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 IRAS 00521-7054 13.5029 -70.6421 13.04558 -70.91316 316.631077 -63.690795 302.62218098 -46.48460341 40.2116 56431.8840740741 2013-05-19 21:13:04 56434.2543287037 2013-05-22 06:06:14 708005010 103.045 100 103.053 103.045 0 103.053 2 2 0 2 1 0 0 87.3405 87.3405 204.7697 1 PROCESSED 57611.3837152778 2016-08-11 09:12:33 56809 2014-06-01 00:00:00 56443.6034259259 2013-05-31 14:28:56 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 080036 The existence of a broad iron line in AGN is still very debated. Amongst the several claims of detection of broad iron lines performed in the last decade, that of IRAS 00521-7054 is one of the most surprising. This type-2 object appears to show in fact an extremely broadened iron line, which would require a maximally rotating supermassive black hole and the presence of light bending. However, due to the lack of high-quality broadband studies, alternative explanations, as a clumpy-absorbers scenario, cannot be ruled out. The aim of this proposal is to perform a 100ks observation of IRAS 00521-7054. Thanks to its large band coverage and its good sensitivity in the iron-line region, Suzaku will allow us to clearly understand the origin of the intriguing spectral features of IRAS 00521-7054. EXTRAGALACTIC COMPACT SOURCES 7 B CLAUDIO RICCI JAP 8 AO8 UNDERSTANDING THE ORIGIN OF THE PECULIAR X-RAY SPECTRAL FEATURES OF THE SEYFERT 2 IRAS 00521-7054 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/708005010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '708005010'

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