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+---
+title: "IVOA Newsletter - October 2013"
+date: 2013-10-01T00:01:00+02:00
+tags:
+- news
+---
+
+[Subscribe](http://www.ivoa.net/mailman/listinfo/ivoa-news) | [Newsletter archives](http://www.ivoa.net/newsletter/) | [Write to the editors](mailto:ivoa-news-editors@ivoa.net)
+**IVOA Newsletter Editors:** Mark G. Allen, Deborah Baines, Sarah Emery Bunn,
+Chenzou Cui, Mark Taylor, & Ivan Zolotukhin.
+
+**The International Virtual Observatory Alliance (IVOA) was formed in June 2002
+with a mission to facilitate the international coordination and collaboration
+necessary for the development and deployment of the tools, systems and
+organizational structures necessary to enable the international utilization of
+astronomical archives as an integrated and interoperating virtual observatory.
+The IVOA now comprises 20 VO programs from Argentina, Armenia, Australia,
+Brazil, Canada, China, Europe, France, Germany, Hungary, India, Italy, Japan,
+Russia, South Africa, Spain, Ukraine, the United Kingdom, and the United States
+and an inter-governmental organization (ESA). Membership is open to other
+national and international programs according to the
+[IVOA Guidelines for Participation](http://ivoa.net/Documents/latest/IVOAParticipation.html).
+You can read more about the IVOA and what we do at
+.**
+
+### What is the VO?
+
+The Virtual Observatory (VO) aims to provide a research environment that will
+open up new possibilities for scientific research based on data discovery,
+efficient data access, and interoperability. The vision is of global astronomy
+archives connected via the VO to form a multiwavelength digital sky that can be
+searched, visualized, and analyzed in new and innovative ways. VO projects
+worldwide working toward this vision are already providing science capabilities
+with new tools and services. This newsletter, aimed at astronomers, highlights
+VO tools and technologies for doing astronomy research, recent papers, and
+upcoming events.
+
+---
+
+# IVOA news
+
+{{< side-image image="SAcubed_logo.png" position="left" >}}
+
+### South Africa's Astronomical Agreement for Big Data
+
+The South African National Research Foundation’s three astronomical facilities
+have formed the [South African Astroinformatics Alliance](http://www.sa3.ac.za/)
+(SA3 pronounced “SA cubed”), which serves as a virtual observatory for the
+country. South Africa hosts new and upcoming observational facilities that will
+generate huge amounts of data including the Southern African Large Telescope
+(SALT), the Karoo Array Telescope (MeerKAT) and a large part of the SKA. See
+[the SA3 announcement](http://www.saao.ac.za/sa-astroinformatics-alliance-launched/)
+of their "Astronomical agreement signed for big data!". SA3 is a member of the
+IVOA since October 2012.
+
+{{ side-image >}}
+
+{{< side-image image="logo-euhoumw-transp.png" position="right" >}}
+
+### News from VObs.it: Remote Telescope networks for schools: toward publishing educational data in VO
+
+The [European Hands-On-Universe Milky Way](http://euhou.obspm.fr/public/)
+(EUHOUMW) is an educational project funded by the European Commission to bring
+real radio observations into classrooms, where participating students use five
+remotely controlled educational radio telescopes. EUHOUMW is now evaluating how
+to publish the collected radio data in VO format to enable data sharing (e.g.
+with the Italian optical robotic telescope network), to simplify data management
+of multi-classroom projects, and to more easily incorporate professional data in
+education projects. An unofficial kick-off of the collaboration between EUHOUMW
+and VO was held in Paris, September 5-6, 2013. The topics being addressed
+included; how to tag education data alongside professional data in the VO, and
+the use of "educationalized" VO tools (following
+[educational use of Aladin and Stellarium](http://wwwas.oats.inaf.it/aidawp5/eng_download.html?fsize=medium)).
+Publishing, archiving, and maintaining educational data are topics for the
+September 2013 IVOA Interoperability and ADASS meetings.
+
+{{ side-image >}}
+
+---
+
+# VO applications and implementation highlights
+
+{{< side-image image="alma-vo-screenshot.png" thumbnail="alma-vo-screenshot_thum.png" position="right" >}}
+
+### ALMA VO Service
+
+The Japanese Virtual Observatory (JVO) and ALMA-J teams have opened a VO-based
+data distribution system for ALMA data cubes. The aim is to help users access
+public ALMA data without huge data transfers. Two user applications, ALMAWebQL
+and Vissage, were developed for this system. ALMAWebQL is a component of the JVO
+Portal and enables the user to visualize and make cut-outs of ALMA data cubes in
+a web browser, while Vissage is a desktop application to visualize downloaded
+ALMA data cubes in more detail.
+
+**More Information:**
+
+{{ side-image >}}
+
+{{< side-image image="TheoSSA.png" thumbnail="TheoSSA_thumb.png" position="" >}}
+
+### TheoSSA
+
+The TheoSSA (Theoretical Stellar Spectra Access) service provides access to
+synthetic spectral energy distributions (SEDs) that may be calculated by any
+model-atmosphere code. The database contains pre-calculated SEDs over a wide
+range of effective temperature, surface gravity, and elemental composition. The
+related [TMAW tool](http://astro.uni-tuebingen.de/~TMAW) allows the calculation
+of individual SEDs that presently can consider opacities of the elements H, He,
+C, N, O, Ne, Na, and Mg.
+
+**More Information:**
+
+{{ side-image >}}
+
+{{< side-image image="TIRO.png" thumbnail="TIRO_thumb.png" position="right" >}}
+
+### TIRO
+
+The TIRO (Tuebingen IRon Opacity) service constructs model atoms of Ca, Sc, Ti,
+V, Cr, Mn, Fe, Co, and Ni based on
+[Kurucz' atomic data](http://kurucz.harvard.edu/atoms.html) using a statistical
+approach (introducing super-levels and super-lines) and calculates the
+respective bound-bound and bound-free absorption cross-section.
+
+**More information:**
+
+{{ side-image >}}
+
+{{< side-image image="ivoaBlurbSciencePics.png" thumbnail="ivoaBlurbSciencePics_thumb.png" position="left" >}}
+
+### Iris version 2.0
+
+The US VAO has released Iris 2.0, the latest version of the spectral energy
+distribution (SED) analysis tool. Iris comes with powerful new science
+capabilities which allow the redshifting, interpolation and smoothing of SEDs,
+and measurement of integrated fluxes through simple spectral bandpasses or
+through one of the thousands of photometric filters provided by the Spanish VO
+Filter Profile Service. Users can also apply simple aperture corrections to
+individual photometric points or to whole SED segments. In addition to improved
+visualization capabilities, including the co-plotting of SEDs, Iris 2.0 has
+increased interoperability with other VO tools. You can watch Iris in action in
+this [video tutorial](http://www.youtube.com/watch?v=GMaLgJfxJHI).
+
+**More information:**
+
+{{ side-image >}}
+
+---
+
+# Some recent papers about VO-enabled science
+
+### Featured Paper
+
+
+[The virtual observatory service TheoSSA: Establishing a database of synthetic stellar flux standards. I. NLTE spectral analysis of the DA-type white dwarf G 191-B2B](http://adsabs.harvard.edu/abs/2013arXiv1308.6450R)
+
+_Rauch, T.; Bohlin, R.; Kruk, J. W.; Werner, K. Astronomy & Astrophysics, in press_
+
+H-rich, DA-type white dwarfs are particularly suited as primary standard stars
+for flux calibration. State-of-the-art NLTE models consider opacities of species
+up to trans-iron elements and provide reliable synthetic stellar-atmosphere
+spectra to compare with observation. We establish a database of theoretical
+spectra of stellar flux standards that are easily accessible via a web
+interface. In the framework of the Virtual Observatory, the German Astrophysical
+Virtual Observatory developed the registered service TheoSSA. It provides easy
+access to stellar spectral energy distributions (SEDs) and is intended to ingest
+SEDs calculated by any model-atmosphere code. In case of the DA white dwarf G
+191-B2B, we demonstrate that the model reproduces not only its overall continuum
+shape but also the numerous metal lines exhibited in its ultraviolet spectrum.
+TheoSSA is in operation and contains presently a variety of SEDs for DA white
+dwarfs. It will be extended in the near future and can host SEDs of all primary
+and secondary flux standards. The spectral analysis of G 191-B2B has shown that
+our hydrostatic models reproduce the observations best at an effective
+temperature of 60000 +/- 2000K and a surface gravity of log g = 7.60 +/- 0.05.
+We newly identified Fe VI, Ni VI, and Zn IV lines. For the first time, we
+determined the photospheric zinc abundance with a logarithmic mass fraction of
+-4.89 (7.5 times solar). The abundances of He (upper limit), C, N, O, Al, Si, O,
+P, S, Fe, Ni, Ge, and Sn were precisely determined. Upper abundance limits of
+10% solar were derived for Ti, Cr, Mn, and Co. The TheoSSA database of
+theoretical SEDs of stellar flux standards guarantees that the flux calibration
+of all astronomical data and cross-calibration between different instruments can
+be based on the same models and SEDs calculated with different model-atmosphere
+codes and are easy to compare.
+
+### Refereed Publications
+
+* [Bayesian Analysis to Identify New Star Candidates in Nearby Young Stellar Kinematic Groups](http://adsabs.harvard.edu/abs/2013ApJ...762...88M)
+ _Malo, Lison; Doyon, René; Lafrenière, David; Artigau, Étienne; Gagné, Jonathan; Baron, Frédérique; Riedel, Adric
+ The Astrophysical Journal, Volume 762, Issue 2, article id. 88, 50 pp. (2013)._
+
+* [The Pseudo-evolution of Halo Mass](http://adsabs.harvard.edu/abs/2013ApJ...766...25D)
+ _Diemer, Benedikt; More, Surhud; Kravtsov, Andrey V.
+ The Astrophysical Journal, Volume 766, Issue 1, article id. 25, 15 pp. (2013)._
+
+* [Environmental Effects in the Interaction and Merging of Galaxies in zCOSMOS](http://adsabs.harvard.edu/abs/2013ApJ...762...43K)
+ _Kampczyk, P. et al._
+ _The Astrophysical Journal, Volume 762, Issue 1, article id. 43, 16 pp. (2013)._
+
+* [The Cosmic History of the Spin of Dark Matter Halos within the Large-scale Structure](http://adsabs.harvard.edu/abs/2013ApJ...762...72T)
+ _Trowland, Holly E.; Lewis, Geraint F.; Bland-Hawthorn, Joss
+ The Astrophysical Journal, Volume 762, Issue 2, article id. 72, 12 pp. (2013)._
+
+* [Unveiling the Nature of Unidentified Gamma-Ray Sources. I. A New Method for the Association of Gamma-Ray Blazars](http://adsabs.harvard.edu/abs/2013ApJS..206...12D)
+ _D'Abrusco, R.; Massaro, F.; Paggi, A.; Masetti, N.; Tosti, G.; Giroletti, M.; Smith, H. A.
+ The Astrophysical Journal Supplement, Volume 206, Issue 2, article id. 12, 26 pp. (2013)._
+
+* [Fomalhaut b: Independent Analysis of the Hubble Space Telescope Public Archive Data](http://adsabs.harvard.edu/abs/2013ApJ...769...42G)
+ _Galicher, Raphaël; Marois, Christian; Zuckerman, B.; Macintosh, Bruce
+ The Astrophysical Journal, Volume 769, Issue 1, article id. 42, 12 pp. (2013)._
+
+* [The binary fraction of planetary nebula central stars - I. A high-precision, I-band excess search](http://adsabs.harvard.edu/abs/2013MNRAS.428.2118D)
+ _De Marco, Orsola; Passy, Jean-Claude; Frew, D. J.; Moe, Maxwell; Jacoby, G. H.
+ Monthly Notices of the Royal Astronomical Society, Volume 428, Issue 3, p.2118-2140
+
+* [Galaxy Zoo: bulgeless galaxies with growing black holes](http://adsabs.harvard.edu/abs/2013MNRAS.429.2199S)
+ _Simmons, Brooke D.; Lintott, Chris; Schawinski, Kevin; Moran, Edward C.; Han, Anna; Kaviraj, Sugata; Masters, Karen L.; Urry, C. Megan; Willett, Kyle W.; Bamford, Steven P.; Nichol, Robert C.
+ Monthly Notices of the Royal Astronomical Society, Volume 429, Issue 3, p.2199-2211_
+
+* [Symbiotic stars and other Hα emission-line stars towards the Galactic bulge](http://adsabs.harvard.edu/abs/2013MNRAS.432.3186M)
+ _Miszalski, Brent; Mikołajewska, Joanna; Udalski, Andrzej
+ Monthly Notices of the Royal Astronomical Society, Volume 432, Issue 4, p.3186-3217_
+
+* [Constraints on dark matter annihilation by radio observations of M31](http://adsabs.harvard.edu/abs/2013PhRvD..88b3504E)
+ _Egorov, A. E.; Pierpaoli, E.
+ Physical Review D, vol. 88, Issue 2, id. 023504_
+
+* [Estimating gas masses and dust-to-gas ratios from optical spectroscopy](http://adsabs.harvard.edu/abs/2013MNRAS.432.2112B)
+ _Brinchmann, Jarle; Charlot, Stéphane; Kauffmann, Guinevere; Heckman, Tim; White, Simon D. M.; Tremonti, Christy
+ Monthly Notices of the Royal Astronomical Society, Volume 432, Issue 3, p.2112-2140_
+
+* [The Detection of the Large-scale Alignment of Massive Galaxies at z ~ 0.6](http://adsabs.harvard.edu/abs/2013ApJ...770L..12L)
+ _Li, Cheng; Jing, Y. P.; Faltenbacher, A.; Wang, Jie
+ The Astrophysical Journal Letters, Volume 770, Issue 1, article id. L12, 5 pp. (2013)._
+
+* [Fueling the central engine of radio galaxies. II. The footprints of AGN feedback on the ISM of 3C 236](http://adsabs.harvard.edu/abs/2013A%26A...549A..58L)
+ _Labiano, A.; García-Burillo, S.; Combes, F.; Usero, A.; Soria-Ruiz, R.; Tremblay, G.; Neri, R.; Fuente, A.; Morganti, R.; Oosterloo, T.
+ Astronomy & Astrophysics, Volume 549, id.A58, 14 pp._
+
+* [The stellar mass-size relation for the most isolated galaxies in the local Universe](http://adsabs.harvard.edu/abs/2013MNRAS.434..325F)
+ _Fernández Lorenzo, M.; Sulentic, J.; Verdes-Montenegro, L.; Argudo-Fernández, M.
+ Monthly Notices of the Royal Astronomical Society, Volume 434, Issue 1, p.325-335_
+
+* [The Protoplanetary Disks in the Nearby Massive Star-forming Region Cygnus OB2](http://adsabs.harvard.edu/abs/2013ApJ...773..135G)
+ _Guarcello, M. G.; Drake, J. J.; Wright, N. J.; Drew, J. E.; Gutermuth, R. A.; Hora, J. L.; Naylor, T.; Aldcroft, T.; Fruscione, A.; García-Alvarez, D.; Kashyap, V. L.; King, R.
+ The Astrophysical Journal, Volume 773, Issue 2, article id. 135, 24 pp. (2013)._
+
+* [The local luminosity function of star-forming galaxies derived from the Planck Early Release Compact Source Catalogue](http://adsabs.harvard.edu/abs/2013MNRAS.429.1309N)
+ _Negrello, M.; Clemens, M.; Gonzalez-Nuevo, J.; De Zotti, G. and 17 coauthors
+ Monthly Notices of the Royal Astronomical Society, Volume 429, Issue 2, p.1309-1323_
+
+* [A Cross-correlation Analysis of AGN and Galaxies using Virtual Observatory: Dependence on Virial Mass of Super-Massive Black Hole](http://adsabs.harvard.edu/abs/2013ApJ...775...43K)
+ _Komiya, Yutaka; Shirasaki, Yuji; Ohishi, Masatoshi; Mizumoto, Yoshihiko
+ The Astrophysical Journal, Volume 775, Issue 1, article id. 43, 12 pp. (2013)._
+
+### More Ways to Find VO-related Publications
+
+[All ADS links](http://adsabs.harvard.edu/cgi-bin/nph-abs_connect?db_key=AST&db_key=PRE&qform=AST&arxiv_sel=astro-ph&arxiv_sel=cond-mat&arxiv_sel=cs&arxiv_sel=gr-qc&arxiv_sel=hep-ex&arxiv_sel=hep-lat&arxiv_sel=hep-ph&arxiv_sel=hep-th&arxiv_sel=math&arxiv_sel=math-ph&arxiv_sel=nlin&arxiv_sel=nucl-ex&arxiv_sel=nucl-th&arxiv_sel=physics&arxiv_sel=quant-ph&arxiv_sel=q-bio&sim_query=YES&ned_query=YES&aut_logic=OR&obj_logic=OR&author=&object=&start_mon=&start_year=&end_mon=&end_year=&ttl_logic=OR&title=&txt_logic=OR&text=%22virtual+observatory%22&nr_to_return=200&start_nr=1&jou_pick=ALL&ref_stems=&data_and=ALL&group_and=ALL&start_entry_day=&start_entry_mon=&start_entry_year=&end_entry_day=&end_entry_mon=&end_entry_year=&min_score=&sort=SCORE&data_type=SHORT&aut_syn=YES&ttl_syn=YES&txt_syn=YES&aut_wt=1.0&obj_wt=1.0&ttl_wt=0.3&txt_wt=3.0&aut_wgt=YES&obj_wgt=YES&ttl_wgt=YES&txt_wgt=YES&ttl_sco=YES&txt_sco=YES&version=1) mentioning the "virtual observatory" in the abstract
+
+[All refereed publications](http://adsabs.harvard.edu/cgi-bin/nph-abs_connect?db_key=AST&qform=AST&arxiv_sel=astro-ph&arxiv_sel=cond-mat&arxiv_sel=cs&arxiv_sel=gr-qc&arxiv_sel=hep-ex&arxiv_sel=hep-lat&arxiv_sel=hep-ph&arxiv_sel=hep-th&arxiv_sel=math&arxiv_sel=math-ph&arxiv_sel=nlin&arxiv_sel=nucl-ex&arxiv_sel=nucl-th&arxiv_sel=physics&arxiv_sel=quant-ph&arxiv_sel=q-bio&sim_query=YES&ned_query=YES&aut_logic=OR&obj_logic=OR&author=&object=&start_mon=&start_year=&end_mon=&end_year=&ttl_logic=OR&title=&txt_logic=OR&text=%22virtual+observatory%22&nr_to_return=200&start_nr=1&jou_pick=NO&ref_stems=&data_and=ALL&group_and=ALL&start_entry_day=&start_entry_mon=&start_entry_year=&end_entry_day=&end_entry_mon=&end_entry_year=&min_score=&sort=SCORE&data_type=SHORT&aut_syn=YES&ttl_syn=YES&txt_syn=YES&aut_wt=1.0&obj_wt=1.0&ttl_wt=0.3&txt_wt=3.0&aut_wgt=YES&obj_wgt=YES&ttl_wgt=YES&txt_wgt=YES&ttl_sco=YES&txt_sco=YES&version=1) mentioning the "virtual observatory" in the abstract
+
+---
+
+# VO calendar
+
+* **26-28 September, 2013 - [IVOA Interoperability Meeting](http://www.usvao.org/ivoa-sept-2013/)**
+
+ (Waikoloa, Hawaii, USA)
+
+ The IVOA Interop Meetings are aimed at making significant progress in defining
+ standards and sharing best practices in the development of the world wide
+ Virtual Observatory initiatives. The fall interop will be held just prior to
+ the ADASS Conference (September 26-28), in the same venue. ADASS participants
+ are welcome to attend; there is no registration fee.
+
+* **29 Sept - 3 October 2013 - [Astronomical Data Analysis Software and Systems (ADASS)](http://www.adass.org/index.html)**
+
+ (Waikoloa, Hawaii, USA)
+
+ The ADASS conference provides a forum for scientists and programmers
+ concerned with algorithms, software and software systems employed in the
+ acquisition, reduction, analysis, and dissemination of astronomical data.
+
+* **13-15 November, 2013 - [Hot-wiring the Transient Universe III](http://hotwireduniverse.org/)**
+
+ (Santa Fe, New Mexico, USA)
+
+ Hot-wiring the Transient Universe 3 will explore opportunities and challenges
+ of massively parallel time domain surveys coupled with rapid coordinated
+ multi-wavelength follow-up observations. The interdisciplinary agenda includes
+ future and ongoing science investigations, information infrastructure for
+ publishing observations in real time, as well as novel data science to
+ classify events and systems to optimize follow-up campaigns.
+
+* **November 18, 2013 - [Data-Intensive Scalable Computing Systems (DISCS-2013)](https://ft.ornl.gov/discs-2013/?q=home)**
+
+ (Denver, Colorado, USA)
+
+ The primary goal of the workshop is to bring together researchers and other
+ interested people in the areas of data intensive computing and high
+ performance parallel computing to exchange ideas and discuss approaches for
+ addressing the challenges facing data intensive computing at the extreme
+ scale.
+
+* **9-13 December, 2013 - [Astroinformatics 2013: Knowledge from Data](http://tinyurl.com/astroinfo)**
+
+ (Sydney, Australia)
+
+ Astroinformatics is an emerging discipline at the intersection of
+ astronomy/astrophysics and applied computer science and engineering.
+ Registration and abstract submission for Astroinformatics 2013 are now open.
+
+* **17-19 December 2013 - [VO-Day & Friends](http://vobs.astro.it/index.php/vofriends)**
+
+ (Catania, Italy)
+
+ This workshop, organized by VObs.it and IA2, on behalf of the EURO-VO project,
+ will be a 3-day meeting for the Italian community focusing on VO dissemination
+ and tutorials, the connections of VO with grid/cloud/HPC, and hands-on work on
+ science gateways.
+
+* **7 January 2014 - Building the Astronomical Information Sciences: From NASA's AISR Program to the New AAS Working Group on Astroinformatics and Astrostatistics**
+
+ This special session at the 223rd AAS meeting will showcase science results
+ that were at least partially enabled by modern astroinformatics and
+ astrostatistics tools. There will also be a poster session associated with this
+ Special Session. Abstracts are being accepted via the regular AAS form and are
+ due October 1, 2013.
+
+* **17-20 June, 2014 - [LISA (Library and Information Services in Astronomy VII)](http://www.oacn.inaf.it/lisa7_2014/)**
+
+ (Naples, Italy)
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