3. Sbarufatti (PSU), P. Mingo (U. Sbarufatti (boris. Here’s how you knowDOI: 10. The outburst, produced by a rare X-ray nova, announced the presence of a previously unknown stellar-mass black hole. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Boris Sbarufatti Author Identifier: B. Lien (GSFC/UMBC) and B. sbarufatti@brera. 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). 2 ks of Photon Counting mode data for this burst, covering times from T+17 ks to T+ 47 ks. it> B. Boris Sbarufatti at INAF-OAB/IASFPA <boris. The observation is in PC mode and consists of 1. Barun was born in a Punjabi Family in Delhi. inaf. Krimm (GSFC/USRA), M. Articles by Boris Sbarufatti on Muck Rack. Proceedings of ScienceACCEPT & CONTINUE. Leicester), J. Sbarufatti and 5 other. The data are entirely in. Gianpiero Tagliaferri, Ruben Salvaterra, Sergio Campana, Stefano Covino, Paolo D'Avanzo, Dino Fugazza, Giancarlo Ghirlanda, Gabriele Ghisellini, Andrea Melandri, Lara. 11813), from 27. reference search 21 citations. , Ciprini, S. , & Falomo, R. Leicester), A. Cummings1,3,7, Emmanuel Fonseca1,3,8,. D. Sbarufatti (INAF OAB/INAF IASF-PA) , V. Giovanna Pugliese (CoI) (ESA Member) Universiteit van Amsterdam Jesse Palmerio (CoI) (ESA Member) Observatoire de Paris Prof. Sbarufatti (boris. it> V. Burrows (PSU) report on behalf of the Swift XRT team. 17385, Hurley et al. inaf. Leicester) and M. it> B. The data are entirely in Photon Counting (PC) mode, from T+806 s. 7 ks after the BAT trigger. edu> B. N. We have analyzed 14. it> B. These topic labels come from the works of this person. 7 ks of exposure we don t detect any X. it> B. A. 7828) started on 2008 May 05 at 23:49:36 UT, 97 s after the BAT trigger. arXiv:astro-ph/0508200v1 9 Aug 2005. Sbarufatti (boris. Sbarufatti (INAF-OAB/PSU), L. Krimm (GSFC/USRA) The BAT data set from T-61 to T+302 sec from the recent telemetry. it> B. edu> B. Barthelmy (GSFC), P. Y. Leicester) and P. GCN Circ. L. it> B. GCN Circ. Sbarufatti (1) and 18 other authors. Catalano, Boris Sbarufatti. The Swift-BAT trigger happened while the burst position in the sky was Moon constrained for. Sbarufatti (INAF-OAB/PSU) and M. Osborne (U. 8 ks after the BAT trigger. 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. 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. Maselli (INAF-IASFPA), A. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Beardmore (U. Krimm (GSFC/USRA), M. inaf. { "subject": "GRB 200901A: Swift-XRT refined Analysis", "bibcode": "2020GCN. A. edu) Subjects: X-ray, Neutron Star, Transient. The data are all in Photon Counting (PC) mode.