Opening the dynamic infrared sky

Jamie Soon; Anna M. Moore; Mansi M. Kasliwal; Ryan M. Lau; Kishalay De; Tony D. Travouillon; Mike I. Jones; Eran Ofek; Roger Smith; Valery Terebizh; Dan McKenna; David Hale; Alexandre Delacroix; Scott M. Adams; Jacob E. Jencson; Michael Ashley; Jill Burnham; Jennifer L. Sokoloski; Joss Bland-Hawthorn; Ken C. Freeman; Orsola De Marco; Jeff Cooke; Philip Bland; Stuart Ryder; Roberto Soria; Jarek Antoszewski; Alexander Heger; Lee Spitler; Robert Simcoe

doi:10.1117/12.2312731

Opening the dynamic infrared sky

Jamie Soon^*, Anna M. Moore, Mansi M. Kasliwal, Ryan M. Lau, Kishalay De, Tony D. Travouillon, Mike I. Jones, Eran Ofek, Roger Smith, Valery Terebizh, Dan McKenna, David Hale, Alexandre Delacroix, Scott M. Adams, Jacob E. Jencson, Michael Ashley, Jill Burnham, Jennifer L. Sokoloski, Joss Bland-Hawthorn, Ken C. FreemanOrsola De Marco, Jeff Cooke, Philip Bland, Stuart Ryder, Roberto Soria, Jarek Antoszewski, Alexander Heger, Lee Spitler, Robert Simcoe

^*Corresponding author for this work

Research output: Chapter in Book/Report/Conference proceeding › Conference proceeding contribution › peer-review

2 Citations (Scopus)

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Abstract

While optical and radio transient surveys have enjoyed a renaissance over the past decade, the dynamic infrared sky remains virtually unexplored from the ground. The infrared is a powerful tool for probing transient events in dusty regions that have high optical extinction, and for detecting the coolest of stars that are bright only at these wavelengths. The fundamental roadblocks in studying the infrared time-domain have been the overwhelmingly bright sky background (250 times brighter than optical) and the narrow field-of-view of infrared cameras (largest is VISTA at 0.6 sq deg). To address these challenges, Palomar Gattini-IR is currently under construction at Palomar Observatory and we propose a further low risk, economical, and agile instrument to be located at Siding Spring Observatory, as well as further instruments which will be located at the high polar regions to take advantage of the low thermal sky emission, particularly in the 2.5 micron region.

Original language	English
Title of host publication	Ground-Based and Airborne Telescopes VII
Editors	Heather K. Marshall, Jason Spyromilio
Place of Publication	Bellingham, Washington
Publisher	SPIE
Pages	107004D-1-107004D-12
Number of pages	12
ISBN (Electronic)	9781510619548
ISBN (Print)	9781510619531
DOIs	https://doi.org/10.1117/12.2312731
Publication status	Published - 6 Jul 2018
Event	Ground-Based and Airborne Telescopes VII 2018 - Austin, United States Duration: 10 Jun 2018 → 15 Jun 2018

Publication series

Name	Proceedings of SPIE
Publisher	SPIE
Volume	10700
ISSN (Print)	0277-786X
ISSN (Electronic)	1996-756X

Conference

Conference	Ground-Based and Airborne Telescopes VII 2018
Country/Territory	United States
City	Austin
Period	10/06/18 → 15/06/18

Bibliographical note

Copyright 2018 Society of Photo-Optical Instrumentation Engineers (SPIE). One print or electronic copy may be made for personal use only. Systematic reproduction and distribution, duplication of any material in this paper for a fee or for commercial purposes, or modification of the content of the paper are prohibited.

Keywords

all-sky survey
Antarctica
DREAMS
Gattini-IR
infrared
Palomar Observatory
polar regions
Siding Spring Observatory

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10.1117/12.2312731

Publisher version (open access)Final published version, 1.23 MBLicence: Other

Cite this

Soon, J., Moore, A. M., Kasliwal, M. M., Lau, R. M., De, K., Travouillon, T. D., Jones, M. I., Ofek, E., Smith, R., Terebizh, V., McKenna, D., Hale, D., Delacroix, A., Adams, S. M., Jencson, J. E., Ashley, M., Burnham, J., Sokoloski, J. L., Bland-Hawthorn, J., ... Simcoe, R. (2018). Opening the dynamic infrared sky. In H. K. Marshall, & J. Spyromilio (Eds.), Ground-Based and Airborne Telescopes VII (pp. 107004D-1-107004D-12). Article 107004D (Proceedings of SPIE; Vol. 10700). SPIE. https://doi.org/10.1117/12.2312731

@inproceedings{340a4d995b214e70abbd7cff28215952,

title = "Opening the dynamic infrared sky",

abstract = "While optical and radio transient surveys have enjoyed a renaissance over the past decade, the dynamic infrared sky remains virtually unexplored from the ground. The infrared is a powerful tool for probing transient events in dusty regions that have high optical extinction, and for detecting the coolest of stars that are bright only at these wavelengths. The fundamental roadblocks in studying the infrared time-domain have been the overwhelmingly bright sky background (250 times brighter than optical) and the narrow field-of-view of infrared cameras (largest is VISTA at 0.6 sq deg). To address these challenges, Palomar Gattini-IR is currently under construction at Palomar Observatory and we propose a further low risk, economical, and agile instrument to be located at Siding Spring Observatory, as well as further instruments which will be located at the high polar regions to take advantage of the low thermal sky emission, particularly in the 2.5 micron region.",

keywords = "all-sky survey, Antarctica, DREAMS, Gattini-IR, infrared, Palomar Observatory, polar regions, Siding Spring Observatory",

author = "Jamie Soon and Moore, {Anna M.} and Kasliwal, {Mansi M.} and Lau, {Ryan M.} and Kishalay De and Travouillon, {Tony D.} and Jones, {Mike I.} and Eran Ofek and Roger Smith and Valery Terebizh and Dan McKenna and David Hale and Alexandre Delacroix and Adams, {Scott M.} and Jencson, {Jacob E.} and Michael Ashley and Jill Burnham and Sokoloski, {Jennifer L.} and Joss Bland-Hawthorn and Freeman, {Ken C.} and {De Marco}, Orsola and Jeff Cooke and Philip Bland and Stuart Ryder and Roberto Soria and Jarek Antoszewski and Alexander Heger and Lee Spitler and Robert Simcoe",

note = "Copyright 2018 Society of Photo-Optical Instrumentation Engineers (SPIE). One print or electronic copy may be made for personal use only. Systematic reproduction and distribution, duplication of any material in this paper for a fee or for commercial purposes, or modification of the content of the paper are prohibited.; Ground-Based and Airborne Telescopes VII 2018 ; Conference date: 10-06-2018 Through 15-06-2018",

year = "2018",

month = jul,

day = "6",

doi = "10.1117/12.2312731",

language = "English",

isbn = "9781510619531",

series = "Proceedings of SPIE",

publisher = "SPIE",

pages = "107004D--1--107004D--12",

editor = "Marshall, {Heather K.} and Jason Spyromilio",

booktitle = "Ground-Based and Airborne Telescopes VII",

address = "United States",

}

Soon, J, Moore, AM, Kasliwal, MM, Lau, RM, De, K, Travouillon, TD, Jones, MI, Ofek, E, Smith, R, Terebizh, V, McKenna, D, Hale, D, Delacroix, A, Adams, SM, Jencson, JE, Ashley, M, Burnham, J, Sokoloski, JL, Bland-Hawthorn, J, Freeman, KC, De Marco, O, Cooke, J, Bland, P, Ryder, S, Soria, R, Antoszewski, J, Heger, A, Spitler, L & Simcoe, R 2018, Opening the dynamic infrared sky. in HK Marshall & J Spyromilio (eds), Ground-Based and Airborne Telescopes VII., 107004D, Proceedings of SPIE, vol. 10700, SPIE, Bellingham, Washington, pp. 107004D-1-107004D-12, Ground-Based and Airborne Telescopes VII 2018, Austin, United States, 10/06/18. https://doi.org/10.1117/12.2312731

Opening the dynamic infrared sky. / Soon, Jamie; Moore, Anna M.; Kasliwal, Mansi M. et al.
Ground-Based and Airborne Telescopes VII. ed. / Heather K. Marshall; Jason Spyromilio. Bellingham, Washington: SPIE, 2018. p. 107004D-1-107004D-12 107004D (Proceedings of SPIE; Vol. 10700).

Research output: Chapter in Book/Report/Conference proceeding › Conference proceeding contribution › peer-review

TY - GEN

T1 - Opening the dynamic infrared sky

AU - Soon, Jamie

AU - Moore, Anna M.

AU - Kasliwal, Mansi M.

AU - Lau, Ryan M.

AU - De, Kishalay

AU - Travouillon, Tony D.

AU - Jones, Mike I.

AU - Ofek, Eran

AU - Smith, Roger

AU - Terebizh, Valery

AU - McKenna, Dan

AU - Hale, David

AU - Delacroix, Alexandre

AU - Adams, Scott M.

AU - Jencson, Jacob E.

AU - Ashley, Michael

AU - Burnham, Jill

AU - Sokoloski, Jennifer L.

AU - Bland-Hawthorn, Joss

AU - Freeman, Ken C.

AU - De Marco, Orsola

AU - Cooke, Jeff

AU - Bland, Philip

AU - Ryder, Stuart

AU - Soria, Roberto

AU - Antoszewski, Jarek

AU - Heger, Alexander

AU - Spitler, Lee

AU - Simcoe, Robert

N1 - Copyright 2018 Society of Photo-Optical Instrumentation Engineers (SPIE). One print or electronic copy may be made for personal use only. Systematic reproduction and distribution, duplication of any material in this paper for a fee or for commercial purposes, or modification of the content of the paper are prohibited.

PY - 2018/7/6

Y1 - 2018/7/6

N2 - While optical and radio transient surveys have enjoyed a renaissance over the past decade, the dynamic infrared sky remains virtually unexplored from the ground. The infrared is a powerful tool for probing transient events in dusty regions that have high optical extinction, and for detecting the coolest of stars that are bright only at these wavelengths. The fundamental roadblocks in studying the infrared time-domain have been the overwhelmingly bright sky background (250 times brighter than optical) and the narrow field-of-view of infrared cameras (largest is VISTA at 0.6 sq deg). To address these challenges, Palomar Gattini-IR is currently under construction at Palomar Observatory and we propose a further low risk, economical, and agile instrument to be located at Siding Spring Observatory, as well as further instruments which will be located at the high polar regions to take advantage of the low thermal sky emission, particularly in the 2.5 micron region.

AB - While optical and radio transient surveys have enjoyed a renaissance over the past decade, the dynamic infrared sky remains virtually unexplored from the ground. The infrared is a powerful tool for probing transient events in dusty regions that have high optical extinction, and for detecting the coolest of stars that are bright only at these wavelengths. The fundamental roadblocks in studying the infrared time-domain have been the overwhelmingly bright sky background (250 times brighter than optical) and the narrow field-of-view of infrared cameras (largest is VISTA at 0.6 sq deg). To address these challenges, Palomar Gattini-IR is currently under construction at Palomar Observatory and we propose a further low risk, economical, and agile instrument to be located at Siding Spring Observatory, as well as further instruments which will be located at the high polar regions to take advantage of the low thermal sky emission, particularly in the 2.5 micron region.

KW - all-sky survey

KW - Antarctica

KW - DREAMS

KW - Gattini-IR

KW - infrared

KW - Palomar Observatory

KW - polar regions

KW - Siding Spring Observatory

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DO - 10.1117/12.2312731

M3 - Conference proceeding contribution

AN - SCOPUS:85051255722

SN - 9781510619531

T3 - Proceedings of SPIE

SP - 107004D-1-107004D-12

BT - Ground-Based and Airborne Telescopes VII

A2 - Marshall, Heather K.

A2 - Spyromilio, Jason

PB - SPIE

CY - Bellingham, Washington

T2 - Ground-Based and Airborne Telescopes VII 2018

Y2 - 10 June 2018 through 15 June 2018

ER -

Opening the dynamic infrared sky

Abstract

Publication series

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Bibliographical note

Keywords

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