A. 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. Brett Sholtis was a health reporter for WITF/Transforming Health until early 2023. Page (U Leicester) and B. sbarufatti@brera. Mangano (INAF-IASF PA) report on behalf of the Swift-XRT team: We have analyzed the 3. Leicester), K. Sbarufatti (INAF-OAB/IASFPA), J. 9 ks exposure. 5 ks of of Swift-XRT data of GRB 090912 (trigger 362633; Ukwatta, et al. Swift did not slew. Boris Sbarufatti at INAF-IASF-Pa <sbarufatti@ifc. (GCN Circ. Burrows (PSU) and P. Boris Sbarufatti Author Identifier: B. 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. Mangano, V. Boris Sbarufatti at INAF-OAB/IASFPA <boris. 4 ks, with a 1. inaf. 5 UT, 92. it> B. P. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Kennea (PSU), A. 9 ks to T+391. it> B. Cummings (GSFC/UMBC), report on behalf of the Swift Team. T. Mangano (INAF-IASF PA) report on behalf of the Swift-XRT team: We have analyzed the 3. Boris Sbarufatti at INAF-OAB/IASFPA <boris. of Warwick) report on behalf of the Swift team: We report on further analysis of BAT trigger 778435/possible GRB 171013A (Sbarufatti et al. , GCN 7564) on 2008-04-07 at 04:25:49, ~43 hours after the trigger. M. La Parola, V. 1S", "createdOn": 1374845329000, "circularId": 15038, "submitter": "Boris. name RA Dec 15–150 keV band 15–30 keV band 15–70 keV bandBoris Sbarufatti at INAF-OAB/IASFPA <boris. The optical spectrum of PKS 1222+216 and its black hole massBoris Sbarufatti at INAF-OAB/IASFPA <boris. The data consist of 642 s in. L. A. Sbarufatti (INAF-OAB/IASFPA), J. 0 ks after the BAT trigger. Osborne (U. 9 ks to T+391. Authors: L Rhodes, M Caleb, BW Stappers, A Andersson, MC Bezuidenhout, LN Driessen, I Heywood. 7 ks after the BAT trigger. Boris Sbarufatti at INAF-IASF-Pa <[email protected]@brera. 1 ks. Beardmore (U. inaf. P. Boris Sbarufatti at INAF-OAB/IASFPA <boris. 11813), from 27. inaf. 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. it Stefano Ciprini 1. Boris Sbarufatti at INAF-IASF-Pa <[email protected] Sbarufatti. inaf. An official website of the United States government. Burst Advocate for this burst is B. Evans (U. 3 ks after the BAT trigger. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Melandri (INAF-OAB), T. error circle (Sbarufatti et al. sbarufatti@brera. Boris Sbarufatti at INAF-IASF-Pa <sbarufatti@ifc. Leicester) report on behalf of the Swift XRT team. Sbarufatti (INAF-OAB/IASFPA) reports on behalf of the Swift-XRT team: We have analysed 6. Burst Advocate for this burst is B. Sbarufatti (INAF-OAB/PSU), L. 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. 6560 ), consisting of 150 s in Window Timing. McCauley (PSU), J. sbarufatti@brera. edu> B. inaf. Holland (GSFC/USRA), H. Evans (U. We use the 80cm telescope of CHanging Event Survey at the YaoAn observation station(101. This image from Webb’s NIRCam (Near-Infrared Camera) instrument highlights GRB 230307A’s kilonova and its former home galaxy. (GCN 6891) due to the large offset between the initial BAT position and XRT position. T. Siegel (PSU) report on behalf of the Swift-XRT team: We have analysed 15 ks of XRT data for GRB 150317A (Siegel et. Marshall (NASA/GSFC), A. 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. sbarufatti@brera. ESO VLT optical spectrum of RBS 1915, a X-ray selected BL Lac object. T. Boris Sbarufatti at INAF-IASF-Pa <[email protected]> B. Kennea (PSU), K. inaf. sbarufatti@brera. B. Fig 1 - uploaded by Boris Sbarufatti. Leicester) report on behalf of the Swift-XRT team: Swift-XRT has conducted further observations of the field of the Fermi/LAT. Boris Sbarufatti at INAF-IASF-Pa <sbarufatti@ifc. [email protected] ks of exposure we don t detect. E. Mangano, V. Krimm (GSFC/USRA), M. edu> P. 2 ks of Photon Counting mode data for this burst, covering times from T+17 ks to T+ 47 ks. Perugia Section, Via A. 9 days) (Cummings, GCN Circ. Page (U Leicester), [email protected]. Together they form a unique fingerprint. Barthelmy (GSFC) report on behalf of the Swift team: UVOT took a finding chart exposure of 100. inaf. Maselli (INAF-IASFPA), A. 17722). Barthelmy (GSFC), P. P. et al. Swift took a second epoch of data for the LAT/IPN GRB 150202B (Axelsson et al. Swift slewed. A. 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. D'Avanzo (INAF-OAB) and P. it> V. 5 ks of XRT data for GRB. The lightcurve is quite complex. V. it> B. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Leicester), C. Sbarufatti (INAF-OAB/IASFPA), J. Osborne (U. 0 ks after the BAT trigger. 1 Università dell'Insubria, via Valleggio 11, 22100 Como, Italy e-mail: boris. From: Boris Sbarufatti [v1] Mon, 20 Oct 2008 14:06:52 UTC (133 KB) Full-text links: Download: Download a PDF of the paper titled ESO VLT optical spectroscopy of BL Lacertae objects. 29529). et al. B. Melandri (INAF-OAB), B. The lightcurve is quite complex. Lien (GSFC/UMBC) and S. 5 ks of XRT data for GRB 100117A (De Pasquale et al. inaf. GCN Circ. ESO VLT optical spectrum of OQ 012, a radio-selected BL. P. 11813 ). Sbarufatti, V. 2 ks and T+516. inaf. A. 4 ks after the BAT trigger. The best position for the X-ray afterglow is the XRT. In extremely urgent cases, after trying the Burst Advocate, you can contact the. Pascoli, I-06123 Perugia, Italy 2. GCN Circ. it> B. B. Download. Simpson (PSU) report on behalf of the Swift-XRT team: We have analyzed 8. 3 ks of XRT data for GRB 110915A (Holland et al. A. The Swift-BAT trigger happened while the burst position in the sky was Moon constrained for. sample objects are given in Sbarufatti et al. , GCN Circ. The data are entirely in. Please contact the BA by email if you require additional information regarding Swift followup of this burst. Articles by Boris Sbarufatti on Muck Rack. Boris Sbarufatti at INAF-OAB/IASFPA <boris. inaf. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Sbarufatti, V. Sbarufatti, B. Sbarufatti, V. (2008). U. it> B. Cummings (GSFC), M. Melandri (INAF-OAB) and B. 22007). inaf. . D'ai (INAF-IASFPA), [email protected]@brera. Osborne (U. A. Mangano (INAF/IASF PA) and D. 2009). Sbarufatti (INAF-OAB/IASFPA) reports on behalf of the Swift-XRT team: We have analysed 6. Kennea (PSU), A. The data consist of 642 s in. La Parola (INAF-IASF PA) and W. The data are all in Photon Counting (PC) mode. Mangano (INAF-IASFPA) on behalf of the Swift-XRT [email protected] paper argues that the Cow is a monster black hole shredding a. 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. , GCN Circ 9461) at 19:26:22 UT, 3026 seconds after the BAT trigger, as soon as the burst went. B. In extremely urgent cases, after trying the Burst Advocate,. Embed figure. News; Events; Alumni; Faculty and Staff Directory2 dark and has been convincingly associated with a bright star-forming galaxy at a redshift of 0. L. P. Sbarufatti (INAF-OAB/PSU), P. La Parola (INAF-IASF PA) and W. All content in this area was uploaded by Boris Sbarufatti. Boris Sbarufatti at INAF-OAB/IASFPA <boris. 2006) it remains one of the f ew bright sour ces. Swiftimmediately slewed to GRB 090417B and narrow-field observations began observing 387 s (XRT) and 378 s (UVOT) after the BAT trigger. La Parola, B. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Sbarufatti (INAF-OAB/PSU), D. Lien (GSFC/UMBC) and B. Download. it> V. Maselli (INAF-IASFPA), A. inaf. Evans (U. , GCN 12063 ), observed from 138 ks to 425 ks after the Konus-Wind. Boris Sbarufatti at INAF-IASF-Pa <[email protected] Sbarufatti at INAF-OAB/IASFPA <boris. 3 ks of XRT data for GRB 110915A (Holland et al. GCN Circ. Sbarufatti (INAF-OAB/IASFPA), J. Kennea (PSU), B. it> B. The data are entirely in. M. Holland (CRESST/USRA/GSFC) report on behalf of the Swift-XRT team: We have analysed 3. GCN Circ. 8600,8602). La Parola (INAF-IASF Pa), T. The K-band luminosity functions of super star clusters in luminous infrared galaxies, their slopes, and the effects of blending #5. T. A. Sbarufatti (INAF-OAB/PSU) report on behalf of the Swift Team: At 08:02:13 UT, the Swift Burst Alert Telescope (BAT) triggered and located GRS 1716-249/GRO J1719-24/V2293 Oph (trigger=731535). Guidorzi (INAF OAB) and D. , GCN Circ. inaf. Sbarufatti (PSU), A. News; Events; Alumni; Faculty and Staff Directory; Utility Menu. Cummings (GSFC), M. Download PDF. 1. A. Burrows (PSU), B. L. inaf. inaf. Krimm (NSF), N. Sbarufatti, V. Kennea (PSU), A. Mangano (INAF/IASF_PA) and C. Sbarufatti (boris. inaf. Leicester) and P. it> B. it> Sbarufatti B. Swift immediately slewed to GRB 090417B and narrow-field observations began observing 387 s (XRT) and 378 s (UVOT) after the BAT trigger. edu) Subjects: X-ray, Neutron Star, Transient. , GCN Circ. Leicester), J. it> B. 9 ks after the Swift/BAT trigger. Evans (U. Page (U. Sbarufatti, R. N. An official website of the United States government. Page and Silvia Zane and A. Gehrels (GSFC), S. Cummings1,3,7, Emmanuel Fonseca1,3,8,. 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. Sbarufatti et al. Embed figure. Swift immediately slewed to -3 GRB 090417B and narrow-field observations. ) is showing up in garmin connect. A. Of the two unknown sources reported by. Pagani (U. III. III. Krimm (GSFC/USRA) The BAT data set from T-61 to T+302 sec from the recent telemetry. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Osborne (U. D. Download. Maselli (INAF-IASFPA) and P. Melandri (INAF-OAB), D. P. The BAT ground analysis using the data set from T-240 to T+962 s shows nothing. N. Racusin, Eleonora. 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. T. Starling (CoI) (ESA Member) Prof. 7 ks to 35. GCN Circ. D. it). R. Holland1,2,3, Boris Sbarufatti4, Rongfeng Shens, Patricia Schady6, Jay R. 26031), from 3. Evans ([email protected] ks of XRT data for GRB 110106B (Sbarufatti et al. The data comprise 235 s in Windowed Timing (WT). sbarufatti AT 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). Perley, W. Evans (U. Download Table | Journal of Observations from publication: European Southern Observatory Very Large Telescope Optical Spectroscopy of BL Lacertae Objects. Nial Rahil Tanvir (CoI) (ESA Member) Prof. Vanden Berk (PSU) report on behalf of the Swift Team: XRT slewed to the source after 23 minutes due. Tohuvavohu (U Toronto) report on behalf of the Neil Gehrels Swift Observatory Team: At 13:32:56 UT, the Swift Burst Alert. We consider a sample of 49 BL Lac objects from an ongoing spectroscopic program at the ESO VLT (B. Table 3 - uploaded by Boris Sbarufatti. 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. Sbarufatti (INAF-OAB/PSU) and C. 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. 06. Kennea (PSU), B. We analyzed 3. GCN Circ. 9 ks of XRT data for the Swift/BAT-detected burst: GRB110319B (Cummings et [email protected]@inaf. Sbarufatti (PSU) reports on behalf of the Swift-XRT team: We have analysed 831 s of XRT data for GRB 170906B (Sbarufatti et al. Gehrels (GSFC), S. Sbarufatti (INAF-OAB/IASFPA), J. Palmer (LANL) report on behalf of the Swift-XRT team: We have analysed 6. Boris Sbarufatti (CoI) (ESA Member) INAF - Osservatorio Astronomico di Brera Dr. 29529). We present the detection of persistent soft X-ray radiation with –1042 erg s–1 at the location of the. Burrows (PSU) report on behalf of the Swift XRT team. Table 1 - uploaded by Boris Sbarufatti. A. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Beardmore (U Leicester), J. inaf. Leicester), A. Osborne (U. R. Beardmore (U. et al. GCN Circ. GCN Circ. inaf. inaf. (GCN Circ. (GCN Circ. Sbarufatti (INAF-OAB/PSU) and D. 11525), from 339 s to 30. , GCN Circ. Dr. A. 10983), from 68 s to 58. , & Falomo, R. The XRT began observing the field at 2011-03-23 17:57:33 UT, that is T+340 ks ( 3. it> B. III. 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. Sbarufatti et al. Boris Sbarufatti at INAF-OAB/IASFPA <boris. T. Sbarufatti (PSU), K. 9 ks after the Swift/BAT trigger. This is illustrated in. Evans (U. Mangano (INAF IASF-Pa) report on behalf of the Swift-XRT team. Mangano (PSU), M. Produced by a rare X-ray nova, this outburst announced the presence of a previously unknown stellar-mass black hole that is located 20,000 to 30,000 light-years away. 7685) in Window Timing mode, 146 s after the BAT trigger. Siegel (PSU) report on behalf of the Swift team. V. 5 minutes. Barthelmy (GSFC), P. 0 ks after the BAT trigger. GCN Circ. Y. Here’s how you knowNASA's Swift satellite detected high-energy X-rays a few degrees from the center of our galaxy, toward the constellation Sagittarius. GCN Circ. 9 ks after the BAT trigger. , GCN circ. Raised by her mother, Sara and her. Johan P. it> B. Leicester), V.