edu) Subjects: X-ray, Neutron Star, Transient. The refined position for the afterglow, obtained using the XRT-UVOT alignment and matching UVOT field sources to the USNO-B1 catalogue (see. Page, Silvia Zane, Alice A. Krimm (NSF), N. N. Sbarufatti (INAF-OAB/IASFPA), J. D. Boris Sbarufatti at INAF-OAB/IASFPA <boris. 0 seconds after the BAT trigger. We report on Swift-XRT observations of GRB 081203B (Copete et al. de Pasquale (INAF-IASFPA), A. 5 minutes. GCN Circ. 5 ks of XRT data for GRB 110420B (Sbarufatti et al. Stroh (PSU), D. 3 ks of XRT data for GRB 110915A (Holland et al. D. , GCN Circ 9461) at 19:26:22 UT, 3026 seconds after the BAT trigger, as soon as the burst went. sample objects are given in Sbarufatti et al. Morris (GWU/GSFC) report on behalf of the Swift-XRT team: We have analysed 9. { "subject": "BAT trigger 778435 is not a GRB. Sbarufatti, V. Mangano (INAF IASF-PA), B. 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. GCN Circ. The data are entirely in Photon Counting (PC. 5 ks to T+25. 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). H. 8600, 8602) 16. Gropp (PSU) and P. 11440), from 126. Boris Sbarufatti at INAF-OAB/IASFPA <boris. These topic labels come from the works of this person. Leicester), P. D. Sbarufatti (INAF-OAB/PSU), M. 2002) and the possible host galaxy of GRB 090417B. 4 ks after the BAT trigger. Pagani (U. inaf. derived absolute magnitudes of the host galaxies are consistent with the distribution of M R of BL Lac hosts given. 1K", "createdOn": 1598983743000, "circularId": 28341, "submitter": "Boris. Sbarufatti, V. 11813 ). Page (U. A. 7 ks after the BAT trigger. GCN Circ. Lara Nava, Ruben Salvaterra, Giancarlo Ghirlanda, Gabriele Ghisellini, Sergio Campana, Stefano Covino, Paolo D’Avanzo, Andrea Melandri, Boris Sbarufatti, Gianpiero. 528N) in Yunnan Province, China. Sbarufatti (INAF OAB/IASF PA), V. The peak count rate was ~1,000 counts/sec (15-350 keV), at 0 sec after the trigger. October 25, 2023 Source: NASA/Goddard Space Flight Center Summary: A team of scientists has used multiple space and ground-based telescopes to observe an. La Parola, [email protected]° decl: 59. from publication: European. Raised by her mother, Sara and her. Osborne (U. 9 ks exposure. Here’s how you knowNASA's Swift satellite detected high-energy X-rays a few degrees from the center of our galaxy, toward the constellation Sagittarius. { "subject": "GRB 200901A: Swift-XRT refined Analysis", "bibcode": "2020GCN. 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. it> B. GCN Circ. 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. Osborne (U. P. These topic labels come from the works of this person. Sbarufatti (INAF-OAB/PSU) and C. 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. Boris Sbarufatti at PSU <bxs60@psu. A. The data comprise 185 s in Windowed Timing (WT) mode (the first 7 s were taken. . 3 ks after the BAT trigger. Vanden Berk at PSU/Swift D. From: Boris Sbarufatti [v1] Mon, 20 Oct 2008 14:06:52 UTC (133 KB) Full-text links: Download: Download a PDF of the paper titled ESO VLT optical spectroscopy of BL Lacertae objects. 10968 ), from 96 s to 25. Tohuvavohu (U Toronto) report on behalf of the Neil Gehrels Swift Observatory Team: At 13:32:56 UT, the Swift Burst Alert. Marshall (NASA/GSFC), A. Siegel (PSU) report on behalf of the Swift team. 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. Barun Sobti consuming alcohol. new redshifts, by B. Melandri (INAF-OAB), D. 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. Boris Sbarufatti at INAF-IASF-Pa <[email protected] Sbarufatti at INAF-OAB/IASFPA <boris. et al. All content in this area was uploaded by Boris Sbarufatti. 7 ks to 35. Sbarufatti (INAF-OAB/PSU) and C. Boris Sbarufatti at INAF-OAB/IASFPA <boris. it). Boris Sbarufatti at INAF-OAB/IASFPA <boris. , Sbarufatti et al. Johan P. sbarufatti AT brera. GCN Circ. et al. M. it> S. Sbarufatti (INAF-OAB/IASFPA), S. (GCN 12067). Melandri (INAF-OAB), D. The BAT ground analysis using the data set from T-240 to T+962 s shows nothing. Sbarufatti (INAF-OAB/PSU) and D. circle (Sbarufatti et al. La Parola, V. L. Evans (U. inaf. D. Boris Sbarufatti at INAF-IASF-Pa <sbarufatti@ifc. The best position for the X-ray afterglow is the XRT. inaf. (2005a, 2006). Romano, C. Boris Sbarufatti at INAF-OAB/IASFPA <boris. La Parola, B. inaf. Markwardt (CRESST/GSFC/UMD) report on behalf of the Swift-XRT team: We have analysed 4. Krimm (GSFC/USRA) The BAT data set from T-61 to T+302 sec from the recent telemetry. Pagine. sbarufatti AT brera. 5 ks of Photon Counting data for GRB 110604A (Barthelmy et al. T. Sbarufatti, V. V. 3 ks after the BAT trigger. A. it> B. Roma-BZCA T blazars in the P alermo BA T Survey B. D'Avanzo (INAF-OAB), J. Sbarufatti (PSU), A. Osborne (U. Burrows (PSU) report on behalf of the Swift XRT team. 2 ks to 134. csv file with my fitbit activities for the past month. GCN Circ. Kennea (PSU), B. it> B. P. 11944), from 2. it> B. Sbarufatti (INAF-OAB/PSU), P. of Warwick) report on behalf of the Swift team: We report on further analysis of BAT trigger 778435/possible GRB 171013A (Sbarufatti et al. We analyzed 3. Sbarufatti (PSU), P. 7 ks of exposure we don t detect any X. sbarufatti AT brera. Krimm (NSF), N. Sbarufatti (INAF-OAB/IASFPA) and S. 7 ks to 35. Leicester) report on behalf of the Swift-XRT team: Swift-XRT has conducted further observations of the field of the MAXI-detected burst. 9 ks to T+391. Articles by Boris Sbarufatti on Muck Rack. 345 was measured for. P. D. R. A. it> S. LaPorte (PSU) report on behalf of the. Sbarufatti (INAF-OAB/IASFPA), J. Copy caption. Download PDF. inaf. 1 ks. C. Leicester), A. Holland (CRESST/USRA/GSFC) report on behalf of the Swift-XRT team: We have analysed 3. Mangano (PSU), M. H. GCN Circ. Cummings (GSFC/UMBC), report on behalf of the Swift Team. Cummings (GSFC), M. Mangano (INAF/IASF Pa) report on behalf of the Swift XRT team Swift XRT began observations of GRB 080710 (Sbarufatti et al. Oates, Alberto J. , Ciprini, S. Barthelmy (GSFC), P. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Swiftimmediately slewed to GRB 090417B and narrow-field observations began observing 387 s (XRT) and 378 s (UVOT) after the BAT trigger. , GCN Circ. The data are entirely in Photon. UT on 2009 Apr17 (Sbarufatti et al. and III respectively , where the criteria of selec-Boris Sbarufatti at INAF-OAB/IASFPA <boris. 3 ks after the BAT trigger. Warwick) and S. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Barthelmy (GSFC), J. 28341. , GCN Circ. Sbarufatti (INAF-OAB/IASFPA), J. 2 ks of Photon Counting mode data for this burst, covering times from T+17 ks to T+ 47 ks. Table 1 - uploaded by Boris Sbarufatti. inaf. A. Mangano (INAF/IASFPA) report on behalf of the Swift XRT team: Further observations of the field of GRB 110420B (Sbarufatti et al. 5 ks of of Swift-XRT data of GRB 090912 (trigger 362633; Ukwatta, et al. Morris (GWU/GSFC) report on behalf of the Swift-XRT team: We have analysed 9. it> B. Mangano, V. Ralph A. error circle (Sbarufatti et al. N. it). GCN Circ. B. 4 ks. Mark Kennedy (CoI) (ESA Member). Leicester), M. inaf. Maselli (INAF-IASFPA) and P. of Warwick) report on behalf of the Swift team: We report on further analysis of BAT trigger 778435/possible GRB 171013A (Sbarufatti et al. La Parola (INAF-IASF PA) and W. Evans (U. Please contact the BA by email if you require additional information regarding Swift followup of this burst. P. Boris Sbarufatti (CoI) (ESA Member) INAF - Osservatorio Astronomico di Brera Dr. (INAF-IASFPA) report on behalf of the Swift Team: We have analyzed the Swift-XRT data of XRF 090702 (Paizis, et al. This distribution has a mean value of. Boris Sbarufatti at INAF-OAB <boris. Leicester) and P. Mangano (INAF-IASFPA) and J. Berger & Fox (2009) measured a redshift of z = 0. TITLE: GCN CIRCULAR NUMBER: 28307 SUBJECT: GRB 200829A: Swift detection of a burst with an optical afterglow DATE: 20/08/29 14:18:33 GMT FROM: Boris Sbarufatti at PSU M. , Treves, A. Lien (GSFC/UMBC) and B. Mingo (U. L. it> B. inaf. { "subject": "GRB 130725B - UVOT-enhanced XRT position", "bibcode": "2013GCN. 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/IASFPA), R. R. Siegel (PSU) report on behalf of the Swift team. Boris Sbarufatti at PSU <[email protected] Sharan Salafia, Maria Edvige Ravasio, Sergio Campana, Paolo D’Avanzo, Boris Sbarufatti & Gianpiero Tagliaferri. it> D. L. Crossref. III. Sbarufatti (INAF-IASFPA), P. 4 ks after the BAT trigger. E. 11813 ). , GCN Circ. D. Markwardt (CRESST/GSFC/UMD) report on behalf of the Swift-XRT team: We have analysed 4. Sbarufatti (INAF-OAB/PSU), A. Sbarufatti (INAF-OAB/IASFPA) reports on behalf of the Swift-XRT team: We have analysed 6. (GCN Circ. Sbarufatti (INAF OAB/INAF IASF-PA) and C. Sbarufatti, V. name RA Dec 15–150 keV band 15–30 keV band 15–70 keV bandBoris Sbarufatti at INAF-OAB/IASFPA <boris. 2 ks and T+516. Burrows (PSU), [email protected] Sbarufatti at INAF-OAB/IASFPA <boris. 9 ks of XRT data for the Swift/BAT-detected burst: GRB110319B (Cummings et al. 9 ks exposure. Boris Sbarufatti; Stefano Ciprini; Jari Kotilainen [. Boris Sbarufatti at INAF-OAB/IASFPA <boris. Burst Advocate for this burst is B. it> B. (Sbarufatti et al. Beardmore (U. Rhaana L. Assuming the standard relativistic fireball model forSkip to main content Utility Menu. Mangano (INAF IASF-Pa), C. Copy reference. B. D'Ai (INAF-IASFPA), A. Page and Silvia Zane and A. 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. 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 XRT began observing GRB 080405 (Cummings et al. Melandri (INAF-OAB), B. 1S", "createdOn": 1507910607000, "circularId": 22010, "submitter": "Boris Sbarufatti at. N. Leicester), A. Description of the variables in the GRBweb catalogue. A. Boris Sbarufatti at INAF-IASF-Pa <sbarufatti@ifc. Oates (Uni. inaf. Page (U. GRB 090417B was an unusually long burst with a T 90 duration of at least 2130 s and a multi-peaked light curve at energies of 15-150 keV. C. Boris Sbarufatti at INAF-IASF-Pa <sbarufatti@ifc. Sbarufatti and V. , 2006Shaw et al. Sbarufatti, V. J. Kuin (UCL-MSSL), S Laha (GSFC/UMBC/CRESST) and A. , Mangano V. 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. Leicester) report on behalf of the Swift-XRT team: Swift-XRT has performed follow-up observations of the. H. Sbarufatti B. Boris Sbarufatti at INAF-IASF-Pa <sbarufatti@ifc. Gropp (PSU), J. Authors: Marco Landoni, Renato Falomo, Aldo Treves, Boris Sbarufatti. Download. it> B. The. P. L. sbarufatti@brera. Mangano, B. Melandri (INAF-OAB), B. 5. 7 ks after the trigger. 7687). Boris Sbarufatti at INAF-OAB/IASFPA <boris. Leicester) report on behalf of the Swift-XRT team Swift-XRT has performed follow up observations of GRB 210218A (Sbarufatti et al. 12335), from 82 s to 7. R. Page (U. Perley, W. Sbarufatti (INAF-OAB/IASFPA) and V. We aim to determine the redshift (or stringent lower limits) of a number of bright BL Lacs objects. La Parola, V. it> B. Sbarufatti (INAF-OAB/IASFPA), R. Castro-Tirado, Javier Gorosabel, Judith L. 1 ks. Sbarufatti (INAF-OAB/PSU), H. Maselli (INAF-IASFPA), A. inaf. Sbarufatti (INAF-OAB/PSU) and C. inaf. Boris Sbarufatti at INAF-OAB/IASFPA <boris. , & Falomo, R. it> S. Guidorzi (Univ. In the XRT field of view we detect a single faint. Brett Sholtis was a health reporter for WITF/Transforming Health until early 2023. Tweet. 9905). Download PDF Abstract: Aims. inaf. inaf. Overview; Fingerprint; Abstract. K. Sbarufatti, V. 11525), from 339 s to 30. P. inaf. 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. 4-3658}, author={Craig B. Evans (U. Boris Sbarufatti at PSU <bxs60@psu. N. it> B. Gehrels (GSFC), S. Mangano (INAF-IASFPA) on behalf of the Swift-XRT [email protected] paper argues that the Cow is a monster black hole shredding a. Kuin (UCL-MSSL), A. GCN Circ. D. A. Here’s how you knowUsing Webb’s spectacular sensitivity, scientists captured the first mid-infrared spectrum from space of a kilonova, which marked Webb’s first direct look at an individual heavy element from such an event. it> B. Content may be subject to copyright. The data consist of 642 s in. Leicester), C. Together they form a unique [email protected]@brera. Astronomy & Astrophysics; Research output: Contribution to journal › Article › peer-review. Evans (U. Sbarufatti (INAF OAB/INAF IASF-PA) , V. Sbarufatti, V. D'Avanzo (INAF-OAB), J. Stroh (PSU), D. 2002) and the possible host galaxy of GRB 090417B. 6 ks [email protected] ks after the trigger. La Parola (INAF-IASFPA), S. Lien (GSFC/UMBC), F. FRB 20121102A: images of the bursts and the varying radio counterpart. (INAF-IASFPA) report on behalf of the Swift Team: We have analyzed the Swift-XRT data of XRF 090702 (Paizis, et al. , Kotilainen, J. Mangano (INAF-IASF PA) report on behalf of the Swift-XRT team: We have analyzed the 3.