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1
Two accreting protoplanets around the young star PDS 70
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Two accreting protoplanets around the young star PDS 70

Nature astronomy, 2019-08, Vol.3 (8), p.749-754 [Peer Reviewed Journal]

The Author(s), under exclusive licence to Springer Nature Limited 2019. ;ISSN: 2397-3366 ;EISSN: 2397-3366 ;DOI: 10.1038/s41550-019-0780-5

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2
STARS WERE BORN IN SIGNIFICANTLY DENSER REGIONS IN THE EARLY UNIVERSE
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STARS WERE BORN IN SIGNIFICANTLY DENSER REGIONS IN THE EARLY UNIVERSE

The Astrophysical journal, 2014-06, Vol.787 (2), p.1-9 [Peer Reviewed Journal]

ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.1088/0004-637X/787/2/120

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3
New criteria for the selection of galaxy close pairs from cosmological simulations: evolution of the major and minor merger fraction in MUSE deep fields
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New criteria for the selection of galaxy close pairs from cosmological simulations: evolution of the major and minor merger fraction in MUSE deep fields

Astronomy and astrophysics (Berlin), 2019-11, Vol.631 [Peer Reviewed Journal]

Attribution ;ISSN: 0004-6361 ;EISSN: 1432-0746 ;DOI: 10.1051/0004-6361/201935597

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4
Galaxies with Wolf-Rayet signatures in the low-redshift Universe : A survey using the Sloan Digital Sky Survey
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Galaxies with Wolf-Rayet signatures in the low-redshift Universe : A survey using the Sloan Digital Sky Survey

Astronomy and astrophysics (Berlin), 2008, Vol.485 (3), p.657-677 [Peer Reviewed Journal]

2008 INIST-CNRS ;Distributed under a Creative Commons Attribution 4.0 International License ;ISSN: 0004-6361 ;EISSN: 1432-0746 ;DOI: 10.1051/0004-6361:200809783 ;CODEN: AAEJAF

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5
Nearly all the sky is covered by Lyman-α emission around high-redshift galaxies
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Nearly all the sky is covered by Lyman-α emission around high-redshift galaxies

Nature (London), 2018-10, Vol.562 (7726), p.229-232 [Peer Reviewed Journal]

Copyright Nature Publishing Group Oct 11, 2018 ;ISSN: 0028-0836 ;ISSN: 1476-4687 ;EISSN: 1476-4687 ;DOI: 10.1038/s41586-018-0564-6 ;PMID: 30275476

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6
Extended Lyman α haloes around individual high-redshift galaxies revealed by MUSE
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Extended Lyman α haloes around individual high-redshift galaxies revealed by MUSE

Astronomy and astrophysics (Berlin), 2016-03, Vol.587, p.A98 [Peer Reviewed Journal]

Distributed under a Creative Commons Attribution 4.0 International License ;ISSN: 0004-6361 ;EISSN: 1432-0746 ;DOI: 10.1051/0004-6361/201527384

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7
The physical properties of star-forming galaxies in the low-redshift Universe
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The physical properties of star-forming galaxies in the low-redshift Universe

Monthly notices of the Royal Astronomical Society, 2004-07, Vol.351 (4), p.1151-1179 [Peer Reviewed Journal]

2004 INIST-CNRS ;ISSN: 0035-8711 ;EISSN: 1365-2966 ;DOI: 10.1111/j.1365-2966.2004.07881.x ;CODEN: MNRAA4

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8
The MUSE-Wide Survey: survey description and first data release
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The MUSE-Wide Survey: survey description and first data release

Astronomy and astrophysics (Berlin), 2019-04, Vol.624 [Peer Reviewed Journal]

Distributed under a Creative Commons Attribution 4.0 International License ;ISSN: 0004-6361 ;EISSN: 1432-0746 ;DOI: 10.1051/0004-6361/201834656

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9
THE EXTENDED He II λ4686-EMITTING REGION IN IZw 18 UNVEILED: CLUES FOR PECULIAR IONIZING SOURCES
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THE EXTENDED He II λ4686-EMITTING REGION IN IZw 18 UNVEILED: CLUES FOR PECULIAR IONIZING SOURCES

Astrophysical journal. Letters, 2015-03, Vol.801 (2) [Peer Reviewed Journal]

2015. The American Astronomical Society. All rights reserved. ;Distributed under a Creative Commons Attribution 4.0 International License ;ISSN: 2041-8205 ;EISSN: 2041-8213 ;DOI: 10.1088/2041-8205/801/2/L28

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10
The MUSE 3D view of the Hubble Deep Field South
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The MUSE 3D view of the Hubble Deep Field South

Astronomy and astrophysics (Berlin), 2015-03, Vol.575, p.A75 [Peer Reviewed Journal]

Distributed under a Creative Commons Attribution 4.0 International License ;ISSN: 0004-6361 ;EISSN: 1432-0746 ;DOI: 10.1051/0004-6361/201425419

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11
Recovering the systemic redshift of galaxies from their Lyman alpha line profile
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Recovering the systemic redshift of galaxies from their Lyman alpha line profile

Monthly notices of the Royal Astronomical Society. Letters, 2018-07, Vol.478 (1), p.L60-L65 [Peer Reviewed Journal]

Distributed under a Creative Commons Attribution 4.0 International License ;ISSN: 1745-3933 ;EISSN: 1745-3933 ;DOI: 10.1093/mnrasl/sly058

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12
The host galaxies of radio-loud active galactic nuclei: mass dependences, gas cooling and active galactic nuclei feedback
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The host galaxies of radio-loud active galactic nuclei: mass dependences, gas cooling and active galactic nuclei feedback

Monthly Notices of the Royal Astronomical Society, 2005-09, Vol.362 (1), p.25-40 [Peer Reviewed Journal]

2005 INIST-CNRS ;Distributed under a Creative Commons Attribution 4.0 International License ;ISSN: 0035-8711 ;EISSN: 1365-2966 ;DOI: 10.1111/j.1365-2966.2005.09192.x ;CODEN: MNRAA4

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13
The MUSE Extremely Deep Field: The cosmic web in emission at high redshift
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The MUSE Extremely Deep Field: The cosmic web in emission at high redshift

Astronomy and astrophysics (Berlin), 2021-03, Vol.647 [Peer Reviewed Journal]

Distributed under a Creative Commons Attribution 4.0 International License ;ISSN: 0004-6361 ;EISSN: 1432-0746 ;DOI: 10.1051/0004-6361/202039887

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14
Evidence for ram pressure stripping in a cluster of galaxies at z = 0.7
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Evidence for ram pressure stripping in a cluster of galaxies at z = 0.7

Astronomy and astrophysics (Berlin), 2019-11, Vol.631 [Peer Reviewed Journal]

Distributed under a Creative Commons Attribution 4.0 International License ;ISSN: 0004-6361 ;ISSN: 1432-0746 ;EISSN: 1432-0746 ;DOI: 10.1051/0004-6361/201936133

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15
POSSIBLE SIGNATURES OF A COLD-FLOW DISK FROM MUSE USING A z ∼ 1 GALAXY–QUASAR PAIR TOWARD SDSS J1422−0001
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POSSIBLE SIGNATURES OF A COLD-FLOW DISK FROM MUSE USING A z ∼ 1 GALAXY–QUASAR PAIR TOWARD SDSS J1422−0001

The Astrophysical journal, 2016-04, Vol.820 (2), p.121 [Peer Reviewed Journal]

ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/0004-637X/820/2/121

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16
Resolved scaling relations and metallicity gradients on sub-kiloparsec scales at z ≈ 1
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Resolved scaling relations and metallicity gradients on sub-kiloparsec scales at z ≈ 1

Monthly notices of the Royal Astronomical Society, 2019-10, Vol.489 (1), p.224-240 [Peer Reviewed Journal]

Distributed under a Creative Commons Attribution 4.0 International License ;ISSN: 0035-8711 ;EISSN: 1365-2966 ;DOI: 10.1093/mnras/stz2114

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17
The triggering probability of radio-loud AGN: A comparison of high and low excitation radio galaxies in hosts of different colors
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The triggering probability of radio-loud AGN: A comparison of high and low excitation radio galaxies in hosts of different colors

Astronomy and astrophysics (Berlin), 2012-05, Vol.541, p.A62 [Peer Reviewed Journal]

2015 INIST-CNRS ;ISSN: 0004-6361 ;EISSN: 1432-0746 ;DOI: 10.1051/0004-6361/201219052 ;CODEN: AAEJAF

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18
Long-term results after intracoronary injection of autologous mononuclear bone marrow cells in acute myocardial infarction: the ASTAMI randomised, controlled study
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Long-term results after intracoronary injection of autologous mononuclear bone marrow cells in acute myocardial infarction: the ASTAMI randomised, controlled study

Heart (British Cardiac Society), 2009-12, Vol.95 (24), p.1983-1989 [Peer Reviewed Journal]

BMJ Publishing Group Ltd and British Cardiovascular Society. All rights reserved. ;2015 INIST-CNRS ;Copyright: 2009 BMJ Publishing Group Ltd and British Cardiovascular Society. All rights reserved. ;ISSN: 1355-6037 ;EISSN: 1468-201X ;DOI: 10.1136/hrt.2009.178913 ;PMID: 19833610

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19
Kinematics, turbulence, and star formation of z ∼ 1 strongly lensed galaxies seen with MUSE
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Kinematics, turbulence, and star formation of z ∼ 1 strongly lensed galaxies seen with MUSE

Monthly notices of the Royal Astronomical Society, 2018-06, Vol.477 (1), p.18-44 [Peer Reviewed Journal]

Distributed under a Creative Commons Attribution 4.0 International License ;ISSN: 0035-8711 ;EISSN: 1365-2966 ;DOI: 10.1093/mnras/sty555

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20
MUSE crowded field 3D spectroscopy of over 12 000 stars in the globular cluster NGC 6397
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MUSE crowded field 3D spectroscopy of over 12 000 stars in the globular cluster NGC 6397

Astronomy and astrophysics (Berlin), 2016-04, Vol.588 [Peer Reviewed Journal]

ISSN: 0004-6361 ;EISSN: 1432-0746 ;DOI: 10.1051/0004-6361/201527065

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