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 FAIRALL 9 20.9481 -58.8141 20.470954 -59.074601 340.57309 -59.156739 295.06951561 -57.81752905 48.1772 54258.155462963 2007-06-07 03:43:52 54260.5766666667 2007-06-09 13:50:24 702043010 167.7983 164 167.7983 167.8063 0 167.8143 2 2 0 2 1 0 0 136.4834 136.4834 209.1758 2 PROCESSED 57538.9238425926 2016-05-30 22:10:20 54773 2008-11-03 00:00:00 54265.5470717593 2007-06-14 13:07:47 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 021313 Recently, deep observations of a number of Seyfert AGN with XMM-Newton and Suzaku have established variable and relativistic iron lines as robust features in roughly half of all deep Seyfert spectra. In these sources, the spin of the black hole can be constrained directly through fits to the relativistic iron line. A sample of excellent spectra from well-chosen AGN will facilitate a better understanding of the innermost regime near to black holes, and make correlations with parameters like radio luminosity, star formation rate, and galaxy and black hole mass possible for the first time. We propose to obtain observations of 4 under-exposed Seyfert AGN with promising evidence for broad lines to robustly constrain their spin parameters. EXTRAGALACTIC COMPACT SOURCES 7 A JON MILLER USA 2 AO2 REVEALING BLACK HOLE SPIN IN RELATIVISTIC SEYFERT AGN XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/702043010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '702043010'

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