Constraining the geometry of the nuclear wind in PDS 456 using a novel emission model

Free Access

Table 1.

Journal of the observations.

Epoch	Telescope	Obs. ID	Date and time	T_tot (ks)^a	Instrument	T_net (ks)^b	Net counts (k)^c	Extraction^d
3	XMM	0721010501	2013-09-15 18:30:00	120.5	pn	102.2	207.6	35/60
	NuSTAR	60002032006	2013-09-15 17:56:07	119.1	FPMA	44.0	4.3	80/80
					FPMB	44.0	4.0	80/80

4	XMM	0721010501	2013-09-20 02:29:39	112.1	pn	94.9	188.5	35/60
	NuSTAR	60002032008	2013-09-20 03:06:07	113.8	FPMA	58.5	5.9	80/80
					FPMB	58.5	5.7	80/80

Notes.

^(a),(b)

Observation lengths, in ks, before and after filtering, respectively.

^(c)

Net counts in units of 10³ photons in the 3–10(30) keV band for XMM-Newton(NuSTAR).

^(d)

Extraction regions for source and/or background in arcsec.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.