Sbarufatti, V. Sakamoto (AGU) and B. , GCN Circ. 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. 17722). Mangano, V. The import was successful (after i edited the . 5 @inproceedings{Pasquale2017GRB1R, title={GRB 130831A: Rise and demise of a magnetar at z = 0. Burst Advocate for this burst is B. N. V. R. Boris Sbarufatti at INAF-IASF-Pa <sbarufatti@ifc. The XRT began observing the field at 2011-03-23 17:57:33 UT, that is T+340 ks ( 3. Morris (GWU/GSFC) report on behalf of the Swift-XRT team: We have analysed 9. A. , GCN 12063 ), observed from 138 ks to 425 ks after the Konus-Wind. Semantic Scholar extracted view of "GRB 150527A: Swift-XRT refined Analysis. 1S", "createdOn": 1423508950000, "circularId": 17429, "submitter": "Boris. We analyzed 3. GCN Circ. D. 10998), from 48 s to 39. Burst Advocate for this burst is B. Mangano (INAF IASF-PA), B. Table 1 - uploaded by Boris Sbarufatti. Boris Sbarufatti at INAF-IASF-Pa <[email protected] ks after the BAT trigger. (2005b, 2006a, 2009), Paper I, II. 7 ks to 35. 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. Holland (CRESST/USRA/GSFC) report on behalf of the Swift-XRT team: We have analysed 3. Sbarufatti 1, A. Beardmore (U. sbarufatti@brera. It was optically dark and has been associated with a bright star-forming galaxy at a redshift of. Embed figure. sbarufatti@brera. sbarufatti AT brera. GCN Circ. it> B. it> B. D. 2 ks of XRT data for GRB 110106B (Sbarufatti et [email protected] Sbarufatti at INAF-OAB/IASFPA <boris. A. 11944), from 2. Tohuvavohu (U. (GCN 6891) due to the large offset between the initial BAT position and XRT position. B. 10968 ), from 96 s to 25. Leicester), K. 3 ks after the BAT trigger. The K-band luminosity functions of super star clusters in luminous infrared galaxies, their slopes, and the effects of blending #5. Mangano (INAF/IASFPA) report on behalf of the Swift-XRT team: We have analyzed 4. A. N. These topic labels come from the works of this person. Leicester) report on behalf of the Swift-XRT team: Swift-XRT has performed follow-up observations of the Swift/BAT-detected burst. inaf. inaf. Boris Sbarufatti at INAF-IASF-Pa <sbarufatti@ifc. 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. We have analyzed 14. Sbarufatti (PSU), A. GCN Circ. it). 21822), from 63 s to 924 s after the BAT trigger. A. inaf. 2 ks to 134. Berger & Fox (2009) measured a redshift of z = 0. 21822), from 63 s to 924 s after the BAT trigger. Maselli (INAF-IASFPA), A. Sbarufatti (boris. H. Swift immediately slewed to the target. Cummings (GSFC/UMBC), N. 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. Y. Leicester) report on behalf of the Swift XRT team. Sbarufatti (INAF OAB/IASF PA), V. 0 ks to 196. inaf. inaf. (GCN Circ. sbarufatti@brera. D'Elia (ASDC), A. Sbarufatti (INAF-OAB/PSU), H. sbarufatti@brera. Kennea (PSU), N. The optical spectrum of PKS 1222+216 and its black hole massBoris Sbarufatti at INAF-OAB/IASFPA <boris. Melandri (INAF-OAB), T. This image from Webb’s NIRCam (Near-Infrared Camera) instrument highlights GRB 230307A’s kilonova and its former home galaxy. Evans (U. 3 ks after the BAT trigger. The Swift-BAT trigger happened while the burst position in the sky was Moon constrained for. Sbarufatti, V. Maselli (INAF-IASFPA), A. Romano, C. D'Avanzo (INAF-OAB), J. La Parola, V. 7685) in Window Timing mode, 146 s after the BAT trigger. it> B. , GCN 7564) on 2008-04-07 at 04:25:49, ~43 hours after the trigger. Leicester) and K. Sbarufatti, V. Sbarufatti, V. 2002) and the possible host galaxy of GRB 090417B. Holland (CRESST/USRA/GSFC) report on behalf of the Swift-XRT team: We have analysed 3. Leicester) report on behalf of the Swift-XRT team Swift-XRT has performed follow up observations of GRB 210218A (Sbarufatti et al. B. Boris Sbarufatti at INAF-IASF-Pa <[email protected] AT brera. inaf. , GCN Circ 9461) at 19:26:22 UT, 3026 seconds after the BAT trigger, as soon as the burst went. Credential Certification: Boris Sbarufatti (bxs60@psu. Leicester) report on behalf of the Swift-XRT team: Swift-XRT has performed follow-up observations of the Fermi/LAT-detected burst. inaf. 1 ks after the BAT trigger. GCN 17385 table; GRB_name: GRB150202B: GCN_number: 17385: Detection_method: Fermi LAT Det: t_trigger: 23:59:08. ///// TITLE: GCN CIRCULAR NUMBER: 5856 SUBJECT: GRB 061126: Swift/UVOT Afterglow Detection DATE: 06/11/26 09:53:47 GMT FROM: Daniel E. it> S. The lightcurve is quite complex. The data comprise 180 s in. 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. LaPorte (PSU) report on behalf of the. Lien. M. Mangano, V. We analyzed 3. Markwardt and Span and David M. edu> B. GCN Circ. M. (2008) 1 . 9 ks after the Swift/BAT trigger. Boris Sbarufatti at INAF-IASF-Pa <[email protected]> B. R. Sbarufatti (INAF OAB/INAF IASF-PA) and C. Sbarufatti (INAF-OAB/IASFPA), S. D'Avanzo (INAF-OAB) and P. it> Boris Sbarufatti (INAF-OAB/PSU) reports on behalf of the Swift XRT team We have analysed 4. Sbarufatti (INAF-OAB/PSU), D. inaf. it>. Download PDF. Maselli (INAF-IASFPA), A. The data are entirely in. GCN Circ. inaf. D'Elia (ASDC), A. Vanden Berk at PSU/Swift D. P. D'Elia (ASDC), N. Sbarufatti (PSU), A. 4 ks after the BAT trigger. Sbarufatti B. L. 11525), from 339 s to 30. 6560 ), consisting of 150 s in Window Timing. Boris Sbarufatti at INAF-OAB/IASFPA <boris. (GCN Circ. 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. 6 ks to 14. inaf. sbarufatti@brera. Sbarufatti, V. Evans (U. Barthelmy (GSFC), P. sbarufatti@brera. derived absolute magnitudes of the host galaxies are consistent with the distribution of M R of BL Lac hosts given. Gehrels (GSFC), S. 145 (2013) 114 • e-Print: 1302. Sbarufatti, V. Mingo (U. Dive into the research topics where Boris Sbarufatti is active. De Pasquale (MSSL) report on behalf of the Swift Team. Copy caption. et al. In extremely urgent cases, after trying the Burst Advocate, you can contact the. Oates (MSSL) report on behalf of the Swift-XRT and Swift-UVOT teams We have analysed 4. Boris Sbarufatti at INAF-OAB/IASFPA <boris. 2 ks of XRT data for GRB 130725B (Swenson et al. 5 ks of Photon Counting data for GRB 110604A (Barthelmy et al. P. 8462) at 17:46:11. The field of MMA began with the detection of neutrinos from the Sun and fromBoris Sbarufatti at INAF-IASF-Pa <[email protected]@brera. GCN Circ. Vanden Berk (PSU) report on behalf of the Swift Team: XRT slewed to the source after 23 minutes due. 2 ks of XRT data for GRB 110106B (Sbarufatti et al. Download. L. B. . GCN Circ. 0 ks after the BAT trigger. 9 days) (Cummings, GCN Circ. A. 5 hours after the trigger. inaf. D'Avanzo (INAF-OAB) and P. Download. D'Avanzo (INAF-OAB) and P. inaf. Authors: Marco Landoni, Renato Falomo, Aldo Treves, Boris Sbarufatti. Ukwatta (GSFC/GWU) report on behalf of the Swift Team: We have analyzed the first 22. , GCN Circ. Mangano, V. (Sbarufatti et al. Pagani (U. C. it Stefano Ciprini 1. Leicester), A. Strazzeri, O. Sbarufatti (boris. La Parola (INAF-IASF PA) and W. 9 ks exposure. Swift slewed. Pagine. Leicester) and M. Boris Sbarufatti was quoted saying: "The pattern we're seeing is observed in X-ray novae where the central object is a black hole. B. Guidorzi (INAF OAB) and D. The data comprise 24 s in Windowed Timing (WT) mode with the. GCN Circ. Evans (U. De Pasquale (MSSL) report on behalf of the Swift Team. Melandri (INAF-OAB), D. Sbarufatti (INAF-OAB/PSU), H. “The pattern we’re seeing is observed in X-ray novae where the central object is a black hole. J. We report on Swift XRT observations of the field of the Fermi-LAT discovered GRB 170424A (N. 17722). Sbarufatti, V. A. An official website of the United States government. Corpus ID: 115633452; Swift Detects a New Outburst of the Millisecond Accreting Pulsar SAX J1808. 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, V. Sbarufatti (INAF-OAB/IASFPA), S. sbarufatti@brera. J. it> B. Barthelmy (GSFC), V. Mangano (INAF IASF-PA), B. 6 ks, with a 3. Romano, C. T. edu> B. Krimm (GSFC/USRA) The BAT data set from T-61 to T+302 sec from the recent telemetry. 2 ks to 134. (INAF-IASFPA) report on behalf of the Swift Team: We have analyzed the Swift-XRT data of XRF 090702 (Paizis, et al. Boris Sbarufatti at INAF-OAB/IASFPA <boris. 2 ks of Photon Counting mode data for this burst, covering times from T+17 ks to T+ 47 ks. Please contact the BA by email if you require additional information regarding Swift followup of this burst. Sbarufatti (INAF OAB/INAF IASF-PA) , V. Kennea (PSU), B. 7 ks to 35. An extension of the sample, by B. The data comprise 9 s in Windowed Timing (WT) mode (taken while Swift was slewing. M. In 3. 6 ks to 14. Boris Sbarufatti at INAF-OAB/IASFPA <boris. sbarufatti@brera. inaf. 11440), from 126. There will be no XRT or UVOT data until this time. inaf. 9 ks to T+391. 3 ks after the BAT trigger. GCN 7789 table; GRB_name: GRB080603A: GCN_number: 7789: Detection_method: Other: Circular_text: TITLE: GCN CIRCULAR NUMBER: 7789 SUBJECT: GRB 080603 OA candidate DATE: 08/06/03 12:02:13 GMT FROM: Ryan Chornock at UC Berkeley R. Starling (CoI) (ESA Member) Prof. Mangano (INAF/IASF_PA) and C. Page (U Leicester), [email protected]. A. Sbarufatti (INAF-OAB/IASFPA), R. A. A. Gropp (PSU), J. GCN Circ. UT on 2009 Apr17 (Sbarufatti et al. Boris Sbarufatti at PSU <bxs60@psu. The data comprise 288 s in Windowed Timing (WT) mode (the first. Mangano, B. 1000° Circular_text: TITLE: GCN CIRCULAR NUMBER: 17385 SUBJECT: GRB 150202B: Fermi-LAT detection DATE: 15/02/03 08:25:40 GMT FROM: Magnus Axelsson at Stockholm U. We report on Swift-XRT observations of GRB 081203B (Copete et al. J. Burst Advocate for this burst is. M. Page (U. inaf. sbarufatti@brera. La Parola (INAF-IASF Pa), T. H. Fig 1 - uploaded by Boris Sbarufatti. Cummings (GSFC), M. K. Sbarufatti (PSU), K. We have analyzed 14. In the XRT field of view we detect a single faint. 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. 2 ks and T+516. 3 ks of XRT data for GRB 100725A (Markwardt et al. Gropp (PSU) and P. 0 ks after the BAT trigger. 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). Osborne (U. 0 seconds after the BAT trigger. inaf. A. 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. (INAF-IASFPA) and T. Mangano (INAF/IASF_PA) and C. Margutti (INAF-OAB), S. Morris (GWU/GSFC) report on behalf of the Swift-XRT team: We have analysed 9. 22010. 16, 2012, resulted from a flood of gas. Vanden Berk (PSU), B. it> S. 11525), from 339 s to 30. An extension of the sample, by B. La Parola, B. Sbarufatti (INAF-OAB/PSU), M. Boris Sbarufatti at INAF-IASF-Pa <[email protected]@brera. P. At the present day, spectroscopic follow up of unclassified blazars have been mainly performed with 4 m or 8 m class telescopes (e. it> B. B. A. Kennea (PSU), A. , GCN circ. U. Gehrels (GSFC), S. Leicester) and P. Catalano, Boris Sbarufatti. et al. Evans (U. A. , GCN Circ. Please contact the BA by email if you require additional information regarding Swift followup of this burst. Boris Sbarufatti Research Astronomer at INAF 1y Report this post Day 2 of the "Astrophysical Polarimetry in the Time-Domain Era" conference in Lecco. Leicester), K. Download full-text PDF Read full-text. Mangano (INAF-IASFPA) on behalf of the Swift-XRT [email protected] paper argues that the Cow is a monster black hole shredding a. it> B. Osborne (U. Swift took a second epoch of data for the LAT/IPN GRB 150202B (Axelsson et al. 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. Fogli freschi d'inchiostro; Dita D'Inchiostro's Club; Passato; Mappe d'InchiostroJ. inaf. 06. A. 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.