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The archive of digitized plates obtained on Wide aperture Maksutov meniscus telescope with main mirror 50 cm at the Fesenkov Astrophysical Institute (FAI), Almaty, Kazakhstan. They represent the results of photometric and spectral observations of stars, star clusrets, active galaxies, nebulaes, etc. for about 50 years - from 1950 to 1997. Observations were carried out in the optical range. Telescope specifications: diameter of main mirror D = 500 mm, focal length F = 1200 mm.

Sgr E is a massive star formation complex found toward the Galactic center that consists of numerous discrete, compact HII regions. It is located at the intersection between the central molecular zone (CMZ) and the far dust lane of the Galactic bar, similar to "hot spots" seen in external galaxies. Compared with other Galactic star formation complexes, the Sgr E complex is unusual because its HII regions all have similar radio luminosities and angular extents, and they are deficient in ~10{mu}m emission from their photodissociation regions (PDRs). Our Green Bank Telescope radio recombination line observations increase the known membership of Sgr E to 19 HII regions. There are 43 additional HII region candidates in the direction of Sgr E, 26 of which are detected for the first time here using MeerKAT 1.28GHz data. Therefore, the true HII region population of Sgr E may number >60. Using APEX SEDIGISM ^13^CO 2->1 data we discover a 3.0x10^5^M_{sun}_ molecular cloud associated with Sgr E, but find few molecular or far-infrared concentrations at the locations of the Sgr E HII regions. Comparison with simulations and an analysis of its radio continuum properties indicate that Sgr E formed upstream in the far dust lane of the Galactic bar a few million years ago and will overshoot the CMZ, crashing into the near dust lane. We propose that the unusual infrared properties of the Sgr E HII regions are caused by their orbits about the Galactic center, which have possibly stripped their PDRs. Cone search capability for table J/ApJ/901/51/table2 (SgrE HII region radio continuum parameters) Cone search capability for table J/ApJ/901/51/table3 (Candidate SgrE HII region radio continuum parameters) Cone search capability for table J/ApJ/901/51/table4 (NH3 line parameters)

Slides presented by the speakers at the International Conference "Digital Publishing for the Humanities - Nw Technologies and Ideas" - Rome, Bibliotheca Hertziana - Max Planck Institute for Art History 18-19 October 2022

The archive of digitized plates obtained on AZT-8 at the Fesenkov Astrophysical Institute (FAI), Almaty, Kazakhstan. They represent the results of photometric observations of stars, comets, nebulae etc. for 50 years - from 1950 to 2000. Observations were carried out in the optical range. Telescope specifications: diameter of main mirror D = 700 mm, focal length F = 11000 mm.

These bathymetric data were produced using the interferometric side-scan sonar onboard the Haliotis Research Vessel, Operated by Genavir, for the French Oceanographic Fleet, in September 2022, during the oceanographic campaign HISOPE (l'Haliotis pour l’Imagerie Sismique d’Orbetello et Pyrgi Etrusques). The investigated area is located in front of the prominent archeological site of Pyrgi, the etruscan harbor of Cerveteri. At the site, next to the sea, is found a series of etruscan temples, surrounded by an etruscan city largely destroyed by coastal erosion. A roman castrum dating back to the 3rd century BCE covers part of the site and is also partly eroded by the sea. Above the castrum is built a fortified medieval village as well as a large renaissance castle (Santa Severa), built over a submerged lava dome (the Massicciata reef). In 2019, foundations of an etruscan monument were discovered 150 m offhshore, over a larger reef located south of the archeological site (the Secche di Macchiatonda). The goal of this campaign was to map the seafloor along this stretch of eroded coastline, in order to determine the location of the coastline in Etruscan time, such as to better understand the geography of the site when the harbor was settled. One of the main questions is why this specific site was chosen to develop a port, despite its exposure to waves. Acquisition took place under stormy conditions, such that only 1.5 day of acquisition was possible over the 7 days planned. Geoswath mapping was conducted under heavy swell conditions along the sandy coast, north of of the castle of Santa Severa, then in front of the sandy coast, south of the castle, and finally over the extensive Secche di Macchiatonda reef in the south. Data were acquired by eng. Quentin Layahe, Genavir, onboard the Haliotis, piloted by Serge Garcia, and post-processed using the software Globe, developed by the IFREMER, by Dr.Gilles Brocard (Archéorient, University of Lyon 2, France) and Alessandro Conforti, research engineer at the CNR (Italian national center for research) at Orosi, Sardinia.

Das EBDC Business Expectations Panel, BEP, besteht aus den wichtigsten Variablen des ifo Konjunkturtests und den entsprechenden Bilanzdaten aus den Unternehmensdatenbanken Amadeus (Bureau van Dijk) und Hoppenstedt (Hoppenstedt Firmeninformationen GmbH). Der ifo Konjunkturtest wird monatlich vom ifo Institut erhoben. Er setzt sich aus den EInzelerhebungen für die Sektoren Bau, Dienstleister, Handel und Verarbeitendes Gewerbe zusammen. Kern des Fragenprogramms sind qualitative Urteile zu aktuellen ökonomischen Parametern der Unternehmen wie z.B. der allgemeinen Situation, dem Umsatz, der Nachfrage, Kreditrestriktionen oder den Beschäftigten sowie Fragen zu den Entwicklungen in den kommenden Monaten, u.a. den Geschäfts-, Beschäftigten- oder Preiserwartungen. Die Bilanzdaten der Unternehmensdatenbanken wurden mit Hilfe der Programms Matching-Software MTB (Merge Toolbox), welche am „Center for quantitative Methods and Survey Research“ der Universität Konstanz entwickelt wurde dazu gespielt. The EBDC Business Expectations Panel, BEP, consists of the main variables of the ifo Business Survey and the corresponding balance sheet data from firm databases Amadeus (Bureau vanDijk) and Hoppenstedt(Hoppenstedt Information GmbH).The ifo Business Survey has been conducted by the ifo Institute on a monthly basis. The core of the questionnaire consists of qualitative assessments on the current economic parameters of companies such as, for example, the general situation, turnover, demand, credit constraints and staff numbers, as well as questions on trends in the forthcoming months in areas like business, employment and price expectations. The financial variables were merged by using the matching software MTB (Merge Toolbox) developed at the Center for Quantitative Methods and Survey Research of the University of Konstanz. Self-administered questionnaire

The archive of digitized plates obtained on Schmidt telescope (large camera) at the Fesenkov Astrophysical Institute (FAI), Almaty, Kazakhstan. They represent the results of photometric observations of stars, star clusrets, active galaxies, nebulaes, etc. for 35 years - from 1964 to 1989. Observations were carried out in the optical range. Telescope specifications: diameter of main mirror D = 397 mm, focal length F = 773 mm.

These bathymetric data were produced using the interferometric side-scan sonar onboard the Haliotis Research Vessel, Operated by Genavir, for the French Oceanographic Fleet, in October 2022, during the oceanographic campaign HISOPE (l'Haliotis pour l’Imagerie Sismique d’Orbetello et Pyrgi Etrusques). The investigated area is located in front of the tombolo di Feniglia, in the Gulf of Porto Ercole. The goal of the campaign was to image the sedimentary architecture of the Tombolo di Feniglia Acquisition took place from October 1st to October 6th 2022. Data were acquired by eng. Quentin Layahe, Genavir, onboard the Haliotis, piloted by Serge Garcia, and post-processed using the software Globe, developed by the IFREMER, by Dr.Gilles Brocard (Archéorient, University of Lyon 2, France) and Alessandro Conforti, research engineer at the CNR (Italian national center for research) at Orosi, Sardinia.