Publication
Assembly bias evidence in close galaxy pairs
The growth channel of massive galaxies involving mergers can be studied via close pairs as putative merger progenitors, where the stellar populations of the...
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PublicationAssessing the accuracy of star formation rate measurements by direct star count in molecular cloudsStar formation estimates based on the counting of young stellar objects (YSOs) are commonly carried out for nearby star-forming regions in the Galaxy, and in...
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PublicationAssociation of cold gas, massive galaxies, and AGNs in a filamentary protocluster traced by triple narrow-band imagingWe investigate galaxy populations in the HS 1700+64 protocluster at $z=2.30$, characterized by two prominent linear filaments traced by spatially extended ${\rm...
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PublicationAstrometry and photometry of stars and star clusters in M33We present positions and magnitudes of stars and star clusters in a 1° × 1° area centered on M33. The survey is based on deep archival ground-based images using...
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NewsAstronomers discover that the first galaxies had very different shapes to today's galaxiesThanks to images obtained by the James Webb Telescope (JWST), an international scientific team in which the Instituto de Astrofísica de Canarias (IAC)...
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NewsAstronomers discover tiny galaxy with extraordinary star formation in distant UniverseUsing first-of-their-kind observations from the James Webb Space Telescope (JWST), an international scientific team, in which the Instituto de Astrofísica de...
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NewsAstronomers find a galaxy unchanged since the early universeResearchers at the Instituto de Astrofísica de Canarias (IAC) confirm the first detection of a relic galaxy with the Hubble Space Telescope. The results of this...
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NewsAstronomers find the first galaxy whose ultraviolet luminosity is comparable to that of a quasarAn international scientific team, led by researchers at the Centre for Astrobiology (CAB, CSIC-INTA) and with participation by the Instituto de Astrofísica de...
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PublicationASW<SUP>2</SUP>DF: Census of the obscured star formation in a galaxy cluster in formation at z = 2.2We report the results of the deep and wide Atacama Large Millimeter/submillimeter Array (ALMA) 1.2 mm mapping of the Spiderweb protocluster at z = 2.16. The...