about
An accreting pulsar with extreme properties drives an ultraluminous x-ray source in NGC 5907.The XMM-Newton Bright Serendipitous Survey: First Extragalactic ResultsThe XMM-NewtonHBS28 sample: Studying the obscuration in hard X-ray selected AGNsA hard medium survey with ASCAXMM-Newtonobservations reveal AGN in apparently normal galaxiesBL Lacertae: Complex spectral variability and rapid synchrotron flare detected with BeppoSAXThe extended medium sensitivity survey distant cluster sample - X-ray data and interpretation of the luminosity evolutionThe luminosity function and cosmological evolution of X-ray-selected BL Lacertae objectsThe number count distribution for X-ray-selected BL Lacertae objects and constraints on the luminosity functionMS 1603.6+2600, an unusual X-ray selected binary system at high galactic latitudeA cooling flow in a high-redshift, X-ray-selected cluster of galaxiesBL Lac objects from the extended medium sensitivity survey: The surface densityThe optical and radio properties of X-ray selected Bl Lacertae ObjectsA red envelope around a dominant elliptical galaxy in an X-ray selected poor clusterBeppoSAXobservations of 1-Jy BL Lacertae objects - IBeppoSAX observations of 1 Jy BL lacertae objectsWhat can BeppoSAX tell us about X-ray spectra of BL Lacs?Radio afterglows of a complete sample of bright Swift GRBs: predictions from present days to the SKA eraThe changing look of PKS 2149-306A sample of X-ray emitting normal galaxies from the BMW–HRI CatalogueThe European Large‐AreaInfrared Space ObservatorySurvey V: ABeppoSAXHard X‐Ray Survey of the S1 RegionBeppoSAX observations of 1-Jy BL Lacertae objects -- IIA pilot study for the creation of a large BL Lac sampleAn X-ray and optical study of the cluster A33The last gift of BeppoSAX: PDS observations of the two blazars 1ES 0507-040 and PKS 1229-021The BL Lacertae objects OQ 530 and S5 0716+714. Simultaneous observations in the X-rays, radio, optical and TeV bandsBeppoSAX spectral survey of BL Lacs – New spectra and resultsHard synchrotron BL lacs: The case of 1ES 1101-232Extreme synchrotron BL Lac objects. Stretching the blazar sequenceThe 0.1-200 keV spectrum of the blazar PKS 2005-489 during an active stateInvestigating early-type galaxy evolution with a multiwavelength approach – I. X-ray properties of 12 galaxies observed with Swift and XMM–NewtonAre jet ubiquitous in ULXs?NGC 2276: a remarkable galaxy with a large number of ultraluminous X-ray sourcesSpectral variability in Swift and Chandra observations of the ultraluminous source NGC 55 ULX1Ultraluminous X-ray sources: a deeper insight into their spectral evolutionX-ray variability and energy spectra from NGC 5408 X–1 with XMM–NewtonChandra observations of the collisional ring galaxy NGC 922Hot gas in groups: NGC 5328 and the intriguing case of NGC 4756 withXMM-NewtonSeyfert’s Sextet: where is the gas?Simultaneous X-ray and optical observations of true type 2 Seyfert galaxies
P50
Q38951180-6EAFFED8-5799-4F09-8AB2-140D89A39DA5Q57676363-2395DC9B-2802-4B83-ABD8-407C50956034Q57676375-1A16F463-2E64-44B4-9DC9-5B12427B7F51Q57676380-22749834-4DFD-4A0E-A2CC-B9BF9FE0B7E9Q57676382-26E7521B-E20C-400E-A081-8ABF73C47E2EQ58073939-8715F240-04D6-4FA5-8F73-305167F3E021Q58908557-37FEBE86-6017-4608-A930-46CE3ADFB719Q58908593-0BCDF293-89C6-42BC-A490-F1447FAF17C8Q58908596-53592781-71CD-49A3-95D9-B83D21C018A6Q58908604-1C2378E6-FF8D-4E18-8298-716F5A3105FAQ58908616-F2049851-AC42-423E-B385-AB1CAACAE11FQ58908622-D92E02BD-2143-4FB5-BDE4-74EB49C309A1Q58908628-6640E047-0063-4DDD-B32A-8D659B90EE3AQ58909927-48C6F08C-C81F-4E6B-B291-E6029A75E0BEQ58912397-01842250-842F-481B-B880-63475128BCF3Q58912465-063E5010-3823-4C97-8F03-E7AF9A4DC246Q58912477-E68E023E-DB86-4285-881A-FB3F098A7E9FQ58913098-8B061794-A7B1-40AB-9978-D355C4200896Q58913304-ECCEF980-2C16-463A-9411-D72C8E7D28C5Q58913627-D4466137-91EF-4A6A-BDF2-2843BC7A5A01Q58913860-D0C18F8E-B33C-4B4E-908E-BCBB0455474FQ58914111-E299FEB1-7680-44CB-9462-871B5D66C985Q58923663-A422E7FE-2637-4010-92DF-7139D4C94270Q58982959-34E2CB4E-E6AE-4D55-AD93-BA65C7376FC6Q58983624-F5784090-FADA-4A88-904E-17F824FBF2D0Q58983708-C1240472-26B3-450D-825A-ED179201CFE5Q58983760-1711D023-60D9-4005-AC7F-55BF84E58182Q58983773-9A7F8137-D822-4267-8996-3AFFE1731E88Q58983846-01D9A8A8-2F5A-426D-A136-E67BB50C1198Q58983857-A1C42DA4-5F19-4392-AFF7-742964447986Q58984156-070155C7-E4A4-468E-835C-B3116BC6F726Q58984162-EC9E5608-DA95-4326-8158-B8FCF8EFDE29Q58984169-668258D7-EBC1-4286-9327-3E574E5F65B1Q58984175-1ACCDE29-70B2-47E9-BB43-10FEBC2D67C3Q58984181-FF85402E-ADCC-4967-BA48-957819898EC1Q58984187-235AF2E1-F8C8-44EC-B3DC-34F72F1B050EQ58984194-7CDD1FDE-DE90-418D-8B24-BAF37D36D2AEQ58984200-513B7FC2-54CC-40D5-86F0-73CF6C5A0723Q58984208-883FEFA3-D364-4F15-B8E9-F3C97BFC1E35Q58984214-E7C25E3E-F545-4BCE-A92E-505416692F41
P50
description
researcher ORCID ID = 0000-0001-5840-9835
@en
wetenschapper
@nl
name
Anna Wolter
@ast
Anna Wolter
@en
Anna Wolter
@es
Anna Wolter
@nl
type
label
Anna Wolter
@ast
Anna Wolter
@en
Anna Wolter
@es
Anna Wolter
@nl
altLabel
A. Wolter
@en
prefLabel
Anna Wolter
@ast
Anna Wolter
@en
Anna Wolter
@es
Anna Wolter
@nl
P106
P1153
56269191000
7005563659
P21
P31
P496
0000-0001-5840-9835