A dataset provided by the European Space Agency

Name: Broad-band multifrequency variability of 3C 454.3 during a radio outburst
Published: 2008-06-22T00:00:00Z

Proposal ID	040170
Title	Broad-band multifrequency variability of 3C 454.3 during a radio outburst
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0401700201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0401700401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0401700501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0401700601
DOI	https://doi.org/10.5270/esa-rmvxjwn
Principal Investigator, PI	Dr Claudia M. Raiteri
Abstract	In spring 2005 the blazar 3C 454.3 was observed exceptionally bright at opticaland X-ray frequencies. In late August the source was bright in the mm band, andnow the flux increase detected in the cm band is likely the start of a long-termradio outburst. Many low-energy data have been collected by the WEBT consortium,revealing strong spectral changes. We propose to observe this source withXMM-Newton in different phases of the radio outburst. Coordinated observationsin the radio, NIR, and optical bands will be carried out by the WEBT, andgamma-ray data will be provided by the AGILE satellite. All these data willcomplement those acquired during the optical outburst and will allow to shedlight on the variability mechanisms as well as on the jet structure and geometry.
Publications	The XMM Cluster Survey: optical analysis methodology and the first data release \|Mehrtens, Nicola, Romer, A. Kathy, et al. \| MNRAS \| 423-1024 \| 2012 \| 2012MNRAS.423.1024M \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.423.1024M WEBT and XMM-Newton observations of 3C 454.3 during the post-outburst phase. Detection of the little and big blue bumps \|Raiteri, C. M., Villata, M., et al. \| A&A \| 473-819 \| 2007 \| 2007A&A...473..819R \| http://ui.adsabs.harvard.edu/#abs/2007A&A...473..819R A new activity phase of the blazar 3C 454.3. Multifrequency observations by the WEBT and XMM-Newton in 2007-2008 \|Raiteri, C. M., Villata, M., et al. \| A&A \| 491-755 \| 2008 \| 2008A&A...491..755R \| http://ui.adsabs.harvard.edu/#abs/2008A&A...491..755R The XMM Cluster Survey: X-ray analysis methodology \|Lloyd-Davies, E. J., Romer, A. Kathy, et al. \| MNRAS \| 418-14 \| 2011 \| 2011MNRAS.418...14L \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.418...14L Classification of X-Ray Sources in the XMM-Newton Serendipitous Source Catalog \|Lin, Dacheng, Webb, Natalie A., \| ApJ \| 756-27 \| 2012 \| 2012ApJ...756...27L \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...756...27L An XMM-Newton Survey of the Soft X-Ray Background. II. An All-Sky Catalog of Diffuse O VII and O VIII Emission Intensities \|Henley, David B., Shelton, Robin L., \| ApJS \| 202-14 \| 2012 \| 2012ApJS..202...14H \| http://ui.adsabs.harvard.edu/#abs/2012ApJS..202...14H The diversity of quasars unified by accretion and orientation \|Shen, Yue, Ho, Luis C., \| Natur \| 513-210 \| 2014 \| 2014Natur.513..210S \| http://ui.adsabs.harvard.edu/#abs/2014Natur.513..210S Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift \|Yershov, V. N., \| Ap&SS \| 354-97 \| 2014 \| 2014Ap&SS.354...97Y \| http://ui.adsabs.harvard.edu/#abs/2014Ap&SS.354...97Y Blazar 3C 454.3 in Outburst and Quiescence during 2005-2007: Two Variable Synchrotron Emission Peaks \|Ogle, Patrick M., Wehrle, Ann E., et al. \| ApJS \| 195-19 \| 2011 \| 2011ApJS..195...19O \| http://ui.adsabs.harvard.edu/#abs/2011ApJS..195...19O The long-lasting activity of 3C 454.3. GASP-WEBT and satellite observations in 2008-2010 \|Raiteri, C. M., Villata, M., et al. \| A&A \| 534-87 \| 2011 \| 2011A&A...534A..87R \| http://ui.adsabs.harvard.edu/#abs/2011A&A...534A..87R Sunyaev-Zel.dovich effect or not? Detecting the main foreground effect of most galaxy clusters \|Xiao, Weike, Chen, Chen, et al. \| MNRAS \| 432-41 \| 2013 \| 2013MNRAS.432L..41X \| http://ui.adsabs.harvard.edu/#abs/2013MNRAS.432L..41X Peak of spectral energy distribution plays an important role in intra-day variability of blazars? \|Gupta, Alok C., Kalita, Nibedita, et al. \| MNRAS \| 462-1508 \| 2016 \| 2016MNRAS.462.1508G \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.462.1508G The Interaction of the Fermi Bubbles with the Milky Way.s Hot Gas Halo \|Miller, Matthew J., Bregman, Joel N., \| ApJ \| 829-9 \| 2016 \| 2016ApJ...829....9M \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...829....9M The Million Optical - Radio/X-ray Associations (MORX) Catalogue \|Flesch, Eric W., \| PASA \| 33-52 \| 2016 \| 2016PASA...33...52F \| http://ui.adsabs.harvard.edu/#abs/2016PASA...33...52F Signature of inverse Compton emission from blazars \|Gaur, Haritma, Mohan, Prashanth, et al. \| MNRAS \| 473-3638 \| 2018 \| 2018MNRAS.473.3638G \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.473.3638G Anisotropy of the galaxy cluster X-ray luminosity-temperature relation \|Migkas, Konstantinos, Reiprich, Thomas H., \| A&A \| 611-50 \| 2018 \| 2018A&A...611A..50M \| http://ui.adsabs.harvard.edu/#abs/2018A&A...611A..50M The 3CR Chandra Snapshot Survey: Extragalactic Radio Sources with Redshifts between 1 and 1.5 \|Stuardi, C., Missaglia, V., et al. \| ApJS \| 235-32 \| 2018 \| 2018ApJS..235...32S \| http://ui.adsabs.harvard.edu/#abs/2018ApJS..235...32S The XMM Cluster Survey: Present status and latest results \|Viana, P. T. P., Mehrtens, N., et al. \| AN \| 334-462 \| 2013 \| 2013AN....334..462V \| http://ui.adsabs.harvard.edu/#abs/2013AN....334..462V X-ray Emission of ICRF Sources \|Voitsekhovskiy, V. V., Tugay, A. V., et al. \| OAP \| 31-47 \| 2018 \| 2018OAP....31...47V \| http://ui.adsabs.harvard.edu/#abs/2018OAP....31...47V Testing emergent gravity on galaxy cluster scales \|Tamosiunas, Andrius, Bacon, David, et al. \| JCAP \| 5-53 \| 2019 \| 2019JCAP...05..053T \| http://ui.adsabs.harvard.edu/#abs/2019JCAP...05..053T Chandra Follow-up of the SDSS DR8 Redmapper Catalog Using the MATCha Pipeline \|Hollowood, Devon L., Jeltema, Tesla, et al. \| ApJS \| 244-22 \| 2019 \| 2019ApJS..244...22H \| http://ui.adsabs.harvard.edu/#abs/2019ApJS..244...22H Stellar mass as a galaxy cluster mass proxy: application to the Dark Energy Survey redMaPPer clusters \|Palmese, A., Annis, J., et al. \| MNRAS \| 493-4591 \| 2020 \| 2020MNRAS.493.4591P \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.493.4591P An X-Ray- and SZ-bright Diffuse Source toward M31: A Local Hot Bridge \|Qu, Zhijie, Huang, Rui, et al. \| ApJ \| 907-14 \| 2021 \| 2021ApJ...907...14Q \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...907...14Q Classification of 4XMM-DR9 sources by machine learning \|Zhang, Yanxia, Zhao, Yongheng, \| MNRAS \| 503-5263 \| 2021 \| 2021MNRAS.503.5263Z \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.5263Z Probing the physical properties of the intergalactic medium using blazars \|Dalton, Tony, Morris, Simon L., et al. \| MNRAS \| 508-1701 \| 2021 \| 2021MNRAS.508.1701D \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.508.1701D The Solar Cycle Temporal Variation of the Solar Wind Charge Exchange X-Ray Lines \|Qu, Zhijie, Koutroumpa, Dimitra, et al. \| ApJ \| 930-21 \| 2022 \| 2022ApJ...930...21Q \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...930...21Q Study of Intra-Day Flux Distributions of Blazars Using XMM-Newton Satellite \|Wani, Kiran, Gaur, Haritma, \| Univ \| 8-578 \| 2022 \| 2022Univ....8..578W \| http://ui.adsabs.harvard.edu/#abs/2022Univ....8..578W The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O VII, O VIII, and Fe L-shell Transitions \|Pan, Zeyang, Qu, Zhijie, et al. \| ApJS \| 271-62 \| 2024 \| 2024ApJS..271...62P \| http://ui.adsabs.harvard.edu/#abs/2024ApJS..271...62P Robust constraints on feebly interacting particles using XMM-Newton \|Luque, Pedro De la Torre, Balaji, Shyam, \| PhRvD \| 109-L101305 \| 2024 \| 2024PhRvD.109j1305L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j1305L Multimessenger search for electrophilic feebly interacting particles from supernovae \|Luque, Pedro De la Torre, Balaji, Shyam, \| PhRvD \| 109-103028 \| 2024 \| 2024PhRvD.109j3028L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j3028L Importance of Cosmic-Ray Propagation on Sub-GeV Dark Matter Constraints \|De la Torre Luque, Pedro, Balaji, Shyam, \| ApJ \| 968-46 \| 2024 \| 2024ApJ...968...46D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...968...46D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2006-07-02T21:25:07Z/2007-05-31T17:24:10Z
Version	17.56_20190403_1200
Mission Description	The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs second cornerstone of the Horizon 2000 Science Programme. It carries 3 high throughput X-ray telescopes with an unprecedented effective area, and an optical monitor, the first flown on a X-ray observatory. The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations. Since Earths atmosphere blocks out all X-rays, only a telescope in space can detect and study celestial X-ray sources. The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community, applying for observational periods on a competitive basis.
Creator Contact	https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk
Date Published	2008-06-22T00:00:00Z
Keywords	"optical bands", "XMM-Newton", "xmm newton", "gamma ray data", "jet structure", "low energy data", "term radio outburst", "blazar 3c 454", "radio outburst", "agile satellite", "XMM", "shed light", "mm band", "3c 454", "optical outburst", "variability mechanisms", "spring 2005", "webt consortium", "xray frequencies", "cm band"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Claudia M. Raiteri, 2008, 'Broad-band multifrequency variability of 3C 454.3 during a radio outburst', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-rmvxjwn