10968 ), from 96 s to 25. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Burst Advocate for this burst is B. D'ai (INAF-IASFPA), [email protected]@brera. Copy caption. inaf. 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 with other Swift team members at. D'Avanzo (INAF-OAB), V. 29529). it Stefano Ciprini 1. it> B. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Dive into the research topics where Boris Sbarufatti is active. 4 ks, with a 1. it> B. inaf. In the XRT field of view we detect a single faint. Boris Sbarufatti at INAF-OAB/IASFPA <boris. GCN Circ. D. Boris Sbarufatti at INAF-IASF-Pa <[email protected]. inaf. Barun Sobti’s childhood image. Embed figure. Page (U. , GCN 12063 ), observed from 138 ks to 425 ks after the Konus-Wind. Page (U. inaf. We have analysed 12 ks of XRT data for GRB 150801B (Sbarufatti et al. LaPorte (PSU) report on behalf of the. inaf. Burrows (PSU), J. Oates. GCN Circ. Baumgartner (GSFC/UMBC) The Swift-XRT began observing GRB 080506 (trigger=311159, Baumgartner et al. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Sbarufatti (INAF-OAB/PSU), P. Page (U Leicester), [email protected]. it> Via. Nial Rahil Tanvir (CoI) (ESA Member) Prof. Gehrels and Erik Andrew. inaf. Due to an observing constraint, Swift will not slew until T0+49. 270 UTC: ra: 86. 6466 ) with total exposure time of 3. sbarufatti@brera. Gropp (PSU), J. 17385, Hurley et al. 17722). R. (GCN 12067). 4 ks. Maselli (INAF-IASFPA), A. The data comprise 24 s in Windowed Timing (WT) mode with the. A. it> V. Sbarufatti (boris. Kennea (PSU), A. 0 ks to 196. 1 ks after the BAT trigger. B. GCN [email protected]@brera. The Astronomical Observatory of Brera; Show all 7 authors Hide. Leicester), A. Sbarufatti. D'Avanzo (INAF-OAB), J. 6560 ), consisting of 150 s in Window Timing. Stephen T. Boris Sbarufatti at INAF-OAB/IASFPA <boris. H. Sbarufatti (INAF-OAB/IASFPA) and S. Credential Certification: Boris Sbarufatti ([email protected] Sbarufatti at INAF-OAB/IASFPA <boris. 5 ks of Photon Counting data for GRB 110604A (Barthelmy et al. Sbarufatti, V. References. Table 3 - uploaded by Boris Sbarufatti. Kuin (UCL-MSSL), S Laha (GSFC/UMBC/CRESST) and A. it> B. 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. F. Boris Sbarufatti was quoted saying: "The pattern we're seeing is observed in X-ray novae where the central object is a black hole. Due to an observing constraint, Swift will not slew until T0+49. inaf. GCN Circ. , GCN Circ. 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. it> B. 5 hours after the trigger. Sbarufatti (INAF-OAB/IASFPA) and V. Axelsson. Name Institution Dr. Mangano (INAF IASF-PA), B. 9 ks of XRT data for the Swift/BAT-detected burst: GRB110319B (Cummings et al. Sbarufatti (INAF-OAB/IASFPA) and S. 9 ks after the Swift/BAT trigger. L. P. sbarufatti@brera. Om Sharan Salafia, Maria Edvige Ravasio, Sergio Campana, Paolo D’Avanzo, Boris Sbarufatti & Gianpiero Tagliaferri. Krimm (NSF), N. Barthelmy (GSFC), T. inaf. Evans (U. Sbarufatti, V. A. sbarufatti@brera. Guidorzi (INAF OAB) and D. D. sbarufatti@brera. 2 ks of Photon Counting mode data for this burst, covering times from T+17 ks to T+ 47 ks. Download a PDF of the paper titled ESO-VLT optical spectroscopy of BL Lac objects: I. R. 2009) and identified it as an SDSS galaxy (Strauss et al. it> B. , GCN Circ. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Leicester) report on behalf of the Swift-XRT team: Swift-XRT has conducted further observations of the field of the MAXI-detected burst. Leicester), J. Boris Sbarufatti at INAF-OAB/IASFPA <boris. , GCN Circ. GCN Circ. Mangano (INAF/IASF PA) and D. Table 1 - uploaded by Boris Sbarufatti. Download. We have analyzed 14. The data comprise 24 s in Windowed Timing (WT) mode with the. Leicester), K. 9603) on 2009 July 2 at 14:15 UT, 3. Y. GCN Circ. Mangano (INAF-IASFPA), K. Mangano, V. Received: 19 April 2006We present the analysis of the extraordinarily bright Gamma-Ray Burst (GRB) 130427A under the hypothesis that the GRB central engine is an accretion–powered magnetar. “The pattern we’re seeing is observed in X-ray novae where the central object is a black hole. 8 ks after the BAT trigger. Barthelmy (GSFC), J. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Sbarufatti (INAF-IASFPA), and S. 3 ks of XRT data for GRB 110915A (Holland et al. 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. 9603) comprising 6 ks in Photon Counting (PC) mode from T+16. Kennea (PSU), B. Cummings (GSFC/UMBC), report on behalf of the Swift Team. Kuin (UCL-MSSL), S Laha (GSFC/UMBC/CRESST) and A. Markwardt and Span and David M. The data comprise 177 s in Windowed Timing (WT). 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. Content may be subject to copyright. 21822), from 63 s to 924 s after the BAT trigger. View publication. error circle (Sbarufatti et al. 7828) started on 2008 May 05 at 23:49:36 UT, 97 s after the BAT trigger. This is 1. inaf. Sbarufatti (INAF-OAB/PSU), P. M. N. 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@brera. Margutti (INAF-OAB), S. The source has faded with respect to the initial. it> P. H. Y. g. inaf. Sbarufatti (INAF-OAB/PSU) and D. M. 14862), from 184. D. Rhaana L. inaf. Evans (U. The data comprise 288 s in Windowed Timing (WT) mode (the first. circle (Sbarufatti et al. (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. edu> B. J. 2009) and identified it as a Sloan Digital Sky Survey (SDSS) galaxy (Strauss et al. sbarufatti@brera. it> S. La Parola (INAF-IASFPA), S. sbarufatti@brera. Barun was born in a Punjabi Family in Delhi. (GCN 12067). U. An X-ray outburst caught by NASA’s Swift on Sept. directly from the image (Sbarufatti et al. J. Boris Sbarufatti at INAF-OAB/IASFPA <boris. C. 21822), from 63 s to 924 s after the BAT trigger. Sbarufatti (boris. Mangano (INAF IASF-Pa) report on behalf of the Swift-XRT team. 10979), from 82 s to [email protected]. , GCN Circ. Y. afterglows. 7828) started on 2008 May 05 at 23:49:36 UT, 97 s after the BAT trigger. Kennea (PSU), B. Mangano, V. Page (U. , GCN Circ. 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. Holland (GSFC/USRA), H. Boris Sbarufatti at INAF-OAB/IASFPA <boris. B. Maselli (INAF-IASFPA) and P. Markwardt (CRESST/GSFC/UMD) report on behalf of the Swift-XRT team: We have analysed 4. Leicester) report on behalf of the Swift-XRT team Swift-XRT has performed follow up observations of GRB 210218A (Sbarufatti et al. inaf. D. inaf. sbarufatti@brera. Sbarufatti, V. it> B. edu> P. 7 ks after the BAT trigger. 3 ks of XRT data for GRB 110915A (Holland et al. A. D. 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. 5. it> V. it> B. A. it> B. 11525), from 339 s to 30. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Evans ([email protected]> S. H. Sbarufatti, V. We have analyzed 14. , GCN 7564) on 2008-04-07 at 04:25:49, ~43 hours after the trigger. Please contact the BA by email if you require additional information regarding Swift followup of this burst. inaf. Mangano (INAF/IASF_PA) and C. it> B. 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. it> B. Pagani (U. Barthelmy (GSFC), P. These. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Baumgartner (GSFC/UMBC) The Swift-XRT began observing GRB 080506 (trigger=311159, Baumgartner et al. The data comprise 288 s in Windowed Timing (WT) mode (the first. K. Sbarufatti (INAF-OAB/PSU) and D. Leicester), V. Boris Sbarufatti at INAF-OAB/IASFPA <boris. (Sbarufatti et al. GCN Circ. Sbarufatti (PSU), A. Sbarufatti (INAF-OAB/PSU), M. , Treves, A. Sbarufatti (INAF-OAB/PSU), F. 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. Boris Sbarufatti at INAF-OAB/IASFPA <boris. it> V. Barthelmy (GSFC), [email protected] ks of Photon Counting data for GRB 110604A (Barthelmy et al. 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. Melandri (INAF-OAB), D. Evans (U. of Warwick) report on behalf of the Swift team: We report on further analysis of BAT trigger 778435/possible GRB 171013A (Sbarufatti et al. An official website of the United States government. 5}, author={Massimiliano de Pasquale and M. D. Sbarufatti (INAF-OAB/IASFPA) report on behalf of the Swift-XTR team We have analysed 4. , GCN Circ. 3 ks after the BAT trigger. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Oates (MSSL) report on behalf of the Swift-XRT and Swift-UVOT teams We have analysed 4. Kennea (PSU), A. The data comprise 185 s in Windowed Timing (WT) mode (the first 7 s were taken. Physics Department University of Perugia, and I. 5 ks of XRT data for GRB 110420B (Sbarufatti et al. D'ai (INAF-IASFPA), A. 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. , GCN Circ 9461) at 19:26:22 UT, 3026 seconds after the BAT trigger, as soon as the burst went. Leicester), V. (2005), we estimate a redshift z = 0. Laha (GSFC/UMBC/CRESST) and B. P. GCN Circ 7794) for three orbits which consisted of 200 s of Windowed Timing mode data starting 68 s after the trigger and 990. it> B. De Pasquale (MSSL) report on behalf of the Swift Team. Under the assumption that the host gal-axy luminosity is confined in a narrow range (e. 2005 Sbarufatti et al. G. Born in Chalkis, a small town near Athens, Greece, Sara Fortis never knew her father, who passed away when she was only two months old. edu) Subjects: X-ray, Neutron Star, Transient. 5 edit Updated on Nov 18, 2022 Research works(15) Cited By Date of paper 2004 2023 Number of authors 10 authors or less 8. Download. There will be no XRT or UVOT data until this time. Mangano (INAF-IASF PA) and D. A. P. L. Sbarufatti et al. A. Mingo (U. Burst Advocate for this burst is B. it> B. N. Pagani (U. 4 ks after the BAT trigger. inaf. inaf. Boris Sbarufatti at PSU <bxs60@psu. it> V. De Pasquale (MSSL) report on behalf of the Swift Team. 9 days) (Cummings, GCN Circ. D. Boris Sbarufatti at INAF-OAB/IASFPA <boris. sbarufatti@uninsubria. Download PDF. La Parola (INAF-IASF PA) and W. Leicester) and M. it> B. , GCN 17394 ) shows no evidence for detection of a source and only apparently random. Sbarufatti (INAF-OAB/IASFPA), V. Sbarufatti (INAF-OAB/IASFPA), V. Swiftimmediately slewed to GRB 090417B and narrow-field observations began observing 387 s (XRT) and 378 s (UVOT) after the BAT trigger. M. 0 ks after the BAT trigger. Sbarufatti (INAF-OAB/IASFPA), J. Evans ([email protected] ks of XRT data for GRB 110106B (Sbarufatti et al. Sbarufatti (PSU), K. , GCN Circ. 10983), from 68 s to 58. The refined position for the afterglow, obtained using the XRT-UVOT alignment and matching UVOT field sources to the USNO-B1 catalogue (see. Osborne (U. Sbarufatti (INAF-OAB/IASFPA), R. L. Dive into the research topics where Boris Sbarufatti is active. Boris Sbarufatti at PSU <[email protected] Sharan Salafia, Maria Edvige Ravasio, Sergio Campana, Paolo D’Avanzo, Boris Sbarufatti & Gianpiero Tagliaferri. R. We analyzed 3. N. Leicester) and K. 10968 ), from 96 s to 25. 5 ks to T+25. We report on Swift-XRT observations of GRB 081203B (Copete et al. Melandri (INAF-OAB), B. D'ai (INAF-IASFPA), A. D. A. Our observation starts at 13:48:57 UT and ends at 13:54:24 UT Nov 22, 2019, with five exposure 60 seconds in white filter. Romano, C. 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. inaf. inaf. Cummings (GSFC/UMBC), report on behalf of the Swift Team. inaf. The data comprise 1. Of the two unknown sources reported by. 9 ks to T+391. A. 0 ks after the BAT trigger. GCN Circ. 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. A. Mangano (INAF IASF-Pa) report on behalf of the Swift-XRT team. name RA Dec 15–150 keV band 15–30 keV band 15–70 keV bandBoris Sbarufatti at INAF-OAB/IASFPA <boris. B. D. 10979), from 82 s to [email protected]. reference search 21 citations. 10998), from 48 s to 39. Boris Sbarufatti at INAF-IASF-Pa <sbarufatti@ifc. B. GCN Circ. , GCN circ. , GCN 12063 ), observed from 138 ks to 425 ks after the Konus-Wind. inaf. Stamatikos (NASA/ORAU) and D. Melandri (INAF-OAB), D. GCN Circ. We obtained James Webb Space Telescope mid-infrared (mid-IR) imaging and spectroscopy 29 and 61 days after. it> B. 9 ks of XRT data for GRB 101204A (Cummings et al. L. Amaral-Rogers et al. It is not an astrophysical event. Mangano (INAF/IASFPA) report on behalf of the Swift XRT team: Further observations of the field of GRB 110420B (Sbarufatti et al. Strazzeri, O. Markwardt (CRESST/GSFC/UMD) report on behalf of the Swift-XRT team: We have analysed 4.