Hiddo Algera

Leiden University

Netherlands

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Articles (10)

Year:

2025

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2025

Year:

2025

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2025

Year:

2025

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2025

Year:

2024

Year:

2024

Year:

2024

Year:

2024

Collaborators (5)

Carlos Gómez-Guijarro

Københavns Universitet

DENMARK

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Takafumi Tsukui

Australian National University

AUSTRALIA

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Shuowen Jin

Technical University of Denmark

DENMARK

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Tom Bakx

Chalmers University of Technology

SWEDEN

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Nikolaj Bjerregaard Sillassen

Technical University of Denmark

DENMARK

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Hiddo Algera

Research Interests

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Articles (10)

The ALMA REBELS survey: [O iii]88μm line scans of UV-bright z ≳ 7.6 galaxies

Detection of [O iii]88 μm in JADES-GS-z14-0 at z = 14.1793

Realistic multitemperature dust: how well can we constrain the dust properties of high-redshift galaxies?

The dust emissivity index β in infrared-bright galaxies at 1.5 < z < 4.2

REBELS-IFU: dust attenuation curves of 12 massive galaxies at z ≃ 7

Revealing the hidden cosmic feast: A z = 4.3 galaxy group hosting two optically dark, efficiently star-forming galaxies

REBELS-25: discovery of a dynamically cold disc galaxy at z = 7.31

A novel high-z submm galaxy efficient line survey in ALMA Bands 3 through 8 – an ANGELS pilot

Characterising the contribution of dust-obscured star formation at z ≳ 5 using 18 serendipitously identified [C ii] emitters

Comparisons between Resolved Star Formation Rate and Gas Tracers in the Strongly Lensed Galaxy SDSS J0901+1814 at Cosmic Noon

Collaborators (5)

Carlos Gómez-Guijarro

Takafumi Tsukui

Shuowen Jin

Tom Bakx

Nikolaj Bjerregaard Sillassen

Make your next move.

Hiddo Algera

Research Interests

Explore related searches

Contact this professor

Articles (10)

The ALMA REBELS survey: [O iii]88μm line scans of UV-bright z ≳ 7.6 galaxies

Detection of [O iii]88 μm in JADES-GS-z14-0 at z = 14.1793

Realistic multitemperature dust: how well can we constrain the dust properties of high-redshift galaxies?

The dust emissivity index β in infrared-bright galaxies at 1.5 &lt; z &lt; 4.2

REBELS-IFU: dust attenuation curves of 12 massive galaxies at z ≃ 7

Revealing the hidden cosmic feast: A z = 4.3 galaxy group hosting two optically dark, efficiently star-forming galaxies

REBELS-25: discovery of a dynamically cold disc galaxy at z = 7.31

A novel high-z submm galaxy efficient line survey in ALMA Bands 3 through 8 – an ANGELS pilot

Characterising the contribution of dust-obscured star formation at z ≳ 5 using 18 serendipitously identified [C ii] emitters

Comparisons between Resolved Star Formation Rate and Gas Tracers in the Strongly Lensed Galaxy SDSS J0901+1814 at Cosmic Noon

Collaborators (5)

Carlos Gómez-Guijarro

Takafumi Tsukui

Shuowen Jin

Tom Bakx

Nikolaj Bjerregaard Sillassen

Make your next move.

The dust emissivity index β in infrared-bright galaxies at 1.5 < z < 4.2