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British electronic music group
Redshift is a British electronic music group, founded in 1996 by Mark Shreeve. Their musical style is rooted in the early to mid 1970s German electronic
Redshift_(group)
Change in wavelength of light
In physics, a redshift is an increase in the wavelength, or equivalently, a decrease in the frequency, of electromagnetic radiation (such as light). The
Redshift
Topics referred to by the same term
Marvel Comics universe Redshift (group), an English electronic music group The Redshift, an album by Omnium Gatherum "Redshift" (Enter Shikari song) "Red
Redshift_(disambiguation)
Large astronomical structure
scientists have expressed doubt whether these structures really exist. Redshift, represented by "z," is a fundamental concept in astrophysics. It measures
Large_quasar_group
Physical effect in general relativity
In physics and general relativity, gravitational redshift (known as Einstein shift in older literature) is the phenomenon that electromagnetic waves or
Gravitational_redshift
2008 studio album by Omnium Gatherum
The Redshift is the fourth studio album by Finnish melodic death metal band Omnium Gatherum. It is the band's second release for the Candlelight Records
The_Redshift
Concept in cosmology
information from redshifts. Two years later, astronomers Roger G. Clowes and Luis E. Campusano discovered the Clowes–Campusano LQG, a large quasar group measuring
Large-scale structure of the universe
Large-scale_structure_of_the_universe
with a spectroscopic redshift. UDFy-38135539, discovered in 2009, with z=8.6, does not appear on this list because its claimed redshift is disputed. Follow-up
List_of_galaxies
Physical hypothesis
Redshift quantization, also referred to as redshift periodicity, redshift discretization, preferred redshifts and redshift-magnitude bands, is the hypothesis
Redshift_quantization
Visual grouping of five galaxies
7320 indicates a small redshift (790 km/s) while the other four exhibit large redshifts (near 6,600 km/s). Since galactic redshift is proportional to distance
Stephan's_Quintet
Models of the universe which deviate from then-current scientific consensus
equation of state of Dark Energy for 4 common models as a function of redshift. Our current universe is at z = 0 {\displaystyle z=0} , and the cosmological
Non-standard_cosmology
Possible large cosmic structure
their redshifts spectroscopically. They subdivided them to different group subsamples of different redshifts, initially with five groups, six groups, seven
Hercules–Corona Borealis Great Wall
Hercules–Corona_Borealis_Great_Wall
Active galactic nucleus (AGN) containing a supermassive black hole
usually categorized as a subclass of the more general category of AGN. The redshifts of quasars are of cosmological origin. The term quasar originated as a
Quasar
Anglo-Australian Telescope survey, 1997–2002
In astronomy, the 2dF Galaxy Redshift Survey (Two-degree-Field Galaxy Redshift Survey), 2dF or 2dFGRS is a redshift survey conducted by the Australian
2dF_Galaxy_Redshift_Survey
Energy driving the accelerated expansion of the universe
be used to accurately measure distances. Comparing this distance to the redshift (which measures the speed at which the supernova is receding) shows that
Dark_energy
Vast empty spaces between filaments with few or no galaxies
three-dimensional mapping of the universe. Through redshift surveys, their depth was calculated from the individual redshifts of the galaxies due to the expansion of
Void_(astronomy)
American astronomer (1927-2013)
non-standard cosmology incorporating intrinsic redshift. Arp developed those views in a book, Seeing Red: Redshift, Cosmology and Academic Science, in 1998
Halton_Arp
Galaxy in the constellation Sextans
Cosmos Redshift 7 (also known as COSMOS Redshift 7, Galaxy Cosmos Redshift 7, Galaxy CR7 or CR7) is a high-redshift Lyman-alpha emitter galaxy. At a redshift
Cosmos_Redshift_7
Loose group of galaxies in the constellation Ursa Major
The M101 Group is a loose group of galaxies located in the constellation Ursa Major. The group is named after the brightest galaxy in the group, the Pinwheel
M101_Group
Observation in physical cosmology
galaxy's recessional velocity is typically determined by measuring its redshift, a shift in the frequency of light emitted by the galaxy. The discovery
Hubble's_law
Galaxy group in Ursa Major and Camelopardalis
97–111. Yun, M. S. (1999). "Tidal Interactions in M81 Group". Galaxy Interactions at Low and High Redshift. Vol. 186. p. 81. Bibcode:1999IAUS..186...81Y. doi:10
M81_Group
Class of hypothetical redshift mechanisms
light is a class of hypothetical redshift mechanisms that was proposed as an alternative explanation for the redshift-distance relationship. These models
Tired_light
Cosmological formulas for expanding universe
small redshifts. The expressions for these distances are most practical when written as functions of redshift z {\displaystyle z} , since redshift is always
Distance_measure
Galaxy cluster in the constellation of Cassiopeia
342/Maffei Group (also known as the IC 342 Group or the Maffei 1 Group) corresponds to one or two galaxy groups close to the Local Group. The member
IC_342/Maffei_Group
Loosely grouped galaxy group in the constellation Sculptor
Sculptor Group is a loose group of galaxies visible near the south galactic pole. The group is one of the closest groups of galaxies to the Local Group; the
Sculptor_Group
Group of galaxies in the constellation Draco
The NGC 5866 Group is a small group of galaxies located in the constellation Draco. The group is named after NGC 5866, the galaxy with the highest apparent
NGC_5866_Group
Very distant gamma-ray burst detected in 2009
determine that its redshift is z = 8.2, making it one of the most distant objects detected at that time with a spectroscopic redshift (GN-z11, discovered
GRB_090423
Galaxy group in the constellation Leo
The M96 Group (also known as the Leo I Group) is a group of galaxies in the constellation Leo. This group contains between 8 and 24 galaxies, including
M96_Group
In 1958, cluster Cl 0024+1654 and Cl 1447+2619 were estimated to have redshifts of z=0.29 and z=0.35 respectively. However, they were not spectroscopically
List of galaxy groups and clusters
List_of_galaxy_groups_and_clusters
Visual grouping of galaxies in the constellation Pegasus
non-group member, NGC 7320, might be a member of a true NGC 7331 group, having a similar redshift to that nearby galaxy. Wild's Triplet Zwicky's Triplet Robert's
NGC_7331_Group
Quasar in the constellation Boötes
quasar, or quasi-stellar object, that has a redshift of 3.235. A group of three foreground galaxies at a redshift of about 1 are behaving as gravitational
CLASS_B1359+154
Region of overdensity of galaxies
their redshifts are large enough and regular enough to reveal that they are slightly drawn towards the attraction. The variations in their redshifts are
Great_Attractor
Aggregation of galaxies with 50 or fewer members
mass, redshift and fossilness in Magneticum hydrodynamic simulations An old galaxy group: Chandra X-ray observations of the nearby fossil group NGC 6482
Galaxy_group
Group of galaxies in the constellation Leo
known as the M66 Group) is a small group of galaxies about 35 million light-years away in the constellation Leo. This galaxy group consists of the spiral
Leo_Triplet
British composer (1957–2022)
Buller. In 1996, Shreeve formed the group Redshift with his brother Julian, James Goddard and Rob Jenkins. The group has recorded nine albums to date and
Mark_Shreeve
Test of gravitational redshift
of general relativity to be verified. The measurement of gravitational redshift and blueshift by this experiment validated the prediction of the equivalence
Pound–Rebka_experiment
All of space observable from the Earth at the present
progressively redder and fainter light. For instance, objects with the current redshift z from 5 to 10 will only be observable up to an age of 4–6 billion years
Observable_universe
Galaxy in the constellation Centaurus
during a redshift survey of the ESO/SRC Survey Fields 444 and 445 of the Klemola 27 group (now known as the IC 4329 galaxy group). The group consists
ESO_383-76
Mathematical model of the Big Bang
an expansion of the spatial metric that is well documented, both as the redshift of prominent spectral absorption or emission lines in the light from distant
Lambda-CDM_model
Galaxy cluster in constellation Canes Venatici
The M51 Group is a group of galaxies located in Canes Venatici. The group is named after the brightest galaxy in the group, the Whirlpool Galaxy (M51A)
M51_Group
British astronomer
research on redshift in radio galaxies and quasars. After seven years working in England (where he helped establish the astrophysics group at Liverpool
James_Dunlop_(astronomer)
Spatial distortion in cosmology
Redshift-space distortions are an effect in observational cosmology where the spatial distribution of galaxies appears squashed and distorted when their
Redshift-space_distortions
Largest known gravitationally bound object in universe; aggregation of galaxies
clusters. Groups of radio sources (that may include diffuse structures or AGN) have been used as tracers of cluster location. At high redshift imaging around
Galaxy_groups_and_clusters
Type Ia supernova in Ursa Major (UMa for short)
(pronounced: Supernova Hope) is a Type Ia supernova discovered in 2023, at a redshift of z=1.78. It is a supernova discovered in a gravitationally lensed subject
SN_H0pe
Increase in distance between parts of the universe
dynamics. For photons, expansion leads to the cosmological redshift. While the cosmological redshift is often explained as the stretching of photon wavelengths
Expansion_of_the_universe
Largest structures in the universe, made of galaxies
Bagoly, Zsolt (2014). "Possible structure in the GRB sky distribution at redshift two". Astronomy & Astrophysics. 561: id.L12. arXiv:1401.0533. Bibcode:2014A&A
Galaxy_filament
Physical theory of the cosmos
of light elements, the cosmic microwave background (CMB) radiation, the redshift of galaxies and the large-scale structure of the universe. The observed
Big_Bang
Series of galaxy clusters
of members of the group. Column 5: Brightest member of the group Column 6: Redshift of the group. Column 7: Distance of the group (Millions of light-years)
Leo_Cloud
Hypothetical group of multiple universes
My Quest for the Ultimate Nature of Reality. Knopf Doubleday Publishing Group. ISBN 978-0-307-59980-3. J. Schmidhuber (1997): A Computer Scientist's View
Multiverse
Group of galaxies in the constellations Centaurus, Hydra and Virgo
and Jerjen found that NGC 5011C has an optical redshift of 647 km/s and thus is a member of the Cen A group rather than of the distant Centaurus galaxy cluster
Centaurus_A/M83_Group
Cosmological time duration
galaxies seemed to be (the dimmer they appeared) the greater was their redshift, and thus the faster they seemed to be moving away. This was the first
Age_of_the_universe
Series of galaxy clusters
of members of the group. Column 5: Brightest member of the group Column 6: Redshift of the group. Column 7: Distance of the group (Millions of light-years)
Virgo_III_Cloud
American astronomer (1889–1953)
the redshift remained unclear. Lemaître predicted on theoretical grounds based on Albert Einstein's equations for general relativity the redshift-distance
Edwin_Hubble
Astronomical catalogue of galaxy clusters
galaxies is an all-sky catalog of 4,073 rich galaxy clusters of nominal redshift z ≤ 0.2. This catalog supplements a revision of George O. Abell's original
Abell_catalogue
Galaxy cluster in the constellation Dorado
from the list. In 2006, the list was refined again by Firth et al. Using redshift data, they excluded eleven (as being background galaxies or interloper)
Dorado_Group
American businessman (born 1964)
receiving corporate welfare. This followed revelations by the non-profit group New Food Economy which found that one third of Amazon workers in Arizona
Jeff_Bezos
Galaxy group in the constellations Corvus and Crater
NGC 4038 Group is a group of galaxies in the constellations Corvus and Crater. The group may contain between 13 and 27 galaxies. The group's best known
NGC_4038_Group
Fluctuations in the density of the normal matter of the universe
recombination happened when the universe was around 379,000 years old, or at a redshift of z = 1089. At this age, the size of BAO bubbles were 450,000 light-years
Baryon_acoustic_oscillations
Cosmological phenomenon
them. The distance can then be compared to the supernovae's cosmological redshift, which measures how much the universe has expanded since the supernova
Accelerating expansion of the universe
Accelerating_expansion_of_the_universe
Large quasar group consisting of 34 quasars
in the observable universe. It was named U1.28 because of its average redshift of 1.28, and is located in the constellation of Leo. It was also notable
Clowes–Campusano_LQG
Galaxy cluster in the constellation Capricornus
"This redshift corresponds to a distance of 120Mpc or 400 million light years (using H0 = 75km/s/Mpc and q0 = 0.1). At the distance of the group, this
HCG_87
Small group of galaxies in the constellation of Pisces
The M74 Group (also known as the NGC 628 Group) is a small group of galaxies in the constellation Pisces. The face-on spiral galaxy M74 (NGC 628) is the
M74_Group
Cosmological model in which the universe does not expand
After the discovery of the redshift-distance relationship (deduced by the inverse correlation of galactic brightness to redshift) by American astronomers
Static_universe
Type of starburst galaxy
scientific literature by Yang et al. (2017) as GPs that were at a distance of redshift z=0.05 or less, although similar galaxies had originally been named BBs
Blueberry_galaxy
Trace radiation from the early universe
However, the photons have grown less energetic due to the cosmological redshift associated with the expansion of the universe. The surface of last scattering
Cosmic_microwave_background
2016 studio album by Cult of Luna & Julie Christmas
more seriously when Cult of Luna curated the May 2014 festival Beyond the Redshift in London. Cult of Luna wanted Christmas to participate and perform her
Mariner_(album)
Galaxy in the constellation Centaurus
distance of 155.6 ± 10.9 Mly (47.70 ± 3.35 Mpc). In addition, two non-redshift measurements give a distance of 155.74 ± 30.17 Mly (47.750 ± 9.250 Mpc)
NGC_3783
Mercury, the bending of light in gravitational fields, and the gravitational redshift. The precession of Mercury was already known; experiments showing light
Tests_of_general_relativity
Large Quasar Group
comprehensive Sloan Digital Sky Survey, a major multi-imaging and spectroscopic redshift survey of the sky. They reported that the grouping was, as they announced
Huge-LQG
Family of linear transformations
group O(3,1), a Lie group. In other words, the Lorentz group is O(3,1). As presented in this article, any Lie groups mentioned are matrix Lie groups.
Lorentz_transformation
Representation of the symmetry group of spacetime in special relativity
The Lorentz group is a Lie group of symmetries of the spacetime of special relativity. This group can be realized as a collection of matrices, linear
Representation theory of the Lorentz group
Representation_theory_of_the_Lorentz_group
Topics referred to by the same term
Sachs–Wolfe effect, a gravitational redshift of CMB radiation Institute for the Study of War, an American research group International School Winterthur,
ISW
Neighboring supercluster in the constellations Pavo, Indus and Telescopium
Sculptor Void. In 1983, in a paper by Winkler et al it was suggested based on redshift maps of the distribution of galaxies that the Pavo–Indus Supercluster may
Pavo–Indus_Supercluster
Basin of attraction home to the Milky Way
For example, South African astronomer Tony Fairall stated in 1988 that redshifts suggested that the Virgo and Hydra–Centaurus superclusters may be connected
Laniakea_Supercluster
German-born theoretical physicist (1879–1955)
predicted the phenomena of gravitational time dilation, gravitational redshift and gravitational lensing. In 1911, Einstein published another article
Albert_Einstein
Cosmological epoch c. 370,000 years after the Big Bang
atoms. Recombination occurred about 378000 years after the Big Bang (at a redshift of z = 1100). The "re-" in "recombination" is misleading, since the Big
Recombination_(cosmology)
Zodiac constellation straddling the celestial equator
one of which is HCG 62. A Hickson Compact Group, HCG 62 is at a distance of 200 Mly from Earth (redshift 0.0137) and possesses a large central elliptical
Virgo_(constellation)
Cosmological process in the early universe
than the ionization rate. At around 379,000 years after the Big Bang (redshift z = 1089), this recombination left most normal matter in the form of neutral
Reionization
Paid subscription service offered by Amazon
In-Garage At CES 2019, Amazon announced a partnership with the Chamberlain Group, allowing packages to be placed in customers' garages with myQ-enabled openers
Amazon_Prime
Galaxy in the constellation Hydra
The galaxy lies about 110 million light years away from Earth based on redshift-independent methods, which means, given its apparent dimensions, that NGC
NGC_3124
Closest neighboring galaxy supercluster
20 Mpc (65.2 Mly), and lies at a distance of 19 Mpc (62.0 Mly) with a redshift of 1161 km/s. Region A is almost parallel to the supergalactic plane. Region
Southern_Supercluster
Theories about the end of the universe
(GWB) Microwave (CMB) · Neutrino (CNB) Expansion · Future Hubble's law · Redshift Expansion of the universe FLRW metric · Friedmann equations Lambda-CDM
Ultimate_fate_of_the_universe
Galaxy group in the constellation Ursa Major
The M109 Group (also known as the NGC 3992 Group or Ursa Major cloud) is a group of galaxies about 55 million light-years away in the constellation Ursa
M109_Group
Study of the origin of the universe (structure and evolution)
have been made to map the universe in redshift space. By combining redshift with angular position data, a redshift survey maps the 3D distribution of matter
Observational_cosmology
Galaxy in the constellation Coma Berenicies
Hubble distance of 52.7 ± 3.8 Mly (16.17 ± 1.17 Mpc). However, 26 non-redshift measurements give a much closer distance of 24.56 ± 1.58 Mly (7.530 ± 0
NGC_4559
Galaxy in the constellation Virgo
distance of 369.6 ± 25.9 Mly (113.32 ± 7.94 Mpc). Additionally, 16 non-redshift measurements give a similar mean distance of 374.23 ± 10.11 Mly (114.738 ± 3
NGC_5185
Galaxy in the constellation Ursa Major
star-forming galaxies – III. Calibration of the LX-SFR relation up to redshift z ≈ 1.3". Monthly Notices of the Royal Astronomical Society. 437 (2): 1698–1707
NGC_3631
Galaxy in the constellation Virgo
Hubble distance of 142.4 ± 10.0 Mly (43.66 ± 3.08 Mpc). However, two non-redshift measurements give a closer distance of 131.11 ± 3.59 Mly (40.200 ± 1.100 Mpc)
NGC_4653
Compact astronomical body
mass have a common cause. Using the principle, Einstein predicted the redshift and the lensing effect of gravity on light; his prediction of gravitational
Black_hole
Group of galaxies in the constellation Leo
Hickson Compact Group 44 (HCG 44) is a group of galaxies in the constellation Leo It is situated around 80 million light years from Earth. Also a part
Hickson_44
Group of galaxies in the constellation Leo
about three degrees northwest of third magnitude star 93 Leonis. The redshift of the brightest member, NGC 3753 places Copelands Septet as a part of
Copeland_Septet
Galaxy cluster in the constellation Sextans
current age of the universe. It was discovered in 2018 by analysing the redshifts of 10,000 objects observed with the Very Large Telescope in Chile. The
Hyperion_proto-supercluster
Historical local supercluster home to the Milky Way
a chance alignment of galaxies. The issue was resolved with the large redshift surveys of the late 1970s and early 1980s, which convincingly showed the
Virgo_Supercluster
known galaxy, which existed only 290 million years after the Big Bang. Its redshift of 14.32 exceeds the previous record of 13.2, set by JADES-GS-z13-0. 31
2024_in_science
Elliptical or lenticular galaxy in the constellation Leo
the NGC 3937 Group, which is part of the Coma Supercluster. The group has a velocity dispersion of 306 km/s. Other members of the group are NGC 3910,
NGC_3937
Star orbiting close to Sagittarius A*
the KECK/UCLA Galactic Center Group (led by Andrea Ghez) revealed a combined transverse Doppler and gravitational redshift up to 200 km/s/c, in agreement
S2_(star)
Astronomical object discovered in 2006
carbon-rich atmosphere at a redshift of z~0.14", possibly representing the core collapse and explosion of a carbon star. Gänsicke's group concurs with Barbary
SCP_06F6
American multinational technology conglomerate
In Spain, the company faced legal complaints over its policies, while a group of US Senators wrote an open letter to Bezos expressing concerns about workplace
Amazon_(company)
Galaxy group in the constellation Andromeda
VV 166, sometimes also called the NGC 70 Group or Arp 113, is a galaxy group in Andromeda. The main group was discovered in 1784 by William Herschel, who
NGC_68_Group
Cloud-based service and infrastructure
in 2023 include Kingfisher plc, the Government of Kuwait, Deutsche Börse Group, Unity Technologies, Uber, FanCode, Daimler, and Wix.com. Cloud database
Google_Cloud_Platform
REDSHIFT GROUP
REDSHIFT GROUP
Surname or Lastname
English
English : topographic name for someone living to the east of a main settlement, from Middle English easter ‘eastern’, Old English ēasterra, in form a comparative of ēast ‘east’ (see East).English : habitational name from a group of villages in Essex, named from Old English eowestre ‘sheepfold’.English : nickname for someone who had some connection with the festival of Easter, such as being born or baptized at that time (Old English ēastre, perhaps from the name of a pagan festival connected with the dawn).Translation of the German family name Oster.
Girl/Female
Tamil
Goddess Lakshmi, Assembly, Group
Surname or Lastname
English
English : variant of Haugh.German : topographic name from Middle High German houfe ‘heap’, e.g. of stones, or in southern Germany, a nickname from the same word in the sense ‘crowd’, ‘group of soldiers’.
Girl/Female
Tamil
Goddess Lakshmi, Assembly, Group
Boy/Male
Indian
A group of people, Indestructible, The Sky, Bralunan or the supreme spirit
Surname or Lastname
English
English : habitational name from any of the various places so called. The majority, with examples in at least fourteen counties, get the name from Old English hÅh ‘ridge’, ‘spur’ (literally ‘heel’) + tÅ«n ‘enclosure’, ‘settlement’. Haughton in Nottinghamshire also has this origin, and may have contributed to the surname. A smaller group of Houghtons, with examples in Lancashire and South Yorkshire, have as their first element Old English halh ‘nook’, ‘recess’. In the case of isolated examples in Devon and East Yorkshire, the first elements appear to be unattested Old English personal names or bynames, of which the forms approximate to Huhha and Hofa respectively, but the meanings are unknown.
Surname or Lastname
English
English : habitational name from a place in Lancashire, so named from Old English gor ‘dirt’, ‘mud’ + tūn ‘enclosure’, ‘settlement’.Introduced in America by a family from Gorton, Lancashire, England (three miles from Manchester), the name Gorton was also adopted by a religious group known as the Gortonites. They were followers of Samuel Gorton (c. 1592–1677), whose unorthodox religious beliefs, which included denying the doctrine of the Trinity, caused him to seek religious toleration by emigrating to Boston in 1637 with his family. In conflict with authorities in Massachusetts Bay, Plymouth, and Newport, he eventually settled in Shawomet, RI, and renamed it Warwick. He died there in 1677, leaving three sons and at least six daughters.
Surname or Lastname
English and Scottish
English and Scottish : habitational name from any of the numerous and widespread places so called. The majority of these are named with Old English middel ‘middle’ + tūn ‘enclosure’, ‘settlement’; a smaller group, with examples in Cumbria, Kent, Northamptonshire, Northumbria, Nottinghamshire, and Staffordshire, have as their first element Old English mylen ‘mill’.
Surname or Lastname
English
English : habitational name from any of a group of places in Bedfordshire and Cambridgeshire, named with Old English hætt ‘hat’, probably the name of a hill (see Hatt) + lēah ‘wood’, ‘clearing’.
Surname or Lastname
German
German : patronymic from a personal name (Latin Gallus) which was widespread in Europe in the Middle Ages (see Gall 2).German : nickname for someone in the service of the monastery of St Gallen, or a habitational name for someone from the city in Switzerland so named.English : variant of Gallier.Hungarian (Gallér) : from gallér ‘collar’, hence a metonymic occupational name for a taylor, in particular a maker of military garments.Jewish (Ashkenazic) : from German Galle ‘bile’, ‘gall’, with the agent suffix -er. This surname seems to have been one of the group of names selected at random from vocabulary words by government officials.
Surname or Lastname
English
English : habitational name from any of the numerous places so called, which split more or less evenly into two groups with different etymologies. One set (with examples in Berkshire, Dorset, Gloucestershire, Hampshire, Herefordshire, Somerset, and Wiltshire) is named from the Old English weak dative hēan (originally used after a preposition and article) of hēah ‘high’ + Old English tūn ‘enclosure’, ‘settlement’. The other (with examples in Cambridgeshire, Dorset, Gloucestershire, Herefordshire, Northamptonshire, Shropshire, Somerset, Suffolk, and Wiltshire) has Old English hīwan ‘household’, ‘monastery’. Compare Hine as the first element.
Boy/Male
Tamil
Cloud we can Say it as a group of clouds before rain
Surname or Lastname
English
English : habitational name from any of a group of places in Worcestershire which take their name affixes from the River Deverill (e.g. Brixton Deverill, Kingston Deverill). The river is thought to be named from Welsh dwfr ‘river’ + iâl ‘fertile uplands’.English and Irish : variant of Devereux.
Surname or Lastname
English and Scottish
English and Scottish : said to be a habitational name from Granson on Lake Neuchâtel. The first known bearer of the surname is Rigaldus de Grancione (fl. 1040). The name was taken to Britain by Otes de Grandison (died 1328) and his brother. They were among a group of Savoyards who settled in England when Henry III married a granddaughter of the Count of Savoy.
Boy/Male
Tamil
Well known, The group of people use to play traditional music at Shivaji ‘s period, Shayar or Shahir
Surname or Lastname
English
English : occupational name for a keeper of swine, Middle English foreman, from Old English fÅr ‘hog’, ‘pig’ + mann ‘man’.English : status name for a leader or spokesman for a group, from Old English fore ‘before’, ‘in front’ + mann ‘man’. The word is attested in this sense from the 15th century, but is not used specifically for the leader of a gang of workers before the late 16th century.Czech and Jewish (from Bohemia, Moravia) : occupational name for a carter, Czech forman, a loanword from German.
Surname or Lastname
English
English : probably a topographic name for someone who lived by a group of five ash trees (Middle English ashe) or a habitational name from a place so named, for example Five Ashes in East Sussex.
Girl/Female
Tamil
Goddess Lakshmi, Assembly, Group
Boy/Male
Tamil
World, A group of shells
Surname or Lastname
English
English : habitational name from a group of villages near Huntingdon, called Great, Little, and Steeple Gidding, named from Old English Gyddingas ‘people of Gydda’, a personal name of uncertain origin.
REDSHIFT GROUP
REDSHIFT GROUP
Girl/Female
Hindu, Indian, Traditional
The Primal Lakshmi
Boy/Male
Muslim/Islamic
It's a proper name a Sahabas' name and the youngest fighter in Al Islam
Boy/Male
Hindu, Indian
Lord Shiva
Boy/Male
Hindu
Son of Hari
Boy/Male
Indian, Kannada, Tamil
Handsome
Boy/Male
Hindu
God, Courageous
Girl/Female
Indian
Made of gold, Golden
Girl/Female
Hindu, Indian
Loving; Well Loved
Girl/Female
Australian, Danish, Dutch, French, German, Hebrew, Swedish
Jehovah Increases; He will Increase; Feminine of Joseph
Girl/Female
Persian American Greek Latin Russian
Woman.
REDSHIFT GROUP
REDSHIFT GROUP
REDSHIFT GROUP
REDSHIFT GROUP
REDSHIFT GROUP
n.
A cluster, crowd, or throng; an assemblage, either of persons or things, collected without any regular form or arrangement; as, a group of men or of trees; a group of isles.
n.
To form a group of; to arrange or combine in a group or in groups, often with reference to mutual relation and the best effect; to form an assemblage of.
n.
One of several species of valuable food fishes of the genus Epinephelus, of the family Serranidae, as the red grouper, or brown snapper (E. morio), and the black grouper, or warsaw (E. nigritus), both from Florida and the Gulf of Mexico.
n.
A dyestuff of the induline group, made from aniline, and used as a substitute for indigo in dyeing wool and silk a violet-blue or a gray-blue color.
n. pl.
An extensive artificial group of birds including the wading, swimming, and cursorial birds.
n.
A group of minerals having, a micaceous structure. They are hydrous silicates, derived generally from the alteration of some kind of mica. So called because the scales, when heated, open out into wormlike forms.
imp. & p. p.
of Group
n. pl.
An extensive artificial division of the animal kingdom, including the parasitic worms, or helminths, together with the nemerteans, annelids, and allied groups. By some writers the branchiopods, the bryzoans, and the tunicates are also included. The name was used in a still wider sense by Linnaeus and his followers.
n. pl.
A more restricted group, comprising only the helminths and closely allied orders.
n.
An element of the chromium group, found in certain rare minerals, as pitchblende, uranite, etc., and reduced as a heavy, hard, nickel-white metal which is quite permanent. Its yellow oxide is used to impart to glass a delicate greenish-yellow tint which is accompanied by a strong fluorescence, and its black oxide is used as a pigment in porcelain painting. Symbol U. Atomic weight 239.
n.
An assemblage of objects in a certain order or relation, or having some resemblance or common characteristic; as, groups of strata.
p. pr. & vb. n.
of Group
n.
A rare element of the nitrogen-phosphorus group, found combined, in vanadates, in certain minerals, and reduced as an infusible, grayish-white metallic powder. It is intermediate between the metals and the non-metals, having both basic and acid properties. Symbol V (or Vd, rarely). Atomic weight 51.2.
n. pl.
A group of butterflies including those known as virgins, or gossamer-winged butterflies.
n.
An individual, or group of individuals, of a species differing from the rest in some one or more of the characteristics typical of the species, and capable either of perpetuating itself for a period, or of being perpetuated by artificial means; hence, a subdivision, or peculiar form, of a species.
a.
Of or pertaining to a verb; as, a verbal group; derived directly from a verb; as, a verbal noun; used in forming verbs; as, a verbal prefix.
n.
An extinct genus of large Eocene ungulates allied to Dinoceras. This name is sometimes used for nearly all the known species of the group. See Dinoceras.
n. pl.
An extensive group of mammals including all those that have hoofs. It comprises the Artiodactyla and Perissodactyla.