VizieR Online Data Catalog: Multiwavelength obs. of BL Lac in 2012-2013 (Wehrle+, 2016)

Our Herschel target of opportunity observations began on 2012 October 29 (MJD 56229) and continued for the three-month visibility window. We arranged for daily Swift pointings starting on 2012 October 27 through 2013 February 1. We also arranged for two intense periods of every-orbit Swift monitoring on 2012 December 11-12 and 2013 January 11-12. We obtained target of opportunity observations with NuSTAR on 2012 December 11-12. Observations of BL Lac every two to four days were carried out at the SMA on Mauna Kea, HI during the Herschel observation window, and intermittently thereafter. Monitoring observations with CARMA at 3mm were already underway. VLBA monitoring continued throughout the time range reported here as part of the ongoing Boston University (BU) γ-ray blazar monitoring program. Observations at other wavebands were already underway by other collaborations, e.g., the Whole Earth Blazar Telescope. In addition, roughly weekly Swift observations have been carried out for several years by A. Falcone and M. Stroh (Stroh & Falcone 2013ApJS..207...28S).

Herschel SPIRE and PACS FIR observations of BL Lac are presented in table 1 and sections 2.2 and 2.5. SMA millimeter and submillimeter observations are presented in tables 1, 2 and 3 and sections 2.3 and 2.5. Millimeter observations with CARMA are presented in table 4 and sections 2.4 and 2.5. Swift optical, UV and X-ray observations are presented in tables 5 and 6 and section 2.6. Hard X-ray observations with NuSTAR are presented in section 2.7. γ-ray observations with Fermi are presented in section 2.8. The 7mm band observations are presented in section 2.9. The BU group obtained 2.4-10keV X-ray fluxes with the RXTE PCA three times per week from 2005 March 3 to 2011 December 31; see table 10 and Appendix.

(7 data files).