[CNG2015] PLCK G145.2+50.9 , the SIMBAD biblio

[CNG2015] PLCK G145.2+50.9 , the SIMBAD biblio (9 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST14:21:03


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Title First 3 Authors
2015A&A...581A.105C 18       D               2 17 87 Planck's dusty GEMS: The brightest gravitationally lensed galaxies discovered with the Planck all-sky survey. CANAMERAS R., NESVADBA N.P.H., GUERY D., et al.
2016MNRAS.458.4383H 41           X         1 23 25 Early science with the Large Millimeter Telescope: observations of extremely luminous high-z sources identified by Planck. HARRINGTON K.C., YUN M.S., CYBULSKI R., et al.
2018A&A...620A..61C 3 16 48 Planck's dusty GEMS. VI. Multi-J CO excitation and interstellar medium conditions in dusty starburst galaxies at z = 2-4. CANAMERAS R., YANG C., NESVADBA N.P.H., et al.
2019ApJ...871...51F 644       D     X C       15 115 8 PLCK G165.7+67.0: analysis of a massive lensing cluster in a Hubble Space Telescope census of submillimeter giant arcs selected using Planck/Herschel. FRYE B.L., PASCALE M., QIN Y., et al.
2019A&A...624A..23N 17       D               5 12 7 Planck's Dusty GEMS. VII. Atomic carbon and molecular gas in dusty starburst galaxies at z = 2 to 4. NESVADBA N.P.H., CANAMERAS R., KNEISSL R., et al.
2019AJ....158...34D 43           X         1 14 27 Ultra-bright CO and [CI] emission in a lensed z = 2.04 submillimeter galaxy with extreme molecular gas properties. DANNERBAUER H., HARRINGTON K., DIAZ-SANCHEZ A., et al.
2021A&A...645A..45C 1759       D     X C F     39 45 10 Planck's Dusty GEMS. VIII. Dense-gas reservoirs in the most active dusty starbursts at z ∼ 3. CANAMERAS R., NESVADBA N.P.H., KNEISSL R., et al.
2022MNRAS.517..962D viz 18       D               1 385 17 Dust, CO, and [C I]: cross-calibration of molecular gas mass tracers in metal-rich galaxies across cosmic time. DUNNE L., MADDOX S.J., PAPADOPOULOS P.P., et al.
2024ApJ...961....2K 270       D     X C       5 30 ~ PASSAGES: The Wide-ranging, Extreme Intrinsic Properties of Planck-selected, Lensed Dusty Star-forming Galaxies. KAMIENESKI P.S., YUN M.S., HARRINGTON K.C., et al.

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