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 IRAS13224-3809 201.327 -38.416 200.607672 -38.155977 214.865009 -27.173801 310.18598264 23.97820794 118.5234 54126.2420601852 2007-01-26 05:48:34 54131.0849421296 2007-01-31 02:02:19 701003010 197.9376 200 197.9536 197.9376 0 197.9516 2 2 0 2 1 0 0 169.6526 169.6526 418.3978 4 PROCESSED 57537.0458912037 2016-05-29 01:06:05 54777 2008-11-07 00:00:00 54139.7293287037 2007-02-08 17:30:14 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 010028 We propose a 200 ks continuous observation of the narrow-line Seyfert 1 galaxy IRAS13224-3809 in order to understand its remarkable and puzzling spectral and variability properties. Suzaku data will enable us to disentangle the two interpretations adopted so far, namely partial covering and relativistically blurred reflection. If the latter then the appearance of the source is controlled by general relativistic effects. In addition, the ability for Suzaku to conduct long continuous observations will allow us to monitor IRAS13224-3809 for giant amplitude flaring (as seen with ROSAT); therefore enabling us to enhance our understanding of AGN variability. EXTRAGALACTIC COMPACT SOURCES 7 B YASUO TANAKA JAP 1 AO1 THE REMARKABLE NARROW LINE SEYFERT 1 GALAXY IRAS13224-3809 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/701003010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '701003010'

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