Rosario González-Riestra and Pedro M. Rodríguez-Pascual
XMM-Newton Science Operations Centre, ESAC
Introduction
BiRD is a browsing and visualization tool for XMM-Newton RGS fluxed
spectra. It allows the user to browse and examine the data before
downloading them from the XSA for full analysis.
The BiRD interface makes possible to select spectra through a variety
of parameters, such as (e.g.) date of observation, level of exposure
or type of object.
It also provides some basic visualization utilities, both for the RGS
spectra and spectral images, as well as for the EPIC-pn images taken
in parallel.
What is RGS?
The Reflection Grating Spectrometer in one of the instruments
on-board XMM-Newton. Its purpose is to obtain high spectral
resolution (from 100 to 500, FWHM) X-ray spectroscopy in the range
5-38 Å.
Two of the three XMM-Newton X-ray telescopes are equipped with RGS
instruments. After the first week of operations, an electronic
component of one one of the RGS2 chips failed, affecting the
wavelength range from 20.0 to 24.1 Å. A similar problem
occurred in early September 2000 with one of the chips of RGS1
covering 10.6 to 13.8 Å. The total effective area is thus
reduced by a factor of two in these wavelength bands.
A detailed description of the characteristics and performance of the
RGS instruments can be found in the
XMM-Newton Handbook.
The
RGS Chapter in the XMM SAS (Science Analysis System) User's
Guide provides useful information about RGS data products and
their analysis.
What are fluxed spectra?
RGS fluxed spectra are computed dividing the extracted spectrum by
the effective area calculated from its corresponding response matrix
(see the description of the SAS task rgsfluxer).
This procedure neglects the redistribution of monochromatic response
into the dispersion channels, and therefore these spectra should not
be used for any detailed spectral analysis of the data
(e.g. measurement of line widths).
Nevertheless, fluxed spectra are extremely useful for visualizing
the data free from the peculiarities of the instrument. This is
especially so because of the possibility of combining data from both
cameras into a single spectrum, thus eliminating many of the gaps
between functioning detectors.
Fluxed spectra are given in physical units
(photons/cm²/s/Å vs. Å).
Data were processed with the SAS metatask rgsproc.
rgsproc was run using the target coordinates given in the
XMM-Newton proposal
First order spectra (without background subtraction) were
generated using 100% of the spatial PSF. A model background spectrum
(generated with the SAS task rgsbkgmodel)
was used for the background correction
Response matrices were computed for each spectrum with rgsrmfgen
Finally, a fluxed spectrum was created for each observation
combining all the available RGS1 and RGS2 first order spectra with rgsfluxer
Additional Information available in BiRD
In addition to the spectra themselves, the BiRD interface provides
other information that might be useful for the interpretation of the
data:
Start time of the observation
Target name as provided in the XMM-Newton proposal
Target coordinates as provided in the XMM-Newton proposal
RGS effective exposure time (taken as the average of the
exposure time of the RGS1 and RGS2 spectra)
An estimation of the quality of the combined RGS1+RGS2 fluxed spectrum
SIMBAD was queried to derive a first target identification and
classification using the target name given in the XMM-Newton
proposal as input. In the cases where a SIMBAD object could not be
unambiguously selected using the target name, the procedure was
done manually, examining the different identifications of nearby
objects. For a number of cases, the type of object was obtained
from the abstract of the scientific justification of the proposal.
Some particular cases:
Survey fields have been assigned the SIMBAD Type 'Region
defined in the sky'
Solar System objects have been assigned Types 'Planet' or
'Comet', as applicable
Some Numbers...
Object Types
The BiRD database includes 2744 different objects. Thirty two of them
have been observed more than fifteen times:
Object
SIMBAD Type
N. of observations
M 31
LINER-type Active Galaxy Nucleus
67
EXO 0748-676
Low Mass X-ray Binary
51
Mkn 421
BL Lac - type object
47
Galactic Centre
Region defined in the sky
38
N 132D
SuperNova Remnant
32
AB Dor
Rotationally variable Star
31
3C 273
Quasar
27
Coma Cluster
Cluster of Galaxies
27
HR 1099
Variable of RS CVn type
27
Crab
Pulsar
26
M 33
Galaxy
25
SNR 0102-72.3
SuperNova Remnant
25
CAL 83
X-ray Binary
22
Lockman Hole
Region defined in the sky
22
AMS 16
Quasar
21
Capella
Variable of RS CVn type
21
Object
SIMBAD Type
N. of observations
SMC
Galaxy
20
Her X-1
Low Mass X-ray Binary
20
PKS 2155-304
BL Lac - type object
19
Eta Car
Variable Star
19
PKS-0558-504
Seyfert 1 Galaxy
18
BPM 16274
White Dwarf
17
HD 81809
Spectroscopic binary
17
NGC 4051
Seyfert 1 Galaxy
17
Vela
SuperNova Remnant
17
BPM 16274
Star
16
Chandra Deep Field-South
Region defined in the sky
16
Zeta Puppis
Variable of BY Dra type
16
Subaru/XMM Deep Field
Region defined in the sky
16
Cygnus Loop
SuperNova Remnant
16
Cas A
SuperNova Remnant
16
SN 1006
SuperNova Remnant
16
These objects belong to 139 different types. SIMBAD types with more
than twenty different objects are:
SIMBAD Type
N. of objects
N. of observations
Cluster of Galaxies
313
638
Seyfert 1 Galaxy
294
568
Quasar
175
293
Seyfert 2 Galaxy
168
241
Galaxy
166
281
SuperNova Remnant
98
325
X-ray source
90
117
Pulsar
85
254
Low Mass X-ray Binary
71
268
Radio Galaxy
65
87
Star
48
149
High Mass X-ray Binary
48
135
Cataclysmic Variable Star
47
60
LINER-type Active Galaxy Nucleus
42
146
Cataclysmic Var. AM Her type
42
75
Variable Star
38
73
High proper-motion Star
38
45
gamma-ray Burst
36
55
Interacting Galaxies
34
72
T Tau-type Star
32
60
SIMBAD Type
N. of objects
N. of observations
HII Galaxy
32
41
Nova
31
61
gamma-ray source
31
58
BL Lac - type object
30
124
Open (galactic) Cluster
29
48
Group of Galaxies
29
46
Region defined in the sky
26
584
Radio-source
25
37
Galaxy in Cluster of Galaxies
24
31
Wolf-Rayet Star
23
53
Dwarf Nova
23
31
White Dwarf
21
55
Galaxy in Group of Galaxies
21
34
Active Galaxy Nucleus
21
27
Variable of RS CVn type
18
75
Globular Cluster
17
33
SuperNova
17
26
Emission-line Star
16
35
Galaxy in Pair of Galaxies
16
21
Exposure Times
The median exposure time of the RGS spectra is 20 ksec. Observations
longer than 125 ksec (i.e. about one revolution long) are:
ObsId
Object
SIMBAD Type
Texp (sec)
0147440101
IC 4329A
Seyfert 1 Galaxy
135369
0112210501
NGC 3783
Seyfert 1 Galaxy
134625
0204730301
GX 339-4
Low Mass X-ray Binary
134439
0606150101
QSO B1126-041
Seyfert 1 Galaxy
133892
0605540101
AWM 7
Cluster of Galaxies
133639
0147800201
ZwCl 0335+0956
Cluster of Galaxies
133509
0504370401
BL Lac
BL Lac - type object
133495
0202670801
SGR A*
Radio-source
133276
0604960401
Chandra Deep Field-South
Region defined in the sky
133228
0555780201
Chandra Deep Field-South
Region defined in the sky
132787
0202670601
SGR A*
Radio-source
132741
0204730201
GX 339-4
Low Mass X-ray Binary
132679
0306870101
Mrk 335
Seyfert 1 Galaxy
132595
0300430101
NGC 3256
Interacting Galaxies
132436
0555780101
Chandra Deep Field-South
Region defined in the sky
132393
0202670701
SGR A*
Radio-source
132278
0302900101
NGC 5408
Emission-line galaxy
131670
0600540601
Mkn 335
Seyfert 1 Galaxy
131622
0305540701
rho Oph
Star in Nebula
131262
0200370101
BP TAU
T Tau-type Star
131035
0202670501
SGR A*
Radio-source
130243
0504370701
QSO B2356-309
BL Lac - type object
130107
0503490201
1RXS J224322.6-093549
X-ray source
129604
0400620101
NGC 1399
Galaxy in Cluster of Galaxies
129525
0109890501
Abell 665
Cluster of Galaxies
128961
ObsId
Object
SIMBAD Type
Texp (sec)
0555630501
SN 1006
SuperNova Remnant
128955
0505140401
NGC 1365
Seyfert 1 Galaxy
128677
0554680101
NGC 5044
Galaxy in Group of Galaxies
128349
0502290101
PSR J0030+0451
Pulsar
128288
0111800101
M 81
LINER-type Active Galaxy Nucleus
127908
0505140201
NGC 1365
Seyfert 1 Galaxy
127659
0555170301
PKS 0558-504
Seyfert 1 Galaxy
127403
0152840101
3C120
Seyfert 1 Galaxy
127355
0504780501
HCG 62
Cluster of Galaxies
126709
0501790101
NGC 2547
Cluster of Stars
126685
0300270201
XX Cha
T Tau-type Star
126639
0200080701
Jupiter
Planet
126621
0155960501
PSR J1210-5226
Pulsar
126405
0109141301
Mkn 766
Seyfert 1 Galaxy
126404
0101440801
SU Aur
Variable Star of Orion Type
126126
0107460701
NGC 3516
Seyfert 1 Galaxy
126094
0555170401
PKS 0558-504
Seyfert 1 Galaxy
125899
0505140501
NGC 1365
Seyfert 1 Galaxy
125796
0555170501
PKS 0558-504
Seyfert 1 Galaxy
125680
0155960301
PSR J1210-5226
Pulsar
125677
0560180401
GRB 980618A
gamma-ray Burst
125445
0147800101
Sersic 159-03
Cluster of Galaxies
125281
0555781001
Chandra Deep Field-South
Region defined in the sky
125275
0555782301
Chandra Deep Field-South
Region defined in the sky
125254
 
The Brightest Targets
The brightest objects observed with RGS (those having more than 25 cts/sec
in the extracted RGS1 spectrum over the full wavelength range) are: