77 research outputs found
The European Large Area ISO Survey - ISOPHOT results using the MPIA-pipeline
The European Large Area ISO Survey (ELAIS) will provide Infrared observations
of 4 regions in the sky with ISO. Around 2000 Infrared sources have been
detected at 7 and 15 microns (with ISOCAM), 90 and 175 microns (with ISOPHOT))
over 13 square degrees of the sky. We present the source extraction pipeline of
the 90 microns ISOPHOT observations, describe and discuss the results obtained
and derive the limits of the ELAIS observational strategy.Comment: 4 pages, 5 figures, to appear in the ISO conference "The Universe as
seen by ISO", 1998, UNESCO, Pari
Iteration Method to Derive Exact Rotation Curves from Position-Velocity Diagrams of Spiral Galaxies
We present an iteration method to derive exact rotation curves (RC) of spiral
galaxies from observed position-velocity diagrams (PVD), which comprises the
following procedure. An initial rotation curve, RC0, is adopted from an
observed PV diagram (PV0), obtained by any simple method such as the
peak-intensity method. Using this rotation curve and an observed radial
distribution of intensity (emissivity), we construct a simulated PV diagram
(PV1). The difference between a rotation curve obtained from this PV1 and the
original RC (e.g., difference between peak-intensity velocities) is used to
correct the initial RC to obtain a corrected rotation curve, RC1. This RC1 is
used to calculated another PVD (PV2) using the observed intensity distribution,
and to obtain the second iterated RC (RC2). This iteration is repeated until
PV converges to PV0, so that the differences between PV and PV0 becomes
minimum. Finally RC is adopted as the most reliable rotation curve. We apply
this method to some observed PVDs of nearby galaxies, and show that the
iteration successfully converges to give reliable rotation curves. We show that
the method is powerful to detect central massive objects.Comment: To appear in ApJ.Letters, 5 pages Latex with 4 figure
Near-infrared surface photometry of spiral galaxies
We present -band surface photometry of a sample of 31 inclined Sa-Scd
galaxies, together with additional - and -band data for four of them. In
this first paper of a series, profiles are presented, together with global and
isophotal parameters. Our profiles are compared to similar , and
data collected from other sources. Three galaxies exhibit previously unknown
small bars in their center, while in five others, such bars may also be
present. Four objects present a narrow elongated feature in their center
aligned with their major axis, which could be an inward extension of the disk.
A few galaxies display very thin spiral arms. Color-color diagrams indicate
that the extinction inside the four galaxies for which we have images is
limited to .Comment: Accepted in Astronomy and Astrophysics (Supplements). 11 pages LaTeX
with l-aa style file and 3 figures included. Figure 4 (35 pages of figures
taking over 3.5 MB uuencoded gzipped tared) is available at
ftp://ftp.iap.fr/pub/from_users/gam/PAPERS/hsm_fig4.u
On the nature of the ISO-selected sources in the ELAIS S2 region
We have studied the optical, near-IR and radio properties of a complete
sample of 43 sources detected at 15-micron in one of the deeper ELAIS
repeatedly observed region. The extragalactic objects in this sample have
15-micron flux densities in the range 0.4-10 mJy, where the source counts start
diverging from no evolution models. About 90% of the sources (39 out of 43)
have optical counterparts brighter than I=21 mag. Eight of these 39 sources
have been identified with stars on the basis of imaging data, while for another
22 sources we have obtained optical spectroscopy, reaching a high
identification percentage (30/43, ~70%). All but one of the 28 sources with
flux density > 0.7 mJy are identified. Most of the extragalactic objects are
normal spiral or starburst galaxies at moderate redshift (z_med~0.2); four
objects are Active Galactic Nuclei. We have used the 15-micron, H_alpha and
1.4-GHz luminosities as indicators of star-formation rate and we have compared
the results obtained in these three bands. While 1.4-GHz and 15-micron
estimates are in good agreement, showing that our galaxies are forming stars at
a median rate of ~40 Mo/yr, the raw H_alpha-based estimates are a factor ~5-10
lower and need a mean correction of ~2 mag to be brought on the same scale as
the other two indicators. A correction of ~2 mag is consistent with what
suggested by the Balmer decrements H_alpha/H_beta and by the optical colours.
Moreover, it is intermediate between the correction found locally for normal
spirals and the correction needed for high-luminosity 15-micron objects,
suggesting that the average extinction suffered by galaxies increases with
infrared luminosity.Comment: 19 pages, 11 figures (3 in JPEG format), MNRAS, accepte
Discovery of the heavily obscured supernova 2002cv
On the 13th of May 2002, supernova 2002cv was discovered using a
near-infrared camera working at the AZT-24 1.1m telescope at Campo Imperatore
(AQ-Italy). After the infrared detection a simultaneous photometric follow-up
was started at optical wavelengths. The preliminary results confirm a heavily
obscured object with a V-K color not lower than 6 magnitudes, making SN 2002cv
the most reddened supernova ever observed. This finding, along with the recent
discovery of another obscured supernova, suggests a critical revision of the
rates known to date. The estimate of the visual extinction and the light curves
are provided here. These latter indicate that our SN 2002cv observations are
the earliest available for a type-Ia supernova at IR wavelengths.Comment: 4 page
Cosmicflows-2: The Data
Cosmicflows-2 is a compilation of distances and peculiar velocities for over
8000 galaxies. Numerically the largest contributions come from the
luminosity-linewidth correlation for spirals, the TFR, and the related
Fundamental Plane relation for E/S0 systems, but over 1000 distances are
contributed by methods that provide more accurate individual distances:
Cepheid, Tip of the Red Giant Branch, Surface Brightness Fluctuation, SNIa, and
several miscellaneous but accurate procedures. Our collaboration is making
important contributions to two of these inputs: Tip of the Red Giant Branch and
TFR. A large body of new distance material is presented. In addition, an effort
is made to assure that all the contributions, our own and those from the
literature, are on the same scale. Overall, the distances are found to be
compatible with a Hubble Constant H_0 = 74.4 +-3.0 km/s/Mpc. The great interest
going forward with this data set will be with velocity field studies.
Cosmicflows-2 is characterized by a great density and high accuracy of distance
measures locally, falling to sparse and coarse sampling extending to z=0.1.Comment: To be published in Astronomical Journal. Two extensive tables to be
available on-line. Table 1 available at http://edd.ifa.hawaii.edu select
catalog `Cosmicflows-2 Distances
The European Large Area ISO Survey: ELAIS
The European Large Area ISO Survey (ELAIS) has surveyed 12 square degrees of
the sky at 15 and 90 microns, and subsets of this area at 6.75 and 175 microns,
using the Infrared Space Observatory (ISO). This project was the largest single
open time programme executed by ISO, taking 375 hours of data. A preliminary
catalogue of more than 1000 galaxies has been produced. In this talk we
describe the goals of the project, describe the follow-up programmes that are
in progress, and present some first scientific results including a provisional
number count analysis at 15 and 90 microns.Comment: 5 pages, 3 figures, 4 tables, to appear in 'The universe as seen by
ISO', eds P.Cox and M.F.Kessler, 1998, UNESCO, Paris, ESA Special
Publications Series (SP-427
Astro-WISE: Chaining to the Universe
The recent explosion of recorded digital data and its processed derivatives
threatens to overwhelm researchers when analysing their experimental data or
when looking up data items in archives and file systems. While current hardware
developments allow to acquire, process and store 100s of terabytes of data at
the cost of a modern sports car, the software systems to handle these data are
lagging behind. This general problem is recognized and addressed by various
scientific communities, e.g., DATAGRID/EGEE federates compute and storage power
over the high-energy physical community, while the astronomical community is
building an Internet geared Virtual Observatory, connecting archival data.
These large projects either focus on a specific distribution aspect or aim to
connect many sub-communities and have a relatively long trajectory for setting
standards and a common layer. Here, we report "first light" of a very different
solution to the problem initiated by a smaller astronomical IT community. It
provides the abstract "scientific information layer" which integrates
distributed scientific analysis with distributed processing and federated
archiving and publishing. By designing new abstractions and mixing in old ones,
a Science Information System with fully scalable cornerstones has been
achieved, transforming data systems into knowledge systems. This break-through
is facilitated by the full end-to-end linking of all dependent data items,
which allows full backward chaining from the observer/researcher to the
experiment. Key is the notion that information is intrinsic in nature and thus
is the data acquired by a scientific experiment. The new abstraction is that
software systems guide the user to that intrinsic information by forcing full
backward and forward chaining in the data modelling.Comment: To be published in ADASS XVI ASP Conference Series, 2006, R. Shaw, F.
Hill and D. Bell, ed
FIRBACK IV: Towards the nature of the 170microns source population
We present a detailed study of the brighter ( detections) sources
in the 170m FIRBACK northern N1 ISO survey, with the help of complementary
data in the optical, radio, and mid-IR domain. For 82% of them, an optical
galaxy counterpart is identified, either as the unique source of the IR
emission, or as part of a multiple identification. With less than 15% of AGNs,
these sources are essentially local, moderate starbursters with a dominating
cold dust component. and represent a population of cold galaxies rather
neglected up to now. Their colours do not match those of the far-IR Cosmic IR
Background (CIB), to which they contribute less than 5%. The bulk of the
sources contributing to the CIB is thus to be searched for in more distant
galaxies, possibly counterparts of the fainter FIRBACK sources still under
study. These bright, local, galaxies however play an important role in the
evolution of IR galaxies: they dominate the number counts at high 170 m
fluxes, and represent half of the contribution at 250 mJy. Although not
particularly massive (typically M*), they form more stars than a typical spiral
galaxy and many are bulge dominated, that could represent the remnant of a
former merger. The fainter part of this population may represent the missing
link with the higher-z sources found in sub-mm observations.Comment: 40 pages, 10 figures, accepted for publication in Astronomy &
Astrophysic
Photometric study of the IC 65 group of galaxies
We carry out a photometric study of a poor group of late-type galaxies around
IC 65, with the aim: (a) to search for new dwarf members and to measure their
photometric characteristics; (b) to search for possible effects of mutual
interactions on the morphology and star-formation characteristics of luminous
and faint group members; (c) to evaluate the evolutionary status of this
particular group. We make use of our BRI CCD observations, DPOSS blue and red
frames, and the 2MASS JHK frames. In addition, we use the HI imaging data, the
far-infrared and radio data from the literature. Search for dwarf galaxies is
made using the SExtractor software. Detailed surface photometry is performed
with the MIDAS package. Four LSB galaxies were classified as probable dwarf
members of the group and the BRI physical and model parameters were derived for
the first time for all true and probable group members. Newly found dIrr
galaxies around the IC 65 contain a number of H II regions, which show a range
of ages and propagating star-formation. Mildly disturbed gaseous and/or stellar
morphology is found in several group members. Various structural, dynamical,
and star-forming characteristics let us conclude that the IC 65 group is a
typical poor assembly of late-type galaxies at an early stage of its dynamical
evolution with some evidence of intragroup (tidal) interactions.Comment: 21 pages, 16 figures, submitted to A&
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