about
The Kepler-454 system: a small, not-rocky inner planet, a jovian world, and a distant companionAn Earth-sized planet with an Earth-like density.Broadband observations of the naked-eye gamma-ray burst GRB 080319B.GRB 090423 at a redshift of z approximately 8.1.The Kepler-10 planetary system revisited by HARPS-N: a hot rocky world and a solid neptune-mass planetThe GAPS programme with HARPS-N at TNGStellar parameters of early-M dwarfs from ratios of spectral features at optical wavelengthsProject overview and update on WEAVE: the next generation wide-field spectroscopy facility for the William Herschel TelescopeSPACE: the spectroscopic all-sky cosmic explorerThe GAPS programme with HARPS-N at TNGCharacterization of the planetary system Kepler-101 with HARPS-NAn Ultra-short Period Rocky Super-Earth with a Secondary Eclipse and a Neptune-like Companion around K2-141Introducing the CTA conceptDesign concepts for the Cherenkov Telescope Array CTA: an advanced facility for ground-based high-energy gamma-ray astronomyThree’s Company: An Additional Non-transiting Super-Earth in the Bright HD 3167 System, and Masses for All Three PlanetsThe orbit and mass of the third planet in the Kepler-56 systemCharacterizing K2 planet discoveries: a super-earth transiting the bright K dwarf HIP 116454Challenging gamma-ray burst models through the broadband dataset of GRB 060908The GAPS programme with HARPS-N at TNGThe GAPS programme with HARPS-N at TNGThe GAPS programme with HARPS-N at TNGThe GAPS programme with HARPS-N at TNGThe GAPS Programme with HARPS-N at TNGThe GAPS programme with HARPS-N at TNG. I. Observations of the Rossiter-McLaughlin effect and characterisation of the transiting system Qatar-1The complex light curve of the afterglow of GRB071010AEyes on K2-3: A system of three likely sub-Neptunes characterized with HARPS-N and HARPSThe Kepler-19 System: A Thick-envelope Super-Earth with Two Neptune-mass Companions Characterized Using Radial Velocities and Transit Timing VariationsKEPLER-21b: A ROCKY PLANET AROUND AV= 8.25 mag STARThe HARPS-N Rocky Planet SearchTHE MASS OF Kepler-93b AND THE COMPOSITION OF TERRESTRIAL PLANETSRewritable photochromic focal plane masksShort timescale photometric and polarimetric behavior of two BL Lacertae type objectsA Path to the Stars: The Evolution of the SpeciesREM: Automatic for the PeopleThe REM Observing SoftwareGRB 080319B: the prompt emission of the “Naked Eye Burst”REM near-IR and optical multiband observations of PKS 2155-304 in 2005GRB 070311: a direct link between the prompt emission and the afterglowREM near-IR and optical multiband observations of PKS 2155-304 in 2005REM observations of GRB 060418 and GRB 060607A: the onset of the afterglow and the initial fireball Lorentz factor determination
P50
Q27011605-52841729-E6FD-4D59-B777-C1DEBE60BEC7Q34381252-633B18B4-A71E-469F-B180-AAC8F7E06D90Q34825232-347B54FB-5DD8-4059-AEAD-B31D8AFB0391Q35010025-315FE020-5A2F-4F31-ADD8-4BC1368AB4D8Q55920224-EF63E1F5-1E84-4EDC-B33E-594698D6FE86Q56156390-3E5A0E94-3661-439E-89A5-32BA7DDA7A6EQ56169216-7B63E3C7-B3F9-4276-9758-A7D64557C51AQ56432039-904E8A89-2CDD-4A29-B445-A23FF0272928Q56555882-0D088D76-2F00-431E-AC70-389756626EE0Q56561515-500CEF14-A62D-43C8-802F-E82D28700466Q56562182-11CB253D-A78E-426D-804D-6313B5008700Q56659307-FEB31665-BE37-4233-8AAA-4AD6D768433CQ56933543-05D9605A-DA57-41EA-A958-F35CE087FC9FQ56933794-2BBA0A8A-6A6F-4B0F-8221-65881B59B254Q57406195-517F6C43-AA8B-4934-9220-A2289A1DA39BQ57549033-C3F6222E-D840-480F-B3AE-0650196F3E83Q57549056-17DB4F84-C9EE-4B83-B4A3-787A72CE9829Q57579321-05A6D1ED-D4F6-4B60-9794-4313BE42270EQ57594359-87E4527B-93FD-4977-8F06-732C9BF7E8FCQ57594362-86255BD5-0C54-47C7-8471-CAFFE00DCB37Q57594366-F14E1A77-C2CD-4F6D-887A-BAEE074E21F6Q57594367-AA75442C-5B07-408F-ACF5-4ECD0A282F77Q57594383-8CD728F6-620F-4EB2-9160-4B4C46331AA2Q57594390-7D7B45D6-6BA7-4DAC-BE6A-AF28D302E23EQ57602970-6627A008-554F-41D4-8512-49BB5C19E3D9Q57627107-D9146FF5-A8A0-4A75-B053-7B6EE434571BQ57627176-14D8A8CE-9203-4EDE-940F-231D8D9929BCQ57627225-7643E7EE-54C4-4355-81B8-59FB7A1B979EQ57627251-C105C4B4-C648-4EAD-A339-88C30D22C56BQ57627306-C66AB608-7106-4A0F-8FE3-EA9932E97266Q57890108-FC609F5F-59F0-4FAE-9531-6904795402C7Q58073407-F347250E-4117-40FE-8EA7-3C287D436C29Q58649146-4B3BDF97-A08F-49BD-926E-63C0ECFC5664Q58649154-4CCE9AD6-7838-4F91-9BE7-01089D9750F5Q58649707-7612608B-C508-41E9-B62A-3A605E05AC48Q58908778-5DB45CEE-83E8-49C9-BE6A-B4E4CE9A273AQ58908798-98896414-879A-44E4-95F3-0075B085176BQ58908801-03875468-C38A-4D05-BC57-5B3B4FE4CF73Q58908808-D73EC975-4AE2-494C-B1DE-BCCD09F48314Q58908811-D5B1FEB3-E95A-4790-9086-D6D598D87F61
P50
description
hulumtues
@sq
researcher
@en
wetenschapper
@nl
հետազոտող
@hy
name
E Molinari
@nl
E Molinari
@sl
Emilio Molinari
@en
Emilio Molinari
@es
type
label
E Molinari
@nl
E Molinari
@sl
Emilio Molinari
@en
Emilio Molinari
@es
altLabel
E Molinari
@en
prefLabel
E Molinari
@nl
E Molinari
@sl
Emilio Molinari
@en
Emilio Molinari
@es
P106
P1153
7102949556
P21
P31
P496
0000-0002-1742-7735