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 MKN 335 1.5763 20.2091 0.933386 19.930785 9.740827 17.860354 108.75916207 -41.41726175 71.5255 56457.9792939815 2013-06-14 23:30:11 56461.868287037 2013-06-18 20:50:20 708016020 154.8168 300 154.8648 154.8168 0 154.8568 2 2 0 2 1 0 0 141.5908 141.5908 335.8944 3 PROCESSED 57611.6590162037 2016-08-11 15:48:59 56383 2013-04-01 00:00:00 56512.7189467593 2013-08-08 17:15:17 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 081411 The idea of this proposal is trigger a 300ks observation with Suzaku of the Narrow Line Seyfert 1 Galaxy Mkn 335 during one of its low X-ray flux states. The goal here is to measure its underlying broad-band continuum with Suzaku during a low state and compare it with the 2006 high-state observations. Mkn 335 is one of the best examples of an AGN that went into a deep minimum X-ray flux state. Two competing models can explain these extreme low states: reflection models and partial covering absorber models. Both models still require a variable underlying intrinsic continuum. The science driver is to find out what is causing these low X-ray flux states that have been observed in several NLS1s. EXTRAGALACTIC COMPACT SOURCES 7 A DIRK GRUPE USA 8 AO8-TOO INTRINSIC LOW-STATE X-RAY LUMINOSITY OF THE NLS1 MKN 335 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/708016020/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '708016020'

Your request has been accepted.
The download will start soon automatically.

Go to top of this page ⏏