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 NGC 7603 349.73 0.2557 349.089402 -0.017972 350.656446 4.302592 80.07171077 -54.72674929 67.5296 56080.5080208333 2012-06-02 12:11:33 56082.6598726852 2012-06-04 15:50:13 707003010 101.2567 100 101.2602 101.2657 0 101.2567 2 2 0 2 1 0 0 96.0023 96.0023 185.9037 2 PROCESSED 57605.6196875 2016-08-05 14:52:21 56464 2013-06-21 00:00:00 56096.2688541667 2012-06-18 06:27:09 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 070010 X-ray spectra from Seyfert galaxies often consist of various emission components such as from an accretion disk and dusty torus. Because of this complexity, interpretation of reprocessed feature (Fe lines and reflection continuum) in X-ray spectra is often ambiguous. We selected a Seyfert 1 with very weak mid infrared emission from the putative torus relative to X-rays from an accretin disk bu using AKARI IR and XMM X-ray catalogs. We will measure a ``pure'' accretion disk spectrum without contamination of reprocessed emission from the torus, and castrain extent of an accretion disk, which is expected to depend on an Eddington ratio, from the reprocessed X-ray emission. EXTRAGALACTIC COMPACT SOURCES 7 B YUICHI TERASHIMA JAP 7 AO7 PURE ACCRETION DISK SPECTRUM OF THE SEYFERT 1 NGC 7603 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/707003010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '707003010'

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