{"id":612,"date":"2020-05-05T19:17:36","date_gmt":"2020-05-05T17:17:36","guid":{"rendered":"http:\/\/ahead.astropa.inaf.it\/?page_id=612"},"modified":"2022-07-02T11:03:54","modified_gmt":"2022-07-02T09:03:54","slug":"beatrixinaf-oab-ahead-2020","status":"publish","type":"page","link":"http:\/\/ahead.astropa.inaf.it\/index.php\/infrastructures-ahead-2020\/beatrixinaf-oab-ahead-2020\/","title":{"rendered":"BeaTriX@INAF\/OAB"},"content":{"rendered":"<p>BEaTriX, Merate, Lecco, Italy<\/p>\n<p lang=\"it-IT\" align=\"justify\"><span lang=\"en-US\">BEaTriX (Beam Expander Testing X-ray facility) is a laboratory present at <\/span><span lang=\"en-US\">INAF-Osservatorio Astronomico Brera in its premises of Merate. It is a unique pathfinder facility characterized by a <\/span><span lang=\"en-US\">broad (170 <\/span><span lang=\"en-US\">\u00d7<\/span><span lang=\"en-US\"> 60 mm<\/span><sup><span lang=\"en-US\">2<\/span><\/sup><span lang=\"en-US\">), uniform and parallel X-ray beam (divergence <\/span><span lang=\"en-US\">\u223c<\/span> <span lang=\"en-US\">2 arcsec HEW) <\/span><span lang=\"en-US\">at the energy of 4.51 keV<\/span><span lang=\"en-US\">, highly monochromatic (FWHM = 30-50 eV). A second beam line is going to be added at the energy of 1.49 keV.<\/span><\/p>\n<p>The system is very compact (9 \u00d7 18 m2), positioned on a stable foundation (gray in Figure 1) designed and built to isolate the beam line from vibrations. The facility works at a vacuum level of 10-3 mbar, easily evacuated in a short time. The vacuum pumping system is entirely based on magnetic turbo pumps, and oil-free pre-vacuum and backing pumps, to avoid optics contamination. The small size of the facility also contributes to reduce the evacuation time with respect to bigger X-ray facilities. Moreover, the modular compartments design, guaranties that the vacuum can be broken independently in the different sectors, enabling to replace the optics under test in a short time: simulations have shown that the experimental chamber (F in Figure 1) can be evacuated in about 30min. The experimental chamber opens into an ISO5 clean tent, to allow samples to be loaded and unloaded in a clean environment. Venting is performed in all the system with dried dehumidified air. A thermal box is also present therein (Figure 3), to radiatively heat the X-ray optics under test, at temperature ranging from -10 to +50 \u00b0C; some gradients can also be applied. A software based on the NI Labview platform allows all the BEaTriX operations.<\/p>\n<p>BEaTriX prime goal is to prove that it is possible to perform the acceptance tests (PSF and Aeff) of the ATHENA Silicon Pore Optics (SPO) Mirror Modules (MM) at the production rate of 3 MM\/day. Nevertheless, the facility can also be used to test other X-ray optics: the limit in size is 365 \u00d7 365 \u00d7 600 mm, given by the thermal box structure; the limit in weight is 5kg, interfacing structure included (for the SPO case, the interface is 2.6 kg), given by the hexapod maximum load (see later).<\/p>\n<table style=\"border-collapse: collapse; width: 100%;\">\n<tbody>\n<tr>\n<td style=\"width: 50%;\"><a href=\"http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2022\/07\/Beatrix_Fig1L.png\" data-rel=\"lightbox-image-0\" data-rl_title=\"\" data-rl_caption=\"\" title=\"\"><img loading=\"lazy\" decoding=\"async\" class=\"alignright size-full wp-image-992\" src=\"http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2022\/07\/Beatrix_Fig1L.png\" alt=\"\" width=\"3228\" height=\"1612\" srcset=\"http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2022\/07\/Beatrix_Fig1L.png 3228w, http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2022\/07\/Beatrix_Fig1L-300x150.png 300w, http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2022\/07\/Beatrix_Fig1L-1024x511.png 1024w, http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2022\/07\/Beatrix_Fig1L-768x384.png 768w, http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2022\/07\/Beatrix_Fig1L-1536x767.png 1536w, http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2022\/07\/Beatrix_Fig1L-2048x1023.png 2048w\" sizes=\"(max-width: 3228px) 100vw, 3228px\" \/><\/a><\/td>\n<td style=\"width: 50%;\"><a href=\"http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2022\/07\/Beatrix_Fig1R.png\" data-rel=\"lightbox-image-1\" data-rl_title=\"\" data-rl_caption=\"\" title=\"\"><img loading=\"lazy\" decoding=\"async\" class=\"alignright size-full wp-image-991\" src=\"http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2022\/07\/Beatrix_Fig1R.png\" alt=\"\" width=\"1361\" height=\"540\" srcset=\"http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2022\/07\/Beatrix_Fig1R.png 1361w, http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2022\/07\/Beatrix_Fig1R-300x119.png 300w, http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2022\/07\/Beatrix_Fig1R-1024x406.png 1024w, http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2022\/07\/Beatrix_Fig1R-768x305.png 768w\" sizes=\"(max-width: 1361px) 100vw, 1361px\" \/><\/a><\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n<p style=\"text-align: center;\"><em>Figure 1. Left: the mechanical design of the facility in the laboratory. Right: the optical design<\/em><\/p>\n<p lang=\"it-IT\" align=\"justify\"><span lang=\"en-US\">The source is a micro-focused X-ray emitter (A) with focal spot size of 35 \u00b5m <\/span><span lang=\"en-US\">\u00d7 35 \u00b5m<\/span><span lang=\"en-US\">. The 4.51 keV line is emitted by a Ti anode. The source is in UHV environment, separated by a 100 <\/span><span lang=\"en-US\">\u00b5<\/span><span lang=\"en-US\">m thick Be window. It can be aligned with mechanical adjustments in air. <\/span><span lang=\"en-US\">The flux of the Ti source was measured to be 6 \u00d7 10<\/span><sup><span lang=\"en-US\">11<\/span><\/sup><span lang=\"en-US\"> ph\/sec\/sterad. <\/span><\/p>\n<p lang=\"it-IT\" align=\"justify\"><span lang=\"en-US\">The beam is propagated through the short arm (B) onto the Optical Chamber (rectangular tank in Figure 1), where the optical components for the beam moderation are present. The parabolic mirror (C) is used for beam collimation; diffraction on 4 symmetrically cut crystals (D) have the function to monochromate the beam, while the asymmetrically cut crystal (E) expand the beam and reflect it at about 90 deg. The emerging beam has then a size of 170 mm in the horizontal direction and 60 mm in the vertical direction. <\/span><\/p>\n<p lang=\"it-IT\" align=\"justify\"><span lang=\"en-US\">An Si-PIN detector (Amptek, X123 with 25mm<\/span><sup><span lang=\"en-US\">2<\/span><\/sup><span lang=\"en-US\"> area \/ 500 <\/span><span lang=\"en-US\">\u00b5<\/span><span lang=\"en-US\">m thickness \/ 25 <\/span><span lang=\"en-US\">\u00b5<\/span><span lang=\"en-US\">m Be window) in present in front of the last crystal to monitor the flux and the alignment stability (Fig. 2 right).<\/span><\/p>\n<p lang=\"it-IT\" align=\"justify\"><span lang=\"en-US\">The monochromation system (D) can optimize either the horizontal divergence or the flux. Two different configurations can be adopted one in which the <\/span><span lang=\"en-US\">vertical divergence only is optimized (max flux), and one in which both vertical and horizontal divergences play a key role and need to be optimized. This is obtained with a rotation of the second CCC (yellow motor in Fig. 2 left). The <\/span><span lang=\"en-GB\">performance of BEaTriX in the t<\/span><span lang=\"en-US\">wo different configurations were simulated as follows, with <\/span><span lang=\"en-US\">t<\/span><span lang=\"en-GB\">he experimental results well in line with the<\/span><span lang=\"en-GB\"> expectations<\/span><span lang=\"en-US\">:<\/span><\/p>\n<ul>\n<li>\n<p lang=\"it-IT\" align=\"justify\"><span lang=\"en-US\">High flux \u2013 low collimation (CCC aligned at max flux)<\/span><\/p>\n<ul>\n<li>\n<p lang=\"it-IT\" align=\"justify\">flux = 60 ph\/s\/cm<sup>2<\/sup><\/p>\n<\/li>\n<li>\n<p lang=\"it-IT\" align=\"justify\"><span lang=\"en-US\">collimation: <\/span><span lang=\"en-GB\">HEW<\/span><span lang=\"en-GB\">ver<\/span><span lang=\"en-GB\"> = 1.46 arcsec, HEW<\/span><span lang=\"en-GB\">hor<\/span><span lang=\"en-GB\"> = 2.44 arcsec<\/span><\/p>\n<\/li>\n<\/ul>\n<\/li>\n<li>\n<p lang=\"it-IT\" align=\"justify\"><span lang=\"en-US\">Low flux \u2013 high collimation (second CCC rotated by about 10 arcsec from the position of max flux)<\/span><\/p>\n<ul>\n<li>\n<p lang=\"it-IT\" align=\"justify\">flux = 10 ph\/s\/cm<sup>2<\/sup><\/p>\n<\/li>\n<li>\n<p lang=\"it-IT\" align=\"justify\"><span lang=\"en-US\">collimation: <\/span><span lang=\"en-GB\">HEW<\/span><span lang=\"en-GB\">ver<\/span><span lang=\"en-GB\"> = 1.46 arcsec, HEW<\/span><span lang=\"en-GB\">hor<\/span><span lang=\"en-GB\"> = 4.78 arcsec<\/span><\/p>\n<\/li>\n<\/ul>\n<\/li>\n<\/ul>\n<table style=\"border-collapse: collapse; width: 100%;\">\n<tbody>\n<tr>\n<td style=\"width: 25%;\"><a href=\"http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2022\/07\/Beatrix_Fig2R-1.png\" data-rel=\"lightbox-image-2\" data-rl_title=\"\" data-rl_caption=\"\" title=\"\"><img loading=\"lazy\" decoding=\"async\" class=\"alignright size-full wp-image-1002\" src=\"http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2022\/07\/Beatrix_Fig2R-1.png\" alt=\"\" width=\"479\" height=\"284\" srcset=\"http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2022\/07\/Beatrix_Fig2R-1.png 479w, http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2022\/07\/Beatrix_Fig2R-1-300x178.png 300w\" sizes=\"(max-width: 479px) 100vw, 479px\" \/><\/a><\/td>\n<td style=\"width: 25%;\"><a href=\"http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2022\/07\/Beatrix_Fig2L.png\" data-rel=\"lightbox-image-3\" data-rl_title=\"\" data-rl_caption=\"\" title=\"\"><img loading=\"lazy\" decoding=\"async\" class=\"alignright size-full wp-image-989\" src=\"http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2022\/07\/Beatrix_Fig2L.png\" alt=\"\" width=\"511\" height=\"383\" srcset=\"http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2022\/07\/Beatrix_Fig2L.png 511w, http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2022\/07\/Beatrix_Fig2L-300x225.png 300w\" sizes=\"(max-width: 511px) 100vw, 511px\" \/><\/a><\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n<p lang=\"it-IT\"><em><span lang=\"en-US\">Figure 2. Design (left) and picture (right) of the components inside the Optical Chamber. From right: the paraboloidal mirror, the two CCCs in charge of the monochromation, the BE crystal. The Beam Monitor is visible in front of the BE.<\/span><\/em><\/p>\n<table style=\"border-collapse: collapse; width: 100%;\">\n<tbody>\n<tr>\n<td style=\"width: 33.3333%;\"><a href=\"http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2022\/07\/Beatrix_Fig3L.png\" data-rel=\"lightbox-image-4\" data-rl_title=\"\" data-rl_caption=\"\" title=\"\"><img loading=\"lazy\" decoding=\"async\" class=\"wp-image-987 aligncenter\" src=\"http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2022\/07\/Beatrix_Fig3L.png\" alt=\"\" width=\"331\" height=\"416\" \/><\/a><\/td>\n<td style=\"width: 33.3333%;\"><a href=\"http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2022\/07\/Beatrix_Fig3C.png\" data-rel=\"lightbox-image-5\" data-rl_title=\"\" data-rl_caption=\"\" title=\"\"><img loading=\"lazy\" decoding=\"async\" class=\"alignright size-full wp-image-988\" src=\"http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2022\/07\/Beatrix_Fig3C.png\" alt=\"\" width=\"1054\" height=\"796\" srcset=\"http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2022\/07\/Beatrix_Fig3C.png 1054w, http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2022\/07\/Beatrix_Fig3C-300x227.png 300w, http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2022\/07\/Beatrix_Fig3C-1024x773.png 1024w, http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2022\/07\/Beatrix_Fig3C-768x580.png 768w\" sizes=\"(max-width: 1054px) 100vw, 1054px\" \/><\/a><\/td>\n<td style=\"width: 33.3333%;\"><a href=\"http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2022\/07\/Beatrix_Fig3R.png\" data-rel=\"lightbox-image-6\" data-rl_title=\"\" data-rl_caption=\"\" title=\"\"><img loading=\"lazy\" decoding=\"async\" class=\"wp-image-986 aligncenter\" src=\"http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2022\/07\/Beatrix_Fig3R.png\" alt=\"\" width=\"304\" height=\"389\" \/><\/a><\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n<p lang=\"it-IT\" align=\"left\"><em><span lang=\"en-US\">Figure 3. Left: MM mounted on its supporting structure, connected to the hexapod. <\/span><span lang=\"en-US\">Centre: design of the MM Chamber, showing the thermal box (grey), the MM supporting structure in titanium (brown), the lightened beam in stainless-steel (grey), the hexapod (red) and the linear stage (blue). <\/span><span lang=\"en-US\">Right: top view of the thermal box inside the MM Chamber, with the top cover removed for the installation of the thermal box.<\/span><\/em><\/p>\n<p>The focused beam is propagated through the long arm (G) into the detector (H), placed at 12 m distance. The detector is a directly illuminated CCD with sensor size of 27.6 mm \u00d7 27.6 mm and pixel 13.5 mm. It is connected to the long arm, and motorized in air for movements in the vertical (range = 1500 mm) and horizontal (range = 150 mm) directions. A focal range of 500 mm is obtained also with in air motorization and a properly designed bellow in front of the CCD. The long arm is made of 6 tubes to leave the possibility to modify in the future the focal length of the facility: major setup changes will be necessary but in principle focal distances other than 12 m are possible\u00a0 (f<sub>std<\/sub> = 12000 \u00b1 250 mm; f<sub>possible-1<\/sub> = 10295 \u00b1 250 mm; f<sub>possible-2<\/sub> = 8295 \u00b1 250 mm).<\/p>\n<p><a href=\"http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2020\/12\/BEaTriX-19nov2020-scaled.jpg\" data-rel=\"lightbox-image-7\" data-rl_title=\"\" data-rl_caption=\"\" title=\"\"><img loading=\"lazy\" decoding=\"async\" class=\"alignleft size-full wp-image-865\" src=\"http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2020\/12\/BEaTriX-19nov2020-scaled.jpg\" alt=\"\" width=\"2560\" height=\"1686\" srcset=\"http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2020\/12\/BEaTriX-19nov2020-scaled.jpg 2560w, http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2020\/12\/BEaTriX-19nov2020-300x198.jpg 300w, http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2020\/12\/BEaTriX-19nov2020-1024x674.jpg 1024w, http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2020\/12\/BEaTriX-19nov2020-768x506.jpg 768w, http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2020\/12\/BEaTriX-19nov2020-1536x1011.jpg 1536w, http:\/\/ahead.astropa.inaf.it\/wp-content\/uploads\/2020\/12\/BEaTriX-19nov2020-2048x1348.jpg 2048w\" sizes=\"(max-width: 2560px) 100vw, 2560px\" \/><\/a><\/p>\n<p><em>Figure 4: A picture of the BEATriX facility in the INAF\/Osservatorio of Brera premise<\/em><\/p>\n<p lang=\"it-IT\" align=\"justify\"><span lang=\"en-US\">In the MM chamber (cylindrical tank in Figure 1, and Figure 3), the beam encounters the MM (F), and it is thereby focused. The MM is motorized in vacuum, in order to be aligned to the beam: a hexapod, with max load of 5kg, is <\/span><span lang=\"en-US\">used to this purpose (red in <\/span><span lang=\"en-US\">Figure 3 center)<\/span><span lang=\"en-US\">. The hexapod is mounted on a translational stage (blue in <\/span><span lang=\"en-US\">Figure 3 center)<\/span><span lang=\"en-US\">,<\/span><span lang=\"en-US\"> used to move the MM out from the beam, for the direct beam measurements. <\/span><span lang=\"en-US\">The MMs are installed, by means of 6 <\/span><span lang=\"en-US\">Neodymium magnets,<\/span><span lang=\"en-US\"> on a titanium interface <\/span><span lang=\"en-US\">made by 3 parts, that can be adjusted to adapt to the width of the different MMs. <\/span><span lang=\"en-US\">A<\/span><span lang=\"en-US\"> thermal box (<\/span><span lang=\"en-US\">internal size: 350 mm \u00d7 350 mm \u00d7 600 mm<\/span><span lang=\"en-US\">) is also present to radiatively cool\/heat the X-ray optics under test, in the temperature range <\/span><span lang=\"en-GB\">T=293\u00b125K. <\/span><span lang=\"en-US\">Two of the radiating panels are removable, giving accessibility to the MM and enabling possible temperature gradients of the MM in X and Y. <\/span><\/p>\n<p lang=\"it-IT\" align=\"justify\"><span lang=\"en-US\">The beam focused by the MM is propagated through the long arm (G) into the detector (H), placed at 12 m distance. The detector is a directly illuminated CCD with sensor size of 27.6 mm \u00d7 27.6 mm and pixel 13.5 <\/span><span lang=\"en-US\">\uf06d<\/span><span lang=\"en-US\">m. It is connected to the long arm, and motorized in air for movements in the vertical (range = 1500 mm) and horizontal (range = 150 mm) directions. <\/span><span lang=\"en-US\">A focal range of 500 mm is obtained also with in air motorization and a properly designed bellow in front of the CCD. The long arm is made of 6 tubes to leave the possibility to modify in the future the focal length of the facility: major setup changes will be necessary but in principle focal distances other than 12 m are possible (f<\/span><sub><span lang=\"en-US\">std<\/span><\/sub><span lang=\"en-US\"> = 12000 \u00b1 250 mm; f<\/span><sub><span lang=\"en-US\">possible-1<\/span><\/sub><span lang=\"en-US\"> = 10295 \u00b1 250 mm; f<\/span><sub><span lang=\"en-US\">possible-2<\/span><\/sub><span lang=\"en-US\"> = 8295 \u00b1 250 mm). <\/span><\/p>\n<p>Reference papers :<\/p>\n<ul>\n<li>Basso S., Salmaso B., Spiga D. et al., First light of BEaTriX, the new testing facility for the modular X-ray optics of the ATHENA mission (2022),\u00a0 arXiv e-prints, arXiv:2206.15468<\/li>\n<li>Salmaso, B., et al. BEaTriX, the Beam Expander Testing X-ray facility for testing ATHENAs SPO modules: progress in the realisation, Proc. SPIE 11119, 111190N (2019)<a href=\"https:\/\/doi.org\/10.1117\/12.2530430\"><em> https:\/\/doi.org\/10.1117\/12.2530430<\/em><\/a><\/li>\n<li>Basso, S., et al. Thermal simulations for characterization of ATHENA Mirror Modules with a radiating box in the BEaTriX facility, Proc. SPIE 111191, 111191I (2019)\u00a0<a href=\"https:\/\/doi.org\/10.1117\/12.2530622\"><em>https:\/\/doi.org\/10.1117\/12.2530622<\/em><\/a><\/li>\n<li>Spiga, D., et al. Optical simulations for the laboratory-based, expanded and collimated X-ray beam facility BEaTriX, Proc. SPIE 11110, 111100E (2019) <a href=\"https:\/\/doi.org\/10.1117\/12.2530066\"><em>https:\/\/doi.org\/10.1117\/12.2530066<\/em><\/a><\/li>\n<\/ul>\n\n","protected":false},"excerpt":{"rendered":"<p>BEaTriX, Merate, Lecco, Italy BEaTriX (Beam Expander Testing X-ray facility) is a laboratory present at INAF-Osservatorio Astronomico Brera in its premises of Merate. It is a unique pathfinder facility characterized by a broad (170 \u00d7 60 mm2), uniform and parallel X-ray beam (divergence \u223c 2 arcsec HEW) at the energy of 4.51 keV, highly monochromatic &#8230; <a title=\"BeaTriX@INAF\/OAB\" class=\"read-more\" href=\"http:\/\/ahead.astropa.inaf.it\/index.php\/infrastructures-ahead-2020\/beatrixinaf-oab-ahead-2020\/\" aria-label=\"More on BeaTriX@INAF\/OAB\">Read more<\/a><\/p>\n","protected":false},"author":245,"featured_media":0,"parent":704,"menu_order":40,"comment_status":"closed","ping_status":"closed","template":"","meta":{"_mi_skip_tracking":false,"footnotes":""},"class_list":["post-612","page","type-page","status-publish"],"_links":{"self":[{"href":"http:\/\/ahead.astropa.inaf.it\/index.php\/wp-json\/wp\/v2\/pages\/612"}],"collection":[{"href":"http:\/\/ahead.astropa.inaf.it\/index.php\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"http:\/\/ahead.astropa.inaf.it\/index.php\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"http:\/\/ahead.astropa.inaf.it\/index.php\/wp-json\/wp\/v2\/users\/245"}],"replies":[{"embeddable":true,"href":"http:\/\/ahead.astropa.inaf.it\/index.php\/wp-json\/wp\/v2\/comments?post=612"}],"version-history":[{"count":25,"href":"http:\/\/ahead.astropa.inaf.it\/index.php\/wp-json\/wp\/v2\/pages\/612\/revisions"}],"predecessor-version":[{"id":1006,"href":"http:\/\/ahead.astropa.inaf.it\/index.php\/wp-json\/wp\/v2\/pages\/612\/revisions\/1006"}],"up":[{"embeddable":true,"href":"http:\/\/ahead.astropa.inaf.it\/index.php\/wp-json\/wp\/v2\/pages\/704"}],"wp:attachment":[{"href":"http:\/\/ahead.astropa.inaf.it\/index.php\/wp-json\/wp\/v2\/media?parent=612"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}