Danh sách những thiên thể xa nhất

Bách khoa toàn thư mở Wikipedia

Danh sách những thiên thể xa nhất đã được khoa học phát hiện và xác minh. Việc đo khoảng cách được xác định dựa trên công nhận tuổi của vũ trụ tính từ Vụ Nổ Lớn khoảng 13,787±0,020 tỉ năm ánh sáng. Việc đo khoảng cách tới các thiên thể ở xa hầu hết thực hiện thông qua việc đo độ dịch chuyển đỏ theo định luật Hubble

Đã xác nhận[sửa | sửa mã nguồn]

Danh sách các thiên thể xe nhất xác nhận bằng dịch chuyển đỏ quang phổ
Ảnh Tên Dịch chuyển đỏ
(z) 		Khoảng cách§
(Gly)[1][2][3][4] 		Loại Ghi chú
F200DB-045 zp = 20,4+0,3
−0,3[5]
hoặc 0,70+0,19
−0,55[6] or 0,40+0,15
−0,26[7] 		13,725[1] / 13,745[2] / 13,623[3] / 13,621[4] Galaxy Lyman-break galaxy discovered by JWST[5]
NOTE: The redshift value of the galaxy presented by the procedure in one study[6] may differ from the values presented in other studies using different procedures.[5][7][8]
F200DB-175 zp = 16,2+0,3
−0,0 		13,657[1] / 13,677[2] / 13,555[3] / 13,554[4] Galaxy Lyman-break galaxy discovered by JWST[5]
S5-z17-1 z = 16,0089±0,0004
hoặc 4,6108±0,0001 		13,653[1] / 13,673[2] / 13,551[3] / 13,550[4] Galaxy Lyman-break galaxy discovered by JWST; tentative (5.1σ) ALMA detection of a single emission line possibly attributed to either [C II] (z = 4,6108±0,0001) hoặc [O III] (z = 16,0089±0,0004).[9][10]
F150DB-041 zp = 16,0+0,2
−0,2[5]
or 3,70+002
−059[6] 		13,653[1] / 13,673[2] / 13,551[3] / 13,549[4] Galaxy Lyman-break galaxy discovered by JWST[5][6]
SMACS-z16a zp = 15,92+0,17
−0,15[11]
or 2,96+0,73
−0,21[6] 		13,651[1] / 13,671[2] / 13,549[3] / 13,548[4] Galaxy Lyman-break galaxy discovered by JWST[11][6]
F200DB-015 zp = 15,8+3,4
−0,1 		13,648[1] / 1,.668[2] / 13,546[3] / 13,545[4] Galaxy Lyman-break galaxy discovered by JWST[5]
F200DB-181 zp = 15,8+0,5
−0,3 		13,648[1] / 13,668[2] / 13,546[3] / 13,545[4] Galaxy Lyman-break galaxy discovered by JWST[5]
F200DB-159 zp = 15,8+4,0
−15,2 		13,648[1] / 13,668[2] / 13,546[3] / 13,545[4] Galaxy Lyman-break galaxy discovered by JWST[5]
F200DB-086 zp = 15,4+0,6
−14,6[5]
or 3,53+10,28
−1,84[6] 		13,639[1] / 13,659[2] / 13,537[3] / 13,536[4] Galaxy Lyman-break galaxy discovered by JWST[5][6]
SMACS-z16b zp = 15,32+0,16
−0,13[11]
or 15,39+0,18
−0,26[6] 		13,637[1] / 13,657[2] / 13,535[3] / 13,534[4] Galaxy Lyman-break galaxy discovered by JWST[6][11]
F150DB-048 zp = 15,0+0,2
−0,8 		13,629[1] / 13,649[2] / 13,527[3] / 13,526[4] Galaxy Lyman-break galaxy discovered by JWST[5]
F150DB-007 zp = 14,6+0,4
−0,4 		13,619[1] / 13,639[2] / 13,517[3] / 13,516[4] Galaxy Lyman-break galaxy discovered by JWST[5]
F150DB-004 zp = 14,0+0,4
−2,0 		13,602[1] / 13,622[2] / 13,500[3] / 13,499[4] Galaxy Lyman-break galaxy discovered by JWST[5]
F150DB-079 zp = 13,8+0,5
−1,9 		13,596[1] / 13,616[2] / 13,494[3] / 13,493[4] Galaxy Lyman-break galaxy discovered by JWST[5]
F150DA-007 zp = 13,4+0,6
−2,0 		13,583[1] / 13,603[2] / 13,481[3] / 13,480[4] Galaxy Lyman-break galaxy discovered by JWST[5]
F150DA-053 zp = 13,4+0,3
−2,3 		13,583[1] / 13,603[2] / 13,481[3] / 13,480[4] Galaxy Lyman-break galaxy discovered by JWST[5]
F150DA-050 zp = 13,4+0,6
−10,0 		13,583[1] / 13,603[2] / 13,481[3] / 13,480[4] Galaxy Lyman-break galaxy discovered by JWST[5]
F150DA-058 zp = 13,4+0,6
−12,5[5]
3,42+0,30
−0,20[6] 		13,583[1] / 13,603[2] / 13,481[3] / 13,480[4] Galaxy Lyman-break galaxy discovered by JWST[5][6]
F150DA-038 zp = 13,4+0,4
−13,2 		13,583[1] / 13,603[2] / 13,481[3] / 13,480[4] Galaxy Lyman-break galaxy discovered by JWST[5]
HD1 z = 13,27 13,579[1] / 13,599[2] / 13,477[3] / 13,476[4] Galaxy Kỷ lục Guinness về thiên hà xa nhất đã xác nhận
Lyman-break galaxy (5σ confidence) followed with a tentative ALMA detection of a single [O III] oxygen emission line only (4σ confidence)[12]
JADES-GS-z13-0 z = 13,20+0,04
−0,07 		13,576[1] / 13,596[2] / 13,474[3] / 13,473[4] Galaxy Lyman-break galaxy, detection of the Lyman break with JWST/NIRSpec, not yet been through the peer-review process[13]
JADES-GS-z12-0 z = 12,63+0,24
−0,08 		13,556[1] / 13,576[2] / 13,454[3] / 13,453[4] Galaxy Lyman-break galaxy, detection of the Lyman break with JWST/NIRSpec, not yet been through the peer-review process[13]
GLASS-z12 z = 12,117+0,01
−0,01 		13,536[1] / 13,556[2] / 13,434[3] / 13,433[4] Galaxy Lyman-break galaxy discovered by JWST/NIRCam, confirmed by ALMA detection of [O III] emission[14]
JADES-GS-z11-0 z = 11,58+0,05
−0,05 		13,512[1] / 13,532[2] / 13,410[3] / 13,409[4] Galaxy Lyman-break galaxy, detection of the Lyman break with JWST/NIRSpec, not yet been through the peer-review process[13]
GN-z11 z = 10,957±0,001 13,481[1] / 13,501[2] / 13,380[3] / 13,379[4] Galaxy Lyman-break galaxy; detection of the Lyman break with HST at 5.5σ[15] and carbon emission lines with Keck/MOSFIRE at 5.3σ[16]
UDFj-39546284 z = 10,38+0,07
−0,06 		13,449[1] / 13,469[2] / 13,348[3] / 13,347[4] Galaxy Lyman-break galaxy, detection of the Lyman break with JWST/NIRSpec, not yet been through the peer-review process[13]
JD1 z = 9,756+0,017
−0,007 		13,409[1] / 13,429[2] / 13,308[3] / 13,307[4] Galaxy Lyman-break galaxy, detection of the Lyman break with JWST/NIRSpec, not yet been through the peer-review process[17]
MACS1149-JD1 z = 9,1096±0,0006 13,361[1] / 13,381[2] / 13,261[3] / 13,260[4] Galaxy Detection of hydrogen emission line with the VLT, and oxygen line with ALMA[18]
EGSY8p7 z = 8,683+0,001
−0,004 		13,325[1] / 13,345[2] / 13,225[3] / 13,224[4] Galaxy Lyman-alpha emitter; detection of Lyman-alpha with Keck/MOSFIRE at 7.5σ confidence[19]
SMACS-4590 z = 8,496 13,308[1] / 13,328[2] / 13,208[3] / 13,207[4] Galaxy Detection of hydrogen, oxygen, and neon emission lines with JWST/NIRSpec[20][21][22][23]
A2744 YD4 z = 8,38 13,297[1] / 13,317[2] / 13,197[3] / 13,196[4] Galaxy Lyman-alpha and [O III] emission detected with ALMA at 4.0σ confidence[24]
MACS0416 Y1 z = 8,3118±0,0003 13,290[1] / 13,310[2] / 13,190[3] / 13,189[4] Galaxy [O III] emission detected with ALMA at 6.3σ confidence[25]
GRB 090423 z = 8,23+0,06
−0,07 		13,282[1] / 13,302[2] / 13,182[3] / 13,181[4] Gamma-ray burst Lyman-alpha break detected[26]
RXJ2129-11002 z = 8,16±0,01 13,175[1] Galaxy [O III] doublet, Hβ, and [O II] doublet as well as Lyman-alpha break detected with JWST/NIRSpec prism [27]
RXJ2129-11022 z = 8,15±0,01 13,174[1] Galaxy [O III] doublet and Hβ as well as Lyman-alpha break detected with JWST/NIRSpec prism [27]
EGS-zs8-1 z = 7,7302±0,0006 13,228[1] / 13,248[2] / 13,129[3] / 13,128[4] Galaxy Lyman-break galaxy[28]
SMACS-6355 z = 7,665 13,221[1] / 13,241[2] / 13,121[3] / 13,120[4] Galaxy Detection of hydrogen, oxygen, and neon emission lines with JWST/NIRSpec[20][21][22][23]
z7_GSD_3811 z = 7,6637±0,0011 13,221[1] / 13,240[2] / 13,121[3] / 13,120[4] Galaxy Lyman-alpha emitter[29]
SMACS-10612 z = 7,658 13,221[1] / 13,241[2] / 13,120[3] / 13,119[4] Galaxy Detection of hydrogen, oxygen, and neon emission lines with JWST/NIRSpec[20][21][22]>[23]
QSO J0313–1806 z = 7,6423±0,0013 13,218[1] / 13,238[2] / 13,119[3] / 13,118[4] Quasar Lyman-alpha break detected[30]
ULAS J1342+0928 z = 7,5413±0,0007 13,206[1] / 13,226[2] / 13,107[3] / 13,106[4] Quasar Redshift estimated from [C II] emission[31]
z8 GND 5296 z = 7,51 13,202[1] / 13,222[2] / 13,103[3] / 13,102[4] Galaxy Lyman-alpha emitter[32]
A1689-zD1 z = 7,5±0,2 13,201[1] / 13,221[2] / 13,102[3] / 13,101[4] Galaxy Lyman-break galaxy[33]
GS2_1406 z = 7,452±0,003 13,195[1] / 13,215[2] / 13,096[3] / 13,095[4] Galaxy Lyman-alpha emitter[34]
GN-108036 z = 7,213 13,164[1] / 13,184[2] / 13,065[3] / 13,064[4] Galaxy Lyman alpha emitter[35]
SXDF-NB1006-2 z = 7,2120±0,0003 13,164[1] / 13,184[2] / 13,065[3] / 13,064[4] Galaxy [O III] emission detected[36]
BDF-3299 z = 7,109±0,002 13,149[1] / 13,169[2] / 13,051[3] / 13,050[4] Galaxy Lyman-break galaxy[37]
ULAS J1120+0641 z = 7085±0,003 13,146[1] / 13,166[2] / 13,048[3] / 13,047[4] Quasar Redshift estimated from Si III]+C III] and Mg II emission lines[38]
A1703 zD6 z = 7,045±0,004 13,140[1] / 13,160[2] / 13,042[3] / 13,041[4] Galaxy Gravitationally-lensed Lyman-alpha emitter[39]
BDF-521 z = 7,008±0,002 13,135[1] / 13,155[2] / 13,037[3] / 13,036[4] Galaxy Lyman-break galaxy[37]
G2_1408 z = 6,972±0,002 13,130[1] / 13,150[2] / 13,032[3] / 13,030[4] Galaxy Lyman-alpha emitter[40]
IOK-1 z = 6,965 13,129[1] / 13,149[2] / 13,030[3] / 13,029[4] Galaxy Lyman-alpha emitter[35]
LAE J095950.99+021219.1 z = 6,944 13,126[1] / 13,146[2] / 13,028[3] / 13,027[4] Galaxy Lyman-alpha emitter[41]
SDF-46975 z = 6,844 13,111[1] / 13,131[2] / 13,013[3] / 13,012[4] Galaxy Lyman-alpha emitter[35]
PSO J172.3556+18.7734 z = 6,823+0,003
−0,001 		13,107[1] / 13,127[2] / 13,010[3] / 13,009[4] Quasar
(astrophysical jet) 		Redshift estimated from Mg II emission[42]

§ The tabulated distance is the light travel distance, which has no direct physical significance. See discussion at distance measures and Observable Universe

Ứng cử viên[sửa | sửa mã nguồn]

Danh sách ứng cử viên thiên thể xa nhất
Danh pháp Dịch chuyển đỏ
(z) 		Khoảng cách§
(Gly) 		Thể loại Ghi chú
F200DB-045 zp = 204+03
−03[5]
or 070+019
−055[6] or 040+015
−026[7] 		13.725[1] / 13.745[2] / 13.623[3] / 13.621[4] Galaxy Lyman-break galaxy discovered by JWST[5]
NOTE: The redshift value of the galaxy presented by the procedure in one study[6] may differ from the values presented in other studies using different procedures.[5][7][8]
CEERS-93316 zp = 1639+032
−022[43]
or 1625+024
−046[9] 		13.661[1] / 13.681[2] / 13.559[3] / 13.558[4] Galaxy Lyman-break galaxy discovered by JWST[9][43]
F200DB-175 zp = 162+03
−00 		13.657[1] / 13.677[2] / 13.555[3] / 13.554[4] Galaxy Lyman-break galaxy discovered by JWST[5]
S5-z17-1 z = 160089±00004
or 46108±00001 		13.653[1] / 13.673[2] / 13.551[3] / 13.550[4] Galaxy Lyman-break galaxy discovered by JWST; tentative (5.1σ) ALMA detection of a single emission line possibly attributed to either [C II] (z = 46108±00001) or [O III] (z = 160089±00004).[9][10]
F150DB-041 zp = 160+02
−02[5]
or 370+002
−059[6] 		13.653[1] / 13.673[2] / 13.551[3] / 13.549[4] Galaxy Lyman-break galaxy discovered by JWST[5][6]
SMACS-z16a zp = 1592+017
−015[11]
or 296+073
−021[6] 		13.651[1] / 13.671[2] / 13.549[3] / 13.548[4] Galaxy Lyman-break galaxy discovered by JWST[11][6]
F200DB-015 zp = 158+34
−01 		13.648[1] / 13.668[2] / 13.546[3] / 13.545[4] Galaxy Lyman-break galaxy discovered by JWST[5]
F200DB-181 zp = 158+05
−03 		13.648[1] / 13.668[2] / 13.546[3] / 13.545[4] Galaxy Lyman-break galaxy discovered by JWST[5]
F200DB-159 zp = 158+40
−152 		13.648[1] / 13.668[2] / 13.546[3] / 13.545[4] Galaxy Lyman-break galaxy discovered by JWST[5]
F200DB-086 zp = 154+06
−146[5]
or 353+1028
−184[6] 		13.639[1] / 13.659[2] / 13.537[3] / 13.536[4] Galaxy Lyman-break galaxy discovered by JWST[5][6]
SMACS-z16b zp = 1532+016
−013[11]
or 1539+018
−026[6] 		13.637[1] / 13.657[2] / 13.535[3] / 13.534[4] Galaxy Lyman-break galaxy discovered by JWST[6][11]
F150DB-048 zp = 150+02
−08 		13.629[1] / 13.649[2] / 13.527[3] / 13.526[4] Galaxy Lyman-break galaxy discovered by JWST[5]
F150DB-007 zp = 146+04
−04 		13.619[1] / 13.639[2] / 13.517[3] / 13.516[4] Galaxy Lyman-break galaxy discovered by JWST[5]
F150DB-004 zp = 140+04
−20 		13.602[1] / 13.622[2] / 13.500[3] / 13.499[4] Galaxy Lyman-break galaxy discovered by JWST[5]
F150DB-079 zp = 138+05
−19 		13.596[1] / 13.616[2] / 13.494[3] / 13.493[4] Galaxy Lyman-break galaxy discovered by JWST[5]
F150DA-007 zp = 134+06
−20 		13.583[1] / 13.603[2] / 13.481[3] / 13.480[4] Galaxy Lyman-break galaxy discovered by JWST[5]
F150DA-053 zp = 134+03
−23 		13.583[1] / 13.603[2] / 13.481[3] / 13.480[4] Galaxy Lyman-break galaxy discovered by JWST[5]
F150DA-050 zp = 134+06
−100 		13.583[1] / 13.603[2] / 13.481[3] / 13.480[4] Galaxy Lyman-break galaxy discovered by JWST[5]
F150DA-058 zp = 134+06
−125[5]
342+030
−020[6] 		13.583[1] / 13.603[2] / 13.481[3] / 13.480[4] Galaxy Lyman-break galaxy discovered by JWST[5][6]
F150DA-038 zp = 134+04
−132 		13.583[1] / 13.603[2] / 13.481[3] / 13.480[4] Galaxy Lyman-break galaxy discovered by JWST[5]
F150DA-010 zp = 128+06
−15 		13.562[1] / 13.582[2] / 13.460[3] / 13.459[4] Galaxy Lyman-break galaxy discovered by JWST[5]
S5-z12-1 zp = 1257+123
−046 		13.553[1] / 13.573[2] / 13.452[3] / 13.451[4] Galaxy Lyman-break galaxy discovered by JWST[9]
CEERS-27535 4 zp = 1256+175
−027 		13.553[1] / 13.573[2] / 13.452[3] / 13.451[4] Galaxy Lyman-break galaxy discovered by JWST[43]
SMACS-1566 zp = 1229+150
−044 		13.542[1] / 13.562[2] / 13.441[3] / 13.440[4] Galaxy Lyman-break galaxy discovered by JWST[43]
SMACS-z12b
(F150DA-077) 		zp = 1226+017
−016[6][11]
or 134+04
−17[5] 		13.541[1] / 13.561[2] / 13.440[3] / 13.439[4] Galaxy Lyman-break galaxy discovered by JWST[5][6][11]
SMACS-z12a zp = 1220+021
−012 		13.539[1] / 13.559[2] / 13.437[3] / 13.436[4] Galaxy Lyman-break galaxy discovered by JWST[6][11]
CR2-z12-4 zp = 1208+211
−125 		13.534[1] / 13.554[2] / 13.432[3] / 13.431[4] Galaxy Lyman-break galaxy discovered by JWST[9]
SMACS-10566 zp = 1203+057
−026 		13.532[1] / 13.552[2] / 13.430[3] / 13.429[4] Galaxy Lyman-break galaxy discovered by JWST[43]
XDFH-2395446286 zp = 120+01
−02 		13.530[1] / 13.550[2] / 13.429[3] / 13.428[4] Galaxy Lyman-break galaxy detected by JWST and Hubble[44]
CR2-z12-2 zp = 1196+144
−087 		13.529[1] / 13.549[2] / 13.427[3] / 13.426[4] Galaxy Lyman-break galaxy discovered by JWST[9]
9-BUSCAR zp = 1191+010
−022 		13.527[1] / 13.547[2] / 13.425[3] / 13.424[4] Galaxy Lyman-break galaxy discovered by JWST[45]
SMACS-8347 zp = 1190+027
−039 		13.526[1] / 13.546[2] / 13.425[3] / 13.424[4] Galaxy Lyman-break galaxy discovered by JWST[43]
CEERS-26409 4 zp = 1190+160
−070 		13.526[1] / 13.546[2] / 13.425[3] / 13.424[4] Galaxy Lyman-break galaxy discovered by JWST[43]
F150DB-069 zp = 118+17
−02 		13.522[1] / 13.542[2] / 13.420[3] / 13.419[4] Galaxy Lyman-break galaxy discovered by JWST[5]
CEERS J141946.36+525632.8
(Maisie's Galaxy) 		zp = 118+03
−02 		13.522[1] / 13.542[2] / 13.420[3] / 13.419[4] Galaxy Lyman-break galaxy discovered by JWST[43][46]
XDFH-2334046578 zp = 118+04
−05 		13.522[1] / 13.542[2] / 13.420[3] / 13.419[4] Galaxy Lyman-break galaxy detected by JWST and Hubble[44]
CR2-z12-3 zp = 1166+069
−071 		13.515[1] / 13.535[2] / 13.414[3] / 13.413[4] Galaxy Lyman-break galaxy discovered by JWST[9]
CR2-z12-1 zp = 1163+051
−053 		13.514[1] / 13.534[2] / 13.413[3] / 13.412[4] Galaxy Lyman-break galaxy discovered by JWST[9]
F150DB-088 zp = 116+03
−02 		13.513[1] / 13.533[2] / 13.411[3] / 13.410[4] Galaxy Lyman-break galaxy discovered by JWST[5]
F150DB-084 zp = 116+04
−04 		13.513[1] / 13.533[2] / 13.411[3] / 13.410[4] Galaxy Lyman-break galaxy discovered by JWST[5]
F150DB-044 zp = 114+04
−113 		13.503[1] / 13.523[2] / 13.402[3] / 13.401[4] Galaxy Lyman-break galaxy discovered by JWST[5]
XDFH-2404647339 zp = 114+04
−05 		13.503[1] / 13.523[2] / 13.402[3] / 13.401[4] Galaxy Lyman-break galaxy detected by JWST and Hubble[44]
F150DB-075 zp = 114+04
−01[5]
004+001
−001[6] 		13.503[1] / 13.523[2] / 13.402[3] / 13.401[4] Galaxy Lyman-break galaxy discovered by JWST[5][6]
F150DA-062 zp = 114+03
−03[5]
178+020
−008[6] 		13.503[1] / 13.523[2] / 13.402[3] / 13.401[4] Galaxy Lyman-break galaxy discovered by JWST[5][6]
CEERS-127682 zp = 1140+059
−051 		13.503[1] / 13.523[2] / 13.402[3] / 13.401[4] Galaxy Lyman-break galaxy discovered by JWST[43]
CEERS-5268 2 zp = 1140+030
−111 		13.503[1] / 13.523[2] / 13.402[3] / 13.401[4] Galaxy Lyman-break galaxy discovered by JWST[43]
F150DA-060 zp = 114+06
−82 		13.503[1] / 13.523[2] / 13.402[3] / 13.401[4] Galaxy Lyman-break galaxy discovered by JWST[5]
F150DA-031 zp = 114+10
−82 		13.503[1] / 13.523[2] / 13.402[3] / 13.401[4] Galaxy Lyman-break galaxy discovered by JWST[5]
F150DA-052 zp = 114+08
−106 		13.503[1] / 13.523[2] / 13.402[3] / 13.401[4] Galaxy Lyman-break galaxy discovered by JWST[5]
F150DB-054 zp = 114+05
−108 		13.503[1] / 13.523[2] / 13.402[3] / 13.401[4] Galaxy Lyman-break galaxy discovered by JWST[5]
SMACS-z11d zp = 1128±032
or 235+030
−067 		Galaxy Lyman-break galaxy discovered by JWST[6]
CEERS-77241 zp = 1127+039
−070 		Galaxy Lyman-break galaxy discovered by JWST[43]
CEERS-6647 zp = 1127+058
−028 		Galaxy Lyman-break galaxy discovered by JWST[43]
CEERS-622 4 zp = 1127+048
−060 		Galaxy Lyman-break galaxy discovered by JWST[43]
SMACS-z11c zp = 1122±032
or 384+005
−004 		Galaxy Lyman-break galaxy discovered by JWST[6]
SMACS-z11b zp = 1122±056
or 694+007
−007 		Galaxy Lyman-break galaxy discovered by JWST[6]
F150DA-005 zp = 112+04
−03 		Galaxy Lyman-break galaxy discovered by JWST[5]
F150DA-020 zp = 112+02
−79 		Galaxy Lyman-break galaxy discovered by JWST[5]
CEERS-61486 zp = 1115+037
−035 		Galaxy Lyman-break galaxy discovered by JWST[43]
SMACS-z11e
(F150DA-081) 		zp = 1110+021
−034[6]
or 134+06
−22[5] 		Galaxy Lyman-break galaxy discovered by JWST[5][6]
SMACS-z11a zp = 1105+009
−008[11]
or 173+018
−004[6] 		Galaxy Lyman-break galaxy discovered by JWST[6][11]
CR3-z12-1 zp = 1105+224
−047 		Galaxy Lyman-break galaxy discovered by JWST[9]
F150DA-026 zp = 110+05
−03 		Galaxy Lyman-break galaxy discovered by JWST[5]
F150DA-036 zp = 110+04
−78 		Galaxy Lyman-break galaxy discovered by JWST[5]
SMACS-z10e zp = 1089+016
−014[11]
or 138+137
−024[6] 		Galaxy Lyman-break galaxy discovered by JWST[6][11]
F150DB-040 zp = 108+03
−02 		Galaxy Lyman-break galaxy discovered by JWST[5]
EGS-14506 zp = 1071+034
−062 		Galaxy Lyman-break galaxy discovered by JWST[47]
MACS0647-JD zp = 106±03 Galaxy Gravitationally lensed into three images by a galaxy cluster; detected by JWST and Hubble[48][49]
GLASS-z10
(GLASS-1698)[43] 		z = 10.38 Galaxy Lyman-break galaxy discovered by JWST; tentative (4.4σ) ALMA detection of [O III] emission line only[50][51]
EGS-7860 zp = 1011+060
−082 		Galaxy Lyman-break galaxy discovered by JWST[47]
SPT0615-JD zp = 99+08
−06 		13.419[1] Galaxy [52]
A2744-JD zp≅9.8 13.412[1] Galaxy Galaxy is being magnified and lensed into three multiple images, geometrically supporting its redshift.[53][54]
MACS1149-JD1 zp≅9.6 13.398[1][55] Candidate galaxy or protogalaxy [56]
GRB 090429B zp≅9.4 13.383[1][57] Chớp gamma [58] The photometric redshift in this instance has quite large uncertainty, with the lower limit for the redshift being z>7.
UDFy-33436598 zp≅8.6 13.317[1] Candidate galaxy or protogalaxy [59]
UDFy-38135539 zp≅8.6 13.317[1] Candidate galaxy or protogalaxy A spectroscopic redshift of z = 8.55 was claimed for this source in 2010,[60] but has subsequently been shown to be mistaken.[61]
BoRG-58 zp≅8 13.258[1] Cụm thiên hà hoặc protocluster Protocluster candidate[62]

§ The tabulated distance is the light travel distance, which has no direct physical significance. See discussion at distance measures and Observable Universe

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  1. ^ a b c d e f g h i j k l m n o p q r s t u v w x y z aa ab ac ad ae af ag ah ai aj ak al am an ao ap aq ar as at au av aw ax ay az ba bb bc bd be bf bg bh bi bj bk bl bm bn bo bp bq br bs bt bu bv bw bx by bz ca cb cc cd ce cf cg ch ci cj ck cl cm cn co cp cq cr cs ct cu cv cw cx cy cz da db dc dd de df dg dh di Staff (2015). “UCLA Cosmological Calculator”. UCLA. Truy cập ngày 6 tháng 8 năm 2022. Light travel distance was calculated from redshift value using the UCLA Cosmological Calculator, with parameters values as of 2015: H0=67.74 and OmegaM=0.3089 (see Table/Planck2015 at "Lambda-CDM model#Parameters" )
  2. ^ a b c d e f g h i j k l m n o p q r s t u v w x y z aa ab ac ad ae af ag ah ai aj ak al am an ao ap aq ar as at au av aw ax ay az ba bb bc bd be bf bg bh bi bj bk bl bm bn bo bp bq br bs bt bu bv bw bx by bz ca cb cc cd ce cf cg ch ci cj ck cl cm cn co cp cq cr cs ct cu cv cw cx cy cz Staff (2018). “UCLA Cosmological Calculator”. UCLA. Truy cập ngày 6 tháng 8 năm 2022. Light travel distance was calculated from redshift value using the UCLA Cosmological Calculator, with parameters values as of 2018: H0=67.4 and OmegaM=0.315 (see Table/Planck2018 at "Lambda-CDM model#Parameters" )
  3. ^ a b c d e f g h i j k l m n o p q r s t u v w x y z aa ab ac ad ae af ag ah ai aj ak al am an ao ap aq ar as at au av aw ax ay az ba bb bc bd be bf bg bh bi bj bk bl bm bn bo bp bq br bs bt bu bv bw bx by bz ca cb cc cd ce cf cg ch ci cj ck cl cm cn co cp cq cr cs ct cu cv cw cx cy cz Staff (2022). “ICRAR Cosmology Calculator”. International Centre for Radio Astronomy Research. Truy cập ngày 6 tháng 8 năm 2022. ICRAR Cosmology Calculator - Set H0=67.4 and OmegaM=0.315 (see Table/Planck2018 at "Lambda-CDM model#Parameters")
  4. ^ a b c d e f g h i j k l m n o p q r s t u v w x y z aa ab ac ad ae af ag ah ai aj ak al am an ao ap aq ar as at au av aw ax ay az ba bb bc bd be bf bg bh bi bj bk bl bm bn bo bp bq br bs bt bu bv bw bx by bz ca cb cc cd ce cf cg ch ci cj ck cl cm cn co cp cq cr cs ct cu cv cw cx cy cz Kempner, Joshua (2022). “KEMPNER Cosmology Calculator”. Kempner.net. Truy cập ngày 6 tháng 8 năm 2022. KEMP Cosmology Calculator - Set H0=67.4, OmegaM=0.315, and OmegaΛ=0.6847 (see Table/Planck2018 at "Lambda-CDM model#Parameters")
  5. ^ a b c d e f g h i j k l m n o p q r s t u v w x y z aa ab ac ad ae af ag ah ai aj ak al am an ao ap aq ar as at au av aw ax ay az ba bb bc bd be bf bg bh bi bj bk bl Lỗi chú thích: Thẻ <ref> sai; không có nội dung trong thẻ ref có tên Yan2023
  6. ^ a b c d e f g h i j k l m n o p q r s t u v w x y z aa ab ac ad ae af ag ah ai aj ak al am an Adams, N. J.; và đồng nghiệp (tháng 11 năm 2022). “Discovery and properties of ultra-high redshift galaxies (9 < z < 12) in the JWST ERO SMACS 0723 Field”. Monthly Notices of the Royal Astronomical Society. 518 (3): 4755–4766. arXiv:2207.11217. Bibcode:2023MNRAS.518.4755A. doi:10.1093/mnras/stac3347. Lỗi chú thích: Thẻ <ref> không hợp lệ: tên “Adams2022” được định rõ nhiều lần, mỗi lần có nội dung khác
  7. ^ a b c d Morishita, Takahiro; Stiavelli, Massimo (2023). “Physical Characterization of Early Galaxies in the Webb's First Deep Field SMACS J0723.3-7323”. The Astrophysical Journal Letters. 946 (2): L35. arXiv:2207.11671v2. Bibcode:2023ApJ...946L..35M. doi:10.3847/2041-8213/acbf50. S2CID 254220684. Lỗi chú thích: Thẻ <ref> không hợp lệ: tên “MorishitaStiavelli2022” được định rõ nhiều lần, mỗi lần có nội dung khác
  8. ^ a b Harikane, Yuichi; Ouchi, Masami; Oguri, Masamune; Ono, Yoshiaki; Nakajima, Kimihiko; Isobe, Yuki; Umeda, Hiroya; Mawatari, Ken; Zhang, Yechi (2023). “A Comprehensive Study of Galaxies at z ~ 9–16 Found in the Early JWST Data: Ultraviolet Luminosity Functions and Cosmic Star Formation History at the Pre-reionization Epoch”. The Astrophysical Journal Supplement Series. 265 (1): 5. arXiv:2208.01612v3. Bibcode:2023ApJS..265....5H. doi:10.3847/1538-4365/acaaa9. S2CID 251253150. Lỗi chú thích: Thẻ <ref> không hợp lệ: tên “ARX-20221209” được định rõ nhiều lần, mỗi lần có nội dung khác
  9. ^ a b c d e f g h i j Harikane, Yuichi; và đồng nghiệp (2023). “A Comprehensive Study of Galaxies at z ∼ 9–16 Found in the Early JWST Data: Ultraviolet Luminosity Functions and Cosmic Star Formation History at the Pre-reionization Epoch”. The Astrophysical Journal Supplement Series. 265 (1): 5. arXiv:2208.01612. Bibcode:2023ApJS..265....5H. doi:10.3847/1538-4365/acaaa9. S2CID 251253150.
  10. ^ a b Fujimoto, Seiji (November 2022). "ALMA FIR View of Ultra High-redshift Galaxy Candidates at z ~ 11-17: Blue Monsters hoặc Low- z Red Interlopers?". arΧiv:2211.03896 [astro-ph.GA].  Lỗi chú thích: Thẻ <ref> không hợp lệ: tên “Fujimoto2022” được định rõ nhiều lần, mỗi lần có nội dung khác
  11. ^ a b c d e f g h i j k l m n o Hakim, Atek; và đồng nghiệp (tháng 11 năm 2022). “Revealing galaxy candidates out to z 16 with JWST observations of the lensing cluster SMACS0723”. Monthly Notices of the Royal Astronomical Society. 519 (1): 1201–1220. arXiv:2207.12338. Bibcode:2023MNRAS.519.1201A. doi:10.1093/mnras/stac3144. Lỗi chú thích: Thẻ <ref> không hợp lệ: tên “Hakim2022” được định rõ nhiều lần, mỗi lần có nội dung khác
  12. ^ Harikane, Y.; và đồng nghiệp (tháng 4 năm 2022). “A Search for H-Dropout Lyman Break Galaxies at z ∼ 12–16”. The Astrophysical Journal. 929 (1): 1. arXiv:2112.09141. Bibcode:2022ApJ...929....1H. doi:10.3847/1538-4357/ac53a9. S2CID 246823511.Quản lý CS1: ngày tháng và năm (liên kết)
  13. ^ a b c d Robertson, B. E.; và đồng nghiệp (2023). “Identification and properties of intense star-forming galaxies at redshifts z > 10”. Nature Astronomy. 7 (5): 611–621. arXiv:2212.04480. Bibcode:2023NatAs...7..611R. doi:10.1038/s41550-023-01921-1. S2CID 257968812.
  14. ^ Bakx, Tom J. L. C.; và đồng nghiệp (tháng 1 năm 2023). “Deep ALMA redshift search of a z~12 GLASS-JWST galaxy candidate”. Monthly Notices of the Royal Astronomical Society. 519 (4): 5076–5085. arXiv:2208.13642. doi:10.1093/mnras/stac3723.
  15. ^ Oesch, P. A.; Brammer, G.; van Dokkum, P.; và đồng nghiệp (tháng 3 năm 2016). “A Remarkably Luminous Galaxy at z=11.1 Measured with Hubble Space Telescope Grism Spectroscopy”. The Astrophysical Journal. 819 (2). 129. arXiv:1603.00461. Bibcode:2016ApJ...819..129O. doi:10.3847/0004-637X/819/2/129. S2CID 119262750.
  16. ^ Jiang, Linhua; và đồng nghiệp (tháng 1 năm 2021). “Evidence for GN-z11 as a luminous galaxy at redshift 10.957”. Nature Astronomy. 5 (3): 256–261. arXiv:2012.06936. Bibcode:2021NatAs...5..256J. doi:10.1038/s41550-020-01275-y. S2CID 229156468.
  17. ^ Roberts-Borsani, Guido; Treu, Tommaso; Chen, Wenlei; Morishita, Takahiro; Vanzella, Eros; Zitrin, Adi; Bergamini, Pietro; Castellano, Marco; Fontana, Adriano (2022-10-27). "A shot in the Dark (Ages): a faint galaxy at $z=9.76$ confirmed with JWST". arΧiv:2210.15639 [astro-ph.GA]. 
  18. ^ T. Hashimoto, N. Laporte, K. Mawatari, R. S. Ellis, A. K. Inoue, E. Zackrisson, G. Roberts-Borsani, W. Zheng, Y. Tamura, F. E. Bauer, T. Fletcher, Y. Harikane, B. Hatsukade, N. H. Hayatsu, Y. Matsuda, H. Matsuo, T. Okamoto, M. Ouchi, R. Pello, C. Rydberg, I. Shimizu, Y. Taniguchi, H. Umehata, N. Yoshida (2019). “The Onset of Star Formation 250 Million Years After the Big Bang”. Nature. 557 (7705): 312–313. arXiv:1805.05966. Bibcode:2018Natur.557..392H. doi:10.1038/s41586-018-0117-z. PMID 29765123. S2CID 21702406.Quản lý CS1: sử dụng tham số tác giả (liên kết)
  19. ^ Adi Zitrin, Ivo Labbe, Sirio Belli, Rychard Bouwens, Richard S. Ellis, Guido Roberts-Borsani, Daniel P. Stark, Pascal A. Oesch, Renske Smit (2015). “Lyman-alpha Emission from a Luminous z = 8.68 Galaxy: Implications for Galaxies as Tracers of Cosmic Reionization”. The Astrophysical Journal. 810 (1): L12. arXiv:1507.02679. Bibcode:2015ApJ...810L..12Z. doi:10.1088/2041-8205/810/1/L12. S2CID 11524667.Quản lý CS1: sử dụng tham số tác giả (liên kết)
  20. ^ a b c Curti, Mirko; và đồng nghiệp (tháng 1 năm 2023). “The chemical enrichment in the early Universe as probed by JWST via direct metallicity measurements at z 8”. Monthly Notices of the Royal Astronomical Society. 518 (1): 425–438. arXiv:2207.12375. Bibcode:2023MNRAS.518..425C. doi:10.1093/mnras/stac2737.
  21. ^ a b c Carnall, A. C.; và đồng nghiệp (tháng 1 năm 2023). “A first look at the SMACS0723 JWST ERO: spectroscopic redshifts, stellar masses, and star-formation histories”. Monthly Notices of the Royal Astronomical Society: Letters. 518 (1): L45–L50. arXiv:2207.08778. Bibcode:2023MNRAS.518L..45C. doi:10.1093/mnrasl/slac136.
  22. ^ a b c Schaerer, D.; và đồng nghiệp (tháng 9 năm 2022). “First look with JWST spectroscopy: Resemblance among z ∼ 8 galaxies and local analogs”. Astronomy & Astrophysics. 665: 6. arXiv:2207.10034. Bibcode:2022A&A...665L...4S. doi:10.1051/0004-6361/202244556. S2CID 252175886. L4.
  23. ^ a b c Katz, Harley; và đồng nghiệp (tháng 1 năm 2023). “AFirst insights into the ISM at z > 8 with JWST: possible physical implications of a high [O III] λ4363/[O III] λ5007”. Monthly Notices of the Royal Astronomical Society. 518 (1): 592–603. arXiv:2207.13693. Bibcode:2023MNRAS.518..592K. doi:10.1093/mnras/stac2657.
  24. ^ Laporte, N.; Ellis, R. S.; Boone, F.; Bauer, F. E.; Quénard, D.; Roberts-Borsani, G. W.; Pelló, R.; Pérez-Fournon, I.; Streblyanska, A. (2017). “Dust in the Reionization Era: ALMA Observations of a z = 8.38 Gravitationally Lensed Galaxy”. The Astrophysical Journal. 832 (2): L21. arXiv:1703.02039. Bibcode:2017ApJ...837L..21L. doi:10.3847/2041-8213/aa62aa. S2CID 51841290.
  25. ^ Tamura, Y.; Mawatari, K.; Hashimoto, T.; Inoue, A. K.; Zackrisson, E.; Christensen, L.; Binggeli, C; Matsuda, Y.; Matsuo, H.; Takeuchi, T. T.; Asano, R. S.; Sunaga, K.; Shimizu, I.; Okamoto, T.; Yoshida, N.; Lee, M.; Shibuya, T.; Taniguchi, Y.; Umehata, H.; Hatsukade, B.; Kohno, K.; Ota, K. (2017). “Detection of the Far-infrared [O III] and Dust Emission in a Galaxy at Redshift 8.312: Early Metal Enrichment in the Heart of the Reionization Era”. The Astrophysical Journal. 874 (1): 27. arXiv:1806.04132. Bibcode:2019ApJ...874...27T. doi:10.3847/1538-4357/ab0374. S2CID 55313459.
  26. ^ Tanvir, N. R.; Fox, D. B.; Levan, A. J.; Berger, E.; Wiersema, K.; Fynbo, J. P. U.; Cucchiara, A.; Krühler, T.; Gehrels, N.; Bloom, J. S.; Greiner, J.; Evans, P. A.; Rol, E.; Olivares, F.; Hjorth, J.; Jakobsson, P.; Farihi, J.; Willingale, R.; Starling, R. L. C.; Cenko, S. B.; Perley, D.; Maund, J. R.; Duke, J.; Wijers, R. A. M. J.; Adamson, A. J.; Allan, A.; Bremer, M. N.; Burrows, D. N.; Castro-Tirado, A. J.; và đồng nghiệp (2009). “A gamma-ray burst at a redshift of z~8.2”. Nature. 461 (7268): 1254–7. arXiv:0906.1577. Bibcode:2009Natur.461.1254T. doi:10.1038/nature08459. PMID 19865165. S2CID 205218350.
  27. ^ a b Langeroodi, Danial; Hjorth, Jens; Chen, Wenlei; Kelly, Patrick L.; Williams, Hayley; Lin, Yu-Heng; Scarlata, Claudia; Zitrin, Adi; Broadhurst, Tom; Diego, Jose M.; Huang, Xiaosheng; Filippenko, Alexei V.; Foley, Ryan J.; Jha, Saurabh; Koekemoer, Anton M.; Oguri, Masamune; Perez-Fournon, Ismael; Pierel, Justin; Poidevin, Frederick; Strolger, Lou (2022). “Evolution of the Mass-Metallicity Relation from Redshift z≈8 to the Local Universe”. The Astrophysical Journal. 804 (2). arXiv:2212.02491. Bibcode:2015ApJ...804L..30O. doi:10.1088/2041-8205/804/2/L30. S2CID 55115344.
  28. ^ P. A. Oesch, P. G. van Dokkum, G. D. Illingworth, R. J. Bouwens, I. Momcheva, B. Holden, G. W. Roberts-Borsani, R. Smit, M. Franx, I. Labbe, V. Gonzalez, D. Magee (2015). “A Spectroscopic Redshift Measurement for a Luminous Lyman Break Galaxy at z = 7.730 using Keck/MOSFIRE”. The Astrophysical Journal. 804 (2): L30. arXiv:1502.05399. Bibcode:2015ApJ...804L..30O. doi:10.1088/2041-8205/804/2/L30. S2CID 55115344.Quản lý CS1: sử dụng tham số tác giả (liên kết)
  29. ^ Song, M.; Finkelstein, S. L.; Livermore, R. C.; Capak, P. L.; Dickinson, M.; Fontana, A. (2016). “Keck/MOSFIRE Spectroscopy of z = 7–8 Galaxies: Lyman-alpha Emission from a Galaxy at z = 7.66”. The Astrophysical Journal. 826 (2): 113. arXiv:1602.02160. Bibcode:2016ApJ...826..113S. doi:10.3847/0004-637X/826/2/113. S2CID 51806693.
  30. ^ Wang, Feige; Yang, Jinyi; Fan, Xiaohui; Hennawi, Joseph F.; Barth, Aaron J.; Banados, Eduardo; Bian, Fuyan; Boutsia, Konstantina; Connor, Thomas; Davies, Frederick B.; Decarli, Roberto; Eilers, Anna-Christina; Farina, Emanuele Paolo; Green, Richard; Jiang, Linhua; Li, Jiang-Tao; Mazzucchelli, Chiara; Nanni, Riccardo; Schindler, Jan-Torge; Venemans, Bram; Walter, Fabian; Wu, Xue-Bing; Yue, Minghao (2021). “A Luminous Quasar at Redshift 7.642”. The Astrophysical Journal. 907 (1): L1. arXiv:2101.03179. Bibcode:2021ApJ...907L...1W. doi:10.3847/2041-8213/abd8c6. S2CID 231572944.
  31. ^ Bañados, Eduardo; và đồng nghiệp (6 tháng 12 năm 2017). “An 800-million-solar-mass black hole in a significantly neutral Universe at a redshift of 7.5”. Nature. 553 (7689): 473–476. arXiv:1712.01860. Bibcode:2018Natur.553..473B. doi:10.1038/nature25180. PMID 29211709. S2CID 205263326.
  32. ^ S. L. Finkelstein, C. Papovich, M. Dickinson, M. Song, V. Tilvi, A. M. Koekemoer, K. D. Finkelstein, B. Mobasher, H. C. Ferguson, M. Giavalisco, N. Reddy, M. L. N. Ashby, A. Dekel, G. G. Fazio, A. Fontana, N. A. Grogin, J.-S. Huang, D. Kocevski, M. Rafelski, B. J. Weiner, S. P. Willner (2013). “A galaxy rapidly forming stars 700 million years after the Big Bang at redshift 7.51”. Nature. 502 (7472): 524–527. arXiv:1310.6031. Bibcode:2013Natur.502..524F. doi:10.1038/nature12657. PMID 24153304. S2CID 4448085.Quản lý CS1: sử dụng tham số tác giả (liên kết)
  33. ^ Watson, Darach; Christensen, Lise; Knudsen, Kirsten Kraiberg; Richard, Johan; Gallazzi, Anna; Michałowski, Michał Jerzy (2015). “A dusty, normal galaxy in the epoch of reionization”. Nature. 519 (7543): 327–330. arXiv:1503.00002. Bibcode:2015Natur.519..327W. doi:10.1038/nature14164. PMID 25731171. S2CID 2514879.
  34. ^ Larson, R. L.; Finkelstein, S. L.; Pirzkal, N.; Ryan, R.; Tilvi, V.; Malhotra, S.; Rhoads, J.; Finkelstein, K.; Jung, I.; Christensen, L.; Cimatti, A.; Ferreras, I.; Grogin, N.; Koekemoer, A. M.; Hathi, N.; O'Connell, R.; Östlin, G.; Pasquali, A.; Pharo, J.; Rothberg, B.; Windhorst, R. A. (2018). “Discovery of a z = 7.452 High Equivalent Width Lyman alpha Emitter from the Hubble Space Telescope Faint Infrared Grism Survey”. The Astrophysical Journal. 858 (2): 113. arXiv:1712.05807. Bibcode:2018ApJ...858...94L. doi:10.3847/1538-4357/aab893. S2CID 119257857.
  35. ^ a b c 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 (2011). “Spectroscopic Confirmation of Three z-Dropout Galaxies at z = 6.844 – 7.213: Demographics of Lyman-Alpha Emission in z ~ 7 Galaxies”. The Astrophysical Journal. 744 (2): 83. arXiv:1107.3159. Bibcode:2012ApJ...744...83O. doi:10.1088/0004-637X/744/2/83. S2CID 119306980.
  36. ^ Inoue, Akio K.; và đồng nghiệp (tháng 6 năm 2016). “Detection of an oxygen emission line from a high redshift galaxy in the reionization epoch” (PDF). Science. 352 (6293): 1559–1562. arXiv:1606.04989. Bibcode:2016Sci...352.1559I. doi:10.1126/science.aaf0714. PMID 27312046. S2CID 206646433.
  37. ^ a b Vanzella; và đồng nghiệp (2011). “Spectroscopic Confirmation of Two Lyman Break Galaxies at Redshift Beyond 7”. The Astrophysical Journal Letters. 730 (2): L35. arXiv:1011.5500. Bibcode:2011ApJ...730L..35V. doi:10.1088/2041-8205/730/2/L35. S2CID 53459241.
  38. ^ Daniel J. Mortlock; Stephen J. Warren; Bram P. Venemans; và đồng nghiệp (2011). “A luminous quasar at a redshift of z = 7.085”. Nature. 474 (7353): 616–619. arXiv:1106.6088. Bibcode:2011Natur.474..616M. doi:10.1038/nature10159. PMID 21720366. S2CID 2144362.
  39. ^ Schenker, Matthew A.; và đồng nghiệp (tháng 1 năm 2012). “Keck Spectroscopy of Faint 3 < z < 8 Lyman Break Galaxies: Evidence for a Declining Fraction of Emission Line Sources in the Redshift Range 6 < z < 8”. The Astrophysical Journal. 744 (2): 7. arXiv:1107.1261. Bibcode:2012ApJ...744..179S. doi:10.1088/0004-637X/744/2/179. S2CID 119244384.
  40. ^ Fontana, A.; Vanzella, E.; Pentericci, L.; Castellano, M.; Giavalisco, M.; Grazian, A.; Boutsia, K.; Cristiani, S.; Dickinson, M.; Giallongo, E.; Maiolino, M.; Moorwood, A.; Santini, P. (2010). “The lack of intense Lyman~alpha in ultradeep spectra of z = 7 candidates in GOODS-S: Imprint of reionization?”. The Astrophysical Journal. 725 (2): L205. arXiv:1010.2754. Bibcode:2010ApJ...725L.205F. doi:10.1088/2041-8205/725/2/L205. S2CID 119270473.
  41. ^ Rhoads, James E.; Hibon, Pascale; Malhotra, Sangeeta; Cooper, Michael; Weiner, Benjamin (2012). “A Lyman Alpha Galaxy at Redshift z = 6.944 in the COSMOS Field”. The Astrophysical Journal. 752 (2): L28. arXiv:1205.3161. Bibcode:2012ApJ...752L..28R. doi:10.1088/2041-8205/752/2/L28. S2CID 118383532.
  42. ^ Bañados, Eduardo; Mazzucchelli, Chiara; Momjian, Emmanuel; Eilers, Anna-Christina; Wang, Feige; Schindler, Jan-Torge; Connor, Thomas; Andika, Irham Taufik; Barth, Aaron J.; Carilli, Chris; Davies, Frederick B.; Decarli, Roberto; Fan, Xiaohui; Farina, Emanuele Paolo; Hennawi, Joseph F.; Pensabene, Antonio; Stern, Daniel; Venemans, Bram P.; Wenzl, Lukas; Yang, Jinyi (2021). “The Discovery of a Highly Accreting, Radio-loud Quasar at z = 6.82”. The Astrophysical Journal. Harvard University. 909 (1): 80. arXiv:2103.03295. Bibcode:2021ApJ...909...80B. doi:10.3847/1538-4357/abe239. S2CID 232135300. Truy cập ngày 26 tháng 3 năm 2021.
  43. ^ a b c d e f g h i j k l m n o Donnan, C. T.; và đồng nghiệp (tháng 11 năm 2022). “The evolution of the galaxy UV luminosity function at redshifts z ≃ 8 - 15 from deep JWST and ground-based near-infrared imaging”. Monthly Notices of the Royal Astronomical Society. 518 (4): 6011–6040. arXiv:2207.12356. Bibcode:2023MNRAS.518.6011D. doi:10.1093/mnras/stac3472.
  44. ^ a b c Bouwens, Rychard J.; và đồng nghiệp (2023). “Evolution of the UV LF from z ∼ 15 to z ∼ 8 using new JWST NIRCam medium-band observations over the HUDF/XDF”. Monthly Notices of the Royal Astronomical Society. 523: 1036–1055. arXiv:2211.02607. doi:10.1093/mnras/stad1145.
  45. ^ Rodighiero, Giulia; và đồng nghiệp (tháng 1 năm 2023). “JWST unveils heavily obscured (active and passive) sources up to z 13”. Monthly Notices of the Royal Astronomical Society: Letters. 518 (1): L19–L24. arXiv:2208.02825. Bibcode:2023MNRAS.518L..19R. doi:10.1093/mnrasl/slac115.
  46. ^ Finkelstein, Steven L.; và đồng nghiệp (tháng 12 năm 2022). “A Long Time Ago in a Galaxy Far, Far Away: A Candidate z ∼ 12 Galaxy in Early JWST CEERS Imaging”. The Astrophysical Journal Letters. 940 (2): 15. arXiv:2207.12474. Bibcode:2022ApJ...940L..55F. doi:10.3847/2041-8213/ac966e. S2CID 251066925. L55.
  47. ^ a b Whitler, Lily; và đồng nghiệp (tháng 12 năm 2022). “On the ages of bright galaxies 500 Myr after the Big Bang: insights into star formation activity at z ≳ 15 with JWST”. Monthly Notices of the Royal Astronomical Society. 519 (1): 157–171. arXiv:2208.01599. Bibcode:2023MNRAS.519..157W. doi:10.1093/mnras/stac3535.
  48. ^ 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 (1): 32. arXiv:1211.3663. Bibcode:2013ApJ...762...32C. doi:10.1088/0004-637x/762/1/32. S2CID 119114237.
  49. ^ Hsiao, Tiger Yu-Yang; và đồng nghiệp (2023). “JWST Reveals a Possible z ∼ 11 Galaxy Merger in Triply Lensed MACS0647–JD”. The Astrophysical Journal Letters. 949 (2): L34. arXiv:2210.14123. Bibcode:2023ApJ...949L..34H. doi:10.3847/2041-8213/acc94b. S2CID 253107903.
  50. ^ Naidu, Rohan P.; và đồng nghiệp (tháng 11 năm 2022). “Two Remarkably Luminous Galaxy Candidates at z ≈ 10 − 12 Revealed by JWST”. The Astrophysical Journal Letters. 940 (1): 11. arXiv:2207.09434. Bibcode:2022ApJ...940L..14N. doi:10.3847/2041-8213/ac9b22. S2CID 250644267. L14.
  51. ^ Yoon, Ilsang (October 2022). "ALMA Observation of a z≳10 Galaxy Candidate Discovered with JWST". arΧiv:2210.08413 [astro-ph.GA]. 
  52. ^ Salmon, Brett; Coe, Dan; Bradley, Larry; Bradač, Marusa; Huang, Kuang-Han; Strait, Victoria; Oesch, Pascal; Paterno-Mahler, Rachel; Zitrin, Adi; Acebron, Ana; Cibirka, Nathália; Kikuchihara, Shotaro; Oguri, Masamune; Brammer, Gabriel B; Sharon, Keren; Trenti, Michele; Avila, Roberto J; Ogaz, Sara; Andrade-Santos, Felipe; Carrasco, Daniela; Cerny, Catherine; Dawson, William; Frye, Brenda L; Hoag, Austin; Jones, Christine; Mainali, Ramesh; Ouchi, Masami; Rodney, Steven A; Stark, Daniel; Umetsu, Keiichi (2018). “A Candidate z∼10 Galaxy Strongly Lensed into a Spatially Resolved Arc”. The Astrophysical Journal. 864: L22. arXiv:1801.03103. doi:10.3847/2041-8213/aadc10. S2CID 78087820.
  53. ^ “Hubble Finds Distant Galaxy Through Cosmic Magnifying Glass”. NASA. 23 tháng 4 năm 2015.
  54. ^ Zitrin, Adi; Zheng, Wei; Broadhurst, Tom; Moustakas, John; Lam, Daniel; Shu, Xinwen; Huang, Xingxing; Diego, Jose M.; Ford, Holland; Lim, Jeremy; Bauer, Franz E.; Infante, Leopoldo; Kelson, Daniel D.; Molino, Alberto (2014). “A Geometrically Supported z ∼ 10 Candidate Multiply Imaged by the Hubble Frontier Fields Cluster A2744” (PDF). The Astrophysical Journal. 793 (1): L12. arXiv:1407.3769. Bibcode:2014ApJ...793L..12Z. doi:10.1088/2041-8205/793/1/L12. S2CID 43853349.
  55. ^ “NASA Telescopes Spy Ultra-Distant Galaxy”. NASA.
  56. ^ Zheng, W.; Postman, M.; Zitrin, A.; Moustakas, J.; Shu, X.; Jouvel, S.; Høst, O.; Molino, A.; Bradley, L.; Coe, D.; Moustakas, L. A.; Carrasco, M.; Ford, H.; Benítez, N.; Lauer, T. R.; Seitz, S.; Bouwens, R.; Koekemoer, A.; Medezinski, E.; Bartelmann, M.; Broadhurst, T.; Donahue, M.; Grillo, C.; Infante, L.; Jha, S. W.; Kelson, D. D.; Lahav, O.; Lemze, D.; Melchior, P.; Meneghetti, M. (2012). “A magnified young galaxy from about 500 million years after the Big Bang”. Nature. 489 (7416): 406–408. arXiv:1204.2305. Bibcode:2012Natur.489..406Z. doi:10.1038/nature11446. PMID 22996554. S2CID 4415218.
  57. ^ Penn State Science, "Cosmic Explosion is New Candidate for Most Distant Object in the Universe", Derek. B. Fox , Barbara K. Kennedy , 25 May 2011
  58. ^ Space Daily, Explosion Helps Researcher Spot Universe's Most Distant Object, 27 May 2011
  59. ^ “ESA Science & Technology: The Hubble eXtreme Deep Field (annotated)”.
  60. ^ David Shiga. “Dim galaxy is most distant object yet found”. New Scientist.
  61. ^ Bunker, Andrew J.; Caruana, Joseph; Wilkins, Stephen M.; Stanway, Elizabeth R.; Lorenzoni, Silvio; Lacy, Mark; Jarvis, Matt J.; Hickey, Samantha (2013). “VLT/XSHOOTER and Subaru/MOIRCS spectroscopy of HUDF.YD3: no evidence for Lyman &”. Monthly Notices of the Royal Astronomical Society. 430 (4): 3314. arXiv:1301.4477. Bibcode:2013MNRAS.430.3314B. doi:10.1093/mnras/stt132.
  62. ^ Trenti, M.; Bradley, L. D.; Stiavelli, M.; Shull, J. M.; Oesch, P.; Bouwens, R. J.; Munoz, J. A.; Romano-Diaz, E.; Treu, T.; Shlosman, I.; Carollo, C. M. (2011). “Overdensities of Y-dropout Galaxies from the Brightest-of-Reionizing Galaxies Survey: A Candidate Protocluster at Redshift z ≈ 8”. The Astrophysical Journal. 746 (1): 55. arXiv:1110.0468. Bibcode:2012ApJ...746...55T. doi:10.1088/0004-637X/746/1/55. S2CID 119294290.

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