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 | RE J1034+396 | 158.663 | 39.6488 | 157.936699 | 39.907419 | 144.538164 | 28.290615 | 180.26295059 | 59.06449262 | 115.7032 | 56245.9648726852 | 2012-11-14 23:09:25 | 56248.0689583333 | 2012-11-17 01:39:18 | 707039010 | 99.9113 | 100 | 99.9193 | 99.9113 | 0 | 99.9193 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 93.446 | 93.446 | 181.7639 | 3 | PROCESSED | 57608.0485416667 | 2016-08-08 01:09:54 | 56640 | 2013-12-14 00:00:00 | 56274.6249884259 | 2012-12-13 14:59:59 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 072005 | Understanding the nature of the emission from the extreme active galaxy, RE J1034+396 can help us to unravel the properties of accretion as the Eddington limit is reached. A fleeting glimpse of the unique quasi-periodic oscillation (QPO) in this source has shown a complex timing behaviour with the emission below ~2 keV apparently crucial to its presence. Thus by understanding the origin and properties of the soft emission we can probe the physical mechanism of signals that cannot be resolved in stellar mass X-ray binaries but must be associated with the regions closest to the black hole. A new observation with Suzaku will allow a much deeper analysis of the soft emission and will shed light on how its changing properties can trigger such unique behaviour as the QPO. | EXTRAGALACTIC COMPACT SOURCES | 7 | C | MATTHEW MIDDLETON | EUR | 7 | AO7 | REVEALING THE NATURE OF RE J1034+396 AND THE EXTREME SOFT EXCESS | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/707039010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '707039010'
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