22 research outputs found
Multi-wavelength observations of Galactic hard X-ray sources discovered by INTEGRAL. I. The nature of the companion star
Context: The INTEGRAL hard X-ray observatory has revealed an emerging
population of highly obscured X-ray binary systems through multi-wavelength
observations. Previous studies have shown that many of these sources are
high-mass X-ray binaries hosting neutron stars orbiting around luminous and
evolved companion stars. Aims: To better understand this newly-discovered
population, we have selected a sample of sources for which an accurate
localisation is available to identify the stellar counterpart and reveal the
nature of the companion star and of the binary system. Methods: We performed an
intensive study of a sample of thirteen INTEGRAL sources, through
multi-wavelength optical to NIR photometric and spectroscopic observations,
using EMMI and SofI instruments at the ESO NTT telescope. We performed accurate
astrometry and identified candidate counterparts for which we give the optical
and NIR magnitudes. We detected many spectral lines allowing us to determine
the spectral type of the companion star. We fitted with stellar black bodies
the mid-infrared to optical spectral energy distributions of these sources.
From the spectral analysis and SED fitting we identified the nature of the
companion stars and of the binary systems. (abridged).Comment: A&A in press; The official date of acceptance is 15/12/2007; 25
pages, 6 figures, 8 tables. New version with language editing required by
edito
Optical design of the SOXS spectrograph for ESO NTT
An overview of the optical design for the SOXS spectrograph is presented.
SOXS (Son Of X-Shooter) is the new wideband, medium resolution (R>4500)
spectrograph for the ESO 3.58m NTT telescope expected to start observations in
2021 at La Silla. The spectroscopic capabilities of SOXS are assured by two
different arms. The UV-VIS (350-850 nm) arm is based on a novel concept that
adopts the use of 4 ion-etched high efficiency transmission gratings. The NIR
(800- 2000 nm) arm adopts the '4C' design (Collimator Correction of Camera
Chromatism) successfully applied in X-Shooter. Other optical sub-systems are
the imaging Acquisition Camera, the Calibration Unit and a pre-slit Common
Path. We describe the optical design of the five sub-systems and report their
performance in terms of spectral format, throughput and optical quality. This
work is part of a series of contributions describing the SOXS design and
properties as it is about to face the Final Design Review.Comment: 9 pages, 9 figures, published in SPIE Proceedings 1070
The Acquisition Camera System for SOXS at NTT
SOXS (Son of X-Shooter) will be the new medium resolution (R4500 for a
1 arcsec slit), high-efficiency, wide band spectrograph for the ESO-NTT
telescope on La Silla. It will be able to cover simultaneously optical and NIR
bands (350-2000nm) using two different arms and a pre-slit Common Path feeding
system. SOXS will provide an unique facility to follow up any kind of transient
event with the best possible response time in addition to high efficiency and
availability. Furthermore, a Calibration Unit and an Acquisition Camera System
with all the necessary relay optics will be connected to the Common Path
sub-system. The Acquisition Camera, working in optical regime, will be
primarily focused on target acquisition and secondary guiding, but will also
provide an imaging mode for scientific photometry. In this work we give an
overview of the Acquisition Camera System for SOXS with all the different
functionalities. The optical and mechanical design of the system are also
presented together with the preliminary performances in terms of optical
quality, throughput, magnitude limits and photometric properties.Comment: 9 pages, 7 figures, SPIE conferenc
Fauna Europaea: Diptera -Brachycera
Link to publication Citation for published version (APA): Pape, T., Beuk, P., Pont, A. C., Shatalkin, A. I., Ozerov, A. L., Woźnica, A. J., ... de Jong, Y. (2015). Fauna Europaea: 3, [e4187]. https://doi.org/10.3897/BDJ.3.e4187 General rights It is not permitted to download or to forward/distribute the text or part of it without the consent of the author(s) and/or copyright holder(s), other than for strictly personal, individual use, unless the work is under an open content license (like Creative Commons). Disclaimer/Complaints regulations If you believe that digital publication of certain material infringes any of your rights or (privacy) interests, please let the Library know, stating your reasons. In case of a legitimate complaint, the Library will make the material inaccessible and/or remove it from the website. Please Ask the Library: https://uba.uva.nl/en/contact, or a letter to: Library of the University of Amsterdam, Secretariat, Singel 425, 1012 WP Amsterdam, The Netherlands. You will be contacted as soon as possible. Abstract Fauna Europaea provides a public web-service with an index of scientific names (including important synonyms) of all extant multicellular European terrestrial and freshwater animals and their geographical distribution at the level of countries and major islands (east of the Urals and excluding the Caucasus region). The Fauna Europaea project comprises about 230,000 taxonomic names, including 130,000 accepted species and 14,000 accepted subspecies, which is much more than the originally projected number of 100,000 species. Fauna Europaea represents a huge effort by more than 400 contributing taxonomic specialists throughout Europe and is a unique (standard) reference suitable for many user communities in science, government, industry, nature conservation and education. The Diptera-Brachycera is one of the 58 Fauna Europaea major taxonomic groups, and data have been compiled by a network of 55 specialists. Within the two-winged insects (Diptera), the Brachycera constitute a monophyletic group, which is generally given rank of suborder. The Brachycera may be classified into the probably paraphyletic 'lower brachyceran grade' and the monophyletic Eremoneura. The latter contains the Empidoidea, the Apystomyioidea with a single Nearctic species, and the Cyclorrhapha, which in turn is divided into the paraphyletic 'aschizan grade' and the monophyletic Schizophora. The latter is traditionally divided into the paraphyletic 'acalyptrate grade' and the monophyletic Calyptratae. Our knowledge of the European fauna of Diptera-Brachycera varies tremendously among families, from the reasonably well known hoverflies (Syrphidae) to the extremely poorly known scuttle flies (Phoridae). There has been a steady growth in our knowledge of European Diptera for the last two centuries, with no apparent slow down, but there is a shift towards a larger fraction of the new species being found among the families of the nematoceran grade (lower Diptera), which due to a larger number of small-sized species may be considered as taxonomically more challenging. Most of Europe is highly industrialised and has a high human population density, and the more fertile habitats are extensively cultivated. This has undoubtedly increased the extinction risk for numerous species of brachyceran flies, yet with the recent re-discovery of Thyreophora cynophila (Panzer), there are no known cases of extinction at a European level. However, few national Red Lists have extensive information on Diptera. For the Diptera-Brachycera, data from 96 families containing 11,751 species are included in this paper
APASS Landolt-Sloan BVgri photometry of RAVE stars. I. Data, effective temperatures, and reddenings
We provide AAVSO Photometric All-Sky Survey (APASS) photometry in the Landolt BV and Sloan g′r′i′ bands for all 425,743 stars included in the fourth RAVE Data Release. The internal accuracy of the APASS photometry of RAVE stars, expressed as the error of the mean of data obtained and separately calibrated over a median of four distinct observing epochs and distributed between 2009 and 2013, is 0.013, 0.012, 0.012, 0.014, and 0.021 mag for the B, V, g′, r′, and i′ bands, respectively. The equally high external accuracy of APASS photometry has been verified on secondary Landolt and Sloan photometric standard stars not involved in the APASS calibration process and on a large body of literature data on field and cluster stars, confirming the absence of offsets and trends. Compared with the Carlsberg Meridian Catalog (CMC-15), APASS astrometry of RAVE stars is accurate to a median value of 0.098 arcsec. Brightness distribution functions for the RAVE stars have been derived in all bands. APASS photometry of RAVE stars, augmented by 2MASS JHK infrared data, has been χ2 fitted to a densely populated synthetic photometric library designed to widely explore temperature, surface gravity, metallicity, and reddening. Resulting Teff and EB-V, computed over a range of options, are provided and discussed, and will be kept updated in response to future APASS and RAVE data releases. In the process, we find that the reddening caused by a homogeneous slab of dust, extending for 140 pc on either side of the Galactic plane and responsible for EB-V poles = 0.036 ± 0.002 at the Galactic poles, is a suitable approximation of the actual reddening encountered at Galactic latitudes |b| ≥ 25°
Development status of the SOXS instrument control software
SOXS (Son Of X-Shooter) is a forthcoming instrument for ESO-NTT, mainly
dedicated to the spectroscopic study of transient events and is currently
starting the AIT (Assembly, Integration, and Test) phase. It foresees a visible
spectrograph, a near-Infrared (NIR) spectrograph, and an acquisition camera for
light imaging and secondary guiding. The optimal setup and the monitoring of
SOXS are carried out with a set of software-controlled motorized components and
sensors. The instrument control software (INS) also manages the observation and
calibration procedures, as well as maintenance and self-test operations. The
architecture of INS, based on the latest release of the VLT Software (VLT2019),
has been frozen; the code development is in an advanced state for what concerns
supported components and observation procedures, which run in simulation. In
this proceeding we present the INS current status, focusing in particular on
the ongoing efforts in the support of two non-standard, "special" devices. The
first special device is the piezoelectric slit exchanger for the NIR
spectrograph; the second special device is the piezoelectric tip-tilt corrector
used for active compensation of mechanical flexures of the instrument.Comment: 8 pages, 4 figure
The common path of SOXS (Son of X-Shooter)
Son of X-Shooter (SOXS) will be a high-efficiency spectrograph with a mean Resolution-Slit product of 4500 (goal 5000) over the entire band capable of simultaneously observing the complete spectral range 350-2000 nm. It consists of three scientific arms (the UV-VIS Spectrograph, the NIR Spectrograph and the Acquisition Camera) connected by the Common Path system to the NTT and the Calibration Unit. The Common Path is the backbone of the instrument and the interface to the NTT Nasmyth focus flange. The light coming from the focus of the telescope is split by the common path optics into the two different optical paths in order to feed the two spectrographs and the acquisition camera. The instrument project went through the Preliminary Design Review in 2017 and is currently in Final Design Phase (with FDR in July 2018). This paper outlines the status of the Common Path system and is accompanied by a series of contributions describing the SOXS design and properties after the instrument Preliminary Design Review