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
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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