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.
observation_id
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
exposure
awarded_exposure
resolve_exposure
resolve_data_mode
resolve_with_filter_be
resolve_with_filter_fe55
resolve_with_filter_nd
resolve_with_filter_poly
resolve_with_filter_open
resolve_with_filter_undef
is_resolve_gatevalve_closed
is_resolve_mxs1
is_resolve_mxs2
is_resolve_mxs3
is_resolve_mxs4
resolve_code
gen_code
processing_status
processing_date
public_date
distribution_date
processing_version
caldb_version
processing_software
proposal_id
proposal_abstract
proposal_category
proposal_category_code
proposal_priority
pi_name
co_pi_name
proposal_affiliated_country
proposal_cycle
proposal_type
proposal_title
observation_status
data_access_url
ql_access_url
ql_image_url
corner1_ra
corner1_dec
corner2_ra
corner2_dec
corner3_ra
corner3_dec
corner4_ra
corner4_dec
corner5_ra
corner5_dec
corner6_ra
corner6_dec
corner1_ra_b1950
corner1_dec_b1950
corner2_ra_b1950
corner2_dec_b1950
corner3_ra_b1950
corner3_dec_b1950
corner4_ra_b1950
corner4_dec_b1950
corner5_ra_b1950
corner5_dec_b1950
corner6_ra_b1950
corner6_dec_b1950
corner1_ecliptic_lon
corner1_ecliptic_lat
corner2_ecliptic_lon
corner2_ecliptic_lat
corner3_ecliptic_lon
corner3_ecliptic_lat
corner4_ecliptic_lon
corner4_ecliptic_lat
corner5_ecliptic_lon
corner5_ecliptic_lat
corner6_ecliptic_lon
corner6_ecliptic_lat
corner1_galactic_lon
corner1_galactic_lat
corner2_galactic_lon
corner2_galactic_lat
corner3_galactic_lon
corner3_galactic_lat
corner4_galactic_lon
corner4_galactic_lat
corner5_galactic_lon
corner5_galactic_lat
corner6_galactic_lon
corner6_galactic_lat
resolve_adr_mode
resolve_thr_name
resolve_shp_date
1 201018010 GX1+4 263.00753 -24.74524 262.23961 -24.70949 263.65029 -1.45994 1.93662 4.79626 93.08029 60759.21671 2025-03-25 05:12:04 60760.57644 2025-03-26 13:50:04 47.379 40.000 47.379 PX_NORMAL N Y N N Y Y Y OFF OFF OFF OFF 313430 11310 PROCESSED 2025-04-11 10:44:48 2026-04-16 00:00:00 2025-04-12 10:44:48 03.00.013.010 gen20241115_xtd20241115_rsl20241115 Hea_21Aug2024_V6.34_XRISM_21Aug2024_V001 000011098 One of the big questions in neutron stars is how the strong magnetic field is formed and evolved. We propose a 40 ks observation of a low-mass X-ray binary pulsar GX 1+4, which has long been suspected to have a very high magnetic field strength, perhaps ~ 1e14 G. Thanks to the excellent energy resolution of the Resolve, the proposed observation enables us for the first time to resolve the profile of the Fe K alpha lines and to measure the magnetic field strength above 1e13 G, which is impossible to probe using the cyclotron resonance scattering feature (CRSF). From this observation we can determine whether or not the source is the first magnetar binary ever detected. Moreover, Resolve may provide a unique opportunity to search for the proton CRSF. BH AND NS BINARIES 2 B TOSHIHIRO TAKAGI JAP 1 NOR DETERMINING THE MAGNETIC FIELD STRENGTH OF THE LOW MASS X-RAY BINARY PULSAR GX 1+4: A UNIQUE MAGNETAR BINARY? archived https://data.darts.isas.jaxa.jp/pub/xrism/data/obs/rev3/2/201018010/ Quick Look 263.03582 -24.72218 262.97923 -24.71938 262.97677 -24.76205 262.98612 -24.76247 262.98555 -24.77092 263.03271 -24.77334 262.26802 -24.68657 262.21147 -24.6835 262.20876 -24.72616 262.21811 -24.72662 262.21749 -24.73507 262.26461 -24.73772 263.67486 -1.43567 263.62336 -1.43537 263.6232 -1.47809 263.63171 -1.4781 263.6316 -1.48656 263.6745 -1.48691 1.97004 4.78717 1.94442 4.83187 1.90723 4.81059 1.91151 4.80323 1.9041 4.79908 1.92537 4.7618 HELIUM A75A 2021-12-13 00:00:00

Used SQL

SELECT * FROM xrism_resolve_data WHERE observation_id = '201018010'

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