A dataset provided by the European Space Agency

Name: HIGH RESOLUTION SPECTROSCOPY AND TIMING OF THE ISOLATED NEUTRON STAR RBS1774
Published: 2005-07-01T00:00:00Z

Proposal ID	020115
Title	HIGH RESOLUTION SPECTROSCOPY AND TIMING OF THE ISOLATED NEUTRON STAR RBS1774
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0201150101
DOI	https://doi.org/10.5270/esa-dkab7qb
Principal Investigator, PI	Dr SILVIA ZANE
Abstract	Isolated neutron stars hold the key to understand the structure and evolution ofNSs and promise insights into the behaviour of matter at ultra-high densities.The seven ROSAT INSs identified to date offer an unique opportunity in thisrespect thanks to their clean thermal emission originating directly from thestar surface. The aim is to obtain a high quality spectrum of the last of theROSAT INS candidates to be studied in detail, RBS 1774. This will provide anaccurate position, essential to allow an unambiguous identification of theoptical counterpart; pin down the temperature of the surface emission; revealany prominent spectral features or magnetospheric non-thermal component; findany pulsations to a limit of 2% semiamplitude.
Publications	XMM-Newton Detection of Pulsations and a Spectral Feature in the X-Ray Emission of the Isolated Neutron Star 1RXS J214303.7+065419/RBS 1774 \|Zane, S., Cropper, M., et al. \| ApJ \| 627-397 \| 2005 \| 2005ApJ...627..397Z \| http://ui.adsabs.harvard.edu/#abs/2005ApJ...627..397Z Constraining the Spin-Down of the Nearby Isolated Neutron Star RX J2143.0+0654 \|Kaplan, D. L., van Kerkwijk, M. H., \| ApJ \| 692-62 \| 2009 \| 2009ApJ...692L..62K \| http://ui.adsabs.harvard.edu/#abs/2009ApJ...692L..62K The XMM-Newton serendipitous survey. V. The Second XMM-Newton serendipitous source catalogue \|Watson, M. G., Schroder, A. C., et al. \| A&A \| 493-339 \| 2009 \| 2009A&A...493..339W \| http://ui.adsabs.harvard.edu/#abs/2009A&A...493..339W Statistical evaluation of the flux cross-calibration of the XMM-Newton EPIC cameras \|Mateos, S., Saxton, R. D., et al. \| A&A \| 496-879 \| 2009 \| 2009A&A...496..879M \| http://ui.adsabs.harvard.edu/#abs/2009A&A...496..879M 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 New Optical/Ultraviolet Counterparts and the Spectral Energy Distributions of Nearby, Thermally Emitting, Isolated Neutron Stars \|Kaplan, D. L., Kamble, A., et al. \| ApJ \| 736-117 \| 2011 \| 2011ApJ...736..117K \| http://ui.adsabs.harvard.edu/#abs/2011ApJ...736..117K The plasma emission model of RBS1774 \|Chkheidze, N., \| A&A \| 527-2 \| 2011 \| 2011A&A...527A...2C \| http://ui.adsabs.harvard.edu/#abs/2011A&A...527A...2C VLT/FORS2 observations of the optical counterpart of the isolated neutron star RBS 1774 \|Mignani, R. P., Zane, S., et al. \| A&A \| 530-39 \| 2011 \| 2011A&A...530A..39M \| http://ui.adsabs.harvard.edu/#abs/2011A&A...530A..39M The magnificent seven: magnetic fields and surface temperature distributions \|Haberl, Frank, \| Ap&SS \| 308-181 \| 2007 \| 2007Ap&SS.308..181H \| http://ui.adsabs.harvard.edu/#abs/2007Ap&SS.308..181H An All-Sky Atlas of Radio/X-ray Associations \|Flesch, E., \| PASA \| 27-283 \| 2010 \| 2010PASA...27..283F \| http://ui.adsabs.harvard.edu/#abs/2010PASA...27..283F Accurate X-ray position and multiwavelength observations of the isolated neutron star RBS1774 \|Rea, N., Torres, M. A. P., et al. \| MNRAS \| 379-1484 \| 2007 \| 2007MNRAS.379.1484R \| http://ui.adsabs.harvard.edu/#abs/2007MNRAS.379.1484R Unveiling the thermal and magnetic map of neutron star surfaces though their X-ray emission: method and light-curve analysis \|Zane, Silvia, Turolla, Roberto, \| MNRAS \| 366-727 \| 2006 \| 2006MNRAS.366..727Z \| http://ui.adsabs.harvard.edu/#abs/2006MNRAS.366..727Z XMM-Newton observations of the isolated neutron star 1RXS J214303.7+065419/RBS1774 \|Cropper, Mark, Zane, Silvia, et al. \| Ap&SS \| 308-161 \| 2007 \| 2007Ap&SS.308..161C \| http://ui.adsabs.harvard.edu/#abs/2007Ap&SS.308..161C The isolated neutron star RBS1774 revisited. Revised XMM-Newton X-ray parameters and an optical counterpart from deep LBT-observations \|Schwope, A. D., Erben, T., et al. \| A&A \| 499-267 \| 2009 \| 2009A&A...499..267S \| http://ui.adsabs.harvard.edu/#abs/2009A&A...499..267S 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 XMM-Newton serendipitous ultraviolet source survey catalogue \|Page, M. J., Brindle, C., et al. \| MNRAS \| 426-903 \| 2012 \| 2012MNRAS.426..903P \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.426..903P Cross-correlation of the 2XMMi catalogue with Data Release 7 of the Sloan Digital Sky Survey \|Pineau, F.-X., Motch, C., et al. \| A&A \| 527-126 \| 2011 \| 2011A&A...527A.126P \| http://ui.adsabs.harvard.edu/#abs/2011A&A...527A.126P Exploring X-ray and radio emission of type 1 AGN up to z virgul 2.3 \|Ballo, L., Heras, F. J. H., et al. \| A&A \| 545-66 \| 2012 \| 2012A&A...545A..66B \| http://ui.adsabs.harvard.edu/#abs/2012A&A...545A..66B Unifying the observational diversity of isolated neutron stars via magneto-thermal evolution models \|Vigano, D., Rea, N., et al. \| MNRAS \| 434-123 \| 2013 \| 2013MNRAS.434..123V \| http://ui.adsabs.harvard.edu/#abs/2013MNRAS.434..123V 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 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 Ensemble X-ray variability of active galactic nuclei. II. Excess variance and updated structure function \|Vagnetti, F., Middei, R., et al. \| A&A \| 593-55 \| 2016 \| 2016A&A...593A..55V \| http://ui.adsabs.harvard.edu/#abs/2016A&A...593A..55V 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 Magnetic fields in neutron stars \|Vigano, Daniele, \| PhDT \| 0-7 \| 2013 \| 2013PhDT.........7V \| http://ui.adsabs.harvard.edu/#abs/2013PhDT.........7V Narrow phase-dependent features in X-ray dim isolated neutron stars: a new detection and upper limits \|Borghese, A., Rea, N., et al. \| MNRAS \| 468-2975 \| 2017 \| 2017MNRAS.468.2975B \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.468.2975B The Magnificent Seven in the dusty prairie \|Posselt, B., Popov, S. B., et al. \| Ap&SS \| 308-171 \| 2007 \| 2007Ap&SS.308..171P \| http://ui.adsabs.harvard.edu/#abs/2007Ap&SS.308..171P 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 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 Cyclotron lines in highly magnetized neutron stars \|Staubert, R., Trumper, J., et al. \| A&A \| 622-61 \| 2019 \| 2019A&A...622A..61S \| http://ui.adsabs.harvard.edu/#abs/2019A&A...622A..61S Universal detection of high-temperature emission in X-ray isolated neutron stars \|Yoneyama, Tomokage, Hayashida, Kiyoshi, et al. \| PASJ \| 71-17 \| 2019 \| 2019PASJ...71...17Y \| http://ui.adsabs.harvard.edu/#abs/2019PASJ...71...17Y 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 Hard X-Ray Excess from the Magnificent Seven Neutron Stars \|Dessert, Christopher, Foster, Joshua W., \| ApJ \| 904-42 \| 2020 \| 2020ApJ...904...42D \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...904...42D 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 Axion Emission Can Explain a New Hard X-Ray Excess from Nearby Isolated Neutron Stars \|Buschmann, Malte, Co, Raymond T., et al. \| PhRvL \| 126-21102 \| 2021 \| 2021PhRvL.126b1102B \| http://ui.adsabs.harvard.edu/#abs/2021PhRvL.126b1102B 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 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 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 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	2004-05-31T15:27:48Z/2004-05-31T23:55:17Z
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	2005-07-01T00:00:00Z
Keywords	"unambiguous identification", "resolution spectroscopy", "prominent spectral", "optical counterpart", "magnetospheric nonthermal component", "rosat inss", "rosat ins candidates", "quality spectrum", "surface emission", "clean thermal emission", "promise insights", "star surface", "ROSAT", "rbs 1774"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr SILVIA ZANE, 2005, 'HIGH RESOLUTION SPECTROSCOPY AND TIMING OF THE ISOLATED NEUTRON STAR RBS1774', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-dkab7qb