The<i>XMM-Newton</i>serendipitous survey

Webb, N.; Coriat, M.; Traulsen, I.; Ballet, J.; Motch, C.; Carrera, Francisco J.; Koliopanos, Filippos; Authier, J.; Calle, I. de la; Ceballos, M. T.; Colomo, Elena; Chuard, Dimitri; Freyberg, M. J.; García, T. Tepper; Kolehmainen, Mari; Lamer, G.; Lin, Dacheng; Maggi, Pierre; Michel, Laurent; Page, C. G.; Page, M. J.; Perea-Calderón, J. V.; Pineau, F.-X.; Rodríguez, P.; Rosen, S. R.; Santos-Lleo, M.; Saxton, R. D.; Schwope, A. D.; Tomás, L.; Watson, M. G.; Zakardjian, A.

doi:10.1051/0004-6361/201937353

Cited by 266 publications

(124 citation statements)

References 33 publications

Supporting

Mentioning

120

Contrasting

Order By: Relevance

“…1. The detection of this source is also reported in the 4XMM−DR10 catalog (Webb et al 2020) with an observed flux in the 0.2-12 keV band of F 0.2−12 =(2.4±0.2)×10 −13 erg cm −2 s −1 . We note that the same field has been previously observed on 2011 May 05 in the framework of the XMM-Newton slew survey (Saxton et al 2008).…”

Section: Igr J20155+3827supporting

confidence: 70%

Multiwavelength observations of the Galactic X-ray binaries IGR J20155+3827 and Swift J1713.4−4219

Onori

Fiocchi

Masetti

et al. 2021

Monthly Notices of the Royal Astronomical Society

View full text Add to dashboard Cite

In recent years, thanks to the continuous surveys performed by INTEGRAL and Swift satellites, our knowledge of the hard X-ray/soft gamma-ray sky has greatly improved. As a result it is now populated with about 2000 sources, both Galactic and extra-galactic, mainly discovered by IBIS and BAT instruments. Many different follow-up campaigns have been successfully performed by using a multi-wavelength approach, shedding light on the nature of a number of these new hard X-ray sources. However, a fraction are still of a unidentified nature. This is mainly due to the lack of lower energy observations, which usually deliver a better constrained position for the sources, and the unavailability of the key observational properties, needed to obtain a proper physical characterization. Here we report on the classification of two poorly studied Galactic X-ray transients IGR J20155+3827 and Swift J1713.4−4219, for which the combination of new and/or archival X-ray and Optical/NIR observations have allowed us to pinpoint their nature. In particular, thanks to XMM-Newton archival data together with new optical spectroscopic and archival Optical/NIR photometric observations, we have been able to classify IGR J20155+3827 as a distant HMXB. The new INTEGRAL and Swift data collected during the 2019 X-ray outburst of Swift J1713.4−4219, in combination with the archival optical/NIR observations, suggest a LMXB classification for this source.

show abstract

Section: Igr J20155+3827supporting

confidence: 70%

Multiwavelength observations of the Galactic X-ray binaries IGR J20155+3827 and Swift J1713.4−4219

Onori

Fiocchi

Masetti

et al. 2021

Monthly Notices of the Royal Astronomical Society

View full text Add to dashboard Cite

show abstract

“…This temporary source list is utilized to generate background images for each instrument (with the input sources removed), using esplinemap with METHOD = ASMOOTH. This adaptive-smoothing method has been widely adopted in recent XMM-Newton catalogs (e.g., Traulsen et al 2019Traulsen et al , 2020Webb et al 2020), as it can well characterize the local X-ray background level. 3.…”

Section: First-pass Source Detection and Astrometric Correctionmentioning

confidence: 99%

The XMM-SERVS Survey: XMM-Newton Point-source Catalogs for the W-CDF-S and ELAIS-S1 Fields

Brandt

Chen

et al. 2021

ApJS

View full text Add to dashboard Cite

We present the X-ray point-source catalogs in two of the XMM-Spitzer Extragalactic Representative Volume Survey (XMM-SERVS) fields, W-CDF-S (4.6 deg 2 ) and ELAIS-S1 (3.2 deg 2 ), aiming to fill the gap between deep pencil-beam X-ray surveys and shallow X-ray surveys over large areas. The W-CDF-S and ELAIS-S1 regions were targeted with 2.3 and 1.0 Ms of XMM-Newton observations, respectively; 1.8 and 0.9 Ms exposures remain after flare filtering. The survey in W-CDF-S has a flux limit of 1.0 × 10 −14 erg cm −2 s −1 over 90% of its area in the 0.5-10 keV band; 4053 sources are detected in total. The survey in ELAIS-S1 has a flux limit of 1.3 × 10 −14 erg cm −2 s −1 over 90% of its area in the 0.5-10 keV band; 2630 sources are detected in total. Reliable optical-to-IR multiwavelength counterpart candidates are identified for ≈89% of the sources in W-CDF-S and ≈87% of the sources in ELAIS-S1. A total of 3129 sources in W-CDF-S and 1957 sources in ELAIS-S1 are classified as active galactic nuclei (AGNs). We also provide photometric redshifts for X-ray sources; ≈84% of the 3319/2001 sources in W-CDF-S/ELAIS-S1 with optical-to-near-IR forced photometry available have either spectroscopic redshifts or high-quality photometric redshifts. The completion of the XMM-Newton observations in the W-CDF-S and ELAIS-S1 fields marks the end of the XMM-SERVS survey data gathering. The ≈12,000 pointlike X-ray sources detected in the whole ≈13 deg 2 XMM-SERVS survey will benefit future large-sample AGN studies.

show abstract

“…The authors list as possible optical counterpart HV 2289 -an early-B type supergiant with an orbital period of P = 6.94 d (Bianchi & Pakull 1984). X-ray positions from Einstein and ROSAT are not precise enough to allow a secure optical identification, but the source was also detected by XMM-Newton (4XMM J050123.3−703333 in the 4XMM-DR9 catalogue; Webb et al 2020) with a position error of 1. 5 (1σ ).…”

Section: X-ray Binariesmentioning

confidence: 99%

The ASKAP-EMU Early Science Project: 888 MHz radio continuum survey of the Large Magellanic Cloud

Pennock

Loon

Filipović

et al. 2021

Monthly Notices of the Royal Astronomical Society

View full text Add to dashboard Cite

We present an analysis of a new 120 deg2 radio continuum image of the Large Magellanic Cloud (LMC) at 888 MHz with a bandwidth of 288 MHz and beam size of $13\rlap{.}^{\prime \prime }9\times 12\rlap{.}^{\prime \prime }1$, from the Australian Square Kilometre Array Pathfinder (ASKAP) processed as part of the Evolutionary Map of the Universe (EMU) survey. The median Root Mean Squared noise is 58 μJy beam−1. We present a catalogue of 54,612 sources, divided over a Gold list (30,866 sources) complete down to 0.5 mJy uniformly across the field, a Silver list (22,080 sources) reaching down to < 0.2 mJy and a Bronze list (1,666 sources) of visually inspected sources in areas of high noise and/or near bright complex emission. We discuss detections of planetary nebulæ and their radio luminosity function, young stellar objects showing a correlation between radio luminosity and gas temperature, novæ and X-ray binaries in the LMC, and active stars in the Galactic foreground that may become a significant population below this flux level. We present examples of diffuse emission in the LMC (H ii regions, supernova remnants, bubbles) and distant galaxies showcasing spectacular interaction between jets and intracluster medium. Among 14,333 infrared counterparts of the predominantly background radio source population we find that star-forming galaxies become more prominent below 3 mJy compared to active galactic nuclei. We combine the new 888 MHz data with archival Australia Telescope Compact Array data at 1.4 GHz to determine spectral indices; the vast majority display synchrotron emission but flatter spectra occur too. We argue that the most extreme spectral index values are due to variability.

show abstract

TheXMM-Newtonserendipitous survey

Cited by 266 publications

References 33 publications

Multiwavelength observations of the Galactic X-ray binaries IGR J20155+3827 and Swift J1713.4−4219

Multiwavelength observations of the Galactic X-ray binaries IGR J20155+3827 and Swift J1713.4−4219

The XMM-SERVS Survey: XMM-Newton Point-source Catalogs for the W-CDF-S and ELAIS-S1 Fields

The ASKAP-EMU Early Science Project: 888 MHz radio continuum survey of the Large Magellanic Cloud

Contact Info

Product

Resources

About