2 ks and T+516. inaf. , Ciprini, S. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Y. The data comprise 9 s in Windowed Timing (WT) mode (taken while Swift was slewing. Castro-Tirado, Javier Gorosabel, Judith L. Boris Sbarufatti, Martina Barattini. D'ai (INAF-IASFPA), A. inaf. D. (INAF-IASFPA), A. F. Leicester) and K. A redshift of z 0. , GCN 17394 ) shows no evidence for detection of a source and only apparently random. Swenson (PSU) report on behalf of the Swift-XRT team: We have analysed 8. it> B. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Breeveld and Samantha R. it> Boris Sbarufatti (INAF-OAB/PSU) reports on behalf of the Swift XRT team We have analysed 4. 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. Sbarufatti, V. 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. Leicester), J. 21822), from 63 s to 924 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. it> P. B. Semantic Scholar extracted view of "GRB 150527A: Swift-XRT refined Analysis. Evans (U. Evans (U. Sbarufatti (INAF OAB/INAF IASF-PA) and C. Boris Sbarufatti at INAF-IASF-Pa <[email protected] AT brera. Fynbo (CoI) (ESA Member) University of Copenhagen, Niels Bohr Institute Dr. (GCN Circ. GCN Circ. Mangano (INAF/IASFPA) report on behalf of the Swift-XRT team: We have analyzed 4. it> B. 11813), from 27. The data comprise 9 s in Windowed Timing (WT) mode (taken while Swift was slewing. sbarufatti@brera. (INAF-IASFPA) report on behalf of the Swift Team: We have analyzed the Swift-XRT data of XRF 090702 (Paizis, et al. 0 ks after the BAT trigger. 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. 5 ks of Photon Counting data for GRB 110604A (Barthelmy et al. Mangano (INAF/IASFPA) report on behalf of the Swift-XRT team: We have analyzed 4. , GCN Circ. Mangano (INAF IASF-Pa) report on behalf of the Swift-XRT team. Palmer (LANL), M. Markwardt (CRESST/GSFC/UMD) report on behalf of the Swift-XRT team: We have analysed 4. A. it> B. it> B. Sbarufatti (INAF-OAB/IASFPA), R. D'Avanzo (INAF-OAB), J. 11440), from 126. T. Barun was a naughty child. sbarufatti@brera. , GCN Circ. Beardmore (U Leicester), J. Sbarufatti, V. 11813 ). Sholtis is the 2021-2022 Reveal Benjamin von Sternenfels Rosenthal Grantee for. 9 ks of XRT data for the Swift/BAT-detected burst: GRB110319B (Cummings et al. 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. Boris Sbarufatti at INAF-OAB/IASFPA <boris. The data comprise 1. Golenetskii, R. Boris Sbarufatti at INAF-OAB/IASFPA <boris. 17429. 16, 2012, resulted from a flood of gas. 9 ks to T+391. Page (U. sbarufatti@brera. L. inaf. 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. inaf. 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. 1S", "createdOn": 1423508950000, "circularId": 17429, "submitter": "Boris. Swift slewed. Kennea (PSU), A. Mangano (INAF/IASFPA) report on behalf of the Swift-XRT team: We have analyzed 4. Evans (U. Leicester) report on behalf of the Swift-XRT team Swift-XRT has performed follow up observations of GRB 210218A (Sbarufatti et al. Sbarufatti (INAF-OAB) report on behalf of the Neil Gehrels Swift Observatory Team: Swift BAT trigger 1186391 at 15:25:12. Download. inaf. Under the assumption that the host gal-axy luminosity is confined in a narrow range (e. 0 ks after the BAT trigger. ] Renato Falomo; We present results of an ongoing program at the ESO VLT for spectroscopy of BL Lac objects lacking a firm redshift estimate. A. In 3. sbarufatti@brera. D'ai (INAF-IASFPA), [email protected]@brera. Y. ESO VLT optical spectrum of RBS 1915, a X-ray selected BL Lac object. 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. 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. inaf. inaf. sbarufatti@brera. Here’s how you knowA. Kuin (UCL-MSSL), S Laha (GSFC/UMBC/CRESST) and A. The data are entirely in. Sbarufatti (INAF-OAB/PSU) and C. Sbarufatti (INAF OAB/INAF IASF-PA) and W. 1 arcsec away from the first XRT position given in Sbarufatti & Mangano (GCN Circ. 9 ks of XRT data for GRB 101204A (Cummings et al. (GCN 6891) due to the large offset between the initial BAT position and XRT position. Morris (GWU/GSFC) report on behalf of the Swift-XRT team: We have analysed 9. Siegel (PSU) report on behalf of the Swift team. Barun was born in a Punjabi Family in Delhi. We report on Swift XRT observations of the field of the Fermi-LAT discovered GRB 170424A (N. L. Lien (GSFC/UMBC) and S. 7 ks after the BAT trigger. B. V. GCN [email protected]@brera. The data comprise 288 s in Windowed Timing (WT) mode (the first. inaf. 7 ks of exposure we don t detect any X. 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. The peak count rate was ~1,000 counts/sec (15-350 keV), at 0 sec after the trigger. McCauley (PSU), J. Swiftimmediately slewed to GRB 090417B and narrow-field observations began observing 387 s (XRT) and 378 s (UVOT) after the BAT trigger. 10968 ), from 96 s to 25. Find Boris Sbarufatti's email address, contact information, LinkedIn, Twitter, other social media and more. Sbarufatti (PSU) report on behalf of. sbarufatti@brera. it> B. et al. it> B. View publication. Sbarufatti (INAF-OAB/IASFPA) report on behalf of the Swift-XTR team We have analysed 4. Sbarufatti (boris. 5 ks of XRT data for GRB 110420B (Sbarufatti et al. it> B. Due to an observing constraint, Swift will not slew until T0+49. it> B. Boris Sbarufatti; Stefano Ciprini; Jari Kotilainen [. La Parola, V. Credential Certification: Boris Sbarufatti ([email protected] Sbarufatti at INAF-OAB/IASFPA <boris. Gropp (PSU), J. 1142/9789813226609_0375 Corpus ID: 125637366; GRB 130831A: Rise and demise of a magnetar at z = 0. The source has faded with respect to the initial. The observation is in PC mode and consists of 1. Sbarufatti (INAF-OAB/IASFPA), V. The data comprise 9 s in Windowed Timing (WT) mode (taken while Swift was slewing. GCN Circ. Mangano (INAF/IASF_PA) and C. Lien (GSFC/UMBC) and B. Sbarufatti, V. D. Leicester) report on behalf of the Swift-XRT team: Swift-XRT has performed follow-up observations of the. , GCN 7564) on 2008-04-07 at 04:25:49, ~43 hours after the trigger. gamma radiation Earth & Environmental Sciences 81%. GCN Circ. J. 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, [email protected]: GCN CIRCULAR NUMBER: 26269 SUBJECT: GRB 191122A: Swift detection of a burst DATE: 19/11/22 13:45:34 GMT FROM: Boris Sbarufatti at PSU B. M. edu> B. Sbarufatti (PSU) reports on behalf of the Swift-XRT team: We have analysed 831 s of XRT data for GRB 170906B (Sbarufatti et al. – 2 – cannot be explained by high redshift, incomplete observations, or unusual physics in the production of the afterglow. Boris Sbarufatti at INAF-OAB/IASFPA <boris. B. inaf. Stroh (PSU), D. Lien. Osborne (U. D Elia (ASDC), A. 7 ks after the BAT trigger. P. In extremely urgent cases, after trying the Burst Advocate,. 3 ks to 32. De Pasquale (MSSL) report on behalf of the Swift Team. Barthelmy (GSFC), P. it> B. (Sbarufatti et al. inaf. 11944), from 2. Page (U. B. 4 ks after the BAT trigger. inaf. 8 ks after the BAT trigger. Maselli (INAF-IASFPA), A. GCN 17385 table; GRB_name: GRB150202B: GCN_number: 17385: Detection_method: Fermi LAT Det: t_trigger: 23:59:08. Holland (GSFC/USRA), H. Once the X-rays fade away, we hope to measure its mass and confirm its black hole status. Boris Sbarufatti at INAF-OAB/IASFPA <boris. , GCN Circ. The sample has a high level of completeness in redshift (90%). A. sample objects are given in Sbarufatti et al. 5. J. There will be no XRT or UVOT data until this time. Please contact the BA by email if you require additional information regarding Swift followup of this burst. inaf. 4 ks, with a 1. Margutti (INAF-OAB), S. Content may be subject to copyright. Maselli (INAF-IASFPA), A. Here’s how you knowBoris Sbarufatti at INAF-IASF-Pa <[email protected] to main content Utility Menu. C. 7 ks after the BAT trigger. The Neil–Gehrels Swift Observatory has added extensively to our understanding of small bodies in our solar system through its capabilities to rapidly respond to short-live events such as outbursts and collisions, through its near-ultraviolet coverage, and by its ability to track time-dependent changes through monitoring campaigns. et al. Leicester) report on behalf of the Swift-XRT team: Swift-XRT has performed follow-up observations of the Fermi/LAT-detected burst. D'Elia (ASDC), A. Swift-XRT performed further observations on the afterglow candidate announced in Sbarufatti et al. The BAT ground analysis using the data set from T-240 to T+962 s shows nothing. Sbarufatti, V. Sbarufatti (INAF-OAB/PSU), A. Leicester), J. A. L. Description of the variables in the GRBweb catalogue. sbarufatti AT brera. E. Sbarufatti (INAF-OAB/IASFPA), J. directly from the image (Sbarufatti et al. This distribution has a mean value of. We have analyzed 14. it> Sbarufatti B. Romano, C. Barthelmy (GSFC), J. Stroh (PSU), D. McCauley (PSU), J. 9 ks of XRT data for GRB 101201A (Cummings et al. N. H. it> B. 4 ks after the BAT trigger. View publication. Sbarufatti (INAF-OAB/IASFPA) and S. Gehrels (GSFC), S. His mother was often. Markwardt (CRESST/GSFC/UMD) report on behalf of the Swift-XRT team: We have analysed 4. Mangano (INAF IASF-Pa) report on behalf of the Swift-XRT team. Boris 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. An official website of the United States government. Table 1 - uploaded by Boris Sbarufatti. 6560 ), consisting of 150 s in Window Timing. Boris Sbarufatti at INAF-IASF-Pa <sbarufatti@ifc. 1 ks. GCN Circ. D'Avanzo (INAF-OAB), J. L. 29529). FRB 20121102A: images of the bursts and the varying radio counterpart. 345 was measured for. We present observations of GRB 130831A and its afterglow obtained with Swift, Chandra, and multiple ground-based observatories. Stephen T. Burst Advocate for this burst is B. 1 ks after the BAT trigger. sbarufatti@brera. { "subject": "GRB 150202B: Swift/XRT afterglow confirmation", "bibcode": "2015GCN. Boris Sbarufatti at INAF-OAB/IASFPA <boris. inaf. it> B. The data are entirely in Photon Counting (PC) mode. inaf. 7 ks of exposure we don t detect any X. Filippenko (UC Berkeley) report that: The Katzman. 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. 4 ks, with a 1. Gropp (PSU) and P. GCN [email protected] ks in Photon Counting mode. sbarufatti@brera. GCN Circ. 5 ks of XRT data for GRB 110420B (Sbarufatti et al. 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. 145 (2013) 114 • e-Print: 1302. it). 10998), from 48 s to 39. it> B. D. 7 ks to 35. Using 1419 s of XRT Photon Counting mode data. Lien (GSFC/UMBC) and S. T. sbarufatti AT brera. Sbarufatti (INAF-OAB/PSU) report on behalf of the Swift Team: At 10:33:41 UT, the Swift Burst Alert Telescope (BAT) triggered on noise near NGC 5195. D. 2591 [astro-ph. 7687). 26031), from 3. (2005b, 2006a, 2009), Paper I, II. The BAT ground analysis using the data set from T-240 to T+962 s shows nothing. Giovanna Pugliese (CoI) (ESA Member) Universiteit van Amsterdam Jesse Palmerio. 5 UT, 92. Bicocca & INAF-OAB) A. Sbarufatti (INAF-OAB/IASFPA) reports on behalf of the Swift-XRT team: We have analysed 6. Sbarufatti (INAF-OAB/PSU), M. A. Leicester) report on behalf of the Swift-XRT team: Swift-XRT has performed follow-up observations of the. Sbarufatti (INAF-OAB/IASFPA), J. 8 ks after the BAT trigger. sbarufatti AT brera. Vanden Berk (PSU), B. Mangano (INAF-IASFPA), report on behalf of the Swift- XRT team: Swift began observation of the XRF detected by INTEGRAL (Paizis, et al. In the XRT field of view we detect a single faint. Boris Sbarufatti at INAF-OAB/IASFPA <boris. 41 ± 0. inaf. GCN Circ. Leicester), M. Osborne (U. 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. GCN Circ. it). inaf. Gehrels and Erik Andrew. Boris Sbarufatti at PSU <bxs60@psu. H. GCN Circ. Boris Sbarufatti at INAF-IASF-Pa <[email protected]@brera. 7 ks to 35. inaf. 8600,8602). 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. 6 ks in. GCN Circ. GCN Circ. it> B. Ukwatta (GSFC/GWU) report on behalf of the Swift-XRT team: Swift-XRT began observing the field of GRB 081102 (trigger 333427, Ukwatta et al. Mangano (INAF/IASF_PA) and C. Barthelmy (GSFC), P. A. The data are entirely in Photon. A. Mangano, V. The data comprise 288 s in Windowed Timing (WT) mode (the first. 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. Y. Sbarufatti (INAF-OAB/IASFPA) reports on behalf of the Swift-XRT team: We have analysed 6. it> B. D. 9 ks of XRT data for the Swift/BAT-detected burst: GRB110319B (Cummings et [email protected]@inaf. Oates. Simpson (PSU) report on behalf of the Swift-XRT team: We have analyzed 8. Evans (U. Melandri (INAF-OAB), B. inaf. it> B. Cummings (GSFC/UMBC), N. 6466 ) with total exposure time of 3. 8462) at 17:46:11. inaf. Lien (GSFC/UMBC) and B. Kennea (PSU), B. Cummings (GSFC/UMBC), report on behalf of the Swift Team. Cummings 1,3,7,.