List of galaxies

Size (left) and distance (right) of a few well-known galaxies put to scale.
This is a dynamic list and may never be able to satisfy particular standards for completeness. You can help by expanding it with reliably sourced entries.

The following is a list of notable galaxies.

There are about 51 galaxies in the Local Group (see list of nearest galaxies for a complete list), on the order of 100,000 in our Local Supercluster and an estimated number of about one to two trillion in all of the observable universe.

The discovery of the nature of galaxies as distinct from other nebulae (interstellar clouds) was made in the 1920s. The first attempts at systematic catalogues of galaxies were made in the 1960s, with the Catalogue of Galaxies and Clusters of Galaxies listing 29,418 galaxies and galaxy clusters, and with the Morphological Catalogue of Galaxies, a putatively complete list of galaxies with photographic magnitude above 15, listing 30,642. In the 1980s, the Lyons Groups of Galaxies listed 485 galaxy groups with 3,933 member galaxies. Galaxy Zoo is a project aiming at a more comprehensive list: launched in July 2007, it has classified over one million galaxy images from The Sloan Digital Sky Survey, The Hubble Space Telescope and the Cosmic Assembly Near-Infrared Deep Extragalactic Legacy Survey.[1]

There is no universal naming convention for galaxies, as they are mostly catalogued before it is established whether the object is or isn't a galaxy. Mostly they are identified by their celestial coordinates together with the name of the observing project (HUDF, SDSS, 3C, CFHQS, NGC/IC, etc.)

Named galaxies

This is a list of galaxies that are well known by something other than an entry in a catalog or list, or a set of coordinates, or a systematic designation.

Image Galaxy Constellation Origin of name Notes
Andromeda Andromeda Andromeda, which is shortened from "Andromeda Galaxy", gets its name from the area of the sky in which it appears, the constellation of Andromeda. Andromeda is the closest big galaxy to the Milky Way and is expected to collide with the Milky Way around 4 billion years from now. The two will eventually merge into a single new galaxy called Milkomeda.
Black Eye Galaxy Coma Berenices It has a spectacular dark band of absorbing dust in front of the galaxy's bright nucleus, giving rise to its nicknames of the "Black Eye" or "Evil Eye" galaxy.
Bode's Galaxy Ursa Major Named for Johann Elert Bode who discovered this galaxy in 1774.
Cartwheel Galaxy Sculptor Its visual appearance is similar to that of a spoked cartwheel.
Cigar Galaxy Ursa Major Appears similar in shape to a cigar.
Comet Galaxy Sculptor This galaxy is named after its unusual appearance, looking like a comet. The comet effect is caused by tidal stripping by its galaxy cluster, Abell 2667.
Cosmos Redshift 7 Sextans The name of this galaxy is based on a redshift (z) measurement of nearly 7 (actually, z = 6.604).[2] Galaxy Cosmos Redshift 7 is reported to be the brightest of distant galaxies (z > 6) and to contain some of the earliest first stars (first generation; Population III) that produced the chemical elements needed for the later formation of planets and life as we know it.[2]
Hoag's Object Serpens Caput This is named after Art Hoag, who discovered this ring galaxy. It is of the subtype Hoag-type galaxy, and may in fact be a polar-ring galaxy with the ring in the plane of rotation of the central object.
Large Magellanic Cloud Dorado/Mensa Named after Ferdinand Magellan This is the fourth largest galaxy in the Local Group, and forms a pair with the SMC, and from recent research, may not be part of the Milky Way system of satellites at all.[3]
Small Magellanic Cloud Tucana Named after Ferdinand Magellan This forms a pair with the LMC, and from recent research, may not be part of the Milky Way system of satellites at all.
Mayall's Object Ursa Major This is named after Nicholas Mayall, of the Lick Observatory, who discovered it.[4][5][6] Also called VV 32 and Arp 148, this is a very peculiar looking object, and is likely to be not one galaxy, but two galaxies undergoing a collision. Event in images is a spindle shape and a ring shape.
Milky Way Sagittarius (centre) The appearance from Earth of the galaxy – a band of light. The galaxy containing the Sun and its Solar System, and therefore Earth.
Pinwheel Galaxy Ursa Major Similar in appearance to a pinwheel (toy).
Sombrero Galaxy Virgo Similar in appearance to a sombrero.
Sunflower Galaxy Canes Venatici Similar in appearance to a sunflower.
Tadpole Galaxy Draco The name comes from the resemblance of the galaxy to a tadpole. This shape resulted from tidal interaction that drew out a long tidal tail.
Whirlpool Galaxy Canes Venatici From the whirlpool appearance this gravitationally disturbed galaxy exhibits.

Naked-eye galaxies

This is a list of galaxies that are visible to the naked eye, for at the very least, keen-eyed observers in a very dark-sky environment that is high in altitude, during clear and stable weather.

Naked-eye Galaxies
Galaxy Apparent Magnitude Distance Constellation Notes
Milky Way -6.5 (excluding the Sun[nb 1]) 0 Sagittarius (centre) This is the galaxy containing the Sun and its Solar System, and therefore Earth.. Most things visible to the naked-eye in the sky are part of it, including the Milky Way composing the Zone of Avoidance.[7]
Large Magellanic Cloud 0.9 160 kly (50 kpc) Dorado/Mensa Visible only from the southern hemisphere. It is also the brightest patch of nebulosity in the sky.[7][8][9]
Small Magellanic Cloud (NGC 292) 2.7 200 kly (60 kpc) Tucana Visible only from the southern hemisphere.[7][10]
Andromeda Galaxy (M31, NGC 224) 3.4 2.5 Mly (780 kpc) Andromeda Once called the Great Andromeda Nebula, it is situated in the Andromeda constellation.[7][11]
Triangulum Galaxy (M33, NGC 598) 5.7 2.9 Mly (900 kpc) Triangulum Being a diffuse object, its visibility is strongly affected by even small amounts of light pollution, ranging from easily visible in direct vision in truly dark skies to a difficult averted vision object in rural/suburban skies.[12]
Centaurus A (NGC 5128) 6.84 13.7 ± 0.9 Mly (4.2 ± 0.3 Mpc) Centaurus Centaurus A has been spotted with the naked eye by Stephen James O'Meara.[13]
Bode's Galaxy (M81, NGC 3031) 6.94 12 Mly (3.6 Mpc) Ursa Major Highly experienced amateur astronomers may be able to see Messier 81 under exceptional observing conditions.[14][15][16]
Messier 83 (NGC 5236) 8.2 14.7 Mly (4.5 Mpc) Hydra M83 has reportedly been seen with the naked eye.[17]

Observational firsts

First Galaxy Constellation Year Notes
First spiral galaxy Messier 51 Canes Venatici 1845 Lord William Parsons, Earl of Rosse discovered the first spiral nebula from observing M51 (recognition of the spiral shape without the recognition of the object as outside the Milky Way).[18]
Notion of galaxy Milky Way Galaxy & Messier 31 Sagittarius (centre) & Andromeda 1923 Recognition of the Milky Way and the Andromeda nebula as two separate galaxies by Edwin Hubble.
First Seyfert galaxy NGC 1068 (M77) Cetus 1943 (1908) The characteristics of Seyfert galaxies were first observed in M77 in 1908, however, Seyferts were defined as a class in 1943.[19]
First radio galaxy Cygnus A Cygnus 1951/2 Of several items, then called radio stars, Cygnus A was identified with a distant galaxy, being the first of many radio stars to become a radio galaxy.[20][21]
First quasar 3C273
3C48		 Virgo
Triangulum		 1962
1960		 3C273 was the first quasar with its redshift determined, and by some considered the first quasar. 3C48 was the first "radio-star" with an unreadable spectrum, and by others considered the first quasar.
First superluminal galactic jet 3C279 Virgo 1971 The jet is emitted by a quasar
First low-surface-brightness galaxy Malin 1 Coma Berenices 1986 Malin 1 was the first verified LSB galaxy. LSB galaxies had been first theorized in 1976.[22]
First superluminal jet from a Seyfert III Zw 2 Pisces[23] 2000 [24]

Prototypes

This is a list of galaxies that became prototypes for a class of galaxies.

Prototype Galaxies
Class Galaxy Constellation Date Notes
BL Lac object BL Lacertae (BL Lac) Lacerta This AGN was originally catalogued as a variable star, and "stars" of its type are considered BL Lac objects.
Hoag-type Galaxy Hoag's Object Serpens Caput This is the prototype Hoag-type Ring Galaxy
Giant LSB galaxy Malin 1 Coma Berenices 1986 [25]
FR II radio galaxy
(double-lobed radio galaxy) 		Cygnus A Cygnus 1951 [26]
starburst galaxy Cigar Galaxy Ursa Major

Closest and most distant known galaxies by type

Title Galaxy Constellation Distance Notes
Closest galaxy Canis Major Dwarf Canis Major 0.025 Mly Discovered in 2003, a satellite of the Milky Way, slowly being cannibalised by it.
Most distant galaxy GN-z11 Ursa Major z=11.09 With an estimated distance of about 32 billion light-years, astronomers announced it as the most distant astronomical galaxy known.[27]
Closest quasar 3C 273 Virgo z=0.158 First identified quasar, this is the most commonly accepted nearest quasar.
Most distant quasar ULAS J1120+0641 Leo z=7.085 Discovered in June 29, 2011 via UKIRT Infrared Deep Sky Survey; first quasar discovered beyond the redshift of 7.
Closest radio galaxy Centaurus A (NGC 5128, PKS 1322-427) Centaurus 13.7 Mly [28]
Most distant radio galaxy TN J0924-2201 Hydra z=5.2
Closest Seyfert galaxy Circinus Galaxy Circinus 13 Mly This is also the closest Seyfert 2 galaxy. The closest Seyfert 1 galaxy is NGC 4151.
Most distant Seyfert galaxy z=
Closest blazar Markarian 421 (Mrk 421, Mkn 421, PKS 1101+384, LEDA 33452) Ursa Major z=0.030 This is a BL Lac object.[29][30]
Most distant known blazar Q0906+6930 Ursa Major z=5.47 This is a flat spectrum radio-loud quasar type blazar.[31][32]
Closest BL Lac object Markarian 421 (Mkn 421, Mrk 421, PKS 1101+384, LEDA 33452) Ursa Major z=0.030 [29][30]
Most distant BL Lac object z=
Closest LINER
Most distant LINER z=
Closest LIRG
Most distant LIRG z=
Closest ULIRG IC 1127 (Arp 220/APG 220) Serpens Caput z=0.018 [33]
Most distant ULIRG z=
Closest starburst galaxy Cigar Galaxy (M82, Arp 337/APG 337, 3C 231, Ursa Major A) Ursa Major 3.2 Mpc [34][35]
Most distant starburst galaxy SPT 0243-49 z= 5.698 [36][37]

Closest galaxies

5 Closest Galaxies
Rank Galaxy Distance Notes
1 Milky Way Galaxy 0 This is the galaxy containing the Sun and its Solar System, and therefore Earth.
2 Canis Major Dwarf 0.025 Mly
3 Virgo Stellar Stream 0.030 Mly
4 Sagittarius Dwarf Elliptical Galaxy 0.081 Mly
5 Large Magellanic Cloud 0.163 Mly Largest satellite galaxy of the Milky Way
6 Small Magellanic Cloud 0.197 Mly

  • Mly represents millions of light-years, a measure of distance.
  • Distances are measured from Earth, with Earth being at zero.

Nearest Galaxies by Type
Title Galaxy Date Distance Notes
Nearest galaxy Milky Way always 0 This is the galaxy containing the Sun and its Solar System, and therefore Earth.
Nearest galaxy to our own Canis Major Dwarf 2003 0.025 Mly The absolute closest galaxy
Nearest dwarf galaxy Canis Major Dwarf 2003 0.025 Mly
Nearest major galaxy to our own Andromeda Galaxy always 2.54 Mly First identified as a separate galaxy in 1923
Nearest giant galaxy Centaurus A 12 Mly
Nearest Neighboring Galaxy Title-holder
Galaxy Date Distance Notes
Canis Major Dwarf 2003 0.025 Mly
Sagittarius Dwarf Elliptical Galaxy 1994 − 2003 0.081 Mly
Large Magellanic Cloud antiquity − 1994 0.163 Mly This is the upper bound, as it is nearest galaxy observable with the naked-eye.
Small Magellanic Cloud 1913–1914 0.197 Mly This was the first intergalactic distance measured. In 1913, Ejnar Hertzsprung measures the distance to SMC using Cepheid variables. In 1914, he did it for LMC.
Andromeda Galaxy 1923 2.5 Mly This was the first galaxy determined to not be part of the Milky Way.

  • Mly represents millions of light-years, a measure of distance.
  • Distances are measured from Earth, with Earth being at zero.

Most distant galaxies

Most Remote Galaxies by Type
Title Galaxy Date Redshift Notes
Candidate most remote galaxy (photometric redshift) UDFj-39546284 2011 z=11.9(?) This was proposed to be the remotest object known at time of discovery. In late 2012, its distance was revised from z=10.3 to 11.9,[38][39] however, recent re-analyses suggest it is likely to be at much lower redshift.[40]
Most remote galaxy confirmed (spectroscopic redshift) GN-z11 2016 z=11.09 As of March 2016, GN-z11 was the most distant known galaxy.[27]
Most remote quasar ULAS J1120+0641 2011 z=7.085 This is the undisputed most remote quasar of any type, and the first with a redshift beyond 7.
Most distant non-quasar SMG Baby Boom Galaxy (EQ J100054+023435) 2008 z=4.547 [41]
grand-design spiral galaxy Q2343-BX442 2012 z=2.18 [42]

  • z represents redshift, a measure of recessional velocity and inferred distance due to cosmological expansion
Timeline of Most Remote Galaxy Record-holders
Galaxy Date Distance
(z=Redshift) 		Notes
GN-z11 2016 −  z=11.09 Announced March 2016.[27]
EGSY8p7
(EGSY-2008532660)		 2015 − 2016 z=8.68 This galaxy's redshift was determined by examining its Lyman-alpha emissions, which were released in August 2015.[43][44][45]
EGS-zs8-1 2015 − 2015 z=7.730 This was the most distant galaxy as of May 2015.[45][46][47]
Z8 GND 5296 2013 − 2015 z=7.51 [48]
SXDF-NB1006-2 2012 − 2013 z=7.215 [49]
GN-108036 2012 − 2012 z=7.213 [50]
BDF-3299 2012 − 2013 z=7.109 [51]
IOK-1 2006 − 2010 z=6.96 This was the remotest object known at time of discovery. In 2009, gamma ray burst GRB 090423 was discovered at z=8.2, taking the title of most distant object. The next galaxy to hold the title also succeeded GRB 090423, that being UDFy-38135539.[52][53][54]
SDF J132522.3+273520 2005 − 2006 z=6.597 This was the remotest object known at time of discovery.[54][55]
SDF J132418.3+271455 2003 − 2005 z=6.578 This was the remotest object known at time of discovery.[55][56][57][58]
HCM-6A 2002 − 2003 z=6.56 This was the remotest object known at time of discovery. The galaxy is lensed by galaxy cluster Abell 370. This was the first galaxy, as opposed to quasar, found to exceed redshift 6. It exceeded the redshift of quasar SDSSp J103027.10+052455.0 of z=6.28[56][57][59][60][61][62]
SSA22−HCM1 1999 − 2002 z=5.74 This was the remotest object known at time of discovery. In 2000, the quasar SDSSp J104433.04-012502.2 was discovered at z=5.82, becoming the most remote object in the universe known. This was followed by another quasar, SDSSp J103027.10+052455.0 in 2001, the first object exceeding redshift 6, at z=6.28[63][64]
HDF 4-473.0 1998 − 1999 z=5.60 This was the remotest object known at the time of discovery.[64]
RD1 (0140+326 RD1) 1998 z=5.34 This was the remotest object known at time of discovery. This was the first object found beyond redshift 5.[64][65][66][67][68]
CL 1358+62 G1 & CL 1358+62 G2 1997 − 1998 z=4.92 These were the remotest objects known at the time of discovery. The pair of galaxies were found lensed by galaxy cluster CL1358+62 (z=0.33). This was the first time since 1964 that something other than a quasar held the record for being the most distant object in the universe. It exceeded the mark set by quasar PC 1247-3406 at z=4.897[64][66][67][69][70][71]

From 1964 to 1997, the title of most distant object in the universe were held by a succession of quasars.[71] That list is available at list of quasars.

8C 1435+63 1994 − 1997 z=4.25 This is a radio galaxy. At the time of its discovery, quasar PC 1247-3406 at z=4.73, discovered in 1991 was the most remote object known. This was the last radio galaxy to hold the title of most distant galaxy. This was the first galaxy, as opposed to quasar, that was found beyond redshift 4.[64][72][73][74]
4C 41.17 1990 − 1994 z=3.792 This is a radio galaxy. At the time of its discovery, quasar PC 1158+4635, discovered in 1989, was the most remote object known, at z=4.73 In 1991, quasar PC 1247-3406, became the most remote object known, at z=4.897[64][73][74][75][76]
1 Jy 0902+343 (GB6 B0902+3419, B2 0902+34) 1988 − 1990 z=3.395 This is a radio galaxy. At the time of discovery, quasar Q0051-279 at z=4.43, discovered in 1987, was the most remote object known. In 1989, quasar PC 1158+4635 was discovered at z=4.73, making it the most remote object known. This was the first galaxy discovered above redshift 3. It was also the first galaxy found above redshift 2.[64][76][77][78][79]
3C 256 1984 − 1988 z=1.819 This is a radio galaxy. At the time, the most remote object was quasar PKS 2000-330, at z=3.78, found in 1982.[64][80]
3C 241 1984 z=1.617 This is a radio galaxy. At the time, the most remote object was quasar PKS 2000-330, at z=3.78, found in 1982.[81][82]
3C 324 1983 − 1984 z=1.206 This is a radio galaxy. At the time, the most remote object was quasar PKS 2000-330, at z=3.78, found in 1982.[64][81][83]
3C 65 1982 − 1983 z=1.176 This is a radio galaxy. At the time, the most remote object was quasar OQ172, at z=3.53, found in 1974. In 1982, quasar PKS 2000-330 at z=3.78 became the most remote object.
3C 368 1982 z=1.132 This is a radio galaxy. At the time, the most remote object was quasar OQ172, at z=3.53, found in 1974.[64]
3C 252 1981 − 1982 z=1.105 This is a radio galaxy. At the time, the most remote object was quasar OQ172, at z=3.53, found in 1974.
3C 6.1 1979 - z=0.840 This is a radio galaxy. At the time, the most remote object was quasar OQ172, at z=3.53, found in 1974.[64][84]
3C 318 1976 - z=0.752 This is a radio galaxy. At the time, the most remote object was quasar OQ172, at z=3.53, found in 1974.[64]
3C 411 1975 - z=0.469 This is a radio galaxy. At the time, the most remote object was quasar OQ172, at z=3.53, found in 1974.[64]

From 1964 to 1997, the title of most distant object in the universe were held by a succession of quasars.[71] That list is available at list of quasars.

3C 295 1960 - z=0.461 This is a radio galaxy. This was the remotest object known at time of discovery of its redshift. This was the last non-quasar to hold the title of most distant object known until 1997. In 1964, quasar 3C 147 became the most distant object in the universe known.[64][71][85][86][87]
LEDA 25177 (MCG+01-23-008) 1951 − 1960 z=0.2
(V=61000 km/s)		 This galaxy lies in the Hydra Supercluster. It is located at B1950.0 08h 55m 4s +03° 21′ and is the BCG of the fainter Hydra Cluster Cl 0855+0321 (ACO 732).[64][87][88][89][90][91][92][93]
LEDA 51975 (MCG+05-34-069) 1936 - z=0.13
(V=39000 km/s)		 The brightest cluster galaxy of the Bootes cluster (ACO 1930), an elliptical galaxy at B1950.0 14h 30m 6s +31° 46′ apparent magnitude 17.8, was found by Milton L. Humason in 1936 to have a 40,000 km/s recessional redshift velocity.[91][94][95]
LEDA 20221 (MCG+06-16-021) 1932 - z=0.075
(V=23000 km/s)		 This is the BCG of the Gemini Cluster (ACO 568) and was located at B1950.0 07h 05m 0s +35° 04′[94][96]
BCG of WMH Christie's Leo Cluster 1931 − 1932 z=
(V=19700 km/s)		 [96][97][98][99]
BCG of Baede's Ursa Major Cluster 1930 − 1931 z=
(V=11700 km/s)		 [99][100]
NGC 4860 1929 − 1930 z=0.026
(V=7800 km/s)		 [101][102]
NGC 7619 1929 z=0.012
(V=3779 km/s)		 Using redshift measurements, NGC 7619 was the highest at the time of measurement. At the time of announcement, it was not yet accepted as a general guide to distance, however, later in the year, Edwin Hubble described redshift in relation to distance, leading to a seachange, and having this being accepted as an inferred distance.[101][103][104]
NGC 584 (Dreyer nebula 584) 1921 − 1929 z=0.006
(V=1800 km/s)		 At the time, nebula had yet to be accepted as independent galaxies. However, in 1923, galaxies were generally recognized as external to the Milky Way.[91][101][103][105][106][107][108]
M104 (NGC 4594) 1913 − 1921 z=0.004
(V=1180 km/s)		 This was the second galaxy whose redshift was determined; the first being Andromeda - which is approaching us and thus cannot have its redshift used to infer distance. Both were measured by Vesto Melvin Slipher. At this time, nebula had yet to be accepted as independent galaxies. NGC 4594 was originally measured as 1000 km/s, then refined to 1100, and then to 1180 in 1916.[101][105][108]
M81 antiquity - 20th century
antiquity - 1913 (based on redshift)
antiquity - 1930 (based on Cepheids)
 11.8 Mly (z=-0.10) This is the lower bound, as it is remotest galaxy observable with the naked-eye. It is 12 million light-years away. Redshift cannot be used to infer distance, because it is moving toward us faster than cosmological expansion.
Messier 101 1930 - Using the pre-1950s Cepheid measurements, M101 was one of the most distant so measured.
Triangulum Galaxy 1924–1930 In 1924, Edwin Hubble announced the distance to M33 Triangulum.
Andromeda Galaxy 1923–1924 In 1923, Edwin Hubble measured the distance to Andromeda, and settled the question of whether or not there were galaxies, or if everything was in the Milky Way.
Small Magellanic Cloud 1913–1923 This was the first intergalactic distance measured. In 1913, Ejnar Hertzsprung measures the distance to SMC using Cepheid variables.

  • z represents redshift, a measure of recessional velocity and inferred distance due to cosmological expansion
  • quasars and other AGN are not included on this list, since they are only galactic cores, unless the host galaxy was observed when it was most distant

Timeline notes

  • MACS0647-JD, discovered in 2012, with z=10.7, does not appear on this list because it has not been confirmed with a spectroscopic redshift.[109]
  • UDFy-38135539, discovered in 2009, with z=8.6, does not appear on this list because its claimed redshift is disputed.[110] Follow-up observations have failed to replicate the cited redshift measurement.
  • A1689-zD1, discovered in 2008, with z=7.6, does not appear on this list because it has not been confirmed with a spectroscopic redshift.
  • Abell 68 c1 and Abell 2219 c1, discovered in 2007, with z=9, do not appear on this list because they have not been confirmed.[111]
  • IOK4 and IOK5, discovered in 2007, with z=7, do not appear on this list because they have not been confirmed with a spectroscopic redshift.
  • Abell 1835 IR1916, discovered in 2004, with z=10.0, does not appear on this list because its claimed redshift is disputed. Some follow-up observations have failed to find the object at all.
  • STIS 123627+621755, discovered in 1999, with z=6.68, does not appear on this list because its redshift was based on an erroneous interpretation of an oxygen emission line as a hydrogen emission line.[112][113][114]
  • BR1202-0725 LAE, discovered in 1998 at z=5.64 does not appear on the list because it was not definitively pinned. BR1202-0725 (QSO 1202-07) refers to a quasar that the Lyman alpha emitting galaxy is near. The quasar itself lies at z=4.6947[65][68]
  • BR2237-0607 LA1 and BR2237-0607 LA2 were found at z=4.55 while investigating around the quasar BR2237-0607 in 1996. Neither of these appear on the list because they were not definitively pinned down at the time. The quasar itself lies at z=4.558[115][116]
  • Two absorption dropouts in the spectrum of quasar BR 1202-07 (QSO 1202-0725, BRI 1202-0725, BRI1202-07) were found, one in early 1996, another later in 1996. Neither of these appear on the list because they were not definitively pinned down at the time. The early one was at z=4.38, the later one at z=4.687, the quasar itself lies at z=4.695[64][117][118][119][120]
  • In 1986, a gravitationally lensed galaxy forming a blue arc was found lensed by galaxy cluster CL 2224-02 (C12224 in some references). However, its redshift was only determined in 1991, at z=2.237, by which time, it would no longer be the most distant galaxy known.[121][122]
  • An absorption drop was discovered in 1985 in the light spectrum of quasar PKS 1614+051 at z=3.21 This does not appear on the list because it was not definitively fixed down. At the time, it was claimed to be the first non-QSO galaxy found beyond redshift 3. The quasar itself is at z=3.197[64][123]
  • In 1975, 3C 123 was incorrectly determined to lie at z=0.637 (actually z=0.218)[124][125]
  • From 1964 to 1997, the title of most distant object in the universe was held by a succession of quasars.[71] That list is available at list of quasars.
  • 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, no galaxy was spectroscopically determined.[87]

Galaxies by brightness and power

Title Galaxy Data Notes
Intrinsically brightest galaxy Baby Boom Galaxy Starburst galaxy located 12 billion light years away
Brightest galaxy to the naked eye Large Magellanic Cloud Apparent magnitude 0.6 This galaxy has high surface brightness combined with high apparent brightness.
Intrinsically faintest galaxy Boötes Dwarf Galaxy (Boo dSph) Absolute magnitude -6.75 This does not include dark galaxies.
Lowest surface brightness galaxy Andromeda IX
Most luminous galaxy WISE J224607.57-052635.0 As of May 21, 2015, WISE-J224607.57-052635.0-20150521 is the most luminous galaxy discovered and releases 10,000 times more energy than the Milky Way galaxy, although smaller. Nearly 100 percent of the light escaping from this dusty galaxy is infrared radiation.[126][127] (Image)
Brightest distant galaxy (z > 6) Cosmos Redshift 7 Galaxy Cosmos Redshift 7 is reported to be the brightest of distant galaxies (z > 6) and to contain some of the earliest first stars (first generation; Population III) that produced the chemical elements needed for the later formation of planets and life as we know it.[2][128]

Galaxies by mass and density

Title Galaxy Data Notes
Least massive galaxy Segue 2 ~550,000 MSun This is not considered a star cluster, as it is held together by the gravitational effects of dark matter rather than just the mutual attraction of the constituent stars, gas and black holes.[129][130]
Most massive galaxy ESO 146-IG 005 ~30×1012 MSun Central galaxy in Abell 3827, 1.4 Gly distant.[131][132]
Most dense galaxy M85-HCC1 This is an ultra-compact dwarf galaxy [133]
Least dense galaxy
Most massive spiral galaxy ISOHDFS 27 1.04×1012 MSun The preceding most massive spiral was UGC 12591[134]
Least massive galaxy with globular cluster(s) Andromeda I [135]

Field galaxies

List of field galaxies
Galaxy Data Notes
NGC 4555
SDSS J1021+1312 [136]

A field galaxy is a galaxy that does not belong to a larger cluster of galaxies and hence is gravitationally alone.

Interacting galaxies

Galaxies in tidal interaction
Galaxies Data Notes
The Magellanic Clouds are being tidally disrupted by the Milky Way Galaxy, resulting in the Magellanic Stream drawing a tidal tail away from the LMC and SMC, and the Magellanic Bridge drawing material from the clouds to our galaxy.
The smaller galaxy NGC 5195 is tidally interacting with the larger Whirlpool Galaxy, creating its grand design spiral galaxy architecture.
These three galaxies interact with each other and draw out tidal tails, which are dense enough to form star clusters. The bridge of gas between these galaxies is known as Arp's Loop.[137]
NGC 6872 is a barred spiral galaxy with a grand design spiral nucleus, and distinct well-formed outer barred-spiral architecture, caused by tidal interaction with satellite galaxy IC 4970.
Tadpole Galaxy The Tadpole Galaxy tidally interacted with another galaxy in a close encounter, and remains slightly disrupted, with a long tidal tail.
Galaxies in non-merger significant collision
Galaxies Data Notes
Arp 299 (NGC 3690 & IC 694) These two galaxies have recently collided and are now both barred irregular galaxies.
Galaxies disrupted post significant non-merger collisions
Galaxies Data Notes
Mayall's Object This is a pair of galaxies, one which punched through the other, resulting in a ring galaxy.

Galaxy mergers

Galaxies undergoing near-equal merger
Galaxies Data Notes
Antennae Galaxies (Ringtail Galaxy, NGC 4038 & NGC 4039, Arp 244) 2 galaxies Two spiral galaxies currently starting a collision, tidally interacting, and in the process of merger.
Butterfly Galaxies (Siamese Twins Galaxies, NGC 4567 & NGC 4568) 2 galaxies Two spiral galaxies in the process of starting to merge.
Mice Galaxies (NGC 4676, NGC 4676A & NGC 4676B, IC 819 & IC 820, Arp 242) 2 galaxies Two spiral galaxies currently tidally interacting and in the process of merger.
NGC 520 2 galaxies Two spiral galaxies undergoing collision, in the process of merger.
NGC 2207 and IC 2163 (NGC 2207 & IC 2163) 2 galaxies These are two spiral galaxies starting to collide, in the process of merger.
NGC 5090 and NGC 5091 (NGC 5090 & NGC 5091) 2 galaxies These two galaxies are in the process of colliding and merging.
NGC 7318 (Arp 319, NGC 7318A & NGC 7318B) 2 galaxies These are two starting to collide
Four galaxies in CL0958+4702 4 galaxies These four near-equals at the core of galaxy cluster CL 0958+4702 are in the process of merging.[138]
Galaxy protocluster LBG-2377 z=3.03 This was announced as the most distant galaxy merger ever discovered. It is expected that this proto-cluster of galaxies will merge to form a brightest cluster galaxy, and become the core of a larger galaxy cluster.[139][140]
Recently merged galaxies of near-equals
Galaxy Data Notes
Starfish Galaxy (NGC 6240, IC 4625) This recently coalesced galaxy still has two prominent nuclei.
Galaxies undergoing disintegration by cannibalization
Disintegrating Galaxy Consuming Galaxy Notes
Canis Major Dwarf Galaxy Milky Way Galaxy The Monoceros Ring is thought to be the tidal tail of the disrupted CMa dg.
Virgo Stellar Stream Milky Way Galaxy This is thought to be a completely disrupted dwarf galaxy.
Sagittarius Dwarf Elliptical Galaxy Milky Way Galaxy M54 is thought to be the core of this dwarf galaxy.
Objects considered destroyed galaxies
Defunct Galaxy Destroyer Notes
Omega Centauri Milky Way Galaxy This is now categorized a globular cluster of the Milky Way. However, it is considered the core of a dwarf galaxy that the Milky Way cannibalized.[141]
Mayall II Andromeda Galaxy This is now categorized a globular cluster of Andromeda. However, it is considered the core of a dwarf galaxy that Andromeda cannibalized.

Galaxies with some other notable feature

Galaxy name Distance Constellation Property Notes
M87 Virgo This is the central galaxy of the Virgo Cluster, the central cluster of the Local Supercluster[142]
M102 Draco (Ursa Major) This galaxy cannot be definitively identified, with the most likely candidate being NGC 5866, and a good chance of it being a misidentification of M101. Other candidates have also been suggested.
NGC 2770 Lynx "Supernova Factory" NGC 2770 is referred to as the "Supernova Factory" due to three recent supernovae occurring within it.
NGC 3314 (NGC 3314a and NGC 3314b) Hydra exact visual alignment This is a pair of spiral galaxies, one superimposed on another, at two separate and distinct ranges, and unrelated to each other. It is a rare chance visual alignment.
ESO 137-001 Triangulum Australe "tail" feature Lying in the galaxy cluster Abell 3627, this galaxy is being stripped of its gas by the pressure of the intracluster medium (ICM), due to its high speed traversal through the cluster, and is leaving a high density tail with large amounts of star formation. The tail features the largest amount of star formation outside of a galaxy seen so far. The galaxy has the appearance of a comet, with the head being the galaxy, and a tail of gas and stars.[143][144][145][146]
Comet Galaxy Sculptor interacting with a galaxy cluster Lying in galaxy cluster Abell 2667, this spiral galaxy is being tidally stripped of stars and gas through its high speed traversal through the cluster, having the appearance of a comet.
4C 37.11 230 Mpc Perseus Least separation between binary central black holes, at 24 ly (7.3 pc) OJ 287 has an inferred pair with a 12-year orbital period, and thus would be much closer than 4C 37.11's pair.
SDSS J150636.30+540220.9 ("SDSS J1506+54") z=0.608 Boötes
15h 06m 36.30s+54° 02′ 20.9″		 Most efficient star production Most extreme example in the list of moderate-redshift galaxies with the highest density starbursts yet observed found in the Wide-field Infrared Survey Explorer data (Diamond-Stanic et al. 2012).[147]
Cosmos Redshift 7 z = 6.604 (12.9 billion light-years) Sextans Brightest distant galaxy (z > 6) Galaxy Cosmos Redshift 7 is reported to be the brightest of distant galaxies (z > 6) and to contain some of the earliest first stars (first generation; Population III) that produced the chemical elements needed for the later formation of planets and life as we know it.[2][128]
This is a dynamic list and may never be able to satisfy particular standards for completeness. You can help by expanding it with reliably sourced entries.

Lists of galaxies

See also

Notes

  1. ↑ Using the formula for addition of apparent magnitudes, the added magnitudes of all stars in the Milky Way but our Sun (-6.50) and our Sun (-26.74) differs from the apparent magnitude of just our sun by less than 10^-8 Archived 2016-03-04 at the Wayback Machine.

References

  1. ↑ B.D. Simmons; et al. (2014). "Galaxy Zoo: CANDELS barred discs and bar fractions". MNRAS. 445 (4): 3466–3474. arXiv:1409.1214. Bibcode:2014MNRAS.445.3466S. doi:10.1093/mnras/stu1817.
  2. 1 2 3 4 Sobral, David; Matthee, Jorryt; Darvish, Behnam; Schaerer, Daniel; Mobasher, Bahram; Röttgering, Huub J. A.; Santos, Sérgio; Hemmati, Shoubaneh (4 June 2015). "Evidence For POPIII-Like Stellar Populations In The Most Luminous LYMAN-α Emitters At The Epoch Of Re-Ionisation: Spectroscopic Confirmation". The Astrophysical Journal. 808: 139. arXiv:1504.01734. Bibcode:2015ApJ...808..139S. doi:10.1088/0004-637x/808/2/139.
  3. ↑ Williams, Matt (November 2016). "What are Magellanic clouds?". phys.org.
  4. ↑ Smith, Robert T. (1941). "The Radial Velocity of a Peculiar Nebula". Publications of the Astronomical Society of the Pacific. 53: 187. Bibcode:1941PASP...53..187S. doi:10.1086/125301.
  5. ↑ Burbidge, E. Margaret (1964). "The Strange Extragalactic Systems: Mayall's Object and IC 883". Astrophysical Journal. 140: 1617. Bibcode:1964ApJ...140.1617B. doi:10.1086/148070.
  6. ↑ Baade, W.; Minkowski, R. (1954). "On the Identification of Radio Sources". Astrophysical Journal. 119: 215. Bibcode:1954ApJ...119..215B. doi:10.1086/145813.
  7. 1 2 3 4 Karen Masters (December 2003). "Curious About Astronomy: Can any galaxies be seen with the naked eye?". Ask an Astronomer. Archived from the original on 2008-12-20. Retrieved 2008-11-01.
  8. ↑ "Magellanic Cloud". Astronomy Knowledge Base. University of Ottawa. Archived from the original on 2006-07-05.
  9. ↑ "The Large Magellanic Cloud, LMC". SEDS. Archived from the original on 2014-02-23.
  10. ↑ "The Small Magellanic Cloud, SMC". SEDS. Archived from the original on 2015-03-07.
  11. ↑ "Messier 31". SEDS. Archived from the original on 2015-12-19.
  12. ↑ John E. Bortle (February 2001). "The Bortle Dark-Sky Scale". Sky & Telescope.
  13. ↑ Barbara Wilson & Larry Mitchell. "The Revised AINTNO 100". Archived from the original on 2010-01-05.
  14. ↑ Stephen Uitti. "Farthest Naked Eye Object". Archived from the original on 2008-08-19. Retrieved 2008-11-01.
  15. ↑ "Messier 81". SEDS. Archived from the original on 2015-12-23.
  16. ↑ S. J. O'Meara (1998). The Messier Objects. Cambridge University Press. ISBN 0-521-55332-6.
  17. ↑ Inglis, Mike. "Galaxies". Patrick Moore’s Practical Astronomy Series: 157–189. doi:10.1007/978-1-84628-736-7_4.
  18. ↑ SEDS, Lord Rosse's drawings of M51, his "Question Mark" "Spiral Nebula" Archived 2015-06-26 at the Wayback Machine.
  19. ↑ SEDS, Seyfert Galaxies Archived 2013-09-21 at the Wayback Machine.
  20. ↑ Burbidge, G. (1999). "Baade & Minkowski's Identification of Radio Sources". Astrophysical Journal. 525: 569. Bibcode:1999ApJ...525C.569B.
  21. ↑ Baade, W.; Minkowski, R. "Identification of the Radio Sources in Cassiopeia, Cygnus a, and Puppis a.". The Astrophysical Journal. 119: 206. Bibcode:1954ApJ...119..206B. doi:10.1086/145812.
  22. ↑ Scientific American, "The Ghostliest Galaxies", GD Bothun, Vol. 276, No. 2, February 1997, pp.40-45, Bibcode: 1997SciAm.276b..40B
  23. ↑ http://iopscience.iop.org/1538-3881/122/4/2055/datafile8.txt
  24. ↑ Brunthaler, A.; et al. (2000). "III Zw 2, the first superluminal jet in a Seyfert galaxy". Astronomy & Astrophysics Letters. 357: 45. arXiv:astro-ph/0004256. Bibcode:2000A&A...357L..45B.
  25. ↑ Ken Crosswell, "Malin 1: A Bizarre Galaxy Gets Slightly Less So" Archived 2011-06-14 at the Wayback Machine., 22 January 2007
  26. ↑ Moffet, Alan T. "The Structure of Radio Galaxies". Annual Review of Astronomy and Astrophysics. 4: 145–170. Bibcode:1966ARA&A...4..145M. doi:10.1146/annurev.aa.04.090166.001045.
  27. 1 2 3 Drake, Nadia (March 3, 2016). "Astronomers Spot Most Distant Galaxy—At Least For Now". National Geographic. Archived from the original on March 6, 2016. Retrieved March 10, 2016.
  28. ↑ Sub-parsec-scale structure and evolution in Centaurus A Introduction Archived 2009-07-04 at the Wayback Machine. ; Tue November 26 15:27:29 PST 1996
  29. 1 2 The 2006 Giant Flare in PKS 2155-304 and Unidentified TeV Sources Archived 2009-03-20 at the Wayback Machine.
  30. 1 2 Julie McEnery. "Time Variability of the TeV Gamma-Ray Emission from Markarian 421". Iac.es. Archived from the original on 2009-01-12. Retrieved 2008-11-01.
  31. ↑ bNet, Ablaze from afar: astronomers may have identified the most distant "blazar" yet Archived 2009-08-03 at the Wayback Machine., Sept, 2004
  32. ↑ Romani; David Sowards-Emmerd; Lincoln Greenhill; Peter Michelson (2004). "Q0906+6930: The Highest-Redshift Blazar". The Astrophysical Journal. 610: L9–L11. arXiv:astro-ph/0406252. Bibcode:2004ApJ...610L...9R. doi:10.1086/423201.
  33. ↑ Rodríguez Zaurín, J.; Tadhunter, C. N.; González Delgado, R. M. (2008). "Optical spectroscopy of Arp220: the star formation history of the closest ULIRG". Monthly Notices of the Royal Astronomical Society. 384 (3): 875–885. arXiv:0711.0166. Bibcode:2008MNRAS.384..875R. doi:10.1111/j.1365-2966.2007.12658.x.
  34. ↑ Murray, Steven (1999). "ACIS Imaging of the Starburst Galaxy M82". Chandra Proposal ID #01700041: 362. Bibcode:1999cxo..prop..362M.
  35. ↑ Starburst Galaxies: Proceedings of a Workshop (page 27) ; 2001 ; ISBN 3-540-41472-X
  36. ↑ Science Daily, "'Monster' Starburst Galaxies Discovered in Early Universe" Archived 2018-03-13 at the Wayback Machine., NRAO, 13 March 2013 (accessed 13 March 2013)
  37. ↑ Vieira, J. D.; et al. "Dusty starburst galaxies in the early Universe as revealed by gravitational lensing". Nature. 495: 344–347. arXiv:1303.2723. Bibcode:2013Natur.495..344V. doi:10.1038/nature12001. PMID 23485967.
  38. ↑ Hubble; "Hubble finds a new contender for galaxy distance record" Archived 2012-07-27 at WebCite, 26 January 2011
  39. ↑ Wall, Mike (December 12, 2012). "Ancient Galaxy May Be Most Distant Ever Seen". Space.com. Archived from the original on December 14, 2012. Retrieved December 12, 2012.
  40. ↑ Brammer, Gabriel B.; van Dokkum, Pieter G.; Illingworth, Garth D.; Bouwens, Rychard J.; Labbé, Ivo; Franx, Marijn; Momcheva, Ivelina; Oesch, Pascal A. (2013). "A Tentative Detection of an Emission Line at 1.6 mum for the z ~ 12 Candidate UDFj-39546284". The Astrophysical Journal. 765: L2. arXiv:1301.0317. Bibcode:2013ApJ...765L...2B. doi:10.1088/2041-8205/765/1/l2.
  41. ↑ Capak, Peter; Carilli, C. L.; Lee, N.; Aldcroft, T.; Aussel, H.; Schinnerer, E.; Wilson, G. W.; Yun, M. S.; Blain, A. (2008). "Spectroscopic Confirmation of an Extreme Starburst at Redshift 4.547". The Astrophysical Journal. 681 (2): L53–L56. arXiv:0806.0657. Bibcode:2008ApJ...681L..53C. doi:10.1086/590555.
  42. ↑ David R. Law; Alice E. Shapley; Charles C. Steidel; Naveen A. Reddy; Charlotte R. Christensen; Dawn K. Erb (2012-07-18). "High velocity dispersion in a rare grand-design spiral galaxy at redshift z = 2.18". Nature. 487: 338–340. arXiv:1207.4196. Bibcode:2012Natur.487..338L. doi:10.1038/nature11256. PMID 22810697. Retrieved 2012-07-20.
  43. ↑ W. M. Keck Observatory (6 August 2015). "A new record: Keck Observatory measures most distant galaxy". Astronomy Now. Archived from the original on 12 August 2015.
  44. ↑ Mike Wall (5 August 2015). "Ancient Galaxy Is Most Distant Ever Found". Space.com. Archived from the original on 7 August 2015.
  45. 1 2 Jonathan O'Callaghan & Ellie Zolfagharifard (16 July 2015). "A galaxy that rally IS far, far away: Astronomers confirm star system 13.1 billion light-years away is the most distant known in the universe". Daily Mail (London). Archived from the original on 16 September 2015.
  46. ↑ Oesch, P.A.; et al. (3 May 2015). "A Spectroscopic Redshift Measurement for a Luminous Lyman Break Galaxy at z=7.730 using Keck/MOSFIRE". The Astrophysical Journal. 804: L30. arXiv:1502.05399. Bibcode:2015ApJ...804L..30O. doi:10.1088/2041-8205/804/2/L30.
  47. ↑ "Galaxy breaks record for farthest ever seen". Associated Press. CBC News. 6 May 2015. Archived from the original on 7 May 2015.
  48. ↑ Finkelstein, S. L.; Papovich, C.; Dickinson, M.; Song, M.; Tilvi, V.; Koekemoer, A. M.; Finkelstein, K. D.; Mobasher, B.; Ferguson, H. C.; Giavalisco, M.; Reddy, N.; Ashby, M. L. N.; Dekel, A.; Fazio, G. G.; Fontana, A.; Grogin, N. A.; Huang, J.-S.; Kocevski, D.; Rafelski, M.; Weiner, B. J.; Willner, S. P. (2013). "A galaxy rapidly forming stars 700 million years after the Big Bang at redshift 7.51". Nature. 502: 524–527. arXiv:1310.6031. Bibcode:2013Natur.502..524F. doi:10.1038/nature12657. PMID 24153304.
  49. ↑ Shibuya, Takatoshi; Kashikawa, Nobunari; Ota, Kazuaki; Iye, Masanori; Ouchi, Masami; Furusawa, Hisanori; Shimasaku, Kazuhiro; Hattori, Takashi (2012). "The First Systematic Survey for Lyalpha Emitters at z = 7.3 with Red-sensitive Subaru/Suprime-Cam". The Astrophysical Journal. 752: 114. arXiv:1112.3997. Bibcode:2012ApJ...752..114S. doi:10.1088/0004-637x/752/2/114.
  50. ↑ Ono, Yoshiaki; Ouchi, Masami; Mobasher, Bahram; Dickinson, Mark; Penner, Kyle; Shimasaku, Kazuhiro; Weiner, Benjamin J.; Kartaltepe, Jeyhan S.; Nakajima, Kimihiko; Nayyeri, Hooshang; Stern, Daniel; Kashikawa, Nobunari; Spinrad, Hyron (2012). "Spectroscopic Confirmation of Three z-dropout Galaxies at z = 6.844-7.213: Demographics of Lyalpha Emission in z ~ 7 Galaxies". The Astrophysical Journal. 744: 83. arXiv:1107.3159. Bibcode:2012ApJ...744...83O. doi:10.1088/0004-637X/744/2/83.
  51. ↑ Vanzella, E.; Pentericci, L.; Fontana, A.; Grazian, A.; Castellano, M.; Boutsia, K.; Cristiani, S.; Dickinson, M.; Gallozzi, S.; Giallongo, E.; Giavalisco, M.; Maiolino, R.; Moorwood, A.; Paris, D.; Santini, P. (2011). "Spectroscopic Confirmation of Two Lyman Break Galaxies at Redshift Beyond 7". The Astrophysical Journal. 730: L35. arXiv:1011.5500. Bibcode:2011ApJ...730L..35V. doi:10.1088/2041-8205/730/2/l35.
  52. ↑ Lehnert, M. D.; Nesvadba, N. P. H.; Cuby, J.-G.; Swinbank, A. M.; Morris, S.; Clément, B.; Evans, C. J.; Bremer, M. N.; Basa, S. (2010). "Spectroscopic confirmation of a galaxy at redshift z = 8.6". Nature. 467 (7318): 940–942. arXiv:1010.4312. Bibcode:2010Natur.467..940L. doi:10.1038/nature09462. PMID 20962840.
  53. ↑ Iye, M; Ota, K; Kashikawa, N; et al. (2006). "A galaxy at a redshift z = 6.96". Nature. 443: 186–188. arXiv:astro-ph/0609393. Bibcode:2006Natur.443..186I. doi:10.1038/nature05104. PMID 16971942. Archived from the original on 2008-05-16.
  54. 1 2 Yoshi Taniguchi (2008). "Star Forming Galaxies at z > 5". Proceedings of the International Astronomical Union. 3. arXiv:0804.0644. doi:10.1017/S1743921308020796.
  55. 1 2 PASJ: Publ. Astron. Soc. Jpn. 57, 165-182, February 25, 2005; The SUBARU Deep Field Project: Lymanα Emitters at a Redshift of 6.6
  56. 1 2 BBC News, Most distant galaxy detected Archived 2008-12-01 at the Wayback Machine., Tuesday, 25 March 2003, 14:28 GMT
  57. 1 2 SpaceRef, Subaru Telescope Detects the Most Distant Galaxy Yet and Expects Many More, Monday, March 24, 2003
  58. ↑ Kodaira; Taniguchi; Kashikawa; Kaifu; Ando; Karoji (2003). "The Discovery of Two Lyman-α Emitters Beyond Redshift 6 in the Subaru Deep Field". Publications of the Astronomical Society of Japan. 55: L17–L21. arXiv:astro-ph/0301096 |class= ignored (help). Bibcode:2003PASJ...55L..17K. doi:10.1093/pasj/55.2.L17. Cite uses deprecated parameter |class= (help)
  59. ↑ New Scientist, New record for Universe's most distant object Archived 2014-12-31 at the Wayback Machine., 17:19 14 March 2002
  60. ↑ BBC News, Far away stars light early cosmos Archived 2006-05-17 at the Wayback Machine., Thursday, 14 March 2002, 11:38 GMT
  61. ↑ Hu, E. M.; Cowie, L. L.; McMahon, R. G.; Capak, P.; Iwamuro, F.; Kneib, J.-P.; Maihara, T.; Motohara, K. (2002). "A Redshift [CLC][ITAL]z[/ITAL][/CLC] = 6.56 Galaxy behind the Cluster Abell 370". The Astrophysical Journal. 568 (2): L75–L79. arXiv:astro-ph/0203091. Bibcode:2002ApJ...568L..75H. doi:10.1086/340424.
  62. ↑ K2.1 HCM 6A — Discovery of a redshift z = 6.56 galaxy lying behind the cluster Abell 370 Archived 2011-05-18 at the Wayback Machine.
  63. ↑ Hu, Esther M.; McMahon, Richard G.; Cowie, Lennox L. (1999). "An Extremely Luminous Galaxy at [CLC][ITAL]z[/ITAL][/CLC] = 5.74". The Astrophysical Journal. 522: L9–L12. arXiv:astro-ph/9907079. Bibcode:1999ApJ...522L...9H. doi:10.1086/312205.
  64. 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 Publications of the Astronomical Society of the Pacific, 111: 1475–1502, 1999 December; SEARCH TECHNIQUES FOR DISTANT GALAXIES; INTRODUCTION
  65. 1 2 New York Times, Peering Back in Time, Astronomers Glimpse Galaxies Aborning, October 20, 1998
  66. 1 2 Astronomy Picture of the Day, A Baby Galaxy Archived 2011-07-04 at Wikiwix, March 24, 1998
  67. 1 2 Arjun Dey; Hyron Spinrad; Daniel Stern; Graham; Chaffee (1998). "A Galaxy at z=5.34". The Astrophysical Journal. 498: L93–L97. arXiv:astro-ph/9803137 |class= ignored (help). Bibcode:1998ApJ...498L..93D. doi:10.1086/311331. Cite uses deprecated parameter |class= (help)
  68. 1 2 "Previous What's New in Cosmology's". www.astro.ucla.edu. Archived from the original on 1 May 2018. Retrieved 1 May 2018.
  69. ↑ Franx, Marijn; Illingworth, Garth D.; Kelson, Daniel D.; Van Dokkum, Pieter G.; Tran, Kim-Vy (1997). "A Pair of Lensed Galaxies at [CLC][ITAL]z[/ITAL][/CLC] = 4.92 in the Field of CL 1358+62". The Astrophysical Journal. 486 (2): L75–L78. arXiv:astro-ph/9704090. Bibcode:1997ApJ...486L..75F. doi:10.1086/310844.
  70. ↑ Astronomy Picture of the Day, Behind CL1358+62: A New Farthest Object Archived 2011-07-04 at Wikiwix, July 31, 1997
  71. 1 2 3 4 5 "Astrophysics and Space Science" 1999, 269/270, 165-181 ; GALAXIES AT HIGH REDSHIFT - 8. Z > 5 GALAXIES Archived 2008-12-05 at the Wayback Machine. ; Garth Illingworth
  72. ↑ Wil van Breugel; Carlos De Breuck; Adam Stanford; Huub Röttgering; George Miley; Daniel Stern; Dante Minniti; Chris Carilli (1999). "Ultra-Steep Spectrum Radio Galaxies at Hy Redshifts". arXiv:astro-ph/9910311 |class= ignored (help).
  73. 1 2 Hyron Spinrad; Arjun Dey; Graham (1995). "Keck Observations of the Most Distant Galaxy: 8C1435+63 at z=4.25". The Astrophysical Journal. 438: L51. arXiv:astro-ph/9411007. Bibcode:1995ApJ...438L..51S. doi:10.1086/187713.
  74. 1 2 New Scientist, Galaxy hunters close to the edge Archived 2014-08-15 at the Wayback Machine., 5 November 1994
  75. ↑ Miley, G. K.; Chambers, K. C.; van Breugel, W. J. M.; Macchetto, F. (1992). "Hubble Space Telescope imaging of distant galaxies - 4C 41.17 at Z = 3.8". Astrophysical Journal. 401: L69. Bibcode:1992ApJ...401L..69M. doi:10.1086/186673.
  76. 1 2 Chambers, K. C.; Miley, G. K.; van Breugel, W. J. M. (1990). "4C 41.17 - A radio galaxy at a redshift of 3.8". Astrophysical Journal. 363: 21. Bibcode:1990ApJ...363...21C. doi:10.1086/169316.
  77. ↑ Science News, Farthest galaxy is cosmic question - 0902+34 Archived 2012-07-09 at Archive.is April 23, 1988
  78. ↑ Science News, Two distant galaxies provide new puzzles - 4c 41.17, B2 09021+34 Archived 2012-07-09 at Archive.is, November 14, 1992
  79. ↑ Paola Mazzei; Gianfranco De Zotti (1995). "Dust in High Redshift Radio Galaxies and the Early Evolution of Spheroidal Galaxies". Monthly Notices of the Royal Astronomical Society. 279: 535–544. arXiv:astro-ph/9509108 |class= ignored (help). Bibcode:1996MNRAS.279..535M. doi:10.1093/mnras/279.2.535. Cite uses deprecated parameter |class= (help)
  80. ↑ Le Fevre, O.; Hammer, F.; Nottale, L.; Mazure, A.; Christian, C. (1988). "Peculiar morphology of the high-redshift radio galaxies 3C 13 and 3C 256 in subarcsecond seeing". Astrophysical Journal. 324: L1. Bibcode:1988ApJ...324L...1L. doi:10.1086/185078.
  81. 1 2 Lilly, S. J.; Longair, M. S. (1984). "Stellar populations in distant radio galaxies". Royal Astronomical Society. 211: 833–855. Bibcode:1984MNRAS.211..833L. doi:10.1093/mnras/211.4.833.
  82. ↑ Longair, M. S. (1984). "The Most Distant Galaxies". Journal of the British Astronomical Association. 94: 97. Bibcode:1984JBAA...94...97L.
  83. ↑ "3C324 - Most Distant Galaxy". Bibcode:1983S&T....65..321S. |access-date= requires |url= (help)
  84. ↑ Smith, H. E.; Junkkarinen, V. T.; Spinrad, H.; Grueff, G.; Vigotti, M. (1979). "Spectrophotometry of three high-redshift radio galaxies - 3C 6.1, 3C 265, and 3C 352". The Astrophysical Journal. 231: 307. Bibcode:1979ApJ...231..307S. doi:10.1086/157194.
  85. ↑ "The Discovery of Radio Galaxies and Quasars". caltech.edu. Archived from the original on 3 March 2016. Retrieved 1 May 2018.
  86. ↑ McCarthy, P J (1993). "High Redshift Radio Galaxies". Annual Review of Astronomy and Astrophysics. 31: 639–688. Bibcode:1993ARA&A..31..639M. doi:10.1146/annurev.aa.31.090193.003231.
  87. 1 2 3 Sandage, Allan (1961). "The Ability of the 200-INCH Telescope to Discriminate Between Selected World Models". Astrophysical Journal. 133: 355. Bibcode:1961ApJ...133..355S. doi:10.1086/147041.
  88. ↑ Hubble, E. P. (1953). "The law of red shifts (George Darwin Lecture)". Monthly Notices of the Royal Astronomical Society. 113: 658–666. Bibcode:1953MNRAS.113..658H. doi:10.1093/mnras/113.6.658.
  89. ↑ OBSERVATIONAL TESTS OF WORLD MODELS; 6.1. Local Tests for Linearity of the Redshift-Distance Relation Archived 2008-09-20 at the Wayback Machine. ; Annu. Rev. Astron. Astrophys. 1988. 26: 561-630
  90. ↑ Humason, M. L.; Mayall, N. U.; Sandage, A. R. (1956). "Redshifts and magnitudes of extragalactic nebulae". Astron. J. 61: 97. Bibcode:1956AJ.....61...97H. doi:10.1086/107297.
  91. 1 2 3 "1053 May 8 meeting of the Royal Astronomical Society". The Observatory. 73: 97. 1953. Bibcode:1953Obs....73...97.
  92. ↑ Merrill, Paul W. (1958). "From Atoms to Galaxies". Astronomical Society of the Pacific Leaflets. 7: 393. Bibcode:1958ASPL....7..393M.
  93. ↑ Bolton, J. G. (1969). "Extragalactic Radio Sources". Astronomical Journal. 74: 131. Bibcode:1969AJ.....74..131B. doi:10.1086/110786. A&AAid:AAA001.141.093
  94. 1 2 Humason, M. L. (1936). "The Apparent Radial Velocities of 100 Extra-Galactic Nebulae". Astrophysical Journal. 83: 10. Bibcode:1936ApJ....83...10H. doi:10.1086/143696.
  95. ↑ THE FIRST 50 YEARS AT PALOMAR: 1949–1999 ; The Early Years of Stellar Evolution, Cosmology, and High-Energy Astrophysics; 5.2.1. The Mount Wilson Years Archived 2008-07-04 at the Wayback Machine. ; Annu. Rev. Astron. Astrophys. 1999. 37: 445-486
  96. 1 2 Chant, C. A. (1932). "Notes and Queries (Doings at Mount Wilson-Ritchey's Photographic Telescope-Infra-red Photographic Plates)". Journal of the Royal Astronomical Society of Canada. 26: 180. Bibcode:1932JRASC..26..180C.
  97. ↑ Humason, Milton L. (1931). "Apparent Velocity-Shifts in the Spectra of Faint Nebulae". Astrophysical Journal. 74: 35. Bibcode:1931ApJ....74...35H. doi:10.1086/143287.
  98. ↑ Hubble, Edwin; Humason, Milton L. (1931). "The Velocity-Distance Relation among Extra-Galactic Nebulae". Astrophysical Journal. 74: 43. Bibcode:1931ApJ....74...43H. doi:10.1086/143323.
  99. 1 2 Humason, M. L. (1931). "The Large Apparent Velocities of Extra-Galactic Nebulae". Astronomical Society of the Pacific Leaflets. 1: 149. Bibcode:1931ASPL....1..149H.
  100. ↑ Humason, M. L. (1930). "The Rayton short-focus spectrographic objective". Astrophys. J. 71: 351. Bibcode:1930ApJ....71..351H. doi:10.1086/143255.
  101. 1 2 3 4 Trimble, Virginia (1996). "H_0: The Incredible Shrinking Constant, 1925–1975". Publications of the Astronomical Society of the Pacific. 108: 1073. Bibcode:1996PASP..108.1073T. doi:10.1086/133837.
  102. ↑ "The Berkeley Meeting of the Astronomical Society of the Pacific, June 20–21, 1929". Publications of the Astronomical Society of the Pacific. 41: 244. 1929. Bibcode:1929PASP...41..244.. doi:10.1086/123945.
  103. 1 2 From the Proceedings of the National Academy of Sciences; Volume 15 : March 15, 1929 : Number 3 ; THE LARGE RADIAL VELOCITY OF N. G. C. 7619 Archived 2008-07-20 at Wikiwix ; January 17, 1929
  104. ↑ THE JOURNAL OF THE ROYAL ASTRONOMICAL SOCIETY OF CANADA / JOURNAL DE LA SOCIÉTÉ ROYALE D'ASTRONOMIE DU CANADA; Vol. 83, No.6 December 1989 Whole No. 621 ; EDWIN HUBBLE 1889–1953 Archived 2008-07-19 at Wikiwix
  105. 1 2 National Academy of Sciences; Biographical Memoirs: V. 52 - VESTO MELVIN SLIPHER; ISBN 0-309-03099-4
  106. ↑ Bailey, S. I. (1920). "Comet Skjellerup". Harvard College Observatory Bulletin No. 739. 739: 1. Bibcode:1920BHarO.739....1B.
  107. ↑ New York Times, DREYER NEBULA NO. 584 INCONCEIVABLY DISTANT; Dr. Slipher Says the Celestial Speed Champion Is 'Many Millions of Light Years' Away. Archived 2016-03-04 at the Wayback Machine. ; January 19, 1921, Wednesday
  108. 1 2 New York Times, NEBULA DREYER BREAKS ALL SKY SPEED RECORDS; Portion of the Constellation of Cetus Is Rushing Along at Rate of 1,240 Miles a Second. Archived 2016-03-13 at the Wayback Machine. ; January 18, 1921, Tuesday
  109. ↑ Coe, Dan; Zitrin, Adi; Carrasco, Mauricio; Shu, Xinwen; Zheng, Wei; Postman, Marc; Bradley, Larry; Koekemoer, Anton; Bouwens, Rychard; Broadhurst, Tom; Monna, Anna; Host, Ole; Moustakas, Leonidas A.; Ford, Holland; Moustakas, John; van der Wel, Arjen; Donahue, Megan; Rodney, Steven A.; Benítez, Narciso; Jouvel, Stephanie; Seitz, Stella; Kelson, Daniel D.; Rosati, Piero (2013). "CLASH: Three Strongly Lensed Images of a Candidate z ≈ 11 Galaxy". The Astrophysical Journal. 762: 32. arXiv:1211.3663. Bibcode:2013ApJ...762...32C. doi:10.1088/0004-637x/762/1/32.
  110. ↑ Lehnert, M. D.; Nesvadba, N. P. H.; Cuby, J.-G.; Swinbank, A. M.; Morris, S.; Clément, B.; Evans, C. J.; Bremer, M. N.; Basa, S. (2010). "Spectroscopic confirmation of a galaxy at redshift z = 8.6". Nature. 467 (7318): 940–942. arXiv:1010.4312. Bibcode:2010Natur.467..940L. doi:10.1038/nature09462. PMID 20962840.
  111. ↑ New Scientist, Baby galaxies sighted at dawn of universe Archived 2015-01-18 at the Wayback Machine., 22:34 10 July 2007
  112. ↑ Lawrence Livermore National Laboratory, Lab scientists revoke status of space object Archived 2008-09-22 at the Wayback Machine.
  113. ↑ Hsiao-Wen Chen; Lanzetta; Sebastian Pascarelle; Noriaki Yahata (2000). "The Unusual Spectral Energy Distribution of a Galaxy Previously Reported to be at Redshift 6.68". Nature. 408: 562–564. arXiv:astro-ph/0011558 |class= ignored (help). Bibcode:2000Natur.408..562C. doi:10.1038/35046031. Cite uses deprecated parameter |class= (help)
  114. ↑ BBC News, Hubble spies most distant object, Thursday, April 15, 1999
  115. ↑ Hu; McMahon (1996). "Detection of Lyman-alpha Emitting Galaxies at Redshift z=4.55". Nature. 382 (6588): 231–233. arXiv:astro-ph/9606135. Bibcode:1996Natur.382..231H. doi:10.1038/382231a0.
  116. ↑ 31/01/02 ; "DAZLE NEAR IR NARROW BAND IMAGER" (PDF). Archived from the original (PDF) on 2008-07-27.  (570 KB) ; DAZLE-IoA-Doc-0002
  117. ↑ ESO Press Release 11/95, ESO Astronomers Detect a Galaxy at the Edge of the Universe, 15 September 1995
  118. ↑ New Scientist, Trouble at the edge of time Archived 2015-05-07 at the Wayback Machine., 21 October 1995
  119. ↑ Wampler, E. J.; et al. (1996). "High resolution observations of the QSO BR 1202-0725: deuterium and ionic abundances at redshifts above z=4". Astronomy & Astrophysics. 316: 33. arXiv:astro-ph/9512084. Bibcode:1996A&A...316...33W.
  120. ↑ Elston, Richard; Bechtold, Jill; Hill, Gary J.; Ge, Jian (1996). "A Redshift 4.38 MG II Absorber toward BR 1202-0725". Astrophysical Journal Letters. 456: L13. Bibcode:1996ApJ...456L..13E. doi:10.1086/309853.
  121. ↑ Smail, I.; Ellis, R. S.; Aragon-Salamanca, A.; Soucail, G.; Mellier, Y.; Giraud, E. (1993). "The Nature of Star Formation in Lensed Galaxies at High Redshift". R.a.s. Monthly Notices V.263. 263: 628–640. Bibcode:1993MNRAS.263..628S. doi:10.1093/mnras/263.3.628.
  122. ↑ "Gravitational Lenses II: Galaxy Clusters as Lenses". uni-bonn.de. Archived from the original on 22 February 2008. Retrieved 1 May 2018.
  123. ↑ Djorgovski, S.; Strauss, Michael A.; Spinrad, Hyron; McCarthy, Patrick; Perley, R. A. (1987). "A galaxy at a redshift of 3.215 - Further studies of the PKS 1614+051 system". Astronomical Journal. 93: 1318. Bibcode:1987AJ.....93.1318D. doi:10.1086/114414. ISSN 0004-6256.
  124. ↑ NED, Searching NED for object "3C 123"
  125. ↑ Spinrad, H. (1975). "3C 123: a distant first-ranked cluster galaxy at z = 0.637". Astrophys. J. 199: L3. Bibcode:1975ApJ...199L...3S. doi:10.1086/181835.
  126. ↑ Staff (May 21, 2015). "PIA19339: Dusty 'Sunrise' at Core of Galaxy (Artist's Concept)". NASA. Archived from the original on May 22, 2015. Retrieved May 21, 2015.
  127. ↑ Staff (21 May 2015). "WISE spacecraft discovers most luminous galaxy in universe". PhysOrg. Archived from the original on 22 May 2015. Retrieved 22 May 2015.
  128. 1 2 Overbye, Dennis (17 June 2015). "Astronomers Report Finding Earliest Stars That Enriched Cosmos". New York Times. Archived from the original on 17 June 2015. Retrieved 17 June 2015.
  129. ↑ Sci-News.com, "Segue 2: Most Lightweight Galaxy in Universe" Archived 2015-01-13 at the Wayback Machine., Natali Anderson, 11 June 2013 (accessed 11 June 2013)
  130. ↑ "SEGUE 2: THE LEAST MASSIVE GALAXY". The Astrophysical Journal. 770: 16. arXiv:1304.6080. Bibcode:2013ApJ...770...16K. doi:10.1088/0004-637X/770/1/16.
  131. ↑ Astronomy Now, "Heavyweight galaxy is king of its cluster" Archived 2013-02-15 at the Wayback Machine., Keith Cooper, 13 May 2010 (accessed 9 March 2013)
  132. ↑ Research.gov, "Astronomers Discover Most Massive Galaxy Yet, Formed by 'Galactic Cannibalism'" Archived 2014-03-06 at the Wayback Machine. (accessed 9 March 2013)
  133. ↑ "Undergraduates discover the densest galaxies known". Space Daily. 29 July 2015. Archived from the original on 18 August 2015.
  134. ↑ ESO Press Release 25/00 , Most Massive Spiral Galaxy Known in the Universe Archived 2008-06-16 at the Wayback Machine. , 8 December 2000
  135. ↑ Grebel (2000). "Star Clusters in Local Group Galaxies". ASP Conference Series. 211: 262–269. arXiv:astro-ph/9912529. Bibcode:2000ASPC..211..262G.
  136. ↑ Chandra X-Ray Observatory at Havard, "Abell 644 and SDSS J1021+1312: How Often do Giant Black Holes Become Hyperactive?" Archived 2012-05-15 at the Wayback Machine., 20 December 2010 (accessed 7 July 2012)
  137. ↑ Sky and Telescope, Stars in the Middle of Nowhere, 10 January 2008
  138. ↑ Sky and Telescope, Galaxy Monster Mash, 9 August 2007
  139. ↑ ABC News, Found! Oldest galaxy pile-up Archived 2015-01-24 at the Wayback Machine., Wednesday, 9 April 2008
  140. ↑ Cooke, Jeff; Barton, Elizabeth J.; Bullock, James S.; Stewart, Kyle R.; Wolfe, Arthur M. (2008). "A Candidate Brightest Protocluster Galaxy atz= 3.03". The Astrophysical Journal. 681 (2): L57–L60. arXiv:0803.3808. Bibcode:2008ApJ...681L..57C. doi:10.1086/590406.
  141. ↑ "Black hole found in Omega Centauri". UPI.com. 10 April 2008. Archived from the original on 22 October 2012.
  142. ↑ "Local Large-Scale Structure". Hayden Planetarium. 15 September 2008. Archived from the original on 28 August 2008.
  143. ↑ Goldman, Stuart (28 September 2007). "New Stars in a Galaxy's Wake". Sky & Telescope.
  144. ↑ "Orphan' Stars Found in Long Galaxy Tail" (Press release). NASA. 20 September 2007. Archived from the original on 4 November 2008.
  145. ↑ Sun; Donahue; Voit (2007). "H-alpha tail, intracluster HII regions and star-formation: ESO137-001 in Abell 3627". arXiv:0706.1220 [astro-ph].
  146. ↑ Fraser Cain (20 September 2007). "Galaxy Leaves New Stars Behind in its Death Plunge". Universe Today. Archived from the original on 12 October 2008.
  147. ↑ Geach et al., A Redline Starburst: CO(2–1) Observations of an Eddington-Limited Galaxy Reveal Star Formation At Its Most Extreme Draft version 27 February 2013 Archived 13 March 2018 at the Wayback Machine.
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