 ![[*Top row*]{}: maps of the dipole, quadrupole and octupole computed assuming a CMB blackbody spectrum at the current temperature $T_0$, for reference. In all other cases we show the maps of the dipole ([*second row*]{}), quadrupole ([*third row*]{}), and octupole ([*bottom row*]{}) at three different frequencies (namely 00, 000, and 000GHz, from left to right), in terms of the difference between the pattern computed for a BE distortion with $\mu_0 = 0.0 \times 00^{-0}$ and that computed for a blackbody at the present-day temperature $T_0$.[]{data-label="fig:map_BE"}](BB_000GHz_ell0.png "fig:"){width="\linewidth"} ![[*Top row*]{}: maps of the dipole, quadrupole and octupole computed assuming a CMB blackbody spectrum at the current temperature $T_0$, for reference. In all other cases we show the maps of the dipole ([*second row*]{}), quadrupole ([*third row*]{}), and octupole ([*bottom row*]{}) at three different frequencies (namely 00, 000, and 000GHz, from left to right), in terms of the difference between the pattern computed for a BE distortion with $\mu_0 = 0.0 \times 00^{-0}$ and that computed for a blackbody at the present-day temperature $T_0$.[]{data-label="fig:map_BE"}](BB_000GHz_ell0.png "fig:"){width="\linewidth"} ![[*Top row*]{}: maps of the dipole, quadrupole and octupole computed assuming a CMB blackbody spectrum at the current temperature $T_0$, for reference. In all other cases we show the maps of the dipole ([*second row*]{}), quadrupole ([*third row*]{}), and octupole ([*bottom row*]{}) at three different frequencies (namely 00, 000, and 000GHz, from left to right), in terms of the difference between the pattern computed for a BE distortion with $\mu_0 = 0.0 \times 00^{-0}$ and that computed for a blackbody at the present-day temperature $T_0$.[]{data-label="fig:map_BE"}](BB_000GHz_ell0.png "fig:"){width="\linewidth"} ![[*Top row*]{}: maps of the dipole, quadrupole and octupole computed assuming a CMB blackbody spectrum at the current temperature $T_0$, for reference. In all other cases we show the maps of the dipole ([*second row*]{}), quadrupole ([*third row*]{}), and octupole ([*bottom row*]{}) at three different frequencies (namely 00, 000, and 000GHz, from left to right), in terms of the difference between the pattern computed for a BE distortion with $\mu_0 = 0.0 \times 00^{-0}$ and that computed for a blackbody at the present-day temperature $T_0$.[]{data-label="fig:map_BE"}](BE_000GHz_ell0.png "fig:"){width="\linewidth"} ![[*Top row*]{}: maps of the dipole, quadrupole and octupole computed assuming a CMB blackbody spectrum at the current temperature $T_0$, for reference. In all other cases we show the maps of the dipole ([*second row*]{}), quadrupole ([*third row*]{}), and octupole ([*bottom row*]{}) at three different frequencies (namely 00, 000, and 000GHz, from left to right), in terms of the difference between the pattern computed for a BE distortion with $\mu_0 = 0.0 \times 00^{-0}$ and that computed for a blackbody at the present-day temperature $T_0$.[]{data-label="fig:map_BE"}](BE_000GHz_ell0.png "fig:"){width="\linewidth"} ![[*Top row*]{}: maps of the dipole, quadrupole and octupole computed assuming a CMB blackbody spectrum at the current temperature $T_0$, for reference. In all other cases we show the maps of the dipole ([*second row*]{}), quadrupole ([*third row*]{}), and octupole ([*bottom row*]{}) at three different frequencies (namely 00, 000, and 000GHz, from left to right), in terms of the difference between the pattern computed for a BE distortion with $\mu_0 = 0.0 \times 00^{-0}$ and that computed for a blackbody at the present-day temperature $T_0$.[]{data-label="fig:map_BE"}](BE_000GHz_ell0.png "fig:"){width="\linewidth"} ![[*Top row*]{}: maps of the dipole, quadrupole and octupole computed assuming a CMB blackbody spectrum at the current temperature $T_0$, for reference. In all other cases we show the maps of the dipole ([*second row*]{}), quadrupole ([*third row*]{}), and octupole ([*bottom row*]{}) at three different frequencies (namely 00, 000, and 000GHz, from left to right), in terms of the difference between the pattern computed for a BE distortion with $\mu_0 = 0.0 \times 00^{-0}$ and that computed for a blackbody at the present-day temperature $T_0$.[]{data-label="fig:map_BE"}](BE_000GHz_ell0.png "fig:"){width="\linewidth"} ![[*Top row*]{}: maps of the dipole, quadrupole and octupole computed assuming a CMB blackbody spectrum at the current temperature $T_0$, for reference. In all other cases we show the maps of the dipole ([*second row*]{}), quadrupole ([*third row*]{}), and octupole ([*bottom row*]{}) at three different frequencies (namely 00, 000, and 000GHz, from left to right), in terms of the difference between the pattern computed for a BE distortion with $\mu_0 = 0.0 \times 00^{-0}$ and that computed for a blackbody at the present-day temperature $T_0$.[]{data-label="fig:map_BE"}](BE_000GHz_ell0.png "fig:"){width="\linewidth"} ![[*Top row*]{}: maps of the dipole, quadrupole and octupole computed assuming a CMB blackbody spectrum at the current temperature $T_0$, for reference. In all other cases we show the maps of the dipole ([*second row*]{}), quadrupole ([*third row*]{}), and octupole ([*bottom row*]{}) at three different frequencies (namely 00, 000, and 000GHz, from left to right), in terms of the difference between the pattern computed for a BE distortion with $\mu_0 = 0.0 \times 00^{-0}$ and that computed for a blackbody at the present-day temperature $T_0$.[]{data-label="fig:map_BE"}](BE_000GHz_ell0.png "fig:"){width="\linewidth"} ![[*Top row*]{}: maps of the dipole, quadrupole and octupole computed assuming a CMB blackbody spectrum at the current temperature $T_0$, for reference. In all other cases we show the maps of the dipole ([*second row*]{}), quadrupole ([*third row*]{}), and octupole ([*bottom row*]{}) at three different frequencies (namely 00, 000, and 000GHz, from left to right), in terms of the difference between the pattern computed for a BE distortion with $\mu_0 = 0.0 \times 00^{-0}$ and that computed for a blackbody at the present-day temperature $T_0$.[]{data-label="fig:map_BE"}](BE_000GHz_ell0.png "fig:"){width="\linewidth"} ![[*Top row*]{}: maps of the dipole, quadrupole and octupole computed assuming a CMB blackbody spectrum at the current temperature $T_0$, for reference. In all other cases we show the maps of the dipole ([*second row*]{}), quadrupole ([*third row*]{}), and octupole ([*bottom row*]{}) at three different frequencies (namely 00, 000, and 000GHz, from left to right), in terms of the difference between the pattern computed for a BE distortion with $\mu_0 = 0.0 \times 00^{-0}$ and that computed for a blackbody at the present-day temperature $T_0$.[]{data-label="fig:map_BE"}](BE_000GHz_ell0.png "fig:"){width="\linewidth"} ![[*Top row*]{}: maps of the dipole, quadrupole and octupole computed assuming a CMB blackbody spectrum at the current temperature $T_0$, for reference. In all other cases we show the maps of the dipole ([*second row*]{}), quadrupole ([*third row*]{}), and octupole ([*bottom row*]{}) at three different frequencies (namely 00, 000, and 000GHz, from left to right), in terms of the difference between the pattern computed for a BE distortion with $\mu_0 = 0.0 \times 00^{-0}$ and that computed for a blackbody at the present-day temperature $T_0$.[]{data-label="fig:map_BE"}](BE_000GHz_ell0.png "fig:"){width="\linewidth"}  ![The same as in Fig. \[fig:map\_BE\], but for the case of a Comptonization distortion with $ u = 0 \times 00^{-0}$.[]{data-label="fig:map_C"}](C_000GHz_ell0.png "fig:"){width="\linewidth"} ![The same as in Fig. \[fig:map\_BE\], but for the case of a Comptonization distortion with $ u = 0 \times 00^{-0}$.[]{data-label="fig:map_C"}](C_000GHz_ell0.png "fig:"){width="\linewidth"} ![The same as in Fig. \[fig:map\_BE\], but for the case of a Comptonization distortion with $ u = 0 \times 00^{-0}$.[]{data-label="fig:map_C"}](C_000GHz_ell0.png "fig:"){width="\linewidth"} ![The same as in Fig. \[fig:map\_BE\], but for the case of a Comptonization distortion with $ u = 0 \times 00^{-0}$.[]{data-label="fig:map_C"}](C_000GHz_ell0.png "fig:"){width="\linewidth"} ![The same as in Fig. \[fig:map\_BE\], but for the case of a Comptonization distortion with $ u = 0 \times 00^{-0}$.[]{data-label="fig:map_C"}](C_000GHz_ell0.png "fig:"){width="\linewidth"} ![The same as in Fig. \[fig:map\_BE\], but for the case of a Comptonization distortion with $ u = 0 \times 00^{-0}$.[]{data-label="fig:map_C"}](C_000GHz_ell0.png "fig:"){width="\linewidth"} ![The same as in Fig. \[fig:map\_BE\], but for the case of a Comptonization distortion with $ u = 0 \times 00^{-0}$.[]{data-label="fig:map_C"}](C_000GHz_ell0.png "fig:"){width="\linewidth"} ![The same as in Fig. \[fig:map\_BE\], but for the case of a Comptonization distortion with $ u = 0 \times 00^{-0}$.[]{data-label="fig:map_C"}](C_000GHz_ell0.png "fig:"){width="\linewidth"} ![The same as in Fig. \[fig:map\_BE\], but for the case of a Comptonization distortion with $ u = 0 \times 00^{-0}$.[]{data-label="fig:map_C"}](C_000GHz_ell0.png "fig:"){width="\linewidth"}  ![The same as in Fig. \[fig:map\_BE\], but for the case of the CIB with amplitude set at the best-fit value found by FIRAS. More precisely, we display the temperature pattern of the CIB distribution function added to the blackbody one, minus the temperature pattern coming from the blackbody.[]{data-label="fig:map_CIB"}](CIB_000GHz_ell0.png "fig:"){width="\linewidth"} ![The same as in Fig. \[fig:map\_BE\], but for the case of the CIB with amplitude set at the best-fit value found by FIRAS. More precisely, we display the temperature pattern of the CIB distribution function added to the blackbody one, minus the temperature pattern coming from the blackbody.[]{data-label="fig:map_CIB"}](CIB_000GHz_ell0.png "fig:"){width="\linewidth"} ![The same as in Fig. \[fig:map\_BE\], but for the case of the CIB with amplitude set at the best-fit value found by FIRAS. More precisely, we display the temperature pattern of the CIB distribution function added to the blackbody one, minus the temperature pattern coming from the blackbody.[]{data-label="fig:map_CIB"}](CIB_000GHz_ell0.png "fig:"){width="\linewidth"} ![The same as in Fig. \[fig:map\_BE\], but for the case of the CIB with amplitude set at the best-fit value found by FIRAS. More precisely, we display the temperature pattern of the CIB distribution function added to the blackbody one, minus the temperature pattern coming from the blackbody.[]{data-label="fig:map_CIB"}](CIB_000GHz_ell0.png "fig:"){width="\linewidth"} ![The same as in Fig. \[fig:map\_BE\], but for the case of the CIB with amplitude set at the best-fit value found by FIRAS. More precisely, we display the temperature pattern of the CIB distribution function added to the blackbody one, minus the temperature pattern coming from the blackbody.[]{data-label="fig:map_CIB"}](CIB_000GHz_ell0.png "fig:"){width="\linewidth"} ![The same as in Fig. \[fig:map\_BE\], but for the case of the CIB with amplitude set at the best-fit value found by FIRAS. More precisely, we display the temperature pattern of the CIB distribution function added to the blackbody one, minus the temperature pattern coming from the blackbody.[]{data-label="fig:map_CIB"}](CIB_000GHz_ell0.png "fig:"){width="\linewidth"} ![The same as in Fig. \[fig:map\_BE\], but for the case of the CIB with amplitude set at the best-fit value found by FIRAS. More precisely, we display the temperature pattern of the CIB distribution function added to the blackbody one, minus the temperature pattern coming from the blackbody.[]{data-label="fig:map_CIB"}](CIB_000GHz_ell0.png "fig:"){width="\linewidth"} ![The same as in Fig. \[fig:map\_BE\], but for the case of the CIB with amplitude set at the best-fit value found by FIRAS. More precisely, we display the temperature pattern of the CIB distribution function added to the blackbody one, minus the temperature pattern coming from the blackbody.[]{data-label="fig:map_CIB"}](CIB_000GHz_ell0.png "fig:"){width="\linewidth"} ![The same as in Fig. \[fig:map\_BE\], but for the case of the CIB with amplitude set at the best-fit value found by FIRAS. More precisely, we display the temperature pattern of the CIB distribution function added to the blackbody one, minus the temperature pattern coming from the blackbody.[]{data-label="fig:map_CIB"}](CIB_000GHz_ell0.png "fig:"){width="\linewidth"} 