The Close AGN Reference Survey (CARS) - IFU survey data and the BH mass dependence of long-term AGN variability

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Volume 659 (March 2022)

A&A, 659 (2022) A124

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Table 2.

Observational parameters.

Target	Instrument ^(a)	Date ^(b)	t_exp^(c)	θ_FWHM^(d)	q_phot^(e)	ID ^(f)	Comment ^(g)
		[yyyy-mm–dd]	[s]	[″]
HE0021−1810	MUSE/WFM	2015-01-12	700	0.77	0.85	094.B-0345(A)	Twilight observations
HE0021−1819	MUSE/WFM	2015-01-12	1400	0.61	1.05	094.B-0345(A)
HE0040−1105	MUSE/WFM	2015-01-12	800	0.62	1.10	094.B-0345(A)
HE0045−2145	MUSE/WFM	2015-07-18	900	0.66	0.97	095.B-0015(A)	Starburst galaxy
HE0108−4743	MUSE/WFM	2015-01-11	600	1.32	1.59	094.B-0345(A)
HE0114−0015	MUSE/WFM	2015-08-24	900	0.50	1.10	095.B-0015(A)
HE0119−0118	MUSE/WFM	2015-01-12	600	0.65	1.03	094.B-0345(A)
HE0150−0344	MUSE/WFM	2015-01-10	1200	1.07	1.03	094.B-0345(A)	Starburst galaxy
HE0203−0031	MUSE/WFM	2015-07-18	800	1.12	0.91	095.B-0015(A)	Changing-look AGN
HE0212−0059	MUSE/WFM	2017-11-14	7700	0.58	0.97	099.B-0249(A)	Changing-look AGN
HE0224−2834	MUSE/WFM	2015-08-11	900	1.47	0.95	095.B-0015(A)
HE0227−0913	MUSE/WFM	2015-01-10	1200	1.03	1.01	094.B-0345(A)
HE0232−0900	MUSE/WFM	2015-01-11	1200	1.03	1.99	094.B-0345(A)
HE0253−1641	MUSE/WFM	2014-12-26	800	0.84	1.63	094.B-0345(A)
HE0345+0056	MUSE/WFM	2014-12-26	1600	0.80	1.02	094.B-0345(A)
HE0351+0240	MUSE/WFM	2014-12-26	1600	0.65	1.66	094.B-0345(A)
HE0412−0803	MUSE/WFM	2014-11-30	1600	0.67	1.09	094.B-0345(A)
HE0429−0247	MUSE/WFM	2015-01-10	3200	0.85	1.85	094.B-0345(A)
HE0433−1028	MUSE/WFM	2014-12-28	1800	0.51	1.59	094.B-0345(A)
HE0853−0126	PMAS/Larr	2018-12-10	2400	1.15	1.47	H18-3.5-010
HE0853+0102	MUSE/WFM	2015-01-12	2400	0.59	1.04	094.B-0345(A)
HE0934+0119	MUSE/WFM	2015-04-13	1350	0.66	1.01	095.B-0015(A)
HE0949−0122	PMAS/Larr	2018-12-10	3300	1.71	1.65	H18-3.5-010
HE1011−0403	MUSE/WFM	2015-01-14	600	0.72	1.07	094.B-0345(A)
HE1017−0305	MUSE/WFM	2015-06-25	900	0.64	1.11	095.B-0015(A)
HE1029−1831	MUSE/WFM	2015-01-14	600	0.62	1.08	094.B-0345(A)
HE1107−0813	MUSE/WFM	2015-07-11	2700	0.61	1.09	095.B-0015(A)
HE1108−2813	MUSE/WFM	2015-01-15	400	0.43	0.98	094.B-0345(A)
HE1126−0407	MUSE/WFM	2015-07-11	1800	0.70	1.08	095.B-0015(A)
HE1237−0504	MUSE/WFM	2017-04-24	2700	0.46	0.98	099.B-0242(B)	No sky frames taken
HE1248−1356	MUSE/WFM	2015-07-11	600	0.47	0.96	095.B-0015(A)
HE1310−1051	VIMOS/HR-blue-old	2009-04-22	2000	1.69	0.73	083.B-0801(A)
	VIMOS/HR-orange	2009-04-25	3000	1.39	1.04	083.B-0801(A)
HE1330−1013	MUSE/WFM	2015-06-20	600	0.67	0.82	095.B-0015(A)
HE1338−1423	VIMOS/HR-blue-old	2009-04-27	2000	1.44	0.77	083.B-0801(A)
	VIMOS/HR-orange	2009-04-27	3000	1.35	0.97	083.B-0801(A)
HE1353−1917	MUSE/WFM	2015-06-20	900	0.69	0.85	095.B-0015(A)
HE1417−0909	MUSE/WFM	2015-06-20	1350	0.65	0.61	095.B-0015(A)
HE2128−0221	MUSE/WFM	2015-05-21	1350	0.70	0.90	095.B-0015(A)
HE2211−3903	MUSE/WFM	2015-05-28	900	0.42	0.80	095.B-0015(A)
HE2222−0026	MUSE/WFM	2015-06-19	1350	0.60	0.91	095.B-0015(A)
HE2233+0124	MUSE/WFM	2015-06-25	1350	0.77	0.57	095.B-0015(A)
HE2302−0857	MUSE/WFM	2015-05-29	600	0.63	1.13	095.B-0015(A)

Notes.

^(a)

IFU instrument used to conduct the observations for a given target. The no-AO mode with the nominal wavelength range is used for MUSE, the Lens-Array with 1″ sampling for PMAS, and the 066 sampling for the high-resolution grating observations with VIMOS.

^(b)

Date of the observing night for the observations.

^(c)

Total on source exposure time combined for the final cube after rejecting low-quality individual exposures.

^(d)

Seeing in the final combined cubes inferred from 2D Moffat modeling of the broad Hα (or Hβ for the VIMOS/HR-blue setup) intensity maps. In case of Mrk1018 and the two starburst galaxies, we use the median FWHM of the guide star instead which is less precise.

^(e)

Empirically estimated photometric scale factor q_phot = f_IFU/f_ref between the MUSE data and PANSTARRS or SKYMAPPER broad band images.

^(f)

Proposal ID of the data set under which the program was executed at the respective observatories.

^(g)

Additional important comment about the observation or the target itself.

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