H-ATLAS J091043.0-000322 , the SIMBAD biblio

H-ATLAS J091043.0-000322 , the SIMBAD biblio (31 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.20CEST04:33:11

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
2010Sci...330..800N 11 15 348 The detection of a population of submillimeter-bright, strongly lensed galaxies. NEGRELLO M., HOPWOOD R., DE ZOTTI G., et al.
2012ApJ...749...65G viz 15       D               1 141 59 Herschel-ATLAS: toward a sample of ∼1000 strongly lensed galaxies. GONZALEZ-NUEVO J., LAPI A., FLEUREN S., et al.
2012ApJ...757..135L 830       D     X C       21 19 76 Measurements of CO redshifts with z-spec for lensed submillimeter galaxies discovered in the H-ATLAS survey. LUPU R.E., SCOTT K.S., AGUIRRE J.E., et al.
2013MNRAS.435.2753P 16       D               1 43 23 H-ATLAS: estimating redshifts of Herschel sources from sub-mm fluxes. PEARSON E.A., EALES S., DUNNE L., et al.
2013ApJ...779...25B 212       D     X         6 66 171 Gravitational lens models based on Submillimeter Array imaging of Herschel-selected strongly lensed sub-millimeter galaxies at z > 1.5. BUSSMANN R.S., PEREZ-FOURNON I., AMBER S., et al.
2014ApJ...780..142F 2504   K A S   X C       62 3 16 The second-generation z (redshift) and early universe spectrometer. I. First-light observation of a highly lensed local-ulirg analog at high-z. FERKINHOFF C., BRISBIN D., PARSHLEY S., et al.
2014MNRAS.440.1999N 923       D     X C       23 10 55 Herschel -ATLAS: deep HST/WFC3 imaging of strongly lensed submillimetre galaxies. NEGRELLO M., HOPWOOD R., DYE S., et al.
2014MNRAS.440.2013D 136       D     X         4 10 44 Herschel-ATLAS: modelling the first strong gravitational lenses. DYE S., NEGRELLO M., HOPWOOD R., et al.
2014A&A...568A..62D 16       D               1 467 300 The applicability of far-infrared fine-structure lines as star formation rate tracers over wide ranges of metallicities and galaxy types. DE LOOZE I., CORMIER D., LEBOUTEILLER V., et al.
2014ApJ...794..142G 16       D               2 108 133 Star formation relations and CO spectral line energy distributions across the J-ladder and redshift. GREVE T.R., LEONIDAKI I., XILOURIS E.M., et al.
2016A&A...591A..73G 41           X         1 21 34 ALMA finds dew drops in the dusty spider's web. GULLBERG B., LEHNERT M.D., DE BREUCK C., et al.
2016A&A...595A..80Y viz 418       D     X C       10 38 49 Submillimeter H2O and H2O+ emission in lensed ultra- and hyper-luminous infrared galaxies at z∼ 2-4. YANG C., OMONT A., BEELEN A., et al.
2017ApJ...834....5S 85             C       1 19 80 The spatially resolved [CII] cooling line deficit in galaxies. SMITH J.D.T., CROXALL K., DRAINE B., et al.
2017ApJ...837...12W 48 17 The interstellar medium in high-redshift submillimeter galaxies as probed by infrared spectroscopy. WARDLOW J.L., COORAY A., OSAGE W., et al.
2017MNRAS.465.3558N viz 16       D               2 101 96 The Herschel-ATLAS: a sample of 500 µm-selected lensed galaxies over 600 deg2. NEGRELLO M., AMBER S., AMVROSIADIS A., et al.
2017ApJ...850..170O 1991     A D     X C       49 13 14 High dense gas fraction in intensely star-forming dusty galaxies. OTEO I., ZHANG Z.-Y., YANG C., et al.
2017A&A...608A.144Y viz 43           X         1 32 90 Molecular gas in the Herschel-selected strongly lensed submillimeter galaxies at z∼ 2-4 as probed by multi-J CO lines. YANG C., OMONT A., BEELEN A., et al.
2018A&A...610A..53M viz 975     A S   X C       22 2 8 Chandra and ALMA observations of the nuclear activity in two strongly lensed star-forming galaxies. MASSARDI M., ENIA A.F.M., NEGRELLO M., et al.
2018MNRAS.475.3467E 16       D               1 21 6 The Herschel-ATLAS: magnifications and physical sizes of 500-µm-selected strongly lensed galaxies. ENIA A., NEGRELLO M., GURWELL M., et al.
2018MNRAS.475.4939A 99       D         F     3 34 8 ALMA observations of lensed Herschel sources: testing the dark matter halo paradigm. AMVROSIADIS A., EALES S.A., NEGRELLO M., et al.
2018ApJ...867..140L 3047 T   A D     X C       73 4 7 Resolving star formation on subkiloparsec scales in the high-redshift galaxy
SDP.11 using gravitational lensing. 		LAMARCHE C., VERMA A., VISHWAS A., et al.
2018MNRAS.481...59Z 798       D     X C F     18 70 41 Far-infrared Herschel SPIRE spectroscopy of lensed starbursts reveals physical conditions of ionized gas. ZHANG Z.-Y., IVISON R.J., GEORGE R.D., et al.
2019A&A...622A.106M viz 17       D               1 612 ~ Multifrequency filter search for high redshift sources and lensing systems in Herschel-ATLAS. MANJON-GARCIA A., HERRANZ D., DIEGO J.M., et al.
2019A&A...627A..31G viz 17       D               1 8390 ~ SHALOS: Statistical Herschel-ATLAS lensed objects selection. GONZALEZ-NUEVO J., SUAREZ GOMEZ S.L., BONAVERA L., et al.
2019ApJ...880...92J 60       D     X         2 17 18 Spatially resolved water emission from gravitationally lensed dusty star-forming galaxies at z ∼ 3. JARUGULA S., VIEIRA J.D., SPILKER J.S., et al.
2021A&A...645A..45C 174           X C       3 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.
2020PASJ...72...41L 187       D       C F     4 41 ~ HCN 3-2 survey towards a sample of local galaxies. LI F., WANG J., FANG M., et al.
2021A&A...652A..23F viz 17       D               1 66 8 Measuring chemical abundances with infrared nebular lines: HII-CHI-MISTRY-IR. FERNANDEZ-ONTIVEROS J.A., PEREZ-MONTERO E., VILCHEZ J.M., et al.
2022MNRAS.511.1408G 152       D     X         4 35 2 The far-infrared/radio correlation for a sample of strongly lensed dusty star-forming galaxies detected by Herschel. GIULIETTI M., MASSARDI M., LAPI A., et al.
2022ApJ...928..179L 179           X C       3 25 2 Multiphase ISM in the z = 5.7 Hyperluminous Starburst SPT 0346-52. LITKE K.C., MARRONE D.P., ARAVENA M., et al.
2023A&A...679A.131R viz 140         O X         3 138 ~ Diagnosing the interstellar medium of galaxies with far-infrared emission lines II. [C II], [O I], [O III], [N II], and [N III] up to z = 6. RAMOS PADILLA A.F., WANG L., VAN DER TAK F.F.S., et al.

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