IBIS: The Imager on-board INTEGRAL

By Pietro Ubertini, F. Lebrun, G. Cocco, A. Bazzano, A. Bird, K. Broenstad, A. Goldwurm, G. Rosa, C. Labanti, P. Laurent and 10 more. 2003

851 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/426b59384493463fda6bce342837aa1b05647ae9

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Citations in the corpus

Polarization of the Crab Pulsar and Nebula as Observed by the INTEGRAL/IBIS Telescope (2008, background): “With its double layer of finely pixellated detectors (Ubertini et al. 2003), the IBIS telescope on board the Integral satellite is well suited for polarimetry studies, between 200 keV and 5 MeV.”
THE FOURTH IBIS/ISGRI SOFT GAMMA-RAY SURVEY CATALOG (2009, background): “Instrumental details and sensitivity can be found in Ubertini et al. (2003).”
INTEGRAL Detection of the First Prompt Gamma-Ray Signal Coincident with the Gravitational-wave Event GW170817 (2017, background): “…2003) is an observatory with multiple instruments: a gamma-ray spectrometer (20 keV–8MeV, SPI; Vedrenne et al. 2003), an imager (15 keV–10MeV, IBIS; Ubertini et al. 2003), an X-ray monitor (3–35 keV, JEM-X; Lund et al. 2003), and an optical monitor (V band, Optical Monitoring Camera (OMC);…”
INTEGRAL observations of the cosmic X-ray background in the 5–100 keV range via occultation by the Earth (2006, methodology): “A pure statistical error (joint fit to JEM-X, IBIS/ISGRI and SPI data) in the normalization of the CXB component is ∼1%.”
The 105-Month Swift-BAT All-sky Hard X-Ray Survey (2018, methodology): “In the past decades, the International Gamma-Ray Astrophysics Laboratory (INTEGRAL, Winkler et al. 2003) has monitored hard X-ray sources using the Imager on Board the INTEGRAL Satellite (IBIS, Ubertini et al. 2003).”
The Third IBIS/ISGRI Soft Gamma-Ray Survey Catalog (2006, methodology): “The IBIS imaging instrument is optimised for survey work with a large (30◦) field of view with excellent imaging and spectroscopy capability (Ubertini et al. 2003), and has formed the basis of several previous INTEGRAL surveys.”
INTEGRAL/IBIS all-sky survey in hard X-rays (2007, background): “We used data from the ISGRI detector of the IBIS telescope, which is well suited for carrying out imaging surveys in hard X-rays.”
INTEGRAL observations of recurrent fast X-ray transient sources (2005, background): “…published by EDP Sciences and available at http://www.edpsciences.org/aa or http://dx.doi.org/10.1051/0004-6361:20053103 The IBIS/ISGRI detector (Ubertini et al. 2003; Lebrun et al. 2003) on board the INTEGRAL satellite (Winkler et al. 2003) is particularly suited to detect new or already known…”
The INTEGRAL/IBIS scientific data analysis (2003, methodology): “For the IBIS standard mode (Ubertini et al. 2003, Di Cocco et al. 2003) the following data sets are provided, for each elementary observation interval (science window) which corresponds to a constant pointing or slew satellite mode: - ISGRI event list: position, arrival time, pulse-height channel,…”
Hard X-ray view of the past activity of Sgr A in a natural Compton mirror (2004, background): “The several-fold increased effective area of the telescope IBIS (Ubertini et al. 2003) compared to the previous spaceborne hard X-ray imager GRANAT/SIGMA, opens up a possibility to study hard X-ray sources located in crowded regions of the sky, at flux levels (above 20keV) down to 1 mCrab (Revnivtse”
Multi-messenger observations of a binary neutron star merger (2017, background): “Wavelength References GROND/– 2017 Aug 20 04:49:21 2.67 optical, IR GCN 21608, Chen et al. (2017) VIRT/– 2017 Aug 20 05:27:49 2.7 optical GCN 21609, Gendre et al. (2017) SALT/– 2017 Aug 20 06:14:37 2.73 optical GCN 21610, Shara et al. (2017) Swift/XRT 2017 Aug 20 08:42:40 2.83 x-ray GCN 21612, Evans”
Discovery of Luminous Pulsed Hard X-Ray Emission from Anomalous X-Ray Pulsars 1RXS J1708–4009, 4U 0142+61, and 1E 2259+586 by INTEGRAL and RXTE (2006, background): “…(INTEGRAL) spacecraft (Winkler et al. 2003), launched 2002 October 17, carries two main gamma-ray instruments: the high angular resolution Imager on Board the INTEGRAL Satellite ( IBIS; Ubertini et al. 2003) and the high energy resolution Spectrometer on INTEGRAL (SPI; Vedrenne et al. 2003).”
Probing clumpy stellar winds with a neutron star (2007, methodology): “In this paper we aim at studying the clumping of stellar wind in HMXB using the hard X-ray variability observed by the IBIS/ISGRI instrument (Ubertini et al. 2003; Lebrun et al. 2003) on board the INTErnational GammaRay Astrophysics Laboratory (INTEGRAL, Winkler et al. 2003) which could be used to…”
THE SPACE DENSITY OF COMPTON-THICK ACTIVE GALACTIC NUCLEUS AND THE X-RAY BACKGROUND (2009, methodology): “Using the IBIS coded-mask telescope (Ubertini et al. 2003), INTEGRAL surveyed ∼80% of the sky down to a flux of 5 mCrab in the 17-60 keV.”
INTEGRAL Discovery of a Burst with Associated Radio Emission from the Magnetar SGR 1935+2154 (2020, methodology): “Our results are based mainly on data obtained with the Imager on-board INTEGRAL (IBIS) instrument (Ubertini et al. 2003) that provides images in a 30×30 deg2 field of view thanks to a coded mask coupled to two detector arrays: INTEGRAL Soft Gamma Ray Imager (ISGRI) and Pixellated Imaging Caesium…”
ISGRI: The INTEGRAL soft gamma-ray imager (2003, neutral): “A spectral coverage from several tens of keV to several MeV was one of the main requirements for the INTEGRAL imager IBIS (Ubertini et al. 2003).”
The INTEGRAL Science Data Centre (ISDC) (2001, methodology): “There is approximatelyone burst per day in the anticoincidence shield data and one per month in the field of view of IBIS.”
WATCHDOG: A COMPREHENSIVE ALL-SKY DATABASE OF GALACTIC BLACK HOLE X-RAY BINARIES (2015, background): “One of which is the Integral Soft Gamma-Ray Imager (IBIS/ISGRI; Ubertini et al. 2003), which has a primary energy range of 20–60 keV, an energy resolution of 8% at 100 keV, and a field of view of 29 square degrees.”
An Embedded X-Ray Source Shines through the Aspherical AT 2018cow: Revealing the Inner Workings of the Most Luminous Fast-evolving Optical Transients (2018, methodology): “…with the latest available calibration files, we extracted the hard X-ray spectrum from the ISGRI detector (Lebrun et al. 2003) on the IBIS instrument (Ubertini et al. 2003) of INTEGRAL (Winkler et al. 2003) for each of the ∼2 ks long individual pointing of the telescope dithering around the source.”