2017PASP..129a4002M


Query : 2017PASP..129a4002M

2017PASP..129a4002M - Publ. Astron. Soc. Pac., 129, part no 1, 4002-14002 (2017/January-0)

The IPAC image subtraction and Discovery pipeline for the intermediate Palomar Transient Factory.

MASCI F.J., LAHER R.R., REBBAPRAGADA U.D., DORAN G.B., MILLER A.A., BELLM E., KASLIWAL M., OFEK E.O., SURACE J., SHUPE D.L., GRILLMAIR C.J., JACKSON E., BARLOW T., YAN L., CAO Y., CENKO S.B., STORRIE-LOMBARDI L.J., HELOU G., PRINCE T.A. and KULKARNI S.R.

Abstract (from CDS):

We describe the near real-time transient-source discovery engine for the intermediate Palomar Transient Factory (iPTF), currently in operations at the Infrared Processing and Analysis Center (IPAC), Caltech. We coin this system the IPAC/iPTF Discovery Engine (or IDE). We review the algorithms used for PSF-matching, image subtraction, detection, photometry, and machine-learned (ML) vetting of extracted transient candidates. We also review the performance of our ML classifier. For a limiting signal-to-noise ratio of 4 in relatively unconfused regions, bogus candidates from processing artifacts and imperfect image subtractions outnumber real transients by ≃10:1. This can be considerably higher for image data with inaccurate astrometric and/or PSF-matching solutions. Despite this occasionally high contamination rate, the ML classifier is able to identify real transients with an efficiency (or completeness) of ≃97% for a maximum tolerable false-positive rate of 1% when classifying raw candidates. All subtraction-image metrics, source features, ML probability-based real-bogus scores, contextual metadata from other surveys, and possible associations with known Solar System objects are stored in a relational database for retrieval by the various science working groups. We review our efforts in mitigating false-positives and our experience in optimizing the overall system in response to the multitude of science projects underway with iPTF.

Abstract Copyright: © 2016. The Astronomical Society of the Pacific. All rights reserved.

Journal keyword(s):

Simbad objects: 1

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Number of rows : 1
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 NGC 7000 Cl* 20 58 47 +44 19.8           ~ 427 0

Query : 2017PASP..129a4002M

Basic data :
NGC 7000 -- Cluster of Stars
Other object types:
otypes_help
Rad (CTB,GRS,...), HII (1976A&AS,LBN,...), Cl* (2020A&A,Villafranca)
ICRS coord. (ep=J2000) :
20 58 47.0 +44 19 48 [ ] E ~
FK4 coord. (ep=B1950 eq=1950) :
20 56 59.6 +44 08 06 [ ]
Gal coord. (ep=J2000) :
085.5012 -00.9846 [ ]
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Hierarchy : number of linked objects
whatever the membership probability is (see description here ) :

: 1
: 4
: 594 Display criteria :

Identifiers (15) :
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NGC 7000 LBN 373 NAME Bermuda Cluster Villafranca O-014 NW
CTB 100 NAME NORTH AMER NEB NRL 21 [DGW65] 138
GRS G084.70 -01.00 NAME North America SH 2-117 [PT56] 49
LBN 085.75-01.48 NAME North America Nebula Villafranca O-014

References (427 between 1850 and 2026) (Total 427)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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Collections of Measurements Description of Measurements

Distance : 2   

   

Observing logs
ISO : 4   

   


External archives :

Data at NED - NASA/IPAC Extragalactic Database : NGC 7000

Link by name to the catalogue in VizieR :

NGC 7000

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