DARTS/Astro Query System - SQL Search -
All the tables available for SQL Search and information on each table are listed in the Available Data page. Please see the User Guide for the usage of "SQL Search".
total 1
No. |
object_name
|
center_ra
|
center_dec
|
center_ra_b1950
|
center_dec_b1950
|
center_ecliptic_lon
|
center_ecliptic_lat
|
center_galactic_lon
|
center_galactic_lat
|
roll_angle
|
observation_start_time_mjd
|
observation_start_time
|
observation_end_time_mjd
|
observation_end_time
|
observation_id
|
exposure
|
awarded_exposure
|
xis0_exposure
|
xis1_exposure
|
xis2_exposure
|
xis3_exposure
|
xis0_observation_mode
|
xis1_observation_mode
|
xis2_observation_mode
|
xis3_observation_mode
|
hxd_observation_mode
|
hxd_coarse_clock_rate_exposure
|
hxd_first_clock_rate_exposure
|
hxd_normal_clock_rate_exposure
|
hxd_all_clock_rate_exposure
|
hxd_wam_exposure
|
quantity_of_hxd_burst
|
processing_status
|
processing_date_mjd
|
processing_date
|
public_date_mjd
|
public_date
|
distribution_date_mjd
|
distribution_date
|
processing_version
|
processing_count
|
processing_software
|
proposal_id
|
proposal_abstract
|
proposal_category
|
proposal_category_code
|
proposal_priority
|
pi_name
|
co_pi_name
|
proposal_affiliated_country
|
proposal_cycle
|
observation_type
|
proposal_title
|
main_instrument
|
has_xis_injection
|
data_access_url
|
ql_access_url
|
ql_image_url
|
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1 | MCG-6-30-15 | 203.9717 | -34.2976 | 203.255303 | -34.04246 | 215.173232 | -22.546653 | 313.28966663 | 27.67858669 | 102.4356 | 53758.5062962963 | 2006-01-23 12:09:04 | 53761.0835648148 | 2006-01-26 02:00:20 | 700007020 | 98.4834 | 300 | 98.4834 | 98.4834 | 98.4834 | 98.4834 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 81.8922 | 81.8922 | 222.6497 | 3 | PROCESSED | 57532.8430902778 | 2016-05-24 20:14:03 | 54247 | 2007-05-27 00:00:00 | 54059.5463773148 | 2006-11-20 13:06:47 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 001035 | The broad iron line in the Seyfert 1 galaxy MCG-6-30-15 shows that most of the power is released at 2--4 gravitational radii enabling the strong gravity, accretion flow and energy release in that exciting regime to be studied. The spectral variability of the source decomposes into a highly variable power law and a reflection-dominated component, containing the iron line and Compton hump, which varies significantly but with much less amplitude. This can be explained by the extreme gravitational light bending occuring in this region. We propose to observe MCG--6-30-15 for 4 x 50~ks in order to determine for the first time the variability of the reflection over a wide range of energies from below 1 keV to above 40 keV and timescales . | EXTRAGALACTIC COMPACT SOURCES | 7 | A | ANDREW FABIAN | JAP | 0 | SWG | REFLECTION, ABSORPTION AND STRONG GRAVITY AROUND THE SPINNING BLACK HOLE IN MCG--6-30-15 | XIS | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/700007020/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '700007020'
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