Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies | Paper Citation Record

Observation 50ea2571-12bb-46d9-88fb-8302b9faacea · outbound

This paper cites The ALMA Spectroscopic Survey Large Program: the infrared excess of z = 1.5 –10 UV-selected galaxies and the implied high-redshift star formation history,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies The ALMA Spectroscopic Survey Large Program: the infrared excess of z = 1.5 –10 UV-selected galaxies and the implied high-redshift star formation history,

Reference 1

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:25.954971Z

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Observation 97c85c38-8dae-4934-9d78-4daebb8b1fbe · outbound

This paper cites A dominant population of optically invisible massive galaxies in the early Universe,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies A dominant population of optically invisible massive galaxies in the early Universe,

Reference 2

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:25.946896Z

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Observation 39b50141-e0a4-46a4-b71e-7f606036e66a · outbound

This paper cites Jekyll & Hyde: quiescence and extreme obscuration in a pair of massive galaxies 1.5 Gyr after the Big Bang,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies Jekyll & Hyde: quiescence and extreme obscuration in a pair of massive galaxies 1.5 Gyr after the Big Bang,

Reference 3

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:25.938233Z

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No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 21001700-a8f6-49cd-8b35-fe878e212b54 · outbound

This paper cites Quiescent galaxies 1.5 billion years after the Big Bang and their progenitors,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies Quiescent galaxies 1.5 billion years after the Big Bang and their progenitors,

Reference 4

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:25.929503Z

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Observation e30cbcad-eb4d-41ca-a0ed-9bb23305d32b · outbound

This paper cites Multiwavelength study of massive galaxies at z ∼2. II. Widespread Compton-thick active galactic nuclei and the concurrent growth of black holes and bulges,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies Multiwavelength study of massive galaxies at z ∼2. II. Widespread Compton-thick active galactic nuclei and the concurrent growth of black holes and bulges,

Reference 5

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:25.920606Z

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No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation b3b06591-11b9-4e1a-83ae-8626ea7c82a1 · outbound

This paper cites A highly consistent framework for the evolution of the star-forming “main sequence.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies A highly consistent framework for the evolution of the star-forming “main sequence

Reference 6

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:25.912457Z

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Observation 08f33a0f-a63d-4d7b-baf1-849b00e7ad64 · outbound

This paper cites The main sequence of star-forming galaxies across cosmic times,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies The main sequence of star-forming galaxies across cosmic times,

Reference 7

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:25.903815Z

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Observation 48f4a6c1-cd25-4b8e-8656-fc5e4c8b2bbe · outbound

This paper cites The rate of star formation,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies The rate of star formation,

Reference 8

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:25.895702Z

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No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation ebef5a73-14f9-4231-a20f-34be6ead03ca · outbound

This paper cites Star formation in galaxies along the Hubble sequence,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies Star formation in galaxies along the Hubble sequence,

Reference 9

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:25.887486Z

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No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 7da9cabf-6bc2-4907-8a7c-4299a7940c62 · outbound

This paper cites Luminous infrared galaxies,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies Luminous infrared galaxies,

Reference 10

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:25.879338Z

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Observation 6f3d161e-96ef-4257-8d39-c923b39e3f87 · outbound

This paper cites The MASSIVE survey – III. Molecular gas and a broken Tully–Fisher relation in the most massive early-type galaxies,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies The MASSIVE survey – III. Molecular gas and a broken Tully–Fisher relation in the most massive early-type galaxies,

Reference 11

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:25.871494Z

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No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation e1c32b23-5c6a-4bb5-9b04-6b73fb474cee · outbound

This paper cites GMASS ultradeep spectroscopy of galaxies at z ∼ 2. II. Superdense passive galaxies: how did they form and evolve?,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies GMASS ultradeep spectroscopy of galaxies at z ∼ 2. II. Superdense passive galaxies: how did they form and evolve?,

Reference 12

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:25.863100Z

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No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 05a805bc-a066-4a4a-b992-aae0bb6896f5 · outbound

This paper cites A massive, quiescent galaxy at a redshift of 3.717,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies A massive, quiescent galaxy at a redshift of 3.717,

Reference 13

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:25.854776Z

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No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 74dfd09b-da41-4ed2-b478-7cbec59f8ab1 · outbound

This paper cites Optically faint massive Balmer break galaxies at z > 3 in the CANDELS/ GOODS fields,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies Optically faint massive Balmer break galaxies at z > 3 in the CANDELS/ GOODS fields,

Reference 14

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:25.846633Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation fc9da265-4c11-4e25-8069-064d5b6c0266 · outbound

This paper cites Illuminating the dark side of cosmic star formation two billion years after the Big Bang,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies Illuminating the dark side of cosmic star formation two billion years after the Big Bang,

Reference 15

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:25.837919Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation dc08b6f5-f478-4f14-b096-a0c691a69bd7 · outbound

This paper cites The hidden side of cosmic star formation at z > 3: bridging optically dark and Lyman- break galaxies with GOODS-ALMA,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies The hidden side of cosmic star formation at z > 3: bridging optically dark and Lyman- break galaxies with GOODS-ALMA,

Reference 16

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:25.829883Z

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No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 33cfe059-fb06-4a03-ad7f-ee80d84ea465 · outbound

This paper cites GOODS-ALMA: 1.1 mm galaxy survey. I. Source catalog and optically dark galaxies,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies GOODS-ALMA: 1.1 mm galaxy survey. I. Source catalog and optically dark galaxies,

Reference 17

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:25.821041Z

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No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation e33c5ab1-5182-4708-9bb5-666169adc7b2 · outbound

This paper cites Discovery of a dark, massive, ALMA-only galaxy at z ∼ 5–6 in a tiny 3 mm survey,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies Discovery of a dark, massive, ALMA-only galaxy at z ∼ 5–6 in a tiny 3 mm survey,

Reference 18

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:25.812782Z

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No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 8646a6d7-8c95-4291-89cb-cb3e8cb05e05 · outbound

This paper cites ALMA 26 arcmin² survey of GOODS-S at 1 mm (ASAGAO): near-infrared-dark faint ALMA sources,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies ALMA 26 arcmin² survey of GOODS-S at 1 mm (ASAGAO): near-infrared-dark faint ALMA sources,

Reference 19

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:25.803266Z

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Observation 16b19b47-b13d-43de-badf-4fb7dbe0a9ce · outbound

This paper cites The ALPINE-ALMA [CII] survey: the nature, luminosity function, and star formation history of dusty galaxies up to z ∼ 6,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies The ALPINE-ALMA [CII] survey: the nature, luminosity function, and star formation history of dusty galaxies up to z ∼ 6,

Reference 20

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:25.794657Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 9bd69b1a-e4a9-4f39-8226-ec57d173d515 · outbound

This paper cites An ALMA survey of the S2CLS UDS field: optically invisible submillimetre galaxies,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies An ALMA survey of the S2CLS UDS field: optically invisible submillimetre galaxies,

Reference 21

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:25.786203Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation bc3d69a9-7963-48c1-bf65-ef5881eee049 · outbound

This paper cites The nature of extremely red H –[4.5] > 4 galaxies revealed with SEDS and CANDELS,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies The nature of extremely red H –[4.5] > 4 galaxies revealed with SEDS and CANDELS,

Reference 22

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:25.777764Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 37751ebc-5683-45d6-a2fe-24af3cd89083 · outbound

This paper cites Stellar mass functions of galaxies at 4 < z < 7 from an IRAC-selected sample in COSMOS/UltraVISTA: limits on the abundance of very massive galaxies,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies Stellar mass functions of galaxies at 4 < z < 7 from an IRAC-selected sample in COSMOS/UltraVISTA: limits on the abundance of very massive galaxies,

Reference 23

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:25.769070Z

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No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 9baa2582-7b0d-4fee-b8cb-4e7013e37be4 · outbound

This paper cites The ALPINE-ALMA [CII] survey: data processing, catalogs, and statistical source properties,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies The ALPINE-ALMA [CII] survey: data processing, catalogs, and statistical source properties,

Reference 24

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:25.760606Z

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No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 37d7246b-0f8d-4c03-81b7-ea4abd106c43 · outbound

This paper cites The ALPINE-ALMA [CII] survey: multi-wavelength ancillary data and basic physical measurements,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies The ALPINE-ALMA [CII] survey: multi-wavelength ancillary data and basic physical measurements,

Reference 25

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:25.751676Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 264e9a64-eee4-4a2b-b0aa-00085866ab27 · outbound

This paper cites The Herschel view of the dominant mode of galaxy growth from z = 4 to the present day,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies The Herschel view of the dominant mode of galaxy growth from z = 4 to the present day,

Reference 26

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:25.742740Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 8d92bbe6-b112-45c4-81e9-130cdf287842 · outbound

This paper cites The star formation main sequence in the Hubble Space Telescope Frontier Fields,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies The star formation main sequence in the Hubble Space Telescope Frontier Fields,

Reference 27

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:25.733066Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation a1fd54e9-e4ca-4a82-9a4e-04585898262b · outbound

This paper cites The James Webb Space Telescope mission,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies The James Webb Space Telescope mission,

Reference 28

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:25.724491Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation a11e266e-5774-4f41-bf19-d2577f2e3016 · outbound

This paper cites CEERS key paper. IV . A triality in the nature of HST-dark galaxies,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies CEERS key paper. IV . A triality in the nature of HST-dark galaxies,

Reference 29

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:25.716534Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation fa22c97d-1932-41f5-a99e-c16be06007a7 · outbound

This paper cites JWST/MIRI reveals the true number density of massive galaxies in the early Universe.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies JWST/MIRI reveals the true number density of massive galaxies in the early Universe

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-05T12:04:19.310903Z

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Unavailable: canonical work link unavailable.

Observation 3a552709-629e-423a-9bac-2fd0803daed3 · outbound

This paper cites Unveiling the nature of infrared bright, optically dark galaxies with early JWST data,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies Unveiling the nature of infrared bright, optically dark galaxies with early JWST data,

Reference 31

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:25.707611Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 1cd29756-372b-4f12-ac2b-6cbc97dbcf24 · outbound

This paper cites JWST reveals a population of ultrared, flattened galaxies at 2 ≲ z ≲ 6 previously missed by HST,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies JWST reveals a population of ultrared, flattened galaxies at 2 ≲ z ≲ 6 previously missed by HST,

Reference 32

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:25.698204Z

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No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 5931e170-6e51-4799-b64e-9da5b35b22a3 · outbound

This paper cites A population of red candidate massive galaxies 600 Myr after the Big Bang,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies A population of red candidate massive galaxies 600 Myr after the Big Bang,

Reference 33

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:25.689738Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation d290515d-cfaf-4a2a-8f7d-7f9212ac5333 · outbound

This paper cites The galaxies missed by Hubble and ALMA: the contribution of extremely red galaxies to the cosmic census at 3 < z < 8,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies The galaxies missed by Hubble and ALMA: the contribution of extremely red galaxies to the cosmic census at 3 < z < 8,

Reference 34

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:25.680652Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 2296af36-ed16-41ee-8556-eba36d20541e · outbound

This paper cites JWST unveils heavily obscured (active and passive) sources up to z ∼ 13,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies JWST unveils heavily obscured (active and passive) sources up to z ∼ 13,

Reference 35

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:25.671441Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 300bb035-aabd-4d42-ae4b-e78a029e34ce · outbound

This paper cites The ALMA REBELS survey: cosmic dust temperature evolution out to z ∼ 7,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies The ALMA REBELS survey: cosmic dust temperature evolution out to z ∼ 7,

Reference 36

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:25.661261Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation b89b7c26-896c-4d05-a881-e3c6d5dab890 · outbound

This paper cites A Herschel/PACS far-infrared line emission survey of local luminous infrared gal- axies,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies A Herschel/PACS far-infrared line emission survey of local luminous infrared gal- axies,

Reference 37

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:25.651620Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation fe0f5970-65c2-402c-9a86-4470befcbd79 · outbound

This paper cites Herschel-PACS observations of [OI] 63 μm towards submillimetre galaxies at z ∼ 1,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies Herschel-PACS observations of [OI] 63 μm towards submillimetre galaxies at z ∼ 1,

Reference 38

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:25.642514Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 9c6b7d51-0b2f-490c-9563-53bcdaad947e · outbound

This paper cites Galactic stellar and substellar initial mass function,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies Galactic stellar and substellar initial mass function,

Reference 39

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:25.633751Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 45b5c8f1-0300-4a49-8c8b-98509818b355 · outbound

This paper cites Cosmic star-formation history,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies Cosmic star-formation history,

Reference 40

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:25.625362Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 57bfd3d4-3180-4d06-b409-d3f45bcd9d92 · outbound

This paper cites Simulating galaxy formation with the IllustrisTNG model,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies Simulating galaxy formation with the IllustrisTNG model,

Reference 41

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:25.616487Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation c2ae0c1b-c267-406e-a23e-54bc76943283 · outbound

This paper cites The impact of clustering and angular resolution on far-infrared and millimeter con- tinuum observations,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies The impact of clustering and angular resolution on far-infrared and millimeter con- tinuum observations,

Reference 42

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:25.608005Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 9e2bbf57-04e6-4d66-9d0a-d99b26ca3265 · outbound

This paper cites COSMOS2020: the galaxy stellar mass function. The assembly and star formation cessation of galaxies at 0.2 < z ≤ 7.5,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies COSMOS2020: the galaxy stellar mass function. The assembly and star formation cessation of galaxies at 0.2 < z ≤ 7.5,

Reference 43

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:25.599518Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation cf737f41-05a7-4c5d-96d5-b51143ec2ed4 · outbound

This paper cites Galaxy formation in the Planck cosmology – I. Matching the observed evolution of star formation rates, colours and stellar masses,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies Galaxy formation in the Planck cosmology – I. Matching the observed evolution of star formation rates, colours and stellar masses,

Reference 44

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:25.590466Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation e1303c61-e080-4b5b-a80b-6c94ab12d239 · outbound

This paper cites ISM masses and the star formation law at z = 1 to 6: ALMA observations of dust con- tinuum in 145 galaxies in the COSMOS survey field,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies ISM masses and the star formation law at z = 1 to 6: ALMA observations of dust con- tinuum in 145 galaxies in the COSMOS survey field,

Reference 45

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:25.486517Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 25e38c46-aef2-421e-b339-a33b95af97d5 · outbound

This paper cites JWST CEERS probes the role of stellar mass and morphology in obscuring gal- axies,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies JWST CEERS probes the role of stellar mass and morphology in obscuring gal- axies,

Reference 46

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:25.198331Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 84fe4c33-173a-4109-a251-a7d12e8b750b · outbound

This paper cites Quiescent or dusty? Unveiling the nature of extremely red galaxies at z > 3,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies Quiescent or dusty? Unveiling the nature of extremely red galaxies at z > 3,

Reference 47

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:25.043750Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation c58d6efb-ca1b-41f0-8c0c-c353d6a8e575 · outbound

This paper cites A NIRCam-dark galaxy detected with the MIRI/F1000W filter in the MIDIS/ JADES Hubble Ultra Deep Field,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies A NIRCam-dark galaxy detected with the MIRI/F1000W filter in the MIDIS/ JADES Hubble Ultra Deep Field,

Reference 48

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:24.885946Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 30d0ec5d-6523-4494-9d7e-01b7109a49fd · outbound

This paper cites Accelerated formation of ultra-massive galaxies in the first billion years,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies Accelerated formation of ultra-massive galaxies in the first billion years,

Reference 49

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:24.688702Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 229b28df-86e4-4245-8118-c40d07f6de93 · outbound

This paper cites The contribution of AGNs and star-forming galaxies to the mid-infrared as revealed by their spectral energy distributions,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies The contribution of AGNs and star-forming galaxies to the mid-infrared as revealed by their spectral energy distributions,

Reference 50

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:24.543034Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation a06e019f-c1f0-4d89-b597-177defcf93c6 · outbound

This paper cites New hope for obscured AGN: the PRIMA-NewAthena alliance,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies New hope for obscured AGN: the PRIMA-NewAthena alliance,

Reference 51

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:24.301862Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 709aa5b0-df96-4802-b5d8-b5e05d0b1ff6 · outbound

This paper cites Infrared line diagnostics of active galactic nuclei,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies Infrared line diagnostics of active galactic nuclei,

Reference 52

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:24.106696Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 46932126-4db8-4a1e-986e-87f373b9a4fe · outbound

This paper cites Nebular properties from far-infrared spectroscopy,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies Nebular properties from far-infrared spectroscopy,

Reference 53

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:23.797360Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 609d25c3-a09c-4acc-a285-91f2427ead0c · outbound

This paper cites Dust and nebular emission. I. Models for normal galaxies,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies Dust and nebular emission. I. Models for normal galaxies,

Reference 54

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:23.564185Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation d33b3fb2-1052-4aa8-a0ab-e6b6aedf815c · outbound

This paper cites Extragalactic results from the Infrared Space Observatory,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies Extragalactic results from the Infrared Space Observatory,

Reference 55

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:23.326970Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation faa43a02-4164-4359-ab4d-96d44e604d8f · outbound

This paper cites Observations of ultraluminous infrared galaxies with the Infrared Spectrograph on the Spitzer Space Telescope. II. The IRAS Bright Galaxy Sample,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies Observations of ultraluminous infrared galaxies with the Infrared Spectrograph on the Spitzer Space Telescope. II. The IRAS Bright Galaxy Sample,

Reference 56

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:23.137702Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation c8cbcaf0-10ff-4fbf-a4d9-3c426eaf18a2 · outbound

This paper cites Optical and mid-infrared line emission in nearby Seyfert galaxies,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies Optical and mid-infrared line emission in nearby Seyfert galaxies,

Reference 57

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:22.928011Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 059d7014-8cdd-49e2-9480-4ec43337daa9 · outbound

This paper cites an unresolved cited work.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies Unresolved cited work

Reference 58

Resolution: unresolved; raw_fallback, observed 2026-08-05T12:04:22.753677Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 1334e86e-d89c-45f3-a9a2-3740f8552124 · outbound

This paper cites Disentangling the co-evolution of galaxies and supermassive black holes with PRIMA,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies Disentangling the co-evolution of galaxies and supermassive black holes with PRIMA,

Reference 59

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:22.552989Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 19e49392-c934-4bdf-9ed5-b0e459e1e851 · outbound

This paper cites Overcoming confusion noise with hyperspectral imaging from PRIMAger,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies Overcoming confusion noise with hyperspectral imaging from PRIMAger,

Reference 60

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:22.394819Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 9e036384-2ac2-44bd-9528-6a7553c1f5da · outbound

This paper cites Tracing black hole accretion with SED decomposition and IR lines: from local galaxies to the high-z Universe,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies Tracing black hole accretion with SED decomposition and IR lines: from local galaxies to the high-z Universe,

Reference 61

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:22.226845Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation f2733e08-c049-4df6-9a34-8459318188cc · outbound

This paper cites Origins Space Telescope: predictions for far-IR spectroscopic surveys,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies Origins Space Telescope: predictions for far-IR spectroscopic surveys,

Reference 62

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:22.078553Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 471f5a93-ca03-4538-adc9-3c99598d4f51 · outbound

This paper cites Bolometric luminosity, black hole growth time and slim accretion discs in active galactic nuclei,.

Need for PRIMA to understand the nature and ISM physical conditions of HST-dark galaxies Bolometric luminosity, black hole growth time and slim accretion discs in active galactic nuclei,

Reference 63

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T12:04:21.967232Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

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Reference resolution

Outbound references

Pith citing papers