about
Submillimetre galaxies reside in dark matter haloes with masses greater than 3 × 10¹¹ solar massesHerMES: Halo occupation number and bias properties of dusty galaxies from angular clustering measurementsThe suppression of star formation by powerful active galactic nucleiThe 3D structure of the Virgo cluster from H-band Fundamental Plane and Tully--Fisher distance determinationsGALEX Ultraviolet Observations of the Interacting Galaxy NGC 4438 in the Virgo ClusterThe dust morphology of the elliptical Galaxy M 86 with SPIREThe GALEX Ultraviolet Atlas of Nearby GalaxiesMolecular hydrogen deficiency in H I-poor galaxies and its implications for star formationThe Herschel Virgo Cluster Survey VI. The far-infrared view of M 87The Herschel Virgo Cluster Survey III. A constraint on dust grain lifetime in early-type galaxiesThe next generation Virgo cluster survey. VI. The kinematics of ultra-compact dwarfs and globular clusters in M87CO in late-type galaxies within the central region of Abell 1367The Next Generation Virgo cluster Survey. X. Properties of ultra-compact dwarfs in the M87, M49, and M60 regionsSpectacular tails of ionized gas in the Virgo cluster galaxy NGC 4569The Herschel Virgo Cluster Survey - VIII. The Bright Galaxy SampleThe GALEX Ultraviolet Virgo Cluster Survey (GUViCS)HerMES: CANDIDATE GRAVITATIONALLY LENSED GALAXIES AND LENSING STATISTICS AT SUBMILLIMETER WAVELENGTHSCapturing a Star Formation Burst in Galaxies Infalling onto the Cluster A1367Probing evolutionary mechanisms in galaxy clusters: neutral atomic hydrogen in Abell 1367The far-ultraviolet emission of early-type galaxiesRam pressure stripping of the multiphase ISM in the Virgo cluster spiral galaxy NGC 4438Cold dust and young starbursts: spectral energy distributions of Herschel SPIRE sources from the HerMES survey★Evolution of dust temperature of galaxies through cosmic time as seen by HerschelFirst results from HerMES on the evolution of the submillimetre luminosity functionHerMES: deep galaxy number counts from a P(D) fluctuation analysis of SPIRE Science Demonstration Phase observationsHerMES: Far infrared properties of known AGN in the HerMES fieldsHerMES: The SPIRE confusion limitHerMES: The submillimeter spectral energy distributions of Herschel/SPIRE-detected galaxiesHerschel unveils a puzzling uniformity of distant dusty galaxiesMeasures of star formation rates from infrared (Herschel) and UV (GALEX) emissions of galaxies in the HerMES fieldsThe Deep SPIRE HerMES Survey: spectral energy distributions and their astrophysical indications at high redshiftThe HerMES SPIRE submillimeter local luminosity functionThe Herschel Multi-Tiered Extragalactic Survey: source extraction and cross-identifications in confusion-dominated SPIRE imagesThe far-infrared/radio correlation as probed by HerschelThe HI properties of galaxies in the Coma I cloud revisitedMeasuring star formation with resolved observations: the test case of M 33CALIFA, the Calar Alto Legacy Integral Field Area survey I. Survey presentationNGC 4370: a case study for testing our ability to infer dust distribution and mass in nearby galaxiesThe identification of dust heating mechanisms in nearby galaxies using Herschel 160/250 and 250/350 μm surface brightness ratiosThe Herschel Virgo Cluster Survey XVIII. Star-forming dwarf galaxies in a cluster environment
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Q27014149-D50C61B6-6203-4E06-B4D2-FC02C12300F9Q27019552-4822D642-A825-493A-B635-54895530DE2EQ50511312-A78A79D0-731A-43F7-A565-B0CFD0507C4EQ53953121-4796A748-12D0-49D4-93DF-0C6382F200E0Q53953503-DB2DEB47-C8B9-47CA-8C2D-79B154F4B704Q53953526-04797D47-6E2B-4D25-A91C-0DBCA2014E3FQ54195946-4A22792F-7189-4654-AB2C-8DC47F2D2FC9Q54195954-F8668B6A-94C2-4097-A6FA-EE6310829830Q55893405-30FC83A9-2D3E-4605-96C8-D79976D752E4Q55893417-FBF06580-614E-47C7-A5B7-003F7FC19EFDQ55893435-61136CF5-E6BE-4FCB-9928-D456E3D52989Q56001846-BDC9C7E7-A112-4D59-94EF-BE116851C2D1Q56031951-EEB11C2C-208A-4580-B7EB-1D3175E7ED82Q56032071-B3428090-E1B6-4ACF-AC13-C89725338D98Q56032292-B3B37A61-E31A-4EC6-A879-4DBD5329A72FQ56169300-C05D8229-7769-4C3D-93A4-FD62B5E236CCQ56423936-8001E6C6-DFB6-4317-A552-9A47DC3F33BCQ56553876-377A6B1F-6D6F-49BC-B691-489C20163641Q56555247-F388DD82-2A2B-4CFD-9BDA-A2486490D62EQ56555313-AAE56038-77EE-405F-B2BC-C47FF08B6EFAQ56557922-DFBE3D52-0EE1-4991-9C9F-276646EFDC0DQ56583399-908B6033-70D8-4A95-A147-57B57AC4F410Q56583655-C94DA3F8-DA7D-4CF1-A49E-E61BE81E6781Q56583823-DC616BFB-1017-466B-93DC-6D8E509AEB1CQ56584127-6AFD67F0-A250-4E1D-9F07-367F51F007D9Q56584401-7325A46D-12C4-418E-B2B4-FC5EDC991270Q56584847-7BE61450-D711-4B6D-8652-14019F8B5A69Q56585050-BC3D9529-C1F7-4A79-920A-924AD210C5D1Q56585269-12453057-A1B5-4CBB-A72C-8D67DCC8A126Q56585540-D4E846ED-4FC6-47A6-9343-31F8E022D053Q56585938-FC7A405A-D822-468A-99EA-AA0876F938BEQ56586052-5CBFF38A-41B3-497C-B242-EED3CB720240Q56586238-79F4310A-1D72-4CBE-A7CB-1CC6D93DB123Q56586358-D616EB4A-3F96-4712-9184-A8B81776380EQ56672720-023CEFB4-09A9-4A0D-A397-B91E63B7B2F7Q56914276-533C2DE6-E944-4D11-AD77-F05DDE34B3D8Q57444295-9128C6D9-A96F-481C-B718-16DD75D77FADQ57602887-E2B64B59-A16F-4E52-8A09-5D26A636D5BCQ57602891-97FC9EC2-F1A4-4ECE-9656-E5CEA0DA51AFQ57602894-1F9959CE-E914-43B6-9FD8-DC8C89AE3CA6
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description
Italiaans onderzoeker
@nl
Italian astrophysicist
@en
astrofísico italiano
@es
astrophysicien italien
@fr
réaltfhisiceoir Iodálach
@ga
name
Alessandro Boselli
@ast
Alessandro Boselli
@en
Alessandro Boselli
@es
Alessandro Boselli
@fr
Alessandro Boselli
@ga
Alessandro Boselli
@nl
Alessandro Boselli
@sl
Alessandro Boselli
@sq
type
label
Alessandro Boselli
@ast
Alessandro Boselli
@en
Alessandro Boselli
@es
Alessandro Boselli
@fr
Alessandro Boselli
@ga
Alessandro Boselli
@nl
Alessandro Boselli
@sl
Alessandro Boselli
@sq
altLabel
A. Boselli
@en
prefLabel
Alessandro Boselli
@ast
Alessandro Boselli
@en
Alessandro Boselli
@es
Alessandro Boselli
@fr
Alessandro Boselli
@ga
Alessandro Boselli
@nl
Alessandro Boselli
@sl
Alessandro Boselli
@sq
P1412
P1006
P214
P269
P4285
P1006
P103
P1559
Alessandro Boselli
@it
P21
P214
P269
P27
P31
P4285
P496
0000-0002-9795-6433
P569
1965-01-01T00:00:00Z
P734
P735
P7859
lccn-no2011154593