New DSH planetary nebulae and candidates from optical and infrared surveys

Matthias Kronberger; Quentin A. Parker; George H. Jacoby; Agnes Acker; Filipe Alves; Ivan Bojicic; Paul Eigenthaler; David J. Frew; Dianne Harmer; Dana Patchick; Warren Reid; Johannes Schedler

doi:10.1088/1742-6596/728/7/072012

New DSH planetary nebulae and candidates from optical and infrared surveys

Matthias Kronberger, Quentin A. Parker, George H. Jacoby, Agnes Acker, Filipe Alves, Ivan Bojicic, Paul Eigenthaler, David J. Frew, Dianne Harmer, Dana Patchick, Warren Reid, Johannes Schedler

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Abstract

To date, the planetary nebula (PN) survey of the Deep Sky Hunters collaboration has led to the detection of more than 250 previously unknown candidate planetary nebulae (PNe). About 60% of them were found during the past two years and are expected to be true, likely or possible PNe because careful vetting has already thrown out more doubtful objects. The majority of the new PN candidates are located within the boundaries of the SHS and IPHAS Ha surveys and were discovered by combining MIR data from the WideField Infrared Survey Explorer (WISE) with optical data from the IPHAS, SHS and DSS surveys, and UV data from the Galaxy Evolution Explorer(GALEX).

Original language	English
Article number	072012
Pages (from-to)	1-2
Number of pages	2
Journal	Journal of Physics: Conference Series
Volume	728
Issue number	7
DOIs	https://doi.org/10.1088/1742-6596/728/7/072012
Publication status	Published - 8 Aug 2016
Event	11th Pacific Rim Conference on Stellar Astrophysics - The University of Hong Kong, Hong Kong, China Duration: 14 Dec 2015 → 17 Dec 2015 http://www.scifac.hku.hk/event/PRCSA2015/

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title = "New DSH planetary nebulae and candidates from optical and infrared surveys",

abstract = "To date, the planetary nebula (PN) survey of the Deep Sky Hunters collaboration has led to the detection of more than 250 previously unknown candidate planetary nebulae (PNe). About 60% of them were found during the past two years and are expected to be true, likely or possible PNe because careful vetting has already thrown out more doubtful objects. The majority of the new PN candidates are located within the boundaries of the SHS and IPHAS Ha surveys and were discovered by combining MIR data from the WideField Infrared Survey Explorer (WISE) with optical data from the IPHAS, SHS and DSS surveys, and UV data from the Galaxy Evolution Explorer(GALEX).",

author = "Matthias Kronberger and Parker, {Quentin A.} and Jacoby, {George H.} and Agnes Acker and Filipe Alves and Ivan Bojicic and Paul Eigenthaler and Frew, {David J.} and Dianne Harmer and Dana Patchick and Warren Reid and Johannes Schedler",

note = "Version archived for private and non-commercial use with the permission of the author/s. For further rights please contact the author/s or copyright owner.; 11th Pacific Rim Conference on Stellar Astrophysics, PRCSA2015 ; Conference date: 14-12-2015 Through 17-12-2015",

year = "2016",

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doi = "10.1088/1742-6596/728/7/072012",

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TY - JOUR

T1 - New DSH planetary nebulae and candidates from optical and infrared surveys

AU - Kronberger, Matthias

AU - Parker, Quentin A.

AU - Jacoby, George H.

AU - Acker, Agnes

AU - Alves, Filipe

AU - Bojicic, Ivan

AU - Eigenthaler, Paul

AU - Frew, David J.

AU - Harmer, Dianne

AU - Patchick, Dana

AU - Reid, Warren

AU - Schedler, Johannes

N1 - Version archived for private and non-commercial use with the permission of the author/s. For further rights please contact the author/s or copyright owner.

PY - 2016/8/8

Y1 - 2016/8/8

N2 - To date, the planetary nebula (PN) survey of the Deep Sky Hunters collaboration has led to the detection of more than 250 previously unknown candidate planetary nebulae (PNe). About 60% of them were found during the past two years and are expected to be true, likely or possible PNe because careful vetting has already thrown out more doubtful objects. The majority of the new PN candidates are located within the boundaries of the SHS and IPHAS Ha surveys and were discovered by combining MIR data from the WideField Infrared Survey Explorer (WISE) with optical data from the IPHAS, SHS and DSS surveys, and UV data from the Galaxy Evolution Explorer(GALEX).

AB - To date, the planetary nebula (PN) survey of the Deep Sky Hunters collaboration has led to the detection of more than 250 previously unknown candidate planetary nebulae (PNe). About 60% of them were found during the past two years and are expected to be true, likely or possible PNe because careful vetting has already thrown out more doubtful objects. The majority of the new PN candidates are located within the boundaries of the SHS and IPHAS Ha surveys and were discovered by combining MIR data from the WideField Infrared Survey Explorer (WISE) with optical data from the IPHAS, SHS and DSS surveys, and UV data from the Galaxy Evolution Explorer(GALEX).

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U2 - 10.1088/1742-6596/728/7/072012

DO - 10.1088/1742-6596/728/7/072012

M3 - Conference paper

AN - SCOPUS:84989235052

SN - 1742-6588

VL - 728

SP - 1

EP - 2

JO - Journal of Physics: Conference Series

JF - Journal of Physics: Conference Series

IS - 7

M1 - 072012

T2 - 11th Pacific Rim Conference on Stellar Astrophysics

Y2 - 14 December 2015 through 17 December 2015

ER -

New DSH planetary nebulae and candidates from optical and infrared surveys

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