㻲㼕㼎㼑㼞㼛㼜㼠㼕㼏㻌㻿㼜㼑㼏㼠㼞㼛㼙㼑㼠㼑㼞ἰἽἓἋἬἁἚἽЎή֥ἉἋἘἲ

㻌㻭㼢㼍㼚㼠㼑㼟♫䠄䜸䝷䞁䝎䠅䛿ᑠᆺ㧗ᛶ⬟䝣䜯䜲䝞䞊ධᑕᆺศගჾ䜢㛤Ⓨ䛧䛶㻞㻡ᖺ௨ୖ⤒䛱䚸䛥䜙䛻㐍໬䛧䛯㧗ᛶ⬟ᆺ䚸㉸ᑠᆺ㧗ศゎ⬟ᆺ➼䚸ḟୡ௦䛻ᑐᛂ䛩䜛㐍໬ᆺศගჾ䜢㛤Ⓨ䛧⥆䛡䛶䛔䜎䛩䚹㻌᪂㛤Ⓨ䛾䜶䝺䜽䝖䝻䝙䜽䝇䝪䞊䝗㻔㻭㻿㻙㻣㻜㻝㻜㻕䛻䜘䜚䚸㼁㻿㻮㻟㻚㻜㉸㧗㏿㏻ಙ䞉䜼䜺䝡䝑䝖㻱㼠㼔㼑㼞㼚㼑㼠ఏ㏦➼䛜ᐇ⌧䛧䚸௒ᚋ䛣䛾㻱㼂㻻䝅䝸䞊䝈䛜୰ᚰ䛸䛺䜚䜎䛩䚹᭱᪂䛾㻯㻹㻻㻿ᢏ⾡䜢㥑౑䛧䛯㻯㻹㻻㻿䝕䜱䝔䜽䝍䜢᥇⏝䛧䚸㻱㼂㻻䝅䝸䞊䝈䛸⤌䜏ྜ䜟䛫䛯㻯㻹㻻㻿ไᚚ䞉㉸㧗㏿ศගჾ䛜Ⓩሙ䛧䚸㻱㼂㻻䛸㻯㻹㻻㻿䛜୺ὶ䛸䛺䜚䜎䛧䛯䚹䜎䛯㉸ᑠᆺ㏆㉥እศගჾ䛜㛤Ⓨ䛥䜜䚸㧗ᛶ⬟䛺䝁䞁䝟䜽䝖ᆺ䜒ὀ┠䛥䜜䚸᭦䛻㉸㧗㏿䝬䝹䝏䝏䝱䞁䝛䝹ศගჾ䠄㻨㻝㻜㼏㼔㻕㻌䛿⏘ᴗ⏝䝥䝻䝉䝇䝁䞁䝖䝻䞊䝹➼䛾ᗈᖏᇦ䜔ከゅⓗ䛺ィ 䛾䝙䞊䝈䛻᭷ຠ䛷䛩䚹䛴䜎䜚㻭㼢㼍㻿㼜㼑㼏䛿ྛ✀䛾䜰䝥䝸䜿䞊䝅䝵䞁䛻ᑐᛂ䛷䛝䜛䝬䝹䝏䝇䝨䜽䝖䝹ศගჾ䝅䝇䝔䝮䛺䛾䛷䛩䚹䚷䚷㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌඲䛶䛾ศගჾᮏయ䛻ᶆ‽䝋䝣䝖䛜௜ᒓ䛩䜛௚䚸⏝㏵䛻ᛂ䛨䛯䜰䝥䝸䜿䞊䝅䝵䞁ᑓ⏝䝋䝣䝖➼䜢ྲྀ䜚ᥞ䛘䛶䛔䜎䛩䚹䜎䛯㇏ᐩ䛺ᰯṇ⏝ග※䜔䝣䜯䜲䝞䞊䚸䜰䜽䝉䝃䝸䞊䛿໚ㄽ䛾䛣䛸䚸䜹䝇䝍䝮཯ᑕ䝥䝻䞊䝥➼䛾≉ὀ䜒୍ᮏ䛛䜙ᢎ䜚᭱㐺䛺 ᐃ䝅䝇䝔䝮䜢ᵓᡂ䛩䜛䛣䛸䛜ྍ⬟䛷䛩䚹㻭㼢㼍㻿㼜㼑㼏 䝣䜯䜲䝞䞊ධᑕᆺศගჾ

᪂㛤Ⓨ 䞉 ḟୡ௦㐍໬ᆺ

3.0 ㉸㧗㏿ 㻛㻝㻳㼎㼜㼟㻱㼀㻴 㻱㼂㻻 䝅䝸䞊䝈 㧗ឤᗘ 䞉 㧗Ἴ㛗ศゎ⬟ 䞉 㧗㏿ᛂ⟅ 䞉 ప䝜䜲䝈3᭱᪂䛾㧗ᛶ⬟ 㻯㻹㻻㻿 䝕䜱䝔䜽䝍䞊᭱ᵟᶔᵿᵱᶎᶃᶁᴾᵱᶃᶌᶑᵪᶇᶌᶃ

ᵟᶔᵿᵱᶎᶃᶁᴾᵱᶒᵿᶐᵪᶇᶌᶃ

䝴䞊䝄䞊䛾䝸䜽䜶䝇䝖䛻ᛂ䛘䜛ᙧ䛷๰䜙䜜䛯ศගჾ䛷䚸 ⺯ගィ 䚸 䝹䝭䝛䝑䝉䞁䝇ィ 䚸䝷䝬䞁ィ ➼䚸 ㏻ᖖ䜘䜚㧗䛔䝟䝣䜷䞊䝬䞁䝇䜢せồ䛥䜜䜛䜰䝥䝸䜿䞊䝅䝵䞁䛻ᑐᛂ䚹䠖䖃Ἴ㛗ᇦ㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻞㻜㻜㻌㻙㻝㻝㻢㻜㼚㼙䠖䖃㏞ග㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻜㻚㻜㻠㻙㻝䠂䠖䖃㼁㼂 㔞Ꮚຠ⋡㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻢㻜䠂䠄㻞㻜㻜㻙㻟㻜㻜㼚㼙㻕䠖䖃㻿㻛㻺㻌ẚ㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌䚷㻌㻝㻞㻜㻜㻌㻦㻌㻝㻌㻔㻴㻱㻾㻻㻕䠖䖃᭱ᑠἼ㛗ศゎ⬟㻌㻌㻌䚷㻌㻌㻜㻚㻜㻢㻙㻞㻜㼚㼙㻌㻌$YD6SHF8/6;/(92$YD6SHF+6;/(92[[PPJ[[PPJ

[[PPNJᶆ‽୓⬟ᆺ䛧䛛䜒㧗Ἴ㛗ศゎ⬟䛜ᚓ䜙䜜䚸䜹䝷䞊 䞉 ཯ᑕ 䞉 Ⓨග 䞉 ⭷ཌ➼ྛ✀ィ 䛻ᑐᛂ䚹㻱㼂㻻㻗㻯㻹㻻㻿 ไᚚ䛾᭱᪂ᆺ䛿㧗㏿ከ䝏䝱䞁䝛䝹䝅䝇䝔䝮䛻䛶⏘ᴗ⏝䝥䝻䝉䝇ไᚚ䛻᭱㐺䚹᪂㛤Ⓨ䛾 㼀㻱㻯 ෭༷䝕䜱䝔䜽䝍䞊䛻䜘䜚䝜䜲䝈䛜㣕㌍ⓗ䛻๐ῶ䛧䚸 ග䛾ᑡ䛺䛔⎔ቃୗ䛷䛾ィ 䜔⺯ගィ 䚸 䝥䝷䝇䝏䝑䜽ᡂศศᯒ䚸ኴ㝧ගⓎ㟁⏝䝰䝙䝍䞊䛾Ⓨග ᐃ➼䛻ᑐᛂ䚹䠖䖃Ἴ㛗ᇦ㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻞㻜㻜㻙㻝㻝㻜㻜㼚㼙䠖䖃㏞ග㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻜㻚㻜㻠㻙㻝㻌䠂䠖䖃㻿㻛㻺 ẚ䚷䚷㻌㻌㻌㻌㻌㻌㻌㻌㻌䚷㻌㻌㻌㻌㻟㻜㻜㻌㻦㻌㻝䠖䖃᭱▷㟢ග᫬㛫㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻥䃛㼟㻌㻔㻠㻜㻥㻢㻯㻸㻙㻱㼂㻻㻕䠖䖃᭱ᑠἼ㛗ศゎ⬟㻌㻌㻌㻌㻌㻌㻌㻜㻚㻜㻡㻙㻞㻜㼚㼙㻌㻌䠖䖃Ἴ㛗ᇦ㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻥㻜㻜㻔㻝㻜㻜㻜㻕㻙㻞㻡㻜㻜㼚㼙䠖䖃㏞ග㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻨㻝㻌䠂䠖䖃㻿㻛㻺 ẚ 䠄㻸㻺㻕㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻡㻜㻜㻜㻌㻦㻌㻝䠖䖃᭱▷㟢ග᫬㛫㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻝㻜䃛㼟㻌㻌㻌䠖䖃䝎䜲䝘䝭䝑䜽䝺䞁䝆㻌㻌㻌㻌㻌㻥㻜㻜㻜㻌㻦㻌㻝㻌㻔㻝㻚㻣㻙㻱㼂㻻㻕

ࠉ$YD6SHF8/6&/(92[[PPJ$YD6SHF+(52 +6&[7(&(92ࠉ$YD6SHF8/6[(92[[PPJ

ࠉ$YD6SHF8/6&/(92[[PPJ$YD6SHF8/6[7(&(92 ᵬᵣᵵᵟᶔᵿᵱᶎᶃᶁᴾᵬᵧᵰᴾᵪᶇᶌᶃ$YD6SHF'XDO&KDQQHO[[PPNJ $YD6SHF)DVW[[PPJ$YD6SHF0XOWL&KDQQHOࠉ$YD6SHF1,5(92ᵬᵣᵵ

$YD6SHF0LQL1,5[[PPJ[[PPNJ$YD6SHF1,5+6&(92[[PPNJ

ࠉ$YD6SHF1,5+6&(92[[PPNJ

[[PPFK [[PPFK

ᵟᶔᵿᵱᶎᶃᶁᵋᵡᶍᶋᶎᵿᶁᶒᵪᶇᶌᶃ

ᵭᵣᵫᴾᵱᶎᶁᶒᶐᶍᶋᶃᶒᶃᶐᶑ

ᵟᶔᵿᵱᶎᶃᶁᵋᵰᵱᵆᵱᶊᶇᶒᴾᶉᶇᶒᵇගᏛ䝧䞁䝏䛿 㼁㼂㻛㼂㻵㻿 ⏝䚸 㻺㻵㻾 ⏝䛾ྛ✀ィ 䛻ᑐᛂ䚹 䝬䜲䜽䝻䝥䝻䝉䝑䝃䝪䞊䝗䛿ᐃ䛻ᛂ䛨䛶䝕䜱䝔䜽䝍䞊䜔䝋䝣䝖䜴䜵䜰䛸⤌ྜ䜟䛫䛶⮬ᅾ䛺౑⏝䛜ྍ⬟䚹ᐃ⏝㏵䛻ᛂ䛨䛶䝇䝸䝑䝖ᖜ䛾ኚ᭦䛜䛷䛝ṇ䛧䛔ィ 䛜ྍ⬟䛺✲ᴟ䛾ศගჾ䚹ឤᗘ䛸䝇䝹䞊䝥䝑䝖䛾䛹䛱䜙䜢ඃඛ䛩䜛䛛䜢䝇䝸䝑䝖䛾஺᥮䛷 ᐃẖ䛻㑅ᢥྍ⬟䚹㻠㻜㻥㻢㻔㻞㻜㻠㻤㻕 䝢䜽䝉䝹䛾᭱᪂ 㻯㻹㻻㻿 䝸䝙䜰䝕䜱䝔䜽䝍ไᚚ䛸㧗ᛶ⬟ගᏛ䝧䞁䝏䛷㧗䝟䝣䜷䞊䝬䞁䝇ᐇ⌧䟿᭦䛻 㻞㻡㻢 䝢䜽䝉䝹䛾 㻵㼚㻳㼍㻭㼟 䝕䜱䝔䜽䝍䛸⤌ྜ䜟䛫䛯㉸ᑠᆺ㏆㉥እศගჾ䛜᪂Ⓩሙ䟿 ᗘᏳᐃᛶ䛻ඃ䜜 㻸㻵㻮㻿 䜔◊✲㛤Ⓨ⏝ 㻻㻱㻹䚸 㣗ရศู䛻᭱㐺䚹
$YD6SHF0LQL&/ $YD6SHF0LQL1,5䖃Ἴ㛗ᇦ㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻞㻜㻜㻙㻝㻝㻜㻜㼚㼙䠖䖃᭱ᑠἼ㛗ศゎ⬟㻌㻌㻌㻌㻜㻚㻜㻥㼚㼙䠖䖃䝎䜲䝘䝭䝑䜽䝺䞁䝆㻌㻌㻟㻜㻜㻜㻌㻦㻌㻝䠖䖃㏞ග㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻨㻜㻚㻞䠂䚷䚷䠖䠖䖃᭱ᑠ㟢ග᫬㛫㻌㻌㻌㻌㻌㻌㻌㻌㻟㻜䃛㼟䖃ගᏛ䝧䞁䝏Ἴ㛗ᇦ㻌㻌㻌㻦䚷㻌㻞㻜㻜㻙㻝㻝㻢㻜㼚㼙䚷䚷㻌㻌䚷䚷䚷䚷䚷䚷㻌㻌㻌㻌㻌㻌㻌㻌㻌䚷㻌㻦㻌㻌㻌㻝㻜㻜㻜㻙㻞㻡㻜㻜㼚㼙㻌㻔㻺㻵㻾㻕䖃䝬䜲䜽䝻䝥䝻䝉䝑䝃䝪䞊䝗 䠖㻌㻝㻢 䝡䝑䝖 㻭㻛㻰㻘 䝁䞁䝞䞊䝍䚷䚷㼁㻿㻮㻟㻚㻜㻛㻝㻳㼎㼜㼟㻱㼀㻴㻘㻝㻜㻜㻌㻹㼜㼕㼤㼑㼘㻌䝯䝰䝸䞊ಖᏑ 㻔㻭㻿㻙㻣㻜㻝㻜㻕㻥㻜㻜㻙㻝㻣㻡㻜㼚㼙㻢㻢㻡㻘㻜㻜㻜㻔 ឤᗘ䠅㻣㻡㻜㻜㻌㻦㻌㻝
㻝㻌䠂
$YD%HQFK8/68/67(&㻝㻜䃛㼟[[PPJ[[PPNJ

䖃㻭㼢㼍㻿㼜㼑㼏㻙㼁㻸㻿 䛾ྛ䝍䜲䝥 㻘㻌㻭㼢㼍㼜㼑㼏㻙㻴㻱㻾㻻㻘䚷䚷㻌㻭㼢㼍㻿㼜㼑㼏㻙㻺㻵㻾㻌䛾ྛ䝍䜲䝥䛻ᑐᛂ䖃䝇䝸䝑䝖䝃䜲䝈 㻦㻌㻌㻞㻡㻘㻡㻜㻘㻝㻜㻜㻘㻞㻜㻜㻘㻡㻜㻜䃛㼙ᵟᶔᵿᵱᶎᶃᶁᵋᵫᶓᶊᶒᶇᵋᵡᶆ

[[PPJ$YD%HQFK+6&[[PPJ$YD%HQFK+6[[PPJ$YD%HQFK7(&$YD6SHF0LQL&/[[PPJ

ᵬᵣᵵ

$YD6SHF0LQL1,5[[PPJ[[PPJ[[PPNJ$YD%HQFK01 ᵬᵣᵵ[[PPJ$6
[PPJ$6

⏘ᴗ⏝䝥䝻䝉䝇ไᚚ䜔ከゅⓗ 䞉 ᗈᇦィ 䛻᭱㐺䚹䖃᭱኱ 㻝㻜㼏㼔 ᵓ⠏ྍ⬟䚸 㻯㼔 ẖ䛻⊂❧✌ാ䚷䚷㻌䖃㻯㼔 ẖ䛻㐪䛖Ἴ㛗䜔㟢ග᫬㛫䛾タᐃ䛜ྍ⬟$YD6SHF(920XOWL&K
&K [[PP GHVNWRS[PPJ'HYHORSHUNLWV$6 ⏝ᅇ㊰௜

&K [[PP 5DFNPRXQWḟୡ௦㐍໬ᆺศගჾ 㻔㻱㼂㻻㻛㻯㻹㻻㻿㻕㻱㼂㻻 䝅䝸䞊䝈
㻯㻹㻻㻿 ไᚚ

᪂㛤Ⓨ䜶䝺䜽䝖䝻䝙䜽䝇䝪䞊䝗 㻔㻭㻿㻙㻣㻜㻝㻜㻕 䛻䜘䜚 㼁㻿㻮㻟㻚㻜㻔㻡㻳㼎㼜㼟㻕 㧗㏿㏻ಙ䚸 㻸㻭㻺 ⤒⏤ 㻝㻳㼎㼜㼟㻱㼀㻴 ┤᥋㐲㊥㞳䝕䞊䝍ఏ㏦䚸 䝯䝰䝸䞊 㻔㻝㻜㻜㻹㼜㼕㼤㼑㼘㻕 ෆ㒊ಖᏑᶵ⬟䚸 እ㒊䝖䝸䜺䞊ᶵ⬟䚸 ከ䝏䝱䞁䝛䝹ᵓ⠏䛺䛹ᐇ⌧᭱᪂䛾 㻯㻹㻻㻿 ᢏ⾡䛷䝤䝹䞊䝭䞁䜾䜔䝇䝭䜰⌧㇟䛜⏕䛨䜛䛣䛸䛺䛟䚸 㧗ᗘ䛺ಙྕฎ⌮䛻䜘䜚ప䝜䜲䝈䛷㻯㻯㻰 䝉䞁䝃䛸ྠ➼䛾ឤᗘ䜔Ἴ㛗ศゎ⬟䛜ᚓ䜙䜜㈝⏝ຠᯝ䜒኱䛝䛔ᵟᶔᵿᵱᶎᶃᶁᵋᵫᶇᶌᶇᵐᵎᵒᵖᵍᵒᵎᵗᵔᵡᵪᴾ ㉸ᑠᆺ 㻯㻹㻻㻿 ไᚚ 䞉 㧗䝟䝣䜷䞊䝬䞁䝇ᆺ㻔㻞㻜㻜㻙㻝㻝㻜㻜㼚㼙㻕㻠㻜㻥㻢㻔㻞㻜㻠㻤㻕㼜㼕㼤㼑㼘㼟 䛾᭱᪂ 㻯㻹㻻㻿 䝸䝙䜰䝕䜱䝔䜽䝍ไᚚ䛸㏞ග䛾ᑡ䛺䛔ගᏛ䝧䞁䝏䛷㧗䝟䝣䜷䞊䝬䞁䝇䜢ᐇ⌧䚹ᗘᏳᐃᛶ 䞉
Ἴ㛗Ᏻᐃᛶ䛻ඃ䜜䚸 ◊✲㛤Ⓨ⏝ 㻻㻱㻹 䜔⤌䜏㎸䜏䛻᭱㐺䛷ᛂ⏝䛿↓㝈኱䕺䜹䝷䞊ィ 㻌䕺⎔ቃィ 㻌䕺䝷䝬䞁䖃㻌㻌ගᏛ䝧䞁䝏㻌䠖㻌㻌㻲㻩㻣㻡㼙㼙㻙㻹㻺㻘㻌㏞ග㻨㻜㻚㻞㻑㻌䖃㻌㻌䝎䜲䝘䝭䝑䜽䝺䞁䝆㻌䠖㻌㻌㻌㻟㻟㻜㻜㻌㻦㻌㻝䚷ศග䕺໬Ꮫᐇ㦂䚷䕺ᛂ⏝ィ 㻌䖃㻌㻌Ἴ㛗ศゎ⬟䠖䚷㻜㻚㻜㻥㻙㼚㼙䚷䖃䚷㻿㻛㻺್㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻦㻌䚷㻟㻟㻜㻌㻦㻌㻝䖃䚷㟢ග᫬㛫㻌㻌㻌䠖㻌㻌㻟㻜䃛㼟䡚㻡㻜㼟䖃䚷ᑍἲ䠖䚷㻥㻡㻌㼤㻌㻢㻤㻌㼤㻌㻞㻜㻌㼙㼙㻘㻌㻝㻣㻠㼓㻌ᵟᶔᵿᵱᶎᶃᶁᵋᵫᶇᶌᶇᵋᵬᵧᵰᵐᵓᵔᵋᵏᵌᵕᴾ
㻔㻥㻜㻜㻙㻝㻣㻡㻜㼚㼙㻕㉸ᑠᆺ 㻵㼚㻳㼍㻭㼟 ไᚚ 䞉 ㏆㉥እ㧗ឤᗘᆺ㻞㻡㻢㼜㼕㼤㼑㼘㼟 䛾 㻵㼚㻳㼍㻭㼟 䝕䜱䝔䜽䝍䛸㏞ග䛾ᑡ䛺䛔ගᏛ䝧䞁䝏䜢䝁䞁䝟䜽䝖䛻⤫ྜ䛧䚸 ㉸ᑠᆺ䛷㏆㉥እ㧗䝟䝣䜷䞊䝬䞁䝇䜢ᐇ⌧䚹ᗘᏳᐃᛶ 䞉 Ἴ㛗Ᏻᐃᛶ䛻ඃ䜜䚸 ◊✲㛤Ⓨ⏝ 㻻㻱㻹 䜔⤌䜏㎸䜏䛻᭱㐺䕺㣗ရศᯒ㻌䕺⏘ᴗ⏝䝸䝃䜲䜽䝹ศู䖃㻌㻌ගᏛ䝧䞁䝏㻌䠖㻌㻌㻲㻩㻣㻡㼙㼙㻙㻹㻺㻌䖃㻌㻌䝎䜲䝘䝭䝑䜽䝺䞁䝆㻌䠖㻌㻌㻣㻡㻜㻜㻌㻦㻌㻝㻌㻔㻸㻺㻕䕺ᚤᙅගィ 㻌䕺䝥䝷䝇䝏䝑䜽䛾ศᯒ㻌䖃㻌㻌ឤᗘ䠖㻢㻢㻡㻘㻜㻜㻜䠄㼏㼛㼡㼚㼠㻛䃛㼃㻌㼜㼑㼞㻌㼙㼟㻕㻌㻔㻴㻿㻕 䖃䚷㻿㻛㻺್㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻦㻌䚷㻡㻜㻜㻜㻌㻦㻌㻝㻌㻔㻸㻺㻕䖃䚷㟢ග᫬㛫㻌㻌㻌䠖㻌㻌㻝㻜䃛㼟䡚㻡㼟䚷㻔㻸㻺㻕䖃䚷ᑍἲ䠖䚷㻥㻡㻌㼤㻌㻢㻤㻌㼤㻌㻞㻜㻌㼙㼙㻘㻌㻝㻤㻡㼓㻌ᵟᶔᵿᵱᶎᶃᶁᵋᵳᵪᵱᵐᵎᵒᵖᵍᵒᵎᵗᵔᵡᵪᵋᵣᵴᵭ 㻯㻹㻻㻿 ไᚚ 䞉 㧗㏿ 䞉 㧗Ἴ㛗ศゎ⬟ᆺ㻔㻞㻜㻜㻙㻝㻝㻜㻜㼚㼙㻕㧗㏿䛾ᶆ‽୓⬟ᆺ䛷㧗䝟䝣䜷䞊䝬䞁䝇䛜ᚓ䜙䜜ᇶᮏⓗ䛺ィ 䛿໚ㄽ䛾䛣䛸ከ䝏䝱䞁䝛䝹䝅䝇䝔䝮䛻ᑐᛂ䚹 㧗ゎീᗘ 㻠㻜㻥㻢㼜㼕㼤㼑㼘㼟 䛾㻯㻹㻻㻿 䝕䜱䝔䜽䝍䜢ᦚ㍕䛧䛶㏞ග䛾Ṥ䛹䛺䛔⎔ቃ䛷᭱ᑠ㟢ග᫬㛫䛻䛶ィ 䛜ྍ⬟䕺⏘ᴗ⏝䝥䝻䝉䝇䝁䞁䝖䝻䞊䝹䖃㻌㻌ගᏛ䝧䞁䝏㻌䠖㻌㻲㻩㻣㻡㼙㼙㻘㻌㏞ග㻨㻜㻚㻞㻑㻌䖃㻌㻌䝎䜲䝘䝭䝑䜽䝺䞁䝆㻌䠖㻌䚷㻠㻜㻜㻜㻌㻦㻌㻝䖃㻌㻌Ἴ㛗ศゎ⬟䠖㻌㻜㻚㻜㻡㻙㻞㻜㼚㼙䖃㻌㻌㏞ග㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌䠖䚷㻌㻜㻚㻝㻥㻙㻝㻚㻜䠂䕺ගศᯒ㻌䕺⎔ቃィ 㻌䕺໬Ꮫᐇ㦂䚷䚷䚷䚷䚷䚷䚷
䖃㻌㻌㟢ග᫬㛫㻌㻌㻌䠖㻌㻥䃛㼟䡚㻠㻜㼟䚷㻔㻠㻜㻥㻢㻯㻸㻕䚷 䖃㻌㻌㻿㻛㻺್㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻦㻌䚷㻌㻟㻟㻡㻌㻦㻌㻝ᵟᶔᵿᵱᶎᶃᶁᵋᵦᵣᵰᵭᴾᵆᵋᵣᵴᵭᵇ
㻔㻞㻜㻜㻙㻝㻝㻢㻜㼚㼙㻕䕺䝷䝬䞁ศග㻌䕺㻸㻵㻮㻿䕺䝥䝷䝈䝬ィ䚷䚷㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌䚷

㧗㏿ 䞉 㧗ឤᗘ 䞉 㧗Ἴ㛗ศゎ⬟ᆺ㻱㼂㻻 䛸㧗ᛶ⬟ 㼀㻱 ෭༷ 㻯㻯㻰 ⫼㠃↷ᑕᆺ䝕䜱䝔䜽䝍ไᚚ䛸䛾䝁䞁䝡䛷ప䝜䜲䝈 䞉 㧗 㻿㻛㻺 ್ 䞉 㧗䝎䜲䝘䝭䝑䜽䝺䞁䝆䜢ᐇ⌧䖃㻌㻌ගᏛ䝧䞁䝏㻌䠖㻌㻲㻩㻝㻜㻜㼙㼙㻘㻌㻺㻭㻌㻦㻌㻜㻚㻝㻟㻌䖃㻌㻌䝎䜲䝘䝭䝑䜽䝺䞁䝆㻌䠖㻌䚷㻠㻜㻜㻜㻜㻌㻦㻌㻝䕺ග䛾ᑡ䛺䛔⎔ቃ䛷䛾⺯ගィ䖃㻌㻌Ἴ㛗ศゎ⬟䠖㻌㻜㻚㻞㻙㻣㼚㼙䖃㻌㻌㏞ග㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌䠖䚷㻌㻜㻚㻡㻙㻝㻚㻜䠂䖃㻌㻌㟢ග᫬㛫㻌㻌㻌䠖㻌㻡㻚㻞㼙㼟䡚㻢㻜㼟䚷䖃㻌㻌㻿㻛㻺್㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻦㻌䚷㻝㻞㻜㻜㻌㻦㻌㻝䕺䝷䝬䞁ᛂ⏝ศග䚷ᵟᶔᵿᵱᶎᶃᶁᵋᵳᵪᵱᵐᵎᵒᵖᶖᵔᵒᵋᵣᵴᵭ㧗㏿ 䞉 㼁㼂 䞉 㻺㻵㻾 ㉸㧗ឤᗘᆺ㻱㼂㻻 䛸 㻞㻜㻠㻤㼤㻢㻠㼜㼕㼤㼑㼘㼟 䛾 㻯㻯㻰 ⫼㠃↷ᑕᆺ䝕䜱䝔䜽䝍ไᚚ䛻䜘䜚 㼁㼂㻒㻺㻵㻾 ᇦ䛻䛶㉸㧗ឤᗘᐇ⌧䚹 ྠ 㼀㻱㻯 ᆺ䜘䜚ప䝁䝇䝖㻔㻞㻜㻜㻙㻝㻝㻢㻜㼚㼙㻕䖃㻌㻌ගᏛ䝧䞁䝏㻌䠖㻌㻲㻩㻣㻡㼙㼙㻘㻌㻌䖃㻌㻌ឤᗘ䠖㻌㻢㻡㻜㻘㻜㻜㻜㻌㻔㼏㼛㼡㼚㼠㼟㻛䃛㼃㻌㼜㼑㼞㻌㼙㼟㻕䖃㻌㻌㟢ග᫬㛫㻌㻌㻌䠖㻌㻞㻚㻠㼙㼟䡚㻢㻜㻜㼟䚷䖃㻌㻌Ἴ㛗ศゎ⬟䚷䚷䚷䚷㻌䠖㻌䚷㻜㻚㻜㻥㻙㻞㻜㼚㼙䖃㻌㻌㼁㼂㔞Ꮚຠ⋡㻌㻌㻌㻌㻌㻌㻌㻌䠖㻌㻌㻌㻌㻢㻜䠂䖃㻌㻌㻿㻛㻺್㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻦㻌䚷㻌㻠㻡㻜㻌㻦㻌㻝ᵟᶔᵿᵱᶎᶃᶁᵋᵬᵧᵰᵐᵓᵔᵍᵓᵏᵐᵋᵏᵌᵕᵋᵣᵴᵭᴾ
㻔㻥㻜㻜㻙㻝㻣㻡㻜㼚㼙㻕䕺㼁㼂 ᨺᑕ⥺ ᐃ䕺⺯ගィ 䚷䕺䝷䝬䞁ィ㠀෭༷㏆㉥እ㧗㏿ 䞉 㧗ឤᗘᆺ㻱㼂㻻 䛸 㻵㼚㻳㼍㻭㼟 䝸䝙䜰䞊䜰䝺䜲䝕䜱䝔䜽䝍䛻䜘䜚 㻝㻣㻜㻜㼚㼙 ㎾䛾㏆㉥እ䛻䛶㉸㧗ឤᗘ 䞉 㧗䝎䜲䝘䝭䝑䜽䝺䞁䝆 䞉 ᭱▷㟢ග᫬㛫䜢ᐇ⌧䖃䚷ගᏛ䝧䞁䝏㻌䠖㻌㻲㻩㻡㻜㼙㼙㻘㻌㻺㻭㻌㻦㻌㻜㻚㻞㻠䖃㻌㻌䝎䜲䝘䝭䝑䜽䝺䞁䝆㻌䠖㻌㻌㻌㻥㻜㻜㻜㻌㻦㻌㻝㻌㻔㻸㻺㻕䕺Ỉศྵ᭷㔞䛾ィ 䚷䖃䚷ឤᗘ䠖㻤㻘㻞㻜㻜㻘㻜㻜㻜䠄㼏㼛㼡㼚㼠㻛䃛㼃㻌㼜㼑㼞㻌㼙㼟㻕㻌㻔㻴㻿㻕 䖃䚷㻿㻛㻺್㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌䠖㻌㻌㻌㻡㻜㻜㻜㻌㻦㻌㻝㻌㻔㻸㻺㻕䕺ᾮయ 䞉 ಶయ 䞉 ⢊య䛾䜲䞁䝷䜲䞁ィ 䚷䖃㻌㻌㟢ග᫬㛫㻌㻌㻌䠖㻌㻝㻜䃛㼟䡚㻞㻜㼟㻌㻔㻸㻺㻕䖃㻌㻌㻴㻿䝰䞊䝗䛸㻸㻺䝰䞊䝗ษ᥮䛘䛜ྍ⬟ᵟᶔᵿᵱᶎᶃᶁᵋᵬᵧᵰᵐᵓᵔᵍᵓᵏᵐᵋᵐᵌᵓᵋᵦᵱᵡᵋᵣᵴᵭᴾ㏆㉥እ㧗㏿ 䞉 㧗ឤᗘᆺ㻱㼂㻻 䛸 㼀㻱 ෭༷ 㻵㼚㻳㼍㻭㼟 䝸䝙䜰䞊䜰䝺䜲 㻞 䝇䝔䞊䝆䝕䜱䝔䜽䝍䛻䜘䜚 㻞㻡㻜㻜㼚㼙 ㎾䛾୰㉥እᇦ䛷ప䝜䜲䝈 䞉 㧗ឤᗘ䛾ィ㻔㻝㻜㻜㻜㻙㻞㻡㻜㻜㼚㼙㻕䝕䜱䝔䜽䝍䞊

䚷䖃䚷ගᏛ䝧䞁䝏㻌䠖㻌㻲㻩㻝㻜㻜㼙㼙㻘㻌㻺㻭㻌㻦㻌㻜㻚㻝㻟䖃㻌㻌䝎䜲䝘䝭䝑䜽䝺䞁䝆㻌䠖㻌㻌㻌㻡㻝㻜㻜㻌㻦㻌㻝㻌㻔㻸㻺㻕䖃䚷ឤᗘ䠖㻌㻥㻥㻜㻘㻜㻜㻜䠄㼏㼛㼡㼚㼠㻛䃛㼃㻌㼜㼑㼞㻌㼙㼟㻕㻌㻔㻴㻿㻕 䖃䚷㻿㻛㻺್㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌 䠖㻌䚷㻟㻣㻜㻜㻌㻦㻌㻝㻌㻔㻸㻺㻕䖃㻌㻌㟢ග᫬㛫㻌㻌㻌䠖㻌㻝㻜䃛㼟䡚㻝㻜㻜㼙㼟㻌㻔㻸㻺㻕䖃㻌㻌㻴㻿䝰䞊䝗䛸㻸㻺䝰䞊䝗ษ᥮䛘䛜ྍ⬟ឤᗘ 㻔㼏㼛㼡㼚㼠㼟㻛䃛㼃㻌㼜㼑㼞㻌㼙㼟㻕 ᭤⥺ 䠄㻿㼠㼍㼞㻸㼕㼚㼑㻕䜢ᐇ⌧䕺䝥䝷䝇䝏䝑䜽䛾ᡂศศᯒ䚷䕺ኴ㝧ගⓎ㟁⏝䝰䝙䝍䞊䛾Ⓨග ᐃ䚷ឤᗘ᭤⥺ 㻔㻿㼑㼚㼟㻸㼕㼚㼑㻕ឤᗘ᭤⥺ 㻔㻺㻵㻾㻌㻸㼕㼚㼑㻕䝕䜱䝔䜽䝍䛾䝍䜲䝥㻌䛻䜘䜚ྛ䝰䝕䝹䛾≉㛗䛜䛒䜚㻌⏝㏵䛻ᛂ䛨䛯ィ 䛜ྍ⬟䜾䝺䞊䝔䜱䞁䜾ຠ⋡㻭㼢㼍㻿㼜㼑㼏㻙㼁㻸㻿㻠㻜㻥㻢㻯㻸㻙㻱㼂㻻 ᶆ‽ 䞉 ୓⬟ᆺ䚷䚷Ἴ㛗ศゎ⬟ 䠄㻳㼘㼍㼠㼕㼚㼓㻌㻒㻌㻿㼘㼕㼠㻕䚷䝇䝨䜽䝖䝹䝺䞁䝆䛸䜾䝺䞊䝔䜱䞁䜾䜢㑅䜆䛣䛸䛷᭱㐺䛺ィ 䛜ྍ⬟㻢㻜㻜㻌㻸㼕㼚㼑㻛㼙㼙㻌㻳㼘㼍㼠㼕㼚㼓㻝㻞㻜㻜㻌㻸㼕㼚㼑㻛㼙㼙㻌㻳㼘㼍㼠㼕㼚㼓㼁㻸㻿㻣㻡㼙㼙 ගᏛ䝧䞁䝏 㻘㻌㻯㻹㻻㻿 䝕䜱䝔䜽䝍䛾 㻱㼂㻻 䝍䜲䝥䛻䜘䜚㧗㏿䛷㧗Ἴ㛗ศゎ⬟䛾ィ 䛜ྍ⬟䛺୓⬟ᆺ 㻔㻞㻜㻜㻙㻝㻝㻜㻜㼚㼙㻕䖃Ἴ㛗ศゎ⬟ 䠖 㻜㻚㻜㻡 䡚 㻞㻜㼚㼙䖃㻿㻛㻺 ẚ䚷䚷䚷 䠖㻌㻟㻟㻡㻌㻦㻌㻝䖃㟢ග᫬㛫䚷䚷㻦㻌㻌㻥䃛㼟 䡚 㻠㻜㼟㻌䖃㏞ග㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻦㻌㻌㻜㻚㻝㻥㻌䡚㻌㻝㻚㻜㻑䖃ឤᗘ㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻌㻦㻌㻌㻞㻝㻤㻘㻜㻜㻜㻔㼏㼛㼡㼚㼠㼟㻛䃛㼃㻌㼜㼑㼞㻌㼙㼟㻕䜾䝺䞊䝔䜱䞁䜾䛿Ἴ㛗㛫䛾㛫㝸䜢Ỵ䜑䚸 䝇䝸䝑䝖䛿ග䛜㏻㐣䛩䜛ᖜ䜢ไ㝈䛩䜛䛾䛷䝣䜯䜲䝞䞊䝁䜰ᚄ䛸ඹ䛻Ἴ㛗ศゎ⬟䛻ᙳ㡪䛩䜛*

EVO SERIESTHE NEXT EVOLUTIONARY STEP FOR SPECTROMETRYAVANTES’ EVO SERIES
Avantes is proud to announce the latest
additions to our EVO-series spectrometersin the UV/VIS and NIR range.

EVO series; why?
With the introduction of the AS-7010
electronics board, Avantes brought new
and improved functionality to theirspectrometers. This circuit board brings
USB3 and Ethernet
communication options to you.
These options offer faster data speeds,
longer distances and network
integration for your application. Our
improved electronics deliver morenoise-free signals for yourmeasurements and the on-board
memory capabilities ensure plentyof capacity for future features.
Spectrometers using this AS7010
electronics platform are the next
EVOlutionary step in spectrometry.
Avantes bundled these spectrometersin the EVO line of products, which aredescribed in this brochure.

CMOS and CCD
Avantes offers a broad range ofspectrometers with different detector
technologies.
For our Starline spectrometers, thestandard Si CCD technology was thedominant technology for years.
However, this dominant position islosing ground to CMOS technology.
Wanting to be prepared for the future,
Avantes embraced the CMOS
technology at an early stage and now
offers this latest, state-of-the-art
technology as the new standard for our
spectrometers.
In the NIRline spectrometers we use
InGaAs detectors and in the SensLine
we use back-thinned CCD detectors.

EVO Series; UV/VIS spectrometer
Offers GigaEthernet and USB3.0
communication, more memory and fast
data processing. Using the latest CMOS
technology, these spectrometers are readyfor the next decade!

Timing and Triggering
Numerous applications require for aspectrometer to be triggered at atimesensitive
moment. For example whenmeasuring in production lines, or withpulsed or flashed events like solar
simulators or led measurements .
Our state-of-the-art electronics, in
combination with the right detector
choice will provide you with anexcellent instrument for continuous,
repetitive, stable measurements.
For decades, Avantes spectrometers
have been well known for their
excellent timing and trigger
performance.


AvaSpec-HEROThe AvaSpec-HERO is the answer for
those in need of high resolution andhigh sensitivity! It combines high-end,
cooled back-thinned detector
technology , a 100mm symmetrical
Czerny-Turner optical bench and stateof-the-art electronics to enable noisefree signal measurement in the mostdemanding environment. The ideal
choice in the EVO series. A real HERO for
your application!


EVOlutionary spectroscopy:• Speed• Network integration• Multi-channel benefits

AVANTES’ EVO SERIES
Product line overview

EVO series in our product lines
Product lines
Starline

Sensline

NIRlineAvaSpec-ULS2048CL-EVO

AvaSpec-HERO

AvaSpec-NIR256/512-1.7-EVO

AvaSpec-ULS4096CL-EVO

AvaSpec-ULS2048XL-EVO

AvaSpec-NIR256/512-1.7-HSC-EVO

AvaSpec-HS2048XL-EVO
AvaSpec-ULS2048x64-EVO
AvaSpec-ULS2048x64TEC-EVO

USB 3.0
Gigabit Ethernet
More memory

info@avantes.com | www.avantes.com | 3

AvaSpec-NIR256/512-2.5-HSC-EVO

Spectrometers

AvaSpec-ULS2048CL-EVO
StarLine CMOS Spectrometer
AvaSpec-ULS2048CL-EVO

spectra onboard and realize morefunctionality.

Using CMOS instead of theconventional CCD detectors, thisspectrometer offers you the latest
technology.
In combination with our latest AS-7010
electronics, it offers you a versatiledevice including USB3.0 communication
with 10x higher speed compared
to USB2, and a second communication
port which offers Gigabit Ethernet for
integration in your company networkand possibility for long distancecommunication.
Besides the high-speed communication
options, the EVO series offers a fast
microprocessor and increased
memory to help you store more

Options include a detector collectionlens to enhance sensitivity in the 200
to 1100 nm range and an order-sorting
filter to reduce second-order effects.
The AvaSpec-ULS2048CL-EVO isavailable with a wide range of slit sizes,
gratings and fiber-optic entrance
connectors as well.
It comes complete with AvaSoft-Basic
software, USB cable and an extensive
manual.
The AvaSpec-ULS2048CL-EVO is alsoavailable as OEM unit, bench only or
Rackmount version.

Technical Data
Optical bench
Wavelength range

ULS symmetrical Czerny-Turner, 75 mm focal length
200 - 1100 nm

Resolution

0.06 – 20 nm, depending on configuration (see table)

Stray light

0.19 - 1.0%, depending on the grating

Sensitivity

375,000 counts/µW per ms integration time

Detector

CMOS linear Image Sensor

Signal/noise

300:1

AD converter

16-bit, 6 MHz

Integration time

30 µs – 59 s

InterfaceUSB 3.0 high speed, 5 Gbps
Gigabit Ethernet 1 Gbps

Digital IO

HD-26 connector, 2 Analog in, 2 Analog out, 13 Digital bidirectional,
trigger, sync., strobe, laser

Power supply
Dimensions, weight

Default USB3 power, 500 mA
Or 12VDC, 300 mA
177 x 127 x 44,5 mm (1 channel), 1135 grams

Timing and Triggering
Sample speed with on-board averaging
Data transfer speed
Min. delay / jitter

0.38 ms/scan
0.38 ms/scan (USB3), 1.0 ms (ETH)
0.9 / 0.02 µs

Detector Specifications
Sensitivity
photons/count@ 600 nmSensitivity
in cts/µW
per msint. time

QE(%) @ peak

Signal/noise

Dark noise(counts
RMS)

Dynamic
range

2375,000

80%

300:1

16

4000

4 | info@avantes.com | www.avantes.com

Grating Selection Table
Use

Useable range(nm)

Spectral range(nm)

Lines/mm

Blaze (nm)Order code

UV/VIS/NIR

200 - 1100**

891**

300

300

UA

UV/VIS/NIR

200 - 1100**

891**

300

300/1000

UNA-DBUV/VIS

200 - 850

515

600

300

UB

UV

200 - 750

247 - 218*

1200

250

UC

UV

200 - 650

163 - 143*

1800

UV

UD

UV

200 - 580

113 - 69*

2400

UV

UE

UV

200 - 400

69 - 45*

3600

UV

UF

UV/VIS

250 - 850

515

600

400

BB

VIS/NIR

300 - 1100**

792**

300

500

VA

VIS

360 - 1000

495

600

500

VB

VIS

300 - 800

247 - 218*

1200

500

VC

VIS

350 - 750

142 - 89*

1800

500

VD

VIS

350 - 640

74 - 49*

2400

VIS

VE

NIR

500 - 1050

495

600

750

NB

NIR

500 - 1050

218 - 148*

1200

750

NC

NIR

600 - 1160

346 - 297

830

800

SI

NIR

600 - 1100**

495**

300

1000

IA

NIR

600 - 1100

495

600

1000

IB

* depends on the starting wavelength of the grating; the higher the wavelength, the bigger the dispersion and the smaller the range to select.
** please note that not all 2048 pixels will be used for the useable range.

Resolution Table (FWHM in nm)
Slit size (µm)
Grating (lines/mm)

10

25

50

100

200

500

300

1.0

1.4

2.5

4.8

9.2

21.3

600

0.40 - 0.53*

0.7

1.2

2.4

4.6

10.8

830

0.32

0.48

0.93

1.7

3.4

8.5

1200

0.20 - 0.28*

0.27 - 0.38*

0.52 - 0.66*

1.1

2.3

5.4

1800

0.10 - 0.18*

0.20 - 0.29*

0.34 - 0.42*

0.8

1.6

3.6

2400

0.09 - 0.13*

0.13 - 0.17*

0.26 - 0.34*

0.44 - 0.64*

1.1

2.7

0.06 - 0.08*

0.10

0.19

0.4

0.8

1.8

3600

* depends on the starting wavelength of the grating; the higher the wavelength, the bigger thedispersion and the better the resolution.

Options-RS
DCL-UV/VIS-200
SLIT-XX
SLIT-XX-RS
SLIT-XX-RS-FCPCOSF-YYY
OSC• Replaceable slit
• Quartz detector collection lens (200 - 1100 nm)• Slit size, please specify XX = 5, 10, 25, 50, 100, 200 or 500 µm• Replaceable slit with SMA connector , specify slit size XX = 25, 50, 100, 200 or 500 µm.
Only available for AvaSpec-ULS2048CL-EVO-RS• As SLIT-XX-RS, but with FC/PC connector• Order-sorting filter for reduction of second-order effects
please specify YYY = 305, 395, 475, 515, 550 or 600 nm• Order-sorting coating with 600 nm long-pass filter for BB (>305 nm)
and VB gratings, recommended with OSF-305

OSC-UA• Order-sorting coating with 350 and 600 nm linear variable filter for UA, VA gratings

OSC-UB• Order-sorting coating with 350 and 600 nm long-pass filter for UB or BB (<350 nm)
gratings-FCPC• FC/PC fiber-optic connector

info@avantes.com | www.avantes.com | 5

Spectrometers

AvaSpec-ULS4096CL-EVO
StarLine CMOS Spectrometer
AvaSpec-ULS4096CL-EVO

The AvaSpec-ULS4096CL-EVO uses
the latest CMOS technology instead of
the conventional CCD detectors, whichmeans this spectrometer is completely
up to date and ready for the next
decade.

Besides the high speed
communication options, the EVO seriesalso offers a fast microprocessor andimproved memory which can help you
to store more spectra onboard andrealize more functionality.

The dominant position of CCD
detectors in the spectrometer field isfading and new technologies like CMOS
have evolved and become a suitable
alternative.

The AvaSpec-ULS4096CL-EVO isavailable with a wide range of slit
sizes, gratings and fiber-optic entrance
connectors as well. The AvaSpecULS4096CL-EVO is also available as
OEM unit, bench only or Rackmountversion.

In combination with our latest AS-7010
electronics it offers you a versatiledevice including USB3 communication
with 10 times higher speed compared
to USB2 and a second communication
port that offers Gigabit Ethernet.

With its 4096 pixels, this spectrometeris tailored for high-resolution
applications like plasma monitoringand LIBS.

Technical Data
Optical bench
Wavelength range

ULS symmetrical Czerny-Turner, 75 mm focal length
200 - 1100 nm

Resolution

0.05 – 20 nm, depending on configuration (see table)

Stray light

0.19 - 1.0%, depending on the grating

Sensitivity

218,000 counts/µW per ms integration time

Detector

CMOS linear Image Sensor

Signal/noise

335:1

AD converter

16-bit, 6 MHz

Integration time

9 µs – 40 s

InterfaceUSB 3.0 high speed, 5 Gbps
Gigabit Ethernet 1 Gbps

Digital IO

HD-26 connector, 2 Analog in, 2 Analog out, 13 Digital bidirectional,
trigger, sync., strobe, laser

Power supply
Dimensions, weight

Default USB3 power, 500 mA
Or 12VDC, 300 mA
177 x 127 x 44,5 mm (1 channel), 1135 grams

Timing and Triggering
Sample speed with on-board averaging
Data transfer speed
Min. delay / jitter

0.7 ms/scan
0.7 ms/scan (USB3), 1.0 ms (ETH)
0.9 / 0.02 µs

Detector Specifications
Sensitivity
photons/count@ 600 nmSensitivity
in cts/µW
per msint. time

QE(%) @ peak

Signal/noise

Dark noise(counts
RMS)

Dynamic
range

2

218,000

80%

325:1

16

4000

6 | info@avantes.com | www.avantes.com

Grating Selection Table
Use

Useable range(nm)

Spectral range(nm)

Lines/mm

UV/VIS/NIR

200 - 1100**

891**

300

300

UA

UV/VIS/NIR

200 - 1100**

891**

300

300/1000

UNA-DBUV/VIS

200 - 850

515

600

300

UB

UV

200 - 750

247 - 218*

1200

250

UC

UV

200 - 650

163 - 143*

1800

UV

UD

UV

200 - 580

113 - 69*

2400

UV

UE

Blaze (nm)Order code

UV

200 - 400

69 - 45*

3600

UV

UF

UV/VIS

250 - 850

515

600

400

BB

VIS/NIR

300 - 1100**

792**

300

500

VA

VIS

360 - 1000

495

600

500

VB

VIS

300 - 800

247 - 218*

1200

500

VC

VIS

350 - 750

142 - 89*

1800

500

VD

VIS

350 - 640

74 - 49*

2400

VIS

VE

NIR

500 - 1050

495

600

750

NB

NIR

500 - 1050

218 - 148*

1200

750

NC

NIR

600 - 1160

346 - 297

830

800

SI

NIR

600 - 1100**

495**

300

1000

IA

NIR

600 - 1100

495

600

1000

IB

* depends on the starting wavelength of the grating; the higher the wavelength, the bigger the dispersion and the smaller the range to select.
** please note that not all 4096 pixels will be used for the useable range.

Resolution Table (FWHM in nm)
Slit size (µm)
Grating (lines/mm)

10

25

50

100

200

500

300

0.50 - 0.70

1.20 - 1.30*

2.17

4.6

9.00

20.0

600

0.30 - 0.36*

0.58 - 0.60

1.17

2.20

4.5

10.0

830

0.25

0.48

0.93

1.7

3.4

8.0

1200

0.14 - 0.18*

0.30

0.62

1.08

2.2

5.0

1800

0.09 - 0.11*

0.18

0.36 - 0.40*

0.78

1.5

3.7

2400

0.07 - 0.09*

0.13 - 0.15*

0.26 - 0.32*

0.40 - 0.64*

1.1

2.7

0.05 - 0.06*

0.10

0.19

0.4

0.8

2.0

3600

* depends on the starting wavelength of the grating; the higher the wavelength, the bigger thedispersion and the better the resolution.

Options-RS
DCL-UV/VIS-200
SLIT-XX
SLIT-XX-RS
SLIT-XX-RS-FCPCOSF-YYY
OSC• Replaceable slit
• Quartz detector collection lens (200 - 1100 nm)• Slit size, please specify XX = 5, 10, 25, 50, 100, 200 or 500 µm• Replaceable slit with SMA connector , specify slit size XX = 25, 50, 100 or 200 µm.
Only available with AvaSpec-ULS4096CL-EVO-RS• As SLIT-XX-RS, but with FC/PC connector• Order-sorting filter for reduction of second-order effects
please specify YYY = 305, 395, 475, 515, 550 or 600 nm• Order-sorting coating with 600 nm long-pass filter for BB (>305 nm)
and VB gratings, recommended with OSF-305

OSC-UA• Order-sorting coating with 350 and 600 nm linear variable filter for UA, VA gratings

OSC-UB• Order-sorting coating with 350 and 600 nm long-pass filter for UB or BB (<350 nm)
gratings-FCPC• FC/PC fiber-optic connector

info@avantes.com | www.avantes.com | 7

Spectrometers

AvaSpec-HERO
SensLine Back-thinned CCD Spectrometer
AvaSpec-HSC1024x58TEC-EVO

The AvaSpec-Hero is our top-of-theline
spectrometer!
Based on our High-Sensitivity Compact
optical (HSC) bench (f=100mm;
NA=0.13) and a 1024x58 back-thinned
CCD detector, it offers the best of bothworlds: high sensitivity and resolution!
The instrument is equipped with a
TE Cooling enabling long integration
times in low light applications. In
conjunction with our AS7010
electronics, including a high end AD
convertor, noise is kept to a minimum,
which offers you an excellent Signal toNoise and Dynamic Range
performance.

From low-light fluorescenceapplications to the most demanding
Raman applications; the AvaSpec-Hero
is your ideal companion.
Of course the Digital IO ports enabling
external triggering, control ofshutters, and pulsed light sources fromthe Avantes line of instruments arecompatible with the HERO as well.
The Avaspec-HERO is standard
equipped for use with replaceable slits,
offering optimal flexibility for a variety
of applications.

Technical Data: AvaSpec-HSC1024x58TEC-EVO
Optical bench
Wavelength range

HSC symmetrical Czerny-Turner, 100 mm focal length, NA: 0.13
200 - 1160 nm

Resolution

0.2 - 7 nm, depending on configuration (see table)

Stray light

0.5%, depending on the grating

Sensitivity

445,000 counts/µW per ms integration time

Detector

CCD array image sensor with one stage TE Cooled, 1024 pixels

Signal/noise

1200:1

Dynamic range

40,000AD converter

16-bit, 250 kHz

Integration time

5.2 ms – 60 sec

InterfaceUSB 3.0 high speed, 5 Gbps
Gigabit Ethernet 1 Gbps

Digital IO

HD-26 connector, 2 Analog in, 2 Analog out, 3 Digital bidirectional,
trigger, sync., strobe, laser.

Power supply
Dimensions, weight

12VDC, 1.5A
185 x 161 x 185 mm, 3500 grams

Timing and Triggering
Sample speed with on-board averaging
Data transfer speed
Min. delay / jitter

5.2 ms/scan
5.2 ms/scan (USB3 and ETH)
-5220 µs / 5220 µs

Detector Specifications
Sensitivity
photons/count@ 600 nmSensitivity
in cts/µW
per msint. time

QE(%) @ peak

Signal/noise

Dark noise(counts
RMS)

Dynamic
range

16445,000

92%

1200:1

2

40,000

10 | info@avantes.com | www.avantes.com

Grating Selection Table
Use

Useable range(nm)

Spectral range(nm)

Lines/mm

Blaze (nm)Order code

UV/VIS/NIR

200 - 1160

770 - 760*

300

300

HSC0300-0.30

UV/VIS/NIR

250 - 1160

770 - 760*

300

420

HSC0300-0.42

VIS/NIR

250 - 1160

577 - 553

400

550

HSC0400-0.55

UV/VIS

200 - 850

373 - 340*

600

400

HSC0600-0.40

VIS/NIR

250 - 1160

373 - 340*

600

650

HSC0600-0.65

VIS/NIR

500 - 1160

268 - 220*

830

900

HSC0830-0.90

UV/VIS

200 - 1160

182 - 130*

1200

400

HSC1200-0.40

VIS/NIR

500 - 1050

182 - 130*

1200

750

HSC1200-0.75

UV/VIS

200 - 850

84 - 61*

2400

270

HSC2400-0.27* depends on the starting wavelength of the grating; the higher the wavelength, the bigger the dispersion and the smaller the range to select.

Resolution Table (FWHM in nm)
Slit size (µm)
Grating (lines/mm)

10

25

50

300

1.70

1.90

400

1.40

1.55

600

0.80

0.85

830

0.60

1200

0.32
0.18

2400

100

200

500

2.45

3.0

5.50

5.50

2.00

2.55

4.70

5.50

1.10

1.70

3.00

5.50

0.70

0.9

1.25

2.00

5.50

0.35

0.48

0.80

1.30

5.50

0.20

0.29

0.40

0.65

5.50

* Above values are average values. Due to optical properties resolution will be better in the lower
wavelengths than in the higher wavelength range.

Options
SLIT-XX-RS
SLIT-XX-RS-FCPC• Replaceable slit with SMA connector, specificy slit size XX = 10, 25, 50, 100, 200
or 500 µm.
• As SLIT-XX-RS, but with FC/PC connector

SLITKIT-SMA• Slit kit containing 25, 50, 100, 200 or 500 μm slits, and the tools to replace the slit.
SMA-connectors

SLITKIT-FCPC• As SLITKIT-SMA, but with FC/PC connectors

OSF-YYY-3• Order sorting filter for reduction of second-order effects, 3 mm thick, please specify
YYY = 305, 395, 475, 515, 550, 600 nm

OSC-HSC300• Order sorting coating for use with grating HSC0300-xx

OSC-HSC600• Order sorting coating for use with grating HSC0600-xx and HSC0400-xx

The new AvaSpec-HERO is the answer
for those in need of high resolution ándhigh sensitivity!

info@avantes.com | www.avantes.com | 11

Spectrometers

AvaSpec-ULS2048XL-EVO
SensLine Back-thinned CCD Spectrometer
AvaSpec-ULS2048XL-EVO

Combining exceptional quantum
efficiency with high speed is thevalue proposition of the AvaSpecULS2048XL-EVO spectrometer.

To further enhance sensitivity, adetector collection lens is available toimprove sensitivity up to 60% whencombined with larger core fibers.

Unlike many back-thinned CCD
spectro-meters with two dimensional
arrays, the AvaSpec-ULS2048XL-EVO
has large, monolithic pixels of 14x500
microns with exceptional efficiency in
the UV range, from 200 to 400 nm, andthe NIR range, from 950 to 1160 nm.

Options include an order-sorting filter
to reduce second-order effects andpurge ports for deep-UV
measurements. The AvaSpecULS2048XL-EVO comes with a wide
range of slit sizes, gratings and may
be configured with SMA or FC/PC fiberoptic
entrance connectors.

The instrument has an electronic
shutter, which enables integration
times as low as 2 microseconds.

Connection to your PC is handled via aUSB3-connection or Ethernet,
delivering a scan every 2 milliseconds.

Technical Data
Optical bench
Wavelength range

ULS, Symmetrical Czerny-Turner, 75 mm focal length
200 - 1160 nm

Resolution

0.09 –20 nm, depending on configuration (see table)

Stray light< 0.5%

Sensitivity

460,000 counts/µW per ms int. time

UV quantum efficiency
Detector

60% (200-300 nm)
Back-thinned CCD image sensor 2048 pixels

Signal/noise

525:1

AD converter

16-bit, 1 MHz

Integration time
Interface

2 µs – 20 seconds
USB 3.0 high speed, 5 Gbps
Gigabit Ethernet 1 Gbps

Readout noise

9.8 cnt RMS

Dark noise

4.5 cnt RMS

Dynamic range
Digital IO
Power supply
Dimensions, weight

13,700HD-26 connector, 2 Analog in, 2 Analog out, 3 Digital in, 12 Digital out,
trigger, synchronization
Default USB power, 700 mA. Or external 12VDC, 360 mA
175 x 127 x 44,5 mm (1 channel), 1180 grams

Timing and Triggering
Sample speed with on-board averaging
Data transfer speed
Min. Delay / Jitter2.44 ms/scan
2.44 ms/scan (USB3)
0.37 / 25 ns

Detector Specifications
Sensitivity
photons/count@ 600 nmSensitivity
in cts/µW
per msint. time

QE(%) @ peak

Signal/noise

Dark noise(counts
RMS)

Dynamic
range

4

460,000

78%

525:1

5

13,70012 | info@avantes.com | www.avantes.com

Grating Selection Table
Use

Useable range(nm)

Spectral range(nm)

Lines/mm

Blaze (nm)Order code

UV/VIS/NIR

200 - 1160**

960**

300

300

UA

UV/VIS/NIR

200 - 1100**

900**

300

300/1000

UNA-DBUV/VIS

200 - 850

520

600

300

UB

UV

200 - 750

250 - 220*

1200

250

UC

UV

200 - 650

165 - 145*

1800

UV

UD

UV

200 - 580

115 - 70*

2400

UV

UE

UV

200 - 400

70 - 45*

3600

UV

UF

UV/VIS

250 - 850

520

600

400

BB

VIS/NIR

300 - 1160**

860**

300

500

VA

VIS

360 - 1000

500

600

500

VB

VIS

300 - 800

250 - 200*

1200

500

VC

VIS

350 - 750

145 - 100*

1800

500

VD

VIS

350 - 640

75 - 50*

2400

VIS

VE

NIR

500 - 1050

500

600

750

NB

NIR

500 - 1050

220 - 150*

1200

750

NC

NIR

600 - 1160

350 - 300

830

800

SI

NIR

600 - 1160**

560**

300

1000

IA

NIR

600 - 1160

500

600

1000

IB

* depends on the starting wavelength of the grating; the higher the wavelength, the bigger the dispersion and the smaller the range to select.
** please note that not all 2048 pixels will be used for the useable range.

Resolution Table (FWHM in nm)
Slit size (µm)
Grating (lines/mm)

10

25

50

100

200

500

300

1.40

1.50

2.5

4.8

9.2

21.3

600

0.70 - 0.80*

0.75 - 0.85*

1.2

2.4

4.6

10.8

830

0.42 - 0.48*

0.50 - 0.58*

0.93

1.7

3.4

8.5

1200

0.25 - 0.31*

0.37 - 0.43*

0.52 - 0.66*

1.1

2.3

5.4

1800

0.17 - 0.21*

0.26 - 0.32*

0.34 - 0.42*

0.8

1.6

3.6

2400

0.12 - 0.18*

0.18 - 0.24*

0.26 - 0.34*

0.44 - 0.64*

1.1

2.7

3600

0.09 - 0.12*

0.11 - 0.15*

0.19

0.4

0.8

1.8

* depends on the starting wavelength of the grating; the higher the wavelength, the bigger thedispersion and the better the resolution.

Options-RS
DCL-UV/VIS-200
SLIT-XX
SLIT-XX-RS
SLIT-XX-RS-FCPC• Replaceable slit
• Quartz detector collection lens (200 - 1100 nm)• Slit size, please specify XX = 10, 25, 50, 100, 200 or 500 µm• Replaceable slit with SMA connector , specify slit size XX = 25, 50, 100, 200 or 500 µm.
Only available with AvaSpec-ULS2048XL-EVO-RS• As SLIT-XX-RS, but with FC/PC connector

OSF-YYY• Order-sorting filter for reduction of second-order effects, 1 mm thick,please specify YYY= 305, 395, 475, 515, 550 or 600 nm

OSC• Order-sorting coating with 600 nm long-pass filter for BB (>350 nm)
and VB gratings, recommended with OSF-305

OSC-UA• Order-sorting coating with 350 and 600 nm linear variable filter for UA, VA gratings

OSC-UB• Order-sorting coating with 350 and 600 nm long-pass filter for UB or BB (<350 nm)
gratings-FCPC• FC/PC fiber-optic connector

info@avantes.com | www.avantes.com | 13

Spectrometers

AvaSpec-HS2048XL-EVO
SensLine Back-thinned CCD Spectrometer
AvaSpec-HS2048XL-EVO

For high-sensitivity applications wherehigh resolution is not of paramount concern,
the AvaSpec-HS2048XL-EVO is an
exceptional instrument. Featuring Avantes’
HS optical bench which has a full 0.22
numerical aperture for superior throughput,
the AvaSpec-HS2048XL has a back-thinned
CCD detector with 2048 pixels measuring
14X500 icrons.
Unlike many back-thinned CCD spectrometers, which have two dimensional
arrays, the HS2048XL has largemonolithic pixels with exceptional
efficiency in the UV, from 200-400 nm, andthe NIR, from 950-1160 nm, while retaining
sensitivity in the visible range.

The unique optical design features torroid
collimating and focusing mirrors to control
image magnification and enhance efficiency.
The instrument also features an electronic
shutter, which enables integration times as
low as 2 microseconds.
For configurations that require second-orderfiltering, order-sorting filters are available.
The AvaSpec-HS2048XL is available with awide range of slit sizes, gratings and may be
configured with SMA or FC/ PC fiber-optic
entrance connectors.entrance connectors.

Technical Data
Optical bench
Wavelength range

High-sensitivity asymmetrical design, 37.5 mm focal length; NA – 0.22, f/2.27
200 - 1160 nm

Resolution

1 - 20 nm, depending on configuration (see table)

Stray light<1%

Sensitivity

1,250,000 counts/µW per ms int. time

Detector

Back-thinned CCD image sensor 2048 pixels

Signal/noise

525:1

AD converter

16-bit, 1 MHz

Integration time
Interface
Dynamic range
Digital IO
Power supply
Dimensions, weight

2 µs – 600 seconds
USB 3.0 high-speed, 5 Gbps
Gigabit Ethernet, 1 Gbps
14,900HD-26 connector, 2 Analog in, 2 Analog out, 3 Digital in, 12 Digital out,
trigger, synchronization
Default USB power, 700 mA. or external 12VDC, 360 mA
175 x 165 x 85 mm, 1950 grams

Timing and Triggering
Sample speed with on-board averaging
Data transfer speed
Min. delay / jitter2.44 ms/scan
2.44 ms/scan (USB3)
0.37 µs / 25 ns

Detector Specifications
Sensitivity
photons/count@ 600 nmSensitivity
in cts/µW
per msint. time

QE(%) @ peak

Signal/noise

Dark noise(counts
RMS)

Dynamic
range

4

1,250,000

78%

525:1

5

14,900

14 | info@avantes.com | www.avantes.com

Grating Selection Table
Use

Useable range(nm)

Spectral range(nm)

UV/VIS/NIR

200 - 1160

UV/VIS

200 - 660

Lines/mm

Blaze (nm)Order code

900

500

330

HS500-0.33

440

1000

250

HS1000-0.25

UV

200 - 850

520

600

300

HS600-0.30

UV/VIS

200 - 850

520

600

400

HS600-0.40

UV/VIS

300 - 1160

860

500

560

HS500-0.56

VIS

360 - 1000

500

600

500

HS600-0.50

NIR

500 - 1050

500

600

750

HS600-0.75

VIS

350 - 850

460

900

550

HS900-0.55

VIS

400 - 722

322

1200

500

HS1200-0.5

NIR

600 - 1100

500

600

1000

HS600-1.0

NIR

600 - 1160

350

830

900

HS830-0.9

NIR

750 - 990

240

1200

1000

HS1200-1.0

Resolution table (FWHM in nm)
Slit size (µm)
Grating (lines/mm)

10

25

50

100

200

500

500

2.6

4.5

5.5

6.5

10.0

22.0

600

2.2

3.8

4.5

5.5

7.5

18.0

830*

2.1

3.6

4.0

5.0

7.0

15.0

900*

2.0

3.5

3.8

4.8

6.8

14.5

1000*

1.9

3.3

3.6

4.6

6.6

14.0

1.8

3.0

3.3

4.3

6.2

13.5

1200*

* theoretical values

Options
SLIT-XX• Slit size, please specify XX = 10, 25, 50, 100, 200 or 500 μm

OSF-YYY• Order-sorting filter for reduction of second-order effects, 1 mm thick,please specify YYY = 305, 385, 475, 515, 550 or 600 nm

OSC-HS500• Order-sorting coating with 350 and 600 nm long-pass filter for HS500 gratings
in AvaSpec-HS

OSC-HS600• Order-sorting coating with 350 and 600 nm long-pass filter for HS600 gratings
in AvaSpec-HS

OSC-HS900• Order-sorting coating with 600 nm long-pass filter for HS900 gratings in AvaSpec-HS

OSC-HS1000• Order-sorting coating with 350 nm long-pass filter for HS1000 gratings in AvaSpec-HS

FCPC• FC/PC fiber optic connector

The AvaSpec-HS2048XL-EVO is ideallysuited for diffuse reflection (UV, VIS, NIR)
measurements and fluorescence

info@avantes.com | www.avantes.com | 15

Spectrometers

AvaSpec-ULS2048x64TEC-EVO SensLine
Thermoelectrically Cooled Fiber-Optic Spectrometer
AvaSpec-ULS2048x64TEC-EVO

Available soon:
The AvaSpec-ULS2048x64TEC-EVO
is an updated version of our AvaSpecULS2048x64TEC spectrometer, withimproved electronics and cooling.

reduce the temperature of the CCD chip
to -30°C against ambient, improving thedark baseline and PRNU level significantly.
The detector cooling also reduces the darknoise by a factor of 2-3.

This instrument enhances the Sensline
series with its cooled, back-thinned
detector. The back-thinned detecor has
good sensitivity in the UV and IR region.
The 64 pixelheight (0.89 mm) enables
catching as many photons as possible
while the cooling enables long integration
times up to 120 seconds with low-noiselevels.

The AvaSpec-ULS2048x64TEC-EVO uses a
special low-noise version of the 2048x64
detector with integrated cooling.
All the features mentioned above makethis instrument ideally suited formeasuring low-light applications, such as
fluorescence or low-light Raman measurements.

The instrument features Peltier coolingdevice integrated into our exclusive ultralow stray light optical bench, which can

Optimal flexibility is guaranteed with thereplaceable slit, making the instrument
suitable for various kinds of applications.

Technical Data
Optical bench
Wavelength range

ULS Symmetrical Czerny-Turner, 75 mm focal length
200 - 1160 nm

Resolution

0.09 –20 nm, depending on configuration (see table)

Stray light<1%, depending on the grating

Sensitivity

300,000 counts/µW per ms integration time

Detector
Temperature-cooled CCD

Backthinned CCD, 2048x64 pixels, low noise, integrated coolingMax. ∆T = -30°C versus ambient. Optimal setting: 5°C

Signal/noise

550:1

AD converter

16-bit, 500 KHz

Dynamic range

19,000Dark noise

5 cntsIntegration time

9.7 ms – 120 s

InterfaceUSB 3.0 high speed, 5 Gbps
Gigabit Ethernet 1 Gbps

Digital IO

HD-26 connector, 2 Analog in, 2 Analog out, 13 Digital bidirectional, trigger,
sync., strobe, laser

Power supply
Dimensions, weight

12 VDC, 1.5 A
185 x 145 x 185 mm, 3500 grams

Timing and Triggering
Sample speed with on-board averaging

9.7 ms/scan

Data transfer speed

9.7 ms/scan

Min. delay / jitter

9.7 ms

Detector Specifications
Sensitivity
photons/count@ 600 nmSensitivity
in cts/µW
per msint. time

QE(%) @ peak

Signal/noise

Dark noise(counts
RMS)

Dynamic
range

5.9
4

1,250,000
300,000

78%

550:1
525:1

5

19,00014.90016 | info@avantes.com | www.avantes.com

Grating Selection Table
Use

Useable range(nm)

Spectral range(nm)

Lines/mm

Blaze (nm)Order code

UV/VIS/NIR

200-1160**

960**

300

300

UA

UV/VIS/NIR

200-1100**

900**

300

300/1000

UNA-DBUV/VIS

200-850

520

600

300

UB

UV

200-750250-220*

1200

250

UC

UV

200-650

165-145*

1800

UV

UD

UV

200-580

115-70*

2400

UV

UE

UV

200-400

70-45*

3600

UV

UF

UV/VIS

250-850

520

600

400

BB

VIS/NIR

300-1160**

860**

300

500

VA

VIS

360-1000

500

600

500

VB

VIS

300-800

250-200*

1200

500

VC

VIS

350-750

145-90*

1800

500

VD

VIS

350-640

75-50*

2400

VIS

VE

NIR

500-1050

500

600

750

NB

NIR

500-1050

220-150*

1200

750

NC

NIR

600-1160

350-300

830

800

SI

NIR

600-1160**

560**

300

1000

IA

NIR

600-1160

500

600

1000

IB

* depends on the starting wavelength of the grating; the higher the wavelength, the bigger the dispersion and the smaller the range to select.
** please note that not all 2048 pixels will be used for the useable range.

Resolution Table (FWHM in nm)
Slit size (µm)
Grating (lines/mm)

10

25

50

100

200

500

300

1.40

1.50

2.5

4.8

9.2

21.3

600

0.70-0.80*

0.75-0.85*

1.2

2.4

4.6

10.8

830

0.42-0.48*

0.50-0.58*

0.93

1.7

3.4

8.5

1200

0.25-0.31*

0.37-0.43*

0.52-0.66*

1.1

2.3

5.4

1800

0.17-0.21*

0.26-0.32*

0.34-0.42*

0.8

1.6

3.6

2400

0.12-0.18*

0.18-0.24*

0.26-0.34*

0.44-0.64*

1.1

2.7

0.09-0.12*

0.11-0.15*

0.19

0.4

0.8

1.8

3600

* depends on the starting wavelength of the grating; the higher the wavelength, the bigger thedispersion and the better the resolution.

Options
DCL-UV/VIS-200
SLIT-XX-RS
SLIT-XX-RS-FCPCOSF-YYY
OSC• Detector Collection Lens to enhance sensitivity, Quartz, 200-1100 nm• Replaceable slit with SMA connector. Specify slit size XX= 10, 25, 50, 100, 200 or 500 µm• As SLIT-XX-RS, but with FC/PC connector• Order-sorting filter for reduction of 2nd order effects, 1 mm thick,please specify YYY= 305, 395, 475, 515, 550 or 600 nm• Order-sorting coating with 600 nm long-pass filter for BB (>350 nm)
and VB gratings, recommended with OSF-305

OSC-UA• Order-sorting coating with linear variable filter for UA, VA gratings

OSC-UB• Order-sorting coating with 350 and 600 nm long-pass filter for UB or BB (<350 nm)
gratings

info@avantes.com | www.avantes.com | 17

Spectrometers

AvaSpec-ULS2048x64-EVO SensLine
High UV and NIR Sensitivity Spectrometer
Alongside the cooled AvaSpecULS2048x64TEC-EVO with low-noise
detector, Avantes also offers the morecost-effective, uncooled AvaSpecULS2048x64-EVO. With its standard
2048x64 backthinned CCD detector, thisspectrometer is perfect for less demanding
applications in the UV and NIR range.

AvaSpec-ULS2048x64-EVO

For applications that require integration
times lower than 2 seconds, the cooling
option is often not needed. For example,
this uncooled AvaSpec-ULS2048x64-EVO
has an established track record invarious DOAS applications all over theworld because of its high UV response
and 0.9 mm detector height that enables
detecting the wavelengths of interest.

Options include an order-sorting filter, toreduce second-order effects and purge
ports for deep-UV measurements. The
AvaSpec-ULS2048x64-EVO comes with awide range of slit sizes, gratings and canbe configured with SMA or FC/PC fiberoptic entrance connectors.
The AvaSpec-ULS2048x64-EVO uses theAS7010 electronics board offering USB3 (10times faster than USB2), Gigabit Ethernet
and better signal processing.
Connection to your PC is handled via USB3connection or Ethernet, delivering a scan
every 2 milliseconds. The instrument comescomplete with AvaSoft-basic software, USB
cable and an extensive manual.

Technical Data
Optical bench
Wavelength range

ULS, Symmetrical Czerny-Turner, 75 mm focal length
200 - 1160 nm

Resolution

0.09 –20 nm, depending on configuration (see table)

Stray light< 1%, depending on the grating

Sensitivity

650,000 counts/µW per ms int. time

Detector

Back-thinned CCD image sensor 2048x64 pixels (height: 0.89 nm)

Signal/noise

450:1

AD converter

16-bit, 1.33 MHz

Integration time
Interface

2.4 ms – 25 seconds
USB 3.0 high-speed, 5 Gbps
Gigabit Ethernet 1 Gbps

Readout noise

7.5 cnt RMS

Dark noise

11.5 cnt RMS

Dynamic range
Digital IO
Power supply
Dimensions, weight6100
HD-26 connector, 2 Analog in, 2 Analog out, 13 Digital bidirectional, trigger,
sync., strobe, laser
Default USB power, 885 mA. Or external 12VDC, 420 mA
175 x 127 x 44,5 mm (1 channel), 1180 grams

Timing and Triggering
Sample speed with on-board averaging

2.4 ms/scan

Data transfer speed

2.4 ms/scan

Min. delay / jitter

2.4 ms

Detector Specifications
Sensitivity
photons/count@ 600 nmSensitivity
in cts/µW
per msint. time

QE(%) @ peak

Signal/noise

Dark noise(counts
RMS)

Dynamic
range

3.9

650,000

78%

450:1

11.5

1600

18 | info@avantes.com | www.avantes.com

Grating Selection Table
Use

Useable range(nm)

Spectral range(nm)

Lines/mm

UV/VIS/NIR

200-1160**

960**

300

300

UA

UV/VIS/NIR

200-1100**

900**

300

300/1000

UNA-DBUV/VIS

200-850

520

600

300

UB

UV

200-750250-220*

1200

250

UC

UV

200-650

165-145*

1800

UV

UD

UV

200-580

115-70*

2400

UV

UE

UV

200-400

70-45*

3600

UV

UF

Blaze (nm)Order code

UV/VIS

250-850

520

600

400

BB

VIS/NIR

300-1160**

860**

300

500

VA

VIS

360-1000

500

600

500

VB

VIS

300-800

250-200*

1200

500

VC

VIS

350-750

145-100*

1800

500

VD

VIS

350-640

75-50*

2400

VIS

VE

NIR

500-1050

500

600

750

NB

NIR

500-1050

220-150*

1200

750

NC

NIR

600-1160

350-300

830

800

SI

NIR

600-1160**

560**

300

1000

IA

NIR

600-1160

500

600

1000

IB

* depends on the starting wavelength of the grating; the higher the wavelength, the bigger the dispersion and the smaller the range to select.
** please note that not all 2048 pixels will be used for the useable range.

Resolution Table (FWHM in nm)
Slit size (µm)
Grating (lines/mm)

10

25

50

100

200

500

300

1.40

1.50

2.5

4.8

9.2

21.3

600

0.70 - 0.80*

0.75-0.85*

1.2

2.4

4.6

10.8

830

0.42 - 0.48*

0.50-0.58*

0.93

1.7

3.4

8.5

1200

0.25 – 0.31*

0.37 – 0.43*

0.52-0.66*

1.1

2.3

5.4

1800

0.17 – 0.21*

0.26 – 0.32*

0.34-0.42*

0.8

1.6

3.6

2400

0.12 – 0.18*

0.18 – 0.24*

0.26-0.34*

0.44-0.64*

1.1

2.7

3600

0.09 – 0.12*

0.11 – 0.15*

0.19

0.4

0.8

1.8

* depends on the starting wavelength of the grating; the higher the wavelength, the bigger thedispersion and the better the resolution.

Options-RS
DCL-UV/VIS-200
SLIT-XX
SLIT-XX-RS
SLIT-XX-RS-FCPCOSF-YYY
OSC• Replaceable slit
• Quartz detector collection lens (200 - 1100 nm)• Slit size, please specify XX = 5, 10, 25, 50, 100, 200 or 500 µm• Replaceable slit with SMA connector , specify slit size XX = 25, 50, 100, 200 or 500 µm.
Only available for AvaSpec-ULS2048CL-EVO-RS• As SLIT-XX-RS, but with FC/PC connector• Order-sorting filter for reduction of second-order effects
please specify YYY = 305, 395, 475, 515, 550 or 600 nm• Order-sorting coating with 600 nm long-pass filter for BB (>305 nm)
and VB gratings, recommended with OSF-305

OSC-UA• Order-sorting coating with 350 and 600 nm linear variable filter for UA, VA gratings

OSC-UB• Order-sorting coating with 350 and 600 nm long-pass filter for UB or BB (<350 nm)
gratings-FCPC• FC/PC fiber-optic connector

info@avantes.com | www.avantes.com | 19

AvaSpec-ULS2048x64-EVO SensLine High UV and NIR
Sensitivity Back-thinned CCD Spectrometer
Alongside the cooled AvaSpecULS2048x64TEC-EVO with low-noise
detector, Avantes also offers the morecost-effective, uncooled AvaSpecULS2048x64-EVO. With its standard
2048x64 backthinned detector, thisspectrometer is perfect for less demanding
applications in the UV and NIR range.
For applications that require integration
times lower than 2 seconds, the cooling
option is often not needed. For example,
this uncooled AvaSpec-ULS2048x64-EVO has
an established track record in various DOAS
applications all over the world because of
its high UV response and 0.9 mm detector
height that enables detecting the
wavelengths of interest.

Options include an order-sorting filter, toreduce second-order effects and purge ports
for deep-UV measurements. The AvaSpecULS2048x64-EVO comes with a wide rangeof slit sizes, gratings and can be configured
with SMA or FC/PC fiber-optic entrance connectors.

AvaSpec-ULS2048x64-EVO

The AvaSpec-ULS2048x64-EVO uses theAS7010 electronics board offering USB3 (10times faster than USB2), Gigabit Ethernet
and better signal processing.
Connection to your PC is handled via USB3connection or Ethernet, delivering a scan
every 2 milliseconds. The instrument comescomplete with AvaSoft-basic software, USB
cable and an extensive manual.

Technical Data
Optical bench
Wavelength range

ULS, Symmetrical Czerny-Turner, 75 mm focal length
200 - 1160 nm

Resolution

0.09 –20 nm, depending on configuration (see table)

Stray light< 1%, depending on the grating

Sensitivity

650,000 counts/µW per ms int. time

Detector

Back-thinned CCD image sensor 2048x64 pixels (height: 0.89 nm)

Signal/noise

450:1

AD converter

16-bit, 1.33 MHz

Integration time
Interface

2.4 ms – 25 seconds
USB 3.0 high-speed, 5 Gbps
Gigabit Ethernet 1 Gbps

Sample speed with on-board averaging

2.4 ms/scan

Readout noise

7.5 cnt RMS

Dark noise

11.5 cnt RMS

Dynamic range
Data transfer speed
Digital IO
Power supply
Dimensions, weight6100
2.4 ms/scan (USB3)
HD-26 connector, 2 Analog in, 2 Analog out, 13 Digital bidirectional, trigger,
sync., strobe, laser
Default USB power, 885 mA. Or external 12VDC, 420 mA
177 x 127 x 44,5 mm (1 channel), 1180 grams

info@avantes.com | www.avantes.com | 1

09-2019

Grating Selection Table for AvaSpec-ULS2048x64-EVO

Spectrometers

Use

Useable range(nm)

Spectral range(nm)

Lines/mm

UV/VIS/NIR

200-1160**

960**

300

300

UA

UV/VIS/NIR

200-1100**

900**

300

300/1000

UNA-DBUV/VIS

200-850

520

600

300

UB

UV

200-750250-220*

1200

250

UC

UV

200-650

165-145*

1800

UV

UD

UV

200-580

115-70*

2400

UV

UE

Blaze (nm)Order code

UV

200-400

70-45*

3600

UV

UF

UV/VIS

250-850

520

600

400

BB

VIS/NIR

300-1160**

860**

300

500

VA

VIS

360-1000

500

600

500

VB

VIS

300-800

250-200*

1200

500

VC

VIS

350-750

145-100*

1800

500

VD

VIS

350-640

75-50*

2400

VIS

VE

NIR

500-1050

500

600

750

NB

NIR

500-1050

220-150*

1200

750

NC

NIR

600-1160

350-300

830

800

SI

NIR

600-1160**

560**

300

1000

IA

NIR

600-1160

500

600

1000

IB

* depends on the starting wavelength of the grating; the higher the wavelength, the bigger the dispersion and the smaller the range to select.
** please note that not all 2048 pixels will be used for the useable range

Resolution Table (FWHM in nm) for AvaSpec-ULS2048x64EVO
Slit size (µm)
Grating (lines/mm)
300

10

25

50

100

200

500

1.40

1.50

2.5

4.8

9.2

21.3

600

0.70 - 0.80*

0.75-0.85*

1.2

2.4

4.6

10.8

830

0.42 - 0.48*

0.50-0.58*

0.93

1.7

3.4

8.5

1200

0.25 – 0.31*

0.37 – 0.43*

0.52-0.66*

1.1

2.3

5.4

1800

0.17 – 0.21*

0.26 – 0.32*

0.34-0.42*

0.8

1.6

3.6

2400

0.12 – 0.18*

0.18 – 0.24*

0.26-0.34*

0.44-0.64*

1.1

2.7

0.09 – 0.12*

0.11 – 0.15*

0.19

0.4

0.8

1.8

3600

* depends on the starting wavelength of the grating; the higher the wavelength, the bigger thedispersion and the better the resolution

Ordering Information
AvaSpec-ULS2048x64-EVO• Ultra-low Stray-light Fiber-optic Spectrometer, 75 mm AvaBench, 2048x64 pixel backthinned CCD detector, USB powered, high-speed USB3.0 and ETH interface, incl. AvaSoftBasic, USB interface cable.
Specify grating, wavelength range and options

Options-RS
DCL-UV/VIS-200
SLIT-XX
SLIT-XX-RS
SLIT-XX-RS-FCPCOSF-YYY
OSC• Replaceable slit
• Quartz detector collection lens (200 - 1100 nm)• Slit size, please specify XX = 5, 10, 25, 50, 100, 200 or 500 µm• Replaceable slit with SMA connector , specify slit size XX = 25, 50, 100, 200 or 500 µm.
Only available for AvaSpec-ULS2048CL-EVO-RS• As SLIT-XX-RS, but with FC/PC connector• Order-sorting filter for reduction of second-order effects
please specify YYY = 305, 395, 475, 515, 550 or 600 nm• Order-sorting coating with 600 nm long-pass filter for BB (>305 nm)
and VB gratings, recommended with OSF-305

OSC-UA• Order-sorting coating with 350 and 600 nm linear variable filter for UA, VA gratings

OSC-UB• Order-sorting coating with 350 and 600 nm long-pass filter for UB or BB (<350 nm)
gratings-FCPC• FC/PC fiber-optic connector

www.phototechnica.co.jp〒336-0017 埼玉県さいたま市南区南浦和 1-2-17

TEL:048-871-0067

FAX:048-871-0068

e-mail:voc@phototechnica.co.jp

AvaSpec-ULS2048x64TEC-EVO SensLine
Thermoelectrically Cooled Fiber-Optic Spectrometer
AvaSpec-ULS2048x64TEC-EVO

The AvaSpec-ULS2048x64TEC-EVO
is an updated version of our AvaSpecULS2048x64TEC spectrometer, withimproved electronics and cooling.

The AvaSpec-ULS2048x64TEC-EVO uses a
special low-noise version of the 2048x64
detector with integrated cooling.

This instrument enhances the Sensline series
with its cooled, back-thinned
detector. The back-thinned detecor has goodsensitivity in the UV and IR region.
The 64 pixelheight (0.89 mm) enables catching as many photons as possible while thecooling enables long integration times up to
120 seconds with low-noise levels.
The instrument features Peltier coolingdevice integrated into our exclusive ultra-low
stray light optical bench, which can reduce
the temperature of the CCD chip to -30°C
against ambient, improving the dark baseline and PRNU level significantly. The detector cooling also reduces the dark noise by afactor of 2-3.

All the features mentioned above make this
instrument ideally suited formeasuring low-light applications, such as
fluorescence or low-light Raman measurements.
Optimal flexibility is guaranteed with thereplaceable slit, making the instrument
suitable for various kinds of applications.
The above mentioned qualities make the
AvaSpec-ULS2048x64TEC-EVO an excellent
choice for low light-level applications, suchas fluorescence and Raman measurements,
where integration times of more than 5 seconds may be needed.

Technical Data
Optical bench
Wavelength range

ULS Symmetrical Czerny-Turner, 75 mm focal length200-1160 nm

Resolution

0.09 –20 nm, depending on configuration (see table)

Stray light<1%, depending on the grating

Sensitivity

300,000 counts/µW per ms integration time

Detector
Temperature-cooled CCD

Backthinned CCD, 2048x64 pixels, low noise, integrated coolingMax. ∆T = -30°C versus ambient. Optimal setting: 5°C

Signal/noise

550:1

AD converter

16-bit, 500 KHz

Dynamic range

19,000Dark noise

5 cntsIntegration time
InterfaceSample speed with on-board averaging
Data transfer speed
Digital IO
Power supply
Operating temperature
Cooling
Dimensions, weight

9.7 ms–120 s
USB 3.0 high speed, 5 Gbps
Gigabit Ethernet 1 Gbps
9.7 ms/scan
9.7 ms/scan (USB3)
9.7 ms/scan (ETH)
HD-26 connector, 2 Analog in, 2 Analog out, 13 Digital bidirectional, trigger,
sync., strobe, laser
12 VDC, 1.5 A
0-40°C
30°C versus ambient
185 x 145 x 185 mm, 3500 grams

info@avantes.com | www.avantes.com | 45

Grating Selection Table for AvaSpec-ULS2048x64TEC-EVO

Spectrometers

Useable range
(nm)

Use

Spectral range(nm)

Lines/mm

Blaze (nm)Order code

UV/VIS/NIR

200-1160**

960**

300

300

UA

UV/VIS/NIR

200-1100**

900**

300

300/1000

UNA-DBUV/VIS

200-850

520

600

300

UB

UV

200-750250-220*

1200

250

UC

UV

200-650

165-145*

1800

UV

UD

UV

200-580

115-70*

2400

UV

UE

UV

200-400

70-45*

3600

UV

UF

UV/VIS

250-850

520

600

400

BB

VIS/NIR

300-1160**

860**

300

500

VA

VIS

360-1000

500

600

500

VB

VIS

300-800

250-200*

1200

500

VC

VIS

350-750

145-90*

1800

500

VD

VIS

350-640

75-50*

2400

VIS

VE

NIR

500-1050

500

600

750

NB

NIR

500-1050

220-150*

1200

750

NC

NIR

600-1160

350-300

830

800

SI

NIR

600-1160**

560**

300

1000

IA

NIR

600-1160

500

600

1000

IB

* depends on the starting wavelength of the grating; the higher the wavelength, the bigger the dispersion and the smaller the range to select.
** please note that not all 2048 pixels will be used for the useable range

Resolution Table (FWHM in nm) for AvaSpec-ULS2048x64TEC
Slit size (µm)
Grating (lines/mm)

10

25

50

100

200

500

300

1.40

1.50

2.5

4.8

9.2

21.3

600

0.70-0.80*

0.75-0.85*

1.2

2.4

4.6

10.8

830

0.42-0.48*

0.50-0.58*

0.93

1.7

3.4

8.5

1200

0.25-0.31*

0.37-0.43*

0.52-0.66*

1.1

2.3

5.4

1800

0.17-0.21*

0.26-0.32*

0.34-0.42*

0.8

1.6

3.6

2400

0.12-0.18*

0.18-0.24*

0.26-0.34*

0.44-0.64*

1.1

2.7

3600

0.09-0.12*

0.11-0.15*

0.19

0.4

0.8

1.8

* depends on the starting wavelength of the grating; the higher the wavelength, the bigger thedispersion and the better the resolution

Ordering Information
AvaSpec-ULS2048x64TEC-EVO

Thermoelectrically cooled fiber-optic spectrometer, 75 mm ultra-low stray light AvaBench,
2048x64 pixel, TE-cooled and regulated low-noise CCD detector, USB3/ETH high-speed
interface and replaceable slit, incl. AvaSoft-Basic, USB cable, desktop housing. Specify
grating, wavelength range and options

Options
DCL-UV/VIS-200
SLIT-XX-RS
SLIT-XX-RS-FCPCOSF-YYY
OSC• Detector Collection Lens to enhance sensitivity, Quartz, 200-1100 nm• Replaceable slit with SMA connector. Specify slit size XX= 10, 25, 50, 100, 200 or 500 µm• As SLIT-XX-RS, but with FC/PC connector• Order-sorting filter for reduction of 2nd order effects, 1 mm thick,please specify YYY= 305, 395, 475, 515, 550 or 600 nm• Order-sorting coating with 600 nm long-pass filter for BB (>350 nm)
and VB gratings, recommended with OSF-305

OSC-UA• Order-sorting coating with linear variable filter for UA, VA gratings

OSC-UB• Order-sorting coating with 350 and 600 nm long-pass filter for UB or BB (<350 nm)
gratings

www.phototechnica.co.jp〒336-0017 埼玉県さいたま市南区南浦和 1-2-17

TEL:048-871-0067

FAX:048-871-0068

e-mail:voc@phototechnica.co.jp

Spectrometers

AvaSpec-NIR256/512-1.7-EVO
NIRLine Near-Infrared Spectrometer
AvaSpec-NIR256/512-1.7-EVO

The AvaSpec-NIR256/512-1.7-EVO
spectrometers pair the same trusted
InGaAs array detectors with our ultra
low-noise electronics board featuringUSB3 and Giga-Ethernet connection
port. Digital and analog I/O ports
enable external triggering and control
over the shutter and pulsed lightsources
and choose from two distinct softwarecontrolled gain-setting modes,
high-sensitivity mode (HS, default) andthe low-noise (LN) mode.

For measurements in the near-infrared
range out to 1.7 μm, Avantes offers a
new series of uncooled spectrometer
configurations. The AvaSpec-NIR2561.7-EVO and the AvaSpec-NIR512-1.7EVO offer the same high-sensitivity
optical bench with the next generationof electronics. Both instruments deliver
the same exceptional performance
specifications such as a sample speedof only 0.53 ms/scan and integration
times as fast as 20 μs, as the Avantes
instruments you have come to trust.

These affordable, uncooled instruments
are USB powered and are available
with a choice of four gratings andreplaceable slits to match the bandwith
and requirements fitting yourapplication.

For applications where resolution iskey, or more datapoints for modellingare required, the 512 pixel detector willbe the best choice.

Technical Data
AvaSpec-NIR256-1.7-EVO
Optical bench

AvaSpec-NIR512-1.7-EVO

Symmetrical Czerny-Turner, 50 mm focal length,
900-1750 nm

Wavelength range

2 - 50 nm

Resolution (slit & grating dependent)<1%

Stray lightSensitivity HS in counts /µW per ms

8,200,000(integral 1000-1750 nm)

3,800,000(integral 1000-1750 nm)

Dynamic range HS

6000:1

Integration time HS

20 µs – 500 ms
1900:1Signal/noise HS
Sensitivity LN in counts /µW per ms

469,000(integral 1000-1750 nm)

222,000(integral 1000-1750 nm)

Dynamic range LN

9000:1

Integration time LN

20 µs – 20 seconds
5000:1Signal/noise LN
Detector
AD converter
InterfaceSample speed with on-board averaging
Data transfer speed
Digital IO
Power supply
Dimensions, weight

InGaAs linear array,
256 pixels, 50 µm x 500 µm

InGaAs linear array,
512 pixels, 25 µm x 500 µm

16-bit, 500 kHz

16-bit, 500 kHz

USB3.0 high speed, 5 Gbps, Gigabit Ethernet 1 Gbps
0.53 ms/scan
0.53 ms/scan (USB3)
HD-26 connector, 2 Analog in, 2 Analog out, 13 Digital IO bi-directional,
trigger, synchronization, strobe, laser
Default USB power, 600 mA or
external 12VDC, 320mA (4W)
185 x 100 x 184 mm, 2700 grams

20 | info@avantes.com | www.avantes.com

Grating Selection Table
Use

Useablerange (nm)Spectral range(nm)

Lines/mm

Blaze (nm)Order code

NIR

900 - 1750

850

200

1500

NIR200-1.5

NIR1000 - 1700

340

400

1600

NIR400-1.6

NIR

900 - 1400

200

600

1200

NIR600-1.2

NIR1300 - 1600

152

600

1600

NIR600-1.6

Resolution Table (FWHM in nm)
Slit size (µm)
Grating (lines/mm)

25*

50

100

200

500

200

6

8

12

22

50

400

2.5

3

6

12

25

600

n.a.

2

4

8

18

							* only for AvaSpec-NIR512

Options
SLIT-XX-RS
SLIT-XX-RS-FCPC• Replaceable slit with SMA connector, specify slit size XX = 25*, 50, 100 or 200 µm• As SLIT-XX-RS, but with FC/PC connector							For external triggering, Avantes offers the AvaTrigger;
featuring optical triggering, an external TTL
and manual triggering through the push of a button.

info@avantes.com | www.avantes.com | 21

* only for AvaSpec-NIR512

Spectrometers

AvaSpec-NIR256/512-1.7-HSC-EVO
NIRLine Near-Infrared Spectrometer
AvaSpec-NIR256-1.7-HSC-EVO

trusted InGaAs array detectors with
our ultra-low-noise electronics board,
featuring USB3 and Giga-Ethernet
connection port.

For measurements in the near-infrared
range up to 1.7 μm, Avantes offers a
new series of cooled spectrometer
configurations. The AvaSpec-NIR2561.7-HSC-EVO and the AvaSpec-NIR5121.7-HSC-EVO offer the high-sensitivity,
100mm optical bench (HSC) with thenext generation of electronics.

The instruments are
standard equiped with areplaceable slit. Digital and analog I/O
ports enable external triggering andcontrol over the shutter and pulsed
lightsources and the choice between
two distinct software-controlled gainsetting
modes, high-sensitivity mode
(HS, default) and the low-noise mode
(LN).

Both instruments deliver exceptional
performance specifications, such asa high sample speed and integration
times as fast as 20 μs, as the Avantes
instruments you have come to trust.
For applications where resolution iskey, or more datapoints for modellingare required, the 512 pixel detector willbe the best choice.

Cooling ensures optimal noise
condition even at longer integration
times. All NIR-1.7 instruments offer
four different gratings, making it
possible to choose the bandwidth
fitting your application.

The AvaSpec-NIR256/512-1.7-HSC-EVO
spectrometers pair the same

Technical Data
AvaSpec-NIR256-1.7-HSC-EVO
Optical bench

900 - 1750 nm

Wavelength range
Resolution (slit & grating dependent)

AvaSpec-NIR512-1.7-HSC-EVO

Symmetrical Czerny-Turner, 100 mm focal length,
1 stage TE-cooled

1.9 - 32 nm

1.7 - 32 nm<1%

Stray lightSensitivity HS in counts /µW per
ms

4,800,000(integral 1000-1750 nm)

2,500,000(integral 1000-1750 nm)

Dynamic range HS

4900:1Signal/noise HS

5000:120 µs – 500 ms

Integration time HS
Sensitivity LN in counts /µW per
ms

160,000(integral 1000 - 1750 nm)

83,000(integral 1000 - 1750 nm)

Dynamic range LN

7600:1Signal/noise LN

5000:120 µs – 20 seconds

Integration time LN
Detector
AD converter

TE-cooled InGaAs linear array,
256 pixels, 50 µm x 500 µm

TE-cooled InGaAs linear array,
512 pixels, 25 µm x 500 µm

16-bit, 1,2 MHz

16-bit, 1,2 MHz

InterfaceUSB3.0 high speed, 5 Gbps, Gigabit Ethernet 1 Gbps

Digital IO

HD-26 connector, 2 Analog in, 2 Analog out, 13 Digital IO bi-directional,
trigger, synchronization, strobe, laser
12VDC, 12W

Power supply

185 x 160 x 184 mm, 3.6 kg

Dimensions, weight

Timing and Triggering
Sample speed with on-board averaging
Data transfer speed
Min. delay / jitter

0.13 ms/scan

0.24 ms/scan (USB3)

0.4 ms/scan (USB3)

0.53 ms/scan (USB3)
4.92 µs / 0.38 ns

22 | info@avantes.com | www.avantes.com													Grating Selection Table
Use

Useable range(nm)

Spectral range
(nm)

NIR

900 - 1700

NIR
NIR
NIR

Lines/mm

Blaze (nm)Order code

800 - 660*

150

1250

NIR150-1.2

994 - 1280

278

300

1200

NIR300-1.2

950 - 1800

262 - 230*

400

1200

NIR400-1.2

960 - 1800

262 - 230*

400

1600

NIR400-1.6

256/512													 * only for AvaSpec-NIR512

Resolution Table (FWHM in nm)
Slit size (µm)
Grating (lines/mm)

25*

50

100

200

500

150

4.0

5.7

7.0

12.8

32

300

1.8

2.3

3.0

4.0

10

400

1.7

1.9

2.5

3.3

8.3

Options
SLIT-XX-RS
SLIT-XX-RS-FCPC• Replaceable slit with SMA connector, specify slit size XX = 25*, 50, 100 ,200 or 500 µm• as SLIT-XX-RS, but with FC/PC connector* only for AvaSpec-NIR512

For external triggering, Avantes offers the AvaTrigger;
featuring optical triggering, an external TTL
and manual triggering through the push of a button.

info@avantes.com | www.avantes.com | 23

Spectrometers

AvaSpec-NIR256/512-2.5-HSC-EVO
NIRLine Near-infrared Spectrometer
AvaSpec-NIR256-2.5-HSC-EVO

For applications where resolution is
key or more datapoints for modellingare required, the 512 pixel detector willbe the best choice.

The NIR spectrometers in our EVO
series offer more sensitivity, lowweight and small size. They are basedon a 100 mm optical bench with an
NA of 0.13, offering optimal balance
between resolution and sensitivity.

Also available on the –HSC is the user
selectable gain-setting mode: LN (lownoise,standard setting), which gives
you a longer integration time andhigher signal to noise ratio, and HS
mode (high-sensitivity) for measuring
in low light conditions. Analog anddigital IO ports enable external
triggering and control of shuttered andpulsed light sources from the AvaLight
series.

The 2.5-HSC series feature 256 or 512
pixel InGaAs detectors and areavailable in multiple configurations.
These instruments are perfect foranalyzing grain, corn, wheat, soya,
polymers, but also for medical uses,
process monitoring and otheranalyses.
The 256 pixel detectors offer the best
sensitivity for most applications.

Technical Data
AvaSpec-NIR256-2.5-HSC-EVO
Optical benchTE-cooled symmetrical Czerny Turner, 100 mm focal length
1000 - 2500 nm

Wavelenght range
Resolution
Pixel dispersion (with NIR 075-1.7 grating)

AvaSpec-NIR512-2.5-HSC-EVO

4.4 - 85.0 nm

2.6 - 85.0 nm

6.2 nm

3.1 nmStray light<1.0%

Sensitivity HS in counts / µW per ms(1000 - 2500 nm)

990,000

Signal/noise HS

1800:1

480,000
1900:1
10 µs - 5 ms

Integration time HS
Sensitivity LN in counts / uW per ms(1000 - 2500 nm)

55,00026,600Signal/noise LN

4000:1

3700:1
10 µs - 100 ms

Integration time LN
Detector
Pixel size (WxH)
AD converter
InterfaceSample speed with on-board averaging
Data transfer speed
Digital IO

InGaAs linear array with 2-stage
TE-cooling, 256 pixel

InGaAs linear array with 2-stage
TE-cooling, 512 pixel

50 x 250 µm

25 x 250 µm
16 bit, 500 kHz
USB 3.0 high speed, 5 Gbps
Gigabit Ethernet 1 Gbps
0.54 ms/scan (USB3)
1.11 ms/scan (USB3)

HD-26 connector, 2 Analog in, 2 Analog out, 13 Digital bi-directional, trigger, sync,
strobe, laser

Power supply

12 V, 40W

Operating temperature range

0 - 40 °C

Cooling
Dimensions, weight

45 °C versus ambient
185 x 145 x 185 mm, 3.5 kg

24 | info@avantes.com | www.avantes.com

Grating Selection Table
Use

Useable range
(nm)

NIR

1000 - 2500

NIR

1000 - 2500

Spectral range(nm)

Lines/mm

Blaze (nm)Order code

1500

75

1700

NIR075-1.7

1173 - 1150*

100

2500

NIR100-2.5

NIR1000 - 2500

800 - 660*

150

2000

NIR150-2.0

NIR1000 - 2500

815 - 700*

150

2600

NIR150-2.6

NIR1000 - 2500

574 - 530*

200

1500

NIR200-1.5*Depends on the starting wavelength of the grating; the higher the wavelength, the bigger the dispersion and the smaller the range to select.

Resolution Table (FWMH in nm)
Slit size (µm)
Grating (lines/mm)

25*

50

100

200

500

75

8.9

12.9

16.0

33.9

84.5

100

7.2

9.5

12.0

20.0

50.0

150

4.0

5.7

7.0

12.8

32.0

200

2.6

4.4

5.2

9.3

23.3

Options
SLIT-XX-RS• Slit size, please specify XX = 25, 50, 100, 200 or 500 μm

This instrument is perfect for grain, corn, wheat, soya and other analyses.

info@avantes.com | www.avantes.com | 25

Spectrometers

Detector Specifications
StarLine & SensLine

StarLine and SensLine Detectors

Detector Specifications (based on a 16-bit AD converter)
StarLine

SensLine

HAM-2048CL

HAM-4096CL

SONY-2048L

HAM-2048XL

HAM-1024x58

CMOS linear array

CMOS linear array

CCD linear array

Back-thinned
CCD array

Cooled Back-thinned
CCD array2048, 14 µm

4096, 7 µm

2048, 14 µm

2048, 14 µm

1024 x 58, 24 µm

Pixel width x height(µm)

14 x 200

7 x 200

14 x 200

14 x 500

24 x 24(total height 1.4 mm)

Pixel well depth(electrons)

80,00080,00090,000200,000

1,000,000

Sensitivity
Photons/
count @600 nm

2

2

4

4

16

375,000(AvaSpecULS2048CL)

218,000(AvaSpecULS4096CL)

470,000(AvaSpecULS2048L)

460,000(AvaSpecULS2048XL)

445,000(AvaSpec-HERO)

Peak wavelength

700 nm

700 nm

450 nm

650 nm

650 nmQE (%) @ peak

80%

80%

40%

78%

92%

Signal/Noise

300:1

335:1

300 :1525 :1

1200:1

Dark noise (counts
RMS)

16

16

20

5

2

Dynamic Range

4000

4000

3300

3800

40000

Photo-responsive
non-uniformity

± 5%

± 5%

± 5%

± 3%

± 3%

Wavelength range(nm)

200 - 1100

200 - 1100

200* - 1100

200 - 1160

200 - 1160

6 MHz

6 MHz

2 MHz

1 MHz

250 kHz

Detector

Type# Pixels, pitch

Sensitivity
in counts/µW per
ms integration time

Frequency							 * DUV coating

26 | info@avantes.com | www.avantes.com

Detector Specifications
NIRLineNIRLine Detectors

Detector Specifications (NIR)
NIRLineDetector

HAM-256-1.7

HAM-512-1.7

SU-256-1.7

SU-512-1.7

HAM-256-2.5

HAM-512-2.5

TypeLinear InGaAs
array

Linear InGaAs
array

Linear InGaAsarraywith 1-stage TE
cooling

Linear InGaAsarraywith 1-stage TE
cooling

Linear InGaAsarraywith 2-stage TE
cooling

Linear InGaAsarraywith 2-stage TE
cooling# Pixels, pitch

256, 50 µm

512, 25 µm

256, 50 µm

512, 25 µm

256, 50 µm

512, 25 µm

pixel width x height(µm)

50 x 500

25 x 500

50 x 500

25 x 500

50 x 250

25 x 250

Sensitivity HS
in counts/µW per ms

8,200,000(integral 1000 1750 nm)

3,880,000(integral 1000 170 nm)

4,800,000(integral 1000 1750 nm)

2,500,000(integral 1000 1750 nm)

990,000(integral 1000 2500 nm)

480,000(integral 1000 2500 nm)

1900:1

1900:1

5000:1

5000:1

1800:1

1900:1

Dark noise HS(counts RMS)

16

16

16

16

16

15

Dynamic Range HS

6000

6000

4900

4900

3500

4300

Sensitivity LN
in counts/µW per ms

469,000(integral 1000 1750 nm)

222,000(integral 1000 1750 nm)

160,000(integral 1000 1750 nm)

83,000(integral 1000 1750 nm)

55,000(integral 1000 2500 nm)

26,600(integral 1000 2500 nm)

5000:1

5000:1

5000:1

5000:1

4000:1

3700:1

12

12

12

12

12

13

Signal/Noise (HS)Signal/Noise (LN)
Dark noise LN(counts RMS)
Dynamic Range LN

9000

9000

7600

7600

4500

5100

Peak wavelength1550 nm

1550 nm

1500 nm

1500 nm2300 nm2300 nmQE (%) @ peak

90%

90%

70%

70%

65%

65%

Photo-responsive
non-uniformity

± 5%

± 5%

10%

10%

± 5%

± 5%

Defective pixels
(max)

0

0

0

0

12

26

Wavelength range(nm)

900 - 1750

900 - 1750

900 - 1750

900 - 1750

1000 - 2500

1000 - 2500

Frequency

500 kHz500 kHz

1.2 MHz

1.2 MHz500 kHz500 kHz

info@avantes.com | www.avantes.com | 27

Spectrometers

Sensitivity Curve StarLine

Sensitivity Curve SensLine

www.phototechnica.co.jp〒336-0017 埼玉県さいたま市南区南浦和 1-2-17

TEL:048-871-0067

FAX:048-871-0068

e-mail:voc@phototechnica.co.jp

09-201928 | info@avantes.com | www.avantes.com