A dataset provided by the European Space Agency

Name: The isolated neutron star candidate RBS1223
Published: 2003-02-16T00:00:00Z

Proposal ID	009001
Title	The isolated neutron star candidate RBS1223
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0090010101
DOI	https://doi.org/10.5270/esa-2rbbhu5
Principal Investigator, PI	Dr Axel Schwope
Abstract	In the ROSAT Bright Survey (RBS) we have almost completely (>99\)identified the more than 2000 brightest high-galactic latitude sources from the ROSAT All-Sky Survey Bright Source Catalogue (1RXS). A smallnumber of sources has empty X-ray error boxes on POSS plates. ROSAT HRIfollow-up observations of RBS1223, a soft object with extreme X-ray to optical flux ratio, confirm a relatively bright X-ray source. Optical imaging down to 26 mag at Keck II reveals no optical counterpart. Chances are high that this is a new isolated neutron star (INS). We propose a 30 ksec observation with XMM in order to i) obtain a high-quality X-ray spectrum of the source and ii) search for possible periodicities.
Publications	The pulsed X-ray light curves of the isolated neutron star RBS1223 \|Schwope, A. D., Hambaryan, V., et al. \| A&A \| 441-597 \| 2005 \| 2005A&A...441..597S \| http://ui.adsabs.harvard.edu/#abs/2005A&A...441..597S Narrow absorption features in the co-added XMM-Newton RGS spectra of isolated neutron stars \|Hohle, M. M., Haberl, F., et al. \| MNRAS \| 419-1525 \| 2012 \| 2012MNRAS.419.1525H \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.419.1525H 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 A broad absorption feature in the X-ray spectrum of the isolated neutron star RBS1223 (1RXS J130848.6+212708) \|Haberl, F., Schwope, A. D., et al. \| A&A \| 403-19 \| 2003 \| 2003A&A...403L..19H \| http://ui.adsabs.harvard.edu/#abs/2003A&A...403L..19H AXPs and X-ray-dim isolated neutron stars: recent XMM-Newton and Chandra results \|Haberl, F., \| AdSpR \| 33-638 \| 2004 \| 2004AdSpR..33..638H \| http://ui.adsabs.harvard.edu/#abs/2004AdSpR..33..638H 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 The complex X-ray spectrum of the isolated neutron star RBS1223 \|Schwope, Axel D., Hambaryan, Valeri, et al. \| Ap&SS \| 308-619 \| 2007 \| 2007Ap&SS.308..619S \| http://ui.adsabs.harvard.edu/#abs/2007Ap&SS.308..619S 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 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 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 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 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 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 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	2001-12-31T03:03:07Z/2001-12-31T08:42:26Z
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	2003-02-16T00:00:00Z
Keywords	"optical counterpart", "keck ii reveals", "ii search", "XMM", "poss plates", "quality xray spectrum", "2000 brightest", "soft object", "optical flux ratio", "ROSAT", "galactic latitude sources", "rosat hri", "optical imaging"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Axel Schwope, 2003, 'The isolated neutron star candidate RBS1223', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-2rbbhu5