Sbarufatti, V. 9603) on 2009 July 2 at 14:15 UT, 3. Boris Sbarufatti at INAF-OAB/IASFPA <boris. it> B. inaf. Filippenko (UC Berkeley) report that: The Katzman. Sbarufatti (INAF-OAB/PSU), D. 5 ks of Photon Counting data for GRB 110604A (Barthelmy et al. The data comprise 288 s in Windowed Timing (WT) mode (the first. 17722). Mangano (INAF-IASFPA), report on behalf of the Swift- XRT team: Swift began observation of the XRF detected by INTEGRAL (Paizis, et al. The data comprise 177 s in Windowed Timing (WT). Evans (U. 2005 Sbarufatti et al. Table 3 - uploaded by Boris Sbarufatti. Sbarufatti, V. inaf. Siegel (PSU) report on behalf of the Swift team: Examination of the full BAT data set for Swift trigger 629693 (Siegel et al. Giovanna Pugliese (CoI) (ESA Member) Universiteit van Amsterdam Jesse Palmerio (CoI) (ESA Member) Observatoire de Paris Prof. These topic labels come from the works of this person. 15029), from 53 s to 35. UT on 2009 Apr17 (Sbarufatti et al. " 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. Barthelmy (GSFC), T. inaf. . 2 ks to 134. , 2003, Ap&SS, 285, 367. Sbarufatti (INAF OAB/INAF IASF-PA) , V. The enhanced XRT position was given in Osborne et al. The data comprise 24 s in Windowed Timing (WT) mode with the. 6 ks in. 28341. Leicester), A. it> B. T. Melandri (INAF-OAB), B. Leicester), K. Kennea (PSU), A. Swenson (PSU) report on behalf of the Swift-XRT team: We have analysed 8. Lien (GSFC/UMBC) and B. Markwardt (CRESST/GSFC/UMD) report on behalf of the Swift-XRT team: We have analysed 4. Stroh (PSU), D. Sbarufatti (PSU) ), J. 7687). 4 ks. Burrows (PSU) and P. J. , & Falomo, R. Kennea (PSU), H. sbarufatti@uninsubria. 2 ks to 69. it> D. GCN Circ. Leicester) report on behalf of the Swift-XRT team Swift-XRT has performed follow up observations of GRB 210218A (Sbarufatti et al. , GCN Circ. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Leicester), C. This is 1. 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. 2005b). Boris Sbarufatti at INAF-OAB/IASFPA <boris. 5 ks of Photon Counting data for GRB 110604A (Barthelmy et al. The source has faded with respect to the initial. GCN Circ. it). Sbarufatti (INAF-OAB/IASFPA) reports on behalf of the Swift-XRT team: We have analysed 6. E. inaf. inaf. 1K", "createdOn": 1598983743000, "circularId": 28341, "submitter": "Boris. ESO VLT optical spectroscopy of BL Lac objects. GCN Circ. Sbarufatti, V. Sbarufatti, B. Boris Sbarufatti at INAF-OAB/IASFPA <boris. E. 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. 7828) started on 2008 May 05 at 23:49:36 UT, 97 s after the BAT trigger. 10979), from 82 s to [email protected]. Cummings (GSFC/UMBC), N. Mangano (INAF IASF-Pa), C. In extremely urgent cases, after trying the Burst Advocate,. Morris (GWU/GSFC) report on behalf of the Swift-XRT team: We have analysed 9. Cummings (GSFC/UMBC), report on behalf of the Swift Team. N. Boris Sbarufatti at INAF-IASF-Pa <sbarufatti@ifc. T. Our earliest-time LRIS images do not cover the position of the X-ray source reported by Sbarufatti et al. 4 ks after the BAT trigger. inaf. Sbarufatti (boris. name RA Dec 15–150 keV band 15–30 keV band 15–70 keV bandBoris Sbarufatti at INAF-OAB/IASFPA <boris. The data comprise 9 s in Windowed Timing (WT) mode (taken while Swift was slewing. 1 ks after the BAT trigger. In extremely urgent cases, after trying the Burst Advocate, you can contact the Swift PI by phone. Swift immediately slewed to -3 GRB 090417B and narrow-field observations. A. Copy reference. D'Avanzo (INAF-OAB), J. Page (U Leicester), [email protected]. inaf. 5 ks of XRT data for GRB 100117A (De Pasquale et al. GCN Circ. sbarufatti@brera. Kennea (PSU), K. Sbarufatti (INAF-OAB/IASFPA) and S. The sample has a high level of completeness in redshift (90%). Oates (Uni. 7 ks to 35. A. GCN Circ. J. 11813 ). The optical spectrum of PKS 1222+216 and its black hole massBoris Sbarufatti at INAF-OAB/IASFPA <boris. 270 UTC: ra: 86. Content may be subject to copyright. Leicester) report on behalf of the Swift-XRT team Swift-XRT has performed follow up observations of GRB 210218A (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. N. A. 9 days) (Cummings, GCN Circ. inaf. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Leicester), K. There will thus be no XRT or UVOT data for this trigger before this time. 9 ks exposure. 9603) comprising 6 ks in Photon Counting (PC) mode from T+16. 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. Semantic Scholar extracted view of "GRB 150527A: Swift-XRT refined Analysis. edu> B. The XRT began observing the field at 2011-03-23 17:57:33 UT, that is T+340 ks ( 3. H. GCN Circ. it> B. inaf. 11944), from 2. Sbarufatti over 6 years ago. A. sbarufatti@brera. , GCN Circ 9461) at 19:26:22 UT, 3026 seconds after the BAT trigger, as soon as the burst went. J. B. Y. 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. 9 ks after the Swift/BAT trigger. P. Mangano, V. Dive into the research topics where Boris Sbarufatti is active. We fit the continuum by a power law after correction for the host. inaf. D'Avanzo (INAF-OAB), V. C. Sbarufatti (boris. inaf. In the XRT field of view we detect a single faint. Mangano (INAF IASF-PA), B. 7 ks after the BAT trigger. La Parola, V. Due to a Sun observing constraint, Swift cannot slew to the BAT position until 05:00 UT on 2011 April 11. it> B. Sbarufatti (INAF-OAB/IASFPA) and S. Barthelmy (GSFC), J. Beardmore (U. Burst Advocate for this burst is B. 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. A. Melandri (INAF-OAB), D. Oates (U. 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. Raised by her mother, Sara and her. L. sbarufatti@brera. Beardmore (U. et al. Margutti (INAF-OAB), S. Boris Sbarufatti (CoI) (ESA Member) INAF - Osservatorio Astronomico di Brera Dr. 3 ks of XRT data for GRB 100725A (Markwardt et al. Y. 8600,8602). Boris Sbarufatti at INAF-IASF-Pa <[email protected]@brera. Cancel;"The pattern we're seeing is observed in X-ray novae where the central object is a black hole," said Boris Sbarufatti, an astrophysicist at Brera Observatory in Milan, Italy, currently working. 15029), from 53 s to 35. inaf. Burrows (PSU) report on behalf of the Swift XRT team. L. Using t he imaging redshift method by Sbarufatti et al. Here’s how you knowBoris Sbarufatti at INAF-IASF-Pa <[email protected] to main content Utility Menu. Sbarufatti (INAF-OAB/IASFPA) reports on behalf of the Swift-XRT team: We have analysed 6. V. Sbarufatti, V. Barthelmy (GSFC), [email protected] ks of Photon Counting data for GRB 110604A (Barthelmy et al. : New ESO VLT spectroscopy of BL Lacertae objects Fig. it). Barthelmy (GSFC), J. Boris Sbarufatti at PSU <[email protected]> Boris Sbarufatti (INAF-OAB/PSU) reports on behalf of the Swift XRT team We have analysed 4. Boris Sbarufatti at PSU <[email protected] T. Sbarufatti (PSU), K. it> B. View publication. 4 minutes. it> B. D'Avanzo (INAF-OAB) and P. sbarufatti AT brera. Axelsson. Boris Sbarufatti at INAF-OAB/IASFPA <boris. , 2006Shaw et al. inaf. An Extension of the Sample | We. D. Please contact the BA by email if you require additional information regarding Swift followup of this burst. We report on Swift-XRT observations of GRB 081203B (Copete et al. 2002) and the possible host galaxy of GRB 090417B. Moretti (INAF-OAB) report, on behalf of the Swift-XRT team We have analysed the first three orbits of Swift XRT data for GRB070621 (Sbarufatti et al. D. The data comprise 9 s in Windowed Timing (WT) mode (taken while Swift was slewing. Content may be subject to copyright. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Boris Sbarufatti Research Astronomer at INAF 1y Report this post Day 2 of the "Astrophysical Polarimetry in the Time-Domain Era" conference in Lecco. 21822), from 63 s to 924 s after the BAT trigger. Burrows (PSU) report on behalf of the Swift XRT team. Boris Sbarufatti at INAF-IASF-Pa <[email protected] ks, with a 3. L. 11525), from 339 s to 30. sbarufatti AT brera. N. Burst Advocate for this burst is B. Oates. The observation is in PC mode and consists of 1. Evans (U. Boris Sbarufatti at PSU <bxs60@psu. it> Sbarufatti B. 9 ks to T+391. De Pasquale (MSSL) report on behalf of the Swift Team. { "subject": "GRB 130725B - UVOT-enhanced XRT position", "bibcode": "2013GCN. Barthelmy (GSFC), P. " by A. 5 ks of XRT data for GRB 191019a (Simpson et al. B. (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. A. , GCN Circ. it> P. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Pascoli, I-06123 Perugia, Italy 2. Osborne (U. Barthelmy (GSFC) report on behalf of the Swift team: UVOT took a finding chart exposure of 100. 5 UT, 92. Beardmore (U Leicester), J. , GCN 7564) on 2008-04-07 at 04:25:49, ~43 hours after the trigger. A. Sbarufatti (PSU) reports on behalf of the Swift-XRT team: We have analysed 831 s of XRT data for GRB 170906B (Sbarufatti et al. D. An official website of the United States government. De Pasquale (MSSL) report on behalf of the Swift Team. Sbarufatti, V. 0 ks after the BAT trigger. 3 ks after the BAT trigger. Burrows (PSU), J. B. The data comprise 24 s in Windowed Timing (WT) mode with the. La Parola (INAF-IASF PA) and W. 10998), from 48 s to 39. Sbarufatti (INAF OAB/INAF IASF-PA) and C. it> V. Leicester), J. B. Evans (U. M. Copy reference. Mangano (INAF/IASF_PA) and 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. Leicester), K. (Sbarufatti et al. GCN Circ. R. The Swift-BAT trigger happened while the burst position in the sky was Moon constrained for. Sbarufatti (INAF-OAB/IASFPA), J. inaf. GCN Circ. Sbarufatti (boris. 17385, Hurley et al. it> B. Sbarufatti (INAF-OAB/IASFPA), V. Boris Sbarufatti at INAF-IASF-Pa <sbarufatti@ifc. View publication. it> B. Mangano (INAF/IASFPA) report on behalf of the Swift XRT team: Further observations of the field of GRB 110420B (Sbarufatti et al. Download. The outburst, produced by a rare X-ray nova, announced the presence of a previously unknown stellar-mass black hole. Kuin (UCL-MSSL), S Laha (GSFC/UMBC/CRESST) and A. An official website of the United States government. it> B. Mangano (INAF-IASFPA) and J. 6 ks to 14. B. The field of MMA began with the detection of neutrinos from the Sun and fromBoris Sbarufatti at INAF-IASF-Pa <[email protected]@brera. Boris Sbarufatti at INAF-OAB/IASFPA <boris. GCN Circ. These. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Gropp (PSU) and P. P. 21822), from 63 s to 924 s after the BAT trigger. U. Y. Boris Sbarufatti at INAF-OAB/IASFPA <boris. sbarufatti@brera. A. Leicester), A. 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. 12335), from 82 s to 7. We have analyzed 14. Beardmore (U Leicester), J. inaf. Boris Sbarufatti at INAF-OAB/IASFPA <boris. 21822), from 63 s to 924 s after the BAT trigger. Detailed description of the adopted techniques and results are reported in Sbarufatti et al. (GCN Circ. inaf. 6 ks in. A. Lien (GSFC/UMBC) and B. , GCN 17394 ) shows no evidence for detection of a source and only apparently random. Baumgartner (GSFC/UMBC) The Swift-XRT began observing GRB 080506 (trigger=311159, Baumgartner et al. 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. These. Sbarufatti, V. 1S", "createdOn": 1423508950000, "circularId": 17429, "submitter": "Boris. The data are entirely in Photon Counting (PC. La Parola, V. 6560 ), consisting of 150 s in Window Timing. inaf. inaf. sbarufatti@brera. 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. A. Boris Sbarufatti; Aldo Treves; Renato Falomo; The HST snapshot imaging survey of 110 BL Lac objects (Urry et al. it> V. it> B. , GCN circ. csv file with my fitbit activities for the past month. Rhaana L. An official website of the United States government. it> B. , 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. Evans (U. Sbarufatti (INAF-OAB/PSU), H. inaf. GCN Circ. it). 9 ks of XRT data for the Swift/BAT-detected burst: GRB110319B (Cummings et al. reference search 21 citations. INFN - Sezione di Milano-Bicocca, Piazza della Scienza 2, Milano (MI), Italy. Please contact the BA by email if you require additional information regarding Swift followup of this burst. Palmer (LANL), M. Sbarufatti (INAF-OAB/IASFPA), R. , GCN Circ 7790) on June 3, 14:11 UT, 173 minutes after the trigger. 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. An official website of the United States government. Sbarufatti, V. Page (U Leicester) and B. Mangano (INAF IASF-Pa) report on behalf of the Swift-XRT team. Maselli (INAF-IASFPA), A. Vanden Berk at PSU/Swift D. GCN Circ. Embed figure. 21822), from 63 s to 924 s after the BAT trigger. it> B. It is not an astrophysical event. it> B. Swift took a second epoch of data for the LAT/IPN GRB 150202B (Axelsson et al. Melandri (INAF-OAB), D. We analysed data from the first 10 orbits, consisting of 151 s in Windowed. 7828) started on 2008 May 05 at 23:49:36 UT, 97 s after the BAT trigger. 1086/519450 Corpus ID: 14317593; Swift Observations of GRB 070110: An Extraordinary X-Ray Afterglow Powered by the Central Engine @article{Troja2007SwiftOO, title={Swift Observations of GRB 070110: An Extraordinary X-Ray Afterglow Powered by the Central Engine}, author={Eleonora Troja and Gaspare. sbarufatti@brera. We report on Swift XRT observations of the field of the Fermi-LAT discovered GRB 170424A (N. Barthelmy (GSFC), P. The detection and the measurement of very weak spectral features are difficult to assess because they depend on theThe peak count rate was ~6000 counts/sec (15-350 keV), at ~0 sec after the trigger. 7957) at 08:02 UT, 49 minutes after the trigger. Boris Sbarufatti at INAF-OAB/IASFPA <boris. D'Avanzo (INAF-OAB), J. Under the assumption that the host gal-axy luminosity is confined in a narrow range (e. We analyzed 3. Sbarufatti, V. Krimm (GSFC/USRA) The BAT data set from T-61 to T+302 sec from the recent telemetry. 7195. inaf. Kennea (PSU), B. edu> B.