The RapidXMM upper limit server: X-ray aperture photometry of the XMM-Newton archival observations

Author:

Ruiz A1ORCID,Georgakakis A1ORCID,Gerakakis S2,Saxton R3,Kretschmar P4,Akylas A1,Georgantopoulos I1

Affiliation:

1. Institute for Astronomy & Astrophysics, National Observatory of Athens , V. Paulou & I. Metaxa 11532, Greece

2. Planetek Hellas , 44 Kifisias Ave, Athens Space Cluster Bldg C, 15125 Marousi, Athens, Greece

3. TPZ-VEGA for ESA, XMM-Newton SOC, ESAC , Apartado 78, E-28691 Villanueva de la Cañada, Madrid, Spain

4. ESA-European Space Astronomy Centre , E-28691 Villanueva de la Cañada, Madrid, Spain

Abstract

ABSTRACT This paper presents the construction of the RapidXMM database that is available through the XMM-Newton Science Archive and offers access to upper limits and aperture photometry across the field of view of the XMM-Newton Pointed and Slew Survey observations. The feature of RapidXMM is speed. It enables the fast retrieval of X-ray upper limits and photometry products in three energy bands (0.2–2, 2–12, and 0.2–12 keV) for large numbers of input sky positions. This is accomplished using the Hierarchical Equal Area Iso Latitude pixelation of the sphere (HEALPix). The pre-calculated upper-limits and associated X-ray photometry products are reprojected into the HEALPix grid of cells before being ingested into the RapidXMM database. This results in tables of upper limits and aperture photometry within HEALPix cells of size ≈3 arcsec (Pointed observations) and 6 arcsec (Slew Survey). The database tables are indexed by the unique integer number of the HEALPix cells. This reduces spatial nearest-neighbour queries by sky position to an integer-matching exercise and significantly accelerates the retrieval of results. We describe in detail the processing steps that lead from the science products available in the XMM-Newton archive to a database optimized for sky queries. We also present two simple show-case applications of RapidXMM for scientific studies – searching for variable X-ray sources and stacking analysis of X-ray faint populations.

Funder

European Space Agency

ESA

NASA

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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