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263 results on '"Messias H."'

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51. The hidden side of cosmic star formation at z > 3:Bridging optically dark and Lyman-break galaxies with GOODS-ALMA

52. z-GAL:A NOEMA spectroscopic redshift survey of bright Herschel galaxies: I.Overview

53. z -GAL:A NOEMA spectroscopic redshift survey of bright Herschel galaxies II. Dust properties

54. The hidden side of cosmic star formation at z > 3

55. Bright extragalactic ALMA redshift survey (BEARS) III: detailed study of emission lines from 71Herscheltargets

56. Ultra Steep Spectrum Radio Sources in the Lockman Hole: SERVS Identifications and Redshift Distribution at the Faintest Radio Fluxes

57. BJS commission on surgery and perioperative care post-COVID-19

58. Orbital motion near Sagittarius A*

60. The Spitzer Extragalactic Representative Volume Survey (SERVS): Survey Definition and Goals ( PASP, 124, 714, [2012] )

61. The bright extragalactic ALMA redshift survey (BEARS) – II. Millimetre photometry of gravitational lens candidates

62. The bright extragalactic ALMA redshift survey (BEARS) I: redshifts of bright gravitationally lensed galaxies from the Herschel ATLAS

63. GOODS-ALMA 2.0: Source catalog, number counts, and prevailing compact sizes in 1.1 mm galaxies

64. The bright extragalactic ALMA redshift survey (BEARS) I: Redshifts of bright gravitationally lensed galaxies from the Herschel ATLAS

66. The bright extragalactic ALMA redshift survey (BEARS) I: redshifts of bright gravitationally lensed galaxies from the Herschel ATLAS

67. Epidemiological, clinical and laboratory aspects of Angiostrongylus cantonensis infection: an integrative review

68. Close-up view of a luminous star-forming galaxy at z=2.95

70. Polarimetric Properties of Event Horizon Telescope Targets from ALMA

71. Cosmic evolution of molecular gas mass density from an empirical relation between $\rm L_{1.4GHz}$ and $\rm L^{\prime}_{CO}$

72. Polarimetric Properties of Event Horizon Telescope Targets from ALMA

73. A Spitzer survey of Deep Drilling Fields to be targeted by the Vera C. Rubin Observatory Legacy Survey of Space and Time

74. Turbulent Gas in Lensed Planck-selected Starbursts at z ∼ 1–3.5

75. Close-up view of a luminous star-forming galaxy at z = 2.95

76. Ultra Steep Spectrum Radio Sources in the Lockman Hole: SERVS Identifications and Redshift Distribution at the Faintest Radio Fluxes

77. GOODS-ALMA: Optically dark ALMA galaxies shed light on a cluster in formation at z = 3.5

79. NOEMA redshift measurements of bright Herschel galaxies

80. A SCUBA-2 selected herschel-SPIRE dropout and the nature of this population

81. GOODS-ALMA: 1.1 mm galaxy survey

82. GOODS-ALMA:Optically dark ALMA galaxies shed light on a cluster in formation at z=3.5

83. The ALMA Frontier Fields Survey

84. A SCUBA-2 selected Herschel-SPIRE dropout and the nature of this population

86. VALES V:a kinematic analysis of the molecular gas content in H-ATLAS galaxies at z similar to 0.03-0.35 using ALMA

87. Cosmic evolution of molecular gas mass density from an empirical relationship between L1.4 GHz and L′CO.

88. GOODS-ALMA: 1.1 mm galaxy survey

89. VALES V: a kinematic analysis of the molecular gas content inH-ATLAS galaxies atz ∼ 0.03–0.35 using ALMA

90. GOODS-ALMA:1.1 mm galaxy survey I. Source catalog and optically dark galaxies

91. The ALMA Phasing System: A Beamforming Capability for Ultra-high-resolution Science at (Sub)Millimeter Wavelengths

92. The ALMA Frontier Fields Survey

93. Molecular gas, dust, and star formation in galaxies

94. GRB 980425 host: [C II], [O I], and CO lines reveal recent enhancement of star formation due to atomic gas inflow

95. The ALMA Frontier Fields Survey

96. GRB 980425 host: [C II], [O I], and CO lines reveal recent enhancement of star formation due to atomic gas inflow

97. WITNESSING THE BIRTH OF THE RED SEQUENCE: ALMA HIGH-RESOLUTION IMAGING OF [C II] AND DUST IN TWO INTERACTING ULTRA-RED STARBURSTS ATz= 4.425

99. VALES V: a kinematic analysis of the molecular gas content in H-ATLAS galaxies at z ∼ 0.03–0.35 using ALMA.

100. Lens Models of Herschel-selected Galaxies from High-resolution Near-IR Observations

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