about
A variable absorption feature in the X-ray spectrum of a magnetar.Confirmation of X-ray absorption by warm-hot intergalactic medium in the Sculptor wallDark matter–baryons separation at the lowest mass scale: the Bullet Group★Molecular gas in the X-ray bright group NGC 5044 as revealed by ALMAA phase-variable absorption feature in the X-ray spectrum of the magnetar SGR 0418+5729Dark matter line emission constraints from NuSTAR observations of the Bullet clusterANuSTAROBSERVATION OF THE CENTER OF THE COMA CLUSTERNuSTAROBSERVATIONS OF THE BULLET CLUSTER: CONSTRAINTS ON INVERSE COMPTON EMISSIONCLASH-x: a comparison of lensing and X-ray techniques for measuring the mass profiles of galaxy clustersThe XXL survey: First results and futureThe XXL SurveyOn the Connection between Turbulent Motions and Particle Acceleration in Galaxy ClustersStudying the WHIM content of large-scale structures along the line of sight to H 2356-309NewXMM-Newtonobservation of the Phoenix cluster: properties of the cool coreThe evolution of the spatially resolved metal abundance in galaxy clusters up toz= 1.4Gas clumping in galaxy clustersThe stripping of a galaxy group diving into the massive cluster A2142Abell 2142 at large scales: An extreme case for sloshing?Self-similarity of temperature profiles in distant galaxy clusters: the quest for a universal lawThe gas distribution in the outer regions of galaxy clustersAnXMM-Newtonspatially-resolved study of metal abundance evolution in distant galaxy clustersBack and forth from cool core to non-cool core: clues from radio halosX-ray observations of PKS 0745-191 at the virial radius: are we there yet?Gas temperature profiles in galaxy clusters with Swift XRT: observations and capabilities to map nearR200Mass profiles andc − MDMrelation in X-ray luminous galaxy clusters (Corrigendum)Mass profiles andc − MDMrelation in X-ray luminous galaxy clustersNon-thermal emission in the core of Perseus: results from a long XMM-Newton observationMerging Clusters in the Core of Superclusters: A Multiwavelength ViewTemperature and metallicity maps in cool core clusters of galaxiesAnswering a SAX question: Ni and Fe abundances in the core of the Perseus clusterNi Abundance in the Core of the Perseus Cluster: An Answer to the Significance of Resonant ScatteringXMM-Newtonobservation of the interacting cluster Abell 3528Abundance Gradients and the Role of Supernovae in M87Cold fronts and metal anisotropies in the X-ray cool core of the galaxy cluster Zw 1742+3306Updates on the background estimates for the X-IFU instrument onboard of the ATHENA missionThe XXL survey XV: evidence for dry merger driven BCG growth in XXL-100-GC X-ray clustersConstraints on the winds of hot subdwarf stars from X-ray observations of two sdB binaries with compact companions: CD -30 11223 and PG 1232-136The XXL SurveyThe XXL SurveyThe XXL Survey
P50
Q45023597-8A30CB5D-06A9-4FD6-BD76-0E12C9CC80D0Q53953482-307187B9-50C1-4EAE-A28A-CCB81B4F72D5Q56446430-E808929B-5265-4EFC-87B3-E46CADA3B50BQ56914442-00C4853C-1FAC-4D55-A13B-7E8BAC5B4D75Q56949297-9D1C09AA-EB5D-4F0F-999A-ABB13D32FA0EQ57444962-3D5F59A5-49D3-4871-8776-50B9757DC266Q57444966-7F109475-26D8-41D9-888A-80B0AE6CC9D8Q57444968-67058713-6C37-4CBF-8156-52C5A54B4A83Q57686597-EDA94532-B346-44FF-AE8F-2587BA67E4C0Q57913559-510B8C73-FFC7-4918-AA63-53A37C787C2DQ57913567-28A63B02-CDCA-4A5F-9A5B-48587959DD4DQ58359688-20D04807-581A-4003-A76F-AEA6BA802E1AQ58913229-F8492C04-8EC6-42A1-A22E-7E3FC51CA250Q58914234-9FD34F4A-3A38-4738-9D80-55515C5FC749Q58914235-5DC22FD1-51B1-4CC9-8D59-A3ECB9D05FF7Q58914236-18DFF5BF-6850-4623-A95A-79C5DE2EB329Q58914240-A5E4215C-A9A6-4B04-B55A-E2AE5F4AB30FQ58914243-3DF75B3D-B369-4D80-9303-4DA1654C6A44Q58914256-F20A8660-87B3-4B92-96B4-F5C6483ADE81Q58914258-C89AA8D1-3B68-47AC-9142-ECFCA44F2566Q58914263-4F53A768-5DBE-4F03-BD13-FD999728DB16Q58914265-A8F0F131-08E1-4175-965A-BDDFA4BA0F65Q58914270-120A9D1C-44B0-4274-B811-3FB9E6EB8F58Q58914272-F155FEA1-5C5E-436D-8329-B37F697589A7Q58914274-E5ADD7A5-2367-42CC-AFFB-37D80469E064Q58914280-0E39ABEA-A2E0-44AB-B940-38DCF13C6DFCQ58914298-C8CEAE2E-9024-4D28-A989-0FF39B79804BQ58914313-ACA48C02-7EF9-4C7A-9F57-6D3D0DC08AB5Q58914323-EE35E0E4-3647-472D-A9F7-299380AB0541Q58914327-6D4EF0B2-96E3-4D2D-BECF-23D9F83C9D0CQ58914340-2EAE3EA8-B189-46A8-8A0A-52710F01D9CFQ58914345-95D0FF6C-5702-4080-A107-7E40E96FB2C8Q58914369-1C83278A-8BEA-480C-8206-DCC7AFEE3337Q58915537-92490DDE-C290-4208-A538-B1850C669DB3Q58921038-6EDDB26F-C180-40B5-9CDA-19AF5E4DAC0AQ58922670-82832015-E773-4485-97F0-958A0A1906A0Q59703027-FE257E11-92A4-4224-9B44-D2B80B867E1FQ59734844-F26F5646-7D9A-4DAC-AAAE-B07F9BAB6D8BQ59734848-CC7E189B-08A4-43CD-A954-A68035676C48Q59756316-542B5AE6-1D32-4195-B466-D9CBA90C2017
P50
description
hulumtues
@sq
onderzoeker
@nl
researcher
@en
հետազոտող
@hy
name
Fabio Gastaldello
@ast
Fabio Gastaldello
@en
Fabio Gastaldello
@es
Fabio Gastaldello
@nl
Fabio Gastaldello
@sl
type
label
Fabio Gastaldello
@ast
Fabio Gastaldello
@en
Fabio Gastaldello
@es
Fabio Gastaldello
@nl
Fabio Gastaldello
@sl
prefLabel
Fabio Gastaldello
@ast
Fabio Gastaldello
@en
Fabio Gastaldello
@es
Fabio Gastaldello
@nl
Fabio Gastaldello
@sl
P106
P1153
36005154700
P21
P31
P496
0000-0002-9112-0184