Imaging redshifts of BL Lac ob jects. Evans (U. N. Sbarufatti (INAF-IASFPA), and S. GCN Circ. GCN Circ. Download scientific diagram | Spectral decomposition for objects RBS 1752 and RBS 1915. GCN Circ. sbarufatti@brera. gamma radiation Earth & Environmental Sciences 81%. inaf. it> B. V. Content may be subject to copyright. Breeveld, Samantha R. Filippenko (UC Berkeley) report that: The Katzman. sbarufatti AT brera. III. Sbarufatti over 6 years ago. 9 ks to T+391. Once the X-rays fade away, we hope to measure its mass and confirm its black hole status,” said Boris Sbarufatti from Brera Observatory in Milan, Italy, who currently. 7687). GCN Circ. P. Barthelmy (GSFC), P. Detailed description of the adopted techniques and results are reported in Sbarufatti et al. View publication. D'Avanzo (INAF-OAB) and P. Boris Sbarufatti at INAF-OAB/IASFPA <boris. A. 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. inaf. Maselli (INAF-IASFPA), A. Swift-XRT performed further observations on the afterglow candidate announced in Sbarufatti et al. D'Avanzo (INAF-OAB), J. Content may be subject to copyright. 2006) it remains one of the f ew bright sour ces. The data comprise 9 s in Windowed Timing (WT) mode (taken while Swift was slewing. 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). The spectrum reported by Chavushyan et al. 12335), from 82 s to 7. 1 ks after the BAT trigger. Osborne (U. Sbarufatti (INAF-OAB/IASFPA) and S. 8 ks after the BAT trigger. Boris Sbarufatti at INAF-IASF-Pa <[email protected] Sbarufatti. Sbarufatti B. K. 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. P. Boris Sbarufatti; Aldo Treves; Renato Falomo; The HST snapshot imaging survey of 110 BL Lac objects (Urry et al. Kennea (PSU), A. Sbarufatti (INAF-OAB/PSU), L. L. Strazzeri, O. Dive into the research topics where Boris Sbarufatti is active. Swift took a second epoch of data for the LAT/IPN GRB 150202B (Axelsson et al. Download. Leicester), P. Mangano, V. 2005 Sbarufatti et al. Barthelmy (GSFC), J. Boris Sbarufatti at INAF-IASF-Pa <sbarufatti@ifc. Melandri (INAF-OAB), D. inaf. La Parola (INAF-IASFPA), S. Leicester) report on behalf of the Swift-XRT team: Swift-XRT has performed follow-up observations of the. La Parola (INAF-IASF Pa), T. it> B. Ralph A. 7685) in Window Timing mode, 146 s after the BAT trigger. Siegel (PSU) report on behalf of the Swift team: Examination of the full BAT data set for Swift trigger 629693 (Siegel et al. P. 4 ks after the BAT trigger. et al. We analyzed 3. 2 ks of Photon Counting. The data comprise 9 s in Windowed Timing (WT) mode (taken while Swift was slewing. Kennea (PSU), A. 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. Hagen (PSU) report on behalf of the Swift team Swift performed a follow up observation of GRB 150418A, with a pointing in the direction of Source #1 reported by Sbarufatti et al. Description of the variables in the GRBweb catalogue. Mangano, V. edu> B. 10979), from 82 s to 11. Proceedings of ScienceACCEPT & CONTINUE. The lightcurve is quite complex. D'Ai (INAF-IASFPA), D. it>. 7 ks after the trigger. 5 ks of Photon Counting data for GRB 110604A (Barthelmy et al. Krimm (GSFC/USRA) The BAT data set from T-61 to T+302 sec from the recent telemetry. it> B. Page, Silvia Zane, Alice A. Leicester) and M. Barun was a naughty child. 12335), from 82 s to 7. A. 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. 9 days) (Cummings, GCN Circ. 3 ks after the BAT trigger. It is not an astrophysical event. L. An official website of the United States government. email. M. Barthelmy (GSFC), [email protected] ks of Photon Counting data for GRB 110604A (Barthelmy et al. 7685) in Window Timing mode, 146 s after the BAT trigger. Copy reference. Mangano (INAF-IASFPA) and J. Content may be subject to copyright. We analysed data from the first 10 orbits, consisting of 151 s in Windowed. 2 ks and T+516. We report on Swift-XRT observations of GRB 081203B (Copete et al. it> B. Simpson (PSU) report on behalf of the Swift-XRT team: We have analyzed 8. it> V. 7197) and by Schady & Sbarufatti (GCN Circ. Oates, Alberto J. 9 ks after the BAT trigger. Kennea (PSU), A. Boris Sbarufatti at INAF-OAB/IASFPA <boris. N. Krimm (NSF), N. inaf. (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. inaf. 11944) have shown that the X-ray source reported by Sbarufatti et al. Sbarufatti (INAF-OAB/IASFPA), S. Sbarufatti (boris. et al. 2 ks of XRT data for GRB 110106B (Sbarufatti et al. 6 ks in. News; Events; Alumni; Faculty and Staff Directory; Utility Menu. Evans (U. Boris Sbarufatti, Stefano Ciprini, Jari Kotilainen, Roberto Decarli, Aldo Treves, Angelo Veronesi, Renato Falomo Astronomy & Astrophysics Research output : Contribution to journal › Conference article › peer-reviewA. Burst Advocate for this burst is B. (GCN Circ. 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. 10968 ), from 96 s to 25. it> B. Sbarufatti (INAF-OAB/IASFPA), J. 7957) at 08:02 UT, 49 minutes after the trigger. it> B. inaf. In extremely urgent cases, after trying the Burst Advocate,. Bicocca & INAF-OAB) A. inaf. The. D'Avanzo (INAF-OAB), J. Boris Sbarufatti at INAF-OAB/IASFPA <boris. 5 minutes. T. GCN Circ. B. 1. 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. sbarufatti@brera. edu) Subjects: X-ray, Neutron Star, Transient. it> S. 11525), from 339 s to 30. Barthelmy (GSFC), J. 17722). sbarufatti@brera. A. A. 3 ks of XRT data for GRB 110915A (Holland et al. , GCN circ. A. Boris Sbarufatti at PSU <bxs60@psu. 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. GCN Circ. Sbarufatti (INAF-OAB/IASFPA) and S. B. Fig 1 - uploaded by Boris Sbarufatti. Sbarufatti (boris. This burst shows an uncommon drop in the X-ray light curve at about 100 ks after the trigger, with a decay slope of α 7. Page (U Leicester) and B. Lien (GSFC/UMBC) and B. 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. Together they form a unique fingerprint. View publication. 10998), from 48 s to 39. La Parola, V. 2 ks of XRT data for GRB 130518B (Cummings GCN Circ. 11813 ). 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. 3 ks of XRT data for GRB 100725A (Markwardt et al. N. We have analysed 12 ks of XRT data for GRB 150801B (Sbarufatti et al. 1 ks. 17722). Mangano (INAF IASF-Pa) report on behalf of the Swift-XRT team. it> V. Boris Sbarufatti at INAF-IASF-Pa <[email protected], the position is marginally consistent with the known X. Boris Sbarufatti at INAF-OAB/IASFPA <boris. The Swift-BAT trigger happened while the burst position in the sky was Moon constrained for. We returned to the field starting at 14:10:52 UT and acquired 2x120s in R-band and 2x120s in the RG850 filter through high airmass. The data comprise 24 s in Windowed Timing (WT) mode with the. Sbarufatti (INAF-OAB/IASFPA) report on behalf of the Swift-XTR team We have analysed 4. Stroh (PSU), D. 8600,8602). Sbarufatti (INAF-IASFPA), P. 0 ks after the BAT trigger. D'ai (INAF-IASFPA), A. 5 hours after the trigger. Sbarufatti (INAF OAB/INAF IASF-PA) and C. 2 ks to 383. Giovanna Pugliese (CoI) (ESA Member) Universiteit van Amsterdam Jesse Palmerio. GCN Circ. 22007). A. 8600,8602). 9603) on 2009 July 2 at 14:15 UT, 3. Sbarufatti et al. Leicester) report on behalf of the Swift-XRT team: Swift-XRT has performed follow-up observations of the Swift/BAT-detected burst. Lien (GSFC/UMBC), A. sbarufatti@brera. , GCN Circ. 528N) in Yunnan Province, China. We obtained James Webb Space Telescope mid-infrared (mid-IR) imaging and spectroscopy 29 and 61 days after. , GCN Circ. inaf. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Boris Sbarufatti at INAF-IASF-Pa <sbarufatti@ifc. Oates (Uni. Mangano (INAF-IASF PA) and D. In extremely urgent cases, after trying the Burst Advocate, you can contact the. Due to an observing constraint, Swift will not slew until T0+49. Sbarufatti (1) and 18 other authors. 5 hours after the trigger. The data are entirely in Photon Counting (PC. Sbarufatti (INAF-OAB/PSU), H. Kennea (PSU), K. Leicester), K. Maselli (INAF-IASFPA), A. 22010. 1K", "createdOn": 1598983743000, "circularId": 28341, "submitter": "Boris. it> B. GCN Circ. 17398) between T+515. Table 2 - uploaded by Boris Sbarufatti. 2009). it> B. it> B. sbarufatti@brera. Methods. de Pasquale (INAF-IASFPA), A. R. 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. it> [email protected] ks after the BAT trigger. Boris Sbarufatti at INAF-IASF-Pa <[email protected]> B. D'Avanzo (INAF-OAB), J. The data comprise 185 s in Windowed Timing (WT) mode (the first 7 s were taken. 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. , GCN 12063 ), observed from 138 ks to 425 ks after the Konus-Wind. it> B. Leicester) and P. Sbarufatti (INAF-OAB/IASFPA), R. Lien (GSFC/UMBC) and B. Mangano, V. N. Pagani (U. Cummings (GSFC), M. Burrows (PSU), J. Evans (U. Barthelmy (GSFC), P. 2 Ciprini et al. Mangano, B. inaf. Sbarufatti, V. 0 ks after the BAT trigger. 28341. The XRT began observing GRB 080405 (Cummings et al. GCN Circ. , GCN 12063 ), observed from 138 ks to 425 ks after the Konus-Wind. Sbarufatti (INAF OAB/IASF PA), V. Lien (GSFC/UMBC), F. Download a PDF of the paper titled ESO-VLT optical spectroscopy of BL Lac objects: I. Sbarufatti, V. Sbarufatti (INAF-OAB/PSU), M. Swift did not slew. Mangano (INAF-IASF PA) and D. inaf. it 2 INAF, Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio 5, 35122 Padova, Italy 3 Tuorla Observatory, University of Turku, Väisäläntie 20, 21500 Piikkiö, Finland . sbarufatti@uninsubria. 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. B. it> S. 1 Università dell'Insubria, via Valleggio 11, 22100 Como, Italy e-mail: boris. An official website of the United States government. 2591 [astro-ph. Burrows (PSU) report on behalf of the Swift XRT team. B. Omodei et al. P. B. Mangano (INAF IASF-Pa) report on behalf of the Swift-XRT team. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Please contact the BA by email if you require additional information regarding Swift followup of this burst. The data are entirely in. L. B. it> B. 5 ks of Photon Counting data for GRB 110604A (Barthelmy et al. Boris Sbarufatti Research Astronomer at INAF 1y Report this post Day 2 of the "Astrophysical Polarimetry in the Time-Domain Era" conference in Lecco. Sbarufatti (INAF-OAB/PSU) and C. Sbarufatti et al. 6 ks in Photon Counting mode. CO] pdf DOI cite claim. inaf. 1811E, 25. Hagen (PSU) report on behalf of the Swift team Swift performed a follow up observation of GRB 150418A, with a pointing in the direction of Source #1 reported by Sbarufatti et al. N. Evans ([email protected] ks of XRT data for GRB 110106B (Sbarufatti et al. it> B. 12335), from 82 s to 7. The observation is in PC mode and consists of 1. 11944), from 2. Marshall (NASA/GSFC), A. Boris Sbarufatti at INAF-OAB/IASFPA <boris. D'Elia (ASDC), A. Y. P. The data comprise 185 s in Windowed Timing (WT) mode (the first 7 s were taken. it> Via. Kennea (PSU), A. Kennea (PSU), B. Romano, C. Mangano (INAF IASF-Pa) report on behalf of the Swift-XRT team. His mother was often. Melandri (INAF-OAB), V. it>. La Parola (INAF-IASF PA) and W. So exactly what is the Cow? Using data from multiple NASA missions, including the Neil Gehrels Swift Observatory and the Nuclear Spectroscopic Telescope Array (NuSTAR), two groups are publishing papers that provide possible explanations for the Cow’s origins. Melandri (INAF-OAB), J. , GCN Circ 7790) on June 3, 14:11 UT, 173 minutes after the trigger. Melandri (INAF-OAB), B. 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. The data comprise 1. Mangano, V. 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. (2008) 1 . 2 ks to 134. 7198). A. 5 ks of XRT data for GRB 110420B (Sbarufatti et al. B. The data consist of 240 s in Windowed Timing (WT) mode, starting 1603 seconds after the trigger followed. .