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1
Absorption Line Oscillator Strengths for the C 2Π(0)-A 2Σ+(0) Band of Nitric Oxide
Published 2023-01-01Subjects: Get full text
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2
Cross-correlation Techniques to Mitigate the Interloper Contamination for Line Intensity Mapping Experiments
Published 2024-01-01Subjects: “…Line intensities…”
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3
Why Are Optical Coronal Lines Faint in Active Galactic Nuclei?
Published 2024-01-01Subjects: Get full text
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4
Laboratory Measurement of CH2DOH Line Intensities in the Millimeter-wave Region
Published 2023-01-01Subjects: Get full text
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5
Laboratory Measurement of Millimeter-wave Transitions of 13CH2DOH for Astronomical Use
Published 2022-01-01Subjects: Get full text
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6
S-type Stars: Line List for the A2Π–X2Σ+ Band System of LaO
Published 2023-01-01Subjects: Get full text
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7
Emission Line Intensity Ratios of Fe xxvi/ xxv/ xxiv in Solar Flares Observed by Hinotori
Published 2024-01-01Subjects: Get full text
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8
Steep Balmer Decrement in Weak AGNs May Not Be Caused by Dust Extinction: Clues from Low-luminosity AGNs and Changing-look AGNs
Published 2023-01-01Subjects: Get full text
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9
Deuterated Polycyclic Aromatic Hydrocarbons in the Interstellar Medium: The Aliphatic C–D Band Strengths
Published 2023-01-01Subjects: Get full text
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10
Characterizing the Conditional Galaxy Property Distribution Using Gaussian Mixture Models
Published 2023-01-01Subjects: Get full text
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12
LIMpy: A Semianalytic Approach to Simulating Multiline Intensity Maps at Millimeter Wavelengths
Published 2023-01-01Subjects: “…Line intensities…”
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13
Probing Dark Energy and Modifications of Gravity with Ground-based millimeter-wavelength Line Intensity Mapping
Published 2024-01-01Subjects: Get full text
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14
X-Ray Spectroscopy of the Dwarf Nova Z Chamaeleontis in Quiescence and Outburst Using the XMM-Newton Observatory
Published 2024-01-01Subjects: Get full text
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15
Reconstruction of Cosmological Initial Density Field with Observations from the Epoch of Reionization
Published 2024-01-01Subjects: Get full text
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16
Critically Evaluated Atomic Data for the Au iv Spectrum
Published 2023-01-01Subjects: Get full text
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17
The Weakness of Soft X-Ray Intensity: Possible Physical Reason for Weak-line Quasars
Published 2024-01-01Subjects: Get full text
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19
High Resolution Infrared Spectroscopy in Support of Ozone Atmospheric Monitoring and Validation of the Potential Energy Function
Published 2022-01-01Subjects: Get full text
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20
Métodos empleados en el análisis de espectroscopía óptica de emisión: una revisión
Published 2015-01-01Subjects: Get full text
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