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 | IRAS18325-5926 | 279.2243 | -59.4565 | 278.116624 | -59.498471 | 275.782962 | -36.20075 | 335.92469241 | -21.3483138 | 281.9669 | 54399.3814699074 | 2007-10-26 09:09:19 | 54401.4169444444 | 2007-10-28 10:00:24 | 702118010 | 78.4348 | 80 | 78.4348 | 78.4428 | 0 | 78.4428 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 74.2917 | 74.2917 | 175.8357 | 0 | PROCESSED | 57540.4011458333 | 2016-06-01 09:37:39 | 54777 | 2008-11-07 00:00:00 | 54409.305474537 | 2007-11-05 07:19:53 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 022025 | We propose a 80 ks observation of the Seyfert galaxy IRAS 18325-5926. Previous observations show evidence for reflection from highly ionized matter, absorption features in the 8-10 keV band, and a possible roll-over of the continuum spectrum at around 30 keV. The observation goal is to elucidate the continuum roll-over and to investigate variability of the spectral features, which would have many important implications for the physical condition and the geometry of the accretion disc and the illuminating source. This study will provide crucial keys to understand the geometry of primary X-ray source and immediate surroundings. The broad-band coverage and the high sensitivity at the hard X-ray band provided by Suzaku are ideally suited to study this unique AGN. | EXTRAGALACTIC COMPACT SOURCES | 7 | C | KAZUTAMI MISAKI | EUR | 2 | AO2 | HARD X-RAY SPECTRUM OF IRAS 18325-5926: REFLECTION FROM AN IONIZED DISC AND CONTINUUM ROLL-OVER | HXD | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/702118010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '702118010'
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