HILIGT, upper limit servers I-Overview

被引：29

作者：

Saxton, R. D. ^{[1
]}

Koenig, O. ^{[2
]}

Descalzo, M. ^{[3
]}

Belanger, G. ^{[4
]}

Kretschmar, P. ^{[4
]}

Gabriel, C. ^{[4
,5
]}

Evans, P. A. ^{[6
]}

Ibarra, A. ^{[7
]}

Colomo, E. ^{[1
]}

Sarmiento, M. ^{[7
]}

Salgado, J. ^{[8
]}

Agrafojo, A. ^{[8
]}

Kuulkers, E. ^{[9
]}

机构：

[1] European Space Astron Ctr ESAC, Telespazio UK Ltd European Space Agcy ESA, Camino Bajo Castillo S-N, Madrid 28692, Spain

[2] Friedrich Alexander Univ Erlangen Nurnberg, Dr Karl Remeis Sternwarte & Erlangen Ctr Astropar, Sternwartstr 7, D-96049 Bamberg, Germany

[3] Tech Univ Denmark DTU, Dept Elect Engn, Orsteds Plads 326, DK-2800 Lyngby, Denmark

[4] European Space Astron Ctr ESAC, European Space Agcy ESA, Camino Bajo Castillo S-N, Madrid 28692, Spain

[5] Comm Space Res COSPAR, 2 Pl Maurice Quentin, F-75039 Paris 01, France

[6] Univ Leicester, Sch Phys & Astron, Xray & Observat Astron Grp, Univ Rd, Leicester LE1 7RH, Leics, England

[7] European Space Astron Ctr ESAC, QUASAR Sci Resources European Space Agcy ESA, Camino Bajo Castillo S-N, Madrid 28692, Spain

[8] European Space Astron Ctr ESAC, Aurora Technol BV European Space Agcy ESA, Camino Bajo Castillo S-N, Madrid 28692, Spain

[9] European Space Res & Technol Ctr ESTEC, European Space Agcy ESA, Keplerlaan 1, NL-2201 AZ Noordwijk, Netherlands

来源：

ASTRONOMY AND COMPUTING | 2022年 / 38卷

关键词：

Catalogs; Surveys; X-rays: general; Instrumentation: detectors; Upper limit; Aperture photometry; X-RAYS; 3C; 273; CATALOG;

D O I：

10.1016/j.ascom.2021.100531

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The advent of all-sky facilities, such as the Neil Gehrels Swift observatory, the All Sky Automated Search for Supernovae (ASAS-SN), eROSITA and Gaia has led to a new appreciation of the importance of transient sources in solving outstanding astrophysical questions. Identification and catalogue cross-matching of transients has been eased over the last two decades by the Virtual Observatory but we still lack a client capable of providing a seamless, self-consistent, analysis of all observations made of a particular object by current and historical facilities. HILIGT is a web-based interface which polls individual servers written for XMM-Newton, INTEGRAL and other missions, to find the fluxes, or upper limits, from all observations made of a given target. These measurements are displayed as a table or a time series plot, which may be downloaded in a variety of formats. HILIGT currently works with data from X-ray and Gamma-ray observatories. (C)& nbsp;2021 Elsevier B.V. All rights reserved.

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页数：8

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