A dataset provided by the European Space Agency

Name: Generic ToO/DDT Proposal for AO16
Published: 2019-05-03T22:00:00Z

Proposal ID	081121
Title	Generic ToO/DDT Proposal for AO16
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0811210101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0811212701 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0811212801 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0811212901 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0811213001 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0811213301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0811213401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0811213501
DOI	https://doi.org/10.5270/esa-2vl4012
Principal Investigator, PI	Dr NORBERT SCHARTEL (PS)
Abstract	1) GW17081727) GW17081728) Swift J0243.6+612429) Swift J0243.6+612430) C2016 R2 PANSTARRS31) C2016 R2 PANSTARRS32) C2016 R2 PANSTARRS33) Fermi J1544-064934) Swift J1658.2-424235) PSR J1946+2052
Publications	The Binary Neutron Star Event LIGO/Virgo GW170817 160 Days after Merger: Synchrotron Emission across the Electromagnetic Spectrum \|Margutti, R., Alexander, K. D., et al. \| ApJ \| 856-18 \| 2018 \| 2018ApJ...856L..18M \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...856L..18M The evolution of the X-ray afterglow emission of GW 170817/ GRB 170817A in XMM-Newton observations \|D.Avanzo, P., Campana, S., et al. \| A&A \| 613-1 \| 2018 \| 2018A&A...613L...1D \| http://ui.adsabs.harvard.edu/#abs/2018A&A...613L...1D An XMM-Newton look at the strongly variable radio-weak BL Lac Fermi J1544-0639 \|Ursini, F., Bassani, L., et al. \| A&A \| 622-116 \| 2019 \| 2019A&A...622A.116U \| http://ui.adsabs.harvard.edu/#abs/2019A&A...622A.116U A long-lived neutron star merger remnant in GW170817: constraints and clues from X-ray observations \|Piro, L., Troja, E., et al. \| MNRAS \| 483-1912 \| 2019 \| 2019MNRAS.483.1912P \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.483.1912P Exploring the Interstellar Medium Using an Asymmetric X-Ray Dust Scattering Halo \|Jin, Chichuan, Ponti, Gabriele, et al. \| ApJ \| 875-157 \| 2019 \| 2019ApJ...875..157J \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...875..157J Two Years of Nonthermal Emission from the Binary Neutron Star Merger GW170817: Rapid Fading of the Jet Afterglow and First Constraints on the Kilonova Fastest Ejecta \|Hajela, A., Margutti, R., et al. \| ApJ \| 886-17 \| 2019 \| 2019ApJ...886L..17H \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...886L..17H Properties of jet and surrounding material of GW/GRB 170817A \|Ziaeepour, Houri, \| MNRAS \| 490-2822 \| 2019 \| 2019MNRAS.490.2822Z \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.490.2822Z A year in the life of GW 170817: the rise and fall of a structured jet from a binary neutron star merger \|Troja, E., van Eerten, H., et al. \| MNRAS \| 489-1919 \| 2019 \| 2019MNRAS.489.1919T \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.489.1919T Multi-wavelength observations of the BL Lac object Fermi J1544-0649: One year after its awakening \|Tam, P. H. T., Pal, P. S., et al. \| JHEAp \| 26-45 \| 2020 \| 2020JHEAp..26...45T \| http://ui.adsabs.harvard.edu/#abs/2020JHEAp..26...45T An underlying clock in the extreme flip-flop state transitions of the black hole transient Swift J1658.2-4242 \|Bogensberger, D., Ponti, G., et al. \| A&A \| 641-101 \| 2020 \| 2020A&A...641A.101B \| http://ui.adsabs.harvard.edu/#abs/2020A&A...641A.101B 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 First Multimessenger Observations of a Neutron Star Merger \|Margutti, Raffaella, Chornock, Ryan, \| ARA&A \| 59-155 \| 2021 \| 2021ARA&A..59..155M \| http://ui.adsabs.harvard.edu/#abs/2021ARA&A..59..155M The Panchromatic Afterglow of GW170817: The Full Uniform Data Set, Modeling, Comparison with Previous Results, and Implications \|Makhathini, S., Mooley, K. P., et al. \| ApJ \| 922-154 \| 2021 \| 2021ApJ...922..154M \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...922..154M Accurate flux calibration of GW170817: is the X-ray counterpart on the rise? \|Troja, E., O.Connor, B., et al. \| MNRAS \| 510-1902 \| 2022 \| 2022MNRAS.510.1902T \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.510.1902T The new age of Gamma Ray Bursts: physics and multi-messengers \|Ghisellini, G., Ghirlanda, G., et al. \| MmSAI \| 93-139 \| 2022 \| 2022MmSAI..93b.139G \| http://ui.adsabs.harvard.edu/#abs/2022MmSAI..93b.139G Impacts of symmetry energy slope on the oscillation frequencies of neutron stars with short-range correlation and admixed dark matter \|Hong, Bin, Ren, ZhongZhou, et al. \| CQGra \| 40-125007 \| 2023 \| 2023CQGra..40l5007H \| http://ui.adsabs.harvard.edu/#abs/2023CQGra..40l5007H The current state of disk wind observations in BHLMXBs through X-ray absorption lines in the iron band \|Parra, M., Petrucci, P. -O., et al. \| A&A \| 681-49 \| 2024 \| 2024A&A...681A..49P \| http://ui.adsabs.harvard.edu/#abs/2024A&A...681A..49P 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 Potential biases and prospects for the Hubble constant estimation via electromagnetic and gravitational-wave joint analyses \|Gianfagna, Giulia, Piro, Luigi, et al. \| MNRAS \| 528-2600 \| 2024 \| 2024MNRAS.528.2600G \| http://ui.adsabs.harvard.edu/#abs/2024MNRAS.528.2600G From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources \|Rodriguez, Antonio C., \| PASP \| 136-054201 \| 2024 \| 2024PASP..136e4201R \| http://ui.adsabs.harvard.edu/#abs/2024PASP..136e4201R 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	2017-12-29T18:19:47Z/2018-03-29T15:23:01Z
Version	19.17_20220121_1250
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	2019-05-03T22:00:00Z
Keywords	"swift j0243", "J0243.6", "swift j1658", "c2016 r2 panstarrs", "fermi j1544 0649", "psr j1946"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr NORBERT SCHARTEL openParPSclosePar, 2019, 'Generic ToO/DDT Proposal for AO16', 19.17_20220121_1250, European Space Agency, https://doi.org/10.5270/esa-2vl4012