Shimizu et al., 2015 - Google Patents
Decreased specific star formation rates in AGN host galaxiesShimizu et al., 2015
View HTML- Document ID
- 5474651266312580711
- Author
- Shimizu T
- Mushotzky R
- Meléndez M
- Koss M
- Rosario D
- Publication year
- Publication venue
- Monthly Notices of the Royal Astronomical Society
External Links
Snippet
We investigate the location of an ultra-hard X-ray selected sample of active galactic nuclei (AGN) from the Swift Burst Alert Telescope (BAT) catalogue with respect to the main sequence (MS) of star-forming galaxies using Herschel-based measurements of the star …
- 230000015572 biosynthetic process 0 title abstract description 49
Classifications
-
- G—PHYSICS
- G01—MEASURING; TESTING
- G01N—INVESTIGATING OR ANALYSING MATERIALS BY DETERMINING THEIR CHEMICAL OR PHYSICAL PROPERTIES
- G01N21/00—Investigating or analysing materials by the use of optical means, i.e. using infra-red, visible or ultra-violet light
- G01N21/17—Systems in which incident light is modified in accordance with the properties of the material investigated
- G01N21/25—Colour; Spectral properties, i.e. comparison of effect of material on the light at two or more different wavelengths or wavelength bands
- G01N21/31—Investigating relative effect of material at wavelengths characteristic of specific elements or molecules, e.g. atomic absorption spectrometry
- G01N21/35—Investigating relative effect of material at wavelengths characteristic of specific elements or molecules, e.g. atomic absorption spectrometry using infra-red light
-
- G—PHYSICS
- G01—MEASURING; TESTING
- G01N—INVESTIGATING OR ANALYSING MATERIALS BY DETERMINING THEIR CHEMICAL OR PHYSICAL PROPERTIES
- G01N33/00—Investigating or analysing materials by specific methods not covered by the preceding groups
- G01N33/26—Investigating or analysing materials by specific methods not covered by the preceding groups oils; viscous liquids; paints; inks
- G01N33/28—Oils, i.e. hydrocarbon liquids
-
- G—PHYSICS
- G01—MEASURING; TESTING
- G01N—INVESTIGATING OR ANALYSING MATERIALS BY DETERMINING THEIR CHEMICAL OR PHYSICAL PROPERTIES
- G01N21/00—Investigating or analysing materials by the use of optical means, i.e. using infra-red, visible or ultra-violet light
- G01N21/84—Systems specially adapted for particular applications
-
- G—PHYSICS
- G01—MEASURING; TESTING
- G01N—INVESTIGATING OR ANALYSING MATERIALS BY DETERMINING THEIR CHEMICAL OR PHYSICAL PROPERTIES
- G01N21/00—Investigating or analysing materials by the use of optical means, i.e. using infra-red, visible or ultra-violet light
- G01N21/62—Systems in which the material investigated is excited whereby it emits light or causes a change in wavelength of the incident light
-
- G—PHYSICS
- G06—COMPUTING; CALCULATING; COUNTING
- G06F—ELECTRICAL DIGITAL DATA PROCESSING
- G06F17/00—Digital computing or data processing equipment or methods, specially adapted for specific functions
- G06F17/30—Information retrieval; Database structures therefor; File system structures therefor
-
- G—PHYSICS
- G01—MEASURING; TESTING
- G01J—MEASUREMENT OF INTENSITY, VELOCITY, SPECTRAL CONTENT, POLARISATION, PHASE OR PULSE CHARACTERISTICS OF INFRA-RED, VISIBLE OR ULTRA-VIOLET LIGHT; COLORIMETRY; RADIATION PYROMETRY
- G01J3/00—Spectrometry; Spectrophotometry; Monochromators; Measuring colour
- G01J3/28—Investigating the spectrum
-
- G—PHYSICS
- G01—MEASURING; TESTING
- G01N—INVESTIGATING OR ANALYSING MATERIALS BY DETERMINING THEIR CHEMICAL OR PHYSICAL PROPERTIES
- G01N2201/00—Features of devices classified in G01N21/00
-
- G—PHYSICS
- G01—MEASURING; TESTING
- G01N—INVESTIGATING OR ANALYSING MATERIALS BY DETERMINING THEIR CHEMICAL OR PHYSICAL PROPERTIES
- G01N30/00—Investigating or analysing materials by separation into components using adsorption, absorption or similar phenomena or using ion-exchange, e.g. chromatography or field flow fractionation
- G01N30/02—Column chromatography
Similar Documents
Publication | Publication Date | Title |
---|---|---|
Shimizu et al. | Decreased specific star formation rates in AGN host galaxies | |
Casey et al. | Are dusty galaxies blue? Insights on UV attenuation from dust-selected galaxies | |
Zou et al. | The host-galaxy properties of type 1 versus type 2 active galactic nuclei | |
Azadi et al. | The MOSDEF survey: AGN multi-wavelength identification, selection biases, and host galaxy properties | |
Lehmer et al. | The evolution of normal galaxy X-ray emission through cosmic history: constraints from the 6 Ms Chandra Deep Field-South | |
Budzynski et al. | The similarity of the stellar mass fractions of galaxy groups and clusters | |
Elbaz et al. | GOODS–Herschel: an infrared main sequence for star-forming galaxies | |
D'Andrea et al. | Spectroscopic properties of star-forming host galaxies and type Ia supernova hubble residuals in a nearly unbiased sample | |
Sana et al. | The VLT-FLAMES Tarantula Survey-VIII. Multiplicity properties of the O-type star population | |
Álvarez-Márquez et al. | Dust properties of Lyman-break galaxies at z~ 3 | |
Arnouts et al. | Encoding of the infrared excess in the NUVrK color diagram for star-forming galaxies | |
Manara et al. | Hubble Space telescope measures of mass accretion rates in the Orion nebula cluster | |
Rosario et al. | The host galaxies of X-ray selected active galactic nuclei to z= 2.5: Structure, star formation, and their relationships from CANDELS and Herschel/PACS | |
Ade et al. | Planck intermediate results. XV. A study of anomalous microwave emission in Galactic clouds | |
van Aarle et al. | The optically bright post-AGB population of the LMC | |
Bayo et al. | Spectroscopy of very low-mass stars and brown dwarfs in the Lambda Orionis star-forming region-II. Rotation, activity and other properties of spectroscopically confirmed members of Collinder 69 | |
Nilsson et al. | The nature of z~ 2.3 Lyman-α emitters | |
Cicone et al. | The final data release of ALLSMOG: a survey of CO in typical local low-M∗ star-forming galaxies | |
Lawrence et al. | Slow-blue nuclear hypervariables in PanSTARRS-1 | |
Bodensteiner et al. | The young massive SMC cluster NGC 330 seen by MUSE-II. Multiplicity properties of the massive-star population | |
Okada et al. | Probing the role of polycyclic aromatic hydrocarbons in the photoelectric heating within photodissociation regions | |
Laskar et al. | EXPLORING THE GALAXY MASS–METALLICITY RELATION AT z∼ 3–5 | |
Galbany et al. | Type Ia supernova properties as a function of the distance to the host galaxy in the SDSS-II SN survey | |
Barbary et al. | THE HUBBLE SPACE TELESCOPE* CLUSTER SUPERNOVA SURVEY. II. THE TYPE Ia SUPERNOVA RATE IN HIGH-REDSHIFT GALAXY CLUSTERS | |
Sierchio et al. | The decay of debris disks around solar-type stars |