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 | 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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